TIMEEVENT DESCRIPTIONLOCATION

UNIVERSE
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6) Light particles become trapped with each other and so form structures such
as protons, atoms, molecules, planets, stars, galaxies, and clusters of
galaxies.

This forming of light particles into atoms may be the result of particle
collision, gravitation (an attraction of matter with itself) or a combination
of both.
  
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7) All of the billions of galaxies we see are only a tiny part of the universe.
We will never see most of the universe because no light particles from there
can ever reach us.

Most galaxies are too far away for even one particle of light they emit to be
going in the exact direction of our tiny location, and all the light particles
they emit are captured by atoms in between there and here.

One estimate has 70e21 (sextillion) stars in only the universe we can see. That
is 10 times more stars than grains of sand on all the earth.

As telescopes grow larger, the number of galaxies we see will increase.
  
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4) There is a pattern in the universe. Light particles move from highly dense
volumes of space to volumes of less density. In low density volumes, light
particles slowly accumulate to form atoms of Hydrogen and Helium which exist as
gas clouds (like the Magellanic Clouds or Orion nebula). These gas clouds,
called nebulae continue to accumulate trapped light particles. At points of
high density planets and stars form and the cloud is eventually dense enough to
become a galaxy of stars. The stars emit light particles back out to the rest
of the universe, where the light again becomes trapped and forms new clouds.
Around each star are many planets and pieces of matter. On many of the planets
rotating around stars, living objects evolve that can copy themselves by
converting matter around them into more of them. Living objects need matter to
replace matter lost from the constant emitting of light particles (decay). Like
bacteria, these living objects grow in number, with the most successful
organisms occupying and moving around many stars. These advanced organisms then
move the groups of stars they control, as a globular cluster, away from the
plane of the spiral galaxy. As time continues, all of the stars of a galaxy are
occupied by living objects who have organized their stars into globular
clusters, and these globular clusters together, form a globular galaxy. The
globular galaxy may then exist for a long time living off the matter emitting
from stars, in addition to the accumulation of light particles from external
sources.

So free light particles are trapped into volumes of space that grow in density
first forming atoms, then gas clouds, then stars, a spiral galaxy, and finally
a globular galaxy.

Stars at our scale may be light particles at a much larger scale, just as light
particles at our scale may be stars at a much smaller scale. This system may go
on infinitely in both larger and smaller scale.

For any given volume of space, there is a ratio of light particles going in
versus light particles going out. If more light particles are entering than
exiting the volume has a deficit of light particles, and so acts as a vacuum
and grows in size, if more particles are exiting than entering, the volume is
already very dense, has a surplus of light particles, and is losing density.
  
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8) An expanding universe seems unlikely to me. The supposed red-shifted calcium
absorption lines may be a mistaken observation, for one reason because of the
different sizes of spectra as clearly seen in the 1936 Humason image, and
because distance of light source changes the position, but not the frequency of
spectra.

Beyond this, the claim of a "background radiation" is probably simply low
frequencies of light particles from light sources that are close enough to be
detected. Most light sources are too far away for even one particle emitted
from them to reach us.
  
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9) Quasars may be very distant regular galaxies.

  
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10) Globular clusters and elliptical galaxies may be made by intelligent life,
and spiral galaxies formed without the direct help of living objects. The star
types are almost all long lived yellow stars, and there is little or no
Hydrogen or Helium "dust" as there are in spiral galaxies. The stars in
elliptical galaxies are light weeks apart, much closer together than our star
which is 4 light years to the closest star system. Life orbiting any star of a
spiral galaxy probably would leave the plane of the galaxy by going up or down.

  
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12) How photons form atoms may still be unknown. Perhaps simply from
gravitational attraction, or maybe there need to be large groups of photons to
limit available spaces for photons to move in (for example in stars, or
galactic centers, and or supernovas.

  
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14) Photons take on a variety of shapes at different scales from the smallest
forms in light, up to atoms, molecules, molecule groups (like living objects),
planets, stars, galaxies, galactic clusters and the visible universe is the
largest formation of photons we can see.

  

LIFE
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22) In a star system, because of gravitation, heavier masses move closer to the
center and lighter masses move farther out.
  
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32) Allende Meteorite 4,566 million years old.

  
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34) Oldest "terrestrial" zircon; evidence that the crust and liquid water are
on the surface of earth. A terrestrial zircon is not from a meteorite. This
zircon if from Gneiss in West Australia that is 4.4 billion years old.
  
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18) Larger molecules like amino acids, phosphates and sugars, the components of
living objects, form on Earth.

These molecules are made in the oceans, fresh water, and atmosphere of earth
(and other planets) by lightning, light particles with ultraviolet frequency
from the Sun, and from ocean floor volcanoes.
  
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19) Nucleic acids form on Earth. One of these RNA molecules may be the ancestor
of all of life on Earth, being part of the series of copies that leads to all
later living objects on Earth.

Even if bacteria survived the journey from a different star to this star and
seeded the earth, the chemical evolution of the first cell is necessary
somewhere in the universe.

The initial building blocks of living objects are very easy to produce, but the
next step is more difficult: assembling the simple building blocks into
longer-chain molecules, or polymers. Amino acids link up to form longer
polymers called proteins, simple fatty acids plus alcohols link up to form
lipids (oils and fats), simple sugars like glucose and sucrose link together to
form complex carbohydrates and starches, and finally, the nucleotide bases
(plus phosphates and sugars) link up to form nucleic acids, the genetic code of
organisms, known as RNA and DNA.

How nucleic acids (polymers made of nucleotides), proteins (polymers made of
amino acids), carbohydrates (polymers made of sugars) and lipids (glycerol
attached to fatty acids) evolved is not clearly known. Possibly all proteins,
carbohydrates and lipids are strictly the products of living objects.

Some proteins and nucleic acids have been formed in labs by using clay which
can dehydrate and which provides long linear crystal structures to build
proteins and nucleic acids on. Amino acids join together to form polypeptides
when an H2O molecule is formed from a Hydrogen (H) on 1 amino acid and a
hydroxyl (OH) on the second.

Perhaps proteins, carbohydrates, lipids and DNA are the products of living
objects, with RNA being made without the help of living objects.

The most popular theory now has RNA (and potentially lipids) evolving first
before any living objects. But perhaps proteins evolved first, and a protein
linked together the first nucleic acid.

A bacteria can survive the trip between two stars, and possibly a eukaryote
cell could survive frozen and be waken up again many years later, but it seems
unlikely that a multicellular eukaryotic organism could survive and be revived
from one star to another.

Probably bacteria from a variety of stars lands on all planets and asteroids,
and is revived on many where the temperature allows them to copy.

There is still a large amount of experiment, exploration and education that
needs to be done to understand the origins of living objects on planet earth.
  
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25) An RNA molecule may evolve that can copy other RNA molecules.

Perhaps RNA molecules, called "ribozymes" evolve which can make copies of RNA,
by connecting free floating nucleotides that match a nucleotide on the same or
a different RNA, much like tRNA do in assembling amino acids into proteins. But
until such ribozyme RNA molecules are found, the only molecule known to copy
nucleic acids are proteins called polymerases.

These early RNA molecules may have been protected by liposomes (spheres of
lipids).

This process of RNA (and then later DNA) duplication is the most basic aspect
of life on Earth, and for all the diversity, the one common element of all life
is this constant process of DNA duplication, which will later evolve to include
cell division. This starts the unbroken thread of copying and division that
connects the earliest ancestor, perhaps some RNA molecule, to all life on earth
that has ever lived.

This may be the start of the constant conversion of other matter into nucleic
acids. This constant copying will ultimately result in billions of living
objects on earth.
  
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167) The first proteins on Earth. Transfer RNA molecules evolve (tRNA), and
link amimo acids into proteins using other RNA molecules (mRNA) as a template.

For the first time, a nucleic acid functions both as a template for building
other nucleic acid molecules, and also as a template for building proteins
(with the help of tRNA molecules).

This protein assembly system is the main system responsible for all the
proteins on Earth.

Whether the first tRNA and protein assembly evolved before or after the
evolution of the ribosome is currently unknown.

Random mutations in the copying (and perhaps even in the natural formation) of
RNA molecules probably creates a number of the necessary tRNAs (tRNA, are RNA
molecules responsible for matching free floating amino acid molecules to
three-nucleotide sequences on other RNA molecules).

This is a precellular, pre-ribosome protein assembly system, where tRNA
(transfer RNA) molecules build polypeptide chains of amino acids by linking
directly to other RNA strands.

Part of each tRNA molecule bonds with a specific amino acid, and a 3 nucleotide
sequence from a different part of the tRNA molecule bonds with the opposite
matching 3 nucleotide sequence on an mRNA molecule.

Since there are tRNA molecules for each amino acid (although some tRNAs can
attach to more than one amino acid), there must have been a slow accumulation
of various tRNA molecules for each of the 20 amino acids used in constructing
polypeptides in cells living now. Perhaps after the evolution of the first
tRNA, the first polypeptides were chains of all the same one amino acid. With
the evolution of a second tRNA polypeptides would have more variety because now
two amino acids would be available to build polypeptides.

This polypeptide assembly system may exist freely in water, or within a
liposome. This system builds many more proteins than would be built without
such a system. The mRNA with the code to make copier RNA, now also contains the
code to produce various tRNA molecules. These molecules function as a unit, and
proto-cell, with the rest of the mRNA initially containing random codes for
random proteins.
  
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168) The ribosome evolves. First Ribosomal RNA (rRNA).

The ribosome may function as a protocell, providing a platform for more
efficient protein production. A single RNA may contain all the instructions
needed to make more ribosomes.

Ribosomes are the cellular organelles that carry out protein synthesis, through
a process called translation. They are found in both prokaryotes and
eukaryotes. These molecular machines are responsible for accurately translating
the linear genetic code on the messenger RNA (mRNA), into a linear sequence of
amino acids to produce a protein. All cells contain ribosomes because growth
requires the continued synthesis of new proteins. Ribosomes can exist in great
numbers, ranging from thousands in a bacterial cell to hundreds of thousands in
some human cells and hundreds of millions in a frog ovum. Ribosomes are also
found in mitochondria and chloroplasts.

This early ribosome may function as a protocell, holding an mRNA molecule which
is used as a template by tRNA molecules to assemble amino acids into proteins.
A single mRNA molecule may contain the instructions for an RNA polymerase and
for all the necessary rRNA, and tRNA molecules needed to make more ribosomes.

This ribosomal RNA may serve as an early ribosome. As time continues the
ribosome will grow to include two more RNA molecules, some protein molecules,
and a second half that will make polypeptide construction more efficient.

The modern ribosome is a large ribonucleoprotein (RNA-protein) complex, roughly
20 to 30 nanometers in diameter. It is formed from two unequally sized
subunits, referred to as the small subunit and the large subunit. The two
subunits of the ribosome must join together to become active in protein
synthesis. However, they have distinguishable functions. The small subunit is
involved in decoding the genetic information, while the large subunit has the
catalytic activity responsible for peptide bond formation (that is, the joining
of new amino acids to the growing protein chain).
  
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40) A protein can copy RNA. This protein is called an RNA polymerase, and may
be more efficient than RNA itself, at copying other RNA molecules, or may be
the first molecule that can copy RNA.

An RNA polymerase must have been one of the first useful proteins to be
assembled by the early (presumably) precellular protein production system.
Eventually an mRNA that codes for the necessary tRNA, and RNA polymerase may be
copied many times.
  
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166) The first Deoxyribonucleic acid (DNA) molecule. A protein evolves that can
assemble DNA from RNA.

This protein, built by a ribosome, changes ribonucleotides into
deoxyribonucleotides, which allows the first DNA molecule on Earth to be
assembled.

Ribonucleotide reductase may be the molecule that allows DNA to be the template
for the line of cells that survives to now.

If RNA and DNA evolved at the same or different times is not clear yet.
Possibly RNA and DNA were created by the same process.
  
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212) A protein can copy DNA molecules, a DNA polymerase.
  
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20) The first cell on earth (a bacterium). DNA is surrounded by a membrane of
proteins made by ribosomes. The first cytoplasm.

This cell may form in either fresh or salt water, near the sunlit water surface
or near underwater volcanoes on the ocean floor.

Binary fission evolves. A protein duplicates DNA within the cell and then the
cell divides into two parts.

Procaryotes reproduce by binary fission. The chromosome begins to replicate at
a specific place on the chromosome called the "origin of replication" producing
two origins. As the chromosome continues to replicate, one origin moves rapidly
toward to opposite end of the cell. While the chromosome is replicating, the
cell grows longer. When replication is complete and the bacterium has reached
about twice its initial size, its plasma membrane grows inward, dividing the
parent cell into two child cells, each with a complete genome.

The DNA of this cell contains the template for itself: a copying molecule (DNA
polymerase), and the necessary mRNA, tRNA, and rRNA molecules needed to build
the cytoplasm. For the first time, ribosomes and DNA build cell structure. DNA
protected by cytoplasm is more likely to survive and be copied. Copies of this
cell also have cytoplasm.

This cell structure forms the basis of all future cells of every living object
on earth. These first cells are probably anaerobic (do not require free oxygen)
and heterotrophic, meaning that they do not make their own food: amino acids,
nucleotides, phosphates, and sugars. These early bacteria depend on obtaining
external sources of these molecules and light particles in the form of heat to
reproduce and grow.

Amino acids, nucleotides, water, and other molecules enter and exit the
cytoplasm only because of a difference in concentration from inside and outside
the cell (passive transport) and represent the beginnings of the first
digestive system.

This membrane forms the first protective barrier between for DNA and the
external universe, and serves as a container to hold water.

Two important evolutionary steps evolve: DNA duplication in cytoplasm, and cell
(DNA with cytoplasm) division. Not only must the DNA copy and divide, but the
cell membrane must divide too.

A system of division may evolve which attaches the original and newly
synthesized copy of DNA to the cytoplasm, so that as the cell grows, the two
copies of DNA can be separated and the first membraned cells can divide into
two cells.

The process of DNA duplication is probably similar if not the same process
using the same proteins that were used to duplicate DNA without cytoplasm.

It is possible that bacteria could arrive on Earth from some other star, or
even from a different galaxy and be the ancestor of all life on Earth.
  
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183) The first lipids on Earth; (fats, oils, waxes). Cells evolve that make
proteins that can assemble lipids.
  
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196) Active transport evolves. Cells evolve in which both proteins and ATP are
used to transport molecules into and out of the cytoplasm.

Active transport enabled a cell to maintain internal concentrations of small
molecules that differ from the cell's surroundings.

A transport protein that generates voltage across a membrane is called an
"electrogenic pump". Proton pumps, the main electrogenic pumps of plants,
fungi, and bacteria are proteins that create an voltage across membranes. Using
ATP, a proton pump moves a positive charge in the form of hydrogen ions out of
the cell.

Another example of active transport is how Escherichia coli imports lactose
using an ion gradient-mediated active transport. Lactose is transported across
the plasma membrane by a membrane associated permease which is coded for by a
gene of the lac operon.
  
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64) Operons evolve which allow for turning off the assembly of any protein.

Operons, sequences of DNA that allow certain proteins coded by DNA to not be
built, evolve. Proteins bind with these DNA sequences to stop RNA polymerase
from building mRNA molecules which would be translated into proteins. Operons
allow a bacterium to produce certain proteins only when necessary. Bacteria
before now can only build a constant stream of all proteins encoded in their
DNA.
  
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27) Peptidoglycan occurs only in the Bacteria (except for those without a cell
wall, such as Mycoplasma). Peptidoglycan is a long-chain polymer of two
repeating sugars (N-acetylglucosamine and N-acetyl muramic acid), in which
adjacent sugar chains are linked to one another by peptide bridges that give
the link rigid stability. The nature of the peptide bridges differs
considerably between species of bacteria. Peptidoglycan synthesis is the target
of many useful antimicrobial agents, including the β-lactam antibiotics (e.g.,
penicillin) that block the cross-linking of the peptide bridges. Some of the
proteins that animals synthesize as natural antibacterial defense factors
attack the cell walls of bacteria.
  
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77) Archaea (also called archaebacteria) evolve. Phylum Nanoarcheota.

Eubacteria and Archaea are the two major lines of Prokaryotes. Prokaryotes are
the most primitive living objects ever found. Prokaryotes differ from the later
evolved eukaryotes in have a circle of DNA located in their cytoplasm (not
chromosomes) and have no nucleus. There are many widely varying estimates of
when the last common ancestor between Eubacteria and Archaea evolved. At least
one genetic comparison shows the common ancestor of Eubacteria and Archaea
evolving now.
  
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292) (It seems logical that the prokaryote flagellum would evolve in
proteobacteria because most prokaryotes with a flagellum are in the
Proteobacteria domain. There is a unity between pili, flagellum, and exchange
of DNA (sex), in particular, in the proteobacterium E. Coli.)
  
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78) Archaea Phylum: Korarchaeota evolves according to genetic comparison.
This group,
originally identified by two environmental sample sequences from the Obsidian
Pool hot spring in Yellowstone National Park, currently includes only
environmental DNA sequences and no Korarchaeota have been cultured yet.
  
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180) Archaea Phylum: Euryarchaeota {YRE-oR-KE-O-Tu} (methanogens, halobacteria)
evolve according to genetic comparison.

Earliest cell response to light.

The Euryarchaeota {YRE-oR-KE-O-Tu} are a major group of Archaea (or
Archaebacteria). They include the methanogens, which produce methane and are
often found in intestines, the halobacteria, which survive extreme
concentrations of salt, and some extremely thermophilic aerobes and anaerobes.
They are separated from the other archaeans based mainly on rRNA sequences.

The Euryarchaeotes may be the living object with the most primitive DNA still
found on earth (depending on the accurate determination of the origin of
Eubacteria and Archaea).

Halophilic archaebacteria, such as Halobacterium salinarum, use sensory
rhodopsins for phototaxis (positive or negative movement along a light gradient
or vector).
  
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181) Genetic comparison shows the Archaea Phylum, Crenarchaeotes evolving now.

The phylum Crenarchaeota, commonly referred to as the Crenarchaea, contains
many extremely thermophilic (hot-loving) and psychrophilic (cold-loving)
organisms. They were originally separated from the other archaeons based on
rRNA sequences, since then physiological features, such as lack of histones
have supported this division. Until recently all cultured crenarchaea have been
thermophilic or hyperthermophilic organisms, some of which have the ability to
grow up to 113 degrees C. These organisms stain gram negative and are
morphologically diverse having rod, cocci, filamentous and unusually shaped
cells.
  
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49) replace wiki source
  
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43) The simple equation of photosynthesis is: 6 H2O + 6 CO2 + photons = C6H12O6
(glucose) + 6O2. The detailed steps of photosynthesis are called the "Calvin
Cycle". Prokaryote cells can now produce their own glucose to store and be
converted to ATP by glycolysis and fermentation later.

Of the 5 phyla of eubacteria that can photosynthesize, only 1, cyanobacteria,
produces oxygen.
  
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Akilia Island, Western Greenland  
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45) Oldest sediment, the Banded Iron Formation begins.
Banded Iron Formation is
sedimentary rock that spans from 3.8 to 1.8 billion years ago, made of
iron-rich silicates (like silicon dioxide SiO2) with alternating layers of
black colored ferrous (reduced) iron and red colored ferric (oxidized) iron and
represents a seasonal cycle where the quantity of free oxygen in the ocean
rises and falls, possibly linked to photosynthetic organisms.
Akilia Island, Western Greenland  
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189) Possible earliest fossils. Microstructures from Isua Banded iron
formation, Southerwest Greenland. Because of the simple shape, the biotic
nature of these fossils is not certain.
(Isua BIF) SW Greenland  
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Isua, Greenland  
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Isua, Greenland  
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215) The Carbon-13 to Carbon-12 ratio in 3700+ million year old carbon grains
is consistent with biotic remains, possibly the remains of planktonic
photosynthesizing organisms. These carbon-13 "depleted" grains support the
earlier finding by Mojzsis et al of carbon-13 to carbon-12 ratios that imply
living objects on Greenland earlier than 3850 million years before now.
Isua, Greenland  
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Warrawoona, Western Australia, and, Fig Tree Group, South Africa  
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Warrawoona, northwestern Western Australia and Onverwacht Group, Barberton
Mountain Land, South Africa  
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North Pole, Australia  
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190) Earliest fossils of coccoid {KoKOED} (spherical) bacteria from the
Kromberg Formation, Swaziland System, South Africa.
Kromberg Formation, Swaziland System, South Africa  
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71) Earliest fossil evidence of prokaryote reproduction by budding.

Fossils from Swartkoppie chert, South Africa are oldest evidence of procaryotes
that reproduce by budding and not binary fission.

Budding evolves in prokaryotes. Like binary division, budding is a form of
asexual reproduction. However, with budding a new individual develops from a
certain point of the parent organism. The new individual may separate to exist
independently, or the buds may remain attached, forming colonies. Budding is
characteristic of a few unicellular organisms (certain bacteria, yeasts,
protozoans) but some metazoan animals (certain cnidarian species) regularly
reproduce by budding.
Swartkoppie, South Africa  
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(Sulphur Springs Deposit) Pilbara Craton of Australia  
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66) Earliest acritarch fossils (unicellular microfossils with uncertain
affinity). These acritarchs are also the earliest possible eukaryote fossils.

Organic-walled microfossils of large size (50 micrometres or more) and of
uncertain biological affinities are known as acritarchs. The oldest known
acritarchs are from rocks of the Moodies Group of South Africa that date to
about 3.2 billion years ago, and are almost twice as old as the next known
acritarchs which come from mid-Proterozoic rocks that are about 1.8 billion
years old.

Acritarchs, the name coined by Evitt in 1963 which means "of uncertain origin",
are an artificial group. The group includes any small (most are between 20-150
microns across), organic-walled microfossil which cannot be assigned to a
natural group. They are characterised by varied sculpture, some being spiny and
others smooth. They are believed to have algal affinities, probably the cysts
of planktonic eukaryotic algae. They are valuable Proterozoic and Palaeozoic
biostratigraphic and palaeoenvironmental tools.

Living spherical prokaryotic cells rarely exceed 20 microns in diameter, but
eukaryotic cells are nearly always larger than 60 microns. Although their
precise nature is uncertain, acritarchs appear to be phytoplankton that grew
thick coverings during a resting stage in their life cycle. Some resemble the
resting stage of modern marine algae known as dinoflagellates (known from the
"red tides" that periodically poison fish and other marine animals).

Chitinozoa are large (50-2000 microns) flask-shaped palynomorphs which appear
dark, almost opaque when viewed using a light microscope. They are important
Palaeozoic microfossils as stratigraphic markers.

The oldest known Acritarchs are recorded from shales of Palaeoproterozoic
(1900-1600 Ma) age in the former Soviet Union. They are stratigraphically
useful in the Upper Proterozoic through to the Permian. From Devonian times
onwards the abundance of acritarchs appears to have declined, whether this is a
reflection of their true abundance or the volume of scientific research is
difficult to tell.

Although these acritarch fossils may be from eukaryotes, they may also be from
ancestors of eukaryotes before a nucleus existed which there may be some
genetic support for.
(Moodies Group) South Africa  
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178) Eubacteria Phylum Firmicutes evolves (low G+C {Guanine and Cytosine count}
Gram positive bacteria: botulism, tetanus, anthrax).
  
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288) First endospores. The ability to form endospores evolve in some
firmicutes. An endospore is a tough reduced dry form of a bacterium triggered
by a lack of nutrients that protects the bacterium, and allows it to be revived
after long periods of time. Some 25 million year old spores have been revived.
  
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177) Gender and sex (conjugation) evolve in Escherichia Coli {esRriKEo KOlE}
bacteria. Conjugation is the exchange of DNA (plasmids) by a donor {male}
bacterium through a pilus to a recipient {female} bacterium. This may be the
process that evolves into eukaryote sexual reproduction.

In addition to pili and conjugation, proteins that can cut DNA and other
proteins that can connect two strands of DNA together evolve.

Some protists (cilliates and some algae) reproduce sexually by conjugation.
So perhaps
conjugation is related to the transition from a single circle of DNA to
multiple linear chromosomes in eukaryotes. If conjugation in eukaryotes
descends directly from a proteobacteria then perhaps the ancestor of all
eukaryotes, or certainly those that can conjugate was a proteobacteria.
  
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179) The Phylum Actinobacteria have 5 Orders:
ORDER Acidimicrobiales
ORDER Actinobacteriales
ORDER Coriobacteriales
ORDER Rubrobacteriales
ORDER
Sphaerobacteriales
  
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174) Genetic comparison shows the Eubacteria Phylum, Spirochaetes (Syphilis,
Lyme disease) evolving now.

The spirochaetes (or spirochetes) are a phylum of distinctive bacteria, which
have long, helically coiled cells. They are distinguished by the presence of
flagella running lengthwise between the cell membrane and cell wall, called
axial filaments. These cause a twisting motion which allows the spirochaete to
move around. Most spirochaetes are free-living and anaerobic, but there are
numerous exceptions.

Spirochaetes only have one order:
ORDER Spirochaetales
and 3 families.
  
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175)
  
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217) Chlamydiae have a life-cycle involving two distinct forms. Infection takes
place by means of elementary bodies (EB), which are metabolically inactive.
These are taken up within a cellular vacuole, where they grow into larger
reticulate bodies (RB), which reproduce. Ultimately new elementary bodies are
produced and expelled from the cell.

Verrucomicrobia is a recently described phylum of bacteria. This phylum
contains only a few described species (Verrucomicrobia spinosum, is an example,
the phylum is named after this). The species identified have been isolated from
fresh water and soil environments and human feces. A number of as-yet
uncultivated species have been identified in association with eukaryotic hosts
including extrusive explosive ectosymbionts of protists and endosymbionts of
nematodes residing in their gametes.

Evidence suggests that verrucomicrobia are abundant within the environment, and
important (especially to soil cultures). This phylum is considered to have two
sister phyla Chlamydiae and Lentisphaera.

There are three main species of chlamydiae that infect humans:

* Chlamydia trachomatis, which causes the eye-disease trachoma and the
sexually transmitted infection chlamydia;
* Chlamydophila pneumoniae, which causes a
form of pneumonia;
* Chlamydophila psittaci, which causes psittacosis.


CLASS Chlamydiae
ORDER Chlamydiales

PHYLA Verrucomicrobia
ORDER Verrucomicrobiales
  
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6309)
  
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6310) Verrucomicrobia is a recently described phylum of bacteria. This phylum
contains only a few described species (Verrucomicrobia spinosum, is an example,
the phylum is named after this). The species identified have been isolated from
fresh water and soil environments and human feces. A number of as-yet
uncultivated species have been identified in association with eukaryotic hosts
including extrusive explosive ectosymbionts of protists and endosymbionts of
nematodes residing in their gametes.

Evidence suggests that verrucomicrobia are abundant within the environment, and
important (especially to soil cultures). This phylum is considered to have two
sister phyla Chlamydiae and Lentisphaera.

There are three main species of chlamydiae that infect humans:

* Chlamydia trachomatis, which causes the eye-disease trachoma and the
sexually transmitted infection chlamydia;
* Chlamydophila pneumoniae, which causes a
form of pneumonia;
* Chlamydophila psittaci, which causes psittacosis.


CLASS Chlamydiae
ORDER Chlamydiales

PHYLA Verrucomicrobia
ORDER Verrucomicrobiales
  
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216)
  
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80)
  
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299)
  
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60) Eukaryotic cell. The first cell with a nucleus. The first protist. The
nucleus may develop from the infolding of plasma membrane.

The word "Eukaryote" is from the Greek "eu" which means "true" and "karyon"
which means "kernel", in this case refering to the nucleus.

All cells have several basic features in common: They are all bounded by a
selective barrier, called the plasma membrane. Enclosed by the membrane is a
semifluid, jellylike substance called cytosol, in which organelles and other
components are found. All cells contain chromosomes, which carry genes in the
form of DNA. And all cells have ribosomes, tiny bodies that make proteins
according to instructions from the genes.

There are some difference between prokaryotic and eukaryotic cells:
In prokaryotic
cells the DNA is concentrated in a region that is not membrane enclosed called
the "nucleoid" while in eukaryotic cells most of the DNA is contained in a
nucleus that is bounded by a double membrane. Eukaryotic cells are generally
much larger than prokaryotic cells. Typical bacteria are between 1-5 um in
diameter, while eukaryotic cells are typically 10-100 um in diameter. Unlike
prokaryotic cells, eukaryotic cells have a cytoskeleton. The cytoskeleton
enables eukaryotic cells to change their shape and to surround and engulf other
cells. Eukaryotic cells also have internal structures that prokaryotic cells
lack such as mitochondria and plastids. DNA in prokaryotic cells is usually in
the form of a single cicular chromosome (sometimes with additional small
circles of DNA known as plasmids), while DNA in the nucleus of eukaryotes
contains linear chromosomes (some organelles in eukaryotes also contain DNA,
most mitochondrial and chloroplast DNA is also circular reflecting their
prokaryote origin).

All protists, fungi, animals and plant cells descend from this common
eukaryotic cell ancestor.

Like prokaryotes, this first eukaryote cell is probably haploid, having only a
single unique DNA. Most later eukaryotes will be diploid, having two sets of
DNA.


Other alternative theories are that the nucleus may be a captured bacterium,
virus, or plasmid.

That a eukaryote cell survived the journey from a different star or galaxy
cannot be ruled out.
  
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62)
Northwestern Australia  
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192)
(Bulawaya rock sequence) Zimbabwe  
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214)
  
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65) Eukaryote cells with linear chromosomes (instead of a circular chromosome)
evolve.

Perhaps the first eukaryote descended from one of those prokaryotes with linear
DNA.

Some prokaryotes without a single circular chromosome are: Agrobacterium
tumefaciens (Proteobacteria), Borrellia burgdorferi (Spirochaete), Streptomyces
griseus (Actinobacteria).
Some prokaryotes do not have just one circle of DNA. Brucella
melitensis has 2 circular chromosomes. Agrobacterium tumefaciens has a circular
and a linear chromosome. Streptomyces griseus can have one linear chromosome.
Borrelia burgdorferi contains a linear chromosome and a number of variable
circular and linear plasmids. Chromosomes are linear in eukaryotic nuclei, but
circular in eukaryote organelles except for the mitochondria of most cnidarians
and some other forms.
  
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291) Eukaryote cell evolves two intermediate stages between cell division and
DNA synthesis.

In prokaryotes, DNA synthesis can take place uninterrupted between cell
divisions, but eukaryotes duplicate their DNA exactly once during a discrete
period between cell divisions. This period is called the S (for synthetic)
phase. It is preceded by a period called G1 (meaning "first gap") and followed
by a period called G2, during which nuclear DNA synthesis does not occur.

For the first time, a cell is not constantly synthesizing DNA and then having a
division period (as is the case for all known prokaryotes), but this cell has a
period in between cell division and DNA synthesis where DNA synthesis is not
performed.
  
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72) Mitosis evolves in Eukaryote cells.

Mitosis is the process in eukaryotic cell division in which the chromosomes are
separated and the nucleus divides resulting in two new nuclei, each of which
contains a complete and identical copy of the parental chromosomes. Mitosis is
usually immediately followed by cytokinesis, the division of the cytoplasm.

All eukaryote cells divide using the same general plan. The cell division cycle
contains four stages, G1 ("first gap"), S ("synthesis"), G2 ("second gap"), and
M ("mitotic phase". The first three stages are called "interphase" which
alternates with the mitotic phase. Interphase is a much longer stage that often
accounts for 90% of the cycle. During interphase the cell grows and copies its
chromosomes in preparation for cell division. In the mitotic phase, mitosis,
division of the nucleus is followed by cytokinesis.

Mitosis is thought to have evolved from
prokaryote binary fission. That some proteins involved in prokaryote binary
fission are related to eukaryotic proteins that function in mitosis supports
the idea that mitosis evolved from prokaryote binary fission. Possible
intermediate stages can be seen in some protists. In dinoflagellates,
replicated chromosomes are attached to the nuclear envelope which remains in
one piece during cell division. Microtubules from outside the nucleus pass
through the nucleus inside cytoplasmic tunnels. The nucleus then divides in a
process similar to prokaryote binary fission. In diatoms and yeasts the nuclear
envelope also reamins together during cell division, but inthese eukaryotes the
microtubules form a spindle within the nucleus. Microtubules separate the
chromosomes and the nucleus splits into two nuclei. Finally, in most eukaryotes
including plant and animal cells, the spindle forms outside the nucleus, and
the nuclear envelope breaks down during mitosis. Microtubules separate the
chromosomes, and the nuclear envelope then forms again.
  
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170)
  
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73) Eukaryote sex evolves. Two identical cells fuse (isogamy). First diploid
cell. First zygote. Increase in genetic variety. Haplontic life cycle.

Eukaryotic sexual reproduction, which is initially the fusion of two cells and
their nuclei, probably first occurs in a single cell protist that usually
reproduces asexually by mitosis. Two haploid eukaryote cells (cells with one
set of chromosomes each) merge and then their nuclei merge (karyogamy) to form
the first diploid cell, a cell with two sets of chromosomes, the first zygote.

This fusion of two haploid cells results in the first diploid single-celled
organism, which then may immediately divide (both nucleus and cytoplasm by a
single division) back to two haploid cells.

Because of sex, two cells with different DNA can mix providing more genetic
variety. Having two chromosome sets also provides a backup copy of important
genes (sequences that code for proteins, or nucleic acids) that might be lost
with only a set of single chromosomes.

This first sexual eukaryote cell and its descendants will have a life cycle
with two phases, alternating between haploid and diploid.

Conjugation, the second major kind of sexual phenomenon, which occurs in the
eukaryotes ciliates, involves the fusion of gametic nuclei instead of
independent gamete cells.

"Syngamy" refers to gamete fusion and "karyogamy" to nucleus fusion. In most
cases syngamy is immediately followed by karyogamy, as a result, a fertilized
zygote is produced.

Note that gender (anisogamy) probably evolves later, initially sex is probably
the fusion of two indistinguishable cells (isogamy).

Some protists have diploid nuclei with two chromosomes of each type, such as
those found in the somatic cells of most higher animals and plants, and other
protists have haploid nuclei with unpaired chromosomes, such as those found in
the gametes of higher animals and plants; polyploid nuclei with several sets of
chromosomes also occur in protists. Diploid nuclei in protists may undergo a
process of meiosis to produce haploid nuclei (a reduciton division), but more
commonly both haploid and diploid nuclei divide by mitosis to produce two child
nuclei like the original parent cell.

Some of the genes related to the process of meiosis occur in Giardia, one of
the most primitive living protists, which is evidence that meiosis may have
evolved before the evolution of all known eukaryotes.

Now, two cells with different DNA can mix providing more chance of variety and
mutation. Two chromosome sets provides a backup copy of important genes
(sequences that code for proteins, or nucleic acids) that might be lost with
only a set of single chromosomes.

This first sexual eukaryote cell and its descendants will have two phases, a
gamophase (haploid until syngamy becoming diploid), and a zygophase (from
diploid until meiosis becoming haploid).

For sexual species there are 3 basic life cycles:
1) Haploid (Haplontic) life cycle:
(zygotic meiosis) Life as haploid cells, cell division immediately after
creation of zygote from fusion. (All fungi, Some green algae, Many protozoa)
2) Diploid
(Diplontic) life cycle: (gametic meiosis) Instead of immediate cell division,
zygote reproduces by mitosis. Haploid gametes never copy by mitosis. (animals,
some brown algae)
3) Haplodiploid (Haplodiplontic, Diplohaplontic, Diplobiontic) life
cycle: (sporic meiosis) Diploid cell (sporocyte) meiosis results in two haploid
sporophytes (gamonts), not two haploid gametes. These haploid cells then
differentiate? or mitosis? to form haploid gametes. Haplodiplontic organisms
have alternation of generations, one generation involves diploid
spore-producing single or multicellular sporophytes (makes spores) and the
other generation involves haploid single or multicellular gamete-producing
multicellular gametophytes (makes gametes). (Plants and many algae)

These first sexual cells are haplontic, with zygotic meiosis; they reproduce
asexually through mitosis as haploid cells, fusing to a diploid cell without
mitosis, then dividing back into haploid cells.

An important evolutionary step evolves here in that now two cells can
completely merge into one cell. This merge not only includes their nuclei, but
also their cytoplasm (although the DNA do not merge). Before now, as far as
has ever been observed, no two cells have ever completely merged, although,
through conjugation some prokaryotes have been observed to exchange DNA.

This is the beginning of the label "gamete" for haploid cells that can merge to
form a diploid zygote. In addition, the label "gametocyte" or "gamont" is any
polyploid cell that divides (meiosis) into haploid gamete cells which can merge
to form a zygote.


The alternation of meiosis and fertilization is common to all organisms that
reproduce sexually, but there are three main different types of life cycles;
haplontic, haplodiplontic, and diplontic. Haplontic organisms are predominantly
haploid; mitosis does not occur in the diploid phase. In Haplodiplontic
organisms, mitosis occurs in both the haploid and diploid phases. Diplontic
organisms are predominantly diploid; mitosis does not occur in the haploid
phase. Most fungi and some protists including some algae have a "haplontic"
life cycle where after gametes fuse and form a diploid zygote, meiosis occurs
without a multicellular diploid offspring developing. Meiosis produces not
gametes but haploid cells that then divide by mitosis and give rise to either
unicellular descendents or a haploid multicellular adult organism. The haploid
oganism then carries out further mitoses producing cells that develop into
gametes. The only diplod stage found in these species is the singe-celled
zygote. Plants and some algae have a second type of lifestyle called
"haplodiplontic" or "alternation of generations". This type includes both
diploid and haploid stages that are multicellular. The multicellular diploid
stage is called the "sporophyte". Meiosis in the sporophyte produces haploid
cells called spores. Unlike a gamete, a haploid spore doesn't fuse with another
cell but divides mitotically, generating a multicellular haploid stage called
the gametophyte. Cells of the gametophyte give rise to gametes by mitosis.
Fusion of two haploid gametes at fertilizations results in a diploid zygote,
which develops into the next sporophyte generation. A third type of sexual life
cycle, "diplontic", occurs in animals in which gametes are the only haploid
cells. Meiosis occurs in germ cells producing haploid gametes that no other
cell division prior to fertilization. After fertilization the diploid zygote
divides by mitosis producing a multicellular organism that is diploid.
  
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206) Meiosis evolves (one-step meiosis: 2 haploid cells or two pronuclei fuse
into a diploid cell and a divide into 2 haploid cells).

Meiosis, which looks similar to mitosis, is the process of cell division in
sexually reproducing organisms that reduces the number of chromosomes in
reproductive cells from diploid to haploid, leading to the production of
gametes in animals and spores in plants.

Most protists divide by two-step meiosis, and meiosis with only one cell
division is rare. Some view one-divisional meiosis as having an independent and
secondary origin while others view one-step meiosis as the primitive meiotic
process.

Without the reduction back to haploid, genomes would double in size with every
generation.

Mitosis and one-step meiosis are the same with the only exception that: in
meiosis two haploid cells join (or 2 pronuclei fuse) before cell division, but
in mitosis the DNA is duplicated internally in the nucleus before cell
division.

Meiosis can be one step (one fusion and then one cell division) or two step
(fusion, DNA duplication and then two divisions). Probably one step meiosis
evolved first and two step meiosis later. The Protists Pyrsonympha and
Dinenympha have up to a four step meiosis.

Because meiosis is similar and complex in detail in all species that do
meiosis, people think that meiosis only evolved once, and was inherited by all
species that do meiosis.
  
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210)
  
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296)
  
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298) Sex between a flagellated gamete and an unflagellated gamete evolves in
protists (oogamy {OoGomE}, a form of anisogamy).
  
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300) Only a few species exhibit this property (e.g. the Oxymonad Notilla,
Diatoms, Dasicladales {Acetabularia}, in many foraminiferans, and in
gregarines).

Gamontogamy may have evolved into two-step meiosis.

The vast majority of eukaryotes living now that reproduce sexually fuse haploid
cells. All "gametes" are haploid cells that can merge, diploid cells that can
merge are gamonts. Gamonts (Meiocytes) are cells that produce gametes.

In theory this should be very similar if not exactly like haploid cell fusion,
so perhaps this is not a major evolutionary step.
  
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295) Two-step meiosis (diploid DNA copies and then the cell divides twice into
four haploid cells).

Meiosis and mitosis are similar in being nucleus and cell division, but are
different.
Differences between meiosis and mitosis:
1) At least one crossover per
homologous pair happens in 2 step meiosis but crossover usually does not happen
in mitosis. (explain crossover)
2) Two step meiosis involves cell divisions that happen
one after the other, where the cell division of mitosis only happens after one
DNA duplication (there are never 2 mitosis divisions together without a DNA
duplication between them to my knowledge).

The cell division in two step meiosis that involves a separation of sister
chromatids (not homologous chromosome pairs) is basically identical to mitosis.
For two step meiosis, this is the second nucleus and cell division.

Later multistep meiosis evolves, where there may be as many as 4 divisions (for
example in the protists Pyrsonympha and Dinenympha).

(Determine if it can be said that meiosis is simply a division after the fusion
of two nuclei while mitosis is a division after an internucleus DNA copy.
Clearly the duplication of two complete nuclei within a single Eukaryote cell
must include the inte r-nucleus copying of DNA - and is probably similar to a
typical prokaryote cell division. This process just goes further in duplicating
the nuclear membrane too. Then the division after the fusion of two nuclei must
be basically the same as a mitosis division. So really, in this view, the
unique processes are: DNA, nucleus, and/or cell copy, nucleus and/or cell
fusion, nucleus and/or cell division.)
  
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171) The Eubacteria phylum "Deinococcus-Thermus" evoles now (includes Thermus
Aquaticus {used in PCR}, Deinococcus radiodurans {can survive long exposure to
radiation}).

The Deinococcus-Thermus are a small group of bacteria comprised of cocci highly
resistant to environmental hazards. There are two main groups. The
Deinococcales include a single genus, Deinococcus, with several species that
are resistant to radiation; they have become famous for their ability to eat
nuclear waste and other toxic materials, survive in the vacuum of space and
survive extremes of heat and cold. The Thermales include several genera
resistant to heat. Thermus aquaticus was important in the development of the
polymerase chain reaction where repeated cycles of heating DNA to near boiling
make it advantageous to use a thermo-stable DNA polymerase enzyme. These
bacteria have thick cell walls that give them gram-positive stains, but they
include a second membrane and so are closer in structure to those of
gram-negative bacteria.

PHYLUM Deinococcus-Thermus
CLASS Deinococci
ORDER Deinococcales
ORDER Thermales
  
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172)
  
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315) PHYLUM Chloroflexi
CLASS Chloroflexi
CLASS Thermomicrobia
  
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52) End of the Archean and start of the Proterozoic {PrOTReZOiK or ProTReZOiK}
Eon.

The Proterozoic spans from 2,500 to 542 million years ago, and represents 42%
of Earth's history.
  
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56) Banded Iron Formation starts to appear in many places.
  
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59)
  
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316) (Determine if this is just an example of a cell forming a spore. Clearly
forming a spore can be viewed as cell differentiation. But clearly, a cell
changes form in small ways all the time.)

Which cell differentiation is first is unknown, between cells that form spores,
or cysts, and the cell differentiation that is observed in cyanobacterial
filamentous cells.

Heterocysts are specialized nitrogen-fixing cells formed by some filamentous
cyanobacteria, such as Nostoc punctiforme and Anabaena sperica, during nitrogen
starvation. They fix nitrogen from dinitrogen (N2) in the air using the enzyme
nitrogenase, in order to provide the cells in the filament with nitrogen for
biosynthesis. Nitrogenase is inactivated by oxygen, so the heterocyst must
create a microanaerobic environment. The heterocysts' unique structure and
physiology requires a global change in gene expression. For example,
heterocysts:

* produce three additional cell walls, including one of glycolipid that
forms a hydrophobic barrier to oxygen
* produce nitrogenase and other proteins
involved in nitrogen fixation
* degrade photosystem II, which produces oxygen
* up
regulate glycolytic enzymes, which use up oxygen and provide energy for
nitrogenase
* produce proteins that scavenge any remaining oxygen

Cyanobacteria usually obtain a fixed carbon (carbohydrate) by photosynthesis.
The lack of photosystem II prevents heterocysts from photosynthesising, so the
vegetative cells provide them with carbohydrates, which is thought to be
sucrose. The fixed carbon and nitrogen sources are exchanged though channels
between the cells in the filament. Heterocysts maintain photosystem I, allowing
them to generate ATP by cyclic photophosphorylation.

Single heterocysts develop about every 9-15 cells, producing a one-dimensional
pattern along the filament. The interval between heterocysts remains
approximately constant even though the cells in the filament are dividing. The
bacterial filament can be seen as a multicellular organism with two distinct
yet interdependent cell types. Such behaviour is highly unusual in prokaryotes
and may have been the first example of multicellular patterning in evolution.
Once a heterocyst has formed, it cannot revert to a vegetative cell, so this
differentiation can be seen as a form of apoptosis. Certain heterocyst-forming
bacteria can differentiate into spore-like cells called akinetes or motile
cells called hormogonia, making them the most phenotyptically versatile of all
prokaryotes.

The mechanism of controlling heterocysts is thought to involve the diffusion of
an inhibitor of differentiation called PatS. Heterocyst formation is inhibited
in the presence of a fixed nitrogen source, such as ammonium or nitrate. The
bacteria may also enter a symbiotic relationship with certain plants. In such a
relationship, the bacteria do not respond to the availability of nitrogen, but
to signals produced by the plant. Up to 60% of the cells can become
heterocysts, providing fixed nitrogen to the plant in return for fixed carbon.

The cyanobacteria that form heterocysts are divided into the orders Nostocales
and Stigonematales, which form simple and branching filaments respectively.
Together they form a monophyletic group, with very low genetic variability.
  
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322) Nitrogen fixation. Cells can make nitrogen compounds like ammonia from
Nitrogen gas.

Without bacteria that convert N2 into nitrogen compounds, the supply of
nitrogen necessary for much of life would be seriously limited and would
drastically slow evolution on earth.

Nitrogen fixation is the process by which
nitrogen is taken from its relatively inert molecular form (N2) in the
atmosphere and converted into nitrogen compounds useful for other chemical
processes (such as, notably, ammonia, nitrate and nitrogen dioxide).

Nitrogen fixation is performed naturally by a number of different prokaryotes,
including bacteria, and actinobacteria certain types of anaerobic bacteria.
Many higher plants, and some animals (termites), have formed associations with
these microorganisms.

The best-known are legumes (such as clover, beans, alfalfa and peanuts,) which
contain symbiotic bacteria called rhizobia within nodules in their root
systems, producing nitrogen compounds that help the plant to grow and compete
with other plants. When the plant dies, the nitrogen helps to fertilize the
soil. The great majority of legumes have this association, but a few genera
(e.g., Styphnolobium) do not.
West Africa  
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290)
  
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198)
  
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199) Eukaryote Golgi Apparatus evolves (packages proteins and lipids into
vesicles for delivery to targeted destinations).

A vesicle is a closed structure, found only in eukaryotic cells, that is
completely surrounded by a membrane but, unlike a vacuole, contains material
that is not in the liquid state.

(Is this the only form of cellular digestion?)
  
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47) Evidence of free oxygen accumulating in the air of Earth for the first
time, most recent uraninite {YRANninIT}, a mineral that cannot exist for much
time if exposed to oxygen.
  
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48) The oldest "Red Beds", iron oxide formed on land, begin here, and are also
evidence of more free oxygen in the air of Earth.
  
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150)
  
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63) A parasitic bacterium, closely related to Rickettsia prowazekii, an aerobic
proteobacteria, is engulfed by an early eukaryote cell and over time a
symbiotic relationship evolves, where the Rickettsia forms the mitochondria.

Mitochondria are membrane-bound organelle found in the cytoplasm of almost all
eukaryotic cells where cellular respiration occurs and most of the ATP in a
eukaryote cell is produced. Mitochondria are typically round to oval in shape
and range in size from 0.5 to 10 μm. The number of mitochondria per cell
varies widely; for example, in humans, erythrocytes (red blood cells) do not
contain any mitochondria, whereas liver cells and muscle cells may contain
hundreds or even thousands. Mitochondria are unlike other cellular organelles
in that they have two distinct membranes and a unique genome and reproduce by
binary fission; these features indicate that mitochondria share an evolutionary
past with prokaryotes.

In eukaryotes the mitochondria perform the Citric Acid Cycle and Oxidative
phosphorylation using oxygen to breakdown pyruvagte from glycolysis into CO2
and H2O, and provide up 36 ATP molecules.

This presumes that all known living eukaryotes descend from a eukaryote that
had mitochondria, and that eukaryotes without mitochondria, like the
metamonada, lost their mitochondria secondarily.
  
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99)
  
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61)
(Banded Iron Formation) Michigan, USA  
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151)
  
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46) End of the Banded Iron Formation.
  
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6279) Earliest possible multicellular brown algae (and Stramenopiles) fossil.
These fossils help support a limit for multicellular algal fossil (metaphyta)
of at least 1700 million years ago.

If eukaryote these would be the earliest eukaryote fossils with both
filamentous multicellularity and cell differentiation and also the earliest
algae fossil with leaf structures.

Knoll et al write in 2006 that: "Examination of Tuanshanzi structures in
outcrop by one of us (A. H. Knoll) suggests that the features in question can
alternatively be interpreted as rare, fortuitously shaped fragments deposited
among many irregular mat shards.".
(Tuanshanzi Formation) Jixian Area, North China  
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152)
  
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197)
  
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202) Ribosomal RNA shows the Protist Phylum Amoebozoa (also called
Ramicristates) which includes amoeba and slime molds evolving now.

The Amoebozoa are a major group of amoeboid protozoa, including the majority
that move by means of internal cytoplasmic flow. Their pseudopodia are
characteristically blunt and finger-like, called lobopodia. Most are
unicellular, and are common in soils and aquatic habitats, with some found as
symbiotes of other organisms, including several pathogens. The Amoebozoa also
include the slime moulds, multinucleate or multicellular forms that produce
spores and are usually visible to the unaided eye.

Mycetozoa are the slime molds.
4. Plasmodial Slime Molds
a. Plasmodial
slime molds exist as a plasmodium. (the earlier evolved acrasid cellular slime
molds exist as individual amoeboid cells.)
b. This diploid multinucleated
cytoplasmic mass creeps along, phagocytizing decaying plant material.
c.
Fan-shaped plasmodium contains tubules of concentrated cytoplasm in which
liquefied cytoplasm streams.
d. Under unfavorable environmental conditions
(e.g., drought), the plasmodium develops many sporangia
that produce
spores by meiosis.
e. When mature, spores are released and survive until
more favorable environmental conditions return;
then each releases a
haploid flagellated cell or an amoeboid cell.
f. Two flagellated or
amoeboid cells fuse to form diploid zygote that produces a multi-nucleated
plasmodium.

Nuclear division in giant amoebas (Peolobiont/Amoebozoa) is neither mitosis nor
binary fission, but incorporates aspects of both (Fig. 3-7). Chromosomes are
attached permanently to the nuclear membrane by their centromeres (MTOCs,
microtubule organizing centers), and the nuclear membrane remains intact
throughout division. After DNA duplication produces two chromatids, the point
of attachment, the MTOC duplicates or divides, and microtubules are assembled
between the two resulting MTOCs. Elongating microtubules form something akin to
a spindle within the nuclear membrane that pushes the daughter chromosomes
apart and elongate the membrane-bounded nucleus until it blebs in half in
something akin to binary fission. Simple assembly of microtubules accomplishes
the separation of daughter genomes in this simple nuclear division. In typical
eukaryotic mitosis, the separation of daughter chromosomes is accomplished by a
dual action, the disassembly of spindle fibers connecting the daughter
chromosome to the polar MTOC, and assembly of spindle fibers running pole to
pole.

Thomas Cavalier-Smith and Ema E. -Y. Chao write: "Amoebozoa are a key protozoan
phylum because of the possibility that they are ancestrally uniciliate and
unicentriolar (Cavalier-Smith 2000a,b); present data on the DHFR-TS gene fusion
leaves open the possibility that they might be the earliest-diverging
eukaryotes (Stechmann and Cavalier-Smith 2002), but they may be evolutionarily
closer to bikonts or even opisthokonts. Amoebozoa comprise two subphyla
(Cavalier-Smith 1998a): Lobosa, classical aerobic amoebae with broad ("lobose")
pseudopods (including the testate Arcellinida), and Conosa (slime molds
{Mycetozoa, e.g., Dictyostelium} and amitochondrial-often
uniciliate-archamaebae {entamoebae, mastigamoebae}). Contrary to early analyses
(Sogin 1991; Cavalier-Smith 1993a), there is no reason to regard Amoebozoa as
polyphyletic; the defects of those classical uncorrected rRNA trees are shown
by trees using 123 proteins that robustly establish the monophyly of both
Archamoebae and Conosa (Bapteste et al. 2002). Unless the tree's root is within
Conosa, Dictyostelium and Entamoeba must have evolved independently from
aerobic flagellates by ciliary losses. A recent mitochondrial gene tree based
on concatenating six different proteins grouped Dictyostelium with Physarum
(99% support) and both Mycetozoa as sisters to Acanthamoeba (99% support), thus
providing strong evidence for the monophyly of Mycetozoa and the grouping of
Lobosa and Conosa as Amoebozoa (Forget et al. 2002)-the same tree also strongly
supports the idea based on morphology that Allomyces should be excluded from
Chytridiomycetes (in the separate class Allomycetes) and is phylogenetically
closer to zygomycetes and higher fungi (Cavalier-Smith 1998a, 2000c).
Furthermore, the derived gene fusion between two cytochrome oxidase genes, coxI
and coxII (Lang et al. 1999), strongly supports the holophyly of Mycetozoa.
Since Archamoebae secondarily lost mitochondria, the root cannot lie among them
either-although anaerobiosis in Archamoebae is derived, it is unjustified to
conclude from this that their simple ciliary root organization, which was a key
reason for considering them early eukaryotes (Cavalier-Smith 1991c), is also
secondarily derived (Edgcomb et al. 2002). Thus the root of the eukaryote tree
cannot lie within the Conosa.

As Mycetozoa and Archamoebae have very long-branch rRNA sequences, Conosa were
excluded from the analysis in Fig. 1, which includes only Lobosa. Although the
monophyly of Acanthamoebida (99%) and of Euamoebida (85%) is well supported,
the basal branching of the Lobosa is so poorly resolved that the monophyly of
Lobosa might appear open to question. The four lobosan lineages apparently
diverged early. However, in the 279- and 227-species trees, which included
Conosa, anaeromonads did not intrude into the Amoebozoa as they do in Fig. 1,
and Amoebozoa were monophyletic (low support) except for the exclusion of M.
invertens. M. invertens is another wandering branch, which in some taxon
sample/methods groups very weakly with other Amoebozoa, but more often ends up
in a different place in each tree! We concur with the judgment of Milyutina et
al. (2001)Edgcomb et al. (2002) that it should not be regarded as a pelobiont
or Archamoeba, but as a lobosan that independently became an anaerobe with
degenerate mitochondria. Its tendency to drift around the tree, coupled with
its short branch, suggests that it may be a particularly early-diverging
amoebozoan lineage. If so, its unicentriolar condition would give added support
to the idea that Amoebozoa are ancestrally uniciliate, if it could be shown
that Amoebozoa are either holophyletic or not at the base of the tree.

Most, if not all, amoebae evolved from amoeboid zooflagellates by multiple
ciliary losses (Cavalier-Smith 2000a). As the uniciliate condition is
widespread within Amoebozoa (Cavalier-Smith 2000a, 2002b), it may be their
ancestral condition; if so, ordinary nonciliate amoebozoan amoebae arose
several times independently. Evolution of amoebae from zooflagellates by
ciliary loss also occurred separately in Choanozoa to produce Nuclearia and in
several bikont groups, notably Percolozoa (heterolobosean amoebae, e.g.,
Vahlkampfia) and Cercozoa. However, we cannot currently exclude the possibility
that the eukaryote tree is rooted within the lobosan Amoebozoa, in which case
one of its nonciliate lineages (Euamoebida or Vanellidae) might be primitively
nonciliate and the earliest-diverging eukaryotic lineage. However, as the idea
that the nucleus and a single centriole and cilium coevolved in the ancestral
eukaryote (Cavalier-Smith 1987a) retains its theoretical merits, we think it
more likely that all Amoebozoa are derived from a uniciliate ancestor and that
crown Amoebozoa are a clade.".

Amoebozoa vary greatly in size. Many are only 10-20 μm in size, but they also
include many of the larger protozoa. The famous species Amoeba proteus may
reach 800 μm in length, and partly on account of its size is often studied as
a representative cell. Multinucleate amoebae like Chaos and Pelomyxa may be
several millimetres in length, and some slime moulds cover several square feet.


The cell is typically divided into a granular central mass, called endoplasm,
and a clear outer layer, called ectoplasm. During locomotion the endoplasm
flows forwards and the ectoplasm runs backwards along the outside of the cell.
Many amoebae move with a definite anterior and posterior; in essence the cell
functions as a single pseudopod. They usually produce numerous clear
projections called subpseudopodia (or determinate pseudopodia), which have a
defined length and are not directly involved in locomotion.

Other amoebozoans may form multiple indeterminate pseudopodia, which are more
or less tubular and are mostly filled with granular endoplasm. The cell mass
flows into a leading pseudopod, and the others ultimately retract unless it
changes direction. Subpseudopodia are usually absent. In addition to a few
naked forms like Amoeba and Chaos, this includes most amoebae that produce
shells. These may be composed of organic materials, as in Arcella, or of
collected particles cemented together, as in Difflugia, with a single opening
through which the pseudopodia emerge.

The primary mode of nutrition is by phagocytosis: the cell surrounds potential
food particles, sealing them into vacuoles where the may be digested and
absorbed. Some amoebae have a posterior bulb called a uroid, which may serve to
accumulate waste, periodically detaching from the rest of the cell. When food
is scarce, most species can form cysts, which may be carried aerially and
introduce them to new environments. In slime moulds, these structures are
called spores, and form on stalked structures called fruiting bodies or
sporangia.

Most Amoebozoa lack flagella and more generally do not form
microtubule-supported structures except during mitosis. However, flagella occur
among the pelobionts, and many slime moulds produce biflagellate gametes. The
flagella is generally anchored by a cone of microtubules, suggesting a close
relationship to the opisthokonts. The mitochondria characteristically have
branching tubular cristae, but have been lost among pelobionts and the
parasitic entamoebids, collectively referred to as archamoebae based on the
earlier assumption that the absence was primitive.

Traditionally all amoebae with lobose pseudopods were treated together as the
Lobosea, placed with other amoeboids in the phylum Sarcodina or Rhizopoda, but
these were considered to be unnatural groups. Structural and genetic studies
identified several independent groups: the percolozoans, pelobionts, and
entamoebids. In phylogenies based on rRNA their representatives were separate
from other amoebae, and appeared to diverge near the base of eukaryotic
evolution, as did most slime molds.

However, revised trees by Cavalier-Smith and Chao in 1996 suggested that the
remaining lobosans do form a monophyletic group, and that the archamoebae and
Mycetozoa are closely related to it, although the percolozoans are not.
Subsequently they emended (to improve by editing) the older phylum Amoebozoa to
refer to this supergroup. Studies based on other genes have provided strong
support for the unity of this group. Patterson treated most with the testate
filose amoebae as the ramicristates, based on mitochondrial similarities, but
the latter are now removed to the Cercozoa.

Amoebae are difficult to classify, and relationships within the phylum remain
confused. Originally it was divided into the subphyla Conosa, comprising the
archamoebae and Mycetozoa, and Lobosa, including the more typical lobose
amoebae. Molecular phylogenies provide some support for this division if the
Lobosa are understood to be paraphyletic. They also suggest the morphological
families of naked lobosans may correspond at least partly to natural groups:

* Leptomyxida
* Amoebidae
* Hartmannellidae
* Paramoebidae
* Vannellidae
* Vexilliferidae
* Acanthamoebidae
* Stereomyxidae

However, many amoebae have not yet been studied via molecular techniques,
including all those that produce shells (Arcellinida).

PHYLUM Amoebozoa (Lühe, 1913 emend.) Cavalier-Smith, 1998
CLASS
Breviatea
CLASS Variosea
CLASS Phalansterea (T. Cavalier-Smith,
2000)
SUBPHYLUM Lobosa (Carpenter, 1861) Cavalier-Smith, 1997 (lobose
amoebas)
CLASS Amoebaea
CLASS Testacealobosea (includes shelled lobosid
amebas {testate amoebas})
CLASS Holomastigea T. Cavalier-Smith, 1997
("1996-1997")
SUBPHYLUM Conosa (Cavalier-Smith, 1998)
INTRAPHYLUM
Mycetozoa (De Bary, 1859) Cavalier-Smith, 1998 (Slime Molds)
SUPERCLASS Eumyxa
(Cavalier-Smith, 1993) Cavalier-Smith, 1998
CLASS Protostelea (C.J.
Alexopoulos & C.W. Mims, 1979 orthog. emend.)
CLASS Myxogastrea (E.M.
Fries, 1829 stat. nov. J. Feltgen, 1889 orthog. emend.) (plasmodial slime
molds)
SUPERCLASS Dictyostelia (Lister, 1909) Cavalier-Smith, 1998
CLASS
Dictyostelea™ (D.L. Hawksworth et al., 1983, orthog. emend.)
INTRAPHYLUM
Archamoebae (Cavalier-Smith, 1983) Cavalier-Smith, 1998
CLASS Pelobiontea
(F.C. Page, 1976 stat. nov. T. Cavalier-Smith, 1981)
CLASS Entamoebea
(T. Cavalier-Smith, 1991)

SUBPHYLUM Lobosa


SUBPHYLUM Conosa
The Conosea unifies amoebae which usually possess flagellate stages
or are amoeboflagellates. This clade consists of two relatively solid groups
� the Mycetozoa and Archamoebae, grouped by Cavalier-Smith (1998) in the
taxon Conosa, as well as a number of independent lineages, including two
flagellates � Phalansterium (Cavalier-Smith et al. 2004) and Multicilia
(Nikolaev et al. 2004), and two gymnamoebae � Gephyramoeba and Filamoeba
(Amaral Zettler et al. 2000). Because of large variations of the substitution
rates in SSU rRNA genes within this clade, its internal relationships are not
resolved yet.

The Mycetozoa comprises two distinct groups of "slime molds", the Myxogastria
and Protostelia (Dykstra and Keller 2000). This is a well-defined group of
protists, characterized by the ability to form so-called "fruiting bodies". In
some lineages of Mycetozoa the fruiting body is raised over the substratum on a
distinct stalk. Both groups possess complex life cycles including an
aggregation of cells, however the essential difference between them is that in
Protostelia, only a pseudoplasmodium is formed (without fusion of the cells
constituting the aggregate), while in Myxogastria a true plasmodium is formed
(the cells completely fuse, forming a single organism) (Olive 1975; Dykstra and
Keller 2000). The monophyly of Mycetozoa was proposed based on elongation
factor 1-alpha gene sequences (Baldauf and Doolittle 1997) but it is not always
recovered in SSU rRNA trees (Cavalier-Smith et al. 2004; Nikolaev et al.
2004).

The Archamoebae comprise amoeboid and amoeboflagellate protists characterized
by a secondary absence of mitochondria (mostly due to parasitism or life in
anoxic environments). This group includes the free-living genera Mastigamoeba,
Mastigella, and Pelomyxa (the pelobionts) and the parasitic genera Entamoeba
and Endolimax (the entamoebids). The consistent grouping of all these
amitochondriate amoeboid organisms in both SSU rRNA and actin gene phylogenies
(Fahrni et al. 2003) suggests a single loss of the mitochondria during the
evolution of Amoebozoa.

CLASS Amoebaea
ORDER Euamoebida Lepsi, 1960
FAMILY Amoebidae (Ehrenberg 1838)
The
Amoebidae are a family of amoebozoa, including naked amoebae that produce
multiple pseudopodia of indeterminate length. These are roughly cylindrical in
form, with a central stream of granular endoplasm, and do not have
subpseudopodia. During locomotion one pseudopod typically becomes dominant, and
the others are retracted as the body flows into it. In some cases the cell
moves by "walking", with the relatively permanent pseudopodia serving as limbs.


The most important genera are Amoeba and Chaos, which are set apart from the
others by longitudinal ridges. They group together on molecular trees,
suggesting the Amoebidae are a natural group. Shelled amoebozoans have not been
studied molecularly but produce very similar pseudopodia, so although they are
traditionally classified separately they may be closely related to this group.


GENUS Amoeba (Bery de St. Vincent 1822)
Amoeba (also spelled ameba) is a genus
of protozoa that moves by means of temporary projections called pseudopods, and
is well-known as a representative unicellular organism. The word amoeba is
variously used to refer to it and its close relatives, now grouped as the
Amoebozoa, or to all protozoa that move using pseudopods, otherwise termed
amoeboids.

Amoeba itself is found in freshwater, typically on decaying vegetation from
streams, but is not especially common in nature. However, because of the ease
with which they may be obtained and kept in the lab, they are common objects of
study, both as representative protozoa and to demonstrate cell structure and
function. The cells have several lobose pseudopods, with one large tubular
pseudopod at the anterior and several secondary ones branching to the sides.
The most famous species, Amoeba proteus, is 700-800 μm in length, but many
others are much smaller. Each has a single nucleus, and a simple contractile
vacuole which maintains its osmotic pressure, as its most recognizable
features.

Early naturalists referred to Amoeba as the Proteus animalcule, after a Greek
god who could change his shape. The name "amibe" was given to it by Bery St.
Vincent, from the Greek amoibe, meaning change.

A good method of collecting amoeba is to lower a jar upside down until it is
just above the sediment surface. Then one should slowly let the air escape so
the top layer will be sucked into the jar. Deeper sediment should not be
allowed to get sucked in. It is possible to slowly move the jar when tilting it
to collect from a larger area. If no amoeba are found, one can try introducing
some rice grains into the jar and waiting for them to start to rot. The
bacteria eating the rice will be eaten by the amoeba, thus increasing the
population and making them easier to find.

Family Hartmannellidae (Volkonsky 1931)
The Hartmannellidae are a common family of
amoebozoa, usually found in soils. When active they tend to be roughly
cylindrical in shape, with a single leading pseudopod and no subpseudopodia.
This form somewhat resembles a slug, and as such they are also called limax
amoebae. Trees based on rRNA show the Hartmannellidae are paraphyletic to the
Amoebidae and Leptomyxida, which may adopt similar forms.

FAMILY Vannellidae (Bovee 1970)
The Vannellidae are a distinctive family of
amoebozoa. During locomotion they tend to be flattened and fan-shaped, although
some are long and narrow, and have a prominent clear margin at the anterior. In
most amoebae, the endoplasm glides forwards through the center of the cell, but
in vannellids the cell undergoes a sort of rolling motion, with the outer
membrane sliding around like a tank tread.

These amoebae are usually 10-40 μm in size, but some are smaller or larger.
The most common genus is Vannella, found mainly in soils, but also in
freshwater and marine habitats. Trees based on rRNA support the monophyly of
the family.

SUBPHYLUM Conosa Cavalier-Smith, 1998
INTRAPHYLUM Archamoebae (Cavalier-Smith,
1983) Cavalier-Smith, 1998
CLASS Pelobiontea F.C. Page, 1976 stat. nov. T.
Cavalier-Smith, 1981
ORDER Pelobiontida (Page 1976)
The pelobionts are a small group
of amoebozoa. The most notable member is Pelomyxa, a giant amoeba with multiple
nuclei and inconspicuous non-motile flagella. The other genera, called
mastigamoebae, are often uninucleate, have a single anterior flagellum used in
swimming, and produce numerous determinate pseudopodia.

Pelobionts are closely related to the entamoebids and like them have no
mitochondria; in addition, pelobionts also do not have dictyosomes. At one
point these absences were considered primitive. However, molecular trees place
the two groups with other lobose amoebae in the phylum Amoebozoa, so these are
secondary losses.

SUBPHYLUM Conosa Cavalier-Smith, 1998
INTRAPHYLUM Archamoebae (Cavalier-Smith,
1983) Cavalier-Smith, 1998
CLASS Entamoebea T. Cavalier-Smith, 1991
The entamoebids
or entamoebae are a group of amoebozoa found as internal parasites or
commensals of animals. The cells are uninucleate small, typically 10-100 μm
across, and usually have a single lobose pseudopod taking the form of a clear
anterior bulge. There are two major genera, Entamoeba and Endolimax. They
include several species that are pathogenic in humans, most notably Entamoeba
histolytica, which causes amoebic dysentery.

Entamoebids lack mitochondria. This is a secondary loss, possibly associated
with their parasitic life-cycle. Studies show they are close relatives of the
pelobionts, another group of amitochondriate amoebae, but unlike them
entamoebids retain dictyosomes. Both groups are now placed alongside other
lobose amoebae in the phylum Amoebozoa.

Studying Entamoeba invadens, David Biron of the Weizmann Institute of Science
and coworkers found that about one third of the cells are unable to separate
unaided and recruit a neighboring amoeba (dubbed the "midwife") to complete the
fission. He writes:

"When an amoeba divides, the two daughter cells stay attached by a tubular
tether which remains intact unless mechanically severed. If called upon, the
neighbouring amoeba midwife travels up to 200 μm towards the dividing amoeba,
usually advancing in a straight trajectory with an average velocity of about
0.5 μm/s. The midwife then proceeds to rupture the connection, after which all
three amoebae move on."

They also reported a similar behavior in Dictyostelium.

Entamoeba coli is a non-pathogenic species of entamoebid that is important
clinically in humans only because it can be confused with Entamoeba
histolytica, which is pathogenic, on microscopic examination of stained stool
specimens. A simple finding of Entamoeba coli trophozoites or cysts in a stool
specimen requires no treatment.

Entamoeba histolytica is an anaerobic parasitic protozoan, classified as an
entamoebid. It infects predominantly humans and other primates. Diverse mammals
such as dogs and cats can become infected but usually do not shed cysts (the
environmental survival form of the organism) with their feces, thus do not
contribute significantly to transmission. The active (trophozoite) stage exists
only in the host and in fresh feces; cysts survive outside the host in water
and soils and on foods, especially under moist conditions on the latter. When
swallowed they cause infections by excysting (to the trophozoite stage) in the
digestive tract.

Endolimax nana, a small entamoebid that is a commensal of the human intestine,
causes no known disease. It is most significant in medicine because it can
provide false positives for other tests, such as for the related species
Entamoeba histolytica which causes amoebic dysentery, and because its presence
indicates that the host once consumed feces. It forms cysts with four nuclei
which excyst in the body and become trophozoites. Endolimax nana nuclei have a
large endosome somewhat off-center and small amounts of visible chromatin or
none at all.

Actinopod reproduction may involve binary fission or the formation of swarmer
cells, and sexual processes occur in some groups. Their mitochondrial cristae
are usually tubular, but in some groups there are vesicular or flattened,
plate-like cristae.

(Are amoeba haplodiploid?)
  
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173) Earliest probable fungi microfossils, "Tappania plana". If true this would
be the oldest eukaryote fossil.

Neoproterozoic fossils of Tappania from the Neoproterozoic (800-900 MY) have
fused branches, a process found in higher fungi.
(Roper Group) Northern Australia  
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220) Protists Opisthokonts (ancestor of Fungi, Choanoflagellates and Animals).
Mitochondria with flattened christae.
  
1,300,000,000 YBN
38)
(earlest red alga fossils:) (Hunting Formation) Somerset Island, arctic
Canada  
1,300,000,000 YBN
67) First "plastids". Cyanobacteria form plastids (chloroplasts) through
symbiosis, within a eukaryote cell (endosymbiosis). Like mitochondria, these
organelles copy themselves and are not made by the cell DNA.

Chloroplasts use their green pigment to trap light particles to synthesize
carbon compounds from carbon dioxide and water supplied by the host plant.

This is a primary plastid endosymbiosis, and genetic analysis supports the
theory that all green plants, which are eukaryotes with double membrane
plastids, are descended from a single common ancestor. All primary plastids are
surrounded by two membranes, because the cyanobacteria was enclosed in a
vacuole. The inner wall being that of the bacterium, the outer wall that of the
alga. Most plastids contain a single, circular chromosome of about 200
kilobases and encode about 100-120 genes, while a free-living cyanobacteria
typically has a genome of about 2500 Kilobases. The genes that remain in the
plastid are primarily involved in photosynthesis, transcription and translation
of plastid genes, and ATP synthesis. But, most of the genes needed to maintain
the plastid are encoded in the cell nucleus.

A secondary plastid endosymbiosis, where an algae cell is captured instead of a
cyanobacteria, which results in a plastid with more than two membranes, has
happened at least three times. Euglenozoa and chlorarachniophytes acquired
plastids from green alga, and the Chromalveolates (the most abundant group with
secondary plastids) acquired them from a red alga.

A third (tertiary) plastid endosymbiosis occurs when an alga containing a
plastid of secondary endosymbiotic origin (for example a chromist) is engulfed
and reduced to a photosynthetic organelle. Dinoflagellates are the only group
currently known to have tertiary plastids. Tertiary plastids in dinoflagellates
have been acquired from haptophyte and prasinophyte algae and from diatoms.
Currently there are five plastids known in dinoflagellates, each with its own
evolutionary history.

There are different kinds of plastids including aleuroplasts, amyloplasts,
chloroplasts, chromoplasts, elaioplasts, and etioplasts.
  
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209)
  
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219) unicellular to multicellular (up to 1 m) mostly free-living but some
parasitic or symbiotic, with chloroplasts containing phycobilins. Cell walls
made of cellulose with mucopolysaccharides penetrated in many red algae by
pores partially blocked by proteins (complex referred to as pit connections).
Usually with separated phases of vegetative growth and sexual reproduction.
Common and widespread, ecologically important, economically important (source
of agar). No flagella. Ultrastructural identity: Mitochondria with flat
cristae, sometimes associated with forming faces of dictyosomes. Thylakoids
single, with phycobilisomes, plastids with peripheral thylakoid. During
mitosis, nuclear envelope mostly remains intact but some microtubules of
spindle extend from noncentriolar polar bodies through polar gaps in the
nuclear envelope. Synapomorphy: No clear-cut feature available; possibly pit
connections Composition: About 4,000 species.
  
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323)
  
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187) A captured red alga (rhodophyte), through endosymbiosis, becomes a plastid
in the ancestor of all chromalveolates.

A secondary plastid endosymbiosis, where an algae cell is captured instead of a
cyanobacteria, has happened at least three times. A secondary plastid symbiosis
results in a plastid with more than two membranes. Two groups have acquired
plastids from green algae independently: the euglenozoa, which are fresh-water
algae, and the chlorarachniophytes. The most abundant groups with secondary
plastids acquired them from the red algae. Five algal lineages have plastids of
red algal origin. These include the crytophytes, the haptophytes, the
Strameopiles, which all together are the Chromista, and the Alveolates
apicomplexans and dinoflagellates. The alveolate ciliates are thought to have
lost their plastid and no traces of the organelle have yet been found. The
parasitic apicomplexans have lost the ability to do photosynthesis, probably
because of their intercellular lifestyle, but do maintain a vestigial organelle
derived from a plastid called the apicoplast, which is surrounded by four
membranes and has a small genome.
  
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15) Differentiation in multicellular eukaryote. Gamete (or spore) cells and
somatic cells. Unlike gamete cells, somatic cells are asexual (non-fusing), and
are not omnipotent. Start of death by aging.

Cell differentiation is how cells in a multicellular organism become
specialized to perform specific functions in a variety of tissues and organs.

All cells of an organism, except the sperm and egg cells, the cells from which
they arise (gametocytes) and undifferentiated stem cells, are somatic cells.

Although the DNA in each cell of a multicellular organism is the same, each
differentiated cell type produces a different set of specific proteins, for
example liver cells make albumin while lens cells make crystallin.

Another early cell differentiation are that only the cell at the tip of the
filament can divide while the older cells below the tip do not divide.
  
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88)
  
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201)
(Hunting Formation) Somerset Island, arctic Canada  
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301)
  
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153)
  
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221)
  
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6295)
(Stirling Range Formation) Southwestern Australia  
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305) Chromista "Cryptophyta" {KriPTuFITu} (Cryptomonads {KRiPToMunaDZ}).
  
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6280)
  
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86) (I think it's tough to say that the more ancient Heterokonts, brown algae
(Phaeophyta), and golden algae (Chrysophyta) are not also plants, and the
oldest living plants. Perhaps glaucophyta are the first green plants, or
perhaps that should be reserved for multicellular species.)
  
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188) Plant Green Algae evolves now according to genetic comparison. Green Algae
is composed of the two Phlya Chlorophyta (volvox, sea lettuce) and Charophyta
(Spirogyra).

The first land plants most likely evolved from green algae.

Cysts resembling modern Micromonadophyceae cysts date from about 1.2 billion
years ago. Tasmanites formed the Permian "white coal", or tasmanite, deposits
of Tasmania and similar deposits in Alaska. Certain Ulvophyceae fossils that
date from about one billion years ago are abundant in Paleozoic rocks.

Knoll et al cite the earliest recognized green algae fossil as Proterocladus
which dates to 750 million years ago.
  
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75)
  
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6284)
  
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87) Excavate Discicristates {DiSKIKriSTATS}, ancestor of protists which have
mitochondria with discoidal shaped cristae (includes euglenids, leishmanias
{lEsmaNEuZ}, trypanosomes {TriPaNiSOMZ}, kinetoplastids {KiNeTuPlaSTiDZ}, and
acrasid {oKrASiD} slime molds).

The discicristates include photosynthetic flagellates, such as the green
Euglena, and parasitic ones, such as Trypanosoma, which causes sleeping
sickness. There are also the acrasid slime molds, which are not closely related
to the amoebozoan dictyostelid and plasmodial slime molds.

Some euglenids exhibit colonialism and have a cell covering ("pellicle").

In eukaryote mitochondria there are three kinds of christae (the inner membrane
protrustions of mitochondria): discoidal, tubular, and flattened. Discoidal are
found in kinetoplasts and euglynoids, tubular christae are found in diatoms,
crysophyte algae, and apicomplexans, and Flattened cristae are found in
opisthokonts (animals and fungi) and both green and red algae.
  
1,080,000,000 YBN
97) A eukaryote eye evolves; the first three-dimensional response to light.

Eyes evolve at least eight times independently in eukaryotes.

The earliest eye probably evolves from a plastid. The first proto eye is a
light sensitive area in a unicellular eukaryote.

Eukaryotes are the first organisms to evolve the ability to follow light
direction in three dimensions in open water.

Halophilic archaebacteria, such as Halobacterium salinarum, use sensory
rhodopsins (SRs) for phototaxis (positive or negative movement along a light
gradient or vector), and some cyanobacteria (e.g. Anabaena, Synechocystis) can
slowly orient along a light vector.

Eukaryotes are the first organisms to evolve the ability to follow light
direction in three dimensions in open water. The eukaryotic sensory
integration, sensory processing and the speed and mechanics of tactic responses
is fundamentally different from that found in prokaryotes. Both single-celled
and multi-cellular eukaryotic phototactic organisms have a fixed shape, are
polarized, swim in a spiral and use cilia for swimming and phototactic
steering. Three-dimensional phototaxis can be found in five out of the six
eukaryotic major groups (opisthokonts, Amoebozoa, plants, chromalveolates,
excavates, rhizaria).
  
1,080,000,000 YBN
203)
  
1,050,000,000 YBN
169)
  
1,050,000,000 YBN
297) Diplontic life cycle; organism is predominantly diploid, mitosis in the
haploid phase does not occur.
  
1,050,000,000 YBN
304)
  
1,040,000,000 YBN
313) The ciliophora, apicomplexa and dinoflagelatta are under the title
alveolata because they have an alveolar membrane system, which contains
flattened membrane-bound sacs (alveoli) lying beneath the outer cell membrane.

In dinoflagellates, the chromosomes are always visible and do not condense
prior to mitosis. The chromosomes are attached to the nuclear envelope, which
persists during mitosis.

The main method of reproduction of the dinoflagellates is by longitudinal cell
division, with each daughter cell receiving one of the flagella and a portion
of the theca and then constructing the missing parts in a very intricate
sequence. Some nonmotile species form zoospores, which may be colonial. A
number of species reproduce sexually, mostly by isogamy, but a few species
reproduce by anisogamy.

Dinoflagellate zygotes are similar to some acritarchs (early eukaryote
fossils).

The earliest undisputed, structural fossils of dinoflagellates are cysts dating
from the Triassic (251-201 Ma), with a few likely Permian records. Some
Silurian (c410 Ma) fossils have been attributed to the group but the relation
is uncertain. Acritarchs are microfossils with no known affinity. Some people
have tried to link acritarchs with dinoflagellates. Some later acritarchs from
the Jurassic and Cretaceous, have been shown to be dinoflagellate cysts and so
are no longer treated like acritarchs. A correlation has been noted between the
presence of triaromatic dinosteroids and acritarch abundance, implying that
these acritarchs may be the cysts of ancestral dinoflagellates.

If acritachs are dinoflagellates, then dinoflagellates may date back to at
least 1.8 billion years and perhaps even 3.5 billion years to the earliest
known acritarchs.
Dinosterane, derived from dinosterol produced by
dinoflagellates, occurs in the 1.1 Ga Nonesuch Formation, in the United States.
  
1,005,000,000 YBN
306) Earliest certain Stramenopiles fossil a xanthophyte (or yellow-green
algae): "Palaeovaucheria".
(Lakhanda Group) Siberia  
1,000,000,000 YBN
154)
  
1,000,000,000 YBN
223)
  
1,000,000,000 YBN
324) Protists (Mesomycetozoea {me-ZO-mI-SE-TO-ZO-u} (also called DRIPS).

Mesomycetozoea are in the protist Phylum Choanozoa (which includes
Choanoflagellates). This phylum contains the first protozoans
(Choanoflagellates), thought to be the ancestor of sponges.

DRIP is an acronym for a small group of parasites mostly of fish and other
freshwater animals.
  
985,000,000 YBN
309) Protist Phylum Oomycota {Ou-mI-KO-Tu} evolves according to genetic
comparison, (includes the Class Oomycetes) (Water molds).

Oomycetes (Water molds), with about 580 species, vary from unicellular, to
multicellular highly brached filamentous forms.

Oomycetes have mitochondria with tubular christae.

Oomycetes grow by closed (or nearly closed) mitosis with pairs of centrioles
near the poles.
  
965,000,000 YBN
155)
  
900,000,000 YBN
326)
  
900,000,000 YBN
6281)
  
855,000,000 YBN
286) In sponges all cells are "totipotent", which means that every cell is
capable of becoming any of the sponge's different cell types. Any isolated cell
is capable of growing an entire new sponge. In sponges there is no distinction
between germ line and soma.

Some people think that multicellular organisms arose at least six times: in
animals, fungi and several groups of algae.
  
850,000,000 YBN
81) The first animal and first metazoan evolves (Porifera: sponges). Metazoans
are multicellular and have differentiation (their cells perform different
functions). There are only three major kinds of metazoans: sponges, cnidarians,
and bilaterians (which include all insects and vertebrates).

Sponges have a variety of different cell types: cells that line surfaces
(pinacocytes, porocytes, choanocytes), cells that secrete the skeleton
(collencytes, sclerocytes), contractile cells (myocytes), archaeocytes
(amoeboid cells that play a major role in digestion and food transport), and
several other cell types.

Sponges have many holes which is why they are good at holding water in the
bath.

All sponge cells are totipotent and are capable of regrowing a new sponge.
Mixtures of sponge cells of two species reconstitute into the separate sponge
species. The process involves cell-cell recognition, which is a basic attribute
for building and retaining a multicellular body. The molecular mechanisms that
guide this process involve many proteoglycans (compounds made of 95%
polysaccharide and 5% protein) on the cell surface.

Sponges have no nerve cells or muscles. Like plants their movement is at the
cellular level. Sponges live by passing a constant current of water through
their body from which they filter food particles.

The sponges have no obvious symmetry while Cnidarians have radial symmetry, and
Ctenophores have biradial symmetry. Porifera have a simple level of cellular
integration and are loosely constructed, but all other later animals including
cnidarians and ctenophores have cells which are grouped together as tissues
that are arranged in layers.

All sponges are capable of sexual and asexual reproduction. There is a large
diversity of sexual reproductive sequences in sponges. Sperm are formed from
choanocytes, and eggs from choanocytes or archaeocytes. Generally, sperm are
contained in spermatic cysts, which are choanocyte chambers transformed by
spermatogenesis. Eggs are distributed throughout the mesohyl. Some sponges are
oviparous (zygote develops outside the body). Following gamete release,
fertilization and development occur externally. Other sponges are viviparous,
with fertilization and development both occurring in the mesohyl.

Some sponges can live for over 1000 years.
  
850,000,000 YBN
224)
  
850,000,000 YBN
517)
  
804,000,000 YBN
319) Protist Phylum "Radiolaria" {rADEOlaREo} evolves now according to genetic
comparison. Radiolaria are ocean protozoa, many with silica shells.

Radiolarians are protists found in the upper layers of all oceans.
Radiolarians, are mostly spherically symmetrical, and known for their complex
and beautifully tiny skeletons, called "tests". Tests are usually made of
silica. Pseudopodia extend through the perforated skeleton. A chitinous central
capsule encloses the nuclei and divides the cytoplasm into two zones. The outer
cytoplasm contains many vacuoles that control the organism’s buoyancy.

Asexual reproduction is by budding, binary fission, or multiple fission.
Generally, the skeleton divides, and each daughter cell regenerates the missing
half. In some cases, however, one daughter cell escapes and develops an
entirely new shell, the other daughter remaining within the parent skeleton.
  
804,000,000 YBN
321) Protist Phylum "Foraminifera" evolves now according to genetic
comparison.

Foraminifera (or "forams" for short), are unicellular protists characterized by
long, fine pseudopodia that extend from a uninucleated or multinucleated
cytoplasmic body encased within a test, or shell. Shell sizes may be as large
as 5 cm in diameter and vary in shape and chemical composition.

Foraminifera are the most diverse and most widely studied of microfossils.
Forams are related to the amoeba but unlike an amoeba they have a shell. Forams
secret skeletons of calcium carbonate (the mineral calcite), which is different
than radiolarians which secrete skeletons of silica. Most are marine and live
on or in the sea bottom (are benthic) but one family, Globigerinidae, are tiny
and buoyant and make up a major part of the marine plankton.

Foraminifera, especially the calcareous forms, have a fossil record stretching
back to the Early Cambrian, and are especially important biostratigraphically.

Much of the Earth's chalk, limestone, and marble is composed largely of
foraminiferan tests.
  
780,000,000 YBN
79) Metazoan Phylum "Placozoa" evolves.

Placozoans look like amoebas but are multicellular. The only known species in
this phylum is Trichoplax adhaerens. Trichoplax lives in the sea and feeds on
single celled organisms, mostly algae. Trichoplax has only 4 cell types
compared to the more than 200 cell types in humans. Trichoplax has two main
cell layers, like a cnidarian or ctenophore. Between these two layers are a few
contractile cells that are similar to muscle cells, however placozoans lack
muscle and nerve cells and have no symmetry or organs. Trichoplax has only 1
hox gene (Trox-2).

Possible eggs have been observed, but they degrade at the 32-64 cell stage.
Neither embryonic development nor sperm have been observed, however Trichoplax
genomes show evidence of sexual reproduction.
  
767,000,000 YBN
312) Protist Phylum "Ciliophora" ("Ciliates") evolves according to genetic
comparison (includes parameceum). Earliest mitochondria with tubular christae.

There are about 12,000 described species of ciliates. Ciliates are very common
in benthic and planktonic communities in both marine and fresh water. Both
sessile and free moving types are known and many are ecto- or endosymbionts,
including some parasitic species. Most are single celled, but branching and
linear colonies are known in several species. Ciliates have a fixed shape which
is maintained by the alveolar membrane system and underlying fibrous layer.
Ciliates use their cilia for locomotion. Mitochondria in ciliates have tubular
cristae. Ciliates have two distinct types of nuclei, a hyperpolyploid
macronucleus and a diploid micronucleus. Ciliates reproduce by asexual
reproduction using transverse binary fission, and by sexual reproduction using
conjugation: a pair of ciliates fuse and exchange micronuclei through a
cytoplasmic connection at a point of joining. Ciliates include many different
feeding types. Some are filter feeders, others capture and inject other
protists or small invertebrates, many eat algal filaments or diatoms, some eat
attached bacteria, and a few are saprophytic parasites (live on dead or
decaying organic matter). In almost all ciliates feeding is restricted to a
specialized area containing the "cytostome or "cell mouth". Food vacuoles are
formed at the cytosome and then circulated through the cytoplasm as digestion
occurs. A few ciliates (for example Laboea, and Stronbidium) contain
photosynthetically functional chloroplasts derived from injested algae. The
chloroplasts lie free in the cytoplasm, beneath the pellicle, where they
actively contribute to the ciliate's carbon budget.

A few ciliates (for example tintinnids), secrete external skeletons, or
loricae, which have been found in the fossil record as early as the Late
Proterozoic in the Doushantuo Formation (580 million years ago). Biomarkers for
ciliates have been found dating back ever farther to 850 million years ago.
  
767,000,000 YBN
314)
  
750,000,000 YBN
41) Cells that group as tissues that are arranged in layers evolve in
metazoans.
  
750,000,000 YBN
83) First nerve cell (neuron), and nervous system evolves in the ancestor of
the Ctenophores and Cnidarians. This leads to the first ganglion and brain.
Earliest touch and sound detection.

The most primitive extant organisms that contain a neuron cell are the
ctenophora.

Simple and sessile cnidarians have no sense organs, but they do have sensory
cells in both tissues that respond to light, chemical or mechanical stimuli.
These sensory cells are often structurally similar to those of vertebrates.
Each has a cilium that protrudes into the water. The sensory cells synapse (are
closely spaced to) with nerve cells, allowing the animal to generally respond
to stimuli at a distance instead of responding at the site of the stimulus.

Some Cnidarians have ganglia, aggregations of nerve cells.
  
750,000,000 YBN
96)
  
750,000,000 YBN
204) Earliest known fossil protozoan (single celled nonphotosynthesizing
eukaryotes) and earliest fossil of a testate amoeba.

This fossil indicates that the last common ancestor of animals and fungi
appeared at least 750 million years ago.

This fossil was found in the Grand Canyon in Arizona.
( black shales of Chuar Group) Grand Canyon, Arizona, USA  
750,000,000 YBN
225)
  
750,000,000 YBN
414)
  
750,000,000 YBN
458) Fungi Phylum "Glomeromycota" (Arbuscular {oRBuSKYUlR} mycorrhizal
{MIKerIZL} fungi).

Glomeromycota {GlO-mi-rO-mI-KO-Tu} are also know by their class name
Glomeromycetes {GlO-mi-rO-mI-SETS}
  
713,000,000 YBN
6320) Earliest chemical biomarker evidence of animals (metazoans), steranes
associated with demosponges.

Demosponges comprise 85% of all extant sponge species.
(Huqf Supergroup) South Oman Salt Basin, Oman  
700,000,000 YBN
82) Radiata Phylum Cnidarians {NIDAREeNS} evolve (sea anemones, corals,
jellyfish). Earliest animal eye.

Cnidaria {NIDAREeo} are a phylum of invertebrate animals composed of the sea
anemones, corals, jellyfish, and hydroids. Cnidarians are radially symmetrical.
The mouth, located at the center of one end of the body, opens into a
gastrovascular cavity, which is used for digestion and distribution of food,
there is no anus. Cnidarians have a body wall composed of three layers: an
outer epidermis, an inner gastrodermis, and a middle mesogloea. Tentacles
encircle the mouth and are used in part for food capture. Specialized stinging
structures, called nematocysts, are a characteristic of the phylum and are
located in the tentacles and often in other body parts. These contain a coiled
fiber that can be extruded suddenly. Some nematocysts contain toxic substances
and are defense mechanisms, while others are adhesive, helping to anchor the
animal or to entangle prey.

Cnidarians have two alternate body plans, the polyp and the medusa. A sea
anemone or Hydra is a typical polyp: non-moving, mouth on top, bottom end fixed
to the ground like a plant. A jellyfish is a typical medusa, swimming through
the open sea. Many cnidarians have both polyp and medusa forms, alternating
them through life cycle, like caterpillar and butterfly. Polyps often reproduce
by budding, like plants. A new baby polyp grows on the side of a freshwater
Hydra, eventually breaking off as a separate individual clone of the parent. In
many marine relatives of Hydra, the clone doesn't break off but stays attached,
and becomes a branch like a plant. Sometimes more than one kind of polyp grows
on the same polyp tree, specialized for different roles, such as feeding,
defense, or reproduction.

Cnidarians have a nervous system which is a network, not centralized into a
brain, ganglia or major nerve trunks. They also have muscles which are
contracted to propel them. Their digestive organ is a single cavity with only
one opening which is both mouth and anus. They have no circulatory system. All
cnidarians have cells called cnidocytes, each with its own cell-sized harpoon
called a cnida. All cnidarians have cnidae, and only cnidarians have them. Once
triggered the harpoon cell cannot be used again, but are constantly replaced.

Simple and sessile cnidarians have no sense organs, but they do have sensory
cells in both tissues that respond to light, chemical or mechanical stimuli.
These sensory cells are often structurally similar to those of vertebrates.
Each has a cilium that protrudes into the water. The sensory cells and nerve
cells are separated by a small space (synapse), allowing the animal to
generally respond to stimuli at a distance instead of responding at the site of
the stimulus. Medusae and complex motile colonies of Cnidaria have more complex
sense organs: the statocyts detect the degree of tilt of the body, and the
ocelli {OSeLlE or OSeLlI} are light receptors. Cnidarian ocelli range from
patches of photoreceptors alternating with pigment cells, to complex structures
in which the light receptors have a cup shaped shield of pigmented cells behind
them and are covered by a lens formed from cytoplasmic extensions from
neighboring cells {see image}.

Cnidarians see in black or white, because their eyes have only one pigment, for
color vision the eye must have more than one pigment.

Porifera (sponges have no obvious symmetry), while Cnidarians are radially
symmetrical and Ctenophores are biradially symmetrical.

There are differences between Cnidaria and Ctenophora. In Cnidaria, cells have
a single flagellum or cilium, while the cells of Ctenophora have large numbers
of cilia. Stinging cells called cnidocytes, are unique to cnidarians, and
adhesive cells called "coloblasts" are unique to Ctenophora. Ctenophora swim by
using arrays of fused cilia arranged in eight rows, while the Cnidaria move by
means of muscle contraction of an epithelial cell. Cnidarians lack true muscle
cells. The muscle fibers in Cnidaria are always extensions of an epithelial
cell. Ctenophora have true muscles. Unlike Cnidaria, Ctenophora have gonoducts
and gonopores by which gametes exit the body.

Cnidaria do not have complex reproductive organs; gonads develop in the body
wall or mesenteries by differentiation of interstitial cells. In many species
the gonads are absorbed again after spawning has occurred. Gonads may be formed
in the tissue and gametes released directly into the water or gonads may be
endodermal and the gametes released into the water through breaks in the body
wall or through the mouth. Genders are usually separate, but some species are
hermaphroditic (produce both ova and sperm). Sperm are released into the water
and fertilization is usually external. In species that brood their eggs,
fertilization occurs at the brooding site, which may be in the gastrovascular
cavity or on the outside of the body. Sperm are often attracted to the eggs by
highly specific chemicals.

Digestion in Cnidarians starts in the gastrovascular cavity, but once the food
is reduced to particles small enough to enter the digestive cells of the
gastrodermis, digestion is completed inside the cell (intracellularly).

Cnidarians make the great barrier reef which is more than 2,000 kilometers
long. The cnidarian, the box jellyfish, is one of the most dangerously venomous
animals on earth.
  
700,000,000 YBN
226) The second largest Fungi phylum, "Basidiomycota" {Bo-SiDEO-mI-KO-Tu}
evolves now according to genetic comparison (most mushrooms, rusts, club
fungi).

The Division Basidiomycota is a large taxon within the Kingdom Fungi that
includes those species that produce spores in a club-shaped structure called a
basidium. Essentially the sibling group of the Ascomycota, it contains some
30,000 species (37% of the described fungi)
  
700,000,000 YBN
227) The largest Fungi phylum "Ascomycota" {aS-KO-mI-KO-Tu} evolves now
according to genetic comparison: (yeasts, truffles, Penicillium, morels, sac
fungi).

There are 47,000 described Ascomycota species.
  
700,000,000 YBN
523)
  
680,000,000 YBN
222) Fungi Ascomycota Class "Archaeascomycetes" (fission yeast, pneumonia
fungus) evolve.
  
675,000,000 YBN
156)
  
650,000,000 YBN
69) Start of 60 million year (Varanger) Ice Age (650-590 mybn).
  
630,000,000 YBN
107) Bilateral species evolve (two sided symmetry).
Earliest animal brain (ganglion,
memory). First triploblastic species (third embryonic layer: the mesoderm).

In bilaterians food enters in one end (the mouth) and waste exists at the
opposite end (the anus). There is an advantage for sense organs: light, sound,
touch, smell, and taste detection to be located on the head near the mouth to
help with catching food.

Unlike the diploblastic Cnidaria and Ctenophora, flatworms and all later
metazoans are triploblastic. A third embryonic layer, the mesoderm, lies
between the ectoderm and endoderm. This layer increases the options for the
development of organs with specific functions, formed by the association of
tissues of various kinds.

The earliest brain (ganglion, memory) develop in a bilaterian worm.

This begins the Animal Subkingdom "Bilateria".
  
630,000,000 YBN
403) Earliest extant bilaterian: Acoelomorpha (acoela flat worms and
nemertodermatida).

The phylum Acoelomorpha (acoela flat worms and nemertodermatida) is the oldest
surviving bilaterian. This begins the Subkingdom "Bilateria".

Acoelomorpha lack a digestive track, anus and coelom.

Flatworms have no lungs or gills and breathe through their skin. Flatworms also
have no circulating blood and so their branched gut presumably transports
nutrients to all parts of the body.
  
630,000,000 YBN
459)
  
630,000,000 YBN
532) Cylindrical gut, anus, and through-put of food evolves in a bilaterian.

All bilaterally symmetrical metazoans except the Phyla Acoelomorpha and
Platyhelminthes, have a tubular gut with an anus, mouth, and through-put of
food. The Phyla Nemertea and Entoprocta are the earliest bilaterians with an
anus.
  
630,000,000 YBN
593) The genital pore, vagina, and uterus evolve in a bilaterian.
  
630,000,000 YBN
660) The penis evolves in a bilaterian.
  
625,000,000 YBN
6328)
  
610,000,000 YBN
95) (Perhaps the space in between body and gut walls separates potentially
harm-food food from mixing with and damaging important mechanical, chemical and
other parts of the metazoan.)
  
600,000,000 YBN
91)
Sonora, Mexico|Adelaide, Australia| Lesser Karatau Microcontinent,
Kazakhsta  
600,000,000 YBN
98)
  
590,000,000 YBN
70)
  
590,000,000 YBN
93) Bilaterians Protostomes evolve. Protostomes are divided into two major
groups: the Ecdysozoa {eK-DiS-u-ZOu} and the Lophotrochozoa {LuFoTroKoZOu}. The
Ecdysozoa are animals that molt or lose their outer skin as they grow, and
include Priapulids {PrIaPYUliDZ}, Nematodes, Tardigrades {ToRDiGRADZ},
Onychophorens {oniKoFereNS}, and the arthropods {which is a large group
including all crustaceans and insects}. The Lophotrochozoa, is subdivided into
the Platyzoa {PlaTiZOu}, which includes rotifers, gastrotrics and
Platyhelminthes, and the Trochozoa, which includes bryozoans {BrI-u-ZO-iNZ},
Nemertea {ne-mR-TEu}, Phoronids {FerOniDZ}, brachiopods {BrA-KE-O-PoDZ},
Entoprocts {eNtoProKTS}, molluscs and annelids.
  
580,000,000 YBN
131) First shell (or skeleton) evolves in unicellular protists.

The first known shell belongs to unicellular protists ciliates called the
tintinnids. This shell is called a lorica. These fossils are thought to be in
shallow marine waters, not far from the coastline.

Similar modes of skeleton formation have evolved independently in different
groups to fulfill similar needs.

These are also the earliest known ciliate fossils.

Unfortunately there has been no consistent terminology for coverings. The
terms lorica, shell, test, and case are often used synonymously. Euglenozoa
have an outside covering which is called a "pellicle". A pellicle usually has
openings for injestion, egestion, and water expulsion. Some ciliates
(tintinnids) secrete an external skeleton called a "lorica", which start to
appear in the fossil record around 500 million years ago. Foraminifera secrete
a heavy shell of silica or calcium carbonate. The shape of Dinoflagellates is
maintained by alveoli beneath the cell surface, and by a layer of supporting
microtubules. In some, these alveoli are filled with polysaccharides, typically
cellulose, and these dinoflagellates are said to be "thecate", or "armored",
while dinoflagellates that have empty alveoli are said to be "athecate", or
"naked". Diatoms secrete silicon in the form of an internal test or frustule,
that contains two parts called valves. Beneath the test is the cell membrane
enclosing the nucleus, chloroplasts and cytoplasm. Some protists build a "test"
of sand grains or other particles cemented together. Resistant covering are
sometime formed for brief parts of the life cycle. This is especially true for
parasites, which usually pass from one host to another as cysts or spores,
covered by a resistant membrane that protects them while out of the host.

In addition to its supportive function, the animal skeleton may provide
protection, facilitate movement, and aid in certain sensory functions. Support
of the body is achieved in many protozoans by a simple stiff, translucent,
nonliving envelope called a pellicle. In nonmoving (sessile) coelenterates,
such as coral, whose colonies attain great size, body support is provided by
non-living structures, both internal and external, which form supporting axes.
In the many groups of animals that can move, body support is provided either by
external structures known as exoskeletons or by internal structures known as
endoskeletons.

The skeleton may be on the body surface, for example the lateral sclerites of
centipedes and the shell of crabs. These structures carry no muscle and form
part of a protective surface armor. Similarly, the scales of fish, the
projecting spines of echinoderms (for example sea urchins), the needle-like
structures (spicules) of sponges, and the tubes of hydroids, raised from the
body surface, all provide protection. The bones of the vertebrate skull protect
the brain. In the more advanced vertebrates and invertebrates, many skeletal
structures provide a rigid base for the insertion of muscles as well as
providing protection.

The skeleton assists movement in a variety of ways, depending on the nature of
the animal. The bones of vertebrates and the exoskeletal and endoskeletal units
of the cuticle of arthropods (insects, spiders, crabs, etc.) support opposing
sets of muscles.
(Doushantuo Formation) Beidoushan, Guizhou Province, South China  
580,000,000 YBN
165) Earliest bilaterian fossil, Vernanimalcula, 178 um in length. First fossil
of organism with bilateral symmetry, mouth, digestive track, gut and anus.
(Doushantuo Formation) China  
580,000,000 YBN
318) Protostome Infrakingdom Ecdysozoa {eK-DiS-u-ZOu} evolves. Ecdysozoa are
animals that molt (lose their outer skin) as they grow. This is the ancestor of
round worms, and arthropods (which includes insects and crustaceans {also known
as "shell-fish"}).
  
580,000,000 YBN
331) Protosomes Lophotrochozoa {Lu-Fo-Tro-Ku-ZO-u} evolve. Ancestor of all
brachiopods {BrA-KE-O-PoDZ}, bryozoans {BrI-u-ZO-iNZ}, and molluscs.
  
580,000,000 YBN
6293) Earliest cnidarian fossil.

These are fossil cnidarian embryos and larvae from Doushantuo Formation in
China.

Cnidarians which possessed hard skeletons, in particular the corals, have left
a significant fossil record of their existence.
(Doushantuo Formation) Beidoushan, Guizhou Province, South China  
578,000,000 YBN
92)
  
575,000,000 YBN
139) Earliest sea pen fossils ("Charnia"). A member of the Cnidarnian
Anthozoans (sea pens, corals, anemones).

Sea pens are grouped in the Class "Pennatulacea".

Some people have suggested that a fossil from China shows that the fronds are
ciliated which implies that these fossil organisms are possibly more closely
related to Ctenophores than sea pens.
(Drook Formation) Avalon Peninsula, Newfoundland  
570,000,000 YBN
89) Protostome Lophotrochozoa {Lu-Fo-Tro-Ku-ZO-u} subgroup Trochozoa evolve.
Ancestor of all Bryozoans, Nemerteans, Phoronids, Brachiopods {BrA-KE-O-PoDZ},
Molluscs and Annelids.
  
570,000,000 YBN
94)
(Doushantuo formation) China  
570,000,000 YBN
105) Bilaterians Deuterostomes evolve. This is the ancestor of all Echinoderms
(iKIniDRMS } (Phylum Echinodermata: sea cucumbers, sea urchins, starfish),
hemichordates (Phylum Hemichordata: acorn worms), and Chordates (Phylum
Chordata: all tunicates, fish, amphibians, reptiles, mammals, and birds).
  
570,000,000 YBN
311) Bilaterians Chaetognatha {KE-ToG-nutu} evolve (Arrow Worms).

Earliest teeth. Animals start to eat other animals.

The evolution of teeth and then of animal predation starts an "arms race" that
rapidly transforms ecosystems around the Earth. So in this sense hard teeth
evolve first and then the shell evolves as an advantage to survival.

Chaetognaths are bilaterally symmetrical enterocoelous animals, with an
elongated cylndrical body; they are usually colourless, transparent or slightly
opaque. The body is divided in three parts by internal partitioning: head,
trunk and tail. The head is slightly rounded and separated from the trunk by a
constricted neck. Each side of the head bears a group of curved grasping hooks
and one or two rows of teeth, called the anterior and posterior teeth; the
hooks and teeth are made of chitin. A pair of uniquely arranged pigmented
eyespots is present.

The earliest Chaetognath fossil is from around 520 mya.

The placement (phylogeny) of the Chaetognatha within the Bilateria is currently
somewhat uncertain. Some place them as protostomes, others as deuterostomes.
Some people group them with the Ecdysozoa, others as Lophotrochozoa, others as
an independent group in between Ecdysozoa and Lophotrochozoa.

Chaetognatha appears close to the base of the protostome tree in most studies
of their molecular phylogeny. This may be evidence that protostomes descend
from a deuterostome ancestor, like a chaetognath.
  
570,000,000 YBN
327) Protostome Lophotrochozoa {Lu-Fo-Tro-Ku-ZO-u} subgroup Platyzoa
{PlaT-i-ZO-u} evolves. Ancestor of rotifers, gastrotrichs and Platyhelminthes
(flatworms).

Thomas Cavalier-Smith proposed the new infrakingdom in 1998 for "ciliated
non-segmented acoelomates or pseudocoelomates lacking vascular system; gut
(when present) straight, with or without anus".
  
570,000,000 YBN
345)
  
570,000,000 YBN
346) Deuterostome Phylum Echinodermata ("Echinoderms" (iKIniDRMS }) (sea
cucumbers, sea urchins, sand dollars, star fish).
  
565,000,000 YBN
347) Deuterostome Phylum Chordata evolves. Chordates are a very large group
that include all tunicates {TUNiKiTS}, fishes, amphibians, reptiles, mammals,
and birds. The most primitive living chordate is the tunicate. Chordates get
their name from the notochord, the cartilage rod that runs along the back of
the animal, in the embryo if not in the adult.

Chordata is the highest phylum in the animal kingdom, which includes the
lancelets or amphioxi (Cephalochordata), the tunicates (Urochordata), the acorn
worms and pterobranchs (Hemichordata), and the vertebrates (Craniata)
comprising the lampreys, sharks and rays, bony fish, amphibians, reptiles,
birds, and mammals. Members of the first three groups, the lower chordates, are
small and strictly marine. The vertebrates are free-living; the aquatic ones
are primitively fresh-water types with marine groups being advanced; and the
members include animals of small and medium size, as well as the largest of all
animals.

The typical chordate characteristics are the notochord, the dorsal hollow nerve
cord, the pharyngeal slits, and a postanal tail. The notochord appears in the
embryo as a slender, flexible rod filled with gelatinous cells and surrounded
by a tough fibrous sheath, and contains, at least in some forms, transverse
striated muscle fibers; it lies above the primitive gut. In lower chordates and
the early groups of vertebrates, the notochord persists as the axial support
for the body throughout life, but it is surrounded and gradually replaced by
segmental vertebrae in the higher fish.
  
565,000,000 YBN
348) Earliest extant chordate: Tunicates {TUNiKiTS} evolve (sea squirts).
  
565,000,000 YBN
6294) Earliest coral fossil (corals are cnidarian anthozoans).

These are fossil cnidarian coral (tabulata) from Doushantuo Formation in
China.

The tabulata are an extinct Paleozoic order of corals of the subclass
Zoantharia characterized by an exclusively colonial mode of growth and by
secretion of a calcareous exoskeleton of slender tubes.
(Doushantuo Formation) Beidoushan, Guizhou Province, South China  
560,000,000 YBN
117) Earliest chordate fossil.
(Flinders Ranges, 490 km north of Adelaide) Australia  
560,000,000 YBN
349)
  
560,000,000 YBN
6290) Earliest extant fish, Lancelets {laNSleTS} (also called amphioxus
{aMFEoKSeS}).

Lancelets are the most primitive chordates to have a liver and a kidney, which
are not found in hemichordates or tunicates.

The Lancelet is a protochordate and not a vertebrate. Lancelets have only a
nerve tube on the notochord and no brain other than a small swelling at the
front end of the nerve tube. They also have an eye-spot. There are gill slits
at the sides used for filter feeding and not primarily for breathing which
would mean that gills for breathing evolve later. The Lancelet is not like a
worm in not being cylindrical, and swims like a fish using its muscles with
side-to-side undulations.
  
560,000,000 YBN
6292) Oldest mollusc fossil.
  
560,000,000 YBN
6318) Earliest animal shell (or skeleton).
Earliest evidence of animals eating other
animals (predation).
Appearance of the small shelly fossils and deep burrows correlated with
a decline in stromatolites possibly from feeding.

The earliest animal shells are made by tiny organisms with simple tubelike
skeletons, such as Cloudina and Sinotubulites in addition to sponge skeleton
fossils.

The shell of Cloudina is made of Calcium carbonate (CaCO3), possibly made by
some kind of worm.


Predatory bore holes have been found in Cloudina shells. This is the oldest
evidence of predation known.

The earliest animal shells are agglutinated tubes built of foreign objects by
the animals inhabiting them, an example being the worm Onuphionella, with its
collection of mica flakes lining its shelter.

The appearance of the small shelly fossils and deep burrows are correlated with
a decline in stromatolites. Before the appearance of small invertebrate
animals, nothing fed on cyanobacterial mats. Some small shelly fossils must be
primitive molluscs that graze on stromatolites. Stromatolites survive today
only in environments that are hostile to grazing invertebrates. Tehse include
lagoons too salty for grazing snails like Shark Bay, Australia, and shallow
channels in the Bahamas where currents are too strong for clinging
invertebrates.

The soft-bodied multicellular (but non-skeletonized) Ediacaran fauna appear
starting around 600 mybn and may represent the next logical step up from
single-celled life. The next stage is the appearance of small mineralized
shells starting around 545 million years ago. These small shells are referred
to as "small shelly fossils" and were first reported by a team of Soviet
scientists headed by Alexi Rozanov of the Paleontological Institute in Moscow.
Rozanov reports in 1966 that the oldest limestones of Cambrian age contain many
small and unfamiliar skeletons, few larger than 1 cm (1/2 inch) long. These
fossils are referred to as "small shelly fossils". At the time these are the
earliest known fossils of hard skeletons. Their discovery rewrites the story of
the earliest Cambrian and sheds light on the Cambrian radiation.

Most of the small shelly fossils are made of calcium phosphate, the same
mineral that makes up the bones of vertebrates, but today, most marine
invertebrate shells are made of calcium carbonate (the minerals calcite and
aragonite). To some scientists this suggests that the later appearance of large
calcified trilobites and other fossils, represents a time when atmospheric
oxygen is abundant enough to allow calcite skeletons to be secreted.

There is evidence that seawater chemistry favored aragonite precipitation
during the late Precambrian and favored calcite precipitation during the
Tommotian, and that carbonate skeletal mineralogy is determined by the
chemistry of seawater at the time carbonate skeletons first evolve in a clade.

Prokaryotic cyanobacteria also develop the ability to secrete carbonate
skeletons around the same time.

Eventually, the expansion of infaunal life destroys the widespread and vast
cyanobacterial mats in shallow regions of the sea.
(Ara Formation) Oman|Lijiagou, Ningqiang County, Shaanxi Province  
559,000,000 YBN
103)
  
550,000,000 YBN
108)
  
550,000,000 YBN
109)
  
550,000,000 YBN
110)
  
550,000,000 YBN
111)
  
550,000,000 YBN
112)
  
550,000,000 YBN
113)
  
550,000,000 YBN
116)
  
550,000,000 YBN
118)
  
550,000,000 YBN
119)
  
550,000,000 YBN
157)
  
550,000,000 YBN
328) Ecdysozoa Superphylum "Aschelminthes" evolves. This includes the 5 Phyla:

Kinorhyncha (kinorhynchs),
Loricifera (loriciferans),
Nematoda (round worms),
Nematomorpha (horsehair
worms),
Priapulida (priapulids).
  
550,000,000 YBN
329)
  
550,000,000 YBN
6339)
(Rawnsley Quartzite -same as White Sea Assemblage) Nilpena, South
Australia  
547,000,000 YBN
333) Trochozoa Phyla Phoronida (phoronids {FerOniDZ}).
  
547,000,000 YBN
334) Trochozoa Phylum Brachiopoda (brachiopods {BrAKEOPoDZ}).

Brachiopods are marine invertebrates that have bivalve dorsal and ventral
shells enclosing a pair of tentacled, armlike structures that are used to sweep
minute food particles into the mouth. Also called lampshells.
  
547,000,000 YBN
335) The Lophotrochozoa (Trochozoa) Phylum Entoprocta (entoprocts).
  
544,000,000 YBN
310)
southwestern Mongolia  
543,000,000 YBN
101)
  
543,000,000 YBN
336) Lophotrochozoa (Trochozoa) Phylum Bryozoa (Bryozoans or moss animals).
  
542,000,000 YBN
53) End of the "Precambrian". End of the Proterozoic and start of the
Phanerozoic {FaNReZOiK} Eon, and the start of the Cambrian Period.

The term "Precambrian", was traditionally used for the division of time older
than the Phanerozoic, and is currently considered to be informal and without
specific stratigraphic rank.
  
542,000,000 YBN
114)
Ediacara, Australia  
542,000,000 YBN
6297) The Cambrian radiation, (or "Cambrian explosion"), the rapid
diversification of multicellular animals between 542 and 530 million years ago
that results in the appearance of many (between 20 and 35) of the major phyla
of animals. An increase of animals with shells.

It was once thought that the Cambrian rocks contained the first and oldest
fossil animals, but these are now to be found in the earlier Ediacaran (or
Vendian) strata. Ediacaran animals are soft-bodied and so are infrequently
preserved. When animals begin to develop hard parts, their probability of
preservation greatly improves. The first animals to develop hard parts are
small shelly fossils, like sponge spicules, gastropods, and others with
uncertain affinity. Small shelly fossils can be found back into the
Neoproterozoic.

Two fossil locations preserve this period on Earth, the Burgess Shale in
British Columbia Canada, and the Chengjiang in the Yunnan Province of China.
The Burgess Shale fossils were discovered in 1909 by Charles D. Wolcott (CE
1850-1927), and are shiny black impressions on the shale bedding planes. Many
are the remains of animals that lacked hard parts. Altogether there are four
major groups of arthropods (trilobites, crustaceans, and the groups that
include scorpions and insects), in addition to sponges, onycophorans, crinoids,
mollusks, three phyla of worms, corals, chordates, and many species that cannot
be placed in any known phylum. The Chengjiang Fauna resemble that of the
Burgess Shale, but the Chengjiang fossils are older and better preserved. The
fossils include many soft-bodied animals that are not usually not preserved.
For example jellyfish show the detailed structure of tentacles, radial canals,
and muscles, and on soft-bodies worms, eyes, segmentation, digestive organs,
and patterns on the outer skin can be recognized. The Chengjiang fossils
include the earliest fossil of a fish.

One theory is that the Cambrian radiation is triggered by predation, since the
oldest traces of feeding within the mud occur around this time in addition to
the various ways to protect the body by secretion of a mineral skeleton or
building tubes by collected mineral grains that are developed by animals around
this time.
  
541,000,000 YBN
132)
  
540,000,000 YBN
104) Platyzoa Platyhelminthes {PlaTEheLmiNtEZ} evolve (flatworms).
  
540,000,000 YBN
6287) Platyzoa Phylum Gastrotricha (Gastrotrichs {GaSTreTriKS}).
  
539,000,000 YBN
461) The first circulatory system (blood cells actively moved by muscle
contraction) evolves in bilaterians.

Circulatory systems can be divided into two kinds, "open" and "closed", both
which contain a circulatory fluid or blood. In an open circulatory system, the
blood and body cavity (hemocoelic) fluid are one and the same; the blood, often
called hemolymph, empties from vessels into the body cavity (hemocoel) and
directly bathes organs. In a closed circulatory system blood is kept separate
from the coelomic {SElomiK} fluid. Circulatory systems, open or closed,
generally have structural mechanisms for pumping the blood and maintaining
adequate blood pressures. Beyond the influence of general body movements, most
of these structures fall into the categories: contractile vessels (as in
annelids); osiate hearts (as in arthropods); and chambered hearts (as in
molluscs and vertebrates). The method of initiating contraction of these
different pumps (the pacemaker mechanism) may be intrinsic (originating within
the muscles of the structure itself) or extrinsic (originating from motor
nerves from outside the structure).

Nemerteans, cylindrical worms evolved from an earlier ancestor, have a network
of blood channels in the mesenchyme (undifferentiated tissue between organs)
but have no heart or pumping vessel. This bilaterian, a coelomate (the earliest
of which are the molluscs), like some surviving coelomates, has a series of
channels or blood spaces outside the coelom tissue, that form a circulatory
system, often with muscle cell contractible walls connected to the larger
vessels that act as pumps to move the blood cells through the channels.
  
539,000,000 YBN
506)
  
537,000,000 YBN
341) The Lophotrochozoa (Trochozoa) Phylum Nemertea {ne-mR-TEu} (ribbon worms).
  
537,000,000 YBN
344) The Lophotrochozoa Phylum Sipuncula (peanut worms) evolve.
  
533,000,000 YBN
342) Trochozoa Mollusks evolve.

The phylum name is derived from mollis, meaning soft, referring to the soft
body within a hard calcareous shell. Soft-bodied mollusks make extensive use of
ciliary and mucous mechanisms in feeding, locomotion, and reproduction. The
Mollusca are a successful phylum with probably over 110,000 living species,
more than double the number of vertebrate species. More than 99% of living
molluscan species belong to two classes: Gastropoda {GaSTroPeDu} (snails) and
Bivalvia (muscles and clams). These two classes can make up a dominant fraction
of the animal biomass in many natural communities, both marine and
fresh-water.

The haemocoel forms the major body cavity of molluscs, usually in the form of
several large, connected sinuses. Haemocyanin is the chief oxygen-carrying
blood pigment, although a number of species have haemoglobin. A heart of
variable complexity is usually present. A coelomic space is represented by the
pericardium, kidneys and gonads.

Among the most primitive mollusks are the Aplacophora which do not have shells
but their epidermis secretes aragonite (calcareous) spicules and their body has
a repetition of structures along their front-back (antero-posterior) axis.
Mollusks are thought, by some, to be descended from a segemented worm (annelid)
because of this segmented repetition of structure which is lost in most of the
other later evolved mollusks. But others think mollusks descend from a
nonsegmented ancestor.

An early Cambrian fossil mollusk named Maikhanella, which has a shell made from
sclerites that are only loosely fused together, implies that after millions of
years of evolution the spines become more fused into a single, rigid shell
familiar in mollusks of the present time.

Among the earliest fossil mollusks known from the Cambrian are simple
cap-shaped shells, similar to an extant mollusk named "Neopilina". Neopilina is
clearly a mollusk with a single cap-shaped shell secreted by the mantle, as
well as a mouth, digestive tract, anus, and gills. But unlike all other known
mollusks alive today, Neopilina still retains the segmentation of its worm-like
ancestors. Around the body are segemented gills, kidneys, hearts, gonads, and
paired retractor muscles to pull down the shell.

Beyond the difference in segmentation, in terms of skeleton, some annelids have
chaetae which are tiny, spinelike structures and are derived from single
epidermal cells, while mollusks are covered by a thick sheet of skin called a
mantle which secretes a hard calcareous (KaL-KAREuS} (calcium) skeleton
(aragonite or calcite), either as tiny sclerites or as plates. A sclerite
{SKli-rIT} is a chitinous or calcareous plate, spicule, or similar part of an
invertebrate, especially one of the hard outer plates forming part of the
exoskeleton of an arthropod. In addition annelids have a well developed coelon
and a closed circulatory system while mollusks have a reduced coelon and an
open circulatory system.
  
530,000,000 YBN
338) The Ecdysozoa Phylum Arthropoda "Arthropods" evolve (includes crustaceans
and insects).

Arthropods can be compared to a segmented worm encased in a rigid exoskeleton.

The phylum Arthropoda is the largest phylum in the animal kingdom. Arthropoda
consists of more than one million known invertebrate species in four subphyla:
Uniramia (includes insects), Chelicerata (includes arachnids and horseshoe
crabs), Crustacea (crustaceans), and Trilobita (trilobites). All arthropods
have a segmented body with bilateral symmetry covered by an exoskeleton
containing chitin, which serves as both armor and as a surface for muscle
attachment. Each body segment may have pair of jointed appendages. The phylum
includes carnivores, herbivores, omnivores, detritus feeders, filter feeders,
and parasites in both aquatic and terrestrial environments.
  
530,000,000 YBN
339) The Ecdysozoa Phylum Onychophora (onychophorans) evolves.

Onychophorans, know as "velvet worms", are the living transitional form between
worms and arthropods. Although they have segmented worm-like bodies, they also
have jointed appendages, antennae, and shed their cuticle like arthropods do.
  
530,000,000 YBN
340) The Ecdysozoa Phylum Tardigrada (tardigrades) evolves.

Tardigrades are slow-moving, microscopic invertebrates, related to the
arthropods. Tardigrades have four body segments, eight legs, and live in water
or damp moss. Tardigrades are also called "water bears".
  
530,000,000 YBN
343) The Lophotrochozoa (Trochozoa) Phylum Annelida (segmented worms) evolves.

Annelids are various worms or wormlike animals, characterized by an elongated,
cylindrical, segmented body and including the earthworm and leech.
  
530,000,000 YBN
350) Chordata Vertebrates evolve. This Subphylum, Vertebrata, contains most
fishes, and all amphibians, reptiles, mammals, and birds.

The characteristic features of the Vertebrata are a vertebral column, or
backbone, and a cranium, which protects the central nervous system (brain and
spinal cord) and major sense organs.

Vertebrates evolved from a lower chordate similar to the present-day
Cephalochordata (lancelets). Vertebrates originate in fresh water and develop a
kidney as their organ of water balance. The main line of evolution in the
vertebrates which leads to the tetrapods remains in fresh waters, however,
several vertebrate lines invade the oceans.
  
530,000,000 YBN
351) Vetebrates Jawless fish (agnatha) evolve.

Some extinct jawless fish, that lived in the Devonian 'Age of Fish', such as
ostracoderms, had hard, bony armor plating.
  
530,000,000 YBN
386) Earliest vertebrate and fish fossil.

Haikouichthys ercaicunensis: About 25 mm in length.
(Chengjiang) Kunming, Yunnan Province, China  
525,000,000 YBN
6329) Earliest hemichordate fossil: a Pterobranch "graptolite".
(Chengjiang Konservat-Lagerstätte) Yunnan Province, China  
521,000,000 YBN
137) Start of Sirius Passet fossils in Canada, early Cambrian fossils (521
mybn).

  
520,000,000 YBN
133) Earliest trilobite fossils.

Trilobites are numerous extinct marine arthropods of the Paleozoic Era.
Trilobites have a segmented body divided by grooves into three vertical lobes
and are found as fossils throughout the world.

There is a transition, after the soft-bodied (unshelled) organisms of the
Ediacaran are the earliest small cylindrical shells of Cloudina and
Sinotubulites, later in the Proterozoic, to the clam-like shells of the
brachiopods in the Tommotian (Early Cambrian) to the segmented calcite and
chitin shells of the trilobites in the Atdabianian.

One fossil arthropod, known as aglaspids, may be related to both trilobites and
horseshoe crabs. Horseshoe crabs are not true crabs, but instead are members of
the group known as the Chelicerata- a group that includes spiders and
scorpions. True crabs are a family within the Crustacea, a different group
entirely. So horseshoe crabs may be descended from trilobites.

The segmented shell of the trilobite, which provides more movement then the
clam shell may have been a selective advantage. (verify)

The largest known trilobite, Isotelus rex, reached 72 centimeters in length.
  
520,000,000 YBN
134) Trilobite, Brachiopod, and Echinoderm fossils abundant all over earth.

  
520,000,000 YBN
135) Start of Chengjiang fossils in China, early Cambrian fossils (520 to 515
mybn).

  
520,000,000 YBN
144) Two agnathan (jawless) lamprey-like and primitive hagfish fossils found in
Chengjiang.

  
520,000,000 YBN
148)
  
520,000,000 YBN
6296) Earliest worm fossil, a Chaetognath {KETOnat} (arrow worm).

The fossil is a member of the phylum Chaetognatha (also called arrow worm),
with only about 100 living species, is found in oceans throughout the world and
plays an important role in the food web as primary predators
(Maotianshan Shale ) near Haikou, Kunming, China  
517,000,000 YBN
115) Earliest certain Echinoderm fossils, Helicoplacus.

Helicoplacoids are stem group echinoderms with spiral plating and three
ambulacra arranged radially around a lateral mouth. They are the most primitive
echinoderms and the first to show a radial arrangement of the water vascular
and ambulacral systems. Unlike later echinoderms, their skeleton shows no
dorsal/ventral (aboral/oral) differentiation. They were probably sedentary
suspension feeders.

One theory is that Echinoderms evolved from sessile filter feeding organisms
similar to Pterobranchs.
(Poleta Formation) Bishop, California, USA  
513,000,000 YBN
6351) Ancestor of all Arthropod Crustacea (shrimps, crabs, lobsters,
barnicles).

The earliest crustacean fossils are from the early Cambrian (542-513 MYBN) of
Shropshire, England.

Molecular phylogenetics has suggested to some that the subphylum Crustacea may
be paraphyletic including the Hexapods within it, and so the Hexapoda and
Crustacea have been named Pancrustacea. Not all experts agree that Crustacea is
paraphyletic, some put hexapods as descended from the Atelocerata, a
hypothetical ancestor of both myriapoda and hexapoda that split from the
crustaceans before the Myriapod and Hexapod branching, citing complex
anatomical features shared by Myriapod and Hexapod and not the crustaceans that
would need to be independently evolved, in particular the tentorium {internal
head skeleton}, tracheae {fine respiratory tubules}, and Malpighian tubules of
the Myriapods and Hexapods).
(earliest fossils) Shropshire, England  
507,000,000 YBN
136) Start of Burgess shale fossils in Canada, middle Cambrian fossils (507
mybn).

  
507,000,000 YBN
140) Aysheaia (onychophoran, also described as lobopod) fossil, from Burgess
shale.
  
507,000,000 YBN
141) Sponge fossil, from Burgess shale.

  
507,000,000 YBN
142)
  
507,000,000 YBN
143)
  
507,000,000 YBN
145) Priapulid worm fossils of Burgess Shale.
  
507,000,000 YBN
146) Opabinia fossils of Burgess Shale.
  
507,000,000 YBN
147) Anomalocaris fossils of Burgess Shale.
  
507,000,000 YBN
149)
Burgess Shale  
505,000,000 YBN
74) Oldest fossil of an arthropod in the process of moulting (ecdysis), the
soft-bodied arthropod Marrella splendens.
(Burgess Shale) British Columbia, Canada.  
505,000,000 YBN
6291) Early Chordata fossil "Pikaia".
(Burgess Shale) Mount Wapta, British Columbia  
501,000,000 YBN
6348) Arthropod subphylum Myriapoda {mEREaPeDu} (centipedes and millipedes).

The earliest possible Myriapoda fossil are marine fossils from the middle
Cambrian of Utah and the late Cambrian (488-501 MYBN) of East Siberia, and the
earliest certain Myriapod fossils, are land Myriapods from the late Silurian
(416 MYO) from Shropshire, England.
(earliest possible fossils Marine deposits)(Wheeler Formation) Utah, USA and
(Ust-Majan formation) East Siberia|(earliest fossils) Shropshire, England  
495,000,000 YBN
138) Start of Orsted fossils in ???, late Cambrian fossils (495 mybn).

  
488,300,000 YBN
121) End of the Cambrian (542-488.3 mybn), and start of the Ordovician
{ORDiVisiN} (488.3-443.7 mybn) Period.
  
488,000,000 YBN
6314) The Ordovician radiation.
During the Ordovician (488-444 million years ago), the
number of genera will quadruple.
  
488,000,000 YBN
6349) Arthropod subphylum Chelicerata (KeliSuroTo) (horseshoe crabs, mites,
spiders, scorpions).

Chelicerata probably appeared during the Cambrian period. By the late
Cambrian there is evidence for both Pycnogonida and Euchelicerata. The earliest
pycnogonid (sea spider) fossils are larval sea spiders from the Late Cambrian
(488-501 MYO), Orsten of Sweden.
(sea spider fossils, Orsten) Sweden  
475,000,000 YBN
244) Non-vascular plants evolve, Bryophyta, (ancestor of Liverworts, Hornworts,
Mosses).

The Bryophytes are the simplest land plants, and reproduce with spores.

The Division Bryophyta contains green, seedless land plants that contain at
least 18,000 species and are divided into three classes: mosses, liverworts,
and hornworts. Bryophytes are distinguished from vascular plants and seed
plants by the production of only one spore-containing organ in their
spore-producing stage. Most bryophytes are 2-5 cm (0.8-2 in.) tall. Bryophytes
are found throughout the surface of earth, from polar regions to the tropics,
they are most abundant in humid environments, though none is marine. Bryophytes
are extremely tolerant of dry and freezing conditions.
  
475,000,000 YBN
352) Jawless fish lampreys and hagfish lines separate.

  
475,000,000 YBN
398) Plants live on land. Earliest fossil spores belonging to land plants.
These spores look like the spores of living liverworts and Cooksonia.

Plants conquer land before animals do, and like animals may move to land not by
sea but by freshwater.
Caradoc, Libya  
472,000,000 YBN
402) The first animals live on land, arthropods Myriapoda (centipedes and
millipedes).

The earliest fossil land tracks are from the Ordovician and are at least 472
MYO. The organism that produced these fossil tracks is possibly an
Euthycarcinoidea, a rare arthropod group thought to be descended from the
Myriapods.

Marine stem-group hexapods support the theory that the invasion of the land
occurred independently by the Myriapoda and Hexapoda. Adaptation to life on
land also occurred independently in the Crustacea (Isopoda), Cheliceriformes
(Chelicerata), Tardigrada, and Onychophhora.
(earliest arthropod tracks) Kingston, Ontario, Canada  
470,000,000 YBN
234) Non-vascular plants Hornworts.
  
460,000,000 YBN
84)
Wisconsin, USA  
460,000,000 YBN
235) Non-vasular plants Mosses.
  
460,000,000 YBN
353) Jawed vertebrates evolve, Infraphylum Gnathostomata {no toST omoTo}. This
large group includes all jawed fish, amphibians, reptiles, mammals, and birds.
First vertebrate teeth.

The jaw evolves from parts of the gill skeleton. The earliest jawed
vertebrates, have no bone, there skeleton is made of cartilage. Humans have
cartilage too, for example, in the lining of joints and the human skeleton
starts as flexible cartilage in the embyro. Most of the human skeleton becomes
ossified when mineral crystals, mostly calcium phosphate, become integrated
into the skeleton. Except for teeth, the shark skeleton never undergoes this
mineral transformation. Sharks lack the swim bladder of the later bony fish,
and many sharks have to swim continuously to maintain their desired level in
the water. Sharks and rays almost all live in the sea. Unlike the bony fish, no
sharks ever climb onto land. Sharks have been the top of the food chains of the
sea for hundreds of millions of years. The largest shark known is the whale
shark, Rhincodon typus, which can be up to 12 meters long and weigh 12 tons.
Oceans  
460,000,000 YBN
404) Jawed fishes Chondrichthyes {KoN-DriK-tE-EZ} (Cartilaginous fishes:
ancestor of all sharks, rays, skates, and sawfishes).

The fossil record of Chondrichthyans dates to around 455 million years ago, but
the earliest Chondrichthyan fossil dates to 409 million years ago.
  
450,000,000 YBN
158)
  
443,700,000 YBN
122) End of the Ordovician (488.3-443.7 mybn), and start of the Silurian
(443.7-416) Period.
  
443,000,000 YBN
90) End-Ordovician mass extinction. 60% of all genera are observed extinct.

Many species go extinct, mostly trilobites, echinoderms, corals, nautiloids,
brachiopods, graptolites, conodonts, and acritarchs.
  
440,000,000 YBN
236) Vascular plants evolve (Phylum: Tracheophytes).

Vascular plants are any plant that has a specialized conducting system
consisting mostly of phloem (food-conducting tissue) and xylem
(water-conducting tissue), collectively called vascular tissue. The phloem
transports sugar and the xylem transports water and salts. Ferns, gymnosperms,
and flowering plants are all vascular plants. In contrast to the nonvascular
bryophytes, where the gametophyte is the dominant phase, the dominant phase
among vascular plants is the sporophyte. Because they have vascular tissues,
these plants have true stems, leaves, and roots, modifications of which enable
species of vascular plants to survive in a variety of habitats under diverse,
even extreme, environmental conditions. This ability to flourish in so many
different habitats is the primary reason that vascular plants have become
dominant among terrestrial plants.

Earliest spores of vascular plants.
  
440,000,000 YBN
360) Ray-finned fishes (Jawed, Class Osteichthyes, Subclass Actinopterygii)
evolve. This is the fist bony fish (Osteichthyes) which includes the
ray-finned, lobefin, and lung fishes. Bony-fish have a skeleton at least partly
composed of true bone. Other features include, in most species, a swim bladder
(an air-filled sac to give buoyancy), gill covers over the gill chamber, bony
platelike scales, a skull with sutures, and external fertilization of eggs.

Most of the ray-finned fish are known as teleosts. They exist in both salt and
freshwater. The name ray is because their fins have a skeleton similar to a
handheld fan. The teleost fish are a very successful evolutionary line, with
about 23,500 species, 30 times the number of shark species.

Fish with a swim bladder use the bladder to change their depth, to sink, the
fish absorbs some molecules of gas from its swim bladder into the blood which
reduces the volume of the bladder, to rise, the fish does the reverse,
releasing molecules of gas from the blood into the swim bladder increasing the
volume of the bladder.

Some teleost fish can gulp air from the surface, but still use their gills to
extract oxygen from the oxygenated gill water. However, the lung does not
evolve from gills but from the swim bladder. The swim bladder appears to have
evolved from a primitive lung, and some surviving teleosts, for example
bowfins, gars and bichirs (BiCRZ), still use the swim bladder for breathing.

The Anabas and mudskipper are two teleost fish that can walk over land. The
mudskipper can crawl on land using its pectoral (arm) fin muscles which can
support its weight, and eats insects and spiders.
Ocean and fresh water  
440,000,000 YBN
6172) The first lung evolves, in ray-finned fishes, from the swim bladder. Some
surviving teleosts, such as bowfins, gars, and bichirs still use their swim
bladder for breathing. Fish that breathe air through their gill chamber evolved
breathing through a completely different route than those fish that breathe
with a lung.

Bichirs (BiCR) are among the most primitive of the ray-finned fishes. Instead
of the swim bladder of most ray-finned fishes, the bichir has a pair of lungs,
which enables it to survive out of water for several hours.
Ocean (presumably)  
425,000,000 YBN
377) Jawed fishes, Lobefin fishes evolve. Coelacanths. Lobefin fish have a
fleshy lobe at the base of each fin.
There are 2 living species of coelacanths
known.

The Coelacanths are well known in the fossil record, but were thought to have
gone extinct before the dinosaurs, but are found to be still alive in 1938.
  
420,000,000 YBN
6350) Arthropods Hexapoda {HeKsoPeDu} (arthropods with six legs, includes all
insects).
The closest relative of the Hexapoda is most likely the Branchiopoda, the brine
shrimps and their
allies.

The earliest hexapod fossils are 396 million years old and from the Rhynie
chert of Scotland. They are Rhyniella praecursor and a pair of mandibles
described as Rhyniognatha hirsti.

The proturans, (class Protura), are any of a group of about 150 species of
minute (0.5 to 2 mm), pale, wingless, blind, primitive insects that live in
damp humus and soil and feed on decaying organic matter. Proturans, frequently
known as telsontails, include some of the most primitive hexapods.

The first major division among hexapods is between Entognatha and Ectognatha.
Ectognatha are more widely known as the Insecta. In entognaths the mouthpart
appendages are recessed within a gnathal pouch on the head capsule. Ectognathy
is more primitive and all other hexapods have ectognathous mouthparts.
(Rhynie chert) Scotland  
417,000,000 YBN
378) Lobefin fish, Lungfishes.

There are only six species of lungfish alive today. The Australian lungfish has
a single lung, the others have two. The African and South American species bury
themselves in mud during the dry season, breathing air through a little
breathing hole in the mud.

The earliest fossil lungfish dates to around this time.
  
416,000,000 YBN
123) End of the Silurian (443.7-416 mybn), and start of the Devonian {DiVONEiN}
(416-359.2 mybn) Period.
  
415,000,000 YBN
401) Earliest fossil of land plant, Cooksonia. This is also the oldest fossil
of a vascular land plant.

Cooksonia is only a few centimeters tall. It has slender, leafless branches
with Y shaped forks, topped by capsules that relase microscopic spores. Some
fossils have a dark stripe in their stems which may be the remains of vascular
tissue, used by plants to move water.

They have been found in an area stretching from Siberia to the Eastern USA, and
in Brazil. They are found mostly in the area of Euramerica, and most of the
type specimens are from Britain.
(Wenlock strata) Devilsbit Mountain district of County Tipperary, Ireland  
410,000,000 YBN
6352) The most primitive living insects are the order Archaeognatha, the
Bristletails, of which there are around 500 known species. The members of this
order are distinctive because their mandibles connect with the head capsule in
only one place (monocondylic). The mandibles of all other insects have two
points of articulation with the head (dicondylic). Other ancestral features of
Archaeognatha include their method of reproduction in which species do not
copulate and sperm transfer is indirect even though fertilization is
internalized.

In the most primitive wingless insects (apterygotes) such as the silverfish
Lepisma, there is almost no change in form throughout growth to the adult.
These are known as ametabolous insects.

Engel and Grimaldi write: "...By most measures of evolutionary success, insects
are unmatched: the longevity of their lineage, their species numbers, the
diversity of their adaptations, their biomass, and their ecological impact.
...".

The insects co-radiate with angiosperms; 85% of the 250,000 species of
angiosperms are pollinated by insects. The diversity of flowers is due in large
part to the insects lured to them.
  
410,000,000 YBN
6354) Early arachnid fossils: trigonotarbids, spider-like arthropods with
lung-books, the typical breathing organs of most of the larger recent living
Arachnids.
Unlike true spiders, Pleophrynus lacks poison and silk glands.
(Rhynie chert) Scotland  
410,000,000 YBN
6363) Dicondylic insects (insects in which the mandible has two points of
articulation with the head instead of one). Ancestor of Insects Zygentoma
(Silverfish). Silverfish and all pterygota (winged insects) have dicondylic
mandibles. This second articulation results in the movement of the mandible
being roughly confined to a single plane of motion instead of the rotating
motion possible in Archeognatha (bristletails) and Entognatha (springtails and
relatives).

Silverfish have more in common with insects than the more primitive
bristletails.
  
400,000,000 YBN
159)
  
400,000,000 YBN
399) Earliest fossil of an insect; thought to be a winged insect.

The oldest known insect fossil for which there is significant remaining
structure (head and thorax fragments) is a bristletail (Archaeognatha),
estimated to be 390 to 392 million years old.
Rhynie Chert , Scotland (and Gaspé Peninsula of Québec, Canada)  
390,000,000 YBN
411) The first flying animal, an arthropod insect. Ancestor of all winged
insects (Pterygota {TARiGOTu}) (Mayflies, Dragonflies, Damselflies).

The most primitive living pterygotes are the Ephemeroptera (Mayflies) and the
Odonata (Dragonflies and damselflies). Unlike most other flying insects both
the Ephemeroptera and Odonata have freshwater aquatic larvae, presumed to be an
ancestral habit.

Arthropods evolve flight 90 million years before the first flight among
vertebrates.

Insect wings evolved only once, and all winged insects descend from the first
winged insect.

How flight evolved in insects is still debated. A terrestrial origin of
pterygotes is supported by the fact that the most basal insects (apterygotes),
the Zygentoma and Archeognatha are fully terrestrial. One theory suggests that
wings develop as fixed extensions to the thoracic terga, called paranotal
lobes. The paranotal lobes provide early insects with the ability to glide, and
eventually to control the aerial descent of the insect from perches of tall
plants, and from one Carbiniferous gymnosperm sporangia (which are located on
branchlets) to another. Another theory has the wing evolving like the movable
abdominal gills on aquatic naiads of mayflies which look like tiny wings and
move in a similar way. The development of wings may have helped early insects
to escape predators.

The earliest full body imprint fossil of a flying insect is like a may-fly
(Ephemeropterida) that landed in soft mud, during the late Carboniferous
(318-299 mybn) around a fresh water habitat in Massachusetts. Some wing
impressions from the Czech Republic date to 324 mybn.

The Pterygota is the larger of two subclasses of Insecta. All have wings in the
adult stage or have lost their wings secondarily.

Some interesting facts about Mayflies are:
-The subimagos of mayflies are the only
insects that molt when they have wings.
-Mayflies have paired genital openings. During
copulation, the two penes of the male are inserted simultaneously into the two
openings of the female. Sperm is transferred quickly (there is no
spermatophore) and eggs are fertilized immediately.
-A few species of mayflies reproduce
parthenogenically -- no males have ever been found.
-Although most mayflies are
herbivores, a few are predaceous.
-Adult mayflies do not feed. Their digestive system is
filled with air, making them light enough to float.
-Some mayfly species require up to
four years to complete development. In that time they may molt more than 20
times.
(Wamsutta Formation) southeastern Massachusetts and Upper Silesian Basin, Czech
Republic  
386,000,000 YBN
406) Oldest fossil spider (Attercopus {aTRKoPuS}).
These spiders represent the first use of
silk by animals.
(Givetian of) Gilboa, New York  
385,000,000 YBN
405) The first forests. Earliest large trees fossils.

First progymnosperms (treelike plants).
Gilboa, New York, USA  
380,000,000 YBN
6330) The fish "Tiktaalik" {TiK ToLiK}, an important transition between fish
and amphibian.
(Fram Formation) Nunavut Territory, Canada  
375,000,000 YBN
380) The first tetrapods (organisms with four feet), the amphibians evolve in
fresh water. The first vertebrate limbs (arms and legs) and fingers. Ancestor
of caecillians, frogs, toads, and salamanders.

Almost no amphibians live in sea water.

The earliest fossil amphibian is Elginerpeton, found in Scotland, dates back
368 million years.The earliest well known amphibians come from around 360
million years ago, and are Acanthostega and Ichthyostega. Acanthostega
represents the most primitive tetrapod that has hands and feet for which there
is a full skeleton. Acanthostega has eight toes per limb, no fin rays, a large
load-bearing pelvis and is thought to have retained gills into adulthood.
Ichthyostega is a large carnivore, ranging in size from 0.5 - 1.2 m. The
earliest known Ichthyostega comes from 363 million year old deposits in
Greenland (then on the equator). Ichthyostega is largely aquatic but has
massive broad ribs that may be used for support of internal organs while on
land.
Fresh water, Greenland (on the equator)  

SCIENCE
375,000,000 YBN
2599)
Ellesmere Island, Nunavut, in northern Canada  
368,000,000 YBN
407) Oldest amphibian (and tetrapod) fossil.
Tetrapods are four-limbed, vertebrate
animals (all vertebrates except fish).
Elgin, Morayshire, Scotland  
367,000,000 YBN
408) Late Devonian mass extinction caused by ice age. 57% of all genera are
observed extinct.

70% of all species go extinct. This include 3 of 5 trilobite orders, 90% of
brachiopod genera, and major loss of reefs.
  
365,000,000 YBN
160)
  
363,000,000 YBN
379) The first vertebrates live on land (amphibians).
Fresh water, Greenland (on the equator)  
360,000,000 YBN
237) Vascular plants ferns evolve.

Ferns are are flowerless, seedless vascular plants having roots, stems, and
fronds (the leaf-like part of a fern or leaf of a palm) and reproducing by
spores.

There are around 12,000 species of Ferns (Plant division Pteridophyta), which
are nonflowering vascular plants that have true roots, stems, and complex
leaves and reproduce by spores. The life cycle is characterized by an
alternation of generations between the mature, fronded form (the sporophyte)
familiar in greenhouses and gardens and the form that strongly resembles a moss
or liverwort (the gametophyte).
  
360,000,000 YBN
6353) The Neoptera, folding wing insects. Neoptera, means "new wing".

Ephemeroptera and Odonata, the most primitive living pterygota, do not live on
the ground. It seems likely that selective pressures on the first winged
insects heavily favor the development of some mechanism for folding the wings
against the body after landing, making them less conspicuous, less awkward, and
less susceptible to breakage. The neoptera represent a remarkably successful
lineage and are the ancestors of all "higher" orders of insects.

Unfoldable wings appear in butterflies and various moths, in many dipterans and
some hymenopterans.
(Fossil: Archimylacris eggintoni, Coseley Lagerstätte) Staffordshire, UK  
359,200,000 YBN
124) End of the Devonian (416-359.2 mybn), and start of the Carboniferous
(359.2-299 mybn) Period.
  
359,000,000 YBN
243)
Scotland  
350,000,000 YBN
361) Ray-finned fishes, (Chondrostei), Sturgeons and Paddlefish.
  
350,000,000 YBN
362) Ray finned fishes: Bichirs evolve.
  
350,000,000 YBN
6355) The Neoptera: Dictyoptera {DiKTEoPTRu} (Cockroaches, Termites, and
Mantises).

Paleozoic "roachoids" are among the most abundant animals that live in the
extensive coal swamps of the Carboniferous. Earliest fossils are from the early
part of the Late Carboniferous (around 320 MYBN).
  
340,000,000 YBN
384) The hard-shell egg evolves. The Amniota {aMnEOtu} (ancestor of reptiles,
mammals and birds). The hard-shell egg is waterproof. This is the start of
vertebrate internal fertilization, because on land the egg cannot be fertilized
as most fishes and amphibians do, by a male swimming near the eggs and spraying
them with sperm. Amniote males and females must copulate so that the sperm can
reach the eggs inside the female. Much of the development of Amniote fetuses
occurs inside the female, not in the water.

Amniotes (reptiles, mammals, and birds) are distinguished from non-amniote
tetrapods (amphibians) by the presence of complex embryonic membranes. One of
these, the amnion, gives its name to the group.

This group of tetropods, the Amniota, will branch into Sauropsida
{SOR-roP-SiDu} (which includes reptiles and birds) and Synapsida {Si-naP-Si-Du}
(which includes mammals).

All living amniotes (reptiles, birds, and mammals) lay hard-shelled eggs,
except in most mammals and some snakes and lizards, where egg laying has been
replaced by live birth.

The earliest known amniotes, Westlothiana (~338 MY) and Hylonomus (~300 MY),
are also the earliest known reptiles.
Bathgate, West Lothian, Scotland  
338,000,000 YBN
410) Earliest amniote fossil.

The next earliest amniote fossil is Hylonomus, a small lizard-like reptile that
was trapped in the trunk of a swamp tree in what is now Joggins, Nova Scotia,
Canada (~300 MYBN).
Bathgate, West Lothian, Scotland  
335,000,000 YBN
6331) The tetrapod Amniota divide into the Sauropsida {SOR-roP-SiDu} (which
includes reptiles and birds) and the Synapsida {Si-naP-Si-Du} (which includes
mammals).

The Sauropsida include birds, dinosaurs and modern reptiles. Sauropsids have
two major lineages: the Parareptilia (turtles) and the Eureptilia (dinosaurs,
crocodiles and birds).

The Synapsida are a subclass of extinct amniota from which mammals descend.
Synapsids are sometimes called "mammal-like reptiles" but it is incorrect to
call them reptiles because they diverge at the beginning of amniote evolution,
before the reptiles do. There are two major groups of synapsids: pelycosaurs
(sail-backed) and therapsids (mammal-like).

The earliest Sauropsid fossils, are Lethiscus(~ 330 MYA) and Westlothiana (~328
MY) from Scotland. The earliest Synapsid fossil is Protoclepsydrops (~314 MY)
from Joggins, Nova Scotia, although some people reject the Protoclepsydrops
fossil in favor the next oldest possible synapsid fossils, such as Echinerpeton
and Archaeothyris from Florence, Nova Scotia (~307 MY).
(earliest possible Synapsid fossil: Cumberland group, Joggins formation.)
Joggins, Nova Scotia, Canada  
330,000,000 YBN
409)
  
330,000,000 YBN
6307) The Synapsids Pelycosauria {PeLiKuSOREu} evolve (includes Edaphosaurus
{eDaFoSORuS}, Dimetrodon).

There are two main groups of synapsids: pelycosaurs (sail-backed reptiles) and
therapsids (mammal-like reptiles). Pelycosaurs arise in the mid-Carboniferous
from cotylosaurs and soon enjoy an extensive radiation through the early
Permian, coming to constitute about half of the known amniote genera of the
time. Some like Edaphosaurus are herbivorous, however, most are carnivores that
prey on fish and aquatic amphibians. Pelycosaurs differ in size but not in
design. The most notable feature in some species is a broad "sail" along the
back consisting of an extensive layer of skin supported internally by a row of
fixed neural spines projecting from successive vertebrae. If the sail is
brightly colored, it might have been used in courtship or in bluff displays
with rivals, similar to ornamentations in birds. The sail may be a sun light
collector: when turned broadside to the sun, blood moving through the sail is
heated, then carried to the rest of the body. Somewhat suddenly pelycosaurs
decline in numbers and are extinct by the end of the Permian. Therapsides
evolve from them, and largely replace the Pelycosauria for a time as the
dominant terrestrial vertebrates.
  
325,000,000 YBN
381) The Amphibians: Caecilians evolve.
  
320,000,000 YBN
238) Gymnosperms evolve. Gymnosperm is Greek for "Naked Seed". Gymnosperms are
the earliest surviving seed plants, Spermatophyta, and ancestor of all Cycads,
Ginkos and Conifers) evolve.

The most primitive extant Gymnosperms, the Cycads evolve now.

The earliest known seed bearing plants are the Pteridosperms, seed ferns known
only from the fossil record. Gymnosperms are the most primitive seed bearing
plants still living.

A gymnosperm is any woody plant that reproduces by means of a seed (or ovule)
in direct contact with the environment, as opposed to an angiosperm, or
flowering plant, whose seeds are enclosed by mature ovaries, or fruits. The
four surviving gymnosperm divisions are Pinophyta (conifers, the most
widespread), Cycadophyta (cycads), Ginkgophyta (ginkos), and Gnetophyta (a
small division with only three genera). More than half are trees; most of the
rest are shrubs. Those widely found in the Northern Hemisphere are junipers,
firs, larches, spruces, and pines; in the Southern Hemisphere, podocarps. The
wood of gymnosperms is often called softwood to differentiate it from the
hardwood of angiosperms. Many timber and pulp trees are also planted as
ornamentals. Gymnosperms also are a minor source of food; of essential oils
used in soaps, air fresheners, disinfectants, pharmaceuticals, cosmetics, and
perfumes; of tannin, used for curing leather; and of turpentines. Gymnosperms
were a major component in the vegetation that was compressed over millions of
years into coal. Most are evergreen. They produce male and female reproductive
cells in separate male and female strobili.
  
320,000,000 YBN
6356) The Neoptera: Orthoptera evolve (Crickets, Grasshoppers, Locusts, Walking
sticks).

The Orthoptera and the later Hemiptera are termed hemimetabolous, and are said
to undergo incomplete metamorphosis. In incomplete metamorphosis, the general
form is constant until the final molt, when the larva undergoes substantial
changes in body form to become a winged adult with fully developed genitalia.

Many insects in the order Orthoptera produce sound (known as a "stridulation")
by rubbing their wings against each other or their legs, the wings or legs
containing rows of corrugated bumps. The tympanum or ear is located in the
front tibia in crickets, mole crickets, and katydids, and on the first
abdominal segment in the grasshoppers and locusts.


One characteristic of Orthoptera are jumping hind legs and a thick femur packed
with muscles. Orthopterans are the most "vocal" of all the orders, with calling
behavior playing a major role in the biolkogy and evolution of the order.
Mating calls are critical to recognize many species. Males regularly chorus on
warm evenings for females. Sound is produced wither by rubbing a specialized
area of the wing against a corresponding area on the other, overlapping
forewing or by scraping the legs against stiff edges of the forewings. Scrapers
of files are used to create the rasping sounds which are amplified by the
specialized membranes of the wings called "mirrors".

The earliest Orthoptera fossils are from the Late Permian of France.
  
320,000,000 YBN
6364) Neoptera: Plectopterida (Stoneflies, webspinners, and zorapterans).
  
317,000,000 YBN
385) Sauropsids Reptiles evolve (ancestor of all turtles, crocodiles,
pterosaurs, dinosaurs and birds).

The class Reptila contains approximately 8,700 species and is a group of
air-breathing vertebrates that have internal fertilization, and with the
exception of the birds, have a scaly body, and are cold-blooded. Most species
have short legs (or none), long tails, and lay eggs. Living reptiles include
the scaly reptiles (snakes and lizards: Squamata), the crocodiles (Crocodylia),
the turtles (Testudines), and the unique tuatara (Sphenodontida). Being
cold-blooded, reptiles are not found in very cold regions; in regions with cold
winters, reptiles usually hibernate. Reptiles range in size from geckos that
measure about 3 cm (1 in.) long to the python, which grows to 9m (30 ft); the
largest turtle, the marine leatherback, weighs about 1,500 lb (680 kg). Extinct
reptiles include the dinosaurs, the pterosaurs, and the dolphin-like
ichthyosaurs.
(Joggins Formation) Nova Scotia, Canada  
315,000,000 YBN
453) Allegheny mountains form as a result of the collision of Europe and
eastern North America.
Add other mountain range origins too.
  
310,000,000 YBN
6357) The Neoptera: Paraneoptera (bark lice, true lice, thrips, and the
Hemiptera {HemiPTRu} who have mouthparts adapted for piercing and sucking:
Cicadas, Aphids, and "true bugs": such as Bed bugs, and Stink bugs).

The evolutionary history of the Paraneoptera is reflected in structure and
function of their mouthparts. There is a general trend from the "picking"
mouthparts of bark lice with standard insect mandibles, to the probing and
puncturing mouthparts of thrips and anopluran lice, and the distinctive
piercing-sucking rostrum or beak of the Hemiptera.

The Paraneopteran family tree splits into two major branches, one with the lice
and the other with the thrips and Hemiptera (aphids, cicadas and Heteroptera:
the true bugs). The bark-lice and book lice are very basal Paraneopterans.

Not long after the piercing and sucking mouthparts evolve, Hemiptera divides
into two sister groups. In one group, Homoptera, (leafhoppers, cicadas, aphids,
etc.) , the rostrum is relatively short (1-3 segments) and emerges from near
the ventral posterior margin of the head. In members of the second group,
Heteroptera, the rostrum is relatively long (3-4 segments) and arises near the
front or lower front of the head (prognathous or hypognathous). These insects
are known as the "true bugs".
  
310,000,000 YBN
6359) Ancestor of all Neoptera Holometabola: Holometabolous insects (beetles,
bees, true flies, and butterflies). Complete metamorphosis.

Neoptera Holometabola (also called Endopterygota) are insects that have
complete metamorphosis (holometabolous development), These insects have four
developmental stages in the life cycle: egg, larva, pupa, and adult (imago).
Unlike hemimetabolous insects in which the immature structures (legs, eyes,
antennae, etc.) must also serve the adults, holometabolous insects have a
larval stage and acquire a completely new body during the pupal stage. Start of
larvae.

The larva is a defining feature of Holometabola. There are two theories about
how larva evolved. One is that holometabolous larvae and hemimetabolous nymphs
are homologous life stages, the other theory is that the holometabolan larva is
a protracted version of the hemimetabolous pronymph- that larvae are
essentially free-living embryos. The pronymph is a stage between hatching and
the first instar nymph in hemimetabolous insects.
  
310,000,000 YBN
6366) Holometabolous Insects: Panorpida {PaNORPidu}, ancestor of all Mecoptera
(scorpionflies), Siphonaptera (fleas), Diptera (true flies), Trichoptera
{TriKoPTRu} (caddis flies), and Lepidoptera (moths and butterflies).
  
305,000,000 YBN
242) Earliest frogs fossil, Prosalire.
  
305,000,000 YBN
382) Amphibians: Anura {unRu} (Frogs and Toads) evolve.

The order Anura, are tailless amphibians that include all frogs and toads.
  
305,000,000 YBN
383) Amphibians: Salamanders evolve.
  
300,000,000 YBN
162)
  
300,000,000 YBN
387) Reptiles Testudines {TeSTUDinEZ}: Ancestor of Turtles, Tortoises and
Terrapins.

Testudines is the order of all turtles, tortoises and terrapins. Testudines are
reptiles, most are aquatic or semiaquatic, fresh water or marine, but lay eggs
on land. They have webbed feet or flippers and their body is covered by a horny
shell from which only the legs, head and neck, and tail protrude when needed.
The upper shell is called the carapace and the undershell the plastron.

Tortoises are any of various terrestrial turtles, especially one of the family
Testudinidae, characteristically having thick clublike hind limbs and a high,
rounded carapace.

Terrapins are any of various North American aquatic turtles of the family
Emydiolae, especially the genus Malaclemys, which includes the diamondback
terrapin.

There are inconsistencies in terminology. In the USA "turtle" is used broadly
for all reptiles with a shell, "terrapin" applies to a large family, Emydidae,
and "tortoise" refers to the slow moving terrestrial species (the land turtles)
that enter water only to drink or soak. In Great Britain and Australia
"tortoise" is applied generally to all members of the group except the marine
species with paddle-shaped limbs which are called "turtles".

DOMAIN Eukaryota - eukaryotes
KINGDOM Animalia Linnaeus, 1758 - animals
SUBKINGDOM Bilateria
(Hatschek, 1888) Cavalier-Smith, 1983 - bilaterians
BRANCH Deuterostomia Grobben,
1908 - deuterostomes
INFRAKINGDOM Chordonia (Haeckel, 1874) Cavalier-Smith, 1998

PHYLUM Chordata Bateson, 1885 - chordates
SUBPHYLUM Vertebrata Cuvier, 1812 -
vertebrates
INFRAPHYLUM Gnathostomata auct. - jawed vertebrates

SUPERCLASS Tetrapoda Goodrich, 1930 - tetrapods
SERIES Amniota

CLASS Sauropsida
SUBCLASS Anapsida
ORDER Testudines
- turtles
  
300,000,000 YBN
1310) Stramenopiles Golden algae (Chrysophyta {KriSoFiTu}).
  
299,000,000 YBN
125) End of the Carboniferous (359.2-299 mybn), and start of the Permian
(299-251 mybn) Period.
  
299,000,000 YBN
6360) Holometabola: Coleoptera {KOlEoPTRu} (Beetles).

The earliest fossil beetle, Adiphlebia lacoana.

Coleoptera contains 350,000 named species and is the largest order of organisms
and 40% of all insects.

Well known beetles are: Ladybugs, Fireflies, Dung beetles, Japanese beetles,
weevils, and scarabs.

Some beetles have horns, in particular the Scarabaeoidea (scarab related
families). The male usually has horns, females very rarely do and they are
always small, which indicates that horns are the product of sexual selection,
or intense competition among males for mating. In many Scarabaeoidea males
fight to control access to breeding sites and to females. Some beetles secrete
defensive fluids, and are bioluminescent (like the familiar Lampyridae more
commonly called "lightning bugs" or "fireflies"). Among all bioluminescent
insects the mechanism of light emission involves a luciferan in the presence of
oxygen, the enzyme luciferase, and ATP. The reaction of these produces
oxyluciferin, CO2 and light.
(Pennsylvanian deposit) Mazon Creek, Illinois, USA  
290,000,000 YBN
239) Gymnosperms: Ginkgophyta (Ginkgos).
  
290,000,000 YBN
6358) Holometabola: Hymenoptera (bees, ants, and wasps).

The earliest fossil evidence of Hymenoptera is the stem gall of
Pteridotorichnos stipitopteri in the Late Carboniferous. A gall is an abnormal
swelling of plant tissue caused by insects, microorganisms, or external injury.
But the earliest definitive Hymenoptera, recognized by the distinctive wing
venation, are from the Triassic.

The Hymenoptera are currently divided into two suborders: "Symphyta" (sawflies
and wood wasps) and the Apocrita (true wasps or parasitic wasps) which includes
the Aculeata (ants, bees, and other stinging wasps).

In all members of the Hymenoptera order, females have two sets of chromosomes
(are diploid), being the union of two gametes, but males are produced from
unfertilized eggs and so have only a single copy of the genome (are haploid),
although diploid males do sometimes occur. Hymenoptera are well known as
parasitoids. Parasitoids, unlike parasites develop from nutrients extracted
from a single host, and they kill the host as a direct result or indirect
result (a parasite, while inflicting minimal to severe ill effects, does not
kill its host). The host remains alive for the larger part of the of the
parasitoid's period of feeding. Some larvae even change the behavior of their
host to the benefit of the parasitoid. Some bees are cleptoparasitic, instead
of the adult contructing and supplying her own nest, females steal into the
nest of a host bee and deposit an egg into the brood cell before escaping.
  
290,000,000 YBN
6367) Holometabolous Insects Antliophora (ancestor of Diptera: true flies and
Mecopterids: scorpionflies and fleas).
  
287,000,000 YBN
6308) Synapsid Therapsids evolve (Cynodonts).

Therapsids evolve from Pelycosaurs and largely replace them for a time as the
dominant terrestrial vertebrates. Therapsids appear in the late Permian and
prosper during the early Triassic. The Therapsids are quadruperal and their
feet have five digits, but their legs are more directly positioned under the
weight of their body. This reflects a more efficient and active mode of
locomotion. Teeth are differentiated into distinct types. Some herbivorous
therapsids become specialized for rooting or grubbing, some for digging, some
for browsing. The overall selection for more efficient terrestrial locomotion
and feeding specializations results in greateer diversity within therapsids.
There is some evidence that therapsids become endothermic in parallel with
their archosaur (avian) contemporaries.

One particularly successful group of therapsids are the cynodonts. Some are
herbivores but more are carnivores. They arise in the late Permian and become
dominant land carnivores in the early part of the Triassic, until largely
replaced by the terrestrial sauropsids of the late Triassic. Cynodonts have
teeth specialized for slicing together with muscular cheeck that keep the food
between tooth rows that chew the food. The Cynodont limbs are direectly under
the body, contributing to the ease and efficiency of ative terrestrial
locomotion. In addition, extensive turbinals are likely present in the nose.
These are thin, scrolled, and folded plates of bone that warm and humidify the
incoming air (as well as hold the olfactory epithelium). These characteristics
suggest that cynodonts had an endothermic metabolism. During their evolution
the cynodonts decline in body size from the size of a large dog to slightly
larger than a weasel. By the Triassic, only one group of cynodonts, the
mammals, will remain and eventually prosper after the great dinosaur
extinctions at the end of the Cretaceous.
  
280,000,000 YBN
6365) Ancestor of Holometablous insects Neuropterida (Neuroptera: lacewings,
Raphidioptera: snakeflies, and Megaloptera: alderflies and dobsonflies).
  
280,000,000 YBN
6368) Holometabolous Insects Mecopterids (ancestor of Mecoptera: scorpionflies
and Siphonaptera: fleas).
  
274,000,000 YBN
307) Ancestor of all Protists: Phaeophyta {FEoFiTu} (Brown Algae).

The Phaeophyta are a phylum (division) of the kingdom Protista consisting of
those organisms commonly called brown algae. Many of the Earth's familiar
seaweeds are members of Phaeophyta. There are approximately 1,500 species. Like
the chrysophytes, brown algae derive their color from the presence, in the cell
chloroplasts, of several brownish carotenoid pigments, including fucoxanthin,
in addition to the photosynthetic pigments chlorophyll a and c. With only a few
exceptions, brown algae are marine, growing in the colder oceans of the world,
many in the tidal zone, where they are subjected to great stress from wave
action; others grow in deep water. Among the brown algae are the largest of all
algae, the giant kelps, which may reach a length of over 100 ft (30 m). Fucus
(rockweed), Sargassum (gulfweed), and the simple filamentous Ectocarpus are
other examples of brown algae.

The cell wall of the brown algae consists of a cellulose differing chemically
from that of plants. The outside is covered with a series of gelatinous pectic
compounds, generically called algin; this substance, for which the large brown
algae, or kelps, of the Pacific coast are harvested commercially, is used
industrially as a stabilizer in emulsions and for other purposes. The normal
food reserve of the brown algal cell is a soluble polysaccharide called
laminarin; mannitol and oil also occur as storage products. The body, or
thallus, of the larger brown algae may contain tissues differentiated for
different functions, with stemlike, rootlike, and leaflike organs, the most
complex structures of all algae.

Some groups of brown algae have evolved an interesting type of alternation of
generations, in which physiologically independent haploid gametophyte plants
produce gametes, the fusion of which initiates the diploid sporophyte
generation. The mature sporophyte plant produces, through meiosis, haploid
spores, which develop into new gametophytes. The two generations, or phases,
may be indistinguishable in size and form, or they may differ greatly. The
genus Ectocarpus, for example, is found growing attached to larger algae. It
has similar-looking gametophyte and sporophyte plants. In the kelps, however,
the gametophyte is only a microscopic filament, in contrast to the occasionally
tree-sized sporophyte.
  
270,000,000 YBN
240) Gymnosperms: Pinophyta {PInoFiTu} (Conifers: includes Pine, Fir, Spruce,
Redwood, Cedar, Juniper, Hemlock, Larch, and Cypress).

The gymnosperms, are a division of seed plants characterized as vascular plants
with roots, stems, and leaves, and with seeds that are not enclosed in an ovary
but are borne on cone scales or exposed at the end of a stalk.
  
266,000,000 YBN
308) Protist Stramenopiles: Diatoms.

Diatoms are microscopic one-celled or colonial algae, having cell walls of
silica consisting of two interlocking symmetrical valves.

The silica shell often has intricate and beautiful sculpturing. Diatoms are
usually yellowish or brownish, and are found in fresh and saltwater, in moist
soil, and on the moist surface of plants. Diatoms carry chlorophylls a and c
and the carotenoid fucoxanthin contained in plastids. They reproduce asexually
by cell division.
  
260,000,000 YBN
232) Earliest warm-blooded and hair growing animal.

This is possibly a therocephalian reptile..

Both birds and mammals are endothermic (also called "warm blooded") as opposed
to other vertebrates which are ectothermic (or "cold blooded) and cannot
internally generate heat.
Endothermy is the physiological maintenance, by a body, of
a constant temperature independent of the external environmental temperature.
Hair for insulation is correlated to endothermy. Endothermy allows birds and
mammals to maintain a high and relatively constant body temperature, even at
rest, during a wide range of external environmental conditions.

Respiratory conchae (or turbinates) (small curved bones in the nasal passage,
some which reduce respiratory water loss with rapid breathing), found in the
primitive therocephalian Glanosuchus and in several cynodonts, are the first
reliable morphological indicator of endothermy. Although the actual nasal
turbinal bones are rarely preserved in fossils, their presence can be deduced
from characteristic ridges on the walls of the nasal cavity. Ridges probably
associated with respiratory turbinals first appear among advanced therapsids,
the therocephalians and cynodonts. This suggests that the evolution of the
higher oxygen consumption rates of mammals may begin as early as the Late
Permian and develop in parallel in therocephalians and cynodonts, with full
mammalian endothermy taking perhaps 40 to 50 million more years to develop.

The earliest fossil that has hair is a Pterosaur fossil that is around 215
million years old, and some argue that Pterosaurs are endothermic
(warm-blooded).

The common ancestor of monotremes is 180 MYBN, and all monotremes are
endothermic.
  
260,000,000 YBN
364) Ray-finned fishes: Gars.
  
256,000,000 YBN
6362) Holometabola: Diptera {DiPTRe} true flies, single pair of wings:
mosquito, gnat, fruit fly, house fly).
  
255,000,000 YBN
389) Reptiles: Tuataras {TUeToRoZ} evolve.

The tuatara is a lizardlike reptile, and is the last survivor of the reptilian
order Rhynchocephalia, which flourishes in the early Mesozoic era before the
rise of the dinosaurs. Also called sphenodon, it is found on islands off the
New Zealand coast and in Karori Wildlife Sanctuary, Wellington, New Zealand.
The olive colored, yellow-speckled tuatara reaches a length of 60 cm (2 ft) or
more. It is very lizardlike in external form, with a crest of spines down its
neck and back. However, its internal anatomy, its scales, and the attachment of
its teeth are different from those of lizards, and its body chemistry allows it
to function at temperatures close to freezing. Like certain lizards, tuataras
have a vestigial third eye (pineal eye) on top of their head, but this organ is
probably not sensitive to light. Tuataras usually inhabit the breeding burrows
of certain small petrels (sea birds). They feed on small animals, especially
insects, and reproduce by laying eggs. Captive tuataras mature in about 20
years, and it appears that their life span may exceed a century by several
decades.
(Islands of) New Zealand  
251,400,000 YBN
102) End-Permian mass extinction. 82% of all genera are observed extinct.

The Permian–Triassic extinction event is the Earth's most severe extinction
event, with up to 96% of all marine species and 70% of terrestrial vertebrate
species becoming extinct It is the only known mass extinction of insects.

The are 5 known major mass extinctions.

Many organisms go extinct. Among invertebrates: all fusulinid forminifera,
rugose and tabulate corals, trilobites, eurypterids, strophomenid brachiopods,
and 5 orders of insects go extinct. Among vertebrates: two-thirds of
amphibians, reptiles, and therapsids go extinct.
  
251,000,000 YBN
54) End of the Paleozoic and start of the Mesozoic Era, and the end of the
Permian (299-251 mybn) and start of the Triassic (251-201.6 mybn) period.
  
251,000,000 YBN
452)
  
251,000,000 YBN
6306) Oldest fossil amniote egg.
Texas (verify)  
250,000,000 YBN
241) Fourth oldest living Plant Division "Gnetales".
Gnetophyta - Gnetum, Ephedra,
Welwitschia 80 species.
  
250,000,000 YBN
368) Bowfin (Ray-finned) fishes evolve.

Bowfins (Amiiformes) are a primitive bony freshwater fish of central and
eastern North America, with a long spineless dorsal fin.
  
245,000,000 YBN
392) Reptiles: Crocodilia {KroKoDiLEu} (Crocodiles, allegators, and caimans
{KAmeNS}) evolve.
  
228,000,000 YBN
412) Reptiles: Dinosaurs evolve.
(Ischigualasto Formation) Valley of the Moon, Ischigualasto Provinvial Park,
northwestern Argestina  
228,000,000 YBN
611) Dinosaurs divide into two major lines: Ornithischians {ORnitiSKEiNZ}
(Bird-hipped dinosaurs) and Saurischians {SoriSKEiNZ} (Lizard-hipped
dinosaurs). The Ornithischians will evolve into both bipedal and quadrupedal
plant-eaters (herbavores), and the Saurischians will evolve into bipedal
meat-eaters (carnivores) and quadrupedal plant-eaters.
  
228,000,000 YBN
6282) Saurischian {SoriSKEiN} Dinosaurs split into two major lines: The
Sauropodomorpha (SoroPiDimORFu} and the Therapoda {tiRoPiDu}.

Sauropodomorphs are divided into prosauropods and sauropods, are mostly
plant-eating, and include the large, long-necked dinosaurs like Apatosaurus.

Theropod {tERePoD} dinosaurs are bipedal and carnivorous and include
Allosaurus, Tyrannosaurus, and Velociraptor. All birds descend from a Therapod
ancestor.
(Ischigualasto Formation) Valley of the Moon, Ischigualasto Provinvial Park,
northwestern Argestina  
228,000,000 YBN
6283) Earliest dinosaur fossil, the Theropod Eoraptor.
This dinosaur is a cat-sized meat
eater.
(Ischigualasto Formation) Valley of the Moon, Ischigualasto Provinvial Park,
northwestern Argestina  
225,000,000 YBN
126)
(Dockum Formation) Kalgary, Crosby County, Texas, USA  
225,000,000 YBN
6370) Holometabolous Insect Order Tricoptera: Caddisflies. Caddisflies are
closely related to the Lepidoptera (butterflies and moths).
  
220,000,000 YBN
400) Earliest mammal fossil (Adelobasileus).

This is a fingernail-sized skull found in Texas.
(Dockum Formation) Kalgary, Crosby County, Texas, USA  
220,000,000 YBN
428) The first flying vertebrate (Pterosaur).
Oldest Pterosaur fossils (Preondactylus and
Eudimorphodon).

Pterosaurs have hair, and some argue have endothermy (are warm-blooded) and
actively fly (contracting their wing muscles to flap, as opposed to only
glide).

Bonde and Christiansen cite a report of a juvenile Eudimorphon ranzii with skin
and 'hairy' impressions. However, Benton only cites the pterosaur fossils from
the Upper Jurassic and that the details of pterosaur hair are currently
disputed.
  
210,000,000 YBN
317) Reptile Order: Squamata evolves (ancestor of lizards and snakes).
  
210,000,000 YBN
369)
  
210,000,000 YBN
390) Reptiles Iguania evolves: (iguanas, chameleons, and spiny lizards).
  
210,000,000 YBN
391) Reptiles: Scleroglossa evolve (snakes, skinks, and geckos).
  
210,000,000 YBN
413)
  
210,000,000 YBN
6313) Earliest extant Teleosts: Bonytongues.

Teleosts (Subdivision Teleostei) are a large group of fishes with bony
skeletons, including most common fishes, different from cartilaginous fishes
such as sharks and rays.

Teleosts will grow to include (bonytongues, eels, herrings, anchovies, carp,
minnows, piranha, salmon, trout, pike, perch, seahorse, cod).

DOMAIN Eukaryota - eukaryotes
KINGDOM Animalia Linnaeus, 1758 - animals
SUBKINGDOM Bilateria
(Hatschek, 1888) Cavalier-Smith, 1983 - bilaterians
BRANCH Deuterostomia Grobben,
1908 - deuterostomes
INFRAKINGDOM Chordonia (Haeckel, 1874) Cavalier-Smith, 1998

PHYLUM Chordata Bateson, 1885 - chordates
SUBPHYLUM Vertebrata Cuvier, 1812 -
vertebrates
INFRAPHYLUM Gnathostomata auct. - jawed vertebrates
CLASS
Osteichthyes Huxley, 1880
SUBCLASS Actinopterygii - ray-finned
fishes
INFRACLASS Cladistia
INFRACLASS Actinopteri

SUPERDIVISION Neopterygii
DIVISION Halecostomi

SUBDIVISION Teleostei
  
209,500,000 YBN
489) Triconodonta (extinct mammals) evolve.
Kingdom: Animalia
Phylum: Chordata
Class: Mammalia
Order:
Triconodonta
  
201,600,000 YBN
127) End of the Triassic (251-201.6 mybn), and start of the Jurassic
(201.6-145.5 mybn) Period.
  
201,400,000 YBN
228)
  
200,000,000 YBN
370)
  
200,000,000 YBN
6285)
  
200,000,000 YBN
6372) Ornithischians Thyreophora {tIrEoFeru} evolve; ancestor of the armored
ankylosaurs {ANKilOSORZ} and the plated stegosaurs {STeGeSORZ}.

One of the most primitive Thyreophorans is Scutellosaurus which has rows of
armored plates along its body and tail.
(Kayenta Formation) Arizona, USA  
195,000,000 YBN
246) Sauropods {SoRuPoDZ} evolve; ancestor of the large, long-necked dinosaurs
like Apatosaurus {uPaTuSORuS}, Brachiosaurus {BrAKEuSORuS}, and Diplodocus
{DiPloDiKuS}.
western USA  
195,000,000 YBN
6373) Ornithischians ornithopoda {ORnitoPiDu} evolve; the duck-billed
dinosaurs, ancestor of the Hadrosaurs.

One of the most primitive Ornithopods is Heterodontosaurus.
  
190,000,000 YBN
358) Cartilaginous fishes: squalea {SKWAlEo} evolve, ancestor of all rays,
skates, and sawfishes.
  
190,000,000 YBN
359) Cartilaginous fishes: "Galea" {GAlEu} evolve, (ancestor of all sharks:
includes great white, hammerhead, mako, tiger and nurse sharks).
  
190,000,000 YBN
371) Teleosts: herrings and anchovies.
  
190,000,000 YBN
6289)
Pangea  
190,000,000 YBN
6347) Holometabola Lepidoptera {lePiDoPTRu} evolve (moths, butterflies,
caterpillars).

The Lepidoptera comprise the largest lineage of plant-feeding organisms. The
plant eating beetles form the other largest group.

Butterflies are only about 6% of all species the Lepidoptera, the rest being
moths. Because unlike the day flying butterflies, moths are generally smaller,
night flying insects, butterflies get all the attention.

The Leptidoptera, among all Orders of insects, appears to have radiated most
recently.
Dorset, England  
185,000,000 YBN
194) Earliest diatom fossils.
  
180,000,000 YBN
456) Biota
Domain Eukaryota - eukaryotes
Kingdom Animalia Linnaeus, 1758 - animals

Subkingdom Bilateria (Hatschek, 1888) Cavalier-Smith, 1983 - bilaterians
Branch
Deuterostomia Grobben, 1908 - deuterostomes
Infrakingdom Chordonia (Haeckel, 1874)
Cavalier-Smith, 1998
Phylum Chordata Bateson, 1885 - chordates

Subphylum Vertebrata Cuvier, 1812 - vertebrates
Infraphylum Gnathostomata
auct. - jawed vertebrates
Superclass Tetrapoda Goodrich, 1930 -
tetrapods
Series Amniota
Mammaliaformes Rowe, 1988

Class Mammalia Linnaeus, 1758 - mammals

Subclass Prototheria Gill, 1872:vi
Order Platypoda (Gill,
1872) McKenna in Stucky & McKenna in Benton, ed., 1993:740

Order Tachyglossa (Gill, 1872) McKenna in Stucky & McKenna in Benton, ed.,
1993:740
Australia, Tasmania and New Guinea  
170,000,000 YBN
372) DOMAIN Eukaryota - eukaryotes
KINGDOM Animalia Linnaeus, 1758 - animals
SUBKINGDOM
Bilateria (Hatschek, 1888) Cavalier-Smith, 1983 - bilaterians
BRANCH Deuterostomia
Grobben, 1908 - deuterostomes
INFRAKINGDOM Chordonia (Haeckel, 1874) Cavalier-Smith,
1998
PHYLUM Chordata Bateson, 1885 - chordates
SUBPHYLUM Vertebrata
Cuvier, 1812 - vertebrates
INFRAPHYLUM Gnathostomata auct. - jawed
vertebrates
CLASS Osteichthyes Huxley, 1880
SUBCLASS
Actinopterygii - ray-finned fishes
INFRACLASS Cladistia

INFRACLASS Actinopteri
SUPERDIVISION Neopterygii
DIVISION
Halecostomi
SUBDIVISION Teleostei
  
170,000,000 YBN
373) DOMAIN Eukaryota - eukaryotes
KINGDOM Animalia Linnaeus, 1758 - animals
SUBKINGDOM
Bilateria (Hatschek, 1888) Cavalier-Smith, 1983 - bilaterians
BRANCH Deuterostomia
Grobben, 1908 - deuterostomes
INFRAKINGDOM Chordonia (Haeckel, 1874) Cavalier-Smith,
1998
PHYLUM Chordata Bateson, 1885 - chordates
SUBPHYLUM Vertebrata
Cuvier, 1812 - vertebrates
INFRAPHYLUM Gnathostomata auct. - jawed
vertebrates
CLASS Osteichthyes Huxley, 1880
SUBCLASS
Actinopterygii - ray-finned fishes
INFRACLASS Cladistia

INFRACLASS Actinopteri
SUPERDIVISION Neopterygii
DIVISION
Halecostomi
SUBDIVISION Teleostei
  
165,000,000 YBN
457) Ancestor of all Marsupials. This is the last common ancestor of Eutheria
(includes Placental) and Metatheria (includes Marsupial) mammals.

Marsupium means pouch in Latin. Marsupials are born as tiny embryos and crawl
through their mother's fur into the pouch where they clamp their mouths to a
nipple (teat). The other main group of mammals are called placentals because
they feed their embryos with a placenta which allows the baby top be born much
later. The pouch is like an external womb.

The earliest known marsupial is Sinodelphys szalayi, which lived in China
around 125 million years ago (mya).
China  
161,000,000 YBN
6369) Holometabola Siphonaptera: fleas.

The oldest flea fossils, which are much larger than modern species date to this
time.
(Jiulongshan Formation) Daohugou, Ningcheng County, Inner Mongolia  
160,000,000 YBN
163)
(Daxigou) Jianchang County, Liaoning Province, China  
150,000,000 YBN
330) Stegosaurus, an armored, plant-eating Thyreophoran {tIRrEoFereN} dinosaur
lives around this time. Stegosaurus has sharp spikes on its tail and large bony
plates on its back. The plates may be used for display or for controlling its
body temperature.
western USA  
150,000,000 YBN
374) DOMAIN Eukaryota - eukaryotes
KINGDOM Animalia Linnaeus, 1758 - animals
SUBKINGDOM
Bilateria (Hatschek, 1888) Cavalier-Smith, 1983 - bilaterians
BRANCH Deuterostomia
Grobben, 1908 - deuterostomes
INFRAKINGDOM Chordonia (Haeckel, 1874) Cavalier-Smith,
1998
PHYLUM Chordata Bateson, 1885 - chordates
SUBPHYLUM Vertebrata
Cuvier, 1812 - vertebrates
INFRAPHYLUM Gnathostomata auct. - jawed
vertebrates
CLASS Osteichthyes Huxley, 1880
SUBCLASS
Actinopterygii - ray-finned fishes
INFRACLASS Cladistia

INFRACLASS Actinopteri
SUPERDIVISION Neopterygii
DIVISION
Halecostomi
SUBDIVISION Teleostei
  
150,000,000 YBN
393)
  
150,000,000 YBN
394) Oldest bird (and feather) fossil, Archaeopteryx.

The Archaeopteryx fossil is from the Solnhofen Limestone of the Upper Jurassic
of Germany.

John Ostrom describes the historical background of the Archaeopteryx fossils:
"...
Possibly no other zoological specimens, fossil or Recent, are considered so
importa
nt as are those of Archeopteryx lithographica (see Figs 1, 2 and 3).
Certainly few
other specimens have generated such widespread interest or
provoked as much
speculation and controversy. The reasons are several: these
specimens are the oldest
(Tithonian = Late Jurassic) known fossil bird remains;
they are extremely rare, only
five specimens (excluding the solitary feather) are
known at present; several of
these preserve remarkably detailed impressions of
feathers and an extraordinary
mixture of reptilian and avian characters; and
most important of all, because of
the last fact, out of all presently known fossil
and living organisms, these specimens
are widely recognized as constituting the
best example of an organism perfectly
intermediate between two higher
taxonomic categories-representing an ideal
transitional stage between ancestral
and descendant stocks. Archaeopteryx may well be the
most impressive fossil
evidence of the fact of organic evolution.
...
The first still-verifiable evidence of Jurassic birds is the imprint of a
solitary feather in a small slab of these same Solnhofen limestones (Fig. 2A).
This find was reported by von
Meyer (1861a) in a letter to Professor H. Bronn,
published in Bronn’s Neues
Jahrbuch fur Mineralogie (p. 561). Less than two months
later, von Meyer
(1861b) reported the discovery in the same limestone strata of a
partial
skeleton associated with distinct impressions of feathers. This find, the now
well-k
nown London specimen (Fig. 1A), is currently in the British Museum
(Natural History)
in London. At first, some scholars questioned the authenticity
of both specimens, but von
Meyer (1862) established them as genuine.".

Some scientists view Archaeopteryx as probably a flightless feathered dinosaur.
Solnhofen, Germany  
150,000,000 YBN
6334) Probable fungi microfossils of "Tappania plana" with fused branches, a
process found in higher fungi.
(Wynniatt Formation) Victoria Island, northwestern Canada  
150,000,000 YBN
6374) Sauropods {SoRuPoDZ} are common; large, long-necked dinosaurs like
Apatosaurus {uPaTuSORuS}, Brachiosaurus {BrAKEuSORuS}, and Diplodocus
{DiPloDiKuS}.
western USA  
146,000,000 YBN
490) Multituberculata (extinct major branch of mammals) evolve.
  
145,000,000 YBN
245) The first flowering plant (angiosperm).

Almost all grains, beans, nuts, fruits, vegetables, herbs and spices come from
plants with flowers. Tea, coffee, chocolate, wine, beer, tequila, and cola all
come from flowing plants. Much of our clothing comes from flowering plants too:
cotton and linen are made from "fibers" of flowering plants, as are rope and
burlap, and many commercial dyes are extracted from other flowering plants.
Many drugs also come from flowering plants including: aspirin, digitalis,
opium, cocaine, marijuana, and tobacco.

Aside from primitive flowers like the Magnoliids, most later angiosperms can be
divided into the more primitive Monocotyledons (Monocots), flowering plants
that have a single cotyledon (seed leaf) in the embryo, and the more recent
Dicotyledons (Dicots), which have two cotyledons in the embryo. The dicots
contain two groups that account for two-thirds of all angiosperm species: the
asterids, and the rosids.

The earliest fossil evidence of angiosperms is pollen 130-140 MYO in Israel,
Morocco, Libya, and possibly China. The earliest macrofossils are leaves and
flowers around 120-130 MYO.

Archaefructus, is an early angiosperm fossil that dates to around 125 MYO from
northeastern China. Archaefrcutus does not have petals or sepals, but does have
carpels and stamens which are attached to an elongated stem with the staminate
(pollen-producing) flowers below, and pistillate (fruit-producing) flowers
above. This ancient flower is similar in some ways to Trithuria, a genus of
Nymphaeles (waterlilies).

Estimates of angiosperm origins based on molecular divergence are typically far
older than those estimates based on fossils. These rate estimates may be a
result of using living species in a group where the basal branches of a lineage
have been extensively pruned by extinction, which may be the case for the
angiosperm tree.
Israel, Morocco, Libya, and possibly China  
145,000,000 YBN
415) Oldest flower fossil, Archaefructus, in China, a submerged wetland plant.
(Yixian Formation) Liaoning Province, northeastern China  
144,000,000 YBN
128) End of the Jurassic (201.6-145.5 mybn), and start of the Cretaceous
(145.5-65.5 mybn) Period.
  
143,000,000 YBN
6288) Earliest extant flowering plant (Angiosperm) "Amborella".
  
140,000,000 YBN
247) The second most primitive living Angiosperms, the Water Lilies
("Nymphaeales").

70 species.
  
138,000,000 YBN
248) Angiosperm "Austrobaileyales".
  
136,000,000 YBN
249) Angiosperm "Chloranthaceae".

70 living species.
  
136,000,000 YBN
460) Enantiornithes {iNaNTEORNitEZ} evolve (early birds).
  
134,000,000 YBN
250) Ancestor of all flowers: "Magnoliids" {maGnOlEiDZ} (nutmeg, avocado,
sassafras, cinnamon, black and white pepper, camphor, bay (or laurel) leaves,
magnolias.).

There are 9,000 living species.
  
133,000,000 YBN
253) Flowers Eudicots {YUDIKoTS} evolve (the largest lineage of flowers).

Eudicots are also called "tricolpates" which refers to the structure of the
pollen.

The two main groups of the Eudicots are the "rosids" and the "asterids".
  
132,000,000 YBN
462)
  
130,000,000 YBN
375) Teleosts: Perch, seahorses, flying fish, pufferfish, barracuda.
  
130,000,000 YBN
376) Teleosts: cod, anglerfish.
  
130,000,000 YBN
6338) Feathered dinosaur microraptors fossils.
Northeastern China  
125,000,000 YBN
395)
(Yixian Formation) Liaoning Province, northeastern China  
120,000,000 YBN
463) Neornithes {nEORnitEZ} evolve (modern birds: the most recent common
ancestor of all living birds).

Neornithes is the subclass of Aves that contains all of the known birds other
than those placed in the Archaeornithes. Neornithes includes more than 30
orders, both fossil and living, its members are characterized by a bony, keeled
sternum with fully developed powers of flapping flight (secondarily lost in a
number of groups); a short tail with fused vertebrae to which all tail feathers
attach; a large fused pelvic girdle; and a large brain and eyes contained
within a fused braincase. In addition Neornithes have a fully-separated
four-chambered heart and typically exhibit complex social behaviors.
  
120,000,000 YBN
6361) Bees. The earliest bee fossil is from the Late Cretaceous, but presumed
nests that date to 95 MYO indicate that bees are older, perhaps as old as
around 120 MYO.
  
119,000,000 YBN
251) Ancestor of all Angiosperm "Ceratophyllaceae".

Closest surviving relative of all eudicots.

6 living species.
  
112,000,000 YBN
252) Flowers Monocotyledons (or "Monocots") evolve: Flowering plants that have
a single cotyledon (or seed leaf) in the embryo.

Monocots are the second largest lineage of flowers after the Eudicots (formally
Dicotyledons) with
70,000 living species (20,000 species of orchids, and 15,000
species of grasses).

The two main orders of Monocots are "Base Monocots" and "Commelinids".
  
112,000,000 YBN
481) Earliest Monotreme fossil, Steropodon galmani, the earliest platypus-like
species.
Earliest Monotreme fossil, Steropodon galmani, the earliest platypus-like
species.
Lightning Ridge in north central New South Wales, Australia  
110,000,000 YBN
416)
Oklahoma, USA  
108,000,000 YBN
254) Flowers: "Basal Eudicots" (buttercup, clematis, poppy (source of opium and
morphine), macadamia, lotus, sycamore).
  
106,000,000 YBN
267) Flowers "Core Eudicots" (carnation, cactus, caper, buckwheat, rhubarb,
sundew, venus flytrap, old world pitcher plants, beet, quinoa, spinach,
currant, sweet gum, peony, witch-hazel, mistletoe, grape plants.).
  
105,000,000 YBN
417) Sauropod Argentinosaurus {oRJeNTiNuSORuS}, a long-neck (sauropod)
titanosaur from South America, possibly the longest animal of all time, at an
estimated 130 to 140 feet length.
  
105,000,000 YBN
491) Ancestor of all placental mammal Afrotheres evolves (elephants, manatees,
aardvarks).

Afrotheres originate in Africa and are the earliest extant placental mammals.
Africa  
100,000,000 YBN
164)
  
100,000,000 YBN
418)
South America  
100,000,000 YBN
464)
  
100,000,000 YBN
465) Birds "Ratites" evolve (ostrich, emu, cassowary {KaSOwaRE}, kiwis).
  
100,000,000 YBN
480) Kollikodon ritchiei, an extinct monotreme.
  
95,000,000 YBN
419) The Therapod {tERePoD} Spinosaurus {SPINuSORuS}, perhaps the largest
meat-eating dinosaur, estimated to have been 45 to 50 feet long.

The only skeleton ever found was destroyed during World War 2.
  
95,000,000 YBN
498) Mammals "Xenarthrans" {ZeNoRtreNZ} evolve (Sloths, Anteaters, Armadillos).
  
93,000,000 YBN
256) Flowers: "Rosids" evolve (Basal Rosids include: geranium, pomegranate,
myrtle, clove, guava, allspice, and eucalyptus).
  
93,000,000 YBN
258) Flowers "Eurosid I" Order "Celastrales".
  
93,000,000 YBN
261) Angiosperm Eudicot "Eurosids I" Order "Fabales" {FoBAlEZ}.

Fabales include many beans (green, lima, kidney, pinto, navy, black, mung,
fava, cow (or black-eyed), popping), pea, peanut, soy {used in tofu, miso,
tempeh, and milk}, lentil, chick pea (or garbonzo) {used in falafel}, lupin,
clover, alfalfa {used as sprouts}, cassia {Kasu}, jicama, Judas tree, tamarind
{TaMuriND}, acacia {uKAsYu}, mesquite.
  
93,000,000 YBN
265) Angiosperms "Base Monocots" evolve (vanilla, orchid, asparagus, onion,
garlic, agave, aloe, lily).
  
93,000,000 YBN
266) Monocots "Commelinids" {KomelIniDZ} evolve (palms, coconut, corn, rice,
barley, oat, wheat, rye, sugarcane, bamboo, grass, pineapple, papyrus, turmeric
{TRmRiK}, banana, ginger).
  
93,000,000 YBN
268) Angiosperm Eudicot "Eurosids I" Order "Zygophyllales" evolves.
  
93,000,000 YBN
274) Ancestor of flowers "Basal Asterids". Earliest surviving Order "Cornales"
(dogwoods, tupelos, dove tree).
  
93,000,000 YBN
275) Angiosperm "Basal Asterids" Order "Ericales" {AReKAlEZ} .
Ericales includes
kiwifruit (kiwi), Impatiens, ebony, persimmon, heather, crowberry,
rhododendrons, azalias, cranberries, blueberries, lingonberry, bilberry,
huckleberry, brazil nut, primrose, sapodilla, mamey sapote (sapota), chicle,
balatá, canistel, new world pitcher plants {carniverous}, tea {Camellia
sinensis}
  
93,000,000 YBN
277) Angiosperm "Euasterids I" evolve, with earliest surviving order
"Garryales".
  
93,000,000 YBN
282) Angiosperm "Euasterids II" order "Aquifoliales" (includes holly).
  
93,000,000 YBN
283) Angiosperm "Euasterids II" order "Apiales" {APEAlEZ} evolving now.
Apiales
includes dill, angelica, chervil {CRViL}, celery, caraway, cumin, sea holly,
poison hemlock, coriander (or cilantro), carrot, lovage {LuViJ}, parsnip, anise
{aNiS}, fennel, cicely {SiSelE}, parsley, ivy, ginseng.
  
93,000,000 YBN
285) Angiosperms "Euasterids II" order "Asterales" {aSTRAlEZ} evolves.

Asterales includes burdock, tarragon, daisy, marigold, safflower, chrysanthemum
(mums), chickory, endive, artichoke, sunflower, sunroot (Jerusalem artichoke),
lettuce, chamomile, black-eyed susan, salsify {SoLSiFE}, dandelion, and zinnia.
  
91,000,000 YBN
259) Flowers: Eurosid I "Malpighiales" {maLPiGEAlEZ} evolves (includes gamboge
{GaM BOJ}, mangosteen {mANGuSTEN}, coca {used in cocaine and drinks}, rubber
tree, cassava (or manioc {maNEoK}) {used like a potato, and in tapioca}, castor
oil, poinsettia, flax, acerola {aSorOlu} (barbados cherry), willow, poplar,
aspen, and violet (or pansy).
  
91,000,000 YBN
260) Angiosperm Eudicot "Eurosids I" Order "Oxalidales" (fly-catcher plant,
wood sorrel family {leaves show "sleep movements"}, oca {edible tuber}).
  
90,000,000 YBN
270) Angiosperm Eudicots "Eurosids II" evolves: the most primitive Order is
"Brassicales" {BraSiKAlEZ}.

Brassicales includes horseradish, rapeseed, mustard {plain, brown, black,
indian, sarepta, asian}, rutabaga, kale, Chinese broccoli (kai-lan {KI laN}),
cauliflower, collard greens, cabbage (white and red {used in coleslaw and
sauerkraut}), Brussels sprouts, kohlrabi {KOLroBE}, broccoli, watercress,
radish, wasabi, mignonette {miNYuNeT}, and papaya.
  
89,000,000 YBN
262) Angiosperm "Eurosids I" Order "Rosales" {ROZAlEZ}.

Rosales includes hemp (cannibis, marijuana) {used for rope, oil, recreational
drug}, hackberry, hop {used in beer}, breadfruit, cempedak, jackfruit, marang,
paper mulberry, fig, banyan, strawberry, rose, red raspberry, black raspberry,
blackberry, cloudberry, loganberry, salmonberry, thimbleberry, serviceberry,
chokeberry, quince, loquat, apple, crabapple, pear, plum, cherry, peach,
apricot, almond, jujube, and elm.
  
89,000,000 YBN
279) Flowers "Euasterids I" order "Gentianales" {JeNsinAlEZ} evolves.
Gentianale
s includes gentian, dogbane, carissa (Natal plum), oleander, logania, and
coffee.
  
88,000,000 YBN
284) Angiosperm "Euasterids II" order "Dipsacales".
Dipsacales includes Elderberry,
Honeysuckle, Teasel, Corn Salad.
  
86,000,000 YBN
278) Angiosperm "Euasterids I" order "Solanales" {SOlanAlEZ} evolve.
Solanales
includes deadly nightshade or belladonna, capsicum (bell pepper, paprika,
Jalapeño, Pimento), cayenne pepper {KI YeN}, datura, tomato, mandrake,
tobacco, petunia, tomatillo, potato, eggplant, morning glory, sweet potato, and
water spinach.
Americas  
85,000,000 YBN
263) Angiosperm "Eurosids I" Order "Cucurbitales" (KYUKRBiTAlEZ} evolve.
Cucurbitales
includes watermelon, musk, cantaloupe, honeydew, casaba, cucumbers, gourds,
pumpkins, squashes (acorn, buttercup, butternut, cushaw {Kuso}, hubbard,
pattypan, spaghetti), zucchini, and begonia.
Americas  
85,000,000 YBN
264) Angiosperm "Eurosids I" Order "Fagales" {FaGAlEZ} evolves.
Fagales includes many
flowers that produce edible nuts: Birch, Hazel {nut}, Filbert {nut}, Chestnut,
Beech {nut}, Oak {used for wood, and cork}, Walnut, Pecan, Hickory, and
Bayberry.
  
85,000,000 YBN
466) Birds "Galliformes" {GaLliFORmEZ} evolve (Chicken, Turkey, Pheasant,
Peacock, Quail).
  
85,000,000 YBN
467) Birds "Anseriformes" {aNSRiFORmEZ} evolve (waterfowl: ducks, geese,
swans).

The "Anseriformes" are an order of birds, characterized by a broad, flat bill
and webbed feet.
  
85,000,000 YBN
499) Ancestor of all placental mammal "Laurasiatheres" evolves. This major line
of mammals includes the Insectivora (shrews, moles, hedgehogs), Chiroptera
(bats), Cetartiodactyla (camels, pigs, deer, sheep, hippos, whales),
Perissodactyla (horses, rhinos), Carnivora (cats, dogs, bears, seals, walruses)
and Pholidota (pangolins).

Laurasiatheres originate in the old northern continent Laurasia.
Laurasia  
84,000,000 YBN
454) The Rocky mountains start to form.
  
82,000,000 YBN
271) Angiosperm "Eurosids II" Order "Malvales" {moLVAlEZ} evolve.
Malvales includes
okra, marsh mallow {malO}, kola nut, cotton, hibiscus, balsa, and cacao {KoKoU}
(used in chocolate).
Americas  
82,000,000 YBN
272) Angiosperm "Eurosids II" Order "Sapindales" {SaPiNDAlEZ} evolves.
Sapindales includes maple, buckeye, horse chestnut, longan, lychee, rambutan,
guarana, bael, langsat (or duku), mahogany, cashew, mango, pistachio, sumac,
peppertree, poison-ivy, frankincense, and the citris trees: orange, lemon,
grapefruit, lime, tangerine, pomelo, and kumquat}.
Americas  
82,000,000 YBN
420) Hadrosaurs, Ornithopod {ORniTePoD} duck-billed dinosaurs.

Duck-billed dinosaurs (hadrosaurs) are common. The Hadrosaurs Maiasaurs are
examples of dinosaurs from which fossil nests, eggs, and baby dinosaurs have
been found.
  
82,000,000 YBN
500) Laurasiatheres "Insectivora" evolves (shrews, moles, hedgehogs).
  
81,000,000 YBN
281) Angiosperms "Euasterids I" family "Boraginaceae" (includes forget-me-not).
  
80,000,000 YBN
421) The Ornithiscian Ceratopsian dinosaurs evolve. Protoceratops, an early
shield-headed (ceratopsian) dinosaur fossil.

This is the first dinosaur discovered with fossil eggs. These eggs and nests
were found in Mongolia in the 1920's.
Mongolia, China  
80,000,000 YBN
422) Therapods {tERePoD} Dromaeosaurs {DrOmEoSORZ}: Raptor fossils.

Raptors (dromaeosaurs) are Cretaceous dinosaurs, which have large, hook claws
on their feet. Velociraptor is one example.

The most famous Velociraptor is a skeleton preserved in combat with a
Protoceratops from Mongolia, China.
  
80,000,000 YBN
482) Marsupials "Didelphimorphia" evolve (New World opossums).
Americas  
80,000,000 YBN
501) Laurasiatheres mammals "Megachiroptera" {KIroPTRu} (Old World fruit bats)
and "Microchiroptera" (Echolocating Bats) evolve.
Laurasia  
78,000,000 YBN
502) Laurasiatheres "Cetartiodactyla" {SiToRTEODaKTilu} evolve (ancestor of all
Artiodactyla {oRTEODaKTiLu} also called "even-toed ungulates" {uNGYUlATS or
uNGYUliTS}: camels, pigs, ruminants {includes deer, giraffe, cattle, sheep, and
antelope}, hippos, and all Cetacea {SiTASEu or SiTAsEu}: Whales, and
Dolphins).

Hippos are the closest living relative to whales.

Cetartiodactyla is an unranked taxonomic group, equivalent to a superorder,
containing the orders Artiodactyla and Cetacea. It is proposed on the basis of
molecular evidence suggesting a close evolutionary relationship between the two
orders.

The artiodactyla are an order comprising the even-toed ungulates (hoofed
mammals). There are two main radiations: the predominantly omnivorous
Bunodontia, including suoids (such as pigs, peccaries, and hippos); and the
more herbivorous Selenodontia, including camels and ruminants (such as deer,
giraffe, cattle, sheep, and antelope). Artiodactyla contains about 213 living
species, making it the fifth most speciose order of mammals. First known from
the early Eocene, artiodactyls have proliferated during the last 55 million
years to reach great diversity (especially among the family Bovidae). Their
radiation is often contrasted with that of the odd-toed ungulates, or
Perissodactyla (horses, rhinos, and tapirs). Artiodactyls are also important
for human economy and agriculture, comprising most of the domestic animals,
providing milk, wool, and most of the meat supply.

Ruminants are any of various hoofed, even-toed, usually horned mammals of the
suborder Ruminantia, such as cattle, sheep, goats, deer, and giraffes,
characteristically having a stomach divided into four compartments and chewing
a cud consisting of regurgitated, partially digested food.

Cetacea is an order or marine mammals that includes the whales, dolphins, and
porpoises, characterized by a nearly hairless body, anterior limbs modified
into broad flippers, vestigial posterior limbs, and a flat notched tail.
Laurasia  
77,000,000 YBN
483) Marsupials "Paucituberculata" evolve (Shrew opossums).

The Marsupial Order Paucituberculata contains 6 surviving species confined to
Andes mountains in South America.
Andes Mountains, South America  
76,000,000 YBN
503) Laurasiatheres order "Perissodactyla" {PeriSODaKTilu} evolve (also called
"odd-toed ungulates") {uNGYUlATS or uNGYUliTS} (Horses, Tapirs {TAPRZ },
Rhinos).

Perissodactyla is an order of herbivorous, odd-toed, hoofed mammals, including
the living horses, zebras, asses, tapirs, rhinoceroses, and their extinct
relatives. They are defined by a number of unique specializations, but the most
diagnostic feature is their feet. Most perissodactyls have either one or three
toes on each foot, and the axis of symmetry of the foot runs through the middle
digit.
Laurasia  
75,000,000 YBN
423) Ceratopsian dinosaurs are common (Monoclonius, Styrakosaurus,
Triceratops). Triceratops, is the largest of its kind, reaching 30 feet in
length.
  
75,000,000 YBN
492) Afrotheres: Aardvark.
Africa  
75,000,000 YBN
504) Laurasiatheres order "Carnivora" (Cats, Dogs, Bears, Weasels, Hyenas,
Seals, Walruses).
Laurasia  
75,000,000 YBN
505)
Laurasia  
74,000,000 YBN
280) Angiosperm "Euasterids I" order "Lamiales" {lAmEAlEZ} evolves.

Lamiales includes lavender, mint, peppermint, basil, marjoram {moRJ uruM},
oregano, perilla, rosemary, sage, savory, thyme, teak, sesame, corkscrew
plants, bladderwort, snapdragon, olive, ash, lilac, and jasmine.
  
73,000,000 YBN
484) Australian Marsupial Order Peramelemorphia evolves (Bandicoots and Bilbies
{BiLBEZ}).
Australia  
70,000,000 YBN
424) Two of the largest meat-eating dinosaurs known are common (both Therapods
{tERePoD}): Tyrannosaurus rex is the top predator in North America and
Giganotosaurus is in South America.
Americas  
70,000,000 YBN
425) The Thyreophoran {tIRrEoFereNZ} ankylosaurs evolve (shield back and/or
clubbed tail dinosaurs) and are the most heavily armored land-animals known.
These plant-eating dinosaurs are low to the ground for optimal protection. Many
have spikes that stick out from their bone-covered back. Ankylosaurus even has
bony plates on its eyelids.
  
70,000,000 YBN
426) Mosasaurs {mOSeSORZ}, marine reptiles evolve.
  
70,000,000 YBN
469) Birds "Podicipediformes" {PoDiSiPeDeFORmEZ} (grebes {GreBS}).
  
70,000,000 YBN
493) Afrotheres: Tenrecs and golden moles.
Africa  
70,000,000 YBN
494) Afrotheres: Elephant Shrews.
Africa  
70,000,000 YBN
507) Placental Mammal Order "Lagomorpha": Rabbits, Hares, and Pikas {PIKuZ}.

Rabbits were once classified as rodents, because they also have very prominent
gnawing teeth at the front, but were separated into their own order called
"Lagomorpha". Lagomorphs and rodents are grouped together in a cohort named
"Glires".
  
70,000,000 YBN
516) Placental Mammals: Tree Shrews and Colugos {KolUGOZ}.
  
70,000,000 YBN
1383) Theropod Giant bird-like dinosaur Gigantoraptor.
  
66,000,000 YBN
120) Largest Pterosaur and largest flying animal ever known, Quetzalcoatlus
{KeTZLKWoTLuS}.
Quetzalcoatlus has a wing span of 40 ft.
  
65,500,000 YBN
129) End of the Mesozoic and start of the Cenozoic Era, and the end of the
Cretaceous (145.5-65.5 mybn), and start of the Tertiary (65.5-1.8 mybn) Period.
  
65,500,000 YBN
397) End-Cretaceous mass extinction. 47% of all genera are observed extinct.
Dinosaurs
become extinct.
Also called the K-T (Kretaceous-Tertiary) extinction.
Huge amounts of lava erupted
from India, and a comet or meteor collided with the Earth in what is now the
Yucatan Peninsula of Mexico. No large animals survived on land, in the air, or
in the sea.

Extinction of 60% of plant species, and all dinosaurs, mosasaurs, pterodactyls,
plesiosaurs and pliosaurs.
  
65,000,000 YBN
429) There is a rapid increase in new species of fossil mammals after the
extinction of the dinosaurs.

Most early Cenozoic mammal fossils are small.
  
65,000,000 YBN
468) Birds "Gruiformes" {GrUiFORmEZ} evolve (cranes, rails, bustards).
  
65,000,000 YBN
470) Birds "Strigiformes" {STriJiFORmEZ} evolve (owls).
  
65,000,000 YBN
485) Australian marsupial order "Notoryctemorphia" evolve (Marsupial moles).
Australia  
65,000,000 YBN
486) Australian Marsupial order "Dasyuromorphia" (Tasmanian Devil, Numbat).
Australia  
65,000,000 YBN
487) Marsupial Order "Microbiotheria" evolves (Monita Del Monte).
  
65,000,000 YBN
488) Australian Marsupial Order "Diprotodontia" {DIPrOTODoNsEu} evolve
(Wombats, Kangeroos, Possums, Koalas).
Australia  
65,000,000 YBN
508) Rodents evolve. Mammal Order "Rodentia".
Rodent suborder: "Myomorpha" {MIemORFu}
(rats, mice, gerbils, voles {VOLZ}, lemmings, hamsters).

Rodents are an order of mammals characterized by a single pair of ever-growing
upper and lower incisors, a maximum of five upper and four lower cheek teeth on
each side, and free movement of the lower jaw in an anteroposterior direction.

Rodents are the most diverse group of mammals on Earth, consisting of over 2000
species, more than 40% of the known species of mammals on Earth today. Rodents
range in size from mice, weighing only a few grams, to the Central American
capybara, which is up to 130 cm (4 ft) in length and weighs up to 79 kg (170
lb). Rodents have been found on every continent except Antarctica. Rodents
include the semiaquatic swimming (beavers and muskrats), gliding ("flying"
squirrels), burrowing (gophers and African mole rats), arboreal (dormice and
tree squirrels), and hopping (kangaroo rats and jerboas). Nearly all rodents
are herbivorous, with a few exceptions that are partially insectivorous to
totally omnivorous, such as the domestic rat. The great adaptability and rapid
evolution and diversity of rodents are mainly due to their short gestation
periods (only 3 weeks in some mice) and rapid turnover of generations. The most
diagnostic feature of the Rodentia is the presence of two pair of ever-growing
incisors (one pair above and one below) at the front of the jaws. These teeth
have enamel only on the front surface, which allows them to wear into a
chisellike shape, giving rodents the ability to gnaw.
  
65,000,000 YBN
509) Rodents: Beavers, Pocket gophers, Pocket mice and kangaroo rats evolve.
  
65,000,000 YBN
807) Ancestor of camels and llamas splits from the Even-Toed Ungulates line
(Cetardiodactyla).

This is just after death of dinosaurs. Both these ancestors are still small
and probably look like shrews.
  
64,000,000 YBN
585) Birds Psittaciformes {SiTaS-iFORmEZ} (Parrots).
  
63,000,000 YBN
510) Rodents: Springhares and Scaly-tailed Squirrels.
  
63,000,000 YBN
587) Primates evolve, most likely in Africa or the Indian subcontinent.

The order primates contains more than 300 species, including monkeys, apes, and
humans. The primates are one of the most diverse orders of mammals on Earth.
They include the lemurs (more than 70 species in six families), the lorises
(three or more species in one subfamily), the tarsiers (six or more species in
one family), the New World monkeys (almost 100 species in five families), the
Old World monkeys (more than 100 species in one family), and the apes and
humans (about 20 species in two families). The oldest known fossil remains of
primates are about 60 million years old.

Unlike most other mammalian orders, the primates cannot be defined by a
diagnostic suite of specializations, but are characterized by a combination of
primitive features and progressive trends. These include: 1) Increased
dominance of vision over olfaction, with eyes more frontally directed,
development of stereoscopic vision, and reduction in the length of the snout.
2) Eye sockets of the skull completely encircled by bone. 3) Loss of an incisor
and premolar from each half of the upper and lower jaws with respect to
primitive placental mammals. 4) Increased size and complexity of the brain,
especially those centers involving vision, memory, and learning. 5) Development
of grasping hands and feet, with a tendency to use the hands rather than the
snout as the primary exploratory and manipulative organ. 6) Progressive
elaboration of the placenta in conjunction with longer gestation period, small
litter size (only one or two infants), and precocial young. 7) Increased period
of infant dependency and more intensive parenting.
Africa or India  
62,000,000 YBN
495) Afrotheres: Elephants.
Africa  
60,000,000 YBN
430) In South America, the Andes mountains start to form.
  
60,000,000 YBN
431) Earliest fossil rodent.
  
60,000,000 YBN
432) The cat-like Laurasiatheres Creodonts {KrEuDoNTS} like Oxyaena are
common.

Creodonts are the dominant predators throughout the Eocene and Oligocene and
occupy many of the same niches as the carnivores which eventually replace them.
There are two families of Creodonts, Oxyaenidae and the more widespread
Hyaenodontidae which includes Megistotherium one of the largest land predators
to have ever lived.

The last creodont, Dissopsalis carnifex, became extinct about 9 million years
ago, giving the group a more than 50-million-year history.
  
60,000,000 YBN
586) Earliest primate fossils.

The earliest primate fossils belong to the primate order "Plesiadapiformes" and
are found near the start of the Paleocene (~55 mybn). These include Purgatorius
from Montana, Plesiadapis, and Dryomomys from Wyoming, and Altiatlasius which
appears in Africa and is known from a handful of isolated upper and lower teeth
from Morocco.

During the early Cenozoic the Earth is much warmer and more densely populated
with plants and trees, and there is a large diversity of different early
primates, but the planet becomes cooler and drier in the Oligocene and the
forests disappear and primates vanish from North America and Europe and become
restricted to Southeast Asia and Africa. During the Oligocene, one group of
primates, the New World Monkeys (Cebidae) manage to cross the South Atlantic
Ocean and then radiate into great diversity.
Morocco, Africa, (Willwood Formation) Clarks Fork Basin, Wyoming, USA), and
Montana, USA  
60,000,000 YBN
796)
  
60,000,000 YBN
808) The ancestors of pigs splits from the line that leads to the Ruminants
(cattle, goats, sheep, giraffes, bison, buffalo, deer, wildebeast, antelope),
hippos, dolphins, and whales.
  
59,000,000 YBN
496) Afrotheres: Hyraxes.
Africa  
59,000,000 YBN
497) Afrotheres: Manatee and Dugong.
  
58,000,000 YBN
511) Rodents: Dormice, Mountain Beaver, Squirrels and Marmots {moRmuTS}.
  
58,000,000 YBN
524) Primates: Tarsiers {ToRSERZ}.
  
57,000,000 YBN
433) Earliest hooved mammal fossil.
Earliest hooved mammal fossil.
  
55,800,000 YBN
588) Widespread appearance of primates.

Cantius and Teilhardina are the earliest euprimates in North America, followed
quickly by Steinius and others. Cantius and Teilhardina also appear in Europe
with Donrussellia.
  
55,000,000 YBN
435) Rhinoceros-like Placental mammals Uintatherium {YUiNTutEREuM} are the
largest land animals at this time.
  
55,000,000 YBN
436) Horses. Earliest fossil horse, Hyractotherium, about the size of a dog).
  
55,000,000 YBN
512)
  
55,000,000 YBN
809) Last common ancestor of Ruminants with Hippos, Dolphins and Whales.
  
54,970,000 YBN
434) Earliest primate skull.

From the Hunan Province, China. Other fossils from the same genus are found in
Europe.
The earliest euprimates can be distinguished as Cantius, Donrussellia and
Teilhardina.
Hunan Province, China  
54,000,000 YBN
810) Last common ancestor between hippos with dolphins and whales.
  
53,500,000 YBN
812) Earliest fossils of marine mammal "Pakicetus".
  
52,500,000 YBN
6179) Earliest bat fossils (Icaronycteris and Onychonycteris).
(Green River Formation) Wyoming  
51,000,000 YBN
513) Rodents: Old World Porcupines.
  
50,000,000 YBN
437) Elephants. Earliest elephant fossil, an unnamed fossil from Algeria.
Algeria, Africa  
50,000,000 YBN
438) Himalayan mountains start to form as India collides with Eurasia.
This
will continue for millions of years.
Himalyia Mountains, India  
50,000,000 YBN
518) Primates: Lorises {LORiSEZ}, Bushbabies, Pottos {PoTTOZ}.
  
50,000,000 YBN
816) Earliest Ambulocetus (an early whale) fossil.
  
49,000,000 YBN
439) The largest meat-eating land animals of the Paleocene and Eocene epochs
were flightless birds, like Diatryma from America, and Gastornis from Europe.
  
49,000,000 YBN
472) Birds "Caprimulgiformes" (nightjars, night hawks, potoos, oilbirds).
  
49,000,000 YBN
474) Birds "Falconiformes" {FaLKeNiFORmEZ} (falcons, hawks, eagles, Old World
vultures).
  
49,000,000 YBN
514)
  
49,000,000 YBN
515) Rodents: New World porcupines, guinea pigs, agoutis {uGUTEZ}, capybaras
{KaPuBoRoZ}.
  
46,000,000 YBN
817) Earliest Rodhocetus fossil (early whale).
  
45,000,000 YBN
519) Primate: Aye-aye {I-I}.
  
40,000,000 YBN
440) In Europe the Alpine mountains start to form.
Alpine mountains  
40,000,000 YBN
441)
  
40,000,000 YBN
525) Ancestor of all Primates "New World Monkeys" (Sakis, Spider, Howler and
Squirrel monkeys, Capuchins {KaP YU CiNZ}, Tamarins).

The ancestor of all New World monkeys probably originates in Africa, but all
surviving descendants now live in the Americas, which suggests that a small
group of New World monkeys got across the early Atlantic Ocean to South
America, perhaps by rafting on fallen trees over a chain of islands.
Africa  
40,000,000 YBN
815) Earliest Basilosaurus fossil (early whale).
Basilosaurus was renamed "Zeuglodon"
by Richard Owen because it is a mammal not a reptile (saurus=lizard).
  
37,000,000 YBN
442) Oldest fossil of dog, similar to a weasel, Hesperocyon.
  
37,000,000 YBN
471) Birds "Apodiformes" {oPoD-i-FORmEZ} (hummingbirds, swifts).
  
37,000,000 YBN
473)
  
37,000,000 YBN
475) Birds: Cuculiformes {KUKUliFORmEZ} evolve (cuckoos, roadrunners).
  
37,000,000 YBN
476) Birds "Piciformes" {PESiFORmEZ} (woodpeckers, toucans).
  
35,000,000 YBN
811) Last common ancestor of dolphins and whales.

(Toothed and Baleen split.)
  
34,000,000 YBN
813)
  
34,000,000 YBN
814) Earliest Baleen {BulEN} whale fossils, Janjucetus and Llanocetus.
  
33,000,000 YBN
560) Primates Aegyptopithecus evolves in East Africa.
  
30,000,000 YBN
443) The largest land mammal ever known, the hornless Rhinoceros,
Paraceratherium lives at this time.
India  
30,000,000 YBN
520) Primates: True Lemurs.
  
28,000,000 YBN
477) Birds "Passeriformes" {PaSRiFORmEZ} (perching songbirds) evolve. This
order includes many common birds: crows, jays, sparrows, warblers,
mockingbirds, robins, orioles, bluebirds, vireos {VEREOZ}, larks, finches.

More than half of all species of bird are passerines. Sometimes known as
perching birds or, less accurately, as songbirds, the passerines are one of the
most spectacularly successful vertebrate orders: with around 5,400 species,
they are roughly twice as diverse as the largest of the mammal orders, the
Rodentia.
  
27,000,000 YBN
521)
  
25,000,000 YBN
444) Earliest cat fossil, "Proailurus".
  
25,000,000 YBN
522)
  
25,000,000 YBN
531) Ancestor of all Primates "Old World Monkeys" (Macaques, Baboons,
Mandrills, Proboscis and Colobus {KoLiBeS} monkeys).

This is also the last common ancestor of the Old World monkeys and the
hominoids, the superfamily Hominoidea, which includes apes and humans.

There are around 100 species of Old World Monkey.
(perhaps around Lake Victoria) Africa  
24,000,000 YBN
662) The ancestor of all Hominoids (Gibbons and Hominids) loses its tail.

This may be a genetic mutation or because a tail might be an obstacle for
species like gibbons that swing from branch to branch as opposed to more
ancient primates that leap from branches.
  
23,000,000 YBN
478) Monotreme: Echidna.
Australia, Tasmania and New Guinea  
23,000,000 YBN
479) Monotreme: Duck-Billed Platypus.
Australia and Tasmania  
22,000,000 YBN
526) New World Monkeys: Sakis, Uakaris {WoKoREZ}, and Titis {TETEZ}.
  
22,000,000 YBN
527) New World Monkeys: Howler, Spider and Woolly monkeys.

  
22,000,000 YBN
528) New World Monkeys: Capuchin {KaPYUCiN} and Squirrel monkeys.

Americas  
22,000,000 YBN
558) Afropithecus evolves in Africa.

This tree-dwelling ape had some anatomical features in common with the
better-known Proconsul, and it also seems to have been closely related to
Sivapithecus as well.
  
22,000,000 YBN
559) Hominoid Proconsul evolves in East Africa.
  
21,000,000 YBN
529) New World Monkeys: Night (or Owl) monkeys.
  
21,000,000 YBN
530) New World Monkeys: Tamarins {TaMariNZ} and Marmosets {moRmoSeTS}.
  
21,000,000 YBN
556) Hominoid Kenyapithecus evolves in Africa.
  
20,000,000 YBN
549) The ancestor of all Homonids may move (over land) from Africa into
Eurasia.

An alternative theory has this ancestor in Africa, with a large number of
Africa to Eurasia migrations by later species.
  
18,000,000 YBN
537) Primates: Gibbons.
Gibbons are very sexual, and polygamous.
There are 12 species of Gibbons.
South-East Asia  
16,000,000 YBN
555) Hominoid Oreopithecus.
  
15,000,000 YBN
553) Lufengpithecus evolves in China.

  
14,000,000 YBN
542) Earliest extant Hominid: Orangutans.
South-East Asia  
13,000,000 YBN
551) Dryopithecus evolves in Eurasia.
  
12,500,000 YBN
552) Hominoid Sivapithecus, possible ancestor of modern orangutan. The animal
was about the size of a chimpanzee but had the facial morphology of an
orangutan; it ate soft fruit (detected in the toothwear pattern) and was
probably mainly arboreal.
Petwar platein, Pakistan and India  
10,500,000 YBN
538) Gibbons: Crested Gibbons.
South-East Asia  
10,000,000 YBN
533) Old World Monkeys: Colobus {KoLiBeS} monkeys.
Africa  
10,000,000 YBN
534) Old World Monkeys: Langurs {LoNGURZ} and Proboscis monkeys.

Asia  
10,000,000 YBN
535) Old World Monkeys: Guenons {GenONZ}.

  
10,000,000 YBN
543) Hominids: Gorillas evolve in Africa.

The earliest possible Gorilla fossils, are some teeth found in Ethiopia and
date to around 10 million years old and a jaw from Kenya that is around 9.8
million years old.
Africa  
9,000,000 YBN
550) The ancestor of all Gorillas, Chimpanzees, and archaic humans may move
over land from Eurasia back into Africa.

Alternatively, this ancestor could have evolved in Africa if many earlier
ancestors frequently migrated to Eurasia.
  
7,750,000 YBN
539) Gibbons: Siamangs {SEumANGZ}.
South-East Asia  
6,000,000 YBN
540) Gibbons: Hylobates {HIlOBATEZ}.
South-East Asia  
6,000,000 YBN
541) Gibbons: Hoolocks {HUleKS}.
South-East Asia  
6,000,000 YBN
544) Chimpanzees evolve. Last common ancestor of chimpanzees and humans.
Africa  
6,000,000 YBN
565) Hominid fossils "Toumai" (Sahelanthropus), from Chad, central Africa
Kingdom:
Animalia
Phylum: Chordata
Class: Mammalia
Order: Primates
Family: Hominidae
Subfamily: Homininae
Tribe: Hominini
Subtribe: Hominina
Genus:
Sahelanthropus (Brunet et al, 2002)
Species: S. tchadensis (Brunet et al, 2002)
Chad, Central Africa  
6,000,000 YBN
566) Hominid fossils "Orrorin" in Kenya, east Africa.
Lukeino Formation, Kenya  
6,000,000 YBN
1490)
Argentina  
5,000,000 YBN
554) Hominid Gigantopithecus {JIGaNTOPitiKuS} evolves in China.
  
4,400,000 YBN
546) Hominid: Ardipithecus. Earliest bipedal primate.

Some theories to explain why bipedalism evolved are:
1) to carry food home, for
later use or for others (a leopard uses its jaws)
2) using weapons is easier
3) walking may
be more efficient in traveling long distances.
4) sexual selection

Primates walking upright on two legs may signal that hominids have become the
top of the food chain on land, which might be the result of the use of tools,
since other land animals cannot defend themselves or attack others with tools.
Lukeino Formation, Tugen Hills, Kenya, Africa  
4,000,000 YBN
547) Hominid: Australopithecus (x-STrA-lO-PitiKuS}.
Sterkfontein, South Africa  
3,700,000 YBN
570) Hominid footprints in Laetoli {lITOlE}, thought to be made by
Australopithicus Afarensis.

Some analysts have noted that the smaller of the two clearest trails suggests
that whoever left the prints was burdened on one side - perhaps a female
carrying an infant on her hip.
Laetoli, Tanzania  
3,390,000 YBN
269) Hominids use stones as tools. Earliest evidence of stone used as tool.
Dikika, Ethiopia  
3,180,000 YBN
571) Australopithecus afarensis fossil, "Lucy".
  
3,000,000 YBN
446) North and South America connect.
  
2,700,000 YBN
564) Hominid: Paranthropus {Pa raN tru PuS}, a line of extinct early bipedal
hominids.
Africa  
2,500,000 YBN
455) Oldest formed stone tools.

This begins the Paleolithic or "Stone Age".

Other species have been observed to use tools, including Chimpanzees using
sticks they sharpen with their teeth to rouse pray.
Gona, Ethiopia  
2,400,000 YBN
827)
  
2,200,000 YBN
447) Hominids: Homo Habilis evolve in Africa (earliest member of the genus
"Homo").

This is when the human brain begins to get bigger.

Homo habilis is thought to be the ancestor of Homo ergaster.

As the habilis brain grows, habilis gains a larger memory for storing sensory
information such as eye images, sounds, pain, etc. and to play back remembered
images and sounds in thought.
(Kenya and Tanzania) Africa  
2,000,000 YBN
545) Hominids: Bonobos {BunOBOZ}.
Africa  
1,800,000 YBN
130) End of the Tertiary {TRsEARE} (65-1.8 mybn), and start of the Quaternary
{KWoTRnARE or KWoTRNRE} (1.8 mybn-now) Period.
  
1,800,000 YBN
563) Homo erectus {hOmO ireKTuS} evolves.

Some people call Homo Erectus in Africa, "Homo Ergaster", and think that
Ergaster leaves Africa and evolves into Homo erectus in Asia, and into Homo
Neaderthalensis in Europe and western Asia.
Lake Turkana, East Africa  
1,700,000 YBN
449) Homo erectus moves into Eurasia from Africa.

Homo sapiens have been around for only 200,000 years, but Homo erectus lived
for almost a million years before going extinct.
  
1,500,000 YBN
583) Earliest evidence of use of fire, burned bones from Swartkrans cave in
South Africa.

This fire could have been made by Australopithecus (or Paranthropus) robustus
and an early species of Homo, possibly Homo erectus.
(Swartkrans cave) Swartkrans, South Africa  
1,440,000 YBN
448) Latest Homo Habilis fossil.

This skull shows that Homo habilis and Homo erectus both were living at this
time.
Kenya, Africa  
1,000,000 YBN
589) Homo erectus evolves less body hair, except head hair, facial hair,
airpit, chest and groin areas.

This is thought to be driven by male sexual selection of less haired females,
perhaps because less hair means less body lice and so is more desirable.

No other surviving apes have taken this direction. Perhaps wearing furs and
other clothes for heat may have eliminated the need for bodily hair.
  
1,000,000 YBN
1479)
Madrid, Spain  
970,000 YBN
200) Hominids wear clothing.

That humans (Homo antecessor) wear clothing at this time is implied by the cold
climate that occurred at the same time that stone tools found in the area were
used.

The earliest genetic evidence of humans wearing clothes, is based on the
differences of the head and body louse and puts the change to around 80,000
years before now.
Happisburgh, Norfolk, UK  
790,000 YBN
584)
Gesher Benot Ya`aqov, Israel  
400,000 YBN
615) Oldest evidence of spear.
Schöningen, Germany.  
200,000 YBN
548) Humans (Homo sapiens) evolve in Africa.

The oldest Homo sapiens fossils (Omo I and II) are from Ethiopia.
Ethiopia, Africa  
200,000 YBN
561) Genetic evidence that complex human language evolves in early Homo
species.
  
200,000 YBN
590) Humans language of thirty short sounds begins to develop. All words are
single syllable.

This is the beginning of the transition from the verbal language of chimps and
monkeys, that will result in the "staccato" (short sound duration) language
humans use now.

Either the majority of the 30 basic sounds in human language (U, o, K, S, etc.)
were learned before humans moved out of Africa, or after. That sapiens of
Eurasia, Australia and America do not have unique base sounds is evidence that
the 30 plus base sounds of all human language completely developed in Africa
before the sapiens movement from Africa into Eurasia, Australia and the
Americas. In addition, that the native humans of Eurasia, Australia and America
have different words, is evidence that word of mouth, being not adequate to
spread words, was not adequate to spread the base sounds shared by all humans,
after their move out of Africa.

It is difficult to determine when but probably early Homo sapiens in Africa
evolve a larger vocabulary of sound combinations to label objects and
activities than the other more primitive primates like the chimpanzees.

These sounds eventually become shortened and more finely controlled, perhaps
quicker communication being a selective advantage, and ultimately evolve to the
30 plus basic sounds used to construct words in all human languages. The vowel
sounds may develop before any consonants. Perhaps the earliest vowels are: U
(food), o (mama), O (no), E (eat) and perhaps i (big), e (bed), u (cup). (These
sounds are in use by the first Sumerian writing.) For centuries early human
language may have been vowels only until consonants attached to vowels are
added and in regular use.

The first consonants are probably (the so-called "stop consonants") T and D,
then K and G, then perhaps B and P. But it may be impossible to know the order,
and the number of years between the three sound families.

Initially, this language may be very simple, one sound applying to many objects
and situations. Some time near here, words made of more than one sound
(compound words) evolves, then objects and actions might have compound sounds,
although still one word.

Clearly many mammals and birds have a vocabulary of remembered sounds, which
are used to label other species, objects, and situations. Chimpanzees use
sounds that sound similar to sounds humans make, for example the U (in food),
and perhaps "E", although not sounded in short duration breaths.

Perhaps the development of language is assisted by trading which requires
object name translation, because these new sounds and words are remembered,
accepted, and included into the language of both trading groups.

Clearly some less common vowel sounds evolve later based on these main sounds,
for example "i" (big), "u" (cup), "v" (food), "a" (cat), etc.

Perhaps there are some base (letter) sounds that have been lost to the past.
  
190,000 YBN
601) The "Stop" family of sounds, B, D, G, K, P and T are in use.

The major sounds of language for any species can be cataloged and sorted into
groups. Humans language has 30 or so base sounds which can be grouped into at
least 4 major families, all of which probably originated at different times.

The short duration, "stop" family of sounds (B,D,G,K,P,T) probably evolve the
earliest of all consonent sounds in the language of sapiens. Initially, these
sounds may have formed (naturally) before the long vowel sound (for example a
"B" sound when opening the mouth to howl a vowel sound). This language may be
simply single syllable consonant plus vowel words (for example "GO", "Po",
etc.) with short durations. This is basically the form of language all humans
use today, short duration (50 ms each) sounds from a family of only 30 sounds,
combined together to form words used to describe objects and activities
(nouns), movements and actions (verbs), and later a second word added to
further describe objects (adjectives) and actions (adverbs).

This "short duration" language, means communication must have been very routine
and optimized, which implies that this happened through hunting or perhaps
through trading where language is a selective advantage.
  
170,000 YBN
600) The "Fricative" sound family is in use (the sounds S, Z, s, H, F, V).

The "S" sounds may have been an imitation of snakes, and may have represented
an early snake alarm signal to others. The sound "s" may be related to cause
fear in others to signal to be quiet.
  
160,000 YBN
591) Second oldest human (Homo sapiens) skull, like the oldest in Ethiopia,
Africa.
Ethiopia, Africa  
150,000 YBN
592) The sounds M, N, L, and R are in use.

The M and N family are called "Nasals", and the L and R family are called
"Liquids".
  
130,000 YBN
450) Homo Neanderthalensis evolves in Europe and Western Asia.

The oldest Neanderthal fossil is from Croatia.

For decades, anthropologists treated Neanderthals as a subspecies of Homo
sapiens, (Homo sapiens Neaderthalensis), but recent work suggests that they
were a distinct species and did not interbreed with or give rise to Homo
sapiens sapiens. The best evidence for this comes from the Skhul and Qafzeh
caves in Israel, where layers bearing Neaderthals remains are interbedded and
alternate with layers containing early modern humans. In addition, Neaderthals
appear later than the earliest archaic Homo sapiens, so they can not be the
ancestors of Homo sapiens. Recently Neaderthal DNA has been sequenced, and they
are clearly not Homo sapiens, and are now named Homo Neaderthalensis.

Neanderthal mitochondrial DNA has been compared to sapiens and a common
ancestor of the two is estimated to be 500,000, long before the oldest sapien
fossils in Africa, which supports the idea that sapiens did not evolve or
interbreed with Neanderthals.
Europe and Western Asia  
120,000 YBN
572) Start of Wurm glaciation (120,000-20,000 YBN), which connects a land
bridge between Asia and America.
  
100,000 YBN
[98000 BC]
257) Theory of Gods.

The explanation that many phenomena in the universe are controlled by objects
with human and animal bodies that have supernatural powers is one of the
earliest theories that tries to explain how the universe works.

This theory will last for all of recorded history to the present time, over
5000 years. Although polytheism will fall in popularity to monotheism which is
introduced around 1300 BCE by the Egyptian Pharoah Amenhotep IV.

The theory of gods is recorded in the earliest recorded stories of history 4600
years before now.

The theory that a god or gods controls the universe is perhaps the oldest
theory that is still believed by some humans.

Perhaps by this time Humans have created a word to mean "every thing" like
"universe" or "world".
Africa  
100,000 YBN
[98000 BC]
6333)
(es-Skhul cave) Mount Carmel, Israel  
95,000 YBN
[93000 BC]
594)
  
92,000 YBN
[90000 BC]
597) Oldest Homo sapiens skull outside Africa, in Israel, the Jebel Qafzeh
skull.
(Skhul Cave) Mount Carmel, Israel  
60,000 YBN
[58000 BC]
573) Earliest evidence of humans in Americas, from a rock shelter in Pedra
Furada, Brazil.
The evidence is controversial. Some people argue that the chipped
stones are geoartifacts, but the artifact finders argue that the chips are too
regular to be made from falling rocks.
  
53,300 YBN
[51300 BC]
557) Homo Erectus extinct. Most recent Homo Erectus fossil in Southeast Asia
(Java).
This shows that Homo erectus lived at the same time as Homo sapiens.
These ages are
20,000 to 400,000 years younger than previous age estimates for these hominids
and indicate that H. erectus may have survived on Java at least 250,000 years
longer than on the Asian mainland, and perhaps 1 million years longer than in
Africa.
Ngandong, Indonesia  
46,000 YBN
[44000 BC]
577) Earliest evidence of water ship. Sapiens from Southeast Asia reach
Australia by water ship.

Earliest sapians fossils Australia, "Mungo man".
  
43,000 YBN
[41000 BC]
1187) Earliest known mine: "Lion Cave" in Swaziland, Africa is in use. At this
site, which by radiocarbon dating is 43,000 years old, paleolithic humans mined
for the iron-containing mineral hematite, which they ground to produce the red
pigment ochre. Sites of a similar age where Neanderthals may have mined flint
for weapons and tools have been found in Hungary.
Swaziland, Africa  
40,800 YBN
[01/01/38800 BC]
1262) Earliest known human-made painting.

In El Castillo Cave in Spain, one of several large red disks on the "Panel de
las Manos", made by using a blowing technique, has a minimum age of 40.8 ky.
This age is measured using uranium-series disequilibrium of calcite deposits
overlying or underlying the cave art. This implies that depictions of the human
hand are among the oldest art known from Europe. The cave art may have been
created by the first anatomically modern humans in Europe or possibly by
Neanderthals.
(The Panel de las Manos,) El Castillo Cave, Spain|Southern France  
40,000 YBN
[38000 BC]
598) Oldest Homo sapiens fossils in Europe from the Cro-Magnon site in France
This
time (40,000 YA) also marks the decline of Neaderthal populations until their
extinction 10,000 years later.
  
40,000 YBN
[38000 BC]
604) Earliest evidence of oil lamp.
Southwest France  
40,000 YBN
[38000 BC]
5871) Oldest indisputable musical instrument, a flute made from the wing bone
of a vulture.
Hohle Fels Cave, Germany  
39,000 YBN
[37000 BC]
599) Sapiens reach China.

Earliest Homo sapiens fossil in China, from the Zhoukoudian Cave in China.
(Tianyuan Cave) Zhoukoudian, China  
38,000 YBN
[36000 BC]
574)
  
35,000 YBN
[33000 BC]
3943)
Hohle Fels Cave, Germany  
35,000 YBN
[33000 BC]
4191)
Russia  
32,000 YBN
[30000 BC]
602) Weaving and textiles.

The earliest evidence of weaving are 32,000 year old flax fibers. Some of the
flax fibers are spun, dyed, and knotted.

Other early evidence of weaving is from textile and flexible basketry
impressions on burnt clay from Pavlov in the Czech Republic which date to
between 27,000-25,000 ybn (see image). The oldest woven cloth so far discovered
is made from flax, dates to about 9000 ybn, and comes from Çayönü, Turkey.
Dzudzuana Cave, Georgia  
31,700 YBN
[29700 BC]
42) Humans raise dogs. (Dog domesticated). One theory supported by evidence is
that dog anatomy changes abruptly from wolf anatomy as a result of
domestication by humans.
Goyet cave, Belgium  
30,000 YBN
[28000 BC]
575) Mitochondrial DNA shows a sapiens migration to the Americas now.
  
29,000 YBN
[27000 BC]
6215) Earliest ceramic object, the Venus figurines.

The Venus figurines are created around this time. The Venus of Dolní
Věstonice is the oldest of these ceramic objects at 29,000 years old. This
figurine, together with a few others from nearby locations, is the oldest known
ceramic in the world, predating the earliest pottery of China (18,000) by
11,000 years. Some of the figurines appear to be wearing clothing.
Dolni Věstonice, Czechoslovakia  
28,000 YBN
[26000 BC]
451) Neanderthals extinct. Most recent Neanderthal fossil.

Genetic evidence suggests interbreeding took place with Homo sapiens between
roughly 80,000 and 50,000 years ago in the Middle East, resulting in 1–4% of
the genome of people from Eurasia having been contributed by Neanderthals.
Gorham's Cave, Gibraltar, Spain  
26,000 YBN
[24000 BC]
6224) Earliest "fired" clay (clay dried and hardened by fire).
Dolní Věstonice, Pavlov, Czech Republic  
23,000 YBN
[21000 BC]
6231) Earliest human-made structure. A stone wall. The oldest wall in Jericho,
also a stone wall dates to 8,000 BCE.
(Theopetra Cave) Kalambaka, Greece  
20,000 YBN
[18000 BC]
576) Y Chromosome DNA shows a sapiens migration to the Americas now.
  
20,000 YBN
[18000 BC]
1291)
in the Peloponnese, in the southeastern Argolid, is a cave overlooking the
Argolic Gulf opposite the Greek village of Koilada.  
19,000 YBN
[17000 BC]
6184) Cereal gathering.
Near East (Southwest Asia Turkey, Lebanon, Israel, Iraq, Jordan, Saudi
Arabia)  
18,000 YBN
[16000 BC]
603) Oldest evidence of pottery.

The oldest known ceramic objects are the "Venus" figurines which date back to
29,000 years before present, 11,000 years earlier.
(Yuchanyan cave), Daoxian County, Hunan Province, China  
17,000 YBN
[15000 BC]
6225) Earliest rope, a 30 cm fragment of rope, only 7 or 8 mm in diameter.
Lascaux, France  
14,000 YBN
[12000 BC]
6227) Earliest known map.
Mezhirich, Ukraine  
13,000 YBN
[11000 BC]
578) Humans enter America. Oldest human bones in America.

The earliest bones of a human in the Americas, a skull (Peñon woman) from
Mexico and bones from "Arlington Springs" woman, in the California Channel
Islands date to now.

These three bones are discovered on the Channel Islands, on a ridge called
Arlington, just off the California coastline.
Mexico City and Arlington Canyon on Santa Rosa Island, California, USA  
13,000 YBN
[11000 BC]
579)
  
12,500 YBN
[10500 BC]
582) Human artifacts from Monte Verde, southern Chile.

This date puts the possibility of walking over the Being Straight in doubt.
  
11,500 YBN
[9500 BC]
581) Spear Head from Clovis, New Mexico.
  
11,500 YBN
[9500 BC]
719) Earliest evidence of rice cultivation in China.
Yangtze (in Hubei and Hunan provinces), China  
11,130 YBN
[9130 BC]
1292)
=9130BCE  
11,000 YBN
[9000 BC]
606) Oldest city, Jericho.

Jericho is located in the West bank, near the Jordan river (east of
Mediterranean).

Jericho is one of the earliest continuous settlements on Earth, starting from
perhaps about 9000 bce. This city provides evidence of the first permanent
settlements.
Jericho, (modern West Bank) Palestine  
11,000 YBN
[9000 BC]
608) Oldest saddle quern {KWRN}.

A saddle quern consists simply of a flat stone bed and a rounded stone to be
operated manually against it, to grind grain into flour.
Abu Hureyra, Syria  
11,000 YBN
[9000 BC]
617) Goats kept, fed, milked, and killed for food.
Euphrates river valley at Nevali Çori, Turkey (11,000 bp), and the Zagros
Mountains of Iran at Ganj Dareh (10,000).  
11,000 YBN
[9000 BC]
1290)
Pangmapha district, Mae Hong Son Province, northwest Thailand  
10,700 YBN
[8700 BC]
829) Humans shape metal objects.
Oldest copper (and metal) artifact, from Northern
Iraq.
This starts the "Copper Age" (Chalcolithic).
This is a copper ear ring.
Copper is the first metal
shaped by humans.
Northern Iraq  
10,500 YBN
[8500 BC]
6315) Sheep raised for wool, skins, meat and dung (for fuel).
Northern Zagros to southeastern Anatolia|(Middle East) Eastern
Mediterranean  
10,350 YBN
[8350 BC]
828)
  
10,000 YBN
[8000 BC]
205) Pigs raised and killed for food.
(Near East) Eastern Mediterranean and Island South East Asia|southeastern
Anatolia  
10,000 YBN
[8000 BC]
614) Oldest evidence of bow and arrow.

The earliest potential arrow heads date from about 64,000 ybn in the South
African Sibudu Cave.

The first actual bow fragments are the Stellmoor bows from northern Germany.
Stellmoor (near Hamburg), Germany  
10,000 YBN
[8000 BC]
1259) Clay tokens of various geometrical shapes are used for counting in
Sumer.

From the neolithic age (7000 BCE) on, stone tokens used to represent counted
units, such as sheep or grain, are gradually replaced by tokens of baked clay.
Clay has the advantage of being formed into any desired shape. Clay tokens are
particularly popular in stoneless Babylonia. Large quantities of clay tokens
found in various geometric shapes such as spheres, rhombuses, discs, and
tetrahedrons are thought to represent different specific numerical values.

These tokens may initially be kept in small bags of materials like cloth or
leather. But after 4000 BCE, tokens will be kept inside clay bullas (spherical
clay sealed containers used to protect the contents until broken).
eastern Iran, southern Turkey, Israel, Sumer (modern Iraq)|Babylonia|Syria,
Sumer and Highland Iran  
10,000 YBN
[8000 BC]
6233)
Jericho (modern West Bank)  
10,000 YBN
[8000 BC]
6316) Cows raised for milk, meat and for plowing.
upper Euphrates Valley  
9,300 YBN
[7300 BC]
6185) Wheat grown.
southeastern Turkey and northern Syria (Nevali Cori, Turkey)  
9,240 YBN
[7240 BC]
1478) Oldest domesticated plants in the Americas. Squash grown in Peru.
Paiján, Peru  
9,000 YBN
[7000 BC]
273) Woven cloth. The oldest woven cloth is made from flax, comes from
Çayönü, Turkey.

Weaving apparently precedes spinning of yarn; woven fabrics probably originate
from basket weaving.
Çayönü, Turkey  
9,000 YBN
[7000 BC]
1288) Mehrgarh, an Indus Valley neolithic city begins now.

Mehrgarh is one of the most important Neolithic (7000 BCE to 3200 BCE) sites in
archaeology. Mehrgarh lies on the "Kachi plain of Baluchistan, Pakistan, and is
one of the earliest sites with evidence of farming (wheat and barley) and
herding (cattle, sheep and goats) in South Asia.
  
9,000 YBN
[7000 BC]
1289)
Iraq  
8,600 YBN
[6600 BC]
848) Symbols created on a tortoise shell from a neolithic grave in China may be
the ancestors of Chinese writing.

These symbols predate the earliest recorded writings from Mesopotamia by more
than 2,000 years. The archaeologists say they bear similarities to written
characters used thousands of years later during the Shang dynasty, which lasted
from 1700-1100 BC.

This creates a space of about 5,000 years between these symbols and the next
oldest which may indicate that they are not related.
Jiahu, in central China's Henan Province  
8,410 YBN
[6410 BC]
580)
  
8,200 YBN
[6200 BC]
1295)
Catal Huyuk  
8,000 YBN
[6000 BC]
605) Oldest known boat, the Pesse canoe, a dug-out boat.
Netherlands  
8,000 YBN
[6000 BC]
607) Oldest flint sickle.

A sickle has a semicircular blade and is used for cutting grain or tall grass.
Oldest
flint sickle.

A sickle has a semicircular blade and is used for cutting grain or tall grass.
Palestine  
8,000 YBN
[6000 BC]
609) Einkorn (one-seeded wheat) grown.
  
8,000 YBN
[6000 BC]
610) Flax grown. The flax plant is the source of flaxseed for linseed oil and
fiber for linen products.
  
8,000 YBN
[6000 BC]
612) Barley grown.
  
8,000 YBN
[6000 BC]
613) Millet grown. Millet is a grass grown for its grains and as hay to feed
animals.
  
8,000 YBN
[6000 BC]
616) City "Catal Hüyük" {CaTL HvEK or KeToL HoYqK} in modern Turkey.
Çatal Hüyük, (modern:) Turkey  
8,000 YBN
[6000 BC]
6220) Earliest drum. Giant frame drums are used in the temples of ancient
Sumer. Mesopotamian objects from about 3000 bce depict frame drums and small
cylindrical drums played horizontally and vertically. Early Egyptian artifacts
(c. 4000 bce) show a drum with skins stretched by a network of thongs.

Mesopotamian art works show at least four types of drums: 1) shallow or frame
drums of all sizes, 2) a small cylindrical drum held in a horizontal position,
3) a large drum played with foot, and 4) a small drum with one head, carried
vertically on a belt and struck with both hands.
Moravia, Czeck Republic  
7,300 YBN
[5300 BC]
626)
south Iraq, shore of Persian Gulf  
7,000 YBN
[5000 BC]
618) City of Sumer (in Mesopotamia, modern southern Iraq).
Sumer. (Mesopotamia, modern southern Iraq)  
7,000 YBN
[5000 BC]
619) City of Ur (in Sumer).
  
7,000 YBN
[5000 BC]
620)
  
7,000 YBN
[5000 BC]
627) Oldest evidence of copper melting and casting.

Moorey writes "Casting involves, at its simplest, pouring liquid metal into a
suitably shaped mould of baked clay, stone, metal, or sand. The earliest moulds
to survive in archaeological contexts are one-piece, of clay or stone. They
remained usual for the manufacture of simple tools, flat weapons such as tanged
arrowheads, bar-ingots...and jewellery. Simple jewellery moulds of stone are
more common in excavations than their more complex relatives used for tools and
weapons. ...
Two-piece (bivalve) moulds, probably of baked clay at first, were
introduced some time in the fourth millenium, if not before, with core pieces
for sockets when required, as on axe, adze- and hammer0heads. ...It was
probably common practice to cast the simple tools in open moulds and
subsequently hammer them to the desired shape. ...".
Belovode, Eastern Serbia  
7,000 YBN
[5000 BC]
631)
  
7,000 YBN
[5000 BC]
727) Earliest Reed boats.
Kuwait  
7,000 YBN
[5000 BC]
1296) The city of Uruk is founded in southern Babylonia. Uruk will last until
the 400s CE.
Uruk, southern Babylonia  
6,900 YBN
[4900 BC]
648) Oldest evidence of sail boat.
Mesopotamia  
6,500 YBN
[01/01/4500 BC]
1263)
Vinča, a suburb of Belgrade (Serbia)  
6,500 YBN
[4500 BC]
1293)
Nabta, Egypt  
6,250 YBN
[4250 BC]
720) Earliest evidence of Corn (maize) grown in Mexico.
Oaxaca, Mexico  
6,000 YBN
[4000 BC]
633)
  
6,000 YBN
[4000 BC]
1061)
Ukraine  
6,000 YBN
[4000 BC]
6232) Sun-dried mud brick and mud-brick house.

Mud brick, dried in the sun, is one of the first building materials. Before
sun-dried bricks, perhaps mud deposited by a river could be used to shape into
huts or building units for protection from the weather. In the ancient city of
Ur, in Mesopotamia (modern Iraq), the first true arch of sun-baked brick is
made about 4000 BCE. The arch itself has not survived, but a description of it
includes the first known reference to mortars other than mud. A bitumen mixture
is used to bind the bricks together. Burned brick can be produced simply by
containing a fire with mud bricks.

The early Ubaid period settlement is founded on marshy soil and may have been a
camping place, because no walls exist at this level. A thick layer of reed
matting is the earliest sign of occupation. Above that in later Ubaid levels,
walls are found to have been built, first of pisé (Clay, earth, or gravel
beaten down until it is solid and used as a building material for floors and
walls) and then mud-brick.
Ur, Mesopotamia (modern Iraq)  
5,800 YBN
[3800 BC]
6235)
Harran, Mesopotamia  
5,500 YBN
[3500 BC]
621) Earliest plow (used to break up ground). Pictographs from Mesopotamia show
a beam-ard, a simple machine that scratches a trench without turning the soil.
Mesopotamia  
5,500 YBN
[3500 BC]
622) Irrigation (artificial supply of water to land to maintain or increase
yields of food crops), in the "Middle east" (eastern part of Mediterranean).
Middle east (eastern part of Mediterranean)  
5,500 YBN
[3500 BC]
625) Donkeys raised and used for transport.

Perhaps the donkey also provides food in times of starvation.
  
5,500 YBN
[3500 BC]
634) The Egyptian Calendar. The "years" of ancient Egyptian history consisted
of 12 months of 30 days each and 5 additional ("epagomenal") days at the end.
  
5,500 YBN
[3500 BC]
636)
  
5,500 YBN
[3500 BC]
646) The earliest known wheel, a pottery wheel, in Mesopotamia.

Sir Leonard Woolley who excavates Ur (in modern Iraq) between 1922 and 1934,
writes "...Low down in this 'Uruk' stratum we found a remarkable object, a
heavy disc of baked clay about 3 feet in diameter with a central pivot-hole and
a small hole near the rim to take a handle; it was a pooter's wheel as used by
the makers of the Uruk vases, the earliest known example of that invention
whereby man passed from the age of pure handicraft into the age of
machinery....".

Moorey writes "There are no certain illustrations of potters' wheels from
Mesopotamia and the material evidence is ... meagre... No certain example of a
tournette - a slowly turning wheel- has yet been published from a prehistoric
context, though their use has been assumed from the evidence of the vessels
produced on them. Nissen...has postulated the emergence of a 'pivoted working
surface (tournette)' towards the end of the Halaf period {ULSF: 5500 BC},
largely on the basis of changes in the type and layout of painted patterns on
pottery at this time. By the end of the Ubaid period {ULSF: 4000BC}, he argued,
a more sophisticated device had appeared to be fully exploited for the first
time in the Uruk period: 'setting the wheel's axle in bearings and hence the
creation of an actual potter's wheel. It is possible that plano-convex disks
of gypsum from Tell Abada in the Hamrin, where there is other evidence for
on-site pottery manufacture, may have been pivoted for pot-building on the
upper flat surface...".

Another similar pottery wheel dates back to the Protoliterate Period which is
approximately 3500BC-2900BC. The piece was excavated at the site of Choga Mish
(Iran) and is one of a few pieces to have survived the excavation due to the
destruction of the dig house during the Iranian Revolution.
Mesopotamia (and a similar pottery wheel from Choga Mish, Iran)  
5,500 YBN
[3500 BC]
1260) Writing (on clay tablets). First numbers. First stamp (or seal).

The first writing begins as numbers on clay tablets and stamped seals.

This system of writing on clay tablets will evolve into modern written
language. Writing was first used to solve simple accounting problems; for
example to count large numbers of sheep or bales of hay. Writing may have
arisen out of the need for arithmetic and storage of information, but will grow
to record and perpetuate stories, songs, and most of what we know about human
history.
Sumer (Syria, Sumer, Highland Iran)  
5,500 YBN
[3500 BC]
1285) Symbols on pottery from Harrapa an Indus Valley civilization.
Harrapa, Indus Valley  
5,500 YBN
[3500 BC]
6223) Sundial, earliest timekeeping device. The first device for indicating the
time of day was probably the gnomon, dating from about 3500 bc. The gnomon is a
vertical object and the length of it's shadow indicates the time of day. The
earliest known sundial still preserved is an Egyptian shadow clock of green
schist dating to the 8th century BCE. The hour-glass, which uses a fixed
quantity of fine sand falling through a small hole, is also invented around
this time..
China and Chaldea  
5,490 YBN
[3490 BC]
702) Earliest cotton grown.
Northwestern Peru|Indus valley  
5,400 YBN
[3400 BC]
913)
  
5,310 YBN
[3310 BC]
704) Ox pulled vehicles with wheels in Krakow Poland. This is the earliest
evidence for both animal pulled vehicles and wheeled vehicles. The earliest
instance of a wheeled vehicle is from the TRB (Funnel Beaker) culture in
Bronocice, in north-east Krakow Poland and is a pot incised decoration that has
the repeated motif of a schematically rendered four-wheeled vehicle. Note the
Y-junction with the yoke.

Stuart and Piggot reject the claim that the first wheeled vehicle originated in
Sumer, home of the earliest pottery wheel, writing: "...The calibrated range of
date for phase III at Bronocice, to which the cup with the wagon representation
belongs is c. 3530-3310 BC, but it would be improper to compare this date with
that of 3200-3100 BC assigned to Uruk IVa, in which sledge-on-wheels
pictographs appear. ...".
(TRB - Funnel Beaker culture) Bronocice, Krakow, Poland  
5,300 YBN
[3300 BC]
1261) Symbols of the Alphabet.

Now along with numbers on clay tablets are symbols that represent the
commodity (such as cows, sheep, and cereals). These symbols represent the
earliest record of what will become the modern alphabet.

First training and industry of scribes. This will ultimately evolve into the
modern school system. Writing will be continuously taught eventually in all
major civilizations (even through the Dark Ages) until now.

These tablets are all economic records, used to keep a record of objects owned
or traded, and contain no stories. Writing begins as a method for increasing
the human memory to keep track of the many transactions of a city, and not for
the purpose of recording or remembering stories.

The symbol for ox ("gud" in Sumerian, later "aleph" in Egyptian) will become
the letter "A" (alpha), the symbol for house, (/e/ in Sumerian and /bitum/ in
Akkadian ) will become "B" (beta).

These symbols are drawn with curved lines which will later be replaced by the
easier and faster to draw straight lines and later the wedges of cuneiform. In
Latin "Cuneus" means "wedge".

Around 1200 symbols have been identified in these ancient texts, around 60 are
numerals.

This writing is evidence that most of the 30 or so basic sounds of humans
language were already in use by the origin of writing.

One text from this time is a "titles and professions", which is the most
popular list, copies of these lists span over a thousand years. This list
describes titles and professions probably arranged according to rank, starting
with the symbol for king, and is evidence that the social order is already well
defined in a strict hierarchy by the time writing is invented.

This early writing shows that there is a standardized system of measures in
place. Tablets describe quantities of bread, jars of beer, silver, barley,
fish, cows, lambs, laborer-days, and specific measures of land.

Among tablets found in the third millenium BCE (2000-2999 BCE) are long lists
of names of trees, plants, animals (including insects and birds), countries,
cities and villages, and of stones and minerals. These lists represent a
familiarity with botany, zoology, geography and mineralology. Sumerian scholars
also prepared mathematical tables and detailed mathematical problems with their
solutions.

From tablets dating to 2000 BCE, scribes who identify themselves all appear to
be males indicating that few if any females are formally taught to be scribes.
In addition the parents of the scribes are all high ranking wealthy people.
Sumer  
5,250 YBN
[3250 BC]
637) Scribes in Sumer (seeing that writing is smudged when writing in columns)
change from writing in columns to writing left to right. Pictures are also
turned 90 degrees.
  
5,200 YBN
[3200 BC]
650) Oldest artifact with cuneiform writing, at Uruk which is a large city at
this time. These are clay and stone tablets that have names of humans (thought
to be wage lists), lists of objects, plus receipts and memos. Pictures are not
drawn with pointed reed, but drawn with (diagonally) cut reed-stem pressed in
to the wet clay to make wedges. What were pictures (of oxen, etc.) are changed
to be made of all single presses, not pictures drawn freehand. This writing
contains about 600 unique symbols.
  
5,200 YBN
[3200 BC]
1266) Earliest writing in Egypt.
a group ivory, bone and stone tags attached to jugs,
bags and boxes containing linens and oils in the tomb of King Scorpian I in
Egypt.


Günter Dreyer, director of the German Institute of Archaeology in Cairo, found
writing on a group ivory, bone and stone tags attached to jugs, bags and boxes
containing linens and oils in the tomb of King Scorpian I in Egypt which date
to around 3,400 to 3,200 BCE. The tags are thought to indicate the quantity or
size (on number tags) and the origin location or institution of the
commodities.
(Tomb U-j supposedly of King Scorpian, Royal Cemetery of:) Abydos (modern:) Umm
el-Qa'ab  
5,100 YBN
[3100 BC]
638)
  
5,100 YBN
[3100 BC]
640)
  
5,100 YBN
[3100 BC]
641) The Narmer Palette, early Egyptian hieroglyphic writing.

Narmer palette (tablet) carved with pictures showing unification of Egypt under
king Narmer, who starts the first Egyptian Dynasty of history (Dynasty 1). The
top of the palette has two faces of the cow-headed goddess Hathor. Between the
Hathor heads is name of Narmer, a "n'r" fish and a "mr" chisel (this is the
oldest egyptian writing).
  
5,100 YBN
[3100 BC]
642)
  
5,000 YBN
[3000 BC]
628) Oldest evidence of bronze (copper mixed with tin) melted, and casted.

Figurines of men and women from Tell Judaidah, Turkey, are the oldest examples
of true bronze (combination of copper and tin) known.
Tell Judaidah, Turkey|Egypt  
5,000 YBN
[3000 BC]
645)
  
5,000 YBN
[3000 BC]
647)
  
5,000 YBN
[3000 BC]
649)
  
5,000 YBN
[3000 BC]
651) Akkadian, Babylonian, and Assyrian languages all use cuneiform writing.
  
5,000 YBN
[3000 BC]
653)
  
5,000 YBN
[3000 BC]
664)
  
5,000 YBN
[3000 BC]
665)
  
5,000 YBN
[3000 BC]
666) Hemp grown in China.
  
5,000 YBN
[3000 BC]
668) Silk making in China.
  
5,000 YBN
[3000 BC]
669) Evidence of the wheel in China.
  
5,000 YBN
[3000 BC]
670)
  
5,000 YBN
[3000 BC]
671) Evidence of the arch in Egypt.
  
5,000 YBN
[3000 BC]
672)
  
5,000 YBN
[3000 BC]
673)
Egypt  
5,000 YBN
[3000 BC]
675) Earliest silver objects, in Ur.
Ur  
5,000 YBN
[3000 BC]
676) Melting wax in clay (cire-perdu) metal casting.
  
5,000 YBN
[3000 BC]
1265) Written symbols combined to form words.

In the proto-cuneiform Sumarian script, symbols are combined to form words
based on their sound.

Evidence of this is the sign /ti/, for "arrow" that is now also defined as the
Sumarian word for "life" /til/ which starts with the same sound. After this
phonetic abstraction, the introduction of multi-symbol words, names and words
for which no symbols had existed can be created. For example, the symbol
originally defined as the Summerian verb "bal" (to dig) can also be spelled
with the syllabic signs "ba" + "al", while the Akkadian word for dig ("heru")
sounds differently.(show image if possible)

The vast majority of Sumerian language is made of one-syllable words. This
suggests that all earlier spoken languages contained only single-syllable
words.

Sumerian contains syllabic symbols, where a symbol represents a consonent and a
vowel together such as /Bo/ (ball), or /Bv/ (put), although some vowel sounds
have one symbol and are true letters. This writing will later be fully
alphabetic when the consonents are represented by one symbol and the vowel at
the end dropped.

Sumerian and the languages that follow in the 3000 year history of cuneiform,
all have monophony (one sound has more than one symbol), and polyphony (many
sounds may be represented by one symbol).
Jemdet Nasr  
5,000 YBN
[3000 BC]
1268)
modern southwest Iran  
5,000 YBN
[3000 BC]
6219) Earliest stringed musical instrument (lyre and harp). The lyre is first
depicted in Sumerian art works around 3000 BC. Harps have the plane of the
strings vertical, not parallel, to the soundboard. There are two main types,
the "arched harp" in which the body is curved into an arch, and an "angular
harp", in which the body and neck form an angle. Sumer has only arched harps,
which originate from the bow. Arched harps are depicted on a stone slab from
Khafage that dates to around 3000 BC.
Sumer (modern Iraq)  
5,000 YBN
[3000 BC]
6222) Inclined plane (ramp).

The inclined plane is thought to be older than any of the other basic machines,
and is based on the concept that moving an object from a lower to higher
elevation is easier when pushed up a flatter slope.
Egypt?  
5,000 YBN
[3000 BC]
6226)
Mesopotamia  
4,980 YBN
[2980 BC]
654)
Sakkara, Egypt  
4,925 YBN
[2925 BC]
643) Hieratic script, a cursive script of traditional Egyptian hieroglyphs
replaces traditional hieroglyphs. Hieratic script was almost always written in
ink with a reed pen on papyrus. The word 'hieratikos' means 'priestly' because
by the Greco-Roman period this writing was used only by priest humans.
  
4,800 YBN
[2800 BC]
629)
  
4,800 YBN
[2800 BC]
1276)
Sumer, Uruk, Kish,   
4,750 YBN
[2750 BC]
320) Earliest metal saw.
Mesopotamia  
4,613 YBN
[2613 BC]
652)
  
4,600 YBN
[01/01/2600 BC]
1258)
Sumer  
4,600 YBN
[2600 BC]
1269) Enmebaragesi is the earliest ruler on the Sumerian king list whose name
is attested directly from archaeological remains, two alabaster vase fragments
with inscriptions about him found at Nippur - where he is said to have built
the first temple according to the Sumerian Tummal chronicle.

Enmebaragesi is also mentioned in a section of the Epic of Gilgamesh, which
places Gilgamesh as a historical king of Uruk.
Kish, a city in Sumer, 80km south of modern Bagdad  
4,600 YBN
[2600 BC]
1271) The oldest known written story (or literature), the Sumerian flood story,
the "Ziusudra epic" is known from a single fragmentary tablet, writing in
Sumerian. The name Ziusudra means "found long life" or "life of long days". The
first part tells the story of the creation of man, animals and the first
cities, Eridu, Badtibira, Larak, Sippar, and Shuruppak. After a missing section
in the tablet, the story describes how the gods send a flood to destroy
mankind. The god Enki (lord of the underworld ocean of fresh water and Sumerian
equivalent of Ea) warns Ziusudra of Shuruppak to build a large boat (the
passage describing the directions for the boat is also lost). When the tablet
resumes, it tells about a terrible storm that rages for seven days. Then (the
god) Utu (|vTv| or |oTo| or |uTu|) (the sun) appears and Ziusudra opens a
window, prostrates himself, and sacrifices an ox and a sheep. After another
break the text resumes, the flood is apparently over, and Ziusudra is
prostrating himself before An (|oN|) (the sky-god) and Enlil (the chief of the
gods), who give him "breath eternal" and take him to live in Dilmun. The rest
of the poem is lost.

More than 80% of all known Sumerian literary compositions have been found at
Nippur.

The name Ziusudra also appears in the WB-62 version of the Sumerian king list
as a king/chief of Shuruppak who reigned for 10 (shar) years. Ziusudra was
preceded in this king list by his father SU.KUR.LAM who was also king of
Shuruppak and ruled 8 (shar) years. On the next line of the King List are the
sentences "The flood swept thereover. After the flood swept thereover, ... the
kingship was in Kish." The city of Kish flourished in the Early Dynastic II
period soon after an archaeologically attested river flood in Shuruppak that
has been radio-carbon dated about 2900 BC. Polychrome pottery from below the
flood deposit have be dated to the Jemdet Nasr period that immediately preceded
the Early Dynastic I period.

The importance of Ziusudra in the King List is that it links the flood
mentioned in the Epics of Ziusudra, Atrahasis, Utnapishtim, etc to river flood
sediments in Shuruppak, Uruk, and Kish that have been radio carbon dated as
2900 BCE. So scholars conclude that the flood hero was king of Shuruppak at the
end of the Jemdet Nasr period (3100-2900) which ended with the river flood of
2900 BCE.

Ziusudra being king of Shuruppak is supported in the Gilgamesh XI tablet by the
reference to Utnapishtim as "man of Shuruppak" at line 23.

A Sumerian document known as "The Instructions of Shuruppak" dated to around
2500 BCE, refers in a later version to Ziusudra indicating that Ziusudra may
have become a venerable figure in the literary tradition by 2500 BCE.

Scholars have found many similarities between the stories of Ziusudra,
Atrahasis, Utnapishtim and Noah.

At this time, the scribes learning in the tablet houses must be transferring
their oral stories onto clay, in addition to studying, copying and imitating
earlier texts. Works created in these years are almost all poetic in form, some
extending to thousands of lines. These texts are mainly myths and epic tales in
the form of narrative poems celebrating the adventures of Sumerian gods and
heros, hymns to gods and kings, lamentations of Sumerian cities, wisdom
compositions that include proverbs, fables, and essays. In the scribal schools,
students attend school from sunrise to sunset, and teachers use a rod to
inflict discipline.

The Sumerians belief in a variety of gods and goddesses, so already, by the
time of the invention of writing we see the theory of gods and goddesses. This
inaccurate belief in a god theory will continue into present times. The
Sumerians have around 50 gods and 50 goddesses so far counted. The view
expressed is the traditional view that many of the gods have human form, many
are related, and they control various objects such as the sky (the god Anu,
also god of heaven which indicates belief in a heaven (but this may be
Christian misinterpretation, do dead people go to sky/heaven in Sumerian
myths?)), the earth (the goddess Ki, consort to Anu), the wind (the god
Ishkur), the sun (the god Utu), the earth (the god Enki), grain (the goddess
Ashnan), venus (the goddess Inanna), and many more.

Many of the gods will be renamed as time continues, for example, the Sumerian
goddess "Inanna", the first god known to be associated with the planet Venus,
is named "Ishtar" by the Akkadians and Babylonians, "Isis" by the Egyptians,
"Aphrodite" by the Greeks, "Turan" by the Etruscans, and "Venus" by the Romans.
The Sumerians call Inanna the "Holy Virgin" and this may indicate an early
example of the erroneous belief that a female that has not had sex is somehow
more pure.

It is possible that the Sumerian influence through their invention of writing
is the origin of the idea of human-like gods controlling nature, but more
likely this idea developed long before writing and spread through oral
interaction only. Possibly the idea of human-like gods was originated even
before humans left Africa. The beginning of writing creates the first memory of
the past, where before writing, any events of history have to be passed on
through talking which vastly reduces the number of events remembered by any
generation of people.
Sumer  
4,500 YBN
[2500 BC]
677) Bronze sickle.
  
4,500 YBN
[2500 BC]
688) Seed drills in Babylonia.
  
4,500 YBN
[2500 BC]
689) First animal and vegetable coloring dyes.
  
4,500 YBN
[2500 BC]
691) Oldest evidence of skis used in Skandinavia.
  
4,500 YBN
[2500 BC]
692)
  
4,500 YBN
[2500 BC]
693)
  
4,500 YBN
[2500 BC]
694)
  
4,500 YBN
[2500 BC]
1052)
  
4,500 YBN
[2500 BC]
1151) Oars mounted on the side of ships for steering are documented from the
3rd millennium BCE in Ancient Egypt in artwork, wooden models, and even
remnants of actual boats. These will evolve into quarter rudders, which will be
used until the end of the Middle Ages in Europe.

Egypt  
4,500 YBN
[2500 BC]
6230) Earliest dice and boardgame. There is a claim of earlier dice and
boardgame from Iran (see image of dice - but there is no image of the actual
board).
Ur, Mesopotamia  
4,450 YBN
[2450 BC]
708) Animal skin (leather) used for writing. After the use of leather, the
refined forms of leather parchment and vellum (made from calf skins) are also
used.
Egypt  
4,400 YBN
[2400 BC]
915)
  
4,400 YBN
[2400 BC]
1277)
Sumer, Lagash, Umma   
4,345 YBN
[2345 BC]
695)
  
4,345 YBN
[2345 BC]
800) Writing on Papyrus.

Fibrous layers within the stem of the papyrus plant are removed and placed side
by side. They are then crossed at right angles with another set of strips. The
two layers form a sheet, which is then dampened and pressed. The gluelike sap
of the plant acts as an adhesive to join the layers together. The sheet is
finally hammered and dried in the sun. These sheets are then joined together
with paste to form a roll.
Egypt  
4,300 YBN
[2300 BC]
667) Earliest evidence of glass making, glass beads.

The first human-made glass beads and pendants are made around 4,300 years ago
(2300 BC) in
the area of modern Iraq and northern Syria (Mesopotamia), with the
first strikingly colored (coreformed) vessels appearing there in the 16th/15th
centuries BC.
Mesopotamia  
4,300 YBN
[2300 BC]
701)
  
4,234 YBN
[2234 BC]
632)
  
4,200 YBN
[2200 BC]
1294)
Lima, Peru  
4,181 YBN
[2181 BC]
696)
  
4,160 YBN
[2160 BC]
697)
  
4,134 YBN
[2134 BC]
698)
  
4,134 YBN
[2134 BC]
699)
  
4,130 YBN
[2130 BC]
6234) Earliest evidence of horn used as musical instrument. Several
inscriptions of the Sumerian priest-king Gudea mention an instrument, si-im,
alongside with the temple drums, a-lal and balag. As si (Akkadian qarnu) means
'horn,' and im 'wind,' there is little doubt that this was a blowing horn. One
of the Carchemish reliefs, dating from about 1250 B.C. depicts a rather short
and thick horn played together with a large frame drum which...corresponds
either to the a-lal or to the balag.
From Gudea's time on (c2130 BCE), the si is
occasionally mentioned; some texts add the metal determinative and some refer
to horns made of gold. ...".

The oldest survivng animal horn is from around 2300 BC, from a deep bog in
Visnum, Sweden. It is a cow horn, dated from the late Iron Age, and has five
finger holes. (verify)

A list of the presents offered by King Tushratta to King Amenophis IV of Egypt
around 1400 BC contains a list of forty horns, all covered with gold and some
studded with precious stones. Seventeen of them are called ox horns. The rest
of the horns are probably not straight trumpets since straight trumpets are
more often made of gold instead of covered with gold.

The earliest specimen of a silver trumpet is from the tomb of Tutankhamen
(1300s bce).
Lagash, Mesopotamia  
4,100 YBN
[2100 BC]
1279) The earliest Health science (medical) text, found in Nippur.

There are more than 10 remedies listed on this clay tablet. Materials used are
mostly from plants, such as cassia, myrtle, asafoetida, thyme, and from trees
such as the willow, pear, fir, fig and date trees, but also include sodium
chloride (salt), potassium nitrate (saltpeter), milk, snake skin, and turtle
shell. For mixtures taken internally, beer, milk and or oil are used to make
the "medicine" more palatable.

In this, the oldest medical text, there are no references to any god, demon,
magic spell or incantation.
Nippur  
4,100 YBN
[2100 BC]
6376) The first place value number system, a sexagesimal (base 60) number
system. Fractional values such as 1/60 and 1/3600 are also in use.

This sexagesimal, base 60, number system is still in use to measure time (60
seconds, 60 minutes), and angles (for example in astronomical and geographic
coordinates).
Babylonia  
4,050 YBN
[2050 BC]
1278) The earliest recorded laws, the Ur-Nammu tablet. Ur-Nammu founded the
Third Dynasty of Ur. The laws are written in Sumerian cuneiform and are damaged
so only a few have been deciphered. One law involves a trial by water, another
describes the return of a slave to their master. Other laws describe monetary
penalties for violent crimes such as for cutting off a foot or nose.

This tablet was found in Nippur.
Ur   
4,040 YBN
[2040 BC]
700)
  
4,000 YBN
[2000 BC]
703)
China  
4,000 YBN
[2000 BC]
705) Stonehenge built.
  
4,000 YBN
[2000 BC]
706) Horse riding in Asian steppes.
  
4,000 YBN
[2000 BC]
709)
  
4,000 YBN
[2000 BC]
710) Shaduf (Shadoof), an irrigation tool.
  
4,000 YBN
[2000 BC]
711) Spoked wheel. Toy-cart wheels made of clay with spokes painted on and in
relief were made in the Harappan civilization of the Indus Valley and
Northwestern India. Spokes make the wheel lighter in weight.
  
4,000 YBN
[2000 BC]
733) Oldest lock, found in ruins of the palace of Khorsabad near Nineveh. The
lock is made of wood and uses a tumbler design, similar to modern locks. This
kind of lock will be used widely in Egypt.
Nineveh  
4,000 YBN
[2000 BC]
830) Shaped iron artifacts made from meteorites.
Oldest iron artifacts, made of iron from
meteorites, in Egypt.

Some might argue this is the beginning of the Iron Age, but others would start
the Iron Age only at smelting and casting of Iron.
Egpyt (and near East)  
4,000 YBN
[2000 BC]
1273)
Ur  
4,000 YBN
[2000 BC]
1275) The "School Days" essay dates to now. This is the story of a scribal
student who is late for school and is caned for various offenses such as
talking and because his copying is not good enough. So the student invites a
teacher to his house for dinner. The teacher is brought from school, seated in
the seat of honor and served dinner. The father of the student dresses the
teacher in a new garment, gives him a gift, and puts a ring on his hand. After
this the teacher praises the student.

Sumer  
4,000 YBN
[2000 BC]
1283)
Nippur  
4,000 YBN
[2000 BC]
1286) The earliest known versions of the Gilgamesh (or Gish-gi(n)-mash) story
are written in Sumerian on clay tablets.
Nippur  
4,000 YBN
[2000 BC]
5860) Earliest written musical composition.
Nippur, Babylonia (now Iraq) (verify)  
4,000 YBN
[2000 BC]
6236) Metal traded as money.

The use of metal for money can be traced back to Babylonia more than 2000 years
bc, but standardization in the form of coins does not occur systematically
until the 7th century bc. Historians generally ascribe the first use of coined
money to Croesus, king of Lydia, a state in Anatolia. The earliest coins are
made of electrum, a natural mixture of gold and silver, and are bean-shaped
ingots bearing a primitive punch mark certifying to either weight or fineness
or both.
Babylonia  
3,842 YBN
[1842 BC]
712) First all phonetic language and alphabet. Proto-semitic alphabet made in
turquoise mines probably by Semitic humans. This alphabet is thought to have
replaced cuneiform, and may be root of all other alphabets.

This first strictly phonetic alphabet is in use until 1797 BCE.

Encyclopedia Britannica states that the evolution of the alphabet involves two
important achievements. The first step is the invention of an all-consonant
writing system. The second is the invention of characters for representing
vowels which is made by Greek people between 800 and 700 bce.

Around this time the Egyptians have a large-scale project to search for
turquoise in the high mountains of southern Sinai at a site today called
Serabit el-Khadem. In this mine an alphabetic script, is found with has far
fewer signs than the Egyptian hieroglyphic system. In 1916, Sir Alan Gardiner,
an English Egyptologist, notices that a group of four signs are frequently
repeated in these inscriptions. Gardiner correctly identified the repetitive
group as a series of four letters in an alphabetic script that represent a word
in a Canaanite language: b-‘-l-t, vocalized as Baalat, "the Mistress".
Gardiner suggests that Baalat was the Canaanite name for Hathor, the goddess of
the turquoise mines.
An important key to the decipherment is a unique bilingual
inscription. It is inscribed on a small sphinx from the temple and features a
short inscription in what appears to be parallel texts in Egyptian and in the
new script.
The Egyptian hieroglyphic inscription on the sphinx reads:
"The beloved of
Hathor, the mistress of turquoise."
Each of the critical letters in the word Baalat is a
picture—a house, an eye, an ox goad and a cross.
Gardiner correctly recognizes
that each pictograph has a single phonic value: The picture stands not for the
depicted word but only for its initial sound. So the pictograph bêt, "house",
represents only the initial consonant b.
This principle is at the root of all of
our alphabetic systems. Each sign in this script stands for one consonant in
the language. (The representation of vowels happens later).
The alphabet is invented
in this way by Canaanites at Serabit in the Middle Bronze Age, in the middle of
the 19th century B.C.E., probably during the reign of Amenemhet III of the
XIIth Dynasty.
(Caanan modern:) Palestine|(turquoise mines ) Serabit el-Khadem, Sinai
Peninsula  
3,800 YBN
[1800 BC]
713)
  
3,800 YBN
[1800 BC]
802)
  
3,800 YBN
[1800 BC]
803)
  
3,786 YBN
[1786 BC]
714)
  
3,700 YBN
[1700 BC]
715)
  
3,700 YBN
[1700 BC]
1280)
Nippur  
3,700 YBN
[1700 BC]
1281)
Nippur and Ur, Sumer  
3,650 YBN
[1650 BC]
716)
  
3,635 YBN
[01/01/1635 BC]
1272) A library of 3,000 clay tablets in a priest's house in Tell ed-Der dates
to this time.

Tell ed-Der  
3,600 YBN
[1600 BC]
804)
  
3,595 YBN
[01/01/1595 BC]
1274)
Babylon  
3,595 YBN
[1595 BC]
6335)
Babylon  
3,551 YBN
[1551 BC]
717)
  
3,550 YBN
[1550 BC]
1282)
Sumer  
3,531 YBN
[1531 BC]
639) First planet recognized, Venus.

Evidence of this comes from the so-called "Venus Tablet of Ammi-saduqa", which
is known only from copies from the 600 BCE only. The Venus Tablet records
astronomical observations placing Venus on the horizon just before sunrise on
the date of the new moon for the 21 year reign of Ammi-saduqa.
Babylon  
3,500 YBN
[1500 BC]
624) Oven-baked mud brick (also called "burned brick").
A burned brick is a mud brick
that been baked in an oven (kiln) at an elevated temperature to harden it, give
it mechanical strength, and improve its resistance to moisture.
Ur, Mesopotamia (modern Iraq)  
3,500 YBN
[1500 BC]
721)
  
3,500 YBN
[1500 BC]
722)
  
3,500 YBN
[1500 BC]
723) Earliest pulley.

The oldest simple pulleys are used in Assyria.
A pulley is a wheel that has a grooved
rim for carrying a rope or other line and turning in a frame. The pulley wheel
is also called a "sheave".

One or more independently rotating pulleys can be used to gain mechanical
advantage, especially for lifting weights. The shafts around which the pulleys
turn may attach them to frames or blocks, and a combination of pulleys, blocks,
and rope is called a block and tackle. The pulley is considered one of the five
simple machines.
Nimroud, Assyria  
3,500 YBN
[1500 BC]
725)
  
3,500 YBN
[1500 BC]
1516)
India  
3,500 YBN
[1500 BC]
6228) Water clock (Clepsydra {KlePSiDru}).

The science of telling the time of day (horology) began around 3500 BC with the
invention of the gnomon and sundial, and the hour-glass. Around 1500 BC, the
Egyptian clepsydra (water clock) used dripping water between two containers
which were marked to indicate the time.

In China, in the 100s CE, astronomer Zhang Heng built a celestial globe whose
movement is regulated by clepsydra. In the 700s Yi Xing and Liang Lingzan
added a mechanical clock.
Egypt  
3,500 YBN
[1500 BC]
6229)
Nippur, Mesopotamia  
3,358 YBN
[1358 BC]
2727) When Akhenaton dies, he will be succeeded briefly by Smenkhkare and then
by a second son-in-law, Tutankhaton. Tutankhaton is forced to change his name
to Tutankhamen, dropping the Aton and embracing Amon, to abandon Amarna and
move back to Thebes, and to pay penance by giving the old gods new riches and
privileges. A few years after the death of the young king, Tutankhamen, the
army takes over the throne led by General Horemheb. Horemheb institutes
counterreforms in order to restore the old system fully.

As was done at the command of Akhenaten years before, the new kings attempt to
erase all traces of the heretical religion. Akhenaten's name and images of the
Aten sun disk are ordered removed from monuments and official king lists.
Akhenaten's temples are dismantled and the stone reused. Amarna is left to
crumble in the desert. Inscriptions refer to Akhenaten only as the heretic
pharaoh of Akhetaten.
There is an interesting similarity between "Aton" and "Satan" being
3 of 4 sounds/letters the same. It may be coincidence, but perhaps Aton was
given a negative connotation to try to erase the history of the origin of
Judaism, or remove suspicions of the monotheistic theorists as copying
Amenhotep. If the name "Aton" is used, people will recognize the ancient deity
Aton, however, by adding a letter, only a subtle reference or connotation to
the ancient God, Aton remains. It is interesting also the way Amon is viewed
against Aton as if rival gods with Amenhotep switching to place his belief in
Aton.

There is a claim that followers of Akhenaton's new monotheistic religion ended
each prayer with the name of Amenhotep and that this is the origin of the use
of the word "amen" at the end of Judean, Christian and Islamic prayers.

What about the possible relation of the word "Aton" to the Greek word "atom"?
Amarna, Egypt  
3,310 YBN
[1310 BC]
728)
  
3,300 YBN
[1300 BC]
729)
  
3,300 YBN
[1300 BC]
914)
  
3,200 YBN
[1200 BC]
730)
  
3,200 YBN
[1200 BC]
731)
  
3,200 YBN
[1200 BC]
734)
  
3,200 YBN
[1200 BC]
735)
  
3,200 YBN
[1200 BC]
736)
  
3,200 YBN
[1200 BC]
737)
  
3,198 YBN
[1198 BC]
738)
  
3,180 YBN
[1180 BC]
805)
  
3,087 YBN
[1087 BC]
739)
  
3,000 YBN
[1000 BC]
741)
  
3,000 YBN
[1000 BC]
742)
  
3,000 YBN
[1000 BC]
743)
  
3,000 YBN
[1000 BC]
744)
  
3,000 YBN
[1000 BC]
745)
  
3,000 YBN
[1000 BC]
746) Complex pulleys. The lifting power of a pulley is multiplied by the number
of strands acting directly upon the moving pulleys.
  
3,000 YBN
[1000 BC]
747)
  
3,000 YBN
[1000 BC]
749)
  
3,000 YBN
[1000 BC]
806)
  
3,000 YBN
[1000 BC]
1048)
  
3,000 YBN
[1000 BC]
6237) Earliest lens, a plano-convex lens (one side plane the other convex) made
from rock-crystal found in Nimrud, a magnifying and burning glass.

Sir David Brewster described the lens writing: "This lens is plano-convex, and
of a slightly oval form, its length being 1 6/10 inch, and its breadth l 4/10
inch. It is about 9/10ths of an inch thick, and a little thicker at one side
than the other. Its plane surface is pretty even, though ill polished and
scratched. Its convex surface has not been ground, or polished, on a spherical
concave disc, but has been fashioned on a lapidary's wheel, or by some method
equally rude. The convex side is tolerably well polished, and though uneven
from the mode in which it has been ground, it gives a tolerably distinct focus,
at the distance of 4 1/2 inches from the plane side. There are about twelve
cavities in the lens, that have been opened during the process of grinding it:
these cavities, doubtless contained either naphtha, or the same fluid which is
discovered in (opazi quartz, and other minerals. As the lens does not show the
polarised rays at great obliquities, its plane surface must be greatly inclined
to the axis of the hexagonal prism of quartz from which it must have been
taken. It is obvious, from the shape and rude cutting of the lens, that it
could not have been intended as an ornament; we are entitled, therefore, to
consider it as intended to be used as a lens, either for magnifying, or for
concentrating the rays of the sun, which it does, however, very imperfectly.".

Another, possibly 5th century BC, lens was found in a sacred cave on Mount Ida
on Crete and is more powerful and of far better quality than the Nimrud lens.
Aristophanes (c450-c388 bce), Greek playwright, in his play "Clouds", around
423 BCE, describes a crystal lens used for burning. Also, Roman writers Pliny
and Seneca refer to a lens used by an engraver in Pompeii.
Nimrud, Mesopotamia (modern Iraq)  
2,999 YBN
[999 BC]
1181) Calamine Brass is first made in this millenium {narrow time}, brass made
with copper and clamine, a zinc ore (instead of zinc metal, because extracting
zinc metal from ore will not be understood until around 1781).

  
2,945 YBN
[945 BC]
748)
  
2,922 YBN
[922 BC]
753)
  
2,910 YBN
[910 BC]
635) The oldest smelted iron artifacts are from Tell Hammeh (az-Zarqa), Jordan
and date to around 2800-2700 years ago, but two charcoal samples from the same
site date to 2930-2910 years before now.

This is the start of the Iron Age, as iron becomes more popular because iron is
more abundant.
in Mesopotamia, Anatolia, and Egypt.

It is possible, under certain conditions, to produce iron when smelting copper,
and so it may be that iron produced before the late Bronze Age may have been
produced in the process of smelting copper, or possibly lead. If iron oxide in
any one of its three forms (haematite; limonite; magnetite) is accidentally or
deliberately added to the furnace charge as a fluxing agent (a mineral added to
the metals in a furnace to promote fusing or to prevent the formation of
oxides), in smelting copper or lead, the iron will combine with the silica in
the ore to form slag that will melt and eventually run off. In circumstances of
high temperature and extreme reducing atmosphere, small bits of relatively pure
iron could have been produced.
Tell Hammeh (az-Zarqa), Jordan  
2,900 YBN
[900 BC]
750)
  
2,850 YBN
[850 BC]
751)
Greece  
2,848 YBN
[848 BC]
752)
  
2,819 YBN
[819 BC]
754)
  
2,800 YBN
[800 BC]
718)
  
2,800 YBN
[800 BC]
818) Theta sound {t} sound invented, (for example in the words "theater",
"fifth") and in use in Greece.

Theta (Θ) is the eighth letter of the Greek alphabet, derived from the
Phoenician letter Teth.

The theta sound survives only in Greek and later languages.
  
2,800 YBN
[800 BC]
1036)
  
2,800 YBN
[800 BC]
5862)
Mesopotamia  
2,785 YBN
[785 BC]
771) Babylonian astronomers can predict eclipses.

The reason there are not two eclipses a month is because the orbit of the Moon
around the Earth is tilted 5 degrees from the Earth's plane of rotation around
the Sun. This means that the moon must be at or near the two points in its
orbit that intersects the Earth's plane of rotation around the Sun when the
Moon is between the Earth and Sun or behind them. This alignment occurs at
least twice a year, and at most rarely 5 times a year.
Usually, if an eclipse of the
Sun occurs, an eclipse of the Moon precedes of follows it by 2 weeks, because
the Sun, Earth and Moon are then in alignment with each other.
  
2,731 YBN
[731 BC]
6299) Lunar eclipses recorded.
Babylon  
2,728 YBN
[728 BC]
755)
  
2,722 YBN
[722 BC]
756)
  
2,716 YBN
[716 BC]
757)
  
2,715 YBN
[715 BC]
758)
  
2,700 YBN
[700 BC]
1062)
Assyria  
2,700 YBN
[700 BC]
1075) Consonant letters can represent more than one sound. Letter "C" sounded
as "K" in addition to traditional "G" sound.

Latin or Etruscan speaking people start using the letter "C" (Gamma), not only
to represent it's traditional sound "G", but also for the sound "K", usually
reserved for the letter "K" (Kappa). This will add confusion to how to
pronounce a word, and violates a more simple, logical system where one letter
equals only one sound.

At this time Latin speaking people start replacing words with K with the letter
"C".
Italy  
2,688 YBN
[688 BC]
916)
  
2,669 YBN
[669 BC]
1287) The "standard" version of the story of Gilgamesh: a wild-man Enkidu is
tamed by having sex with a woman, Enkidu and Gilgamesh destroy Humbaba, the
beast-like guardian of the forest, and a bull sent from Heaven, Enkidu is
killed as a punishment by the Gods, and Gilgamesh visits him in the Underworld.
Nippur  
2,668 YBN
[668 BC]
917)
  
2,668 YBN
[668 BC]
1284) Clay tablet library of Ashurbanipal in Nineveh, an early systematically
organized library from which 20,720 Assyrian tablets and fragments have been
preserved.
Nineveh (Assyria)  
2,664 YBN
[664 BC]
759)
  
2,660 YBN
[660 BC]
644) In Egypt, the Demotic script replaces hieratic in most secular writing,
but hieratic continued to be used by priests for several more centuries.

The Demotic symbol set, is a short hand, very rapid, abbreviated form of
hieratic, and looks like series of "agitated commas". The word "demotic" is
from Greek meaning "of the people" or "popular".
  
2,651 YBN
[651 BC]
6337) All planets visible to the naked eye clearly distinguished from stars
(Mercury, Venus, Mars, Jupiter, and Saturn) in Babylonia. The position of these
five planets compared to the stars is found in a series of baked clay tablet
astronomical "diaries". The earliest datable tablet, from 651 BCE contains the
names of all five planets.
Babylonia  
2,650 YBN
[650 BC]
1066) Evidence of the earliest aquaduct, a channel used to move water from one
place to another, is in Assyria. This aquaduct is built of and carries water
across a valley to the capital city, Nineveh.
Nineveh  
2,640 YBN
[640 BC]
760)
  
2,624 YBN
[624 BC]
761)
  
2,622 YBN
[622 BC]
763)
  
2,622 YBN
[622 BC]
826) Old Testament (The Torah, Hebrew Bible, The Ten Commandments, The Story of
Genesis).

The earliest record of the reading of a “Torah book” is provided by the
narrative describing the reformation instituted by King Josiah of Judah in 622
BCE following the fortuitous discovery of a “book of the Torah” during the
renovation of the Temple.
Judah|(Israel)  
2,621 YBN
[621 BC]
1519)
Athens, Greece  
2,609 YBN
[609 BC]
767)
  
2,609 YBN
[609 BC]
768)
  
2,605 YBN
[605 BC]
918)
  
2,600 YBN
[600 BC]
630) Metal coin money.

Historians generally ascribe the first use of coined money to Croesus, king of
Lydia, a state in Anatolia. The earliest coins are made of electrum, a natural
mixture of gold and silver, and are crude, bean-shaped ingots bearing a
primitive punch mark certifying to either weight or fineness or both.
Lydia, Anatolia  
2,600 YBN
[600 BC]
762) Thales (in Greek: Θαλης) is the first human of record to explain the
universe with out using any gods in the explanation, claiming the universe
originated as water.

Thales explains that moon light is reflected sun light.

Thales measures a pyramid by comparing the pyramid shadow with the shadow from
a stick.
Miletus, Greece  
2,600 YBN
[600 BC]
765)
  
2,600 YBN
[600 BC]
2619) This concept of a Devil will grow to be included in the Christian
religion, and coupled with the concept of a Hell will work as a powerful myth
against science and free inquiry into the scientific nature of the universe.
  
2,590 YBN
[590 BC]
1518) At this time people in Greece have not yet begun to write history or
biography. It will not be until the 400s BCE that accounts of the life of Solon
and his works began to be put together.

Before Solon's reforms, the Athenian state is administered by nine archons
appointed or elected annually by the Areopagus on the basis of noble birth and
wealth. The Areopagus is made of former archons and therefore has, in addition
to the power of appointment, a large amount of influence. The nine archons take
the oath of office while ceremonially standing on a stone in the agora,
declaring their readiness to dedicate a golden statue if they should ever be
found to have violated the laws. There is an assembly of Athenian citizens (the
Ekklesia) but the lowest class (the Thetes) are not admitted and its
deliberative procedures are controlled by the nobles. There is no method to
control or punish an archon who violates a law unless the Areopagus decides to
prosecute the archon.

According to Aristotle, Solon creates a law to allow all citizens to be
admitted into the Ekklesia and for a court (the Heliaia) to be formed from all
the citizens. The Heliaia appears to have been the Ekklesia, or some
representative portion of it, sitting as a jury. Ancient sources credit Solon
with the creation of a Council of Four Hundred, drawn from the four Athenian
income groups to serve as a steering committee for the enlarged Ekklesia.

Solon broadens the financial and social qualifications required for election to
public office. The Solonian constitution divides citizens into four political
classes defined according to assessable property, a classification that might
previously have served the state for military or taxation purposes only. The
standard unit for this assessment is one medimnos (approximately 12 gallons) of
corn.
Athens, Greece  
2,587 YBN
[587 BC]
769)
  
2,585 YBN
[05/08/585 BC]
770)
  
2,580 YBN
[580 BC]
764) Anaximander (Greek: Αναξίμανδρος) (Anaximandros) oNoKSEMoNDrOS
or ANAKSEmANDrOS? (BCE 610-546), friend and student of Thales, describes an
Earth-centered Universe theory, and a theory that humans evolved from fish, the
first recorded theory of evolution in history..

Anaximander had a more abstract idea of the universe than Thales. Anaximander
introduced the science of the ancient east to Greece, made use of the sundial
(known for centuries in Egypt and Babylonia), was the first to draw a map of
the entire known earth. Anaximander recognized that the stars appeared to orbit
the pole star, and so viewed the sky as a complete sphere (not just a
semisphere over the earth). This is the first evidence for the idea of spheres
in astronomy. This would grow to contribute to the complicated and erroneus
system of Ptolomy which will dominate science until Copernicus and Kepler.
Anaximander thinks that the earth is curved to explain the change in position
of the stars, thinking the earth to be a cylinder. The first papyrus by
Anaximander is lost.
Miletus  
2,580 YBN
[580 BC]
1522) The bulk of her poetry, which is well-known and greatly admired
throughout antiquity, has been lost, but her immense reputation has endured.
Because she
writes love poems addressed to both women and men, Sappho has long been
considered bisexual. The word "lesbian" derives from the name of the island of
her birth, Lesbos.
Her homoerotica should be placed in a 600s BCE Greece context. The
poems of Alcaeus and later Pindar record similar romantic bonds between the
members of a given circle
Ancient sources state that Sappho produced nine volumes of
poetry, but only a small proportion of her work survives. Papyrus fragments,
such as those found in the ancient rubbish heaps of Oxyrhynchus, are an
important source. One substantial fragment is preserved on a potsherd. The rest
of what we know of Sappho comes through citations in other ancient writers,
often made to illustrate grammar, vocabulary, or meter. There is a single
complete poem, Fragment 1, Hymn to Aphrodite.

The themes of Sappho's known writing are primarily concerned with her thiasos,
the usual term (not actually found in any of Sappho's surviving writings) for
the female community, with a religious and educational background, that meets
under her leadership. In her poems, Sappho attacks other thiasoi directed by
other women.

The goal of the thiasos is the education of young women, especially for
marriage. Aphrodite is the group's tutelary divinity and inspiration. Sappho is
the intimate and servant of the goddess and her intermediary with the girls. In
the ode to Aphrodite, the poet invokes the goddess to appear, as she has in the
past, and to be her ally in persuading a girl she desires to love her. Frequent
images in Sappho's poetry include flowers, bright garlands, naturalistic
outdoor scenes, altars smoking with incense, perfumed unguents to sprinkle on
the body and bathe the hair-that is, all the elements of Aphrodite's rituals.
In the thiasos the girls are educated and initiated into grace and elegance for
seduction and love. Singing, dancing, and poetry play a central role in this
educational process and other cultural occasions. As is true for other female
contemporary communities, including the Spartan, and for the corresponding
masculine institutions, the practice of homoeroticism (allusions to same gender
physical love and sexuality) within the thiasos plays a role in the context of
initiation and education. In Sappho's poetry love is passion, an inescapable
power that moves at the will of the goddess; it is desire and sensual emotion;
it is nostalgia and memory of affections that are now distant, but shared by
the community of the thiasos. There is a personal poetic dimension, which is
also collective because all the girls of the group recognize themselves in it.
An important part of Sappho's poetry is occupied by epithalamia, or nuptial
songs.

It is not known how her poems were published and circulated in her own lifetime
and for the following three or four centuries. In the era of Alexandrian
scholarship (3rd and 2nd centuries BC), what survives of her work will be
collected and published in a standard edition of nine books of lyrical verse,
divided according to metre. This edition will not endure beyond the early
Middle Ages. By the 8th or 9th century CE Sappho wil be represented only by
quotations in other authors. Only the ode to Aphrodite, 28 lines long, is
complete. The next longest fragment is 16 lines long. Since 1898 these
fragments have been greatly increased by papyrus finds, though, in the opinion
of some scholars, nothing equal in quality to the two longer poems.
Lesbos  
2,575 YBN
[575 BC]
773)
  
2,550 YBN
[550 BC]
1035)
  
2,545 YBN
[545 BC]
919)
  
2,545 YBN
[545 BC]
920) Herodotus' invention will earn him the title "The Father of History" and
the word he uses for his achievement, "historie", which previously had meant
simply "inquiry", will pass into Latin and take its modern connotation of
"history" or "story". This nickname will be given to him by Cicero (De legibus
I,5)
Herodotos writes that doctors are very specialized in Egypt. There are
doctors for eyes, head, teeth, stomach, and for "invisible diseases", which may
be disturbances of the "nervous system". or perhaps simply any disease without
a clear cause (incl bacteria, virus).
  
2,540 YBN
[540 BC]
783)
Miletus  
2,540 YBN
[540 BC]
784) Xenophanes (~570 BC - ~480 BC), a Greek philosopher, poet, social and
religious critic , learns from Pythagoras, but leaves Ionia for Southern Italy,
(to a town named "Elea"). Xenophanes is less mystical than Pythagoras and
writes about the school of Pythagoras. Xenophanes did not believe in
transmigrartion of souls, or in the primitive Greek Gods, but instead in a
monotheism rare to Greek people. Xenophanes finds seashells on mountain tops
and reasons that the earth changes over time, so that mountains must have been
in the sea and then rose, therefore Xenophanes is the first human in history to
make a contribution to the science of Geology. Not until Hutton were any other
contributions to Geology made.

Our knowledge of his views comes from his surviving poetry, all of which are
fragments passed down as quotations by later Greek writers. His poetry
criticized and satirized a wide range of ideas, including the belief in the
pantheon of human-like gods and the Greek people's continued support of
athleticism.

Xenophanes rejected the idea that the gods resembled humans in form. One famous
passage ridiculed the idea by claiming that, if oxen were able to imagine gods,
then those gods would be in the image of oxen. Because of his development of
the concept of a "one god greatest among gods and men" that is abstract,
universal, unchanging, immobile and always present, Xenophanes is often seen as
one of the first monotheists.

This shows that there was a large amount of tolerence of religious criticism,
without any serious punishment.
Elea, Southern Italy  
2,538 YBN
[538 BC]
788)
  
2,530 YBN
[530 BC]
797) Eupalinus, Eupalinus of Megara (20 mi west of athens), a Greek architect,
constructed for the tyrant Polycrates of Samos a tunnel to bring water to the
city, passing the tunnel through a hill for half a mile, starting at both ends,
meeting at the center and unaligned by only a few inches.
Samos, Greece  
2,529 YBN
[529 BC]
772) Pythagoras describes the earth as a sphere. "Pythagorean Theorem" (in a
right triangle: the square of the lengths of the hypotenuse always equals the
sum of the square of the length of the two other sides).

Pythagoras is credited with being the first person to recognize that the
morning star (Phosphorus) and evening star (Hesperus) are the same star, after
this time, the star is called "Aphrodite" (this "star" is later recognized to
be planet Venus). Pythagoras is the first to write that the orbit of the earth
moon is not in the plane of the Earth equator but at an angle to that plane.
Pythagoras is the first to teach that the Sun, Moon, and planets do not follow
the motion of the stars, but have paths of their own. This changes the star
system theory from the theory of Anaximander of a single heavenly crystalline
sphere, to adding separate spheres for the planets. This theory of the star
system will last until Kepler.

Pythagoras moves from Samos to Croton in Southern Italy, to escape the harsh
rule of Polycrates, and starts a school in Croton.

Pythagoras experiments with a monochord, an instrument that has a single string
is stretched over a sound box. The string is fixed at both ends and a moveable
bridge alters the pitch. Pythagoras finds that strings of musical instruments
make higher pitch sounds when made shorter, finding pitch related to length.
Pythagoras finds, for example, twice the length equals 1 octave lower, a 3 to 2
ratio equals a fifth, a 4 to 3 ratio equals a fourth. Pythagoras finds that
also increasing tension raises pitch.

A Pythagorean named Hippasus is credited with the proof that the square root of
2 can not be expressed as a ratio of two numbers (is irrational). Pythagorian
humans decide to keep secret "irrational numbers".

Pythagoras mistakenly thinks that vibrations from the crystaline spheres
rubbing together create a harmonious "Music of the Spheres", which will last
for a long time.
Croton, Italy  
2,525 YBN
[525 BC]
820)
  
2,520 YBN
[520 BC]
785) This skepticism of religion appears to be widespread and higly tolerated
in this time of history in Ionia.
Hecataeus was one of the first classical
writers to mention the Celtic people.
Some have credited Hecataeus with a work entitled
Ges Periodos ("Travels round the Earth" or "World Survey'), in two books each
organized in the manner of a periplus, a point-to-point coastal survey. One on
Europe, is essentially a periplus of the Mediterranean, describing each region
in turn, reaching as far north as Scythia. The other book, on Asia, is arranged
similarly to the Periplus of the Erythraean Sea of which a version of the 1st
century CE survives. Hecataeus described the countries and inhabitants of the
known world, the account of Egypt being particularly comprehensive; the
descriptive matter was accompanied by a map, based upon Anaximander"s map of
the earth, which he corrected and enlarged. The work only survives in some 374
fragments, by far the majority being quoted in the geographical lexicon Ethnika
compiled by Stephanus of Byzantium.

The other known work of Hecataeus was the Genealogiai, a rationally
systematized account of the traditions and mythology of the Greeks, a break
with the epic myth-making tradition, which survives in a few fragments, just
enough to show what we are missing.

Hecataeus' work, especially the Genealogiai, shows a marked scepticism, opening
with "Hecataeus of Miletus thus speaks: I write what I deem true; for the
stories of the Greeks are manifold and seem to me ridiculous."1 Unlike his
contemporary Xenophanes, he did not criticize the myths on their own terms; his
disbelief rather stems from his broad exposure to the many contradictory
mythologies he encountered in his travels.

An anecdote from Herodotus (II, 143), of a visit to an Egyptian temple at
Thebes, is illustrative. It recounts how the priests showed Herodotus a series
of statues in the temple's inner sanctum, each one supposedly set up by the
high priest of each generation. Hecataeus, says Herodotus, had seen the same
spectacle, after mentioning that he traced his descent, through sixteen
generations, from a god. The Egyptians compared his genealogy to their own, as
recorded by the statues; since the generations of their high priests had
numbered three hundred and forty-five, all entirely mortal, they refused to
believe Hecataeus's claim of descent from a mythological figure. This encounter
with the immemorial antiquity of Egypt has been identified as a crucial
influence on Hecataeus's scepticism: the mythologized past of the Hellenes
shrank into insignificant fancy next to the history of a civilization that was
already ancient before Mycenae was built.
Miletus, Greece  
2,515 YBN
[03/12/515 BC]
821)
  
2,515 YBN
[515 BC]
1264)
Persia (Kermanshah Province of Iran)  
2,510 YBN
[510 BC]
786) Heraclitus (~540 BC Ephesus 30 mi north of Miletus, ~540 bc - ~475 bc)
disagrees with Thales, Anaximander, and Pythagorus about the nature of the
ultimate substance, thinking fire to be a fundamental element of the universe.
Heraclitus claims that the nature of everything is change itself. A typically
pessimistic view led to Herkleitos being called the "weeping philosopher". Only
fragments of text by Heraclitus have been found.
Miletus, Greece  
2,510 YBN
[510 BC]
787) Parmenides (~540 BC Elea (now Velia), Italy - ??) a student of Ameinias,
and pre-Socratic philosopher, follows in the tradition of the Ionian exiled
Pythagorus and Xenophanes. Parmenides opposed the view of Heraclitus, claiming
that one object can not turn in to other object fundamentally different.
Parmenides argued that creation (something from nothing) and destruction
(nothing from something) is impossible. Parmenides chose reason over senses,
feeling senses to be untrustworthy. Parmenides founds school in Elea, the
"Eliatic School" based on this philosophy of reason over senses. Zeno was the
most recognized person educated in the school. Zeno, will use distrust of
senses to describe a set of paradoxes.
  
2,508 YBN
[508 BC]
1517)
Athens, Greece  
2,500 YBN
[500 BC]
824)
  
2,500 YBN
[500 BC]
825)
  
2,500 YBN
[500 BC]
831)
  
2,499 YBN
[499 BC]
832)
  
2,490 YBN
[490 BC]
789) Hanno (BCE c530-???), Cathaginian (a branch of the Phoenicians) Navigator,
sails 60 ships with 3000 people, down the coast of Africa in order to start new
settlements. Much of what is learned about Hanno is from an 18 sentence
travel-record, or "Periplus" of this journey, from Herodotus, and Pliny the
Elder. Herodotus will express doubts about the accuracy of Hanno's story,
because of a report that in the far south the sun at noon was in the nothern
half of the sky, which Herodotus will think is impossible, but is in fact true
for the southern hemisphere of earth. This is strong evidence, taken together
with the Periplus of Hanno's journey that Hanno is the first Mediterranean
human to sail over the equator into the Southern Hemisphere. Herodotus also
declares that Hanno claimed to have circumnavigated Africa.
Carthage (modern: Tunis)  
2,490 YBN
[490 BC]
819)
  
2,470 YBN
[470 BC]
836) Anaxagoras views the Sun to be a mass of red-hot metal, that people live
on the Moon, and thinks that the Universe is made of tiny bodies. The
contemporary prevailing belief is that the Sun and the Moon are gods. Diogenes
Laerteus confirms that this is the belief of the Egyptian people writing
(translated from Greek): "...They (the Egyptians) say that the first principle
is matter then that the four elements were formed out of matter and divided and
that some animals were created and that the sun and moon are gods of whom the
former is called Osiris and the latter Isis and they are symbolised under the
names of beetles and dragons and hawks and other animals...".

Anaxagoras (BCE c500-c428) introduces the Ionian science of Thales to Athens,
saying that the universe is not made by a deity, but through the action of
infinite "seeds", which will later develop into atomic theory under Leucippos.
Anaxagoras accurately explains the phases of the earth moon, and both eclipses
of moon and sun in terms of their movements.

Anaxagoras teaches in Athens for 30 years, and the school formed by Anaxagoras
starts the scholarly tradition that lasts for 1000 years.
Athens  
2,470 YBN
[470 BC]
840)
  
2,470 YBN
[470 BC]
907)
  
2,468 YBN
[468 BC]
837)
  
2,467 YBN
[467 BC]
1894) Particle (or wireless) communication. The optical telegraph (or
semaphore)

An optical telegraph is an apparatus for conveying information by using visual
signals, for example, using towers with turnable blades or paddles, shutters,
or hand-held flags etc.

The Greek playwright, Aeschylus, describes in the play "Agamemnon" how news of
the fall of Troy reaches the city of Argos (600 km away) in only a few hours by
the use of fire signals.

Robert Hooke (CE 1635-1703) gives a clear description of an optical telegraph
(or semaphore) using telescopes to the Royal Society in 1684.

Claude Chappe in France will develop one of the first practical optical
telegraphs in 1794.
Greece (presumably)  
2,460 YBN
[460 BC]
835)
  
2,460 YBN
[460 BC]
841) Theory that all matter is made of atoms.

Leukippos (Greek Λευκιππος ) (lEUKEPOS?) (BCE c490-???) is the first
person to support an atomic theory. Leukippos theorizes that the universe is
made of two different elements, which he calls "solid" and "empty", and that
matter is composed entirely of an infinity of small indivisible particles
called atoms, which are constantly in motion, and through their collisions and
regroupings form various compounds.

The most famous among Leucippus' lost works are titled "Megas Diakosmos" ("The
Great Order of the Universe" or "The great world-system") and "Peri Nou" ("On
mind").

The argument for indivisible atoms is said to have been a response to Zeno's
argument about the absurdities that follow if magnitudes are divisible to
infinity.

Leukippos represents the final part of science and logic in Asia Minor before
the destruction of the coastal cities by humans from Persia. Leukippos teaches
Democritos.
Leukippos is the first person to say that every event has a natural cause.
  
2,460 YBN
[460 BC]
842)
  
2,460 YBN
[460 BC]
1037)
  
2,458 YBN
[458 BC]
834)
  
2,454 YBN
[454 BC]
844)
  
2,451 YBN
[451 BC]
906) Protagoras (Greek: Πρωταγόρας) (c. 481-c. 420 BC) publishes an
agnostic text. Diogenes describes it this way (translated from Greek):
"...another of his treatises he begins in this way: "Concerning the Gods, I am
not able to know to a certainty whether they exist or whether they do not. For
there are many things which prevent one from knowing, especially the obscurity
of the subject, and the shortness of the life of man.". And on account of this
beginning of his treatise he was banished by the Athenians. And they burnt his
books in the market-place, calling them in by the public crier, and compelling
all who possessed them to surrender them.".
  
2,450 YBN
[450 BC]
843)
Croton, Italy  
2,450 YBN
[450 BC]
1033)
  
2,450 YBN
[450 BC]
1053)
  
2,450 YBN
[450 BC]
1112)
Yangzhou, Jiangsu, China  
2,438 YBN
[438 BC]
823)
  
2,434 YBN
[434 BC]
839)
  
2,432 YBN
[432 BC]
849) Metonic calendar: 12 years of 12 months, 7 years of 13 months.

Greek astronomer Meton (c440BC Athens - ???) finds that 235 lunar months make
around 19 years, so 12 years of 12 months and 7 years of 13 months will allow
the lunar calendar to match the seasons. The Greek calendar will be based on
the Metonic cycle until 46 BCE when the Julian calendar will be made by Julius
Caesar with the help of Sosigenes. This calendar is also in use in Babylonia
around the same time if not earlier.
Greek astronomer Meton (~440BC Athens - ???) finds
that 235 lunar months (moon rotations of earth) are close to 19 earth years, so
if there are 12 years of 12 lunar months, and 7 years of 13 lunar months, every
19 years, the lunar calendar would match the seasons. This will come to be
called the "Metonic cycle" (although probably recognized by astonomers in
Babylonia before this time). The Greek calendar will be based on the Metonic
cycle until 46 BCE when the Julian calendar will be made by Julius Caesar with
the help of Sosigenes.

This cycle can be used to predict eclipses, forms the basis of the Greek and
Jewish calendars, and is used to determine the date for Easter each year.
Athens, Greece (presumably)  
2,431 YBN
[431 BC]
1372)
Sri Lanka  
2,430 YBN
[430 BC]
838)
Athens, Greece  
2,430 YBN
[430 BC]
845)
Abdera, Thrace  
2,430 YBN
[430 BC]
847) There is much uncertainty, but Hippocrates was born of a family in a
hereditary guild of magicians on the Isle of Cos, described to be descended
from Asklepios, the Greek god of medicine. Hippocrates visits Egypt early in
life, there studies medical works credited to Imhotep. Some people claim that
he was a student of Democritus. Hippocrates teaches in Athens (and other
places), before opening his own school of health in Cos.

Humans that graduate with a "medical" degree must still repeat the oath
credited to Hippocrates (although repeating oaths is stupid, and few if any
actually people actually follow this advice of do no harm, in particular in
psychiatric hospitals).
Cos  
2,430 YBN
[430 BC]
910)
  
2,424 YBN
[424 BC]
1138) Although in the comedy "Clouds", Aristophanes paints Ionian science in a
bad light through a portrayal of Socrates encouraging young people to beat
their parents. But perhaps even then, people paid for such a message to be read
during a play (now newspapers, magazines, television and movies accept money
for such messages), and money for propaganda, a very old (albeit secretive)
system, may have influence Aristophanes even then.
Athens, Greece  
2,409 YBN
[409 BC]
852)
  
2,408 YBN
[408 BC]
5877)
Athens, Greece (or perhaps Macedon)  
2,404 YBN
[404 BC]
855)
  
2,399 YBN
[399 BC]
846)
Athens, Greece  
2,390 YBN
[390 BC]
909)
  
2,387 YBN
[387 BC]
851) Plato's Academy.

Plato (Greek: Πλάτων, Plátōn, "wide, broad-shouldered") (c427BC Athens
- 347 BC Athens) founds a school in western Athens on a piece of land once
owned by a legendary Greek human named "Academus", and so this school comes to
be called "The Academy", and this word will eventually generally apply to any
school. The Academy will be a center for science and education for 900 years
until 529 CE.

Plato is an Athethian aristocrat (of the ruling class or nobility) whose
original name is "Aristocles", but he gets the nick name "Platon" (meaning
"broad") because of his broad shoulders. (Cicero also was a nick name). Plato
is in the "war service" (tph military?) and is interested in politics, but
rejects Athenian democracy.

In this year, Plato returned to Athens. (on the way to Athens, Plato is
supposed to have been captured by pirates and held for ransom).

The Academy has shrine to the muses (mouseion) and is viewed as a religious
organisation by the government.

Plato stayed at the Academy for the rest of his life, except for 2 years in the
360s, when he visited Syracuse, the main city of Greek Sicily, to tutor the new
king Dionysius II. Dionysius II appeared brutal, and Plato returned safely to
Athens. Plato is supposed to have died in his sleep at the age of 80 after
attending a wedding feast of a student. Writing credited to Plato are
consistently popular and are of a series of dialogues between Socrates and
others. Most of what is known about Socrates is from these texts. Like
Socrates, Plato was mainly interested in moral philosophy and hated natural
philosophy (science). To Plato, knowledge had no practical purpose. Plato liked
mathematics, perhaps because the perfection of math, the loftiest form of pure
thought, was different from the reality of the universe (viewed as "gross" and
imperfect). Above the main doorway to the academy were the words in Greek: "Let
no one ignorent of mathematics enter here." Plato did think that math could be
applied to the universe. The planets, he thought, exhibited perfect geometric
form. This is in Timaeus. He describes the 5 and only 5 perfect solids, those
objects with equal faces, lines and angles. (4 sided tetrahedron, six sided
hexahedron (or cube), 8 sided octahedron, 12 sided dodecahedron, and 20 sided
icosahedron. 4 of the 5 represented the 4 elements, while the dodecahdron
represented the whole universe. These solids were first discovered by the
Pythagoreans. Plato thought the planets were spheres and moved in circles
along the crystalline spheres that held them in place. The idea that the
universe must reflect the perfection of abstract mathematics was most popular
until Kepler, even though compromises with reality had to be made constantly,
beginning after the death of Plato with Eudoxus and Callippus. In Timaeus,
Plato invented a moralistic story of a completely fictional land called
"Atlantis". This legend has had unending popularity and has persisted to now.
One Aegean island exploded vocanically in 1400 BC and this may have given rise
to this story. The views of Plato had a strong influence on Christian people
until the 1200s when Aristotle gained more popularity.
Carl Sagan states that:

"Plato and his followers separated the earth from the "heavens" (the rest of
the universe), Plato taught contempt for the real world and disdain for the
practical application of science. Plato served tyrants, and taught the
separation of the body from the mind, a natural enough idea in a slave
society."
and that "{Plato} preferred the perfection of these mathematical
abstractions to the imperfections of everyday life. He believed that ideas were
far more real than the natural world. He advised the astronomers not to waste
their time observing the stars and planets. It was better, he believed, to just
think about them. Plato expressed hostility to observation and experiment. He
taught contempt for the real world and disdain for the practical application of
scientific knowledge. Plato's followers succeeded in extinguishing the light of
science and experiment that had been kindled by Democritus and the other
Ionians. Plato's unease with the world as revealed by the senses was to
dominate and stifle Western philosophy. Even as late as 1600, Johannes Kepler
was still struggling to interpret the structure of the Cosmos in terms of
Pythagorean solids and Platonic perfections." I am not sure that we should
fully blame Pythagoras and Plato for the collapse of science, as much as we
should the tradition of religion that came long before them. But clearly the
support of these incorrect views by a majority of later intellectuals shows
large scale bad judgement. The popularity of Plato is a mystery since Plato
did not make one contribution to science. Sagan says that this popularity is
because the views of Plato justify a corrupt social order, where I think that
this popularity was simply a mistaken belief. In addition the Academy served
as a center for science and education until 529 CE.

In "The Republic", one of the earliest and most influential books on political
theory, Plato presents a plan for the ideal society and government. Plato
disliked Athenian democracy. It was the leaders of the Athenian democracy that
had sentenced his teacher to die for seeking truth and wisdom. Plato preferred
Sparta's model of government. In Sparta, the needs of the state (country) were
put above the individual. Serving the government was more important than
achieving personal goals. Plato believed that too much personal freedom led to
disorder and chaos. Athens was a primary example of this disorder.

" Plato wanted only the most intelligent and best-educated citizens to
participate in government. He divided people into three classes: workers to
produce life's necessities, soldiers to defend the people, and specially
trained leaders to govern the state (country). The specially trained leaders
would be an elite class that included both men and women. The wisest of all
would be a philosopher-king with ultimate authority. The philosopher-king would
be well educated to make decisions for the good of all the people."

"Rather than being remembered for a specific model of the Universe it was his
views on its nature, put forward in his dialogue Timaeus, that were to so
strongly influence subsequent generations. To Plato the Universe was perfect
and unchanging. Stars were eternal and divine, embedded in an outer sphere. All
heavenly motions were circular or spherical as the sphere was the perfect
shape. Such was his influence that the concept of circular paths was not
challenged until Kepler, after many years of painstaking calculations,
discovered the elliptical orbits of planets nearly 2,000 years later."
Athens, Greece  
2,384 YBN
[384 BC]
860)
  
2,378 YBN
[378 BC]
854)
  
2,378 YBN
[378 BC]
861)
  
2,372 YBN
[372 BC]
1038) Diogenes "the Cynic", is a Greek philosopher, born in Sinope (in modern
day Sinop, Turkey) about 412 BCE (according to other sources 399 BCE), and died
in 323 BCE at Corinth.

Diogenes lives with no possessions in a tub belonging to the temple of Cybele.

At the Isthmian Games he lectured to large audiences, who turned to him from
his one-time teacher Antisthenes.

When Plato gave Socrates's definition of man as "featherless bipeds" and was
much praised for the definition, Diogenes plucked a cock and brought it into
Plato's school, and said, "This is Plato's man." After this incident, "with
broad flat nails" was added to Plato's definition.

The ideas of Diogenes of Sinope, as well as most of the other Cynics, arrive
indirectly. No writings of Diogenes survive even though he is reported to have
authored a number of books.

Happiness, for Diogenes, was to be found in radical autonomy. For Diogenes and
the other Cynics the best way to achieve this autonomy was to minimize one's
dependence upon things and people. The ascetic lifestyle that Diogenes
pursued--which involved sleeping out of doors in cold weather and eating
whatever he could obtain--was an expression of this ideal, which also prepared
the Cynic for anything that might happen. Nevertheless, it seems that Diogenes
was not against pleasure (as his masturbation implies): when reproved for
walking out of a brothel (where apparently he had been enjoying, apparently for
free, the services offered) he replied that he should be reproved for walking
in rather than walking out.

Diogenes maintained that all the artificial growths of society were
incompatible with happiness and that morality implies a return to the
simplicity of nature. So great was his austerity and simplicity that the Stoics
would later claim him to be a sage or "sophos", a perfect man. In his words,
"Man has complicated every simple gift of the gods."
  
2,370 YBN
[370 BC]
883)
  
2,366 YBN
[366 BC]
858)
  
2,357 YBN
[357 BC]
856)
  
2,347 YBN
[347 BC]
853)
  
2,342 YBN
[342 BC]
857)
  
2,341 YBN
[341 BC]
867)
  
2,340 YBN
[340 BC]
801)
  
2,336 YBN
[336 BC]
868)
  
2,335 YBN
[335 BC]
859) During the thirteen years (335 BCE-322 BCE) which Aristotle spends as
teacher of the Lyceum, he composes most of his writings. Imitating Plato,
Aristotle writes "Dialogues" in which his doctrines were expounded in somewhat
popular language. He also composes the several treatises on sciences, logic,
metaphysics, and ethics, in which the language is more technical than in the
Dialogues. These writings succeeded in bringing together the works of his
predecessors in Greek philosophy, and how he pursued, either personally or
through others, his investigations in the realm of natural phenomena. Pliny
will claim that Alexander placed under Aristotle's orders all the hunters,
fishermen, and fowlers of the royal kingdom and all the overseers of the royal
forests, lakes, ponds and cattle-ranges, and Aristotle's works on zoology make
this statement believable. Aristotle was fully informed about the doctrines of
his predecessors, and Strabo will assert that he was the first to accumulate a
great library.

During the last years of Aristotle's life the relations between him and
Alexander became very strained, owing to the disgrace and punishment of
Callisthenes, whom Aristotle had recommended to Alexander. Nevertheless,
Aristotle continued to be regarded at Athens as a friend of Alexander and a
representative of Macedonia. Consequently, when Alexander's death became known
in Athens, and the outbreak occurred which led to the Lamian war, Aristotle
shared in the general unpopularity of the Macedonians. The charge of impiety,
which had been brought against Anaxagoras and Socrates, was now brought against
Aristotle. He left the city, saying, "I will not allow the Athenians to sin
twice against philosophy" (Vita Marciana 41). He took up residence at his
country house at Chalcis, in Euboea, and there he died the following year, 322
BC. His death was due to a disease, reportedly 'of the stomach', from which he
had long suffered.

Aristotle's legacy also had a profound influence on Islamic thought and
philosophy during the middle ages. Muslim thinkers such as Avicenna, Farabi,
and Yaqub ibn Ishaq al-Kindi were a few of the major proponents of the
Aristotelian school of thought during the Golden Age of Islam.

Though we know that Aristotle wrote many elegant treatises (Cicero described
his literary style as "a river of gold"), the originals have been lost in time.
All that we have now are the literary notes of his pupils, which are often
difficult to read (the Nicomachean Ethics is a good example). It is now
believed that we have about one fifth of his original works.

Aristotle underestimated the importance of his written work for humanity. He
thus never published his books, only his dialogues. The story of the original
manuscripts of his treatises is described by Strabo in his Geography and
Plutarch in his "Parallel Lives, Sulla": The manuscripts were left from
Aristotle to Theophrastus, from Theophrastus to Neleus of Scepsis, from Neleus
to his heirs. Their descendants sold them to Apellicon of Teos. When Sulla
occupied Athens in 86 BC, he carried off the library of Appellicon to Rome,
where they were first published in 60 BC from the grammarian Tyrranion of
Amisus and then by philosopher Andronicus of Rhodes.

Aristotle did not like the idea of atoms that Democritos had thought about. If
matter was made up of tiny particles there must be spaces between them, spaces
that would have nothing in them - a vacuum. Aristotle's refusal to accept the
possibility that a vacuum could exist came from his ideas about forces. He said
that non-living objects could have "natural" or "forced" motion. The natural
motion of earth and water was downwards because they had "gravity" while air
and fire always rose because they had "levity". An object was given forced
motion when it was thrown into the air and Aristotle concluded that the speed
of an object depended on the force acting on it - no force, no speed.

Arostotle writes "History of Animals".

Though we know that Aristotle wrote many elegant treatises (Cicero described
his literary style as "a river of gold"), the originals have been lost in time.
All that we have now are the literary notes of his pupils, which are often
difficult to read (the Nicomachean Ethics is a good example). It is now
believed that we have about one fifth of his original works.

Aristotle underestimates the importance of his written work for humanity. He
thus never publishes his books, only his dialogues. The story of the original
manuscripts of his treatises is described by Strabo in his "Geography" and
Plutarch in his "Parallel Lives, Sulla": The manuscripts were left from
Aristotle to Theophrastos, from Theophrastos to Neleus of Scepsis, from Neleus
to his heirs. One of Neleus' descendents (it is unknown who), digs up the
buried scrolls and sells them for a large sum in gold to a bibliophile,
Apellicon of Teos. Apellicon of Teos makes a 'botched up' edition titled the
'Lost Texts of Aristotle'. When Sulla occupies Athens in 86 BCE, he will carry
off the library of Appellicon to Rome. The grammarian Tyrannion of Amisus in
Rome, friend of Atticus and Cicero, obtains the scrolls on loan, gives up on
making his own compiled edition and entrusts the project to Andronicus of
Rhodes, who subdivides the treatises into books. The originals are returned to
Sulla's library. This edition of the texts of Aristotle will be published in 60
BCE.

Faustus is the son of the Emperor Sulla, and Pompey's son-in-law. The cultural
elite go to Faustus' house to consult these precious texts of Aristotle. Cicero
writes a letter to Atticus about the delight of Faustus' library. To pay off
debts, Faustus sells the scrolls of Aristotle, and they have never been located
since. Much of this story comes from Strabo who was presumably a pupil of
Tyrannion of Amisus.
Athens, Greece  
2,332 YBN
[332 BC]
880)
  
2,332 YBN
[332 BC]
921) It is possible that the Museum (Mouseion) of Alexandria is built starting
now, and much of the city was constructed by the time Ptolemy arrives to rule 9
years later in 323 BCE.
  
2,327 YBN
[327 BC]
875)
  
2,325 YBN
[325 BC]
865)
  
2,325 YBN
[325 BC]
887) Pytheas PitEoS (Πυθέας) (BCE 380-310) sails to Great Britain and
"Thule" (probably Norway or Iceland). Pytheas is the first person to explain
tides as happening because of the influence of the moon. Only 2000 years later
will Newton explain the attraction of the Moon. Pytheas is also the first
person to show that the North star is not exactly at the pole and makes a small
circle in a day. The written history of Britain begins with Pytheas.
Massalia (now: Marseille France)  
2,323 YBN
[06/10/323 BC]
876)
  
2,323 YBN
[323 BC]
862) After Aristotle moves to Chalcis, Aristotle choses Theofrastos
(Theophrastus) (Greek: Θεόφραστος) (tEOFrASTOS?) (BCE c372-287) to
preside over the Peripatetic school, which he does for thirty-five years. The
Lyceum maintains it's highest quality under Theophrastos. Theophrastos
describes over 500 species of plants and is the founder of botony, the study of
plants. Theophrastus is charged with asebeia (atheism) but acquitted by a jury
in Athens.
Athens  
2,323 YBN
[323 BC]
863) The charge of impiety, which had been brought against Anaxagoras and
Socrates, was now brought against Aristotle. He leaves Athens saying, "I will
not allow the Athenians to sin twice against philosophy" (Vita Marciana 41). He
takes up residence at his country house at Chalcis, where his mother had lived,
in Euboea, and there he dies the following year, 322 BC. His death was due to a
disease, reportedly 'of the stomach', from which he had long suffered.

After the death of Alexander, the anti-Macedonian party accuses Aristotle of
impiety. With the example of Socrates behind him, Aristotle escapes to Chalcis
in Euboea, where he dies in the same year.
Athens  
2,323 YBN
[323 BC]
864)
  
2,323 YBN
[323 BC]
877)
  
2,322 YBN
[03/07/322 BC]
879)
  
2,320 YBN
[320 BC]
866)
  
2,317 YBN
[317 BC]
899)
  
2,316 YBN
[316 BC]
908)
  
2,311 YBN
[311 BC]
885) "Is God willing to prevent evil but not able? Then He is not omnipotent.
Is He able but not willing? Then He is malevolent. Is He both able and willing?
Then whence cometh evil? Is He neither able nor willing? Then why call Him
God?"
Admiting of females and slaves shocks and interests the scholarly people
of the time.

After the official approval of Christianity by Constantine, Epicureanism was
repressed. Epicurus' theory that the gods were unconcerned with human affairs
had always clashed strongly with the Judeo-Christian God, and the philosophies
were essentially irreconcilable. For example, the word for a heretic in the
Talmudic literature is "Apikouros". Lactantius criticizes Epicurus at several
points throughout his Divine Institutes. The school endured a long period of
obscurity and decline. However, there was a resurgance of atomism among
scientists in the 18th and 19th Centuries, and in the late 20th Century, the
school was revived.
  
2,310 YBN
[310 BC]
869) Kidinnu (BCE 340-???), head of the Astronomical school in Sippar
(Babylonia), understands the precession of equinoxes (a wobbling in the
orientation of Earth's axis with a cycle of almost 26,000 years).

Hipparchus will make use of the precession of the equinoxes as documented by
Kidinnu. Kidinnu makes a complicated method of expressing movement of the moon
and planets, differing from the view that these objects must move at a constant
velocity.
(Astronomical School) Sippar, Babylonia  
2,310 YBN
[310 BC]
871)
  
2,310 YBN
[310 BC]
911)
  
2,307 YBN
[307 BC]
901)
  
2,305 YBN
[305 BC]
884) Pre-Christian Greek humans did not object to human dissection, thinking a
"soul" most important, and a dead body just a group of flesh. In Egypt, human
dissection is a serious impiety. He is particularly interested in the brain.
Sev
eral of our sources speak of Herophilus and Erasistratus undertaking not merely
dissections, but also vivisections (dissections on living bodies), on human
subjects. The Christian writer Tertullian (ca. 155-230) describes Herophilus as
‘that butcher who cut up innumerable corpses in order to investigate nature
and who hated mankind for the sake of knowledge" ("On the Soul", chap. 10).
However, Tertullian was totally opposed to the scientific investigations of
pagan researchers and did everything he could to defame them and their work.
Pli
ny and Rufus both refer in general terms to the practice of human dissection
without specifying who first undertook this. Another first century CE source,
the Roman medical writer Celsus, both identifies the men concerned and reports
the arguments that were used to justify this practice and that of vivisection.
In the introduction (23 ff.) of his work "On Medicine" Celsus writes as follows
concerning the group of doctors known as the Dogmatists:
"Moreover since pains
and various kinds of diseases arise in the internal parts, they hold that no
one who is ignorant about those parts themselves can apply remedies to them.
Therefore it is necessary to cut open the bodies of dead men and to examine
their viscera and intestines. Herophilus and Erasistratus proceeded in by far
the best way, they cut open living men-criminals they obtained out of prison
from the kings-and they observed, while their subjects still breathed, parts
that nature had previously hidden, their position, colour, shape, size,
arrangement, hardness, softness, smoothness, points of contact, and finally the
processes and recesses of each and whether any part is inserted into another or
receives the part of another into itself."
The Dogmatists wrote of the
advantages of vivisection over dissection and defended this viewpoint against
the charge of inhumanity by claiming that the good outweighed the evil: ‘nor
is it cruel, as most people state, to seek remedies for multitudes of innocent
men of all future ages by means of the sacrifice of only a small number of
criminals."
Unlike Tertullian, Celsus cannot be accused of malicious distortion. He himself
disagrees with the Dogmatists. 'To cut open the bodies of living men,' he says
later in his introduction (74 f), "is both cruel and superfluous: to cut open
the bodies of the dead is necessary for medical students. For they ought to
know the position and arrangement of parts-which the dead body exhibits better
than a wounded living subject. As for the rest, which can only be learnt from
the living, experience itself will demonstrate it rather more slowly, but much
more mildly, in the course of treating the wounded." The tone of his whole
account is restrained and we have no good grounds for rejecting it. No one can
doubt that religious and moral considerations inhibited the opening of the
human body, whether dead or alive, in antiquity. But that is not to say that
such inhibitions could never, under any circumstances, be overcome. The
situation at Alexandria in the third century BCE was clearly an exceptional one
in the particular combination of ambitious scientists and patrons of science
that existed there at that time. For all the ancients' respect for the dead,
corpses were desecrated often enough by people other than scientists. Moreover,
when we reflect that the ancients regularly tortured slaves in public in the
law courts in order to extract evidence from them, and that Galen, for example,
records cases where new poisons were tried out on convicts to test their
effects, it is not too difficult to believe that the Ptolemies permitted
vivisection to be practised on condemned criminals.

Before Herofilos, doctors were called Asclepiadae, in the sense that they were
spiritual descendants of the Greek God of healing, Asclepius. Much of this new
health research is done in Alexandria and rival capital Antioch. Herofilos and
his students are interested in direct knowledge and precise terminology. Galen
(129-200 CE),will praise Herofilos in relation to the ovarian arteries and
veins observed by Herofilos in the womb, writing "I have not seen this myself
in other animals except occasionally in monkeys. But I do not disbelieve that
Herofilos observed them in women; for he was efficient in other aspects of his
art and his knowledge of facts acquired through anatomy was exceedingly
precise, and most of his observations were made not, as is the case with most
of us, on brute beasts but on human beings themselves." Some of Herofilos'
pupils form their own schools. One such student is Callimachus. According to
Polybius around 150 BCE, the medical profession is dominated by two schools,
the Herophileans and the Callimacheans. Another pupil of Herofilos, Philinus of
Cos, will form a rival school, refered to as the Empiricists, who differed from
Herofilos in disregarding anatomy and physiology, focusing mainly on
therapeutics, claiming that a disease must be treated experimentally. They
based their school on experiment and past history of success.
  
2,305 YBN
[305 BC]
934)
  
2,300 YBN
[300 BC]
927) While in Egypt Hekataeos of Abdura writes that priests teach children two
kinds of writing, sacred (hieratic) and the more common (demotic), in addition
to geometry and arithmetic. Hecataeus writes "they (Egyptians) have preserved
to this day the record concerning each of the stars over an incredible number
of years...they have also observed with great interest the motions, ... orbits
and stoppings of the planets".
Egypt  
2,300 YBN
[300 BC]
1166) This tomb is constructed to look like a temple (it looks similar to
Dendera). The outside is decorated in typical Late Period style, while the
outer court is decorated in a Greek-style.
Egypt  
2,297 YBN
[297 BC]
900)
  
2,297 YBN
[297 BC]
902) Museum of Alexandria.

Ptolemy I Soter (Πτολεμαίου Σωτήρα) starts construction of the
Soma, in Alexandria, a mausoleum where Alexander and subsequent kings will be
stored after death, the famous Lighthouse of Pharos, the research center known
as the Mouseion (a temple to the Muses, a "Mousaeion" (Μουσείον also
Μουσείου, Museum: in actuality a University and Library ) and the Royal
Library (which may have been a separate building near the Mousaeion or may have
been inside the Mousaeion), in the Royal Palaces area. The Mousaeion will house
the smartest scientists of this time. This research center will also include a
zoo. Some of these monuments will take more time to build than 2 decades and
will be completed under the reign of Ptolemy II.
  
2,297 YBN
[297 BC]
925)
  
2,295 YBN
[295 BC]
878) Euclid may have run a school of mathematics in Alexandria. Pappus of
Alexandria (fl. c320 CE) will write that the Greek mathematician Apollonius
learned geometry from the students of Euclid in Alexandria.

Eukleidis is a Greek mathematician, who lived in Alexandria, Egypt during the
reign of Ptolemy I (323 BC283 BC), and is often considered to be the "father of
geometry". His most popular work, Elements, is the most successful textbook in
the history of mathematics. Within it, the properties of geometrical objects
are deduced from a small set of axioms, thereby founding the axiomatic method
of mathematics.

Although best-known for its geometric results, the Elements also includes
various results in number theory, such as the connection between perfect
numbers and Mersenne primes.

Euclid also wrote works on perspective, conic sections, spherical geometry, and
possibly quadric surfaces. Neither the year nor place of his birth have been
established, nor the circumstances of his death.

Although many of the results in Elements originated with earlier
mathematicians, one of Euclid's accomplishments was to present them in a
single, logically coherent framework. In addition to providing some missing
proofs, Euclid's text also includes sections on number theory and
three-dimensional geometry. In particular, Euclid's proof of the infinitude of
prime numbers is in Book IX, Proposition 20.

The geometrical system described in Elements was long known simply as the only
"geometry". Today, however, it is often referred to as Euclidean geometry to
distinguish it from other so-called non-Euclidean geometries which will be
found in the 1800s CE. These new geometries will grow out of more than 2000
years of investigation into Euclid's fifth postulate, one of the most-studied
axioms in all of mathematics, known as the "parallel postulate", the postulate
that no two angles in a triangle can be equal or greater than 2 90 degree
angles. This postulate will be shown to only be true for flat surfaces and
not for the surface of a sphere or hyperboloid.

One story about Euclid is from Stobaeus and relates that one of Euclid's
students, when he had learned the first proposition, asked his teacher, "But
what is the good of this and what shall I get by learning these things?", to
which Euclid calls a slave and says, "Give this fellow a penny, since he must
make gain from what he learns. "
  
2,295 YBN
[295 BC]
926)
  
2,290 YBN
[290 BC]
903)
(Book probably funded by and stored in the Museum of Alexandria) Alexandria,
Egypt  
2,288 YBN
[03/07/288 BC]
881)
  
2,288 YBN
[288 BC]
873)
  
2,288 YBN
[288 BC]
905)
  
2,287 YBN
[287 BC]
872)
(Lyceum) Athens, Greece  
2,287 YBN
[287 BC]
924)
  
2,285 YBN
[285 BC]
1028) Ktesibios (Ctesibius) (TeSiBEOS) (Greek Κτησίβιος), (fl. 285 -
222 BCE) starts the engineering tradition in Alexandria. Ktesibius invents
several devices using compressed air: a water organ, in which air is forced
through the organ pipes by the weight of water, and an air-powered catapult.
Alexandria, Egpyt  
2,283 YBN
[283 BC]
928)
  
2,283 YBN
[283 BC]
929)
  
2,281 YBN
[281 BC]
904)
  
2,281 YBN
[281 BC]
935)
  
2,280 YBN
[06/10/280 BC]
922)
  
2,280 YBN
[280 BC]
1199)
Athens, Greece  
2,275 YBN
[275 BC]
888)
Heliopolis, Egypt  
2,275 YBN
[275 BC]
897)
  
2,275 YBN
[275 BC]
930)
  
2,274 YBN
[274 BC]
886) Erasistratus, is born on the island of Chios in ancient Greece, to a
family with a history of doctors. His father and brother are doctors, and his
mother is the sister of a doctor. He studies health science in Athens and then,
around 280 B.C., enrolls in the University of Cos, a center of the medical
school of Praxagoras. Erisistratos then moves to Asia and is court physician
for Seleucus I, who controls a major portion of what had been the Persian
Empire. Erasistratus then moves to Alexandria, where he teaches and is a
practicing doctor, continuing the work of Herophilus. In his later years, he
retires from being a practice doctor and joins the Alexandrian museum, where he
devotes himself to research. Although Erasistratus writes extensively in a
number of health-related fields, none of his works survive. He is best known
for his observations based on his numerous dissections of human cadavers (and
rumored, his vivisections of criminals, a practice allowed by the Ptolemy
rulers). Erasistratus accurately describes the structure of the brain,
including the cavities and membranes, and makes a distinction between its
cerebrum and cerebellum (larger and smaller parts). He views the brain, not the
heart, as the seat of intelligence. By comparing the brains of humans and other
animals, Erasistratus correctly concludes that a greater number of brain
convolutions results in greater intelligence. He also accurately describes the
structure and function of the gastric (stomach) muscles, and observes the
difference between motor and sensory nerves. Erasistratus promotes hygiene,
diet, and exercise in health care.

In Alexandria, the view at the time is that the nerves carry "nervous spirit",
arteries "animal spirit", and the veins blood, however Erasistratos takes a
step backwards from Herofilos in mistakenly thinking that arteries do not carry
blood. He thinks air is carried from lungs to heart and changed in to the
"animal spirit" that is carried in the arteries.

He is best known for curing Antiochos, Seleucus's son. Erasistratus said that
Antiochos was in love with his stepmother, and that that was what was ailing
him, so he let them marry.
Alexandria, Egpyt  
2,270 YBN
[270 BC]
932)
  
2,265 YBN
[265 BC]
931) Pliny the Elder will record in the 1st century CE that Hermippus (Greek:
Ἕρμιππος) of Smyrna, a student of Callimachus writes a commentary on
the versus of Zoroaster now. This implies that these stories have been
translated from Iranian to Greek.
  
2,260 YBN
[260 BC]
663) Lever.

The earliest remaining writings regarding levers date from the 3rd century BC
and were provided by Archimedes. "Give me a place to stand, and I shall move
the earth with a lever" is a remark of Archimedes who formally stated the
correct mathematical principle of levers (quoted by Pappus of Alexandria).

It is assumed that in ancient Egypt, constructors used the lever to move and
uplift obelisks weighting more than 100 tons.
Mesopotamia  
2,260 YBN
[260 BC]
822) Screw.

Archimedes (Greek: Αρχιμήδης ) (287-212 BCE) is usually credited with
with the concept of the spiral screw. A spiral screw is an inclined plane
wrapped around a cylinder. The spiral is called a "thread", and the distance
between adjacent edges is called the "pitch" of the screw. The pitch is equal
to the distance that the screw advances in one turn in a solid medium.

Although Archimedes is credited with inventing the screw in the 3rd century BC,
his screw is not the fastener kind of screw, but actually is two other
screw-type devices. One is a kind of water pump, still used today for
large-volume, low-lift, industrial applications, the device is now called the
inclined screw conveyor or "Archimedes screw". The second is the "endless
screw", which is the same as the worm of a worm and gear set, one of the five
ancient devices for raising heavy weights.
Syracuse, Sicily  
2,260 YBN
[260 BC]
882) Aristarchos understands that the Earth rotates around the Sun each year
and that the earth rotates around its own axis once a day.

In 450 BC, Philolaus had theorized that the earth moves through space.

Aristarchus’s only extant work is "On the Sizes and Distances of the Sun and
Moon". Aristarchus finds that as observed during a lunar eclipse, the diameter
of Earth’s shadow is twice the diameter of the Moon. Aristarchos uses the
observation that, at the time when the Moon appears half-lit (quarter Moon),
the angular distance between the Moon and the Sun is 87 degrees, to determine
that the Sun is between 18 and 20 times farther away from Earth than the Moon
is. (The actual ratio is about 390.).

The Greek philosopher Cleanthes, the Stoic, declares in his "Against
Aristarchus" that Aristarchus should be indicted for impiety "for putting into
motion the hearth of the universe".

Aristarchus’s work on the motion of Earth has not survived, but his ideas are
known from references by the Greek mathematician Archimedes, the Greek
biographer Plutarch, and the Greek philosopher Sextus Empiricus.

In his manuscript of "Six Books Concerning the Revolutions of the Heavenly
Orbs" (1543), Copernicus will cite Aristarchus as an ancient authority who
supported the motion of Earth, but later crosses out the reference.
(Mousion of Alexandria) Alexandria, Egpyt  
2,260 YBN
[260 BC]
941)
  
2,257 YBN
[257 BC]
891) Archimedes calculates the oldest known example of a geometric series with
the ratio 1/4 (see image).
He proves that the ratio of a circle's perimeter to its
diameter is the same as the ratio of the circle's area to the square of the
radius. He does not call this ratio π but gives a procedure to approximate it
to arbitrary accuracy and gave an approximation of it as between 3 + 10/71
(approximately 3.1408) and 3 + 1/7 (approximately 3.1429). He proves that the
area enclosed by a parabola and a straight line is 4/3 the area of a triangle
with equal base and height. (see image)

Archimedes is the first to identify the concept of center of gravity, and he
found the centers of gravity of various geometric figures, assuming uniform
density in their interiors, including triangles, paraboloids, and hemispheres.

Asimov calls Archimedes the greatest in science and math before Newton.
Archimedes is a
Greek mathematician, physicist, engineer, astronomer, and philosopher born in
the seaport colony of Syracuse, Sicily.

It's possible that in a long duration seige that even the burning of a landed
ship from a roof might be of value.

Cicero writes that the Roman consul Marcellus brought two devices back to Rome
from the sacked city of Syracuse. One device mapped the sky on a sphere and the
other predicted the motions of the sun and the moon and the planets (i.e., an
orrery). He credits Thales and Eudoxus for constructing these devices. For some
time this was assumed to be a legend of doubtful nature, but the discovery of
the Antikythera mechanism has changed the view of this issue, and it is indeed
probable that Archimedes possessed and constructed such devices. Pappus of
Alexandria writes that Archimedes had written a practical book on the
construction of such spheres entitled On Sphere-Making.

Archimedes' works were not widely recognized, even in antiquity. He and his
contemporaries probably constitute the peak of Greek mathematical rigour.
During the Middle Ages the mathematicians who could understand Archimedes' work
were few and far between. Many of his works were lost when the library of
Alexandria was burnt (twice) and survived only in Latin or Arabic translations.
As a result, his mechanical method was lost until around 1900, after the
arithmetization of analysis had been carried out successfully. We can only
speculate about the effect that the "method" would have had on the development
of calculus had it been known in the 16th and 17th centuries.

Archimedes requests that his tombstone include a cylinder circumscribing a
sphere, accompanied by the inscription of his amazing theorem that the sphere
is exactly two-thirds of the circumscribing cylinder in both surface area and
volume.

Writings by Archimedes
* On the Equilibrium of Planes (2 volumes)
This scroll explains the law of
the lever and uses it to calculate the areas and centers of gravity of various
geometric figures.

* On Spirals
In this scroll, Archimedes defines what is now called Archimedes' spiral.
This is the first mechanical curve (i.e., traced by a moving point) ever
considered by a Greek mathematician.

* On the Sphere and The Cylinder
In this scroll Archimedes obtains the result he was
most proud of: that the area and volume of a sphere are in the same
relationship to the area and volume of the circumscribed straight cylinder.

* On Conoids and Spheroids
In this scroll Archimedes calculates the areas and volumes of
sections of cones, spheres and paraboloids.

* On Floating Bodies (2 volumes)
In the first part of this scroll, Archimedes spells out
the law of equilibrium of fluids, and proves that water around a center of
gravity will adopt a spherical form. This is probably an attempt at explaining
the observation made by Greek astronomers that the Earth is round. Note that
his fluids are not self-gravitating: he assumes the existence of a point
towards which all things fall and derives the spherical shape. One is led to
wonder what he would have done had he struck upon the idea of universal
gravitation.
In the second part, a veritable tour-de-force, he calculates the equilibrium
positions of sections of paraboloids. This was probably an idealization of the
shapes of ships' hulls. Some of his sections float with the base under water
and the summit above water, which is reminiscent of the way icebergs float,
although Archimedes probably was not thinking of this application.

* The Quadrature of the Parabola
In this scroll, Archimedes calculates the area of a
segment of a parabola (the figure delimited by a parabola and a secant line not
necessarily perpendicular to the axis). The final answer is obtained by
triangulating the area and summing the geometric series with ratio 1/4.

* Stomachion
This is a Greek puzzle similar to Tangram. In this scroll, Archimedes
calculates the areas of the various pieces. This may be the first reference we
have to this game. Recent discoveries indicate that Archimedes was attempting
to determine how many ways the strips of paper could be assembled into the
shape of a square. This is possibly the first use of combinatorics to solve a
problem.

* Archimedes' Cattle Problem
Archimedes wrote a letter to the scholars in the Library
of Alexandria, who apparently had downplayed the importance of Archimedes'
works. In these letters, he dares them to count the numbers of cattle in the
Herd of the Sun by solving a number of simultaneous Diophantine equations, some
of them quadratic (in the more complicated version). This problem is one of the
famous problems solved with the aid of a computer. The solution is a very large
number, approximately 7.760271 × 10206544 (See the external links to the
Cattle Problem.)

* The Sand Reckoner
In this scroll, Archimedes counts the number of grains of sand
fitting inside the universe. This book mentions Aristarchus of Samos' theory of
the solar system (concluding that "this is impossible"), contemporary ideas
about the size of the Earth and the distance between various celestial bodies.
From the introductory letter we also learn that Archimedes' father was an
astronomer.

* "The Method"
In this work, which was unknown in the Middle Ages, but the importance
of which was realised after its discovery, Archimedes pioneered the use of
infinitesimals, showing how breaking up a figure in an infinite number of
infinitely small parts could be used to determine its area or volume.
Archimedes did probably consider these methods not mathematically precise, and
he used these methods to find at least some of the areas or volumes he sought,
and then used the more traditional method of exhaustion to prove them. Some
details can be found at how Archimedes used infinitesimals.

What an interesting group of people and interesting time it must have been for
the people at the university in Alexandria, perhaps unknown to them, to be with
the smartest and most interesting humans on earth like Aristarchos, Archimedes,
Eritosthenes, etc.). All people eat together at the university which must have
made for some very enlightened conversations.

Archimedes' father is an astronomer. Archimedes learns in Alexandria, and
decides to move back to Syracuse (which is rare for most people in Alexandria)
perhaps because he is related to the King of Syracuse Hieron II.
Archimedes is
independently wealthy and does not depend on the wealth of royal people in
Egypt.

Archimedes is asked by Hieron if a crown from a gold smith was really all gold,
or if the crown had silver mixed in. Archimedes is told that he cannot damage
the crown in the determination. Archimedes can not think of how to solve the
problem until one time he steps in a bath and notes that the water overflows.
Archimedes realizes that the amount of water that falls out is equal to the
volume of his body. If put in water, Archimedes could measure the volume of the
crown, then measure the weight of the crown, and compare this weight with an
equal volume of pure gold. The crown and the piece of gold with the same volume
should weight the same. If the crown weighes more than the pure gold with the
same volume, then the crown is not pure gold. Archimedes, excited by this
realization, ran naked through the streets of Syracuse (although people were
not as disturbed by nudity then) yelling "eureka! eureka!" (or 'Heureka'; Greek
ηὕρηκα; I have found it). The crown is partly silver and the goldsmith
is executed.

Archimedes makes use of levers (Strato was aware of the idea). Archimedes is
told to have said "give me a place to stand and I can move the world". Hieron
is supposed to have challanged Archimedes, and Archimedes said to have lifted a
ship from a harbor on to shore.
  
2,250 YBN
[250 BC]
893)
  
2,250 YBN
[250 BC]
894)
  
2,246 YBN
[246 BC]
898) Eratosthenes of Cyrene (Kurinaios) (Ἐρατοσθένης) (BCE 276-196)
is the first person to accurately calculate the size of the earth.

On the day of summer solstace, the longest day of the year, the Sun is directly
over head in Syene (now Aswan) in southern Egypt, but at the same time in
Alexandria, the Sun is a few degrees from the (perpendicular or) zenith in
Alexandria. The difference is because the surface of the earth is curved and
not flat. Erastosthenes is aware that Syene and Alexandria are almost on the
same line of longitude (or meridian) and also knows the distance between Syene
and Alexandria (Erastothenes hired a human to pace out the distance between
Alexandria and Syene ), and uses this distance and the angle of the Sun to
calculate the diameter of the planet earth. This result is in units of
measurement of space called "stadia". Eratosthenes calculates a distance
between Alexandria and Syene as 5,000 stadia, and calculates that the angle of
the Sun (in Alexandria at noon on the longest day of the year) is 1/50th the
circumference of a circle. This puts the circumference Eratosthenes measures at
at 40,000 km (25,000 miles) which is accurate (the current estimate is
40,075.02 km). This number is larger than most humans can accept and so the
smaller estimate of Poseidonius is accepted. From this large number compared to
the "known" earth, Eratosthenes thought the various seas formed a single
interconnected ocean. Eratosthenes teaches that Africa might be
circumnavigated, and that India can be reached by sailing westwards from
Spain.

Eratosthenes makes the "Sieve of Eratosthenes", a system for determining prime
numbers. Eratosthenes makes a map of the "known" earth which is better than any
before. In astronomy, Eratosthenes measures the angle of the earth's axis with
the plane the sun appears to move in, and gets an accurate value. This value is
called the "obliquity of ecliptic". Eratosthenes makes a star map of 675
stars.

Eratosthenes denounces those who divide mankind into two groups, Greeks and
non-Greeks and advocates the Stoic moral principles of virtue and vice as a
criterion for the division of men.

Eratosthenes is a friend of Archimedes.
Alexandria, Egypt  
2,246 YBN
[246 BC]
933)
  
2,246 YBN
[246 BC]
936)
  
2,245 YBN
[245 BC]
896)
  
2,240 YBN
[240 BC]
923) The Serapeion is a massive raised acropolis of buildings.

The Serapeum is away from the main library in the south west corner of
Alexandria, the Egyptian quarter of Rhakotis. The Serapeum is called the
"daughter library". In the bilingual foundation plaques, the name Serapis is
rendered in the Egyptian form of Osor-Hapi (the Egyptian name is Osorapis). Two
obelisks (a thin 4 sided monument becoming thinner up to the top with a
pyramidal top), are said to have stood there as well as two red granite
sphinxes which are still at the site. A black granite Apis bull (an egyptian
god) now in the Alexandria museum was also in the Serapeum. This shows how the
vision of the Ptolemies was to combine the Egyptian and Greek populations.

Ptolemy 3 creates a temple of Serapis in the South-West part of Alexandria,
some distance from the royal quarters. : The excavations by Alan Rowe and
others in 1943-1944 will find foundation plaques that clearly bear the name of
Ptolemy 3 Euergetes, even though medieval writers will attribute the Serapeum
to Ptolemy 2 At the southern end are two long corridors opening into small
rooms, and in particular a row of 19 uniform rooms, each about 3 by 4 meters.
The excavators theorize that these rooms were used to shelve the scrolls of the
Serapeum library, and that the scrolls were consulted in the corridors.

One source has
the Serapeum started under Ptolemy I Soter but finished under Ptolemy 3 as the
foundation plaques excavated in 1942 indicate.

In the east end is a huge statue of the god Serapeus (who looks like Zeus),
made of wood and covered with ivory and gold, the outstretched arms nearly
reach the two side-walls. In the left hand is a sceptre and under the right
hand was an image of Cerberus, with a triple head of lion, dog and wolf, with a
python coiled around he three heads. An east window behind the statue is
arranged so that the first rays of the rising sun light up the features of the
god.

Under the plateau are underground passages and storerooms.

Aphthonios (a Greek sophist and rhetorician living in the second half of the
4th century CE), in his "Progymnasmata", an introductory book on different
kinds of rhetoric (fable, narration, comparison, etc.), gives a sample for the
style of writing titled "Description" that describes the Sarapeion. Aphthonios
writes:
"Description: the temple in Alexandria, together with the acropolis

Citadels are established for the common security of cities - for they are the
highest points of cities. They are not walled round with buildings, so much as
they wall round the cities. The centre of Athens held the Athenian acropolis;
but the citadel which Alexander established for his own city is in fact what he
named it, and it is more accurate to call this an acropolis than that on which
the Athenians pride themselves. For it is somewhat as this discourse shall
describe.

A hill juts out of the ground, rising to a great height, and called an
acropolis on both accounts, both because it is raised up on high and because it
is placed in the high-point of the city. There are two roads to it, of
dissimilar nature. One is a road, the other a way of access. The roads have
different names according to their nature. Here it is possible to approach on
foot and the road is shared also with those who approach on a wagon; there
flights of steps have been cut and there is no passage for wagons. For flight
after flight leads higher and higher, not stopping until the hundredth step;
for the limit of their number is one which produces a perfect measure.

After the steps is a gateway, shut in with grilled gates of moderate size. And
four massive columns rise up, bringing four roads to one entrance. On the
columns rises a building with many columns of moderate size in front, not of
one colour, but they are fixed to the edifice as an ornament. The building's
roof is domed, and round the dome is set a great image of the universe.

As one enters the acropolis itself a single space is marked out by four sides;
the plan of the arrangement is that of a hollow rectangle. There is a court in
the centre, surrounded by a colonnade. Other colonnades succeed the court,
colonnades divided by equal columns, and their length could not be exceeded.
Each colonnade ends in another at right angles, and a double column divides
each colonnade, ending the one and starting the other. Chambers are built
within the colonnades. Some are repositories for the books, open to those who
are diligent in philosophy and stirring up the whole city to mastery of wisdom.
Others are established in honour of the ancient gods. The colonnades are
roofed, and the roof is made of gold, and the capitals {tops} of the columns
are made of bronze overlaid with gold. The decoration of the court is not
single. For different parts are differently decorated, and one has the exploits
of Perseus. In the middle there rises a column of great height, making the
place conspicuous (someone on his way does not know where he is going, unless
he uses the pillar as a sign of the direction) and makes the acropolis stand
out by land and sea. The beginnings of the universe stand round the capital of
the column. Before one comes to the middle of the court there is set an edifice
with many entrances, which are named after the ancient gods; and two stone
obelisks rise up, and a fountain better than that of the Peisistratids. And the
marvel had an incredible number of builders. As one was not sufficient for the
making, builders of the whole acropolis were appointed to the number of twelve
{by the dozen}.

As one comes down from the acropolis, here is a flat place resembling a
race-course, which is what the place is called; and here there is another of
similar shape, but not equal in size.

The beauty is unspeakable. If anything has been omitted, it has been bracketed
by amazement; what it was not possible to describe has been omitted."
Alexandria, Egypt  
2,240 YBN
[240 BC]
1325) Chinese people possibly ob served Halley's comet as early as 2467 BCE.
China  
2,235 YBN
[235 BC]
890)
  
2,235 YBN
[235 BC]
895)
  
2,230 YBN
[230 BC]
1034) The letter "G" is added to the Latin alphabet in Rome. Before this the
letter "C" could be either the "K" or "G" sound, now the letter "G" will have
the "G" sound and the letter "C" will only have the "K" sound. A more logical
system would be to not add any letter "G", and to use the letter "C" only as
"G", "K" for all "K" sounds, but this simple one letter equals one sound only
system is not recognized. This confusion about how to pronounce the letter "C"
will continue for thousands of years, persisting even today. Later the letter
"C" will also take on an "S" and "CH" sound and "G" will take on the "J" sound,
adding to a simple and unnecessary confusion.
  
2,230 YBN
[230 BC]
1373) Ptolemy II Philadelphus, the ruler of Ptolemaic Egypt and contemporary of
Ashoka, is recorded by Pliny the Elder as sending an ambassador named Dionysius
to the Mauryan court at Pataliputra in India:
"But {India} has been treated of by
several other Greek writers who resided at the courts of Indian kings, such,
for instance, as Megasthenes, and by Dionysius, who was sent thither by
Philadelphus, expressly for the purpose: all of whom have enlarged upon the
power and vast resources of these nations."
Hindustan  
2,212 YBN
[212 BC]
892)
  
2,208 YBN
[208 BC]
1051)
  
2,205 YBN
[205 BC]
937)
  
2,204 YBN
[204 BC]
938)
  
2,204 YBN
[204 BC]
939)
  
2,200 YBN
[200 BC]
1063)
India  
2,196 YBN
[196 BC]
1267)
Egypt  
2,191 YBN
[191 BC]
940)
  
2,189 YBN
[189 BC]
948)
  
2,186 YBN
[186 BC]
1117) The Suàn shù shū is an ancient Chinese collection of writings on
mathematics approximately 7000 characters in length, written on 190 bamboo
strips, recovered from a tomb that appears to have been closed in 186 B.C. This
anonymous collection is not a single coherent book, but is made up of
approximately 69 independent sections of text, which appear to have been
assembled from a variety of sources. Problems treated range from elementary
calculations with fractions to applications of the Rule of False Position and
finding the volumes of various solid shapes.
Zhangjiashan, Hubei Provience, China  
2,175 YBN
[175 BC]
949)
  
2,173 YBN
[173 BC]
955)
  
2,164 YBN
[09/??/164 BC]
1324)
Babylonia  
2,160 YBN
[160 BC]
1029) Pliny will claim, in his "Natural History", that Hipparchos compiled his
catalog of stars so that future astronomers can detect changes in positions and
the possible appearance of novae. Lucio Russo writes that Edmund Halley,
"probably without realizing that he was completing an experiment ... started
two thousand years earlier" will be the first to notice this difference in
1718.

In the 2nd and 3rd centuries coins were made in his honour in Bithynia that
bear his name and show him with a globe; this confirms the tradition that he
was born there.
Hipparchus is believed to have died on the island of Rhodes, where he
spent most of his later life--Ptolemy attributes observations to him from
Rhodes in the period from 141 BC to 127 BC.
Hipparchus is recognized as the
originator and father of scientific astronomy. He is believed to be the
greatest Greek astronomical observer, and many regard him as the greatest
astronomer of ancient times, although Cicero gave preferences to Aristarchus of
Samos. Some put in this place also Ptolemy of Alexandria. Hipparchus' writings
had been mostly superseded by those of Ptolemy, so later copyists have not
preserved them for posterity.
Earlier Greek astronomers and mathematicians were influenced
by Babylonian astronomy to a limited extent, for instance the period relations
of the Metonic cycle and Saros cycle may have come from Babylonian sources.
Hipparchus seems to have been the first to exploit Babylonian astronomical
knowledge and techniques systematically. He was the first Greek known to divide
the circle in 360 degrees of 60 arc minutes (Eratosthenes before him used a
simpler sexagesimal system dividing a circle into 60 parts). He also used the
Babylonian unit pechus ("cubit") of about 2° or 2½°.

Hipparchus also studied the motion of the Moon and confirmed the accurate
values for some periods of its motion that Chaldean astronomers had obtained
before him. The traditional value (from Babylonian System B) for the mean
synodic month is 29 days;31,50,8,20 (sexagesimal) = 29.5305941... d. Expressed
as 29 days + 12 hours + 793/1080 hours this value has been used later in the
Hebrew calendar (possibly from Babylonian sources). The Chaldeans also knew
that 251 synodic months = 269 anomalistic months. Hipparchus extended this
period by a factor of 17, because after that interval the Moon also would have
a similar latitude, and it is close to an integer number of years (345).
Therefore, eclipses would reappear under almost identical circumstances. The
period is 126007 days 1 hour (rounded). Hipparchus could confirm his
computations by comparing eclipses from his own time (presumably 27 January 141
BCE and 26 November 139 BCE according to {Toomer 1980}), with eclipses from
Babylonian records 345 years earlier (Almagest IV.2; {Jones 2001}).

Before Hipparchus, Meton, Euctemon, and their pupils at Athens had made a
solstice observation (i.e., timed the moment of the summer solstice) on June
27, 432 BC (proleptic Julian calendar). Aristarchus of Samos is said to have
done so in 280 BC, and Hipparchus also had an observation by Archimedes.
Hipparchus himself observed the summer solstice in 135 BC, but he found
observations of the moment of equinox more accurate, and he made many during
his lifetime. Ptolemy gives an extensive discussion of Hipparchus' work on the
length of the year in the Almagest III.1, and quotes many observations that
Hipparchus made or used, spanning 162 BCE to 128 BCE. At the end of his career,
Hipparchus wrote a book called Peri eniausíou megéthous ("On the Length of
the Year") about his results.

Before Hipparchus the Chaldean astronomers knew that the lengths of the seasons
are not equal. Hipparchus made equinox and solstice observations, and according
to Ptolemy (Almagest III.4) determined that spring (from spring equinox to
summer solstice) lasted 94 + 1/2 days, and summer (from summer solstice to
autumn equinox) 92 + 1/2 days. This is an unexpected result given a premise of
the Sun moving around the Earth in a circle at uniform speed. Hipparchus'
solution was to place the Earth not at the center of the Sun's motion, but at
some distance from the center. This model described the apparent motion of the
Sun fairly well (of course today we know that the planets like the Earth move
in ellipses around the Sun, but this was not discovered until Johannes Kepler
published his first two laws of planetary motion in 1609). It's not clear if
Hipparchos or Ptolemy found these values.
Hipparchus also undertook to find the
distances and sizes of the Sun and the Moon. He published his results in a work
of two books called Peri megethoon kai 'apostèmátoon ("On Sizes and
Distances") by Pappus in his commentary on the Almagest V.11; Theon of Smyrna
(2nd century) mentions the work with the addition "of the Sun and Moon".

Hipparchus measured the apparent diameters of the Sun and Moon with his
diopter. Like others before and after him, he found that the Moon's size varies
as it moves on its (eccentric) orbit, but he found no perceptible variation in
the apparent diameter of the Sun. He found that at the mean distance of the
Moon, the Sun and Moon had the same apparent diameter

Like others before and after him, he also noticed that the Moon has a
noticeable parallax, i.e., that it appears displaced from its calculated
position (compared to the Sun or stars), and the difference is greater when
closer to the horizon. He knew that this is because the Moon circles the center
of the Earth, but the observer is at the surface - Moon, Earth and observer
form a triangle with a sharp angle that changes all the time. From the size of
this parallax, the distance of the Moon as measured in Earth radii can be
determined. For the Sun however, there was no observable parallax (we now know
that it is about 8.8", more than ten times smaller than the resolution of the
unaided eye).

In the first book, Hipparchus assumes that the parallax of the Sun is 0, as if
it is at infinite distance. He then analyzed a solar eclipse, presumably that
of 14 March 190 BC. Alexandria and Nicaea are on the same meridian. Alexandria
is at about 31° North, and the region of the Hellespont at about 41° North;
authors like Strabo and Ptolemy had fairly decent values for these geographical
positions, and presumably Hipparchus knew them too. So Hipparchus could draw a
triangle formed by the two places and the Moon, and from simple geometry was
able to establish a distance of the Moon, expressed in Earth radii. Because the
eclipse occurred in the morning, the Moon was not in the meridian, and as a
consequence the distance found by Hipparchus was a lower limit. In any case,
according to Pappus, Hipparchus found that the least distance is 71 (from this
eclipse), and the greatest 81 Earth radii.

In the second book, Hipparchus starts from the opposite extreme assumption: he
assigns a (minimum) distance to the Sun of 470 Earth radii. This would
correspond to a parallax of 7', which is apparently the greatest parallax that
Hipparchus thought would not be noticed (for comparison: the typical resolution
of the human eye is about 2'. In this case, the shadow of the Earth is a cone
rather than a cylinder as under the first assumption. Hipparchus observed (at
lunar eclipses) that at the mean distance of the Moon, the diameter of the
shadow cone (of the earth) is 2+½ lunar diameters. That apparent diameter is,
as he had observed, 360/650 degrees (of the sky). With these values and simple
geometry, Hipparchus could determine the mean distance; because it was computed
for a minimum distance of the Sun, it is the maximum average distance possible
for the Moon. With his value for the eccentricity of the orbit, he could
compute the least and greatest distances of the Moon too. According to Pappus,
he found a least distance of 62, a mean of 67+1/3, and consequently a greatest
distance of 72+2/3 Earth radii. With this method, as the parallax of the Sun
decreases (i.e., its distance increases), the minimum limit for the mean
distance is 59 Earth radii - exactly the mean distance that Ptolemy will later
derive.

Hipparchus therefore had the problematic result that his minimum distance (from
book 1) was greater than his maximum mean distance (from book 2). He was
intellectually honest about this discrepancy, and probably realized that
especially the first method is very sensitive to the accuracy of the
observations and parameters (in fact, modern calculations show that the size of
the solar eclipse at Alexandria must have been closer to 9/10 than to the
reported 4/5).

Ptolemy later measured the lunar parallax directly (Almagest V.13) (presumable
against the position of a star?), and used the second method of Hipparchus'
with lunar eclipses to compute the distance of the Sun (Almagest V.15). He will
criticize Hipparchus for making contradictory assumptions, and obtaining
conflicting results (Almagest V.11): but apparently he will fail to understand
Hipparchus' strategy to establish limits consistent with the observations,
rather than a single value for the distance. Hipparchos' results are the best
until his time: the actual mean distance of the Moon is 60.3 Earth radii,
within his limits from book 2.

Pliny (Naturalis Historia II.X) tells us that Hipparchus demonstrated that
lunar eclipses can occur five months apart, and solar eclipses seven months
(instead of the usual six months); and the Sun can be hidden twice in thirty
days, but as seen by different nations. Ptolemy discussed this a century later
at length in Almagest VI.6. The geometry, and the limits of the positions of
Sun and Moon when a solar or lunar eclipse is possible, are explained in
Almagest VI.5. Hipparchus apparently made similar calculations. The result that
two solar eclipses can occur one month apart is important, because this can not
be based on observations: one is visible on the northern and the other on the
southern hemisphere - as Pliny indicates -, and the latter was inaccessible to
the Greek.

Prediction of a solar eclipse, i.e., exactly when and where it will be visible,
requires a solid lunar theory and proper treatment of the lunar parallax.
Hipparchus must have been the first to be able to do this. A rigorous treatment
requires spherical trigonometry, but Hipparchus may have made do with planar
approximations. He may have discussed these things in Peri tes kata platos
meniaias tes selenes kineseoos ("On the monthly motion of the Moon in
latitude"), a work mentioned in the Suda.

Hipparchus is credited with the invention or improvement of several
astronomical instruments, which were used for a long time for naked-eye
observations. According to Synesius of Ptolemais (4th century) he made the
first astrolabion: this may have been an armillary sphere (which Ptolemy
however says he constructed, in Almagest V.1); or the predecessor of the planar
instrument called astrolabe (also mentioned by Theon of Alexandria). With an
astrolabe Hipparchus was the first to be able to measure the geographical
latitude and time by observing stars. Previously this was done at daytime by
measuring the shadow cast by a gnomon, or with the portable instrument known as
scaphion.

Ptolemy mentions (Almagest V.14) that he used a similar instrument as
Hipparchus, called dioptra, to measure the apparent diameter of the Sun and
Moon. Pappus of Alexandria described it (in his commentary on the Almagest of
that chapter), as did Proclus (Hypotyposis IV). It was a 4-foot rod with a
scale, a sighting hole at one end, and a wedge that could be moved along the
rod to exactly obscure the disk of Sun or Moon.

Hipparchus also observed solar equinoxes, which may be done with an equatorial
ring: its shadow falls on itself when the Sun is on the equator (i.e., in one
of the equinoctial points on the ecliptic), but the shadow falls above or below
the opposite side of the ring when the Sun is south or north of the equator.
Ptolemy quotes (in Almagest III.1 (H195)) a description by Hipparchus of an
equatorial ring in Alexandria; a little further he describes two such
instruments present in Alexandria in his own time.

Contributions to geography: Hipparchus applied his knowledge of spherical
angles to the problem of denoting locations on the Earth's surface. Before him
a grid system had been used by Dicaearchus of Messana, but Hipparchus was the
first to apply mathematical rigor to the determination of the latitude and
longitude of places on the Earth. Hipparchus wrote a critique in three books on
the work of the geographer Eratosthenes of Cyrene (3rd century BC), called
Pròs tèn 'Eratosthénous geografían ("Against the Geography of
Eratosthenes"). It is known to us from Strabo of Amaseia, who in his turn
criticised Hipparchus in his own Geografia. Hipparchus apparently made many
detailed corrections to the locations and distances mentioned by Eratosthenes.
It seems he did not introduce many improvements in methods, but he did propose
a means to determine the geographical longitudes of different cities at lunar
eclipses (Strabo Geografia 7). A lunar eclipse is visible simultaneously on
half of the Earth, and the difference in longitude between places can be
computed from the difference in local time when the eclipse is observed. His
approach would give accurate results if it were correctly carried out but the
limitations of timekeeping accuracy in his era made this method impractical.

Previously, Eudoxus of Cnidus in the 4th century B.C. had described the stars
and constellations in two books called Phaenomena and Entropon. Aratus wrote a
poem called Phaenomena or Arateia based on Eudoxus' work. Hipparchus wrote a
commentary on the Arateia - his only preserved work - which contains many
stellar positions and times for rising, culmination, and setting of the
constellations, and these are likely to have been based on his own
measurements.

Hipparchus made his measurements with an equatorial armillary sphere, and
obtained the positions of maybe about 850 stars. It is disputed which
coordinate system he used. Ptolemy's catalogue in the Almagest, which is
derived from Hipparchus' catalogue, is given in ecliptic coordinates.

Hipparchus' original catalogue has not been preserved today. However, an
analysis of an ancient statue of Atlas (the so-called Farnese Atlas) published
in 2005 shows stars at positions that appear to have been determined using
Hipparchus' data..

As with most of his work, Hipparchus star catalogue has been adopted and
expanded by Ptolemy. It has been strongly disputed how much of the star
catalogue in the Almagest is due to Hipparchus, and how much is original work
by Ptolemy. Statistical analysis (e.g. by Bradly Schaeffer, and others) shows
that the classical star catalogue has a complex origin. Ptolemy has even been
accused of fraud for stating that he re-measured all stars: many of his
positions are wrong and it appears that in most cases he used Hipparchus' data
and precessed them to his own epoch three centuries later, but using an
erroneous (too small) precession constant.

In any case the work started by Hipparchus has had a lasting heritage, and has
been worked on much later by Al Sufi (964), and by Ulugh Beg as late as 1437.
It was superseded only by more accurate observations after invention of the
telescope.

Hipparchus (is the first?) ranks stars in six magnitude classes according to
their brightness: he assignes the value of one to the twenty brightest stars,
to weaker ones a value of two, and so forth to the stars with a class of six,
which can be barely seen with the naked eye. A similar system is still used
today (perhaps a system based on number of photons received/second will be
next).

Hipparchus is perhaps most famous for having discovered the precession of the
equinoxes. His two books on precession, On the Displacement of the Solsticial
and Equinoctial Points and On the Length of the Year, are both mentioned in the
Almagest of Claudius Ptolemy. According to Ptolemy, Hipparchus measured the
longitude of Spica and other bright stars. Comparing his measurements with data
from his predecessors, Timocharis and Aristillus, he realized that Spica had
moved 2° relative to the autumnal equinox. He also compared the lengths of the
tropical year (the time it takes the Sun to return to an equinox) and the
sidereal year (the time it takes the Sun to return to a fixed star), and found
a slight discrepancy. Hipparchus concluded that the equinoxes were moving
("precessing") through the zodiac, and that the rate of precession was not less
than 1° in a century.

Ptolemy followed up on Hipparchus' work in the 2nd century AD. He confirmed
that precession affected the entire sphere of fixed stars (Hipparchus had
speculated that only the stars near the zodiac were affected), and concluded
that 1° in 100 years was the correct rate of precession. The modern value is
1° in 72 years.

As far as is known, Hipparchus never wrote about astrology, i.e. the
application of astronomy to the (fraudulent albeit nonviolent and legal)
practice of divination.
  
2,150 YBN
[150 BC]
1039) Seleukos lives in Babylonia and is probably called "Chaldean" or
"Babylonian", but was probably part Greek, and lives during the same time as
Hipparchos.
Strabo will explain that Seleukos understood the yearly changes of
the tides from season to season, revealing the fact that tides show a maximum
change in height with each consecutive high tide (diurnal inequality) during
the solstice, and minimum change of height difference of consecutive high tides
during the equinox. This phenomenon is explained by the fact that the earth is
tilted to the sun, during the solstice, but is not tilted to the sun during the
equinox {add image}, although this could be explained with a tilted sun in an
earth-centered theory. This phenomenon will not be understood again until G. H.
Darwin in 1898.

Plutarch writes: Was {Timaeus} giving the earth motion ..., and should the
earth ... be understood to have been designed not as confined and fixed but as
turning and revolving about, in the way expounded later by Aristarchos and
Seleukos, the former assuming this as a hypothesis and the latter proclaiming
it?"

Aetius will write, "Seleucus the mathematician (also one of those who think the
earth moves) says that the moon's revolution counteracts the whirlpool motion
of the earth".
Seleucia (on the Tigris River), Babylon  
2,145 YBN
[145 BC]
950)
  
2,145 YBN
[145 BC]
951)
  
2,143 YBN
[143 BC]
1337) Shishi, in Chinese means "Stone House", which refers to how the school
was originally built.
Chengdu, China  
2,140 YBN
[140 BC]
1070) The invention of paper. The earliest paper artifact (although without
writing) is made of hemp fibers and comes from a tomb in China.

Before this bamboo and silk are written on in China.

The method of making paper by pouring wood pulp mixed in water into a flat mold
and drying the sediment will take over 1000 years to be understood in Europe,
although it will reach India in the 600s CE.

Paper is considered one of the most important inventions in history, since it
enables China to develop its civilization much faster than with earlier writing
materials (primarily bamboo), and it does the same with Europe when it is
introduced in the 12th century or the 13th century.
Xian, China  
2,134 YBN
[01/01/134 BC]
1041)
  
2,127 YBN
[127 BC]
943)
  
2,120 YBN
[120 BC]
942)
  
2,105 YBN
[01/01/105 BC]
1042) Poseidonios is a Greek Stoic philosopher, politician, astronomer,
geographer, historian, and teacher. He is acclaimed as the greatest polymath of
his age. None of his vast body of work can be read in its entirety today as it
exists only in fragments.

Like Pytheas, Poseidonios thinks that the moon causes the tides, and goes west
to the Atlantic ocean to study tides. Poseidonios uses Canopus in place of the
sun in order to calculate the size of the earth, but his measurement is too
small (as described by Strabo the only source for this data). Ptolemy will
accept this lower number, instead of accurate calculation made by Eratosthenes,
and this will be the accepted value of the Earth's circumference for the next
1,500 years, and may influence Christopher Columbus that the earth can be
circumnavigated. Poseidonius supports the pseudoscience of astrology.

He attempted to measure the distance and size of the Sun. In about 90 BCE
Posidonius estimated the astronomical unit to be a0/rE = 9893, which was still
too small by half. In measuring the size of the Sun, however, he reached a
figure larger and more accurate than those proposed by other Greek astronomers
and Aristarchus of Samos.

Posidonius also calculated the size and distance of the Moon.

Posidonius constructed an orrery, possibly similar to the Antikythera
mechanism. Posidonius's orrery, according to Cicero, exhibited the diurnal
motions of the sun, moon, and the five known planets.
  
2,100 YBN
[100 BC]
952)
  
2,100 YBN
[100 BC]
1064)
Central Asia  
2,100 YBN
[100 BC]
1374)
Rome  
2,080 YBN
[80 BC]
870)
  
2,080 YBN
[80 BC]
1046)
  
2,076 YBN
[76 BC]
1047)
  
2,075 YBN
[75 BC]
1116) Negative numbers.
The first use of negative numbers is in the Chinese mathematics
book "The Nine Chapters on the Mathematical Art" (Jiuˇ zhāng suàn shù).
Negative numbers are in red and positive numbers in black.
The Nine Chapters is
a Chinese counterpart to Euclid’s Elements, which dominates Western
mathematics in the same way the Nine Chapters is the basis of ancient Chinese
mathematics for nearly two millennia. Euclid’s text is uses an axiomatic
method while The Nine Chapters, is a much more down-to-Earth handbook for the
solution of practical problems.
China  
2,070 YBN
[70 BC]
953)
  
2,060 YBN
[60 BC]
958)
  
2,060 YBN
[60 BC]
959)
  
2,056 YBN
[56 BC]
1045) Lucretius (BCE c95-c55) describes light and heat as being made of tiny
atoms that move very fast.

Lucretius {LYUKREsEuS}, Titus Lucretius Carus, Roman poet and philosopher,
writes "De Natura Rerum" (On the Nature of things) which describes a mechanical
Epikourean view of universe in a (longer than average) poem. Influenced by
Democritus, Lucretius supports the idea that all things are made of atoms
including souls and even Gods. Like Epikouros, Lucretius thinks that the Gods
are not concerned with the lives of humans, and death is not to be feared. In
addition Lucretius thinks that there is no after life, only peaceful
nothingness. Lucretius is the first to divide human history in to the stone
age, bronze age, and iron age. Lucretius is the boldest person of this time to
speak out against religion, superstition and mysticism.

In "De rerum natura" Lucretius writes (translated from Latin): "...the velocity
with which these images travel is enormous: light things made of fine atoms
often travel very swiftly, as sunlight; it is natural then that these images
should do the same; of which too there is a constant succession one following
on the other like light or heat from the sun. ...".
Rome, Italy  
2,055 YBN
[08/??/55 BC]
1057)
  
2,050 YBN
[50 BC]
1050)
  
2,048 YBN
[48 BC]
956) A fire set by soldiers for Julius Caesar may have burned only some
storehouses of books, or may have partially or completely burned the Royal
Library too, but in any event, the Royal Mouseion (which possibly housed the
Royal Library) and Sarapeion survived undamaged.
  
2,045 YBN
[45 BC]
954)
  
2,045 YBN
[45 BC]
1056)
  
2,045 YBN
[45 BC]
1523)
Rome, Italy  
2,041 YBN
[41 BC]
957)
  
2,040 YBN
[40 BC]
1058) Earliest waterwheel and elevator (vertical lift).

In the first century BC Roman engineer Vitruvius writes "De architectura",
known today as "The Ten Books of Architecture", a treatise in Latin on
architecture, dedicated to the emperor Augustus. It is the only surviving major
book on architecture from classical antiquity.

In a section of "De architectura" that describes machines rarely used,
Vitruvius describes the undershot water wheel. Vitruvius also describes the
first geared vertical wheel for which there is good evidence. This mill is also
of major significance because it is the first application of gearing which uses
something besides muscle power. This mill has an undershot wheel which, unlike
the breast or overshot wheels, does not make use of the weight of falling
water. An "overshot" waterwheel uses water from above to move the wheel by
filling buckets on the wheel, while an "undershot" waterwheel uses the force of
the water passing below to spin a paddle wheel. A "breast" waterwheel uses the
wheel horizontally.

Vitruvius {ViTrUVEuS} describes lifting platforms that use pulleys and capstans
(apparatus used for hoisting weights, consisting of a vertical spool-shaped
cylinder that is rotated manually or by machine and around which a cable is
wound), or windlasses (hauling or lifting machines consisting of a horizontal
cylinder turned by a crank or a motor so that a line attached to the load is
wound around the cylinder), operated by human, animal, or water power.
Rome  
2,033 YBN
[08/01/33 BC]
961)
  
2,033 YBN
[08/01/33 BC]
962)
  
2,033 YBN
[33 BC]
1059) Strabo was born in a wealthy family from Amaseia, which is in modern
Amasya, Turkey, within Pontus; which had recently become part of the Roman
Empire. He studies under various geographers and philosophers; first in Nysa,
later in Rome. He is philosophically a Stoic and politically a proponent of
Roman imperialism. Later he will make extensive travels to Egypt and Ethiopia,
among others. It is not known when his Geography is written, though comments
within the work itself place the finished version within the reign of Emperor
Tiberius. Some place its first drafts at around 7 CE, others around 18 CE.
Mention is given to the death in 23 CE of Juba, king of Maurousia.

Strabo's History is nearly completely lost. Although Strabo quotes it himself,
and other classical authors mention that it existed, the only surviving
document is a fragment of papyrus now in possession of the University of Milan
(renumbered {Papyrus} 46).

Impressed by the size of the unmapped parts of earth, Strabo suggests that
there are other continents.
Strabo wrongly accepts Homer's geographic descriptions over the
more accurate data of Herodotus.
Strabo writes about the Mouseion in Alexandria in
addition to the original papyri of Aristotle's writing.
Strabo's conversion from a
sphere to plane in inaccurate.

Strabo's "Geography" is an important source for information about the Mouseion
of Alexandria. In book 17, Strabo writes: "The Museum is also a part of the
royal palaces; it has a public walk, an Exedra {a semi-circular room} with
seats, and a large house, in which is the common mess-hall of the men of
learning who share the Museum. This group of men not only hold property in
common, but also have a priest in charge of the Museum, who formerly was
appointed by the kings, but is now appointed by Caesar."
Amasya, Pontus {on the coast of Turkey}  
2,031 YBN
[09/02/31 BC]
967)
Actium, Greece  
2,030 YBN
[08/01/30 BC]
960)
  
2,030 YBN
[08/01/30 BC]
963)
  
2,030 YBN
[30 BC]
3060) The chief teacher of Varro is L. Aelius Stilo, the first systematic
student, critic and teacher of Latin (language) and literature, and of the
antiquities of Rome and Italy. Varro also studies at Athens, especially under
the philosopher Antiochus of Ascalon, whose aim it is to lead back the Academic
school from the scepticism of Arcesilaus and Carneades to the tenets of the
early Platonists, as he understands them.

In 59 Varro wrote a political pamphlet entitled "Trikaranos" ("The
Three-Headed") on the coalition of Pompey, Julius Caesar, and Crassus.

Varro serves under Pompey in the civil war. When he returns to Rome after the
Battle of Pharsalus in 48 BCE, Caesar, the victor, pardons Varro and
commissions Varro to establish a public library of Greek and Latin literature.
Varro then dedicates the second part of his "Antiquitates rerum humanarum et
divinarum" ("Antiquities of Human and Divine Things") to Julius Caesar. After
Julius Caesar is murdered in 44 BCE, under the second triumvirate, Mark Antony
puts Varro's name on the list of those considered to be enemies of the state.
Although his books are burned, his villa plundered, and his library destroyed,
Varro escapes death through the intervention of Octavian (later Augustus).
Thereafter, Varro spends his remaining years in seclusion, reading and
writing.

Varro's distinct literary works are numbered at 74 and the number of separate
"books" at about 620.

Varro writes on a wide variety of subjects, including law, astronomy,
geography, education, and literary history, as well as satires, poems,
orations, and letters. The only complete work to survive is the "Res rustica"
("Farm Topics"), which contains instruction for plant and animal farming.

Varro dedicates his "De lingua Latina" ("On the Latin Language") to Cicero.
This work contains 25 books, of which only parts of books v to x are known, in
addition to other fragments.

Of Varro's "Saturae Menippeae", 90 of the 150 books and nearly 600 fragments
still exist. These satires are humorous medleys in mixed prose and verse in the
manner of the 200s BCE cynic philosopher Menippus of Gadara. According to
biography, these writings try to make serious logical discussion palatable to
the uneducated reader by blending it with humorous treatment of contemporary
society. Two themes run through the satires. One is the absurdity of much of
Greek philosophy; the other, the contemporary preoccupation with material
luxury, in contrast to the old days, when the Romans were thrifty and
self-denying.

Varro wrote "Portraits" which contains brief biographical essays on some 700
famous Greeks and Romans, with likenesses of each.

Of the 25 books of De lingua Latina, books 5-10 survive, although even they are
incomplete. After an introduction (book 1), the work is divided into etymology
(history of language) (2-7), inflection (8-13), and syntax (14-25).

Cicero's praises Varro writing "When we were foreigners and wanderers -
strangers, as it were, in our own land - your books led us home and made it
possible for us at length to learn who we were as Romans and where we lived.".

Varro creates a chronology, although the chronology of Livy is viewed as more
accurate. The Romans call their years after the two supreme magistrates, the
consuls. With a list of magistrates, all past events can be dated.
Rome, Italy  
2,027 YBN
[01/06/27 BC]
1524)
Rome, Italy  
2,027 YBN
[27 BC]
1065)
Rome  
2,019 YBN
[19 BC]
1067)
Pont Du Gard, France  
2,010 YBN
[08/01/10 BC]
964)
  
2,010 YBN
[08/01/10 BC]
965)
  
2,008 YBN
[8 BC]
1071)
Dunhuang, Jiuquan, Gansu province, China  
2,000 YBN
[1960/0 AD]
5737)
(University of California Medical Center) Los Angeles, California, USA  
FUTURE
2,000 YBN
[0 AD]
6298) Artificial muscle wing flapping plane.
  
1,991 YBN
[9 AD]
1055)
  
1,980 YBN
[08/01/20 AD]
966)
  
1,980 YBN
[20 AD]
912) This Celsus is different from the Celsus of the 2nd Century CE who will
write "The True Word", a book critical of Christianity.

His only extant work, the De Medicina, is the only surviving section of a much
larger encyclopedia, and is a primary source on diet, pharmacy and surgery and
related fields. The lost portions of his encyclopedia likely included volumes
on agriculture, law, rhetoric, and military arts. Celsus' De Medicina is one of
the best sources on Alexandrian medical knowledge.

In "Of Medicine", Celsus describes the preparation of numerous ancient
medicinal remedies including the preparation of opioids. In addition, he
describes many 1st century Roman surgical procedures which include treatment
for bladder stones, tonsillectormy, and the setting of fractures.

Celsus is the first to discuss heart attacks. Celsus writes on dentistry and
describes the use of a dental mirror. He describes a "cataract", a condition
where the lens of the eye grows opaque, in addition to a procedure for removing
the clouding. Asimov claims that Celsus is the first to write about insanity
(although I think there must be somebody before this), which is an abstract
label and is the source of many human rights abuse and much pseudoscience.
Celsu
s probably copied much of his writings from the writings of Hippocrates.

Celsus expresses his (in my view, mistaken) belief in the ethicalness of
experimentation on humans, writing in "De Medicina": "It is not cruel to
inflict on a few criminals sufferings which may benefit multitudes of innocent
people through all centuries."

Celsus' work was rediscovered by Pope Nicholas V and published in 1478. His
work became famous for its elegant Latin style.
Gallia Narbonensis, southern France  
1,980 YBN
[20 AD]
1390) Some people question the actual existence of a person named Jesus,
explaining the similarities with stories of past martyrs born on December 25
and executed such as Mithra.
The earliest images of Jesus show Jesus without a
beard.
Galilee  
1,965 YBN
[35 AD]
1049)
  
1,960 YBN
[40 AD]
944)
  
1,959 YBN
[41 AD]
968)
  
1,957 YBN
[43 AD]
1076)
Tingentera, Southern Spain  
1,950 YBN
[50 AD]
1068)
China  
1,950 YBN
[50 AD]
1078) Steam engine.
Heron of Alexandria (Greek: Ήρων ο Αλεξανδρεύς) (CE
c10-c70), a Greek engineer in Alexandria, makes the first recorded steam
engine.

Heron invents an aeopile, which is a hollow metal sphere that rotates from the
power of steam jets that escape through open tubes on each side of the sphere.

The potential of the steam engine will not be understood until the late 1600s.

Heron describes the lever, pulley, wheel, inclined plane, screw, and wedge.
Understands and uses syphons, syringes and gears. Hero uses gears to change the
wheel rotations of a chariot to the rotations of a pointer that indicate the
number of wheel rotations, which is the first odometer (meter that indicates
distance traveled). Hero writes a book on air, which shows that air is a
substance and will not enter a container already filled with air, unless air is
allowed to escape and be replaced. Hero also reasons that because air can be
compressed, air must be made of particles separated by space.
Alexandria, Egypt  
1,950 YBN
[50 AD]
1097)
Alexandria, Egypt  
1,948 YBN
[52 AD]
1079)
Novum Comun, Italy  
1,938 YBN
[62 AD]
945)
  
1,938 YBN
[62 AD]
1080) Hero of Alexandria writes about a lunar eclipse (the shadow of the earth
on the moon) this year.

  
1,934 YBN
[66 AD]
1327)
Judea  
1,930 YBN
[70 AD]
1081) A year after Vespasian is made emperor, Vespasian makes Pliny the Elder,
who is a friend of Vespasian's, procurator in Gallia Narbonensis (the Roman
representative of part of Gaul).

Gaul  
1,927 YBN
[73 AD]
1082) Pliny is made procurator of Hispania Tarraconensis (Governor of a part of
Spain). During his stay in Spain he became familiar with the agriculture and
the mines of the country, in addition to visiting Africa (vii.37)

Spain  
1,925 YBN
[75 AD]
1270)
Sumer/Babylon  
1,923 YBN
[77 AD]
1083) Encyclopedia. Pliny the Elder's "Historia naturalis" ("Natural
History").

Pliny the Elder, ("Gaius Plinius Cecilius Secundus") (PlinE) (CE 23-79)
completes his major work titled "Natural History" in 37 volumes.

"Natural History" is made from copying text of 500 other earlier people and
contains astronomy, geology and zoology. Pliny shows wisdom in rejecting the
idea of immortality.
In addition to "Natural History", Pliny writes a "History
of his Times" in thirty-one books, which has yet to be found.

Historia naturalis serves as a major source for other encyclopaedias for at
least the next 1,500 years. Even today it is still an important record for
details of Roman sculpture and painting.
Spain?  
1,921 YBN
[79 AD]
1084) Pliny the Elder is killed at age 56, by poisonous gas when he goes ashore
to investigate the eruption of Mount Vesuvius.

near Mount Vesuvius, Italy  
1,920 YBN
[80 AD]
1077) These descriptions are accurate and free from superstition.
Tingentera, Southern Spain  
1,919 YBN
[81 AD]
969)
  
1,917 YBN
[83 AD]
766) Magnetic compass.

The first reference to a magnetic compass is from 83 CE, and describes a
"south-controlling spoon" which is thrown on the ground and comes to rest
pointing to the south.

Another early reference to a specific magnetic direction finder device is
recorded in a Song Dynasty book dated to 1040-44. There is a description of an
iron "south-pointing fish" floating in a bowl of water, aligning itself to the
south. The device is recommended as a means of orientation "in the obscurity of
the night".

The Chinese developed both the floating needle and pivoting needle compass. In
1187, English writer Alexander Neckam (1157-1217) describes a "pointer carried
on board {a ship} which enables a course to be followed even when the Polar
star is hidden by clouds.". The "gyrocompass" is invented in 1905 in the United
States by Elmer Ambrose Sperry (1860-1930). The gyrocompass uses the angular
momentum of a gyroscope with the force produced by the Earth's rotation to
maintain a north-south orientation of the spin axis, therefore providing a
stable directional reference.
China (more specific)  
1,903 YBN
[97 AD]
1085) A valuable edition of the De aquis (text and translation) has been
published by C. Herschel (Boston, Mass., 1899). It contains numerous
illustrations; maps of the routes of the ancient aqueducts and the city of Rome
in the time of Frontinus; a photographic reproduction of the only manuscript
(the Monscassinensis); several explanatory chapters, and a concise
bibliography, in which special reference is made to P. de Tissot, Etude sur Ia
condition des agrimensores (1879). There is a complete edition of the works by
A. Dederich (1855), and an English translation of the Strategemata by R. Scott
(1816); more recent editions include that of both the Aqueducts and the
Strategemata in the Loeb Classical Library (1925).
Rome, Italy  
1,900 YBN
[100 AD]
5861)
(now Aidin, Turkey) (verify)  
1,900 YBN
[100 AD]
5872)
(Villa of Cicero) Pompeii, Italy  
1,895 YBN
[105 AD]
1086) Tsai Lun (TSI lUN) (c.50 CE Kueiyang, Kweichow - c.118 CE) is thought by
many to have invented paper from matter like tree bark, hemp, silk and fishing
net, but artifacts of paper have been found that date to before Lun by more
than 100 years.

Tsai Lun is a eunuch person, usually a male that is castrated (testicles are
removed) viewed as a safer (less aggressive) servant for royal people.
Kueiyang, Kweichow?, China  
1,880 YBN
[01/01/120 AD]
1040)
  
1,878 YBN
[122 AD]
1103) Hadrian's Wall is constructed in Britain. Hadrian's Wall (Latin: Vallum
Hadriani) is a stone and turf fortification built by the Roman Emperor Hadrian
(CE 76-138) across the width of Great Britain to prevent military raids by the
tribes of Scotland to the north, to improve economic stability and provide
peaceful conditions in the Roman province of Britannia to the south, to define
the frontier of the Empire physically, and to separate the unruly Selgovae
tribe in the north from the Brigantes in the south and discourage them from
uniting.

The wall is sometimes thought to serve as a border between Scotland and
England, however for most of its length the wall follows a line well south of
the modern border, and neither the Scoti tribe nor the English lived in Britain
at the time of the wall's construction.

Britain  
1,870 YBN
[130 AD]
970) Earth-centered universe of Ptolomy.

Ptolomy's "Almagest" describes an Earth-centered universe.

Claudius Ptolemaeus (Klaudios Ptolemaios) (Greek: Κλαύδιος
Πτολεμαῖος) (CE c100-c170) writes a 13-volume "The Great Treatise",
later named "Almagest", systematizes Alexandrian knowledge of astronomy and
catalogs a thousand stars. Ptolemy creates a mathematical system of epicycles
to explain the apparent motions of the stars and planets based on the incorrect
earth-centered theory. This view dominates Europe until the 1500s.
(some traditions place at) Alexandria  
1,851 YBN
[149 AD]
1088) Galen was born in Pergamum (modern-day Bergama, Turkey), the son of
Nicon, a wealthy architect. His interests were diverse - agriculture,
architecture, astronomy, astrology, philosophy - until he finally focuses on
medicine.

By the age of twenty he had become a therapeutes ("attendant" or "associate")
of the god Asclepius in the local temple for four years. It is after his
father's death in 148 or 149, that he goes abroad to study in Smyrna, Corinth
and Alexandria.
Pergamum, Turkey  
1,850 YBN
[12/27/150 AD]
1109) Hegesippus (c.110 - c.180), is a Christian chronicler of the early Church
who writes against heresies.

His works are lost, save some passages quoted by Eusebius, who tells us that he
wrote Hypomnemata (Memoirs) in five books, in the simplest style concerning the
tradition of the Apostolic preaching. Hegesippus was also known to Jerome. His
work was written to refute the new heresies of the Gnostics and of Marcion. He
appealed principally to tradition as embodied in the teaching which had been
handed down through the succession of bishops, thus providing much information
about the earliest bishops that otherwise would have been lost.

Eusebius says that Hegesippus was a convert from Judaism, for he quoted from
the Hebrew, was acquainted with the Gospel of the Hebrews and with a Syriac
Gospel, and he also cited unwritten traditions of the Jews. He seems to have
lived in some part of the East, possibly Palestine, in the time of Pope
Anicetus (155-166 A.D.) he travelled to Corinth and Rome, collecting on the
spot the teachings of the various churches which he visited, and ascertaining
their uniformity with Rome, according to this excerpt:
"And the Church of the
Corinthians remained in the true word until Primus was bishop in Corinth; I
made their acquaintance in my journey to Rome, and remained with the
Corinthians many days, in which we were refreshed with the true word. And when
I was in Rome, I made a succession up to Anicetus, whose deacon was Eleuterus.
And in each succession and in each city all is according to the ordinances of
the law and the Prophets and the Lord" (quoted in Eusebius, Hist. Eccles. IV,
22).

With great ingenuity J.B. Lightfoot, in Clement of Rome (London, 1890), has
found traces of this list of popes in Epiphanius of Cyprus, Haer., xxvii, 6,
which extends from St Peter to Anicetus in the poem of Pseudo-Tertullian
against Marcion.

Eusebius quotes from Hegesippus a long and perhaps legendary account of the
death of James the Just, "the brother of the Lord", also the story of the
election of his successor Simeon, and the summoning of the descendants of Jude
to Rome by Domitian. A list of heresies against which Hegesippus wrote is also
cited. Dr. Lawlor has argued (Hermathena, XI, 26, 1900, p. 10) that all these
passages cited by Eusebius were connected in the original, and were in the
fifth book of Hegesippus. He has also argued (Journal of Theological Studies,
April, 1907, VIII, 436) the likelihood that Eusebius got from Hegesippus the
statement that John was exiled to Patmos by Domitian. Hegesippus mentioned the
letter of Clement to the Corinthians, apparently in connection with the
persecution of Domitian. It is very likely that the dating of heretics
according to papal reigns in Irenaeus and Epiphanius -- e.g., that Marcion of
Sinope's disciple Cerdon and Valentinus came to Rome under Anicetus -- was
derived from Hegesippus, and the same may be true of the assertion that Hermas,
author of The Shepherd of Hermas, was the brother of Pope Pius (as the Liberian
Catalogue, the poem against Marcion, and the Muratorian fragment all state).

The Church History of Hegesippus appears in an inventory of books in the Abbey
of Corbie; the inventory is of uncertain date, often called 12th century. Zahn
has shown that the work of Hegesippus was still extant in the sixteenth and
seventeenth centuries in three Eastern libraries. (Zeitschrift für
Kirchengeschichte, II (1877-8), 288, and in Theologisches Litteraturblatt
(1893), 495)

The Catholic Encyclopedia writes: "We must lament the loss of other portions of
the Memoirs which were known to exist in the seventeenth century."{1 Cath.
Encyc. 1908 edition}

  
1,850 YBN
[150 AD]
972)
  
1,850 YBN
[150 AD]
973)
  
1,850 YBN
[150 AD]
1087)
Alexandria, Egypt  
1,843 YBN
[157 AD]
1090)
Pergamum, Turkey  
1,838 YBN
[162 AD]
971) Galen is the first person to use a pulse in solving a problem.
Galen also argues
that the mind is in the brain, not in the heart as Aristotle claimed.
Galen does not
recognize blood circulation and wrongly thinks that venous and arterial systems
are separate. Galen recpgnizes that blood must get from one half of the heart
to the other half, and theorizes that there are tiny holes too small to see in
the thick muscular wall separating the two halves. This view will not change
until, 1500 years later, with William Harvey's work in the 17th century. Since
most of his knowledge of anatomy is based on dissection of pigs, dogs, and
Barbary apes, he also presumes wrongly that "rete mirabile", a blood vessel
plexus of ungulates (hooved animal and whales), also existed in the human body.
He also resists the idea of tourniquets to stop bleeding and tragically
vigorously spreads the inaccurate opinion of blood letting as a treatment.

Galen's authority will dominate health science all the way to the 16th century.
With the rise of Christianity, people will not experiment and studies of
physiology and anatomy will stop. Blood letting becomes a standard medical
procedure. Vesalius (1514-1564), more than 1300 years later, will present the
first serious challenge to the dominance of Galen's views.


Galen is attracted to Alexandria because of the reputation of the health
profession there. Galen will be the last great physician of this time. Galen
writes numerous works. Interestingly, those who practice healing through
science and the temple priests who practice the pseudoscience of religious
healing both coexist together in the Serapeum.
Galen will be court physician under
emperor Marcus Aurelius for some time.

According to Isaac Asimov, Galen's best work is in anatomy. Dissection of
humans is viewed as bad in Rome and Galen could only dissect other species,
including dogs, goats, pigs, and monkeys. Galen is describes anatomy in
meticulous detail. Galen writes that muscles work in groups. Galen cuts the
spinal cord of many species at various levels and writes on the resulting
paralysis (loss of movement of the body part). Galen uses the three fluid
theory of Erasistratus.

Galen regards wounds as "windows into the body". Galen performed many audacious
operations that were not again used for almost two millennia, including brain
and eye surgery. To perform cataract surgery, Galen would insert a long
needle-like instrument into the eye behind the lens. He would then pull it back
slightly and remove the cataract. The slightest slip could cause permanent
blindness. Galen had set the standard for modern medicine in many different
ways.

In Rome, Galen writes extensively, lectures and publicly demonstrates his
knowledge of anatomy. Galen gains a reputation as an experienced physician and
his practice had a widespread clientèle. One of them is the consul Flavius
Boethius who introduces him to the Imperial court where Galen becomes a court
physician to Emperor Marcus Aurelius. Later he will also treat Lucius Verus,
Commodus and Septimius Severus. Reputedly, he speaks mostly Greek, which in the
field of medicine is a more highly respected language than Latin at the time.

Galen spends the rest of his life in the Imperial court, writing and
experimenting. He performs vivisections of numerous animals to study the
function of the kidneys and the spinal cord.

Galen transmitted Hippocratic medicine all the way to the Renaissance. His "On
the Elements According to Hippocrates" describes the philosopher's inaccurate
system of four bodily humours, blood, yellow bile, black bile and phlegm, which
were mystically identified with the four classical elements, and in turn with
the seasons. He created his own theories from those principles, and much of
Galen's work can be seen as building on the Hippocratic theories of the body,
rather than being new. Galen mainly ignores the Latin writings of Celsus, but
accepts the ancient works of Asclepiades.

Amongst Galen's own major works is a seventeen-volume "On the Usefulness of the
Parts of the Human Body". Like Pliny, Galen wrongly thinks that everything in
the universe is made by a God for some purpose. He also writes about philosophy
and philology (the study of words and language), as well as extensively writing
on anatomy. His collected works total twenty-two volumes, and he writes a line
a day for most of his life.

Galen's own theories, in accord with Plato's, emphasizes purposeful creation by
a single Creator ( "Nature", in Greek "phusis") - a major reason why later
Christian and Muslim scholars will be able to accept his views and will
preserve his writings. His fundamental principle of life was pneuma (air, or
breath) that later writers will connect with the erronius ancient idea of a
"soul". These writings on philosophy are a product of Galen's well rounded
education, and throughout his life Galen is keen to emphasise the philosophical
element to medicine. Galen maintained the inaccurate opinions that "Pneuma
physicon" (animal spirit) in the brain is responsible for movement, perception,
and senses, that "Pneuma zoticon" (vital spirit) in the heart controls blood
and body temperature, and that "Natural spirit" in the liver handled nutrition
and metabolism. However, he correctly rejects the Pneumatic theory that air
passes through the veins rather than blood.

Galen expands his knowledge partly by experimenting with live animals (in a way
that is clearly painful to the animal and which I vote against, although
science was advanced by such experimentation). One of his methods is to
publicly dissect a living pig, cutting its nerve bundles one at a time.
Eventually he cuts a laryngeal nerve (now also known as Galen's Nerve) and the
pig stops squealing. He also ties the ureters of living animals, swelling the
kidneys, therefore showing that urine comes from the kidneys, and severes
spinal cords to demonstrate paralysis. In addition to working with pigs, Galen
also experiments with barbary apes and goats, but emphasizes that he practises
on pigs due to the fact that, in some respects, they are anatomically similar
to humans. Public dissections are also a highly valuable way of disputing and
disproving the biological theories of others, and are one of the main methods
of academic medical learning in Rome. It is quite common for large numbers of
medical students to attend these public gatherings, which will sometimes turn
into debates where learning is increased.

Galen's books will be the standard book of healing through science until
Vesalius.
It is very possible that Galen excelled in part from use of the Pergamum public
library, a library second only to that of Alexandria.{check in Galen writings}
Galen,
through his works, will transmit the Greek knowledge of healing into the
future.
  
1,838 YBN
[162 AD]
1089) Galen (Greek: Γαληνός) (c.130 CE
Pergamum {now Bergama, Turkey} - c.200 CE probably Sicily), moves to Rome.

Pergamum, Turkey  
1,827 YBN
[03/31/173 AD]
974)
  
1,823 YBN
[177 AD]
1030) According to Origen, Celsus was the author of an anti-Christian work
titled The True Word. This work is lost, but we have Origen's account of it in
his writings.

Celsus, as a Platonist philosopher, argues for monotheism against what he sees
as the Christians' dualism (of Deity and Devil) writing "If one accepts that
all of nature, and everything in the universe, operates according to the will
of God, and that nothing works contrary to his purposes, then one must also
accept that the angels and daimones, hereos - all things in the universe - are
subject to the will of the one God who rules over all." According to Elaine
Pagels, many Pagans in this time tend toward monotheism, however believe in a
unity of all the gods and daimones in one divine source. Celsus writes that the
Christians deviate from monotheism in their "blasphemous" belief in the devil.
Of all the "impious errors" the Christians make, Christians show their greatest
ignorance in "making up a being opposed to God, and calling him 'devil,' or, in
the Hebrew language, 'Satan."' According to Celsus, all such ideas are nothing
but human inventions, and that "it is blasphemy...to say that the greatest
God...has an adversary who constrains his capacity to do good." Celsus
expresses anger that the Christians who claim to worship one God, "impiously
divide the kingdom of God, creating a rebellion in it, as if there were
opposing factions within the divine, including on e that is hostile to God!"
Celsus accuses Christians of "inventing a rebellion" in heaven to justify
rebellion here on earth. The concept of a devil or "Satan" originated in the
500s BCE in Hebrew writings. The earliest known reference to a Satan appears
in the Hebrew Bible in the book of Numbers and in Job as one of God's obedient
servants, a messenger, or angel that obstructs human activity.



Celsus writes his only work of record "True Discourse" (or, "True Reason")
against Christianity in approximately 178 CE. Celsus divides the work into two
sections, the first in which objections are explained from a fictional Jewish
person and the other in which Celsus speaks as the Pagan philosopher that he
is. Celsus ridicules Christians because they advocate blind faith instead of
reason. Around 60 years after it is first published, the book written by Celsus
will inspire a rebuttle written by Origen titled "Contra Celsum", which is the
only source for Celsus' book, who will be later condemned along with other
critics of Christianity such as Porphyry.
  
1,820 YBN
[03/31/180 AD]
975)
  
1,800 YBN
[200 AD]
976)
  
1,800 YBN
[200 AD]
979)
  
1,800 YBN
[200 AD]
1073) Earliest "press-on" printing. Chinese people put ink to Buddhist text
inscribed on marble pillars and apply damp paper to the inscriptions to make a
copy of the text onto the paper. Also around this time, religious seals are
used to transfer pictures and texts of prayers to paper using ink. Ink of a
good consistency for printing is developed in the 300s or 400s, and around the
500s use of a wood block for printing will appear. Movable type will not be
invented until around the years 1041-48.
China  
1,800 YBN
[200 AD]
1093) The Coptic language is invented. Coptic is the Egyptian language, written
with in alphabet almost identical to the Greek alphabet, and will be a valuable
resource in translating the Egyptian language for later scholars because
Egyptian written with hieroglyphs, hieratic and demotic symbols contain no
vowels, but in Coptic vowels are included. Coptic will be the last script used
for the Egyptian language.

Egypt  
1,798 YBN
[202 AD]
1027)
  
1,797 YBN
[03/07/203 AD]
977)
  
1,797 YBN
[03/07/203 AD]
978)
  
1,785 YBN
[215 AD]
980)
  
1,768 YBN
[232 AD]
981)
  
1,755 YBN
[245 AD]
982)
  
1,750 YBN
[250 AD]
1091) 1/6x+1/12x+1/7x+5+x/2+4=x
.1667x+0.083x+.1429x+.5x+9=x
.8926x+9=x x=84
So he grows a beard at 21, gets married at 33, has a son at 38 who
lives for 42 years, and dies 4 years before Diofantos dies at age 84.
  
1,738 YBN
[262 AD]
1031) (reduce and check is exact from wiki)

Porphyry (c.232-c. 304 AD) was a Neoplatonist philosopher. He was born Malchus
("king") in Tyre, but his teacher in Athens, Cassius Longinus, gave him the
name Porphyrius (clad in purple), a punning allusion to the color of the
imperial robes. Under Longinus he studied grammar and rhetoric. In 262 he went
to Rome, attracted by the reputation of Plotinus, and for six years devoted
himself to the study of Neoplatonism. Having injured his health by overwork, he
went to live in Sicily for five years. On his return to Rome, he lectured on
philosophy and completed an edition of the writings of Plotinus (who had died
in the meantime) to gether with a biogrpahy of his teacher. Iamblichus is
mentioned in ancient Neoplatonic writings as his pupis, but this most likely
means only that he was the dominant figure in the next generation of
philosophers. The two men differed publicly on the issue of theurgy. In his
later years, he married Marcella, a widow with seven children and an
enthusiastic student of philosophy. Little more is known of his life, and the
date of his death is uncertain.

Porphyry is best known for his contributions to philosophy. Apart from writing
the Aids to the Study of the Intelligibles, a basic summary of Neoplatonism, he
is especially appreciated for his Introduction to Categories (Introductio in
Praedicamenta), a commentary on Aristotle's Categories. The Introduction
describes how qualities attributed to things may be classified, breaking down
the philosophical concept of substance as a relationship genus/species.

As Porphyry's most influential contribution to philosophy, the Introduction to
Categories incorporated Aristotle's logic into Neoplatonism, in particular the
doctrine of the categories interpreted in terms of entities (in later
philosophy, "universal"). Boethius' Isagoge, a Latin translation of the
Introduction, became a standard medieval textbook in the schools and
universities which set the stage for medieval philosophical-theological
developments of logic and the problem of universals. In medieval textbooks, the
all-important Arbor porphyriana ("Porphyrian Tree") illustrates his logical
classification of substance. To this day, taxonomists benefit from Porphyry's
Tree in classifying everything from plants to animals to insects to whales.

Porphyry is also known as a violent opponent of Christianity and defender of
Paganism; of his Adversus Christianos (Against the Christians) in 15 books,
only fragments remain. He famously said, "The Gods have proclaimed Christ to
have been most pious, but the Christians are a confused and vicious sect."
Counter-treatises were written by Eusebius of Caesarea, Apollinarius (or
Apollinaris) of Laodicea, Methodius of Olympus, and Macarius of Magnesia, but
all these are lost. Porphyry's identification of the Book of Daniel as the work
of a writer in the time of Antiochus Epiphanes, is given by Jerome. There is no
proof of the assertion of Socrates, the ecclesiastical historian, and
Augustine, that Porphyry was once a Christian.

Porphyry was also opposed to the theurgy of his disciple Iamblichus. Much of
Iamblichus' mysteries is dedicated to the defense of mystic theurgic divine
possession against the critiques of Porphyry.

Porphyry was, like Pythagoras, known as an advocate of vegetarianism on
spiritual or ethical grounds. These two philosophers are perhaps the most
famous vegetarians of classical antiquity. He wrote the De Abstinentia (On
Abstinence) and also a De Non Necandis ad Epulandum Animantibus (roughly On the
Impropriety of Killing Living Beings for Food) in support of abstinence from
animal flesh, and is cited with approval in vegetarian literature up to the
present day.

Porphyry also wrote widely on astrology, religion, philosophy, and musical
theory; and produced a biography of his teacher, Plotinus. Another book of his
on the life of Pythagoras, named Vita Pythagorae or Life of Pythagoras, is not
to be confused with the book of the same name by Iamblichus.


In "On Abstinence from Animal Food", Porfurios advocates rights for the other
species, saying "he who forbids men to feed on animals, and thinks it is
unjust, will also say that it is not just to kill them, and deprive them of
life". In this work, Porfurios also argues against sacrificing animals,
writing: "Pythagoreans themselves did not spare animals when they sacrificed to
the gods. ... I intend to oppose these opinions, and those of the multitude".
  
1,735 YBN
[265 AD]
983)
  
1,733 YBN
[267 AD]
984)
  
1,728 YBN
[272 AD]
985) After the occupation of Alexandria by Zenobia, Queen of Palmyra, Emperor
Aurelian attacks in the royal quarter result in so much destruction that
members of the Mouseion either flee the country or take refuge in the
Serapeum.
Ammianus Marcellinus records: "But Alexandria itself was extended, not
gradually, like other cities, but at its very beginning, to great dimensions,
and for a long time was exhausted with internal disputes, until finally, after
many years, when Aurelian was emperor, the civic quarrels escalated into deadly
strife. Its walls were torn down and it lost the greater part of the area which
was called the Brucheion, and which had long been the dwelling place of its
most distinguished men."
Possibly scrolls are transfered to the Serapeum, Kaisareion
or Claudianum annexes.
Epiphanius will write about the Brucheion a few years after
Ammianus, that where the library had once been, "there is now a desert"
(Patrologia Graeca, 43, 252)
  
1,716 YBN
[284 AD]
988)
  
1,710 YBN
[290 AD]
1092)
Panopolis {now Akhmim}, Egypt  
1,703 YBN
[297 AD]
986)
  
1,697 YBN
[303 AD]
987)
  
1,695 YBN
[12/27/305 AD]
1108) Eusebius of Caesarea (c.275 - May 30, 339) (often called Eusebius
Pamphili, "Eusebius {the friend} of Pamphilus") was a bishop of Caesarea in
Palestine and is often referred to as the father of church history because of
his work in recording the history of the early Christian church. An earlier
history by Hegesippus that he referred to has not survived.

The two greatest historical works of Eusebius are his Chronicle and his Church
History. The former (Greek, Pantodape historia, "Universal History") is divided
into two parts. The first part (Greek, Chronographia, "Annals") purports to
give an epitome of universal history from the sources, arranged according to
nations. The second part (Greek, Chronikoi kanones, "Chronological Canons")
attempts to furnish a synchronism of the historical material in parallel
columns, the equivalent of a parallel timeline.

In his Church History or Ecclesiastical History (Historia Ecclesiastica),
Eusebius attempted according to his own declaration (I.i.1) to present the
history of the Church from the apostles to his own time, with special regard to
the following points:
(1) the successions of bishops in the principal sees;
(2) the
history of Christian teachers;
(3) the history of heresies;
(4) the history of the Jews;
(5)
the relations to the heathen;
(6) the martyrdoms.
He grouped his material according to the
reigns of the emperors, presenting it as he found it in his sources. The
contents are as follows:
* Book i: detailed introduction on Jesus Christ
* Book ii: The
history of the apostolic time to the destruction of Jerusalem by Titus
* Book
iii: The following time to Trajan
* Books iv and v: the second century
* Book vi: The
time from Septimius Severus to Decius
* Book vii: extends to the outbreak of the
persecution under Diocletian
* Book viii: more of this persecution
* Book ix: history to
Constantine's victory over Maxentius in the West and over Maximinus in the
East
* Book x: The reëstablishment of the churches and the rebellion and
conquest of Licinius.

Eusebius wrote other minor historical works, a "Life of Constantine" (Vita
Constantini) which is a eulogy.

To the class of apologetic and dogmatic works belong:
(1) the Apology for Origen,
the first five books of which, according to the definite statement of Photius,
were written by Pamphilus in prison, with the assistance of Eusebius. Eusebius
added the sixth book after the death of Pamphilus. We possess only a Latin
translation of the first book, made by Rufinus;
(2) a treatise against Hierocles (a
Roman governor and Neoplatonic philosopher), in which Eusebius combated the
former's glorification of Apollonius of Tyana in a work entitled "A
Truth-loving Discourse" (Greek, Philalethes logos);
(3) Praeparatio evangelica
('Preparation for the Gospel'), commonly known by its Latin title, which
attempts to prove the excellence of Christianity over every pagan religion and
philosophy. The Praeparatio consists of fifteen books which have been
completely preserved. Eusebius considered it an introduction to Christianity
for pagans. But its value for many later readers is more because Eusebius
studded this work with so many fascinating and lively fragments from historians
and philosophers which are nowhere else preserved. Here alone is preserved a
summary of the writings of the Phoenician priest Sanchuniathon of which the
accuracy has been shown by the mythological accounts found on the Ugaritic
tables, here alone is the account from Diodorus Siculus's sixth book of
Euhemerus' wondrous voyage to the island of Panchaea where Euhemerus purports
to have found his true history of the gods, and here almost alone is preserved
writings of the neo-Platonist philosopher Atticus along with so much else.
(4)
Demonstratio evangelica ('Proof of the Gospel') is closely connected to the
Praeparatio and comprised originally twenty books of which ten have been
completely preserved as well as a fragment of the fifteenth. Here Eusebius
treats of the person of Jesus Christ. The work was probably finished before
311;
(5) another work which originated in the time of the persecution, entitled
"Prophetic Extracts" (Eklogai prophetikai). It discusses in four books the
Messianic texts of Scripture. The work is merely the surviving portion (books
6-9) of the General elementary introduction to the Christian faith, now lost.
(6)
the treatise "On Divine Manifestation" (Peri theophaneias), dating from a much
later time. It treats of the incarnation of the Divine Logos, and its contents
are in many cases identical with the Demonstratio evangelica. Only fragments
are preserved;
(7) the polemical treatise "Against Marcellus," dating from about 337;

(8) a supplement to the last-named work, entitled "On the Theology of the
Church," in which he defended the Nicene doctrine of the Logos against the
party of Athanasius.
A number of writings, belonging in this category, have been entirely
lost.

A more comprehensive work of an exegetical nature, preserved only in fragments,
is entitled "On the Differences of the Gospels" and was written for the purpose
of harmonizing the contradictions in the reports of the different Evangelists.

Eusebius follows closely in the footsteps of Origen. No point of this doctrine
is original with Eusebius, all is traceable to his teacher Origen.


Eusebius echos the racist anti-Jewish views associated with the early Christian
people. Eusebius mystically blames the calamities which befell the Jewish
nation on the Jewish people's role in the death of Jesus:
"that from that time
seditions and wars and mischievous plots followed each other in quick
succession, and never ceased in the city and in all Judea until finally the
siege of Vespasian overwhelmed them. Thus the divine vengeance overtook the
Jews for the crimes which they dared to commit against Christ." (Hist. Eccles.
II.6: The Misfortunes which overwhelmed the Jews after their Presumption
against Christ)
  
1,695 YBN
[305 AD]
989)
  
1,685 YBN
[315 AD]
1004)
  
1,681 YBN
[319 AD]
946)
  
1,680 YBN
[320 AD]
1094) In geometry, there are several theorems that are known by the generic
name Pappus's Theorem, attributing them to Pappus of Alexandria. They include:
*
Pappus's centroid theorem,
* the Pappus chain,
* Pappus's harmonic theorem, and
*
Pappus's hexagon theorem

In his "Synogogue", Pappus gives no indication of the date of the authors whose
treatises he makes use of, or of the time at which he himself writes. If we had
no other information than can be derived from his work, we should only know
that he was later than Claudius Ptolemy (c90-c168) whom he often quotes. Suidas
states that he was of the same age as Theon of Alexandria, (father of Hypatia)
who will write commentaries on Ptolemy's great work, the "Syntaxis
mathematica", and will flourish in the reign of Theodosius I (A.D. 372-395).
Suidas says also that Pappus wrote a commentary upon the same work of Ptolemy.
But it seems unbelievable that two contemporaries should have at the same time
and in the same style composed commentaries upon one and the same work, and yet
neither should have been mentioned by the other, whether as friend or opponent.
It is more probable that Pappus's commentary was written long before Theon's,
and is largely included into the work by Theon, and that Suidas, through
failure to disconnect the two commentaries, assigned a like date to both. There
is a chronological table by Theon of Alexandria which, when being copied (in a
10th-century manuscript), has had inserted next to the name of Diocletian (who
ruled 284 CE-305 CE) "at that time wrote Pappus". Similar insertions give the
dates for Ptolemy, Hipparchus and other mathematical astronomers. Rome shows
that it can be deduced from Pappus's commentary on the Almagest that Pappos
observes the eclipse of the sun in Alexandria which takes place on 18 October
320. This fixes clearly the date of 320 for Pappus's commentary on Ptolemy's
Almagest.

Pappos is born and appears to have lived in Alexandria all his life. He
dedicates works to Hermodorus, Pandrosion and Megethion but other than knowing
that Hermodorus is Pappus's son, nothing is known about these other men. Pappus
refers to a friend who is also a philosopher, named Hierius, who encourages
Pappus to study certain mathematical problems. A reference to Pappos in
Proclus's writings says that he headed a school in Alexandria.
Alexandria, Egypt  
1,679 YBN
[321 AD]
4060)
Constantanople  
1,675 YBN
[07/??/325 AD]
947)
  
1,669 YBN
[331 AD]
1375)
Constantanople  
1,660 YBN
[340 AD]
990)
  
1,660 YBN
[340 AD]
991)
  
1,643 YBN
[357 AD]
995)
  
1,638 YBN
[362 AD]
1032)
  
1,637 YBN
[06/26/363 AD]
1044)
  
1,637 YBN
[363 AD]
1010)
  
1,636 YBN
[364 AD]
993)
  
1,636 YBN
[364 AD]
996)
  
1,634 YBN
[366 AD]
1100)
Alexandria, Egypt  
1,630 YBN
[370 AD]
1376)
Cappadocia  
1,626 YBN
[374 AD]
5863) (Saint) Ambrose (CE 339-397), Bishop of Milan, attempts to codify the
growing repertory of chants. This body of Milanese church music, therefore,
comes to be called "Ambrosian chant".

Ambrose also composes hymns, notably "Aeterne rerum Conditor" ("Framer of the
earth and sky") and "Deus Creator omnium" ("Maker of all things, God most
high").
As an example of the early anti-Jewish views of the followers of Jesus (who
ironically was Jewish if he existed at all), in 388 Ambrose criticizes the
emperor Theodosius for having punished a bishop who had burnt a Jewish
synagogue.
Milan, Italy  
1,625 YBN
[375 AD]
992)
  
1,625 YBN
[375 AD]
994)
  
1,620 YBN
[380 AD]
999)
  
1,614 YBN
[386 AD]
997)
  
1,613 YBN
[387 AD]
874) The illogical and racist anti-Jewish anger felt by many early Christian
fathers is shown clearly in the writing of "Saint" John Chrysostom (Greek
Ιωάννης ο
Χρυσόστομος) (347-407),
bishop of Constantinople, who writes "The Jews sacrifice their children to
Satan"

Constantinople,   
1,611 YBN
[389 AD]
1001)
  
1,610 YBN
[390 AD]
1000) By now a circle of friends and students around Hypatia is firmly
established.

  
1,609 YBN
[391 AD]
1002)
  
1,609 YBN
[391 AD]
1003) Library in Alexandria (The Serapeion) destroyed.

The library in the Temple to Serapis (the Serapeion) in Alexandria is violently
destroyed by Christian people and the temple is converted to a Christian
church.

Historian Socrates Scholasticus writes 'At the request of Theophilus, Bishop of
Alexandria, the Emperor issued an order at this time for the demolition of the
heathen temples in that city...' and that 'Theophilus threw down the temple of
Serapis ...The temples were overthrown, and the bronze statues melted down to
make domestic vessels.'. Historian Eunapius (Ευνάπιος) (CE 346-c414)
wrote that 'they wrought havoc with the Serapeum and made war on its
statues....The foundations alone were not removed owing to the difficulty in
moving such huge blocks of stone.' Historian Theodoret, writes, 'The
sanctuaries of the idols were uprooted from their foundations.' Historian
Sozomen (c400-c450) describes the Christians as having uninterruptedly occupied
the Serapeum from its capture by Theophilus to his own time. Historian Rufinus
(who dies in 410 CE) writes that the exterior range of buildings round the edge
of the plateau are practically uninjured, though void of its former pagan
occupiers, but that the great temple of Serapis and the colonnades around it
are levelled to the ground.". Much of the Serapeum lasts as late as the 12th
century.
Alexandria, Egypt  
1,606 YBN
[08/24/394 AD]
1095)
island of Philae, near Aswan  
1,600 YBN
[400 AD]
1005)
  
1,600 YBN
[400 AD]
1072)
Vishnupadagiri, India  
1,600 YBN
[400 AD]
1118)
Bakhshali, Pakistan  
1,600 YBN
[400 AD]
1329)
Mesoamerica  
1,598 YBN
[402 AD]
998) Last known contemporarily written reference to the Mouseion in Alexandria.
Synesios (Synesius) (c370-413 CE), who studies under Hypatia, describes the
pictures of philosophers in the Mouseion. There is no later reference to the
Mouseion's existence in the fifth century.

This is in Chapter 6 of "A Eulogy of Baldness", Synesios writes: "You may look
at the pictures in the Museum, I mean those of Diogenes and Socrates, and
whomever you please of those who in their age were wise, and your survey would
be an inspection of bald heads." This is evidence that the Mouseion survived
intact after the destruction of the Sarapeion in 391. Since Synesios is thought
to have died around 414, and there are no other references after Synesios, it
is possible that the Mouseion was destroyed a short time before or after the
murder of Hypatia.
  
1,588 YBN
[10/15/412 AD]
1006)
  
1,588 YBN
[10/17/412 AD]
1007)
  
1,588 YBN
[412 AD]
1008)
  
1,585 YBN
[03/??/415 AD]
1009) Hypatia (Greek: Υπατία and Ὑπατίας) (c360 - 415), a popular
female philosopher, mathematician and astronomer in Alexandria is murdered by
Christian people.
Many people cite this as the end of ancient science. Clearly, the
seed of science survived, as science grows now, in the time we live in.

Socrates of Scholasticus, a Christian historian alive at the time of the murder
of Hypatia writes (translated from Greek):
"Of Hypatia the Female Philosopher.
There was a woman at
Alexandria named Hypatia, daughter of the philosopher Theon, who made such
attainments in literature and science, as to far surpass all the philosophers
of her own time. Having succeeded to the school of Plato and Plotinus, she
explained the principles of philosophy to her auditors, many of whom came from
a distance to receive her instructions. On account of the self-possession and
ease of manner, which she had acquired in consequence of the cultivation of her
mind, she not unfrequently appeared in public in presence of the magistrates.
Neither did she feel ashamed in coming to an assembly of men. For all men on
account of her extraordinary dignity and virtue admired her the more. Yet even
she fell a victim to the political jealousy which at that time prevailed. For
as she had frequent interviews with Orestes (the Roman Prefect or Governor of
Egypt at the time ), it was slanderously reported among the Christian populace,
that it was she who prevented Orestes from being reconciled to the Bishop. Some
of them therefore, hurried away by a fierce and bigoted zeal, whose ringleader
was a reader named Peter, waylaid her returning home, and dragging her from her
carriage, they took her to the church called Caesareum, where they completely
stripped her, and then murdered her with tiles {the words are
οστράκοις ανείλον, oyster shells, but this word was applied to
brick ceiling tiles}. After tearing her body in pieces, they took her mangled
limbs to a place called Cinaron, and there burnt them. This affair brought
disgrace not only upon Cyril, but also upon the whole Alexandrian church. And
surely nothing can be farther from the spirit of Christianity than the
allowance of massacres, fights, and transactions of that sort. This happened in
the month of March during Lent, in the fourth year of Cyril's episcopate, under
the tenth consulate of Honorius, and the sixth of Theodosius."
(steps of a church called The Caesarium ) Alexandria, Egypt  
1,584 YBN
[416 AD]
1011) Museum in Alexandria closed.

Paulus Orosius describes the temples in Alexandria as having empty bookshelves,
the contents emptied "by men of our time". Adding this together with the Suda
reference to Theon being a member, and the last reference to the Mouseion from
Synesios in 409 with no mention of any destruction before his death in 414, and
no mention of any public library in Alexandria by people writing in the 5th and
6th century, it appears probable that the Mouseion (including any remaining
library) may have been completely and permanently destroyed by 415 or 416.
  
1,577 YBN
[423 AD]
1012)
  
1,569 YBN
[431 AD]
1139) The Council of Ephesus sentences Porfurios' (and other) books against
Christianity to be burned (but does not mention the emperor Julian's
anti-christian writings).

This is the first of 3 major book burnings that will remove any and all
writings that criticize the Christian religion. The result will be very
effective, leaving the only surviving works so far found to be rebuttles of
these works by Christian writers.
Ephesus, (Asia Minor, modern:) Turkey  
1,561 YBN
[439 AD]
1013)
  
1,552 YBN
[448 AD]
1043) Theodosius II (April, 401 - July 28, 450), Eastern Roman Emperor
(408-450) orders all non-Christian books burned. In fighting the ancient
Hellenic tradition, or "Paganism" as it would be later called, the Christian
people destroy much of the science learned and recorded in books stored in
temples to the traditional Greek Gods.

No remains have ever been found from the books critical of the Christian
religion written by Kelsos, Porfurios and others, although some of these
writings are preserved in rebuttles by Christian writers that have survived.
With this law, the anti-Christian writings of Porfurios will be condemned but
those of Julian are ignored.
  
1,550 YBN
[450 AD]
1096) Proclus is born 410 or 411 CE (his birth year is deduced from a horoscope
cast by a disciple, Marinus, and hence is to a degree uncertain) in
Constantinople to a family of high social status in Lycia- his father Particius
is a high legal official, very important in the Byzantine Empire's court
system- and raised in Xanthus, he studies rhetoric, philosophy and mathematics
in Alexandria, Egypt, with the intent of pursuing a judicial position like his
father. Proklos comes back to Constantinople part-way through his studies when
his rector, his principal instructor (one Leonas) has business there, and is a
successful praticing lawyer for a period.

Actually experiencing the practice of law makes Proclus realize that he truly
prefers philosophy, so he returns to Alexandria, and begins studying the works
of Aristotle under Olympiodorus the Elder (he also began studying mathematics
during this period as well with a teacher named Heron {not Hero of
Alexandria}). Eventually, this gifted student became dissatisfied with the
level of philosophical instruction available in Alexandria, and went to Athens,
the preeminent philosophical center of the day, in 431 to study at the
Neoplatonic successor of the famous Academy founded 800 years before by Plato
(in 387 BCE); there he is taught by Plutarch of Athens and Syrianus; he
succeeds Plutarch as head of the Academy, and is in turn succeeded on his death
by Syrianus. He dies around aged 73, and is buried near Mount Lycabettus in a
tomb.

He lives in Athens as an unmarried vegetarian bachelor, prosperous and generous
to his friends, until the end of his life, except for a voluntary one year
exile, which is designed to lessen the pressure put on him by his
political-philosophical activity, little appreciated by the Christian rulers;
he spends the exile travelling and being initiated into various mystery cults
as befitted his universalist approach to religion, trying to become "a priest
of the entire universe."

In addition to his commentaries, Proclus writes two major systematic works.
"The Elements of Theology" is a singular work in the history of ancient
philosophy. It consists of 211 propositions, each followed by a proof,
beginning from the existence of the One (the first principle of all things) and
ending with the descent of individual souls into the material world. The
Platonic Theology is a systematisation of material from Platonic dialogues,
showing from them the characteristics of the divine orders, the part of the
universe which is closest to the One.
Three small works have also survived, only in
Latin translation: "Ten doubts concerning providence"; "On providence and
fate"; and "On the existence of evils".

He also wrote a number of minor works.

Just as a brief summary of Proklos' views, and Neoplatonism, which is very
abstract and have no relation to actual science but simply for context:
There are three
basic concepts in Neoplatonism:
1) "The One" (to Hen) is the first principle in Neoplatonism.
It is the principle which produces all Being. This idea of "The One" is
compared by many to be similar to the idea of a God, and may be related to the
popularity of the monotheism of Christianity.
2) "Intellect" (Nous), is the principle which
is produced below the level of the One.
3) "Soul" (Psuche) is produced by Intellect,
and so is the third principle in the Neoplatonic system. It is a mind, like
Intellect, but it does not grasp all of its own content as once.

By far the greatest transmission of Procline ideas will be through the
Pseudo-Dionysius. This 5th century Christian Greek author wrote under the
pseudonym Dionysius the Areopagite, the figure converted (from Paganism) by St.
Paul in Athens. Because of this fiction, his writings were taken to have almost
apostolic authority. He is an original thinker, and Christian rather than
Pagan, but in his writings can be found a great number of Procline metaphysical
principles. Another important source for Procline influence on the Middle Ages
is Boethius' Consolation of Philosophy, which has a number of Proclus
principles and motifs.
Athens, Greece  
1,524 YBN
[09/04/476 AD]
1098)
Rome, Italy  
1,520 YBN
[480 AD]
1113) Isidore of Alexandria is a Greek philosopher and one of the last of the
Neoplatonists. He lives in Athens and Alexandria toward the end of the 5th
century CE. Isidore becomes head of the school in Athens in succession to
Marinus, who followed Proclus. Isidore is known mainly for teaching Damaskios
the last head of the Academy.
Athens, Greece  
1,511 YBN
[489 AD]
1384)
Gundishapur, Khuzestan (southwest of Iran, not far from the Karun river.)  
1,501 YBN
[499 AD]
1309) Aryabhata (Devanāgarī: आर्यभट) (CE 476-550), Indian
astronomer and mathematician, writes in his "Aryabhatiya" (c499), that the
apparent westward motion of the stars is due to the spherical Earth’s
rotation about its axis. Aryabhata also correctly explains the luminosity of
the Moon and planets to reflected sunlight.

In the 600s the astronomer Brahmagupta will severely criticize the view of
Aryabhata I that the Earth is a spinning sphere, a view that will widely
disseminated by Brahmagupta’s contemporary and rival Bhaskara I.
Kusumapura (modern Patna), India  
1,500 YBN
[500 AD]
1101)
Scandinavia  
1,500 YBN
[500 AD]
1102)
China  
1,500 YBN
[500 AD]
1105)
Rome  
1,480 YBN
[01/01/520 AD]
1099) Boethius' birth date is unknown, generally placed around 480 CE, the same
year of birth as St. Benedict. Boethius was born to a patrician family which
had been Christian for about a century. His father's line included two popes
and both parents count Roman emperors among their ancestors.

Boethius was born in Rome to an ancient and important family which included the
emperor Olybrius and many consuls. His father Fl. Manlius Boethius held that
position in 487 after Odoacer deposed the last Western Roman Emperor. Boethius
holds the same position in 510 in the kingdom of the Ostrogoths.

It is unknown where Boethius received his formidable education in Greek.
Boethius may have studied in Athens, and perhaps Alexandria. Since a Boethius
is recorded as proctor of the school in Alexandria circa AD 470, perhaps the
younger Boethius received some grounding in the classics from his father or a
close relative. In any case, his accomplishment in Greek, though traditional
for his class, was remarkable given the reduced knowledge which accompanies the
end of the empire in this time.
As a result of his increasingly rare education and
experience, Boethius enters the service of Theodoric the Great, who commissions
the young Boethius to perform many roles.
Italy  
1,472 YBN
[528 AD]
1377)
Constantanople  
1,471 YBN
[529 AD]
1014) Roman Emperor Justinian (CE 483-565) closes the schools of Alexandria and
Athens (including Plato's Academy).

The head of the Academy, Damascus and 6 other philosophers seek asylum in
Persia.

Justinian also decrees that all anti-Christian books are to be burned in this
year {exact date}. None of the 'True Doctrine" of Kelsos in the second century,
the 15 books of Porfurios' "Against the Christians" in the third century, and
Julian's "Against the Galileans" of the fourth century have ever been found,
however some of their writing remains in rebuttles by Christian writers, for
example Origen's "Against Kelsos" quotes Kelsos, Macarius Magnes may possibly
preserve some of Porfurios' writing for which even 3 major Christian rebuttles
have never been found, and Kurillos (Cyril) of Alexandria's "Pro Christiana
Religione" reveals some of Julian's writings.
Athens, Greece (and Alexandria,Egypt)  
1,471 YBN
[529 AD]
1378) As often happens with early Christian institutions, the monastery iwas
constructed on top of an older pagan site, a temple of Apollo that crowned the
hill, enclosed by a fortifying wall above the small town of Cassino, still
largely pagan at the time and recently devastated by the Goths. Benedict's
first act is to smash the sculpture of Apollo and destroy the altar. Benedict
rededicats the site to John the Baptist.
Monte Cassino, Italy  
1,471 YBN
[529 AD]
1423)
Byzantium  
1,470 YBN
[530 AD]
1426)
Alexandria, Egypt  
1,467 YBN
[533 AD]
1015)
  
1,463 YBN
[12/27/537 AD]
1106) Nothing remains of the first church that was built on the same site
during the 300s. Following the destruction of the first church, a second was
built by Constantius, the son of Constantine the Great, but was burned down
during the Nika riots of 532, before being rebuilt by Justinian.

Hagia Sophia is one of the greatest surviving examples of Byzantine
architecture. Of great artistic value is its decorated interior with mosaics
and marble pillars and coverings. The temple itself is so richly and
artistically decorated that Justinian proclaimed "Solomon, I have surpassed
thee!" (Νενίκηκά σε
Σολομών). Justinian himself oversees the
completion of the greatest cathedral ever built up to that time, and it will
remain the largest cathedral for 1,000 years until the completion of the
cathedral in Seville.

The name comes from the Greek name Αγία
Σοφία, a contraction of Ναός
της Αγίας του
Θεού Σοφίας (Church of the
Holy Wisdom of God).

The Eastern Orthodox church will be converted to a mosque in 1453, and then
converted into a museum in 1935, the Ayasofya Museum, in Istanbul, Turkey.
Constantinople  
1,460 YBN
[540 AD]
1107) The writings of Procopius are the primary source of information for the
rule of the emperor Justinian. Procopius was the author of a history in eight
books of the wars fought by Justinian I, a panegyric (a formal public speech
delivered in high praise of a person or thing) on Justinian's public works
throughout the empire, and a book known as the Secret History (Greek: Anekdota)
that claims to report the scandals that Procopius could not include in his
published history.

The first seven books of his History of Justinian's Wars, which were published
as a unit, seem to have been largely completed by 545.

The Secret History will be discovered centuries later in the Vatican Library
and published in 1623, but its existence is already known from the Suda, which
refers to it as the Anekdota ("the unpublished composition"). The Secret
History covers the same years as the seven books of the History of Justinian's
Wars and appears to have been written after they were published. Current
consensus generally dates it to 550, or maybe as late as 562.

The De Aedificiis tells us nothing further about Belisarius but it takes a
sharply different attitude towards Justinian. He is presented as an idealised
Christian emperor who built churches for the glory of God and defenses for the
safety of his subjects and who showed particular concern for the water supply.
Theodora, who was dead when this panegyric was written, is mentioned only
briefly but Procopius' praise of her beauty is fulsome. The panegyric is likely
written at Justinian's request, however, and so it is doubtful if its
sentiments are sincere.

Procopius belongs to the school of late antique secular historians who continue
the traditions of the Second Sophistic; they write in Attic Greek, their models
are Herodotus and especially Thucydides, and their subject matter is secular
history. They avoid vocabulary unknown to Attic Greek and insert an explanation
when they have to use contemporary words. Thus Procopius explains to his
readers that ekklesia, meaning a Christian church, is the equivalent of a
temple or shrine and that monks are "the most temperate of Christians...whom
men are accustomed to call monks." (Wars 2.9.14; 1.7.22) In classical Athens,
monks were unknown and an ekklesia was the assembly of Athenian citizens which
passed the laws.

The secular historians dismiss the history of the Christian church, which they
leave to ecclesiastical history-a genre that was founded by Eusebius of
Caesarea. However, Averil Cameron has argued convincingly that Procopius' works
reflect the tensions between the classical and Christian models of history in
6th century Byzantium. Procopius indicates (Secret History 26.18) that he plans
to write an ecclesiastical history himself and, if he had, he would probably
have followed the rules of that genre. But, as far as we know, the
ecclesiastical history remained unwritten.
Constantinople  
1,458 YBN
[542 AD]
1381)
Lyon, France  
1,411 YBN
[589 AD]
1328)
China  
1,400 YBN
[600 AD]
1110) Viking ships use a keel and a mast for a sail.
In this sense a keel refers to a
fin that projects from the bottom of a ship that helps to keep the ship
balanced (Confusingly the word "keel" may also refer to a structural beam that
serves as the foundation of a ship).

  
1,400 YBN
[600 AD]
1111) Earliest known windmill. This windmill uses a vertical shaft and
horizontal sails to grind grain.
Persia (Iran)  
1,400 YBN
[600 AD]
5864) Charlemagne, king of the Franks (CE 768–814), will impose Gregorian
chant on his kingdom, where another liturgical tradition—the Gallican
chant—is in common use. During the 700s and 800s, a process of assimilation
takes place between Gallican and Gregorian chants; and the chant in this
evolved form is the what has reached us in present times.
Rome, Italy  
1,396 YBN
[604 AD]
1104)
Korea  
1,387 YBN
[613 AD]
1391)
Mecca, Arabia (modern Saudi Arabia)  
1,367 YBN
[633 AD]
1114) Isidore was born in Cartagena, Spain, to Severianus and Theodora, part of
an influential family who were instrumental in the political-religious
maneuvering that converted the Visigothic kings from Arianism to Catholicism.
Isidore receives his elementary education in the Cathedral school of Seville.
In this institution, which was the first of its kind in Spain, the trivium (a
theory of education which teaches the three subjects grammar, logic, and
rhetoric) and quadrivium (a secondary more advanced education of the four
subjects: arithmetic, geometry, music, and astronomy) were taught by a body of
learned men, among whom was the archbishop, Leander. Isidore applies himself
with such diligence that he learns Latin, Greek and Hebrew in a short time.
Shockingly the quadrivium is considered preparatory work for the serious study
of philosophy and theology, which are highly abstract and largely fraudulent in
my opinion.

Whether Isidore ever embraced monastic life or not is not known, but though he
may never have been affiliated with any of the religious orders, he esteems
them highly, on his elevation to the episcopate (to bishop) he immediately
constitutes himself protector of the monks and in 619 he pronounces anathema
(denouncement and excommunication) against any ecclesiastic who should in any
way disturb the monasteries.

On the death of Leander, Isidore succeeded to the See (the jurisdiction of a
bishop) of Seville.

His long incumbency in this office is spent in a period of disintegration and
transition. The ancient institutions and classic learning of the Roman Empire
are fast disappearing. In Spain a new civilization is beginning to evolve
itself from the blending racial elements that made up its population. For
almost two centuries the Goths had been in full control of Spain, and their
uneducated manners and contempt of learning threaten greatly to put back the
progress of civilization in Spain.

Isidore supports the intolerant single-minded view of Christianity and works to
end Arianism, the new heresy of Acephales, and all other interpretations of
Christianity.

Isidore presides over the Second Council of Seville, begun 13 November 619, in
the reign of Sisebut. The bishops of Gaul and Narbonne attend, as well as the
Spanish prelates. In the Council's Acts the nature of Christ is fully set
forth, countering Arian conceptions.

At the Fourth National Council of Toledo, begun 5 December 633, all the bishops
of Spain are in attendance. St. Isidore, though far advanced in years, presides
over its deliberations, and is the originator of most of its enactments. The
position and deference granted to the king is remarkable. The church is free
and independent, yet bound in solemn allegiance to the acknowledged king:
nothing is said of allegiance to the bishop of Rome.
Seville, Spain  
1,360 YBN
[640 AD]
1119)
Egypt  
1,360 YBN
[640 AD]
1120) Theophanes records that Greek fire was invented around 670 in
Constantinople by Kallinikos (Callinicus), an architect from Heliopolis in
Syria (now Baalbek, Lebanon). This is the first reported use of a flame
throwing weapon.
Constantinople  
1,358 YBN
[642 AD]
1016)
  
1,358 YBN
[642 AD]
1017)
  
1,340 YBN
[660 AD]
1380) The hospital still resides on the Île de la Cité, its original
location, and is now recognized for extensive support for charities and for the
exceptional quality of doctors and surgeons who have been residents at the
facility.
Paris, France  
1,320 YBN
[680 AD]
1018)
  
1,315 YBN
[685 AD]
1019)
  
1,287 YBN
[713 AD]
1123) Bede's writings are classed as scientific, historical and theological,
reflecting the range of his writings from music and metrics to Scripture
commentaries. Bede quotes Pliny the Elder, Virgil, Lucretius, Ovid, Horace and
other classical writers, but with some disapproval. He knows some Greek, but no
Hebrew. Bede writes in Latin.

The most important and best known of his works is the Historia ecclesiastica
gentis Anglorum, giving in five books and 400 pages the history of England,
ecclesiastical and political, from the time of Caesar to the date of its
completion (731). The first twenty-one chapters, treating of the period before
the mission of Augustine of Canterbury, are compiled from earlier writers such
as Orosius, Gildas, Prosper of Aquitaine, the letters of Pope Gregory I and
others, with the insertion of legends and traditions.

After 596, documentary sources, which Bede took pains to obtain throughout
England and from Rome, are used, as well as oral testimony, which he employed
with critical consideration of its value. He cites his references and is very
concerned about the sources of all his sources, which creates an important
historical chain.

The Historia, like other historical writing from this period cannot be expected
to have the same degree of objectivity as modern historical writings. It was
indeed a form of literature, a mixture of fact, legend and literature. For
example, Bede took liberties by making up fictional quotations from people who
were not his contemporaries.

In Historia Ecclesiastica (I.2), he creates a method of referring to years
prior to the Christian era (anno Domini), which the monk Dionysius Exiguus
created in 525. He uses "ante incarnationis dominicae tempus" (before the time
of the incarnation of the Lord). This and similar Latin terms are roughly
equivalent to the English before Christ.

The noted historian of science, George Sarton, called the eighth century "The
Age of Bede;" clearly Bede must be considered as an important scientific
figure, even though his actual scientific contributions are minimal. He writes
several major works: a work "On the Nature of Things", modeled in part after
the work of the same title by Isidore of Seville; a work "On Time", providing
an introduction to the principles of computing the correct time for Easter; and
a longer work on the same subject; "On the Reckoning of Time", which will
become the cornerstone of clerical scientific education during the so-called
Carolingian renaissance of the ninth century. He also writes several shorter
letters and essays discussing specific aspects of computus and a treatise on
grammar and on figures of speech for his pupils.

"The Reckoning of Time" includes an introduction to the traditional ancient and
medieval view of the cosmos, including an explanation of how the spherical
earth influences the changing length of daylight, of how the seasonal motion of
the Sun and Moon influences the changing appearance of the New Moon at evening
twilight, and a quantitative relation between the changes of the Tides at a
given place and the daily motion of the moon. (Wallis 2004, pp. 82-85,
307-312). Since the focus of his book is calculation, Bede gives instructions
for computing the date of Easter and the related time of the Easter Full Moon,
for calculating the motion of the Sun and Moon through the zodiac, and for many
other calculations related to the calendar.

For calendric purposes, Bede makes a new calculation of the age of the world
since the Creation and begins the practice of dividing the Christian era into
BC and AD. Due to his innovations in computing the age of the world, he is
accused of heresy at the table of Bishop Wilfred, his chronology being contrary
to accepted calculations. Once informed of the accusations of these "lewd
rustics," Bede refutes them in his Letter to Plegwin (Wallis 2004, pp. xxx,
405-415).
Jarrow, Durham  
1,277 YBN
[723 AD]
1795)
?, China  
1,249 YBN
[751 AD]
1253) Abu Musa Jabir ibn Hayyan (Arabic: جابر بن حيان) (CE
c721-c815), with Latinised name Geber, is the first of the important Arab
alchemists and introduces the experimental method into alchemy. Jabir is
credited with being the first to prepare and identify sulfuric and other
acids.

Jabir gives accurate descriptions of valuable chemical experiments. Jabir
describes ammonium chloride, shows how to prepare white lead, prepares weak
nitric acid, and distills vinegar to get strong acetic acid. Jabir also works
with dyes and metals, and experiments with methods for refining metals. Jabir
writes numerous works on alchemy, although many people will later use his name.
Kufa, (now Iraq)  
1,240 YBN
[760 AD]
1020)
  
1,230 YBN
[770 AD]
1060) Earliest wood block Printed book. Diamond Sūtra.
China  
1,230 YBN
[770 AD]
1074) Wood-cut Printing.

Possibly around the 500s CE, carved wood block appears as a substitute to
pressing paper onto marble pillars and seals covered with ink. First, all of
the text is written in ink on a sheet of fine paper, then the written side of
the sheet is applied to the smooth surface of a block of wood, coated with a
rice paste that retains the ink of the text. Next, an engraver cuts away the
uninked areas so that the text stands out in relief and in reverse. To make a
print, the wood block is then inked with a paintbrush, a sheet of paper spread
on it, and the back of the sheet rubbed with a brush. Only one side of the
sheet can be printed. The oldest known printed works are made by this
technique. In Japan about 764–770, Buddhist incantations ordered by Empress
Shōtoku are printed using this technique, and in China in 868, the first known
book, the Diamond Sūtra is printed using wood blocks.
Japan  
1,219 YBN
[781 AD]
1254) Lower case letters.

Flaccus Albinus Alcuinus (Alcuin) (oLKWiN) (c.732-May 19, 804) a scholar,
ecclesiastic, poet and teacher from York, England, accepts an invitation from
Charlesmagne to be head of education for Charlemagne's kingdom which is most of
Western Europe. In the Palace School of Charlemagne, Alcuin will revolutionize
the educational standards of the Palace School, introducing Charlemagne to the
liberal arts and creates an atmosphere of scholarship and learning. In Aachen,
Alcuin designs a method of writing "Carolingian minuscule" to fit as much text
on the expensive parchment. This symbol set is the ancestor of lower-case
letters. All writing before this is done in capital (or majuscule) letters.

In my opinion, while possibly saving space on paper, lower case has complicated
language, and the most simple and logical representation of sound with symbols
is a single "one-letter-for-one-sound" phonetic alphabet that can be used for
all human languages.
Aachen, in north-west Germany, or York, England  
1,211 YBN
[01/01/789 AD]
1256) Aachen, in north-west Germany  
1,204 YBN
[01/01/796 AD]
1255) Alcuin establishes a school in Tours where scribes are trained to
carefully copy manuscripts. The new Carolingian miniscule alphabet letters
created by Alcuin will spread from text copied here and ultimately develop into
the miniscule (or lower case) letters used today.
Tours, France   
1,200 YBN
[800 AD]
1126) The first paddle-boat is invented in China.

China  
1,200 YBN
[800 AD]
1128) Paper making reaches Bagdad, 700 years after being invented in China.

Bagdad  
1,200 YBN
[800 AD]
6221) Earliest bow for stringed instrument. Plucking of stringed instruments
goes back at least 5000 years, but using a bow to play a stringed instrument is
a more recent invention, dating to around the 800s CE.
River Oxus (modern) Turkmenistan (Central Asia)  
1,185 YBN
[815 AD]
1021) "Bayt al-Hikma" (House of Wisdom).

Caliph al-Mamun founds the "Bayt al-Hikma" (House of Wisdom) in Baghdad, Iraq.
(Some people argue that al-Mamun's father al-Rashid founded the Bayt al-Hikma).
A library and observatory are joined to this house. In the House of Wisdom,
many works will be translated from Greek, Persian and Indian into Arabic. Many
original works will be created here too. The House of Wisdom recruits and
supports the most talented scholars.
Baghdad  
1,180 YBN
[820 AD]
1127) "Oseberg ship", a viking ship dates to here. This ship is a clinker-built
ship made of oak.

Tønsberg, Vestfold county, Norway  
1,175 YBN
[825 AD]
1257) Hindu-Arabic numerals (1 through 9), and decimal point notation.

Al-Khwārizmī (Arabic: محمد بن موسى الخوارزمي‎)
(oLKWoriZmE), as a scholar in the House of Wisdom in Baghdad, writes a book on
elementary algebra, "al-Kitāb al-mukhtaṣar fī ḥisāb al-jabr
waʾl-muqābala" ("The Compendious Book on Calculation by Completion and
Balancing"). When this book is translated into Latin in the 1100s, the word for
transposition "al-jabr" will come to represent the science started by Diofantos
(Latin: Diophantus), "Algebra". Algebra is the branch of mathematics that
involves solving equations by using methods such as transposition and
cancellation.
(House of Wisdom) Bagdad, Iraq  
1,171 YBN
[829 AD]
1299)
Sinjar in Mesopotamia, west of Mosul  
1,167 YBN
[833 AD]
1298) Al-Khwārizmī writes a third major work, his Kitāb ṣūrat al-arḍ
("The Image of the Earth"; translated as "Geography"), which presents the
coordinates of localities in the known world based, ultimately, on those in the
Geography of Ptolemy (fl. CE 127–145) but with improved values for the length
of the Mediterranean Sea and the location of cities in Asia and Africa.
Al-Khwārizmī also assists in the construction of a world map for al-Maʾmūn
and participates in a project to determine the circumference of the Earth by
measuring the length of a degree of a meridian through the plain of Sinjār in
Iraq.

Al-Khwarizmi overestimates the circumference of earth as (40,000 miles, actual
is 25,000 miles).(units)

Al-Khwārizmī also compiles a set of astronomical tables (Zīj), based on a
variety of Hindu and Greek sources. This work includes a table of sines,
evidently for a circle of radius 150 units.
Bagdad, Iraq  
1,159 YBN
[841 AD]
1304) Al-Kindi grew up in Kufa where his father was governor, and Kufa had
become a center of the sciences. Al-Kindi becomes especially interested in the
philosophical sciences after going to Baghdad. By this time a major movement of
translation (from Greek) into Arabic had begun (in Baghdad).

al-Kindi's full name is:
Abu Yusuf Ya'qub ibn Ishaq al-Kindi
Many Arabic names follow a
similarf pattern. "Abu Yusuf", abu is "father of" and Yusef is Joseph, so
al-Kindi had a child named Yusef. Ya'qub is the person's first name, in this
case "Jacob". "ibn Ishaq", "ibn" is "son of", "Ishaq" is "Isaac", so al-Kindi's
father's name is Ishaq. Finally, the last name is where they are from or a
profession associated with their family, "al-Kindi" is from the tribe of
Kindah.
Baghdad, Iraq  
1,150 YBN
[850 AD]
1144) Gunpowder.

The earliest Chinese records of gunpowder indicate that it was a byproduct of
Taoist alchemical efforts to develop an elixir of immortality. A book dating
from c. 850 CE called "Classified Essentials of the Mysterious Tao of the True
Origin of Things" warns of one elixir:
"Some have heated together sulfur, realgar
and saltpeter with honey; smoke and flames result, so that their hands and
faces have been burnt, and even the whole house where they were working burned
down.".

The earliest gunpowder, black powder is a mixture of saltpeter (potassium
nitrate), sulfur, and charcoal.
China  
1,150 YBN
[850 AD]
1332) Hunayn ibn Ishaq is appointed by Caliph al-Mutawakkil to the post of
chief physician to the court, a position that ibn Ishaq will hold for the rest
of his life. Hunayn travels to Syria, Palestine, and Egypt to get ancient Greek
manuscripts. From his translators' school in Baghdad, Ibn Ishaq and his
students will transmit Arabic and (more frequently) Syriac versions of
classical Greek texts throughout the Arabic population.

Ibn Ishaq means "son of Isaac".
Baghdad, Iraq  
1,150 YBN
[850 AD]
1333) As a young man, Al-Mutawakkil held no political or military positions of
importance but took a keen interest in religious debates that had far-reaching
political importance.
Samarra (near Baghdad), Iraq  
1,141 YBN
[859 AD]
1336) University and mosque of Al Qaraouine in Fès, Morocco. The oldest
University on Earth, however only Muslims are admitted into the mosque.
Fes, Morocco  
1,124 YBN
[876 AD]
1115) The number zero.

The Babylonians appear to have developed a placeholder symbol that functioned
as a zero by the 3rd century BC, but its precise meaning and use is still
uncertain.

There is no doubt that the symbol for the number zero is invented in India, but
exactly how and for what purpose is unclear.

The oldest symbol "0" in India that can be assigned a definite date, is
inscribed on a temple in Gwalior.
Gwalior, India  
1,124 YBN
[876 AD]
1300) Thabit is a scion of a prominent family settled in Harran (now in
Turkey), a city noted as the seat of a Hellenized Semitic astronomical cult,
the Sabians, of which Thabit was a member. By calling themselves Sabians, after
a group mentioned in the Qur'an, the cult members established themselves as
"People of the Book" and therefore were freed from the requirement of
conversion to Islam.

The Sabians of Harran, are a sect of Hermetists, often confused with the
Mandaeans. As star-worshippers, Sabians show a great interest in astronomy,
astrology, magic, and mathematics. This religious cult is centered around the
symbolism of the planets, and is very interested in the Pythagorean
mathematical and mystical tradition. This sect lives will near the main center
of the Caliphate until 1258, when the Mongols will destroy their last shrine.
During Muslim rule, they are a protected minority, and around the time of
al-Mutawakkil's reign their town will become a center for philosophical,
esoteric, and medical learning. They are joined by the descendants of pagan
Greek scholars who, having been persecuted in Europe, settled in lands that
became part of the Abbasid caliphate. In this time the Muslims are greatly
interested in Greek culture and science, collecting and translating many
ancient Greek works in the fields of philosophy and mathematics. Although they
later became Arabic speakers, in pre-Islamic times, it was common for Sabians
to speak Greek.

Some sources describe Thabit as a money changer in Harran, the sources give two
different accounts of his life.

Thabit and his pupils live in the midst of the most intellectually vibrant, and
probably the largest, city of this time, Baghdad. Ibn Qurra occupies himself
with mathematics, astronomy, astrology, magic, mechanics, medicine, and
philosophy. His native language is Syriac, which is the eastern dialect of
Aramaic (a semitic language) from Edessa, and Thabit knows Greek well.

Only a few of Thabit's works are preserved in their original form.

Through the influence of the mathematician Muhammad ibn Musa ibn Shakir (father
of the three famous Banu Musa mathematician brothers), late in his life Thabit
ibn Qurrah will become court astronomer for the 'Abbasid caliph al-Mu'tadid
(reigns 892-902) and become the Caliph's personal friend.

Several of Thabit ibn Qurrah's works will be translated into Latin and Hebrew
and will prove to be influential in the Latin West. A son, Sinan ibn Thabit,
will become a renowned physician and director of a hospital in Baghdad, and a
grandson, Ibrahim ibn Sinan, will win fame as an important mathematician.
Bagdad, Iraq  
1,122 YBN
[878 AD]
1301) Alfred creates a legal Code, reconciling the long established laws of the
Christian kingdoms of Kent, Mercia and Wessex. These formed Alfred"s "Deemings"
or Book of "Dooms" (Book of Laws). The Doom Book, Code of Alfred or Legal Code
of Aelfred the Great, was the code of laws (dooms, laws, or judgments) compiled
by Alfred the Great from three prior Saxon codes, to which he prefixed the Ten
Commandments of Moses, and incorporated rules of life from the Mosaic Code and
the Christian code of ethics. The title "Doom book" (originally dom-boc or
dom-boke) comes from dōm (pronounced "doom") which is the Anglo-Saxon word
meaning "judgment", or "law".

Apart from the lost Handboc or Encheiridion, which seems to have been only a
commonplace book kept by the king, the earliest work to be translated is the
"Dialogues" of Gregory, a book that is very popular in the Middle Ages. In this
case the translation is made by Alfred's great friend Werferth, Bishop of
Worcester, the king providing a foreword. The next work to be undertaken is
Gregory's "Pastoral Care", especially for the benefit of the parish clergy. In
this translation Alfred keeps very close to his original; but the introduction
Alfred writes for this book is one of the most interesting documents of the
reign, or indeed of English history. The next two works translated are
historical, the "Universal History" of Orosius and Bede's "Ecclesiastical
History of the English People". Probably Orosius was first. In the Orosius
translation, by omissions and additions, Alfred so changes the original as to
produce an almost new work; however in the Bede translation the author's text
closely follows the original with no additions being made, though most of the
documents and some other less interesting matters are omitted.

One of the most interesting translations by Alfred is his translation of "The
Consolation of Philosophy" of Boethius, the most popular philosophical handbook
of the Middle Ages. Here again Alfred deals very freely with his original copy.
Many of the additions to the text can be traced to the glosses and commentaries
Alfred uses and not to Alfred himself. In the Boethius translation is an often
quoted sentence: "My will was to live worthily as long as I lived, and after my
life to leave to them that should come after, my memory in good works." This
book has only survived in two manuscripts. In one of these the writing is
prose, in the other a combination of prose and alliterating verse. The latter
manuscript was severely damaged in the 18th and 19th centuries, and the
authorship of the verse has been much disputed; but likely it also is by
Alfred. In fact, he writes in the prelude that he first created a prose work
and then used it as the basis for his poem, the Lays of Boethius, his crowning
literary achievement. Alfred spends a great deal of time working on these
books, and explains that he gradually wrote through the many stressful times of
his reign to refresh his mind.

The last of Alfred's works is one to which he gave the name "Blostman", i.e.,
"Blooms" or "Anthology". The first half is based mainly on the Soliloquies of
St Augustine of Hippo, the remainder is drawn from various sources, and
contains much that is Alfred's own and highly characteristic of him. The last
words of it may be quoted; they form a fitting epitaph for the noblest of
English kings. "Therefore he seems to me a very foolish man, and truly
wretched, who will not increase his understanding while he is in the world, and
ever wish and long to reach that endless life where all shall be made clear."
Wessex (871-899), a Saxon kingdom in southwestern England.  
1,112 YBN
[888 AD]
1305) Arab astronomer, Al-Battani refines existing values for the length of the
year and of the seasons, for the annual precession of the equinoxes, and for
the inclination of the ecliptic. The inclination of the ecliptic is the angle
made between the plane the earth rotates the sun in (the celestial equator) and
the plane the Earth rotates itself in. The ecliptic is a circle in the
celestial sphere that is the apparent path of the Sun among the constellations
in the course of a year. The ecliptic intersects the plane of the celestial
equator at the vernal and autumnal equinoxes.

This improved value for the length of the year will be used 700 years later in
the Gregorian reform of the Julian Calendar.
ar-Raqqa, Syria  
1,110 YBN
[890 AD]
1129) The Gokstad ship is a late 9th century clinker-built Viking ship found in
a ship burial beneath a burial mound at Gokstad farm in Sandar, Sandefjord,
Vestfold, Norway. Dendrochronolgical (tree ring) dating suggests that the ship
was built of timber that was felled around 890 CE.

Sandar, Sandefjord, Vestfold, Norway  
1,110 YBN
[890 AD]
1302)
Wessex (871-899), a Saxon kingdom in southwestern England.  
1,100 YBN
[900 AD]
1379) Regimen Sanitatis Salernitanum, or the "Salerno Book of Health" from this
school will be first printed in 1484.
This school shows that the people of Italy are
very early in the development of universities, education and women's rights.
Salerno, Italy  
1,100 YBN
[900 AD]
5865) Polyphonic works are called "Organum" (plural: Organa). The earliest
written form of polyphonic music is found in the treatise "Musica enchiriadis"
(c. 900; "Musical Handbook"), in which organum consists of two melodic lines
moving simultaneously note against note. The planchant melody is called the
"vox principalis" (principal voice), and the additional voice is called the
"vox organalis" (the organal, or added, voice). In the simplest parallel
organum, a single organal voice runs a fourth or fifth below the principal
voice. Other examples include four voices, with the principal voice doubled an
octave down and the organal voice doubled an octave up. In some instances, the
two voices start in unison, then move to wider intervals.

At this early stage, there are no rhythmic signs beyond the words of the chant
in the "Musica Enchiriadis", but the pitches are indicated precisely through
the daseian signs in the margin at left. Adapted from grammatical accent marks
in ancient Greek, each of these corresponds to a specific pitch.
northern part of the West Frankish empire|Possibly written in what is now
Eastern France  
1,096 YBN
[904 AD]
1145)
China  
1,095 YBN
[905 AD]
1303) Plaster used to hold broken bones in place. Al-Razi {oL-rAZE} rejects
Islam and other religions.

Al-Razi {oL-rAZE} (full name Abū Bakr Muhammad ibn Zakarīya al-Rāzi Latin:
Rhazes), a Persian physician and chemist, is the first to prepare "plaster of
paris" and describes how it can be used to hold broken bones in place, to
identify and distinguish between smallpox and measles, is the first of record
to divide all substances into animal, vegetable and mineral, accepts the atom
theory, dismisses miracles and mysticism, thinks religion harmful and the cause
of hatred and wars.

Al-Razi openly criticizes religions including the new rising religion of Islam
describing the Koran as (translated) "...a work which recounts ancient myths,
and which at the same time is full of contradictions and does not contain any
useful information or explanation.".
Rayy (near Tehran, Iran)   
1,090 YBN
[910 AD]
1407) Al-Farabi studies music theory and composes music. Some of al-Farabi's
compositions have survived in the rites of the Sufi brotherhoods, in particular
those in Anatolia.
Al-Farabi is a practicing Sufi.

Al-Farabi had great influence on science and philosophy for several centuries,
and was widely regarded to be second only to Aristotle in knowledge (alluded to
by his title of "the Second Teacher"). His work, aimed at synthesis of
philosophy and Sufism, paved the way for Ibn Sina's work.

The major part of al-Farabi's writings are directed to the problem of the
correct ordering of the state. Al-Farabi's views are similar to Plato's
"Republic" in the elitist undemocratic belief that, just as God rules the
universe, so should the philosopher, as the most perfect kind of man, rule the
state; al-Farabi therefore relates the political upheavals of his time to the
separation of the philosopher from government.
Baghdad, Iraq  
1,080 YBN
[920 AD]
6183) Norwegian explorers reach North America.

In 1961 (verify) Helge Ingstad, finds in Northern Newfoundland a site that
establishes the presence of European settlers in North America prior to
Columbus. For seven successive summers expeditions excavate this site under the
leadership of Anne Stine Ingstad, a trained archaeologist. They excavate seven
house sites, a smithy, and four "boat sheds," as well as some open-air hearths
and a charcoal kiln.
All of the walls were built of turf, now largely decomposed, and
nearly
all of the rooms were equipped with simple hearths. The artifacts collected
number in the
hundreds, but most of them are
small iron objects (rivets and nails), slag and
bog-ore, stone implements,
charcoal, and brittle-burned stones; there are two
unquestionably Norse
pieces of handicraft, a soapstone spindle whorl, and a
ring-headed pin
of bronze (thought to be a belt pin). Bones were found of a pig, a
whale, and a seal.
L'Anse Aux Meadows, Newfoundland  
1,064 YBN
[936 AD]
1408) Al-Mas'udi is known as the "Herodotus of the Arabs".
Baghdad, Iraq  
1,040 YBN
[960 AD]
6186) Earliest evidence of rockets. These are gun-powder rockets probably in
hollow bamboo tubes.

Fire-arrow technology is described in the "Complete Compendium of Military
Classics" (960 CE), which provides evidence that Emperor Tseng Kung-Liang had a
group of rocketeers equipped to make and fire powder rockets in combat.

Certainly by the year 1045 CE, the use of gunpowder and rockets forms an
integral aspect of Chinese military tactics.
China  
1,036 YBN
[964 AD]
1502)
Isfahan (Eşfahān), Persia (modern Iran)  
1,030 YBN
[970 AD]
1338) The mosque is built in two years from 969 CE, the year in which its
foundation is laid. Studies will begin in Al-Azhar in Ramadan by October 975
CE, when Chief Justice Abul Hasan Ali ibn Al-No'man starts teaching the book
"Al-Ikhtisar", on the Shiite Jurisprudence.
Al-Azhar University is the leading institution for
Sunni learning in the Islamic world.
Cairo, Egypt  
1,025 YBN
[975 AD]
1839)
?, India (presumably)  
1,024 YBN
[976 AD]
1307)
  
1,021 YBN
[979 AD]
1410)
Cordova, Spain  
1,019 YBN
[981 AD]
1385) The Al-Adudi hospital is named after Emir 'Adud al-Daula. The hospital
will be destroyed in 1258 by the Mongol invasion.
Baghdad, Iraq  
1,018 YBN
[982 AD]
1130) Norse people from Iceland reach Greenland, which they find uninhabited.
They establish three settlements near the very southwestern tip of the island,
where they will live for about 450 years.

Greenland  
1,015 YBN
[985 AD]
1306) In 999 Gerbert will become the first French Pope as Sylvester II.
In a
letter of 984, Gerbert asks Lupitus of Barcelona for a translation of an Arabic
astronomical treatise.
Gerbert may have been the author of a description of the astrolabe
that will be edited by Hermannus Contractus around 50 years later.
Auvergne, France  
1,000 YBN
[1000 AD]
1022) The "Suda", one of the first encyclopedias is compiled, credited to a
person named Suidas.

Suda, or Suidas, breaks with tradition by adopting alphabetical order for its
contents.

There is evidence that the Suda is compiled in the latter part of the 900s.
Passages referring to Michael Psellus (end of 11th century) are considered
later interpolations. The lexicon is arranged alphabetically with some slight
deviations; letters and combinations of letters having the same sound being
placed together. The Suda is both a dictionary and encyclopedia.

The Suda includes numerous quotations from ancient writers; the scholiasts
(commentary on the margin of a manuscript) on Aristophanes, Homer, Sophocles
and Thucydides are also used often. The biographical notices, the author
explains, are condensed from the "Onomatologion" or "Pinax" of Hesychius of
Miletus; other sources were the excerpts of Constantine Porphyrogenitus, the
chronicle of Georgius Monachus, the biographies of Diogenes Laertius and the
works of Athenaeus and Philostratus.


Most of the Suda was lost during the crusader sacking of Constantinople and the
Ottoman pillage of the city in 1453.
The lexicon is arranged, not quite
alphabetically, but according to a system (formerly common in many lagnauges)
called antistoichia; namely the letters follow phonetically, in order of sound
(in the pronunciation of Suida's time, which is the same as modern Greek, and
serves as a key to the authentic pronunciation of each letter, letter group and
word).
Most of the Alexandrian librarians are listed with more details in the Suda.
  
1,000 YBN
[1000 AD]
1054) Paper money.

The first use of paper money occurred in China more than 1,000 years ago.

Initially paper money represents promises to pay specified amounts of metal
coin money (gold and silver) for which carrying in large quantities is
inconvenient and a risk for loss or theft. These promises are initially issued
by individuals or companies as banknotes or as the transferable book entries
that come to be called deposits. Although deposits and banknotes begin as
claims to gold or silver on deposit at a bank or with a merchant, this later
changes. Knowing that everyone will not claim their balance at once, bankers
and merchants start to issue more claims to the gold and silver than the amount
they actually hold. In periods of distress, however, when borrowers did not
repay their loans or in case of overissue, the banks could fail. So gradually,
governments assume a supervisory role. Later paper money—promises to pay in
gold or silver are replaced by Governments with "fiat" paper money— notes
that are legal tender but are not promises to pay something else like gold or
silver.
China  
1,000 YBN
[1000 AD]
1131) Watermills are widely used in Europe at this time.

Europe  
1,000 YBN
[1000 AD]
1132) Motte-and-bailey castles are constructed. Many were built in Britain and
France in the 11th and 12th centuries, especially in England following the
Norman Conquest of 1066.

The motte is a raised earth mound, like a small hill, usually assembled and
topped with a wooden or stone structure known as a keep. The earth for the
mound would be taken from a ditch, dug around the motte or around the whole
castle. The outer surface of the mound could be covered with clay or
strengthened with wooden supports.

The bailey is an enclosed courtyard, typically surrounded by a wooden fence and
overlooked by the motte. A castle could have more than one bailey, sometimes an
inner and an outer.

Europe  
990 YBN
[1010 AD]
1311) Ibn Sina is an infant prodigy that can recite the Quran and many Persian
poems at age 10.
Ibn Sina wrongly believes that transmutation (changing of atoms
from one kind to the other) to be impossible (although only achieved in the
1900s in particle physics by Rutherford, Fermi and others).

Ibn Sina turnes his attention to health at age 16, and achieves full status as
a physician at age 18, Ibn Sina writes that "Medicine is no hard and thorny
science, like mathematics and metaphysics, so I soon made great progress; I
became an excellent doctor and began to treat patients, using approved
remedies." The youthful physician's popularity spreads quickly, and he treats
many patients without asking for payment.

In Hamadan, Ibn Sina is even raised to the office of vizier (a high ranking
advisor to an Arab monarch such as a Caliph, Amir, Malik (king) or Sultan) in
Hamadan.

Ibn Sin'a book حكمت مشرقيه
(hikmat-al-mashriqqiyya, in Latin "Philosophia Orientalis"), which Roger Bacon
will mention, is now lost. According to Averroes this book is pantheistic in
tone.

Ibn Sina is, like all his countrymen, ample in the enumeration of symptoms, and
is said to be inferior to Ali in practical medicine and surgery. Ibn Sina
introduces into medical theory the four causes of the Peripatetic system. The
Canon will still be used as a textbook in the universities of Leuven and
Montpellier up to around the year 1650.

In the museum at Bukhara, there are displays showing many of Ibn Sina's
writings, surgical instruments from the period and paintings of patients
undergoing treatment. Ibn Sina was interested in the effect of the mind on the
body, and writes a great deal on psychology, likely influencing Ibn Tufayl and
Ibn Bajjah.

Some of Ibn Sina's books are dictated from horseback while accompanying a ruler
to some battle.

Ibn Sina writes extensively on the subjects of philosophy, logic, ethics,
metaphysics and other disciplines. Most of his works were written in Arabic,
and some are written in the Persian language. Of linguistic significance even
to this day are a few books that Ibn Sina writes in nearly pure Persian
language (particularly the Danishnamah-yi 'Ala', Philosophy for Ala'
ad-Dawla'). Avicenna's commentaries on Aristotle often correct the philosopher,
encouraging a lively debate in the spirit of ijtihad, (a technical term of
Islamic law that describes the process of making a legal decision by
independent interpretation of the legal sources, the Qur'an and the Sunnah).
Hamadan, Iran  
975 YBN
[1025 AD]
5868) The system of Arezzo consists in the construction by thirds of a system
of four lines, or staff, and the use of letters as clefs. The red F-line and
the yellow C-line were already in use, but Guido adds a black line between the
F and the C and another black line above the C. The neumes (notational signs
used in the Middle Ages that represented specific kinds of melodic motion and
manners of performance) can now be placed on the lines and spaces between and a
definite pitch relationship established. With this system it is no longer
necessary to learn melodies by memory, and Guido declares that his system
reduces the 10 years normally required to become an ecclesiastical singer to
one year.

A well-developed "solmization" (a system of designating musical notes by
syllable names) exists in the music of India, using the syllables ṣa, ṛi,
ga, ma, pa, dha, ni; and similar systems occur in, for example, Chinese,
Southeast Asian, and ancient Greek music. The system that predominates in
European music is introduced by the Italian monk, Guido of Arezzo, who derives
it from the Latin hymn, "Ut queant laxis".

During the half century after Guido’s death (CE 1050-1100), developments
occur more rapidly as the plainsong chant becomes the lower rather than the
upper voice. Then the organal part, vox organalis is freed. The peak of this
freedom is reached in the organums of the monastery of Saint-Martial in
Limoges, France, where the plainsong part is reduced to the role of sustaining
each tone while the organal part performs in free melismata (groups of notes
sung to a single syllable), either improvised or composed. This new style is
called organum purum.
(Cathedral school) Arezzo, Italy  
970 YBN
[1030 AD]
1409) Al-Biruni (full name: Abu Rayhan Muhammad ibn Ahmad al-Biruni) (CE
973-c1051), a Persian scholar, writes about the movement of the Earth relative
to the Sun, and that all astronomical appearances can be explained if the Earth
rotates each day, and notes "the attraction of all things towards the centre of
the earth".
Ghazna, Afghanistan  
962 YBN
[1038 AD]
1308) Pin-hole camera (or camera obscura). Ibn al-Haytham {iBN oL HIteM} (Full
Name: Abu 'Ali al-Hasan ibn al-Haytham) (Arabic and Persian: ابو علی،
حسن بن حسن بن هيثم) (Latinized: Alhazen (oLHoZeN)) (CE
c965-1039), builds the first recorded pin-hole camera (camera obscura).

Ibn al-Haytham's optical work "Ṣūrat al-kusūf" ("On the Shape of the
Eclipse") includes a discussion of the camera obscura).

Al-Haytham is the first of record to understand that light comes from the Sun
and reflects off objects into the eyes contradicting the theory of Euclid and
Ptolemy that rays of light emit from the eye.

Al-Haytham constructs parabolic mirrors (now used in telescopes to better focus
light than a spherical mirror).

Al-Haytham studies the focusing of light.

Like Ptolemy, al-Haytham thinks that the atmosphere has a finite height, and
estimates this height as 10 miles. (actual units)

Al-Haytham's "Optics" will have a major influence not only on 13th-century
thinkers such as Roger Bacon but also on later scientists such as the
astronomer Johannes Kepler (1571–1630), who after 600 years will be the first
to improve on the science of optics..
Cairo, Egypt  
959 YBN
[1041 AD]
1124) The first known movable-type system for printing using ceramic materials
was created in China around 1040 AD by Pi Sheng (990–1051). As described by a
contemporary account of Shen Kua (1031–1095):

"During the reign of Chhing-li {1041-48} Pi Sheng, a man of unofficial
position, made moveable type. His method was as follows: he took sticky clay
and cut in it characters as thin as the edge of a coin. Each character formed,
as it were, a single type. He baked them in the fire to make them hard. He had
previously prepared an iron plate and he had covered his plate with a mixture
of pine resin, wax, and paper ashes. When he wished to print, he took an iron
frame and set it on the iron plate. In this he placed the types, set close
together. When the frame was full, the whole made one solid block of type. He
then placed it near the fire to warm it. When the paste {at the back} was
slightly melted, he took a smooth board and pressed it over the surface, so
that the block of type became as even as a whetstone.
If one were to print only two or
three copies, this method would be neither simple not easy. But for printing
hundreds or thousands of copies, it was marvelously quick. As a rule he kept
two formes going. While the impression was being made from the one forme, the
type was being put in place on the other. When the printing of the one forme
was finished, the other was then ready. In this way the two formed alternated
and the printing was done with great rapidity.
For each character there were several
types, and for certain common characters there were twenty or more types each,
in order to be prepared for the repetition of characters on the same page. When
the characters were not in use, he had them arranged with paper labels, one
label for words of each rhyme-group, and kept them in wooden cases. If any rare
characters appeared that had not been prepared in advance, it was cut as needed
and baked with a fire of straw. In a moment it was finished.
The reason why he did not
use wood is because the tissue of wood is sometimes coarse and sometimes fine,
and wood also absorbs moisture, so that the forme when set up would be uneven.
Also the wood would have stuck in the paste and could not readily have been
pulled out. So it was better to use burnt earthenware. When the printing was
finished, the forme was again brought near the fire to allow the paste to melt,
and then cleansed with the hand, so that the types fell off of themselves and
were not in the least soiled.
When Pi Sheng died, his font of type passed into the
possession of my nephews, and up to this time it has been kept as a precious
possession.".

In about 1313 a magistrate named Wang Chen will have a craftsman carve more
than 60,000 characters on movable wooden blocks so that a treatise on the
history of technology can be published. Chen is also credited with the
invention of horizontal compartmented cases that revolve around a vertical axis
to allow easier handling of the type. But Wang Chen’s innovation, like that
of Pi Sheng, is not followed up in China. However, in Korea, typography is
extensively developed under the stimulus of King Htai Tjong, who, in 1403,
orders the first set of 100,000 pieces of type to be cast in bronze. Nine other
fonts followed from then to 1516; two of them were made in 1420 and 1434,
before Europe discovers typography.

Johannes Gutenberg is generally credited in 1435 with the earliest printing
press in Europe.

One explanation for the fact that printing develops in Europe in the 1400s
instead of in the Far East, even though the principle of printing was known in
the Orient long before is that European writing is based on an alphabet made of
a limited number of symbols. This simplifies the problems involved in
developing techniques for the use of movable type. However, Chinese
handwriting, has some 80,000 symbols, which is not as well fitted to
typography.

The development of printing gives impetus to the growth and accumulation of
knowledge, for example from Diderot’s encyclopaedia to the many publications
currently printed throughout the Earth.
China  
959 YBN
[1041 AD]
1136) Krak des Chevaliers ("fortress of the knights") is built.

east of Tripoli in the Homs Gap  
936 YBN
[1064 AD]
1313) Khayyam means "tentmaker".
Khayyam is funded by the Vizier of the Seljuk Sultan Alp
Arsian and then his successor Malik Shah.
Persia, Iran (presumably)  
934 YBN
[1066 AD]
1326) Having first seen it as a young boy in 989, Eilmer of Malmesbury
declares: "You've come, have you?...You've c-ome, you source of tears to many
mothers, you evil. I hate you! It is long since I saw you; but as I see you now
you are much more terrible, for I see you brandishing the downfall of my
country. I hate you!".
England and New Mexico  
932 YBN
[1068 AD]
1840)
?, India (presumably)  
930 YBN
[1070 AD]
1314)
  
927 YBN
[1073 AD]
1316)
  
923 YBN
[1077 AD]
1315)
  
921 YBN
[03/15/1079 AD]
1317) Sultan Jalal al-Din Malekshah Saljuqi (1072-92) puts Omar Kyayyam's
corrected calendar into effect.

  
919 YBN
[1081 AD]
1312) Al-Zarqali (Latin: Arzachel) (Spanish and Italian: Azarquiel), (In Arabic
أبو أسحاق ابراهيم بن يحيى الزرقالي ),(full name:
Abū Isḥāqibrāhīm Ibn Yaḥyā Al-Naqqāsh) (CE ?-1100), describes the
orbit of Mercury as being oval instead of circular.

In Al-Zarqali's text "Tratado de la lamina de los siete planetas" ("Treatise on
the sheets of the seven planets") contains one of the most debated passages in
medieval astronomy. In the graphic representation included in the Castilian
translation ordered by Alfonso X (The Wise) the orbit of Mercury is not
circular. On this basis it has been alleged that al–ZarqāĪi anticipated
Kepler in stating that orbits–the orbit of Mercury in this case–are
elliptical. Although the Arabic text merely states that an orbit is baydi
("oval").

Al-Zarqali also invents the apparatus called the azafea (Arabic: al-safiha),
which is widely used by navigators until the 1500s.

Al-Zarqali is also credited with the explicit proof of the motion of the
aphelion (of the earth or apogee of the sun) with respect to the fixed stars.
Working
in an observatory in Toledo, Al-Zarqali edits the famous "Tables of Toledo"
(Toledan Zij) {Zij?}, a compilation of astronomical data which are among the
most accurate of the Islamic period. These tables are composed with the help of
several other Muslim and Jewish scientists and will be widely used by both
Latin and Muslim astronomers in later centuries.
Toledo (in Castile, now) Spain  
914 YBN
[1086 AD]
1135)
China  
912 YBN
[1088 AD]
1163)
China  
912 YBN
[1088 AD]
1339) The University of Bologna (Italian: Alma Mater Studiorum Università di
Bologna, UNIBO) is founded, and is one of the oldest and most famous
universities in Europe.
Bologna, Italy  
905 YBN
[1095 AD]
1137)
Jerusalem  
901 YBN
[1099 AD]
1382) This order has survived through the centuries as the St. John's Ambulance
Corps.
Jerusalem  
900 YBN
[1100 AD]
1023)
  
900 YBN
[1100 AD]
1142) Post mill windmills are built in Europe. Post mills are the earliest type
of windmill and have the fan connected to a single post which can be turned in
the direction of the wind.

Europe  
900 YBN
[1100 AD]
1521) The "Charter of Liberties" is issued upon the ascension of King Henry I
to the throne in 1100. It binds the king to certain laws regarding the
treatment of church officials and nobles. The document addressea certain abuses
of royal power by his predecessor, his brother William Rufus, specifically the
over-taxation of the barons.
Henry Beauclerc (meaning: Good Scholar) is the youngest
and considered to be the ablest of William I the Conqueror's sons.
London, England  
900 YBN
[1100 AD]
1841)
?, China (presumably)  
900 YBN
[1100 AD]
5883)
Provence, France (Southern France)  
894 YBN
[1106 AD]
1411) in 1085, al-Ghazali was invited to go to the court of Nizam al-Mulk, the
powerful vizier of the Seljuq sultans. The vizier was so impressed by
al-Ghazali's scholarship that in 1091 he appointed him chief professor in the
Nizamiyah college in Baghdad. While lecturing to more than 300 students,
al-Ghazali was also mastering and criticizing the Neoplatonist philosophies of
al-Farabi and Avicenna (Ibn Sina). He passed through a spiritual crisis that
rendered him physically incapable of lecturing for a time. In November 1095 he
abandoned his career and left Baghdad on the pretext of going on pilgrimage to
Mecca. Making arrangements for his family, he disposed of his wealth and
adopted the life of a poor Sufi, or mystic. After some time in Damascus and
Jerusalem, with a visit to Mecca in November 1096, al-Ghazali settled in Tus,
where Sufi disciples joined him in a virtually monastic communal life. In 1106
he was persuaded to return to teaching at the Nizamiyah college at Nishapur.
Nishapur, Iran  
880 YBN
[1120 AD]
1141) First papermill (factory dedicating to making paper) in Europe.

in Spain, at Xavia (modern Valencia), Europe  
880 YBN
[1120 AD]
1318) Abelard wanders from school to school at Paris, Melun, Corbeil, and
elsewhere. In 1113 or 1114 he goes north to Laon to study theology under Anselm
of Laon, the leading biblical scholar of the day. He quickly developed a strong
contempt for Anselm's teaching, which he finds vacuous, and returns to Paris.
Abelard
teaches openly (publicly?) in Paris but is also given as a private pupil, the
young Héloïse, niece of one of the clergy of the cathedral of Paris, Canon
Fulbert. Abelard and Héloïse fall in love and have a son whom they called
Astrolabe. They then marry secretly. To escape her uncle's wrath Héloïse
withdraws into the convent of Argenteuil outside Paris. Heloise's uncle
Fulbert, the powerful canon of Notre Dame, finds out about their relationship
and hires people to castrate Abelard in 1121 (at the age of 42). I have found
no record of any identity or arrest of anybody for this vicious first degree
assault and battery. In shame Ableard embraces the monastic life, becoming a
monk at the royal abbey of Saint-Denis near Paris and makes the unwilling
Héloïse become a nun at Argenteuil.

Abelard will write "Dialogue of a Philosopher with a Jew and a Christian".
In the early
1130s Pierre and Héloïse will compose a collection of their own love letters
and religious correspondence.
Later in life Pierre Abelard will write an autobiography
"Historia Calamitatum" in Latin. This book is in the form of a letter, and is
clearly influenced by Augustine of Hippo's "Confessions". The "Historia" is
exceptionally readable, and presents a remarkably honest self-portrait of a man
who could be arrogant and often felt persecuted. It provides a clear and
fascinating picture of intellectual life in Paris before the formalization of
the University, of the intellectual excitement of the period, of monastic life,
and of his affair with Heloise, one of history's most famous love stories.
(the royal abbey of Saint-Denis near) Paris, France  
874 YBN
[1126 AD]
1155)
Artois, France  
870 YBN
[1130 AD]
1140)
France  
870 YBN
[1130 AD]
1322) Adelard is the tutor of future King Henry II. During a period of seven
years Adelard travels through Greece, Asia Minor, and North Africa. Adelard
learns arabic.
Bath, England  
868 YBN
[1132 AD]
1146) First cannon and gun.

In Buddhist caves of Western China, a temple in Ta-tsu in Szechuan Province
shows the earliest depiction of a gun. One relief depicts a small demon with
two horns showing flames and a ball being shot from a handheld cannon. A second
relief shows a devil holding a grenade.
Ta-tsu, Szechuan Province, China  
865 YBN
[1135 AD]
1321)
(Mont-Sainte-Geneviève outside) Paris, France  
864 YBN
[1136 AD]
1143) The Basilica of Saint Denis. This is considered to be the first major
structure built in the gothic style.
Construction of the church began in 1136
by the Abbot Suger (1081-1155), but the major construction will not be complete
until the end of the 13th century.
All but three of the monarchs of France from the 10th
century until 1789 have their remains here.

Paris France  
860 YBN
[1140 AD]
1320)
Sens, France  
856 YBN
[1144 AD]
1148) A boy is found dead in England and all Jewish people are blamed. In many
cities, Jewish humans are sentenced to death for child sacrificing.

England  
850 YBN
[1150 AD]
1152) Cog-built ships are built in Europe. Cog-built vessels (Cogs). They are
characterized by flush-laid flat bottom at midships but gradually shifted to
overlapped strakes near the posts. They have full lapstrake planking covering
the sides.

Europe  
850 YBN
[1150 AD]
5866) A more elaborate form of organum (polyphonic or "many-voiced" style)
evolves at the abbeys of Santiago de Compostela, Spain (c. 1137), and
Saint-Martial of Limoges, France (c. 1150), in which a highly florid melody
(duplum) is added above the plainchant "tenor".
Santiago de Compostela, Spain and Saint-Martial of Limoges, France  
850 YBN
[1150 AD]
5882)
(convent) Rupertsberg, Germany  
850 YBN
[1150 AD]
6239)
Europe  
846 YBN
[1154 AD]
1323)
Toledo, Spain  
834 YBN
[1166 AD]
1330) After the death of the philosopher Ibn Tufayl, Averro's succeeded him as
personal physician to the caliphs Abu Ya'qub Yusuf in 1182 and his son Abu
Yusuf Ya'qub in 1184.
Cordova, Spain  
833 YBN
[1167 AD]
1340)
Oxford, England (now: United Kingdom)  
830 YBN
[1170 AD]
1319) University of Paris.

The University of Paris is founded around this time growing out of the
cathedral schools of Notre-Dame.

The university was originally divided into four faculties: three
“superior,” theology, canon law, and medicine; and one “inferior,”
arts. In the faculty of arts, the trivium (grammar, rhetoric, and dialectic)
and the quadrivium (arithmetic, geometry, astronomy, and music) were taught
together with general scientific, literary, and general culture. Each faculty
was headed by a dean, and the dean of the faculty of arts had by the 14th
century become the head of the collective university under the title of rector.
Many colleges were built to accommodate the students. The most celebrated was
the Sorbonne, founded by the theologian Robert de Sorbon about 1257.
Paris, France  
830 YBN
[1170 AD]
5867)
(Notre Dame Cathedral) Paris, France  
825 YBN
[1175 AD]
1149) Arabic copy of Ptolomy "Almagest" is translated to Latin.

  
825 YBN
[1175 AD]
1341)
Modena and Reggio Emilia, Emilia-Romagna, Italy  
824 YBN
[1176 AD]
1334) Maimonides' earliest work, composed in Arabic at the age of 16, is the
"Millot ha-Higgayon" ("Treatise on Logical Terminology"), a study of various
technical terms that were employed in logic and metaphysics. Another early
work, also in Arabic, is the "Essay on the Calendar" (Hebrew title: "Ma'amar
ha'ibur").

Maimon's Greek name is Moses Maimonides, which literally means, "Moses, son of
Maimon".

When the Almohads (Arabic: al-Muwahhidun, "the Unitarians"), who are a
fanatically Islamic people, capture Córdoba in 1148, Jewish people are forced
to submnit to Islam or leave the city. The Maimon family dresses in Islamic
clothes but secretly practices Judaism in their house.

In Fez, Morroco Moses studies at the University of Al Karaouine. During this
time Maimonides' writes his first major work, begun at the age of 23 and
completed at age 33, his commentary on the Mishna, "Kitab al-Siraj", written in
Arabic. The Mishna is a summary of decisions in Jewish law that dates from
earliest times to the 3rd century (CE). While living in Fez, in 1165, Rabbi
Judah ibn Shoshan, with whom Moses had studied, was arrested as a Jewish person
practicing Judism, was found guilty and then executed. After this the Maimon
family moves to Palestine briefly and then to Egypt.

In Egypt, unlike other nations under Islam, Jewish people are free to practice
Judaism openly, but any Jewish human who had once accepted Islam might be put
to death if they go back to Judaism. Moses himself is at one time accused of
being a reconverted Muslim, but is able to prove that he had never actually
accepted Islam.

In Egypt, Maimonides is influenced by Arabic writers such as Ibn Rushd and
Al-Ghazali.

After his commentary on the Mishna, Maimon spends ten years writing "Mishne
Torah" ("The Torah Reviewed"), the code of Jewish law written in a clear Hebrew
style. This code offers a brilliant systematization of all Jewish law and
doctrine. Maimon also writes two minor works on Jewish law: the "Sefer
ha-mitzwot" (Book of Precepts), a digest of law for average people, written in
Arabic; and the "Hilkhot ha-Yerushalmi" ("Laws of Jerusalem"), a digest of the
laws in the Palestinian Talmud, written in Hebrew.

After practicing as a physician, Miamon's popularity grows. Maimon is the
physician to Saladin (who opposes Richard the Lion-Heart in the 3rd crusade).
Maimon rejects Richard the Lion-Heart's invitation to live in England choosing
Egypt (which Asimov described as the more civilized at this time).


In 1233, Rabbi Solomon, a religious zelot of Montpellier, in southern France,
gets church authorities to burn "The Guide for the Perplexed" as a dangerously
heretical book. Maimonides will come to be recognized as a (wise) Jewish
philosopher.

Maimonides' philosophic work, when translated into Latin, will influence
medieval Scholastic writers, and even later people, such as Benedict de Spinoza
and G.W. Leibniz. Maimonides' health writings are part of the hisory of health
science.
  
820 YBN
[1180 AD]
1150) Stern-mounted rudder used in europe. The oldest known depiction of a
stern-mounted rudder can be found on church carvings that date to around 1180.
As the size of ships and the height of the freeboards increased (a vessel's
side between waterline and gunwale), quarter-rudders became less satisfactory
and were replaced in Europe by the more sturdy stern-mounted rudders with
pintle (pin or bolt) and gudgeon (circular metal fitting attached to a rudder
so that the rudder can rotate) attachment from the 12th century.

  
820 YBN
[1180 AD]
1335) In 1213 Neckam will become the Abbot of Circencester.
  
820 YBN
[1180 AD]
5869)
(Notre Dame Cathedral) Paris, France  
816 YBN
[11/??/1184 AD]
1153) Start of the Inquisition.

The Inquisition starts when Pope Lucius III holds a synod at Verona, Italy,
creating the shockingly brutal law that burning is to be the official
punishment for heresy.

Pope Lucius II starts the medieval Inquisition to repress and punish people for
heresy (heretics).
At the Synod of Verona in 1184, Pope Lucius III, in agreement with the
Holy Roman emperor Frederick I Barbarossa, initiates the "Inquisition", by
declaring the excommunication of heretics and their protectors. This requires
bishops to make a judicial inquiry or inquisition, for heresy in their
dioceses. After ecclesiastical trial, heretics who refuse to recant are to be
transferred to civil authorities for punishment—usually death by burning.

The Inquisition will brutally try to enforce belief in religion and slow
progress in science for centuries, murdering many thousands of people, in
particular science and truth loving people, before ending.

The Inquisition lasts until the 1800s.
Verona, Italy  
805 YBN
[1195 AD]
1331)
Lucena, Spain  
798 YBN
[1202 AD]
1393) Little is known about the life of Fibonacci. Leonardo's father,
Guglielmo, a Pisan merchant, was appointed consul over the community of Pisan
merchants in the North African port of Bugia (now Bejaïa, Algeria) and
Leonardo was sent to study calculation with an Arab master. Leonardo later went
to Egypt, Syria, Greece, Sicily, and Provence, where he studied different
numerical systems and methods of calculation.

The first seven chapters of "Liber Abaci" explain the principle of place value,
how the position of a figure determines whether it is a unit, 10, 100, etc.,
and demonstrating the use of the numerals in arithmetical operations. The
techniques are then applied to practical problems such as profit margin,
barter, money changing, conversion of weights and measures, partnerships, and
interest. Most of the work is devoted to speculative mathematics-proportion
(represented by such popular medieval techniques as the Rule of Three and the
Rule of Five, which are rule-of-thumb methods of finding proportions), the Rule
of False Position (a method by which a problem is worked out by a false
assumption, then corrected by proportion), extraction of roots, and the
properties of numbers, concluding with some geometry and algebra.



French-born mathematician Albert Girard will represent this series with a
formula in 1634: un + 2 = un + 1 + un, in which u represents the term and the
subscript its rank in the sequence.
The mathematician Robert Simson at the University of
Glasgow in 1753 will note that the as the numbers increase, the ratio between
succeeding numbers approaches the number a, the golden ratio, 1.6180. The
golden ratio is defined as the ratio that results when a line is divided so
that the whole line has the same ratio to the larger segment as the larger
segment has to the smaller segment. Expressed algebraically, normalising the
larger part to unit length, it is the positive solution of the equation:

x 1
- = ---
1 x-1

or equivalently x2-x-1=0,

1 + √5
which is equal to φ = ------ =
1.618033988749894848204586834366...
2

In the 1800s scientists will find Fibonacci-type sequences in nature; for
example, in the spirals of sunflower heads, in pine cones, in the regular
descent (genealogy) of the male bee, in the related logarithmic (equiangular)
spiral in snail shells, in the arrangement of leaf buds on a stem, and in
animal horns.

Asimov describes Fibonacci as the first great Western mathematician after the
end of Greek science.
Fibonacci will be presented to Holy Roman Emperor Federick II in
1225, because Fibonacci is recognized for learning.
For several years Leonardo
corresponded with Frederick II and his scholars, exchanging problems with them.
Pisa, Italy (guess based on:)  
791 YBN
[1209 AD]
1342) Cambridge and Oxford will have a long history of competition with each
other.
Cambridge, England  
788 YBN
[1212 AD]
1343)
Valladolid province of the autonomous region of Castile-Leon,in northern
Spain.  
785 YBN
[06/15/1215 AD]
1520) The anti-Jewish religious and racist prejudice of Christian people in
this time is evident in clause 11, "And if anyone dies indebted to the Jews,
his wife shall have her dower and pay nothing of that debt..."

In addition, the reality of slavory is evident in clause 27, "If any free man
dies without leaving a will, his chattels shall be distributed by his nearest
kinsfolk and friends under the supervision of the church...".

However, some rights are gained by women, for example clause 8, "No widow shall
be forced to marry so long as she wishes to live without a husband..."
Runnymede, England  
785 YBN
[1215 AD]
1154)
  
782 YBN
[1218 AD]
1344)
Salamanca, west of Madrid, Spain  
780 YBN
[1220 AD]
1345)
Montpellier in the Languedoc-Roussillon région of the south of France.  
780 YBN
[1220 AD]
1394)
Pisa, Italy (guess)  
780 YBN
[1220 AD]
3134) The minute larval insects fasten in myriads on the young shoots, and,
inserting their long proboscides into the bark, draw their nutriment from the
sap of the plant. The insects begin at once to exude the resinous secretion
over their entire bodies; this forms in effect a cocoon. A continuous hard
resinous layer regularly honeycombed with small cavities is deposited over and
around the twig. From this living tomb the female insects, which form the great
bulk of the group, never escape. After their impregnation, which takes place on
the liberation of the males, about three months from their first appearance,
the females develop into a singular amorphous organism consisting in its main
features of a large smooth shining crimson-colored sac - the ovary - with a
beak stuck into the bark, and a few papillary (pipillae are small nipplelike
projections) processes projected above the resinous surface. The red fluid in
the ovary is the substance which forms the lac dye of commerce. To obtain the
largest amount of both resin and dye-stuff it is necessary to gather the twigs
with their living inhabitants in or near June and November. Lac encrusting the
twigs as gathered is known in commerce as "stick lac"; the resin crushed to
small fragments and washed in hot water to free it from coloring matter is
"seed lac"; and this, when melted, strained through thick canvas, and spread
out into thin layers, is known as "shellac", and is the form in which the resin
is usually brought to European markets. Shellac varies in color from a dark
amber to an almost pure black.
Spain  
778 YBN
[1222 AD]
1346)
Padua, Italy  
776 YBN
[06/05/1224 AD]
1347)
Naples, Italy  
775 YBN
[1225 AD]
1395) "Liber quadratorum" is devoted entirely to Diophantine equations of the
second degree (equations that contain squares). The "Liber quadratorum" is
considered Leonardo's masterpiece. "Liber quadratorum" is a systematically
arranged collection of theorems, many invented by Fibonacci, who used his own
proofs to work out general solutions.
Although the "Liber abaci" will be more
influential and of wider scope, "Liber quadratorum" alone ranks Leonardo as the
major contributor to number theory between Diophantus and the 1600s French
mathematician Pierre de Fermat.
Pisa, Italy (guess)  
773 YBN
[1227 AD]
1400) Scot is a believer in and writes works on astrology.
Sicily  
772 YBN
[1228 AD]
1392) Theory that all matter is made of light published by Robert Grosseteste
(GrOSTeST), (CE c1175-1253)

In "De Luce", Grossteste writes "Lux est ergo prima forma corporalis.", "Light
is therefore the first corporeal (material) form".

Grossetest brings in scholars from the Byzantine Empire to translate works from
the original Greek.

Interested in optics, Grosseteste performs experiments with mirrors and lenses
using al-Haytham's (Alhazen's) writings as a guide.

In "De Iride" ("On the rainbow") Grosseteste writes:
"This part of optics, when well
understood, shows us how we may make things a very long distance off appear as
if placed very close, and large near things appear very small, and how we may
make small things placed at a distance appear any size we want, so that it may
be possible for us to read the smallest letters at incredible distances, or to
count sand, or seed, or any sort or minute objects."

Gresseteste's work in optics will be continued by his student Roger Bacon.

In "De Luce" Grosseteste reveals his awareness of atomic theory writing:
"It is
my opinion that this was the meaning of the theory of those philosophers who
held that everything is composed of atoms, and said that bodies are composed of
surfaces, and surfaces of lines, and lines of points."

Grossetest introduces Aristotle to Europe.
Lincoln, England (where de luce is written)  
771 YBN
[1229 AD]
1348)
Toulouse, France  
770 YBN
[1230 AD]
1158) Pope Gregory IX authorizes the killing of witches.

Rome, Italy  
767 YBN
[1233 AD]
1396) Albertus was the eldest son of a wealthy German lord. After his early
schooling, he went to the University of Padua, where he studied the liberal
arts. He joined the Dominican order at Padua in 1223. He continued his studies
at Padua and Bologna and in Germany and then taught theology at several
convents throughout Germany, lastly at Cologne.

Because of his learning, Albertus is suspected of wizardry.
Albertus is called "the
Bishop with the Boots" and the "Ape of Aristotle".
Albertus is the bishop of Regensburg
from 1260-1262.

In the summer of 1248, Albertus will be sent to Cologne to organize the first
Dominican studium generale ("general house of studies") in Germany. Albertus
will preside over this house until 1254 and devote himself to a full schedule
of studying, teaching, and writing. During this period Albertus' main disciple
will be Thomas Aquinas, who will return to Paris in 1252. The two men maintain
a close relationship even though doctrinal differences exist.

In 1277 he traveled to Paris to uphold the recently condemned good name and
writings of Thomas Aquinas, who had died a few years before, and to defend
certain Aristotelian doctrines that both he and Thomas held to be true.

Albertus, like most humans in this time have many flaws including, most likely
believing in a diety, believing most of the lies of the Christian religion,
believing astrology, and that stones have occult properties (in "De
mineralibus").
Paris, France  
766 YBN
[1234 AD]
1125)
Korea  
766 YBN
[1234 AD]
1399) Although of German descent, Frederick prefers to live in Sicily.
At age fourteen
Frederick marries a twenty-five-year-old widow named Constance, the daughter of
the king of Aragon. Both seem to have been happy with the arrangement, and
Constance bears Frederick a son, Henry.
Instead of killing the Saracens of Sicily,
Frederick allows them to settle on the mainland and build mosques. Frederick
also enlists them in his Christian army and even into his personal bodyguards.
As Muslim soldiers, they have the advantage of immunity from papal
excommunication. For these reasons, among others, Frederick II will be listed
as a representative member of the sixth region of Dante's Inferno, The Heretics
who are burned in tombs.
Frederick writes poetry and is a patron of the Sicilian
School of poetry. Frederick's royal court in Palermo, from around 1220 to his
death, sees the first use of a literary form of an Italo-Romance language,
Sicilian. The school and its poetry will be well known to Dante and his peers
and will have a significant influence on the literary form of what was
eventually to become the modern Italian language.
Pope Gregory IX, excommunicates
Frederick II for failing to carry out a crusade to Jerusalem. Frederick
obtained Jerusalem, Bethlehem, and Nazareth from the Sultan al-Kamil of Egypt
nonviolently through negociation.
Sicily  
760 YBN
[1240 AD]
1349)
Siena, Tuscany, Italy  
758 YBN
[1242 AD]
1403)
Oxford, England  
757 YBN
[1243 AD]
1156) Jewish humans are burned at the stake by Christian humans for "host
nailing", that is the Jewish humans are accused of hammering nails through the
"host" or wafer given to Christian people to eat during a Christian service as
a symbol of Jesus.

?  
752 YBN
[1248 AD]
1397)
Cologne  
748 YBN
[05/15/1252 AD]
1157) Pope Innocent IV authorizes torture. "Ad exstirpanda" is the the opening
line designating a papal bull (a public letter in legal form) issued on May 15,
1252, by Pope Innocent IV, which will be confirmed by Pope Alexander IV in
1259, and by Pope Clement IV in 1265. This papl bull explicitly authorizes the
use of torture for eliciting confessions from heretics during the Inquisition
and explicitly condones the practice of executing relapsed heretics by burning
them alive. The bull gives to the State a portion of the property to be
confiscated from convicted heretics. The State in return assumes the burden of
carrying out the penalty.

Rome, Italy  
748 YBN
[1252 AD]
1416) The Tables of Toledo are the most accurate compilation of
astronomical/astrological data (ephemeris) ever seen in Europe at this time.
The Tables were partly the work of Al-Zarqali, known to the West as Arzachel, a
mathematician and astronomer/astrologer who flourished in Cordoba in the 1000s.
Gerard of Cremona (1114â€"1187) edited the Tables of Toledo for Latin
readers.

The tables will not be widely known until a Latin version is prepared in Paris
in the 1320s. Copies will rapidly spread throughout Europe, and for more than
two centuries the Alfonsine Tables will be the best astronomical tables
available. First printed in 1483, the Alfonsine Tables will be an important
source of information for the young Nicolaus Copernicus before his own work
superseded them in the 1550s.

Alfonso X commissioned or co-authored numerous works during his reign. These
works included Cantigas d'escarnio e maldicer, General Estoria and the Libro de
los juegos ("Book of Games").
Castile, Spain  
745 YBN
[1255 AD]
1159) In England, 18 Jewish people are tortured and hanged for sacrificing
children.

England  
741 YBN
[1259 AD]
1412)
in Maragheh (now in Azerbaijan)  
739 YBN
[1261 AD]
1842)
?, China (presumably)  
737 YBN
[1263 AD]
1417) Alderotti is physician to Pope Honorius IV.
Alderotti studies in Bologna
(which, according to Asimov has one of the best health schools (medical school)
in western Europe) and in lectures there in 1260.
Dante mentions him in The
Divine Comedy as a Hippocratist, or follower of Hippocrates.
Bologna, Italy  
735 YBN
[01/20/1265 AD]
1525) Simon de Montfort and most of his followers will be killed a few months
later on Aug. 4, 1265, by Edward I, Kind Henry III's son and future king of
England.
Rome, Italy  
735 YBN
[1265 AD]
1418) Aquinas was sent to the University of Naples, recently founded by the
emperor, where he first encountered the scientific and philosophical works that
were being translated from Greek and Arabic. In this setting Thomas decided to
join the Friars Preachers, or Dominicans, a new religious order founded 30
years earlier, which departed from the traditional paternalistic form of
government for monks to the more democratic form of the mendicant friars
(religious orders whose poverty made it necessary for them to beg alms) and
from the monastic life of prayer and manual labour to a more active life of
preaching and teaching.

In 1245 Aquinas studied at the University of Paris, the most prestigious and
turbulent university of the time. Aquinas went to Paris to the convent of
Saint-Jacques, the great university centre of the Dominicans, and there studied
under Albertus Magnus, a tremendous scholar with a wide range of intellectual
interests.

The logic of Aquinas's position regarding faith and reason requires that the
fundamental consistency of nature be recognized. In the universe or nature
there are laws that describe its operation. Recognizing this fact permits the
construction of a science according to a logos (“rational
structure”). Opponents under the influence of Augustine's doctrines assert
the necessity and power of grace for a nature polluted by sin. This new view
therefore upsets them. This idea that the universe is controlled by laws of
nature leaves the question of where a diety might be located and involved. For
many modern people a diety is everywhere influencing everything either obeying
or disobeying the laws of nature, for others a diety is only responsible for
the creation of the universe, for some there are many dieties, and of course
some people reject the theory that any gods exist.

In January 1274 Thomas Aquinas is be personally summoned by Gregory X to the
second Council of Lyons, which is an attempt to repair the schism between the
Latin and Greek churches. On his way Aquinas is stricken by illness; he stops
at the Cistercian abbey of Fossanova, where he died on March 7. In 1277 the
masters of Paris, the highest theological jurisdiction in the church, condemn a
series of 219 propositions; 12 of these propositions are theses of Aquinas.
This is the most serious condemnation possible in the Middle Ages and its
repercussions are felt in the development of science for several centuries.
Thomas
Aquinas will be canonized a saint in 1323.

Aquinas' philosophical treatistes are:
"De ente et essentia" (before 1256; On Being
and Essence, 1949); "Contra impugnantes Dei cultum et religionem" (1256; An
Apology for the Religious Orders, 1902); "De regno" (De regimine principum) "ad
regem Cypri" (1266; On Kingship, 1949); "De perfectione vitae spiritualis"
(1269â€"70); "De unitate intellectus contra Averroistas" (1270; The Unicity
of the Intellect, 1946); "De aeternitate mundi contra murmurantes"
(1270â€"72); "De substantiis separatis, seu de angelorum natura" (undated;
Treatise on Separate Substances, 1959).
Paris, France  
733 YBN
[1267 AD]
1401) Bacon was born into a wealthy family. His parents are employed by King
Henry III. Bacon was well-versed in the classics and enjoyed the advantages of
an early training in geometry, arithmetic, music, and astronomy.
Bacon studied and later
became a Master at Oxford, lecturing on Aristotle.
Sometime between 1237 and 1245, Bacon
starts to lecture at the University of Paris, the center of intellectual life
in Europe at this time.
Bacon obtains a Master of arts degree, at the university of
Paris by 1241 and resigns in 1247 to devote himself to research. This new
interest in science and experiment is probably caused by his return to Oxford
and the influence there of the great scholar Robert Grosseteste, a leader in
introducing Greek learning to the West, and Grosseteste's student Adam de
Marisco, and Thomas Wallensis, the bishop of St. David's.

Around 1256 Bacon becomes a Friar in the Franciscan Order. As a Franciscan
Friar, Bacon no longer holds a teaching post and after 1260, his activities are
further restricted by a Franciscan statute forbidding Friars from publishing
books or pamphlets without specific approval.
Bacon circumvents this restriction through
his acquaintance with Cardinal Guy le Gros de Foulques, who becomes Pope
Clement IV in 1265. The new Pope issues a mandate ordering Bacon to write him
concerning the place of philosophy within theology. As a result Bacon sends the
Pope his "Opus maius", which presents Bacon's views on how the philosophy of
Aristotle and the new science can be incorporated into a new Theology. Besides
the "Opus maius" Bacon also sends his "Opus minus", "De multiplicatione
specierum", and, perhaps, other works on alchemy and astrology.
Oxford, England  
732 YBN
[1268 AD]
1147)
China  
731 YBN
[08/08/1269 AD]
1420) Peregrinus is a friend of Roger Bacon.
Peregrinus is an engineer in army of
Louis IX.
Peregrinus thinks that the compass needle points to the celestial sphere,
the outermost spheres in Ptolemy's erroneous system.
People initially did not connect
magnetism and electricity, giving each word a different suffix instead of the
same: "magnetity" or "electrism".

Peter's magnetic experiments and instruments in his letter apparently date to a
time period twenty years earlier, judging by references in several works of
Bacon.

The name Peregrinus ("pilgrim") suggests that Peregrinus may have also been a
crusader.

Peregrinus' disciple, Roger Bacon, pays the highest tribute to Peregrinus as an
experimenter and technician in his "Opus tertium" and other works (in which
Peter is called "Petrus de Maharncuria Picardus"). According to Bacon,
Peregrinus is a recluse who devotes himself to the study of nature, is able to
work metals, invents armour and provides assistance more valuable to Louis IX
of France than the king's entire army.

"De magnete" will became a very popular work from the Middle Ages onwards. In
1326, Thomas Bradwardine will quote it in his "Tractatus de proportionibus".
Scholars at Oxford University will make frequent use of it. The first edition
of the letter will be issued at Augsburg, in 1558, by Achilles Gasser.

William Gilbert will acknowledge his debt to Peter of Maricourt and
incorporates this 1200s scientist's experiments on magnetism into his own
treatise, called "De magnete".

Here we see the major centers for the earliest European scientific progress are
Italy, France and England as the transition from the Arab nations leading in
science happens.
Lucera, Italy  
730 YBN
[12/??/1270 AD]
1405) This Condemnation represents a clear and official censorship of free
speech, and free thought in addition to the censorship of scientific and other
writings.
Paris, France  
725 YBN
[1275 AD]
1419) Villanova can speak Arabic and Greek.
Villanova is given a castle and a
professorship at the University of Montpellier in France as a result of
treating royal people.
Villanova is probably of Catalan origin, and studied chemistry,
medicine, physics, and also Arabic philosophy. After having lived at the court
of Aragon, he goes to Paris, where he gains a considerable reputation; but
angers the ecclesiastics and is forced to move, which he does to Sicily. About
1313 he was summoned to Avignon by Pope Clement V, who was ill, but Villanova
dies on the voyage.
Paris, France  
723 YBN
[1277 AD]
1398) Albertus Magnus (Albert the great) (1193-1280) In 1277 he travels to
Paris to uphold the recently condemned good name and writings of Thomas
Aquinas, who had died a few years before, and to defend certain Aristotelian
doctrines that both he and Thomas held to be true.

Paris, France  
723 YBN
[1277 AD]
1404)
Oxford, England  
723 YBN
[1277 AD]
1406)
Paris, France  
720 YBN
[1280 AD]
5873)
Cologne, Germany  
720 YBN
[1280 AD]
6238)
Florence, Italy  
719 YBN
[1281 AD]
1413)
Maragha, Iran  
716 YBN
[1284 AD]
5884) The most famous of the secular plays "Jau de Robin et de Marion" is
written around this time by Adam de le Halle (CE c1250-c1306), the last and
greatest of the trouveres, a poet, musician and innovator of the earliest
French secular theatre. "Jeu de Robin et de Marion" ("A game of Robin and of
Marion") is a dramatization of the pastoral theme of a knight’s wooing of a
pretty shepherdess, with dances and peasants’ dialogue.

Picardy, France  
715 YBN
[1285 AD]
1160) In Munich, 180 Jewish people are burned {to death} after being accused of
bleeding a Christian child to death.

Munich  
710 YBN
[1290 AD]
1350)
Coimbra, Portugal  
703 YBN
[1297 AD]
1422) D'Abano studied a long time at Paris, where he was promoted to the
degrees of Doctor in philosophy and physics. D'Abano's fees as a physician are
reported to be very high.

D'Abano meets Marco Polo.
D'Abano believes in astrology and is suspected of magical
practices, in particular by competing physicians.
After his death, D'Abano is found guilty
and his body is ordered to be exhumed and burned, but a friend secretly removes
it, and the Inquisition has to content itself with the public proclamation of
its sentence and the burning of Abano in effigy as a bundle of straw
representing his person publicly burnt at Padua.

There is a long history of the shockingly brutal execution by fire. There are
reports of Roman authorities murdering Christian martyrs by burning, and the
Roman Emperor Justinian orders death by fire as a punishment for heresy against
Christianity. The burning the D'Abano in effigy is an early report of the
increased efforts to stop the advance of freethinking being nutured in the
Universities in Europe from the reading of ancient Greek and Arabic texts.
Padua, Italy  
702 YBN
[05/15/1298 AD]
1161) In Nuremberg 628 Jewish humans are killed (including scholar Mordecai ben
Hillel) because of a rumor of host nailing.

Nuremberg  
702 YBN
[1298 AD]
1162) The Tower Mill windmill is invented in Europe. A Tower Mill is a type of
windmill which consists of a brick or stone tower, on top of which sits a roof
or cap which can be turned to bring the sails into the wind.

Nuremberg  
702 YBN
[1298 AD]
1421) Although he knew little or no Chinese, he did speak some of the many
languages then used in East Asia- most probably Turkish (in its Coman dialect)
as spoken among the Mongols, Arabized Persian, Uighur (Uygur), and perhaps
Mongol. He was noticed very favourably by Kublai, who took great delight in
hearing of strange countries and repeatedly sent him on fact-finding missions
to distant parts of the empire.

According to Marco's travel account, the Polos ask several times for permission
to return to Europe but the Khan will not agree to their departure. Sometime
around 1292, a Mongol princess is to be sent to Persia to become the consort of
Arghun Khan, and the Polos offer to accompany her. Marco writes that Kublai had
been unwilling to let them go but finally granted permission. They are eager to
leave, in part, because Kublai is nearly 80, and his death (and the consequent
change in regime) might be dangerous for a small group of isolated foreigners.
The Polos also wanted to see their native Venice and their families again.

The princess, with some 600 courtiers and sailors, and the Polos board 14
ships, which leave the port of Quanzhou and sail southward. On the island of
Sumatra ("Lesser Giaua") Polo is impressed by the fact that the North Star
appears to have dipped below the horizon. The fleet follows the west coast of
India and finally anchored at Hormuz. The expedition then proceeds to Khorasan,
handing over the princess not to Arghun, who had died, but to his son Mahmud
Ghazan.

The Polos then depart for Europe and eventually returned to Venice. Soon after
his return to Venice, Polo is taken prisoner by the Genoese, rivals of the
Venetians at sea, during a battle in the Mediterranean. He was then imprisoned
in Genoa. In prison, Marco Polo dictates his adventures to a prisoner from
Pisa, Rustichello, who writes the story in Franco-Italian, a composite tongue
fashionable during the 1200 and 1300s. The original title of the book is
"Divisament dou monde" ("Description of the World"). Polo is soon freed and
returns to Venice.

"Il milione" is an instant success, "In a few months it spread throughout
Italy," Giovanni Battista Ramusio, the 16th-century Italian geographer will
write. There are around 140 different manuscript versions of the text, in three
manuscript groups, in a dozen different languages and dialects.
Genoa, Italy  
700 YBN
[1300 AD]
1121) Earliest mechanical clock.

Time keeping began around 3500 BC with the invention of the gnomon and sundial,
and the hourglass.

The first mechanical clocks in Europe work based on a simple principle. A
weight is suspended from a cord wrapped many times around a driving shaft. As
the weight descends the shaft turns and the movement is transmitted to the
hands, or in many cases just a single hour hand. To regulate the movement so
that the hands rotate at a fixed rate, using an escapement which consists of a
pair of oscillating vanes mounted on a vertical spindle carrying a protruding
pallet that engages with the teeth of a crown wheel. Some regulation of the
rate of oscillation of the vanes is possible through a series of sliding
weights on each arm. One of the oldest surviving examples of this kind of clock
is that from Salisbury Cathedral, which dates to 1386, but does not have its
original escapement. These are weigh-driven clocks. Spring driven clocks do not
appear until the middle of the 1400s.In the 1600s Christiaan Huygens will
invent the pendulum escapement (1657) for weight-driven clocks and the balance
spring (1675) for spring-driven clocks. Only then will putting a minute hand on
a clock be useful.

The first publicly known battery electric clock is invented in 1840. This clock
is driven by a spring and pendulum and uses an electrical impulse to operate a
number of dials. Not until 1906 is the first self-contained battery-driven
clock invented and made public.
Europe  
700 YBN
[1300 AD]
5874)
Florence, Italy  
697 YBN
[1303 AD]
1351)
Coimbra, Portugal  
692 YBN
[09/08/1308 AD]
1352)
Perugia, Italy  
690 YBN
[10/24/1310 AD]
356)
London, England  
690 YBN
[10/24/1310 AD]
656)
London, England  
690 YBN
[10/24/1310 AD]
657)
London, England (presumably)  
690 YBN
[1310 AD]
357)
London, England (presumably)  
690 YBN
[1310 AD]
1424) False Geber probably lives in Spain. (Arab person?).

False-Jabir wrongly assumes that all metals are composed of sulfur and mercury
and gives detailed descriptions of metallic properties in those terms.
False-Jabir also explains the use of an elixir in transmuting base metals into
gold.
Spain  
690 YBN
[1310 AD]
4540)
London, England (presumably)  
688 YBN
[1312 AD]
363)
London, England (presumably)  
688 YBN
[1312 AD]
4539)
London, England (presumably)  
684 YBN
[1316 AD]
1428) De' Luzzi registered at the College of Medicine of the University of
Bologna in 1290 and also is known to have studied in the College of Philosophy.

De' Luzzi lectures while actively practicing health and surgery.

De' Luzzi studies at the health (medical) school in Bologna under Alderotti,
graduates in 1290 and starts teaching there in 1306.

The first such recorded anatomical exploration occurred for legal reasons at
Bologna in 1302, but it is generally believed that academic dissections had
been performed previously. In any event, Mondino reports that in January 1315
he conducted such a procedure on the body of a woman, giving him the
opportunity to examine and study human uterine anatomy.

Asimov writes that the 1300s are a turning point between a focus on religion
and the afterlife to an interest in humans and the earth, which is called
"humanism" and is the beginning of the Renaissance.
Bologna, Italy  
683 YBN
[1317 AD]
1427) Ockham is opposed to Thomas Acquinas' view that logic and religion can
coexist, arguing that religion is a matter of faith.
Ockham studies at Oxford and
lectures there from 1315-1319.
Ockham was young when he entered the Franciscan order.
At the
University of Oxford Ockham apparently between 1317 and 1319 lectures on the
Sentences of Peter Lombard, a 1100s theologian whose work was the official
textbook of theology in the universities until the 1500s. Ockham's lectures are
also set down in written commentaries, of which the commentary on Book I of the
Sentences (a commentary known as "Ordinatio") was actually written by Ockham
himself.
Ockham's opinions aroused strong opposition from members of the theological
faculty of Oxford and Ockham left the university without obtaining his master's
degree in theology. Ockham therefore remains, academically speaking, an
undergraduate, known as an "inceptor" ("beginner") in Oxonian language or, to
use a Parisian equivalent, a "baccalaureus formatus".
In 1327 The Franciscan
General Michael of Cesena is summoned to Avignon to answer charges of heresy,
and asks Ockham to review arguments surrounding Apostolic poverty. The
Franciscan order believed that Jesus and his apostles owned no personal
property, and survived by begging and accepting the gifts of others. This
clashes directly with the beliefs of Pope John XXII.
On May 26, 1328, the Franciscan
General Michael of Cesena flees from Avignon accompanied by Bonagratia and
William Ockham. The three Franciscans stay in Pisa under the protection of
Emperor Louis IV the Bavarian, who had been excommunicated in 1324 and
proclaimed by John XXII to have forfeited all rights to the empire. Because of
this Ockham is excommunicated.

In Munich in 1330 and thereafter Ockham writes fervently against the papacy in
defense of the strict Franciscan notion of poverty.
Oxford, England  
680 YBN
[1320 AD]
5870)
(Royal Court) Paris, France (verify)  
675 YBN
[1325 AD]
5887)
(Abbey of) Robertsbridge, Sussex, UK  
673 YBN
[1327 AD]
1164) Wallingford studies at Oxford University for 6 years and becomes a monk
at St Albans Abbey in Hertfordshire before 9 years further study at Oxford. In
1326, he becomes the abbot of St Albans.
Wallingford's design of an astronomical clock
is described in "Tractatus Horologii Astronomici", in 1327. The clock will be
completed in 1356 about 20 years after his death by William of Walsham, but
will be apparently destroyed during Henry VIII's reformation and dissolution of
St Albans Abbey in 1539.
Richard also designs and constructs a calculation device
known as an equatorium, which he calls an Albion. This can be used for
astronomical calculations such as lunar, solar and planetary longitudes and can
predict eclipses. This is described in "Tractatus Albionis". He publishes other
works on trigonometry, celestial coordinates, astrology and various religious
works.

He suffers from what is then thought to be leprosy (though it may be syphilis,
scrofula or tuberculosis) apparently contracted when he goes to have his
position confirmed by the Pope at Avignon. He dies at St Albans.
Hertfordshire, England  
673 YBN
[1327 AD]
1353)
Timbuktu, Mali, West Africa  
665 YBN
[1335 AD]
1354) Nobel Prize winner Santiago Ramón y Cajal, often considered to be the
Father of Neurosciences, will be taught at the University of Zaragosa.
Zaragosa, Spain  
665 YBN
[1335 AD]
1425) After studies in philosophy at the University of Paris under William of
Ockham, Buridan is appointed professor of philosophy there. Buridan serves as
university rector in 1328 and in 1340, the year in which he condemns Ockham's
views, an act that is sometimes called the first seed of theological
skepticism. Buridan's own works will be condemned and placed on the Index of
Forbidden Books from 1474 to 1481 by partisans of Ockham.

In addition to commentaries on Aristotle's "Organon", "Physics", "De anima",
"Metaphysics", and "Economics", Buridan's works include "Summula de dialecta"
(1487) and "Consequentie" (1493).

Buridan remains a secular cleric, rather than joining a religious order.
Paris, France  
664 YBN
[1336 AD]
1355)
Camerino, Italy  
657 YBN
[09/03/1343 AD]
1356) Galileo Galilei, will be born and study in Pisa, becoming professor of
Mathematics at the Pisan Studium in 1589.
Pisa, Italy  
652 YBN
[04/07/1348 AD]
1357)
Prague, Czech Republic (EU)  
652 YBN
[1348 AD]
1169) Christian people, unaware of the true cause of the bubonic plague, accuse
Jewish people of poisoning the wells, and thousands of innocent Jewish people
are killed. For example, in Speyer, Germany Jewish bodies are piled into huge
wine casks and sent floating down the Rhine. In Basal, Switzerland, 600 Jewish
people are burned for well poisoning.

Bubonic plague is caused by the enterobacteria Yersinia pestis.

Speyer, Germany and Basal, Switzerland  
650 YBN
[1350 AD]
1165) Giovanni Dondi dell'Orologio builds an astronomical clock in Padua.
Dondi's
clock is a seven-sided construction showing the positions of the known planets
as well. Both these clocks, and others like them, are probably less accurate
than their designers wanted: the gear ratios may be exquisitely calculated, but
the realities of friction and limitations of manufacture would prevent them
from being accurate and reliable.

Padua, Italy  
650 YBN
[1350 AD]
1168)
Mediterranean  
650 YBN
[1350 AD]
5886)
France  
648 YBN
[1352 AD]
1402)
Italy  
645 YBN
[1355 AD]
1980)
Paris, France   
640 YBN
[1360 AD]
1977) The fact that Oresme attends the royally sponsored and subsidized College
of Navarre, an institution for students too poor to pay their expenses while
studying at the University of Paris, makes it probable that Oresme comes from a
peasant family.

Oresme studies arts in Paris (before 1342), together with Jean Buridan (the
so-called founder of the French school of natural philosophy), Albert of Saxony
and perhaps Marsilius of Inghen, and there receives the Magister Artium. A
recently discovered papal letter of provision granting Oresme an expectation of
a benefice establishes that he was already a regent master in arts by 1342.
This early dating of Oresme's arts degree places him at Paris during the crisis
over William of Ockham's natural philosophy.

Oresme is a determined opponent of astrology, which he criticizes on religious
and scientific grounds.
Paris, France (presumably)  
639 YBN
[1361 AD]
1358)
Pavia, Itlay  
636 YBN
[1364 AD]
1359) Nicolaus Copernicus will attend this university.
  
636 YBN
[1364 AD]
5885) Guillaume de Machaut (CE c1300-1377), one of the leading French composers
of the Ars Nova musical style of the 1300s, composes "La Messe De Notre Dame",
one of the earliest masses, and best known composition of the age.

(Gothic cathedral) Rheims, France  
635 YBN
[03/12/1365 AD]
1360)
Vienna, Austria  
633 YBN
[03/12/1367 AD]
1361)
Pécs, Hungary  
630 YBN
[1370 AD]
1978)
Paris, France (presumably)  
623 YBN
[1377 AD]
1213) The Bethlem Royal Hospital of London, which was built in 1247 originally
as a priory (or monastary) for those in the "order of the Star of Bethlehem",
starts imprisoning people thought to be mentally ill this year in 1377, and is
the earth's first psychiatric hospital. The word "bedlam" meaning a scene of
uproar or confusion, will derive from Bethlem.
In some way this begins the separation of
the legal and the psychiatric prison systems. This duality will result in those
jailed in psychiatric hospitals being subjected to physical restraint, torture,
violent and nonviolent people being mixed together indiscriminately,
unprotected by the writ of habeus corpus, the right to trial, to finite
sentence and other legal guarantees granted to people jailed in the legal
prison system. The origin of this dual system is from the belief in unusual
(even many times lawful) behavior requiring treatment, belief in many of the
abstract erroneous theories of psychology, in addition to the power of
tradition behind the belief in the punishment those with unorthodox views or
behavior (even as is many times the case, when those unorthodox views, for
example belief in the heliocentric system or atheism, are the more accurate and
healthy although unpopular). In addition, psychiatric hospitals will come to
serve as a primative (albeit brutal and unconsensual) social program, where a
bed and food are provided for people without a room of their own (so called
"homeless people").

This hospital-prison will become infamous for it's brutal treatment of those
imprisoned there. In the 1700s people will pay a penny to see the inmates and
are permitted to bring long sticks to poke the inmates with.

Prisoners are "treated" with bleedings, and nausia inducing substances (like
mercury) because the pain replaces the focus of the "insane" thoughts. Mustard
powders are put on the shaved head of prisoners causing blisters to cause pain
and discomfort, and also fear in the prisoners.

London, England  
623 YBN
[1377 AD]
1979)
Paris, France (presumably)  
621 YBN
[1379 AD]
1414) Khaldun writes an autobiography.
the castle Qal'at ibn Salamah, near what is now the town of Frenda,
Algeria  
614 YBN
[1386 AD]
1362)
Heidelberg, Germany  
609 YBN
[03/04/1391 AD]
1363)
Ferrara, Italy  
603 YBN
[1397 AD]
5897)
Padua, Italy  
602 YBN
[03/04/1398 AD]
1364)
(Myeongnyun-dong, Jongno-gu in central) Seoul and Suwon, South Korea  
600 YBN
[1400 AD]
1024)
  
600 YBN
[1400 AD]
1170) Although the carrack represents the state of the art in later medieval
shipbuilding, there were purposes for which it is not appropriate. Initially
carracks are used for exploration by the Portuguese venturing out along the
west African coast and into the Atlantic Ocean. But large, full-rigged ships
can not always be sailed with the precision necessary for inshore surveying in
unknown waters. The explorers soon come to prefer smaller carracks of around
100 tons, or the light three-masted Mediterranean lateen-rigged vessels known
as caravels.

Because of its smaller size the caravel is able to explore up river in shallow
coastal waters. With the lateen sails (triangular sails) affixed it is able to
go speedily over shallow water and take deep wind, while with the square
Atlantic-type sails attached, the caravel is very fast. Its economy, speed,
agility, and power makes the caravel esteemed as the best sailing vessel of
this time. It generally carried two or three masts with lateen sails, while
later types will have four masts.

Christopher Columbus will set out on his famous expedition in 1492 with the
Santa Maria, a small carrack which will serve as the mother ship, and the Pinta
and the Niña which are caravels.
Speyer, Germany and Basal, Switzerland  
600 YBN
[1400 AD]
5878)
(St. Jerome) England (verify)  
600 YBN
[1400 AD]
5891) Johannes Ciconia (CE c1370-1412) composes music.

Padua, Italy (guess)  
590 YBN
[1410 AD]
1365)
St. Andrews, Scotland  
583 YBN
[1417 AD]
1172) A single manuscript with a poem, "De Rerum Natura" (On the Nature of
Things), by Lucretius (c94 BCE- c49 BCE) is found. This is the only surviving
copy so far from from Lucretius' writings.

?  
580 YBN
[1420 AD]
1429) Henry is the younger son of King John I of Portugal, and great grandson
of Edward III of England.
Henry's designed a strategy where Christian Europe would
outflank Islam by establishing contact with Africa south of the Sahara and with
Asia. This strategy will not be brought to fulfillment until after his death.

In 1420, at the age of 26, Henry is made grand master of the Order of Christ,
the supreme order sponsored by the pope, which had replaced the crusading order
of the Templars in Portugal. While this did not oblige him to take religious
vows, it did oblige him to dedicate himself to a chaste and ascetic life. Henry
did not always refrain from worldly pleasures; as a young man he had fathered a
daughter without marriage (so-called illegitimate). The funds made available
through the order largely finance Henry's enterprise of discovery, which also
seeks to convert Pagans to Christianity, and for this reason all of Henry's
ships have a red cross on their sails.

From Italy Henry's older brother Prince Pedro brings home to Portugal, in 1428,
a copy of Marco Polo's travels that he had translated for Prince Henry's
benefit.

The voyages were made in very small ships, mostly the caravel, a light and
maneuverable vessel that used the lateen sail of the Arabs. Most of the voyages
sent out by Henry consisted of one or two ships that navigated by following the
coast, stopping at night to tie up along some shore.
One of his immediate aims was to
find an African gold supply to strengthen the Portuguese economy and to make
the voyages pay for themselves.
Nuno Tristão and Antão Gonçalves reach Cape
Blanco in 1441. The Portuguese sight the Bay of Arguin in 1443 and build an
important fort there around the year 1448. Dinis Dias soon comes across the
Senegal River and rounds the peninsula of Cap-Vert in 1444. By this stage the
explorers have passed the southern boundary of the desert, and from then on
Henry had one of his wishes fulfilled: the Portuguese had circumvented the
Muslim land-based trade routes across the western Sahara Desert, and slaves and
gold begin arriving in Portugal. By 1452, the influx of gold permits the
minting of Portugal's first gold cruzado coins. A cruzado is equal to 400 reis
at the time. From 1444 to 1446, as many as forty vessels sail from Lagos on
Henry's behalf, and the first private mercantile expeditions begin.

This return of slaves and gold silences the growing criticism that Henry was
wasting money on a profitless enterprise. Afonso V, the King of Protugal, gives
Henry the sole right to send ships to visit and trade with the Guinea coast of
Africa.

Henry's investment in exploration was so large that, despite his great
revenues, Henry will die heavily in debt.
Henry remains single to the end of his
life.

The surname Navigator will be applied to the Prince by the English, though
seldom by Portuguese writers. Henry himself never embarks on voyages of
discovery, but funded navigators, and for this Henry is regarded as the
initiator of the great age of discovery and the European thrust towards world
domination. Henry the Navigator is one of the first few humans to have the
actual day of their birth and death recorded and therefore remembered.
Lagos, Portugal  
580 YBN
[1420 AD]
1430) Ulugh Beg is the grandson of the Mongol warrier Tamerlane, the last of
the barbarian conquerers, succeeds to throne (of?) in 1447
Beg is the only important
scientist of the Mongol people.
Beg is killed by his son in 1449, and Ulugh's
observatory will be destroyed by 1500, its remains will be found in 1908.
The name
"Ulugh Beg" is a nick-name loosely translated as "Great Ruler".
Samarkand, Uzbekistan  
580 YBN
[1420 AD]
5888) John Dunstable (CE 1385-1453) composes music that represents the
transition between late medieval and early Renaissance music. Dunstable’s
influence on European music is seen in his flowing, gently asymmetrical rhythms
and, above all, in his harmonies. Dunstable represents a culmination of the
English tradition of full, sonorous harmonies based on the third and sixth that
persists through the 1300s alongside the more stark and dissonant style of
music on the European continent.

England (and possibly France)  
576 YBN
[1424 AD]
1431)
Samarkand, Uzbekistan  
575 YBN
[1425 AD]
1366)
Leuven, Belgium  
574 YBN
[1426 AD]
1173) A copy of the medical part of the 8 books of an encyclopedia describing
past Greek learning written in Latin by Celsus (25 BCE - 50 CE) is found.

?  
570 YBN
[1430 AD]
5889) Guillaume Dufay (CE c1400—1474) French composer, creates church and
secular music at this time.

(Cambrai cathedral) Cambrai, France (guess)  
570 YBN
[1430 AD]
5890) Gilles Binchois (CE c1400—1460) French composer, creates church and
secular music at this time.

(Chapel of Philip III the Good) Burgundy, France (guess)  
565 YBN
[1435 AD]
1435) Gutenberg will die in debt and unmarried.
When younger Guttenberg had acquired skill
in metalwork.
Exiled from Mainz in the course of a bitter struggle between the guilds of
that city and the patricians, Gutenberg moves to Strassburg (now Strasbourg,
France) probably between 1428 and 1430. Records put his presence there from
1434 to 1444. Gutenberg is involved in such crafts as gem cutting, and also
teaches crafts to a number of pupils.

In March 1434, a letter by him indicates that Guttenberg was living in
Strasbourg, where he had some relatives on his mother's side. He also appears
to have been a goldsmith member enrolled in the Strasbourg militia. In 1437,
there is evidence that he was instructing a wealthy tradesman on polishing
gems, but where he had acquired this knowledge is unknown. In 1436/37
Gutenberg's name also comes up in court in connection with a broken promise of
marriage to a woman from Strasbourg, Ennelin. Whether the marriage actually
took place is not recorded.

In 1438 a five-year contract is drawn up between Gutenberg and three other men:
Hans Riffe, Andreas Dritzehn, and Andreas Heilmann. When Andreas Dritzehn dies
at Christmas 1438, his heirs, trying to circumvent the terms of the contract,
began a lawsuit against Gutenberg in which they demanded to be made partners.
They lose the suit, but the trial reveals that Gutenberg is working on a new
invention. Witnesses testify that a carpenter named Conrad Saspach had advanced
sums to Andreas Dritzehn for the building of a wooden press, and Hans Dünne, a
goldsmith, declared that he had sold to Gutenberg, as early as 1436, 100
guilders' worth of printing materials. Gutenberg, apparently well along the way
to completing his invention, wants to keep secret the nature of the
enterprise.

In October 1448 Gutenberg is back in Mainz to borrow more money, which he
receives from a relative. By 1450 Gutenberg's printing experiments must have
reached a considerable degree of refinement, because Gutenberg is able to
persuade Johann Fust, a wealthy financier, to lend him 800 guilders, a very
large amount for which the tools and equipment for printing are to act as
securities. Two years later Fust makes another investment of 800 guilders for a
partnership in the enterprise. Fust and Gutenberg have a disagreement, Fust,
apparently, wants a safe and quick return on his investment, while Gutenberg
wants perfection instead of a quick return.

On November 6. 1455, the Helmaspergersches Notariatsinstrument (the
Helmasperger notarial instrument) records that Fust won a suit against
Guttenberg. This record is now in the library of the University of Göttingen.
Gutenberg was ordered to pay Fust the total sum of the two loans and compound
interest (probably totaling 2,020 guilders). The traditional belief is that
this settlement ruined Gutenberg, but more recent examination suggests that the
decision favored Gutenberg, allowing him to operate a printing shop through the
1450s and maybe into the 1460s.

The record of trial refers to the printing of books (werck der bucher), that
probably refer to the Forty-two-Line Bible That Gutenberg had probably
already printed by then. The sale of the Forty-two-Line Bible alone is
estimated to have produced many times over the sum owed Fust by Gutenberg, and
there is no other explanation as to why the books are not counted among
Gutenberg's property at the trial, except that Gutenberg sold the books.

After winning his suit, Fust gains control of the type (each page is kept
together with the blocks?) for the Bible and for Gutenberg's second
masterpiece, a Psalter (Psalms), and at least some of Gutenberg's other
printing equipment. Fust continues to print, using Gutenberg's materials, with
the assistance of Peter Schöffer, Fust's son-in-law, who had been Gutenberg's
most skilled employee and a witness against Gutenberg in the 1455 trial. The
first printed book in Europe to bear the name of its printer is a very nicely
designed "Psalter" completed in Mainz on August 14, 1457, which lists Johann
Fust and Peter Schöffer.

In January 1465 the archbishop of Mainz will pension Gutenberg, giving
Gutenberg an annual measure of grain, wine, and clothing and exempting
Gutenberg from certain taxes, so in his last years, Gutenberg was probably not
destitute.
Strassburg (now Strasbourg, France)  
565 YBN
[1435 AD]
1440) Alberti is a musician and organist, writes trajedies in Latin, and is a
mathematician.
Alberti designs some notable churches in Mantua and Romini.
Alberti is educated in law
at the University of Bologna.

Alberti writes in both Latin and the vernacular.
In Florence Alberti is friends with the
sculptor Donatello, cosmographer Paolo Toscanelli and the architect
Brunelleschi.

Some time between 1435 and 1444. Alberti writes "Libri della famiglia" ("Book
on the Family")-which discusses education, marriage, household management, and
money-in the Tuscan dialect. The work is not printed until 1843. Like Erasmus
decades later, Alberti stresses the need for a reform in education. He notes
that "the care of very young children is women's work, for nurses or the
mother," and that at the earliest possible age children should be taught the
alphabet. With great hopes, he gave the work to his family to read, but in his
autobiography Alberti confesses that "he could hardly avoid feeling rage, when
he saw some of his relatives openly ridiculing the work."

Alberti writes a short autobiography around 1438 in Latin and in the third
person, (many but not all scholars consider this work to be an autobiography)
in which he makes unlikely claims such as being capable of "standing with his
feet together, and springing over a man's head." The autobiography survives
thanks to a 1700s transcription by Antonio Muratori. Alberti also claims that
he "excelled in all bodily exercises; could, with feet tied, leap over a
standing man; could in the great cathedral, throw a coin far up to ring against
the vault; amused himself by taming wild horses and climbing mountains." This
may be explained in part because many in the Renaissance promote themselves in
various ways.

Alberti writes "Momus", between 1443 and 1450, which is a misogynist
(anti-women) comedy about the Olympian gods. Jupiter has been identified in
some sources as Pope Eugenius IV and Pope Nicholas V. Alberti borrows many of
its characters from Lucian, one of his favorite Greek writers. The name of its
hero, Momus, refers to the Greek word for blame or criticism. After being
expelled from heaven, Momus, the god of mockery, is eventually castrated.
Jupiter and the other gods come down to earth also, but they return to heaven
after Jupiter breaks his nose in a great storm.

Towards the end of his life, Alberti writes "De iciarchia" ("On the Man of
Excellence and Ruler of His Family") which represents in full flower the
public-spirited Humanism"
Florence, Italy  
563 YBN
[1437 AD]
1432)
Samarkand, Uzbekistan  
560 YBN
[02/12/1440 AD]
1437) Nicholas of Cusa (Nicholas Krebs) (CE 1401-1464) describes space as
infinite in size and that other stars may be inhabited.

The relevant translated text from "De Docta Ignorantia" Book 2 is:
"And so, {the
universe is} unbounded; for it is not the case that anything actually greater
than it, in relation to which it would be bounded, is positable."

Cusa suggests that stars may be distant Suns when he states that the Earth
would look like a star from a distance. Cusa writes: "Hence, if someone were
outside the region of fire, then through the medium of the fire our earth,
which is on the circumference of {this} region, would appear to be a bright
star-just as to us, who are on the circumference of the region of the sun, the
sun appears to be very bright."

On life of other stars:
"Therefore, the inhabitants of other stars-of whatever sort
these inhabitants might be-bear no comparative relationship to the inhabitants
of the Earth."

On the motion of the earth Cusa writes:
"It has already become evident to us
that the earth is indeed moved, even though we do not perceive this to be the
case. For we apprehend motion only through a certain comparison with something
fixed. For example, if someone did not know that a body of water was flowing
and did not see the shore while he was on a ship in the middle of the water,
how would he recognize that the ship was being moved?...".

On the Sun being larger than the Earth:
"And although the Earth is smaller than the
Sun-as we know from the Earth's shadow and from eclipses-we do not know to what
extent the region of the Sun is larger or smaller than the region of the
Earth"

Cusa also compares planets to stars (a good case can be made that planets are
very dim stars), and that the planets move writting:
"Therefore, consider carefully the
fact that just as in the eighth sphere the stars are {moved} around conjectural
poles, so the earth, the moon, and the planets-as stars-are moved at a distance
and with a difference around a pole {which} we conjecture to be where the
center is believed to be. Hence, although the earth-as star-is nearer to the
central pole, nevertheless it is moved and, in its motion, does not describe a
minimum circle, as was indicated."

Instead of Cusa getting in trouble, he is appointed cardinal in 1448, Giordano
Bruno will be murdered for sharing many of these same views in only 152 years.


Cusa builds spectacles (glasses) with concave lenses where earlier glasses used
the easier to make convex lenses that served only the far-sighted (those who
cannot see close objects), these glasses serve the near-sighted (who cannot see
far objects).

Cusa advocates the counting of pulse as a diagnostic aid in healing.
Cusa, Germany  
557 YBN
[1443 AD]
1438) Bessarion writes a treatise directed against George of Trebizond, a
vigorous Aristotelian who had written a polemic against Plato, which was
entitled "In Calumniatorem Platonis" ("Against the Slanderer of Plato").
Bessarion, though a Platonist, is not so thoroughgoing in his admiration of
Plato as Gemistus Pletho is, and strives instead to reconcile the two
philosophies.
Pope Eugenius IV makes Bessarion a cardinal in 1439.
Rome, Italy  
550 YBN
[1450 AD]
1171)
?  
550 YBN
[1450 AD]
1798)
southern Germany, or northern Italy  
548 YBN
[1452 AD]
1441)
Florence, Italy  
547 YBN
[05/29/1453 AD]
1439)
Constantanople  
546 YBN
[1454 AD]
1436) The Guttenberg Bible is sometimes referred to as the Mazarin Bible
because the first copy described by bibliographers was located in the Paris
library of Cardinal Mazarin.
Mainz, Germany  
540 YBN
[1460 AD]
1367)
Basel, Switzerland  
538 YBN
[1462 AD]
1443) Königsberg means "King's Mountain," which is what the Latinized version
of his name, Joannes de Regio monte or Regiomontanus, also means.

In 1475 Regiomontanus is summoned to Rome by Pope Sixtus IV to help reform the
Julian calendar, but Regiomontanus dies in Rome of the plague before completing
the project, and it will wait another century to be corrected.
Regiomontanus is admitted
to the University of Leipzig at age 11, has a Bachelor's Degree at 1452, but
university regulations force him to wait until he turns 21 to receive his
master's degree. Regiomontanus is teaching in 1457.
Regiomontanus lectures on Virgil
and Cicero.
Regiomontanus eventually collaborates with his teacher, the
mathematician-astronomer Georg von Peuerbach, on various astronomical and
astrological projects, including observations of eclipses and comets, the
manufacture of astronomical instruments, and the casting of horoscopes for the
court of the Holy Roman Emperor Frederick III.
Regiomontanus is conservative in
outlook and writes at length arguing how earth cannot move, citing how birds
would be blown away, clouds left behind, building would tumble.
Regiomontanus strongly
believes in astrology, and publishes a book in astrology.
Rome, Italy  
530 YBN
[1470 AD]
5899)
(thought to be:) southern Germany (verify)  
528 YBN
[1472 AD]
1442) Peurbach studies art at the University of Vienna, moves to Italy, which
Asimov describes as an intellectual center at this time and there studies under
Nicholas of Cusa before becoming professor of mathematics and astronomy at the
University of Vienna in 1453.

Peurbach is appointed astrologer to King Ladislas V of Hungary and later to
Emperor Frederick III.
Vienna, Austria  
528 YBN
[1472 AD]
1444)
Nuremberg, (Franconia, now) Germany  
528 YBN
[1472 AD]
1461) Leonardo's parents were unmarried at the time of his birth.
Leonardo grows up on
his father's family's estate, where he was treated as a "legitimate" son and
receives the usual elementary education of that day: reading, writing, and
arithmetic. Leonardo does not seriously study Latin, the key language of
traditional learning, until much later, when he acquires a working knowledge of
it on his own. He also does not apply himself to higher mathematics-advanced
geometry and arithmetic-until he is 30 years old, when he begins to study it
with diligent tenacity.
Leonardo's artistic inclinations must have appeared early. When
Leonardo is about 15, his father, apprentices Leonardo to artist Andrea del
Verrocchio. In Verrocchio's renowned workshop Leonardo receives a multifaceted
training that includes painting, sculpture and technical-mechanical arts.
Leonardo also works in the next-door workshop of artist Antonio Pollaiuolo. In
1472 Leonardo is accepted into the painters' guild of Florence, but he remains
in his teacher's workshop for five more years, after which time he works
independently in Florence until 1481. Many of the surviving pen and pencil
drawings from this period, including many technical sketches (for example of
pumps, military weapons, etc) are evidence of Leonardo's interest in and
knowledge of technical matters very early in his career.
In 1482 Leonardo moved to
Milan to work in the service of Duke Ludovico Sforza rejecting two projects
offered to him in Florence.
Leonardo spends 17 years in Milan, until Ludovico's fall
from power in 1499. Leonardo is listed in the register of the royal household
as "pictor et ingeniarius ducalis" ("painter and engineer of the duke").
Da Vinci is
highly esteemed and is constantly kept busy as a painter and sculptor and as a
designer of court festivals. Da Vince is also frequently consulted as a
technical adviser in the fields of architecture, fortifications, and military
matters, and he serves as a hydraulic and mechanical engineer.

Leonardo keeps a series of journals in which he writes almost daily, as well as
separate notes and sheets of observations, comments and plans which were left
to various pupils and were later bound. Many of the journals have survived to
illustrate Leonardo's studies, discoveries and inventions. Da Vinci write
backwards in mirror-script in voluminous notebooks, which can be easily read
with a mirror as his contemporaries testify. Leonardo is left handed so writing
backwards is more easily done. Leonardo's notebooks add up to thousands of
closely written pages abundantly illustrated with sketches-the most voluminous
literary legacy any painter has ever left behind.

Da Vinci paints famous realistic-appearing paintings such as "Mona Lisa", and
"The Last Supper".
Da Vinci knows neither Greek or Latin.
The funders of Da Vinci include
Cesare Borgia, son of Pope Alexander VI, Louis XII of France, Giulio de Medici,
brother of Pope Leo X, and Francis I of France.
Florence, Italy  
527 YBN
[1473 AD]
1462) Leonardo da Vinci (VENcE) (CE 1452-1519) draws a study of a Tuscan
landscape. This is Da Vinci's earliest dated drawing. The drawing is of the
valley of the Arno River, where Da Vinci lives.

Florence, Italy  
527 YBN
[1473 AD]
5894) Johannes Tinctoris (CE 1436–1511), publishes "Terminorum musicae
diffinitorium" ("Dictionary of Musical Terms, Naples, 1473), which is the
earliest printed dictionary of musical terms.

Naples, Italy (presumably)  
526 YBN
[1474 AD]
1433) Toscanelli observes comets and painstakingly calculates their orbits.
Among these will be Halley's comet in 1456.
Toscanelli is the son of the physician
Dominic Toscanelli. Educated in mathematics at the University of Padua,
Toscanelli leaves in 1424 with the title of a doctor of medicine.
Toscanelli is a friend
of Nicholaus of Cusa.
Florence, Italy  
526 YBN
[1474 AD]
1434)
Florence, Italy  
525 YBN
[1475 AD]
1174) Jewish humans in parts of Europe have to wear pointed hats as an
identifying badge. The humans in the Catholic church force all Jewish humans to
wear these pointed hats, as shown in an image carved into wood (a German
woodcut) {get image}. These Jewish people were burned, charged with sacrificing
Christian children.

Europe  
523 YBN
[1477 AD]
1368) Carl Linnaeus, and Anders Celsius will be professors at Uppsala.
Uppsala, Sweden  
522 YBN
[1478 AD]
1175) Pope Sixtus IV (Pope 1471 to 1484) authorizes Ferdinandand Isabella to
revive the Inquisition to hunt "secret Jews" and Muslim people (at least 2000
humans are eventually killed by the Inquisition).

Sixtus IV issues a bull this year that established an Inquisitor in Seville,
under political pressure from Ferdinand of Aragon, who threatened to withhold
military support from his kingdom of Sicily if he did not.(verify)

He founds the Sistine Chapel where the team of artists he brings together
introduce the Early Renaissance to Rome with the first masterpiece of the
city's new artistic age (Michelangelo's frescoes will be added in a later
phase).

Spain  
521 YBN
[1479 AD]
1369) Almost all educational institutes in Denmark are free for citizens to
attend.
Major contributors to science that will graduate from the University of
Coperhagen include: Tycho Brahe, Ole Rømer, Hans Christian Ørsted, and Niels
Bohr among others.
Copenhagen, Denmark  
520 YBN
[1480 AD]
1463)
Florence, Italy  
520 YBN
[1480 AD]
5892) Josquin des Prez (CE c1450-1521) composes music. Des Prez makes use of
the technique of "pervading imitation", in which a series of musical ideas are
stated imitatively in all voices throughout an entire work, or section of a
work. The first music printer, Ottaviano Petrucci, devoted an entire volume to
Josquin's works, an honor given to no other composer. According to the Oxford
Grove Music Encyclopedia Josquin is the greatest composer of the high
Renaissance.

(cathedral of) Milan, Italy (presumably)  
520 YBN
[1480 AD]
5893) Jean de Ockeghem (CE c1410-1497) composes sacred and secular music, and
is one of the great masters of the Franco-Flemish style that dominates European
music of the Renaissance. Ockeghem makes use of the musical "canon" and
"counterpoint" techniques. Canon is in the strict sense, technique in which
polyphony is derived from a single line that is imitated at fixed or (less
often) variable intervals of pitch and time, for example in the song "Three
Blind Mice" and "Frère Jacques". Starting with the 1500s, the term "canon" is
used for the work itself. Counterpoint in music is defined as melodic material
that is added above or below an existing melody, and the technique of combining
two or more melodic lines in such a way that they establish a harmonic
relationship while retaining their linear individuality and also the use of
contrasting elements in a work of art.

(chapel of Charles VII) Blois, France (guess)  
516 YBN
[05/01/1484 AD]
1449) Columbus is the eldest son of Domenico Colombo, a Genoese wool worker and
merchant, and Susanna Fontanarossa, his wife. His career as a seaman begins
effectively in the Portuguese merchant marine. After surviving a shipwreck off
Cape St. Vincent at the southwestern point of Portugal in 1476, he bases
himself in Lisbon, together with his brother Bartholomew. Both are employed as
chart makers, but Columbus is principally a seagoing entrepreneur. In 1477 he
sails to Iceland and Ireland with the merchant marine, and in 1478 he buys
sugar in Madeira as an agent for the Genoese firm of Centurioni. In 1479 he
meets and married Felipa Perestrello e Moniz, a member of an impoverished noble
Portuguese family. Their son, Diego, is born in 1480. Between 1482 and 1485
Columbus trades along the Guinea and Gold coasts of tropical West Africa and
made at least one voyage to the Portuguese fortress of São Jorge da Mina
there, gaining knowledge of Portuguese navigation and the Atlantic wind systems
along the way. Felipa dies in 1485, and Columbus takes as his mistress Beatriz
Enríquez de Harana of Córdoba, by whom he has his second son, Ferdinand.
Columbus always
writes in Spanish, or Spanish-influenced Latin.
Portugal  
515 YBN
[1485 AD]
1464)
Milan, Italy  
515 YBN
[1485 AD]
1471) Leonardo da Vinci (VENcE) (CE 1452-1519), draws the "Virtuvian Man".

Milan, Italy  
513 YBN
[1487 AD]
1465)
Milan, Italy  
513 YBN
[1487 AD]
1466)
Milan, Italy  
513 YBN
[1487 AD]
1468)
Milan, Italy  
512 YBN
[1488 AD]
1467)
Milan, Italy  
510 YBN
[1490 AD]
5895) Bartolomeo Tromboncino (CE c1470-c1535) and Marchetto Cara (C1470-1525)
compose music in the style called "frottola". For most of the 1400s, French
chanson dominates the music performed in Italy until around 1480 when native
composers set their texts into their own language again, in a style known as
"frottola". Frottola poetry tends to be more lighthearted than the courtly love
of chanson texts. Musically, frottola avoids imitation and counterpoint in
contrast to contemporary chansons. Frottole are characterized by chordal
textures and lively, dance-like rhythms. Frottole can be performed entirely by
instruments, or by any combination of voices and instruments. Frottole are
arranged for solo voice and lute, or for keyboard alone and are in popular
demand at the time.

Mantua, Italy  
510 YBN
[1490 AD]
5901) Arnolt Schlick (CE c1460-c1521), German organist and composer, composes
instrumental music for lute. Schlick's "Spiegel der Orgelmacher und Organisten"
(1511) is the first German treatise on organ building and organ playing. Some
of Schlick's organ pieces are published in his "Tabulaturen etlicher lobgesang"
(1512), the first printed German organ tablatures.
Germany  
509 YBN
[1491 AD]
1176) In Spain Jewish humans tortured by the Holy Inquisition were made to
"confess" to killing a child in a town called "La Guardia".

Spain  
509 YBN
[1491 AD]
1484) In 1486, planning to defend 900 theses he had drawn from diverse Greek,
Hebrew, Arabic, and Latin writers, Pico invites scholars from all of Europe to
Rome for a public disputation. For the occasion he composes his celebrated
"Oration on the Dignity of Man" (1486). A papal commission, however, denounces
13 of the theses as heretical, and the assembly is prohibited by Pope Innocent
VIII. Despite his ensuing "Apologia" for the theses, Pico thinks it prudent to
flee to France but is arrested there. After a brief imprisonment he settles in
Florence, where he became associated with the Platonic Academy, under the
protection of the Florentine prince Lorenzo de' Medici. Except for short trips
to Ferrara, Pico spends the rest of his life there. Pico is absolved from the
charge of heresy by Pope Alexander VI in 1492.

"Disputations..." will not be published until after Mirandola's death.
(written:) Fiesole, Italy;(published:) Bologna, Italy  
508 YBN
[01/??/1492 AD]
1451) The emperor of Cathay, whom Europeans referred to as the Great Khan of
the Golden Horde-was himself held to be interested in Christianity, and
Columbus carefully carries a letter of friendship addressed to him by the
Spanish monarchs.

In the letter that prefaces his journal of the first voyage, Columbus explains
his excitement about his journey, and reveals a racist and vicious religious
fervor (in a war against the "infidels", basically all those not in the cult of
Jesus) typical of people in this time:
"...and Your Highnesses, as Catholic
Christians…took thought to send me, Christopher Columbus, to the said parts of
India, to see those princes and peoples and lands…and the manner which should
be used to bring about their conversion to our holy faith, and ordained that I
should not go by land to the eastward, by which way it was the custom to go,
but by way of the west, by which down to this day we do not know certainly that
anyone has passed; therefore, having driven out all the Jews from your realms
and lordships in the same month of January, Your Highnesses commanded me that,
with a sufficient fleet, I should go to the said parts of India, and for this
accorded me great rewards and ennobled me so that from that time henceforth I
might style myself "Don" and be high admiral of the Ocean Sea and viceroy and
perpetual Governor of the islands and continent which I should discover…and
that my eldest son should succeed to the same position, and so on from
generation to generation forever."
  
508 YBN
[08/03/1492 AD]
1452)
Palos, Spain  
508 YBN
[09/13/1492 AD]
1453)
Atlantic Ocean  
508 YBN
[10/12/1492 AD]
1450) Humans from Europe reach the Americas by crossing the Atlantic Ocean.

Christopher Columbus (CE 1451-1506) lands on a small island (probably San
Salvador) in America.

In America Columbus explores, finds a new race of people, new plants, and many
other new phenomena.

Vikings such as Leif Eriksson had visited North America five centuries
earlier.

In the next 10 years Columbus will makes 3 journeys to the "Indies".

Because of this mistaken belief that Columbus had reached India, the Carribean
will be called the West Indies even up to the present time. That Native
American people are sometimes still referred to as "Indians" shows that this
mistaken view of America being India is still uncorrected.

Beyond planting the royal banner, Columbus spends little time on San Salvador,
being anxious to press on to what he thinks will be Cipango (Japan).
(probably) San Salvador  
508 YBN
[10/28/1492 AD]
1454)
  
508 YBN
[12/05/1492 AD]
1455)
Haiti  
508 YBN
[1492 AD]
1177) Jewish people are expelled from Spain for "racial purification".

Spain  
507 YBN
[01/16/1493 AD]
1456)
Haiti  
507 YBN
[02/26/1493 AD]
1457)
Azores  
507 YBN
[02/26/1493 AD]
1458)
Azores  
507 YBN
[03/15/1493 AD]
1459) On his fourth and final voyage to America, Columbus, stranded with his
crew on the island of Jamaica, correctly predicts an eclipse of the Moon from
his astronomical tables, which frightens and tricks the local peoples into
providing food for them.
Palos, Spain  
506 YBN
[06/07/1494 AD]
1460)
Tordesillas (now in Valladolid province, Spain)  
506 YBN
[1494 AD]
1445) Pacioli becomes a Franciscan Friar around 1470.
Pacioli teaches math at
universities at Perugia, Naples and Rome.
Pacioli meets Leonardo da Vinci at the
court of the Duke of Milan, Ludovico Sforza. In exchange for lessons in math,
Leonardo illustrates one of Pacioli's books.
Venice, Italy  
505 YBN
[1495 AD]
1470) Leonardo da Vinci (VENcE) (CE 1452-1519), paints "the Last Supper".

Milan, Italy  
504 YBN
[1496 AD]
1446)
Bologna, Italy  
504 YBN
[1496 AD]
1448) Two versions of the original manuscript have survived, one in the
Biblioteca Ambrosiana in Milan, the other in the Bibliothèque Publique et
Universitaire in Geneva.
Milan, Italy  
500 YBN
[1500 AD]
1480) Albrecht Dürer, age 28, paints his self portrait. This strikingly
realistic painting is an early representation of the realism that will evolve
in Renaissance era paintings.

Nuremberg, Germany  
498 YBN
[1502 AD]
1493)
  
497 YBN
[1503 AD]
1469) Leonardo da Vinci (VENcE) (CE 1452-1519), paints the Mona Lisa.

Milan, Italy  
496 YBN
[1504 AD]
1474) Vespucci meets Columbus towards the end of Columbus' life and the two are
friendly to each other.
Perhaps had Columbus recognized that he had landed on a new
continent America would be called "Columbia", or "North and South Christica".
  
493 YBN
[1507 AD]
1473)
Milan, Italy  
493 YBN
[1507 AD]
1476) The wall map will be lost for a long time, but a copy is found in a
castle at Wolfegg in southern Germany by Joseph Fischer in 1901. This is the
only known copy of the map.

Some hold that the "Cosmographiae" was written by Matthias Ringmann instead, or
that it was a joint effort.
Saint-Dié, Lorraine, France  
491 YBN
[1509 AD]
1447)
Bologna?,Italy  
491 YBN
[1509 AD]
5903) Hans Sachs (CE 1494-1576), German poet and Meistersinger, composes music
and plays around this time. Wagner makes Sachs a leading character in his opera
"Die Meistersinger von Nürnberg" (1868) uses Sachs.

Germany  
490 YBN
[1510 AD]
1472)
Milan, Italy  
489 YBN
[1511 AD]
1513) In 1516 Erasmus will have "Novum instrumentum" printed in Basel, which is
a heavily annotated edition of the New Testament placing texts in Greek and
revised Latin side by side. Erasmus is therefore, the first editor of the New
Testament.
Erasmus dedicates "In Praise of Folly" to his friend, Thomas More, author of
the famous and controversial book "Utopia".
This work will influence the French satirist
Rabelais.
Erasmus studies at the University of Paris and teaches for some time at
Cambridge University.
written: London, Netherlands  
488 YBN
[1512 AD]
1481) Copernicus studies math and painting at Cracow (Asimov writes that Cracow
is the intellectual center of Poland at this time and will be for many years
after).
Copernicus studies health (medicine) and canon law in Italy for 10 years.
After
reading Regiomontanus Copernicus becomes interested in Astronomy.
In 1497 Copernicus'
uncle is ordained Bishop of Warmia, and Copernicus is named a canon at Frombork
Cathedral.
In 1505 Copernicus returns to Poland where he serves as canon under his uncle
at the cathedral at Frombork (Frauenberg, in German), but never becomes a
priest and never marries.
Copernicus serves as his uncle's doctor.
Frombork, Poland  
487 YBN
[09/25/1513 AD]
1485) In 1500, Balboa, sails to South America.
Balboa settles in Hispaniola in 1502,
where he resides for several years as a planter and pig farmer. In 1509,
wanting to escape his creditors in Santo Domingo, Balboa sets sail as a
stowaway.

In December 1511 King Ferdinand II sends orders that name Balboa interim
governor and captain general of Darién.

The Spaniards are told by Native Americans that to the south lay a sea and a
province infinitely rich in gold, a reference to the Pacific and perhaps to the
Inca Empire. The Native people tell the Spainards that the conquest of that
land would require 1,000 men. Balboa quickly sends messengers to Spain to
request reinforcements. The news creates much excitement in Spain, and a large
expedition is promptly organized. But Balboa is not given command because
charges brought against Balboa by his enemies had turned King Ferdinand II
against him, and, as commander of the armada and governor of Darién, the King
sends out the elderly, powerful nobleman Pedro Arias Dávila (usually called
Pedrarias). The expedition, numbering 2,000 persons, leaves Spain in April
1514.

In his own explorations Balboa manages to collect a great deal of gold, much of
it from the ornaments worn by the native women, and the rest obtained by
violence.

At the end of 1512 and the first months of 1513, Balboa arrives in a region
dominated by the cacique Careta, whom he easily defeats and then befriends.
Careta is baptized and becomes one of Balboa's chief allies; Careta ensures the
survival of the settlers by promising to supply the Spaniards with food. Balboa
then proceeds on his journey, arriving in the lands of Careta's neighbour and
rival, cacique Ponca, who flees to the mountains with his people, leaving his
village open to the plundering of the Spaniards and Careta's men. Days later,
the expedition arrives in the lands of cacique Comagre, fertile but reportedly
dangerous terrain. However, Balboa is received peacefully and even invited to a
feast in his honor; Comagre, like Careta, is then baptized.

It is in Comagre's lands that Balboa first hears of "the other sea". It starts
with a squabble among the Spaniards, unsatisfied by the meagre amounts of gold
they are being allotted. Comagre's eldest son, Panquiaco, angered by the
Spaniards' avarice, knocks over the scales used to measure gold and exclaims:
"If you are so hungry for gold that you leave your lands to cause strife in
those of others, I shall show you a province where you can quell this hunger".
Panquiaco tells them about a kingdom to the south, where people are so rich
that they eat and drink from plates and goblets made of gold, but that the
conquerors will need at least a thousand men to defeat the tribes living inland
and those on the coast of "the other sea". How the native speaking people and
Spanish speaking people communicate is a very interesting puzzle, since neither
had any experience at all with the others language. Individual people must have
had to spend months translating and learning nouns and verbs before any
detailed talk can happen.

The announcement of balboa finding the "South Sea," restores Balboa to royal
favor and Balboa is named "adelantado" (governor) of the Mar del Sur and of the
provinces of Panamá and Coiba.

Pedrarias, the head of the Spanish expedition summons Balboa home on the
pretext that Pedrarias wishes to discuss matters of common concern. Upon
returning Balboa is seized and charged with rebellion, high treason, and
mistreatment of Indians, among other misdeeds. After a farcical trial presided
over by Gaspar de Espinosa, Pedrarias' chief justice, Balboa is found guilty,
condemned to death, and beheaded with four alleged accomplices in January 1519.
a peak in Darién, Panama  
486 YBN
[1514 AD]
1178) Anthony Fitzherbert (1470 - 1538), an English judge, writes the first
systematic attempt to provide a summary of English law, known as La Graunde
Abridgement in 1514, and among others "The Boke of Husbandire", a book on
agriculture.

England  
485 YBN
[1515 AD]
1486) Schöner is ordained a Roman Catholic priest, but later abandons
priesthood and becomes a Lutheran.
Schöner is a professor of mathematics at the
University of Nuremberg.
In 1540, Rheticus will dedicate the first report "Narratio prima"
(an introduction to Copernicus' "De Revolutionibus") to Schöner.
Bamberg, Bavaria, Germany  
485 YBN
[1515 AD]
3222)
  
484 YBN
[1516 AD]
1515) Thomas More may get the idea for "Utopia" when he and Erasmus jointly
translate some of Lucian's works from Greek into Latin. Among these dialogues,
is the story of Menippus, the Greek playwright, descending into the underworld
and describing what he finds there. The other significant influence is Plato's
"Republic", which is a far more politically motivated work about imaginary
lands and is referred to several times in "Utopia".

More will be beheaded in 1535 for refusing to accept King Henry VIII as head of
the Church of England.
London, England  
483 YBN
[10/20/1517 AD]
1492)
  
483 YBN
[10/31/1517 AD]
1389)
Wittenberg, Germany  
481 YBN
[08/10/1519 AD]
1498)
Sanlúcar de Barrameda, Spain  
481 YBN
[09/20/1519 AD]
1491) Ferdinand Magellan (moJeLoN) (c1480-1521), Portuguese explorer, sets sail
to circumnavigate the earth.
Magellan leaves for America with 5 ships in order to find
a way to the Spice Islands of Indonesia. This is the voyage to circumnavigate
the earth that Columbus had intended.
Sanlúcar de Barrameda, Spain  
480 YBN
[04/08/1520 AD]
1494)
Puerto San Julian, Argentina  
480 YBN
[10/21/1520 AD]
1496) Asimov claims that the Pacific Ocean is not actually more passive than
the Atlantic Ocean.
Straight of Magellan  
480 YBN
[12/13/1520 AD]
1495)
Rio de Janeiro, Brazil  
480 YBN
[1520 AD]
1487)
Bamberg, Bavaria, Germany  
479 YBN
[03/06/1521 AD]
1497) After entering the Pacific Ocean, the ships sail near the Chilean coast
until Decemeber 18 when Magellan takes a course northwestward. Not until
January 24, 1521, is land sighted, probably Pukapuka in the Tuamotu
Archipelago.
Guam  
479 YBN
[03/16/1521 AD]
1499) At Massava Magellan secures the first alliance in the Pacific for Spain.

Antonio Pigafetta, a wealthy tourist who paid to be on the Magellan voyage,
provides the only extant eyewitness account of the events culminating in
Magellan's death, as follows:
"When morning came, forty-nine of us leaped into the water
up to our thighs, and walked through water for more than two cross-bow flights
before we could reach the shore. The boats could not approach nearer because of
certain rocks in the water. The other eleven men remained behind to guard the
boats. When we reached land, {the natives} had formed in three divisions to the
number of more than one thousand five hundred people. When they saw us, they
charged down upon us with exceeding loud cries... The musketeers and
crossbow-men shot from a distance for about a half-hour, but uselessly...
Recognising the captain, so many turned upon him that they knocked his helmet
off his head twice... A native hurled a bamboo spear into the captain's face,
but the latter immediately killed him with his lance, which he left in the
native's body. Then, trying to lay hand on sword, he could draw it out but
halfway, because he had been wounded in the arm with a bamboo spear. When the
natives saw that, they all hurled themselves upon him. One of them wounded him
on the left leg with a large cutlass, which resembles a scimitar, only being
larger. That caused the captain to fall face downward, when immediately they
rushed upon him with iron and bamboo spears and with their cutlasses, until
they killed our mirror, our light, our comfort, and our true guide. When they
wounded him, he turned back many times to see whether we were all in the boats.
Thereupon, beholding him dead, we, wounded, retreated, as best we could, to the
boats, which were already pulling off."
Philippines  
479 YBN
[11/06/1521 AD]
1500) The remaining two ships of Magellan's now under the leadership of Cano,
reach the Maluku Islands (the Spice Islands) with 115 men left. They manage to
trade with the Sultan of Tidore, a rival of the Sultan of Ternate, who is the
ally of the Portuguese.

The two remaining ships, laden with valuable spices, attempt to return to Spain
by sailing west. As they leave the Moluccas, however, Trinidad is found to be
taking on water. The crew tries to discover and repair the leak, but fails.
They conclude that Trinidad will need to spend considerable time being
overhauled. The small Victoria was not large enough to accommodate all the
surviving crew. As a result, Victoria with some of the crew sails west through
the Indian Ocean for Spain. Several weeks later, Trinidad left the Moluccas to
attempt to return to Spain via the Pacific route. This attempt fails; the ship
is captured by the Portuguese, and is eventually wrecked in a storm while at
anchor under Portuguese control.

Four crewmen of the original fifty-five on the Trinidad will finally returned
to Spain in 1525. Fifty-one of them had died in war or from disease.

Philippines  
478 YBN
[05/06/1522 AD]
1501) By May 6, 1522, the Victoria, commanded by Juan Sebastián Elcano, rounds
the Cape of Good Hope, with only rice for rations. Twenty crewmen die of
starvation before Elcano reaches the Cape Verde Islands, a Portuguese holding,
where he abandons 13 more crewmembers on July 9 in fear of losing his cargo of
26 tons of spices (cloves and cinnamon).

Cape of Good Hope  
478 YBN
[09/08/1522 AD]
1475) Magellen's crew is the first to circumnavigate the earth..

Juan Sebastian del Cano (KonO) (c1460-1525), Spanish Navigator, returns in a
single remaining ship originally lead by Magellan to Seville, Spain with a crew
that is the first to circumnavigate the earth.

This voyage lasts 3 years and cost 4 ships, but the spices and other
merchendice brought back more than compensate for the loss. This voyage proves
that Eratosthenes estimate of the size of the Earth is correct, and that of
Poseidoinius and Ptolemy wrong, and that a single ocean covers the earth.
Seville, Spain  
477 YBN
[1523 AD]
1488)
Bamberg, Bavaria, Germany(presumably)  
477 YBN
[1523 AD]
5914) Marco Antonio Cavazzoni (c1490-c1570), Italian composer, publishes
"Recerchari, motetti, canzoni, Libro I" (Venice, 1523), the first set of
independently composed keyboard music ever published. Much of these
compositions are astonishingly mature for the time, featuring parallel 5ths and
octaves and harsh dissonance, demonstrating a clear independence from vocal
music.
(Saint Mark's Cathedral) Venice, Italy  
476 YBN
[1524 AD]
1386)
Mexico City, Mexico  
476 YBN
[1524 AD]
1510) Peter Apian is latinized from Peter Bienewitz or Bennewitz
(pā'tər bē'nəvĭts, bĕn'əvĭts).
Apian is a professor of mathematics
at the University of Ingolstadt.

In 1527, Peter Apian is called to the University of Ingolstadt as a
mathematician and printer. His print shop starts small. Among the first books
he prints are the writings of Johann Eck, Martin Luther's antagonist. Later,
Apian's print shop will become well-known for its high-quality editions of
geographic and cartographic works.
Landshut, Bavaria, Germany  
475 YBN
[07/??/1525 AD]
2776) William Tyndale (TinDeL) (CE c1494-1536) translates and prints the New
Testament and Pentateuch into English.

After church authorities in England prevent Tyndale from translating the Bible
there, Tyndale goes to Germany in 1524, receiving financial support from
wealthy London merchants. Tyndale's New Testament translation is completed in
July 1525 and printed at Cologne. Interrupted by an injunction, Tyndale has the
edition completed at Worms. By April 1526 an octavo edition is being sold in
London. When copies enter England, they are denounced by the bishops and
suppressed (1526); Cardinal Wolsey orders Tyndale seized at Worms. In November
all available copies are burned at St. Paul's Cross. (To me this shows clearly
an interest in keeping the public uninformed and uneducated, that information
about the actual substance of the religion is to be kept only for an elite few.
In addition, possibly to obscure and keep abstract the facts surrounding the
religion, since people cannot criticize what they know nothing of. A similar
occurrence has happened in science with the truth about Michael Pupin, the
theory of time dilation, and much of the history of science. Apparently, the
less the public knows, the less they can criticize and uncover dishonesty and
error.)

In 1535 while revising his translations, Tyndale is seized in Antwerp and
confined in Vilvoorde Castle, near Brussels. Tyndale's trial ends in
condemnation for heresy, and Tyndale is strangled at the stake before his body
is burned.

Tyndale's Bible is the first English translation to draw directly from Hebrew
and Greek texts, and the first to take advantage of the new medium of print,
which allows for its wide distribution.
Tyndale is educated at the University of Oxford and
becomes an instructor at the University of Cambridge.
In 1521, while at Cambridge, Tyndale
is friends with a group of humanist scholars meeting at the White Horse Inn.
Tyndale
becomes convinced that the Bible alone should determine the practices and
doctrines of the church and that every believer should be able to read the
Bible in their own language.

In 1528 Tyndale publishes the "The Obedience of a Christian Man" (1528), which
replaces papal authority by royal authority and is heartily approved by King
Henry VIII and "The Parable of the Wicked Mammon" (1528) dealing with Luther's
teaching concerning justification by faith. Both these works are denounced by
Sir Thomas More. The Practice of Prelates (1530), condemning the divorce of
Henry VIII (with Catherine of Aragon), draws the wrath of the king.
Cologne, Germany  
475 YBN
[1525 AD]
1477) Durer's father is a goldsmith
Durer is court painter to emperor Maximillian I and
successor Charles V.
It is clear from his writings that Dürer is highly
sympathetic to Martin Luther, and he may be influential in the City Council
declaring for Luther in 1525. However, Durer dies before religious divisions
had hardened into different churches, and may well have regarded himself as a
reform-minded Catholic to the end.
The most striking painting illustrating Dürer's
growth toward the Renaissance spirit is a self-portrait, painted in 1498
(Prado, Madrid).
Dürer achieves an international reputation as an artist by 1515, when
he exchanges works with the illustrious High Renaissance painter Raphael.
Druerer's work
on fortification is published in 1527, and his work on human proportion is
brought out in four volumes shortly after his death at the age of fifty-six, in
1528.
Nürnberg, Germany  
474 YBN
[1526 AD]
1505)
Basil, Switzerland  
470 YBN
[1530 AD]
1503) As a young man, Hohenheim attends the Bergschule, founded by the wealthy
Fugger family of merchant bankers of Augsburg, where his father teaches
chemical theory and practice. Young people are trained at the Bergschule as
overseers and analysts for mining operations in gold, tin, and mercury, as well
as iron, alum, and copper-sulfate ores.
The young Paracelsus learns about minerals
from miners talking about metals that "grow" in the earth.
Hohenheim enters at
University of Basil in 1510, later moving to the University of Vienna.

Paracelsus is said to have graduated from the University of Vienna with the
baccalaureate in medicine in 1510, when he was 17.
At Ferrara Hohenheim is free to
express his rejection of the prevailing view that the stars and planets control
all the parts of the human body. Hohenheim is thought to have begun using the
name "para-Celsus" (above or beyond Celsus) around this time, regarding himself
as even greater than Celsus, the renowned 1st-century Roman physician known for
his tract on health and medicine.
Paracelsus travels widely seeking out alchemists and
physicians to learn from.
Paracelsus is appointed town physician and lecturer in
medicine at the University of Basel. Students from all parts of Europe begin to
flock into the city. Paracelsus pins a program of his upcoming lectures to the
notice board of the university on June 5, 1527, inviting not only students but
everybody.
Three weeks later, on June 24, 1527, surrounded by a crowd of cheering
students, Paracelsus burns the books of Ibn Sina (Avicenna), the Arab "Prince
of Physicians," and those of the Greek physician Galen, in front of the
university. Luther, just six and a half years before at the Elster Gate of
Wittenberg on Dec. 10, 1520, had burned a papal bull that threatened
excommunication. Paracelsus seemingly remains a Catholic to his death, although
it has been said that his books were placed on the Index Expurgatorius.
Paracelsus denounces
the theory of humors.

Like Luther, Paracelsus lectures and writes in German rather than Latin.
Paracelsus'
lecture hall is always crowded to overflowing. He stresses the healing power of
nature and rages against those methods of treating wounds, such as padding with
moss or dried dung, that prevent natural draining. The wounds must drain, he
insists, saying "If you prevent infection, Nature will heal the wound all by
herself." Paracelsus attacks many other medical frauds of his time including
worthless pills, salves, infusions, balsams, electuaries, fumigants, and
drenches.
In the spring of 1528, in fear Paracelsus flees Basel in the middle of the
night.
Shortly before the flight from Basel, Paracelsus completes the most important
of his earlier works, "Nine Books of Archidoxus", a reference manual on secret
remedies. Between 1530 and 1534 Paracelsus writes his bestknown works, the
"Paragranum" and the "Paramirum", both dealing with cosmology. Paracelsus
returns to medical writing with the "Books of the Greater Surgery" in editions
of 1536 and 1537; this is Paracelsus' only work that is a publishing success.
The "Astronomia magna", done between 1537 and 1539, is said to show his most
mature thinking about nature and humans.

Paracelsus uses mercury and antimony even after practice had shown them to be
toxic.
Paracelsus believes in the 4 element theory of the Greek people and the 3
principles of the Arab people (mercury, sulfur and salt). During all his
travels, Paracelsus spreads the anti-Aristotelian position that the four
elements (earth, air, fire, and water) are composed of primary principles: a
fireproducing principle (sulfur), a principle of liquidity (mercury), and a
principle of solidity (salt).
Paracelsus rejects the magic theories of Agrippa and
Flamel. Paracelsus does not think of himself as a magician and scorns those who
do, though he is a practicing astrologer, as were are, if not all of the
university-trained physicians working at this time in Europe. So Paracelsus
wrongly believes in astrology and the influence of the stars on disease.

Kind of a funny story is that Paracelsus is said to have cured many people in
the plague-stricken town of Stertzing in the summer of 1534 by administering
orally a pill made of bread containing a minute amount of the patient's excreta
he had removed on a needle point. Probably not an effective cure, and very
dangerous because of bacterial (in particular E Coli) infection.
Basel?, Switzerland?  
470 YBN
[1530 AD]
3058) At the University of Padua Fracastoro is a colleague of the astronomer
Copernicus.
As a physician, Fracastoro maintains a private practice in Verona.
Verona, Italy (and possibly mountain villa at Incaffi)  
470 YBN
[1530 AD]
5900) Luis de Milán (CE c1500-c1561), Spanish musician, composes instrumental
music for lute.

(a Ducal court) Valencia, Spain  
469 YBN
[1531 AD]
1546) Servetus defends the botanical view of his friend Fuchs.
Servetus believes and
lectures on astrology.
This is during the Protestant reformation, and Servetus has the
view of a Unitarian (the belief that Jesus was not God, that God is only one
thing not a trinity which includes Jesus and the so-called Holy Spirit).
Servetus
studies medicine in Paris and meets John Calvin, one of the early and most
powerful Protestants there.
Toulouse, France (presumably)  
467 YBN
[1533 AD]
1489)
Bamberg, Bavaria, Germany(presumably)  
467 YBN
[1533 AD]
1542)
Friesland (present day Netherlands)  
466 YBN
[1534 AD]
1514) Although this break of allegiance to traditional Christianity is a
progressive step towards atheism, Henry the VIII is a brutal person who orders
the execution of many nonviolent people such as those who refuse to take an
oath of loyalty such as humanist author of the book "Utopia", Thomas More.
Henry VIII has his own his second wife, Anne Boleyn (c1501/1507-1536) executed.
London (presumably), England  
464 YBN
[1536 AD]
1504) This book restores, and even extends, the excellent reputation Paracelsus
had earned at Basel in his prime. Paracelsus becomes wealthy and is sought
after by royalty.
Basel?, Switzerland?  
463 YBN
[1537 AD]
1536) Fontana (Tartaglia) came from poverty and was largely self educated.
Fontana was
nicknamed "Tartaglia", which means "studderer", because during the French sack
of Brescia in 1512, Fontana's face was slashed by a French soldier, leaving him
with a speech defect. Tartgalia chose to adopt the name.
Fontana teaches mathematics
in various universities in northern Italy, and settles in Venice in 1534 to
teach mathematics.
Venice, Italy (presumably)  
462 YBN
[10/28/1538 AD]
1371)
Santo Domingo, Dominican Republic  
462 YBN
[1538 AD]
1554)
Padua, Italy{4 ans} (presumably)  
462 YBN
[1538 AD]
3059)
Verona, Italy (and possibly mountain villa at Incaffi)  
460 YBN
[1540 AD]
1483)
Frauenburg (Frombork, Poland)  
460 YBN
[1540 AD]
1509)
Ingolstadt, Bavaria, Germany  
459 YBN
[1541 AD]
1557)
Zurich, Swizerland (presumably)  
458 YBN
[1542 AD]
1511) The word "pathology", is somewhat abstract, one dictionary defines
pathology as "the science or the study of the origin, nature, and course of
diseases" which might just as easily be covered by the science of "health".
"Pathology" relates to the path or course a disease routinely takes. The word
"physiology", also somewhat abstract, is defined by one dictionary as "the
branch of biology dealing with the functions and activities of living organisms
and their parts, including all physical and chemical processes". Physiology
deals with the actual physical processes of any part of a living body.
Fernel rejects
astrology as being relevant to healing (medicine). How the word "medicine"
became associated with "healing" I do not know, however, in my opinion, the
word "health" more accurately covers what a physician does. Perhaps a
distinction between the fraudulent religious "healers" and formally educated
"healers" needed to be clearly expressed.

Frenel graduates from the University of Paris 1519, gets a medical degree in
1530, and in 1534 is a professor of "medicine" at University of Paris.
Frenel is the
physician to Henry II of France.
  
458 YBN
[1542 AD]
1540) A genus of flower is named after Fuchs, and the name Fuchs is also the
origin or the word for the color "Fuscia" (a bluish red).
Fuchs receives a medical
(physician) degree at the University of Ingolstadt in 1524.
In 1535 Fuchs is
professor of medicine (health) at the University of Tübingen.
Fuchs is an active
supporter of Vesalius.
Basel, Switzerland  
457 YBN
[1543 AD]
1025)
  
457 YBN
[1543 AD]
1482) The Sun centered theory is revived. Copernicus' (1473-1543) book
supporting a sun centered theory is published.

A few hundred copies of Nicolaus Copernicus' (1473-1543) book, "De
revolutionibus orbium coelestium libri vi" ("Six Books Concerning the
Revolutions of the Heavenly Orbs"), are printed (200 copies still exist). The
original hand written draft exists and shows that Copernicus crossed out an
original reference to Aristarchos.

Rheticus gives the manuscript to Andreas Osiander (1498–1552), a theologian
and strong follower of Luther, who ads an unsigned “letter to the reader”
directly after the title page, which states that the hypotheses contained
within made no pretense to truth and that, in any case, astronomy is incapable
of finding the causes of heavenly phenomena. In addition, the title of the work
is changed from the manuscript’s "On the Revolutions of the Orbs of the
World" to "Six Books Concerning the Revolutions of the Heavenly Orbs", a change
that appears to lessen the book's claim to describe the real universe. These
changes by Osiander are not known until Kepler reveals this in his "Astronomia
Nova" (New Astronomy) in 1609.
(presumably) written in (Frauenburg, East Prussia now:)Frombork, Poland;
(printed in)Nuremberg, Germany  
457 YBN
[1543 AD]
1553) Vesalius' father is the court pharmacist to Emperor Charles V.
Vesalius is
from long line of physicians and pharmacists in Wesel, and this is where the
name Vesalius comes from.
Vesalius studies in Louvain (now Belgium) (1529-1533), and
medical (health) school of the University of Paris (1533-1536) both
conservative centers supporting Galen, and so even as late as 1538 Vesalius
publishes material largely based on Galen. At the University of Paris, Vesalius
learned to dissect animals, has the opportunity to dissect human cadavers, and
devotes much of his time to a study of human bones, at that time easily
available in the Paris cemeteries.

In 1536 Vesalius returns to his native Brabant to spend another year at the
University of Louvain, where the influence of Arab medicine (health science) is
still dominant. At Louvain, Vesalius writes his graduate dissertation on the
900s Arab physician al-Razi (Rhazes).

In 1537, Vesalius then goes to the University of Padua, a progressive
university with a strong tradition of anatomical dissection. On receiving the
M.D. degree the same year, he is appointed a lecturer in surgery with the
responsibility of giving anatomical demonstrations. Since Vesalius dissects
many cadavers, and insisted on doing them himself, instead of relying on
untrained assistants.
Vesalius teaches anatomy at various universities in Italy.
After publishing
this book, Vesalius quits research and becomes the court physician to Charles
V, and his son the Spanish king Phillip II.
When Henry II is fatally wounded at a
tournament (jousting?) in 1559 Vesalius attends to him taking precedence over
Paré.
Asimov claims that Vesalius is accused of heresy, body snatching, and
dissection, and is apparently charged but his royal connections help him, and
his sentence is a trip to the Holy land, but other sources say that Vesalius
made a pilgrimage to Jerusalem.
On the way back the ship he is on is battered by storms,
but does reach Zante where Vesalius dies.
Basel, Switzerland  
456 YBN
[01/24/1544 AD]
3346)
Louvain, Belgium  
456 YBN
[1544 AD]
1179) The writings of Archimedes are translated in to Latin.

?  
455 YBN
[1545 AD]
1537) Cardano's father was a friend of Leonardo da Vinci.
Cardano becomes professor of
medicine at the University of Pavia in 1546.
Cardano believes in astrology.
Cardano is jailed
for some time for casting the horoscope of Jesus.
In 1539 Tartaglia showed Cardano a
method of solving cubic equations six years after Cardano promised to keep the
solution a secret.
?, Italy (presumably)  
455 YBN
[1545 AD]
1543) Pare writes his findings in French instead of Latin because he had no
formal education, and is looked down upon by the arrogant educated
establishment for this.
In 1565 Pare proves that the Bezoar Stone does not cure all
poisonings.
At this time and for 200 more years surgery is viewed as menial labor and done
by barbers, {shockingly and illogically} people who cut hair also perform
operations.
In 1536, Pare attains the rank of master barber-surgeon.
Pare works as a barber-surgeon in the
French army.
Pare is the surgeon to a series of four kings, Henry II and his 3 sons.
Paris, France  
454 YBN
[1546 AD]
1507)
written: Chemnitz, Saxony, Germany| published: Basel, Switzerland  
454 YBN
[1546 AD]
1508)
written: Chemnitz, Saxony, Germany | published: Basel, Switzerland   
454 YBN
[1546 AD]
3057)
Verona, Italy  
451 YBN
[1549 AD]
1555)
  
450 YBN
[1550 AD]
1184) The process begins with wrought iron and charcoal. It uses one or more
long stone pots inside a furnace. Iron bars and charcoal are packed in
alternating layers, with a top layer of charcoal and then refractory matter to
make the pot or 'coffin' air tight. Some manufacturers used a mix of powdered
charcoal, soot and mineral salts, called cement powder, which gave the process
its name. The pots are then heated from below for a week or more. Bars are
regularly examined and when the correct condition is reached the heat is
withdrawn and the pots are left until cool, usually around fourteen days. The
iron gains a little over 1% in mass from the carbon in the charcoal, and
becomes hetrogenous bars of blister steel. The bars are then shortened, bound,
heated and hammered, pressed or rolled to become shear steel.
Bohamia, Czech Republic  
450 YBN
[1550 AD]
1185)
Gotland, Sweden  
450 YBN
[1550 AD]
1506) From 1514 to 1518 Bauer studies classics, philosophy, and philology at
the University of Leipzig, which had recently been exposed to the humanist
revival. Following the custom of the times, he Latinizes his name to Georgius
Agricola (Bauer meaning "farmer"). After teaching Latin and Greek from 1518 to
1522 in a school in Zwickau, Agricola returns to Leipzig to begin the study of
medicine but finds the university in disarray because of theological quarrels.
A lifelong Catholic, he leaves in 1523 for more comfortable surroundings in
Italy. He studies medicine, natural science, and philosophy in Bologna and
Padua, finishing with clinical studies in Venice.
For two years Agricola works at the
Aldine Press in Venice, principally in preparing an edition of Galen's works on
medicine (which will be published in 1525).
From 1527 to 1533 Agricola is town
physician in Joachimsthal, a mining town in the richest metal-mining district
of Europe. Partly in the hope of finding new drugs among the ores and minerals
Agricola visits mines and smelting plants, talking to the better-educated
miners, and reading Classical authors on mining. These years provide the
material for most of his books, beginning with "Bermannus; sive, de re
metallica" (1530), a treatise on the Ore Mountains (Erzgebirge) mining
district.

In 1533 Agricola is appointed the town physician of Chemnitz where he remains
for the rest of his life.
Chemnitz, Saxony, Germany  
449 YBN
[1551 AD]
1549) Reinhold studies and teaches mathematics at the University of Wittenberg
  
449 YBN
[1551 AD]
1560) Belon gets a medical (physician/health) degree from the University of
Paris. King Frances I is one of the patrons of Belon. Belon is killed by
robbers in Paris while picking herbs.
France?  
449 YBN
[1551 AD]
5910) Philippe de Monte (CE 1521-1603) composes music in the form of madrigals,
chansons, masses and motets. The madrigal of this time, the name borrowed from
the 1300s form, has no resemblance in poetic or musical structure to the 1300
madrigal. Compared to the frottola, the earliest Renaissance madrigals, dating
from about 1530, are characterized by quiet and restrained expression, usually
written for three or four voices, mostly homophonic (melody supported by
chords) with occasional bits of imitation.

(Pinelli family) Naples, Italy  
448 YBN
[1552 AD]
1545) Eustacio is professor of medicine (health science) in the Collogio della
Sapienza in Rome (later the University of Rome) until his death.
The fact that his
book became a bestseller more than a century after his death shows the extent
of the religious restrictions on anatomists all through the Renaissance.
Rome, Italy  
447 YBN
[10/27/1553 AD]
1548) According to the Encyclopedia Brittanica, the execution of Michael
Servetus will produce a Protestant controversy on imposing the death penalty
for heresy, draws severe criticism upon John Calvin, and influences Laelius
Socinus, a founder of modern unitarian views.
Geneva, Switzerland  
447 YBN
[1553 AD]
1541) Frisius has a medical (health/physician/doctor) degree from Louvain.
Friesland (present day Netherlands)  
447 YBN
[1553 AD]
1547)
Toulouse, France (presumably)  
447 YBN
[1553 AD]
5911) Thomas Tallis (CE c1505-1585), English composer, composes music.

(Note how similar the Latin word "Gaude" (rejoice) is to the word "God"
Determine when the transition from "Deus" to "God" happened in England and
Germany.)

(Chapel Royal) London, England  
445 YBN
[1555 AD]
1558)
Zurich, Swizerland (presumably)  
445 YBN
[1555 AD]
1559)
Zurich, Swizerland (presumably)  
445 YBN
[1555 AD]
1561)
France?  
445 YBN
[1555 AD]
1773)
Siena?, Italy  
442 YBN
[1558 AD]
1556)
Zurich, Swizerland (presumably)  
441 YBN
[1559 AD]
1544) Colombo gets his medical (physician) degree in 1541 from the University
of Padua.
Columbo replaces Vesalius as anatomy professor.
Columbo goes to Rome to ask
Michelangelo to illustrate a book of anatomy that will surpass Vesalius, but
Michelangelo is in his 70s and refuses the job.
Columbo is the papal surgeon in Rome
until his death.
Columbo is a critic of the new anatomy of Vesalius.
"De re anatomica" is
Colombo's only formal written work.
Rome, Italy (presumably)  
440 YBN
[1560 AD]
1538)
Italy  
440 YBN
[1560 AD]
1563) Della Porta publishes a work on magic, and wrongly believes that magic is
a real phenomenon.
  
440 YBN
[1560 AD]
5906) Orlande de Lassus (CE c1530-1594) Franco-Flemish composer, composes music
around this time.

(court chapel of Duke Albrecht V of Bavaria) Munich, Bavaria (now
Germany)  
439 YBN
[1561 AD]
1562) Fallopius served as canon of the cathedral of Modena and then turned to
the study of medicine (health science) at the University of Ferrara, where he
becomes a teacher of anatomy. Fallopius then holds positions at the University
of Pisa (1548-51) and at Padua (1551-62).
Fallopius dies of tuberculosis before
age 40.
Venice, Italy  
439 YBN
[1561 AD]
5904) Giovanni Pierluigi da Palestrina (CE 1525/1526-1594) composes music in
the Renaissance era. His most famous mass, "Missa Papae Marcelli" ("Mass of
Pope Marcellus") is composed around this time (c1561).

(It's interesting to know that this is the music that surrounded the time and
life of Galileo, Descartes and other people making significant contributions to
science.)

(Saint Maria Maggiore Church) Rome, Italy  
437 YBN
[1563 AD]
5928) Vincenzo Galilei (CE c1520-1591), father of Galileo Galilei (CE
1564-1642), composes music for Lute around this time.

Padua, Italy (verify)  
433 YBN
[1567 AD]
1512)
  
431 YBN
[1569 AD]
1550) The word Mercator translates to "merchant".
Mercator's actual name is Gerhard Kremer,
but he Latinizes his name as is 1500s fad.
Mercator gets a Masters degree from the
University of Louvain in 1532 (at age 20).
Mercator makes instruments for Emperor
Charles V.
In 1544 Mercator is arrested and imprisoned on a charge of heresy. His
inclination to Protestantism, and frequent absences from Louvain to gather
information for his maps, had aroused suspicions. Mercator is one of 43
citizens charged. But the university authorities stand behind Mercator, and he
is released after seven months and resumes his former way of life. Mercator
obtains a privilege to print and publish books continues his scientific
studies.
Mercator studies under Gemma Frisius (the person that recognized that an
accurate time piece is needed to know longitude).

By age 24, Mercator is a skillful engraver, calligrapher, scientific-instrument
maker. In 1535-36 Mercator works with Gaspar à Myrica, (an engraver and
goldsmith) and Frisius in constructing a terrestrial globe and in 1537 a
celestial globe.
In 1552 Mercator moves permanently to Duisburg in the Duchy of Cleve
and becomes well-known. Mercator assists the duke in establishing a grammar
school by helping to design its curriculum. After establishing a cartographic
workshop and employing engravers, Mercator returns to his main interest.
Duchy of Cleves, Germany (presumably)  
431 YBN
[1569 AD]
1551)
Duchy of Cleves, Germany (presumably)  
431 YBN
[1569 AD]
1992) Mathematics historian David Smith describes this wok as the most
teachable and systematic treatment of algebra that appears in Italy up to this
time.
Bologna, Italy  
430 YBN
[1570 AD]
1186) A theodolite is an instrument for measuring both horizontal and vertical
angles, as used in triangulation networks. It is a key tool in surveying and
engineering work, but theodolites have been adapted for other specialized
purposes in fields like meteorology and rocket launch technology.
English  
430 YBN
[1570 AD]
1539)
  
428 YBN
[11/11/1572 AD]
1573) The name "Tycho" is the Latin version of the Danish "Tyge".
Brahe's wealthy and
childless uncle abducted Tycho at a very early age and raised him at his castle
in Tostrup, Scania, also financing Tycho's education.
Brahe enters the University of
Copenhagen at age 13 and studies law and philosophy.
When Brahe observes the predicted
eclipse of the sun on August 21, 1560, he changes his mind from politics to
astronomy and mathematics.
Brahe believes astrology and casts horoscopes, Asimov comments
that astrology is far more lucrative than astronomy in this time.
In 1565 at age 19,
Brahe gets in a dual over a point of mathematics and his nose is cut off, so
Tycho wears a false nose of metal for the rest of his life.
In August 1563,
when Brahe makes his first recorded observation, a conjunction, or overlapping,
of Jupiter and Saturn, he finds that the existing almanacs and ephemerides,
which record stellar and planetary positions, are very inaccurate. The
Copernican tables are several days off in predicting this event. At that point
in his youth, Tycho decides to devote his life to the accumulation of accurate
observations of stars (the so-called heavens), and buys instruments in order to
make his own tables in order to correct the existing tables.
The is a rumor of Brahe
making astronomical observations in court dress.
In 1573, Brahe marries a peasant girl
whom he loves and spends his life with.
In 1588 Frederick II dies, and his successor
Christian IV ends funding for Tycho.
In 1597 Tycho accepts the invitation of Emperor
Rudolf II and goes to Germany.

In his new headquarters in Prague, Brahe finds Johann Kepler as an assistant.
Brahe
corresponds with Galileo.
On his death bed, perhaps from a ruptured bladder, Tycho moans
"Oh, that it may not appear I have lived in vain".
Tycho gives Kepler his observation
data and Kepler prepares the tables of planetary motions. Sagan explains that
Tycho delays giving Kepler all of his data. Maybe there is some relation
between Tycho's realization that the comet had an non-circular orbit and Kepler
recognizing the true orbit (at least in two dimensions) of a ellipse for
planets.
Brahe is the last naked eye astronomer.
Scania, Denmark (now Sweden)  
427 YBN
[1573 AD]
1574) Tycho establishes a printing shop to produce and bind his manuscripts,
imports Augsburg craftsmen to construct the finest astronomical instruments,
gets Italian and Dutch artists and architects to design and decorate his
observatory, and invents a pressure system to provide the then uncommon
convenience of lavatory facilities.
But Frederick II will die in 1588, and
under his son, Christian IV, most of Tycho's income will be stopped, partly
because of the increasing needs of the state for money.
Herrevad Abbey, an abbey near Ljungbyhed, Scania, Denmark (now Sweden)  
427 YBN
[1573 AD]
1575) Brahe's "Astronomiae instauratae mechanica" published in 1598 contains
his autobiography and a description of his instruments.

Tycho will leave Denmark in 1587 and move to Prague, carrying along the records
of his observations and most of his instruments. In 1600 Johannes Kepler will
join him as his assistant. After Tycho's death in 1601, Kepler will prepare
Tycho's astronomical studies for publication in "Astronomiae instauratae
progymnasmata" (1602-1603). Kepler is then free to use the valuable data to
create his own system, (where the planets have elliptical orbits) which will
lay the foundations for Newton's gravitational astronomy.
Island of Hven (now Ven, Sweden)  
426 YBN
[1574 AD]
5908) John Bull (CE c1562-1628), English composer, and one of the leading
keyboard virtuosos of this time composes music. Bull graduates from Cambridge
(1589) and Oxford (1592).

(Is it correct to say that the harpsichord finds popularity in England before
Germany and Italy?)

(John Bull is an example of a somewhat radical change to a much more technical
and faster playing style that Vivaldi will also display. This style is
extremely different from the Gregorian chants and may represent a radical
change in technology and education - in particular the possible birth of neuron
reading.)

(Chapel Royal) London, England  
421 YBN
[1579 AD]
1567) Vieta, is very good at deciphering codes. A Huguenot sympathizer, Vieta
deciphers a complex cipher of more than 500 characters used by King Philip II
of Spain in his war to defend Roman Catholicism from the Huguenots. When
Philip, assuming that the cipher could not be broken, discovered that the
French were aware of his military plans, he complained to the pope that black
magic was being employed against his country.

Vieta occupies a high administrative office under Henry IV.
Vieta is the father of
modern algebra.
Vieta prefers the word "analysis" to "algebra".
?, France  
420 YBN
[1580 AD]
3221)
Netherlands  
419 YBN
[1581 AD]
1588)
London, England  
419 YBN
[1581 AD]
1597) Galileo is the oldest son of Vincenzo Galilei, a musician who made
important contributions to the theory and practice of music and who may perform
some experiments with Galileo in 1588-89 on the relationship between pitch and
the tension of strings.
A Tuscan tradition is that the oldest son gets a variation of
the family last name for first name, and this is why Galileo received his first
name.

Galileo studies to be a physician at the University of Pisa, but after reading
Archimedes, whom Galileo greatly admires, Galileo talks his reluctant father
from allowing Galileo to go into mathematics and science.
In 1585 Galileo leaves the
university without obtaining a degree, and for several years he gives private
lessons in the mathematical subjects in Florence and Siena.
Ironically, Galileo
recognizes that inaccurate time keeping is a major problem, and Huygens will
later use the principle of the pendulum found by Galileo to regulate a clock
solving the problem of accurate time keeping that Galileo has.
(square-cube law I am
doubting and am going to ignore for now)
Galileo's work makes him unpopular in Pisa
and he moves to Padua (in Venetian territory, which according to Asimov is a
region of considerable intellectual freedom at this time), his new job pays 3
times his previous salary, although Asimov paints Galileo as always in debt
from living gaily and generously, always in trouble, and unpopular with
influential people.
Galileo does not wear academic robes, although this costs him
several fines.
Galileo is a popular lecturer and students flock to hear him, coming in
numbers as high as 2000 (although this may be from an exaggerated report).
Galileo's
studies of the sun damage his eyes, and he goes blind in his old age.
After the
telescope, both Venice and Florence offer him lucrative positions. To the
annoyance of the Venetians Galileo choses to move to Florence.
1611 Galileo visits Rome
where he is greeted with honor and delight.
Galileo is refused burial in consecrated
(blessed by religious human?/church property?) ground.
Galileo's "Dialogue" is not
removed from the the Roman Catholic Index of prohibited books until 1825.
In 1965
Pope Paul VI will speak highly of Galileo.
Galileo will not be officially forgiven until
the 1960s...um...a little late.

Galileo (wrote) "By denying scientific principles, one may maintain any
paradox.".
Pisa, Italy  
418 YBN
[1582 AD]
1180) Richard Butt Hakluyt (c.1552 - November 23, 1616), a writer in England,
writes a book "Voyages..." that describes America.

England  
418 YBN
[1582 AD]
1566) In 1565, Clavius lectures at the Collegio Romano in Rome and stays there
for the rest of his life.
Clavius is the last diehard opponent of the sun-centered
theory revived by Copernicus.
Many Protestant nations and people object to the calendar
reform.
Rome, Italy  
417 YBN
[1583 AD]
1569) Scaliger studies at Bordeaux, and in 1559 moves to Paris to study Greek
and Latin and then begins to teach himself Hebrew, Arabic, Syrian, Persian, and
the principal modern languages.
In 1562 Scaliger converts to Protestantism.
Scaliger leaves France for
Geneva in 1572 just before St Bartholomew's Day massacre of Protestant people.
In 1593
Scaliger teaches at Univeristy of Leiden (a Protestant university).
?, France  
416 YBN
[1584 AD]
1576) Giordano Bruno (CE 1548-1600), Italian philosopher, writes 6 Italian
Dialogs in which he explains his belief in the infinity of space, that the
Earth goes around the sun (heliocentric theory), and the atom theory.
Oxford, England  
415 YBN
[1585 AD]
1581) Somewhere people actually took note that Stevinus was from so-called
illegitimate birth, from parents who were not married.
Stevinus marries at 64 and has 4
children.
Stevin is also known as Stevinus, the Latinized form of his name.
Stevin helps
to popularize the practice of writing scientific works in modern languages (in
his case Dutch) rather than Latin, which for so long had been the traditional
European language of learning.
Netherlands (presumably)  
414 YBN
[1586 AD]
1415) Al-Amili becomes a famous religious scholar as the "shaikh al-islam", the
chief relgious authority in the country of Isfahan, the Safavid capital.
Al-Amili's tomb, like that of Nasir al-Din is visited by people who flock
regularly to the Shiite shrine cities, such as Meshed and Kazimain.
Isfahan, Iran  
414 YBN
[1586 AD]
1582)
(possibly Antwerp or Nassau), Netherlands  
414 YBN
[1586 AD]
1583)
Netherlands (presumably)  
414 YBN
[1586 AD]
1598)
Florence or Sienna, Italy  
412 YBN
[1588 AD]
1579) This text is set against contemporary mathematicians and philosophers. At
Helmstedt, Germany, in January 1589 Bruno will be he was excommunicated by the
local Lutheran Church.
?, Germany  
411 YBN
[1589 AD]
1182) Two hundred years will pass before the water closet is popularized.
Somerset, England  
411 YBN
[1589 AD]
5905)
London, England  
411 YBN
[1589 AD]
5913) Dancing becomes popular during the Renaissance. One of the most
comprehensive and popular dance manuals of the Renaissance is Thoinot Arbeau's
"Orchesographie" (1589). In this work Arbeau explains the social necessity of
dance to his student Capriol (translated from French):
"Capriol: I much enjoyed fencing
and tennis, and this placed me upon friendly terms with ypoung men. But,
without knowledge of dancing, I could not please the damsels, upon whom, it
seems to me, the entire reputation of an eligible young man depends.
Arbeau: You are
quite right, as naturally the male and female seek one another, and nothing
does more to stimulate a man to acts of courtesy, honor, and generosity than
love. And if you desire to marry you must realize that a mistress is won by the
good temper and grace displayed while dancing, because ladies do not like to be
present at fencing or tennis, lest a splintered sword or a blow from a tennis
ball cause them injury...".

Europe  
410 YBN
[1590 AD]
1580)
Frankfurt am Main, Germany  
409 YBN
[1591 AD]
1568) Vieta, is very good at deciphering codes. A Huguenot sympathizer, Vieta
deciphers a complex cipher of more than 500 characters used by King Philip II
of Spain in his war to defend Roman Catholicism from the Huguenots. When
Philip, assuming that the cipher could not be broken, discovered that the
French were aware of his military plans, he complained to the pope that black
magic was being employed against his country.

Vieta occupies a high administrative office under Henry IV.
Vieta is the father of
modern algebra.
Vieta prefers the word "analysis" to "algebra".
?, France  
408 YBN
[1592 AD]
1587) Alpini gets a Medical (Health) degree from the University of Padua, and
is a professor of Botany there in 1593.
Venice, Italy  
408 YBN
[1592 AD]
1613) Earliest thermometer.

The invention of the thermometer is generally credited to the Italian
mathematician-physicist Galileo Galilei (1564–1642). Galilei calls this
device a thermoscope.

In Galilei's thermometer, the changing temperature of an inverted glass vessel
produces an expansion or contraction of the air within it, which in turn
changed the level of the liquid with which the vessel's long, open-mouthed neck
is partially filled.

This device is very inaccurate (because of the changing air pressure on earth)
and Amontons 100 years later will improve the design.

This general principle will be perfected in succeeding years by experimenting
with liquids such as mercury and by providing a scale to measure the expansion
and contraction brought about in such liquids by rising and falling
temperatures.
Padua, Italy  
408 YBN
[1592 AD]
5917) Jan Pieterszoon Sweelinck (CE 1562-1621), Netherlands composer.

(Oude Kerk {old church}) Amsterdam, Netherlands  
405 YBN
[1595 AD]
1586)
Scotland (presumably)  
404 YBN
[08/??/1596 AD]
1616) Fabricius is a friend of Tycho Brahe, and Kepler.
Fabricius is murdered by one of
his parisheners, who Fabricius had threatened to expose for theft. Another
story relates that after denouncing a local goose thief from the pulpit, the
accused man struck David Fabricius in the head with a shovel and killed him.
Esens, Frisia (now northwest Germany and northeast Netherlands) (guess)  
404 YBN
[1596 AD]
1183) John Harrington, the inventor of the first flush toilet, writes a book
called "A New Discourse upon a Stale Subject: The Metamorphosis of Ajax" about
his invention. He publishes the book under the pseudonym of Misacmos. The book
makes political allusions to the Earl of Leicester that anger Queen Elizabeth
I, and he will be again banished from the court. The Queen's mixed feelings for
him may be the only thing that saves Harrington from being tried at Star
Chamber.

Somerset, England  
404 YBN
[1596 AD]
1552) The father of Rheticus was a physician who was beheaded for sorcery when
Rheticus was age 14.
Rheticus studies at Zürich where he meets Paracelsus, and
Gesner is a schoolmate.
Rheticus gets a masters degree and teaches Mathematics at the
University of Wittenberg.
Asimov describes Rheticus as "Copernicus' first disciple".
Kassa, Hungary  
404 YBN
[1596 AD]
1621) After failing to find a unique arrangement of polygons that fits known
astronomical observations (even with extra planets added to the system), Kepler
begins experimenting with 3-dimensional polyhedra. He finds that each of the
five Platonic solids can be uniquely inscribed and circumscribed by spherical
orbs; nesting these solids, each encased in a sphere, within one another would
produce six layers, corresponding to the six known planets-Mercury, Venus,
Earth, Mars, Jupiter, and Saturn. By ordering the solids correctly-octahedron,
icosahedron, dodecahedron, tetrahedron, cube-Kepler finds that the spheres can
be placed at intervals corresponding (within the accuracy limits of available
astronomical observations) to the relative sizes of each planet"s path,
assuming the planets circle the Sun. Kepler also finds a formula relating the
size of each planet"s orb to the length of its orbital period: from inner to
outer planets, the ratio of increase in orbital period is twice the difference
in orb radius. However, Kepler later rejected this formula, because it is not
precise enough.

As Kepler indicates in the title, he thinks that he has revealed God"s
geometrical plan for the universe. Much of Kepler"s enthusiasm for the
Copernican system stems from his theological convictions about the connection
between the physical and the spiritual; the universe itself is an image of God,
with the Sun corresponding to the Father, the stellar sphere to the Son, and
the intervening space between to the Holy Spirit. His first manuscript of
Mysterium contains an extensive chapter reconciling heliocentrism with biblical
passages that seem to support geocentrism.
Graz, Austria  
403 YBN
[1597 AD]
1601)
Padua, Italy  
403 YBN
[1597 AD]
5902) John Dowland (CE c1563-1626), English composer, composes music for voice
and lute. Downland graduated from Oxford (1588). In the best of his 84 ayres
for voice and lute (published mainly in 4 vols., 1597, 1600, 1603, 1612),
Dowland raises the level of English song, matching perfectly in music the mood
and emotion of the verse.

London, England  
403 YBN
[1597 AD]
5907) Giovanni Gabrieli (CE c1553-1612), Italian composer, composes music
around this time and represents the highest point of the High Renaissance
Venetian school. This work "In Ecclesiis" is a good example of the "grand
concerto", a genre that combines vocal soloists with choral and instrumental
ensembles.

(St Mark's Cathedral) Venice, Italy  
400 YBN
[02/17/1600 AD]
1578) Giordano Bruno (CE 1548-1600), Italian philosopher, is burned alive at
the stake after a seven year trial.

Bruno might have lived had he recanted as Galileo will, but Bruno chooses not
to.

On Feb. 8, 1600, when the death sentence is formally read to Bruno, he
addresses his judges, saying: "Perhaps your fear in passing judgment on me is
greater than mine in receiving it." Bruno is brought to the Campo de' Fiori,
his tongue in a gag, and burned alive.

One witness, Friar Celestino reports that Bruno stated that (translated) "That
there are many worlds, and all the stars are worlds, and believing that this is
the only world is supreme ignorance.". The sentence states that Bruno said that
it is "...a great blasphemy to say that bread transubstantiates into flesh".
Eight of Bruno's heresies are identified, although this document has not been
found, but if drawn from the original accusation then they probably included
the claim of belief in multiple worlds.

Bruno refuses to accept the cross held out to him at the last moment.

Some victims, such as a Scottish person, in 1595 are burned in a shirt of pitch
which is put over their naked body so that they will not die as quickly, and so
the burning before death can be as painful as possible.

Imagine what a painful, tortuous, cruel, and terrible death, being burned alive
must be. Only the most criminally, vicious, violent and sadistic human could
support inflicting that on a fellow human or any species, in particular a
nonviolent human, no matter how bad they might be.

This punishment may influence Galileo's actions before the Inquisition.

All of Giordano Bruno's works are placed on the "Index Librorum Prohibitorum"
in 1603.
Rome, Italy  
400 YBN
[1600 AD]
1564) In 1612 Fabricius does exhaustive study of chick(en) embyro.
In 1559, Fabricius
gets a medical (physician) at Padua.
In 1565, Fabricius is a professor at Padua.
Fabricius is
a pupil of Fallopius.
The English anatomist William Harvey is Fabricius' pupil.
Padua, Italy (presumably)  
400 YBN
[1600 AD]
1571) Gilbert gets a medical (health) degree from Cambridge in 1569.
Gilbert is the
president of the college of physicians in London in 1600.
In 1601 Gilbert is
appointed court physician to Queen Elizabeth I at 100 pounds/year.
Gilbert follows the work
of Peter Peregrinus.
London, England (presumably)  
398 YBN
[1602 AD]
1594) Sanctorius, is the Latin name of Santorio.
Sanctorius earns a medical Degree from
the University of Padua in 1582.
Sanctorius is the physician to King Sigismund III of
Poland for 14 years
In 1611 Sanctorius teaches at the University of Padua.
(thought about
80,000 different possible diseases?)
Padua, Italy (presumably)  
398 YBN
[1602 AD]
5915) Giulio Caccini (CE 1545-1618) Italian composer and singer composes
operas.

(Medici court) Florence, Italy  
398 YBN
[1602 AD]
5916)
(Medici court) Florence, Italy  
397 YBN
[1603 AD]
1193) Sir Henry Platt in England suggested that coal might be charred in a
manner analogous to the way charcoal is produced from wood. This will
eventually lead to the use of coke in a less costly production of steel that
does not depend on wood. Coke is a solid carbonaceous residue derived from
low-ash, low-sulfur bituminous coal. Bituminous coal is a relatively hard coal
containing a tar-like substance called bitumen. Bituminous coal is an organic
sedimentary rock formed by diagenetic and submetamorphic compression of peat
bog material.
In order to be used for industrial processes, bituminous coal must first be
"coked" to remove volatile components. Coking is achieved by heating the coal
in the absence of oxygen, which drives off volatile hydrocarbons such as
propane, benzene and other aromatic hydrocarbons, and some sulfur gases. This
also drives off a considerable amount of the water contained in the bituminous
coal. Coking coal will be blended with uncoked coal for power generation. The
primary use for coking coal will be in the manufacture of steel, where carbon
must be as volatile and ash free as possible.

England  
397 YBN
[1603 AD]
1565)
Padua, Italy (presumably)  
397 YBN
[1603 AD]
1636) Bayer is a lawyer by profession.
Bayer unsuccessfully tries to impose names from Old
and New Testament onto constellation names. That is good news, and I think it
indicates that the majority of people in astronomy and science generally form
the opposite end of the spectrum from those who strongly support religion,
which is only logical because most of the stories of religions are obvious lies
and those involved in science tend to be less easily fooled and smarter.
Later Roman
numerals will be added to the system.
Augsburg, Germany  
397 YBN
[1603 AD]
1641) Scheiner teaches Hebrew and mathematics, first at Freiburg, then at
Ingolstadt.
Scheiner publishes his last work "Prodromus", a pamphlet against the
heliocentric theory which was published posthumously in 1651.
Dillingen, Germany  
397 YBN
[1603 AD]
3678)
Bologna, Italy  
396 YBN
[01/01/1604 AD]
1622)
Prague, (now: Czech Republic) (presumably)  
396 YBN
[10/??/1604 AD]
1623) Kepler used the occasion both to render practical predictions (for
example Kepler predicts the collapse of Islam and the return of Jesus to earth)
and to speculate theoretically about the universe, for example, that the star
was not the result of chance combinations of atoms and that stars are not suns.
Clearly, all major religions will collapse eventually, in my estimation around
2800 CE, however, there may always be small groups of humans that still worship
certain ancient humans as gods. It is interesting that Kepler could not grasp
the truth that stars are other suns as Nicholas Krebs of Cusa had correctly
understood and publicly recorded earlier.
Prague, (now: Czech Republic) (presumably)  
396 YBN
[1604 AD]
1600)
?  
396 YBN
[1604 AD]
1635)
Prague, (now: Czech Republic) (presumably)  
395 YBN
[1605 AD]
1590) Francis Bacon is not related to Roger Bacon 350 years before.
Bacon studies law
at Cambridge.
In 1584 Bacon enters Parliament.
Bacon is the confidential aide to the earl of Essex.
After
Essex' abortive attempt of 1601 to seize the Queen and force her dismissal of
his rivals, Bacon, views Essex as a traitor, tries and convicts Essex for
treason, and Essex is executed.
In 1621 Bacon is accused of taking bribes as
judge, and evidence is overwhelming.
Some claim Bacon wrote Shakespeare's plays
because Bacon was educated and Shakespeare was not, and Bacon writes in Latin,
(where Shakespeare apparently does not?).
Bacon accepts astrology.
Bacon rejects the sun-centered
theory.
Harvey describes Bacon as writing about science "like a lord chancellor".
London, England (presumably)  
395 YBN
[1605 AD]
1630)
Prague, (now: Czech Republic)  
394 YBN
[1606 AD]
1570)
Leiden, Netherlands (presumably)  
394 YBN
[1606 AD]
1589) Libavius is the Latinized "Libau".
Libavius gets a Medical (Health
Science/Physician) Degree at the University of Jena in 1581.
Libavius is professor of
history and poetry at the University of Jena from 1586 to 1591 and then becomes
town physician and inspector of the Gymnasium at Rothenburg.

Libavius founds a school (the Gymnasium Casimirianum) in Coburg in 1605.
  
394 YBN
[1606 AD]
2099)
Australia  
393 YBN
[1607 AD]
5912)
Mantua, Italy  
392 YBN
[1608 AD]
1618) Telescope and microscope.

Hans Lippershey (LiPRsE) (CE 1570-1619), spectacle maker from the United
Netherlands, is traditionally credited with inventing the telescope (1608).

Lippershey places a double convex lens (the "object glass") at the farther end
of a tube, and a double concave lens (the "eyepiece") at the nearer end.

This is a refracting telescope, which spreads light out using two transparent
lens.

Lippershey applies to the States General of the Netherlands for a 30-year
patent for his instrument, which he called a kijker ("looker"), or else an
annual pension, in exchange for which Lippershey offers not to sell telescopes
to foreign kings. Two other claimants to the invention come forward, Jacob
Metius and Sacharias Jansen. The States General rules that no patent should be
granted because so many people know about the device and that it is so easy to
copy. However, the States General grants Lippershey 900 florins for the
instrument but required its modification into a binocular device.

An interesting truth is that a telescope and microscope are the same thing in
that they take light from a small area and spread it out into a larger area.
One difference is that a telescope draws from a larger area. There is not as
much interest in humans taking light from a large space and compacting it
together into a small area.
Netherlands  
391 YBN
[08/??/1609 AD]
1603)
Venice, Italy  
391 YBN
[12/??/1609 AD]
1604)
Venice, Italy  
391 YBN
[1609 AD]
355)
(University of Pisa) Pisa, Italy  
391 YBN
[1609 AD]
1599)
(University of Padua) Padua, Italy  
391 YBN
[1609 AD]
1602)
?, Italy  
391 YBN
[1609 AD]
1619) German astronomer, Johannes Kepler (CE 1571-1630) shows that planets move
in elliptical orbits with the Sun at one focus of the ellipse.

After the astronomer Tycho Brahe (1546–1601) dies, although there is a
political struggle with Tycho’s heirs, Kepler is ultimately able to work with
Tycho's astronomical data which is accurate to within 2′ of arc. With this
precise data Kepler is able to discover his "first law" (1605), that Mars moves
in an elliptical orbit.

Kepler discovers three major laws of planetary motion: (1) the planets move in
elliptical orbits with the Sun at one focus; (2) A line connecting a planet and
the Sun will sweep over equal areas in equal times (the “area law”)- this
means the closer a planet is to the Sun, the faster the planet will move
according to a fixed and calculable rule; and (3) there is an exact
relationship between the squares of the planets’ periodic times and the cubes
of the radii of their orbits (the “harmonic law”).

Kepler does not publish his discoveries until 1609 in the "Astronomia Nova"
(New Astronomy).

In 1618 Kepler's mother, who dabbles in the occult, is arrested as a witch, and
although not tortured, does not survive long after her release, which is
obtained through the long-term efforts of Johan.
Weil der Stadt (now part of the Stuttgart Region in the German state of
Baden-Württemberg, 30 km west of Stuttgart's center)  
391 YBN
[1609 AD]
1620)
Weil der Stadt (now part of the Stuttgart Region in the German state of
Baden-Württemberg, 30 km west of Stuttgart's center)  
390 YBN
[01/??/1610 AD]
1605) Moons of Jupiter seen and their period determined by Galileo Galilei.

Galileo finds that planet Jupiter has four moons, visible only by telescope,
that circle Jupiter with regular motions. Within a few weeks Galileo determines
the periods of each moon. In addition, Galileo is the first to see that planet
Venus has phases like the moon.

Galileo also finds many more stars can be seen with the telescope than with the
naked eye.

Galileo describes these earth-shaking finds in a little book, "Sidereus
Nuncius" ("The Sidereal Messenger").

Kepler will call these moons "satellites" and they are known as the "Galilean
satellites". These moons are Io, Europa, Ganymede and Callisto.

Jupiter and it's moons is an example of small bodies orbiting a large body and
this is evidence in support of the sun-centered theory, and is definite proof
that not all bodies orbit the Earth.

Galileo is first to see that the planets appear as globes, but the stars
appears as points, and concludes that the stars must be very far away, and that
the universe may be infinitely large.
Venice, Italy  
390 YBN
[1610 AD]
1624) In this work Kepler speculates, among other things, that the distances of
the newly discovered Jovian moons might agree with the ratios of the rhombic
dodecahedron, triacontahedron, and cube. (Of course the theory of perfect
solids is wrong.)
Prague, (now: Czech Republic) (presumably)  
390 YBN
[1610 AD]
1626)
Prague, (now: Czech Republic)  
389 YBN
[06/??/1611 AD]
1617) Dutch astronomer, Johannes Fabricius (FoBrisEuS) (CE 1587-1615), is the
first to show that the Sun has spots and rotates around its own axis.

Johannes (1587-1615) returns from a university in the Netherlands with
telescopes that he and his father David use (in addition to a camera obscura)
to observe the Sun.

Seeing sunspots on the eastern edge of the disk, steadily move to the western
edge, disappear, then reappear at the east again suggests that the Sun rotates
on its axis, which had been postulated before but never backed up with
evidence.

Fabricius (FoBrisEuS) publishes this discovery in "Narratio de maculis in sole
observatis et apparente earum cum sole conversione" ("Account of Spots Observed
on the Sun and of Their Apparent Rotation with the Sun", 1611).
Esens, Frisia (now northwest Germany and northeast Netherlands) (guess)  
389 YBN
[1611 AD]
1625)
Prague, (now: Czech Republic)  
389 YBN
[1611 AD]
1627)
Prague, (now: Czech Republic)  
389 YBN
[1611 AD]
1628)
Prague, (now: Czech Republic)  
389 YBN
[1611 AD]
1629)
Prague, (now: Czech Republic)  
389 YBN
[1611 AD]
1637)
??, Germany  
388 YBN
[01/12/1612 AD]
1642) This book is responsible for an unpleasant argument between Scheiner and
Galileo Galilei.
Ingolstadt, Bavaria, Germany (presumably)  
388 YBN
[1612 AD]
1595)
Padua, Italy (presumably)  
388 YBN
[1612 AD]
3680)
(Collegio Romano) Rome, Italy  
387 YBN
[1613 AD]
1607)
Florence, Italy  
386 YBN
[1614 AD]
1584) Scottish mathematician, John Napier (nAPER) invents exponential notation
and logarithms.

Napier describes his invention in his book "Mirifici Logarithmorum Canonis
Descriptio" ("Description of the Marvelous Canon of Logarithms").

Napier invents exponential notation (in 1594), finding that all numbers can be
expressed in exponential form. That is, 4 can be written as 22, while 8 can be
written as 23, and 5, 6, and 7 can be written as 2 to some fractional power
between 2 and 3. Napier finds that once numbers can be written in such
exponential form, multiplication can be done by adding exponents, and division
can be done by subtracting exponents. In this way, multiplication and division
are as simple as addition and subtraction.

Napier's tables of logarithms are very popular.
Scotland (presumably)  
386 YBN
[1614 AD]
1596)
Padua, Italy (presumably)  
386 YBN
[1614 AD]
1638) Marius is "Mayer" latinized.
Marius studies astronomy under Tycho Brahe.
Marius studies
medicine in Italy.
Marius publishes one of Galileo's books under a different author's
name. (purpose?)
Marius claims to have seen the Jupiter moons in 1609 before Galileo.
??, Germany  
386 YBN
[1614 AD]
5898)
(Magdeburg, Kassel, Halle, Dresden) Germany  
385 YBN
[1615 AD]
5909) Orlando Gibbons (CE 1583-1625), English composer, composes music.
(Chapel Royal) London, England  
385 YBN
[1615 AD]
5920) Heinrich Schütz (CE 1585-1672), German composer, composes mostly sacred
vocal music at this time. Schütz is the greatest German composer of the 1600s
and the first recognized internationally. His output is almost exclusively
sacred. Schütz sets mainly biblical texts and composes the first German opera
"Dafne" (1627).

(electoral court) Dresden, Germany  
384 YBN
[1616 AD]
1608) Psalm 93:1, Psalm 96:10, and 1 Chronicles 16:30 incorrectly state that
"the world is firmly established, it cannot be moved." Psalm 104:5 says, "the
Lord set the earth on its foundations; it can never be moved." Ecclesiastes 1:5
states that "the sun rises and the sun sets, and hurries back to where it
rises."

Before this, in 1613 Galileo wrote a letter to his student Benedetto Castelli
(1528-1643) in Pisa about the problem of squaring the Copernican theory with
certain biblical passages. Inaccurate copies of this letter were sent by
Galileo's enemies to the Inquisition in Rome, and Galileo had to retrieve the
letter and send an accurate copy.

Also earlier, several Dominican fathers in Florence lodged complaints against
Galileo in Rome, and Galileo went to Rome to defend the Copernican cause and
his good name. Before leaving, he finished an expanded version of the letter to
Castelli, now addressed to the grand duke's mother and good friend of Galileo,
the dowager Christina. In his Letter to the Grand Duchess Christina, Galileo
discussed the problem of interpreting biblical passages with regard to
scientific discoveries but, except for one example, did not actually interpret
the Bible.

The people appointed pope always take an alias, perhaps to cover their tracks
when they routinely dispense injustice and idiocy. but probably more likely to
make them appear to be transformed, not a regular human anymore.
Rome, Italy  
384 YBN
[1616 AD]
1644) English Physician, William Harvey (CE 1578-1657), understands the
circulatory system; that the heart is a muscle that contracts to push blood
out, that blood can only move in one direction in blood vessels (not back and
forth as Galen had believed), and that blood moves in a circle from the heart
to the arteries, from the arteries to the veins, and through the veins back to
the heart.
5
Harvey is the first to propose that the heart is a muscle that propels blood
out on a circular course through the body, leaving through arteries and
returning to the heart through veins. From dissection Harvey understands that
the valves separating the two upper chambers (auricles) from the two lower
chambers (ventricles) are one way valves. Blood can move from auricle to
ventricle but not the other way. Fabricius had recognized that there are
one-way values in the veins too, blood in the veins can only travel toward the
heart and not away from it. When Harvey ties an artery, it is the side toward
the heart that bulges with blood. When he ties off a vein, the side away from
the heart bulges. Harvey is the first to recognize that blood moves in one
direction only, not back and forth in the vessels (arteries and veins) as Galen
had believed. Harvey also notes that blood spurts from a cut artery at the same
time as muscular contractions of the heart.

In this year at St. Bartholomew's Hospital, in London, Harvey gives the first
of his Lumleian Lectures before the Royal College of Physicians, the manuscript
notes of which contain the first account of blood circulation.

Some consider Harvey the founder of modern physiology.

The functioning of the heart and the circulation had remained almost at a
standstill ever since the time of the Greco-Roman physician Galen, 1,400 years
earlier. Harvey's courage, penetrating intelligence, and precise methods are to
set the pattern for research in biology and other sciences for succeeding
generations. William Harvey and William Gilbert, the investigator of the magnet
are credited with initiating accurate experimental research in this early
modern period.
-------
6
William, is the oldest of nine children.
Harvey gets a degree from Cambridge in 1597 at
age 19.
Harvey takes medical (health science) courses at the University of Padua
(simov claims that since Mondino 300 years before, the University of Padua
remained as best medical (physician) school on earth), where Harvey studies
with Fabricius ab Aquapendente and others.
Harvey gets a Medical degree in 1602.
Harvey then
returns to England, marries, and creates a successful practice.
Harvey makes news by
examining and exonerating several suspected witches and by performing a
postmortem examination on Thomas Parr, who is reputed to have lived 152 years.
Harvey
is a staunch royalist.
Harvey is court physician to James I, and Charles I until Charles
I is beheaded in 1649.
Harvey is the doctor of Francis Bacon.
By 1616, Harvey has dissected
80 different species of animal.
Harvey survives the English Civil War, although
revolutionaries do break into his home and destroy some notes and specimens.
Des
cartes supports Harvey's theory of blood circulation.
In 1653 appears the first
English edition of De motu cordis, and Harvey's genius is fully recognized.
Harvey gives buildings and a library to the Royal College of Physicians. This
library is in use for less than 14 years, being destroyed in the Great Fire of
London in 1666, so that very few of Harvey's books have survived to the present
day.
In 1654, Harvey is elected president of the College of Physicians, but declines
the privilege, preferring to spend his last years in peace.
London, England  
384 YBN
[1616 AD]
1654) Baffin thinks that no such path exists.
Asimov claims that only for special ice
breaking ships is it possible (to move directly over the top of the earth by
ship). Is there some short path from Europe to India over the north pole? Is
there water under the north pole?
Baffin Bay  
384 YBN
[1616 AD]
1831) Niccolò Zucchi (CE 1586-1670) builds the earliest known reflecting
telescope.

This telescope is before the telescopes of James Gregory and Isaac Newton.

A reflecting telescope focuses light reflected off a parabolic shaped (concave)
mirror instead of through a lens. These telescopes remove the problem of
"chromatic aberration", found in the glass lens refracting telescopes.
Chromatic aberration is the way light is separated into it's component colors
when refracted, this causes objects to appear to be blurred and have colored
edges. The reflecting telescope has the two advantages of no light being
absorbed by the glass lens (or reflected back away from the viewer), and
eliminates the chromatic aberration effect.

With this telescope Zucchi discovers the (cloud) belts of the planet Jupiter
(1630) and examines the spots on Mars (1640).
Rome, Italy  
383 YBN
[1617 AD]
1592) Briggs gets a Masters at Cambridge in 1585, and lectures in 1592.
In 1596
Briggs is a professor of geometry at Greshman College in London.
London, England (preumably)  
383 YBN
[1617 AD]
1653)
Leiden, Netherlands (presumably)  
383 YBN
[1617 AD]
1852)
Venice, Italy (presumably)  
381 YBN
[1619 AD]
1632)
Linz, Austria  
381 YBN
[1619 AD]
1643)
Innsbruck, Austria  
381 YBN
[1619 AD]
1656) Cysat is a pupil of Scheiner, enters Jesuit order in 1604 and becomes a
priest.
Cysat is professor of mathematics at the Jesiut college of Ingolstadt in
Bavaria.
In 1611 Cysat is an early user of the telescope.
Ingolstadt, Bavaria, Germany  
380 YBN
[08/??/1620 AD]
1631)
Linz, Austria  
380 YBN
[1620 AD]
1591)
London, England (presumably)  
379 YBN
[1621 AD]
1651) Dutch mathematician, Willebrord von Roijen Snell (CE 1580-1626),
identifies the law of refraction.

Snell proves that the angle of light passing from one material into a material
of different density is not related to the angle of the light with the surface
as Ptolemy thought, but is related to the sine of the angle. This law is called
Snell's law.

Snell's law was first described in a formal manuscript in a 984 CE writing by
Ibn Sahl, who used it to work out the shapes of lenses that focus light with no
geometric aberrations, known as anaclastic lenses.

It was described again by Thomas Harriot in 1602, who did not publish his
work.

Snell produces a new method for calculating π, the first such improvement
since ancient times.

The index of refraction of some substance varies depending on the wavelength of
the light, in other words the amount a beam of light is bent in some substance
varies depending on the wavelength of the light.
In many media, wave velocity
changes with frequency or wavelength of the wave moving through it. This is
called dispersion. The result is that the angles determined by Snell's law also
depend on frequency or wavelength, so that a ray of mixed wavelengths, such as
white light, will spread or disperse. Such dispersion of light in glass or
water underlies the origin of rainbows, and also is the basis of glass prisms
(or else all the beams of white light would pass through the prism
unseparated), since different wavelengths appear as different colors.

In optical instruments, dispersion leads to chromatic aberration, a
color-dependent blurring that sometimes is the resolution-limiting effect. This
was especially true in refracting telescopes, before the invention of
achromatic objective lenses.
Leiden, Netherlands (presumably)  
379 YBN
[1621 AD]
1662) In 1616 Gassendi gets a docterate in theology.
Gassendi's work will affect Boyle.
Gassendi
vigorously opposes Descartes' view, and Harvey's theory of blood circulation.
Gassendi is
friends with the French playwright Moliére.
In 1645 Gassendi is a professor of
Mathematics at the Collége Royale at Paris.

Even though the Paris parliament declares in 1624 that on penalty of death "no
person should either hold or teach any doctrine opposed to Aristotle," Gassendi
publishes in the same year his "Excertitationes...adversus Aristoteleos"
("Dissertations...against Aristotle"), the first of his many works attacking
both medieval Scholasticism and Aristotelianism. Because Marin Mersenne and the
Pierre Gassendi (1592-1655) are Catholic priests they do not suffer
persecution, for their published attacks on Aristotle, but those judged to be
heretics continue to be burned, and laymen lack church protection.

Adopting the hedonistic ethics of Epicurus, which sought to maximize pleasure
and minimize pain, Gassendi reinterpreted the concept of pleasure in a
distinctly Christian way. Gassendi believes that God endowed humans with free
will and an innate desire for pleasure. Therefore by experiencing pleasure they
are participating in God's divine plans for the creation.
Paris, France (presumably)  
378 YBN
[1622 AD]
1639) Oughtred was educated at Eton College and at King's College, Cambridge,
where he received his bachelor's degree (1596) and master's degree (1600).
Albury, Surrey, England (presumably)  
377 YBN
[1623 AD]
1609)
Florence, Italy (presumably)  
377 YBN
[1623 AD]
1633)
Linz, Austria  
376 YBN
[1624 AD]
1593)
London, England   
376 YBN
[1624 AD]
1610)
Rome, Italy  
376 YBN
[1624 AD]
1667)
Paris, France  
376 YBN
[1624 AD]
6241) Submarine.

Cornelis Drebbel (1572-1633), a Dutch inventor, is usually credited with
building the first submarine. Between 1620 and 1624 he successfully maneuvers
his craft at depths of from 4 to 5 meters beneath the surface during repeated
trials in the Thames River, in England. King James I is said to have gone
aboard the craft for a short ride. Drebbel's submarine resembles that proposed
earlier by William Bourne in 1578, in that its outer hull consists of greased
leather over a wooden frame; oars extend through the sides and, sealed with
tight-fitting leather flaps, providing a means of propulsion both on the
surface and underwater. Drebbel's first craft is followed by two larger ones
built on the same principle.
Thames River, England  
373 YBN
[1627 AD]
1188)
Banská Štiavnica, Slovakia  
373 YBN
[1627 AD]
1634)
Ulm, Germany  
372 YBN
[1628 AD]
1645) Harvey's book makes him famous throughout Europe, though the overthrow of
so many traditional beliefs attracts virulent attacks and abuse from lesser
minds. Harvey refuses to indulge in controversy and makes no reply until 1649,
when he publishes a small book answering the criticisms of a French anatomist,
Jean Riolan.
London, England printed in: Frankfurt, Germany  
371 YBN
[1629 AD]
1672) Cavalieri joins the Jesuit order in 1615.
In 1629, Cavalieri is appointed
professor of mathematics of the University of Bologna
Cavaliei meets Galileo,
corresponds with and considers himself a disciple of Galileo.
written: Bologna, Italy  
370 YBN
[1630 AD]
1649) Wendelin is also known by the Latin name Vendelinus.
Belgium (presumably)  
370 YBN
[1630 AD]
3347)
Rome, Italy  
369 YBN
[1631 AD]
1640)
Arundel, West Sussex, England (presumably)  
369 YBN
[1631 AD]
1655)
Ornans, France (presumably: birth and death location)  
369 YBN
[1631 AD]
1663) Gassendi is the first person to see the transit of a planet across the
face of the Sun. This transit is predicted by Kepler, and arrives within 5
hours of Kepler's estimated time. One reason for these variable times are the
incalculable affects, such as the movement of liquids such as water, and metals
that planets and stars are composed of, in addition to the many asteroids which
exert small gravitational affects. A perfect system of planetary and star
prediction appears to be impossible, and because the affects of uncountable
atoms and molecules can not be accurately calculated, estimates of position for
all larger composite pieces of matter must be constantly updated.
Paris, France (presumably)  
369 YBN
[1631 AD]
1664) Gassendi is the first person to measure the velocity of sound, and shows
that the velocity of sound is independent of its pitch. Aristotle had claimed
that high notes travel faster than low notes.

Gassendi measures the time difference between spotting the flash of a gun and
hearing it the sound over a long distance on a still day. In the 1650s, Italian
physicists Giovanni Alfonso Borelli and Vincenzo Viviani obtained the much
better value of 350 metres per second using the same technique.10]

Gassendi obtains the too high figure of about 478 meters per second (1,570 feet
per second). (actual units) The current estimate for the speed of sound in for
dry air at 0 degrees C is 331.29 meters per second (1,086 feet per second 742
mph).
Paris, France (presumably)  
368 YBN
[1632 AD]
1606)
Venice, Italy  
367 YBN
[06/22/1633 AD]
1611)
Rome, Italy  
367 YBN
[1633 AD]
1666) French Philosopher and mathematician, René Descartes (CE 1596-1650)
(DAKoRT) describes the law of inertia (a body preserves its motion) and
compares light to a ball.

Descartes book "Le Monde ou Traité de la lumière" ("The World or Treatise on
Light") includes the earliest clear statement of the principle of inertia, that
a body will preserve its state of motion or rest.

Also in this book, Descartes compares reflection of light to reflection of a
ball against the wall of a tennis court, but does not explicitly state that
light is made of particles. Newton will use the example of a tennis ball in
being the first to publish the clearly stated theory of light being made of
globular bodies in 1672.

Descartes supressed both "Traite de l'homme" and "Traite de lumiere" after the
condemnation of Galileo in 1633.
Netherlands (presumably)  
366 YBN
[1634 AD]
1659)
Paris, France (presumably)  
366 YBN
[1634 AD]
3344)
London, England  
365 YBN
[1635 AD]
1657) Mersenne is a schoolmate of Descarte, but goes on to enter the church,
joining the Minim Friars in 1611.
Mersenne suggests to Huygens the idea of timing
rolling bodies down a plane by use of a pendulum, which inspires Huygens to
invent the first pendulum clock.
Mersenne's house is an important meeting-place for
philosophers and scientists: the young Pascal met Descartes there in 1647.
Gassendi is one of his close friends. Mersenne is associated with the origins
of mechanistic philosophy.
Paris, France (presumably)  
365 YBN
[1635 AD]
1660) Frequencies of sounds measured.

Marin Mersenne (mRSeN) (CE 1588-1648), French Mathematician, publishes the
multipart "Harmonie universelle" (1636-37), which discusses mechanics, as well
as music theory and musical instruments, and includes the first recorded
measurement of frequency of sound (84 cycles per second).

Mersenne writes: "If one compares two or more strings fixed by the two ends,
one can say that the longest one vibrates a longer time than the shortest, and
that the length of time follows that of the strings; and because the longest
make fewer returns {ULSF: oscillations} than the shortest in the same time, it
appears that all the strings which are different only in length each make as
many retyrns as the others, and consequently that the duration of the returns
of the longest makes up for the speed of those of the shortest, which amass in
little time what the longest makes in more. It is very easy to know the number
of beats or oscillations of all the strings of whatever instrument one wishes,
if one has understood what I have said of these tremblings...the string which
is in unison with a four-foot, open organ pipe makes 48 vibrations in ..a
second, which is the duration of a heart beat... Secondly, that the vibrations
of a strings are multiplied in the same proportion as the sounds become higher
in pitch; and consequently when one knows the number of vibrations of a string,
the pitch of which one knows, one knows as well the number of vibrations of all
sorts of strings, the pitches of which one recognizes.".

Usually A above middle C is taken as a reference pitch. The frequency used for
A, since 1939 440 vibrations per second (440 Hertz), has changed many times
over the years. Marsenne describes this A at 480 vibrations per second, but it
has been as low as 415 vibrations per second.
Paris, France (presumably)  
365 YBN
[1635 AD]
1669) In 1623 Gellibrand gets his Masters at Oxford.
Gellibrand is a Professor of
astronomy at Gresham College in 1627.
Gellibrand is a friend of Briggs.
In 1631 Gellibrand
gets in trouble for puritan views with Anglican people but is acquitted.
?, England  
365 YBN
[1635 AD]
1673)
written: Bologna, Italy (presumably)  
365 YBN
[1635 AD]
3345)
London, England  
364 YBN
[1636 AD]
1219) Havard College is now the undergraduate section and oldest school of
Harvard University.
Cambridge, Massachusetts, USA  
364 YBN
[1636 AD]
1697) Gascoigne dies in the English Civil War as a royalist for King Charles I.
  
363 YBN
[1637 AD]
1615)
Florence, Italy  
363 YBN
[1637 AD]
1668) René Descartes (CE 1596-1650) (DAKoRT) describes the Cartesian
coordinate system, where points are plotted on at two dimensional graph, in "La
Géométrie" ("Geometry") which is published as an appendix to "Discours de la
méthode" ("Discourse on Method").

The Cartesian coordinate system is the familiar two dimensional graph where
points on a plane can be drawn, x along a horizontal line, and y along a
vertical line, in order to plot curves. Descartes is the first to recognize
that every point in a plane can be represented by two numbers, for example
(-2,3), which can represent two units left and three units up. This makes a new
way to visualize mathematical functions such as y=2x+3. This connects algebra
and geometry.
Netherlands (presumably)  
363 YBN
[1637 AD]
1706)
Netherlands (presumably)  
362 YBN
[1638 AD]
1612)
Leiden, Netherlands and Florence, Italy  
362 YBN
[1638 AD]
1701)
England  
361 YBN
[1639 AD]
1387)
Quebec, New France (modern Canada)  
361 YBN
[1639 AD]
1661)
Paris, France (presumably)  
361 YBN
[1639 AD]
1708) Jeremiah Horrocks (CE 1618-1641), is the first human to observe the
transit of Venus.

Horrocks suggests that (by recording the time) of the Venus transit from
various observatories around the earth, the parallax of Venus can be measured.
This parallax can then be used to understand the scale of the star system. This
eventually will be done.

Horrocks is first to show that the moon moves around the earth in an ellipse
with the earth at one focus, which Kepler did not understand.

From Kepler's recently published Rudolphine Tables (1627), Horrocks works out
that a transit of Venus is due on November 24th, 1639 at 3 p.m.

Horrocks will record an account of this day in his "Venus in Sole Visa" ("Venus
in the Face of the Sun"), printed posthumously by Hevelius in 1662. The day is
cloudy but at 3.15, "as if by divine interposition" the clouds disperse.
Horrocks notes a spot of unusual size on the solar disc and begins to trace its
path. Horrocks then writes, "she was not visible to me longer than half an
hour, on account of the Sun quickly setting."

Horrocks corrects the Rudolphine tables of Kepler's in regard to the transit of
Venus.

Horrocks also attempts to determine the solar parallax calculating 15",
compared with a modern value of 8".8. Horrocks estimates the distance of the
Sun from the Earth more correctly than anyone else had done before.

Horrocks is the first astronomer to accept Kepler's elliptical orbits fully.

Horrocks is the first of record to understand that the irregularities in the
orbit of the Moon might be the result of the Sun, and that Jupiter and Saturn
might exert an influence on each other. This is a preview of the theory of
universal gravitation that will be first understood by Newton.
Hoole, Lancashire, England (presumably)  
360 YBN
[1640 AD]
1665)
Paris, France (presumably)  
360 YBN
[1640 AD]
1700) In 1627 Wilkens enters Oxford at age 13.
In 1634 Wilkens earns a masters
degree at age 20, and is ordained a priest few years later.
Wilkens marries the sister
of Oliver Cromwell.
Wilkens is the only person to have headed a college at both the
University of Oxford and the University of Cambridge.
Wilkens serves as Bishop of Chester
from 1668 until his death.
England  
360 YBN
[1640 AD]
1718) Pascal is an infant prodigy in math and science.
In 1648 Pascal will adopt
Jansenism (a Roman Catholic sect founded by Cornelius Jansen, emphasizing
original sin, that is that all humans are born sinful, and without divine help
a human can never become good. Jansenism is marked by strong anti-Jesuit
feeling, Jesuits are a Roman Catholic religious order founded by Saint Ignatius
of Loyola, whose members are sometimes refered to as the "soliers of Christ"
and the "foot soldiers of the Pope"), and turns to religious writing, including
"Pensées" ("thoughts") (published posthumously). In "Pensées" Pascal states
his belief in the inadequacy of reason to solve man's difficulties or to
satisfy his hopes and preaches instead the necessity of mystic faith for true
understanding of the universe and its meaning to man. In his last years Pascal
declares reason an insufficient tool to understanding the universe and Asimov
says he had thus retreated beyond Thales.

Pascal writes 18 Lettres provinciales (Provincial Letters)(January 1656-March
1657) against the Jesuits using the pseudonym Louis de Montalte and angers
Louis XIV. The king orders that the book be shredded and burnt in 1660. The
first ten letters constitute a dialog between a naïve enquirer (presented as
the writer of the letters), a friendly Jansenist, and some Jesuit priests. The
letters are popular, and will be placed on the Catholic Church's Index of
Prohibited Books in 1657.

Pascal's sister Gilberte tells of his asceticism, of his dislike of seeing her
caress her children, and of his apparent revulsion from talk of feminine
beauty.

One of Pascal's famous quotes is Pascal's wager: "Belief is a wise wager.
Granted that faith cannot be proved, what harm will come to you if you gamble
on its truth and it proves false? If you gain, you gain all; if you lose, you
lose nothing. Wager, then, without hesitation, that He exists." In my own view,
it is idiocy and delusion to support the idea of a god, because it is such an
easily concept to disprove, being that humans only recently evolved language,
and created numerous gods...it's like living for the teapot that might be
orbiting Mars...it's idiocy, and all the evidence is against any kind of divine
punishment for not conforming to popular religious myths and claims. This shows
clearly that Pascal, like so many in history, lacked the wisdom and education
to see beyond the claims of religions. The arrogance of those who claim to know
what a god is and wants is almost as bad as the myth of gods itself. I am glad
to be one of the few humans in this time, who will be recognized as not being
duped by religions including the all-popular and powerful Godism.

Pascal suffers increasingly after 1658 from head pains, and dies on in 1662 at
age 39.
18 months before Pascal's death, he devises a system of cheap public
transport for Paris, the so-called ‘carrosses à cinq sols".
Paris, France (presumably)  
359 YBN
[1641 AD]
1698) Sylvius gets his Medical (health science/physician) degree from Basel,
Switzerland.
In 1658, Sylvius is a professor of medicine at the University of Leiden.
Leiden, Netherlands (presumably)  
359 YBN
[1641 AD]
1699)
Leiden, Netherlands (presumably)  
359 YBN
[1641 AD]
6244) Repeating gun.

A repeating rifle is a firearm designed for use with a magazine of cartridges,
each of which is fed into the chamber or breech by lever, bolt action, or some
other method. Before the invention of the cartridge that contains powder, ball,
and primer, a repeater has to have separate magazines for powder and ball.
Alternative arrangements are multiple barrels, multiple breeches, and the
loading of several shots into one barrel and igniting the outermost charge,
which would eject its ball and ignite the next charge. The first effective
breech-loading and repeating flintlock firearms are developed in the early
1600s.

In this year, 1641, Peter Kalthoff is granted a monopoly on magazine guns in
the Netherlands.

(At some time, the light particle as ammunition, and microscopic remote
controlled gun became the most effective and dominant weapon on Earth,
surpassing the hand-held automatic ballistic gun.)
Netherlands  
358 YBN
[1642 AD]
1719)
Rouen, France (presumably)  
358 YBN
[1642 AD]
2098)
New Zealand  
357 YBN
[1643 AD]
1190) Traditionally George Fox has been credited as the founder or the most
important early figure.
Rome, Italy  
357 YBN
[1643 AD]
1650)
Belgium (presumably)  
357 YBN
[1643 AD]
1692) Earliest vacuum.

Italian physicist, Evangelista Torricelli (TORriceLlE) (CE 1608-1647), is the
first human to create a sustained vacuum.

Galileo observed that a hollow cylinder with a piston in a pool of water does
not pull water up completely in the cylinder as is expected, but can only draw
water up into the cylinder 10m (30 feet) above the water level, further pumping
has no effect, the weight of the air pushes the water no higher. Torricelli
investigates this and tries a heavier fluid, filling a 4 foot glass tube closed
at one end with mercury (a liquid at room temperature with a density 13.5 times
water), and closes the other end with a stopper. Torricelli then turns the tube
over and puts it into a pool of Mercury. When the stopper is removed, the
mercury pours out of the tube, but 30 inches of mercury remain in the tube,
supported by the pressure of the air outside the tube pushing down on the dish
of liquid mercury. The weight of the air is presumed to be the reason the
column of Mercury appears to defy gravity. Above the column of mercury in the
tube is a vacuum of empty space (except for small quantities of Mercury vapor).
This is the first human made vacuum. Torricelli notices that the height of the
Mercury in the glass tube changes slightly from day to day, and he correctly
attributes this to a change in pressure of the atmosphere. (The pressure
exerted by one millimeter of mercury is called a Torricelli in his honor). That
air has a finite weight means that it has a finite height, and that the
atmosphere does not extend indefinitely up. In addition, this hints that the
depths of space must be empty space (a vacuum).

This device is also the first barometer, a measure of pressure exerted by air.
Florence, Italy  
357 YBN
[1643 AD]
6322) Claudio (Giovanni Antonio) Monteverdi (CE 1567-1643), Italian composer,
composes the Opera "Incoronazione di Poppea" ("The Coronation of Poppea").
Venice, Italy  
356 YBN
[1644 AD]
1658) Paris, France (presumably)  
356 YBN
[1644 AD]
1694) A member of a noble family of Gdansk, Hevelius is a city councilor and a
brewer. After studying at the University of Leiden in the Netherlands, Hevelius
returns to Gdansk and builds his observatory atop his house.

Hevelius' surname appears in various spellings, among them Hevel, Hewel,
Hewelcke, and Höwelcke.
  
356 YBN
[1644 AD]
2618)
Netherlands (presumably)  
355 YBN
[1645 AD]
1844) French astronomer, librarian and mathematician, Ismaël Bullialdus (CE
1605-1694) recognizes that the strength that the Sun holds the planets with
decreases by the distance squared.

Bullialdus writes: "As for the power by which the Sun seizes or holds the
planets, and which, being corporeal, functions in the manner of hands, it is
emitted in straight lines throughout the whole extent of the world, and like
the species of the Sun, it turns with the body of the Sun. Now, given that it
is corporeal, it becomes weaker, and attenuates at a greater distance and
interval, and the ratio of its decrease in strength is the same as in the case
of light, namely, the duplicate proportion of the distance, but inversely.
Kepler does not deny this, yet he claims the motive power decreases only in
direct proportion to the distance. Furthermore, Kepler claims this attenuation
in the motive power produces a weakening of the power only in longitude,
because local motion impressed by the Sun on the planets (which motion
similarly animates the corporeal parts of the Sun itself) occurs only in
longitude, not in latitude. In response to this Kepler offsets the inadequacy
of this analogy by increasing the quantity matter in the slower planets."
Paris, France  
354 YBN
[1646 AD]
1684)
Rome, Italy (presumably)  
354 YBN
[1646 AD]
1687)
Amsterdam, Netherlands (presumably)  
353 YBN
[1647 AD]
1674)
written: Bologna, Italy (presumably)  
353 YBN
[1647 AD]
1695)
  
352 YBN
[09/19/1648 AD]
1721)
Rouen, France (presumably)  
352 YBN
[1648 AD]
1189) Traditionally George Fox has been credited as the founder or the most
important early figure.
England  
352 YBN
[1648 AD]
1648) In 1634 Helmont is called before the Inquisition for claiming saintly
relics exhibit their effects through magnetic influence. Ecclesiastical court
proceedings of one sort or another were pending against Helmont for more than
20 years.
Vilvoorde, Belgium  
352 YBN
[1648 AD]
1686) Glauber sells many products (including sodium sulfate) as "cure-alls".
In 1648 Glauber
moves to Amsterdam and into the house last owned by an alchemist.
Glauber greatly admires
Paracelsus.
Glauber believes in some of the mystical belief associated with alchemy in
being a firm believer in the so-called "philosophers' stone" and "elixir of
life".
Glauber possibly died as result of working with harmful chemicals.
Amsterdam, Netherlands (presumably)  
351 YBN
[05/19/1649 AD]
1526)
England  
350 YBN
[1650 AD]
1670) Riccioli is an Italian astronomer and Jesuit priest who publicly rejects
the sun-centered theory.
Bologna, Italy (presumably)  
350 YBN
[1650 AD]
1675) Kircher receives a Jesuit education, and is ordained a priest in 1628.
Kircher
leaves the fighting in Germany (part of the Thirty Years' War) and, after
various academic positions at Avignon, France, settles in 1634 in Rome.
Kircher
writes against the Copernican model in his "Magnes" (supporting instead the
model of Tycho Brahe), but in his later "Itinerarium extaticum" (1656, revised
1671) Kircher presented several systems, including the Copernican, as
alternative possibilities.

Kircher assembles one of the first natural history collections, that will forms
the nucleus of the museum that bears his name, the "Museo Kircheriano" at Rome.
Rome, Italy (presumably)  
350 YBN
[1650 AD]
1683) German physicist, Otto von Guericke (GAriKu) (CE 1602-1686) constructs
the first air pump and uses it to produce a vacuum chamber in which he examines
the role of air in combustion and respiration.

This air pump is like a waterpump but airtight and powered by pumping by hand.
Guericke uses the pump to create evacuated containers and shows that a ringing
bell inside the vessel can not be heard, that candles will not burn, and that
animals cannot live in a vacuum. Lavoisier 100 years later will determine the
components of air on Earth. Guericke shows that the pressure of a vacuum
pulling on a piston cannot by stopped by 50 people pulling on a rope attached
to the piston. In 1654, before Emperor Ferdinand III at Regensburg, Guericke
shows that two teams of horses cannot pull apart to semispheres connected
together with a vacuum inside, and then how adding air into the two semispheres
allows them to fall apart effortlessly.

There are two kinds of air pumps in use, mechanical and mercurial.

Guericke believes that comets are normal members of the solar system and make
periodic returns.
Magdeburg, Germany (presumably)  
350 YBN
[1650 AD]
1722)
Rouen, France (presumably)  
350 YBN
[1650 AD]
1753) In 1653 Malpighi gets his medical degree from the University of Bologna,
and lectures mainly there and other universities in Italy.
In 1667, the Royal Society
asks Malpighi to send his scientific communications.
In 1684 Malpighi's villa is burned (as a
result of opposition to his views), his apparatus and microscopes shattered,
and his papers, books, and manuscripts are destroyed.
In 1691, Malpighi retires to Rome to
be physician to Pope Innocent XII.
Bologna, Italy (presumably)  
350 YBN
[1650 AD]
2017) Francis Glisson (CE 1597-1677), publishes a report "De rachitide" (1650;
On Rickets), that gives a clear description of the disease Rickets.

Rickets is a vitamin deficiency disease and will require the discovery of
vitamins by Casimir Funk in 1912.

Glisson is a member of the group that, beginning in 1645, meets regularly in
London and out of which the Royal Society will later emerge. From this
"Invisible College" as it was later known, comes one of the earliest examples
of cooperative research.

A committee of nine is created in 1645 to investigate rickets but because
Glisson's contribution far exceeds that of any other contributor, it is agreed
that Glisson should publish the report.

Like his colleague William Harvey, Glisson is a Cambridge-trained physician.

Both are dedicated to scientific experimentation and careful observation and
description.
Glisson is a professor of physics at Cambridge for 40 years, however makes his
professional home in London.

London, England  
349 YBN
[1651 AD]
1572)
London, England (presumably)  
349 YBN
[1651 AD]
1646)
London, England (presumably)  
349 YBN
[1651 AD]
1647)
London, England (presumably)  
349 YBN
[1651 AD]
1671)
Bologna, Italy  
348 YBN
[1652 AD]
1775) Rudbeck builds up a botanical garden.
Rudbeck teaches at the medical school of
the University of Uppsala, Sweden.
Rudbeck is chancellor at age 31.
Rudbeck believes
Plato's fictional tale of Atlantis, and writes several volumes trying to prove
that Atlantis is really Scandinavia and that Sweden was the source of human
civilization.
Uppsala, Sweden  
346 YBN
[1654 AD]
1693) Ferdinand II funds Steno and Galileo.
In 1657 Ferdinand II helps support the
foundation of the Accademia del Cimento.
Tuscany, Italy (presumably)  
346 YBN
[1654 AD]
1720)
Paris, France (presumably)  
346 YBN
[1654 AD]
2018) This work is based on Glisson's own dissections contributes to the
understanding of the structure and functioning of the liver.
This work includes the
most advanced physiological description of the digestive system to date.

The prevailing mechanical philosophy promotes a view of matter as completely
passive and inert, and Glisson's theory of "irritability" runs counter to this.
Because the passivity of matter is used to ensure a role for a God, Glisson's
active matter is seen as a support for atheism and for that reason Glisson's
works are attacked by the Cambridge Platonists Henry More (1586-1661) and Ralph
Cudworth (1617-1688). The idea of irritability will be picked up by Albrecht
von Haller in the following century and will find a permanent place in
physiology.
London, England  
345 YBN
[03/25/1655 AD]
1763) Dutch physicist and astronomer, Christiaan Huygens (HOEGeNZ) (CE
1629-1695) identifies the first known moon of Saturn, Titan.

In this same year Huygens identifies the ring of Saturn.
Huygens had initially
been attracted to Saturn by its apparently anomalous shape, described by
Galileo as "three spheres which almost touch each other, which never change
their relative positions, and are arranged in a row along the zodiac so that
the middle sphere is three times as large as the others." Intrigued by this
peculiar shape, Huygens realized that its resolution would depend on
constructing improved telescopes, less subject to various aberrations and more
capable of producing detailed images.

Huygens announces his finding in a cipher to protect his priority while
verifying his finding further.

Titan is the largest moon of Saturn and as large as any moon of Jupiter, and
will be shown to be the only moon in this star system with a dense atmosphere.

With six planets and six moons Huygens erroneously declares that there are no
more planets or moons to be found, and is proven wrong in his lifetime by
Cassini who finds 4 more moons of Saturn.

Huygens understands that Saturn will be in the same orientation as the earth
and so the rings will not be visible every 14 years.
The Hague, Netherlands (presumably)  
345 YBN
[1655 AD]
1702) This book promptly brings fame to Wallis, who is then recognized as one
of the leading mathematicians in England.

Wallis deciphers a number of cryptic messages from Royalist partisans that had
fallen into the hands of the Parliamentarians.

In the English civil war, Wallis supports the Parliamentarians against Charles
I.
In 1649, Wallis is appointed to teach at Oxford under the Parliamentary
regime.
Wallis is nationalistic and fights against the Gregorian system in England
(which Wallis views as implying subservience to Rome) and delays this decision
by half a century.

In London, in 1647 Wallis' serious interest in mathematics begins when he reads
William Oughtred's "Clavis Mathematicae" ("The Keys to Mathematics").
(University of Oxford) Oxford, England  
345 YBN
[1655 AD]
1762) Huygens' father is an important official in the Dutch government.
Huygens is educated
at the University of Leiden.
Huygens is friends with Descartes.
From an early age, Huygens shows a
marked mechanical bent and a talent for drawing and mathematics. Some of his
early efforts in geometry impress Descartes, who was an occasional visitor to
the Huygens' household.
Huygens's first published work, on the quadrature of
various mathematical curves, appeared in 1651.
In 1663 Huygens is elected a charter
member of the Royal Society.
In 1666 Louis XIV lures Huygens to France in line with his
policy of collecting scholars for the glory of his regime.
Apart from
occasional visits to Holland, Huygens lives in Paris from 1666 to 1681.
In France
Huygens helps found the French Academy of Sciences.
In 1681 Huygens returns to the
Netherlands (Asimov suggests because he is protestant and Louis XIV is moving
in direction of intolerance of protestants).
The death in 1683 of Huygens' patron,
Jean-Baptiste Colbert, who had been Louis XIV's chief adviser, and Louis's
increasingly reactionary policy, which culminates in the revocation (1685) of
the Edict of Nantes, which had granted certain liberties to Protestants, rules
against Huygens ever returning to Paris.
Huygens visits London in 1689, meets Sir
Isaac Newton and lectures on his own theory of gravitation before the Royal
Society.
He never marries.
Unlike many men of science in the 1600s, Huygens never occupies
himself to any significant extent with either philosophy or theology, devoting
his efforts entirely to the pursuit of science.
The Hague, Netherlands (presumably)  
345 YBN
[1655 AD]
1843)
Paris, France (presumably)  
344 YBN
[03/25/1656 AD]
1769)
The Hague, Netherlands (presumably)  
344 YBN
[1656 AD]
1716) Athanasius Kircher (KiRKR) (CE 1601-1680) is the first to explicitly
print that stars are other Suns with planets around them, which he prints in
his book "Itinerarium extaticum" (Ecstatic journey).

Huygens refers to this work of Kircher's in his 1698 "Cosmotheoros" when
reaffirming that other stars and more distant Suns with planets but correcting
Kircher by supporting the Copernican Sun-centered model.

Kircher is sometimes called the last Renaissance man, important for the large
quantity of knowledge he disseminates.
(Collegio Romano) Rome, Italy (presumably)  
344 YBN
[1656 AD]
1764) Christaan Huygens (HOEGeNZ) (CE 1629-1695) invents the first pendulum
{PeNJUluM or PeNDUluM} clock.

This first pendulum clock is described and illustrated by Huygens in his book,
'Horologium' in 1658.

Galileo had suggested the use of a pendulum to count the time. Galileo had
drawn a design of a clock which connected a pendulum to gears in his old age,
and Huygens built his pendulum clock over ten years after Galileo's death.
Huygen's design, where the dial and hands of a clock are controlled by a
pendulum, is the first truly practical pendulum clock. Huygens attaches a
pendulum to the gears of a clock. The regular swing of the pendulum allows the
clock to achieve greater accuracy, as the hands are turned by the falling
weight, which releases the same amount of energy with each tick.

Huygens shows that a pendulum does not swing in exactly equal times unless it
swings through an arc that is not quite circular but cycloid. He builds
attachments to the pendulum's fulcrum (pivot point at top) that make it swing
in the proper arc and attaches this to the works of the clock, using falling
weights to transfer just enough energy to the pendulum to keep it from coming
to a halt through friction and air resistance. Huygens presents his clock to
the Dutch governing body. This begins the era of accurate timekeeping. Asimov
indicates that it is unlikely physics could progress without such a device.

Although the pendulum clock is the most accurate such device then available,
its motion is easily disturbed by the movement of the ship at sea.

Although Huygens publishes his idea for a precision pendulum in a small booklet
titled "Horologium" in 1658, he will not produce the full theory of the
pendulum for the scientific world until the 1673 publication, "Horologium
oscillatorium sive de moto pendulorum".
The Hague, Netherlands (presumably)  
343 YBN
[1657 AD]
1703)
London, England (presumably)  
343 YBN
[1657 AD]
1717) The academy is discontinued after ten years.

The Accademia del Cimento (Academy of Experiment), an early scientific society,
is founded in Florence.
Florence, Italy  
343 YBN
[1657 AD]
1765)
The Hague, Netherlands (presumably)  
343 YBN
[1657 AD]
1794) Hooke is the son of a clergyman.
Hooke is an infant prodigy in mechanics.
Hooke is accepted to
Oxford in 1653 (at age 18).
Hooke is supports himself by waiting on tables.
In 1662, with
the help of Boyle, Hooke secures the job as Curator of Experiments for the
Royal Society, which he holds from (1662-1677) at £30/year plus the privilege
of lodging at Gresham College. Hooke's task is to report on and/or demonstrate
three to four major experiments to the Royal Society each week. This is the
only paid position in the Royal Society.
In 1663, Hooke is elected a member of the Royal
Society.
From 1677 to 1683 Hooke is secretary of the Royal Society.

Hooke has priority and proper credit disputes with Huygens and most famously
with Newton.

After the London fires of 1666 Hooke is involved in rebuilding projects and
never revisits the microscope.
Hooke designs many buildings including Montague House, the
Royal College of Physicians, Bedlam and Bethlehem Hospital.
Oxford, England (presumably)  
342 YBN
[1658 AD]
1677)
Rome, Italy (presumably)  
342 YBN
[1658 AD]
1767)
The Hague, Netherlands (presumably)  
342 YBN
[1658 AD]
1804) Swammerdam is the son of an apothecary (a historical name for a medical
practitioner who formulates and dispenses health materials to physicians,
surgeons and patients, a role now served by a pharmacist).
Swammerdam studies
medicine at Leiden university, where Steno and Graaf are fellow students.
In
1667 Swammerdam earns his medical degree from Leiden university.
Much to Jan's father's
displeasure, Swammerdam does not practice medicine but continues his
microdissections of insects.
At some point Jan's father stop funding Jan.
In 1673 Swammerdam
meets Flemish mystic Antoinette Bourignon, and later subjects himself to the
tutelage of Bourignon and, for the most part, renounces scientific study.

Swammerdam's work is largely neglected until Hermann Boerhaave revisits and
publishes it 50 years later in 1737 in two volumes called "Biblia naturae"
(Bible of Nature).
Amsterdam, Netherlands (presumably)  
341 YBN
[1659 AD]
1681) Fermat is educated at home, and gets a law degree in 1631 from the
University of Orleans.
Fermat is a councilor for the Toulouse Parliament and devotes his
spare time to mathematics.
Fermat scribbles notes in margins as opposed to publishing or
writing about findings to friends.
Fermat's son publishes his notes five years
after Fermat's death.
Toulouse, France (presumably)  
341 YBN
[1659 AD]
1741) Ray is the son of a blacksmith.
Ray receives his early education at the Braintree
grammar school.
In 1644, with the aid of a fund that had been left in trust to support
needy scholars at the University of Cambridge, Ray matriculates at St.
Catherine's Hall College.
In 1651 Ray earns his masters from Cambridge, and stays on as
lecturer.
In 1662 Ray leaves Cambridge refusing to take an oath to the restored king.
In 1671
Ray is elected as a member in the Royal Society.
Cambridge, England (presumably)  
341 YBN
[1659 AD]
1755)
Bologna, Italy  
341 YBN
[1659 AD]
1766)
The Hague, Netherlands (presumably)  
341 YBN
[1659 AD]
1771) Huygens is not the first to identify the Orion Nebula, as it was already
known earlier (by an Arabic astronomer,) by Nicolas-Claude Fabri de Peiresc in
1610, and Johann Cysat in 1619.
The Hague, Netherlands (presumably)  
341 YBN
[1659 AD]
5918) Barabara Strozzi (CE 1619-1663), Italian composer and singer, composes
music. Strozzi is one of the most successful women composers of the seventeenth
century, and is the most prolific composer of printed secular vocal music in
Venice around the middle of the century, with seven different publications,
along with one of sacred music, issued between 1644 and 1664.

  
340 YBN
[11/28/1660 AD]
1704)
London, England  
340 YBN
[1660 AD]
1682)
Toulouse, France (presumably)  
340 YBN
[1660 AD]
1691)
Magdeburg, Germany (presumably)  
340 YBN
[1660 AD]
1737) Boyle was born in Ireland into one of the wealthiest families in
Britain.
Boyle is an infant prodigy.
Boyle goes to Eaton at 8 and is speaking Greek and Latin.
At 14,
Boyle lives in Italy studying works of Galileo.
Boyle never marries but like most people
probably did get sex at least once and no doubt masturbated regularly for much
of his life.
In 1654 Boyle is invited to Oxford, and lives at the university from c.
1656 until 1668.
The Dutch-Jewish philosopher Spinoza tries to convince Boyle
that reason is superior to experiment.
In 1660 Boyle helps found the Royal
Society of London whose motto is "Nullius in verba" ("Nothing by mere
authority").
Boyle believes in transmutation of gold (through chemistry) and in 1689
convinces the British government to repeal the law forbidding the manufacture
of gold (that sounds like kind of a unusual law and shows the gullibility of
people at this time].
Sadly Boyle's interest in religion grows as he ages. Boyle
learns Hebrew and Aramaic for his biblical studies. In his will he founds the
Boyle Lectures, not on science, but on the defense of Christianity, which
continue to this day.
Oxford, England (presumably)  
340 YBN
[1660 AD]
3142)
Oxford, England (presumably)  
339 YBN
[1661 AD]
1738) Halley is clearly a person who mathematically analyzed orbits translating
earth-based observations into two dimensional curves.
Oxford, England (presumably)  
339 YBN
[1661 AD]
1754) This is a second piece of evidence in support of the circulation theory
of Harvey who died a few years too soon to know. Rudbeck adding the final piece
to the circulatory system with the lymphatic system.
Malphigi sends these findings in
two letters to Borelli in Pisa who publishes them as "De pulmonibus
observationes anatomicae" ("On the lungs"; Bologna, 1661).
In this work
Malphigi also gives a detailed account of the vesicular structure of the human
lung.
Bologna, Italy  
339 YBN
[1661 AD]
1810) Steno is the son of a goldsmith.
Steno is brought up Lutheran.
In 1664 Steno earns
his medical degree from Leiden University.
Steno is court physician to Grand Duke Ferdinand
II of Tuscany.
In 1667, Steno converts to Catholicism and abandons science for religion,
(like Pascal and Swammerdam).
In 1677 Steno rises to the position of bishop.
Amsterdam, Netherlands   
338 YBN
[1662 AD]
1710) Graunt influences, and is influenced by, his friend, the physician Sir
William Petty (CE 1623-1687), author of "Political Arithmetic" and other works
that analyze available facts in a number of areas, including life expectancy
and earning capacity, emphasizing their economic and fiscal implications.
London, England  
338 YBN
[1662 AD]
1739) Robert Boyle (CE 1627-1691) explains that the pressure and volume of a
gas are inversely related (Boyle's Law).

Robert Boyle (CE 1627-1691) with Robert Hooke find that the pressure and volume
of a gas are inversely related (this is called Boyle's Law).

Boyle finds this when using a 17 foot J-shaped tube to trap air using mercury.
Boyle recognizes that when he adds twice the amount of mercury, he is adding
twice the pressure on the air trapped in the end of the tube. When Boyle does
this the air volume is reduced by a half, and in reverse, if pressure is
lowered by removing half of the mercury, the volume of the air expands by two
times.

This inverse relationship of a gases volume to it's pressure is called Boyle's
law (in France it is credited to Mariotte).
Oxford, England (presumably)  
337 YBN
[1663 AD]
1814) James Gregory (1638-1675) publishes an early design of a reflecting
telescope.

Niccolò Zucchi (CE 1586-1670) builds the earliest known reflecting telescope
in 1616.
London, England  
337 YBN
[1663 AD]
2247) Otto von Guericke (GAriKu) (CE 1602-1686) builds the first static
electricity generator by rotating a sulfur globe against a cloth.

Guericke makes the first friction electric machine, by mechanizing the act of
rubbing sulfur. Guericke makes a sphere of sulfur that can be rotated on a
crank-turned shaft, that when stroked with the hand as it rotates accumulates a
large amount of static electricity. Guericke produces sizable electric sparks
from his charged globe, which he reports to Leibniz in a letter in 1672.
Magdeburg, Germany (presumably)  
336 YBN
[07/??/1664 AD]
2328)
London, England (presumably)  
336 YBN
[11/23/1664 AD]
1799) Hooke describes a transverse wave theory of light with a transparent
medium:
"And first for Light it seems very manifest, that there is no luminous Body but
has the parts of it in motion more or less.

First, That all kind of fiery burning Bodies have their parts in motion, I
think, will be very easily granted me. That the spark struck from a Flint and
Steel is in a rapid agitation, I have elsewhere made probable. And that the
Parts of rotten Wood, rotten Fish and the like, are also in motion, I think,
will as easily be conceded by those, who consider, that those parts never begin
to shine till the Bodies be in a state of putrefaction; and that is now
generally granted by all, to be caused by the motion of the parts of putrifying
bodies. That the Bononian stone shines no longer then it is either warmed by
the Sun-beams, or by the flame of a Fire or of a Candle, is the general report
of those that write of it, and of others that have seen it. And that heat
argues a motion of the internal parts is (as I said before) generally granted.

But there is one Instance more, which was first shewn to the Royal Society by
Mr. Clayton a worthy Member thereof, which does make this Assertion more
evident then all the rest: And that is, That a Diamond being rub'd, struck or
heated in the dark, shines for a pretty while after, so long as that motion,
which is imparted by any of those Agents, remains (in the same manner as a
Glass, rubb'd, struck, or (by a means which I shall elsewhere mention) heated,
yields a sound which lasts as long as the vibrating motion of that sonorous
body) several Experiments made on which Stone, are since published in a
Discourse of Colours, by the truly honourable Mr. Boyle. What may be said of
those Ignes fatui that appear in the night, I cannot so well affirm, having
never had the opportunity to examine them my self, nor to be inform'd by any
others that had observ'd them: And the relations of them in Authors are so
imperfect, that nothing can be built on them. But I hope I shall be able in
another place to make it at least very probable, that there is even in those
also a Motion which causes this effect. That the shining of Sea-water proceeds
from the same cause, may be argued from this, That it shines not till either it
be beaten against a Rock, or be some other wayes broken or agitated by Storms,
or Oars, or other percussing bodies. And that the Animal Energyes or Spirituous
agil parts are very active in Cats eyes when they shine, seems evident enough,
because their eyes never shine but when they look very intensly either to find
their prey, or being hunted in a dark room, when they seek after their
adversary, or to find a way to escape. And the like may be said of the shining
Bellies of Gloworms; since 'tis evident they can at pleasure either increase or
extinguish that Radiation.

It would be somewhat too long a work for this place Zetetically to examine, and
positively to prove, what particular kind of motion it is that must be the
efficient of Light; for though it be a motion, yet 'tis not every motion that
produces it, since we find there are many bodies very violently mov'd, which
yet afford not such an effect; and there are other bodies, which to our other
senses, seem not mov'd so much, which yet shine. Thus Water and quick-silver,
and most other liquors heated, shine not; and several hard bodies, as Iron,
Silver, Brass, Copper, Wood, &c. though very often struck with a hammer, shine
not presently, though they will all of them grow exceeding hot; whereas rotten
Wood, rotten Fish, Sea water, Gloworms, &c. have nothing of tangible heat in
them, and yet (where there is no stronger light to affect the Sensory) they
shine some of them so Vividly, that one may make a shift to read by them.

It would be too long, I say, here to insert the discursive progress by which I
inquir'd after the proprieties of the motion of Light, and therefore I shall
only add the result.

And, First, I found it ought to be exceeding quick, such as those motions of
fermentation and putrefaction, whereby, certainly, the parts are exceeding
nimbly and violently mov'd; and that, because we find those motions are able
more minutely to shatter and divide the body, then the most violent heats
menstruums we yet know. And that fire is nothing else but such a dissolution of
the Burning body, made by the most universal menstruum of all sulphureous
bodies, namely, the Air, we shall in an other place of this Tractate endeavour
to make probable. And that, in all extreamly hot shining bodies, there is a
very quick motion that causes Light, as well as a more robust that causes Heat,
may be argued from the celerity wherewith the bodyes are dissolv'd.

Next, it must be a Vibrative motion. And for this the newly mention'd Diamond
affords us a good argument; since if the motion of the parts did not return,
the Diamond must after many rubbings decay and be wasted: but we have no reason
to suspect the latter, especially if we consider the exceeding difficulty that
is found in cutting or wearing away a Diamond. And a Circular motion of the
parts is much more improbable, since, if that were granted, and they be
suppos'd irregular and Angular parts, I see not how the parts of the Diamond
should hold so firmly together, or remain in the same sensible dimensions,
which yet they do. Next, if they be Globular, and mov'd only with a turbinated
motion, I know not any cause that can impress that motion upon the pellucid
medium, which yet is done. Thirdly, any other irregular motion of the parts one
amongst another, must necessarily make the body of a fluid consistence, from
which it is far enough. It must therefore be a Vibrating motion.

And Thirdly, That it is a very short-vibrating motion, I think the instances
drawn from the shining of Diamonds will also make probable. For a Diamond being
the hardest body we yet know in the World, and consequently the least apt to
yield or bend, must consequently also have its vibrations exceeding short.

And these, I think, are the three principal proprieties of a motion, requisite
to produce the effect call'd Light in the Object.

The next thing we are to consider, is the way or manner of the trajection of
this motion through the interpos'd pellucid body to the eye: And here it will
be easily granted,

First, That it must be a body susceptible and impartible of this motion that
will deserve the name of a Transparent. And next, that the parts of such a body
must be Homogeneous, or of the same kind. Thirdly, that the constitution and
motion of the parts must be such, that the appulse of the luminous body may be
communicated or propagated through it to the greatest imaginable distance in
the least imaginable time, though I see no reason to affirm, that it must be in
an instant: For I know not any one Experiment or observation that does prove
it. And, whereas it may be objected, That we see the Sun risen at the very
instant when it is above the sensible Horizon, and that we see a Star hidden by
the body of the Moon at the same instant, when the Star, the Moon, and our Eye
are all in the same line; and the like Observations, or rather suppositions,
may be urg'd. I have this to answer, That I can as easily deny as they affirm;
for I would fain know by what means any one can be assured any more of the
Affirmative, then I of the Negative. If indeed the propagation were very slow,
'tis possible something might be discovered by Eclypses of the Moon; but though
we should grant the progress of the light from the Earth to the Moon, and from
the Moon back to the Earth again to be full two Minutes in performing, I know
not any possible means to discover it; nay, there may be some instances perhaps
of Horizontal Eclypses that may seem very much to favour this supposition of
the slower progression of Light then most imagine. And the like may be said of
the Eclypses of the Sun, &c. But of this only by the by. Fourthly, That the
motion is propagated every way through an Homogeneous medium by direct or
straight lines extended every way like Rays from the center of a Sphere.
Fifthly, in an Homogeneous medium this motion is propagated every way with
equal velocity, whence necessarily every pulse or vitration of the luminous
body will generate a Sphere, which will continually increase, and grow bigger,
just after the same manner (though indefinitely swifter) as the waves or rings
on the surface of the water do swell into bigger and bigger circles about a
point of it, where, by the sinking of a Stone the motion was begun, whence it
necessarily follows, that all the parts of these Spheres undulated through an
Homogeneous medium cut the Rays at right angles.

But because all transparent mediums are not Homogeneous to one another,
therefore we will next examine how this pulse or motion will be propagated
through differingly transparent mediums. And here, according to the most acute
and excellent Philosopher Des Cartes, I suppose the sign of the angle of
inclination in the first medium to be to the sign of refraction in the second,
As the density of the first, to the density of the second. By density, I mean
not the density in respect of gravity (with which the refractions or
transparency of mediums hold no proportion) but in respect onely to the
trajection of the Rays of light, in which respect they only differ in this;
that the one propagates the pulse more easily and weakly, the other more
slowly, but more strongly. But as for the pulses themselves, they will by the
refraction acquire another propriety, which we shall now endeavour to
explicate.
(see image) We will suppose therefore in the first Figure ACFD to be a physical
Ray, or ABC and DEF to be two Mathematical Rays, trajected from a very remote
point of a luminous body through an Homogeneous transparent medium LLL, and
DA, EB, FC, to be small portions of the orbicular impulses which must therefore
cut the Rays at right angles; these Rays meeting with the plain surface NO of a
medium that yields an easier transitus to the propagation of light, and falling
obliquely on it, they will in the medium MMM be refracted towards the
perpendicular of the surface. And because this medium is more easily trajected
then the former by a third, therefore the point C of the orbicular pulse FC
will be mov'd to H four spaces in the same time that F the other end of it is
mov'd to G three spaces, therefore the whole refracted pulse GH shall be
oblique to the refracted Rays CHK and GI; and the angle GHC shall be an acute,
and so much the more acute by how much the greater the refraction be, then
which nothing is more evident, for the sign of the inclination is to the sign
of refraction as GF to TC the distance between the point C and the
perpendicular from G on CK, which being as four to three, HC being longer then
GF is longer also then TC, therefore the angle GHC is less than GTC. So that
henceforth the parts of the pulses GH and IK are mov'd ascew, or cut the Rays
at oblique angles.

It is not my business in this place to set down the reasons why this or that
body should impede the Rays more, others less: as why Water should transmit the
Rays more easily, though more weakly than air. Onely thus much in general I
shall hint, that I suppose the medium MMM to have less of the transparent
undulating subtile matter, and that matter to be less implicated by it, whereas
LLL I suppose to contain a greater quantity of the fluid undulating substance,
and this to be more implicated with the particles of that medium.

But to proceed, the same kind of obliquity of the Pulses and Rays will happen
also when the refraction is made out of a more easie into a more difficult
mediū; as by the calculations of GQ & CSR which are refracted from the
perpendicular. In both which calculations 'tis obvious to observe, that always
that part of the Ray towards which the refraction is made has the end of the
orbicular pulse precedent to that of the other side. And always, the oftner the
refraction is made the same way, Or the greater the single refraction is, the
more is this unequal progress. So that having found this odd propriety to be an
inseparable concomitant of a refracted Ray, not streightned by a contrary
refraction, we will next examine the refractions of the Sun-beams, as they are
suffer'd onely to pass through a small passage, obliquely out of a more
difficult, into a more easie medium."
London, England  
336 YBN
[1664 AD]
1714) As a student at Oxford, Thomas Willis joins the Royalist garrison during
the Civil War.
In the Restoration, Willis gains professional preferment,
becoming Professor of Natural Philosophy at Oxford in (1660-1675). Willis is
one of the founding members of the Royal Society and moves to London just after
the Great Fire, establishing a very large practice in St Martin's Lane.
In 1542
Willis earns a masters degree at Oxford at age 21.
Oxford, England (presumably)  
336 YBN
[1664 AD]
1800)
London, England (presumably)  
336 YBN
[1664 AD]
1801)
London, England (presumably)  
335 YBN
[1665 AD]
1688) Borelli is friends with Malpighi.
Borelli is influenced by the mechanistic view of
Descartes.
Borelli is appointed professor of mathematics at Messina in 1649 and at Pisa in
1656.
During his career, Borelli enjoys the protection of Queen Christina of Sweden,
which shelters him from the attacks from the Italian authorities suffered by
Galileo.
Pisa, Italy (presumably)  
335 YBN
[1665 AD]
1707) Grimaldi is the son of silk merchant.
Grimaldi enters the Jesuit order at 15.
In 1647,
Grimaldi earns his doctorate degree and becomes professor at University of
Bologna.
Grimaldi is an assistant to Ricchioli.
Bologna, Italy (presumably)  
335 YBN
[1665 AD]
1726) Giovanni Domenico Cassini (Ko SEnE) (CE 1625-1712) measures the period of
a Mars day as 24 hours and 40 minutes.

Cassini identifies a number of double stars including the bright star Castor.
Bologna, Italy  
335 YBN
[1665 AD]
1756)
Bologna, Italy  
335 YBN
[1665 AD]
1776) In 1665, Lower gets his bachelor from Oxford.
In 1667, Lower is elected to the
Royal Society.
In London Lower carries out research, some in partnership with Robert
Hooke.
London?, England  
335 YBN
[1665 AD]
1812)
Paris, France   
334 YBN
[12/22/1666 AD]
1712)
Paris, France  
334 YBN
[1666 AD]
1689)
Pisa, Italy (presumably)  
334 YBN
[1666 AD]
1723) Sydenham takes the side of the Parliamentarians. All five Sydenham
brothers (Thomas was the youngest) and their father served as officers in
Cromwell's rebel army. Thomas was wounded, two of his brothers were killed,
their mother was murdered by Royalist troops, and the eldest brother, William,
became a leading figure in Cromwell's protectorate.

Because of the fighting Sydenham does not get his bachelor's degree until 1648
age 24.

Sydenham is friends with Robert Boyle and John Locke.

Sydenham revives the Hippocratic methods of observations and experience.
Sydenham is
recognized as a founder of clinical medicine and epidemiology (study of factors
affecting the health and illness of populations). Sydenham emphasizes detailed
observations of patients and maintains accurate records.
Sydenham is called "the English
Hippocrates" before his death.
London, England (presumably)  
334 YBN
[1666 AD]
1757)
Bologna, Italy  
334 YBN
[1666 AD]
1758)
Bologna, Italy  
334 YBN
[1666 AD]
1803) Hooke is inspired by his optical theories to develop the idea that
planetary motions can be explained in terms of a single attractive force from
the sun bending the straight-line motion of a planet into an elliptical orbit.
In addition, Hooke theorizes that this force would vary in inverse proportion
to the square of the distance between the sun and the planet.

When Newton proves this relationship (in addition to adding a gravitational
constant and object mass), at the request of Edmund Halley in 1684, Newton will
not correct Halley's assumption that Newton had reached the idea himself. This
proof, of course, is the centerpiece of Newton's "Principia Mathematica", which
Halley will persuade Newton to write. Hooke is outraged when he hears that his
original idea is not acknowledged in the "Principia".
London, England (presumably)  
334 YBN
[1666 AD]
1853) Leibniz is born into a Lutheran family near the end of the Thirty Years'
War, which has laid Germany in ruins.
Leibniz is the son of a professor of philosophy
who dies when Gottfried is 6.
Leibniz is a child prodigy.
Leibniz learns Latin at eight,
Greek at 14 (although I have to wonder how well, it is easy to claim but to be
fluent language takes years of learning all of the idioms for example, in
addition to simply the thousands of nouns and verbs)
Leibniz earns a degree in law
from the University of Leipzig in 1665.
Among the great philosophers of this time,
Leibniz is the only one who has to earn a living. As a result, Leibniz serves
in a variety of positions for people of royalty.
Leibniz proposes that education be made
more practical, and that academies be founded.
Leibniz sees as one of his tasks to bring
about a reconciliation between the religious divisions in the Western half of
the religion based on Jesus.
Leibniz works on hydraulic presses, windmills, lamps,
submarines, clocks, and a wide variety of mechanical devices.
Leibniz devises a means of
perfecting carriages and experiments with phosphorus.
While in the mines of the Harz
Mountains, Leibniz hypothesizes that the Earth was at first molten.
Leibniz is an
atomist.
Leibniz meets Huygens.
In 1673 Leibniz is elected to the Royal Society.
Leibniz develops a water
pump run by windmills, which serves the mines of the Harz Mountains, where
Leibniz often works as an engineer from 1680 to 1685.
After the king of France,
Louis XIV takes Strasbourg and lays claim to 10 cities in Alsace in 1681,
Leibniz suggests to his prince a method of increasing the production of linen
and a process for the desalinization of water.
Leibniz formed a goal of writing a
history of the Earth, which includes such matters as geological events and
descriptions of fossils, but never writes it. Leibniz searches monuments and
linguistics for the origins and migrations of peoples, in addition to the birth
and progress of the sciences.
In 1691 Leibniz is named librarian at
Wolfenbüttel and propagates his ideas through articles in scientific journals.
All of these writings oppose Cartesianism, which is judged to be damaging to
faith.
In 1697, Leibniz publishes "De Rerum Originatione" ("On the Ultimate Origin of
Things") which tries to prove that the ultimate origin of things can be nothing
other than a God.
In 1700 Leibniz and Newton are the first foreign members to be
elected into the Parisian Academy of Sciences.
Leibniz is an advisor to Louis XIV and
Peter the Great, Czar of Russia, who Leibniz meets for the first time in
October 1711.
Leibniz turns down an offer to take charge of the Vatican Library.
Leibniz never
marries (yes, but no doubt...ok you understand)
Leibniz is a universal letter
writer with more than 600 correspondents to both educated men and women.
Only
Leibniz's secretary attends his funeral.
Leipzig, Germany (presumably)  
333 YBN
[06/15/1667 AD]
1815) Denis (also Denys) is the personal physician to King Louis XIV.
?, France  
333 YBN
[1667 AD]
1813)
Florence, Italy (presumably)  
333 YBN
[1667 AD]
1816)
Padua?, Italy  
333 YBN
[1667 AD]
5922) Dieterich Buxtehude (CE c1637-1707), Danish (or German) composer composes
music around this time. Most of Buxtehude's instrumental music is for the
organ: about half consists of freely composed music. Buxtehude represents the
climax of the 1600s north German school, and he significantly influences Johann
Sebastian Bach.

(Marienkirche {Saint Mary's church}) Lübeck, Germany  
332 YBN
[11/26/1668 AD]
3257)
London, England (presumably)  
332 YBN
[1668 AD]
1727) Gian Cassini (Ko SEnE) (CE 1625-1712) establishes Jupiter's period of
rotation as nine hours fifty-six minutes, by observing the movement of spots of
Jupiter's clouds.

Cassini is the first to observe the shadows of Jupiter's moons as they pass
between Jupiter and the Sun.


Cassini issues a table of the motions of Jupiter's moons, which will later
serve the Danish astronomer Ole Rømer (Roemer) in his measuring the velocity
of light and proving that this velocity is finite in 1675.
(Observatory at) Panzano (near Bologna), Italy  
332 YBN
[1668 AD]
1736) Redi is known as a poet mainly for his Bacco in Toscana (1685; "Bacchus
in Tuscany").
In 1647, Redi receives his medical degree from the University of Pisa.
He taught
in the Studio at Florence in 1666.
Redi is employed as personal physician to
Ferdinand II and Cosimo III, both grand dukes of Tuscany.
Florence, Italy (presumably)  
332 YBN
[1668 AD]
1817)
Padua?, Italy  
332 YBN
[1668 AD]
1818) De Graaf earns his undergraduate degree from the University of Leiden
where he is a student of Sylvius.
In 1665 De Graaf earns a medical degree from
University of Angers, France.
De Graaf is the first to appreciate the work of
Leeuwenhoek, and introduces Leeuwenhoek's work to the Royal Society.
De Graaf dies in
1673, at age 32.
Delft, Netherlands (presumably)  
332 YBN
[1668 AD]
1830)
Cambridge, England  
331 YBN
[03/08/1669 AD]
3258)
The Hague, Netherlands (presumably)  
331 YBN
[07/??/1669 AD]
1827)
Cambridge, England  
331 YBN
[07/??/1669 AD]
1828)
Cambridge, England  
331 YBN
[1669 AD]
1735) Erasmus Bartholin (BoRTUliN) (CE 1625-1698), Danish physician, is the
first to record the "double refraction" phenomenon of calcite (Iceland
feldspar).

Bartholin receives a transparent crystal from Iceland (now called Iceland spar)
and notes that objects viewed through the crystal are seen double. Bartholin
presumes that light traveling through the crystal is refracted at two angles,
so that two rays of light emerge where one had entered. This phenomenon is
therefore called "double refraction" (and Birefringence). In addition,
Bartholin recognizes that when the crystal is rotated, one image remains fixed
while the other rotates around it. The ray giving rise to the fixed image
Bartholin calls the ordinary ray, and the other the extraordinary ray.

Newton explains so-called "double refraction" in "Opticks" as the result of
rays of light having four sides, two that are responsible for the "unusual"
(extraordinary) refraction, the other two sides responsible for the usual
refraction. Thomas Young will explain double-refraction 150 years in terms of a
wave-theory of light.

Calcite is the most common form of natural calcium carbonate (CaCO3), a widely
distributed mineral known for the beautiful development and great variety of
its crystals. Calcite is polymorphous (same chemical formula but different
crystal structure) with the minerals aragonite and vaterite and with several
forms that apparently exist only under somewhat extreme experimental
conditions.


Bartholin publishes this phenomenon in "Experimenta crystalli islandici
disdiaclastici quibus mira & insolita refractio detegitur". (Hafniæ 1669)
("Experiments with the double refracting Iceland crystal which led to the
discovery of a marvelous and strange refraction", 1959).

I view all refraction phenomena as most likely light particle collision
(reflection) phenomena.
Copenhagen, Denmark  
331 YBN
[1669 AD]
1774) The motivation for Brand's find is a search for the philosopher's stone
in urine.

Brand no doubt refines his production method over time; the version published
later by Leibniz is

* Boil urine to reduce it to a thick syrup.
* Heat until a red oil distills up
from it, and draw that off.
* Allow the remainder to cool, where it consists of
a black spongy upper part and a salty lower part.
* Discard the salt, mix the red
oil back into the black material.
* Heat that mixture strongly for 16 hours.
* First
white fumes come off, then an oil, then phosphorus.
* The phosphorus may be passed into
cold water to solidify.

The chemical reaction Brand stumbles on is as follows. Urine contains
phosphates PO43-, as sodium phosphate (ie. with Na+), and various carbon-based
molecules. Under strong heat the oxygens from the phosphate react with carbon
to produce carbon monoxide CO, leaving elemental phosphorus P, which comes off
as a gas. Phosphorus condenses to a liquid below about 280°C and then
solidifies (to the white phosphorus allotrope) below about 44°C (depending on
purity). This same essential reaction is still used today (but with mined
phosphate ores, coke for carbon, and electric furnaces).

The phosphorus Brand's process yielded was far less than it could have been.
The salt part he discarded contained most of the phosphate. He used about 5,500
litres of urine to produce just 120 grams of phosphorus. If he'd ground up the
entire residue he could have got 10 times or 100 times more (1 litre of adult
human urine contains about 1.4g phosphorus).
Hamburg, Germany (presumably)  
331 YBN
[1669 AD]
1793) Becher is the son of Luthuran minister.
Becher, as economic advisor to Holy Roman
Emperor Leopold I, suggests a Rhine-Danube canal to facilitate trade between
Austria and the Netherlands.
?, Germany  
331 YBN
[1669 AD]
1805)
Amsterdam, Netherlands (presumably)  
331 YBN
[1669 AD]
1811)
Amsterdam, Netherlands   
330 YBN
[1670 AD]
1742)
Cambridge?, England  
330 YBN
[1670 AD]
1908) Spinoza is born in Amsterdam, where his family had settled after fleeing
religious persecution in Portugal.
In 1656 Spinoza is banned from his synagogue on
charges of atheism. The edict asks for God to curse him and warns "that none
may speak with him by word of mouth, nor by writing, nor show any favor to him,
nor be under one roof with him.". Spinoza then Christianizes his name to
Benedict.

Spinoza conducts a large correspondence with various scientists and
philosophers. Two of the most important were Henry Oldenburg, the first
secretary of the British Royal Society, and Gottfried Wilhelm von Leibniz, who
visits Spinoza in 1676.

Spinoza is offered the chair of philosophy at the University of Heidelberg but
declines it, seeking to preserve his independence.

Spinoza died in The Hague in 1677, at age 44, of consumption aggravated by
inhaling dust while polishing lenses.
The Hague, Netherlands  
330 YBN
[1670 AD]
5921) Jean-Baptiste Lully (CE 1632-1687), French composer of Italian birth,
collaborates with Molière on a series of comédies-ballets which culminate in
"Le bourgeois gentilhomme" (1670).

(Is this the earliest evidence of ballet?)
(Court of King Louis XIV) Paris, France  
329 YBN
[1671 AD]
1713) Picard is a Roman Catholic priest.
Picard studies astronomy under Gassendi.
In 1655, Picard
succeeds Gassendi as professor of Astronomy at the Collège de France.
Picard is one of
the charter members of the French Academy of Sciences.
Paris, France (presumably)  
329 YBN
[1671 AD]
1715)
Oxford, England (presumably)  
329 YBN
[1671 AD]
1729) Giovanni Cassini (Ko SEnE) (CE 1625-1712) identifies the moon of Saturn,
Iapetus (IoPeTuS).

Cassini uses a telescope over 100 feet long.
(Paris Observatory) Paris, France   
329 YBN
[1671 AD]
1796)
Amsterdam, Netherlands  
329 YBN
[1671 AD]
1832)
Cambridge, England  
329 YBN
[1671 AD]
1834)
Cambridge, England  
329 YBN
[1671 AD]
1854)
Mainz, Germany  
329 YBN
[1671 AD]
2119)
Oxford, England (presumably)  
328 YBN
[02/19/1672 AD]
1829) The theory that light is a particle is revived. Color determined to be a
property of light, not of objects. Glass prism in use. White light separated
into and recreated from primary colors. Light of different colors shown to
refract at different angles.

Isaac Newton (CE 1643-1727) theorizes that light may be "...globular
bodies...". Newton shows that white light can be separated into and recreated
from primary colors. Newton also shows that color is a property of light, not a
property of objects light is reflected off of, explaining that objects
illuminated with one color appear as that color and that there are no colors in
the dark.

This is Newton's first published paper. This letter recounts the experiments
Newton had conducted six years earlier.

Both Robert Hooke and Christiaan Huygens support a wave theory and lead the
opposition to Newton's new corpuscular theory of light.

This paper divides scientists into two groups, those who support the
corpuscular interpretation of light (light as a particle), and those who view
light as being like sound, a wave where particles of a medium, thought to be
ether, move a signal. These two sides continue to this day, although the wave
interpretation has changed from being made of particles of an aether, to a
non-material electromagnetic translational wave, however currently a large
group of people accept a compromise that light is both a particle and a wave.

This light as a particle, or corpuscular, theory will dominate for 100 years,
but will fall to the theory of light as a wave in the 1800s with the rise in
popularity of Thomas Young's interpretation of light rays canceling each other
out, and using Newton's rings to correctly determine the various wavelengths of
different colors of light. However, the light as a particle theory will emerge
again in the 1900s, Maxwell Planck will view light as made of quanta as a
result of his analysis of the black-body phenomenon.

In 1633 Descartes had described light as being like a "ball".

Newton addresses objections and questions about his corpuscular theory for
light in a November letter. For example, describing the sensation of color:
"...as Modes of Sensation, excited in the mind by various motions, figures, or
sizes of the corpuscles of Light ...".

Note that while supporting a corpuscular theory for light, Newton also supports
the theory that an aether fills the universe, writing in November: "...
assuming the Rays of Light to be small bodies, emitted every way from Shining
substances, those, when they impinge on any Refracting or Reflecting
superficies, must as necessarily excite Vibrations in the æther, as Stones do
in water when thrown into it. ...".

Note too that Newton does not explicitly recognize the idea that all matter is
made of light, first theorized (although not explicitly light in the form of
particles) by Robert Grosseteste in 1208.

My own view is that light is a material particle and the fundamental particle
of all matter, that light beams have no amplitude and do not move in sine wave
shapes but move in straight lines, that light particles can collide with each
other, that light waves do not "cancel" each other out as Thomas Young thought,
and that wavelength is perhaps more accurately called "particle interval". I
think reflection explains the spreading out of light in so-called diffraction
and interference and the phenomenon of polarization. But these questions need
to be examined more and more experiments performed to understand fully what the
true nature of light and the universe is.
Cambridge, England  
328 YBN
[1672 AD]
1191) Perhaps Willis is referring to violence in self defense, but this is
doubtful since unusual and terrible tortures (using various devices) and
painful dangerous procedures are inflicted on people thought to have a mental
disorder. But on the issue of violence as relates to so-called mental disorder,
for some reason, many people tolerate violence such as assault and murder, by
using the excuse that the so-called violenter (the doer of the violence) has a
psychiatric disorder, instead of jailing people who use first strike violence
on nonviolent people, no matter what the reason. Violent and nonviolent people
are all thrown together in psychiatric hospitals, and classified according to
abstract theoretical diseases with no diagnostic evidence. Violence done by
people in psychiatric hospitals by either patients or staff is generally not
made public nor prosecuted.
London, England  
328 YBN
[1672 AD]
1685)
Magdeburg, Germany (presumably)  
328 YBN
[1672 AD]
1730) Giovanni Cassini (Ko SEnE) (CE 1625-1712) identifies a moon of Saturn,
Rhea {rEo} (Ancient Greek: Ῥέᾱ).
Paris, France  
328 YBN
[1672 AD]
1731) The scale of our star system is determined from the parallax of Mars.

(Italian:) Giovanni Domenico Cassini (Ko SEnE) (French:) Jean Dominique Cassini
(KoSE nE) (CE 1625-1712) measures the parallax of planet Mars from his own
measurements in Paris and Jean Richer's (rEsA) (CE 1630-1696) simultaneous
measurements in French Guiana. The relative distances of the planets were known
since the time of Kepler, so only one distance is needed to know the rest. This
provides a scale to the star system, allowing the distance to all the other
planets to be calculated.

Aristarchus of Samos had concluded that the Sun is 19 times more distant than
the moon. Around 1620, Johannes Kepler, using observations of Mars from Tycho
Brahe estimates the distance to the Sun to be at least 1800 times the diameter
of Earth. This distance to Mars can be measured by comparing the position of
Mars to the bright star ψ Aquarii which Mars appears very close to on October
1, 1672. From observations made by Richer in Cayenne and by Picard and Romer in
France, Cassini makes the first approximation of a true determination of the
scale of the solar system and therefore, the distance to the Sun from planet
Earth. Cassini concludes that this distance must be 86 million miles.

From the measurement of the distance from earth to Mars (state actual units),
Cassini calculates that the Sun is 87 million miles from the earth, a value
confirmed by Flamsteed in this same year. While being too low by 7%, this is
the (most accurate measurement and larger than all earlier estimates:
Aristarchos had the sun 5 million miles, Poseidonius 40 million miles, Kepler
guessed 15 million miles).

Richer finds that a pendulum clock moves more slowly in Cayenne than in Paris
by two and a half minutes a day. The conclusion is that the force of gravity is
weaker in Cayenne because it is farther from the center of the earth than
Paris. Perhaps Richer noticed the difference in the clock because of the clock
being slower than the 24 hour day. This will lead Newton (and Huygens) to
conclude that the earth is larger near the equator. This would make the earth
an oblate spheroid, which it is, the surface of earth at the equator is 13
miles {km} farther from the center of the earth than the surface at the poles.
Paris, France;Guiana, South America  
328 YBN
[1672 AD]
1759)
Bologna, Italy  
328 YBN
[1672 AD]
1778)
Paris, France (presumably)  
328 YBN
[1672 AD]
1806)
Amsterdam, Netherlands (presumably)  
328 YBN
[1672 AD]
1807)
Amsterdam, Netherlands (presumably)  
328 YBN
[1672 AD]
1809)
Amsterdam, Netherlands (presumably)  
328 YBN
[1672 AD]
1820) Along with the Italian microscopist Marcello Malpighi, Grew is considered
to be among the founders of the science of plant anatomy.
Grew is the only son
of a clergyman.
Grew's father was on the side of the Parliament in the English
Civil War.
In 1671 Grew earned his medical degree from the University of Leiden,
Netherlands.
Grew is an early member of the Royal Society, and in 1677 is secretary with
Hooke.
In 1676, Grew is the first to use the term "comparative anatomy" in a lecture
before the Royal Society.
presented: London, England  
327 YBN
[1673 AD]
1709)
Gdansk, Poland  
327 YBN
[1673 AD]
1770)
Paris, France (presumably)  
327 YBN
[1673 AD]
1819)
Delft, Netherlands (presumably)  
327 YBN
[1673 AD]
1833)
Oxford, England (presumably)  
327 YBN
[1673 AD]
3377)
Paris, France (presumably)  
326 YBN
[09/07/1674 AD]
1781) Antoni van Leeuwenhoek (lAVeNHvK) (CE 1632-1723) is the first to observe
protists (single-cell organisms with one or more nucleus that are the ancestor
of all multicellular organisms).

Leeuwenhoek examines cloudy water from a nearby lake and discovers that it is
filled with tiny "animalcules," which modern people recognize as protists.

Leeuwenhoek looks at many things including teeth scrapings, and ditch water.
Leeuwenhoe
k notes the fine structure of muscle, skin, hair, ivory, and insects.
Leeuwenhoek finds
tiny creatures parasitic on fleas which will inspire Jonathan Swift to write
his famous quatrain
"So naturalists observe, a flea
Has smaller fleas that on his
prey;
And these have smaller still to bite 'em;
And so proceed ad infinitum."

The microscopes made by Robert Hooke (1635-1703) and other contemporaries are
compound microscopes, with both an objective lens and an eyepiece, but
Leeuwenhoek uses simple microscopes, with a single bead-like lens mounted
between two small thin metal sheets, usually brass. The object to be viewed is
mounted on a pin on one side of the lens, and the eye is placed, almost
touching the lens, on the other. The microscopes are successful because the
tiny spherical lenses are exquisitely ground, or, in a few cases, blown.
Delft, Netherlands  
326 YBN
[1674 AD]
1749)
?, England  
326 YBN
[1674 AD]
1783)
Delft, Netherlands  
326 YBN
[1674 AD]
1825) Mayow earns his Bachelor's degree from Oxford in 1665.
In 1670, Mayow earns his
doctorate in civil law.
Mayow dies around age 36.
Oxford, England  
326 YBN
[1674 AD]
2410)
Lyons, France  
325 YBN
[12/07/1675 AD]
1838)
Cambridge, England (presumably)  
325 YBN
[1675 AD]
1732) Giovanni Cassini (Ko SEnE) (CE 1625-1712) identifies the "Cassini
division", the dark gap between the rings A and B of Saturn.

Cassini thinks that the ring might be made of many tiny objects, but most
astronomers including Herschel view the ring as solid and Cassini's division as
only dark markings on it.
James Maxwell will provide mathematical evidence to
support Cassini's theory 150 years later.
Paris, France  
325 YBN
[1675 AD]
1760)
Bologna, Italy  
325 YBN
[1675 AD]
1780) In 1653 Wren earns a masters degree from Oxford.
In 1657 Wren is professor of
astronomy at Gresham College.
Wren designs St Paul's Cathedral in London after the fire
of 1666.
Wren is a royalist.
Wren is a charter member of Royal Society, and president in 1681.
Wren
wants to redesign London to be more logical, but the land owners stop it.
On a
nearby wall Wren's son later places a dedication: "Lector, si monumentum
requiris, circumspice" ("Reader, if you seek a monument, look about you").

Wren's scientific work is highly regarded by Sir Isaac Newton and Blaise
Pascal.
Wren's speculations on the nature of gravity lay the groundwork for Newton.

Wren is the leader of the English Baroque (architectural) school and remains
the most famous architect in English history.
London, England  
325 YBN
[1675 AD]
1835)
Cambridge, England  
325 YBN
[1675 AD]
1836)
Cambridge, England  
325 YBN
[1675 AD]
1859) Flamsteed is acquainted with Newton and enters Cambridge.
Flamsteed starts his
scientific career under the patronage of William Brouncker, the first president
of the Royal Society, having impressed Brouncker by computing an almanac of
celestial events for 1670.
Flamsteed is forced to become a priest to the parish of
Burstow, Surrey for a source of income from 1684 until his death.
In 1677 Flamsteed
becomes a member of the Royal Society.
Flamsteed is forced to take private pupils to
augment his income. A small inheritance from his father, who dies in 1688,
provides the money to construct a mural arc, a wall-mounted instrument for
measuring the altitudes of stars as they pass the meridian.
Newton expects Flamsteed to
provide his observations, but Flamsteed refuses until he will be finished, and
they become angry with each other. Finally in 1708 Halley publishes a number of
Flamsteed's observations with George of Denmark funding the cost of printing.
Flamsteed become furious, and burns at least 300 copies of the work. (wins
court case)
Greenwich, England  
325 YBN
[1675 AD]
2875)
Paris, France (presumably)  
324 YBN
[06/13/1676 AD]
1837)
Cambridge, England   
324 YBN
[10/09/1676 AD]
1782) Antoni van Leeuwenhoek (lAVeNHvK) (CE 1632-1723) is the first to observe
bacteria (prokaryotes, single-cell organisms without a nucleus).

This is Leeuwenhoek's most famous letter (dated October 9, 1676). This letter
communicates the results of a series of experiments on water filled with
pepper. Leeuwenhoek begins by examining some snow-water that he has kept sealed
for three years. He sees no creatures. Leeuwenhoek then added some peppercorns
to the solution, and, after three weeks, observes the sudden appearance of a
tremendous number of "very little animals." Judging by his calculations of
their number and size, historians have concluded that Leeuwenhoek was the first
person to see bacteria. Colleagues reproduce Leuwenhoek's experiments in the
months that follow. Leeuwenhoek does not connect the microscopic organisms with
disease, but his observations lay the foundation for further investigations.

The organisms Leeuwenhoek sees are so small that, in his words, a million would
not occupy the space of a grain of sand. Leeuwenhoek discovers bacteria but
does not recognize them as a radically different form of life from protists.
Delft, Netherlands  
324 YBN
[1676 AD]
1711) Mariottee is a Roman Catholic priest.
Mariotte is one of the founding members of
the Academy of Sciences in Paris in 1666.
Paris, France (presumably)  
324 YBN
[1676 AD]
1725)
London, England (presumably)  
324 YBN
[1676 AD]
1746)
?, England  
324 YBN
[1676 AD]
1747)
?, England  
324 YBN
[1676 AD]
1748)
?, England  
324 YBN
[1676 AD]
1851) Humans measure the speed of light.

The Danish astronomer, Ole (or Olaus) Rømer (ROEmR) (CE 1644-1710), shows that
the speed of light is finite, and calculates the speed of light as (in modern
units) 225,000 km per second (too small according to the modern estimate:
299,792 km per second).

Aristotle and Descartes has supposed the velocity of light to be infinite.
Galileo had documented an attempt to measure the speed of light in 1638. In the
time before portable accurate chronometers, the eclipses of Jupiter's moons are
thought to be provide accurate time measurements to determine longitude.
Galileo had suggested this in 1612. By 1668 Cassini had published a table of
the motions of the moons of Jupiter. In September 1676, Rømer presents the
Paris Academy with a prediction that the egress, or end, of the eclipse of the
innermost moon of Jupiter expected on November 9 will occur ten minutes late
compared to the time expected from averaging all eclipses. Observations confirm
this prediction, and soon afterwards, Rømer presents memoirs in which he
explains the delay as being due to the time light takes to travel across the
space between Jupiter and Earth. Rømer explains that ingresses, when a Moon
disappears into the shadow of Jupiter only occur (or can only be seen) when the
Earth is approaching Jupiter, and egresses, (when a moon of Jupiter moves out
of the shadow of Jupiter) only occur (or can be seen) when the Earth is moving
away from Jupiter. In addition, Rømer explains that the intervals between
ingresses are shorter than the average value, but egresses are separated by
intervals that are longer than the average value. Rømer recognizes that the
changing eclipse intervals are because of the finite speed of light and the
varying distance that light must cover between Jupiter and the Earth, which is
always decreasing for ingresses and increasing for egresses. From the observed
timings, Rømer calculates that light takes 22 minutes to cross the diameter of
the Earth's orbit. Cassini opposes Rømer's explanation, but Huygens, Newton
and others accept it.

Rømer observes that forty orbits of Io, each 42.5 hours, observed as the Earth
moves towards Jupiter are in total 22 minutes shorter than forty orbits of Io
observed as the Earth moves away from Jupiter, and Rømer concludes from this
that light will travel the distance which the Earth travels during eighty
orbits of Io in 22 minutes.

Roemer announces the calculation of the speed of light at the French Academy of
Sciences in Paris.
An article "Demonstration touchant le mouvement de la
lumiere trouvé par M. Römer de l' Academie Royale des Sciences" will be
published in the "Journal des sçavans." on December 7, 1676 which describes
Roemer's finding.
(Paris Observatory) Paris, France  
324 YBN
[1676 AD]
1870) The island of St. Helena is the future exiled home of Napoleon
Bonaparte.

Halley's father is a wealthy business (owner?).
Halley publishes a work on Kepler's laws
when he is 19.
Halley is called the "southern Tycho".
Halley is awarded a master's degree
from Oxford.
Halley is elected to the Royal Society.
In 1684 Halley encourages Newton and funds
the printing of the Principia.
Halley's father is murdered.
Halley dines with Peter the Great on the
czar's visit to England.
In 1704, despite the objections of Flamsteed, Halley is made a
professor of geometry at Oxford.
Halley's comet appeared in 1986 and should return
around 2061].
Halley repeats the suggestion of Kepler that the transit of Venus be
used to determine the distance of Venus through parallax and therefore the
scale of the solar system.
Halley travels widely and measures magnetic variations.
In 1720 Halley
replaces Flamsteed as astronomer royal. Halley spends 20 years doing careful
observations of the moon.
Saint Helena  
323 YBN
[1677 AD]
1784)
Delft, Netherlands  
322 YBN
[06/25/1678 AD]
3862)
(University of Padua) Padua, Italy  
322 YBN
[1678 AD]
1768)
Paris, France (presumably)  
322 YBN
[1678 AD]
1802)
London, England (presumably)  
322 YBN
[1678 AD]
1871) This book establishes Halley's reputation as an astronomer.
In 1678 Halley is elected
a fellow of the Royal Society and the King intercedes so that Halley is granted
an M.A. degree from Oxford University.
London, England (presumably)  
322 YBN
[1678 AD]
3379) Hautefeuille is born of poor parents, raised by the Duchess of Bouillon,
and eventually takes holy orders and becomes an abbé. Hautefeuille spends all
his time in mechanical pursuits, publishing works on acoustics, optics, tidal
phenomena, and watch mechanisms.
Orléans, France  
322 YBN
[1678 AD]
3592) Swammerdam shows this to the Grand Duke of Tuscany.

Swammerdam describes this experiment in his "Biblia Naturae", volume 2, p.
839:-
"Let there be a cylindrical glass tube, in the interior of which is placed a
muscle, whence proceeds a nerve that has been enveloped in its course with a
small silver wire, so as to give us the power of raising it without pressing it
too much, or wounding it. This wire is made to pass through a ring bored in the
extremity of a small copper support and soldered to a sort of piston, or
partition; but the little silver wire is so arranged that, on passing between
the glass and the piston, the nerve may be drawn by the hand and so touch the
copper. The muscle is immediately seen to contract.". Du Verney in 1700 makes a
similar observation.

Floriano Caldani (1756) and Giambattista Beccaria (1758) will demonstrate
electrical excitability in the muscles of dead frogs, and Luigi Galvani will
demonstrate this clearly (1791). Galvani is most remembered for the connection
of electricity and muscle contraction.

From this will spring the science of reading from and writing to neuron cells,
which enables the remote sending of images and sounds to be seen and hear
directly in the brain.
Amsterdam, Netherlands (presumably)  
321 YBN
[03/??/1679 AD]
1858)
Hannover, Germany  
321 YBN
[05/27/1679 AD]
1527)
(presumably) London, England  
321 YBN
[1679 AD]
1734)
Paris, France  
321 YBN
[1679 AD]
1761)
Bologna, Italy;(p 2: published London, England)  
321 YBN
[1679 AD]
1863) In 1669 Papin earns a medical degree at Angers.
Papin is an assistant to Huygens
in Paris and helps with his air pump experiments.

Papin helps improve Boyle's air pump.
Papin corresponds with Leibniz.
In 1675 Papin goes to
England to be Boyle's assistant.
In 1680 the steam digester earns Papin membership in the
Royal Society, and he cooks a meal for the Society in his digester, in addition
to one for King Charles II.
Papin is a Huguenot (French Protestant) and is
greatly affected by the increasing restrictions placed on Protestants by Louis
XIV of France and the King's ultimate revocation of the Edict of Nantes in
1685. In Germany Papin is able to live with fellow Huguenot exiles from
France.
Papin is professor of mathematics at the University of Marburg from 1687 to
1696.
In 1707 Papin returns to London where he lives in obscurity and poverty until
his death.
London, England  
320 YBN
[01/06/1680 AD]
1848)
Cambridge, England (presumably)  
320 YBN
[06/04/1680 AD]
1787)
Delft, Netherlands  
320 YBN
[07/08/1680 AD]
2326)
London, England (presumably)  
320 YBN
[1680 AD]
1690)
Rome, Italy (presumably)  
320 YBN
[1680 AD]
1740) In this year Boyle is offered the presidency of the Royal Society (in
1680) and the episcopacy but declines both.
London, England (presumably)  
320 YBN
[1680 AD]
1865)
London, England (presumably)  
320 YBN
[1680 AD]
3378)
Paris, France  
319 YBN
[11/04/1681 AD]
1786)
Delft, Netherlands  
319 YBN
[1681 AD]
1824)
London, England (presumably)  
318 YBN
[03/03/1682 AD]
1788)
Delft, Netherlands  
318 YBN
[1682 AD]
1821)
presented: London, England  
317 YBN
[09/12/1683 AD]
1785)
Delft, Netherlands  
317 YBN
[1683 AD]
1724)
London, England (presumably)  
317 YBN
[1683 AD]
1728)
Paris, France  
317 YBN
[1683 AD]
3594)
Paris, France (presumably)  
317 YBN
[1683 AD]
5925) Arcangelo Corelli (CE 1653-1713), Italian violinist and composer,
composes music around this time. Corelli is the first composer whose fame is
based exclusively on his nonvocal music. Corelli's reputation is based mainly
on his sonatas and his 12 Concerti Grossi, which establish the concerto grosso
form. Corelli writes four sets of 12 trio sonatas each (1681-95), a set of 12
solo sonatas (1700), and the concerti grossi (1714).

(Notice how all 3 songs have a similar sound to Pachelbel's Canon - perhaps
this is a traditional sound of the baroque period- a kind of slow string
chromatic and 1-4 2-5 3-6 etc descent pattern.)
Rome, Italy  
316 YBN
[10/??/1684 AD]
1855) The idiotic conflict over who developed differential and integral
calculus between Newton and Leibniz (mainly by Newton) has serious and
far-reaching effects on the development of science. For example, this conflict
results in the cutting off of free communication of ideas between the English
scientists and those of Europe. Leibniz's notation is more efficient than
Newton's and is most popular form of calculus used today.
(develops in) Paris, France; (publishes in) Hannover, Germany  
316 YBN
[11/??/1684 AD]
1847) In August 1684, the British astronomer Edmond Halley visited Newton in
Cambridge to ask him if he could provide a mathematical explanation for the
elliptical orbits of planets.
Upon learning that Newton had solved the problem, Halley
asks Newton's to send the demonstration. Three months later Halley receives the
short tract entitled "De Moto".
Cambridge, England (presumably)  
316 YBN
[1684 AD]
1733) Giovanni Cassini (Ko SEnE) (CE 1625-1712) identifies the moons of Saturn:
Dione (DIOnE) (Greek Διώνη) and Tethys (TEtuS) (Greek Τηθύς).
(Paris Observatory) Paris, France  
316 YBN
[1684 AD]
1822)
London, England (presumably)  
315 YBN
[1685 AD]
1705)
London, England (presumably)  
315 YBN
[1685 AD]
3348)
(Würzburg praemonstrantensian monastery)Würzburg, Germany  
314 YBN
[03/??/1686 AD]
3259)
Hannover, Germany (presumably)  
314 YBN
[09/??/1686 AD]
3262)
Paris?, France (guess)  
314 YBN
[1686 AD]
1874)
London, England (presumably)  
314 YBN
[1686 AD]
1879) In 1691 Fontenelle is elected to the French Academy of Sciences, and in
1697 is the secretary.
Fontenelle writes "Histoire de l'Académie des Sciences", an annual
summary of the work of the Academy starting in 1702.
Fontenelle lives to one month
short of 100.
Fontenelle is a close friend of Montesquieu and well known to
Voltaire, who will make light of Fontenelle in his Micromégas (1752), a
dissertation on the smallness of man in relation to the cosmos.
Although
Fontenelle is generally a modernist, he fails to see the truth of Newtonian
physics.
Paris, France (presumably)  
314 YBN
[1686 AD]
1880) French science writer, Bernard le Bovier de Fontenelle (FonTneL) (CE
1657-1757) publishes "Histoire des oracles" (1687; "History of the Oracles"),
based on a Latin treatise by the Dutch writer Anton van Dale (1683), in which
Fontenelle subjects pagan religions to criticisms that the reader may
inevitably see as applicable to Christianity as well.

The same antireligious bias is seen in Fontenelle's amusing satire "Relation de
l'île de Bornéo" (1686; "Account of the Island of Borneo"), in which a civil
war in Borneo is used to symbolize the conflicts between Catholics (Rome) and
Calvinists (Geneva).

Paris, France (presumably)  
313 YBN
[1687 AD]
1845) Law of gravitation. Isaac Newton (CE 1642-1727) describes the universal
law of gravitation, that all matter attracts other matter with a force that is
the product of their masses, and the inverse of their distance squared.

In his book "Philosophiae Naturalis Principia Mathematica" (Mathematical
Principles of Natural Philosophy, 1687), referred to as "Principia", Newton
codifies three laws of motion. The first is the principle of inertia: a body at
rest remains at rest and a body in motion remains in motion at a constant
velocity as long as outside forces are not involved. This confirms Buridan's
suggestion 300 years before and ends the theory that angels or spirits
constantly push the planets. Planets move because nothing exists in the space
they move to stop them after the initial impulse. The second law of motion
defines a force in terms of mass and acceleration (force = mass x acceleration)
and this is the first clear distinction between the mass of a body
(representing its resistance to acceleration; or in other words the quantity of
inertia it possesses), and its weight (representing the amount of gravitational
force between itself and another body). The third law of motion states that for
every action there is an equal and opposite reaction.

The famous equation Newton publishes is: F=Gm1m2/d^2 where m1 and m2 are the
masses of two objects (for example, the earth and moon), d is the distance
between their centers, G is the gravitational constant, and F is the force of
gravitational attraction between them. Newton holds that this law is true for
any two objects in the universe. So this laws comes to be called the law of
"universal gravitation".

Newton's second law describes the equation F=ma, that the force used to move an
object, and likewise the force a moving object has, is proportional to the
object's mass and acceleration. Substituting a=F/m in the F=Gm1m2/d^2 equation,
the force of acceleration on any mass from another mass can be calculated as
a2=Gm1/r^2.

Newton is the first to estimate the mass or amount of matter contained in a
planet.

That the Sun holds planets with a strength that decreases with distance squared
shown from Ismaël Bullialdus in 1645. Robert Hooke had explained this inverse
distance squared relation to Newton in his letter of 1679.

In his book "Optics" in 1704, Newton suggests that light particles are bent by
gravity writing: " Do not Bodies act upon Light at a distance, and by their
action bend its rays, and is not this action (cæteris paribus) strongest at
the least distance?", but never suggests a mass for light particles.

I think that it cannot be ruled out that the observed phenomenon of gravitation
may be the result, strictly of many particle collisions, or even perhaps the
result of some more complex phenomenon involving living objects at various
scales in space (similar to the way living objects at our scale, persumably
shape globular galaxies).
Cambridge, England (presumably)  
313 YBN
[1687 AD]
1890) Admontons goes deaf while still young, but like Edison considers it a
blessing because he can focus on his work.
Amontons also demonstrates an
optical telegraph and proposes the use of his clepsydra (water clock) for
keeping time on a ship at sea.
Paris, France  
313 YBN
[1687 AD]
3895)
Livorno, Italy  
311 YBN
[1689 AD]
5926) Henry Purcell (CE 1659-1695), English composer, composes music around
this time.

In time Purcell becomes increasingly in demand as a composer, and his theater
music in particular makes his name familiar to many who know nothing of his
church music or the odes and welcome songs he wrote for the court. Much of the
theatre music consists of songs and instrumental pieces for spoken plays, but
during the last five years of his life Purcell collaborates on five
"semi-operas" in which the music is a large part, with "divertissements",
songs, choral numbers and dances.

Purcell's only true opera (i.e. with music throughout) is Dido and Aeneas,
written for a girls school at Chelsea, a suburb of London, and first performed
by the pupils in 1689 although a few outsiders are probably brought in to play
the men's parts.

The Oxford Groove Encyclopedia states that "Purcell was one of the greatest
composers of the Baroque period and one of the greatest of all English
composers."

(Baroque music, with the characteristic bold horns sounds so triumphal.)

(Chapel Royal) London, England  
310 YBN
[12/??/1690 AD]
1862)
Greenwich, England  
310 YBN
[1690 AD]
1200) Polhem's father dies when Christopher is only 10 years old.
Polhem lives with
his uncle in Stockholm and in Stockholm attends a German school until the age
of 12 when his uncle dies leaving Polhem, once again without the possibility of
education.
Polhem works as a farmhand on Vansta, a property in Södertörn, Stockholm for
10 years.
Hungering for knowledge within his fields of interest, mathematics
and mechanics, Plhem soon realizes that he will get no further without learning
Latin. Self-studies are attempted, but given up; Polhem realizes he needs a
tutor. In exchange for constructing a complex clock, Polhem is given Latin
lessons by a local vicar.

Word of Polhem's mechanical skill spreads quickly and a member of the clergy
writes the professor of mathematics at Uppsala University, Anders Spole to
recommend Polhem. Spole presents two broken clocks to Polhem and offers to let
him study under him if Polhem can repair them, Polhem repairs the clocks with
no difficulty and begins recovering years of lost education in 1687, at the age
of 26.
In 1687 Polhem enters the University of Uppsala.
In gratitude for his services the
Swedish government ennobles Polhem in 1716.
Sweden  
310 YBN
[1690 AD]
1696)
Gdansk, Poland  
310 YBN
[1690 AD]
1849)
Cambridge, England (presumably)  
310 YBN
[1690 AD]
1864) From the time of Papin's settlement in Germany he carries on an active
correspondence with Huygens and Leibniz, which is still preserved, and in one
of his letters to Leibniz, in 1698, Papin mentions that he is engaged on a
machine for raising water to a great height by the force of fire.
In a later
communication Papin speaks also of a little carriage he has constructed to be
propelled by this force. Again in 1702 Papin writes about a steam "ballista",
which he anticipates would "promptly compel France to make an enduring peace."
(perhaps a steam powered metal projectile gun?) In 1705 Leibniz sends Papin a
sketch of Thomas Savery's engine for raising water, and this stimulates Papin
to further exertions.
Leipzig, Germany  
310 YBN
[1690 AD]
1867)
Leipzig, Germany  
310 YBN
[1690 AD]
1873) The earliest applications of diving bells were probably for commercial
sponge fishing. A diving bell was used to salvage a cannon from the Swedish
warship Vasa in the period immediately following its sinking in 1628.

In a demonstration, Halley and five companions dive to 60 feet in the River
Thames, and remained there for over one and a half hours. Halley's bell is of
little use for practical salvage work, as it was very heavy, but he does make
improvements to it over time, later extending his underwater exposure time to
over 4 hours.
London, England (presumably)  
310 YBN
[1690 AD]
1888)
?, Sweden  
310 YBN
[1690 AD]
3263)
Leipzig, Germany  
309 YBN
[1691 AD]
1744)
Cambridge?, England  
309 YBN
[1691 AD]
1869) Havers is the son of a rector (the head of a school).
In 1668 Havers enters
Cambridge but does not graduate.
In 1687 Havers gets a medical license after graduating
from University of Utrecht in the Netherlands.
London, England (presumably)  
307 YBN
[1693 AD]
1745)
Cambridge?, England  
307 YBN
[1693 AD]
1750)
?, England  
307 YBN
[1693 AD]
1856) The Encyclopedia Britannica, states that, in criticizing the Cartesian
formulation of the laws of motion, known as mechanics, Leibniz becomes, in
1676, the founder of a new formulation, known as dynamics, which substitutes
kinetic energy for the conservation of movement.
Hannover, Germany  
307 YBN
[1693 AD]
1878) Edmond Halley (CE 1656-1742) prepares detailed mortality tables for the
city of Breslau, a Polish-German town known for keeping meticulous records.
This is one of the first attempts to relate mortality and age in a population,
which leads to modern insurance practices which are based on the idea of
earning income from life insurance using the probability of death in an average
person, while providing the service of allowing people to financially help
their family in the event of (in particular an unexpected) death.

London, England (presumably)  
306 YBN
[03/03/1694 AD]
1789)
Delft, Netherlands  
306 YBN
[10/23/1694 AD]
5923)
(Stuttgart and/or) Gotha, Germany (verify)  
306 YBN
[1694 AD]
1388)
Halle, Saxony-Anhalt  
306 YBN
[1694 AD]
1797)
London, England (presumably)  
306 YBN
[1694 AD]
5957) Elisabeth-Claude Jacquet de la Guerre (CE 1666-1729), French composer,
composes the opera "Cephale et Procris".

Paris, France (performed)   
305 YBN
[06/10/1695 AD]
1792)
Delft, Netherlands  
305 YBN
[1695 AD]
1883)
Oxford, England  
305 YBN
[1695 AD]
1891)
Paris, France (presumably)  
305 YBN
[1695 AD]
3260) Leibniz begins: "Since we first mentioned a new science of dynamics,
which was still to be founded, many prominent men in various places have asked
for a fuller explanation of its teachings. but as we have not yet found leisure
to write a book, we shall here set down some things which may cast some light
on it - light which will be returned to us with interest if we succeed in
eliciting the opinions of men who combine force of insight with distinction of
style. We confess that their judgment will be most welcome and we hope, useful
in advancing the perfection of the work.
We have suggested elsewhere that there is
something besides extension in corporeal things; indeed, that there is
something prior to extension, namely, a natural force everywhere implanted by
the Author of nature - a force which does not consist merely in a simple
faculty such as that with which the Scholastics seem to have contented
themselves but which is provided besides with a striving or effort (conatus seu
nisus) which has its full effect unless impeded by a contrary striving. This
nisus sometimes appears to the senses, and is in my opinion to be understood on
rational grounds, as present everywhere in matter, even where it does not
appear to sense. but if we cannot ascribe it to God by some miracle, it is
certainly necessary that this force be produced by him within bodies
themselves. Indeed, it must constitute the inmost nature of the body, since it
is the character of substance to act, and extension means only the continuation
or diffusion of an already presupposed acting and resisting substance. So far
is extension itself from comprising substance!
It is beside the point here that all
corporeal action arises from motion and that motion itself comes only from
other motion already existing in the body or impressed upon it from without.
For like time, motion taken in an exact sense never exists, because a whole
does not exist if it has no coexisting parts. Thus there is nothing real in
motion itself except that momentaneous state which must consist of a force
striving toward change. Whatever there is in corporeal nature besides the
object of geometry, or extension, must be reduced to this force. This reasoning
does justice, at last, both to truth and to the teachings of the ancients. Our
age has already saved from contempt the corpuscles of Democritus, the ideas of
Plato, and the tranquility of the Stoics which arises from the best possible
connection (nexus) of all things; now we shall reduce the Peripatetic tradition
of forms or entelechies, which has rightly seemed enigmatic and scarcely
understood by its authors themselves, to intelligible concepts. Thus we believe
that this philosophy, accepted for so many centuries, must not be discarded but
be explained in a way that makes it consistent within itself (where this is
possible) and clarifies and amplifies it with new truths."

Leibniz writes "Active force, which may well be called power, as it is by some,
is of two kinds. The first is primitive force, which is in all corporeal
substance as such, since I believe that a body entirely at rest is contrary to
the nature of things. The second is derivative force, which is exercised in
various ways through a limitation of primitive force resulting from the
conflict of bodies with each other. Primitive force, which is nothing but the
first entelechy (note: entelechy eNTeLeKE is an actuality as opposed to a
potentiality and in vitalist philosophy, a vital agent or force directing
growth and life), corresponds to the soul or substantial form, but for this
very reason it relates only to general causes which cannot suffice to explain
phenomena. Therefore I agree with those who deny that forms are to be used in
investigating the specific and special causes of sensible things. This I must
emphasize to make it clear that in restoring to the forms their proper function
of revealing the sources of things to us, I am not trying to return to the word
battles of the more popular Scholastics. A knowledge of forms is necessary,
meanwhile, for philosophizing rightly, and no one can claim to have grasped the
nature of body adequately unless he has paid some attention to such things and
has come to understand that the crude concept of a corporeal substance which
depends only on sensory imagery and has recently been carelessly introduced by
an abuse of the corpuscular philosophy (which is excellent and more true in
itself) is imperfect, not to say false. This can also be shown by considering
that such a concept of body does not exclude cessation or rest from matter and
cannot provide reasons for the laws of nature which apply to derivative force.

Passive force is likewise of two kinds - primitive and derivative. The
primitive force of suffering or of resisting constitutes the very thing which
the Scholastics call materia prima, if rightly interpreted. It brings it about,
namely, that one body is not penetrated by another but opposes an obstacle to
it and is at the same time possessed of a kind of laziness, so to speak, or a
repugnance to motion, and so does not allow itself to be set in motion without
somewhat breaking the force of the body acting upon it. Hence the derivative
force
of suffering thereafter shows itself in various way in secondary matter.
But setting aside these general and primary considerations, and having
established the fact that every body acts by virtue of its form and suffers or
resists by virtue of its matter, we must now proceed to the doctrine of
derivative forces and resistances and discuss the question of how bodies
prevail over or resist each other in various way by their varied impulses. For
to these derivative forces apply the laws of action, which are not only known
by reason but also verified by sense itself through phenomena.
Here, therefore, we
understand by derivative force, or the force by which bodies actually act and
are acted upon by each other, only that force which is connected with motion
(local motion, that is) and which in turn tends to produce further local
motion. For we admit that all other material phenomena can be explained through
local motion. Motion is the continuous change of place and thus requires time.
But as the moving body has its motion in time, so it has a velocity at every
moment of time, a velocity which is the greater in the degree that more space
is passed through in less expenditure of time. This velocity along with
direction is called conatus. Impetus, however, consists in the product of the
mass (molis) of the body by its velocity, and so its quantity is that which
Cartesians usually call the quantity of motion, that is, the momentaneous
quantity, although speaking more accurately, the quantity of motion, having an
existence in time, is an integral of the impetuses (whether equal or unequal)
existing in the moving body multplied by the corresponding intervals of time.
In our debate with the Cartesians, however, we have followed their way of
speaking. yet in the scientific use of terms, as we may conveniently
distinguish an increase which has already taken place, or one still to come,
from one which is now occurring, designating this latter as the increment or
element of the increase; so we can distinguish the falling of a body at the
present moment from the fall which has already taken place which it increases.
So we can also distinguish the present or instantaneous element of motion from
the motion extended through time and call it 'motion'. Then what is popularly
called motion would be called quantity of motion. But although we can readily
comply with any accepted terminology after its meaning is established, we must
be careful about terms until this is done, in order not to be misled by their
ambiguity.
Furthermore, just as the calculation of motion carried out through
time is integrated from an infinite number of impetuses, so in turn the impetus
itself (even though it is a momentaneous thing) arises from a succession of an
infinite number of impacts on the same moving body; so it too contains a
certain element from which it can arise only through infinite repetitions.
Assume a tube AC rotating about a fixed center C with a definite uniform
velocity and in the horizontal plane of this page (Figure 29). Assume a ball B
moving within the tube without any chain or impediment and hence beginning to
move by centrifugal force. It is obvious that the beginning of the conatus of
receding from the center (the conatus, namely, by which the ball D tends toward
the end of the tube is infinitely small with respect to the impetus which it
already has from the rotation or that by which the ball B tends from D to D
along with the tube itself, while retaining its distance from the center. But
if the centrifugal impulsion proceeding from the rotation is continued for some
time, there must arise in the ball, from its own progression, a certain
complete centrifugal impetus D'B' comparable to the impetus of rotation DD'.
Hence the nisus is obviously twofold, an elementary or infinitely small one
which I also call a solicitation and one formed by the continuation or
repetition of these elementary impulsions, that is, the impetus itself. but I
do not mean that these mathematical entities are really found in nature as such
but merely that they are means of making accurate calculations of an abstract
mental kind.
Hence force is also of two kinds: the one elementary, which I also
call dead force, because motion does not yet exist in it but only a
solicitation to motion, such as that of the ball in the tube or a stone in a
sling even while it is still held by the string' the other is ordinary force
combined with actual motion, which I call living force (vis viva). An example
of dead force is centrifugal force, and likewise the force of gravity or
centripetal force; also the force with which a stretched elastic body begins to
restore itself. But in impact, whether this arises from a heavy body which has
been falling for some time, or from a bow which has been restoring itself for
some time, or from some similar cause, the force is living and arises from an
infinite number of continuous impressions of dead force. This is what Galileo
meant when in an enigmatic way, he called the force of impact infinite as
compared with the simple impulsion of gravity. But even though impetus is
always combined with living force, the two are nonetheless different, as we
shall show below.
Living force in any aggregate of bodies can further be
understood in two senses - namely, as total and partial. Partial force in turn
is either relative or directive, that is, either proper to the parts themselves
or common to all. Respective or proper force is that by which the bodies
included in an aggregate can interact upon each other; directive or common
force is that by which the aggregate can itself also act externally. I call
this 'directive' because the integral force of total direction is conserved in
this partial force. Moreover, if it were assumed that the aggregate should
suddenly become rigid by the cessation of the motion of the parts relative to
each other, this alone would be left. Thus absolute total force is composed of
relative and directive force taken together. but this can be understood better
from the rules to be treated below.
So far as we know, the ancients had a knowledge
of dead force only, and it is this which is commonly called mechanics, which
deals with the level, the pulley, the inclined plane (applicable to the wedge
and screw), the equilibrium of liquids, and similar matters concerned only with
the primary conatus of bodies in itself, before they take on an impetus through
action. Although the laws of dead force can be carried over, in a certain way,
to living force, yet great caution is necessary, for it is at this point that
those who confused in general with the quantity resulting from the product of
mass by velocity were misled because they saw that dead force is proportional
to these factors. As we pointed out long ago, this happens for a special
reason, namely, that when for example, different heavy bodies fall, the descent
itself of the quantities of space passed through in the descent are, at the
very beginning of motion while they remain infinitely small or elementary,
proportional to the velocities or to the conatuses of descent. But when some
progress has been made and living force has developed, the acquired velocities
are no longer proportional to the spaces alreadyh passed through in the descent
but only to their elements. Yet we have already shown, and will show more
fully, that the force must be calculated in terms of these spaces themselves.
Though he used another name, and indeed, another concept, Galileo began the
treatment of living force and was the first to explain how motion arises from
the acceleration of heavy falling bodies. Descartes rightly distinguished
between velocity and direction and also saw that in the collision of bodies
that state results which least changes the prior conditions. but he did not
rightly estimate this minimum change, since he changes wither the direction
alone or the velocity alone, while the whole change must be determined by the
joint effect of both together. He failed to see how this was possible, however,
because two such heterogeneous things did not seem to him to be capable of
comparison or of simultaneous treatment - he being concerned with modalities
rather than with realities in this connection; not to speak of his other errors
in his teachings on this problem.
Honoratius Fabri, Marcus Marci, John Alph. Borelli,
Ignatius Baptista Pardies, Claude Deschales, and other most acute men have
given us things that are not to be despised in the doctrine of motion, yet they
have not avoided these capital errors. So far as I know, Huygens, whose
brilliant discoveries have enlightened our age, was also the first to arrive at
the pure and transparent truth in this matter, and to free this doctrine from
fallacies, by formulating certain rules which were published long ago. Almost
the same rules were obtained by Wren, Wallis, and Mariotte, all excellent men
in this field, though in differing measure. but there is no unity of opinion
about the causes; hence men who are outstanding in these studies do not always
accept the same conclusions. It would seem, indeed, that the true foundations
of this science have not yet been revealed. Not everyone has accepted the
proposition which seems certain to me - that rebound or reflection results only
from elastic force, that is, from the resistance offered by an internal motion.
nor has anyone before me explained the concept of forces itself, a matter which
has always disturbed the Cartesians and others who could not undetsand that the
sum of motion or of impetuses, which they take for the quantity of forces, can
be different after collision than it was before, because they believed that
such a change would change the quantity of forces as well.
..."

Use of the concept of entelechy and vis-viva both imply belief in the erroneous
theory of vitalism, the doctrine that phenomena are only partly controlled by
mechanical forces and in biology, a doctrine that ascribes the functions of a
living organism to a vital principle distinct from chemical and physical
forces.

The phenomenon of "partial force" being either relative or directive, relating
to individual parts or common to all, may be similar to the important idea of
collective movement versus individual movement - my argument is that the
electric effect may be a composite effect of many particles from gravity only -
and I want to model these phenomena - where a collective movement appears from
a distance to be an unusual individual movement, for example, larger than the
force of gravity, but as the result of many particles grouped together. I would
call these "composite" (combined) or "individual". But it may be that Leibniz
is describing something else.
Hannover, Germany (presumably)  
303 YBN
[1697 AD]
1823)
London, England (presumably)  
303 YBN
[1697 AD]
1887)
Stockholm, Sweden  
302 YBN
[07/02/1698 AD]
1868) On this day, Savery patents his steam engine.
Savery is a military engineer,
rising to the rank of captain by 1702.
?, England  
302 YBN
[1698 AD]
1777) The size and distance of other stars is measured.

Christaan Huygens (HOEGeNZ) (CE 1629-1695) makes the first specific estimate of
the distance and size of the stars by comparing the size of Sirius to a
fractional portion of the Sun.

Huygens reports in his "Cosmotheoros" (1699), his experiment of drilling a
series of holes in a brass plate, holding the plate up to the Sun, and
comparing the holes to his memory of the appearance of the star Sirius. The
hole that matches is effectively 1/27,664 the apparent size of the Sun. So
Huygens concludes that Sirius, must be 27,664 times farther from us than the
Sun, or about half a light-year away. According to Carl Sagan, had Huygens
known that Sirius is intrinsically brighter than the Sun, he would have almost
calculated the modern estimate of 8.8 light-years away.

Huygens accepts like Nicolas of Cusa that stars are uniformly distributed
through out space and each star has a number of planets.

Huygens also reaffirms the view of Athanasius Kircher (KiRKR) (CE 1601-1680)
that the fixed stars are other suns with planets going around them, but
supports the Copernican Sun-centered theory over the Earth centered-theories of
Tycho Brahe that Kircher supported.
The Hague, Netherlands (presumably)  
301 YBN
[1699 AD]
1886) Built in 1699 in Stjärnsund, the factory produces a number of products,
deriving from the idea that Sweden should export fewer raw materials and
process them within their own borders instead. The factory is a failure; it
meets large resistance among workers who fear they will be replaced by
machinery. Eventually most of the factory is destroyed in a fire in 1734,
leaving only the part of the factory that produces clocks left. The factory
continues producing clocks, known for their high quality and low price.
Although the popularity of the clocks is less during the beginning of the
1800s, clock-making continues to this day at Stjärnsund, still producing
around twenty clocks of the Polhem design per year.

Economically, the factory is unfeasible, but the king at the time, Charles XII,
is supportive and gives Polhem freedom from taxes to encourage his efforts.

The factory of Stjärnsund is visited by Carolus Linnaeus, who writes about the
factory in his diaries as "Nothing is more optimistic than Stjärnsund" ("Intet
är spekulativare än Stjärnsund").
Stjärnsund, Sweden  
301 YBN
[1699 AD]
1893)
Paris, France (presumably)  
301 YBN
[1699 AD]
1896)
Paris, France (presumably)  
301 YBN
[1699 AD]
2008) Malebranche explains his medium theory of light in a lecture given to the
Paris academy devoted to the subject of light and colors. Malebranche is guided
by the analogy of pitch in sound to color in light.
According to Malebranche white has
the greatest frequency, followed by yellow, red and blue, with black having
frequency zero.

In 1712 Malebranche will publish an amended and extended version of his ideas
in which Malebranche adopts Newton's idea of 7 homogenious colors, which he
distinguishes according to their frequency
Paris, France  
300 YBN
[01/02/1700 AD]
1790)
Delft, Netherlands  
300 YBN
[07/11/1700 AD]
1857)
Berlin, Germany  
300 YBN
[1700 AD]
1885) Stahl is born into a wealthy and privileged family.
Stahl earns a medical degree
at Jena in 1684.
Stahl is the son of a minister.
Stahl marries 4 times.
Asimov comments "(Stahl) had
rational views on mental disease". To me this shows, possibly some arrogance or
ignorance in Asimov, by his acceptance of the shockingly brutal and mostly
pseudoscience theories and, hello, unconsensual surgeries of psychology.
In
1694 Stahl becomes professor of theoretical medicine at the newly founded
Prussian University in Halle.
Stahl moves to Berlin in 1715 to serve as the first
royal physician and court counselor to Frederick William I of Prussia, a post
that he holds until his death in 1734. From 1715 Stahl also presides over
Berlin's Medical Board, which becomes the Higher Medical Board for all of
Prussia in 1725. Stahl is instrumental in the founding of the Berlin
Medical-Surgical College in 1723.
Halle, Germany  
300 YBN
[1700 AD]
3593)
Paris, France (presumably)  
300 YBN
[1700 AD]
5924) Tomaso Giovanni Albinoni (CE 1671-1751), Italian composer, composes
around this time. Albinoni is remembered mainly for his instrumental music.

(Tell story of the famous "Adagio".)

(Notice the similar impressive fast scales/arpeggios on violin style similar to
Vivaldi in this work.)

Venice, Italy  
300 YBN
[1700 AD]
6251)
Florence, Italy  
299 YBN
[1701 AD]
1195) The seed drill is invented by Jethro Tull. The seed drill allows farmers
to sow seeds in well-spaced rows at specific depths. Prior to this farmers
simply cast seeds on the ground by hand, to grow where they landed
(broadcasting). Some of the broadcast seeds are cast on unprepared ground where
they never germinate, germinate prematurely only to be killed by frost or die
from lack of access to water and nutrients.

England  
299 YBN
[1701 AD]
1875) To obtain these readings, under instructions from the Admiralty, Halley
commands the war sloop "Paramour Pink" in 1698-1700 on the first sea voyage
undertaken for purely scientific purposes, this one to observe variations in
compass readings in the South Atlantic and to determine accurate latitudes and
longitudes of various ports.
London, England (presumably)  
298 YBN
[12/25/1702 AD]
1791)
Delft, Netherlands  
298 YBN
[1702 AD]
1882) Gregory is the only one in the part of the country he lives in who has a
barometer, which he uses to gather knowledge about the weather. Gregory incurs
the suspicion of the ignorant and superstitious as a dealer in the "black art",
and narrowly escapes being formally tried by the presbytery of the bounds for
witchcraft or conjuration.

David Gregory is the nephew of James Gregory (who designed a reflecting
telescope before Newton).
In 1683 David Gregory is hired as professor of
mathematics at the University of Edinburgh at the recommendation of Newton and
Flamsteed.
David Gregory claims to be first to give public lectures on Newtonian theory.
Da
vid Gregory is hired as professor of astronomy at Oxford.
David Gregory is a friend of
Newton's.
Oxford, England (presumably)  
298 YBN
[1702 AD]
1892)
Paris, France (presumably)  
297 YBN
[1703 AD]
3261)
(written in 1656) Paris, France (presumably)  
297 YBN
[1703 AD]
5932) Antonio (Lucio) Vivaldi (CE 1678-1741), Italian composer, composes trio
Sonatas.

In 1703 Vivaldi is ordained a priest (and later becomes known as the "Red
Priest" for his red hair). He spent most of his career teaching violin and
leading the orchestra at a Venetian girls' orphanage. Vivaldi popularizes
effects such as pizzicato (Played by plucking rather than bowing the strings)
and muting (to soften or muffle the sound of an instrument).

(Vivaldi is an example of the dramatic change that occurred perhaps around 1600
to a very technical high speed playing which is very far from the Gregorian
chants. This clearly must reflect a change in the collective mind and education
of society - to a radically more technical and skillful level. John Bull is an
earlier example of this. It may relate to the radical neuron reading being
discovered. Identify the first "technical" composers. I would look to the
keyboard and violin works, like tocattas.)

(Notice Vivaldi wears a wig - an apparently early indication of this fashion.)

(Ospedale della Pietá Girls' ophanage) Venice, Italy  
297 YBN
[1703 AD]
5942) Johann Sebastian Bach (CE 1685-1750), German composer and organist,
composes his first Violin Sonata (BWV 1001).

(the ducal court) Weimar, Germany  
296 YBN
[1704 AD]
1743)
Cambridge?, England  
296 YBN
[1704 AD]
1826) Newton suggests that light particles are affected by gravity.

In the first edition of his "Opticks", Newton writes: "Do not Bodies act upon
Light at a distance, and by their action bend its rays, and is not this action
(cæteris paribus) strongest at the least distance?".
(mint) London, England (presumably)  
296 YBN
[1704 AD]
5927) Alessandro Scarlatti (CE 1660-1725), Italian composer, composes the opera
"Humanità e Lucifero" ("Humanity and Lucifer") which is about the victory of
Humanity over Satan.

Scarlatti is important in the development of opera and is considered the
founder of the so‐called "Neapolitan school" of opera. His 115 operas include
only one comic opera, "Il trionfo dell'onore" (Naples 1718). Sixty‐four
survive, wholly or in part.

(Lucifer is represented by the tenor.)

(Notice a similarity to melody of Beethoven's 5th symphony. It's apparently
basically the same 4 notes and time but the last note is ascending. There is
also the similar repeating the appegio on higher notes.)

(Teatro Pratolino) Florence, Italy (verify)  
295 YBN
[1705 AD]
1872)
London, England (presumably)  
295 YBN
[1705 AD]
1876)
  
294 YBN
[1706 AD]
1897) Hauksbee is the son of a draper (merchant in cloth or dry goods).
Hauksbee is an
instrument maker.
Hauksbee is a pupil of Boyle's.
In 1705 Hauksbee is elected to the Royal
Society.
London, England (presumably)  
294 YBN
[1706 AD]
1916) Giovanni Battista Morgagni (MoRGonYE) (CE 1682-1771), Italian anatomist,
publishes the first volume of "Adversaria Anatomica" (1706-19) which
establishes his reputation as an accurate anatomist.

"Adversaria Anatomica" is a collection of medical essays communicated to the
Academia Inquietorum which establishes Morgagni in the scientific community.

Padua, Italy  
293 YBN
[01/05/1707 AD]
5930) Alessandro Scarlatti (CE 1660-1725), Italian composer, composes the opera
"Mitridate Eupatore" (1707).

(Teatro San Giovanni Grisostomo) Venice, Italy (verify)  
293 YBN
[1707 AD]
1866)
Hesse-Kassel?, Germany  
293 YBN
[1707 AD]
3256)
Cambridge, England (presumably)  
292 YBN
[02/04/1708 AD]
5938)
(Saint Blasius’s church) Mühlhausen, Germany  
292 YBN
[1708 AD]
1196) Meissen porcelain, the first European porcelain is successfully produced
in a trial firing by Ehrenfried Walther von Tschirnhaus.

Saxony, Germany  
292 YBN
[1708 AD]
1902) Boerhaave is the son of a clergyman.
In 1689 Boerhaave received a Doctor of
Philosophy (PhD) from the University of Leiden.
In 1693 Boerhaave earns a medical
degree at Harderwyck.
Boerhaave spends all of his professional life at the University of
Leiden, serving as professor of botany (1709 ), and of medicine, rector of the
university, professor of practical medicine, and professor of chemistry.
Students come
from all over Europe to study under Boerhaave.
Peter the Great visits Boerhaave.
Boerhaave is
sometimes known as the Dutch Hippocrates.
Boerhaave is regarded as the founder of the
clinical teaching and of the modern academic hospital.
Boerhaave's reputation as one of
the greatest physicians of the 1700s lays partly in his attempts to collect,
arrange, and systematize the mass of medical information that has accumulated
up to his time.
Boerhaave dies extremely wealthy.
Leiden, Netherlands (presumably)  
292 YBN
[1708 AD]
4481)
Paris, France  
291 YBN
[1709 AD]
1194) Other ironmasters following Darby's lead, find that the process is not so
easy to adapt. It is later learned that Darby's coal supply, from Cumbria, just
happens to have a lower than normal sulfur content, which is necessary in order
to producing quality iron. Ironmasters will slowly adapt the blast furnace
process with the introduction of various types of flux that cleans out the
impurities in the coal, and by the mid-1700s iron production will increase.
England  
291 YBN
[1709 AD]
1898)
London, England (presumably)  
291 YBN
[1709 AD]
1904)
Leiden, Netherlands (presumably)  
291 YBN
[1709 AD]
1926)
Amsterdam, Netherlands (presumably)  
290 YBN
[1710 AD]
1752)
?, England  
290 YBN
[1710 AD]
3773) Berkeley writes essays against the freethinkers, for Richard Steele an
essayist.

In politics Berkeley is a Hanoverian Tory.

In his "Treatise Concerning the Principles of Human Knowledge, Part I" (1710),
Berkeley puts all objects of sense, including tangibles, within the mind;
rejects material substance, material causes, and abstract general ideas; while
affirming spiritual substance.
(Trinity College) Dublin, Ireland  
289 YBN
[1711 AD]
1779)
London, England  
289 YBN
[1711 AD]
2329)
England (presumably)  
288 YBN
[1712 AD]
1860) Flamsteed was obliged to turn his data over to the Royal Society, of
which Newton was president.
Greenwich, England  
288 YBN
[1712 AD]
1889) Newcomen is a blacksmith.
Newcomen may have consulted with Hooke on the operation of
vacuums.
In 1698 Newcomen goes into partnership with Savory who had already built the
first steam engine and held comprehensive patents.
Dudley Castle, Staffordshire, England  
287 YBN
[1713 AD]
1751)
?, England  
287 YBN
[1713 AD]
1850) Isaac Newton (CE 1642-1727) publishes a second edition of "Principia" in
which he fires volleys at the philosophies of Leibniz and Descartes in the
"General Scholium" he adds to the second edition.

Cambridge, England (presumably)  
286 YBN
[1714 AD]
1925) Fahrenheit is the son of a wealthy merchant.
Fahrenheit moves to Amsterdam from his
native Danzig (now Gdańsk in Poland) to become a glass blower and
instrument maker.
Alcohol alone boils at too low a temperature to allow high
temperatures to be measured.
Alcohol and water change volume with changing temperature
too unevenly.
In 1724 Fahrenheit's report on his thermometer earns him election to the
Royal Society.

Galileo had invented the thermometer in about 1600, using changes in air volume
as an indicator. Since the volume of air also varies considerably with changes
in atmospheric pressure, liquids of various kinds were quickly substituted.
Using mercury Fahrenheit fixes his zero point by using the freezing point of a
mixture of ice and salt as this gives him the lowest temperature he can reach.
Fahrenheit's other fixed point is taken from the temperature of the human body,
which he puts at 96°. Given these two fixed points the freezing and boiling
points of water then work out at the familiar 32° and 212°.
Amsterdam, Netherlands (presumably)  
285 YBN
[1715 AD]
5941) Johann Sebastian Bach (CE 1685-1750), German composer and organist,
composes "Suite in E minor for Lautenwerk", (BWV 996).

The Lautenwerk (also called Lautenclavecin, Lauten-Clavicymbel, and
Lautenclavier) is the German term for a lute-harpsichord. This is a keyboard
instrument with gut, rather than steel, strings, which are plucked by a quill.
Bach owned two harpsichords at the time of his death, according to an inventory
of his belongings, though neither has survived. The Lautenwerk was played like
the harpsichord, though with a softer sound because of the gut strings. The
instrument was also known in France (‘clavecin-luth’) and Italy
(‘arpicordo leutato’), but most popular in Germany. Even so, the instrument
was relatively rare, even in the Baroque, compared to the standard harpsichord.

(the ducal court) Weimar, Germany  
284 YBN
[1716 AD]
5931) François Couperin (CE 1668-1733), French composer publishes "L′art de
toucher le clavecin" ("The Art of Playing the Harpsichord", 1716) which is the
most valuable instrumental treatise of its time. Couperin starts composing for
harpsichord starting in 1713.

(Saint Gervais Cathedral) Paris, France (presumably)  
284 YBN
[1716 AD]
5939)
Weimar, Germany  
284 YBN
[1716 AD]
5940)
(the ducal court) Weimar, Germany  
283 YBN
[1717 AD]
1944) François Marie Arouet (Voltaire), (CE 1694-1778) is at first exiled and
then imprisoned in the Bastille for writing offensive verses.

Voltaire has a mistress named Émilie Du Châtelet.
Voltaire maintains a long
correspondence with Crown Prince Frederick of Prussia (later Frederick II) and
exchanged letters with Catherine II of Russia.
Over the course of his life Voltaire
writes 28 tragedies on a variety of subjects.
Voltaire is a prolific writer, and produces
works in almost every literary form, authoring plays, poetry, novels, essays,
historical and scientific works, over 20,000 letters and over two thousand
books and pamphlets.
Voltaire became wealthy through wise investment.
In 1758, Voltaire buys a
property on the Swiss border in order to safeguard himself against attacks by
police from either country.

A Voltaire quote is "Divorce is probably of nearly the same date as marriage. I
believe, however, that marriage is some weeks the more ancient."

Wolfgang Amadeus Mozart wrote to his father the year of Voltaire's death,
saying, "The arch-scoundrel Voltaire has finally kicked the bucket....".

At his estate at Ferney, Voltaire renovates the church and has "Deo erexit
Voltaire" ("Voltaire erected this to God") carved on the facade.

Voltaire uses the word "l'infâme" (the infamous thing) to designate the
church, especially when the church is identified with intolerance.

Voltaire never ceased to acknowledge a degree of genius in Shakespeare, yet
spoke of Shakespeare as "a drunken savage."

According to the Columbia Encyclopedia Voltaire opposes the atheism and
materialism of Helvétius and Holbach, and states "If God did not exist, he
would have to be invented," (which in my opinion is wrong, there is no need for
the existence of any dieties).

Voltaire writes between fifty and sixty plays, including a few unfinished
ones.
Voltaire writes numerous histories:
* History of Charles XII, King of Sweden (1731)
* The
Age of Louis XIV (1752)
* The Age of Louis XV (1746 - 1752)
* Annals of the Empire -
Charlemagne, A.D. 742 - Henry VII 1313, Vol. I (1754)
* Annals of the Empire -
Louis of Bavaria, 1315 to Ferdinand II 1631 Vol. II (1754)
* Essai sur l'histoire
générale et sur les mœurs et l'esprit des nations (7 vol., 1756; tr. 1759)
*
History of the Russian Empire Under Peter the Great (Vol. I 1759; Vol. II 1763)

Paris, France  
283 YBN
[1717 AD]
5946) Johann Sebastian Bach (CE 1685-1750), German composer and organist,
composes "Cello Suite No. 1 in G major" (BWV 1007).

Cöthen, Germany (verify)  
283 YBN
[1717 AD]
5951)
(River Thames) London, England  
282 YBN
[1718 AD]
1846) Theory that Universe is mostly made of empty space and that light moves
in a straight line.

These new views are added as extra Queries in the last part of the second
edition of Newton's "Opticks".

Isaac Newton rejects the theory of light as a motion through a medium in favor
of a universe mostly made of empty space and supports the theory that light
moves in a straight line.

Rejecting the idea that light is a motion Newton writes: "Are not all
Hypotheses erroneous, in which Light is supposed to consist in Pression or
Motion, propagated through a fluid Medium?". In support of the Universe being
mostly empty space Newton writes:
"Mr. Boyle has shew'd that Air may be rarified above
ten thousand times in Vessels of Glass; and the Heavens are much emptier of Air
than any Vacuum we can make below.". Newton expresses doubts about the
existance of an aether in writing: "And for rejecting such a Medium, we have
the Authority of those the oldest and most celebrated Philosophers of Greece
and Phoenicia, who made a Vacuum, and Atoms, and the Gravity of Atoms, the
first Principles of their Philosophy". Newton supports the theory that light
moves in a straight line writing "...if it {Light} consisted in Pression or
Motion, propagated either in an instant or in time, it would bend into the
Shadow. For Pression or Motion cannot be propagated in a Fluid in right
Lines...but will bend and spread every way into the ...medium which lies beyond
the Obstacle....The Waves, Pulses or Vibrations of the Air, wherein Sounds
consist bend...For a bell or a Cannon may be heard beyond a Hill which
intercepts the sight of the sounding Body...But Light is never known to ...bend
into the Shadow.".



Query 4 implies that reflection, refraction and inflection (diffraction) are
all controlled by one principle.

Query 5 reveals that Newton accepts the view of heat as motion.

Newton does not recognize that all matter may be made of particles of light,
but does theorize in Query 30 that bodies and Light may be convertible into one
another.
Cambridge, England (presumably)  
282 YBN
[1718 AD]
1899) De Moivre is the son of a surgeon.
A French Huguenot, de Moivre is jailed as a
Protestant upon the revocation of the Edict of Nantes by Louis XIV in 1685.
When de Moivre is released shortly thereafter, he flees to England.
De Moivre
is one of the people France loses to other more tolerant nations.
In London, De Moivre
becomes close friends with Halley and Newton.
In 1697 De Moivre is elected to the Royal
Society.
(De Moivre founds analytical trigonometry, just as Descartes converts geometry
to algebraic formulas, so does De Moivres for trigonometry. t: i don't
understand, he graphically displays trigonmetry?]
London, England (presumably)  
281 YBN
[1719 AD]
5948)
(court of Prince Leopold) Cöthen, Germany and (church of St. Thomas) Leipzig,
Germany   
280 YBN
[1720 AD]
1917) Réaumur is commissioned by Louis XIV (1710) to compile a report on the
industry and arts of France, which is published as the "Description des arts et
métiers" ("Description of the Arts and Skilled Trades").
In 1708 Réaumur is admitted to
the French Academy of Sciences.
Paris, France  
280 YBN
[1720 AD]
1958) Maclaurin is the son of a minister.
Maclaurin is raised by an uncle, also a
minister, after his parents both die.
Maclaurin is a child prodigy and enters the
University of Glasgow at age 11.
In 1715 Maclaurin masters in mathematics (at
age 17).
In 1717 Maclaurin is a professor of mathematics at Mariscal College,
Aberdeen (at age 19).
In 1719 Maclaurin is elected to the Royal Academy (at age 21)
and meets Newton in London.
In 1742 Maclaurin writes in defense of Newton's priority in
forming calculus against philosopher George Berkeley.
In 1745, when Jacobites (supporters
of the Stuart king James II and his descendants) march on Edinburgh, Maclaurin
takes a prominent part in preparing trenches and barricades for the city's
defense, but when the Jacobites take Edinburgh, Maclaurin flees to England.



Colin Maclaurin
Encyclopædia Britannica Article

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born February 1698, Kilmodan,
Argyllshire, Scotland
died June 14, 1746, Edinburgh

Photograph:Maclaurin, engraving by S. Freeman; in the British Museum
Maclaurin,
engraving by S. Freeman; in the British Museum
Courtesy of the trustees of the British
Museum; photograph, J.R. Freeman & Co. Ltd.
Scottish mathematician who developed and
extended Sir Isaac Newton's work in calculus, geometry, and gravitation.

A child prodigy, he entered the University of Glasgow at age 11. At the age of
19 he was elected a professor of mathematics at Marischal College, Aberdeen,
and two years later he became a fellow of the Royal Society of London. At this
time he became acquainted with Newton. In his first work, Geometrica Organica;
Sive Descriptio Linearum Curvarum Universalis (1720; "Organic Geometry, with
the Description of the Universal Linear Curves"), Maclaurin developed several
theorems similar to some in Newton's Principia, introduced the method of
generating conic sections (the circle, ellipse, hyperbola, and parabola) that
bears his name, and showed that certain types of curves (of the third and
fourth degree) can be described by the intersection of two movable angles.

On the recommendation of Newton, he was made a professor of mathematics at the
University of Edinburgh in 1725. In 1740 he shared, with the Swiss
mathematicians Leonhard Euler and Daniel Bernoulli, the prize offered by the
French Academy of Sciences for an essay on tides.

His two-volume Treatise of Fluxions (1742), a defense of the Newtonian method,
was written in reply to criticisms by Bishop George Berkeley of England that
Newton's calculus was based on faulty reasoning. Apart from providing a
geometric framework for Newton's method of fluxions, the treatise is notable on
several counts. It contains solutions to a number of geometric problems, shows
that stable figures for a homogeneous rotating fluid mass are the ellipsoids of
revolution, and gives for the first time the correct theory for distinguishing
between maxima and minima in general (see calculus of variations), pointing out
the importance of the distinction in the theory of the multiple points of
curves. It also contains a detailed discussion of infinite series, including
the special case of Taylor series now named in his honour.

In 1745, when Jacobites (supporters of the Stuart king James II and his
descendants) were marching on Edinburgh, Maclaurin took a prominent part in
preparing trenches and barricades for the city's defense. As soon as the rebel
army captured Edinburgh, Maclaurin fled to England until it was safe to return.
The ordeal of his escape ruined his health, and he died at age 48.

Maclaurin's "Account of Sir Isaac Newton's Philosophical Discoveries" will be
published posthumously, as will be his "Treatise of Algebra" (1748).
Aberdeen, Scotland (presumably)  
280 YBN
[1720 AD]
5945) Johann Sebastian Bach (CE 1685-1750), German composer and organist,
composes "Partita No. 3" (BWV 1006).

(the ducal court) Weimar, Germany  
279 YBN
[1721 AD]
1223) Johann Sebastian Bach (March 21, 1685 - July 28, 1750) a prolific German
composer and organist, presents six concertos, the "Brandenburg concertos" (BWV
1046-1051) in 1721 but these are probably composed earlier, and will become
very popular.

Germany  
279 YBN
[1721 AD]
5929) Alessandro Scarlatti (CE 1660-1725), Italian composer, composes the opera
"La Griselda".

(Viceroy of Naples Court) Naples, Italy  
279 YBN
[1721 AD]
5947) Johann Sebastian Bach (CE 1685-1750), German composer and organist,
composes "Violin Concerto No. 1 In A Minor" (BWV 1041).

Cöthen, Germany (verify)  
279 YBN
[1721 AD]
5955)
Cöthen, Germany (verify)  
278 YBN
[1722 AD]
1934)
Kew, England  
278 YBN
[1722 AD]
5944)
(the ducal court) Weimar, Germany  
278 YBN
[1722 AD]
5949)
(church of St. Thomas) Leipzig, Germany   
278 YBN
[1722 AD]
5950)
(church of St. Thomas) Leipzig, Germany   
277 YBN
[1723 AD]
3322) Maraldi is born in Perinaldo/Nica, Italy, as a nephew of G.D. Cassini.
Jacques
Philippe (or Giacomo Filippo) Maraldi comes to Paris in 1687 to assist his
uncle at the Paris Observatory and in geodesic work.
  
276 YBN
[1724 AD]
1881) Bernard le Bovier de Fontenelle (FonTneL) (CE 1657-1757) publishes "De
l'origine des fables" (1724; "Of the Origin of Fables"), in which Fontenelle
supports the theory that similar fables arise independently in several cultures
and also lightly addresses comparative religion.

Paris, France (presumably)  
276 YBN
[1724 AD]
1903)
Leiden, Netherlands (presumably)  
276 YBN
[1724 AD]
1970) Daniel Bernoulli (BRnULE) (CE 1700-1782), Swiss mathematician writes
"Exercitationes quaedam Mathematicae" on differential equations and the physics
of flowing water.
This book will win him a position at the influential Academy of
Sciences in St. Petersburg, Russia.

Daniel Bernoulli is the second son of Johann Bernoulli, who first teaches him
mathematics.

Italy?  
275 YBN
[1725 AD]
1861)
London, England (presumably)  
275 YBN
[1725 AD]
3604)
Lyon, France  
275 YBN
[1725 AD]
5933) Antonio (Lucio) Vivaldi (CE 1678-1741), Italian composer, composes
Mandolin Concerto (RV425).

Venice, Italy  
275 YBN
[1725 AD]
5934) The simplicity of Vivaldi's funeral on July 28, 1741, suggests that he
dies in considerable poverty.
Venice, Italy  
275 YBN
[1725 AD]
5943)
(Saint Thomas Church) Leipzig, Germany  
274 YBN
[1726 AD]
1945) Voltaire (CE 1694-1778) is assaulted by people hired by, a young
nobleman, the chevalier de Rohan, who resented witty writings made at Rohan's
expense by Voltaire. Far from obtaining justice, Voltaire is then imprisoned in
the Bastille through the influence of the powerful Rohan family, and is
released only upon his promise to go to England.
During the more than two years
(1726-28) in England, Voltaire meet many literary people of the period through
his friend Lord Bolingbroke. Voltaire is impressed by the greater freedom of
thought in England and is deeply influenced by Newton and Locke.

Paris, France  
274 YBN
[1726 AD]
3381) In 1703 Hales earns a masters degree in theology from Cambridge.
In 1753 Hales is
elected a foreign member of French Academy.
Teddington, England (presumably)  
273 YBN
[1727 AD]
1909) This work will be republished in 1733 as volume 1 of Hales' "Statical
Essays".
Cambridge, England  
273 YBN
[1727 AD]
1991) (Over the course of his lifetime:)

1768 Euler publishes a very successful popularization of science (science
history?).
Euler publishes no less than 856 separate works.
Euler's collected works are more than
seventy volumes.
Euler began replacing geometric proofs with algebraic proofs.
Euler is one of
the first to develop the methods of the calculus on a wide scale.
Euler is
credited with being the first to use the Greek letter Sigma for summation.
In 1739 Euler
writes the "Tentamen novae theoriae musicae", hoping to eventually integrate
musical theory as part of mathematics.
In 1741 Euler accepts the invitation of Frederick II
of Prussia to join the newly reorganized Berlin Academy of Sciences. Euler
spends twenty-five years in Berlin, during which time Euler is closely
associated with the academy's president, Pierre-Louis Moreau de Maupertuis
(1698-1759).
During this time in the "Republic of Letters", Euler participates in several
controversies including a dispute on the monads of Leibniz, which Euler
vehemently opposes and a controversy about Maupertuis's "Principle of Least
Action," in which Euler supports his colleague Maupertuis against Johann Samuel
König and Voltaire.
Maupertuis's dies in 1759 and Euler becomes the de facto leader and
administrator of the Berlin Academy, but without the official title of
president.
Euler's strained relations with Frederick II lead Euler to accept an
invitation from Catherine the Great to rejoin the In "Rettung der Göttlichen
Offenbahrung Gegen die Einwürfe der Freygeister" ("Defense of the Divine
Revelation against the Objections of the Freethinkers") is primarily an
argument for the divine inspiration of scripture, which presents Euler as a
staunch Christian and a biblical literalist.
De Morgan relates a story about Czarina
(Elizabeth) being displeased with the antireligious views of Denis Diderot, and
persuading Euler to help her in suppressing Diderot. Diderot is informed that a
learned mathematician has an algebraic demonstration of the existence of a
deity and would like to give this proof to Diderot before the Court, to which
Diderot agrees. Euler advanced towards Diderot and states "Monsier, a+bn/n=x,
donc Dieu existe; respondez!", De Morgan writes that Diderot does not
understand algebra, and is embarrassed while laughter arises on all sides.
According to De Morgan Diderot then asks permission to return to France which
is granted. However amusing the anecdote may be, it is almost certainly false,
given that Diderot was actually a capable mathematician who had published
mathematical treatises. (I find this story to be very biased in favor of belief
in a Deity. In addition, no math equation proves the existence of a Deity. It
is amazing that there appears to be a universe that may have no end in size,
magnification or microfication, but that does not equal evidence of a Deity,
simply that there is an awesome and incomprehensible universe, there is no need
or evidence for a Deity. We can be in deep respect and awe of the universe
without any Deities, and in particular in the form of a human, knowing the
history of the traditional beliefs of Deities who lived in the clouds of an
earth-centered universe, and then monotheism, etc.)
St. Petersburg Academy which
Euler does in 1766 remaining there until his death in 1783.
Saint Petersburg, Russia (presumably)  
273 YBN
[1727 AD]
2620)
London, England (presumably)  
272 YBN
[08/??/1728 AD]
1913) In 1724, Bering is appointed by Peter I (the Great), Tsar of Russia, to
determine whether Asia and North America are connected by land. Peter the
Great, who is modernizing Russia, wants Russia's vast new holdings in Siberia
mapped. The Russian leaders are interested in both colonial expansion in North
America and in finding a northeast passage, that is a sea route to China around
Siberia.
In 1648 a Russian, Semyon Dezhnyov, had sailed through the Bering Strait, but
his report went unnoticed until 1736.

Bering leads the expedition over 6,000 miles of wilderness and reaches Okhotsk
on the Pacific coast on September 30, 1726, nineteen months after leaving St.
Petersburg. The group then builds ships and sails to the Kamchatka Peninsula.
The ship Gabriel is built (on the Kamchatka Peninsula), and on July 14, 1728,
Bering begins his first exploration. The Gabriel sails northward, rounding East
Cape on August 14. Since the Asiatic coast trends westward and no land appears
to the north, Bering decides that he has fulfilled his mission, correctly
concluding that Siberia and America are not joined; Bering then turns back at
latitude 67° 18' to avoid wintering on a desolate and unknown shore. The
expedition spends the winter at Kamchatka, where Bering sees numerous signs
indicating land to the east. But bad weather during the following summer
frustrates his attempts to locate this land, and the expedition returns to St.
Petersburg in March 1730.

The Bering Strait and Bering Sea are named after Vitus Bering.
Bering Straight  
272 YBN
[1728 AD]
1202) Daniel Defoe writes "Is it not enough to make any one mad to be suddenly
clap'd up, stripp'd, whipp'd, ill fed, and worse us'd?" against "treatments"
given with no consent in psychitric hospitals.

  
271 YBN
[01/??/1729 AD]
1931) In 1717 Bradley earns his Masters degree from Oxford.
Bradley is friends
with Newton and Halley.
In 1718 Bradley is elected to the Royal Society.
In 1742 on the death of
Halley, Bradley is appointed third astronomer royal.

Bradley announces this finding in (Phil. Trans. xxxv. 637).
Kew, England  
271 YBN
[1729 AD]
1884)
?, England  
271 YBN
[1729 AD]
1957) Gray is the son of a dyer.
In London Gray assists Dr John Desaguliers, one of
the Royal Society' demonstrators, who gives lectures around the country (and on
the Continent) about new scientific discoveries.

In this position Gray is probably not paid, but provided with a place to live
only. Gray falls into poverty and through the efforts of John Flamsteed and Sir
Hans Sloane (later President of the Royal Society) obtains a pensioned position
at the Charterhouse in London (a home for destitute gentlemen who had served
their country). During this time Gray begins experimenting again with static
electricity, using a glass-tube as a friction generator.
London, England  
271 YBN
[1729 AD]
1962)
??, France (presumably)  
271 YBN
[1729 AD]
5936)
(New Italian Theatre) Paris, France (presumably)  
270 YBN
[1730 AD]
1205)
England  
270 YBN
[1730 AD]
1900)
London, England (presumably)  
270 YBN
[1730 AD]
1941) Brandt is the son of an apothecary.
Brandt studies medicine and chemistry under
Boerhaave.
In 1726 Brandt earns a medical degree but does not practice.
In 1727 Brandt is in charge
of Bureau of Mines at Stockholm.
In 1730 Brandt is made assay master (warden) of the
Stockholm mint.
German miners named a blue metal Kobold after an earth spirit (roots
in polytheism?) they believed had bewitched what they thought was (also blue)
copper ore.
Brandt is hired as professor of chemistry at the University of Uppsala.
Kolbolt
had been used to make a blue dye for a few centuries.
Brandt is one of the first chemist
to speak out against alchemical fraud, dedicating his last years to exposing
fraudulent alchemical processes for producing gold, such as the trick of
dissolving gold in nitric acid and then precipitating the gold out when the
acid is cooled and shaken. Asimov describes Brandy as the first chemist to be
completely free of alchemical taint.
Stockholm, Sweden  
269 YBN
[1731 AD]
1920)
Paris, France (presumably)  
269 YBN
[1731 AD]
2035) Alexis Claude Clairaut (KlArO) (CE 1713-1765), French mathematician
publishes "Recherches sur les courbes à double courbes" at age 18.

Clairaut is the son of a mathematics teacher.
By age ten Clairaut studies L'Hôpital's
work on conic sections and two years later reads a paper to the French
Académie des sciences.

Clairaut collaborates with the Marquise du Châtelet in her French translation
of Newton's "Principia".

Clairaut is noted for his work on differential equations and on curves and for
formulating Clairaut's theorem dealing with geodesic lines on the surface of an
ellipsoid.

Clairaut helps the development of three-dimensional analytic geometry around
1730, when Clairaut, and the Swiss mathematicians Leonhard Euler and Jakob
Hermann produce general equations for cylinders, cones, and surfaces of
revolution.

Paris, France  
269 YBN
[1731 AD]
2956)
London, England  
268 YBN
[06/27/1732 AD]
2105) Interesting that the oldest university in Europe would be the first to
hire a female professor. This shows a strong belief in gender equality in Italy
at an early time relative to other nations.
Bassi has eight to twelve children.
Bologna, Italy  
268 YBN
[1732 AD]
3595)
London, England (presumably)  
267 YBN
[12/??/1733 AD]
1965) Du Fay is the superintendent of gardens for King Louis XV.
Du Fay never
marries.
Du Fay dies of smallpox at age 40.
Paris, France  
267 YBN
[1733 AD]
1197)
England  
267 YBN
[1733 AD]
1901) In 1694 Saccheri is ordained a priest.
In 1697 Saccheri teaches mathematics at
the Jesuit College of Pavia until death.
Other books by Saccheri are: Quaesita
geometrica (1693), Logica demonstrativa (1697), and Neo-statica (1708).
Pavia, Italy  
267 YBN
[1733 AD]
1910)
Cambridge, England  
267 YBN
[1733 AD]
1933)
Kew, England  
267 YBN
[1733 AD]
1943)
Stockholm, Sweden (presumably)  
267 YBN
[1733 AD]
1988) Dolland uses two different kinds of glass which refract the various
colors of light (by different angles), and combines them so that the action of
one glass is counterbalanced by the action of the other (needs to be more
specific). This invention allows larger refracting telescopes (achromatic
telescopes) to be usable. These lens are also used in achromatic microscopes.
London, England (presumably)  
267 YBN
[1733 AD]
5935) Georg Philipp Telemann (CE 1681-1767), German composer, composes his
"Musique de table" (1733).

Telemann is by far the most famous composer in Germany; in a contemporary
dictionary he is assigned four times as much space as J. S. Bach. (Perhaps the
close-sounding association with "Telephone"-man helped his popularity.)

(Hamburg Opera) Hamburg, Germany  
267 YBN
[1733 AD]
5937) Jean-Philippe Rameau (CE 1683-1764), French composer and theorist,
composes his first opera "Hippolyte et Aricie".

(the Opéra) Paris, France (presumably)  
266 YBN
[1734 AD]
1919)
Paris, France (presumably)  
266 YBN
[1734 AD]
2073)
Sweden (presumably)  
265 YBN
[1735 AD]
1936) Harrison is a Yorkshire mechanic.
After 5 months at sea one of Harrison's clock is
off by less than a minute.
Harrison is the son of carpenter.
Harrison's fifth clock is no bigger
than a large watch.
In 1598 Phillip II of Spain offered a similar prize that went
unclaimed.
In 1707 a British fleet miscalculates its position and crashes into
rocks off Cornwall, so in 1713 the British government offers a reward of
£20,000 for an accurate ship's chronometer.
Harrison first became interested in the problem
of an accurate clock in 1728.
In 1765 Harrison finally receives £20,000 reward for
an accurate ship's chronometer.
Harrison's chronometer will be used in 1776 by James Cook on
his voyage to Australia and New Zealand.
London, England  
265 YBN
[1735 AD]
1973) Charles Marie de La Condamine (loKoNDuMEN) (CE 1701-1774), French
geographer is sent by the Académie des Sciences to Peru to make astronomical
observations which will determine the length of a degree of the meridian near
the Equator.
La Condamine accomplishes the first scientific exploration of the Amazon
River.
La Condamine returns to Europe from South America with rubber tree sap and
curare (used as a muscle relaxant).
La Condamine supports a standard system of
measure.
La Condamine speculates on the idea of inoculation against smallpox 22
years before Jenner.
La Condamine confirms that the force of gravity at the
equator is greater than that in Europe, proving that the earth is wider at the
equator and is an oblate spheroid (as opposed to a prolate spheroid as claimed
by Cassini and his son).

Peru, South America  
265 YBN
[1735 AD]
1996) Swedish botanist, Carolus Linnaeus (lin Aus or lin EuS) (CE 1707-1778)
creates a uniform system for categorizing living objects of earth, including
the human species (overshadowing the earlier work of Ray) and is considered the
founder of taxonomy.

In his book "Systema Naturae" (1735), Linnaeus (linAus]) establishes the
classification of living things in a methodical way (overshadowing the earlier
work of Ray). For this Linnaeus is considered the founder of taxonomy. Linnaeus
popularizes a binomial nomenclature where each living object is given a generic
name and then a specific name, and points out exactly how each species differs.

This book is first published in 11 pages, but will have 2,500 pages by the
tenth edition. This book presents a classification of three kingdoms of nature.
Linnaeus groups species into genus, class, order, (later Cuvier will group
orders in phyla). Linnaeus daringly even includes humans in his categorization
calling them "homo sapiens" (man, wise). Linnaeus includes the orangutan in the
same genus as humans naming them "homo troglodytes" ("man, cave-dwelling" but
this name will not endure).

Linnaeus is the first to use the male and female symbols.

Linnaeus also includes minerals in his classification system.
Netherlands  
264 YBN
[1736 AD]
1923) In 1694, Desaguliers' family fled to England as Protestants to escape
persecution by Louis XIV.
Desaguliers is educated at Oxford.
In 1710 Desaguliers is made a
deacon.
The word "insulator" is Latin for "Island", since nonconductors can contain the
electric fluid as the sea contains an island.
Desaguliers at one time assists Sir Isaac
Newton in Newton's experiments and through his speakings and writings was among
Newton's staunch advocates.

Between 1729 and 1736, Stephen Gray and Jean Desaguliers who are friends,
perform a series of experiments which show that a cork and other objects can be
electrified as far away as 800 or 900 feet away by connecting them to a rubbed
glass tube with materials such as metal wires or string made of hemp. Gray and
Desaguliers find that other materials, such as silk, do not allow the distant
objects to be electrified. Gray and Desaguliers find that the distant object
will not become electrified if the transmission line makes contact with the
earth, but only if the object and earth are separated or insulated by
suspending the object on silk threads.
London, England  
264 YBN
[1736 AD]
1966) Maupertuis is from a wealthy family.
In 1731, Maupertuis becomes a member of the
Academy of Sciences in Paris.
The success of Maupertuis' expedition gains him favor
with Frederick the Great, who calls Maupertuis to Berlin.
Maupertuis becomes a
member of the Berlin Academy of Sciences in 1741 and serves as its president
from 1745 to 1753.
Maupertuis helps popularize Newtonian mechanics.
Maupertuis will write
numerous astronomical writings, including "Discours sur la figure des astres"
(1732) and 'Discours sur la parallaxe de la lune" (1741).
Lapland  
263 YBN
[1737 AD]
1808)
Amsterdam, Netherlands (presumably)  
263 YBN
[1737 AD]
1905)
Leiden, Netherlands (presumably)  
263 YBN
[1737 AD]
2001)
Netherlands(presumably)  
262 YBN
[1738 AD]
1226) A valve-type flush toilet is invented by JF Brondel.

  
262 YBN
[1738 AD]
1928)
France (presumably)  
262 YBN
[1738 AD]
1946)
Cirey, France  
262 YBN
[1738 AD]
1971)
Basel, Switzerland (presumably)| (published in ) Strasbourg  
262 YBN
[1738 AD]
2087)
Cambridge, England  
261 YBN
[1739 AD]
1912)
Cambridge, England  
261 YBN
[1739 AD]
1937)
London, England  
261 YBN
[1739 AD]
2088)
Paris, France  
260 YBN
[1740 AD]
1201)
Sheffield, England  
260 YBN
[1740 AD]
1918)
Paris, France (presumably)  
260 YBN
[1740 AD]
2005) Georges Louis Leclerc, comte (count) de Buffon (BYUFoN) (CE 1707-1788),
French naturalist, translates Newton's "The Method of Fluxions" (1740) into
French.

Montbard, France  
260 YBN
[1740 AD]
2006) When done this the "Histoire" will contain:
Vols. 1-15. Quadrupeds, (1749-67),
written with the assistance of Louis Daubenton who provides the anatomical
details.
Vols. 16-24. Birds, (1770-83), written with the assistance of the Abbé Bexon
and G. de Montbeillard.
Vols. 25-31. Supplementary Volumes. These deal mainly with the
quadrupeds, but Vol. 5 (1778) contains Buffon's important "Epochs of Nature".
Vols.
32-36. Minerals, (1783-88).
The final 8 volumes, Reptiles (2 vols., 1788-89), Fish (5
vols., 1798-1803), and Cetacea (1804) will be prepared by E. de Lacepede.


Buffon is not interested in problems of plant and animal classification in
contrast to the publications of the Swedish botanist Carl Linnaeus. In Volume
1, Buffon (wrongly) argues that natural classes such as cats and dogs are
misguided and that only individuals exist in nature. However Buffon accepts
that "two animals belong to the same species as long as they can perpetuate
themselves". In this work Buffon rejects the idea of a common descent for
similar animals arguing that if the ass was derived from the horse that there
would be intermediate forms but that none are found.

Buffon wrongly views apes as corrupted humans, and donkeys as corrupted horses
(Erasmus Darwin will also believe this inaccurate theory).
Montbard, France  
260 YBN
[1740 AD]
2007) The Answers.com Biography of Buffon states that "All of these questions
impinged upon religious matters. While Buffon evidently satisfied all the
outward forms of Christian practice, he almost certainly was a deist in the
1730s and may very well have become an atheist in his later years."

The Oxford University Press, French Literature Companion, states that "while
avoiding direct conflict with the Church, {Buffon's} conception of human nature
and origins was unrepentantly heretical".
Montbard, France  
260 YBN
[1740 AD]
2010)
  
260 YBN
[1740 AD]
2019) Marggraf is the director of the chemical laboratory of the German Academy
of Sciences of Berlin (1754-60) (appointed by Frederick II in 1753).
Berlin, Germany (presumably)  
260 YBN
[1740 AD]
2067) Bonnet finds that the eggs of the spindle-tree aphid female can develop
without being fertilized by sperm.
Bonnet notes the freshwater hydra's ability to
regenerate lost body parts. (identify when)

In 1695 Antoni van Leeuwenhoek (lAVeNHvK) (CE 1632-1723) had identified
parthenogenesis in aphids.
Geneva?, Switzerland (presumably)  
260 YBN
[1740 AD]
2961) Bose conveys electricity from on person to another using water.
Bose is a
professor of natural philosophy at (University of) Wittenberg.
Bose performs public
experiments with his electrostatic machines. One of experiment is actually a
joke. A charming young lady offers a welcoming kiss to somebody from the
audience. However, she stands on an electrically isolated platform and her body
is connected to a hidden charged electrostatic generator. The kiss is
accompanied by an electrical spark. A shock obtained by a man sometimes is very
strong. Bose describes this "funny" experiment in his poem written for countess
Brühl.

In 1760, during a war with Prussia, Bose is kidnapped to Magdeburg, where Bose
dies in the following year.
(University of Wittenberg)Wittenberg, Germany  
259 YBN
[07/16/1741 AD]
1914) Bering had proposed a second exploratory mission (his first mission in
1728 showed that no land bridge exists between Siberia and America), and in
1732 Bering is given command of what is called the "Great Northern Expedition".
This begins as a small proposal but becomes unrealistically inflated by the
government. Bering is to locate and map the American coast as far as the first
European settlement; other groups, coordinated by him, are to chart the
Siberian coast and determine once and for all whether Asia and America are
connected. Bering is in charge of a sizable scientific party, and also ordered
to initiate economic development in eastern Siberia.

Bering will not survive the expedition, however forty-five of the 77 officers
and men of the St. Peter eventually will reach safety in 1742.
This "Great Northern
Expedition", obtains significant geographic and scientific information: mapping
the strait, now named for Bering, dividing Asia and America, the Siberian coast
from the White Sea to the Kolyma River, and the coast of America from Prince of
Wales Island to the Komandorskie Islands.

Bering suffers from scurvy and will die on Bering Island, near Kamchatka.
Bering Straight  
259 YBN
[09/12/1741 AD]
5952)
(composed) London, England and (performed) Dublin, Ireland  
259 YBN
[1741 AD]
1911)
Cambridge, England  
258 YBN
[1742 AD]
1929) Goldbach is the son of a minister.
Goldbach studies medicine and mathematics at the
University of Königsberg.
In 1725 Goldbach is hired as professor of mathematics at the
Imperial Academy of St. Petersburg.
Goldbach is a voluminous correspondent with
mathematicians of the time.
Moscow, Russia  
258 YBN
[1742 AD]
1942)
Stockholm, Sweden  
258 YBN
[1742 AD]
1948) Voltaire (CE 1694-1778) writes the drama "Mahomet, ou le fanatisme") aka
"Fanaticism, or Mahomet", a play in 5 acts, which he describes as "written in
opposition to the founder of a false and barbarous sect to whom could I with
more propriety inscribe a satire on the cruelty and errors of a false prophet."

Cirey, France  
258 YBN
[1742 AD]
1959)
Edinburgh, Scotland  
258 YBN
[1742 AD]
1963) I think it is again important to note that a microscope and telescope are
basically the same thing, magnifiers, they spread out light so a small area
appears to be larger.
Amsterdam, Netherlands  
258 YBN
[1742 AD]
1975) Celsius is a professor of astronomy at Uppsala University from 1730 to
1744, and in 1740 he builds the Uppsala Observatory.
Initially Celsius places the boiling
point at 0 and the freezing point at 100, but this is reversed in 1743.
This scale
will become the (official) "Celsius scale" in 1948.

Celsius publishes "Dissertatio de Nova Methodo Distantiam Solis a Terra
Determinandi" (1730; "A Dissertation on a New Method of Determining the
Distance of the Sun from the Earth") and "De Observationibus pro Figura
Telluris Determinanda in Gallia Habitis, Disquisitio" (1738; "Disquisition on
Observations Made in France for Determining the Shape of the Earth").
Uppsala, Sweden (presumably)  
258 YBN
[1742 AD]
1985) Benjamin Franklin (CE 1706-1790) invents the "Franklin stove", a wood
burning stove made of iron that fits in a fireplace, designed to give greater
warmth, more comfort, and cleaner heating at a lower fuel cost.{7 us hist}
Designed
to be used in an already existing fireplace, the Franklin stove does not
resemble what are now called Franklin stoves.{7 us hist}

Philadelphia, Pennsylvania (presumably)  
258 YBN
[1742 AD]
2011) Albrecht von Haller (HolR) (CE 1708-1777), Swiss physiologist, publishes
"Enumeratio methodica stirpium Helveticarum", (1742) a large book on flora of
Switzerland.
Basel, Switzerland (presumably)  
258 YBN
[1742 AD]
2068)
Geneva?, Switzerland (presumably)  
257 YBN
[1743 AD]
1976) Franklin is the fifteenth child of seventeen born to a poor candlemaker.
(Franklin is
the first person in America to contribute to modern science).
Franklin has only 2 years
of formal schooling.
At 12 Franklin is apprenticed to his brother James, a printer.
Two other
people to try this kite experiment are killed (presumably by lightning?).
{With a Leyden jar
a spark of light and crackling sound could be produced by putting a metal rod
near the charged jar}.
Benjamin Franklin builds a repulsive electroscope using the
electrical repulsion of two linen threads to measure the strength of static
electricity. (chronology - sometime between 1731 and 1753)
Franklin is publicly a
deist, writing in his autobiography started in 1771: "Some books against Deism
fell into my hands; they were said to be the substance of the sermons which had
been preached at Boyle's Lectures. It happened that they wrought an effect on
me quite contrary to what was intended by them. For the arguments of the
Deists, which were quoted to be refuted, appeared to be much stronger than the
refutations; in short, I soon became a thorough Deist.".
Franklin invents a glass
armonica based on the concept of the sound a drinking glass makes when rubbed.
A person plays a melody by touching the rim of spinning glass bowls (each)
mounted on rotating spindles.
(In evaluating Mesmer's method of passing hands over
people, Franklin rejects that Mesmer's method is legitimate, but describes
psychosomatic cures, that cures might be affected by suggestion ).
Franklin
rejects Newton's corpuscular theory of light in favor of the theory of light as
a wave propagated through an all encompassing aether.

Through the group he founded in 1727 to debate questions of morals, politics,
and natural philosophy, the "Junto", or Leather Apron Club, Franklin proposed a
paid city watch, or police force (for Philadelphia).
Franklin is a signer of
both the Declaration of Independence and the Constitution of the United
States.
In 1900 Franklin is chosen as one of the charter members of the Hall of Fame
for Great Americans.
Philadelphia, Pennsylviania, (English Colonies) USA  
257 YBN
[1743 AD]
2023) Johann Georg Gmelin (GumAliN) (CE 1709-1755) German explorer makes a
journey of scientific exploration through Siberia (1733-1743).

Gmelin starts to study medicine at age 14.
Gmelin is the first person to measure
that the level of the Astrakhan in Russia near the Caspian Sea is below that of
the Mediterranean Sea (sea level).
In Eastern Siberia Gmelin identifies ground that is
constantly frozen all summer long, this is called permafrost.

Gmelin's major works are "Flora Sibirica" (4 vols., 1749-1750) and "Reisen
durch Sibirien" (4 vols., 1753).

Astrakhan, Russia  
257 YBN
[1743 AD]
2030) Mikhail Vasilievich Lomonosov (lumunOSuF) (CE 1711-1765) Russian chemist
and writer, publishes "276 zametok po fizike i korpuskulyarnoy filosofi" ("276
Notes on Corpuscular Philosophy and Physics") which sets forth the dominant
ideas of his scientific work.

Saint Petersburg, Russia  
257 YBN
[1743 AD]
2036) Clairaut accompanies Maupertuis on an expedition to Lapland to determine
the length of 1° of a meridian within the Arctic circle to determine that the
shape of the earth is an oblate spheroid. After his return Clairaut publishes
his treatise "Théorie de la figure de la terre" (Theory of the Shape of the
Earth, 1743), which contains "Clairaut's theorem".

Clairaut shows how the shape of the earth can be calculated by measuring the
force of gravity at different locations through the timing of pendulum swings.
Paris, France (presumably)  
257 YBN
[1743 AD]
2037)
Paris, France (presumably)  
257 YBN
[1743 AD]
2057) D'Alembert receives a pension from Louis XV even though D'Alembert's
articles for Diderot were of an "anti-establishment" nature.
D'Alembert refuses
invitations to Berlin from Frederick II and to St Petersburg by Catherine II.
D'Alem
bert bitterly argues with Clauraut about who is the first to work on (the orbit
of) Halley's comet.
Paris, France (presumably)  
256 YBN
[1744 AD]
1924)
London, England  
256 YBN
[1744 AD]
1967) Fermat had explained Snell's law of refraction, which describes the
movement of a ray of light at the boundary of two media of different densities,
based on the idea that a ray of light takes the least time possible in moving
from the first medium to the second. Fermat's explanation implies that light
moves more slowly in a denser medium, to which Maupertuis objects and wants to
explain Snell's law without this principle. (As an aside, very generally
speaking, and there are exceptions, the amount a beam of photons changes
direction in a medium is more for a denser medium which is consistent with the
theory that particles of light as masses encounter more collisions and/or orbit
more other particles in a denser material). Maupertuis views this principle of
least action as the fundamental principle of mechanics, and expects that all
other mechanical laws should be derivable from it. As a believer in a deity,
Maupertuis attempts to use this principle to prove the existence of a God.

A similar principle had previously been formulated by Leonhard Euler as a
result of his mathematical work on the calculus of variations, whereas
Maupertuis had been led to formulate his version of the principle through his
work in optics.

The German mathematician Samuel Koenig accuses Maupertuis of having plagiarized
Gottfried Wilhelm Leibniz's work in this principle. In the ensuing controversy,
Leonhard Euler supports Maupertuis, but Voltaire, (once a supporter of
Maupertuis) satirizes the "earth flattener" so mercilessly that Maupertuis
leaves Berlin in 1753.
Berlin, Germany (presumably)  
256 YBN
[1744 AD]
2058)
Paris, France (presumably)  
256 YBN
[1744 AD]
2059)
Paris, France (presumably)  
256 YBN
[1744 AD]
2060)
Paris, France (presumably)  
256 YBN
[1744 AD]
2121)
  
256 YBN
[1744 AD]
2962) Georg Mathias Bose (CE 1710-1761), German physicist, publishes "Die
Electricität nach ihrer Entdeckung und Fortgang, mit poetischer Feder
entworffen" where describe in poetic form Bose's experiments with electricity,
including the electrification of an isolated human body.

(University of Wittenberg)Wittenberg, Germany  
256 YBN
[1744 AD]
2964) Joseph Priestley comments that the best rubber for the globe, as well as
the tube, is long after this, still thought, by all electricians, to be the
human hand, dry and free from moisture.

In 1746 Winckler transmits electric signal a short distance without wires.
At the
University of Leipzig, in 1739 Winckler is appointed Professor of Philosophy,
in 1741 as Professor of Classical Languages, and then in 1750 as Professor of
Physics..

Johann Heinrich Winckler is Bach's colleague at the St. Thomas School and
writes the traditional text of the cantata "Froher Tag, verlangte Stunden" (BWV
Anh 18) (the music for this cantata has been lost). Winckler contributes and is
associated with Bach: Both Johann Christoph Gottsched and Johann Heinrich
Winckler, prominent exponents of the university, write texts for Bach.
(University of Leipzig) Leipzig, Germany  
255 YBN
[11/04/1745 AD]
1972) Von Kleist studied at the University of Leyden in the 1720's and while a
student there may have encountered the demonstrations in experimental physics
of Professor Gravesande who was involved in electricity at Leyden. Von Kleist
apparently acquired his interest in science while at the University of Leyden.


One source states that von Kleist discovers that electricity can be stored in a
glass bottle if both the inner and outer surfaces of the bottle are covered
with a metallic foil, and a metallic rod is placed in the middle of the
bottle.Von Kleist who studied law in the Dutch university of Leiden, informs
his friends of his discovery. A Dutch physician, Pieter van Musschenbroek, then
publishes the first scientific paper regarding the Kleist bottle, which is then
given the name "Leyden jar". (Just as a comment, there are certainly some times
when an idea is so obvious that two or more people will independently find it,
even around the same time, but I think the more unique, complex or unusual the
discovery or invention, the higher the probability of an individual discoverer
or inventor. In particular when an invention has two or more claimed
discoverers in the same location around the same time, as is the case for the
Leyden jar. In some cases, elements of the invention are in place with one or
more missing pieces, in which case, the chances of duplication are higher.)
Pomerania?, Prussia (coast of Baltic Sea between Germany and Poland)  
255 YBN
[1745 AD]
1244)
England  
255 YBN
[1745 AD]
1906) De La Mettrie is a student of Hermann Boerhaave.
Paris, France (presumably)  
255 YBN
[1745 AD]
1989) Émilie du Châtelet (so TlA) (full name: Gabrielle Émikle le Tonnelier
de Breteuil, marquise du Châtelet) (CE 1706-1749) translates Newton's
"Principia" from Latin into French at the request of Voltaire.

Chatelet publishes a book titled "Institutions de Physique" ("Lessons in
Physics", 1740) in 1740 which is attempts to integrate Cartesian, Newtonian,
and Leibnizian ideas. On the philosophic side the themes she discusses are free
will, God's power and role, and the nature of space, matter, and force.
Châtelet's
"Dissertation sur la nature et la propagation du feu" ("Dissertation on the
nature and the propagation of fire", 1744)
Châtelet is one of the few women
interested in science at this time.
Châtelet is friends with Voltaire and
Maupertuis.
Voltaire and Chatelet work together on scientific and philosophical questions
in addition to having a (sexual) relationship. When Voltaire leaves Chatelet,
she begins a relationship with poet Saint-Lambert, and dies in pregnancy. In
her "Discours sur le bonheur" Chatelet places equal value on love and
intellectual endeavors.

Cirey, France (presumably)  
255 YBN
[1745 AD]
2695) It seems almost that there are two main competing sides throughout the
history of modern science, and Boscovich seems to be supporting the
conservative side which tends to reject atomism, also as applied to particles
of light.

(Although) Boscovich is one of the first scientists of continental Europe to
accept Isaac Newton's gravitational theory.
Boscovich publishes nearly 70 papers on
optics, astronomy, gravitation, meteorology, and trigonometry.

(See image) This is Boscovich's force-distance curve from his "De viribus
vivis" dissertation of 1745. Letters identify 'limit points' where attraction
turns into repulsion and vice versa, inflection points, maxima and minima and
so on. This dissertation presents many of the concepts in Boscovich's later
"Philosophiae naturalis theoria1".
Rome  
255 YBN
[1745 AD]
2965)
(University of Erfurt) Erfurt, Germany  
255 YBN
[1745 AD]
2966)
(University of Erfurt) Erfurt, Germany  
254 YBN
[04/20/1746 AD]
1930) Musschenbroek comes from a family of instrument makers, who at the time
of his birth are making telescopes, microscopes and air pumps.
In 1715 Musschenbroek
earns a medical degree from the University of Leiden and a Ph.D. in 1719.
Luigi
Galvani will use a Leyden jar to move muscles on frog legs in 1780.
Leiden, Netherlands  
254 YBN
[1746 AD]
1995) Leonhard Euler (OElR) (CE 1707-1783), Swiss mathematician, publishes
"Nova theoria lucis et colorum" (A new theory of light and colors) in which
Euler rejects Newton's corpuscular theory of light in favor of the view of
light as a wave propagated through an aetherial medium similar to sound, and
supports the theory that color of light is based on wave-length ("particle
spacing").

In 1699, Nicolas Malebranche (CE 1638-1715) was the first to make public the
theory that color is based on frequency of light.
Berlin, Germany  
254 YBN
[1746 AD]
2003)
Uppsala, Sweden (presumably)  
254 YBN
[1746 AD]
2022)
Berlin, Germany (presumably)  
254 YBN
[1746 AD]
2953) In 1746 the abbé Jean-Antoine Nollet, a physicist who popularizes
science in France, discharges a Leyden jar in front of King Louis XV by sending
current through a chain of 180 Royal Guards. In another demonstration, Nollet
uses wire made of iron to connect a row of Carthusian monks more than a
kilometre long; when a Leyden jar is discharged, the white-robed monks
reportedly leap simultaneously into the air.

In addition to many memoirs Nollet writes "Legons de physique expdrimentale"
(1743), "Essai sur l'electricite des corps" (1747), "Recherches sur les causes
particulieres des phenomenes eiectriques" (1749 and 1754), "Recueil de lettres
sur l'electricite" (1753), "L'Art de faire les chapeaux" (1764) and "L'Art des
experiences" (1770).

It would seem that if there were two particles combining in a spark that some
atom or other form of matter might be formed. Perhaps all the matter is lost to
photons. If the atmosphere so clearly felt around objects electrified with
static electricity is made of particles, what kind of particles? How do they
differ from an electric field from moving current such as around a permanent
magnet or wire? What happens when these particles merge? Is all matter released
as particles of light, or does some matter remain after?

EX: Model particle fields and how they collapse under gravity, forms a line,
releases particles?
Paris, France (presumably)  
254 YBN
[1746 AD]
2968) In 1747, Watson transmits an electric spark from his device through a
wire strung across the River Thames at Westminster Bridge.
London, England  
254 YBN
[1746 AD]
2969) William Watson (CE 1715â€"1787), English physician and scientist,
relates that "Upon shewing some Experiments to Dr. Bevis, to prove my Assertion
that the Stroke was, caeteris paribus, (other things being equal) as the Points
of Contact of Nonelectrics to the Glass, that ingenious Gentleman has very
clearly demonstrated it likewise by the following Experiment: He wrapped up two
large round-bellied Phials in very thin Lead so close as to touch the Glasses
every-where, except their Necks. These were filled with Water, and cork'd, with
a Staple of small Wire running through each Cork into the Water. A Piece of
strong Wire about 5 Inches long, with an Eye at each End, was provided, and at
each End of this hung one of the Phial of Water by the small Staple running
through the Cork. A small Wire Loop then was fasten'd into the Lead at the
Bottom of each Phial, and into these Loops was inserted a Piece of strong Wire
like the former. If then these Phials were hung across the Gun-barrel and
electrified, and a Person standing upon the Floor touched the bottom Wire with
one Hand, and the Gun barrel with the other, he received a most violent Shock
through both his Arms, and across his Breast."
London, England  
254 YBN
[1746 AD]
2977) In this year Jean-Antoine Nollet (CE 1700-1770) publishes "Recherches sur
les Causes Particulieres des Phenomenes Electriques, l'Abbe Nollet", (1753) a
detailed treatise on electricity, and "Lettres sur l Electricite, l'Abbe
Nollet" (1753) which counters Franklin's one-fluid theory of electricity.

Paris, France (presumably)  
253 YBN
[07/11/1747 AD]
1981) Franklin writes "The impossibility of electrising one's self though
standing on wax by rubbing the tube, and drawing the fire from it; and the
manner of doing it, by passing the tube near a person or thing standing on the
floor, &c., had also occurred to us some months before Mr Watson's ingenious
Sequel came to hand, and these were some of the new things I intended to have
communicated to you But now I need only mention some particulars not hinted in
that piece with our reasonings thereupon; though perhaps the latter might well
enough be spared.
1 A person standing on wax and rubbing the tube and another
person on wax drawing the fire they will both of them provided they do not
stand so as to touch one another appear to be electrised to a person standing
on the floor; that is he will perceive a spark on approaching each of them with
his knuckle.
2 But, if the persons on wax touch one another during the
exciting of the tube, neither of them will appear to be electrised.
3 If they
touch one another after exciting the tube and drawing the fire as aforesaid,
there will be a stronger spark between them than was between either of them and
the person on the floor.
4 After such strong spark neither of them discover
any electricity.

These appearances we attempt to account for thus: We suppose, as aforesaid,
that electrical fire is a common element, of which every one of the three
persons above mentioned has his equal share, before any operation is begun with
the tube. A, who stands on wax and rubs the tube, collects the electrical fire
from himself into the glass; and his communication with the common stock being
cut off by the wax, his body is not again immediately supply'd. B, who stands
on wax likewise passing his knuckle along near the tube, receives the fire
which was collected by the glass from A; and his communication with the common
stock being likewise cut off, he retains the additional quantity received. To
C, standing on the floor, both appear to be electrised: for he having only the
middle quantity of electrical fire, receives a spark upon approaching B, who
has an over quantity; but gives one to A, who has an under quantity. If A and B
approach to touch each other the spark is stronger, because the difference
between them is greater: After such touch there is no spark between either of
them and C, because the electrical fire in all is reduced to the original
equality. If they touch while electrising, the equality is never destroy'd, the
fire only circulating. Hence have arisen some new terms among us: we say, B,
and bodies like circumstanced is electrised positively; A, negatively. Or
rather, B is electrised plus; A, minus. And we daily in our experiments
electrise bodies plus or minus, as we think proper. To electrise plus or minus
no more needs to be known than this, that the parts of the tube or sphere that
are rubbed, do, in the instant of the friction, attract the electrical fire,
and therefore take it from the thing rubbing: the same parts immediately, as
the friction upon them ceases, are disposed to give the fire they have
received, to any body that has less. Thus you may circulate it, as Mr Watson
has shewn; you may also accumulate or subtract it upon, or from any body, as
you connect that body with the rubber, or with the receiver, the communication
with the common stock being cut off. We think that ingenious gentleman was
deceived when he imagined in his Sequel that the electrical fire came down the
wire from the deling to the gun barrel, thence to the sphere, and so electrised
the machine and the man turning the wheel, &c., We suppose it was driven off,
and not brought on through that wire; and that the machine and man, &c., were
electrised minus, i.e. had less electrical fire in them than things in
common.".


This book will go through five English editions, three in French, and one each
in Italian and German in the 1700s.
Asimov says Franklin views the earth and sky as
being a large Leyden jar.
Possibly electricity is caused by gravity, combined with
physical restrictions caused by atoms occupying space (like the Pauli exclusion
principle, how only one photon can occupy the quantity of space a photon can
occupy), in other words, electric attraction and repulsion may be a collective
effect of the gravity of many particles in addition to the physical structure
of atomic lattices. Possibly electrons are actually photons or combinations of
photons held together by gravity, since when an electron and positron collide
and are separated into source matter in the form of finite short duration
quantities of photons (check and more specific, how many photons?). We should
not rule out new ideas and interpretations, in particular, for phenomena we
cannot directly observe.

On August 14th, 1747, Franklin sends Peter Collinson a third letter stating
"SIR, I have lately written two long Letters to you on the Subject of
Electricity; one by the Governor's Vessel, the other per Mesnard. On some
further Experiments since, I have observ'd a Phenomenon or two, that I cannot
at present account for on the Principle laid down in those Letters, and am
therefore become a little diffident of my Hypothesis, and asham'd that I have
express'd myself in so positive a manner. In going on with these Experiments,
how many pretty Systems do we build which we soon find ourselves oblig'd to
destroy! If there is no other Use discover'd of Electricity this however is
something considerable, that it may help to make a vain man humble. I must now
request that you would not Expose those Letters; or if you communicate them to
any Friends you would at least conceal my Name. I have not Time to add but that
I am Sir,
Your obliged and most hum Serv
B FRANKLIN"
Philadelphia, PA (English colonies) USA (letter to London, England)  
253 YBN
[09/01/1747 AD]
2970) Franklin writes "The non electric contain'd in the bottle differs when
electrised from a non electric electrised out of the bottle, in this: that the
electrical fire of the latter is accumulated on its surface, and forms an
electrical atmosphere round it of considerable extent; but the electrical fire
is crowded into the substance of the former, the glass confining it. (Later
Franklin observes that the "fire" is in the glass, not the non-electric)
At the same time
that the wire and the top of the bottle, &c. is electrised positively or plus,
the botttom of the bottle is electrised negatively or minus, in exact
proportion; i.e., whatever quantity of electrical fire is thrown in at the top
(inside), an equal quantity goes out of the bottom (outside). To understand
this, suppose the common quantity of electricity in each part of the bottle,
before the operation begins, is equal to 20; and at every stroke of the tube,
suppose a quantity equal to 1 is thrown in; then, after the first stroke, the
quantity contained in the wire and upper part of the bottle will be 21, in the
bottom 19; after the second, the upper part will have 22, the lower 18, and so
on, till, after 20 strokes, the upper part will have a quantity of electrical
fire equal to 40, the lower part none; and then the operation ends; for no more
can be thrown into the upper part, when no more can be driven out of the lower
part. If you attempt to throw more in, it is spued back through the wire, or
flies out in loud cracks through the sides of the bottle.".
Philadelphia, PA, (English Colonies) USA(London, England)  
253 YBN
[1747 AD]
1192) The École Nationale des Ponts et Chaussées (ENPC) ("National school of
Bridges and Roads") is formed in Paris.

Paris, France  
253 YBN
[1747 AD]
1907) De La Mettrie is a student of Hermann Boerhaave.
?, Netherlands  
253 YBN
[1747 AD]
1982)
Philadelphia, Pennsylvania (presumably)  
253 YBN
[1747 AD]
2012)
Göttingen, Germany  
253 YBN
[1747 AD]
2020) Today sugar is made from beets in many countries all over the earth.
Berlin, Germany (presumably)  
253 YBN
[1747 AD]
2031) Mikhail Vasilievich Lomonosov (lumunOSuF) (CE 1711-1765) Russian chemist
and writer, publishes in Latin, "Meditationes de Caloris et Frigoris Causa"
(1747; "Cause of Heat and Cold") in which Lomonosov expresses anti-phlogistic
views supporting the theory of heat as a form of motion as Rumford will do..

Saint Petersburg, Russia  
253 YBN
[1747 AD]
2055) Lind observes on a ten-week cruise (in 1746) that 80 of the 350 semen get
scurvy.
Lind is viewed as the father of naval hygiene.
England  
253 YBN
[1747 AD]
2056)
England (presumably)  
253 YBN
[1747 AD]
2963)
(University of Wittenberg)Wittenberg, Germany  
253 YBN
[1747 AD]
2986)
Paris, France (presumably)  
253 YBN
[1747 AD]
3452) George William Richman (CE 1711-1753) describes the effect of evaporating
fluids producing cold.

This phenomenon is also known as "adiabatic temperature change". Adiabatic is
defined as: occurring without gain or loss of heat (opposite of diabatic, which
is defined as occurring with an exchange of heat). (This must refer to no
external heat being added in the case of gas expansion and compression, since
there is a gain or loss of heat in the expansion or compression of gases.)
(Academy of Petersburg) Petersburg, Russia  
253 YBN
[1747 AD]
4483)
Paris, France  
252 YBN
[01/01/1748 AD]
1960) During the 1720s Bouguer makes some of the earliest measurements in
astronomical photometry (the measurement of light intensity), comparing the
apparent brightness of celestial objects to that of a standard candle flame.
In 1730
Bouguer is made professor of hydrography (geographer of waters of earth) at Le
Havre (in France) succeeding his father.
Bouguer devotes much of his life to the study
of nautical problems such as naval maneuvers, navigation and ship design.
??, France (presumably)  
252 YBN
[02/14/1748 AD]
1932) In 1748 Bradley is awarded the Copley medal for his finding of
"nutation".
Kew, England  
252 YBN
[1748 AD]
2032) Mikhail Vasilievich Lomonosov (lumunOSuF) (CE 1711-1765) Russian chemist
and writer, publishes in Latin, "Tentamen Theoriae de vi Aëris Elastica"
(1748; "Elastic Force of Air").

Saint Petersburg, Russia  
252 YBN
[1748 AD]
2045) In 1768, Needham is the first Roman Catholic clergyman to become a fellow
of the Royal Society of London.
London, England (presumably)  
252 YBN
[1748 AD]
2954)
Paris, France (presumably)  
252 YBN
[1748 AD]
2955) Nollet designs and builds globes.
Paris, France (presumably)  
252 YBN
[1748 AD]
4537)
Berlin, Germany  
251 YBN
[04/29/1749 AD]
2971) In this letter Franklin describes how they ignite alcohol from one side
to the other side of the Delaware river, using only the water as a conductor,
which amazes many people. A wire is connected to a spoon in alcohol and run
over the river and wrapped around the outside of the Leyden jar, the hook of
the Leyden jar is connected to a 3 foot metal rod driving around the margin of
the water, when the hook is charged, the charge is sent over the river through
the water to a second 3 foot metal rod driven into the margin of the water on
the other side which has a thick wire bent near the alcohol, and the spark
completes the circuit igniting the alcohol.
Philadelphia, Pennsylviania, (English Colonies) USA (and London, England)  
251 YBN
[1749 AD]
1877)
London, England (presumably)  
251 YBN
[1749 AD]
1961)
??, France (presumably)  
251 YBN
[1749 AD]
1997)
Uppsala, Sweden (presumably)  
251 YBN
[1749 AD]
2024)
Saint Petersburg, Russia  
251 YBN
[1749 AD]
2046) Interesting events in the life of Denis Didderot:

The Encyclopedia Britannica states that Diderot "progressed relatively slowly
from Roman Catholicism to deism and then to atheism".

In the "Supplément au voyage de Bougainville Diderot", by discussing the mores
people on islands in the South Pacific, Diderot emphasizes his vision of a free
society based on tolerance and develops his views on sexual freedom.
Paris, France (presumably)  
250 YBN
[01/01/1750 AD]
2040)
Cape of Good Hope, Africa  
250 YBN
[1750 AD]
1212) William Cullen (April 15, 1710 - February 5, 1790), a Scottish physician
and chemist, tries bleeding as a cure for "insanity".

Scotland, UK  
250 YBN
[1750 AD]
1245)
Philadelphia, Pennsylvania  
250 YBN
[1750 AD]
1921)
Paris, France (presumably)  
250 YBN
[1750 AD]
1969) Pierre de Maupertuis (moPARTUE) (CE 1698-1759) publishes "Essai de
cosmologie" (1750), which puts forward a mechanistic view of the universe.

Berlin, Germany (presumably)  
250 YBN
[1750 AD]
2025) Wright has a speech impediment.
Wright's father burns his astronomy books thinking
them frivolous.
This idea of the Milky Way as an flat layer of stars will be taken up and
elaborated by Immanuel Kant in his "Universal Natural History and Theory of
Heaven".
  
250 YBN
[1750 AD]
2063)
London, England  
250 YBN
[1750 AD]
2092) The "bluestockings", form started by Elizabeth Vesey, as a group of women
who attempt to replace social evenings spent playing cards with something more
intellectual by having "conversations" to which they invite men of letters and
members of the aristocracy with literary interests. Terribly and sadly, and as
an indication of the popularity of forces against science and women's rights,
the word "bluestocking", will come to be applied derisively to a woman who has
literary or learned interests.

London, England  
249 YBN
[1751 AD]
1211) Richard Mead (August 11, 1673 - February 16, 1754), an English physician,
prints a medical text on "insanity" in which he advocates assault and torture
against those believed to be insane, writing that an insane person should be
"tied down and even beat, to prevent his doing mischief to himself or others."

England  
249 YBN
[1751 AD]
1949) Voltaire (CE 1694-1778) publishes the "Micromégas" (1752), which
emphasizes the littleness of man compared to the scale of the universe.
"Micromégas", is written in the style of Jonathan Swift's "Gulliver's
Travels", in which an eight-league-tall traveler from Sirius comes to inspect
the earth. The visitor from Sirius is divided between horror at the pettiness
and cruelness of humanity and admiration for modern science.

Paris, France (published)  
249 YBN
[1751 AD]
1953) Voltaire (CE 1694-1778) publishes "Siècle de Louis XIV" (1751), a
History of King of France Louis XIV.

Berlin, Germany  
249 YBN
[1751 AD]
1968)
Berlin, Germany (presumably)  
249 YBN
[1751 AD]
1974) Charles Marie de La Condamine (loKoNDuMEN) (CE 1701-1774), French
geographer publishes "Journal du voyage fait par ordre du roi a l'équateur"
(1751; "Journal of a Voyage to the Equator Made by Order of the King") in
addition to a scientific account of his ten year exploration of South America.

Paris, France (presumably)  
249 YBN
[1751 AD]
1984) Benjamin Franklin (CE 1706-1790), just before his death in 1790, signs a
memorial requesting that the Congress abolish slavery in the United States.
This memorandum provokes some congressmen into angry defenses of slavery, which
Franklin expertly mocks in a newspaper piece published a month before he dies.

London, England  
249 YBN
[1751 AD]
2002)
Uppsala, Sweden (presumably)  
249 YBN
[1751 AD]
2047) In 1745 a book seller, André Le Breton approached Diderot wanting a
French translation of Ephraim Chambers' English "Cyclopaedia" (1728 ), after
two other translators had withdrawn from the project. Diderot undertook the
task with the mathematician Jean Le Rond d'Alembert as coeditor, but soon
changed the nature of the publication into a bigger and different project: to
commission the best scholars in France to write articles on every facet of the
new learning of Newton and his followers.

Some scholar suggest that the encyclopedia may have inspired the French
Revolution in 1789 five years after Diderot's death.
Asimov states that if true
perhaps the French government had been right to fear the industrious scribbler.
Paris, France  
249 YBN
[1751 AD]
2070)
  
248 YBN
[01/03/1752 AD]
2009) In a letter sent from Geneva on February 2, 1753 to the astronomer royal,
James Bradley, Melvill suggests that light rays of different colors traveling
at different velocities might account for their differing refraction through a
prism, and that this can be confirmed if the satellites of Jupiter are seen to
change slightly in color as they occult and emerge. This letter was read before
the Royal Society on March 8 and the telescope maker James Short is instructed
to make the necessary observations. Short reports that no such effect could be
seen. In a second letter to Bradley, dated June 2, Melvill (wrongly) suggests
that the rate of light travel concerned in aberration might be affected by the
humors of the eye itself. Melvill dies in Geneva in December 1753 at the age of
twenty-seven. (The speed of photons appears to be very uniform, although
possibly not always the same as the Pound-Rebka experiment may be evidence of.
The various colors photons produce is most likely because of the interval of
space between the photons, the photon interval, or so-called wavelength of a
beam of light.)
Edinburgh, Scotland  
248 YBN
[02/20/1752 AD]
2976)
London, England  
248 YBN
[1752 AD]
1922)
Paris, France (presumably)  
248 YBN
[1752 AD]
1983)
Philadelphia, Pennsylvania (presumably)  
248 YBN
[1752 AD]
2054) Jean Étienne Guettard (GeToRD) (CE 1715-1786), French geologist , upsets
the neptunism theories of Abraham Werner and his followers by identifying the
Auvergne mountains of central France to be of volcanic origin (are they?).

Werner's theory states that all volcanic activity is recent, so no volcanoes as
ancient as the Auvergne ones should exist. Guettard publishes this findings in
his memoir, "On Certain Mountains in France which once have been Volcanoes"
(1752).

In addition Guettard is the first to identify several fossil species from the
Paris area.

France  
248 YBN
[1752 AD]
2064)
London, England (presumably)  
248 YBN
[1752 AD]
2987)
(Petersberg Academy) St Petersberg, Russia  
247 YBN
[02/17/1753 AD]
2658)
Scotland, Great Britain (presumably)  
247 YBN
[07/26/1753 AD]
2985)
St Petersberg, Russia  
247 YBN
[12/??/1753 AD]
2972)
London, England  
247 YBN
[1753 AD]
1927) A solar eclipse in 1706 interests Delisle in astronomy.
Delisle works at the Paris
Observatory.
Peter I (The Great) invites Delisle to build an astronomy in Russia.
Delisle intending
to be in Russia only 4 years, but stays for 22 and trains the first generation
of Russian astronomers.
Delisle returns to Paris in 1747, and is appointed geographic
astronomer to the naval department. (In Paris) Delisle installs an observatory
in the Hôtel Cluny.
Paris, France  
247 YBN
[1753 AD]
1964)
London, England (presumably)  
247 YBN
[1753 AD]
1994)
Berlin, Germany  
247 YBN
[1753 AD]
1998)
Uppsala, Sweden (presumably)  
247 YBN
[1753 AD]
2013)
Göttingen, Germany (presumably)  
247 YBN
[1753 AD]
2957)
London, England  
246 YBN
[1754 AD]
2021)
Berlin, Germany (presumably)  
246 YBN
[1754 AD]
2050) Denis Diderot (DEDrO) (CE 1713-1784), French writer , publishes "Pensées
sur l'interprétation de la nature" ("Thoughts on the Interpretation of
Nature"), a short treatise on the new experimental methods in science.

Paris, France  
246 YBN
[1754 AD]
2120)
Geneva, Switzerland  
245 YBN
[01/25/1755 AD]
1370) Kant Russian State University is technically the oldest university in
Russia, when Russia took possession of Kaliningrad (Lithuanian:
Karaliaučius; German Königsberg, Polish: Królewiec) after World War 2,
which includes the German East-Prussian Albertina University of Königsberg
founded in 1544.
Moscow, Russia  
245 YBN
[05/01/1755 AD]
3249)
(University of Edinburgh) Edinburgh, Scotland  
245 YBN
[11/??/1755 AD]
1528)
Corsica  
245 YBN
[1755 AD]
1214) John Monro (1715-1791) superintendant of Bethlehem Asylum, records giving
one prisoner 61 vomit inducing emetics (a medicine or object that induces
vomiting) in 6 months.

London, England  
245 YBN
[1755 AD]
1990)
Berlin, Germany (presumably)  
245 YBN
[1755 AD]
2026) Mikhail Vasilievich Lomonosov (lumunOSuF) (CE 1711-1765) Russian chemist
and writer, writes a book on Russian grammer ("Rossiyskaya grammatika") that
reforms the language.
Lomonosov is the first to record the freezing of mercury (40 degree
below zero (celsius?)) in a very cold Russian winter.
Lomonosov is the first to prepare
an accurate map of Russia.

Lomonosov is the son of a fisherman, and moves to Moscow at age 19.
In 1736
Lomonosov is one of sixteen students selected to continue their studies at the
newly established secular university at the St. Petersburg Academy of
Sciences.
The Academy sends Lomonosov to study in Germany, from 1736 to 1741, first at
the University of Marburg, where he learns the basic sciences, and later at the
famous mining academy at Freiburg.
In this time German people monopolize science in
Russia and look down on the native Russian people (such as Lomonosov), until
the 1900s.
Lomonosov writes poetry about science.
Lomonsov writes a hymn that lampoons the
theologians who stand in the way of scientific progress.
On one occasion, Lomonosov is
sent to jail as a result of complaints by foreign colleagues regarding his
abusive language at scientific sessions of the Academy.
Lomonosov is friends with the
celebrated German mathematician Leonhard Euler.
A friend of Lomonosov is killed when
they try to repeat Franklin's kite experiment.
Lomonosov supports atomist views.

Saint Petersburg, Russia  
245 YBN
[1755 AD]
2072) In 1781 Kant will publishes his popular (philosophical) work "Critique of
Pure Reason".
Kant is funded by Frederick II of Prussia.
Königsberg, Germany  
245 YBN
[1755 AD]
2089) Black is professor of chemistry at Glasgow (1756-66) and from 1766 at
Edinburgh.
Edinburgh, Scotland  
245 YBN
[1755 AD]
2979)
Peking, China (sent to St. Petersberg Academy)  
244 YBN
[1756 AD]
1215) Pennsylvania Hospital, the first hospital in what is now the United
States, is opened to care for the sick-poor and mentally ill of Philadelphia.
This is also the first psychiatric hospital in what will be the USA.

People are kept in cells watched by other people with whips, are beat,
regularly chained, and put in "madd-shirts" (straight jackets).

Care of the mentally ill will be removed to West Philadelphia in 1841 with the
construction of the Pennsylvania Hospital for the Insane, later known as The
Institute of the Pennsylvania Hospital.

Pennsylviania, USA  
244 YBN
[1756 AD]
1954) Voltaire (CE 1694-1778) publishes "Essai sur l'histoire générale et sur
les mœurs et l'esprit des nations" (7 vol., 1756; tr. 1759), the first attempt
at writing a history of the world as a whole. Voltaire lays as much emphasis on
culture and commerce as on politics and war, and avoids national (prejudice).

Geneva, Switzerland  
244 YBN
[1756 AD]
2016)
Gottingen, Germany  
244 YBN
[1756 AD]
2033) Mikhail Vasilievich Lomonosov (lumunOSuF) (CE 1711-1765) Russian chemist
and writer, publishes in Latin, "Theoria Electricitatis" (1756; "Theory of
Electricity").

Saint Petersburg, Russia  
244 YBN
[1756 AD]
2034) Mikhail Vasilievich Lomonosov (lumunOSuF) (CE 1711-1765) Russian chemist
and writer, publishes "Slovo o proiskhozhdeni sveta" (1756; "Origin of Light
and Colours").

Lomonosov supports a wave theory of light as Young will do (state nature of
wave theory, aether based, sine wave, amplitude, like sound?).

Saint Petersburg, Russia  
244 YBN
[1756 AD]
2061)
Paris, France (presumably)  
244 YBN
[1756 AD]
2066)
London, England (presumably)  
244 YBN
[1756 AD]
2090)
Edinburgh, Scotland  
244 YBN
[1756 AD]
2252)
Bologna, Italy  
243 YBN
[1757 AD]
2039) Lacaille will use Clairaut's calculations of perturbations to improve his
tables of Sun positions published in 1758.
Paris, France   
243 YBN
[1757 AD]
2041) Lacaille gives away copies of his chart to any people who ask even though
poor.
Paris, France (presumably)  
243 YBN
[1757 AD]
2697)
Rome?, Italy  
243 YBN
[1757 AD]
2981)
(Royal Swedish Academy of Sciences) Stockholm, Sweden  
243 YBN
[1757 AD]
3250)
(University of Erlangen) Erlangen, Germany  
242 YBN
[10/21/1758 AD]
4538)
Bath, England  
242 YBN
[11/14/1758 AD]
2038)
Paris, France  
242 YBN
[1758 AD]
1203)
England  
242 YBN
[1758 AD]
1216) William Battie writes "A Treatise on Madness" which describes "cures" for
"insanity".
But "insanity" has never been clearly defined. I think insanity can be reduced
to having inaccurate views, or doing unusual behavior. But many people that
simply cannot get a job, or feed themselves are labeled insane and locked in
psychiatric hospitals which serve as a primative social program of free room
and food.
Battie owns psychiatric hospitals, and a truth that is rarely if ever
mentioned, is that by creating more nonexistent and or trivial diseases, more
people may be tricked into believing that they have a disease and need to buy
drugs and pay a doctor for treatment, which generates more money for those who
own the psychiatric hospitals and get money from the modern snake-oil industry
of psychology. In addition, the widely believed myth and fear of insanity
allows an illegal method for permanently jailing, for example, political
enemies of those in power, without the victim being charged with violating a
law, without receiving a trial, tortured, drugged, experimented on, operated
on, and jailed without finite sentence. Interestingly psychology is the only
remaining health-based fraud (with the passing of phrenology), other frauds
such as astrology, psychics, tarot, and religion are not health based and
generate money strictly from the fraudulent myth.
In its role as a primitive social
program, unwanted relatives (many times unskilled poor female spouses) are
imprisoned in psychiatric hospitals owned by individual people such as Battie.
William Battie owns psychiatric hospitals/prisons in Islington and Clerkenwell
and will die with 100,000-200,000 pounds from this business.

England  
242 YBN
[1758 AD]
1999)
Uppsala, Sweden (presumably)  
242 YBN
[1758 AD]
2048)
Paris, France  
242 YBN
[1758 AD]
2071) Cronstedt also makes a detailed analysis of calcium tungstate, a
previously unknown mineral of high relative density (specific gravity), and
studies the properties of gypsum and a hydrous mineral Cronstedt names zeolite.
Sweden (presumably)  
242 YBN
[1758 AD]
2110) King Louis XV calls Messier the comet ferret.

Asimov relates that at this time the true grandeur of the universe (that the
nebulae are actually other galaxies) was not yet known but is only suspected by
people like Lambert and Kant. There is a slow and very gradual acceptance that
the estimate of the size of the universe by the majority of people on earth
continues to increase, until finally the majority will probably accept that the
universe is either unknowingly, or infinitely large in size and age and scale.
Paris, France (presumably)  
242 YBN
[1758 AD]
2174)
Turin, Italy  
242 YBN
[1758 AD]
2696) The primary elements of matter for Boscovich are indivisible,
non-extended points. In contrast with Newton's hypothesis, direct contact of
these points is not allowed because for impenetrable particles this would imply
a discontinous change in velocity at the moment of contact. Therefore particles
actually never touch: at very short distances the mutual force between them is
repulsive, and increases indefinitely as the distance is diminished. At great
distances, particles attract through the gravitational force. Over the
intermediate range the force is alternatively attractive and repulsive, with
one or more oscillations. Boscovich represents his theory graphically through a
force-distance curve (see image): forces above the horizontal axis are
repulsive, those below it are attractive.

His law of interaction can be considered as the first interatomic model.
(interesting, Newton never hypothesized about gravity between atoms?)

It seems almost that there are two main competing sides throughout the history
of modern science, and Boscovich seems to be supporting the conservative side
which tends to reject atomism, also as applied to particles of light. I accept
the idea of light as the basis of all matter and as taking the form of a
particle, perhaps spherical. This view seems logical to me in recognizing that
planets and stars are spherical material objects, and that galaxies, ultimately
are made of these discrete-unit or point-like objects. However, perhaps
something may be learned from alternative interpretations of the universe, and
people certainly should have every freedom to theorize and to think and believe
whatever they want to.
Vienna  
242 YBN
[1758 AD]
3649)
(lecture at U of Göttingen) Göttingen, Germany  
241 YBN
[02/01/1759 AD]
2973)
London, England (presumably)  
241 YBN
[1759 AD]
1938)
London, England  
241 YBN
[1759 AD]
1939) In 1753 a pocket watch was made for Harrison, to his design, by
watchmaker John Jefferys. This watch performed so well that Harrison realized
that a longitude solution that uses smaller watches.
London, England  
241 YBN
[1759 AD]
1950) Voltaire (CE 1694-1778) publishes "Candide, ou l'Optimisme" (1759)
("Candide, Or All for the Best"), a philosophical fantasy, in which a youth
Candide, disciple of Doctor Pangloss (himself a disciple of the philosophical
optimism of the deceased Gottfried Leibniz), sees and suffers such misfortune
that Candide is unable to believe that (earth is) "the best of all possible
worlds." Having retired with his companions to the shores of the Propontis,
Candide discovers that the secret of happiness is "to cultivate one's garden,"
a practical philosophy excluding excessive idealism and nebulous metaphysics.

Through the allegory of Candide, Voltaire pokes fun at religion and
theologians, governments and armies, philosophies and philosophers. He
comprehensively, if not systematically, enumerates all the evils of the world
to make fun of the doctrine of Optimism, skewering various other sacred cows
along the way. He discusses many evils, but two stand out: the 1755 Lisbon
earthquake and the Seven Years' War-both of which inspired Voltaire to write
Candide.

Voltaire will not openly admit to having written the controversial "Candide"
until 1768 (until then he signed with a pseudonym: "Monsieur le docteur Ralph",
or "Doctor Ralph"), his authorship of the work is hardly disputed. Immediately
after publication, the work and its author are denounced by secular and
religious authorities alike.

By the end of February 1759, The Great Council of Geneva and the administrators
of Paris will have "Candide" banned and orders all copies to be burned. Candide
nevertheless succeeded in selling 20,000-30,000 copies by the end of the year
in over twenty editions, making it a best-seller. The Duke de La Vallière
speculated near the end of January 1759 that Candide might have been the
fastest-selling book ever. In 1762, Candide will be listed in the "Index
Librorum Prohibitorum", the Catholic Church's list of prohibited books.

Paris, France  
241 YBN
[1759 AD]
2141) Catherine II invites Wolff to Russia.
Wolff's name is preserved in several
anatomical names in particular the Wolffian body, an early form of of kidney in
embryonic animals preceding the true kidney.
Halle, Germany  
241 YBN
[1759 AD]
2156) Euler writes Lagrange on October 2, 1759 an enthusiastic letter about the
problem of isoperimetry which Lagrange has in these works solved, and which
Euler had long been working on.

Unlike the ordinary calculus, which analyzes the point characteristics of
specific functions, the calculus of variations deals with the extremum
characteristics of functions as a whole. The work quickly attracts the
attention of Pierre-Louis Moreau de Maupertuis (CE 1698â€"1759), president of
the Berlin Academy, who uses it to support his "principle of least action"
against numerous critics.

Lagrange is the only child of eleven to survive.
In 1755 Lagrange sent Euler a letter on
the "calculus of variations" so impressive that Euler holds back his own work
on the subject to allow Lagrange to publish first.
In 1758 Lagrange helps to
found a society which will later became the Turin Academy of Sciences.
The
Paris Academy of Sciences awards Lagrange prizes for his essays on the
libration of the moon (1764), the satellites of Jupiter (1766), and the
three-body problem (1772).

On the recommendation of Euler and D'Alembert, Frederick II appoints Lagrange
to succeed Euler as director of mathematics at the Berlin Academy of Sciences
at age 40, saying "the greatest king in Europe" ought to have the "greatest
mathematician in Europe" at his court.
Lagrange says Newton is the luckiest man
in the world because the system of the universe can only be worked out once,
and Newton was the person who did it. (Asimov cites Einstein as proof that
there is room for improvement, while I don't cite Einstein for anything other
than possibly an equivalent system of visualizing the force of gravity in 3D
with gravity representing the y dimension (after modifications such as viewing
photons as matter and removing time and space dilation), I think there is
definitely space for improvement, and I am not entirely sure Newton's laws are
the final word on all the matter in the universe in particular in photon
models.)
Lagrange lives in France through the Terror even though he is friends with
Marie Antoinette.
In 1793 Lagrange is appointed to head a commission that will in 1795
create the metric system. The metric system will come to be the universal
language of scientists, although (the majority in the) USA (and Great Britain)
still use the English system.
In 1794 when the École Centrale des Travaux
Publics (later renamed the École Polytechnique) is opened, Lagrange becomes,
with Gaspard Monge, the school's leading professor of mathematics.
Napoleon
makes Lagrange a senator and a count.
Turin, Italy  
241 YBN
[1759 AD]
2157)
Turin, Italy  
241 YBN
[1759 AD]
3011)
St. Petersberg, Russia  
240 YBN
[1760 AD]
2027)
Saint Petersburg, Russia  
240 YBN
[1760 AD]
2029)
Saint Petersburg, Russia  
240 YBN
[1760 AD]
2052) Denis Diderot (DEDrO) (CE 1713-1784), French writer , writes "La
Religieuse" which is about a woman placed in a convent against her will which
contains a sequence that deals examines female homosexuality.

Paris, France (presumably)  
240 YBN
[1760 AD]
2074) In this work Michell gives the conclusions of his study of the disastrous
Lisbon earthquake of 1755. Michell shows that the focus of that earthquake was
underneath the Atlantic Ocean, and proposes erroneously that the cause of
earthquakes was high-pressure steam, created when water comes into contact with
subterranean fires.
Michell is one of the founders of seismology, the science of
earthquakes.
Cambridge, England  
240 YBN
[1760 AD]
2094) In Berlin Lambert receives the patronage of Frederick the Great.
Lambert
corresponds with Immanuel Kant.
Augsburg, Germany  
240 YBN
[1760 AD]
2122) Water separated into hydrogen and oxygen using electricity.

Giovanni Beccaria (CE 1716-1781), Italian physicist, passes electricity sparks
through water and observes bubbles (of Hydrogen and Oxygen gas) released from
the water but incorrectly supposes that the action of the electric matter
promotes the evaporation of water.

Beccaria does not recognize that the gases produced are the components of
water.

Beccaria's main work is the treatise "Dell' Elettricismo Naturale ed
Artificiale" (1753,tr 1776).

It is interesting that Beccaria mistakes bubbles of hydrogen and oxygen for the
bubbles of water gas of boiling water. It is interesting to me that photons in
the form of heat only create bubbles of water vapor, where electrons (which may
be photons) separate the water molecule into Hydrogen and Oxygen.
Turin, Italy  
239 YBN
[1761 AD]
1217) Jewish people are killed in Nancy, France for host nailing.

  
239 YBN
[1761 AD]
1221) Wolfgang Amadeus Mozart (January 27, 1756 - December 5, 1791), at the age
of 5 appears as a keyboard performer for the first time.

Salzburg, Germany  
239 YBN
[1761 AD]
1915) Morgagni graduates from the University of Bologna in 1701 .
(At the
University of Bologna), Morgagni acts as prosector to A.M. Valsalva (one of the
distinguished pupils of Malpighi), whom he assists in preparing Valsalva's
celebrated "De Aure Humana" (1704; "Anatomy and Diseases of the Ear").
In 1712
Morgagni is professor of anatomy at the University of Padua, at age 30, and
will continue to be employed in this position for nearly 60 years.
Morgagni publishes
this book at the age of 79.

An English translation of "De Sedibus" will be made in 1769 by Benjamin
Alexander.
Padua, Italy  
239 YBN
[1761 AD]
2028)
Saint Petersburg, Russia  
239 YBN
[1761 AD]
2042)
Paris, France (presumably)  
239 YBN
[1761 AD]
2044) Lacaille uses Clairaut's calculations of the perturbations of the earth
to improve these tables of the Sun.
Paris, France (presumably)  
239 YBN
[1761 AD]
2079) Guillaume Le Gentil (lujoNTEL) (CE 1725-1792) French astronomer, goes to
India to observe the transit of Venus, but because of Seven Years' War between
Great Britain and France La Gentil must stay on his ship and misses the
observation, but decides to stay in India to try for the 1769 transit which he
also misses because of a cloud. La Gentil returns to France and he was thought
to be dead.
Le Gentil writes a 2 volume book on India.

Le Gentil finds that the duration of the lunar eclipse of 08-30-1765 was
predicted by a Tamil astronomer, based on the computation of the size and
extent of the earth-shadow (going back to Aryabhata, 5th c.), and was found
short by 41 seconds, whereas the charts of Tobias Mayer were long by 68
seconds.

  
239 YBN
[1761 AD]
5958) (Johann Chrysostom) Wolfgang Amadeus Mozart (CE 1756-1791), Austrian
composer, composes his first known compositions at 5 years old (KV 1a-f).
(verify)

Mozart and his older sister, Maria Anna (CE 1751–1829), are prodigies. At age
five Mozart begins to compose and gives his first public performance. Starting
in 1763 Leopold tours throughout Europe with his children. Mozart dies at the
young age of 35.

Salzburg, Austria   
238 YBN
[04/??/1762 AD]
1955) Jean-Jacques Rousseau (CE 1712-1778) prints "Du Contrat Social, Principes
du droit politique" (English: "Of the Social Contract, Principles of Political
Right"), which criticizes religion and is banned in both France and Geneva.
Rousseau is forced to flee arrest.

In this book Rousseau describes government as the servant of the people, and
not their master.
"Social Contract", "Émile" and other works by Rousseau help to
prepare the way for the French Revolution.

The first sentence in "Social Contract" is "Man was born free, but he is
everywhere in chains"

In the Social Contract he claims that true followers of Jesus would not make
good citizens. This was one of the reasons for the book's condemnation in
Geneva.

Paris, France  
238 YBN
[05/??/1762 AD]
1956) Jean-Jacques Rousseau (CE 1712-1778) publishes "L'Émile ou de
l'éducation" (1762) (or "Emile or On Education") a semi-fictitious work
detailing the growth of a young boy of that name, presided over by Rousseau
himself.

Rousseau rejects an education where a child learns only to please the
instructor claiming that this produces people fit to be only masters or slaves,
not free people.

Both "Du contrat social" (1762); and "Émile" (1762), which offend both the
French and Genevan ecclesiastic authorities are burned in Paris and Geneva.

Émile and its author are condemned for religious unorthodoxy in 1762 by the
Parlement de Paris, and Rousseau feels obliged to flee to Switzerland.

Rousseau is most controversial in his own time for his views on religion.
Rousseau's view that man is good by nature conflicts with the doctrine of
original sin and his theology of nature expounded by the Savoyard Vicar in
Émile leads to the condemnation of the book in both Calvinist Geneva and
Catholic Paris.

Paris, France  
238 YBN
[1762 AD]
1218) Pennsylvia psychiatric hospital charges 4 pence to visit.

  
238 YBN
[1762 AD]
2065) This is evidence against the view of those at the Florentine Academy that
water is incompressible.
London, England (presumably)  
238 YBN
[1762 AD]
2187) (John) Hutton uses some of Saussure's data.
Saussure leads the second
expedition to successfully reach the top of Mount Blanc, the highest peak of
the Alps.
Geneva, Switzerland  
238 YBN
[1762 AD]
2715)
(Royal Swedish Academy of Sciences) Stockholm, Sweden  
238 YBN
[1762 AD]
2975)
Berlin, Germany  
238 YBN
[1762 AD]
2978) There is a conflict between who first understood the principle and who
invented an actual electrophorus between Johann Wilcke (1762 or 1764), Cigna
(1762), and Volta(1775).
Turin, Italy (presumably)  
237 YBN
[1763 AD]
2000)
Uppsala, Sweden (presumably)  
237 YBN
[1763 AD]
2043) Also published in this year is Lavaille's "Journal historique du voyage
fait au cap de Bonne-Esperance" (1763).
Paris, France (presumably)  
237 YBN
[1763 AD]
2080)
France  
237 YBN
[1763 AD]
2128) Maskelyne is a member of the Board of Longitude, which was created in
1714 to decide on the award of the £20,000 prize for a solution to the problem
of determining longitude at sea. Possibly Maskelyne's allegience to his lunar
method causes him to refuse to recommed the chronometer of John Harrison for
the award.
London, England (presumably)  
236 YBN
[1764 AD]
1222) Wolfgang Amadeus Mozart (January 27, 1756 - December 5, 1791) composes
his first symphony at age 8.

Salzburg, Germany  
236 YBN
[1764 AD]
1947) Voltaire (CE 1694-1778) publishes "Encyclopédie, the Dictionnaire
philosophique" (1764) ("Philosophical Dictionary").
This work will be enlarged after 1770 as
"Questions sur l'Encyclopédie".

Cirey, France  
236 YBN
[1764 AD]
1952) Voltaire (CE 1694-1778) publishes "Encyclopédie, the Dictionnaire
philosophique" (1764) ("Philosophical Dictionary").
This work will be enlarged after 1770 as
"Questions sur l'Encyclopédie".

In "Philosophical Dictionary" Voltaire uses an alphabetical format to air his
own views on theology, modern religious beliefs, and many other subjects, in a
series of short essays. The Dictionary directs criticism against French
political institutions, Voltaire's personal enemies, the Bible, and the
Catholic Church. Presented in a wryly humorous manner, Voltaire's controversial
thoughts are condemned in Paris, Geneva, and Amsterdam. For safety reasons,
Voltaire denies his authorship.

Cirey, France  
236 YBN
[1764 AD]
1986) Benjamin Franklin (CE 1706-1790) invents bifocals, eyeglasses whose
corrective lenses each contain areas with two distinct optical powers.

Philadelphia, Pennsylvania (presumably)  
236 YBN
[1764 AD]
2091)
Glasgow, Scotland  
236 YBN
[1764 AD]
2160)
Turin, Italy (presumably)  
235 YBN
[05/??/1765 AD]
2145) Watt's father is the treasurer and magistrate of Greenock, runs a
successful ship and house building business. As a young person James Watt uses
his father's workshops equipped with tools, bench and forge to make models (for
example of cranes and barrel organs) and to become familiar with ships'
instruments.

In Glasgow, Watt meets many scientists and becomes friend of Joseph Black, who
developed the concept of "latent heat".
Watt is a member of the Lunar society.
In 1757 Watt is
established at he University of Glasgow as "mathematical instrument maker to
the university".
In 1814 Watt is offered a baronetcy, which he declines.

Watt's interests in applied chemistry lead him to introduce chlorine bleaching
into Great Britain and to devise a famous iron cement. In theoretical
chemistry, Watt is one of the first to argue that water is not an element but a
compound.
Glasgow, Scotland (presumably)  
234 YBN
[01/01/1766 AD]
2959)
(Academy of Geneva) Geneva, Switzerland (presumably)  
234 YBN
[04/05/1766 AD]
3012) Priestley writes "It is now also Mr. Canton's opinion, that electric
atmospheres are not made of effluvia from excited or electrified bodies, but
that they are only an alteration of the state of the electric fluid contained
in, or belonging to the air surrounding them, to a certain distance; that
excited glass, for instance, repels the electric fluid from it, and
consequently, beyond that distance makes it more dense; whereas excited was
attracts the electric fluid existing in the air nearer to it, making it rarer
than it was before.
This will be best understood by a figure. Let A (Plate I,
figure 1) represent unexcited glass or wax. B excited glass, and C excited wax;
and let the dots on each side of A represent a line of particles of the
electric fluid at their proper distance in a natural state. (Here clearly is
the concept of particles of electric fluid, later to be called "electrons")
Let
B and C be carried about where you will in the air, B will make an atmosphere
equally dense, and C an atmosphere equally rare, while the quantity of the
electric fluid each of them contains in the same as at first. When any part of
a conductor comes within the atmosphere of B, the electric fluid it naturally
contains will be repelled by the dense atmosphere, and will recede from it. But
if any part of a conductor be brought within the atmosphere of C, the electric
fluid it natually contains will be attracted by the rare atmosphere, and move
towards it. And thus may the electric fluid contained in any body be condensed
or rarefied; and if the body be a conductor, it may be condensed or rarefied in
any part of it, and some may be easily drawn out of, or an additional quantity
put into it."
London, England  
234 YBN
[05/29/1766 AD]
2113) Hydrogen gas isolated.

Henry Cavendish (CE 1731-1810), English chemist and physicist, produces
"inflammable air" (hydrogen) by dissolving metals in acids and "fixed air"
(carbon dioxide) by dissolving alkalis in acids, and he collected these and
other gases in bottles inverted over water or mercury.

An alkali is any of the soluble hydroxides of the alkali metals-i.e., lithium,
sodium, potassium, rubidium, and cesium. Alkalies are strong bases that turn
litmus paper from red to blue; they react with acids to yield neutral salts;
and they are caustic and in concentrated form are corrosive to organic tissues.
(show periodic table for this)

Cavendish publishes these experiments in a combination of three short chemistry
papers on "factitious airs," or gases produced in the laboratory.

Cavendish's "inflammible air" will be later named Hydrogen by Lavoisier. The
term Cavendish uses "inflammable air" is confusing because inflammable air is
flammable and perhaps "flammable air" would have been a better choice of
words.

Cavendish explains heat as the result of the motion of matter in the 1760s. In
1783 Cavendish will publish a paper on the temperature at which mercury freezes
and in that paper make use of the idea of latent heat, although he does not use
the term "latent heat" because he believes that it implies acceptance of a
material theory of heat.

Cavendish will determine the "specific heat" for a number of substances
(although these heat constants will not be recognized later.

These reactions form equations similar to the equation:
metal + acid + water --> salt +
inflammable air
for example:
Zn + 2HCl → ZnCl2 + H2
London, England  
234 YBN
[07/01/1766 AD]
1951) The 19-year-old Chevalier de La Barre, is tortured, beheaded and his body
burnt on a fire along with a copy of Voltaire's "Philosophical Dictionary", for
having insulted a religious procession and damaging a crucifix.

Voltaire (CE 1694-1778) tried unsuccessfully to stop the murder of La Barre.

It is often said (by Dickens, in "A Tale of Two Cities", among others) that La
Barre was executed for not kneeling or removing his hat before a Catholic
procession (on the feast of Corpus Christi). In fact the original cause of the
inquiry was the mutilation of a cross, a far more serious offense, probably
committed by La Barre's friend Gaillard d'Etalonde (who escaped). In France, La
Barre is a symbol of Christian religious intolerance, along with Jean Calas and
Pierre-Paul Sirven, all championed by Voltaire.

Voltaire, at first scared by the attention the affair draws to him, ended up
defending La Barre's memory and helping d'Etallonde. The sentence against La
Barre will be reversed by the National Convention during the French Revolution
in 1794.

Paris, France (presumably)  
234 YBN
[1766 AD]
2014)
Bern, Switzerland (presumably)  
234 YBN
[1766 AD]
2095)
Berlin, Germany  
234 YBN
[1766 AD]
2103) Johann Daniel Titius (TisuS) (CE 1729-1796), German astronomer, suggests
that the distance of the planets from the Sun follow the series A=4+(2^n *3),
where n=0,1,2,3... this is the series 4,7,10,16,28,52,100... which fits for
Mercury, Venus, Earth, Mars, some unknown object, Jupiter and Saturn. In 70
years Neptune will prove this theory wrong, but it does encourage Olbers and
others to find the asteroid belt in between Mars and Jupiter, (in addition to
inspiring the application of math to physical phenomena). Johann Elert Bode
will explore this theory further.

Wittenberg, Germany  
234 YBN
[1766 AD]
2142) Mesmer's dissertation at the University of Vienna (M.D., 1766), (which
according to the Encyclopedia Britannica, borrows heavily from the work of the
British physician Richard Mead), suggests that the gravitational attraction of
the planets affects human health by affecting an invisible fluid found in the
human body and throughout nature. In 1775 Mesmer will revise his theory of
"animal gravitation" to one of "animal magnetism", wherein the invisible fluid
in the body acts according to the laws of magnetism.

Mesmer passes magnets over people trying to cure disease. Later Mesmer just
uses his hands believing in "animal magnetism".

Braid will examine hypnotism 50 years later, when it is still called
"mesmerism".

(I accept that the power of suggestion, like a placebo, where people think they
might be receiving a legitimate cure, might have some tiny measurable health
effect, but it seems to me, to be based on trickery in some way, for example,
an educated person would know that a person is simply telling them to heal, and
then it is useless. It seems to me to have very little scientific content, but
it seems with my limited information that hypnotism may be an actual phenomenon
for some people, perhaps only a small minority. It's tough to know if
hypnotist shows are fraudulent or legitimate. The power of suggestion also
relates to how people secretly beam images and sounds on to other people's
brains, which is a powerful method to invoke a suggestion in particular in a
person who is not aware that some high school drop out skin head in the
government military, police or phone company is sending images and sounds onto
their brain. This form of suggestion, beaming images and sounds onto brains
through neuron activation, is very powerful for those who are not aware of the
technology (which sadly is most people). As is the case with many suggestion
techniques, once the person receiving the suggestion understands what is being
done to them, the suggestion has less effect. But this secret image and sound
sending technology has been terribly abused to control people like pawns, to
make people kill themselves, to kill other people, to start violent conflict,
and countless other terrible uses.)

(In addition, this is typical of the idea of health care without any kind of
license, in other words, do people stop, fine, or jail people treating people
with fraudulent theories or treatments, or do they allow people to freely
choose to have health treatments that a majority of people find to be
fraudulent or the doctor incompetent?)
(Perhaps the origin of Mesmerism in Vienna is only
coincidence in being the same birthplace of Freud's theories of psychology.
Psychology has grown to be a modern snake-oil cure-all pseudoscience industry
without any chemical diagnostic basis inflicted on people without choice at
worst and a consensual experimental science at best.)

Mesmer believes in a good relationship with his patients and makes his
treatment rooms heavily draped, with music playing, and Mesmer appearing in
long, violet robes.

(Sadly,) Mesmer enjoys a popular following and claims to be able to "channel"
magnetic powers in order to cure a variety of ailments, which Mesmer does for
public display. The medical establishment of Vienna pressure Mesmer to leave
and Mesmer finds favor in Paris at the end of the 1770s.

In 1784 King Louis XVI appoints a commission of scientists and physicians to
investigate Mesmer's methods. Among the commission's members are Benjamin
Franklin and Antoine-Laurent Lavoisier. The commission reports that Mesmer is
unable to support his scientific claims.

Discredited, Mesmer leaves France in 1791 and eventually settles in
Switzerland.
Mesmer's theories will bring on successors who claim they can tap an unseen
magnetic force within the body, and Mesmer is often credited with influencing
the development of hypnotism as psychotherapy (and what should potentially be
called unconsensual psycho-torture techniques since the word "therapy" may
imply consent and or permission from the so-called patient).
Vienna, Austria  
234 YBN
[1766 AD]
2161) This and other planetary model works may be an important source for
seeing early views of how Newton's equation is applied for more than one
object. I apply Newton's equation iteratively, in other words calculating
velocities of all masses for each time unit into the future. I think this is
the most simple method, and after a certain number of bodies I think geometric
or algebraic solutions are too complex. For example, I think people in the past
were trying to use Newton's equation to find algebraic and geometric solutions
to the planet moon motions, basing their solutions on the idea of a static
pattern that repeats. This method may produce equivalent solutions with the
iterative method. An important point is that there are many uncertainties in
terms of distribution of matter in planets, the Sun and moons which will
probably never be accurately handled and will always be estimations.
Turin, Italy (presumably)  
234 YBN
[1766 AD]
3725)
London, England (presumably)  
233 YBN
[1767 AD]
2075)
Thornhill, Yorkshire, England (presumably)  
233 YBN
[1767 AD]
2131) Priestley compares the two-fluid versus one-fluid with acid-base (alkali)
being united and neutral.

Priestley states that a full charge of two or three thousand feet of coated
glass would give a shock as great as a single flash of light, and that new
discoveries can be made by such a power.
In 1752 Priestley attended the Dissenting
Academy at Daventry, Northamptonshire. Dissenters are named for their
unwillingness to conform to the Church of England and are not allowed to enter
English universities by the Act of Uniformity (1662).

Priestley is a Unitarian minister (the Unitarian's deny the divinity of Jesus).
Priestley openly rejects the Calvinist doctrines of original sin and atonement,
rejecting (the false and idiotic myth) of the Trinity, viewing humans as being
capable of improvement.
Priestley openly supports the American colonists revolting against
King George III.
Priestley is against the slave trade.
Priestley is against religious
bigotry.
Priestley sympathizes with the French Revolution.
In 1766 Priestley meets Benjamin Franklin
in England, and this may have been what influenced (Priestley) into science.
Priestley
is the companion of a liberal Lord Shelburne, who lost a government post for
sympathizing with the American colonists.
Priestley believes the phlogiston theory until
death.
-July 14, 1791 some Birmingham pro-French Jacobins have a celebration in honor
of the second anniversary of the fall of the Bastille (Jacobins are liberals).
An angry mob retaliates against the best known Jacobin in the city and burns
down Priestley's house. Priestley uses the text for his Sermon: "Father,
forgive them for they know not what they do"
Priestley is a member of the Lunar
Society. meeting near night of full moon so members can walk home under light
of moon.
Priestley moves to the USA for the last ten years of his life, turning
down an offer to teach at University of Pennsylvania and as Unitarian minister
in New York.
Warrington, England  
232 YBN
[1768 AD]
1993)
St Petersburg, Russia (presumably)  
232 YBN
[1768 AD]
2081)
France  
232 YBN
[1768 AD]
2082) Nicolas Desmarest (DAmureST) (CE 1725-1815) French geologist, publishes
"Géographie physique" (1794; "Physical Geography").

France  
232 YBN
[1768 AD]
2093)
Berlin, Germany  
232 YBN
[1768 AD]
2096) James Cook (CE 1728-1779), English navigator , is chosen by the Royal
Society to take command of the ship "Endeavour" on its voyage to the islands of
Tahiti to transport the gentlemen of the Royal Society and their assistants to
observe a transit of Venus.
The second main objective of this voyage is to discover
the southern continent, Terra Australis, which is believed to exist in order to
symmetrically balance the northern land mass of Eurasia.
The leader of the scientists is
Joseph Banks, aged 26, who is assisted by Daniel Solander, a Swedish botanist,
as well as astronomers (Cook rating as one) and artists to maintain a visual
record.
Cook carries an early nautical almanac and brass sextants, but no chronometer
on the first voyage.
Transits of planets are valuable for determining the distance
between the Earth and the Sun.

London, England  
232 YBN
[1768 AD]
2104) This work by Spallanzani is set against the biological theory created by
Georges Buffon and John Turberville Needham that all living things contain, in
addition to inanimate matter, special "vital atoms" that are responsible for
all physiological activities. Buffon and Needham postulated that, after death,
the "vital atoms" escape into the soil and are again taken up by plants. Buffon
and Needham claim that the small moving objects in pond water (first seen by
Leewenhoek) are not living organisms but only "vital atoms" escaping from the
organic material. Spallanzani studies various forms of microscopic life and
correctly confirms the view of Antonie van Leeuwenhoek that these objects are
living organisms.

Some people object to Spallanzani's conclusions by arguing that by boiling so
long Spallanzani removed some vital principle in the air and that without this
principle the microorganisms could not breed. Pasteur's work will remove this
objection in a century.

Spallanzani's cousin Laura Bassi, is a female professor of physics who has 12
children in her spare time.
Pavia, Italy (presumably)  
232 YBN
[1768 AD]
2133)
Leeds, England  
232 YBN
[1768 AD]
2213) Lavoisier is from a wealthy family.
Lavoisier gets a degree in law, but instead
of practicing law pursues chemical scientific research that will result in his
being admitted into the Academy of Sciences in Paris.
At this time many natural
philosophers still view the four elements (earth, air, fire, and water) as the
primary substances of all matter. Chemists in this time analyze "mixts"
(compounds), such as the salts formed when acids combine with alkalis.
At the time, the
study of specific airs or gases is called pneumatic chemistry.
Lavoisier is viewed as one
of the founders of modern chemistry.
Some describe Lavoisier as the father of modern
chemistry.
Asimov states that Lavoisier is the Newton of chemistry stating that Lavoisier
does for chemistry what Galileo did for physics two centuries earlier.
Lavoisier
invested half a million francs in the Ferme Générale ("General Farm"), a
private firm hired by the French government to collect taxes, in order to fund
his research. The General Farm is a partnership that has a contract with the
royal government to collect certain sales and excise taxes, such as those on
salt and tobacco. This firm gouges the public because anything they collect
over their fixed fee they can keep, and are hated by the public. Lavoisier
earns 100,000 francs a year from this. Asimov argues that Lavoisier puts the
money back into chemical research which helps the public.
In 1771 Lavoisier marries
Marie-Anne the daughter of an important executive of the Ferme Générale. She
is 14 and beautiful and intelligent and throws herself fully into Lavoisier's
work, taking his notes, translating from English (Lavoisier never learns
English), and illustrating his books.
Lavoisier bans Jean-Paul Marat, a journalist,
from membership in the French Academy of Sciences, because the papers Marat
offers on the nature of fire are of no value. Marat remembers this and it will
contribute to the murder of Lavoisier by guillotine.
Lavoisier's work with
street lighting introduces him to combustion.
In 1760 Lavoisier works on on improved
methods of lighting towns.
Lavoisier avoids mentioning the help he receives from
Priestly.
Lavoisier never identifies a new element.
Lavoisier implies that the experiment of
burning Hydrogen is original to him and not Cavindish.
In England, Hutton, Cavendish, and
Priestly refuse to abandon the phlogiston theory, but Black accepts it. In
Sweden, Bergman accepts the new view, and in Germany Klaproth does.
Lavoisier
helps Guyton de Morveau with his writing of an article for chemistry for an
encyclopedia.(diderots?)
Paris, France (presumably)  
232 YBN
[1768 AD]
2229)
Paris, France (presumably)  
232 YBN
[1768 AD]
2667)
Edinburgh, Scotland  
232 YBN
[1768 AD]
2967)
(Vienna? and) London, England  
232 YBN
[1768 AD]
4482)
London, England  
231 YBN
[02/26/1769 AD]
3013)
Turin, Italy  
231 YBN
[03/16/1769 AD]
2108) Louis Antoine de Bougainville (BUGoNVEL) (CE 1729-1811) French navigator
completes the first French journey to sail around the Earth (1766-1769).

In 1768 Bougainville was the first to sight the Solomon Islands.
Bougainville
confirms the existence of marsupials in the eastern islands of Indonesia
(something Buffon refuses to believe).
Bougainville will publish his widely
read account, "Voyage autor du monde" (1771; "A Voyage Round the World", 1772)
in 1771.

Bougainville was commissioned by the French government to circle the Earth in a
voyage of exploration, and set out to sea in December 1766, accompanied by
naturalists and other scientists.

Saint-Malo, France  
231 YBN
[1769 AD]
1206) The first Self-propelled vehicle. A steam-engine powered automobile.

Nicolas-Joseph Cugnot (26 February 1725 - 2 October 1804), a French inventor,
builds what may be the first self-propelled vehicle built on earth using a
steam engine.

Cugnot may be the first to convert the back-and-forth motion of a steam piston
into rotary motion (James Watt does this too in 1781 in England).

Cugnot is trained as a military engineer. He experiments with working models of
steam engine powered vehicles intended for hauling heavy cannons for the French
Army, starting in 1765.

A functioning version of his "Fardier à vapeur" ("Steam wagon") run in this
year, 1769. The following year he builds an improved version. His vehicle is
said to be able to pull 4 tons and travel at speeds of up to 4 km per hour. The
heavy vehicle has two wheels in the back and one in the front, which supports
the steam boiler and was steered by a tiller.
England  
231 YBN
[1769 AD]
1940) King George III of England tests this H5 clock and is reported to have
declared "By God, Harrison, I will see you righted!", (in support of Harrison
getting the full prize money for a timepiece accurate enough to measure
longitude at sea).
London, England  
231 YBN
[1769 AD]
2069) Bonnet publishes this catastrophe theory in "La Palingénésie
philosophique" (1769; "The Philosophical Revival").

The catastrophism theory will be adopted by Georges Cuvier, and strongly
influences geological thinking until the 1820s.
Geneva?, Switzerland (presumably)  
231 YBN
[1769 AD]
2097)
New Zealand  
231 YBN
[1769 AD]
2130) Apart from a completely mechanical loom, Arkwright eliminates all the
major obstacles to producing cotton cloth by machine. Because thread production
is now completely mechanized, all operations previously conducted separately
could be coordinated and carried out under one roof, in a mill, or, as it is
increasingly called, a factory.

With several partners, Arkwright opens factories at Nottingham and Cromford.
Within a few years Arkwright is operating a number of factories equipped with
machinery for carrying out all phases of textile manufacturing from carding to
spinning. Carding is to cleanse, disentangle, and collect together as fibers by
the use of cards in preparation to spin.
Lancashire cottonmasters successfully attack
Arkwright's patent (in 1781 and 1785).
By 1782 Arkwright has capital of £200,000 and
employs 5,000 workers.
At the time of his death Arkwright has 2.5 million dollars, an
enormous sum for this time.
Many people are angry with Arkwright, thinking that he is
taking away jobs.

Some consider Arkwright the "father of the factory system".
  
231 YBN
[1769 AD]
2146)
Glasgow, Scotland (presumably)  
231 YBN
[1769 AD]
2426)
Edinburgh, Scotland  
231 YBN
[1769 AD]
2980)
Beccaria's main work is the treatise "Dell' Elettricismo Naturale ed
Artificiale" (1753,tr 1776).
Turin, Italy (verify)  
231 YBN
[1769 AD]
6323) (Johann Chrysostom) Wolfgang Amadeus Mozart (CE 1756-1791), Austrian
composer, composes "Te Deum Laudemus".
Salzburg, Austria  
230 YBN
[04/19/1770 AD]
2100) James Cook (CE 1728-1779) claims the coast of Australia for Great
Britain.
Australia  
230 YBN
[1770 AD]
2158)
Berlin, Germany  
230 YBN
[1770 AD]
2195)
St. Petersburg, Russia (presumably)  
230 YBN
[1770 AD]
2214)
Paris, France (presumably)  
230 YBN
[1770 AD]
2257) Gahn's company fills an emergency order of copper to the colonists in the
Revolutionary war.
Gahnite (zinc spinel) is named for Gahn.
Uppsala, Sweden  
230 YBN
[1770 AD]
2958) Joseph Priestley writes:
"I find by experience that the (Henley) electrometer
answers all the purposes I have mentioned, with the greatest ease and
exactness. I am now sure of the force of an explosion before a discharge of a
jar or battery, which I had no better method of guessing at before, than by
presenting to them a pair of Mr. Canton’s balls and observing their
divergence at a given distance"
London, England (presumably)  
229 YBN
[07/12/1771 AD]
2207) In 1761 Banks inherits a considerable fortune from his father.
Determined to
receive botanical instruction, he paid Cambridge botanist Israel Lyons to
deliver a series of lectures at Oxford in 1764.
Asimov describes Banks as a rare
example of a wealthy person that uses there money to advance science.
Banks goes on
several major collecting trips, the most famous being the around-the-world
voyage aboard the Endeavour on the 1768-71 expedition led by James Cook, a
journey that makes marsupials known to the people of Europe.
Banks hires a pupil of
Linnaeus and four artists.
Banks is part of the British mission to observe Venus from
Tahiti and then to search for the unknown southern continent and that founds
colonies in Australia. (The Australian accent must have evolved from an English
accent.) Banks is viewed as a hero upon his return.
One ship transporting
breadfruits in 1788 is the "Bounty" under William Bligh who had been a ship's
master under Cook on Cook's final voyage to the Pacific. The crew of the Bounty
mutinied against harsh treatment by the captain and against having to leave
Tahiti.
Banks' "Florilegium", a collection of engravings of plants compiled by Banks
and based on drawings by Swedish botanist Daniel Solander during Cook's 1768-71
voyage, will not be published in full until 1989.
In 1805, Banks is the first to
suggest the identity of the wheat rust and barberry fungus.
Banks is president of the
Royal Society from 1778 to 1820.
Banks develops an extensive botanical collection
which will be donated to the British Museum, and Banks helps establish Kew
Gardens in London. Through Banks' efforts Kew Gardens became arguably the
pre-eminent botanical gardens in the world.
London (where Banks lives), England  
229 YBN
[1771 AD]
2118) Cavendish measures current by shocking himself and estimating the pain.
London, England  
229 YBN
[1771 AD]
2292) Abraham Gottlob Werner (VRNR or VARNR) (CE 1750-1817), German geologist,
establishes the erroneous theory of "Neptunism" that the earth was once all
covered with water and that over time all the minerals were precipitated out of
the water into distinct layers. This theory is in contrast to the Vulcanists
(or Plutonists), who argue that granite and many other rocks are of igneous
origin (the result of volcanic magma, (red hot liquid rock)).

According to Werner the first layer is made of primitive rocks, such as
granite, gneiss, and slates, and contains no fossils. The next strata has
shales and graywacke and contains fossilized fish. Above this are the
limestones, sandstones, and chalks and then the gravels and sands of the
alluvial strata. Lastly, local volcanic activity produced lavas and other
deposits. Because this theory does not allow for a molten core, Werner proposes
that volcanoes are a recent phenomena caused by the spontaneous combustion of
underground coal beds.

For many years Werner's theories prevail over those of the plutonists, led by
James Hutton, who (correctly) identifies the origin of igneous rocks resulting
from (the cooling of) molten material. Neptunism will prevail until Lyell.

Leipzig, Germany  
229 YBN
[1771 AD]
3010)
London, England  
229 YBN
[1771 AD]
5956)
Madrid, Spain (verify)  
228 YBN
[10/20/1772 AD]
2224)
Paris, France (presumably)  
228 YBN
[11/01/1772 AD]
2225)
Paris, France (presumably)  
228 YBN
[1772 AD]
2049) The completion of the "Encyclopédie" in 1772 leaves Diderot without a
source of income. To relieve Diderot of financial worry, Catherine the Great of
Russia buys Diderot's library, requesting him to retain the books until she
requires them, and then appoints him librarian on an annual salary for the
duration of his life. Diderot goes to St. Petersburg in 1773 to thank her for
her financial support and is received with great honor and warmth.

The Oxford University Press states that the Encyclopédie issues a direct
challenge to royal absolutism and the religious supremacy of the Catholic
Church throughout Europe.
Paris, France  
228 YBN
[1772 AD]
2051) Denis Diderot (DEDrO) (CE 1713-1784), French writer , writes "L'Entretien
entre d'Alembert et Diderot" (written 1769, published 1830; "Conversation
Between d'Alembert and Diderot"), and "Le Rêve de d'Alembert" (written 1769,
published 1830; "D'Alembert's Dream"). In these works and his later "Eléments
de physiologie" (1774-80) Diderot develops his materialist philosophy,
speculates on the origins of life without divine intervention and the cellular
structure of matter.

Paris, France  
228 YBN
[1772 AD]
2078)
Thornhill, Yorkshire, England (presumably)  
228 YBN
[1772 AD]
2138) Nitrous oxide is one of several oxides of nitrogen, is colorless with
pleasant, sweetish odor and taste, which when inhaled produces insensibility to
pain preceded by mild hysteria (nervous system excitement, emotion, reaction),
and sometimes laughter.
Nitrous oxide currently is used mainly as an anesthetic in
surgical operations of short duration.
Prolonged inhalation of nitrous oxide causes
death.
Nitrous oxide is also used as a propellant in food aerosols.
Nitrous oxide is
prepared by the action of zinc on dilute nitric acid, by the action of
hydroxylamine hydrochloride (NH2OH×HCl) on sodium nitrite (NaNO2), and, most
commonly, by the decomposition of ammonium nitrate (NH4NO3). (State method
Priestley uses)
Priestley reports in his posthumously published memoir that his
interest in chemistry is a consequence of living next to a brewery during his
ministry at Leeds (1767-1773).
For his work on gases, Priestley will be awarded the Royal
Society's prestigious Copley Medal in 1773.
Leeds, England  
228 YBN
[1772 AD]
2140)
Leeds, England  
228 YBN
[1772 AD]
2162) Lagrange studies situations where three bodies might form stable
configurations providing one body is very low mass. These are now sometimes
referred to as "trojan" systems.
Berlin, Germany  
228 YBN
[1772 AD]
2170) Joining in the anticlericalism of the time, in 1763 Morveau publishes a
long poem attacking the Jesuits anonymously.
In 1787, when spending several months in Paris,
Lavoisier convinces Morveau of the accuracy of Lavoisier's oxygen theory of
combustion.
Guyton De Morveau makes no effort to save his fellow chemist Lavoisier.
?, France  
228 YBN
[1772 AD]
2172)
Dijon, France  
228 YBN
[1772 AD]
2199) Oxygen is a colourless, odourless, tasteless gas.
Oxygen is the fifth least
dense of all elements.
Oxygen is symbol O; at. no. 8; at. wt. 15.9994; m.p.
−218.4°C; b.p. −182.962°C; density 1.429 grams per liter at STP;
valence −2.
Oxygen has an atomic radius of 60 pm.
Oxygen has 3 stable isotopes, the
most common 16 has 8 neutrons, the other two have 9 and 10 neutrons.

In 1757 Scheele is apprenticed to a pharmacist in Göteborg, Sweden.
Scheele refuses to
work as a court chemist for Frederick II.(detail)
Asimov comments that Sweden in proportion
to its population has probably produced more first-rate chemists in the last
two centuries than any other nation.
In his short lifetime, Scheele identifies or helps
to identifies more new substances than any other chemist in a similar period of
time.
Scheele wrote "It is the truth alone that we desire to know and what a joy
there is in discovering it!"
Scheele dies at 43, which may have been from mercury
poisoning.
Uppsala, Sweden  
228 YBN
[1772 AD]
2215)
Paris, France (presumably)  
228 YBN
[1772 AD]
2266) Whether this law is pure coincidence is unknown.

Bode writes astronomy textbooks in 1766 at age 19.

Sagan in the video Cosmos states that in simulations many systems are
physically possible, for example large gas giant planets close to Sun and
terrestrial planets far away.

Planets found by their gravitational effect on a star's Doppler shift indicate
that massive planets can be very close to a star, however planets being moved
closer to a star by life cannot be ruled out.
Berlin, Germany  
228 YBN
[1772 AD]
2285) Nitrogen gas isolated.

Daniel Rutherford (CE 1749-1819) Scottish chemist, (is credited with being) the
first to isolate nitrogen.
Edinburgh, Scotland  
228 YBN
[1772 AD]
4484)
Thornhill, Yorkshire, England (presumably)  
226 YBN
[08/01/1774 AD]
2139) This is Priestley's most famous chemical discovery.
Calne, England  
226 YBN
[1774 AD]
1225) "Act for regulating madhouses, licensing, and inspection" is passed in
England. This law requires physicians to certify that a human is "insane".
However, since this diagnosis describes a nonexistant, lawful, or trivial
condition, this label of "insane" may be used as a way around the due process
of the established legal system.

  
226 YBN
[1774 AD]
2111)
Paris, France (presumably)  
226 YBN
[1774 AD]
2129)
Schiehallion Mountain, North Perthshireit, Scotland  
226 YBN
[1774 AD]
2136)
Calne, England  
226 YBN
[1774 AD]
2137) English chemist Joseph Priestley (CE 1733-1804) writes two volumes of a
General History of the Christian Church to the Fall of the Western Empire (in
1790). Four volumes of the later history of the church will appear between 1802
and 1803.

Calne, England  
226 YBN
[1774 AD]
2200) Chlorine has: atomic number 17; atomic weight 35.453; freezing point
−100.98°C; boiling point −34.6°C; relative density (specific
gravity) 1.56 (−33.6°C); valence 1, 3, 5, 7.

Chlorine is 8th least dense element known.

Chlorine is a toxic, corrosive, greenish yellow gas that is irritating to the
eyes and respiratory system.
Chlorine is two and a half times heavier than air.
Uppsala, Sweden  
226 YBN
[1774 AD]
2201)
Uppsala, Sweden  
226 YBN
[1774 AD]
2216) Antoine Laurent Lavoisier (loVWoZYA) (CE 1743-1794) shows how material in
the air combines with metals when heated, which will end the phlogiston theory
of combustion, and demonstrates the conservation of mass.

Antoine Laurent Lavoisier (loVWoZYA) (CE 1743-1794) heats tin and lead in
closed contained with air. Both metals form a layer of calx on the surface. The
calx is heavier than the original metal, but the vessel still weighs the same
after heating, so Lavoisier concludes that there must be a weight loss
elsewhere, possibly in the air or in the vessel. If the air, then a partial
vacuum must exist in the vessel, and sure enough air rushes in when Lavoisier
opens the vessel, and then the vessel and its contents gain weight. (It is
interesting that atoms in air bonding with a solid creates a vacuum, as I
suppose any gas chemically combining with a solid in a closed container will
create a vacuum of empty space and pressure difference with the atmosphere of
Earth.) Lavoisier therefore shows that the calx (now known as oxide) is made of
a combination of the metal with air, and that rusting (and combustion) do not
involve a loss of phlogiston but a gain of at least a portion of the air. This
experiment will finally end the popularity of the phlogiston theory, and
establish chemistry on its modern basis (in terms of oxygen combustion).
Lavoisier also shows that mass is only shifted from one place to another and
cannot be created or destroyed, which is the law of conservation of mass.

The mass loss from particles of light in the form of particles of light of
various frequencies is apparently too small to be measured and Lavoisier
(presumably) misses this concept. One modern view is that electrons are
composed of photons and vary in mass depending on their orbit as the Bohr model
requires, and in combustion, the photons observed are released from electrons
around the oxygen and fuel atoms, the electrons losing mass in the form of
photons, while the nucleus of all atoms is still preserved. Another view holds
that some atoms completely separate into their source photons in oxygen
combustion.
Paris, France (presumably)  
226 YBN
[1774 AD]
2217)
Paris, France (presumably)  
226 YBN
[1774 AD]
2226)
Paris, France (presumably)  
226 YBN
[1774 AD]
2258) Manganese has atomic number 25; atomic weight 54.9380; melting point
1,244°C; boiling point 1,962°C; relative density 7.21 to 7.44; valence 1, 2,
3, 4, 6, 7.
Depending on form manganese has a valence principally +2, +4, or +7.

Manganese is a pinkish-gray, chemically active metal. Manganese is the first
element in Group 7 of the periodic table. Manganese resembles iron but is
harder and more brittle.
Manganese is the twelfth most abundant element in the Earth's
crust (approximately 0.1%) and occurs naturally in several forms, primarily as
the silicate (MnSiO3) but also as the carbonate (MnCO3) and a variety of
oxides, including pyrolusite (MnO2) and hausmannite (Mn3O4). Land deposits
cause large amounts of manganese oxide to be washed out to sea, where the
manganese oxides aggregated into manganese nodules containing 15-30% Mn.
Manganese
is essential to plant growth and is involved in the reduction of nitrates in
green plants and algae.
Manganese is also a necessary trace element for higher
animals, in which manganese participates in the action of many enzymes. Lack of
manganese causes testicular atrophy, however an excess of manganese in plants
and animals is toxic.

Manganese metal oxidizes superficially in air and rusts in moist air. Manganese
metal burns in air (or oxygen) at elevated temperatures, as does iron.
Uppsala, Sweden  
226 YBN
[1774 AD]
2267)
Berlin, Germany  
226 YBN
[1774 AD]
2293) Werner classifies minerals as Linnaeus had classified living objects 50
years before. (in this book?)
Leipzig, Germany  
226 YBN
[1774 AD]
2664)
Switzerland (presumably)  
226 YBN
[1774 AD]
2841) In 1757 Herschel is German, but escapes to England deserting the
Hannoverian army and the Seven Years' War.
Herschel is an organist and music
teacher
Herschel reads Robert Smith's "A Compleat System of Opticks", which introduces
Herschel to the techniques of telescope construction and interests Herschel in
viewing the night sky.

Most astronomer of this time are content to observe the Sun, Moon, and planets
but Herschel is determined to see distant celestial bodies too. For this
Herschel needs telescopes with larger mirrors to collect enough light, mirror
larger than the opticians can supply for a reasonable cost, and so Herschel
starts to grind his own mirrors from metal disks of copper, tin, and antimony
in various proportions.
In 1781 Herschel's needs are larger than the local foundries can
produce and so Herschel casts molten metal into disks in his basement.
Herschel's telescopes are far superior to even those used at the Greenwich
Observatory.
Herschel also makes his own eyepieces (from glass), the strongest eyepiece
Herschel makes has a magnifying power of 6,450 times.

Herschel grinds 200 lens before making one that satisfies him.
William, his brother
and his sister Caroline all grind many lens together.
William's sister Caroline is the
first important female astronomer.
Caroline reads aloud to William and feeds him bites of
food while he grinds for hours.
After finding Uranus, Herschel is appointed private
astronomer of George III at a salary of 300 guineas a year. (is in England?)

After finding Uranus Herschel becomes famous almost overnight. The Royal
Society of London awards Herschel the Copley Medal for the discovery of Uranus,
and elects Herschel a Fellow. William is appointed as an astronomer to George
III, and the Herschels moved to Datchet, near Windsor Castle.

Herschel sells many of his telescopes to supplement the income for his family.

Herschel meets Laplace and Napoleon, and views Napoleon as pretending to know
more than Napoleon really does.
Herschel reports 4 other satellites of Uranus that
are mistakes.
Herschel thinks the moon of Earth and planets are inhabited.
Herschel thinks that
inside the Sun is a cold solid body that might even be inhabited, thinking
sunspots to be holes in the atmosphere through which the cold surface can be
seen. (I think it might be possible that sun spots are colder than the rest of
the sun, clearly no photons are being emitted there...it could be like small
solidified areas, like an earth crust temporarily forming. I think the correct
view is that these areas are in fact not as hot as the rest of the surface and
that they are formed strictly from the sun magnetic, what I call electric,
field. I guess a magnetic field is thought to be a static electric charge,
while an electric field is made by moving electric charges.)

Herschel stubbornly rejects the accumulating evidence that not all stars are
equally bright (or emit the same quantity of photons in the visible spectrum),
holding to the belief that differences in apparent brightness (or quantity of
visible photons emitted, also related to star size) represent differences in
distances.
Bath, England  
226 YBN
[1774 AD]
2982)
London?, England  
226 YBN
[1774 AD]
5959) (Johann Chrysostom) Wolfgang Amadeus Mozart (CE 1756-1791), Austrian
composer,composes his first piano sonata (Piano Sonata No. 1 in C major, K.
279). (verify)

Munich, Germany (verify)  
225 YBN
[06/10/1775 AD]
2246) In 1774, Volta becomes professor of physics at the Royal School of Como.
In
1779, Volta is appointed to the chair of physics at the University of Pavia.
Volta
describes the electrophorus first in a letter to Priestly.
Galvani sends copies of his
papers to Volta, and the two are friends.
In 1794, Volta receives the Copley medal from
he Royal Society of London before inventing the battery.
Como, Italy  
225 YBN
[1775 AD]
1227)
London, England  
225 YBN
[1775 AD]
2101) James Cook (CE 1728-1779), English navigator , completes three years
(1772-1775) of navigating southern waters down to the Antarctic circle and
proves that there are no other vast southern continents beside Australia, but
does not identify Antarctica itself.

Cook charts Tonga and Easter Island, and discovered New Caledonia in the
Pacific and the South Sandwich Islands and South Georgia Island in the
Atlantic.

Southern Pacific Ocean  
225 YBN
[1775 AD]
2143) Bergman gives early encouragement to Karl Scheele, some of whose work
Bergman publishes.
Uppsala, Sweden (presumably)  
225 YBN
[1775 AD]
2296)
Göttingen, Germany{2 presumably}  
224 YBN
[07/04/1776 AD]
1532) Thomas Jefferson (CE 1743-1826), American statesman and scholar, 3rd
President of the USA, drafts the Declaration of Independence.
Philadelphia, Pennsylvania, (modern: United States)  
224 YBN
[1776 AD]
2109)
Copenhagen, Denmark (published)  
224 YBN
[1776 AD]
2176)
Bath, England  
223 YBN
[1777 AD]
2165)
Paris?, France  
223 YBN
[1777 AD]
2182)
Bath, England  
222 YBN
[1778 AD]
1204)
England  
222 YBN
[1778 AD]
2004) Georges Louis Leclerc, comte (count) de Buffon (BYUFoN) (CE 1707-1788),
French naturalist, translates Stephen Hales' "Vegetable Statics" (1735) into
French.

Buffon experiments to try and prove if Archimedes could burn ships with lens
and decides that it is possible (modern people have determined it to be
possible only for very close ships).
Buffon spends much of his life writing a "Natural
History" which will reach 44 volumes when complete.
In 1739 Buffon is appointed
keeper of the Jardin du Roi (Royal Garden, now "Jardin des Plantes"), a job
Buffon keeps until his death.
Buffon's son is guillotined during the French
Revolution.

Montbard, France  
222 YBN
[1778 AD]
2102) Cook is killed by native people of Hawaii.
Hawaii  
222 YBN
[1778 AD]
2144) Torbern Olof Bergman (CE 1735-1784), Swedish mineralogist publishes "De
Analysi Aquarum" (1778; "On Water Analysis") the first comprehensive account of
the analysis of mineral waters.

Uppsala, Sweden (presumably)  
222 YBN
[1778 AD]
2203) Molybdenum is atomic nunmber 42; at. wt. 95.94; m.p. about 2,617°C; b.p.
about 4,612°C; rel. dens. (sp. gr.) 10.22 at 20°C; valence +2, +3, +4, +5, or
+6. Molybdenum is a hard, malleable, ductile, high-melting, silver-white metal
with a body-centered cubic crystalline structure.

Molybdenum has the sixth highest melting point of any element.
Köping, Sweden (presumably)  
222 YBN
[1778 AD]
2218)
Paris, France (presumably)  
222 YBN
[1778 AD]
2236) In 1793, when the Jardin des Plantes is changed to the National Museum of
Natural History, Lamarck is made professor of "Insects and Worms" (Carl
Linnaeus's terms for invertebrates). By this time Lamarck has a large
invertebrate collection of his own.

Lamarck (with poor intuition) opposes the new view of Lavoisier.
Lamarck publishes
"Recherches sur les causes des principaux faits physiques, et particulièrement
sur celles de la combustion" (1794, "Research on the Causes of Principal
Physical Facts, and Particularly on Those of Combustion"), followed by
"Réfutation de la théorie pneumatique, ou de la nouvelle doctrine des
chimistes modernes" (1796, "Refutation of the Pneumatic Theory, or of the New
Doctrine of Modern Chemists") in which Lamarck opposes Lavoisier's theory of
combustion, comparing it with his own theory. (detail on Lamarck's theory)

Cuvier opposes Lamarck because of Lamarck's sarcastic references to Cuvier's
theories of catastrophism.

Lamarck dies blind and in poverty.
Paris, France (presumably)  
222 YBN
[1778 AD]
2237)
Paris, France (presumably)  
222 YBN
[1778 AD]
2248) Methane is a colorless, odorless gas that is the main component of
natural gas, a component of firedamp in coal mines, and a product of the
anaerobic bacterial decomposition of vegetable matter under water (from which
methane gets the alternate name of "marsh" gas).

Methane is the simplest member of the paraffin series of hydrocarbons.
Methane's chemical formula is CH4. Methane is lighter than air. Methane has a
relative density of 0.554. methane is only slightly soluble in water. Methane
burns in air, forming carbon dioxide and water vapor.
Como, Italy  
222 YBN
[1778 AD]
5960)
Paris, France (verify)  
221 YBN
[1779 AD]
2106) This is before the cell theory of 1839 and Spallanzani supports the
prevailing view that spermatozoa are parasites within the semen.
Pavia, Italy (presumably)  
221 YBN
[1779 AD]
2112)
London, England  
221 YBN
[1779 AD]
2166)
Paris?, France (presumably)  
221 YBN
[1779 AD]
2188)
Geneva, Switzerland (presumably)  
221 YBN
[1779 AD]
2219)
Paris, France (presumably)  
221 YBN
[1779 AD]
3251)
Berlin, Germany  
220 YBN
[1780 AD]
1208)
Switzerland?  
220 YBN
[1780 AD]
2053) Jean Étienne Guettard (GeToRD) (CE 1715-1786), French geologist , is the
first to geologically map France publishing this in his "Atlas et description
minéralogiques de la France" ("Mineralogical Atlas and Description of
France").
France  
220 YBN
[1780 AD]
2062)
Paris, France (presumably)  
220 YBN
[1780 AD]
2274) According to Asimov, Laplace is reluctant to give credit to others, for
example Lagrange's contributions to their joint work on celestial mechanics.

Napoleon makes Laplace minister of interior, but Laplace proves incompetent and
is promoted to the purely decorative position of Senator. When Louis XVIII
comes to the throne after Napoleon's fall, Laplace is not penalized like Haüy
and Chaptal, but instead Louis XVIII makes Laplace a marquis.

The Encyclopedia Britannica speculates that because Laplace does not hold
strong political views and was not a member of the aristocracy as being
probably why Laplace escapes imprisonment and execution during the French
Revolution.

Napoleon remarks on leafing through Laplace's book that he sees no mention of
God, to which Laplace replies "I had no need of that hypothesis".
Paris, France (presumably)  
220 YBN
[1780 AD]
2286)
Canterbury, England  
219 YBN
[03/13/1781 AD]
2840) German-English astronomer, William Herschel (CE 1738-1822) identifies the
planet Uranus.

This is the first new planet to be discovered since prehistoric times.

In recording double stars systematically, on this day, Herschel enters a pair
of which "the lowest of the two is a curious either nebulous star or perhaps a
comet". Four days later Herschel looks for the object and finds that it has
moved. From this time on Herschel regularly observes the object.

When enough observations (positions) have been made to calculate an orbit,
Hershel and in particular Laplace find that the orbit is nearly circular like a
planet instead of elongated like a comet. In addition the orbit of the object
is located far outside of Saturn. Herschel then understands that he has found a
new planet. This planet is barely visible to the naked eye and has been seen a
number of times before this. Flamsteed recorded it as 34 Tauri in the
constellation Taurus. Hershel tries to name the planet "Georgium Sidus"
("George's star") after George II, then king of England. Lalande suggests the
name "Hershel", but ultimately it is decided to stay with mythological names
for the planets, and Bode's suggestion of "Uranus" after the (Roman God who is
the) father of Saturn (in Greek "Cronos" t: presumably the Greek version of
Uranus). The identification of Uranus caused a large amount of excitement. (in
particular to those who think that Newton had left nothing to find).

Before this Herschel has made two preliminary telescopic surveys (and catalogs)
of outer space, and finds Uranus during a third and most complete survey.

Herschel is the first to systematically report on variable stars.

Hershel wrongly views the Sun as being near the center of a giant collection of
stars in the shape of a grindstone. Harlow Shapley will determine the sun's
correct position.

Hershel suggests the name "€œasteroids"€ (star-like) (in 1802) for the
small objects being found in between the orbit of Mars and Jupiter, for example
Ceres, because they are too small to appear as discs in the telescope but
appear only as points of light. Asimov comments that "€œasteroids" is not a
good name, and "€œplanetoids", or "€œminor planets"€ is more accurate
and considered preferable. (Perhaps there should be a name for all orbiting
objects, orbiting stars, planets, etc. but there would be the problem of two
objects orbiting each other with no clear larger one.)
Bath, England  
219 YBN
[1781 AD]
2123) Darwin is described as a freethinker and radical, who often writes his
opinions and scientific treatises in verse.
Darwin sympathizes with the French
revolutionaries.

Darwin's scientific writings are generally well received until the politician
George Canning produces a very damaging parody of Darwin's work. This is part
of a general campaign by the government against the Lunar Society for its
support of the French and American revolutions, as well as the Lunar Society's
denouncement of slavery.

Darwin's other major works will include "A Plan for the Conduct of Female
Education in Boarding Schools" (1797) and "Phytologia, or the Philosophy of
Agriculture and Gardening" (1800).
Derby, England (presumably)  
219 YBN
[1781 AD]
2147) According to the Encyclopedia Britannica, Matthew Boulton, the
manufacturer of the Soho Works in Birmingham, who funds much of Watt's work,
foreseeing a new market in the corn, malt, and cotton mills, urges Watt to
invent a rotary motion for the steam engine, to replace the reciprocating
action of the original.

William Murdoch is generally credited with inventing the sun-and-planet gear
which is included in James Watt's patent.
Birmingham, England (presumably)  
219 YBN
[1781 AD]
2196) The radius predicted by Bode's law agreed within two percent of the
observed radius.
St. Petersburg, Russia (presumably)  
219 YBN
[1781 AD]
2204)
Köping, Sweden (presumably)  
219 YBN
[1781 AD]
2208) As a priest, Haüy is in danger during the French Revolution, and is
jailed for some time. (It is interesting that priests were jailed in the
Revolution, perhaps for fraud? My vote is to tolerate total free thought,
speech and delusion. To me it is hopeful to see religious people supporting and
involved in science.)
Paris, France (presumably)  
219 YBN
[1781 AD]
2211) Thomas Jefferson (CE 1743-1826), American statesman and scholar,
publishes "Notes on the State of Virginia" (1781), which is part travel guide,
part scientific treatise, and part philosophical meditation, the only book
Jefferson ever publishes. In this work Jefferson advocates ending slavery.

Jefferson
writes "Millions of innocent men, women, and children, since the introduction
of Christianity, have been burnt, tortured, fined, and imprisoned; yet we have
not advanced one inch toward uniformity. What has been the effect of coercion?
To make one-half the world fools and the other half hypocrites. To support
roguery and error all over the earth."

Jefferson experiments with new varieties of grain.
Jefferson studies and classifies
fossils unearthed in New York State.
Jefferson is friends with Joseph Priestley.
Jefferson is a
skillful architect.
Asimov comments that Jefferson is the closest to scientist-in-office
of all Presidents of the USA (Jefferson is 3rd US President).
Jefferson is a strong
advocate of separation of Church and State.
All accounts of Jefferson in his youth
describe him as an obsessive student, often spending 15 hours of the day with
his books, 3 hours practicing his violin, and the remaining 6 hours eating and
sleeping.

Charlottesville, Virginia, USA  
219 YBN
[1781 AD]
2263)
Uppsala, Sweden (presumably)  
219 YBN
[1781 AD]
2304) William Nicholson (CE 1753-1815) English chemist publishes "Introduction
to Natural Philosophy" (1781).

London, England (presumably)  
219 YBN
[1781 AD]
2321) Chaptal is one of first to adopt Lavoisier's new view.
Chaptal is a
strong advocate of science popularization and writing science for the average
person.
Montpellier, France  
218 YBN
[11/??/1782 AD]
2348) Goodricke is deaf and mute throughout his life, probably because of an
illness in childhood.
Despite this handicap, Goodricke is a bright student.
Goodricke
makes this discovery at age 17.
Goodricke reports this to the Royal Society who
award Goodricke with a Copley Medal in 1783.
Variable stars had been discovered by
David Fabricius (1564-1617) nearly 200 years before in the year 1596.
Algol, means
"blinking demon."

John Goodricke's, journal entry November 12, 1782 reads:
"This night looked at
Beta-Persei (Algol) and was much amazed to find its brightness altered. It now
appears to be fourth magnitude... I observed it diligently for about an hour
upwards...hardly believing that it changed its brightness, because I had never
heard of any star varying so quick in its brightness. I thought it might be
perhaps owing to an optical illusion, a defect in my eyes or bad air, but the
sequel will show that its change is true and that it was not mistaken."
York Minster, England  
218 YBN
[1782 AD]
2134)
Birmingham, England  
218 YBN
[1782 AD]
2148)
Birmingham, England (presumably)  
218 YBN
[1782 AD]
2149) Watt describes this invention as "one of the most ingenious, simple
pieces of mechanism I have contrived".
Birmingham, England (presumably)  
218 YBN
[1782 AD]
2190) Tellurium's electron configuration is:
1s22s22p63s23p63d104s24p64d105s25p4

Tellurium is occasionally found uncombined in nature but is more often found
combined with metals, as in the minerals calaverite (gold telluride) and
sylvanite (silver-gold telluride).
Transylvania, Romania (was Hungary at time)  
218 YBN
[1782 AD]
2202) Hydrogen cyanide is highly toxic because it inhibits cellular oxidative
processes.
Köping, Sweden (presumably)  
218 YBN
[1782 AD]
2220)
Paris, France (presumably)  
218 YBN
[1782 AD]
3387)
Red Clay Creek, Delaware, USA  
217 YBN
[05/26/1783 AD]
2076) The is a problem in thinking a star is so massive that particles of light
would return to it, because they would not have sufficient velocity to leave it
to begin with. But even if true that some matter was so large that even
particle of light from a distance would be attracted to it, that presumes that
the most dense matter possible can produce a gravity strong enough to trap a
light particle. This idea of a mass so large that particles of light attach to
it, and cannot escape seems unlikely to me, but of course it cannot be ruled
out. If true, in the visible universe we would notice light beams all bend to
the large unseen influential masses, there would be large spaces with no light.
On earth, we don't see light bend in any direction, light particles appear to
move in the direction they exit from, for example from a flash light. I reject
the idea of black-holes as unlikely because time dilation is probably wrong, as
is a space-time geometry where time is not the same everywhere, and I doubt
that there can be a center of mass so large that even particles of light cannot
escape because probably photons cannot be compressed that tightly, and even if
they were, that might not be enough mass to stop photons from escaping, because
photons take up space, and as a mass grows, it's radius grows, so incoming
photons will always be at a distance from the center of mass, and be more
effected by the outer mass because it is closer. I want to run some simulations
of this. In addition, just to give an idea of how backwards science is right
now, we do not even have an estimate of the mass of a photon, it's absurdly
backward at least publicly. It's interesting also that Michell appears to be
one of those people, right after Newton, who were filling in the blanks that
Newton left out, such as the consequences of light corpuscles obeying the laws
of gravity. This path started in a good direction, but then apparently was sent
astray in the 1800s by the wave theory with an aether medium of light.
Thornhill, Yorkshire, England  
217 YBN
[06/04/1783 AD]
2192) In Paris the Montgolfier brothers fly six miles before a crowd of 300
which includes Benjamin Franklin.
The Montgolfiers are the sons of a paper manufacturer.

Of the brothers, only Michel will actually fly in the balloon, making an ascent
of 3000 feet with seven other people in 1784.
Annonay, France  
217 YBN
[07/15/1783 AD]
2206) Steamboat.

The ship moves upstream with a speed of six miles per hour, in the presence of
thousands of enthusiastic spectators.

Before the pyroscaphe d'Abbans had constructed an experimental boat, and ran it
on the River Doubs during June and July, 1776. The system he used then was the
palmipede, or web-foot, which proved unsatisfactory.
Saône River, near Lyon, France  
217 YBN
[08/27/1783 AD]
2264) Charles confirms Benjamin Franklin's electrical experiments.
Paris, France (presumably)  
217 YBN
[10/15/1783 AD]
2193)
Paris, France  
217 YBN
[11/21/1783 AD]
2194) Human flight by balloon.
During the 25-minute flight using a Montgolfier hot air
balloon, the two travel 12 kilometers from the Château de la Muette to the
Butte-aux-Cailles, then in the outskirts of Paris, attaining an altitude of
3,000 feet.

On June 15, 1785 De Rozier and his companion, Pierre Romain, will be killed
when trying to cross the English channel in a balloon.
Paris, France  
217 YBN
[1783 AD]
1207)
England  
217 YBN
[1783 AD]
1220) Benjamin Rush (December 24, 1745 - April 19, 1813), a US physician and
signer of the Declaration of Independence is an early opponent of slavery and
capital punishment. Rush is on the faculty of the first medical school in
America, "College of Philadelphia", founded in 1765. In the Pennslyvania
psychiatric hospital, Rush does replace the hay beds with hair mattresses,
however he brutally assaults and tortures people under the excuse of
experimentation and treatment. Rush, thinking insanity to be caused by
irregular movements of blood in the brain, bleeds humans. Rush writes that
"four-fifths of the blood in the body" should be taken. Other doctors call such
actions a "murderous dose", and a "dose for a horse". Rush writes "fear,
accompanied with pain and a sense of shame, has sometimes cured this disease".
Rush uses a spinning device called a "gyrator" to spin humans, thinking there
is increased blood flow in brain. Rush uses a "tranquilizer chair" to "cure"
"madness". In this chair a prisoner's arms, wrists and feet are strapped, their
head put in a wooden container, and a bucket is put beneath the chair for
excrement. Some humans are tied in this chair for hours, days, and even months.
The "gyrator" and "trainquilizer chair", used and promoted by Benjamin Rush,
will eventually be removed from Pennsylvania hospital, and viewed as an
instrument of abuse.

  
217 YBN
[1783 AD]
2114)
London, England  
217 YBN
[1783 AD]
2155) Watt (CE 1736-1819) defines the unit "horsepower" as 550 foot-pounds per
second, finding that a strong horse can raise a 150-pound weight nearly 4 feet
in a second. This unit of power is still used, however the metric system uses
the Watt in honor of James Watt. 1 horsepower=746 watts.

These rotary steam engines replace animal power, and it is natural that the new
engine should be measured in terms of the number of horses it replaces. By
using measurements that millwrights, who set up horse gins (animal-driven
wheels), have determined. Watt finds the value of one "horse power" to be equal
to 33,000 pounds lifted one foot high per minute, a value which is still that
of the standard American and English horsepower. The (cost) of erecting the new
type of (rotary) steam engine is therefore based on its horsepower.

Birmingham, England (presumably)  
217 YBN
[1783 AD]
2173)
France  
217 YBN
[1783 AD]
2183)
Slough, England  
217 YBN
[1783 AD]
2189)
Geneva, Switzerland (presumably)  
217 YBN
[1783 AD]
2221)
Paris, France (presumably)  
217 YBN
[1783 AD]
2227)
Paris, France (presumably)  
217 YBN
[1783 AD]
2242)
Paris, France (presumably)  
217 YBN
[1783 AD]
2287) Asimov states that Caroline Herschel is the first female of record to
contribute findings to astronomy. It seems possible that Hypatia may have made
astronomical contributions too.
Caroline herschel does not receive a formal
education.
Herschel leads a harsh life until her brother William invites her to live with
him in Bath, England. Herschel's mother requires William to give her funds to
retain a maid before allowing Caroline to leave.
In Bath, Caroline enrolls in
voice lessons and learns to play the harpsichord, soon becoming an integral
part of William's musical performances at small gatherings.
Both Caroline and William are
musicians and give their last public musical performance in 1782, when William
accepts the private office of court astronomer to George III.
Caroline helps grind
and polish mirrors.
Caroline Herschel executes many of the astronomical calculations
(for) William.
Herschel uses a telescope her brother William built for her.
When William
marries, the two women become good friends.
In 1787 the king (of England) gives Caroline
an annual pension of £50 (to work) as her brother's assistant.
This appointment makes
Caroline Herschel the first female in England to be honored with a government
position.
In 1828, at the age of 75, the Royal Astronomical Society awards Herschel a
gold medal for her monumental works in science. Ten years later, in 1838
Carloine Herschel is made an honorary member of the Royal Astronomical
Society.
On her 96th birthday, Herschel is awarded the gold medal of science by the King
of Prussia.
Herschel dies at age 97.

(Perhaps in someway, at this time female humans, certainly in England, were
becoming less inhibited and obstructed from social and legal equality.)
Datchet, England  
217 YBN
[1783 AD]
2311) There are some reports but no evidence that parachutes were used for
amusement in the 1100s CE.

Apparently Lenormand views parachute as way for people trapped in burning
buildings to leap to safety.
?, France  
217 YBN
[1783 AD]
2320) Fausto D'elhuyar writes several volumes on mineralogy and coining.
Vergara, Spain  
217 YBN
[1783 AD]
5962)
Vienna, Austria (presumably)  
217 YBN
[1783 AD]
5964)
Vienna, Austria (verify)  
216 YBN
[01/15/1784 AD]
2115) Cavendish concludes (wrongly) that dephlogisticated air (oxygen) is
dephlogisticated water and that hydrogen is either pure phlogiston or
phlogisticated water.
Cavendish reported these findings to Joseph Priestley, English
clergyman and scientist, no later than March 1783, but does not publish them
until the following year.

The Scottish inventor James Watt published a paper on the composition of water
in 1783; Cavendish had performed the experiments first but published second.
London, England  
216 YBN
[03/02/1784 AD]
2309) Jean Pierre François Blanchard (BloNsoR) (CE 1753-1809) and an American
physician John Jeffries are the first to float over the English Channel,
carrying the first airmail in history, landing near Calais.

In 1785 Blanchard successfully uses a parachute, dropping a dog (or cat) in a
basket attached to a parachute.

Louis-Sébastien Lenormand had demonstrated a parachute in 1783.
At age 16,
Blanchard constructs a kind of bicycle.
(Dover, England to) Felmores Forest, France.  
216 YBN
[1784 AD]
2152)
Birmingham, England (presumably)  
216 YBN
[1784 AD]
2180)
Datchet, England  
216 YBN
[1784 AD]
5967) (Johann Chrysostom) Wolfgang Amadeus Mozart (CE 1756-1791), Austrian
composer, composes Piano Concerto in F, k. 459.

Vienna, Austria (presumably)  
215 YBN
[01/07/1785 AD]
2310) Jean Pierre François Blanchard (BloNsoR) (CE 1753-1809) and American
physician John Jeffries to cross the English Channel in the air, carrying the
first airmail in history, landing near Calais.
Blanchard throws a dog in a
basket attached to a parachute (which lands unhurt). Later Blanchard will
parachute himself too.
Blanchard tries to use sails to help with propulsion and
steering in balloons. (It seems like sails would work for adding propulsion and
steering control.)

At age 16 Blanchard constructs a kind of bicycle.
Blanchard works on the design of
heavier-than-air vehicles in the 1770s including one vehicle that uses rowing
in the air with oars and tiller.
Blanchard takes up ballooning after the
Montgolfier brothers hot-air-balloon demonstrations in Annonay, France, in
1783.
Blanchard is the first to make balloon flights in England, North America,
Germany, Belgium, and Poland.

Calais, France  
215 YBN
[02/12/1785 AD]
2878)
(Chatham-Place) London, England (presumably)  
215 YBN
[02/17/1785 AD]
3463) Horace Richards writes that se was looked upon by fellows as, after
Franklin, the foremost scientist of the country. His abilities were
highlesteemed abroad, though, as has been seen, the recognition was limited to
his astronomical work. On the death of Franklin he was at once elected to the
presidency of this (the American Philosophical Society), and when six years
later he passed away at the age of sixty-four, his successor, Thomas jefferson,
in accepting the same office summed up his character in the words; "Genius,
Science, modesty, purity of morals, simplicity of manners, marked him one of
Nature's best samples of the Perfection she can cover under the human form.
Surely, no Society, till ours, within the same compass of time, ever had to
deplore the loss of two such members as Franklin and Rittenhouse.".
Philadelphia, Pennsylvania, USA  
215 YBN
[04/??/1785 AD]
2184)
Datchet, England  
215 YBN
[06/02/1785 AD]
2116) Air is shown to be a mixture of gases, and not a single element.

Henry Cavendish (CE 1731-1810) shows, by sparking air to make nitric acid, that
air is a mixture of gases, not a single element as was thought. Cavendish is
the first to recognize that air is composed of around 4 parts nitrogen (at the
time called "phlogisticated air") to 1 part oxygen (at the time called
"dephlogisticated air"). The current estimate is 78% nitrogen and 21% oxygen.
In
addition Cavendish observes that air contains a small volume of gas (1/120)
that is not nitrogen or oxygen. This will be shown to be argon and other inert
gases over 100 years later in 1895 by Rayleigh and Ramsay.
Cavendish observes that,
when he had determined the amounts of phlogisticated air (nitrogen) and
dephlogisticated air (oxygen), there remained a volume of gas amounting to
1/120 of the original volume of common air.

Cavendish writes "In Dr. Priestley's last volume of experiments is related an
experiment of Mr. Warltire's in which it is said that, on firing a mixture of
common and inflammable air by electricity in a closed copper vessel holding
about three pints, a loss of weight was always perceived, on an average about
two grains, though the vessel was stopped in such a manner that no air could
escape by the explosion. (ULSF: Perhaps this could be explained as mass lost
from photons emitted from the reaction in infrared and radio frequency.) It is
also related, that on repeating the experiment in glass vessels, the inside of
the glass, though clean and dry before, immediately became dewy; which
confirmed an opinion he had long entertained, that common air deposits its
moisture by phlogistication. As the latter experiment seemed likely to throw
great light on the subject I had in view ("throw great light" may hint at the
private view that all matter is made of light- and "subject" of the monarchy
which may limit the flow of truth to the public), I thought it well worth
examining more closely. The first experiment also, if there was no mistake in
it, would be very extraordinary and curious; but it did not succeed with me;
for though the vessel I used held more than Mr. Warltire's namely, 24,000
grains of water, and though the experiment was repeated several times with
different proportions of common and inflammable air, I could never perceive a
loss of weight of more than one-fifth of a grain, and commonly none at all. It
must be observed, however, that though there were some of the experiments in
which it seemed to diminish a little in weight, there were none in which it
increased. (*Dr. Priestley, I am informed, has since found the experiment not
to succeed)"
Cavendish uses inflammable air (hydrogen) from zinc for these experiments
and goes on to find no change in weight from inflammable air produced from
iron.
Cavendish starts from an experiment, narrated by Joseph Priestley, in which
John Warltire uses electrolysis (passing an electric current through a
substance to cause a chemical change), by (burning) a mixture of common air and
hydrogen by electricity, with the result that there the volume of air is
lowered and moisture is deposited. Cavendish fires, by electric spark, a
mixture of hydrogen and oxygen (dephlogisticated air), and finds that the
resulting water contained nitric acid, which he argued must be due to the
nitrogen present as an impurity in the oxygen ("phlogisticated air with which
it {the dephlogisticated air} is debased"). {ULSF: Does electrode material not
contaminate the reaction?}
Cavendish then proves this theory correct by passing sparks
through (plain) air forcing (in modern terms) the nitrogen to combine with the
oxygen and dissolving the resulting oxide {ULSF: on the electrode?} in water.
Cavendish proves that air is made of nitrogen by showing that when electric
sparks are passed through common air there is a shrinkage of volume because of
the nitrogen uniting with the oxygen to form nitric acid. Cavendish therefore
understands the composition of nitric acid. Adding more oxygen, Cavendish
expects to use up all the nitrogen, however a small bubble of gas, amounting to
less than 1 per cent of the whole, always remains uncombined. Cavendish
speculates that air contains a small quantity of a gas that is very inert and
resistant to reaction. We now know that this remaining part of air contains
Argon (and the other inert gases). This experiment will not be used for a
century until Ramsey repeats it in the 1890s. Michael Faraday will create laws
that describe electrolysis in 1832.

One way of describing this is that Cavendish performs the opposite of
"electrolysis" (using electricity to split a molecule into two or more parts),
which might be called "electrofusion", and defined as using electricity to join
two or more parts to form a molecule.

In showing both air and water not to be single elements, as was believed around
the time of Pythagoras, Cavendish takes science a large step forward in
improving on a theory that is more than two thousand years old. This work helps
to pull science away from an ancient and traditional mind-set.
London, England  
215 YBN
[1785 AD]
1239)
England  
215 YBN
[1785 AD]
1240)
England  
215 YBN
[1785 AD]
2083) Hutton is called the father of geology.
Edinburgh, Scotland  
215 YBN
[1785 AD]
2107)
Pavia, Italy (presumably)  
215 YBN
[1785 AD]
2132)
Birmingham, England  
215 YBN
[1785 AD]
2167)
Paris?, France (presumably)  
215 YBN
[1785 AD]
2168) Charles Augustin Coulomb (KUlOM) (CE 1736-1806) shows that electrical and
magnetic attraction and repulsion are both proportional to amount of charge and
inversely proportional to distance squared.

This will eventually lead to the famous equation now called Coulomb's law:
F=kq1q2/r^
2 (state who is the first to formally state this equation)

The quantity of electric charge will be named in honor of Coulomb.

In this equation F is the force in Newtons between two charged objects, k is a
constant which depends on the medium in which the charged bodies are immersed,
q1 and q2 are the two charges in Coulombs, and r is the distance in meters
between the centers of the two charged objects. k in a vacuum equals 8.98 x
10^9 Nm^2/C^2 Newton-meters squared per coulombs squared.

Coulomb never explicitly states this relationship in the formal equation that
will be first created by ?.

This view implies to many that there exists a force of electricity, which is
similar to, but different from a force of gravity.
Paris?, France (presumably)  
215 YBN
[1785 AD]
2197)
  
215 YBN
[1785 AD]
2259) Monge is a close friend of Napoleon, and accompanies Napoleon to Egypt in
1798.
Monge serves on the committee of weights and measures that establishes the
metric system in 1791.
Monge publishes "Géométrie descriptive" (1799, "Descriptive
Geometry") and "Application de l'analyse à la géométrie" (1807,
"Applications of Analysis to Geometry").
Following Napoleon's fall from power in 1815 and
the restoration of monarchy, the Bourbons exclude Monge from the French Academy
and deprive Monge of all his honors.
  
215 YBN
[1785 AD]
2271) Berthollet wrongly thinks chlorine is a compound and contains oxygen.

Finding no oxygen in the acids prussic acid or hydrogen sulfide, Berthollet
(correctly) remains skeptical about Lavoisier's theory of acidity as the result
of oxygen.
It has to be fun to find out what some compound substance is made
of.

In 1798, while in Egypt on a business trip, Berthollet meets Napoleon and
teaches Napeleon chemistry. Napoleon makes Berthollet a senator and a count. In
1806 Napoleon also bails Berthollet out with a considerable loan. In 1814
Berthollet signs the Senate's bill deposing Napoleon after Napoleon's defeat at
the Battle of Waterloo.

Proust will prove Berthollet wrong in the view that the composition of products
of a reaction vary with the masses of the reagents.

Berthollet is wrong in viewing heat as a fluid, in opposition to the more
accurate theory of Rumford.
Paris, France (presumably)  
215 YBN
[1785 AD]
2275)
Paris, France (presumably)  
215 YBN
[1785 AD]
2983) In 1773, Nairne had produced a electrostatic generator that could produce
13-inch sparks which Franklin thought promising.
Haarlam, Netherlands  
215 YBN
[1785 AD]
5968)
Vienna, Austria (presumably)  
214 YBN
[12/07/1786 AD]
2960)
London, England (probably)  
214 YBN
[1786 AD]
1209) Winnowing was also done manually by taking a basket of mixed grain and
chaff, or using a winnowing fork on a pile of harvested grain and tossing the
contents into the air, causing the chaff to blow away while the heavier grains
fall back into the basket or ground.
East Lothian, Scotland, United Kingdom  
214 YBN
[1786 AD]
1987)
Philadelphia, Pennsylvania (presumably)  
214 YBN
[1786 AD]
2135)
Birmingham, England  
214 YBN
[1786 AD]
5965)
Vienna, Austria (verify)  
213 YBN
[05/10/1787 AD]
2988) Bennet writes "The experiment which proves that the electricity is
doubled by each operation is this. if the two flips of pendulous leaf gold of
the electrometer be made to diverge to a certain distance by the above process,
that distance will be nearly doubled by repeating the operation. Another proof
of this duplicate accumulation is, that, when the third plate is applied to the
first, the divergency of the leaf gold is apparently undiminished, though in
this situation their electricity is diffused over double the quantity of
surface."
London, England (probably)  
213 YBN
[08/22/1787 AD]
2205) Fitch demonstrates this ship on the Delaware river before a group of
delegates to the Constitutional Convention.
Fitch goes on to built a larger
steamboat to carry passengers and freight. Propelled by paddle wheels, this
ship makes regularly scheduled trips between Philadelphia and New Jersey can
move 8 mi (12.9 km) per hour.
Fitch began to build another steamboat, but its loss in
a storm discouraged his funders.
Little popularity of steam-powered travel with the
public, combined with constant mechanical troubles and uncertain financial
backing, results in the failure of Fitch's business.
  
213 YBN
[08/27/1787 AD]
2265)
Paris, France (presumably)  
213 YBN
[12/13/1787 AD]
3252)
Derby, England (presumably)  
213 YBN
[1787 AD]
2171) A few phlogistonists object to the new system.
Paris, France (presumably)  
213 YBN
[1787 AD]
2178)
Old Windsor, England (presumably)  
213 YBN
[1787 AD]
2272) Potassium chlorate KClO3 is a poisonous crystalline compound that is used
as an oxidizing agent, a bleach, and a disinfectant and in making explosives,
matches, and fireworks.
Paris, France (presumably)  
213 YBN
[1787 AD]
2276) So Laplace explains that the Moon's mean motion is accelerated as long as
the Earth's orbit (around the Sun) tends to become more circular, but when (the
Earth's orbit around the Sun tends to become more elliptical) the reverse
occurs, the Moon decelerates. The inequality is of a period running into
millions of years therefore removing the threat of instability.
Paris, France (presumably)  
213 YBN
[1787 AD]
2288) Caroline Herschel is the first woman to discover a comet.
Datchet, England  
213 YBN
[1787 AD]
2325)
Wittenberg, Germany (presumably)  
213 YBN
[1787 AD]
2665)
Madrid (y Aranjuez), Spain  
213 YBN
[1787 AD]
5966)
Vienna, Austria (presumably)  
212 YBN
[06/05/1788 AD]
2989) (It seems like there must be some balancing between particles on the
Earth and those on smaller insulated objects. Perhaps the source of particles
or electric potential from Earth is larger than that insulated on a small
object.)
London, England (presumably)  
212 YBN
[06/21/1788 AD]
1529)
New Hampshire, USA  
212 YBN
[06/26/1788 AD]
5961)
Vienna, Austria (verify)  
212 YBN
[06/26/1788 AD]
5963)
Vienna, Austria (verify)  
212 YBN
[1788 AD]
1228) There are at this time 22 privately owned psychiatric hospitals in
London.

  
212 YBN
[1788 AD]
1229) The Queen of England calls on Francis Willis to cure King George III of
"madness". Willis thinks George must be broken like a horse and is put in a
straight waist coat, legs tied to a bed, blisters made on the legs, bled with
leeches, and emetics are added to his food.

London, England  
212 YBN
[1788 AD]
2015)
Bern, Switzerland (presumably)  
212 YBN
[1788 AD]
2150)
Birmingham, England (presumably)  
212 YBN
[1788 AD]
2163) This book is typically analytic. Lagrange writes in his preface that "one
cannot find any figures in this work".
This work is published 101 years after Isaac
Newton's "Principia" (1687).
Lagrange is the first to suggest that a description of
mechanical motion can be accomplished in terms of a geometry of four
dimensions.(Four dimensions is more easily understood as simply 4 variables.)
Paris, France  
212 YBN
[1788 AD]
5969)
Vienna, Austria (presumably)  
212 YBN
[1788 AD]
5983) (Johann Chrysostom) Wolfgang Amadeus Mozart (CE 1756-1791), Austrian
composer, composes his 41st Symphony "Jupiter" (k. 551).

Jupiter is the last symphony that Mozart composes. (verify)

The name of the symphony of "Jupiter" apparently dates from the early 1800s
according to Encyclopedia Britannica.

(This seems to be a transition from the very Christian music of Bach to more of
a polytheistic and perhaps scientific song title and theme.)



(It's interesting to think about what Mozart might have composed in his later
life, had he not died at so young an age.)

Vienna, Austria (presumably)  
211 YBN
[06/25/1789 AD]
2984)
London, England (presumably)  
211 YBN
[08/28/1789 AD]
2181)
Slough, England  
211 YBN
[1789 AD]
2177)
Slough, England  
211 YBN
[1789 AD]
2185)
Slough, England  
211 YBN
[1789 AD]
2222)
Paris, France (presumably)  
211 YBN
[1789 AD]
2230) Klaproth is an apothecary (one who prepares and sells drugs or compounds
for medicinal purposes) for many years.
In 1792 Klaproth becomes lecturer in chemistry
at the Berlin Artillery School.
Klaproth will be chosen to be professor of chemistry at
the newly founded University of Berlin in 1810.

Klaproth is an early convert to Lavoisier's theory of oxygen combustion, which
is good since Stahl who created the phlogiston theory was German (and national
or racial prejudice may have impeded acceptance of the more accurate theory).

In addition to more than 200 papers, Klaproth publishes a five-volume chemical
dictionary with F.B. Wolff (1807-10) and a four-volume supplement (1815-19).

Uranium is a heavy silvery-white metallic element, radioactive and toxic,
easily oxidized, and has 14 known isotopes of which U 238 is the most abundant
in nature. The Uranium atom occurs in several minerals, including uraninite and
carnotite.

Uranium is symbol U, atomic number 92; atomic weight 238.03; melting point
1,132°C; boiling point 3,818°C; relative density (specific gravity) 18.95;
and can have a valence of 2, 3, 4, 5, 6.
An isotope of uranium, uranium 235, is
(fissionable, splittable and is) the main fuel for nuclear reactors and atomic
bombs.
Eugene M. Péligot will isolate the element in 1841.
Berlin, (was Prussia) Germany (presumably)  
211 YBN
[1789 AD]
2231) The actual zirconium metal will be isolated in 1824 in impure form by the
Swedish chemist Jöns Jacob Berzelius.
The impure metal, even when 99 percent pure, is
hard and brittle. The white, soft, malleable, and ductile metal of higher
purity will be first produced in quantity in 1925 by the Dutch chemists Anton
E. van Arkel and J.H. de Boer.
Zirconium is highly transparent to neutrons.

Zirconium is symbol Zr; atomic number 40; at. wt. 91.22; m.p. about 1,852°C;
b.p. 4,377°C; rel dens. (sp. gr.) 6.5 at 20°C; valence +2, +3, or +4.
Berlin, (was Prussia) Germany (presumably)  
211 YBN
[1789 AD]
2269) This paper Jussieu submits to the Académie des Sciences is his first
publication.
Jussieu's paper reexamines the taxonomy of the Ranunculaceae (crowfoot).
Jussieu's uncle
Bernard first identifies sea anemones and related creatures as animals instead
of plants.
Paris, France  
211 YBN
[1789 AD]
2270) Jussieu's uncle Bernard first identifies sea anemones and related
creatures as animals instead of plants.
Paris, France  
210 YBN
[1790 AD]
1198)
England  
210 YBN
[1790 AD]
2077) It's amazing how little info there is on Michell, and not even a
portrait.

He is described by a contemporary as:
"John Michell, BD is a little short Man, of a
black Complexion, and fat; but having no Acquaintance with him, can say little
of him. I think he had the care of St. Botolph's Church Cambridge, while he
continued Fellow of Queen's College, where he was esteemed a very ingenious
Man, and an excellent Philosopher. He has published some things in that way, on
the Magnet and Electricity."
(Cole MSS XXXIII, 156, British
Library).
Thornhill, Yorkshire, England (presumably)  
210 YBN
[1790 AD]
2151)
Birmingham, England (presumably)  
210 YBN
[1790 AD]
2153) The Watt (CE 1736-1819) engine has completely replaced the Newcomen
engine by this time.

Birmingham, England (presumably)  
210 YBN
[1790 AD]
2191) Not until Boucher 50 years later will such finds be no longer ignored.
Hoxne, Suffolk, England  
210 YBN
[1790 AD]
2198) Leblanc is unable to provide enough money for his family on the medical
fees he obtains as a surgeon from his patients, and so in 1780 accepts a
position as the private physician to the household of the Duke of Orleans,
later known as the revolutionary figure Philippe Egalite who will be beheaded
in 1793.

The Duke agrees to fund Leblanc's research into a chemical method to convert
salt to soda ash, on the condition that Darcet, a longtime consultant to the
Duke, be included in the process. Leblanc is allowed to set up a laboratory at
the College of Paris, and Darcet assigns J. Dize, his assistant, to collaborate
with Leblanc.

This happens during the French Revolution, and the government awards Leblanc a
15-year secret patent in September 1791 but confiscates his patent and factory
three years later with only a small compensation. In addition the government
forces Leblanc to make public his method. (My own view is of course that there
should be no secrets, in particular in science, but that we should respect and
celebrate inventors and all smart people.) Napoleon will return the factory to
Leblanc around 1800 however Leblanc cannot raise enough capital to reopen it
and takes his own life in 1806.
Paris, France  
210 YBN
[1790 AD]
2297)
Göttingen, Germany{2 presumably}  
210 YBN
[1790 AD]
2305)
London, England (presumably)  
210 YBN
[1790 AD]
2322)
Montpellier, France (presuambly)  
210 YBN
[1790 AD]
2876)
Halle, Germany (presumably)   
210 YBN
[1790 AD]
3269)
England  
209 YBN
[05/03/1791 AD]
1530)
  
209 YBN
[12/15/1791 AD]
1531)
Virginia, USA  
209 YBN
[1791 AD]
1230) Hannah Mills, a quaker woman, dies of ill treatment and neglect at the
York asylum and this leads William Tuke (March 24, 1732 - 1822), an English
businessman and philanthropist and other quakers to build "The Retreat at
York", to implement a more humaine process for quakers viewed as "mentally
ill". The success of this business leads to more stringent legislation in the
interests of those diagnosed with mental diseases. This is a positive step on
the long road to removing the inhuman torture of restraining people to beds
with less movement than a cage provides, and any kind of involuntary treatment,
in particular drugging or coercing to take drugs (or so-called "meds").

York, England  
209 YBN
[1791 AD]
2175) Remote neuron activation (remote neuron writing). Muscle contracted
remotely by using an electric spark and metal connected to a nerve.

Galvani makes an electric pendulum using a frog leg, brass hook and silver
box.

Imagine Galvani's scalpel reduced in size to the size of a dust fiber, about 1
micrometer, and capable of photon communication can can be swallowed or even
breathed in, and then remotely communicated with, and moved around inside a
body, made to activate a neuron, or to attach to a bacterium, perhaps to enter
a cell and function as the first human-made cellular organelle.

Although the use of the scalpel might be interpreted as direct neuron
activation, this is a very similar process to a small electronic device inside
a body that receives remotely produced photons to directly activate a neuron.

Jan Swammerdam had made frog muscle contracted using two different metals in
1678.
Early, in Bologna, Floriano Caldani in 1756 and Giambattista Beccaria in 1758
had demonstrated electrical excitability in the muscles of dead frogs.
Later an
unknown person will focus this principle of remote nerve stimulation to
individual nerves without the need for a metal conductor attached to the nerve.
When this happens is also unknown, perhaps this invention must wait for the
laser. The earliest evidence I am aware of for this remote conductor-less
stimulation, is probably the use of the word "suggest" by Felix Savery in 1826,
and Andre Ampere in 1827, who uses the French form of "suggest" and "muscle
contraction" in the same sentence. This remote neuron activation may advance to
making an individual neuron fire even as far back as the 1800s, and still is a
secret from the public.

Luigi Galvani (GoLVonE) (CE 1737-1798) publishes the results of his using
electricity to make frog leg muscles contract in "De Viribus Electricitatis in
Motu Musculari Commentarius" ("Commentary on the Effect of Electricity on
Muscular Motion").

Luigi Galvani (GoLVonE) (CE 1737-1798) finds that twitching of frog muscles can
occur during a lightning storm or with the aid of an electrostatic machine, but
can also occur with only a metallic contact between leg muscles and the nerves
leading to them. Galvani finds that two different specific kinds of metals
connected together connecting the nerves and the muscle connected to the nerve
can serve as a substitute for the electrostatic machine.

Galvani has found the basic design of an electrical battery, but wrongly
concludes that the electricity comes from the from leg as "animal electricity".
Alessandro Volta will prove that the electricity comes from the metal several
years later.

This find will form the basis of and lead directly to the first electric
battery (voltaic pile) by Volta in 1800 and to the remote contraction of
muscles, by whom, when and where is still unknown to the public.

Galvani wrongly concludes that animal tissue contains an "animal electricity",
that activates nerve and muscle when metal probes connect nerve and muscle
causing muscle to contract. Galvani supposes that this electricity is different
from the "natural" electricity of lightning or eels, and the "unnatural"
electricity from static electricity generating machines.

Galvani and Volta enter into a friendly disagreement, Galvani supporting his
view of animal electricity, with Volta holding the view that the two different
metals are the source of electricity, calling it "metallic electricity".

Galvani and Volta will be shown to be both partly right and partly wrong.
Galvani is correct in attributing muscular contractions to an electrical
stimulus but wrong in identifying it as an "animal electricity." Volta is
correct in denying the existence of an "animal electricity" but is wrong in
implying that every electrophysiological effect requires two different metals
as sources of current.

Galvani is influenced by Franklin's "one fluid theory", where electrical
phenomena are thought to be caused by an electric fluid that results in
positive electricity, while negative electricity is the absence of this fluid.
Franklin explained the Leyden jar as accumulating positive electricity on the
inner conductor while the outer conductor becomes negatively charged.

Galvani views the brain as the most important organ which secretes "electric
fluid" and views the nerves as conductors of the fluid to the nerve and muscle.
Galvani views the tissues of nerves and muscles as being analogous to the outer
and inner surfaces of the Leyden jar.

Galvani writes in "De Viribus Electricitatis" (translated from Latin):
" In my desire
to make that which, with no inconsiderable expenditure of pains, after many
experiments, I have succeeded in discovering in nerves and muscles, so far
useful that both their concealed properties might be revealed, if possible, and
we might be able more surely to heal their diseases, nothing seemed more
suitable for fulfilling such a wish than if I should simply publish my results,
just as they are, for general judgment. For learned and eminent scholars, by
reading my discoveries, will be able, through their own meditations and
experiments, not only to amplify and extend them, but also to attain that which
I indeed have attempted, but perhaps have not fully achieved.
It was also my
desire not to publish this work in a crude and barely incipient form, even
though not perfect and complete, which perhaps I should never have been able to
do. But since I realized that I had neither time nor leisure nor ability
sufficient to accomplish that, I preferred rather to fall short of my own very
reasonable desire than to fail the practical value of the work.
I thought,
therefore, that I should be doing something worth while, if I reported a brief
and accurate account of my discoveries and findings in the order and relation
in which partly chance and fortune presented and partly diligence and industry
revealed them to me; not so much lest more be attributed to me than to fortune,
or more to fortune than to me, but that either I might hand on a torch to those
who had wished to enter this same pathway of experiment, or might satisfy the
honest desire of scholars who are wont to be interested in things which contain
some novelty either in origin itself or in principle.
But to the description of the
experiments I will add some corollaries, and some conjectures and hypotheses,
primarily with this purpose, that I may smooth the way for understanding new
experiments, whereby, if we cannot attain the truth, at least a new approach
thereto may be opened. The affair began at first as follows:
Part One
THE EFFECTS OF
ARTIFICIAL ELECTRICITY ON MUSCULAR MOTION

I dissected and prepared a frog, as in
Fig. 2, Tab. I, and placed it on a table, on which was an electrical machine,
Fig. 1, Tab. 1, widely removed from its conductor and separated by no brief
interval. When by chance one of those who were assisting me gently touched the
point of a scalpel to the medial crural nerves, DD, of this frog, immediately
all the muscles of the limbs seemed to be so contracted that they appeared to
have fallen into violent tonic convulsions. but another of the assistants, who
was on hand when I did electrical experiments, seemed to observe that the same
thing occurred whenever a spark was discharged from the conductor of the
machine, (Fig. I, B).
He, wondering at the novelty of the phenomenon, immediately
apprised me of the same, wrapped in thought though I was and pondering
something entirely different, Hereupon I was fired with incredible zeal and
desire of having the same experience, and of bringing to light whatever might
be concealed in the phenomenon. Therefore I myself also applied the point of a
scalpel to one or other crural nerve at a time when one or other of those who
were present elicited a spark. The phenomenon always occurred in the same
manner: violent contraction in individual muscles of the limbs, just as if the
prepared animal had been seized with tetanus, were induced at the same moment
of time in which sparks were discharged.
But fearing lest these very motions arose rather
from the contact of the point, which perchance acted as a stimulus, than from
the spark, I again tested the same nerves in the same way in other frogs, and
even more severely, but without any spark being elicited at that time by
anyone; but no motions were seen at all. Hence it occurred to me that perhaps
for the induction of the phenomenon both the contact of some body and the
passage of a spark were simultaneously required. Wherefore I applied the edge
of the scalpel again to the nerves and held it motionless, both at the time
when a spark was being elicited and when the machine was perfectly quiet. but
the phenomenon appeared only when the spark was produced.
We repeated the
experiment, always employing the same scalpel; but not without our surprise,
sometimes, when the spark was produces, the aforesaid motions occurred,
sometimes they were lacking.
Aroused by the novelty of the circumstance, we resolved
to test it in various ways, and to experiment, employing nevertheless the same
scalpel, in order that, if possible, we might ascertain the causes of the
unexpected difference; nor did this new labor prove vain; for we found that the
whole thing was to be attributed to the different part of the scalpel by which
we held it with our fingers: for since the scalpel had a bone handle, when the
same handle was held by the hand, even though a spark was produced, no
movements resulted, but they did ensue, if the fingers touched either the
metallic blade or the iron nails securing the blade of the scalpel.
Now, since dry
bones possess a non-conductile, but the metallic blade and the iron nails a
conductile nature, we came into this suspicion, that perhaps it happened that
when we held the bony handle with our fingers, then all access was cut off from
the electric current, in whatever way it was acting on the frog, but that it
was afforded when we touched the blade or the nails communicating therewith.
Therefore,
to place the matter beyond all doubt, instead of a scalpel we used sometimes a
slender glass cylinder H, Fig. 2, wiped clean from all moisture and dust, and
sometimes an iron cylinder G. With the glass cylinder we not merely touched but
rubber the crural nerves, when the spark was elicited, but with all our effort,
the phenomenon never appeared, though innumerable and violent sparks were
elicited from the conductor of the machine, and at a short distance from the
animal; but it appeared when the iron cylinder was even lightly applied to the
same nerves and scanty sparks elicited.
...". Galvani goes on to describe numerous other
experiments. Having tested positive electricity, they test negative
electricity, concluding "...the same contractions were obtained, whether the
spark was elicited from the crook of the Leyden jar at the same time when the
said jar, as they say, was being charged, or in the same place in which it was
charged, or elsewhere, and far removed from the machine.". Galvani finds that
"These phenomena, moreover, occurred when the frogs were equipped not only with
a nerve-conductor, but merely with a muscle-conductor...". They contract the
frgo muscle through glass by containing the frog and conductor in a jar. They
test the crural nerve with a live frog exposing the crural nerve in the thigh
with the conductor applied and find that "...contractions ensued on the passage
of the spark in the corresponding leg alone, only less, as it seemed to us,
than in the dead animal.". Galvani confirms that the contraction works when the
frog is contained in a airless vacuum jar. Galvani writes "These experiments
were all performed in animals wihch are called cold-blooded. These things
having been tested and discovered, nothing was more in my desires than to
perform the same or similar experiments in warm-blooded animals, as for example
in hens and in sheep. The experiment having been tried, the result was the same
in the latter as in the former. but there was need of a different preparation
in the latter; for it was necessary first to expose the crural nerve, not
inside the abdomen, but externally in the thigh itself, and to separate it from
the other parts and bring it to the surface, than apply the conductor to it,
and then elicit the spark from the conductor of the machine, with the leg
either attrached to the living animal or resected from it as soon as possible;
for otherwise, if the customary manner of preparing frogs were employed, the
phenomenon was wholly lacking, perhaps because the power of self-contraction of
the muscles was lacking beforehand, which that long and complex preparation can
release.". Galvani concludes this section by writing:
" but indeed, in this kind of
experiments, whether in warm or in cold animals, there are some things at the
end, and these peculiar and, as I think, not unimportant to note, which never
presented themselves to us. One was that prepared animals were more suitable
for these phenomena, the more advanced they were in age, and also the whiter
their muscles were and the more they were deficient in blood, and therefore
perhaps the muscular contractions were propter and easier and could be excited
much longer in cold than in warm animals; for the former, in comparison with
the latter, have more dilute blood, more difficult to coagulate, and therefore
flowing much more easily from the muscles: another was that prepared animals,
in whom these electric experiments were undertaken, decay and rot much more
quickly than those who have suffered no electric force: finally that even if
the phenomena which we have described thus far as occurring did so in the way
we stated, animals prepared for experiment fail differently. For if the
conductors are applied not to the dissected spinal cord or to the nerves, as we
have been accustomed, but are applied or even attached to the brain or the
muscles, or if nerve conductors are extended or prolonged, or if nerves
according to custom are in the least detached from surrounding parts, the
contractions are wither none or very slight. Many accepted things certainly,
which we have discovered from these experiments, we refer chiefly to this
method of preparing and separating nerves.".

Galvani then writes "Part Two
THE EFFECTS OF ATMOSPHERIC ELECTRICITY ON MUSCULAR
MOTION
Having discovered the effects of artificial electricity on muscular
contractions which we have thus far explained, there was nothing we would
sooner do than to investigate whether atmospheric electricity, as it is called,
would afford the same phenomena, or not: whether, for example, by employing the
same devices, the passage of lightning, as of sparks, would excite muscular
contractions.
Therefore we erected, in the fresh air, in a lofty part of the house, a long
and suitable conductor, namely an iron wire, and insulated it, Fig. 7, and to
it, when a storm arose in the sky, attached by their nerves either prepared
frogs, or prepared legs of warm animals, as in Fig. 20, 21, Tab. IV. Also we
attached another conductor, namely another iron wire, to the feet of the same,
and this as long as possible, that it might extend as far as the waters of the
well indicated in the figure. Moreover, the thing went according to our desire,
just as in artificial electricity; for as often as the lightning broke out, at
the same moment of time all the muscles fell into violent and multiple
contractions, so that, just as the splendor and flash of the lightning are
wont, so the muscular motions and contractions of those animals preceded the
thunders, and, as it were, warned of them; nay, indeed, so great was the
concurrence of the phenomena that the contractions occurred both when no muscle
conductor was also added, and when the nerve conductor was not insulated, nay
it was even possible to observe them beyond hope and expectation when the
conductor was placed on lower ground, Fig. 8, particularly if the lightnings
either were very great, or burst from clouds nearer the place of
experimentation, or if anyone held the iron wire F in his hands at the same
time when the thunderbolts fell. ...". Galvani concludes by noting that
northern lights produces no contractions.

Galvani continues with "Part Three
THE EFFECTS OF ANIMAL ELECTRICITY ON MUSCULAR
MOTION
The effects of stormy atmospheric electricity having been tested, my heart
burned with desire to test also the power of peaceful, everyday electricity.

Wherefore, since I had sometimes seen prepared frogs placed in iron gratings
which surrounded a certain hanging garden of my house, equipped also with
bronze hooks in their spinal cord, fall into the customary contractions, not
only when the sky was lightning, but also sometimes when it was quiet and
serene, I thought these contractions derived their origin from the changes
which sometimes occur in atmospheric electricity. hence, not without hope, I
began diligently to investigate the effects of these changes on these muscular
motions in various ways. Wherefore at different hours, and for many days, I
inspected animals, appropriately adjusted therefor; but there was scarceley any
motion in their muscles. Finally, weary with vain expectation I began to press
the bronze hooks, whereby their spinal cords were fixed, against the iron
gratings, to see whether by this kind of device they excited muscular
contractions, and in various states of the atmosphere, and of electricity
whatever variety and mutation they presented; not infrequently, indeed, I
observed contractions, but bearing no relation to varied state of atmosphere or
of electricity.
Nevertheless, since I had not inspected these contractions except in the
fresh air, for I had not yet experimented in other places, I was on the point
of seeking such contractions from electricity of the atmosphere, which had
crept into the animal and accumulated in him and gone out rapidly from him in
contact of the hook with the iron grating; for it is easy in experimentation to
be deceived, and to think one has seen and discovered what we desire to see and
discover.
But when I had transported the animal into a closed chamber and placed him on
an iron surface, and had begun to press against it the hook fixed in his spinal
cord, behold the same contractions and the same motions! Likewise continuously,
I tried using other metals, in other places, other hours and days; and the same
result; except that the contractions were different in accordance with the
diversity of metals, namely more violent in some, and more sluggish in others.
Then it continually occurred to me to employ for the same experiment other
bodies, but those which transmit little or no electricity, glass for example,
gum, resin, stone, wood, and those which are dry; nothing similar occurred, it
was not possible to observe any muscular motions or contractions. Results of
this sort both brought us no slight amazement and began to arouse some
suspicion about inherent animal electricity itself. Moreover both were
increased by the circuit of very thin nervous fluid which by chance we observed
to be produced from the nerves to the muscles, when the phenomenon occurred,
and which resembled the electric circuit which is discharged in the Leyden jar.
...". Galvani prepares the frog on a hook fixed to its spinal cord and its feet
rest on a silver box. In this way, Galvani finds that, with one hand on the
frog and the other a metal object touching the silver box, the frog leg
contracts. Galvni then gets an assistant, and finds that with the assistant
holding the frog while Galvani touched the box again, there is no contraction.
However, a contraction does occur if their other hands are connected. Galvani
then describes his electric pendulum:
" ...if a frog is held in the fingers so
suspended by one leg that a hook fixed in the spinal cord touches a silver
surface and the other leg freely falls into the same plane, Fig. 11, Tab. III,
as soon as this same leg touches the surface itself immediately the muscles
contract, wherefore the leg rises and is drawn up, but soon relaxes of its own
accord and again falls to the surface, and as soon as it comes into contact
with it, is again elevated for the same reason, and so it continues thereafter
to rise and fall alternatively, so that, like an electric pendulum, the same
leg seems to imitate the other, not without admiration and pleasure on the part
of the beholder. ...". Galvani describes how using an arc or hook of iron and
conducting surface of iron, contractions either fail or are very scanty, but if
one is iron and the other bronze, or much more for silver, contractions will
occur continuously and far greater and far longer. Galvani confirms that
contractions occur even when the frog is immersed in water, but fails immersed
in oil. Galvani covers nerves with metal foil, "preferably of tin, no less than
the physicists are accustomed to accomplish in their magic square and Leyden
jar", Fig. 9, Tab. III, and finds that the muscular contractions grow much
stronger, so that even without an arc, but with a single contact of a body
either conducting or even non-conducting, these "armatured nerves", as Galvani
calls them contract the connected muscle. However, covering muscle in metal
foil causes no difference in contraction, nor for covering the denuded spinal
cord. Galvani finds that with the nerve and muscle removed from the body, that
far fewer contractions take place, however, that contractions arise far more
easily and promptly if the arc is applied to an armatured nerve. Galvani finds
that wrapping the nerves in insulation such as silk and then touching the nerve
with the arc causes no contraction. Galvani describes the way nerves share
electricity, finding that two nerves with the arc applied to one each cause
both connected muscles to contract. Galvani writes "...But perhaps nothing is
more suitable for demonstrating powers of cooperation than if the crural nerves
are prepared according to custom, and the spinal cord and head remain intact,
and the upper limbs intact in nature and position.
For then, if either the crural nerve
or the vertebral column is armatured, and the arc aplied partly to the
armatured part of the crural nerve and partly to the corresponding limb, not
only the lower limbs contract, but the upper ones move also, the eyelids move,
and other parts of the head move, so that on this account, the electric fluid,
aroused by nervous contact of the arc, for the most part flows from the
indicated place of the nerves to the muscles, but partly also through the
nerves seeks the higher regions and is carried as far as the brain, and seems
to carry such effect into it that thence, for whatever reason, motions of other
muscles are excited. Galvani writes:
" moreover, the experiments having been
performed, in birds and quadrupeds, not once but again and again, not only the
principal phenomena appeared, according to desire, as in cold-blooded animals,
namely frogs and turtles, but they both appeared more easily and were far more
conspicuous. it was possible also to observe this peculiarity in both the
living and the dead animal, Figs. 20 and 21, for example that in a lamb or a
chick, with a crural nerve dissected and covered with metal foil and extended
on an armatured glass surface, contractions were obtained without the device of
an arc, but solely by the contact of some conducting body with the same
surface; but they are never obtained when the nerve is extended on a metallic
surface, unless an arc is applied to the animal according to custom.".. Galvani
states his belief that "animal electricity, discovered by us, ... corresponds
not a little with common electricity.", and "...those who have devoted
themselves to this kind of experiments may the better recognize the use and
utility of the arc...".

Galvani dedicates his last chapter, part 4 to "CONJECTURES AND SOME
CONCLUSIONS". In this part, Galvani states numerous conjectures, theories and
ideas for future research. In particular Galvani argues in favor of "animal
electricity" as being different from common electricity. Volta is credited with
disproving this theory. Galvani writes:
"From what is known and explored thys far, I
think it is sufficiently established that there is electricity in animals,
which, with Bartholinus and others, we may be permitted to call by the general
name of animal electricity.". Galvani then goes on to theorize that two kinds
of electricity, positive and negative, cause muscle contraction. Galvani writes
"...it would perhaps be a not inept hypothesis and conjecture, nor altogether
deviating from the truth, which should compare a muscle fibre to a small Leyden
jar, or other similar electric body, charged with two opposite kinds of
electricity; but should liken the nerve to the conductor, and therefore compare
the whole muscle with an assemblage of Leyden jars.". Galvani theorizes on the
three different methods of contracting muscles: 1) from the internal surface of
a Leyden jar, 2) by an arc, and 3) by the production of a spark from an
electric machine. Galvani discusses the torpedo fish and how it can kill or
stupefy other bodies. Galvani writes "...but already we have shown above that
electric fluid is carried through the nerves of muscles; therefore it will be
carried through all: therefore from one common source, namely the cerebrum,
they will drain it, from the source and origin of all: for otherwise there
would be as many sources as there are parts in which nerves terminate; and
although these are very different in nature and construction, they do not seem
suited for the elaboration and secretion of one and the same fluid.
Therefore
we believe it equally true that electricity is prepared by action of the
cerebrum, and that it is extracted from the blood, and that it enters the
nerves, and that it runs through them within, whether they are hollow and free,
or whether, as seems more probable, they carry a very thin lymph, or some other
peculiar similar thin fluid, secreted, as many think, by the cortical
cerebrum.". Galvani distinguishes between voluntary and involuntary motions.
Galvani tries to explain how a spark can cause a muscle contraction writing:
"For at the passage of a spark, electricity breaks out both from the layers of
air surrounding the conductor of the machine and from the nerve-conductors
communicating with the same layers; and negative electricity results on account
of them. Hence the intrinsic positive electricity of muscles runs to the nerves
both with its own strength and with strength from extrinsic electricity, more
abundant whether you borrow it from artificial or natural, as received from
their conductors, and flowing through them, failing both in them and in the
shortly hirtherto mentioned layers of air, it will renew the electricity and
establish itself at equilibrium therewith; not otherwise than as, in a Leyden
jar, the positive electricity of the internal surface in the production of a
spark flows more abundantly to the conductor of the former, for the same
reasons, and goes out therefrom, just as the form of a luminous electric pencil
openly declares.". Galvani suggests that just as electricity can damage a
nerve, possibly self generated electricity might damage a nerve. Galvani does
not explicitly mention the possibility of a person remotely causing a muscle to
move without having to touch the nerve directly, for example with a piece of
metal.

This work of Galvani's is really an epochal work. There are many sciences that
grow from this work. In particular, the very interesting science, of the
difference between life and death, and in particular the role of electricity in
living objects. Related to this, is the science of resuscitation and reviving
back to living a body that has been dead for a period of time. Beyond this is
the major science of using electricity to cause remote muscle contraction,
which develops secretly - it seems very likely, around the early 1800s. In
addition, is the science of radio communication - which involves his use of
electric induction which may be simply the photoelectric effect.

This technology of moving (human muscles) is the focus of much secret research.
Some time, perhaps around 1912, some person figured out how to remotely cause
neurons to fire. Who figured this out first is publicly not known, nor is the
location on earth where this was first found publicly known, not is the precise
method known. Possibly molecules in a neuron absorb certain frequencies of
photons, by making the molecule (which could be even the water molecule, but
may be more specific to neurons) absorb photons, the neuron may be made to
fire. Perhaps the neurons of squid were first used being much larger than the
neurons of other species.
When this process of making neurons fire remotely was
understood, many new possibilities were realized. In particular by remotely
causing the correct neuron to fire, any muscle in any body with a muscular
system can be made to contract.

Sadly, this technology is being terribly abused by the people, mostly
conservative military people who control it, to cause people's muscles to move
in ways which may cause them damage, for example, to cause a person to drive
off a road, or simply to murder people by stopping their lung or heart muscle.
Clearly the amazing potential of being able to control muscles from a distance
is a very powerful tool. This technology could be used to stop pain felt in
surgery without having to use anesthesia, to send images, sounds, and smells to
each other just by thought, to stop a person in the act of violence, for
example, many useful purposes. Ultimately this movement of muscles is a way a
person can possibly completely control all the thoughts and muscles of another
body. A person's body may be made to think and/or move in a way without any
choice. This secret technology opens many new ideas previously never thought
about. Sadly, as will be the case for seeing thought in 1910, and hearing
thought in 1911, uneducated, greedy, powerhungry wealthy people that control
the government and media will usurp this technology for themselves, continually
giving the excuse of "national security", and the advantage keeping the
technology secret from other people gives them. In addition, other major
excuses involve the financial panic or collapse that might happen if
information is freely exchanged by all people, that people will not be able to
"handle" the new reality of the machines and may seek to destroy or otherwise
limit the use of the technology. This remote neuron activation, image, sound
and muscle moving technology is probably one of the most important scientific
advances in the history of earth, and is one of the major science and
technology secrets of the early 1900s. Those include:
1: Detecting status of
neurons
1) Seeing the images the eyes see (October 25?, 1910, Michael I Pupin,
Columbia University, New York City, New York, USA)
2) Seeing the images the brain
generates (October 25?, 1910, Michael I Pupin, Columbia University, New York
City, New York, USA)
3) Hearing the sounds the ears hear (1911?, DP?, Columbia
University?)
4) Hearing the sounds the brain generates (1911?, DP?, Columbia University?)
5)
Detecting smells being smelled
6) Detecting tastes being tasted
7) Detecting touches being
felt
8) Detecting feelings of heat
9) Detecting feelings of pain (from neuron
receptors of pain sensors in skin)
10) Detecting movement of muscles
11) Detecting gland
activity
12) Detecting sexual stimulation

2: Remote Neuron activation (1912?, CIP?, Columbia? California?)
1) Sending images to
appear in front of eyes
2) Sending images to appear on internal thought screen
(the thought screen, a second screen used in the brain, where dreams are seen,
and internal visualizations are drawn, used to plant suggestions in people's
minds such as an image of a food product)
3) Sending sounds to be heard as if outside
body
4) Sending sounds to be heard as if from thoughts (used {many times as their
own voice} to plant suggestions in people's minds)
5) Sending smells
6) Sending tastes
(same neurons as smell?)
7) Sending touches (remotely activating nerve receptors in
brain that receive signals from touch sensors in skin)
8) Sending feeling of heat
(one of the few remote stimulations I have not felt to my knowledge)
9) Sending pain
10)
Sending muscle moves (to neurons that control muscle contraction)
11) causing glands to
secret hormones
12) causing sexual stimulation

3: public but used secretly: causing cancer with photons in microwave

4: secret networks of hidden microphones and cameras by telephone companies,
which must have developed to be microscopic perhaps even as early as 1920.

5: transmutation: forming different atoms, building atoms up using particles to
convert H to He, He to Li, Li, Be, C, N, ...Au, Ag, Converting common atoms
into useful atoms such as hydrogen and oxygen. Potentially making gold from
mercury through particle accelerators.

(State who is the first to clearly publish the possibility of a person moving
the muscles of another body remotely without having to touch the other body.
State any for both science publication, or science fiction.)

This will lead to the development of technology that can read from and write to
neurons, which will enable the remote recording of images of thought, the
sounds of thought, the images a brain sees, the sounds a brain hears, smells,
touches, tastes, and even the writing to neurons, perhaps with roentgen rays
(x-rays, or X particles), which allow a muscle to be contracted from a remote
distance using invisible particle beams.

This is one of the earliest reports of the phenomenon of the electric radiation
which will be the basis of wireless communication using light particles (one
form of which is radio).
Bologna, Italy  
209 YBN
[1791 AD]
2243)
Paris, France (presumably)  
209 YBN
[1791 AD]
2289) Dolomieu is a member of the order of Malta since infancy, and is pardoned
from a sentence of death at age 19 for killing a brother knight in a duel.
Dolom
ieu accompanies Napoleon to Egypt in 1798 and is captured and imprisoned on the
return (to France).
Alps, Northern Italy  
209 YBN
[1791 AD]
2290)
Alps, Northern Italy  
209 YBN
[1791 AD]
2295)
  
209 YBN
[1791 AD]
2342) An unknown mechanism in plants may use titanium to stimulate the
production of carbohydrates and encourage growth. This may explain why most
plants contain about 1 part per million (ppm) of titanium, food plants have
about 2 ppm and horsetail and nettle contain up to 80 ppm.
Cornwall, England  
209 YBN
[1791 AD]
2343) Richter publishes his measurement of how much of a given acid is required
to neutralize a given base in "Anfangsgriinden der Stochiometrie oder Messkunst
chemischer Elemente" (1792-94), and "Ober die neueren Gegenstande in der
Chemie" (1792-1802).
?, Germany  
209 YBN
[1791 AD]
2908)
Pressburg (Bratislava), Slovakia  
209 YBN
[1791 AD]
3380)
?, England  
209 YBN
[1791 AD]
5954)
Vienna, Austria (presumably)  
209 YBN
[1791 AD]
5970)
Vienna, Austria (presumably)  
208 YBN
[09/21/1792 AD]
1534)
Paris, France  
208 YBN
[1792 AD]
2164)
London, England (presumably)  
208 YBN
[1792 AD]
2232)
Berlin, (was Prussia) Germany (presumably)  
208 YBN
[1792 AD]
2251) This device is named a battery because any group of similar objects
working as a unit may be called a battery. Volta will improve on this device,
making things less messy, watery and more compact by using small round plates
of copper and zinc and discs of salt soaked cardboard.

(What kind of voltage and current can be produced by such a device, and what
voltages and currents did Volta measure with his devices?)
Pavia, Italy  
208 YBN
[1792 AD]
2254) I think the science of psychology needs to be made consensual treatment
only, no more people locked in hospitals without consent, and/or against their
objection. Just as no person should be allowed to remove a lung from a person,
no person should be able to drug or operate on another person without consent.
In other words, delusion must be legal. People must never be jailed for holding
beliefs or views different from the majority or in apparent disagreement with
observed reality.

Some clear changes needed are: 1) no tying to bed (restraints) or restricting a
person from bodily movement, no straight jackets 2) no lobotomies 3) no
electroshock, 4) no drugging, forced, or coerced. As always these things can be
done if a person consents and even then, my advice to people out there is to
object, and to presume that most average people do not want to be restrained.

I would define psychology as an experimental science that seeks to understand
and consensually-only try to solve problems of the brain for which the cause is
unknown, generally using methods such as consensual experimental drugs,
touching, talking, etc. I honestly think that more and more as we continue into
the future, psychology is going to be viewed as mostly pseudoscience in
particular once treatment is made consensual only by law, and neurology the
study of the physiology of the brain will probably be the legitimate science of
the brain and so-called mind which Pupin revealed is nothing more than the
remembering of images, sounds and other sensory data in addition to sequences
of muscle contractions.

Beyond this I would say that we should seek to make prisons for nonviolent
people, nice, clean and safe environments. We should focus on trying to show
people in prison where they are going wrong in violating laws, explain science,
evolution, atheism, and history to them, and to try to help them understand and
obey the laws using consensual-only methods. We should generally try to apply
consensual nonviolent honest methods to get people to obey laws, focusing on
locking violent people in jail as opposed to nonviolent people, although those
who repeat nonviolent crimes which are a nuisance to the majority should be
jailed for small amounts of time.

I can see a possible exception for a person with a communicable virus, bacteria
or protist that causes death, damage or severe and permanent illness, being
contained to a volume of space.

Unfortunately, what has happened is that the majority is imposing their beliefs
on to minorities by imprisonment, drugging and torture, and this was precisely
what the founders of freedom of religion sought to oppose. As is the case for
the military, in the psychiatric system, people should never be locked in a
hospital or prison without having violated a law, without an opportunity to
defend the charge against them, without receiving a democratic trial, without
receiving a sentence, and they should never be drugged, restrained or tortured.
It is wrong to jail a person simply because you think their beliefs are
unrealistic, or not based in fact. A perfect example are the religions, who
claims are clearly in contradiction to physical reality. Those people should
not be jailed simply for holding unrealistic beliefs, and the same is true for
those who have nonreligious inaccurate beliefs. One difficult aspect to accept
is when a person may be harming themselves. It is difficult to accept but since
a person must own their own body, they must be allowed to damage their own
body. This extends to drug addiction, to self mutilation, to suicide, to
starvation, to obesity, and similar forms of unhealthy or self hurting
activities. In such cases, it is my opinion that consensual-only help and
services may be provided, for example, providing starving people with food,
giving obese people advice in how to lose weight, helping to clean people's
rooms that choose not to clean them themselves, etc.

Currently, at this time there is a very frightening reality, and that is that
because of the psychiatric system that is in place, any person or group of
people can be locked in psychiatric hospitals indefinitely, without a trial,
with no appeals, no phone calls, nobody allowed to know where they are, and
that is a simple fact. People should realize that there are humans who have
been locked in psychiatric hospitals for years, some for decades, without ever
having violated any single law, never having received any trial, and what is
those people's crime? How many of them would like to be released? How many of
them broke a law but never went to jail? How many broke a violent law, but
didn't go to jail for it? All these questions should concern the average person
I think.

In addition, there is something highly unethical being done by those in the
psychiatric industry. When people can be locked in hospitals without having
violated a law, and taxpayers must pay, the psychiatric hospital owners are
guaranteed income by law. When people must be given psychiatric treatment by
law, the psychiatric doctors are guaranteed income, and when people are forced
by law to take drugs for the most trivial and experimental psychiatric diseases
that guarantees massive income for the drug companies. So in violating a
human's basic right to body, to trial, etc. all these people are getting
guaranteed income from taxpayers and the victims themselves who are forced by
law the buy these drugs and services even if they don't need or more
importantly don't want them.

The irony is that here people viciously jail those who consensually use
recreational drugs, while simultaneously legally forcing people to use drugs
that they don't want to use. Many of these psychiatric victims do "just say
no", as the classic logo states, but it doesn't matter, as they are still
drugged unconsensually anyway.

Any discussion of psychology cannot fail to mention that there exists a massive
mistaken belief, not only in the claims of religions, but in the pseudoscience
claims of psychology. Harmless, realistic, lawful people are outcast and
imprisoned because of this massive mistaken belief. For example, the theories
of psychosis, neurosis and schizophrenia are completely fraudulent, because
there is no known physical, diagnostic test which can detect these so-called
diseases, but yet the label of "psycho" causes terror and fright in people,
even if a person has never been violent or violated a single law, and so it is
with "heretic" or "witch" even though there is no justification for any fear
since the claims of "psycho", "heretic" and "witch" are not based on physical
fact. Many times a person who murdered may be labeled a psycho, heretic or
witch to try to associate violence with the label. People must recognize that
violence is what we should fear, and we should dismiss explanations such as
psychosis, witchcraft and heresy as being the cause of violence. Curiously
there is no disease of "violent", perhaps because people have supported and
tolerated violence for many centuries. But even if there is a disease of
"violent" we should never allow unconsensual treatment. So the important point
to understand is that there simply is no basis for many of the psychological
"diseases" in particular psychosis, neurosis and schizophrenia. Many of these
labels can be reduced to labeling a person with "inaccurate opinions", or
"unusual opinions" or "unusual behavior" all of which should be completely
legal. Many of the so-called diseases coming out of psychology are potentially
true, but trivial, such as attention deficit disorder, where certainly many
people have small attention spans, but that is trivial and not a cause for
tremendous concern, and certainly, no matter what the alleged disease, only
consensual treatments should ever be administered.

At the current time, many people are being misled by terrible people that
control image and sound sending to brains (ie the secret Pupin thought sending
technology), and many of them are being punished for correctly claiming that
"people hear their thoughts".
Paris, France  
208 YBN
[1792 AD]
2282) Delambre turns his interest to science when he is 36.
Pairs, France  
208 YBN
[1792 AD]
2312) In 1777 Murdoch is hired into the engineering business of Matthew Boulton
and James Watt in Birmingham, England.
Murdoch joins the Lunar society.

Around 1784 Murdoch builds the first model of an oscillating (steam?)
engine.(detail how works)

In 1786 Murdoch builds a steam carriage (or road locomotive) that is
unsuccessful.

In 1799 he invented the long D slide valve.(detail: what is and how works?)

Around 1799, Murdoch returns to Birmingham and perfects practical methods for
making, storing, and purifying gas.
Redruth, Cornwall, England  
208 YBN
[1792 AD]
2318) Antoine François, comte de Fourcroy (FURKrWo) (CE 1755-1809), French
chemist, publishes "The Philosophy of Chemistry" (1792, tr. 1795).
Fourcroy is an
early convert to Lavoisier and helps to establish the new chemical
nomenclature.
Fourcroy is a member of the French government and takes a leading part in the
establishment of schools for both primary and secondary education, proving in
particular for scientific studies.

According to Asimov, Fourcroy is a violent partisan of the radicals that
succeed to the seat previously held by the murdered Marat.
Fourcroy does not
use his influence to help Lavoisier, but does use his influence to save other
scientists.

Paris, France  
208 YBN
[1792 AD]
2442) Gauss works on number theory established by Fermat.

Gauss is reluctant to publish anything that could be regarded as controversial,
so some of his most brilliant work is found only after his death. (It is hard
to believe that anything in math could be controversial, but I suppose anything
that might be interpreted as false might be controversial.)

Gauss recognizes that all numbers are of the form a + ib and represents such
numbers by points in a plane.
Gauss has unpublished insights into the nature of
complex functions and their integrals.

Gauss offers a new definition for a prime number, in which the number 3, for
example, remains a prime, while the number 5 becomes composite, since it can be
expressed as a product of complex factor (1 + 2i)(1 − 2i).

As a result of Gauss' survey work, in 1827 Gauss publishes a memoir in which
the geometry of a curved surface is developed in terms of intrinsic, or
Gaussian, coordinates.

Gauss works out a non-Euclidean geometry, a geometry based on axioms different
from those of Euclid, but hesitates to publish. Lobachevski and Bolyai will
publish first.
Gauss is the only child of poor parents.
Gauss is a child prodigy, at
age 3 correcting his fathers sums.
Gauss is a calculating prodigy and retains
the ability to do elaborate calculations in his head most of his life.
Gauss' unusual
mind is recognized and he is educated at the expense of Duke Ferdinand of
Brunswick.
From 1795-8 Gauss studies mathematics at the University of
Göttingen.
From 1818 to 1832 Gauss makes a survey of Hannover.
A statue of Gauss stands on a
pedestal in the shape of a 17-pointed star.
Some people rank Gauss with Archimedes
and Newton as one of the three greatest mathematicians of all time.
Brunswick, Germany  
207 YBN
[04/??/1793 AD]
2359) Whitney graduates from Yale College in 1792.

Perhaps out of guilt in seeing people get rich using the cotton gin (which is
simple to copy) and Whitney and his partner Phineas Miller not able to win
lawsuits against the farmers, some southern US governments award Whitney and
Miller about $90,000. In the end Whitney and Miller gain practically nothing..


When Congress refuses to renew the patent, which expires in 1807, Whitney
(writes) that "an invention can be so valuable as to be worthless to the
inventor". Whitney chooses not to patent his later inventions, including a
milling machine.

(My own view is that inventors should be recognized, but I don't think people
should try to restrict the free-flow and in particular copying of ideas and
information, even so-called intellectual property and invention designs.)
Mulberry Grove, Georgia (presumably)  
207 YBN
[05/30/1793 AD]
2403) Young is born of Quaker parents.
Young is a child prodigy, able to read at age 2.
Youn
g (is reported to have) read through the Bible twice by the age of four, to be
reading and writing Latin at six, and by 14 to have knowledge of at least five
languages.
Young learns Greek, Latin, Hebrew, Arabic, Persian, Turkish, and Ethiopian.
Youn
g can play a variety of musical instruments.
Young is called "Phenomenon Young" at
Cambridge.
In 1799 Young sets up a medical practice in London.
From 1801-3 Young lectures while
professor of natural philosophy at the Royal Institution in London.
Henry
Brougham, a baronet, and influential literary reviewer, according to Asimov,
expresses enmity towards Young's work. (see Young book) Brougham wrongly relies
more on criticisms of Young's character and less on physical phenomena.

In England Newton's particle theory is most popular so Young's wave theory
initially is opposed by the majority of intellectuals.
Wollaston supports Young vigorously.

For a person who changed the popular paradigm of light from particle to wave,
which still stands for the most part today, there is surprising little
information on Young's works. There is only one book "Miscellaneous Works of
the Late Thomas Young" published in 18
London, England  
207 YBN
[08/08/1793 AD]
2228) All the (educational) societies, including the Academy of Sciences, are
suppressed in France, for being to aristocratic.
The Jardin des Plantes is transformed into
the Muséum National d'Histoire Naturelle (National Museum of Natural History).
(on this date too?)

Paris, France (presumably)  
207 YBN
[1793 AD]
2291) When his book is not well received, Sprengel becomes depressed and does
not publish the results of his other botanical research.

Charles Darwin praises Sprengel's book 50 years later in 1841.
Spandau, Germany  
207 YBN
[1793 AD]
2372) Dalton attends John Fletcher's Quaker grammar school in Eaglesfield. When
Dalton is only 12 years old, Fletcher turns the school over to Dalton's older
brother, Jonathan, who asks the younger Dalton to teach. As a result, Dalton
teaches at a Quaker school at age 12. Some of the students are as old as Dalton
and present disciplinary problems. Two years later the Dalton brothers
purchase a school in Kendal, where they teach around 60 students.

Dalton learns from Elihu Robinson and John Gough who were also amateur
meteorologists.

Starting in 1787, Dalton keeps daily records of the weather (atmospheric
pressure, temperature, wind, and humidity) for 57 years to the day he dies,
recording some 200,000 observations.

Dalton's records, carefully preserved for a century are destroyed during the
World War II bombing of Manchester.

In 1793 Dalton moves to Manchester to teach mathematics at a dissenting
academy, the New College.

In 1801, Dalton publishes "Elements of English Grammar".

In 1810 Dalton refuses an invitation to join the Royal Society but is finally
elected in 1822 without his knowledge.

In 1825 Dalton receives a medal (which?) from the Royal Society for his work on
the atomic theory.

In 1831 Dalton helps to found the British Association for the Advancement of
Science.

In 1832, (Dalton is awarded) a doctor's degree from Oxford, at which time
Dalton is presented to King William IV.

In 1838 the Royal Society rejects Dalton's paper "On the Arseniates and
Phosphates" which Dalton has printed privately, noting bitterly that Britain's
chemistry elites, "Cavendish, Davy, Wollaston, and Gilbert are no more".

During most of his life Dalton has little money.
Manchester, England  
206 YBN
[05/08/1794 AD]
2223) Antoine Laurent Lavoisier (loVWoZYA) (CE 1743-1794), his father-in-law,
and 26 other Tax Farmers are killed with a guillotine.

Althought a reformer and political liberal, in 1792 Lavoisier is forced to
resign from his post on the Gunpowder Commission and to move from his house and
laboratory at the Royal Arsenal.

On November 24, 1793, the arrest of all the former tax gatherers is ordered.
Mar
at now a powerful revolutionary leader accuses Lavoisier of ridiculous plots
such as "adding water to the peoples' tobacco" and wildly demanding his death.
Marat is killed in July 1793, (however the trial of Lavoisier and the other tax
farmers continues).
Lavoisier's wife and chemical disciples circulate letters and petitions
to show how much the "father of French chemistry," as he is contemporarily
called, has been useful to the Revolution.
The tax farmers are formally brought to trial on
this day May 8, 1794, and convicted with summary justice of having plundered
the people and the treasury of France, of having adulterated the nation's
tobacco with water, and of having supplied the enemies of France with huge sums
of money from the national treasury.
Lavoisier objects that he is a scientist and the
judge reportedly states that "the republic has no need of scientists" (Chaptal
and Leblanc prove how wrong this is).

The Reign of Terror falls only three months later when the radicals are
overthrown. Asimov comments that Lavoisier was the single biggest loss of the
revolution.

Joseph-Louis Lagrange comments, "It took them only an instant to cut off that
head, and a hundred years may not produce another like it."

Within two years of Lavoisier's death, the regretful French people will unveil
busts of him.

Paris, France (presumably)  
206 YBN
[08/15/1794 AD]
1895)
France  
206 YBN
[1794 AD]
2086)
Edinburgh, Scotland  
206 YBN
[1794 AD]
2249) Pavia, Italy  
206 YBN
[1794 AD]
2255)
Paris, France  
206 YBN
[1794 AD]
2260) The École Polytechnique in Paris, France is established by the National
Convention as the "École Centrale des Travaux Publics" ("Central School of
Public Works") under the leadership of Lazare Carnot and Gaspard Monge (moNZ)
(CE 1746-1818).

Paris, France  
206 YBN
[1794 AD]
2298) This book is widely adopted in Europe and in the USA where it is
translated.
This book contains many misleading attempts to defend the parallel postulate.
Ac
cording to Asimov Laplace, who Asimov characterizes as small minded, expresses
enmity towards Legendre.
Paris, France(presumably)  
206 YBN
[1794 AD]
2327) Ernst Florens Friedrich Chladni (KloDnE) (CE 1756-1827) is one of the
first to claim that meteors (found on earth) fall from the sky, but this is not
believed since meteorites are thought to be of volcanic origin until Jean
Baptiste Biot proves this in 1803.
In this book, Chladni suggests that meteorites are
the debris of an exploded planet.

Wittenberg, Germany (presumably)  
206 YBN
[1794 AD]
2336)
(was Åbo is now)Turku, Finland  
206 YBN
[1794 AD]
2373) Dalton's brother also is color blind.
Colorblindedness is also called
"Daltonism".
Manchester, England  
206 YBN
[1794 AD]
3376)
?, England  
205 YBN
[1795 AD]
2084)
Edinburgh, Scotland (presumably)  
205 YBN
[1795 AD]
2085)
Edinburgh, Scotland (presumably)  
205 YBN
[1795 AD]
2233) Titanium is a silvery-gray, lightweight, high-strength, low-corrosion
structural metal and is used in alloy form for parts in high-speed aircraft.
Berlin, (was Prussia) Germany (presumably)  
205 YBN
[1795 AD]
2645)
England  
205 YBN
[1795 AD]
5971) Ludwig van Beethoven (CE 1770-1827), German composer, publishes his first
Sonata (opus 2).

Beethoven lives through the end of the Classical era and the beginning of the
Romantic era of music which is around 1800.

Vienna, Austria (presumably)  
204 YBN
[01/28/1796 AD]
3321) Henry Brougham publishes a paper defending Newton's interpretation of
inflexion" (as opposed to explaining inflexion as simple particle reflection).

London, England (presumably)  
204 YBN
[07/01/1796 AD]
2280) At the age of 13 is apprenticed to a nearby surgeon, and completes his
apprenticeship at age 21.

Jenner prepares and arranges zoological specimens collected by Captain Cook
after his first voyage to the Pacific. Jenner refuses an offer as naturalist on
Cook's second voyage.

Jenner receives worldwide recognition and many honors (for cowpox vaccination),
but makes no attempt to enrich himself through his discovery.
Berkeley, England (presumably)  
204 YBN
[1796 AD]
2124) Darwin declines the offer to be physician of George III.
Erasmus Darwin is the
grandfather of the naturalist Charles Darwin (by his first wife) and the
biologist Francis Galton (by his second wife).
Derby, England (presumably)  
204 YBN
[1796 AD]
2126)
Derby, England (presumably)  
204 YBN
[1796 AD]
2277)
Paris, France (presumably)  
204 YBN
[1796 AD]
2330) Gall gives lectures and charges admission. Emperor Francis I stops Gall
thinking his philosophy is subversive of religion.
Like Mesmer, a committee
appraises Gall's phrenology and reports unfavorably.
Vienna, Germany  
204 YBN
[1796 AD]
2339)
London, England (presumably)  
204 YBN
[1796 AD]
2390)
Paris, France  
204 YBN
[1796 AD]
5953)
Vienna, Austria (presumably)  
203 YBN
[06/15/1797 AD]
3839)
(read aloud in:) London, England  
203 YBN
[1797 AD]
1231) Jean-Baptiste Pussin (1745-1811) replaces iron shackles with
strait-jackets at Bicêtre Hospital in Paris. Shackles provide more freedom of
bodily movement, straight-jackets leave a person helpless to move their arms
even for example to itch themselves. However, this is viewed as being a more
humaine treatment, and it does represent a change in approach to the prisoners
in psychiatric hospitals.

Paris, France  
203 YBN
[1797 AD]
2159)
Paris, France  
203 YBN
[1797 AD]
2306)
London, England (presumably)  
203 YBN
[1797 AD]
2331) Olbers is a physician that converts the upper portion of his house into
an observatory.
Bremen, Germany  
203 YBN
[1797 AD]
2338) James Hall is President of the Royal Society of Edinburgh.
  
203 YBN
[1797 AD]
2344) Chromium is a hard, steel-gray metal that takes a high polish and is used
in alloys to increase strength and corrosion resistance.

Chromium is added to iron and nickel to produce alloys that have high
resistance to corrosion and oxidation (these have about 70 percent chromium).
Used in small amounts, chromium hardens steel. Stainless steels are alloys of
chromium and iron in which the chromium content is between 10 to 26 percent.

Chromium is atomic number 24; atomic weight 51.996; melting point 1,890°C;
boiling point 2,482°C; specific gravity 7.18; valence 2, 3, 6.

The green colour of emerald, serpentine, and chrome mica and the red colour of
ruby are due to chromium.
Chromium is a relatively abundant element in the Earth's crust.
The
son of a farm laborer, Vauquelin went to work in an apothecary shop where he
befriends Antoine-François Fourcroy who makes Vanquelin his laboratory
assistant from 1783â€"91.

Vauquelin lives with Fourcroy's sisters, who never marry, and Vauquelin returns
their care for him when young by caring for them when they are old.

Vauquelin starts publishing his own work in 1790 and is associated with 376
scientific papers.

Vauquelin will fund Louis-Jacques Thenard, another peasant's son who will go on
to become a famous chemist.
Paris, France  
203 YBN
[1797 AD]
2385) In 1798, Cuvier refuses an invitation to become a naturalist on
Napoleon's expedition to Egypt (1798-1801).

Cuvier has a library of 19,000 books Asimov claims he supposedly virtually
memorized the contents of all of them. (doubt)
Paris, France  
203 YBN
[1797 AD]
2398) Trevithick's schoolmaster describes him as "disobedient, slow and
obstinate". Trevithick's father, a mine manager views young Richard as a
loafer. However Trevithick has an extraordinary talent in engineering and
because of this ability Trevithick is hired as an engineer to several Cornish
ore mines in 1790 at the age of 19.

In all, Trevithick builds 30 (high-pressure) engines. These engines are so
compact that they can be transported in an ordinary farm wagon to the Cornish
mines, where they are known as "puffer whims" because they vent their steam
into the atmosphere.
Trevithick has trouble making his steam-engine trains a financial
success, just as Fitch was to Fulton, so Trevithick is to Stephenson.
Trevithick dies a
poor man and is buried in an unmarked grave.
Cornwall, England (presumably)  
203 YBN
[1797 AD]
2443) This proof is given as Gauss' doctoral thesis.

The Encyclopedia Britannica biographer comments that "Gauss's proof, though not
wholly convincing, was remarkable for its critique of earlier attempts", which
shows that math proofs can be interpreted differently and widely sometimes.
Göttingen, Germany  
203 YBN
[1797 AD]
2666)
London, England (presumably)  
202 YBN
[01/25/1798 AD]
2234)
Berlin, (was Prussia) Germany (presumably)  
202 YBN
[05/14/1798 AD]
2281) Jenner goes to London seeking volunteers for vaccination but (finds none)
in a stay of three months.
At the time, pure cowpox vaccine is not always easy to
obtain, preserve or transmit.
Berkeley, England (presumably)  
202 YBN
[06/02/1798 AD]
1233)
Egypt  
202 YBN
[07/14/1798 AD]
2360) Whitney builds a water‐powered (gun building) factory in Hamden.
There is
some disagreement about whether Whitney's muskets had interchangeable parts.
However, Encyclopedia Britannica states that "Finally, he (Whitney) overcame
most of the skepticism in 1801, when, in Washington, D.C., before
President-elect Thomas Jefferson and other officials, he demonstrated the
result of his system: from piles of disassembled muskets they picked parts at
random and assembled complete muskets."
Hamden, Connecticut, USA  
202 YBN
[07/25/1798 AD]
1234)
Egypt  
202 YBN
[08/07/1798 AD]
1236) The British navy under the command of Nelson, destroy 13 of 17 French war
ships, and form a blockade of Egypt (in the Battle of the Nile). Napoleon and
55,000 men are in Egypt and have no way to get supplies from France. On the
morning of getting the news from Aboukir Bay, Napoleon says "It seems you like
this country. That is very lucky, for we now have no fleet to carry us back to
Europe."

Egypt  
202 YBN
[08/??/1798 AD]
1235) Napoleon founds an institute in Cairo based on the Institute de France in
Paris, to coordinate the research of 150 scientists. Mathematician Gaspard
Monge is president, with Napoleon as Vice President. In jealously the military
officers call the scientists "pekinese dogs", viewing them only as lap-dog
servants to Napoleon.
Of these scientists, Berthollet studies the making of indigo.
Villoteau studies arab music. Larrey strudies opthalmia. Savigny uncovers new
species of water lily. Saint-Hilaire studies the ostrich, crocodile, and
polypterus, a species of nile fish only found in the Nile. Saint-Hilaire
studies mummified ibises, and is the first human to follow the development of a
species through more than 1000 years. Dominique-Vivant Denon, scetches much of
Egypt including the chapel of Amenophis III at Aswan, and this is the only
drawing that has ever been found.

Egypt  
202 YBN
[1798 AD]
1935) This star map is more extensive and accurate than that of Flamsteed.
F. W. Bessel's
catalog in 1818, with 3,000 star positions, will be largely based on Bradley's
observations.

The publication of Bradley's observations are delayed by disputes about their
ownership; but are finally issued by the Clarendon Press, Oxford, in two folio
volumes (1798, 1805).
Oxford, England  
202 YBN
[1798 AD]
2117) The gravitational constant, and the mass, and density of the Earth is
measured.

Henry Cavendish (CE 1731-1810) measures Newton's gravitational constant by
using a modified torsion balance created by John Michell.

Using this constant Cavendish calculates the mass and density of the planet
Earth. That the (average) density of earth is larger than a stone implies a
(dense) core.

Michell suggested this experiment.

Cavendish suspends a rod with a lead ball on each end. A light force applied to
the balls will cause the rod to twist. Cavendish measures how large a twist is
produced by various small forces. Cavendish puts a large lead ball on each side
of the lighter lead balls and from the amount of twist the gravitational force
between the two pairs of balls can be measured. Cavendish calculates the
attraction between the balls from the period of oscillation of the torsion
balance. (more detail, show how, units) Knowing the mass of each ball, their
distance from center to center, (and the force of attraction between them), the
only unknown is the Gravitational constant which Cavendish calculates (as=?).
From this constant, Cavendish calculates the mass of the earth to be 6.6e21
tons and to have a density of about 5 and a half times that of water. (Asimov
claims that Newton guessed this value a century before.) (find Newton's
estimate, how did Newton create his estimate?)

Cavendish succeeds in measuring a gravitational attraction that is only
1/50,000,000 of the weight of the lead balls. The result that Cavendish obtains
for the density of the Earth is within 1 percent of the currently accepted
density.

Humans are still waiting to calculate a mass estimate for a light particle
which may be the basis of all matter in the universe. Is the gravitational
constant the same even for photons? Perhaps if we use a different set of
quantities, such as "number of photons" and "number of photon spaces" we might
be able to find a physics without any need for constants such as the
gravitational constant.

Cavendish publishes his results in Philosophical Transactions of the Royal
Society of London as "the Experiments to Determine the Density of the Earth".

Cavendish never explicitly measures the gravitational constant, and his aim is
to measure the mass and density of earth relative to water through the precise
measurement of gravitational interaction.

I think there is a lot of room for error in this kind of precise measurement of
a quantity so small. People should definitely continue to perform this
experiment, in particular between different size masses and temperatures, in
low gravity such as in orbit of Earth.
London, England  
202 YBN
[1798 AD]
2253)
Paris, France  
202 YBN
[1798 AD]
2278)
Paris, France (presumably)  
202 YBN
[1798 AD]
2279)
Paris, France (presumably)  
202 YBN
[1798 AD]
2303) Thompson receives only 2 years of formal education and at age 13 is
apprenticed to a local merchant. At the age of 19, while teaching in Concord,
New Hampshire, Thompson marries a wealthy widow, 14 years older than he and
therefore acquires an extensive estate and social and political influence. (Did
the female have the right to own the property and money or did she legally have
to surrender it to her husband?)
Thompson is on the side of England in the Revolutionary
War, and spies on the colonialists. When the British troops leave Boston,
Thompson goes with them leaving his wife and child behind.

Like Franklin, Thompson refuses to patent his inventions.
In 1793 while living in Munich,
Bavaria, Thompson is made a count of the Holy Roman Empire and chooses as his
title "Count Rumford", Rumford being the original name of Concord, New
Hampshire, USA.
In 1804 Thompson moves to Paris and in 1805 marries Lavoisier's
widowed wife but the marriage only lasts two years.
In some way, the heat as a
fluid called "caloric" theory, i think will ultimately be seen to be closer to
the correct path, and more intuitive, since there is a strong identity between
caloric and photons, photons are not a fluid, and may or may not be thought of
as heat itself...it depends if you think the photon is the cause of heat, or
the movement of the photon (in addition to the photon itself) is the cause of
heat, but otherwise I think the caloric was an good intuitive theory. The term
"calorie" is still used, but may be replaced my Gigaphotons per second or
similar units. In someway Thompson was partially correct in that, probably the
movement of the photon is a necessary component (although in addition to the
photon itself) to record a measurement of heat.

Thompson writes: "And, in reasoning on this subject, we must not forget to
consider that most remarkable circumstance, that the source of the heat
generated by friction, in these experiments, appeared evidently to be
inexhaustible.
It is hardly necessary to add, that any thing which any
insulated body, or system of bodies, can continue to furnish without
limitation
, cannot possibly be a material substance: and it appears to me to be
extremely difficult, if not quite impossible, to form any distinct idea of any
thing, capable of being excited, and communicated, in the manner the heat was
excited and communicated in these experiments, except it be MOTION.
I am very far from
pretending to know how, or by what means, or mechanical contrivance, that
particular kind of motion in bodies, which has been supposed to constitute
heat, is excited, continued, and propagated, and I shall not presume to trouble
the Society with mere conjectures; particularly on a subject which, during so
many thousand years, the most enlightened philosophers have endeavored, but in
vain, to comprehend."
Bavaria, Germany (presumably)  
202 YBN
[1798 AD]
2337)
(was Åbo is now)Turku, Finland  
202 YBN
[1798 AD]
2345) Beryllium is initially called "glucinum" because of the sweetness of its
compounds, and will be renamed "beryllium" in 1957.

Beryl is a mineral composed of beryllium aluminum silicate, Be3Al2(SiO3)6.

Beryl is a silicate. The silicates make up about 95 percent of the Earth's
crust and upper mantle. Silicates are the major constituents of most igneous
rocks and are found in sedimentary and metamorphic rock too. Silicates are
important parts of rock from the moon of Earth, meteorites, most asteroids, and
rocks on the surface of Mercury, Venus, and Mars. The basic structural unit of
all silicate minerals is the silicon tetrahedron in which one silicon atom is
surrounded by and bonded to four oxygen atoms, each at the corner of a regular
tetrahedron.

Beryllium is a high-melting, lightweight, corrosion-resistant, rigid,
steel-gray metallic element used as an aerospace structural material, as a
moderator and reflector in nuclear reactors, and in a copper alloy used for
springs, electrical contacts, and nonsparking tools. Beryllium has atomic
number 4; atomic weight 9.0122; melting point 1,278°C; boiling point 2,970°C;
specific gravity 1.848; valence 2.

Beryllium is highly permeable to X-rays, and neutrons are liberated when
beryllium is hit by alpha particles, for example alpha particles from radium or
polonium (about 30 neutrons/million alpha particles). Beryllium emitting
neutrons from collision with alpha particles will lead to the discovery of the
neutron by Chadwick in 1932. Neutrons will prove to be very useful in
separating atoms and transmuting less useful and more common atoms to more
useful and less common atoms, and will open the door to the very useful process
of nuclear fission. (In particular there may already secretly or in the future
be a way to use neutrons to extract large quantities of hydrogen and other
gases which float free from any atoms, which can then by used as fuel by oxygen
combustion).
Paris, France  
202 YBN
[1798 AD]
2353) Senefelder accepts an offer from a music publisher, Johann Anton André,
to set himself up at Offenbach and train others in Senefelder's lithographic
process.

Senefelder develops lithography all over Europe, with the music publisher
Johann Anton André of Offenbach, in London and in Vienna.

In 1800 Senefelder founds a lithography press in London and soon after this is
granted patents in Scotland, England, Ireland and Austria.
Munich, {Bavaria, now} Germany  
202 YBN
[1798 AD]
2361) Malthus has a cleft palate that interferes with his speech.

This work causes some amount of controversy.

In 1803, Malthus publishes a second and larger edition, converting his original
pamphlet into a book with the help of demographic data from European countries.
In this second edition Malthus admits that "moral restraint" in the form of
delayed marriage and (asexuality) might counter the increase in population.

In 1805 Malthus becomes a professor of history and political economy at the
East India Company's college at Haileybury, Hertfordshire.

In 1820, Malthus publishes "Principles of Political Economy" (1820), on
economics.

Malthus will continue publishing later editions until the final and massive
sixth edition of 1826.

(On the topic over overpopulation, what is frustrating to me is that even now,
people have trouble recognizing anything beyond the earth. For example, there
is nothing but endless space and matter in the universe, countless stars,
planets and empty space, and even our own star system is huge. There is far
more matter and space than we will ever possibly be able to make use of. It
seems clear that overpopulation, as long as there is space on the moon and
other planets is not going to be a problem, if we are smart and provide paths
for life to grow. We as humans on Earth are failing to accommodate the growth
of life mainly because of the stupid traditions of religions, antisexuality,
tolerance of violence, secrecy, lack of free info, lack of full democracy and
not embracing the method of science and honesty. As I have said many times,
there is more than enough space and matter in the universe for all of life of
earth and our descendants and this is obvious, but not if we do nothing but
stay here on earth, not bothering to even talk about moving to other stars and
planets let alone proceeding to build ships (such as star ship one) and
humanoid robots like Honda, Sony, and Toyota have done to start that inevitable
future.)

(My own feeling about the idea of allowing humans to reproduce as often as they
want to, theoretically making hundreds of new humans, is that people should
promote birth control for unwanted pregnancy, but provide a minimum standard of
living for all living humans. The key is to start developing the Moon, Mars,
the matter of this star system, and of other stars to allow humans to reproduce
and grow at a regular rate. There is a reality, for example, like bacteria in
an agar dish; there are finite limits on how much matter can be converted to
living objects. In particular if ever humans figure out how to stop aging, the
population of humans will increase much faster. In that event, I can see people
voting to put limits on how many new humans can be made. In addition, people
may vote to nonviolently, without prison, and without violating a person's
body, punish those who produce more than a few new humans or more humans than
they can financially keep from starvation. Perhaps those people who have
produced more humans than allowed by the majority will be physically prevented
from being impregnated or impregnating, or forced to move to the outer newly
developed star systems.)

(Malthus' claim that disease and war occur as a result of overpopulation I
think is inaccurate {although starvation, or cannibalism I can see occurring as
a result of overpopulation}. I see war and first strike violence as completely
unnecessary in a smart and logical population. I think tolerating first strike
violence whether on the small scale and on the large scale is a path to chaos,
disorder and threatens continued survival of life of Earth.)

(This view of overpopulation as being the cause of all problems may influence
the popularity of the brutal eugenic theories that the Nazis and others used to
justify murdering people based on their race, income, and opinions. It may be
that Malthus was the first to publicly and more explicitly apply the idea of
natural selection as described by Hutton to the human species.)
Surrey, England (presumably)  
202 YBN
[1798 AD]
2421) From 1790 to 1793 Buch studies at the Freiberg School of Mining under
Abraham Werner.
Mount Vesuvius, Italy  
202 YBN
[1798 AD]
2877) A quote by Taylor is:
"Mythology is the natural measure of the unenlightened
mind; it contains the aspirings of the soul after higher objects, which are
beyond its reach, and its efforts to realize the dim images faintly formed in
the mind, as the man wandering in darkness strives to give shape to the objects
indistinctly seen to connect them together."
("its efforts to realize the dim images
faintly formed in the mind" only coincidence? or awareness of people trying to
follow this science , or possibly this was understood in the 1800s and a hint
of frustration or concern about the massive idiocy and injustice of keeping
seeing thought secret?)
London, England (presumably)   
202 YBN
[1798 AD]
3253)
Geneva, Switzerland (presumably)  
202 YBN
[1798 AD]
5972) Ludwig van Beethoven (CE 1770-1827), German composer, composes his Piano
Sonata Number 8 in C ("Pathétique") (opus 13).

Vienna, Austria (presumably)  
201 YBN
[06/??/1799 AD]
2392) (Over the course of his life), Humboldt collects 60,000 plants including
thousands of species never described
before.

Humboldt experiments with electricity in nerves and muscles, erroneously
backing Galvani (as opposed to Volta).
During a short stay in the United States at the
end of his journey, Humboldt is received by US President Thomas Jefferson.
Humboldt is
friends with King Louis Philippe of France.
Humboldt is in favor of the French
Revolution.
Humboldt writes against human slavery.

In 1828 Humboldt organizes in Berlin one of the first international scientific
conferences, which is evidence of Humboldt's organizational skills since such
large gatherings of potentially liberal-minded people are frowned on by
governments in the wake of the Napoleonic Wars and the associated rise of
democratic expectations.

Humboldt has a voluminous correspondence: about 8,000 letters remain.
South America  
201 YBN
[08/23/1799 AD]
1238) Napoleon runs the English blockade" and sails for France.

Egypt  
201 YBN
[08/??/1799 AD]
1237)
Rashid, Egypt  
201 YBN
[1799 AD]
2283)
France  
201 YBN
[1799 AD]
2315) Proust provides evidence that that relative quantities of elements in any
compound remain the same no matter what the source used to make the compound or
method of preparation.

Proust shows that copper carbonate contains definite proportions by weight of
copper, carbon and oxygen no matter how the copper carbonate is prepared or how
it is isolated from nature. The preparation is always 5 of copper, 4 of oxygen,
and 1 of carbon.

Proust then shows that this same principle applies for a number of compounds. A
compound is any substance with identical molecules made of more than one
element.
From these experiments Proust formulates the generalization that all compounds
contain elements in certain definite proportions with no exceptions regardless
of conditions of production.

Proust maintains that all compounds are made of components that combine in
fixed proportions by weight.
Proust's law of definite proportions comes under attack in
1803 by the eminent French chemist Claude-Louis Berthollet who claims that
chemicals do not always combine in definite proportions.
Proust shows how Berthollet is
misled by inaccurate analysis and by products Berthollet did not purify
enough.

Swedish chemist Jöns Jacob Berzelius will establish the conceptual
relationship between Proust's law and Dalton's theory in 1811.

This finding helps to persuade Dalton that elements must occur in the form of
atoms.

Dalton's chemical atomic theory in 1801 will eventually settle this dispute
between Berthollet and Proust in favor of Proust and atomism.

This is evidence that the photons emitted from atomic and molecular reactions
may not be completely separated atoms, but only photons that result in atoms of
less mass. But even if entire atoms are destroyed into photons in two atoms
contacting or reacting with each other, the law of definite proportions is
still true, even if some atoms are destroyed into photons, since the
composition of any specific molecule is always the same.
Segovia, Spain  
201 YBN
[1799 AD]
2451) Thénard is the son of poor peasants who work to send him to school.
Thénard
studies chemistry in Paris under conditions of semi-starvation until Vauquelin,
himself the son of a peasant, befriends Thénard.
In 1802, Thénard beomces professor at
the Collège de France.
Thénard works with lifelong friend Gay-Lussac.
Thénard becomes chancellor
of the University of Paris.
Paris, France (presumably)  
201 YBN
[1799 AD]
2483) Davy also discovers hydrogen telluride, and hydrogen phosphide
(phosphine). (chronology)

Davy's collected works (9 vol, 1839-40; repr. 1972) include a biographical
memoir by his brother, John Davy.
Davy is the elder son of middle-(income) parents.
In 1795
Davy is apprenticed to a surgeon and apothecary.
Davy (writes that) when you he has plans
for a volume of poems, but in 1797 when he begins the serious study of science,
Davy's interest in poetry "fled before the voice of truth".
Davy befriends Davies Giddy
(later Gilbert; president of the Royal Society, 1827-30) and Giddy recommends
Davy for a job at the Pneumatic Institution in Bristol.
From 10/1799-03/1801 Davy works
at the Pneumatic Institution in Bristol.
In 1800, the account of Davy's work (at the
Pneumatic institution) published as "Researches, Chemical and Philosophical"
(1800) quickly establishes Davy's reputation (as a good scientist).
In 1801 Davy moves to
London and is invited to lecture at the Royal Institution of Great Britain
newly founded by Joseph Banks and Benjamin Thompson (Rumford) in 1799.
Davy's
brilliant lectures attract a fashionable and intellectual audience. (open to
the public?)
In 1802 Davy becomes professor of chemistry (at the Royal Institution).
In 1805 Davy
receive the Copley Medal for his researches on voltaic cells, tanning, and
mineral analysis.
In 1807 Davy is a charter member of Geological Society of London.
Davy wins an
award for the best work in electricity established by Napoleon, says that while
the governments might be at war but the scientists are not.
Davy does not
accept Dalton's atomic theory. Wollaston tries to convert him.
In 1811 Davy
hires Michael Faraday as an assistant.

In 1812 Davy damages his eyes in a nitrogen trichloride explosion. Faraday
skillfully prepared, but Davy allows it to explode.
From 1820-1827 Davy is
president of the Royal Society.
Davy's assistant is Faraday.
In 1824 Davy tries to block
Faraday's membership into the Royal Society.
Davy twice opposes the election of
Faraday to fellowship in the Royal Society. At one point Davy objects to
honoring Faraday for achieving the first liquefication of chlorine, claiming
that he himself deserves credit for the feat. Another time, Davy says his
opposition is due to his belief that William Wollaston (1766-1828) had preceded
Faraday in discovering electromagnetic rotation. Perhaps Davy is envious of the
success of his former assistant. Faraday does finally become a Fellow of the
Royal Society in 1824.
In his will Davy leaves funds to establish a medal to be given
annually to chemists.
Bristol, England  
200 YBN
[03/20/1800 AD]
2250) Volta finds that not only will two dissimilar metals in contact produce a
small electrical (current), but metals in contact with certain fluids also
produces electrical .

Volta's first battery uses copper and tin or zinc metal strips in a bowl of
salt water to produce an electric potential (or differential) and current.
Volta improves on this device, making things less messy, watery and more
compact by using small round plates of copper and zinc and discs of salt soaked
cardboard. Volta connects these plates in order of copper, zinc, cardboard,
copper, zinc, cardboard, and so on. When a wire is attached to the top and
bottom of this Voltaic pile an electric current passes through it if the
circuit is closed.

This "voltaic pile" consisted of alternating zinc and silver disks separated by
layers of paper or cloth soaked in a solution of either sodium hydroxide or
salt water (brine).

This battery is the basis for all wet-cell batteries.

(What kind of voltage and current can be produced by such a device, and what
voltages and currents did Volta measure with his devices?)

Volta's battery is instantly popular because for the first time there is a
device capable of producing a steady, continuous flow of electricity. All
electrical machines before this, including Volta's electrophorus, can only
produced short bursts of static electricity. The use of constant current will
open up many new inventions and discoveries.

Within a short time the voltaic cell will be put to practical use by William
Nicholson and this leads to the electrical work of Davy (and Faraday and much
of the electrical revolution).
Experiments performed with the voltaic pile will lead Michael
Faraday to create the laws of electrochemistry (around 1834), which establish
the relationship between quantity of electrode material and amount of electric
power.

The unit of electromotive force, the driving force that moves the electric
current, will be named the volt in 1881 in honor of Alessandro Volta.


Volta performs experiments to try to show that the electricity of a voltaic
pile can produce the same results as the static electricity of a Leyden jar,
and that the electricity is the same exact kind of fluid. Volta uses a
"condensatore" (a condensing device, basically a capacitor) and measures the
deflection of a gold leaf in an electroscope. Volta concludes that in order to
produce a large deflection of perhaps 35 degrees, Volta would need a pile with
1800-2000 pairs of copper-zinc elements. (Large sparks will be shown to be the
result mainly of very large voltage differential, in particular when the
phenomenon of the transformer is understood and the induction coil in built. In
my view the comparison of electric particles moving as current, in static
electricity, and in permanent magnets is important and has yet to reveal a
deeper truth connecting all three. Perhaps in which each is explained by a
single force such as gravity.)
Pavia, Italy  
200 YBN
[03/27/1800 AD]
2179) This is the first known identification of invisible light.

In the following year Ritter will extend the visible spectrum in the other
direction. (to me that is so interesting, that is a major find. This finding is
apparently required to see thought 110 years later by Michael Pupin. Looking at
light in unseen frequencies will open up an enormous amount of new images and
information about other stars, and even objects on earth.)
Slough, England  
200 YBN
[05/02/1800 AD]
2307) William Nicholson (CE 1753-1815), English chemist, separates water into
hydrogen and oxygen gas using electric current.

Nicholson copies Volta and builds the first voltaic pile in England.
Nicholson
attaches the wire on both ends of the voltaic pile into water and finds that
the water breaks up into hydrogen and oxygen, which collect separately forming
bubbles at the submerged ends of the wires.
Nicholson "electrolyzed" water,
breaking up the molecules into the individual elements.

Nicholson and friend Anthony Carlisle, a London surgeon, use platinum
electrodes and separate tubes to collect the gases evolved at each electrode.

Hydrogen gas bubbles from around the cathode and oxygen gas from around the
anode in the ratio of two volumes of hydrogen for every one volume of oxygen.

In 1760, Giovanni Beccaria (CE 1716-1781), Italian physicist, was the first of
record to separate water into hydrogen and oxygen gases using electricity
created with a static generator.

In 1785, Henry Cavendish (CE 1731-1810) shows that air is a mixture of gases by
using static electricity electrolysis.

In 1789 Troostwyk and Deiman repeat Beccaria's experiment of separating water
into hydrogen and oxygen using static electricity.
London, England (presumably)  
200 YBN
[06/27/1800 AD]
3254)
Manchester, England  
200 YBN
[06/??/1800 AD]
3597)
(Royal Military Academy at Woolwich) Woolwich, England  
200 YBN
[09/17/1800 AD]
2436) From 1791-5, Ritter is a pharmacist in Liegnitz, Silesia.
Starting in 1796, Ritter
studies medicine at the University of Jena, and teaches there.

Ritter tries to revive the phlogiston theory.
Ritter is interested in "dowsing", (an
inaccurate belief that water, metals, gem stones and hidden objects can be
found by using a y shaped stick, rod or pendulum).

In Munich Ritter becomes involved with experiments with dividing rods and
pendulums which he claims have hidden electricity. Ritter claims that he has
discovered a different form of electrical polarity of the earth than that
caused by magnetic polarity and that this newly discovered effect can be
demonstrated by suspending a gold needle properly. Oersted fails to
successfully copy Ritter's experiment. Ritter's work at the end of 1805 is
questioned by scientists, and during the last part of Ritter's life he gains a
reputation of being unreliable.
Ritter's entry into occult science influences his later
work and such experiments destroy Ritter's science reputation as a competitive
scientist. Because of these experiments and his unsubstantiated claims,
historians have ignored Ritter's work between 1806 and 1810. In spite of the
criticism leveled toward him Ritter continues experimenting, but his science
career was finished. (Perhaps this means, his ability to publish the results of
his experiments? Clearly he was never let go from his teaching job.)

Ritter only lives 34 years.
Jena, Germany (presumably)  
200 YBN
[09/??/1800 AD]
3598)
(Royal Military Academy at Woolwich) Woolwich, England  
200 YBN
[11/??/1800 AD]
2437)
Jena, Germany (presumably)  
200 YBN
[1800 AD]
2154) 500 Watt (CE 1736-1819) engines are working in England.

Birmingham, England (presumably)  
200 YBN
[1800 AD]
2386)
Paris, France  
200 YBN
[1800 AD]
2401) Bichat studies anatomy and surgery under Marc-Antoine Petit, the chief
surgeon at the Hôtel Dieu in Lyon.

Bichat is an extreme vitalist who (wrongly) rejects that physics or chemistry
can possibly aid in the understanding of life.
Bichat does not use a microscope.
In 1800 Bichat
becomes physician at the Hôtel-Dieu in Paris. From 1799 on Bichat abandons
surgery and does only research in anatomy, performing as many as 600 autopsies
in a single year.

Bichat dies at 30, faints and falls down stairs in laboratory.
Asimov states that had
Bichat lived longer Bichat may have surpassed Laënnec as the most
distinguished physician of the early 1800s.
Paris, France  
200 YBN
[1800 AD]
2473) Davy writes that he "breathed 16 quarts of the gas in seven minutes" and
became "completely intoxicated" with it.
Davy persuades his scientific and literary
friends, including Samuel Taylor Coleridge, Robert Southey, and P.M. Roget, to
report the effects of inhaling nitrous oxide. Davy nearly loses his own life
inhaling water gas, a mixture of hydrogen and carbon monoxide sometimes used as
fuel.

(I have tried nitrous oxide I think in the form of a so-called "whip-it" small
gas container used as a propellant for whip cream. The feeling is not very
pleasant in my opinion, sounds become very distant sounding. My memories are
that the feeling is not really understanding what people are saying, I remember
my head feeling very dense or cloudy. It might be fun for people to try just
once to see what the effect is. As I remember, the effect is not very pleasant
to me, but to others perhaps the feeling is pleasant. Perhaps the quantity used
makes a difference in the quality of the effect. It is good to know that
prolonged inhalation of nitrous oxide causes death, although more specific info
in terms of quantity and duration and actual research done are needed.)
Bristol, England  
200 YBN
[1800 AD]
3233) Howard continues "I was led to this discovery, by a late assertion, that
hydrogen is the basis of the muriatic acid: (hydrochloric acid) it induced me
to attempt to combine different substances with hydrogen and oxygen. With this
view, I mixed such substances with alcohol and nitric acid, as I thought might
(by predisposing affinity) favour, as well as attract, an acid combination, of
the hydrogen of the one, and the oxygen of the other. The pure red oxide of
mercury appeared not unfit for this purpose; it was therefore intermixed with
alcohol, and upon both, nitric acid was affused. The acid did not act upon the
alcohol so immediately as when these fluids are alone mixed together, but first
gradually dissolved the oxide: however, after some minutes had elapsed, a smell
of ether was perceptible, and a white dense smoke, much resembling that from
the liquor fumans of Libavius, was emitted with ebullition. The mixture then
threw down a dark coloured precipitate, which by degrees became nearly white.
This precipitate I separated by filtration; and, observing it to be
crystallized in small acicular crystals, of a saline taste, and also finding a
part of the mercury volatilized in the white fumes, I must acknowledge I was
not altogether without hopes that muriatic acid had been formed, and united to
the mercurial oxide. I therefore, for obvious reasons, poured sulphuric acid
upon the dried crystalline mass, when a violent effervescence ensued, and, to
my great astonishment, an explosion took place.".

After being injured a second time with the fulminate of mercury Howard turns to
other projects. Howard determine the chemical composition of meteorites,
showing them all to contain nickel, and more nickel in higher quantities than
earthly minerals other than those minerals in nickel ore. This helps to
establish the extra-terrestrial origin of meteorites.
Howard is awarded the Copley Medal
of the Royal Society for this discovery.
London, England (presumably)  
200 YBN
[1800 AD]
4121) (Trinity College) Cambridge, England  
200 YBN
[1800 AD]
4541)
unknown  
200 YBN
[1800 AD]
4542)
unknown  
200 YBN
[1800 AD]
6324) Ludwig van Beethoven (CE 1770-1827), German composer, composes his first
Symphony.
Vienna, Austria (presumably)  
199 YBN
[01/01/1801 AD]
2261) In 1787 with the aid of the viceroy of Sicily, Pizzi founds the
government Observatory of Palermo where he makes his observations.

Piazzi names Ceres after the Roman goddess of agriculture, once widely
worshiped in Sicily.

Piazzi meets Hershel, and falls off the ladder to Herschel's reflector
telescope and breaks his arm.

Piazzi also establishes a government observatory at Naples in 1817.
Piazzi "Lezioni
elementari di astronomia" in 1817.
Palermo, Sicily  
199 YBN
[06/??/1801 AD]
2368)
London, England  
199 YBN
[11/12/1801 AD]
2405) Thomas Young (CE 1773-1829) determines frequencies and wavelengths
(particle intervals) of light, uses glass diffraction gratings, and puts
forward a theory of light interference.

Young puts forward the theory of light wave interference (to explain lines of
diffraction). This theory states that two (or more) light waves interfere with
each other, where light waves can add together and subtract or cancel each
other out, similar to the way two sound waves can add to or cancel each other
out to produce silence.

Young supports the theory of light as a wave in an aether medium (aether being
like air for sound), which Grimaldi, Huygens, Hooke, Malebranche, Euler and
others supported. Young refers to this theory as the "undulatory" theory.

Young proposes that instead of the retina containing an infinite number of
particles each capable of vibrating in unison with every possible color, there
is only a need for one sensor for each principle color red, yellow and blue.

Young publishes these propositions in "On the theory of light and colors".

Albert Michelson will use this principle of interference to create an
interferometer.

I reject a wave theory for light, in favor of a light as a particle that moves
in straight lines. However, this principle of color determined by photon
interval is still a very important truth without an aether or wave
interpretation. I think that what is being called light interference may be the
result of particle reflection. There are particle explanations for light
interference. The theory that two rays of light combine to destroy each other
violates the conservation of matter (and energy for those who believe in
energy); that matter would disappear into empty space, and seems to me
unlikely. There are particle explanations for light interference, one is the
photons fall into orbit around each other, another is that photons collide with
each other, another is that photons reflect of the sides of the slits, and
finally another is that photons reflect at different angles depending on atomic
structure of the material reflecting the photons. State what humans offered
particle explanations for interference if any.

This key concept, can light cancel itself out like sound, will be divided
between the two already existing schools of particle or wave interpretation of
light. Even after the theory of an aether medium for light falls with the
Michelson-Morley experiment, this concept of light destruction will continue
for wave supporters. I reject the idea that photons can ever be created or
destroyed, and so I reject the idea that two beams of photons can cancel each
other out since in the view I support no photon can ever be destroyed.

The theory of an aether goes back to Aristoteles to the 4th century BCE, over
2000 years before this time. The Michelson-Morley experiment will finally end
the popularity of the belief in an aether.

Young realizes that in terms of color perception that there is not need for a
separate mechanism in the eye for every color, instead that only 3 mechanisms
are necessary one each for the color red, yellow and blue. This concept is
developed later by the German physicist Hermann L.F. von Helmholtz and is known
as the Young-Helmholtz three-color theory. Color photography, televisions and
LCD displays all use this three color principle. I think the photon detectors
in an eye, perhaps neurons, cannot possibly be sensitive enough to detect a
single beam of photons. Photon detectors in the eye are much larger than the
size of a photon, and may themselves also be composed of photons in the form of
atoms. So many millions of beams are needed to "see" light. A neuron might fire
at a rate that is the sum of two separate frequency beams colliding on the same
neuron surface.

Another problem with the idea of light beams canceling each other out into
empty space, is that if you think that light is made of matter than it is a
violation of the conservation of matter, and even if you think that light is
energy, as is the current view, light canceling itself out into empty space is
a violation of the conservation of energy. Matter, and in the popular "modern"
view, energy, cannot simply disappear into empty space without the equivalent
quantity of energy appearing in some other form. In the example of two sound
waves canceling each other into silence, the velocities of the particles in the
medium (air or sound) oppose each other and result in no motion, however for
light no medium has ever been observed, and in my view, there cannot be a wave
without a medium. Given this intuitive piece of evidence, that conservation of
matter and velocity should be observed, every alternative particle
interpretation should be explored in my view. Equating interference patterns
based on color, to determine frequency of light is a major scientific
contribution, and this contribution is still accurate for a particle theory of
light too.
London, England  
199 YBN
[1801 AD]
1232) Philippe Pinel (April 20, 1745 - October 25, 1826), a French physician,
publishes "Traité médico-philosophique sur l'aleniation mentale; ou la
manie". This books will be translated into English in 1806 as "Treatise on
Insanity", and will have an enormous influence on both French, English and
American psychiatrists during the 1800s. The profession of psychiatrists will
grow into a large industry similar to chiropracters and accupuncturers, mostly
benign light-weight science of talk or touch-based therapies, however with
psychiatry there is attached to the payer the illogical stigma of mental
incompetence or unpredictable and/or violent behavior.

Pinel explains that insanity not due to "lesion of the brain", but that humans
have delusions because of shocks of life, for example disappointed love,
business failure, and poverty. Psychology will come to be viewed as distinctly
different from neurology which is the study of nervous system disorders with
physically measurable causes, while most of psychology is pseudoscience being
mostly filled with meaningless abstract "diseases" (such as psychosis,
neurosis, schitzophrenia) and/or overly trivial "diseases" (manic depression,
delusions of grandeur, attention deficit hyperactivity disorder) without clear
definitions or symptoms most of which can be reduced to simply inaccurate
beliefs or delusion. In his book Pinel defines 5 specific types of "insanity".


While at Bicêtre Hospital Pinel does away with bleeding, purging, and
blistering in favor of a therapy that involves close contact with and careful
observation of the patient-prisoners. Pinel visits each prisoner, often several
times a day, and takes careful notes over two years. He engages them in lengthy
conversations. His objective is to assemble a detailed case history and a
natural history of each person's supposed illness.

This is after the French Revolution which brings more moral "treatment" of
those people locked in psychiatric hospitals. Two years before in 1795, Pinel
was appointed chief physician of the Hospice de la Salpêtrière by the new
republic government, a post that he retains for the rest of his life. The
Salpêtrière is, at the time, like a large village, with seven thousand women.
Pinel misses Pussin, and in 1802 secures Pussin's transfer to the
Salpêtrière. Pinel creates an inoculation clinic in his service at the
Salpêtrière in 1799 and the first vaccination in Paris is given there
(perhaps without consent) in April 1800. Inspired by Pussin, Pinel takes a more
humane view of people that are brought to the hospital. Pinel is skeptical of
treatments in medical texts, which he describes as "rarely useful and
frequently injurious" methods formed from "prejudces, hypotheses, pedantry"
(condescending and overly detailed opinions)", ignorence, and the authority of
celebrated names." However, Pinel condones the use of threats and chains when
other means fail. Pinel like many others fails to distinguish clearly between
violent and nonviolent people, mixing the two together instead of requesting to
move the violent to a prison or establishing a more restricted violent-only
section within the psychiatric hospital, and indeed he inflicts assaults on the
prisoners himself.

Paris, France  
199 YBN
[1801 AD]
2127) In 1751 Lalande goes to Berlin to measure the parallax of the moon in
conjunction with Lacaille at the Cape of Good Hope.
In 1798 Lalande makes a balloon
ascension.
Lalande suggests improvements to the parachute.
Lalande is openly anti-Jacobin
and saves many threatened by the Reign of Terror. The Jacobin club is the most
famous political group of the French Revolution, which will become identified
with extreme egalitarianism (belief in human equality) and violence and which
leads the Revolutionary government from mid-1793 to mid-1794, dominated at one
point most famously by Maximilien Robespierre.
Lalande opposes the war policies
of Napoleon Bonaparte.

Other works by Lalande are "Traité d'astronomie" (1764; "Treatise on
Astronomy"), and "Bibliographie astronomique" (1803; "Astronomical
Bibliography").
Paris, France (presumably)  
199 YBN
[1801 AD]
2169)
Paris?, France (presumably)  
199 YBN
[1801 AD]
2209)
Paris, France (presumably)  
199 YBN
[1801 AD]
2238)
Paris, France (presumably)  
199 YBN
[1801 AD]
2256)
Paris, France  
199 YBN
[1801 AD]
2268)
Berlin, Germany  
199 YBN
[1801 AD]
2319) Antoine François, comte de Fourcroy (FURKrWo) (CE 1755-1809), publishes
"A General System of Chemical Knowledge" (11 vol., 1801-2; tr. 1804).

Paris, France (presumably)  
199 YBN
[1801 AD]
2349) Del Rio is chosen by Charles III to learn about mining in France,
England, and Germany in order to develop and modernize the mining industry for
the Spanish Empire.
In 1794, Del Rio is sent to Mexico City to become a professor of
mineralogy at the School of Mines set up by Fausto D'Elhuyar.

Del Rio is forced into exile from 1829-34 after Mexico's war of independence
but returns.

(What is the routine of chemists to analyze ores? How does Del Rio know that he
may have a new element?)


Vanadium is a bright white, soft, ductile metallic element found in several
minerals, notably vanadinite and carnotite. 4 dict]
Vanadium is used to make
rust-resistant steels, and as a catalyst.
Vanadium is atomic number 23; atomic weight
50.942; melting point 1,890°C; boiling point 3,000°C; specific gravity 6.11;
valence 2, 3, 4, 5.
Mexico City, Mexico (presumably)  
199 YBN
[1801 AD]
2350) Niobium is a silvery, soft, ductile metallic element that occurs
primarily in columbite-tantalite and is used in steel alloys, arc welding, and
superconductivity research.
Niobium is atomic number 41; atomic weight 92.906;
melting point 2,468°C; boiling point 4,927°C; specific gravity 8.57; valence
2, 3, 5.


Hatchett is the son of a wealthy coach builder in London, who builds coaches
for royalty. The young Hatchett is said to have turned down an offer from his
father of £3,000 and a seat in Parliament to give up chemistry.

In 1950, the name Niobium will be chosen as the official name for this element
by the International Union of Pure and Applied Chemistry.
  
199 YBN
[1801 AD]
2357) Fulton submits plans to (the government of) France for a submarine which
Fulton argues can help France overcome Britain's naval supremecy. Fulton builds
the Nautilus in 1800, and the submarine works better than any previous
submarine, although much of the submarine is modeled on one designed by David
Bushnell in 1776. The Nautilus is reconstructed and improved in 1801, but the
French government still rejects the project.
Benjamin Franklin poses for Fulton who
paints his portrait.
Fulton is in the process of building a steam warship when
he dies.

Fulton is a member of the 1812 commission that recommends building the Erie
Canal.

In 1813-15 Fulton adapts a catamaran steam ship into the first steam warship or
"steam battery", but the War of 1812 ends before the ship is used.
  
199 YBN
[1801 AD]
2374) It seems unlikely to me that some atoms of gas being larger would exert
more pressure, occupying more space, in addition to offering more matter to
collide with. Perhaps atoms are too small for any difference to be measured, or
perhaps Dalton's law is true and size and mass does not affect pressure.
Manchester, England  
199 YBN
[1801 AD]
2399)
Cornwall, England (presumably)  
199 YBN
[1801 AD]
2404)
London, England  
199 YBN
[1801 AD]
2438)
Jena, Germany (presumably)  
199 YBN
[1801 AD]
2444)
Göttingen, Germany  
199 YBN
[1801 AD]
2445) In his teens Gauss worked out the method of least squares, advancing the
work of Legendre and this is the method Gauss uses to calculate the orbit of
Ceres.
Göttingen, Germany  
199 YBN
[1801 AD]
2508) Hare is the son of a prominent businessman and state senator. Hare is
educated at home, then studies chemistry under James Woodhouse.
Hare's father owns a
brewery but the war of 1812 causes the brewery to fail.
Hare teaches briefly at
the College of William and Mary in Virginia.
From 1818-1847 Hare is professor of
chemistry at the University of Pennsylvania.
In 1854, Hare writes a large book on
communicating with spirits and claims that Benjamin Franklin's spirit (from the
dead) had validated his electrical theories.
Philadelphia, Pennsylvania (presumably)  
199 YBN
[1801 AD]
3382)
Paris, France (presumably)  
199 YBN
[1801 AD]
3388)
Philadelphia, PA, USA  
199 YBN
[1801 AD]
4543)
unknown  
199 YBN
[1801 AD]
5973)
Vienna, Austria (presumably)  
198 YBN
[03/??/1802 AD]
2332)
Bremen, Germany  
198 YBN
[07/01/1802 AD]
3296)
London, England  
198 YBN
[08/03/1802 AD]
2845) Here is the translation of the second more detailed report:
"Gazzetta di Rovereto
(13 August, 1802 )
The Counsellor, Giandomenico de Romagnosi, living in Trento,
known to the
republic of letters by his learned productions, hastens to communicate
to the physicists
of Europe an experiment showing the action of the galvanic fluid on
magnetism.
Having constructed a voltaic pile, of thin discs of copper and zinc,
separated by
flannel soaked in a solution of sal-ammoniac, he attached to one of
the poles one
end of a silver chain, the other end of which passed through a short
glass tube, and
terminated in a silver knob.
This being done, he took an ordinary
compass-box, placed it on a glass stand,
removed its glass cover and touched one end
of the needle with the silver knob, which
he took care to hold by its glass envelope.
After a few seconds contact the needle was
observed to take up a new position,
where it remained even after the removal of the
knob. A fresh application of the
knob caused a still further deflection of the needle,
which was always observed to
remain in the position to which it was last deflected, as
if its polarity were
altogether destroyed.
In order to check this result he approached to the magnetic
needle at the smallest
possible distance (without touching it) either a watch spring or
other iron objects, which
before attracted the magnetic needle very strongly at a
distance four times larger; but
now, under the action of galvanism, had no effect
at all.
To ensure success to the experiment, one needs the following
precautions: not all
the galvanic piles are good for the experiment, but only the
ones whose discs have at
least a thickness of a 'linea' and are two inches of
diameter; it is convenient to use an
insulated pile, and not for a long time in
order to avoid rapid oxidation at the surface
of the discs; it is convenient to keep
the chains suspended in such a way that they
do not touch any body conducting
electricity and to handle them with the glass tube;
sometimes in order to ensure
rapid success to the experiment it is convenient to touch
the point of the needle
with both knobs and then to make it deviate with one of them;
and not forgetting
before that to handle the chains with bare hands in order to excite
the apparatus,
since the galvanic flux has often some interruptions. (clearly here there are
two chains connected to opposite sides of the voltaic pile, and the presumption
is that current is flowing through them.)
The needle used by Mr. Romagnosi was
only one inch of length and one "linea"
of width in the greatest extension near the
pin. It was made of a watch spring well
equilibrated and suspended on a steel pin.

In order to restore the polarity, Romagnosi took the compass box between his
fingers
and thumbs, and held it steadily for some seconds. The needle then returned to
its
original position, not all at once, but little by little, advancing like the
minute or second
hand of a clock.
He then put the needle under the action of
Electricity, both vitreous and resinous,
using a tube of rubbed glass or sealing-wax
("cera di Spagna""). The needle was strongly
attracted and at some distance from the
pipe, while with the knob it did not move. After
removing the tubes the needle
returned to the previous polar direction, while in the ex-
periment with galvanism
it remained in the same deflected position. The magnetic action
of a piece of iron,
which under the action of the galvanic fluid had no effect on the nee-
dle, was
stronger than the opposite force of electricity that was simultaneously
applied.
This experience was made in the month of May, and repeated in the presence
of a
few spectators. In that occasion he also observed very easily the electrical
attraction at
a very sensitive distance. He used a thin thread soaked in a
solution of sal-ammoniac,
and it fastened it to a glass pipe, he then approached the silver
chain to the thread at
the distance of a "linea" and saw the thread flying and
remaining attached to the knob
as in typical electrical experiments.
Mr. Romagnosi believes
it is his duty to publish this experiment that should be-
come part of a treatise
on Galvanism and Electricity in which he plans to discuss an
atmospheric
phenomenon that takes place every year near the Brenner and that strongly
affects the
local population which feels all the effects of galvanism."
(see also Govi's translation)
Trento, Italy  
198 YBN
[1802 AD]
2186)
Slough, England  
198 YBN
[1802 AD]
2239)
Paris, France (presumably)  
198 YBN
[1802 AD]
2245)
Paris, France (presumably)  
198 YBN
[1802 AD]
2365) William Hyde Wollaston (WOLuSTuN) (CE 1766-1828) identifies dark spectral
lines in the spectrum of light from the Sun, however wrongly interprets them as
the natural boundaries of each color.

Wollaston reports this as "A Method of Examining Refractive and Dispersive
Powers, by Prismatic Reflection" in the Philosophical Transactions of the Royal
Society in 1802.

In this paper Wollaston describes his experiment:
"If a beam of day-light be
admitted into a dark room by a crevice of 1/20 an inch broad, and received by
the eye at the distance of 10 or 12 feet, through a prism of flint-glass, free
from veins
, held near the eye, the beam is seen to be separated into the four
following colours only, red, yellowish-green, blue, and violet; in the
proportions represented in Fig 3."

Wollaston goes on to describe the discontinuous spectrum of light from a source
other than the Sun, writing "By candle-light, a different set of appearances
may be distinguished. When a very narrow line of the blue light at the lower
part of the flame is examined alone, in the same manner through a prism the
spectrum ,may be seen divided into five images, at a distance from each other.
The first is broad red, terminated by a bright line of yellow; the 2nd and 3d
are both green; the 4th and 5th are blue, the last of which appears to
correspond with the division of blue and violet in the solar spectrum, or the
line D of Fig 3.
When the object viewed is a blue line of electric light, I have
found the spectrum to be also separated into several images; but the phenomena
are somewhat different from the preceding. It is, however, needless to describe
minutely, appearances which vary according to the brilliancy of the light, and
which I cannot undertake to explain."

It is interesting to note that the spectral "lines" are due to the way light of
different frequencies separates in a prism (or when reflected off a diffraction
grating), and the line is the image of the light passing through a slit
separated into many identical slit copies over the spectrum. So by isolating a
single frequency by viewing only one line of the spectrum, a person can see the
universe at a very specific frequency of light only. in fact, the universe can
be viewed only seeing the light emitted at many frequencies and any specific
frequency just by only viewing the light of one spectral line (although the
image has a very high vertical to horizontal aspect ratio, it can be spread out
farther after initial separation). For example, the Sun can be seen in many
different colors (frequencies) simply by viewing different spectral lines or
spectral dots by using a pinhole instead of a slit. Each dot is a distinct
image of the Sun.

(If seeing eyes and thought was first done in 1810, William, or
"Bill" Wollaston may have played an important part in the secret unpublished
development. That would put Wollaston and this finding within the time range to
be the originator of this finding if in 1810. It seems to me and no doubt to
many other outsiders that do not see, hear or send thought images or sounds,
that this would be too far in the past, and Pupin in 1910 or earlier seems more
likely. But what is all the talk about "ten" before 1910? For example, Faraday
refers to things not being "tenable", but most obviously in a major obituary in
the Proceedings of the Royal Society for Charles Wheatstone, the word
"tenement" is used near the end. This has to be beyond coincidence, but does it
refer to the year 1810? And then, what happened in the year 1810 that was so
important and was so closely related to Charles Wheatstone? Wheatstone's
obituary also ends with "Better World" ("BW") which might refer to Bill
Wollaston, but it is purely a guess.)
London, England  
198 YBN
[1802 AD]
2377) Tantalum is a very hard, silver-gray metal of Group Vb of the periodic
table, characterized by its high density, extremely high melting point, and
excellent resistance to all acids except hydrofluoric at ordinary
temperatures.

Tantalum has atomic number 73; atomic weight 180.948; melting point 2,996°C;
boiling point 5,425°C; relative density 16.6; valence 2, 3, 4, 5.

Tantalum is relatively rare, about as abundant as uranium.

Tantalum capacitors have the highest capacitance per unit volume of any
capacitors and are used extensively in miniaturized electrical circuitry.

Tantalum is quite inert to acid attack except by hydrofluoric acid.

For some time Tantalum is confused with niobium.
Uppsala, Sweden  
198 YBN
[1802 AD]
2439)
Gotha, Germany  
198 YBN
[1802 AD]
2464) In 1805 and 1806 Gay-Lussac travels with Humboldt measuring terrestrial
magnetism.
Napoleon funds Gay-Lussac and his long-time friend and co-worker Thénard to
build a powerful battery to compete with Davy in England who is finding new
elements through the action of electricity.

Gay-Lussac approaches the study of matter as volume-centered as opposed to
mass-centered as English contemporary John Dalton does.

In Gay-Lussac's publications are found the first use of the chemical terms
burette, pipette, and titrate. Titration is a method or the process of
determining the concentration of a dissolved substance in terms of the smallest
amount of a reagent of known concentration required to bring about a given
effect in reaction with a known volume of the test solution. For example,
Gay-Lussac estimates (the quantity) of silver in solution (1832), which
Gay-Lussac titrates with a solution of sodium chloride of known strength.
Gay-Lussac is
the son of a judge who is imprisoned during the French Revolution.
Gay-Lussac's
mathematical ability enables him to pass the entrance examination for the newly
founded École Polytechnique, where students' expenses are paid by the state
(and tuition?).
In 1801 Gay-Lussac becomes chemist Claude-Louis Berthollet's research
assistant at Arcueil.
Gay-Lussac works with Berthollet's son in a factory where chlorine
is used to bleach linen.
In 1808 Gay-Lussac is granted a professorship in physics at
the Faculty of Science in Paris upon its founding.
In 1810 Gay-Lussac receives a
professorship in chemistry at the École Polytechnique.
In 1831 Gay-Lussac is elected to
French Chamber of Deputies under the new regime of Louis-Phillippe.
In 1839 Gay-Lussac enters
the upper house, the Chamber of Peers.
Arcueil, France (presumably)  
198 YBN
[1802 AD]
2484)
London, England  
198 YBN
[1802 AD]
2819)
London, England  
198 YBN
[1802 AD]
5974) Ludwig van Beethoven (CE 1770-1827), German composer, composes his Piano
Sonata 17 in D minor, "Tempest" (opus 31).

Vienna, Austria (presumably)  
197 YBN
[02/27/1803 AD]
3599)
Calais, France  
197 YBN
[10/21/1803 AD]
2375) John Dalton (CE 1766-1844) shows that atoms of different elements vary in
size and mass, and makes the first table of elements by atomic mass.

Dalton theorizes that each chemical element has distinct atoms, and begins to
work out the atomic structures of compounds.

Dalton claims that atoms of different elements vary in size and mass. Before
this, supporters of atomic theory from the times of Democritos to the 1700s
Ruggero Boscovich all believed that atoms of all kinds of matter are alike,
(that is that all atoms are the same size and mass).

Many people believe that having so many different fundamental particles, with
each element having its own kind of atom appear to go against a view of the
simplicity of nature.

Dalton focuses on determining the relative mass of each different kind of atom,
a process that Dalton claims can be accomplished by considering the number of
atoms of each element contained in different chemical compounds.

In a memoir read to the Manchester Literary and Philosophical Society, "On the
Absorption of Gases by Water and Other Liquids", Dalton describes his method of
measuring the masses of various elements according to the way each element
combines with fixed masses of each other. For these measurements of masses to
be meaningful, the elements have to combine in fixed proportions as the French
chemist Joseph-Louis Proust claimed (against the opposition of Claude-Louis
Berthollet).

In the last section of the paper is the first table of atomic weights giving
Hydrogen a value of 1.

Dalton creates the "Law of Multiple Proportions", which is when two elements
form more than one compound, the masses of one element that combine with a
fixed mass of the other are in a ratio of small whole numbers. For example
using elements A and B, various combinations between A and B happen according
to the mass ratios A to B being 1 to 1, 1 to 2, 2 to 1, etc. Proust had shown
in 1788 with the law of definite proportions that compounds only consist of
elements in integer ratios by weight, for example 4 to 1, never 4.1 to 1 or 3.9
to 1. Dalton finds this for methane (carbon:hydrogen= 3:1) and ethylene
(carbon:hydrogen = 6:1) and with various oxides of nitrogen.

Dalton supposes that carbon monoxide consists of one particle of carbon united
with one particle of oxygen, and that the oxygen particle is 4/3 as heavy as
the carbon particle, while carbon dioxide is composed of a particle of carbon
combined with two oxygen particles. This will later be proven to be true.
Understanding the similarity of this theory to that advanced by Democritos (and
Leukippos) 21 centuries earlier, he therefore calls these tiny particles by
Democritos' own term "atoms". However, where Democritos' theory was a logical
deduction based on speculation, Dalton's theory is based on 150 years of
chemical experimentation. Dalton's theory is a chemical theory not a
philosophical theory. Dalton is the first to advance a quantitative atomic
theory, describing that all elements are composed of tiny indestructible atoms,
and that all substances are composed of combinations of these atoms. One
substance can be turned into another by breaking up a particular combination
and forming a new one. All the atoms of one element are identical but differ
from the atoms of other elements only in mass.

Knowing the ratios of each elements mass cannot be used to determine the actual
number of elemental atoms in each compound. For example, methane contains twice
as much hydrogen as ethylene and so Dalton decides that methane has one carbon
and two hydrogen atoms and ethylene has one carbon and one hydrogen atom. Now
people know that the methane molecule (CH4) has one carbon and 4 hydrogen
atoms, while the ethylene molecule (C2H4 has two carbons and 4 hydrogen atoms.
Since Dalton does not understand that Hydrogen usually exists as a two atom
molecule, Dalton views the mass ratio of methane as 1 carbon to 2 (not 1 to 4),
and ethylene as 1 carbon to 1 hydrogen (not 2 to 4).

Note that in giving the "ultimate particles" (as Dalton describes them) various
masses, the concept of the atom is applied to the elements Hydrogen, and
Oxygen, etc, instead of to the light particles those elements are made of,
which are perhaps more accurately called "atoms", being, in theory indivisible.
What we call "atoms" and "subatomic particles" currently are clearly compounds
of light particles.
Manchester, England  
197 YBN
[11/24/1803 AD]
2406) In terms of the double slit experiment, I have not been able to duplicate
a double-slit causing so-called interference, however I have gotten a single
slit to produce bands of colors, using even a single piece of aluminum or steel
on one side of a cardboard box hole, with scratches on the metal clearly
reflecting spectra of colors from Sun light. In addition I have never seen the
double-slit light interference performed, for example on video. I was also
unable to produce light interference using a kit ordered from a science hobby
store. In the high school I went to, this experiment was demonstrated using
water waves not light. However, it seems clear that what works for one slit
(via a metal with scratches and Sun light) should also work for two or more
slits. Again, in my opinion this effect is an effect of reflection of light off
the inside of the slit. For an experiment that changed the popular paradigm for
over a century, like Fitzgerald, Lorentz's and Einstein's theory of
time-dilation, there are surprisingly few examples of video showing explicit
proof of the phenomena. Michelson will make great use of so-called light
interference. Michelson's use of half-silvered mirrors is evidence for the
phenomenon of light interference. But in terms of the double-slit experiment, I
think it should be duplicated and shown to all people on video. It may be that,
like me, people were unable to duplicate the double-slit interference pattern,
and were too embarrassed to mention it, or believed they simply did the
experiment incorrectly.

Some interesting experiments that result from this conclusion that light
particles reflect off the inside of the slit are:
1) Try various machined
curves for the inside of the slits and see how this effects the distribution of
photons/light (for example, triangular cut, round cut, flat cut, 4-sided,
5-sided cuts, etc.).
2) Put absorbing and reflecting material on the sides of
the slits, is there a difference in the intensity of the so-called "diffracted"
light?
3) Are the "double intensity" lines actually double the intensity or simply the
original intensity? If double then this could be the result of two beams sent
to the same location by reflection like the way a lens or mirror focuses light
to a higher intensity and smaller space, but if the same, then clearly no
doubling is happening. have there been experiments to verify this in the 200
years since Young first found this (1803)?.

This view of light as a wave and not a particle, gains popular using the
double-slit experiment, and light interference as proof, and eventually the
particle theory loses favor. This will set back science for 200 years as people
reject the idea of light as a particle until Planck (and secondarily Einstein
who still views light as massless - Planck sees light as massless too?).
Currently my feeling is that most likely light are beams of particles with
frequencies, point-waves without amplitude, in other words straight lines. I am
one of the only people to support a light as a particle only theory, however
there probably are many people who secretly years before me understood that
light is most likely a particle, is matter, and is the basis of all matter in
the universe, a view rejected publicly by most people in science even today.
That all matter is made of photons is claimed not only by me. For example James
H.L. Lawler at http://users.owt.com/flesher/photonics/photon1.html views the
photon as the basis of all matter, although Lawler views photons as being made
of two different charged particles, and supports an expanding universe theory.
Probably many people have figured out over the years that light particles are
probably the basis of all matter, although secretly, not publicly. In addition
finding the belief that the photon is the basis of all matter is very difficult
to find on the Internet or in archived publications.

As an all encompassing statement about this project. I don't have all the
answers, and in my view there are many things in the universe and in science
that have yet to be explained correctly. I think this is the case for the
double-slit experiment, and how white light spreads into its component
frequencies (or colors). I think a light-as-a-particle explanation will be the
most accurate explanation, but I can only offer my computer simulations which
show that what Grimaldi named diffraction is likely the result of light
reflection off the inside of the walls of the opening which Grimaldi nor Young
accounted for in their diagrams. In my own experiments, I produced a colored
band of light from Sun-light reflected off a single piece of metal covering
part of a hole in a cardboard box (Newton and others found a similar result),
Priestley's describes Dechales experiment of finding colored bands reflected
off of scratches in polished metal, and this is evidence that the band of
colors thought to be from light bending is more likely reflection and not
diffraction or refraction, even as far back as 1674. It seems clear that the
light is spread into colors because of reflection on the inside sides of the
slits.

But this question in particular still needs to be fully explained and modeled
to the majority's satisfaction: What is it about a physical groove, for example
on the back of a CD that causes beams of white light to be spread into finer
beams of different frequencies of particles? It seems to me that:
1) the substance of
the reflecting material is important, it must be mirror like (true?)
2) the shape of
the substance is important, it must have at least one slit/groove, perhaps in a
triangle or other shape.
3) perhaps the reflection is due to some characteristic of
photons, perhaps mass, velocity, and/or frequency. We shouldn't rule these
things out.

The mechanical reason why photons are emitted and absorbed in the same
frequency by a certain atom or molecule needs to be thoroughly explored and
explained in terms of light as beams of particles.

In addition, knowing that there has been at least 100 years of secret research
into seeing, hearing and sending thought images, sounds and muscle movements,
with what seems like millions of microscopic lasers in everybody's house and
apartments, how much has been learned about light but kept secret? How
divergent is the story known to the most informed insiders versus the story
known to the outsider public? Is this separation one of more than 100 years?

One question is: Are the photons that separate into blue and red, always the
same photons that separate into blue and red? Or can a photon that forms a red
frequency later be part of a blue frequency? Clearly red and blue shifted
light is evidence that a photon can be part of beams with a variety of
frequencies.

Why do photons with a closer blue frequency bend more than photon beams with a
more spread out red frequency? Is light made of individual beams of distinct
frequencies?

Is white light composed of a variety of single frequency beams that each
occupy their own line in space, separate from each other and remain
microscopically offset from each other when spread out by a prism or grating,
or are all beams combined into one line in space and then spread out by a prism
or grating? It seems clear that even the most small detectors could not be
small enough to detect a single beam of light particles apart from adjacent
neighborings rays.

A simple light that changes from yellow to green is an example of how
individual beams must change frequency. It's interesting to think that a single
beam might have an irregular frequency. In other words a frequency that changes
every photon, it would probably look like a constant changing of colors. Star
light, and sodium light appear to be much more regular. Perhaps when a photon
is detected or received is not important, only when the second photon is
received, and the beginning of a frequency is what defines a color or
wavelength of light. Michelson wrote about coherence, that some beams of
monochromatic light do not have exact frequency over time.
London, England  
197 YBN
[1803 AD]
2125) In "Temple of Nature" Darwin writes "Organic life beneath the shoreless
waves/Was born and nurs'd in ocean's pearly caves;/ First forms minute, unseen
by spheric glass,/ Move on the mud, or pierce the watery mass;/ These, as
successive generations bloom,/ New powers acquire and larger limbs assume;/
Whence countless groups of vegetation spring,/ And breathing realms of fin and
feet and wing."
Derby, England (presumably)  
197 YBN
[1803 AD]
2235) Cerium is the most abundant of the rare-earth metals of the lanthanoid
series.
Cerium rapidly reacts with water to yield hydrogen, and burns brilliantly when
heated.
Ceria, the second rare earth to be discovered (yttria was first), will be shown
to be a mixture of oxides from which seven elements will be separated during
the course of the next century. These other elements are the lighter rare-earth
metals, from lanthanum (atomic number 57) to gadolinium (atomic number 64),
with the exception of promethium.
Cerium occurs in many minerals. Cerium is
also found among the fission products of uranium, plutonium, and thorium.
Cerium is
named after the asteroid Ceres, which was discovered in 1801.
Berlin, (was Prussia) Germany (presumably)  
197 YBN
[1803 AD]
2244)
Paris, France (presumably)  
197 YBN
[1803 AD]
2273) In the long preface to the French translation of British chemist Thomas
Thomson's "System of Chemistry" (1809), which explains atomic theory,
Berthollet (wrongly) objects to the view that all chemical reactions constantly
combine in definite proportions.

At Arcueil Berthollet equips a private laboratory where he forms an informal
Société d'Arcueil where he invites young scientists to meet with him and his
neighbor Pierre-Simon Laplace, and which forms a center of chemical research.
Arcueil, France   
197 YBN
[1803 AD]
2314) It is interesting that gas combustion guns like hand held laser guns are
not publicly acknowledged but probably exist. Most gun powder guns will be
surpassed by the laser which uses photons and is therefore the fastest gun ever
invented, although photon guns, lasers cannot penetrate as much as a more
massive projectile can.
England  
197 YBN
[1803 AD]
2400) In 1808 Trevithick publicises his steam railway locomotive expertise by
building a new locomotive called 'Catch me who can' and charges one shilling
admission to the "steam circus" which includes a ride which is intended to show
that rail travel is faster than by horse.
South Wales, England  
197 YBN
[1803 AD]
2416) Jean Baptiste Biot (BYO) (CE 1774-1862), French physicist, reports on a
meteorite fall which convinces scientists for the first time that rocks fall
from the sky.

Biot with French physicist François Arago measure properties of
gases.(more detail)
In 1793, after graduating from the college of Louis-le-grand in
Paris, Biot joins the army.
In 1795 Biot takes part in a street riot (biot in a
riot?) (as a royalist) during what is called the "White Terror" attempting to
overthrow the Convention (the group that proclaimed the abolition of the
monarchy and the establishment of the republic), which is crushed by the young
general Napoleon Bonaparte on 13 Vendémiaire, year IV (October 5, 1795). This
marks the end of the French Revolution. As a result Biot is imprisoned for
awhile. Monge pleads successfully for the release of Biot.
In 1797, Biot is appointed
professor of mathematics at the University of Beauvais.
In 1800, Biot becomes professor
of mathematical physics at the Collège de France in 1800.
Biot obtains the favor
from Laplace of reading the proof sheets of the "Mecanique celeste".
According to Asimov,
Biot works out an ingenious mathematical treatment of the particle theory of
light that greatly pleases his old sponsor Laplace. (state paper title)
From 1809-49,
Biot is professor of of astronomy at the Sorbonne.
Biot produces many works, the larger
works being: "Traité de géometrie analytique", 1802 (8th ed., 1834); "Traité
de physique expérimentale et mathématique", 4 vols., 1816; "Précis de
physique", 2 vols., 1817; "Traité d'astronomie physique" ("Elementary Treatise
on Physical Astronomy"), 6 vols. with atlas, 1850; "Mélanges scientifiques et
littéraires", 3 vols., 1858 which is a compilation of many of Biot's
critiques, biographies, and accounts of voyages.

Arago changes to support the wave theory of light and Biot and Arago lose their
friendship.
Biot is atheist most of his life but returns to Catholicism in 1846 (at age
72).

Biot is one of the last to uphold the light is a particle (corpuscular) theory
until Planck and Einstein.

It's interesting that corpuscular supporters completely disappear at some point
around this time in history, as far as I can see - either they do not exist, do
not publicly reveal their belief in a corpuscular theory; or any support of a
corpuscular theory is not published until Planck, and even then, the
corpuscular theory, of light as matter is still not the majority view and still
not published.

In fact, physics research in the field of explaining light as particles and
explaining optics in terms of light particles, for example, explaining how
particles of light enter into atomic lattices, etc. for which progress was
being made (as Priestley, for example describes in his history of optics),
completely stops until Planck.
Paris, France (presumably)  
197 YBN
[1803 AD]
2490) Berzelius is an early Swedish supporter of the new chemistry proposed a
generation earlier by Lavoisier.
Berzelius is one of first to accept Dalton's atomic
theory.
Berzelius does not appreciate Avogadro's hypothesis, and has some confusion
distinguishing between atoms and molecules.
Berzelius develops electrical
theories of molecular structure which are wrong, but will maintain a hold on
chemical thinking for decades because of Berzelius' popularity.
Berzelius grows
conservative in his old age, and is on the wrong side of almost all
controversies.

Berzelius introduces many terms in chemistry such as "catalysis", "isomer",
"polymer", "allotrope", "halogen", "protein". (Berzelius recognizes proteins?)

Over the course of his life, Berzelius publishes more than 250 original papers
and many textbooks.
Berzelius id the son of a clergyman-school-master.
From 1796-1802 Berzelius studies medicine
at Uppsala University.
Berzelius then studies chemistry at the Stockholm School of
Surgery.
From 1807-1832 Berzelius is professor of medicine and pharmacy at the
Karolinska Institute, just outside Stockholm in Solna, Sweden.
In 1835 at age 56
Berzelius marries a fine-looking 24 year old female.
Stokholm, Sweden (presumably)  
197 YBN
[1803 AD]
2502)
Stokholm, Sweden (presumably)  
196 YBN
[01/01/1804 AD]
1533)
Haiti  
196 YBN
[02/22/1804 AD]
3596) Don Francisco Sálva Campillo reads a paper before the Academy of
Sciences at Barcelona, in which he describes using the decomposition of water
with a voltaic pile for the purpose of telegraphy.

This paper is called "The Second Treatise on Galvanism applied to Telegraphy".

Barcelona, Spain  
196 YBN
[04/??/1804 AD]
2551) Audubon is the son of a French merchant, planter, and slave trader and a
Creole woman of Saint-Domingue.
In 1794, Audubon and his half sister are legalized by a regular
act of adoption by his father and his wife.
Audubon's father fought at Yorktown in
alliance with George Washington.
Audubon moves to America to take care of his
father's farm and to avoid Napoleon's draft.
Neither the farm nor any of
Audubon's other business interests succeed and Audubon is declared bankrupt in
1819 and imprisoned.
Audubon works as a taxidermist for some amount of time, makes
portraits and teaches drawing, while his wife works (in child care).
By 1820 Audubon
decides to publish his own collection of animals and birds and spends four
years traveling through Louisiana and Mississippi shooting specimens.
Audubon develops the
new technique of inserting wires into the bodies of freshly killed birds in
order to manipulate them into natural positions for his sketching.
Critics of Audubon's
work have pointed to certain fanciful (or even impossible) poses and inaccurate
details.
In 1886 a bird preservation organization takes Audubon's name and eventually
evolved into the National Audubon Society.
Philadelphia, Pennsylvania  
196 YBN
[1804 AD]
2362) Wollaston earns a medical degree from Cambridge in 1793 and practiced
medicine until 1799 when Wollaston goes into chemistry.

In 1800 Wollaston forms a business partnership with Smithson Tennant, a friend
of Wollaston's from Cambridge, to create and sell chemical products.

Wollaston incorrectly rejects Columbium as a new element.

In 1819 the royal commission Wollaston is on disapproves of adopting the
decimal system of weights and measures (the metric system), and as a result
England and the USA will use the less logical English or common system of
weights and measures. (Asimov states that Britain adopts the metric system but
the USA holds out.)

Wollaston supports Young's wave theory of light.

Wollaston creates the Wollaston annual award from the interest on £1000 to
be awarded annually by the Geological Society, London, for outstanding research
into the mineral structure of the Earth.

Wollastonite, a mineral compound of calcium, silicon, and oxygen, is named in
his honor.
London, England  
196 YBN
[1804 AD]
2363) Palladium has atomic number 46; atomic weight 106.4; melting point
1,552°C; boiling point 3,140°C; relative density 12.02 (20°C); valence 2, 3,
4.

Palladium is a precious, silver-white metal that resembles platinum chemically,
is extremely ductile and easily worked and can be beaten into thin leaf.
Palladium
has a face-centered cubic crystalline structure.
Palladium dissolves in aqua regia.
Palladium
forms many compounds, including oxides, chlorides, fluorides, sulfides,
phosphides, and several complex salts. Palladium has a great ability to absorb
hydrogen; when finely divided, one volume of palladium absorbs as many as 900
volumes of the gas.
London, England  
196 YBN
[1804 AD]
2417) This shows a certain amount of reckless and risky daring on the part of
Biot and Lussac to participate in such a dangerous activity.
Paris, France (presumably)  
196 YBN
[1804 AD]
2440)
{France and}Paderborn, Germany  
196 YBN
[1804 AD]
3767)
Calais, France  
196 YBN
[1804 AD]
5975) Ludwig van Beethoven (CE 1770-1827), German composer, composes his Piano
Sonata No. 21 in C major ("Waldstein") Opus 53.

Vienna, Austria (presumably)  
196 YBN
[1804 AD]
5977) Ludwig van Beethoven (CE 1770-1827), German composer, composes his
Symphony 3. The work is to have been dedicated to Napoleon, a hero to
Beethoven, but Beethoven strikes out the dedication on hearing that Napoleon
takes the title of emperor. Outraged in his republican principles, Beethoven
changes the title to "Eroica" and added the words "for the memory of a great
man.".

(Beethoven was apparently in favor of majority rule and opposed to monarchy.)

Vienna, Austria (presumably)  
195 YBN
[10/??/1805 AD]
2411) In 1800 Banks recommends Brown for the post of naturalist on the
Investigator in an expedition to survey the coast of New Holland (Australia).
From 1806 to
1822 Brown is librarian of the Linnean Society.
In 1810 Banks appoints Brown as his
librarian.
In 1820 when Banks dies Brown is left in charge of Banks' house, library and
collection of plants. In 1827, Brown transfers everything to the British Museum
and remains head of a newly formed botanical department.
London, England (presumably)  
195 YBN
[1805 AD]
2364) Rhodium has atomic number 45; atomic weight 102.905; melting point
1,966°C; boiling point 3,727°C; relative density 12.41; valence 2, 3, 4, 5,
6.

Rhodium is a transition metal and one of the group of platinum metals
(ruthenium, osmium, rhodium, iridium, palladium, and platinum) that share
similar chemical and physical properties.
The terrestrial abundance of rhodium is
exceedingly low; it is estimated to be 0.4 parts per billion in the Earth's
crust. It is found as a single isotope, 103Rh.

Rhodium is a precious, silver-white metal mainly used as an alloying agent for
platinum.

Rhodium has a face-centered cubic crystalline structure.
Rhodium is insoluble in most
acids, including aqua regia, but is dissolved in hot concentrated sulfuric
acid. Rhodium compounds include halides, oxides, sulfates, sulfites, a nitrate,
and a sulfide. The salts form rose-colored aqueous solutions.
London, England  
195 YBN
[1805 AD]
2468)
Paris, France (presumably)  
195 YBN
[1805 AD]
3223) Forsyth receives a patent in April 1807.
Belhelvie, Aberdeenshire, Scotland (presumably)  
195 YBN
[1805 AD]
3389)
Philadelphia, PA, USA  
195 YBN
[1805 AD]
6249)
Philadelphia, PA, USA  
194 YBN
[1806 AD]
2299)
Paris, France(presumably)  
194 YBN
[1806 AD]
2301) Legendre finds a connection between the question "Does the integer p
leave a square remainder on division by q?" and the question "Does the integer
q leave a square remainder on division by p?". Legendre finds that when p and q
are primes, both questions have the same answer unless both primes are of the
form 4n - 1. Because this observation connects two questions in which the
integers p and q play mutually opposite roles, it becomes known as the law of
quadratic reciprocity. (perhaps quadratic should be replaced by "squared" or
"second order").
Legendre also gave a method of extending his law to cases when p and q
are not prime.
Paris, France(presumably)  
194 YBN
[1806 AD]
2346)
Paris, France  
194 YBN
[1806 AD]
2474) For this lecture Davy receives the Napoleon Prize from the Institut de
France, despite the fact that England and France are at war.
Davy accepts the award
saying that the governments may be at war but the scientists are not. (An
enlightened view, but clearly scientists will start to keep very important
secrets in particular in the early 1900s, of course the Pupin seeing eyes, and
CP remotely firing neurons, secrets being the worst cases, but clearly there
must be many secrets, generally kept more from the public than government
scientists, but as an outsider, as to what happened, and what is currently
happening on the tiny Earth we can only guess.)
London, England  
194 YBN
[1806 AD]
2488) Benjamin Silliman (CE 1779-1864) US chemist, introduces Priestley's soda
water to America.

Silliman's report on the potential uses of crude-oil products gives impetus to
plans for drilling the first producing oil well, near Titusville,
Pennsylviania.
Silliman has a degree in law, but is asked by the president of Yale to teach
chemistry since there are no chemists to appoint. Silliman accepts and gets
training at the University of Pennsylvania.
In 1807 Silliman observes a meteorite fall with a
colleague, but (because of backward religious view the majority of people treat
meteor stories as unrealistic). Thomas Jefferson states that it is easier to
believe that two Yankee professors would lie than that stones would fall from
heaven. (Interesting that English settlers had only been in the USA for a
century or two and already there was territorial division.)
New Haven, Connecticut, USA  
194 YBN
[1806 AD]
2491)
Stokholm, Sweden (presumably)  
194 YBN
[1806 AD]
2504) The vessel Nadezhda ("Hope") commanded by Krusenstern, completes the
first Russian circumnavigation of the Earth.

?, Russia  
193 YBN
[03/29/1807 AD]
2333)
Bremen, Germany  
193 YBN
[08/17/1807 AD]
2358) This is the first commercially successful steamboat in the U.S.
Albany, New York, USA  
193 YBN
[10/06/1807 AD]
2476) Potassium is a soft, silver-white, highly or explosively reactive
metallic element that occurs in nature only in compounds. Potassium is obtained
by electrolysis of its common hydroxide and found in, or converted to, a wide
variety of salts used especially in fertilizers and soaps.
Potassium has atomic number
19; atomic weight 39.098; melting point 63.65°C; boiling point 774°C;
relative density 0.862; valence 1.

Potassium is extremely reactive, and more reactive than sodium. Potassium
combines so readily with oxygen that Potassium is usually stored submerged in
kerosene or some other hydrocarbon, out of contact with air (Kerosene is
flammable, is that the safest liquid to use?). (Show chemical equation of
potassium and oxygen). Potassium reacts violently with water to form potassium
hydroxide, KOH, releasing hydrogen, which usually ignites.

Like the other alkali metals, potassium reacts violently with water producing
hydrogen. The reaction is notably more violent than that of lithium or sodium
with water, and is sufficiently exothermic that the evolved hydrogen gas
ignites.

2K(s) + 2H2O(l) → H2(g) + 2KOH(aq)


Potassium combines directly with the halogens, sulfur, and other nonmetallic
elements (except nitrogen).

The metal has limited use since it so closely resembles sodium, which is
readily available at lower cost.

Potassium is the second least dense metal; only lithium is less dense. It is a
soft, low-melting solid that can easily be cut with a knife. Freshly cut
potassium is silvery in appearance, but in air it begins to tarnish toward grey
immediately. Potassium must be protected from air for storage to prevent
disintegration of the metal from oxide and hydroxide corrosion.

Potassium and its compounds emit a violet color in a flame. This fact is the
basis of the flame test for the presence of potassium in a sample. (Interesting
that the atom emits the same color perhaps after separating from some compound
molecule?)
London, England  
193 YBN
[10/13/1807 AD]
2477) Sodium is a soft, light, extremely malleable silver-white metallic
element that reacts explosively with water, is naturally abundant in combined
forms, especially in common salt, and is used in the production of a wide
variety of industrially important compounds.
Sodium has atomic number 11; atomic weight
22.99; melting point 97.8°C; boiling point 892°C; relative density 0.971;
valence 1.

Sodium is a dietary essential mineral, whose requirements are usually satisfied
by the normal diet. Sodium deficiency is rare, but it can occur if losses from
heavy sweating are not replaced. A deficiency leads to nausea and muscular
cramps.

Sodium oxidizes rapidly in air and reacts violently with water, liberating
hydrogen (which may ignite) and forming the hydroxide. Sodium must be stored
out of contact with air and water and should be handled carefully. Sodium
combines directly with the halogens. Sodium metal is usually prepared by
electrolysis of the fused chloride (the Downs process); formerly, the chief
method of preparation was by electrolysis of the fused hydroxide (the Castner
process). Metallic sodium has limited use. Metallic sodium is used in sodium
arc lamps for street lighting; pure or alloyed with potassium, and is used as a
heat-transfer liquid, for example in certain nuclear reactors. Sodium compounds
are used through many industries. (Show equations for oxygen and water)

Compared with other alkali metals, sodium is generally less reactive than
potassium and more reactive than lithium.
London, England  
193 YBN
[11/23/1807 AD]
2407) (probably put complete text from light lecture here)
"THE nature of light is a
subject of no material importance to the concerns of life or to the practice of
the arts, but it is in many other respects extremely interesting, especially as
it tends to assist our views both of the nature of our sensations, and of the
constitution of the universe at large. The examination of the production of
colours, in a variety of circumstances, is intimately connected with the theory
of their essential properties, and their causes; and we shall find that many of
these phenomena will afford us considerable assistance in forming our opinon
(known error) respecting the nature and origin of light in general.
It is allowed on
all sides, that light either consists in the emission of very minute particles
from luminous substances, which are actually projected, and continue to move
with the velocity commonly attributed to light, or in the excitation of an
undulatory motion, analogous to that which constitutes sound, in a highly light
and elastic medium pervading the universe; but the judgments of philosophers of
all ages have been much divided with respect to the preference of one or the
other of these opinions. There are also some circumstances which induce those,
who entertain the first hypothesis, either to believe, with Newton (Ph. Tr.
vii. 5087), that the emanation of the particles of light is always attended by
the undulations of an etherial medium, accompanying it in its passage, or to
suppose, with Boscovich (Dissertatio de Lumine, Part II. 1748; and Theoria
Philosophia Naturalis, 410, Venice, 1763, p. 230.), that the minute particles
of light themselves receive, at the time of their emission, certain rotatory
and vibratory motions, which they retain as long as their projectile motion
continues. These additional suppositions, however necessary they may have been
thought for explaining some particular phenomena, have never been very
generally understood or admitted, although no attempt has been made to
accommodate the in any other manner to those phenomena.
We shall proceed to examine in
detail the manner in which the two principal hypotheses respecting light may be
applied to its various properties and affections; and in the first place to the
simple propagation of light in right lines through a vacuum, or a very rare
homogeneous medium. In this circumstance there is nothing inconsistent with
either hypothesis; but it undergoes some modifications, which require to be
noticed, when a portion of light is admitted through an aperture, and spreads
itself in a slight degree in every direction. In this case it is maintained by
Newton that the margin of the aperture possesses an attractive force, which is
capable of inflecting the rays: but there is some improbability in supposing
that bodies of different forms and of various refractive powers should possess
an equal force of inflection, as they appear to do in the production of these
effects; effects and there is reason to conclude from experiments, that such a
force, if it existed, must extend to a very considerable distance from the
surfaces concerned, at least a quarter of an inch, and perhaps much more, which
is a condition not easily reconciled with other phenomena. In the Huygenian
system of undulation, this divergence or diffraction is illustrated by a
comparison with the motions of waves of water and of sound, both of which
diverge when they are admitted into a wide space through an aperture, so much
indeed that it has usually been considered as an objection to this opinion,
that the rays of light do not diverge in the degree that would be expected if
they were analogous to the waves of water. But as it has been remarked by
Newton, that the pulses of sound diverge less than the waves of water, so it
may fairly be inferred, that in a still more highly elastic medium, the
undulations, constituting light, must diverge much less than either. (Plate XX.
Fig. 266.)

With respect, however, to the transmission of light through perfectly
transparent mediums of considerable density, the system of emanation labours
under some difficulties. It is not to be supposed that the particles of light
can perforate with freedom the ultimate atoms of matter, which compose a
substance of any kind ; they must, therefore, be admitted in all directions
through the pores or interstices of those atoms ; for if we allow such
suppositions as Boscovich's, that matter itself is penetrable, that is,
immaterial, it is almost useless to argue the question further. It is certain
that some substances retain all their properties when they are reduced to the
thickness of the ten millionth of an inch at most, and we cannot therefore
suppose the distances of the atoms of matter in general to be so great as the
hundred millionth of an inch. Now if ten feet of the most transparent water
transmits, without interruption, one half of the light that enters it, each
section or stratum of the thickness of one of these pores of matter must
intercept only about one twenty thousand millionth, and so much must the space
or area occupied by the particles be smaller than the interstices between them,
and the diameter of each atom must be less than the hundred and forty
thousandth part of its distance from the neighbouring particles ; so that the
whole space occupied by the substance must be as little filled as the whole of
England would be filled by a hundred men, placed at the distance of about
thirty miles from each other. This astonishing degree of porosity is not indeed
absolutely inadmissible, and there are many reasons for believing the statement
to agree in some measure with the actual constitution of material substances ;
but the Huygenian hypothesis does not require the disproportion to be by any
means so great, since the general direction and even the intensity of an
undulation would be very little affected by the interposition of the atoms of
matter, while these atoms may at the same time be supposed to assist in the
transmission of the impulse, by propagating it through their own substance.
Euler indeed imagined that the undulations of light might be transmitted
through the gross substance of material bodies alone, precisely in the same
manner as sound is propagated ; but this supposition is for many reasons
inadmissible.
A very striking circumstance, respecting the propagation of light, is the
uniformity of its velocity in the same medium. According to the projectile
hypothesis, the force employed in the free emission of light must he about a
million million times us great as the force of gravity at the earth's surface ;
and it must either act with equal intensity on all the particles of light, or
must impel some of them through a greater space than others, if its action be
less powerful, since the velocity is the same in all cases; for example, if the
projectile force is weaker with respect to red light than with respect to
violet light, it must continue its action on the red rays to a greater distance
than on the violet rays. There is no instance in nature besides of a simple
projectile moving with a velocity uniform in all cases, whatever may be its
cause, and it is extremely difficult to imagine that so immense a force of
repulsion can reside in all substances capable of becoming luminous, so that
the light of decaying wood, or of two pebbles rubbed together, may be projected
precisely with the same velocity as the light emitted by iron burning in oxygen
gas, or by the reservoir of liquid fire on the surface of the sun. Another
cause would also naturally interfere with the uniformity of the velocity of
light, if it consisted merely in the motion of projected corpuscles of matter ;
Mr Laplace has calculated (Zachs Geographische Ephemeriden, iv. 1.), that if
any of the stars were 250 times as great in diameter as the sun, its attraction
would be so strong as to destroy the whole momentum of the corpuscles of light
proceeding from it, and to render the star invisible at a great distance ; and
although there is no reason to imagine that any of the stars are actually of
this magnitude, yet some of them are probably many times greater than our sun,
and therefore large enough to produce such a retardation in the motion of their
light as would materially alter its effects. It is almost unnecessary to
observe that the uniformity of the velocity of light, in those spaces which are
free from all material substances, is a necessary consequence of the Huygenian
hypothesis, since the undulations of every homogeneous elastic medium are
always propagated, like those of sound, with the same velocity, as long as the
medium remains unaltered.
On either supposition, there is no difficulty in explaining
equality of the angles of incidence and reflection ; for these angles are equal
as well in the collision of common elastic bodies with others incomparably
larger, as in the reflections of the waves of water and of the undulations of
sound. And it is equally easy to demonstrate, that the sines of the angles of
incidence and refraction must be always in the same proportion at the same
surface, whether it be supposed to possess an attractive force, capable of
acting on the particles of light, or to be the limit of a medium through which
the undulations are propagated with a diminished velocity. There are however
some cases of the production of colours, which lead Us to suppose that the
velocity of light must be smaller in a denser than in a rarer medium ; and
supposing this fact to be fully established, the existence of such an
attractive force could no longer be allowed, nor could the system of emanation
be maintained by any one. (Arago put this remark to the test, Annales de
Chimie, lxxi. 49.)
The partial reflection from all refracting surfaces is supposed
by Newton to arise from certain periodical retardations of the particles of
light, caused by undulations, propagated in all cases through an ethereal
medium. The mechanism of these supposed undulations is so complicated, and
attended by so many difficulties, that the few who have examined them have been
in general entirely dissatisfied with them ; and the internal vibrations of the
particles of light themselves, which Boscovich has imagined, appear scarcely to
require a serious discussion. It may, therefore, safely be asserted, that in
the projectile hypothesis this separation of the rays of light of the same kind
by a partial reflection at every refracting surface, remains wholly
unexplained. In the undulatory system, on the contrary, this separation follows
as a necessary consequence. It is simplest to consider the ethereal medium
which pervades any transparent substance, together with the material atoms of
the substance, as constituting together a compound medium denser than the pure
ether, but not more elastic ;(Some modern writers have adopted the contrary
hypothesis, that the ethereal medium which pervades a substance is of the same
density as it is in void space, but that its elasticity is different. See
Neumann, Memoirs of the Academy of Berlin, vol. xxii. for 1835, and Annalen der
Physik, xxv. 418.) and by comparing the contiguous particles of the rarer and
the denser medium with common elastic bodies of different dimensions, we may
easily determine not only in what manner, but almost in what degree, this
reflection must take place in different circumstances. Thus, if one of two
equal bodies strikes the other, it communicates to it its whole motion without
any reflection ; but a smaller body striking a larger one is reflected, with
the more force as the difference of their magnitude is greater ; and a larger
body, striking a smaller one, still proceeds with a diminished velocity ; the
remaining motion constituting, in the case of an undulation falling on a rarer
medium, a part of a new series of motions which necessarily returns backwards
with the appropriate velocity ; and we may observe a circumstance nearly
similar to this last in a portion of mercury spread out on a horizontal table ;
if a wave be excited at any part, it will be reflected from the termination of
the mercury almost in the same manner as from a solid obstacle.
The total reflection of
light, falling, with a certain obliquity, on the surface of a rarer medium,
becomes, on both suppositions, a particular case of refraction. In the
undulatory system, it is convenient to suppose the two mediums to be separated
by a short space in which their densities approach by degrees to each other, in
order that the undulation may lie turned gradually round, so as to be reflected
in an equal angle ; but this supposition is not absolutely necessary, and the
same effects may be expected at the surface of two mediums separated by an
abrupt termination.
The chemical process of combustion may easily be imagined
either to disengage the particles of light from their various combinations, or
to agitate the elastic medium by the intestine motions attending it : but the
operation of friction upon substances incapable of undergoing chemical changes,
as well as the motions of the electric fluid through imperfect conductors,
afford instances of the production of light in which there seems to be no easy
way of supposing a decomposition of any kind. The phenomena of solar phosphori
appear to resemble greatly the sympathetic sounds of musical instruments, which
are agitated by other sounds conveyed to them through the air : it is difficult
to understand in what state the corpuscles of light could be retained by these
substances so as to be reemitted after a short space of time ; and if it is
true that diamonds are often found, which exhibit a red light after having
received a violet light only, it seems impossible to explain this property, on
the supposition of the retention and subsequent emission of the same
corpuscles.
The phenomena of the aberration of light agree perfectly well
with the system of emanation ; and if the ethereal medium, supposed to pervade
the earth and its atmosphere, were carried along before it, and partook
materially in its motions, these phenomena could not easily be reconciled with
the theory of undulation. But there is no kind of necessity for such a
supposition : it will not be denied by the advocates of the Newtonian opinion
that all material bodies are sufficiently porous to leave a medium pervading
them almost absolutely at rest ; and if this be granted, the effects of
aberration will appear to be precisely the same in either hypothesis.
The unusual
refraction of the Iceland spar has been most accurately and satisfactorily
explained by Huygens, on the simple supposition that this crystal possesses the
property of transmitting an impulse more rapidly in one direction than in
another; whence he infers that the undulations constituting light must assume a
spheroidical instead of a spherical form, and lays down such laws for the
direction of its motion, as are incomparably more consistent with experiment
than any attempts which have been made to accommodate the phenomena to other
principles. It is true that nothing has yet been done to assist us in
understanding the effects of a subsequent refraction by a second crystal, (See
additional remarks at the end of this Lecture.) unless any person can be
satisfied with the name of polarity assigned by Newton to a property which he
attributes to the particles of light, and which he supposes to direct them in
the species of refraction which they are to undergo : but on any hypothesis,
until we discover the reason why a part of the light is at first refracted in
the usual manner, and another part in the unusual manner, we have no right to
expect that we should understand how these dispositions are continued or
modified, when the process is repeated.
In order to explain, in the system of
emanation, the dispersion of the rays of different colours by means of
refraction, it is necessary to suppose that all refractive mediums have an
elective attraction, acting more powerfully on the violet rays, in proportion
to their mass, than on the red. But an elective attraction of this kind is a
property foreign to mechanical philosophy, and when we use the term in
chemistry, we only confess our incapacity to assign a mechanical cause for the
effect, and refer to an analogy with other facts, of which the intimate nature
is perfectly unknown to us. It is not indeed very easy to give a demonstrative
theory of the dispersion of coloured light upon the supposition of undulatory
motion; but we may derive a very satisfactory illustration from the well known
effects of waves of different breadths. The simple calculation of the velocity
of waves, propagated in a liquid perfectly elastic, or incompressible, and free
from friction, assigns to them all precisely the same velocity, whatever their
breadth may be : the compressibility of the fluids actually existing
introduces, however, a necessity for a correction according to the breadth of
the wave, and it is very easy to observe, in a river or a pond of considerable
depth, that the wider waves proceed much more rapidly than the narrower. We
may, therefore, consider the pure ethereal medium as analogous to an infinitely
elastic fluid, in which undulations of all kinds move with equal velocity, and
material transparent substances, on the contrary, as resembling those fluids,
in which we see the large waves advance beyond the smaller; and by supposing
the red light to consist of larger or wider undulations and the violet of
smaller, we may sufficiently elucidate the greater refrangibility of the red
than of the violet light (See Cauchy, Memoire sur la Dispersion de la Lumiere,
Prague, 1835. Powell, Ph. Mag. vi. 16, 107, 189, 262. Ph. Tr. 1835, p. 249,
&c.; and Essay on the Undulatory Theory, as applied to the Dispersion of Light.
Challis. Ph. Mag. viii. Kelland, Trans. Camb. Ph. Soc. vi. 153. Difference of
colour was referred to difference of velocity by Melvil, Ph. Tr. 1753, p. 262,
and Essays, ii. 12.).
It is not, however, merely on the ground of this analogy that
we may be induced to suppose the undulations constituting red light to be
larger than those of violet light : a very extensive class of phenomena leads
us still more directly to the same conclusion; they consist chiefly of the
production of colours by means of transparent plates, and by diffraction or
inflection, none of which have been explained upon the supposition of
emanation, in a manner sufficiently minute or comprehensive to satisfy the most
candid even of the advocates for the projectile system; while on the other hand
all of them may be at once understood, from the effect of the interference of
double lights, in a manner nearly similar to that which constitutes in sound
the sensation of a beat, when two strings forming an imperfect unison, are
heard to vibrate together.
Supposing the light of any given colour to consist of
undulations of a given breadth, or of a given frequency, it follows that these
undulations must be liable to those effects which we have already examined in
the case of the waves of water and the pulses of sound. It has been shown that
two equal series of waves, proceeding from centres near each other, may be seen
to destroy each other's effects at certain points, and at other points to
redouble them ; and the beating of two sounds has been explained from a similar
interference. We are now to apply the same principles to the alternate union
and extinction of colours. (Plate XX. Fig. 267.)
In order that the effects of two
portions of light may be thus combined, it is necessary that they be derived
from the same origin, and that they arrive at the same point by different
paths, in directions not much deviating from each other. This deviation may be
produced in one or both of the portions by diffraction, by reflection, by
refraction, or by any of these effects combined ; but the simplest case appears
to be, when a beam of homogeneous light falls on a screen in which there are
two very small holes or slits, which may be considered as centres of
divergence, from whence the light is diffracted in every direction. In this
case, when the two newly formed beams are received on a surface placed so as to
intercept them, their light is divided by dark stripes into portions nearly
equal, but becoming wider as the surface is more remote from the apertures, so
as to subtend very nearly equal angles from the apertures at all distances, and
wider also in the same proportion as the apertures are closer to each other.
The middle of the two portions is always light, and the bright stripes on each
side are at such distances, that the light coming to them from one of the
apertures, must have passed through a longer space than that which comes from
the other, by an interval which is equal to the breadth of one, two, three, or
more of the supposed undulations, while the intervening dark spaces correspond
to a difference of half a supposed undulation, of one and a half, of two and a
half, or more.
From a comparison of various experiments, it appears that the
breadth of the undulations constituting the extreme red light must be supposed
to be, in air, about one 36 thousandth of an inch, and those of the extreme
violet about one 60 thousandth; the mean of the whole spectrum, with respect to
the intensity of light, being about one 45 thousandth. From these dimensions it
follows, calculating upon the known velocity of light, that almost 500 millions
of millions of the slowest of such undulations must enter the eye in a single
second. The combination of two portions of white or mixed light, when viewed at
a great distance, exhibits a few white and black stripes, corresponding to this
interval: although, upon closer inspection, the distinct effects of an infinite
number of stripes of different breadths appear to be compounded together, so as
to produce a beautiful diversity of tints, passing by degrees into each other.
The central whiteness is first changed to a yellowish, and then to a tawny
colour, succeeded by crimson, and by violet and blue, which together appear,
when seen at a distance, as a dark stripe; after this a green light appears,
and the dark space beyond it has a crimson hue; the subsequent lights are all
more or less green, the dark spaces purple and reddish; and the red light
appears so far to predominate in all these effects, that the red or purple
stripes occupy nearly the same place in the mixed fringes as if their light
were received separately.
The comparison of the results of this theory with experiments
fully establishes their general coincidence; it indicates, however, a slight
correction in some of the measures, on account of some unknown cause, perhaps
connected with the intimate nature of diffraction, which uniformly occasions
the portions of light proceeding in a direction very nearly rectilinear, to be
divided into stripes or fringes a little wider than the external stripes,
formed by the light which is more bent. (Plate XXX Fig. 442, 443.)
When the
parallel slits are enlarged, and leave only the intervening substance to cast
its shadow, the divergence from its opposite margins still continues to produce
the same fringes as before, but they are not easily visible, except within the
extent of its shadow, being overpowered in other parts by a stronger light; but
if the light thus diffracted be allowed to fall on the eye, either within the
shadow or in its neighbourhood, the stripes will still appear; and in this
manner the colours of small fibres are probably formed. Hence if a collection
of equal fibres, for example a lock of wool, be held before the eye when we
look at a luminous object, the series of stripes belonging to each fibre
combine their effects, in such a manner, as to be converted into circular
fringes or coronae. This is probably the origin of the coloured circles or
coronae sometimes seen round the sun and moon, two or three of them appearing
together, nearly at equal distances from each other and from the luminary, the
internal ones being, however, like the stripes, a little dilated. It is only
necessary that the air should be loaded with globules of moisture, nearly of
equal size among themselves, not much exceeding one two thousandth of an inch
in diameter, in order that a series of such coronae, at the distance of two or
three degrees from each other, may be exhibited. (Plate XXX. Fig. 444.)
If, on the
other hand, we remove the portion of the screen which separates the parallel
slits from each other, their external margins will still continue to exhibit
the effects of diffracted light in the shadow on each side; and the experiment
will assume the form of those which were made by Newton on the light passing
between the edges of two knives, brought very nearly into contact; although
some of these experiments appear to show the influence of a portion of light
reflected by a remoter part of the polished edge of the knives, which indeed
must unavoidably constitute a part of the light concerned in the appearance of
fringes, wherever their whole breadth exceeds that of the aperture, or of the
shadow of the fibre.
The edges of two knives, placed very near each other, may
represent the opposite margins of a minute furrow, cut in the surface of a
polished substance of any kind, which, when viewed with different degrees of
obliquity, present a series of colours nearly resembling those which are
exhibited within the shadows of the knives: in this case, however, the paths of
the two portions of light before their incidence are also to be considered, and
the whole difference of these paths will be found to determine the appearance
of colour in the usual manner: thus when the surface is so situated, that the
image of the luminous point would be seen in it by regular reflection, the
difference will vanish, and the light will remain perfectly white, but in other
cases various colours will appear, according to the degree of obliquity. These
colours may easily be seen, in an irregular form, by looking at any metal,
coarsely polished, in the sunshine; but they become more distinct and
conspicuous, when a number of fine lines of equal strength are drawn parallel
to each other, so as to conspire in their effects. (Young's Introduction to
Medical Literature, 1813, p. 559.)
It sometimes happens that an object, of
which a shadow is formed in a beam of light, admitted through a small aperture,
is not terminated by parallel sides; thus the two portions of light, which are
diffracted from two sides of an object, at right angles with each other,
frequently form a short series of curved fringes within the shadow, situated on
each side of the diagonal, which were first observed by Grimaldi,
(Physico-Mathesis de Lumine, Coloribus et Iride, Bonon. 1665.) and which are
completely explicable from the general principle, of the interference of the
two portions encroaching perpendicularly on the shadow. (Plate XXX. Fig. 445.)
But
the most obvious of all the appearances of this kind is that of the fringes
which are usually seen beyond the termination of any shadow, formed in a beam
of light, admitted through a small aperture: in white light three of these
fringes are usually visible, and sometimes four; but in light of one colour
only, their number is greater; and they are always much narrower as they are
remoter from the shadow. Their origin is easily deduced from the interference
of the direct light with a portion of light reflected from the margin of the
object which produces them, the obliquity of its incidence causing a reflection
so copious as to exhibit a visible effect, however narrow that margin may be;
the fringes are, however, rendered more obvious as the quantity of this
reflected light is greater. Upon this theory it follows that the distance of
the first dark fringe from the shadow should be half as great as that of the
fourth, the difference of the lengths of the different paths of the light being
as the squares of those distances; and the experiment precisely confirms this
calculation, with the same slight correction only as is required in all other
cases; the distances of the first fringes being always a little increased. It
may also be observed, that the extent of the shadow itself is always augmented,
and nearly in an equal degree with that of the fringes: the reason of this
circumstance appears to be the gradual loss of light at the edges of every
separate beam, which is so strongly analogous to the phenomena visible in waves
of water. The same cause may also perhaps have some effect in producing the
general modification or correction of the place of the first fringes, although
it appears to be scarcely sufficient for explaining the whole of it. (Plate
XXX. Fig. 446.)
A still more common and convenient method of exhibiting the effects
of the mutual interference of light, is afforded us by the colours of the thin
plates of transparent substances. The lights are here derived from the
successive partial reflections produced by the upper and under surface of the
plate, or when the plate is viewed by transmitted light, from the direct beam
which is simply refracted, and that portion of it which is twice {editor: or
more times} reflected within the plate. The appearance in the latter case is
much less striking than in the former, because the light thus affected is only
a small portion of the whole beam, with which it is mixed; while in the former
the two reflected portions are nearly of equal intensity, and may be separated
from all other light tending to overpower them. In both cases, when the plate
is gradually reduced in thickness to an extremely thin edge, the order of
colours may be precisely the same as in the stripes and coronae already
described; their distance only varying when the surfaces of the plate, instead
of being plane, are concave, as it frequently happens in such experiments. The
scale of an oxid (oxide- typo?), which is often formed by the effect of heat on
the surface of a metal, in particular of iron, affords us an example of such a
series formed in reflected light; this scale is at first inconceivably thin,
and destroys none of the light reflected, it soon, however begins to be of a
dull yellow, which changes to red, and then to crimson and blue, after which
the effect is destroyed by the opacity which the oxid acquires. Usually,
however, the series of colours produced in reflected light follows an order
somewhat different: the scale of oxid is denser than the air, and the iron
below than the oxid; but where the mediums above and below the plate are either
both rarer or both denser than itself, the different natures of the reflections
at its different surfaces appear to produce a modification in the state of the
undulations, and the infinitely thin edge of the plate becomes black instead of
white, one of the portions of light at once destroying the other, instead of
cooperating with it. Thus when a film of soapy water is stretched over a wine
glass, and placed in a vertical position, its upper edge becomes extremely
thin, and appears nearly black, while the parts below are divided by horizontal
lines into a series of coloured bands; and when two glasses, one of which is
slightly convex, are pressed together with some force, the plate of air between
them exhibits the appearance of coloured rings, beginning from a black spot at
the centre, and becoming narrower and narrower, as the curved figure of the
glass causes the thickness of the plate of air to increase more and more
rapidly. The black is succeeded by a violet, so faint as to be scarcely
perceptible; next to this is an orange yellow, and then crimson and blue. When
water or any other fluid, is substituted for the air between the glasses, the
rings appear where the thickness is as much less than that of the plate of air,
as the refractive density of the fluid is greater; a circumstance which
necessarily follows from the proportion of the velocities with which light
must, upon the Huygenian hypothesis, be supposed to move in different mediums.
It is also a consequence equally necessary in this theory, and equally
inconsistent with all others, that when the direction of the light is oblique,
the effect of a thicker plate must be the same as that of a thinner plate, when
the light falls perpendicularly upon it; the difference of the paths described
by the different portions of light precisely corresponding with the observed
phenomena. (Plate XXX. Fig. 447...449.)
Sir Isaac Newton supposes the colours of natural
bodies in general to be similar to these colours of thin plates, and to be
governed by the magnitude of their particles. If this opinion were universally
true, we might always separate the colours of natural bodies by refraction into
a number of different portions, with dark spaces intervening; for every part of
a thin plate which exhibits the appearance of colour, affords such a divided
spectrum, when viewed through a prism. There are accordingly many natural
colours in which such a separation may be observed; one of the most remarkable
of them is that of blue glass, probably coloured with cobalt, which becomes
divided into seven distinct portions. It seems, however, impossible to suppose
the production of natural colours perfectly identical with those of thin
plates, on account of the known minuteness of the particles of colouring
bodies, unless the refractive density of these particles be at least 20 or 30
times as great as that of glass or water; which is indeed not at all improbable
with respect to the ultimate atoms of bodies, but difficult to believe with
respect to any of their arrangements constituting the diversities of material
substances.
The colours of mixed plates constitute a distinct variety of the colours of
thin plates, which has not been commonly observed. They appear when the
interstice hetween two glasses nearly in contact, is filled with a great number
of minute portions of two different substances, as water and air, oil and air,
or oil and water; the light which passes through one of the mediums, moving
with a greater velocity, anticipates the light passing through the other; and
their effects on the eye being confounded and combined, their interference
produces an appearance of colours nearly similar to those of the colours of
simple thin plates, seen by transmission; but at much greater thicknesses,
depending on the difference of the refractive densities of the substances
employed. The effect is observed by holding the glasses between the eye and the
termination of a bright object, and it is most conspicuous in the portion which
is seen on the dark part beyond the object, being produced by the light
scattered irregularly from the surfaces of the fluid. Here, however, the
effects are inverted, the colours resembling those of the common thin plates
seen by reflection; and the same considerations on the nature of the
reflections are applicable to both cases. (Plate XXX. Fig. 450.)
The production of
the supernumerary rainbows, which are sometimes seen within the primary and
without the secondary bow, appears to be intimately connected with that of the
colours of thin plates. We have already seen that the light producing the
ordinary rainbow is double, its intensity being only greatest at its
termination, where the common bow appears, while the whole light is extended
much more widely. The two portions concerned in its production must divide this
light into fringes; but unless almost all the drops of a shower happen to be of
the same magnitude, the effects of these fringes must be confounded and
destroyed; in general, however, they must at least cooperate more or less in
producing one dark fringe, which must cut off the common rainbow much more
abruptly than it would otherwise have been terminated, and consequently assist
the distinctness of its colours. The magnitude of the drops of rain, required
for producing such of these rainbows as are usually observed, is between the
50th and the 100th of an inch; they become gradually narrower as they are more
remote from the common rainbows, nearly in the same proportions as the external
fringes of a shadow, or the rings seen in a concave plate.(Young's Exp. and
Obs. relative to Physical Optics, Ph. Tr. 1804, p. 1. Potter, Math.
Considerations on the Rainbow, Tr. Camb. Ph. Soc. vi. 141.). (Plate XXX. Fig.
451.)
The last species of the colours of double lights, which it will be necessary
to notice, constitutes those which have been denominated, from Newton's
experiments, the colours of thick plates, but which may be called, with more
propriety, the colours of concave mirrors. The anterior surface of a mirror of
glass, or any other transparent surface placed before a speculum of metal,
dissipates irregularly in every direction two portions of light, one before and
the other after its reflection. When the light falls obliquely on the mirror,
being admitted through an aperture near the centre of its curvature, it is easy
to show, from the laws of reflection, that the two portions, thus dissipated,
will conspire in their effects, throughout the circumference of a circle,
passing through the aperture; this circle will consequently be white, and it
will be surrounded with circles of colours very nearly at equal distances,
resembling the stripes produced by diffraction. The analogy between these
colours and those of thin plates is by no means so close as Newton supposed it;
since the effect of a plate of any considerable thickness must be absolutely
lost in white light, after ten or twelve alternations of colours at most, while
these effects would require the whole process to remain unaltered, or rather to
be renewed, after many thousands or millions of changes. (Plate XXX. Fig. 452.)

It is presumed, that the accuracy, with which the general law of the
interference of light has been shown to be applicable to so great a variety of
facts, in circumstances the most dissimilar, will be allowed to establish its
validity in the most satisfactory manner. The full confirmation or decided
rejection of the theory, by which this law was first suggested, can be expected
from time and experience alone; if it be confuted, our prospects will again be
confined within their ancient limits, but if it be fully established, we may
expect an ample extension of our views of the operations of nature, by means of
our acquaintance with a medium, so powerful and so universal, as that to which
the propagation of light must be attributed.".


(very interesting comment that light cannot penetrate an atom, my own view is
that light particles can penetrate atoms and of course atoms are composed
strictly of light particles. Also the reference to Laplace's calculation of a
star so massive that particles of light emitted cannot escape, and the
comparison to light waves with would, presumably, not be affected by gravity.
As pertains to a particle explanation of color dispersal and light
interference, I think that possibly particles of the same frequency may collide
with each other through reflection, sending them in different directions based
on their frequencies. In double refraction, passages in the crystal may follow
the cleavage and also go straight through the crystal, making two clear major
pathways for light particles to be transmitted through the crystal and back
which explain why polarizer filter which may only allow beams in one plane can
be used to filter each image. In some sence the concept of diffraction may be
interpreted by later historians as a comedy of errors in that Grimaldi
misinterpreted the reflection phenomenon creating the very unlikely concept of
bending of light around the slit, and then even Newton did not recognize that
this is reflection, finally Young missed this simple reflection, and this
simple mistake continues to this day. So interference and color dispersion are
real phenomena, but I think diffraction is probably only reflection - as is
interference, however for interference I think photons may reflect off
themselves.)
========
ENERGY
In a later lecture describing energy Young writes "The velocity of a body
descending along a given surface, is the same as that of a body falling freely
through an equal height, not only when the surface is a plane, but also when it
is a continued curve, in which the body is retained by its attachment to a
thread, or is supported by any regular surface, supposed to be free from
friction. (Principia, i. 40) We may easily show, by an experiment on a
suspended ball, that its velocity is the same when it descends from the same
height, whatever may be the form of its path, by observing the height to which
it rises on the opposite side of the lowest point. We may alter the form of the
path in which it descends, by placing pins at different points, so as to
interfere with the thread that supports the ball, and to form in succession
temporary centres of motion; and we shall find, in all cases, that the body
ascends to a height equal to that from which it descended, with a small
deduction on account of friction. (Plate II. Fig. 23.)
Hence is derived the idea
conveyed by the term living or ascending force; for since the height to which a
body will rise perpendicularly, is as the square of its velocity, it will
preserve a tendency to rise to a height which is as the square of its velocity
whatever may be the path into which it is directed, provided that it meet with
no abrupt angle, or that it rebound at each angle in a new direction without
losing any velocity. The same idea is somewhat more concisely expressed by the
term energy, which indicates the tendency of a body to ascend or to penetrate
to a certain distance, in opposition to a retarding force.". (So the modern
concept of "energy" is based on the example given by Leibniz of a falling body
reaching the same height. The one flaw is that, the return distance is not the
same as the fall distance, because on return, the Earth's acceleration
decelerates the velocity of the object. However, perhaps the view is that this
loss of energy is accounted for, being lost because of the acceleration caused
by Earth. Does the Earth absorb this lost energy?)
London, England  
193 YBN
[1807 AD]
2313) Lighting by gas combustion will be replaced by the electric light,
although gas is still used for heating and cooking.
London, England  
193 YBN
[1807 AD]
2323)
Montpellier, France (presuambly)  
193 YBN
[1807 AD]
2352)
Chalon-sur-Saône, France (presumably)  
193 YBN
[1807 AD]
2366)
London, England  
193 YBN
[1807 AD]
2380) In 1798 Fourier with Monge and others accompanies Napoleon on Napoleon's
invasion of Egypt.

In 1808 Fourier is created a baron by Napoleon.

After the fall of Napoleon, Fourier's opposition to Napoleon after Napoleon's
return from Elba offsets Fourier's long service under Napoleon.

Fourier believes heat to be essential to health and always keeps his dwelling
place overheated and covers himself in layer upon layer of clothes.
Fourier dies of a
fall down stairs.
Grenoble, France  
193 YBN
[1807 AD]
3270)
England  
193 YBN
[1807 AD]
3385)
?, Switzerland  
192 YBN
[06/21/1808 AD]
2465) Following Humphry Davy's isolation of minute amounts of sodium and
potassium, Gay-Lussac and Thénard in 1808 prepare both sodium and potassium
metals in reasonable quantities.
During experiments with potassium as a reagent Gay-Lussac
blows up his laboratory, temporarily blinding himself.
Boron has symbol B; atomic
number 5; atomic mass: 10.81; m.p. about 2,300°C; sublimation point about
2,550°C; relative density 2.3 at 25°C; valence +3. Boron is a nonmetallic
element existing as a dark brown to black amorphous powder or as an extremely
hard, usually jet-black to silver-gray, brittle, lustrous, metal-like
crystalline solid.

In the naturally occurring compounds, boron exists as a mixture of two stable
isotopes with atomic weights of 10 and 11.
Paris, France (presumably)  
192 YBN
[06/??/1808 AD]
2393) Charles Darwin, among others admires this work.
Paris, France  
192 YBN
[1808 AD]
1224)
Vienna, Austria  
192 YBN
[1808 AD]
2308)
London, England (presumably)  
192 YBN
[1808 AD]
2371)
London, England  
192 YBN
[1808 AD]
2376)
Manchester, England  
192 YBN
[1808 AD]
2378) Bouvard is astronomer and director of the Paris observatory.
Paris, France (presumably)  
192 YBN
[1808 AD]
2382)
Paris, France  
192 YBN
[1808 AD]
2428) Malus' father was an official in the government before the French
Revolution.
Malus is in the street riot with Biot.
Malus serves as a military engineer in
Napoleon's expedition to Egypt and Syria.
In 1811, despite the war between England and
France, Malus is awarded the Rumford medal of the Royal Society of London.
Malus dies
at 37 of tuberculosis.
Paris, France  
192 YBN
[1808 AD]
2446)
Göttingen, Germany  
192 YBN
[1808 AD]
2478) Barium is a soft, silvery-white alkaline-earth metal, used to deoxidize
copper and in various alloys. Barium has atomic number 56; atomic weight
137.33; melting point 725°C; boiling point 1,140°C; relative density 3.50;
valence 2.
Barium is a chemically active, poisonous metal with a face-centered
cubic crystalline structure. Barium is an alkaline-earth metal in Group 2 of
the periodic table. Barium's principal ore is barite (barium sulfate); Barium
also occurs in the mineral witherite (barium carbonate). The pure metal barium
is obtained by the electrolysis of fused barium salts or, industrially, by the
reduction of barium oxide with aluminum.

Strontium is a soft, silver-yellow metal, easily oxidized, that ignites
spontaneously in air when finely divided. (Interesting that only when finely
divided) Strontium is used in pyrotechnic compounds and various alloys.
Strontium has atomic number 38; atomic weight 87.62; melting point 769°C;
boiling point 1,384°C; relative density 2.54; valence 2.
Strontium has three
allotropic crystalline forms (see allotropy). It is an alkaline-earth metal; in
its physical and chemical properties it resembles calcium and barium, the
elements above and below it in Group 2 of the periodic table. Since strontium
reacts vigorously with water and quickly tarnishes in air, it must be stored
out of contact with air and water. Strontium has many compounds.
(Strontium is one product
of uranium fission.)

Calcium is a silvery, moderately hard metallic element that constitutes
approximately 3 percent of the earth's crust and is a basic component of most
animals and plants. Calcium occurs naturally in limestone, gypsum, and
fluorite, and its compounds are used to make plaster, quicklime, Portland
cement, and metallurgic and electronic materials. Calcium has atomic number 20;
atomic weight 40.08; melting point 842 to 848°C; boiling point 1,487°C;
relative density 1.55; valence 2.
Calcium is crucial to all physiological
function. It must be obtained from the diet, but since an intake of only about
1 g per day is adequate, shortage is rare. The average human body contains just
over 1 kg of calcium, more than 99% of it in the skeleton (and teeth).
Calcium is a
malleable, ductile, silver-white, relatively soft metal with face-centered,
cubic crystalline structure. Chemically Calcium resembles strontium and barium;
calcium is classed with them as an alkaline-earth metal in Group 2 of the
periodic table. Calcium is chemically active; calcium tarnishes rapidly when
exposed to air and burns with a bright yellow-red flame when heated, mainly
forming the nitride. Calcium reacts directly with water, forming the hydroxide.
Calcium combines with many other elements forming many compounds.

Lime (calcium oxide) has been known since ancient times. Calcium metal is
usually prepared by electrolysis of fused calcium chloride to which a little
calcium fluoride has been added.


Magnesium is a light, silvery-white, moderately hard metallic element that in
ribbon or powder form burns with a brilliant white flame. It is used in
structural alloys, pyrotechnics, flash photography, and incendiary bombs.
Magnesium has atomic number 12; atomic weight 24.305; melting point 649°C;
boiling point 1,090°C; relative density 1.74 (at 20°C); valence 2.
Magnesium is
an essential mineral; present in all human tissues, especially bone. Magnesium
is involved in the metabolism of ATP. Magnesium is present in chlorophyll and
so in all green plant foods, and therefore generally plentiful in the diet. A
magnesium deficiency in human beings leads to disturbances of muscle and
nervous system; in cattle, to grass tetany. Magnesium-deficient plants are
yellow (or chlorosed).

Magnesium is a ductile, silver-white, chemically active metal with a hexagonal
close-packed crystalline structure. Magnesium is malleable when heated.
Magnesium is one of the alkaline-earth metals in Group 2 of the periodic table.
magnesium reacts very slowly with cold water. Magnesium is not affected by dry
air but tarnishes in moist air, forming a thin protective coating of basic
magnesium carbonate, MgCO3·Mg(OH)2. When heated, magnesium powder or ribbon
ignites and burns with an intense white light and releases large amounts of
heat, forming the oxide, magnesia, MgO. A magnesium fire cannot be extinguished
by water, since water reacts with hot magnesium and releases hydrogen.
Magnesium reacts with the halogens and with almost all acids. It is a powerful
reducing agent and is used to free other metals from their anhydrous halides.
Magnesium forms many compounds.
London, England  
192 YBN
[1808 AD]
2554) Alexander Wilson (CE 1766-1813) starts publishing "American Ornithology"
(9 vol, 1808-14), drawings of North American birds.

Philadelphia, Pennsylvania  
192 YBN
[1808 AD]
5978) Ludwig van Beethoven (CE 1770-1827), German composer, composes his 6th
Symphony "Pastoral" in F opus 68.

Vienna, Austria  
191 YBN
[11/16/1809 AD]
6341)
London, England  
191 YBN
[1809 AD]
2240)
Paris, France (presumably)  
191 YBN
[1809 AD]
2302) Appert uses the 12,000 francs to establish the first commercial cannery
business, the "House of Appert", at Massy, which operates from 1812 until 1933,
however Appert dies poor.
Paris, France (presumably)  
191 YBN
[1809 AD]
2367)
London, England  
191 YBN
[1809 AD]
2466) Joseph Louis Gay-Lussac (GAlYUSoK) (CE 1778-1850) finds that in forming
compounds gases combine in proportions by volume that can be expressed in small
whole numbers. For example, two parts of hydrogen unite with one part nitrogen
to form ammonia. This law is worked out with help from Humboldt. This
relationship by volume of elements in a compound is used to determine atomic
weights, which Berzelius goes on to do. Dalton refuses to accept Gay-Lussac's
results and stays firmly to the principle of composition be weight only and his
atomic weights continue to be wrong. Avogadro's hypothesis will provide an
explanation for Gay-Lussac's law but is ignored for 50 years.

Dalton rejects this law and seeks to discredit Gay-Lussac's experimental
methods.
Paris, France (presumably)  
191 YBN
[1809 AD]
2481)
London, England  
191 YBN
[1809 AD]
2529) Magendie performs experiments that prove wrong the prevailing view that
absorption takes place only through the lymphatic system, by introducing a
poison into an animal's system through either a blood vessel or quill, Magendie
demonstrates that absorption is instead achieved through the bloodstream and
the skin.
Magendie is viewed as the founder of experimental physiology.
Magendie's father is
among the French revolutionaries.
Magendie is strongly antivitalist.
Magendie gains an
unpleasant reputation as a vivisector, for his use of live animals in his
experiments. On a visit to England in 1824, for instance, his public
presentations of his experiments on the cranial nerves of living dogs caused a
public outcry and a demand for the protection of animals.

In 1837, Magendie is president of the Academy of Sciences.
Magendie wrongly believes
cholera to not be contagious.
Magendie wrongly objects to the use of ether as anesthetic.
Paris, France (presumably)  
191 YBN
[1809 AD]
2669) The Munich Academy of Science receives a paper from an inventor named
Samuel Thomas von Sömmering (CE 1755-1830) that describes a telegraph
containing thirty-five wires, one for each letter of the (German) alphabet and
one for each number. At the transmitting end, arrangements are provided for
passing currents through any one of the wires. At the receiving end the
electrodes are immersed in acidulated water. Completing the circuit causes
bubbles of hydrogen to form in tubes, each one corresponding to a letter or a
number.

Don Francisco Salva Campillo read a paper before the Academy of Sciences at
Barcelona, On February 22, 1804, in which he describes using the decomposition
of water with a voltaic pile for the purpose of telegraphy.

Munich, Germany  
190 YBN
[1810 AD]
2369)
London, England  
190 YBN
[1810 AD]
2370)
London, England  
190 YBN
[1810 AD]
2388)
Paris, France  
190 YBN
[1810 AD]
2412) Brown is disappointed by the low sales of this first volume selling only
24 of 250 printed copies and so does not complete a second volume of other
plant families from Australia.
London, England (presumably)  
190 YBN
[1810 AD]
2480)
London, England  
190 YBN
[1810 AD]
2482) Davy publishes the first part of the Elements of Chemical Philosophy,
which contains much of his own work, however Davy's plan is too ambitious and
he doesn't print subsequent volumes.
Swedish chemist J.J. Berzelius comments
that had this book been completed is would have "advanced the science of
chemistry a full century".
I am sure this book is helpful to those studying chemistry,
although probably many ideas are outdated, perhaps other advances kept secret
or mistaken later theories might be exposed in this book. But also probably a
good book to understand the historical context and foundation of modern
chemistry.

This is an interesting and simple idea that Davy mentions about a substance
gaining weight when gaining heat. For the theory that heat is due to the
absorption of photons by atoms, photon mass is very small, and difficult to
measure. For example, in increasing volume, does mercury also increase mass?
But perhaps in increasing mass, mercury then increases volume to maintain the
same density. It's interesting.
London, England  
190 YBN
[1810 AD]
5976)
Vienna, Austria (presumably)  
189 YBN
[06/??/1811 AD]
2396)
Paris, France  
189 YBN
[1811 AD]
658)
London, England (presumably)  
189 YBN
[1811 AD]
2334)
Bremen, Germany  
189 YBN
[1811 AD]
2432) The concept of molecules.

In this year Amedeo Avogadro (count of Quaregna) (oVOGoDrO) (CE 1776-1856),
Italian physicist, publishes his famous hypothesis in the Paris "Journal de
physique" under the title "Essai d'une manière de déterminer les masses
relatives des molecules élémentaires des corps, et les proportions selon
lesquelles elles entrent dans ces combinaisons." ("Essay on a Manner of
Determining the Relative Masses of the Elementary Molecules of Bodies, and the
Proportions in Which They Enter into These Compounds" Journal de Physique 73,
58-76 (1811) (Alembic Club Reprint No. 4]) in French. Northern Italy is
occupied by the French under Napoleon at the time. Avogadro hypothesizes that
equal volumes of all gases at the same temperature and pressure contain the
same number of molecules.

Avogadro is inspired from the finding of Gay-Lussac that all gases expand to
the same extent with a rise in temperature and Avogadro uses his hypothesis to
explain Gay-Lussac's law of combining volumes.

Avogadro beings by describing the discovery by the French chemist Joseph Louis
Gay-Lussac that when gases combine, they combine in simple integral proportions
by volume. Gay-Lussac shows that two volumes of ammonia (NH3) are composed of
one volume of nitrogen and three volumes of hydrogen, and cites many other
examples of similar cases of (gases combining in) simple, integral
proportions.

The basis of Avogadro's hypothesis is that all gases contain the same number of
particles (atoms, molecules, ions, or other particles) per unit volume.

Avogadro specifies that these particle may not necessarily be atoms but might
be combinations of atoms (which Avogadro calls "molecules"), and Avogadro is
the first to distinguish between atoms and molecules.

Avogadro does not actually use the word "atom" and considered that there are
three kinds of "molecules," including an "elementary molecule" (the modern
"atom").
To distinguish between atoms and molecules, Avogadro uses the terms "molécule
intégrante" (the molecule of a compound (such as H2O)), "molécule
constituante" (the molecule of an element (such as H2)), and "molécule
élémentaire" (atom (such as C)). Avogadro views gaseous elementary molecules
as predominantly diatomic, but also recognizes the existence of monatomic,
triatomic, and tetratomic elementary molecules. (What atoms are
tetratomic?)(How does Avogadro reach the conclusion about diatomic molecules?
What physical observations cause Avogadro to conclude that atoms of gas are
diatomic?)

Avogadro concludes that the number of "integrant molecules" in all gases is
always the same for equal volumes.
Avogadro writes that it is very well conceivable that
the distance between molecules does not vary, in other words, that the number
of molecules contained in a given volume cannot being different.
Avogadro writes
(translated into English): "Setting out from this hypothesis, it is apparent
that we have the means of determining very easily the relative masses of the
molecules of substances obtainable in the gaseous state, and the relative
number of these molecules in compounds; for the ratios of the masses of the
molecules are then the same as those of the densities of the different gases at
equal temperature and pressure, and the relative number of molecules in a
compound is given at once by the ratio of the volumes of the gases that form
it. For example, since the numbers 1.10359 and 0.07321 express the densities of
the two gases oxygen and hydrogen compared to that of atmospheric air as unity,
and the ratio of the two numbers consequently represents the ratio between the
masses of equal volumes of these two gases, it will also represent on our
hypothesis the ratio of the masses of their molecules. Thus the mass of the
molecule of oxygen will be about 15 times that of the molecule of hydrogen, or,
more exactly as 15.074 to 1. In the same way the mass of the molecule of
nitrogen will be to that of hydrogen as 0.96913 to 0.07321, that is, as 13, or
more exactly 13.238, to 1. On the other hand, since we know that the ratio of
the volumes of hydrogen and oxygen in the formation of water is 2 to 1, it
follows that water results from the union of each molecule of oxygen with two
molecules of hydrogen. Similarly, according to the proportions by volume
established by M. Gay-Lussac for the elements of ammonia, nitrous oxide,
nitrous gas, and nitric acid, ammonia will result from the union of one
molecule of nitrogen with three of hydrogen, nitrous oxide from one molecule of
oxygen with two of nitrogen, nitrous gas from one molecule of nitrogen with one
of oxygen, and nitric acid from one of nitrogen with two of oxygen."

Avogadro's hypothesis allows for the calculation of the molecular weights of
gases relative to some chosen standard. Avogadro and his contemporaries
typically use the density of hydrogen gas as the standard for comparison.
Therefore they use the relationship:

Weight of 1 volume of gas or vapor Weight of 1 molecule of gas or vapor
--------
--------------------------- = ------------------------------------
Weight of 1 volume of hydrogen
Weight of 1 molecule of hydrogen

Using this hypothesis, Avogadro determines the correct molecular formula for
water, nitric and nitrous oxides, ammonia, carbon monoxide, and hydrogen
chloride.

When Ritter (and Cavendish before Ritter) electrolyzed water and the hydrogen
and oxygen collected separately, the volume of hydrogen is always twice the
volume of oxygen. Avogadro then uses his hypothesis to explain that the water
molecule contains two hydrogen atoms for each atom of oxygen. Then if oxygen
weighs eight times as much as hydrogen, the individual oxygen atom is sixteen
times as heavy as the individual hydrogen atom (not eight times as Dalton has
suggested).

Later physicists and chemists determined the value of "Avogadro's Number," the
number of gas molecules in one mole (the atomic or molecular weight in grams),
as 6.022 x 1023.
The number of atoms or molecules present in an amount of
substance that has a mass of its atomic (or molecular) weight in grams is
called "Avogadro's number". For example, carbon dioxide has a molecular weight
of 44, therefore 44 grams of carbon dioxide contains Avogadro's number of
molecules, which is 6.0221367×1023 (the number of bodies usually atoms or
molecules per mole) (molecules or atoms/mole).
(Some people might think 44 grams of anything
should contain the same number of atoms as 44 grams of anything else. But
because atomic masses {weights} are different, an atom of hydrogen contains
only 1 proton, where an atom of iron contains 44 protons. So 44 grams of
anything should equal the same number of photons, and the same number of
nucleons {protons and neutrons} but not the same number of atoms since each
atom represents a different mass in other word each atom contains a different
number of protons. The concept of an "atom" is simply a way of containing
protons into groups.) Where Hydrogen has a molecular weight of approximately of
1 g/mol and so only 1 gram of Hydrogen = Avogadro's number in atoms. (But the
same number of photons {and protons} are in 1 gram of Hydrogen as there are in
1 gram of Iron, or any other substance {it is he number of atoms that is
different}.)

Avogadro's hypothesis is ignored for the most part until after his death, for
one reason because the distinction between atoms and molecules is not well
understood. In addition, the concept of polyatomic elementary molecules appears
unlikely to contemporaries because similar atoms are thought to repel each
another.

Avogadro's hypothesis implies a sequence of chemical reactions for which there
is no decisive evidence in favor of at the time. For example, Dalton postulated
that water is formed by the simple addition of the element hydrogen to the
element oxygen, in other words H + O → HO, where Avogadro's hypothesis
describes this reaction as 2H2+ O2 (in the molecular form) → 2H2O.

Ampère accepts this theory, but Dalton rejects it and Berzelius ignores it.
Stanislao Cannizzaro will build on this theory and reduce the confusion between
atoms and molecules in 1858. (What are Dalton's reasons for rejecting
Avogadro's theory?)

Avogadro's hypothesis is now accepted as true, and the value known as
"Avogadro's number" (6.0221367 x 1023), the number of molecules in a gram
molecule, or mole, of any substance, is a fundamental constant of science.
Perhaps the first accurate calculation of the quantity of molecules in a
gram-mole is made by Johann Josef Loschmidt in 1865 who computes the number of
particles in one cubic centimeter of gas in standard conditions. (Did Avogadro
estimate a number for number of particles per mole?)


(The question still remains as to whether atomic size effects volume. I think
we should experiment with very large molecules in gas and large quantities to
see if there can be measured any difference in volume between a gas with small
particles and a gas with large particles. It would seem logical that molecules
with more mass would provide more surface area for collisions and therefore
more pressure. I think the concept of pressure is important in Avogadro's
hypothesis. For example, do gases of different mass but same volume exert
different pressure? I tend to believe that molecule size has little or no
effect in the volume of a gas, but then volume of a gas is measured based on
the container since gas can take the size and shape of any container.)

One important idea to understand clearly is that: the same volume of different
gases have different masses. Two different gases may occupy the same space, in
for example water, but those quantities of gas weigh differently. (Who first
showed this? Priestley? Lavoisier? Cavendish? Dalton?) (In addition the
question of, does the same volume of two different mass gases exert different
pressure? If yes, that might affect the volume of the gas.)

(In terms of the claim that all gases contain the same number of particles per
unit volume: Apparently this claim is extended to liquids and solid. Does this
same principle apply to liquids and solids? Do all liquids and solids contain
the same number of atoms or molecules per unit volume? If no, then this
hypothesis may not be true for gases. Maybe particles are too small to measure
any difference. This conclusion would be more logical if the particles are all
the same size.) (As always, with a new paradigm, I think it is very important
to thoroughly research, understand, and explain every aspect of the finding,
hypothesis, experimental data, etc. because such transitions are very important
in defining our understanding of the universe.)

(Is Avogadro the first to use the word "molecule"?) (Avogadro certainly coins
the word "molecule")(State origin of word molecule. It is interesting the way
that matter is clumped together with atoms and molecules, what groupings are
larger than molecule? I guess: common multi-molecules, radicals, perhaps then
there is just lattices, tissues, etc.)

(It's hard to believe that molecule size and mass doesn't matter to volume or
pressure of a gas, liquid or solid, because more mass must occupy more space.
Maybe an affect is only observed for very compressed matter where space is
important and mostly occupied with matter.)
Vercelli, Italy  
189 YBN
[1811 AD]
2441) Courtois is apprenticed to a pharmacist and subsequently studies at the
Ecole Polytechnique under Antoine Fourcroy.
Courtois' father's saltpeter business runs
into difficulties because saltpeter can be manufactured more cheaply in India,
and Courtois returns to Dijon to help his father.
When the Napoleonic Wars end, and the
need for gunpowder decreases, (the) Coutois' salt-peter factory fails. Courtois
turns to producing iodine but dies in poverty. (This shows how sadly, provoking
and conjuring war is one evil way explosives and weapons producing companies
can use to stay in business, although perhaps that is too criminal for most
weapons manufacturing companies to involve themselves in, in addition to simply
being against war even at the expense of going into poverty or some other
business.)

symbol I, atomic number 53, relative atomic mass 126.9045,

Iodine is a nonmetallic element, with symbol I; atomic number 53; atomic mass.
126.9045; m.p. 113.5°C; b.p. 184.35°C; sp. gr. 4.93 at 20°C; valence
−1, +1, +3, +5, or +7. Iodine is a dark-gray to purple-black, lustrous,
solid, volatile element with a rhombic crystalline structure. iodine is the
heaviest of the naturally occuring halogens and least active of the halogens,
which are found in Group 17 of the periodic table. Iodine is normally diatomic
(2 iodine atoms in each molecule), in the solid, liquid (is there a liquid
state?), and vapor (gas) states. When heated it passes directly from the solid
to the vapor state (sublimation), the vapor having an intense violet color and
a characteristic irritating odor.

Iodine occurs widely, although rarely in high concentration and never in
elemental form. Despite the low concentration of iodine in sea water, certain
species of seaweed can extract and accumulate the element.
Iodine is an essential
ingredient of thyroid hormone, which helps to regulate growth, development, and
metabolic rate. The Reference Nutrient Intake for adults is 140 micrograms each
day. An excess of iodine can be poisonous; a deficit leads to an underactive
thyroid gland. Goiter, a swelling of the thyroid, is often a symptom of
inadequate iodine in the diet.

When heat is applied, iodine crystals sublime (change straight from a solid to
a gas). Any gas that settles on a cold surface will crystallize as the solid,
because iodine cannot exist as a liquid.
Dijon, France  
189 YBN
[1811 AD]
2467)
Paris, France (presumably)  
189 YBN
[1811 AD]
2510) Over the course of his life, Braconnot publishes 112 works.
Nancy, France  
189 YBN
[1811 AD]
2519) In 1808 Poisson publishes "Sur les inégalités des moyens mouvements des
planètes" in which Poisson looks at the mathematical problems which Laplace
and Lagrange had raised about perturbations of the planets.

Poisson's other publications include "Théorie nouvelle de l'action capillaire"
(1831, "A New Theory of Capillary Action") and "Théorie mathématique de la
chaleur" (1835, "Mathematical Theory of Heat").
In 1798 Poisson begins studying
mathematics at the École Polytechnique in Paris under the mathematicians
Pierre-Simon Laplace and Joseph-Louis Lagrange, who become Poisson's lifelong
friends.
In 1802 Poisson becomes a professor at the École Polytechnique.
In 1808 Poisson is
made an astronomer at the Bureau of Longitudes.
In 1809 Poisson is appointed a professor of
pure mathematics at the Faculty of Sciences at the University of Paris when it
is founded.

Poisson writes more than 300 papers on mathematics, physics, and astronomy.
Paris, France  
189 YBN
[1811 AD]
2522) Brewster starts studying for the ministry at Edinburgh University but
after completing the course abandons the Church for science.
Brewster earns his living
by editing various journals and spends much time popularizing science.
In 1807 Brewster
is editor of the newly projected Edinburgh Encyclopaedia, of which the first
part appears in 1808, and the last not until 1830. The work is strongest in the
scientific department, and many of its most valuable articles are from Brewster
himself. At a later period Brewster is one of the leading contributors to the
Encyclopaedia Britannica (seventh and eighth editions), the articles on
Electricity, Hydrodynamics, Magnetism, Microscope, Optics, Stereoscope, Voltaic
Electricity, and others being from Brewster.
Around 1815 Brewster rediscovers the
kaleidoscope, a scientific toy.
Brewster wins the Copley medal.
In 1816 the French
Institute awards Brewster one-half of the prize of three thousand francs for
the two most important discoveries in physical science made in Europe during
the two preceding years.
In 1818 Brewster receives the Rumford Medal for Brewster's
Law.
In 1824 Brewster starts the Edinburgh Journal of Science.
In 1831 Brewster helps found
the British Association for the Advancement of Science.
In 1831, Brewster writes "A
Treatise on Optics" (1831).
In 1855, Brewster writes "Memoirs of the Life, Writings,
and Discoveries of Sir Isaac Newton".
In 1859 Brewster becomes principal of the
University of Edinburgh.

Brewster publishes almost 300 papers, mainly concerning optical measurements.

Brewster never fully accepts the wave theory of light, and so finds his
experimental work marginalized.
Brewster has a daughter after age 75.
Edinburgh, Scotland  
189 YBN
[1811 AD]
2536)
London, England  
189 YBN
[1811 AD]
2548) Other papers by Dulong are concerned with "New determinations of the
proportions of water and the density of certain elastic fluids" (1820, with
Berzelius); the property possessed by certain metals of facilitating the
combination of gases (1823 with Thenard); the refracting powers of gases
(1826); and the specific heats of gases (1829). In 1830 Dulong publishes a
research, undertaken with Arago for the academy of sciences, on the elastic
force of steam at high temperatures. For the purposes of this determination
Dulong creates a continuous column of mercury, constructed with 13 sections of
glass tube each 2 meters long and 5 mm in diameter, in the tower of the old
church of St Genevieve in the College Henri IV. The apparatus is first used to
investigate the variation in the volume of air with pressure, and the
conclusion is that up to twenty-seven atmospheres, the highest pressure
attained in the experiments, Boyle's law is true (that the pressure and volume
of a gas are inversely related).
Dulong begins as a doctor in one of the poorest
districts of Paris, where Dulong hands out medicine without charge and treats
the poor for free, but soon abandons (health for chemical) research.
After acting as
assistant to Berthollet, Dulong becomes professor of chemistry at the faculty
of sciences and the normal and veterinary schools at Alfort.
In 1820 Dulong is
professor of physics at the Ecole Polytechnique, and appointed director in
1830.
Paris, France (presumably)  
189 YBN
[1811 AD]
2558) Arago is educated at the Ecole Polytechnique in Paris.
In 1809 Arago is elected
to the Académie des Sciences and receives the chair of analytical geometry at
the Ecole Polytechnique.
In 1830 Arago succeeds J. B. J. Fourier as the permanent
secretary of the Ecole Polytechnique.
Arago is a vigorous defender of A. J. Fresnel's wave
theory of light against the criticisms of Laplace and Biot, who both supported
the corpuscular theory.
Because Arago is converted to the wave theory of light and
Arago loses Biot's friendship. (Rejecting the idea of light as a particle in
favor of light as a wave in a medium is not intuitive, but after Young had
shown how color is explained by frequency, perhaps the wave theory appeared to
be more modern since the corpuscular group fails to offer a competing
explanation for color such as that color is determined by frequency of
corpuscle.)(A difference in scientific opinion is no reason to break a
friendship.)
In 1838 Arago describes an experiment to determine the speed of light in air
with the speed of light in a denser medium. Shortly before Arago's death, Léon
Foucault and Armand Fizeau will prove that the speed of light is slower in a
denser medium, (and since Newton had theorized that as a corpuscle, light would
move faster through water), many people think this fact supports a wave
interpretation for light. (Surprisingly, the idea that accepting that Newton
was wrong, and that particles of light might be delayed because of collisions
in a denser medium is either not argued or in any event, does not win
popularity if argued.)
Arago is the first French person to receive Royal Society's
Copley medal.
Arago participates in revolutions on the side of the Republicans in 1830
and 1848.
In the Second Republic (1848-1852) Arago serves in the cabinet and is
instrumental in having slavery abolished in the French colonies.
In 1852 Arago resigns
his post when President Napoleon makes himself Emperor Napoleon II and demands
an oath of allegiance. But Napoleon refuses to accept Arago's resignation, and
does not insist on an oath.

(I wonder if this is from some frequencies of light reflecting off the last
atom in one direction and others in the opposite direction, since with the
light-as-a-particle theory it seems possible that particles would bounce off in
at least two directions if colliding inside a refractive object. In this
theory, double refraction is the result of some photons reflecting off atoms
like a pachinko game, exiting at two different angles depending on the last
reflection.)
Paris, France (presumably)  
189 YBN
[1811 AD]
2564) Chevreul writes books on the history and philosophy of science in 1860,
1866, and 1878.
Chevreul attends the Collège de France (1803).
In 1809 Chevreul is an
assistant to Antoine François de Fourcroy.
In 1810 Chevreul is assistant at the Musée
d'Histoire Naturelle.
From 1813 to 1830 Chevreul is professor of physics at the Lycée
Charlemagne.
In 1824 Chevreul becomes director of the dyeworks for the Gobelins Tapestry,
where Chevreul discovers hematoxylin in logwood, quercetin in yellow oak, and
prepares the reduced colorless form of indigo. Chevreul also investigates the
science and art of color with special application to the production of massed
color by aggregations of small monochromatic dots, as in the threads of a
tapestry.
In 1830, Chevreul succeeds Vauquelin as professor of chemistry at the (French
Academy of Sciences) Museum (in Paris).

Chevreul lives to 103 years old. Both his father and mother live to be over 90.
(Perhaps living to old age is inherited. It would be naturally selected for
since the longer a person lives the more chance of reproduction.)
Paris, France (presumably)  
188 YBN
[03/09/1812 AD]
2520)
Paris, France  
188 YBN
[1812 AD]
1241) Benjamin Rush (December 24, 1745 - April 19, 1813) publishes "Medical
Inquires and Observations Upon the Diseases of the Mind", the first psychology
book to be printed in the USA.

Pennsylvania, PA  
188 YBN
[1812 AD]
1242) Joseph Mason Cox (1763-1818) in his "Practical Observations on Insanity",
promotes the use of his invention the "swinging chair" as a treatment for
insanity. Humans are rotated until obedient. These devices will be banned by
people in a number of European governments.

Pennsylvania, PA  
188 YBN
[1812 AD]
2316)
London, England  
188 YBN
[1812 AD]
2347) Glucose (also called Dextrose), is one of a group of carbohydrates known
as simple sugars (monosaccharides). Glucose (from Greek glykys; "sweet") has
the molecular formula C6H12O6. Glucose is found in fruits and honey and is the
major free sugar circulating in the blood of higher animals. Glucose is the
source of energy in cell function, and the regulation of glucose in a body is
very important. Molecules of starch, the major carbohydrate of plants, are made
of thousands of glucose units, as are molecules of cellulose. Glycogen, the
reserve carbohydrate in (most) cells is also made of glucose.
St Petersburg?, Russia?  
188 YBN
[1812 AD]
2389)
Paris, France  
188 YBN
[1812 AD]
2402) Mohs studies at Halle and at the Freiberg Mining Academy under Abraham
Werner.
In 1812 Mohs becames curator of the mineral collection at the Johanneum in
Graz.
(It seems logical to me that there is a relationship between molecular and or
atomic density and hardness. This relates back to Leukippos and Demokritos
naming the atom as some object that is too dense to be cut; some densest
uncuttable object.)
Graz, (Austria now:) Germany  
188 YBN
[1812 AD]
2518)
Yorkshire, England  
188 YBN
[1812 AD]
5979)
Vienna, Austria  
187 YBN
[1813 AD]
2453)
Paris, France (presumably)  
187 YBN
[1813 AD]
2458) In 1796 Candolle arrives in Paris and becomes friends with the French
naturalists Georges Cuvier and Jean-Baptiste de Lamarck.
In 1802 Candolle becomes an
assistant to Cuvier at the Collège de France.
Candolle prepares revisions of Lamarck's
"Flore française" (1805, 1815).
From 1806-1812, at the request of the French
government Candolle makes a botanical and agricultural survey of France.
Candoll
e also writes monographs (scholarly essays) of 100 plant families.
In 1808 Candolle
becomes professor of botany at the University of Montpellier.
From 1817-41 Candolle is the
chair of natural history at the Université de Genève (1817-41), where
Candolle is the first director of the botanical gardens.
Montpellier, France (presumably)  
187 YBN
[1813 AD]
2459) Augustin Pyrame de Candolle (KonDOL) (CE 1778-1841), publishes "Regni
Vegetabilis Systema Naturale" (2 vol, 1818-21, "Natural Classification for the
Plant Kingdom") which develops Candolle's system of classification.

Montpellier, France (presumably)  
187 YBN
[1813 AD]
2460)
Montpellier, France (presumably)  
187 YBN
[1813 AD]
2475)
London, England  
187 YBN
[1813 AD]
2492)
Stokholm, Sweden (presumably)  
187 YBN
[1813 AD]
2503)
Stokholm, Sweden (presumably)  
187 YBN
[1813 AD]
2531) François Magendie (mojoNDE) (CE 1783-1855), demonstrates the largely
passive role of the stomach in vomiting in addition to describing the the
mechanism of swallowing.

Paris, France (presumably)  
187 YBN
[1813 AD]
2596)
Edinburgh, Scotland  
187 YBN
[1813 AD]
2739) Charles Babbage (CE 1792-1871), English mathematician, first has the
idea of mechanically calculating mathematical tables.

From 1820-1822, Babbage makes a small calculator that can perform certain
mathematical computations to six or eight decimals.
Charles Babbage is the son of
Benjamin Babbage, a wealthy banking partner of the Praeds who owns the Bitton
Estate in Teignmouth and Betsy Plumleigh Babbage.
Babbage receives instruction from
several elite schools and teachers during the course of his elementary
education.
In 1814, Babbage graduates from St Peter's College, Cambridge.
In 1812 Babbage helps found
the Analytical Society, along with Sir John Herschel, George Peacock (and
Whewell ) who labor to raise the standard of mathematical instruction in
England, and especially endeavor to supersede the Newtonian by the Leibnizian
notation in the infinitesimal calculus.
In 1814, the same year he takes his degree,
Babbage marries Georgiana Whitmore. They have eight children, only three of
whom survive to maturity.
From 1828 to 1839 Babbage serves as Lucasian Professor of
Mathematics at the University of Cambridge.
In 1830 Babbage writes a controversial book
which denounces the Royal Society as having grown moribund.
(Notice how Babbage
works with people in the Government as Morse did, which may imply development
of secret technology for government military.)
Cambridge, England (presumably)  
187 YBN
[1813 AD]
2818)
Paris, France (presumably)  
187 YBN
[1813 AD]
2846)
Göttingen, Germany (presumably)  
187 YBN
[1813 AD]
3235) Howard turns down an offer of 40,000 pounds and instead licenses his
process.
London, England  
187 YBN
[1813 AD]
3323)
London, England (presumably)  
186 YBN
[03/27/1814 AD]
2485)
Florence, Italy  
186 YBN
[1814 AD]
2262)
Palermo, Sicily  
186 YBN
[1814 AD]
2409) Thomas Young (CE 1773-1829) begins studying the Rosetta stone. After
obtaining additional hieroglyphic writings from other sources, Young succeeds
in providing a nearly accurate translation within a few years and this
contributes heavily to deciphering the ancient Egyptian language. Young will
write an an authoritative article on Egypt in 1818, laying the ground work for
Champollion.

London, England  
186 YBN
[1814 AD]
2433)
Vercelli, Italy  
186 YBN
[1814 AD]
2571) Joseph von Fraunhofer (FroUNHoFR or HOFR) (CE 1787-1826), German
physicist and optician, invents a spectroscope (using a theodolite) by using a
telescope as opposed to paper and maps 576 spectral lines. Theodolites were
designed and used exclusively for surveying before this.

In testing glasses to measure the index of refraction (to make achromatic
lenses), Fraunhofer finds that the solar spectrum contains numerous dark lines.
Fraunhofer finds that even slight imperfections in the prism would have reduced
the sharpness of the image enough to blur out the lines (and perhaps this
explains why Newton may have missed seeing these lines (I have never seen these
lines with the tiny prisms I own). Wollaston had observed only seven lines, 12
years earlier (1802), but Fraunhofer observes nearly six hundred. People now
have identified about ten thousand lines (including beyond the narrow visible
region of light). Fraunhofer maps these lines (using the letter A to K to
describe the main lines, (a system still used today) and determines their
wavelength. (How does Fraunhofer determine wavelength?)

Fraunhofer puts a prism at the focal point of a telescope and finds that light
from a star has dark lines in the spectrum that do not match the pattern of
those in sunlight. (Kirchhoff will develop the understanding of these spectrum
lines further.)

Fraunhofer plots hundreds of spectral lines, and by measuring their wavelengths
(or photon intervals - however there is no calculation of wavelength but only
position on spectrum) Fraunhofer finds that the relative positions of the lines
in the spectra of elements are constant, whether the spectra are produced by
the direct rays of the Sun, by the reflected light of the Moon and planets, by
a gas (flame), or by (the light of) a heated metal in the laboratory.

Fraunhofer's first assignment at the Untzschneider Optical Institute is making
achromatic lenses for telescopes. This work requires the production of highly
homogeneous silicates. Fraunhofer's communication on the results of his
research appears in the Denkschriften (Memoirs) for 1814-1815 of the Academy of
Sciences in Munich. The paper contains a description of the first use of the
dark lines of the solar spectrum as reference points for the measurement of
refraction indexes.

These lines are (sometimes referred to as) Fraunhofer lines. (may only be dark
lines in Sun according to EB verify)

This work sets the stage for the development of spectroscopy.

50 years later Gustav Kirchhoff will determine the elementary composition of
the stars by showing that lines in the solar spectrum result from
characteristic absorption by elements in the atmosphere of the Sun.(Kirchhoff
will show that these lines are from absorption as opposed to simply absence of
light in the frequency. It seems logical that there must be some very tiny
frequencies as a person divides time into smaller units, which would not
contain photons emitted by the Sun.)

(Understanding the concept that light moves in beams of many different
frequencies is important to isolating specific wavelengths of light as Michael
Pupin will do in 1910 in seeing thought; the first image of a human memory.)

Fraunhofer publishes these findings in the journal "Denkschriften der
Königlichen Akademie der Wissenschaften zu München", (1814), 15 Band v, pp
193-226. This work is translated from German into English as "On the Refractive
and Dispersive Power of different Species of Glass in reference to the
improvement of Achromatic Telescopes with an Account of the Lines or Streaks
which cross the Spectrum By JOSEPH FRAUENHOFER" in two parts in the "Edinburgh
Philosophical Journal", (1823) vol IX, pp296 and in "Edinburgh Philosophical
Journal", (1824), vol X, p26.

(It is interesting that the atoms in the prisms or gratings apparently do not
influence the spectra of the source. Perhaps for the prism the photons are not
absorbed but transmitted or more likely reflected through with many collisions,
and for the grating they are not absorbed but reflected.)
Fraunhofer writes
that "In every case, the white light which passed through (the refracting
medium) was still decomposed into all its colours, with this difference only,
that in the spectrum, the colour peculiar to the glass or the fluid was more
brilliant than the rest. Even the coloured flames obtained by burning alcohol,
sulphur, &c, seen through a prism, do not yield a homogeneous light
corresponding to the colour. These flames, however, such as that of a lamp,
particularly that of a candle, and in general, the light produced by the flame
of a fire, exhibit between the red and yellow of the spectrum a clear and well
marked line, which occupies the same place in all the spectra. This line will
become more important in the sequel, and it was one of great utility to me. It
appears to be formed by rays which are not decomposed by the prism, and which
consequently are homogeneous. In the green space we perceive a similar line,
but it is weaker, and less distinct, so that it is often very difficult to
find.".
Fraunhofer finds a double yellow line in the light of a flame (which kind?)
that corresponds exactly to the spectrum of the Sun (later shown to be from
sodium).

Fraunhofer writes "As the lines of the spectrum are seen with every refracting
substance of uniform density, I have employed this circumstance for determining
the index of refraction of any substance for each coloured ray. This could be
done with the greater exactness, as most of the lines are very distinct and
well marked. For this purpose, I selected the largest lines, because with
substances of low refractive power, or with prisms of small refracting angles,
the lines of less magnitude could scarcely be perceived with a strong
magnifying power. The lines which I chose were those marked B, C, D, E, F, G,
H, in Fig. 5 of Plate VII. (Vol. IX.) I made no use of the line b, because it
is too near F, and I endeavoured to use the middle one between D and F.".


So in this way Fraunhofer creates a detailed map of the newly discovered lines
in the spectrum of the Sun. Fraunhofer goes on to explain that the lines
disappear if the aperture (opening) is too large. If the angle of the width of
the aperture is greater than that of the width of the line then the image of
the same line will be projected several times parallel to itself will become
indistinct and disappear when the aperture is too large. Fraunhofer thinks that
the lines may be the result of an illusion caused by "inflection" (diffraction)
by the narrow opening of the slit, and performs an experiment to verify that
(diffraction or) interference is not the cause of the spectral lines.
Fraunhaofer states "Various experiments and changes to which I have submitted
these lines convince me that they have their origin in the nature of the light
of the sun, and that they cannot be attributed to illusion, to aberration, or
any other secondary cause.".

Fraunhofer examines the spectra of planet Venus writing: "In the spectrum
formed by this light I found the same lines such as they appeared in the light
of the sun. That of Venus however, having little intensity compared with that
of the sun reflected from a mirror, the brightness of the violet and the
exterior red rays is very feeble. On this account we perceive even the
strongest lines in these two colours with some difficulty, but in the other
colours they are easily distinguished. I have seen the lines D E b F (Fig 6)
very well terminated and I have recognised that those in b are formed of two,
namely a fine and a strong line. The weakness of the light however prevented me
from seeing that the strongest of these two lines consisted of two and for the
same reason the other finer lines could not be distinguished. By an approximate
measure of the lines DE and EF I am convinced that the light of Venus is in
this respect of the same nature as that of the sun."

Fraunhofer observes the spectra of other stars writing "With the same apparatus
I have also made several observations on some of the brightest fixed stars. As
their light was much fainter than that of Venus, the brightness of their
spectra was consequently still less. I have nevertheless seen without any
illusion in the spectrum of the light of Sirius three large lines which
apparently have no resemblance with those of the sun's light. One of them is in
the green, and two in the blue space. Lines are also seen in the spectrum of
other fixed stars of the first magnitude."
Fraunhofer examines the spectra of
electric light and the light from burning hydrogen, alcohol and sulfur.
Fraunhofer writes "The electric light is, in relation to the lines of the
spectrum, very different from the light of the sun and of a lamp (must be
alcohol lamp). In this spectrum, we meet with several lines, party very clear,
and one of which, in the green space, seems very brilliant, compared with the
other parts of the spectrum. Another line, which is not quite so bright, is in
the orange, and appears to be of the same colour as that in the spectrum of the
light of a lamp; but, in measuring its angle of refraction, I find that its
light is much more strongly refracted, and nearly as much as the yellow rays of
the light of a lamp.". Fraunhofer describes the spectral lines of flames of
various substances writing: "Whether the aperture through which the light of
the lamp passes is wide or narrow, if we cover the point of the flame, and the
lower blue extremity of it, the red line appears less clear, and is more
difficult to be distinguished. hence it appears that this line derives its
origin principally from the light of the two extremities of the flame,
particularly the inferior one.
The reddish line is, in relation to the other parts
of the spectrum, very bright in the spectra of light produced by the flame of
hydrogen gas and alcohol. In the spectrum of the flame of sulphur, it is seen
with difficulty."


Fraunhofer examines the spectra of light produced by electricity writing "In
order to obtain a continuous electrical light I brought to within half an inch
of each other two conductors and I united them by a very fine glass thread. One
of the two was connected with an electrical machine and the other communicated
with the ground. In this manner the light appeared to pass continuously along
the glass fibre which consequently formed a fine and brilliant line of light."
"The
electric light is in relation to the lines of the spectrum very different from
the light of the sun and of a lamp. In this spectrum we meet with several lines
partly very clear and one of which in the green space seems very brilliant
compared with the other parts of the spectrum. Another line which is not quite
so bright is in the orange and appears to be of the same colour as that in the
spectrum of the light of a lamp, but in measuring its angle of refraction, I
find that its light is much more strongly refracted, and nearly as much as the
yellow rays of the light of a lamp. Towards the extremity of the spectrum we
perceive in the red a line of very little brightness, yet its light has the
same refrangibility as that of the clear line of the light of a lamp. In the
rest of the spectrum we may still easily distinguish other four lines
sufficiently bright."

Fraunhofer publishes this as (translated from German) "DETERMINATION OF THE
REFRACTIVE AND THE DISPERSIVE POWER OF DIFFERENT KINDS OF GLASS WITH REFERENCE
TO THE PERFECTING OF ACHROMATIC TELESCOPES."
Benedictbeuern (near Munich), Germany  
186 YBN
[1814 AD]
2609) In 1805 Cauchy finds a simple solution to the problem of Apollonius; to
describe a circle touching three given circles.
In 1811 Cauchy discovers his
generalization of Euler's theorem on polyhedra.

According to the Encyclopedia Britannica Cauchy's greatest contributions to
mathematics, characterized by the clear and rigorous methods that he
introduces, are embodied predominantly in his three great treatises: "Cours
d'analyse de l'École Royale Polytechnique" (1821, "Courses on Analysis from
the École Royale Polytechnique"); "Résumé des leçons sur le calcul
infinitésimal" (1823, "Résumé of Lessons on Infinitesimal Calculus"); and
"Leçons sur les applications du calcul infinitésimal à la géométrie"
(1826-28, "Lessons on the Applications of Infinitesimal Calculus to Geometry").
(This needs more info about specific contributions)

In optics, Cauchy develops the wave theory, and Cauchy's name is associated
with the simple dispersion formula. (show) In elasticity, Cauchy originates the
theory of stress, and Cauchy's results are nearly as valuable as those of S. D.
Poisson.
Augustin Louis Cauchy was born in Paris in 1789, 38 days after the fall of the
Bastille. Cauchy's father, Louis François, was a parliamentary lawyer,
lieutenant of police, and ardent royalist. Sensing the political wind, Cauchy's
father moves the family to his country cottage at Arcueil, where they lived for
nearly 11 years. Here young Cauchy receives a strict religious education from
his mother and an elementary classical education from his father, who writes
his own textbooks in (poetic?) verse.
By 1800 the political situation is
stabilized and the family moved back to Paris.
In 1816, when Gaspard Monge is expelled
from the Academy of Sciences (because of Monge's close friendship with
Napoleon), Cauchy is appointed to fill the vacancy. The same year Cauchy wins
the grand prix of the Institute of France for a paper on wave propagation, now
accepted as a classic in hydrodynamics.

The Revolution of 1830 sends Charles X into exile and Cauchy refuses to give an
oath of allegiance to the new king, Louis Philippe, is stripped of all his
positions, and moves to Switzerland, leaving his family in Paris until they
join him in Prague in 1834.
After the Revolution of 1848, the oath is abolished, and
Cauchy resumes his old professorship at the Polytechnique. Louis Napoleon
reinstates the oath in 1852, but Cauchy is specifically exempted.

Among Cauchy's nearly 800 publications are works on the theory of waves (1815),
algebraic analysis (1821), elasticity (1822), infinitesimal calculus (1823,
1826-28), differential calculus (1827), and the dispersion of light (1836).

Cauchy's collected works, "Oeuvres complètes d'Augustin Cauchy" (1882-1970),
are published in 27 volumes.

According to Asimov Cauchy is aggressively ultraconservative both in politics
and religion.
Answers biography writes that Cauchy, is as rigidly ultraroyalist in
politics as Cauchy is ultra-Catholic in religion.
Paris, France  
185 YBN
[01/03/1815 AD]
3837)
Edinburgh, Scotland  
185 YBN
[07/08/1815 AD]
2597)
Paris, France  
185 YBN
[10/??/1815 AD]
2589) Fresnel starts studying optics in 1814 and is one of the major supporters
of the wave theory of light. Fresnel works on interference, at first being
unaware of the work of Thomas Young, and produces a number of devices for
giving interference effects. Fresnel's biprism is a single prism formed of two
identical narrow-angled prisms base-to-base. Placed in front of a single source
Fresnel's biprism splits the beam into two parts, which can produce
interference fringes. (This claim of interference I would like to verify on
video for all.)

Initially, Fresnel believes that light is a longitudinal wave motion (like
sound), but later decides that light must be a transverse wave to account for
the phenomenon of polarization.

I think that because the frequency of light determines color, and that this
find came from those who viewed light as a wave (starting with Nicolas
Malebranche (CE 1638-1715) in 1699 ) makes the wave interpretation look more
accurate or modern to contemporary people. The corpuscular supporters
completely fail to theorize that frequency of corpuscle determines color,
thinking color is determined by corpuscle size, mass or density. Then the speed
of light not being faster in a denser medium as Newton had predicted set back
faith in the corpuscular theory even though in my mind corpuscles taking more
time in a denser medium seems logical since there is more matter to collide
with. Another interesting point is that wave functions and equations work for
light beams for either particle or wave interpretation because of the periodic
nature of light rays, which are composed of either evenly spaced particles or
evenly spaced vibrations.] (What is the current wave view? I think it is that
of Maxwell but minus the ether. So presumably the light wave is composed only
of light energy in a sine wave shape? This is like having a conversation with
an old person that cannot hear well, because, I want to say...for a wave
interpretation...the prevailing popular theory...you need the medium...and that
appears to have been removed back in early 1900....do you have some kind of
medium for the light? The current view of light is very mixed up as there has
been a compromise between particle and wave groups. The Encyclopedia Britannica
defines light as "electromagnetic radiation" stating that " In its simplest
form, quantum theory describes light as consisting of discrete packets of
energy, called photons. However, neither a classical wave model nor a classical
particle model correctly describes light; light has a dual nature that is
revealed only in quantum mechanics. This surprising wave-particle duality is
shared by all of the primary constituents of nature {e.g., electrons have both
particle-like and wavelike aspects}". I think this is basically what Planck
left in place in the 1940s. In my opinion, although I have never used any of
Planck's equations, I think the quantum can probably be interpreted as a photon
and the basis of all matter. For a wave interpretation there needs to be a
medium, and Michelson-Morley showed that there simply is no detectable medium.
My own vote is for a particle-only interpretation, and recognizing that a wave
interpretation functions as a mathematical equivalent, but probably does not
represent the true phenomena.)

(Wouldn't it seem reasonable to believe that scientists would actively put
forward experimental tests to demonstrate both views and attempt to settle the
debate between particle and wave? Perhaps creating incentives such as monetary
rewards for best experimental evidence for either side. But this was not
done.)

(One thing that is interesting is that an atomic lattice reflects its shape in
light. if it has horizontal rows, light reflecting off it has horizontal rows,
if it has a series of V shapes, photons are reflected in V shapes, etc. A sine
wave structure creates a reflected sine wave shaped beam.)
Perhaps coincidence that:
Fresnel is born in Broglie, France, and years later
Louis-Victor-Pierre-Raymond, 7th duc de Broglie will show how an electron can
be represented mathematically using wave equations, in a way uniting the wave
theory to all matter as particle theories. The wave theory may appeal to those
who rejected the theory of atoms, in particular after Dalton. In the view I
support the ultimate atom is a particle of light.

Fresnel enters the École Polytechnique at age 16.
In 1814, when Napoleon returns
from Elba (03/01/1814), Fresnel supports the royalists and loses his job as a
result.
Fresnel uses a period of house arrest in 1814 to develop the mathematics of
light waves, polarization, birefringence, and diffraction and therefore
prepares the ground for Maxwell's work on electromagnetism.
In 1817 Arago obtains for Fresnel a
permanent assignment in Paris which gives Fresnel the time and resources to
pursue his research on the wave theory.
Fresnel is awarded the Rumford medal from the
Royal Society.
Brewster rejects the wave theory based on the necessity of an ether.
Cauch
y will promote the wave theory of light.
Fresnel dies at the age of 39 of
tuberculosis.
Paris, France  
185 YBN
[1815 AD]
2241)
Paris, France (presumably)  
185 YBN
[1815 AD]
2324) McAdam recommends that roads should be raised for good drainage and
covered with large rocks, then with smaller stones, and finally with fine
gravel or slag, then the road is compacted with a roller.{4 spotlight}
McAdam manages the
British Tar Company. (but doesn't use tar on road?)
Paving of a road is still
sometimes called to "macadamize".

McAdam documents his work in "Remarks on the Present System of Road-Making"
(1816) and "Practical Essay on the Scientific Repair and Preservation of Roads"
(1819).
Bristol, England  
185 YBN
[1815 AD]
2419)
Paris, France (presumably)  
185 YBN
[1815 AD]
2469)
Paris, France (presumably)  
185 YBN
[1815 AD]
2470)
Paris, France (presumably)  
185 YBN
[1815 AD]
2471)
Paris, France (presumably)  
185 YBN
[1815 AD]
2479) The Davy lamp is the result of Davy's efforts after being asked by a
group of clergymen to study the problem of providing illumination in coal mines
without exploding the methane found in mines.

This lamp will save many lives.

Stephenson will claim priority in the invention.

Davy writes in 1816 (in response to an inquiry about patenting his invention):
"No, my good friend, I never thought of such a thing; my sole object was to
serve the cause of humanity, and if I succeeded I am amply rewarded in the
gratifying of having done so".
London, England  
185 YBN
[1815 AD]
2511) Henri Braconnot (BroKunO) (CE 1781-1855), describes that fats are formed
of a solid part ("absolute tallow") and an oily compound ("absolute oil").
Braconnot reaches this conclusion after pressing fats in the cold between
filter papers (Ann Chimie 1815, 93, 225). Furthermore, after saponification and
acidification Braconnot separates a solid fraction similar to "adipocire"
described by Fourcroy (1806), but Braconnot does not observed the solid
fraction's acid properties which leads Chevreul to discover stearic acid in
1820. Saponification is a reaction in which an ester is heated with an alkali,
such as sodium hydroxide, producing a free alcohol and an acid salt, especially
alkaline hydrolysis of a fat or oil to make soap. Saponification is hydrolysis
of fat into its constituent glycerol and fatty acids by boiling with alkali.
The fatty acids will be present as the sodium salts or soaps.(state founder of
saponification process)

Nancy, France  
185 YBN
[1815 AD]
2515) Because Stephenson's curiosity is aroused by the Napoleonic war news, he
enrolls in night school in order to learn to read and write.
Newcastle, England (presumably)  
185 YBN
[1815 AD]
2532)
Paris, France (presumably)  
185 YBN
[1815 AD]
2544) Prout is the son of a tenant farmer.
In 1811, Prout graduates with a medical
degree from the University of Edinburgh.
Prout's life is spent as a practising physician
in London, but he also occupies himself with chemical research.
London, England (presumably)  
185 YBN
[1815 AD]
2565)
Chevreul attends the Collège de France (1803).
In 1809 Chevreul is an assistant
to Antoine François de Fourcroy.
In 1810 Chevreul is assistant at the Musée d'Histoire
Naturelle.
From 1813 to 1830 Chevreul is professor of physics at the Lycée Charlemagne.
In 1830,
Chevreul succeeds Vauquelin as professor of chemistry at the (French Academy of
Sciences) Museum (in Paris).

Chevreul lives to 103 years old. Both his father and mother live to be over 90.
(Perhaps living to old age is inherited. It would be naturally selected for
since the longer a person lives the more chance of reproduction.)
Paris, France (presumably)  
185 YBN
[1815 AD]
2634) George Peacock (PEKoK) (CE 1791-1858), English mathematician, with
Babbage, and John Herschel use the nomenclature of Leibniz, (instead of the
notion of Newton's fluxions for calculus).

This group translates and publishes S. F. Lacroix's "Differential Calculus" in
1816.
While still an undergraduate Peacock forms a league (society?) with John
Herschel and Charles Babbage, which they call the Analytical Society, to
support the use of the continental calculus notation of Leibniz in the famous
struggle of "d-ism versus dot-age", (the battle between notation to use for
calculus, that of Leibniz {d'ism, (a play on "Deism"?)} or Newton {dotism}).
This ends in the introduction into Cambridge of the continental notation (that
of Leibniz) in the infinitesimal calculus to the exclusion of the fluxional
notation of Isaac Newton. I think, like the fonetik alphabet, the more logical,
more simple notation and/or nomenclature will eventually win, or will
eventually be more popular. Only having used Leibniz's notation I cannot give
my own opinion about which is easier to use. One question is why "exclude" the
Newton notation as opposed to personally not using or teaching it? Perhaps
these three simply advised using Leibniz's notation? A person can reject the
notation of fluxions and still accept Newton's other contributions, however,
many people have binary yes/no true/false philosophies where all the works of a
single person are rejected because of political or scientific differences.
Again I think an important idea is that differences in scientific opinion
should not result in anger but simply a difference in opinion.

(Some) mathematicians
follow J. L. Lagrange in using both these notations. The analytical society
formed in 1813 publishes various memoirs, and translates S. F. Lacroix's
"Differential Calculus" in 1816.

One Encyclopedia Britannica article describes this as replacing the cumbersome
symbolism of Newton with the more efficient type invented by Leibniz.

Asimov states that English math had suffered because of the popularity of
Newton, however, I think in retrospect, knowing that Newton's view of light
being a particle, made of matter, is probably the more accurate when compared
to light as a wave which dominates during the 1800s and 1900s and even now in
the 2000s. Peacock is a vigorous supporter of Thomas Young's work, publishing a
memoir of Thomas Young (1855), and the first two volumes of Young's collected
works in three volumes. Perhaps relevant is that Peacock's father is an
Anglican clergyman that might express conservative religious and traditional
views. Certainly some credit is due to Thomas Young for computing the
frequencies of various colors of light. So I am left to wonder if there was a
philosophical opposition to Newton, perhaps a jealousy, perhaps a political
opposition, a religious opposition, or all of these factors combined to cover
the truth of light as a particle and the basis of all matter. It seems like
almost an anti-Newton backlash happens around this time in history, and this
backlash lasts until Planck but is still being felt. Perhaps this anti-Newton
backlash is part of a larger battle between science and religion, which dates
back to the debate of the existence of deities, and then to the divinity of
Moses, Jesus and Muhammad, that is being played out still even now.
In 1809 Peacock
enters Trinity College, Cambridge, where Peacock is "second wrangler" (places
second in exams) in 1812 (Sir J. F. W. Herschel being senior).
Peacock is
elected fellow of his college in 1814, becomes assistant tutor in 1815 and full
tutor in 1823.
Cambridge, England  
185 YBN
[1815 AD]
2784) Borax (also called Tincal), is a soft and light, colorless crystalline
substance. Borax is used as a cleaning compound, hydrated sodium borate,
(sodium tetraborate decahydrate) Na2B4O7·10H2O, and as an anhydrous sodium
borate in the manufacture of glass and various ceramics.

Borax is used as a component of glass and pottery glazes in the ceramics
industry, as a solvent for metal-oxide slags in metallurgy, as a flux in
welding and soldering, and as a fertilizer additive, a soap supplement, a
disinfectant, a mouthwash, and a water softener.
The American Chemical Society's
Cellulose and Renewable Materials Division has established an annual award in
his honor, the Anselme Payen Award.
In 1835, Payen becomes professor of industrial and
agricultural chemistry at the Central School of Arts and Manufactures, Paris.
Paris, France (presumably)  
185 YBN
[1815 AD]
3224)
Philadelphia, Pennsylvania, USA (presumably)  
184 YBN
[02/29/1816 AD]
3838)
Edinburgh, Scotland (presumably)  
184 YBN
[1816 AD]
2351) In 1813 lithography becomes popular in France. Lithography is the process
of printing from a plane surface (such as a smooth stone or metal plate) on
which the image to be printed is ink-receptive and the blank area ink-repellent
usually because it is painted with an oil-based material which repels the
water-based ink. In 1813, Niépce begins to experiment with lithography.
Unskilled in drawing, and unable to get lithographic stone locally, Niépce
tries to find a way to create images automatically (from light). Niépce coats
pewter with various light-sensitive substances to try and capture an image from
superimposed engravings in sunlight.
In April 1816, Niépce starts experimenting with
photography using a camera. Niépce calls photography "heliography"
(sundrawing). Niépce records a view from his workroom window on paper covered
with silver chloride but can only partially fix the image.
Niépce then tries the
light-sensitive material "bitumen of Judea", a kind of asphalt that hardens on
exposure to light. Using this material Niépce succeeds in 1822, in making a
photographic copy of an engraving superimposed on glass. In 1826/27, using a
camera, Niépce makes a view from his workroom on a pewter plate and this is
the first permanently fixed image (on Earth).
In 1826 Niépce makes another heliograph
from an engraved portrait by the Paris engraver Augustin-François Lemaître.
Lemaitre who makes two prints. So Niépce not only solves the problem of
reproducing nature by light, but invents the first photomechanical reproduction
process.

In 1829 Niépce, unable to reduce the exposure times, gives in to the repeated
requests of Louis-Jacques-Mandé Daguerre, a Parisian painter, to form a
partnership to perfect heliography.

Niépce died without seeing any further advance, but, building on his
knowledge, and working with his materials,
Daguerre will eventually succeeded
in reducing the exposure time by discovering a chemical process for developing
(making visible) the latent (invisible) image formed from a brief exposure.
Chalon-sur-Saône, France  
184 YBN
[1816 AD]
2384) Smith has to sell his fossil collection to the British Museum for money
and in 1819 Smith spends 10 weeks in debtor's prison.
In 1831 Smith is the first
recipient of the Wollaston medal from the Geological Society of London.
  
184 YBN
[1816 AD]
2487) Oken (not to be confused with William of Ockham (oKuM) (CE c1285-1349))
is originally named Ockenfuss.
Rudolstadt, Germany  
184 YBN
[1816 AD]
2509) Laënnec writes "In 1816, I was consulted by a young woman labouring
under general symptoms of diseased heart, and in whose case percussion and the
application of the hand were of little avail on account of the great degree of
fatness. The other method just mentioned {the application of the ear to the
chest} being rendered inadmissible by the age and (gender) of the patient, I
happened to recollect a simple and well-known fact in acoustics, and fancied,
at the same time, that it might be turned to some use on the present occasion."
Laennec's recollection alluded to the way in which sound is amplified when
transmitted through certain solid objects. Laënnec proceeds to roll up a
quire (24 sheets of paper) into a cylindrical tube and place one end of it to
the woman's chest. Laënnec writes, " was not a little surprised and pleased
to find that I could thereby perceive the action of the heart in a manner much
more clear and distinct than I had ever been able to do by immediate
application of the ear."

Laënnec names the new instrument "stethoscope," based on the Greek words
"stethos" (meaning chest) and "skopos" (observer).
Laënnec is a pupil of Jean-Nicolas
Corvisart des Marets, whom he succeeds (1823) as physician at the Hôpital de
la Charité in Paris.
In 1822, Laënnec is appointed professor at the Collège de
France.
Laënnec dies (at age 45) from Tuberculosis, probably from person he
was treating.
(Hospital Necker) Paris, France  
184 YBN
[1816 AD]
2611) In December 1813, the French Académie des Sciences announces a
mathematical prize competition on surface wave propagation on liquid of
indefinite depth. In July 1815, 25-year-old Augustin-Louis Cauchy submits his
entry, and, in August, Siméon D. Poisson, one of the judges, deposits a memoir
of his own to record his independent work (Dalmedico 1988). Cauchy is awarded
the prize in 1816, Poisson's memoir is published in 1818, and Cauchy's work
eventually appears in 1827, with an astonishing 188 pages of additional notes.

(People of this time should have realized that in the absence of an aether than
can be seen or measured, they should not presume that an aether exists.)

(Generally, certainly in France at the time of the change from corpuscular to
wave theory, it appears that conservatives support the erroneous wave theory,
while liberals support the more accurate corpuscular theory. There are clear
sides, the conservatives that support a religion, are either fooled by the
ridiculous claims of a religion, or dishonestly play along to be accepted, and
the other side which understands that the ridiculous claims of religions are
probably wrong and is more interested in truth and progress. So there is
probably no coincidence that people who support the lies of religion, are
comfortable supporting a scientific lie. So it perhaps should not be a surprise
that like many unintuitive theories, such as intelligent design versus the
theory of evolution, the big bang versus an infinite universe, time-dilation
versus time everywhere the same, that people with corrupted values and
inaccurate or dishonest beliefs support the less accurate scientific theory or
claim.)
Paris, France  
184 YBN
[1816 AD]
2668)
London, England  
184 YBN
[1816 AD]
5984)
Naples, Italy  
183 YBN
[02/10/1817 AD]
2594) The Academy of Sciences in Paris creates a prize contest for the best
paper to explain the phenomenon of inflexion (diffraction). Fresnel will win
this award in March 1819 for a paper that uses a wave theory for light, even
though many of the people on the judging commission, Biot, Laplace, Poisson,
Arago and Gay-Lussac are corpuscular theory supporters.

After the Institute had pronounced in favor of Fresnel's wave theory, the
interference explanation of diffraction has to be acknowledged by French
corpuscular supporters. Hauy in the 1821 edition of his "Traite'de physique",
and Biot in the third edition of his "Pre'cis expe'rimentale de Physique" in
1824, both give a wave explanation of diffraction where neither had in earlier
editions.

(I think one key component of believability in a theory is strictly if there is
a math formula to explain the phenomenon that is said to express some
theoretical concept of what is actually happening. So in that sense, applying
math to the diffraction phenomena or interpreting the wave math from a
corpuscular view might move science ahead in understanding physical phenomena.
My feeling is that Biot and other corpuscular supporters didn't take the time
or have the creativity necessary to understand the so-called double-slit
experiment. I know I do not have the time or money to pursue a particle
explanation, and to study the interference phenomenon in as much detail as I
want to.)

Paris, France  
183 YBN
[1817 AD]
2284)
Pairs, France  
183 YBN
[1817 AD]
2294)
Leipzig, Germany  
183 YBN
[1817 AD]
2317)
London, England  
183 YBN
[1817 AD]
2387)
Paris, France  
183 YBN
[1817 AD]
2408)
London, England  
183 YBN
[1817 AD]
2431) Cadmiun is a silvery-white ductile metal with a faint bluish tinge.
Cadmium is softer and more malleable than zinc, but slightly harder than tin.
Ca
dmium is a relatively rare element.
Cadmiun has symbol Cd, atomic number 48, closely
related to zinc, with which it is usually associated in nature.
Cadmium has an
atomic weight of 112.40 and a relative density of 8.65 at 20°C (68°F).
Cadmium's melting point of 321°C (610°F) (this seems a low melting point for
a metal) and boiling point of 765°C (1410°F) are lower than those of zinc.
There are eight naturally occurring stable isotopes, and eleven artificial
unstable radio isotopes have been reported. Cadmium is the middle member of
group 12 (zinc, cadmium, and mercury) in the periodic table.

At one time an important commercial use of cadmium was as an electrodeposited
coating on iron and steel for corrosion protection. Nickel-cadmium batteries
are the second-largest application, with pigment and chemical uses third.
Cadmiu
m is used in alkaline nickel-cadmium electric storage cells (interesting name
for batteries), which have a greater storage capacity than an equal weight of
lead-acid storage cells. ultimately one goal of battery making is the lightest
battery for the most and longest prolonged emission of electrons.

Because of cadmium's great neutron-absorbing capacity, especially the isotope
113, cadmium is used in control rods and shielding for nuclear reactors.

Cadmium is reportedly toxic, and cadmium poisoning is a recognized industrial
disease. (More info, what is evidence of toxicity? It must be tough to prove,
but perhaps other species have been tested on.)
Göttingen, Germany  
183 YBN
[1817 AD]
2493) Selenium exhibits allotropy, appearing in a number of forms The three
most important forms are the amorphous (noncrystalline), which is red when in
powder form and black when in vitreous (glassy) form; the red crystalline; and
the gray metallic, which is also crystalline. Of the three, the metallic form
is the most stable under ordinary conditions; the other forms very slowly
convert to the metallic form at room temperature.

Selenium has atomic number 34; atomic weight 78.96; melting point (of gray
selenium) 217°C; boiling point (gray) 684.9°C; relative density (gray) 4.79;
(vitreous) 4.28; valence 2, 4, or 6.

Selenium is directly below sulfur in Group 16 of the periodic table. In
chemical activity and physical properties it resembles sulfur and tellurium.

Selenium is a metalloid (an element intermediate in properties between the
metals and the nonmetals) that is widely distributed throughout the world, but
only in small quantities. (Selenium is also a semiconductor.)

Selenium occasionally occurs uncombined, usually in conjunction with free
sulfur. (Again elements found together that are not only a neutron or helium
nucleus away, but are directly above and below each other.) Selenium is more
commonly found together with the sulfides as the selenides in ores of such
metals as iron, lead, silver, and copper. When any of the selenium-containing
sulfide minerals is roasted, selenium appears as a by-product in the flue
dusts. Selenium is also extracted from the anode slimes that remain after the
electrolytic refining of copper.

A remarkable property (discovered by Willoughby Smith in 1873) of the gray
metallic form of selenium is that its electrical conductivity is greater in
light than in darkness, and the electrical conductivity increases as the
illumination increases. This property has led to use of the metallic form in
the junction rectifier and as a cathode in the photoelectric cell rectifier.

Electrical conductivity of metallic selenium increases when light collides with
it and selenium can also convert light directly into electricity. For these
reason selenium is used in photoelectric cells, solar cells, and photographic
exposure meters. Selenium is also used extensively in rectifiers because
selenium can convert alternating electric current to direct current.

(Selenium is the first element used in the invention of the electric camera.
The electric camera {using the cathode ray tube display} will greatly reduce
the size of cameras, in addition to the time and effort needed to retrieve and
develop film. Selenium therefore plays a large role in the secret history of
cameras that see thought and secretly distributed throughout many people's
houses.)
Stokholm, Sweden (presumably)  
183 YBN
[1817 AD]
2533)
Paris, France (presumably)  
183 YBN
[1817 AD]
2537) Bessel uses a "heliometer", which Bessel designs and Fraunhofer builds to
measure the tiny displacements of 61 Cygni. A heliometer is an instrument
designed for measuring the apparent diameter of the Sun.
In 1804 the young Bessel
writes a paper on Halley's Comet in which Bessel calculates the orbit from
observations made in 1607. Bessel sends this paper to the astronomer Wilhelm
Olbers, who is so impressed that Olbers arranges for the paper to be published
in the important German technical journal "Monatliche Correspondenz" and
proposes Bessel as assistant at the Lilienthal observatory of the celebrated
lunar observer J.H. Schröter.

Bessel is appointed by King Frederick William III of Prussia to supervise the
construction of the observatory at Königsberg and Bessel remains as director
of this observatory from 1810 until he dies.
Königsberg, (Prussia now:) Germany  
183 YBN
[1817 AD]
2584) Pelletier studies and teaches at the Ecole de Pharmacie in Paris until
his retirement in 1842.
Paris, France  
183 YBN
[1817 AD]
2590)
Paris, France  
183 YBN
[1817 AD]
2600) This book will be translated into English for the Cavendish Society from
1848 to 1859.
Gmelin's great uncle was the German explorer Johann Georg Gmelin
(GumAliN) (CE 1709-1755).
Gmelin studies medicine and chemistry at Göttingen, Tubingen and
Vienna.
From 1817-1851 Gmelin is the first chair of chemistry at Heidelberg.
Heidelberg, Germany  
183 YBN
[1817 AD]
2783) Pander investigates Palaeozoic rock strata and is the first to describe
the remains of the ancient, primitive creatures known as conodonts.

The research begun by Pander is continued by his associate, another Baltic
scientist Karl Ernst von Baer (1792-1876).
Pander works on his estate at Carnikava, near
Riga.
Carnikava (near Riga), Latvia  
183 YBN
[1817 AD]
3307) Döbereiner is a coachman's son an so (does not receive) formal
schooling, but is apprenticed to an apothecary, reads widely, and attends
science lectures.
Döbereiner attends the University of Jena.
In 1810, Döbereiner becomes an
assistant professor at the University of Jena.
Jena, Germany  
182 YBN
[11/26/1818 AD]
2340)
Marseilles, France  
182 YBN
[11/26/1818 AD]
2341)
Marseilles, France  
182 YBN
[1818 AD]
2391) In 1793 Geoffroy becomes professor of vertebrate zoology at the National
Museum of Natural History, the chair of invertebrate zoology is held by
Lamarck. (This shows that the French Revolution may have contributed a stimulus
to the theory of evolution, and to the sciences of anatomy, and paleontology.)

In 1798 Geoffroy accompanies Napoleon on his conquest of Egypt and contributes
to the 24 volumes of the "Description de l'Egypte" (1809-28, "Description of
Egypt").
Paris, France  
182 YBN
[1818 AD]
2447)
Hannover, Germany  
182 YBN
[1818 AD]
2452)
Paris, France (presumably)  
182 YBN
[1818 AD]
2489) Benjamin Silliman (CE 1779-1864) founds the "American Journal of Science
and Arts" which is influential in developing American science.

New Haven, Connecticut, USA (presumably)  
182 YBN
[1818 AD]
2512)
Nancy, France  
182 YBN
[1818 AD]
2538)
Königsberg, (Prussia now:) Germany  
182 YBN
[1818 AD]
2547)
London, England (presumably)  
182 YBN
[1818 AD]
2549)
Paris, France (presumably)  
182 YBN
[1818 AD]
2585) The nux vomica tree of India is the main commercial source of strychnine.
Strychnine has a molecular formula of C21H22N2O2. Strychnine is practically
insoluble in water and is soluble only with difficulty in alcohol and other
common organic solvents. Strychnine has an exceptionally bitter taste.

Strychnine has been used in rodent poisons and in smaller doses as a stimulant
in veterinary practice. Strychnine increases the reflex irritability of the
spinal cord, which results in a loss of normal inhibition of the body's motor
cells, causing severe contractions of the muscles; arching of the back is a
common symptom of poisoning. Strychnine rapidly enters the blood, whether taken
orally or by injection, and symptoms of poisoning usually appear within 20
minutes. The symptoms begin with cramps and soon culminate in powerful and
agonizing convulsions that subside after a minute but recur at a touch, a
noise, or some other minor stimulus. Death is usually due to asphyxiation
resulting from continuous spasms of the respiratory muscles. (In my opinion
death by strychnine sounds too painful and long in duration to be a form of
murdering an organism, in particular when neuron activation and other painless
quick methods must exist.)
Paris, France  
182 YBN
[1818 AD]
2593) Biot publishes this in "Me'moire sur les rotations que certaines
substances impriment aux axes de polarisation des rayons lumineux", with the
Academie des Sciences.
Paris, France (presumably)  
182 YBN
[1818 AD]
2712) Michael Faraday (CE 1791-1867) begins a series of successful experiments
on alloys of steel. Later work on steel alloys is based on Faraday's work.

(Royal Institution in) London, England  
182 YBN
[1818 AD]
2790) This find is published in Ehrenberg's doctoral thesis, which describes
250 species of fungi from the Berlin district, of which sixty-two were new to
science.
Berlin, Germany  
182 YBN
[1818 AD]
5981) Nicolò Paganini (CE 1782-1840), Italian violinist and composer, composes
"Caprice No. 24 in A minor", Op. 1. (verify)
Italy  
181 YBN
[12/??/1819 AD]
2768) In 1821 Mitscherlich becomes professor of chemistry at the University of
Berlin.
Berlin, Germany  
181 YBN
[1819 AD]
2212) Thomas Jefferson (CE 1743-1826), American statesman and scholar, founds
the University of Virginia and designs its initial buildings.

Charlottesville, Virginia, USA  
181 YBN
[1819 AD]
2429) Naphthalene is a white crystalline compound, C10H8, derived from coal tar
or petroleum and used in manufacturing dyes, moth repellents, and explosives
and as a solvent. Naphthalene is also called tar camphor.

Kidd is appointed professor of chemistry at Oxford two years after getting his
MD there. This shows how health and chemistry were linked for many years, a
link that is no longer apparent.
London, England (presumably)  
181 YBN
[1819 AD]
2430) As a female, the main higher education institutions are closed to
Germain, however she gets the lecture notes of the mathematician J. L.
Lagrange, which he had delivered at the newly founded Ecole Polytechnique.
Germain also begins
to correspond with prominent mathematicians using the pseudonym Le Blanc and
allows them to assume that she is a man.
Germain sends in a report using a male
pseudonym, (M. Le Blanc) Lagrange is astonished at the value of the report and
even after finding that the author is a woman sponsors (more detail) Germain's
work from then on.
In 1804 Germain initiates a correspondence with Gauss under
her male pseudonym. Gauss learns of Germain's true identity when a family
friend locates Gauss to verify his safety at Germain's request during the
French occupation of Hannover in 1807.

In 1809 the French Academy of Sciences offers a prize for a mathematical
account of the phenomena of vibrating plates described by the German physicist
Ernst F.F. Chladni (and Hooke before Chladni). Germain submits a paper each of
three times, and finally wins on the third try in 1816.
Germain publishes her work
(on the vibrating plates) privately in 1821 as "Recherches sur la théorie des
surfaces élastiques" ("Researches on the Theory of Elastic Surfaces").

Germain is the first woman not related to a member by marriage to attend
Academie des Sciences meetings, and is also the first woman invited to sessions
at the Institut de France.

Gauss arranged for Germain to be awarded an honorary degree from Göttingen but
Germain dies before the degree can be awarded.

Fermat's last theorem states that there is no solution for the equation xn + yn
= zn if n is an integer greater than 2 and x, y, and z are nonzero integers.
Germain proves the special case in which x, y, z, and n are all relatively
prime (have no common divisor except for 1 (and self, needs more explanation))
and n is a prime smaller than 100.
Germain does not publish her work and her result
will first appear in 1825 in a supplement to the second edition of Legendre's
"Théorie des nombres".
Fermat's last theoren will be proved for all cases by the English
mathematician Andrew Wiles in 1995.
Paris, France (presumably)  
181 YBN
[1819 AD]
2513)
Nancy, France  
181 YBN
[1819 AD]
2574) In 1819 Purkinje earns an MD from the University of Prague.
From 1823-1850
Purkinje is chair of physiology and pathology at the University of Breslau,
Prussia.
In 1832, Purkinje acquires a compound microscope.
At the University of Breslau,
Purkinje creates the planet's first independent department of physiology in
1839 and the first official physiological laboratory, known as the
Physiological Institute in 1842.
From 1850-1869 Purkinje is professor of physiology
at the University of Prague.
Prague, (now:) Czech Republic  
181 YBN
[1819 AD]
2586) Pierre Joseph Pelletier (PeLTYA) (CE 1788-1842) and Bienaimé Caventou
(KoVoNTU (1795-1877), isolate brucine, C23H26N204, an alkaloid from "false
Angustura" bark. Brucine crystallizes in prisms with four molecules of water;
when anhydrous brucine melts at 178° (C). Brucine is very similar to
strychnine, both chemically and physiologically.

Brucine, a poisonous white crystalline alkaloid, (is most commonly, like
strychnine) derived from the seeds of nux vomica and closely related plants and
used to denature alcohol.
Brucine is named after the Scottish explorer James Bruce
(1730-1794).
Paris, France  
181 YBN
[1819 AD]
2598)
Paris, France  
181 YBN
[1819 AD]
2719) In 1835 Encke's comet passes close enough to Mercury to allow the mass of
Mercury to be determined for the first time. t: Since the mass of the comet has
only a little effect on Mercury being much smaller than Mercury, the equation
is simply the a=GMmerc/r^2, although how is the distance between the two
calculated? Perhaps the distance between was extrapolated according to
perspective?)

Encke establishes methods for calculating the orbits of minor planets and
orbits of double stars.
Encke is educated at Hamburg and the University of
Göttingen, where Encke works under the direction of Carl Friedrich Gauss.
(Seeberg Observatory near) Gotha, Germany  
181 YBN
[1819 AD]
2720)
(Ecole Polytechnique) Paris, France (presumably)  
181 YBN
[1819 AD]
2728) John Herschel is the only child of William Herschel.
In 1809 Herschel
enters the University of Cambridge in the company of Charles Babbage,
mathematician and inventor of the computer, and George Peacock, also a
mathematician and later a theologian.
In 1812 Herschel, Babbage and Peacock
found the Analytical Society of Cambridge to introduce continental methods of
mathematical calculus into English practice.
Also in 1812, Herschel submits his first
mathematical paper to the Royal Society.
In 1813 Herschel earns first place in
the university mathematical examinations.
In 1820 Gerschel is among the founders of the Royal
Astronomical Society.
London, England (presumably)  
181 YBN
[1819 AD]
3682)
(Royal Institution in) London, England (presumably)  
180 YBN
[01/01/1820 AD]
1248) Forty psychiatric hospitals (mad-houses) are in business in London, up
from twenty, 32 years before in 1788, and this shows the rising popularity of
this trade.

  
180 YBN
[04/21/1820 AD]
2454) (In what has become a classic story in the history of science), Ørsted
is lecturing during a class, and decides to demonstrate the experimental
evidence in support of his conjecture of the possible electric discharge on a
magnetic needle placed near the circuit. During this experiment is when Ørsted
notices that the compass needle moves under a wire with current.
This is the first
connection between electricity and magnetism. This is the beginning of the
study of electromagnetism (electricity and magnetism joined together).

According to Asimov, Scientists had long suspected that there might be some
connection between electricity.

When this finding is announced in 1820, (like many initial science advances) it
sets off an explosion of activity. From this Michael Faraday will create the
electric motor, and electric generator, Carl Gauss and independently Joe Henry
will create the telegraph from this finding.

Ørsted shows that the force of the current on the needle makes itself felt
through glass, metals, and other nonmagnetic substances.


In 1823 Ampere theorizes that magnetism may in fact be electricism, and that a
permanent magnet has a constant current running through it that causes an
electric field. This logical view that magnetism (a magnetic field) is simply
the result of electric current (is an electric field) is surprisingly rejected
by the majority of people in science even to this day. It seems clear that
ultimately, the entire concept of magnetism, including electromagnetism, will
remain in the past, replaced by the more simple and accurate concept of
electricity.

In an 1812 book Oersted publishes in Berlin, Oersted proposes experiments with
galvanic electricity to find out "whether electricity in its most latent state
has any action on a magnet".

Ørsted will publish a condensed account of his of his experiments in Latin on
07/21/1820. Ørsted writes (translated from Latin (give title in Latin)):
"Experiments
on the Effect of a Current of Electricity on the Magnetic Needle

The first experiments respecting the subject which I mean at present to
explain, were made by me last winter, while lecturing on electricity,
galvanism, and magnetism, in the University. It seemed demonstrated by these
experiments that the magnetic needle was moved from its position by the
galvanic apparatus, but that the galvanic circle must be complete, and not
open, which last method was tried in vain some years ago by very celebrated
philosophers. But as these experiments were made with a feeble apparatus, and
were not, therefore, sufficiently conclusive, considering the importance of the
subject, I associated myself with my friend Esmarck to repeat and extend them
by means of a very powerful galvanic battery, provided by us in common. Mr.
Wleugel, a Knight of the Order of Dannebord, and at the head of the Pilots, was
present at, and assisted in, the experiments. There were present likewise
Reinhardt, Professor of Natural History, Mr. Jacobsen, Professor of Medicine,
and that very skillful chemist, Mr. Zeise, Doctor of Philosophy. I had often
made experiments by myself; but every fact which I had observed was repeated in
the presence of these gentlemen.
The galvanic apparatus which we employed consists of
twenty copper troughs, the length and height of each of which was 12 in.; but
the breadth scarcely exceeded 2 1/2 in. Every trough is supplied with two
plates of copper, so bent that they could carry a copper rod, which supports
the zinc plate in the water of the next trough. The water of the troughs
contained one-sixtieth of its weight of sulphuric acid, and an equal quantity
of nitric acid. The portion of each zinc plate sunk in the water is a square
whose side is about 10 in. in length. A smaller apparatus will answer provided
it be strong enough to heat a metallic wire red hot.
The opposite ends of the
galvanic battery were joined by a metallic wire, which, for shortness sake, we
shall call the uniting conductor, or the uniting wire. To the effect which
takes place in this conductor and in the surrounding space, we shall give the
name of the conflict of electricity.
Let the straight part of this wire be placed
horizontally above the magnetic needle, properly suspended, and parallel to it.
If necessary, the uniting wire is bent so as to assume a proper position for
the experiment. Things being in this state, the needle will be moved, and the
end of it next the negative side of the battery will go westward.
If the distance of
the uniting wire does not exceed three-quarters of an inch from the needle, the
declination of the needle makes an angle of about 45°. If the distance is
increased, the angle diminishes proportionally. The declination likewise varies
with the power of the battery.
The uniting wire may change its place, either towards
the east of west, provided it continue parallel to the needle, without any
other change of the effect than in respect to its quantity. Hence the effect
cannot be ascribed to attraction; for the same pole of the magnetic needle,
which approaches the uniting wire, while placed on its east side, ought to
recede from it when on the west side, if these declinations depended on
attractions and repulsions. The uniting conductor may consist of several wires,
or metallic ribbons, connected together. The nature of the metal does not alter
the effect, but merely the quantity. Wires of platinum, gold, silver, brass,
iron, ribbons of lead and tin, a mass of mercury, were employed with equal
success. The conductor does not lose its effect, though interrupted by water,
unless the interruption amounts to several inches in length.
The effect of the
uniting wire passes to the needle through glass, metals, wood, water, resin,
stoneware, stones; for it is not taken away by interposing plates of glass,
metal or wood. Even glass, metal, and wood, interposed at once, do not destroy,
and indeed scarcely diminish the effect. The disc of the electrophorus, plates
of prophyry, a stoneware vessel, even filled with water, were interposed with
the same result. We found the effects unchanged when the needle was included in
a brass box filled with water. It is needless to observe that the transmission
of effects through all these matters has never before been observed in
electricity and galvanism. The effects, therefore, which takes place in the
confluct of electricity are very different from the effects of either of the
electricities.
If the uniting wire be placed in a horizontal plane under the magnetic needle,
all the effects are the same as when it is above the needle, only they are in
an opposite direction; for the pole of the magnetic needle next the negative
end of the battery declines to the east.
That these facts may be the more easily
retained, we may use this formula-the pole above which the negative electricity
enters is turned to the west; under which, to the east.
If the uniting wire is so
turned in a horizontal plane as to form a gradually increasing angle with the
magnetic meridian, the declination of the needle increases, if the motion of
the wire is towards the place of the disturbed needle; but it diminishes if the
wire moves further from that place.
When the uniting wire is situated in the same
horizontal plane in which the needle moves by means of the counterpoise, and
parallel to it, no declination is produced either to the east or west; bu an
inclination takes place, so that the pole, next which the negative electricity
enters the wire, is depressed when the wire is situated on the west side, and
elevated when situated on the east side.
If the uniting wire be placed
perpendicularly to the plane of the magnetic meridian, whether above or below
it, the needle remains at rest, unless it be very near the pole; in that case
the pole is elevated when the entrance is from the west side of the wire, and
depressed, when from the east side.
When the uniting wire is placed perpendicularly
opposite to the pole of the magnetic needle, and the upper extremity of the
wire receives the negative electricity, the pole is moved towards the east; but
when the wire is opposite to a point between the pole and the middle of
theneedle, the pole is moved towards the west. When the upper end of the wire
receives positive electricity, the phenomena are reversed.
If the uniting wire is bent
so as to form two legs parallel to each other, it repels or attracts the
magnetic poles according to the different conditions of the case. Suppose the
wire placed opposite to either pole of the needle, so that the plane of the
parallel legs is perpendicular to the magnetic meridian, and let the eastern
leg be united with the negative end, the western leg with the positive end of
the battery in that case the nearest pole will be repelled either to the east
or west according to the position of the plane of the legs. The eastmost leg
being united with the positive, and the westmost with the negative side of the
battery, the nearest pole will be attracted. When the plane of the legs is
placed perpendicular to the place between the pole and the middle of the
needle, the same effects recur, but reversed.
A brass needle, suspended like a magnetic
needle, is not moved by the effect of the uniting wire. Likewise needles of
glass and of gum lac remain unacted on.
We may now make a few observations
towards explaining these phenomena.
The electric conflict acts only on the magnetic
particles of matter. All non-magnetic bodies appear penetrable by the electric
conflict, while magnetic bodies, or rather their magnetic particles, resist the
passage of this conflict. Hence they can be moved by the impetus of the
contending powers.
It is sufficiently evidence from the preceding facts that the
electric conflict is not confined to the conductor, but dispersed pretty widely
in the circumjacent space.
From the preceding facts we may likewise infer that this
conflict performs circles; for without this condition it seems impossible that
the one part of the uniting wire, when placed below the magnetic pole, should
drive it towards the east, and when placed above it towards the west; for it is
the nature of a circle that the motions in opposite parts should have an
opposite direction. Besides, a motion in circles, joined with a progressive
motion, according to the length of the conductor, ought to form a conchoidal or
spiral line; but this; unless I am mistaken, contributes nothing to explain the
phenomena hitherto observed.
All the effects on the north pole above-mentioned are
easily understood by supposing that negative electricity moves in a spiral line
bent towards the right, and propels the north pole, but does not act on the
south pole. The effects on the south pole are explained in a similar manner, if
we ascribe to positive electricity a contrary motion and power of acting on the
south pole, but not upon the north. The agreement of this law with nature will
be better seen by a repetition of the experiments than by a long explanation.
The mode of judging of the experiments will be much facilitated if the course
of the electricities in the uniting wire be pointed out by marks or figures.
I shall
merely add to the above that I have demonstrated in a book published 5 years
ago that heat and light consist of the conflict of the electricities. From the
observations now stated, we may conclude that a circular motion likewise occurs
in these effects. This I think will contribute very much to illustrate the
phenomena to which the appellation of polarization of light has been given.".

Oersted leaves three accounts of how he made his famous discovery which all
agree but conflict other accounts in which the discovery is described as an
accident. The first account of the discovery as an accident is given in German
by Ludwig Wilhelm Gilbert, the editor of the Annalen der Physik who writes
"What every search and effort had not produced, came to Professor Oersted in
Copenhagen by an accident during his lectures on electricity and magnetism in
the past winter". Another account describing the discovery as an accident is
given in a letter to Michael Faraday by Professor Hansteen's 37 years after the
discovery. Hansteen writes that "...Once, after the end of his lecture, as he
had used a strong galvanic battery in other experiments he said, 'Let us now
once, as the battery is in activity, try to place the wire parallel to the
needle'; as this was made, he was quite struck with perplexity by seeing the
needle making a great oscillation (almost at right angles with the magnetic
meridian). Then he said: 'Let us now invert the direction of the current' and
the needle deviated in the contrary direction. Thus the great detection was
made; and it has been said, not without reason, that 'he tumbled over it by
accident'. He had not before any more idea than any other person that the force
should be transversal. But, as Lagrange has said of Newton on a similar
occasion, 'Such accidents only meet persons who deserve them'.".

Oersted reviews the background of his discovery in his historical sketch of
1821 in order to express his explicit denial that the discovery was made by
accident. This account from Oersted is sometimes ignored in favor of the two
other versions which historian R. C. Stauffer states cannot survive critical
scrutiny. Oersted writes in his first of three accounts as follows:
" Since for a long
time i had regarded the forces which manifest themselves in electricity as the
general forces of nature, I had to derive the magnetic effects from them also.
As proof that I accepted this consequence completely, I can cite the following
passage from my Recherches sur l'identite des forces chimiques et electriques
printed in Paris 1813. 'It must be tested whether electricity in its most
latent state has any action on the magnet as such.' I wrote this during a
journey so that I could not easily undertake the experiments; not to mention
that the way to make them was not at all clear to me at that time, all my
attention being applied to the development of a system of chemistry. I still
remember that, somewhat inconsistently, I expected the predicted effect
particularly from the discharge of a large electric battery and, moreover, only
hoped for a weak magnetic effect. Therefore I did not pursue with proper zeal
the thoughts I had conceived; I was brought back to them through my lectures on
electricity, galvanism and magnetism in the spring of 1820. The auditors were
mostly men already considerably advanced in science; so these lectures and the
preparatory reflections led me on to deeper investigations than those which are
admissible in ordinary lectures. Thus my former conviction of the identity of
electrical and magnetic forces developed with new clarity, and I resolved to
test my opinion by experiment. The preparations for this were made on a day in
which I had to give a lecture the same evening. I therefore showed Canton's
experiment on the influence of chemical effects on the magnetic state of iron.
I called attention to the variations of the magnetic needle during a
thunderstorm, and at the same time I set forth the conjecture that an electric
discharge could act on a magnetic needle placed outside the galvanic circuit. I
then resolved to make the experiment. Since I expected the greatest effect from
a discharge associated with incandescence, I inserted in the circuit a very
fine platinum wire above the place where the needle was located. The effect was
certainly unmistakable, but it seemed to me so confused that I postponed
further investigation to a time when I hoped to have more leisure. At the
beginning of July these experiments were resumed and continued without
interruption until I arrived at the results which have been published.".
(Notice the use of the word "thought", possibly evidence, although very weak,
of seeing eyes by this time.)


Gian Domenico Romagnosi (1761-1835) had published an account of a relationship
between electricity and magnetism in 1802.

The unit of magnetic field strength is named the "oersted" in his honor in
1934.
Copenhagen, Denmark  
180 YBN
[07/21/1820 AD]
2457)
Copenhagen, Denmark (presumably)  
180 YBN
[09/18/1820 AD]
2423) French mathematician and physicist, André Marie Ampère (oMPAR) (CE
1775-1836) relates direction of current in a wire to magnetic force.

Ampère (oMPAR) creates the "right hand screw rule". The right hand is imagined
holding the wire with the thumb pointing in the direction of the current. The
fingers then indicate the direction in which the north pole of a magnet will be
deflected. One can imagine a magnetic force circling the wire. This is the
beginning of the concept of "lines of force" that Faraday will generalize. The
direction of current had to be determined and Ampère decides wrongly to use
Franklin's guess of an excess of "electrical fluid" moving from positive to
negative, which is now known to be backward; electrical fluid (electrons) moves
from negative to positive. So technically in terms of current, this rule should
be the "left hand screw rule".
Paris, France  
180 YBN
[09/25/1820 AD]
2424) In this way, Ampère shows that attraction and repulsion in a current
carrying wire does not need a magnet or iron fillings to be visualized.

Ampère also works with magnetic fields made by currents flowing through a
circular wire. Ampère and Arago both recognize that in theory, wire in a
spiral (helix) shape, a wire curved into a spring shape will behave like a bar
magnet. Ampère calls this kind of helix a solenoid. Sturgeon will put this
into practice (inventing the first inductor), and Henry will refine this
idea.(chronology) This property of a spiral of wire will fuel many of the
inventions such as the telegraph, electric motor, and telephone.

Ampère's experiments names the science of electric currents in motion as
"electrodynamics" and introduces the term "electrostatics" for the older study
of stationary electric charges. (Although, in my mind, there is basically the
field of electronics or electricity, also known as electrical science or
electrical engineering.) (chronology)

(Who is first to measure force of attraction or repulsion between moving
current in a wire and static electricity? Perhaps Weber and Kohlrausche in
measuring a ratio of static to moving {dynamic} electric charge {or the measure
of force causing mechanical movement} in 1854.)

Biot and Savart had interpreted Oersted's discovery as showing that the
electric current had magnetized the wire it was moving in and then interacted
with the magnetic needle in a similar way of two usual magnets. Ampere viewed
Oersted's discovery differently as being the interaction between currents,
which means that there should exist microscopic currents within permanent
magnets. To prove this point, only a week after Arago had demonstrated
Oersted's discovery, Ampere shows at the Academy, that two parallel wires
carrying currents attract one another if the currents are in the same
direction, and repel each other if the currents are in the opposite directions.
Ampere then spends 7 years immersed in experimental research to identify the
correct mathematical expression describing the force between current elements.

Ampère theorizes that a magnet owes its power to elementary current loops
perpendicular to its axis, in other words that all magnetism can be attributed
to electric currents. So current flowing forward in a spiral direction is
viewed to be the reason for a magnetic field in a current carrying wire. In
modern terms, the magnetic field is made of electrons in the current extending
outside the visible wire.

According to Asimov, contemporaries of Ampère are very skeptical of this idea.
Augustin Jean Fresnel (FrAneL) (CE 1788-1827) claims that the materials that
can be made into magnets, iron and steel are poor conductors, and current
moving through a poor conductor causes heat and so all magnets would always be
warm. (find original source)(But possibly the current is so small that the
heating is not noticeable.)

This is the first understanding that a magnetic field is the same as an
electric field, and that a magnetic field is probably caused by current moving
in a permanent magnet, which eliminates the concept of "magnetism" and a
"magnetic field" altogether as being "electrism" and an "electric field".
However, Maxwell and others still view a magnetic field as a separate
phenomenon, different from an electric field. This mistaken belief of magnetism
(or magneticity) being different from electrism (or electricity) has lasted
even to this day.

If this theory is true, even a needle deflected by a permanent magnetic field
is measuring the strength of a current.

(EX: Perhaps a permanent magnet can be created by wiring a very long complete
circuit insulated wire around a cylinder of wood with a hole running through
the center.)

The historian R. Tricker writes of this paper:
"At this stage Ampere is
obviously thinking of macroscopic currents rather than the molecular currents
which he later proposed. The particles of the steel bar of a magnet acted like
the elements of an electric pile and drove a current round the bar producing a
solenoidal electric current. He had arrived at this idea from a similar
postulate about the earth's currents by means of which he explained terrestrial
magnetism. In this case he imagined that the different rocks and minerals in
the earth's crust acted like a pile generating currents in planes parallel to
the equator.
he even suggested that the heat of earth might be caused by such
currents.". Ampere will later theorize that the currents in a magnet must be
distributed throughout its volume, describing these currents as molecular
currents. (I think this is similar to my own view - that the currents flow in a
helix, perhaps with an excess of negative particles at one pole and an excess
of positive particles at the other pole.)
Paris, France  
180 YBN
[10/30/1820 AD]
2418)
Paris, France (presumably)  
180 YBN
[1820 AD]
2455)
Copenhagen, Denmark (presumably)  
180 YBN
[1820 AD]
2486)
Halle, Germany  
180 YBN
[1820 AD]
2505) After Bellingshausen's voyage, the world's ice-free ocean is completely
explored, all that remains is the frozen polar wastes and continental
interiors.
Antarctica  
180 YBN
[1820 AD]
2559)
Paris, France (presumably)  
180 YBN
[1820 AD]
2587) Asimov explains that around this time chemistry is moving from analysis
of naturally occurring molecules to analysis of synthetic molecules.

Quinine (KWIniN, KWInEN) is a white crystalline alkaloid with a bitter taste.
Quinine has the chemical formula: C20H24N2O2. Quinine is obtained from cinchona
bark and is used as a drug mainly in the treatment of malaria. The treatment of
malaria with quinine will mark the first successful use of a chemical compound
in combating an infectious disease.

Cinchonine, like quinine, is an alkaloid, C19H22N2O, derived from the bark of
various cinchona trees and used as an antimalarial agent.

Colchicine is a poisonous, pale-yellow alkaloid, C22H25NO6, obtained from the
autumn crocus and used in plant breeding to induce chromosome doubling and in
medicine to treat gout.
Paris, France  
180 YBN
[1820 AD]
2591) In 1819 Fresnel was nominated a commissioner of lighthouses for which
Fresnel was the first to construct compound lenses as substitutes for mirrors.
Paris, France  
180 YBN
[1820 AD]
2628) John Frederic Daniell (CE 1790-1845), English chemist, invents a
dew-point hygrometer (a device that indicates atmospheric humidity) (Quar.
Journ. Sci., 1820), which is widely used.

Daniell's "Essay on Artificial Climate Considered in Its Applications to
Horticulture" shows the importance of humidity in greenhouses.

Danielle's hygrometer is made with two thin glass bulbs that are hung from a
base and joined with a glass tube. One of the glass bulbs holds ether and a
thermometer that collects and dissipates dew when the other bulb is slowly
cooled and reheated. The condensing temperature is produced by evaporation of
the ether. Daniell's hygrometer, as it is called, enables the easy
determination of vapor that exists in a given mass of atmosphere. The average
temperature recorded by the device is the dew point. (make clearer)

In 1831 Daniell becomes the first professor of chemistry at the newly founded
King's College in London.

In 1839 Daniell publishes "Introduction to the Study of Chemical Philosophy".

In 1841, Daniell becomes a founding member and vice president of the Chemical
Society of London.

Daniell authors many papers that are published in journals of science.
London, England (presumably)  
180 YBN
[1820 AD]
2635) George Peacock (PEKoK) (CE 1791-1858), publishes "A Collection of
Examples of the Application of the Differential and Integral Calculus" which
aids the movement to use the "Continental" calculus notion of Leibniz as
opposed to the fluxion notion of Newton.

Cambridge, England (presumably)  
180 YBN
[1820 AD]
2698) Faraday has an electrical unit of charge named after him (a Faraday is an
amount of electricity measured during electrolysis) and the unit of
capacitance, the farad is named after Faraday.

Faraday wears no wig as wigs had passed out of popularity by the beginning of
the 1800s. Instead Faraday wears a black neck tie, vest and blazer every day,
the neck tie and blazer are still popular today.
Faraday is one of four children of a
blacksmith who moves with his family to London in 1791 to look for work.
Faraday
later recalls being given one loaf of bread that had to last him for a week.
Faraday's
family belongs to a Christian sect called the Sandemanians, a sect that no
longer exists.
Faraday receives only the rudiments of an education, learning to
read, and write in a church Sunday school.
At an early age Faraday earns money by
delivering newspapers for a book dealer and bookbinder.
In 1805, at age 14, Faraday is
apprenticed to the bookbinder and bookseller, and Faraday is therefore exposed
to many books. Faraday is particularly fascinated by the article on electricity
in the third edition of the Encyclopedia Britannica and reads Lavoisier's
textbook on chemistry. (there are other examples of people working with books
that go on to achieve in science. (name examples) I think there is the
potential for a relationship between access to books (and videos, etc) and
wisdom. Now with the Internet, we should see collective wisdom grow much faster
and larger in scale.) (In some sense we can thank the public science lecture
for the electric motor.)
Faraday uses old bottles and lumber to make a crude
electrostatic generator with which Faraday does simple experiments. Faraday
also builds a weak voltaic pile with which he performs experiments in
electrochemistry.
In 1812 a customer gives Faraday tickets to attend the lectures of Humphry Davy
at the Royal Institution. Faraday takes careful notes with colorful diagrams.
Faraday ends with 386 pages which he binds in leather and sends to Banks, the
president of the Royal Society, in the hope of getting a job that will bring
him into closer contact with science. Getting no answer he sends others (he
made copies?) to Davy himself along with an application for a job as an
assistant. Davy is enormously impressed, and when Davy fires his assistant for
brawling (brawling? those are some tough assistants.), Davy offers Faraday the
job. Davy follows the advice of a trustee of the Royal Institution who says
"Let him wash bottles. If he is any good, he will accept the work; if he
refuses, he is not good for anything.".
In 1813 Faraday accepts Davy's offer of
a job as assistant at a salary smaller than the one Faraday is getting as a
bookbinder and washes bottles.
Faraday's first assignment is to accompany Davy
and his wife on a tour of Europe, during which Faraday sometimes has to be a
personal servant to the wife of Davy.
There is a saying that "Faraday was Davy's
greatest discovery", however I think Davy's contributions to science
(identifies and isolates potassium, sodium, barium, strontium, calcium and
magnesium, chlorine, that chlorine support combustion, that hydrochloric acid
contains no oxygen and so hydrogen not oxygen is characteristic of acids) place
Davy near the top of best scientists of history although Faraday probably ranks
higher and Davy's jealousy and/or anger towards Faraday is stupid.
Faraday as Davy's
assistant sees Napoleon, Volta and Vauquelin.
In 1820 Faraday's second
apprenticeship, under Davy, ends, and by this time Faraday has learned
chemistry as thoroughly as anyone alive.
In a court of law, under oath, Faraday
points out some flaws in Davy's invention of the miner's safety lamp.
In 1821
Faraday married Sarah Barnhard.
In 1825 Faraday becomes director of the laboratory.
In
1833 Faraday becomes professor of chemistry at the Royal Institution.
Faraday
gives enormously popular lectures in the style of Davy.
Faraday's reputation as
an analytical chemist leads to his being called as an expert witness in legal
trials and to the building up of clients whose fees help to support the Royal
Institution. (Royal Institution must have taken part of Faraday's fees or
rented Faraday out?)
In 1839 the Encyclopedia Britannica states that Faraday's
"health broke down" and Faraday for six years does little creative science.
Asimov claims that Faraday suffers a nervous breakdown, which is in my view an
inaccurate/fraudulent theory. The theories of psychology, I think are highly
doubtful. I think that people have moments of stress, but there is no single
thing that makes a person suddenly get some kind of disease of the kinds
claimed in psychology, and always the disease or "breakdown" is not easily
described, seldom are specific "symptoms" given and then many times symptoms
given are indicative only of an unusual view or behavior, many times only
mildly unusual but inflated to appear more important. The most I can guess is
that a person changes dramatically, and adopts a very inaccurate view of the
universe. I doubt the phenomenon of "nervous breakdown", but I can accept the
phenomenon of extreme stress resulting in passing out, temporary
unconsciousness, and I can accept that people have periods of belief in a
theory with highly inaccurate claims.

In 1824 Faraday is elected into the Royal Society with Davy casting the only
negative vote.
Faraday strongly favors a more important role for science in
education, but is too gentle to say anything. Babbage is more vocal.
In 1825 Faraday
becomes director of the laboratory.
In 1833 Faraday is made Fullerian professor of
chemistry at the Royal Institution.
In 1844 Faraday, after agonizing, decides to accept the
invitation to have dinner with Queen Victoria on a Sunday when he is due at the
small church he attends. The congregation excommunicates him and he can not be
reinstated until undergoing considerable penance. (what could that involve?)
In the 1850s
when asked to head a project to prepare poisonous gas for use on the
battlefield, Faraday admits that the project is feasible but wants nothing to
do with it.
Faraday keeps a daily record of his 42 years of scientific labors
(1820-62) which is published in 1932 in 7 volumes.

Every year on Christmas Day, Faraday presents his "Faraday Lectures for
Children" which are crowded with interested listeners. The Royal Institution
Christmas lectures for children, begun by Faraday, continue to this day.

In 1855, According to Asimov, Faraday loses his ability to think clearly some
postulate because of chronic mercury poisoning.
The Encyclopedia Britannica authors
expresses a similar view stating "From about 1855, Faraday's mind began to
fail. He still did occasional experiments, one of which involved attempting to
find an electrical effect of raising a heavy weight, since he felt that
gravity, like magnetism, must be convertible into some other force, most likely
electrical. This time he was disappointed in his expectations, and the Royal
Society refused to publish his negative results. More and more, Faraday began
to sink into senility." (The concept that all forces are the result of a single
force is a logical theory, and certainly one worth exploring experimentally and
theoretically. I happen to think all forces are the result of gravity, matter
occupying space, and collision.)
(Faraday is up there with Newton for best in science.
Galileo too, Aristarchos, Edison and many others.)

In 1857 Faraday declines the presidency of the Royal Society.
Queen Victoria
rewards Faraday's lifetime of devotion to science by granting Faraday the use
of a house at Hampton Court and and a knighthood. Faraday accepts the cottage
but rejects the knighthood; saying that he would remain plain Mr. Faraday to
the end. That Faraday rejects knighthood may imply that he is against the
concept of royalty and possibly monarchy or singular rule by heredity. To me,
many knighthoods, baronships, etc are all based on wealth, many times, without
significant contribution to science or life, and represent an empty distinction
other than "wealthy person" in that sense, although clearly there are
exceptions where people do deserve a societal reward for their contribution to
life, but then I think simply a monetary award is better than a change in name.
Maybe Faraday had a similar opinion. It would be interesting to see Faraday's
recorded reasons if any.


In 1865 Faraday writes about psychic phenomena "They who say these things are
not competent witnesses of facts". To an invitation to attend the first séance
of the Davenport brothers Faraday returns the answer, "If spirit
communications, not utterly worthless, should happen to start into activity, I
will trust the spirits to find out for themselves how they can move my
attention. I am tired of them.".

When Sir William Crookes asks Faraday how Faraday reconciles science with
religion, Faraday replies that he keeps his science and religion strictly
apart.

Some of Faraday's works are collected as "Experimental Researches in
Electricity" (3 vol., 1839-55) and "Experimental Researches in Chemistry and
Physics" (1859).

Tyndall, says of Faraday, "Taking him for all and all, I think it will be
conceded that Michael Faraday was the greatest experimental philosopher the
world has ever seen; and I will add the opinion, that the progress of future
research will tend, not to dim or to diminish, but to enhance and glorify the
labours of this mighty investigator."

The 1911 Encyclopedia Britannica states: "We have given a few examples of the
concentration of his efforts in seeking to identify the apparently different
forces of nature, of his far-sightedness in selecting subjects for
investigation, of his persistence in the pursuit of what he set before him, of
his energy in working out the results of his discoveries, and of the accuracy
and completeness with which he made his final statement of the laws of the
phenomenon."

In my own opinion, Michael Faraday is perhaps the number one contributor to
science in the entire history of Earth, or perhaps second to Isaac Newton.
There are certainly other excellent people, but no other person in science
discovered and explained as many great and important truths.
(Royal Institution in) London, England  
180 YBN
[1820 AD]
3374) To me it is very interesting that Reverend Cecil sees part of his role in
life as building and explaining devices such as combustion engines, in other
words, for actively participating in science, engineering and education, in
some sense, to understanding the principles of the universe, which appears to
be for Cecil a natural inclination, but is perhaps an unusual interpretation of
purpose for many and perhaps most reverends.

(Perhaps the gas combustion is more accurately called the gas explosion engine.
The gas combustion phenomenon, like many explosive phenomena form a similar
group of reactions where molecules and/or atoms are separated into their source
light particles - the force comes from the escaping light particles, as far as
I understand it. These are all "exothermic" phenomena, far more particles are
emitted than absorbed.)
(Magdalen College) Cambridge, England  
179 YBN
[06/??/1821 AD]
2595)
Paris, France  
179 YBN
[07/05/1821 AD]
2883) Davy writes "Imperfect conducting fluids do not give (magnetic) polarity
to steel when electricity is passed through them; but electricity passed
through air produces this effect. Reasoning on this phaenomenon, and on the
extreme mobility of the particles of air, I concluded, as M. Arago had likewise
done from other considerations, that the voltaic current in air would be
affected by the magnet. I failed in my first trial, which I have referred to in
a note to my former paper, and in other trials made since by using too weak a
magnet; but I have lately had complete success; and the experiment exhibits a
very striking phaenomenon.
Mr. Pepys having had the goodness to charge the great battery
of the London Institution, consisting of two thousand double plates of zinc and
copper, with a mixture of 1168 parts of water, 108 parts of nitrous acid, and
25 parts of sulphuric acid, the poles were connected by charcoal, so as to make
an arc, or column of electrical light, varying in lenth from one to four
inches, according to the state of rarefaction of the atmosphere in which it was
produced; and a powerful magnet being presented to this arc or column, having
its pole at a very acute angle to it, the arc, or column, was attracted or
repelled with a rotatory motion, or made to revolve, by placing the poles in
different positions, according to the same law as the electrified cylinders of
platinum described in my last paper, being repelled when the negative pole was
on the right hand by the north pole of the magnet, and attracted by the south
pole, and vice versa.
It was proved by several experiments that the motion depended
entirely upon the magnetism, and not upon the electrical inductive power of the
magnet, for masses of soft iron, or of other metals, produced no effect.
The
electrical arc or column of flame was more easily affected by the magnet, and
its motion was more rapid when it passed through a dense than through rarified
air; and in this case, the conducting medium or chain of aeriform particles was
much shorter.
I tried to gain similar results with currents of common
electricity sent through flame, and in vacuo. They were always affected by the
magnet; but it was not possible to obtain so decided a result as with voltaic
electricity, because the magnet itself became electrical by induction, and that
whether it was insulated, or connected with the ground."

It's not clear that Davy observes the illuminated glow produced by a high
electric differential through a vacuum and the deflection of that florescent
beam by a magnet as Gassiot, Plucker and others will illuminate. The battery
Davy uses is large for the time with 2000 copper-zinc plate pairs (but what
voltage is that?). Clearly enough to produce an arc four inches long.

Davy publishes this in "Farther Researches on the Magnetic Phaenomena Produced
by Electricity; With Some New Experiments on the Properties of Electrified
Bodies in Their Relations to Conducting Powers and Temperature" (1821).

This is related to using magnets to move beams of electrons in a Cathode Ray
Tube, which leads to the television.

(Does static electricity move the electrical current in air?)
London, England  
179 YBN
[09/03/1821 AD]
2607) Redfield helps to found the American Association for the Advancement of
Science. (chronology)
New York, USA  
179 YBN
[09/07/1821 AD]
1535)
  
179 YBN
[09/11/1821 AD]
2701) Michael Faraday (CE 1791-1867) invents the first electric motor, which
creates sustained mechanical motion from electricity. An electric motor is a
device that converts electrical energy to mechanical energy. The electric motor
is based on the principle that like poles of a magnet repel one another.

In 1820 Hans Christian �rsted had announced the discovery that the flow of
an electric current through a wire produces a magnetic field around the wire.
Andr�-Marie Amp�re showed that the magnetic force is a circular one,
producing a cylinder of magnetism around the wire. Faraday understands that if
a magnetic pole can be isolated, it ought to move constantly in a circle around
a current-carrying wire because of this circular force.

Davy and William Hyde Wollaston had tried to design an electric motor but had
failed. Faraday, discusses the problem with Davy and Wollaston. Faraday
publishes his results without acknowledging his debt to Wollaston and Davy (and
this causes controversy).

In 1821, a year after Oersted deflected a magnetic needle with an electric
current, Faraday creates an electric motor. Faraday converts electrical and
magnetic force into continuous mechanical movement.(again most likely the same
phenomenon, although not overwhelmingly proven or popularly accepted yet.)
Faraday uses two vessels filled with mercury, each attached to a battery by a
metal rod entering from the bottom of each vessel. The upper levels of the
mercury are connected by a curved metal bar which forms a complete circuit.
(note that mercury is a liquid metal that conducts electricity.) One end of the
curved bridge is fixed in the center of the Mercury container and on the lower
rod a movable magnet (bar or circular magnet?) is attached that can rotate
around the fixed upper rod. On the other end of the curved bridge the upper rod
ends in a hinged wire (which can move freely in a circle) that hangs into the
mercury and is able to rotate around the bottom fixed rod which extends a fixed
magnet upward. When Faraday turns on the current the movable wire rotates
around the fixed magnet while the movable magnet rotates around the fixed wire.
(I will need a visual image for this.)

Faraday successfully converts electrical and magnetic forces into continuous
mechanical movement.

Faraday publishes this in 1821 as "History of the Progress of
Electro-Magnetism".

Davy claims that Faraday got the idea from a conversation between Davy and
Wollaston, but Faraday claims that the conversation only turned his attention
to the problem and that his device is nothing like the one discussed. In
addition, Wollaston had expected the wire to rotate on an axis rather than
rotate around another wire.

The electric generator would be useless without some way of putting it to work
which the electric motor provides. The electric motor is like the opposite of
the electric generator. In an electric generator mechanical force turns a wheel
and produces electricity. In a motor, electricity turns a wheel and produces
mechanical force. The electric motor is used in vacuum cleaners, refrigerators,
computers, robots, video cameras, windshield wipers, windows, doors, thousands
of devices. (The electric motor is even now still being applied to make many
things in life automated.)

In 1821 Faraday shows a simple case of rotation produced between a magnet and a
current of electricity. Some historians credit Anianus Jedlik, Hungarian priest
and teacher, with the first electromagnet armature motor and commutator by
1928. In 1831 Henry, and 1833 Ritchie also constructs a motor with an
electromagnet armature. William Sturgeon will build a motor with a commutator
in 1832. In 1839 Jacobi will propel a boat on the Neva river at 2 1/4 miles per
hour with an electromagnetic engine of about 1 horse-power, using a battery of
64 large Grove's cells. In 1883 Nikola Tesla will invent an alternating current
motor (Induction motor).

In a simple form of electric motor, a wire-wound armature, in which a magnetic
field can be induced by an electric current, is mounted on a rotating shaft and
balanced next to a magnet (the "field" magnet). As one pole of the magnet
repels the similarly induced pole of the armature, the opposite pole on the
similar side of the armature will likewise be repelled by the similar pole of
the magnet. This repulsion will produce a torque on the the armature and it
will start revolving. The repulsion between like poles is supplemented by the
attraction between unlike poles, and the armature will continue revolving in an
effort to bring its north pole in line with the south pole of the field magnet,
and its south pole in line with the north pole of the field magnet. . Just as
this conjunction is reached, the action of the commutator - a conductor on the
rotating armature shaft- reverses the current in the armature windings. The
north and south poles in the armature are then reversed. Momentum carries the
armature past the dead center and the reversed forces of attraction and
repulsion send the armature around to its former position, where the commutator
again reverses the current continuing the motion.

(Describe later progress to more practical electric motors, including the AC
motor and step motor.)

(EX: Prove that a permanent magnet has current running through it. Maybe
increase resistance and look for change in magnetic strength? )

(It may be that an electric motor is only transferring motion from particles in
electric current to a rotor by particle collision.)

(A magnetic field is a "dynamic" or moving electric field, which is different
from a static of unmoving electric field.)

(Was the electric motor actually found much earlier and kept secret, like
neuron reading? If true then Faraday was either an excluded who reinvented the
motor, or an included who got permission to go public with the motor. Perhaps
the electric motor is one of the rare cases where a scientific invention or
innovation is made public very close to the time of it's creation.)
(Royal Institution in) London, England  
179 YBN
[12/20/1821 AD]
2882) Davy states "few sagacious reasoners, who think that our present data are
sufficient to enable us to decide on such very abstruse and difficult parts of
corpuscular philosophy." (clearly showing a preference for corpuscular versus
undulatory theory in 1821)
London, England  
179 YBN
[1821 AD]
2379)
Paris, France (presumably)  
179 YBN
[1821 AD]
2397) In 1802 Seebeck earns an MD from the University of Göttingen but prefers
scientific research.
Berlin, Germany  
179 YBN
[1821 AD]
2427)
London, England  
179 YBN
[1821 AD]
2434)
Turin, Italy (presumably)  
179 YBN
[1821 AD]
2534)
Paris, France (presumably)  
179 YBN
[1821 AD]
2572) In this paper Fraunhofer comments: "T Young had already observed that the
colored fringes which are seen in the interior of the shadow of a hair vanish
if one edge is covered so that the beams of light going by both edges must
combine to produce the interior color bands.".
Benedictbeuern (near Munich), Germany (presumably)  
179 YBN
[1821 AD]
2583)
Switzerland  
179 YBN
[1821 AD]
2588) Caffeine is a bitter white alkaloid, C8H10N4O2. Alkaloids are substances
that have marked physiological effects. Caffeine occurs in tea, coffee,
guarana, maté, kola nuts, and cacao.

Caffeine has a stimulating effect on the central nervous system, heart, blood
vessels, and kidneys. It also acts as a mild diuretic (increases the excretion
of urine).
Paris, France  
179 YBN
[1821 AD]
2610) Cauchy tries to provide the logical foundations for calculus. Bishop
Berkeley had criticized Newton-Leibniz calculus by suggesting that the faulty
reasoning of the calculus leads to correct results because of compensating
errors. Maclaurin and Lagrange accepted this criticism and made efforts to
construct a logical justification for the methods of the differential calculus
unsuccessfully. Cauchy is also unsuccessful, but approaches the problem by
examining the concept of limit. Cauchy defines "limit" as: "When the values
successively assigned to the same variable indefinitely approach a fixed value,
so as to end by differing from it as little as desired, this fixed value is
called the limit of all the others.". (In this work?)
Paris, France  
179 YBN
[1821 AD]
2907) (Sir) Charles Wheatstone (WETSTON) (CE 1802-1875), exhibits the
"enchanted lyre".

This acoustical trick features a lyre suspended by a thin steel wire from the
soundboard of pianos and other instruments in the room above, and which appears
to play 'of itself' by sound conduction and sympathetic resonance of its
strings.

London, England (presumably)  
179 YBN
[1821 AD]
2909) (Sir) Charles Wheatstone (WETSTON) (CE 1802-1875), builds the human
speech device describe by Wolfgang von Kempelen (CE 1734-1804) in 1791.

(This shows clearly that people were looking at reproducing human speech, which
ultimately evolves into the telephone, reproducing sound in the neurons of
brains directly using lasers, and robots that talk by shaping air.)

London, England (presumably)  
178 YBN
[03/??/1822 AD]
3535)
London, England (presumably)  
178 YBN
[06/14/1822 AD]
2757)
Cambridge, England (presumably)  
178 YBN
[07/??/1822 AD]
2354)
Chalon-sur-Saône, France  
178 YBN
[09/01/1822 AD]
1251)
France  
178 YBN
[11/??/1822 AD]
5986) Franz Peter Schubert (CE 1797-1828), Austrian composer, composes his
"Symphony in B Minor" ("Unfinished").

Schubert bridges the transition from Classical and Romantic music, and is noted
for the melody and harmony in his songs (lieder) and chamber music.

Vienna, Austria (presumably)  
178 YBN
[1822 AD]
1246)
Philadelphia, Pennsylvania  
178 YBN
[1822 AD]
2210)
Paris, France (presumably)  
178 YBN
[1822 AD]
2381)
Paris, France  
178 YBN
[1822 AD]
2530) Magendie proves this through the use of young dogs.
Paris, France (presumably)  
178 YBN
[1822 AD]
2592) Jean Victor Poncelet (PoNSlA) (CE 1788-1867), French mathematician,
publishes "Traité des propriétés projectives des figures" (1822, "Treatise
on the Projective Properties of Figures"), a book on projective geometry.

Poncelet is considered one of the founders of modern projective geometry.
In 1812 As a
lieutenant of engineers, Poncelet takes takes part in Napoleon's Russian
campaign, in which Poncelet is abandoned as dead at Krasnoy and then imprisoned
at Saratov, returning to France in 1814.

From 1815 to 1825 Poncelet does military engineering at Metz.
From 1825 to 1835
Ponmcelet is a professor of mechanics at the École d'Application at Metz.
From 1838
to 1848 Poncelet is a professor at the Faculty of Sciences in Paris.
From 1848 to 1850
Poncelet is commandant of the École Polytechnique, with the rank of general.
Metz, France  
178 YBN
[1822 AD]
2601) Potassium ferrocyanide has a formula of K4Fe(CN)6·3H2O. Potassium
ferrocyanide forms yellow crystals with saline taste; soluble in water,
insoluble in alcohol; loses water at 60°C; used in medicine, dry colors,
explosives, and as an analytical reagent. Potassium ferrocyanide is also known
as yellow prussiate of potash.

Although many salts of cyanide are highly toxic, ferro- and ferricyanides are
less toxic because they tend not to release free cyanide.
Heidelberg, Germany  
178 YBN
[1822 AD]
2621) Mantell is a British physician, geologist, and paleontologist.
Mantell
studied the paleontology of the Mesozoic Era (about 245,000,000 to 66,400,000
years ago), particularly in Sussex, a region he made famous in the history of
geological discovery.
Mantell's most remarkable discoveries are made in the
Wealden formations. Mantell demonstrates the fresh-water origin of the strata,
and from them brings to light and describes the remarkable Dinosaurian reptiles
known as Iguanodon, Hylaeosaurus, Pelorosaurus and Regnosaurus.

For these researches Mantell is awarded the Wollaston medal by the Geological
Society and a Royal medal by the Royal Society.

Among other contributions is Mantell's description of the Triassic reptile
Telerpeton elginense.

Dr Mantell authors "Illustrations of the Geology of Sussex" (1827); "Geology of
the South-east of England" (1833); "The Wonders of Geology", 2 vols. (1838; ed.
7,1857); "Geological Excursions round the Isle of Wight, and along the Adjacent
Coast of Dorsetshire" (1847;(1847; ed. 3, 1854); "Petrifactions and their
Teachings" (1851); and "The Medals of Creation" (2 vols., 1854).

According to Asimov Mantell's wife had originally found the tooth and some
bones in a pile of stones by the road.
Sussex, England (presumably)  
178 YBN
[1822 AD]
2742) Charles Babbage (CE 1792-1871), English mathematician, writes in a
letter to Sir H. Davy on the application of machinery to the calculation and
printing of mathematical tables, Babbage discusses the principles of a
calculating engine.

Cambridge, England (presumably)  
178 YBN
[1822 AD]
2785)
Paris, France (presumably)  
178 YBN
[1822 AD]
3467)
Edinburgh, Scotland (presumably)  
177 YBN
[03/06/1823 AD]
3534)
(Royal Institution) London, England  
177 YBN
[03/13/1823 AD]
2699)
(Royal Institution in) London, England  
177 YBN
[04/1/1823 AD]
2709)
(Royal Institution in) London, England  
177 YBN
[06/14/1823 AD]
3297)
Benedictbeuern (near Munich), Germany (presumably)  
177 YBN
[1823 AD]
2335)
Bremen, Germany[1 (presumably)  
177 YBN
[1823 AD]
2506) Döbereiner uses this phenomenon to invent an automatic lighter called
the Döbereiner lamp. In this lamp a jet of hydrogen catches fire from contact
with platinum powder. (A spark from a flint can ignite gas, so I question the
value of such an invention. I don't understand why there were never any
hydrogen gas lamps or lighters. Igniting hydrogen is easy to do with a spark
from a high voltage or from flint. Perhaps hydrocarbons are less expensive to
obtain.)

The decomposition of potassium chlorate using manganese dioxide is a favorite
demonstration of oxygen production in elementary chemistry courses.

Furfural is from the Latin for "bran", has chemical formula C4H3OCHO, is a
viscous, colorless liquid that has a pleasant aromatic odor; upon exposure to
air furfural turns dark brown or black. Furfural boils at about 160�C.
Furfural is commonly used as a solvent; furfural is soluble in ethanol and
ether and somewhat soluble in water. Furfural is prepared commercially by
dehydration of pentose sugars obtained from cornstalks and corncobs, husks of
oat and peanut, and other waste products.
Döbereiner is a coachman's son an so (does
not receive) formal schooling, but is apprenticed to an apothecary, reads
widely, and attends science lectures.
Döbereiner attends the University of Jena.
In 1810,
Döbereiner becomes an assistant professor at the University of Jena.
Jena, Germany (presumably)  
177 YBN
[1823 AD]
2566)
Paris, France (presumably)  
177 YBN
[1823 AD]
2743) Charles Babbage (CE 1792-1871), English mathematician, gets government
(funding) for the design of a projected machine with a 20-decimal capacity.

Charles Babbage converts one of the rooms in his home to a workshop and hires
Joseph Clement to oversee construction of the engine. Every part has to be
formed by hand using custom machine tools, many of which Babbage himself
designs. Babbage takes extensive tours of industry to better understand
manufacturing processes.

With the government grants Babbage begins work on the "Difference Engine", but
decides later that scrapping the difference engine for a new design, the
"Analytical Engine" would be easier.

Cambridge, England (presumably)  
177 YBN
[1823 AD]
2769)
(University of Berlin) Berlin, Germany  
177 YBN
[1823 AD]
2917)
Temesvár, Romania (presumably)  
177 YBN
[1823 AD]
3383)
London, England  
177 YBN
[1823 AD]
3464)
London, England (presumably)  
177 YBN
[1823 AD]
3684)
London, England (presumably)  
176 YBN
[12/09/1824 AD]
4022) Roget is instrumental in founding the University of London (1828).

Roget is best known for his Thesaurus of English Words and Phrases (1852), a
comprehensive classification of synonyms or verbal equivalents which he
assembles during his retirement.
(Royal Institution) London, England (presumably)  
176 YBN
[1824 AD]
2494) Pure silicon is a hard, dark gray solid with a metallic luster and with a
crystalline structure the same as that of the diamond form of carbon, to which
silicon shows many chemical and physical similarities. A brown, powdery form of
silicon has been described that also has a microcrystalline structure.

Silicon has atomic number 14; atomic weight 28.086; melting point 1,410°C;
boiling point 2,355°C; relative density 2.33; valence 4.

Silicon is the element directly below carbon and above germanium in Group 14 of
the periodic table. Silicon is more metallic in its properties than carbon.
Silicon has two allotropic forms, a brown amorphous form, and a dark
crystalline form.

Silicon is the most abundant electropositive (having a positive electric
charge) element in the Earth's crust.

Silicon is the second most abundant element of the earth's crust; it makes up
about 28% of the crust by weight. Oxygen, most abundant, makes up about 47%.
Aluminum, third in abundance, makes up about 8%.

Silicon does not occur uncombined in nature; but is found in practically all
rocks as well as in sand, clays, and soils, combined either with oxygen as
silica (SiO2, silicon dioxide) or with oxygen and other elements (e.g.,
aluminum, magnesium, calcium, sodium, potassium, or iron) as silicates.

Silicon is prepared commercially by reducing (removing the oxygen from) the
oxide by its reaction with coke in electric furnaces. On a small scale, silicon
can be obtained from the oxide by reduction with aluminum.

A purified silicon is used in the preparation of silicones. Silicon of very
high purity is prepared by thermal decomposition of silanes; it is used in
transistors and other semiconductor devices. Silica is widely used in the
production of glass. Silicates in the form of clay are used in pottery, brick,
tile, and other ceramics. Silicon is found in many plants and animals; it is a
major component of the test (cell wall) of diatoms.

Photovoltaic cells for direct conversion of solar energy to electricity use
wafers sliced from single crystals of electronic-grade silicon. (So like
selenium, does silicon become more conductive with light, and also generate
current when light collides with silicon?)

Silicon dioxide is used as the raw material for making elementary silicon and
for silicon carbide. Sizable crystals of silicon are used for piezoelectric
crystals.

Silicon is commercially prepared by the reaction of high-purity silica with
wood, charcoal, and coal, in an electric arc furnace using carbon electrodes.
(Just any kind of wood, that seems kind of primitive. Silicon is not obtained
more cheaply through electrolysis? Describe the arc furnace.) At temperatures
over 1900 °C, the carbon reduces the silica to silicon according to the
chemical equation:

SiO2 + C → Si + CO2.

SiO2 + 2C → Si + 2CO.

Liquid silicon collects in the bottom of the furnace, and is then drained and
cooled. The silicon produced via this process is called metallurgical grade
silicon and is at least 98% pure.

The use of silicon in semiconductor devices demands a much greater purity than
afforded by metallurgical grade silicon. Historically, a number of methods have
been used to produce high-purity silicon.
Stokholm, Sweden (presumably)  
176 YBN
[1824 AD]
2501)
Stokholm, Sweden (presumably)  
176 YBN
[1824 AD]
2545)
London, England (presumably)  
176 YBN
[1824 AD]
2560)
Paris, France (presumably)  
176 YBN
[1824 AD]
2567) Michel Eugéne Chevreul (seVRuL) (CE 1786-1889) publishes
"Considérations générales sur l'analyse organique" (1824, Paris), a general
treatise on organic chemistry.
(Organic chemistry is any chemistry from a living object,
but is now taken to mean anything that has carbon. Still the distinction of
"organic" is misleading since there is no difference between the chemistry of
living things and nonliving things. However, sometimes knowing that some
molecule is commonly found in a living object or originates from a living
object is useful.)

Paris, France  
176 YBN
[1824 AD]
2729) This catalog is compiled between 1821 and 1823 and published in the
"Philosophical Transactions" in 1824.
For this catalog Herschel and South are awarded
the Gold Medal of the Royal Astronomical Society and the Lalande Prize in 1825
from the Paris Academy of Sciences.
London, England (presumably)  
176 YBN
[1824 AD]
2797) Eventually Carnot's views are incorporated by the thermodynamic theory as
developed by Rudolf Clausius in Germany (1850) and William Thomson (later Lord
Kelvin) in Britain (1851).

Carnot accepts the caloric heat theory of Lavoisier.
In 1814, Carnot graduates from the
École Polytechnique.
Sadi remains an army officer for most of his life.
In 1832, Carnot dies, at
age 36, in a cholera epidemic in Paris.
Paris, France  
176 YBN
[1824 AD]
2912) Integral equations are classified according to three different
dichotomies:
Limits of integration
both fixed: Fredholm equation
one variable: Volterra equation
Placement of
unknown function
only inside integral: first kind
both inside and outside integral:
second kind
Nature of known function f
identically zero: homogeneous
not identically zero:
inhomogeneous
Abel dies of Tuberculosis at age 26.
(University of Kristiania (Oslo) )Oslo, Norway (presumably)  
176 YBN
[1824 AD]
3390)
?, England  
176 YBN
[1824 AD]
5980)
Vienna, Austria  
175 YBN
[03/17/1825 AD]
4838)
London, England (presumably)  
175 YBN
[04/14/1825 AD]
3533)
London, England (presumably)  
175 YBN
[07/??/1825 AD]
2461) In 1815, Bretonneau gets his M.D. degree in Paris.
In 1816, Bretonneau is the
chief physician of the hospital at Tours.
Tours, France (presumably)  
175 YBN
[09/27/1825 AD]
2516) In 1813 George Stephenson visited a neighboring colliery (a coal mine and
connected buildings) to examine a "steam boiler on wheels" constructed by John
Blenkinsop to haul coal out of the mines. Blenkinsop mistakenly believed that
the train could not gain traction on smooth wooden rails, and so used a ratchet
wheel running on a cogged third rail, an arrangement that creates frequent
breakdowns.

In 1821 Stephenson heard of a project for a railroad, employing draft horses,
to be built from Stockton to Darlington to facilitate exploitation of a rich
vein of coal (in Stockton?). At Darlington Stephenson interviews the promoter,
Edward Pease, and so impresses Pease that Pease commissions Stephenson to build
a steam locomotive for the line.
Darlington (and Stockdon), England  
175 YBN
[1825 AD]
1243) The "runnelling shield" is first used in the building of the Thames
tunnel.
England  
175 YBN
[1825 AD]
2300)
Paris, France(presumably)  
175 YBN
[1825 AD]
2413)
London, England (presumably)  
175 YBN
[1825 AD]
2456)
Copenhagen, Denmark (presumably)  
175 YBN
[1825 AD]
2526) Sturgeon's father is a shoemaker.
1802-1820 Sturgeon is in the army.
In 1824 Sturgeon
becomes lecturer in science at the East India Company's Royal Military College
at Addiscombe in Surrey.
Surrey, England (presumably)  
175 YBN
[1825 AD]
2568)
Paris, France  
175 YBN
[1825 AD]
2576) Jan (also Johannes) Evangelista Purkinje (PORKiNYA or PURKiNYA) (CE
1787-1869), identifies the germinal vesicle, or nucleus of the unripe ovum,
that now bears his name (1825). (more info)

(Breslau, Prussia now:)Wroclaw, Poland  
175 YBN
[1825 AD]
2700) Benzene is a colorless, flammable, liquid aromatic hydrocarbon, C6H6,
derived from petroleum and used in or to manufacture a wide variety of chemical
products, including DDT, detergents, insecticides, and motor fuels.

Benzene is the chemical that leads to understanding all the aromatics (a
molecule that produces a smell and contains benzene).
(Royal Institution in) London, England  
175 YBN
[1825 AD]
2788) (Surprisingly,) Ehrenberg does not accept the theory of the cell or of
evolution.

Ehrenberg publishes more than 300 scientific papers and books in his lifetime.
Berlin, Germany  
175 YBN
[1825 AD]
2886) Müller, is a shoemaker's son from Koblenz (a cobbler from Koblenz?) in
Germany.
In 1822, Müller graduates in medicine from the University of Bonn.
In 1824 Müller
is granted a lectureship in physiology and comparative anatomy at the
University of Bonn.
In 1833 Müller is called to Berlin to succeed Rudolphi,
where Müller has access to the vast Berlin anatomical collection.
(In Berlin), Müller's
students include the renowned physiologist and physicist Hermann Helmholtz and
the cellular pathologist Rudolf Virchow.
(University of Bonn) Bonn, Germany  
174 YBN
[03/??/1826 AD]
3454) Talbot obtains a monochromatic yellow light burning a cotton wick soaked
in salt water, dried and then lit in an alcohol lamp.

Talbot publishes these findings in "Some experiments on Coloured Flames.", in
the Edinburgh Journal of Science.

Talbot writes "...I would further suggest, that whenever the prism shows a
homogeneous ray of any colour to exist in a flame, this ray indicates the
formation or the presence of a definite chemical compound...." and concludes
"...The bright line in the yellow is caused, without doubt, by the combustion
of the sulphur, and the others may be attributed to the antimony, strontia, &c.
which enter into this composition. For instance, the orange ray may be the
effect of the strontia, since Mr Herschel found in the flame of muriate of
strontia a ray of that colour. If this opinion should be correct and applicable
to the other definite rays, a glance at the prismatic spectrum of a flame may
show it to contain substances, which it would otherwise require a laborious
chemical analysis to detect.".

Talbot's paper in full reads:
"GREAT progress has recently been made in investigating
the properties of light, and yet many of them are still unexamined, or
imperfectly explained. Among these are the colours of flames which not only
appear very various to common observation, but are shown, by the assistance of
a prism, to be entirely different in nature one from another; some being
homogeneous, or only containing one kind of light; others consisting of an
infinite variety of all possible shades of colour.
1. It was discovered by Dr
Brewster, that the flame of alcohol, diluted with water, consists chiefly of
homogeneous yellow rays. On this principle, he proposed the construction of a
monochromatic lamp, and pointed out its advantages for observations with the
microscope. This must be considered a very valuable discovery. The light of
such a lamp, however, is weak, unless the alcohol flame is very large. I have,
therefore, made several attempts to obtain a brighter light, and I think the
following is the most convenient method. A cotton wick is soaked in a solution
of salt, and when dried, placed in a spirit lamp. It gives an abundance of
yellow light for a long time. A lamp with ten of these wicks gave a light
little inferior to a wax candle; its effect upon all surrounding objects was
very remarkable, especially upon such as were red, which became of different
shades of brown and dull yellow. A scarlet poppy was changed to yellow, and the
beautiful red flower of the Lobelia fulgens appeared entirely black. The wicks
were arranged in a line, in order to unite their effect for a microscope. A
common blue glass has the property of absorbing the yellow light of this lamp,
however brilliant, while it transmits the feeble violet rays. If these are also
stopped by a pale yellow glass, the lamp becomes absolutely invisible, though a
candle is seen distinctly through the same glasses. But the most remarkable
quality of this light is its homogeneity, which is perfect as far as I have
been able to ascertain. I speak of the yellow rays, which form the mass of the
light, and quite overpower the feeble effect of the blue and green. The origin
of this homogeneous light appears to me difficult to explain. I have found that
the same effect takes place whether the wick of the lamp is steeped in the
muriate, sulphate, or carbonate of soda, while the nitrate, chlorate, sulphate,
and carbonate of potash, agree in giving a blueish white tinge to the flame.
Hence, the yellow rays may indicate the presence of soda but they,
nevertheless, frequently appear where no soda can be supposed to be present.
2. Mr
Herschel discovered that sulphur, when burning intensely, gives a homogeneous
yellow light. To examine it, I inflame a mixture of sulphur and nitre behind a
screen, having a narrow vertical slit through which the flame could be seen.
This opening, examined with a prism, gave a spectrum in which there was a very
bright yellow line, indicating the combustion of the sulphur. I thought it a
point of considerable interest to determine, whether this yellow ray was
identical with that afforded by the flame of alcohol containing salt, and with
that view, I placed such a flame behind the other, their light passing through
the same opening; so that, if the rays were of a different nature, two yellow
lines should be seen in the spectrum; but if identical, then only one. I found,
upon trial, that the rays coincided; and I obtained a further confirmation of
this, by inflaming the nitre and sulphur, mixed up with a quantity of salt; the
effect of which was, not to produce a second yellow line in the spectrum, but
to increase greatly the brilliancy of the original one. The result of this
experiment points out a very singular optical analogy between soda and sulphur,
bodies hitherto supposed by chemists to have nothing in common.
3. There are other
means of procuring the same light which I shall briefly mention If a clean
piece of platina foil is held in the blue or lower part of a gas flame, it
produces no change in the flame, but if the platina has been touched by the
hand, it gives off a yellow light which lasts a minute or more. If it has been
slightly rubbed with soap, the light is much more abundant, while wax, on the
contrary, produces none. Salt sprinkled on the platina, gives yellow light
while it decrepitates, and the effect may be renewed at pleasure by wetting it.
This circumstance led me to suppose that the yellow light was owing to the
water of crystallization, rather than to the soda, but then it is not easy to
explain why the salts of potash, &c. should not produce it likewise. Wood,
ivory, paper, &c. when placed in the gas flame, give off (besides their bright
flame) more or less of this yellow light which I have always found the same in
its characters. The only principle which these various bodies have in common
with the salts of soda, is water; yet I think that the formation or presence of
water cannot be the origin of this yellow light, because ignited sulphur
produces the very same, a substance with which water is supposed to have no
analogy. {It may be worth remark, though probably accidental, that the specific
gravity of sulphur is 1.99, or almost exactly twice that of water.} It is also
remarkable that alcohol burnt in an open vessel, or in a lamp with a metallic
wick, gives but little of the yellow light; while, if the wick be of cotton, it
gives a considerable quantity, and that for an unlimited time. (I have found
other instances of a change of colour in flames owing to the mere presence of a
substance which suffers no diminution in consequence. Thus, a particle of
muriate of lime on the wick of a spirit lamp will produce a quantity of red and
green rays for a whole evening, without being itself sensibly diminished.) The
bright flame of a candle is surrounded by the same homogeneous yellow light,
which becomes visible when the flame itself is screened. The following
experiment shows its nature more evidently: If some oil is dropped on the wick
of a spirit lamp, the flame assumes the brilliancy of a candle surrounded by an
exterior yellow flame. This appearance only lasts until the oil is consumed.
4. The
flame of sulphur and nitre contains a red ray, which appears to me of a
remarkable nature. While examining the yellow line in the spectrum of this
flame, I perceived another line situated beyond the red end of the spectrum,
from the termination of which it is separated by a wide interval of darkness.
In colour it nevertheless differs but little from the rays which usually
terminate the spectrum. It arises, I believe, from the combustion of the nitre,
as the yellow ray does from that of the sulphur, for I have since observed it
in the flame of a spirit lamp, whose wick had been soaked in nitre or chlorate
of potash. It appeared to me that this ray was so distant from the rest, that
it might be less refrangible than any in solar light; and I have been since
informed by Mr Herschel, that he had already observed it in a similar
experiment, and was impressed with the same idea.
With the hope of establishing
this, I admitted candle light, and that of the nitre lamp which I have just
mentioned, through the same aperture, and noticed how far this isolated red ray
appeared beyond the spectrum of the candle. I then compared, in the same way
the light of the candle with that of the sun, and I found that the great
intensity of the solar light lengthened the red end of the spectrum about as
far, so that I was obliged to leave the question undecided, as the faintness of
the lamp prevented my comparing it directly with the sun. This red ray appears
to possess a definite refrangibility, and to be characteristic of the salts of
potash, as the yellow ray is of the salts of soda, although, from its feeble
illuminating power, it is only to be detected with a prism. If this should be
admitted, I would further suggest, that whenever the prism shows a homogeneous
ray of any colour to exist in a flame, this ray indicates the formation or the
presence of a definite chemical compound. An excellent prism is, however,
requisite to determine the perfect homogeneity of a ray.
5. Phosphorus inflamed
with nitre gives a very brilliant spectrum, in which no colour appears to be
predominant or deficient. It therefore resembles the spectra of ignited lime,
platina, and other solid bodies, and differs totally from the solar spectrum in
which there are now known to be innumerable interruptions of light. And it is
worthy of remark, that no light has been hitherto discovered at all resembling
that of the sun, (when analyzed with a prism) except the light of the other
celestial bodies.
6. The red fire of the theatres examined in the same way, gave a
most beautiful spectrum with many light lines or maxima of light. In the red,
these lines were numerous and crowded, with dark spaces between, besides an
exterior ray greatly separated from the rest, and, probably the effect of the
nitre in the composition. In the orange was one bright line, one in the yellow,
three in the green, a very bright one in the blue, and several that were
fainter. The bright line in the yellow is caused, without doubt, by the
combustion of the sulphur, and the others may be attributed to the antimony,
strontia, &c. which enter into this composition. For instance, the orange ray
may be the effect of the strontia, since Mr Herschel found in the flame of
muriate of strontia a ray of that colour. {Edinburgh Transactions, vol ix, p.
456.} If this opinion should be correct and applicable to the other definite
rays, a glance at the prismatic spectrum of a flame may show it to contain
substances, which it would otherwise require a laborious chemical analysis to
detect.".
London, England  
174 YBN
[07/05/1826 AD]
3440)
(Bureau des Longitudes) Paris, France (presumably)  
174 YBN
[1826 AD]
2355) (Text messages sent electronically over metal wires will be called
"telegrams", and possibly thought images, visual memories of light captured in
eyes and stored in neurons, may be called "thoughtgrams" or "thoughtgraphs" or
"psychograms" as Andre Maurois refers to them in his book "The Thought Reading
Machine" or simply "thought image", "thought photo", "eye image", or "eye
movie")
Chalon-sur-Saône, France  
174 YBN
[1826 AD]
2422)
Berlin?, Germany  
174 YBN
[1826 AD]
2462)
Tours, France (presumably)  
174 YBN
[1826 AD]
2524)
  
174 YBN
[1826 AD]
2541) Friedrich Wilhelm Bessel (CE 1784-1846), makes a correction to the
(length of the?) seconds pendulum, the length of which is precisely calculated
so that it requires exactly one second for a swing.

Königsberg, (Prussia now:) Germany  
174 YBN
[1826 AD]
2744) Charles Babbage (CE 1792-1871), English mathematician, publishes "A
Comparative View of the Various Institutions for the Assurance of Lives" (1826,
London: J. Mawman). (In which Babbage) compiles the first reliable actuarial
tables (tables that reflect the probability of a person living to a certain
age).

Cambridge, England (presumably)  
174 YBN
[1826 AD]
2847) Among Dumas' works are "Traité de chimie appliquée aux arts" (8 vol.,
1828-45).
Dumas is the one of the first people in France to realize the importance of
experimental laboratory teaching.
Student of Dumas include many French chemists,
including Auguste Laurent, Charles-Adolphe Wurtz, and Louis Pasteur.
During Napoleon
III, Dumas serves as minister of agriculture, senator, master of the French
mint, and the equivalent of mayor of Paris, until the fall of Napoleon.
(Ecole Polytechnique) Paris, France (presumably)  
174 YBN
[1826 AD]
2887) This analysis of nerves, in particular of the eye will be one focus of a
student of Müller's, Helmholz, whose student Michael Pupin will be the first
to see thought, that is external images seen by the brain in addition to
internal images produced by the brain.
(University of Bonn) Bonn, Germany  
174 YBN
[1826 AD]
2888) Johannes Peter Müller (MYUlR) (CE 1801-1858), German physiologist,
publishes the voluminous "ur vergleichenden Physiologie des Gesichtssinnes ..."
(1826, "Comparative Physiology of the Visual Sense ...").

This work contains a wealth of new material on human and animal vision,
including the results of analyses of human expressions and research on the
compound eyes of insects and crustaceans.

In this year Müller also publishes "On Imaginary Apparitions" in which Müller
theorizes that the eye as a sensory system not only reacts to external optical
stimuli but can also be excited by internal stimuli generated by the
imagination. Therefore, people who report seeing religious visions, ghosts, or
phantoms may actually be experiencing optical sensations and believe them to be
of external origin, even though the images are not from external stimulus.
(Interesting as relates to the modern phenomenon of images beamed directly onto
the neurons of people's brains without them knowing of their external origin.)

(University of Bonn) Bonn, Germany  
174 YBN
[1826 AD]
2915) Bromine has symbol Br, atomic number 35, atomic weight 79.909, usually
exists as Br2, a dark-red, low-boiling but high-density liquid of intensely
irritating odor, with melting point 7.2°C; boiling point 58.78°C; valence 1,
3, 5, 7.

Bromine is the only nonmetallic element that is liquid at normal temperature
and pressure. Bromine is very reactive chemically; one of the halogen group of
elements, it has properties intermediate between those of chlorine and iodine.
(Mercury appears to me to be the only other element that is a liquid at room
temperature. Perhaps some elements melt at warm temperatures.)

Bromine is almost instantaneously injurious to the skin, and it is difficult to
remove quickly enough to prevent a painful burn that heals slowly. Bromine
vapor is extremely toxic, but its odor gives good warning.

Bromine has many uses including as petroleum additives (ethylene dibromide), in
photographic emulsions (silver bromide), as sedatives, and in flour (potassium
bromate).

Bromine is soluble in water to some extent; the aqueous solution, called
bromine water, acts as an oxidizing agent. Bromine is also soluble in alcohol,
ether, and carbon disulfide. Bromine is less active chemically than chlorine or
fluorine but is more active than iodine. Bromine forms compounds similar to
those of the other halogens. Oxides of bromine are unstable, but two acids,
hypobromous acid, HBrO, and bromic acid, HBrO3, are known. Hydrobromic acid is
the aqueous solution of hydrogen bromide, HBr. Bromine does not occur
uncombined in nature but is found in combination with other elements, notably
sodium, potassium, magnesium, and silver. In compounds bromine is present in
seawater, in mineral springs, and in common salt deposits.
Balard has Berthelot first as
pupil, then as assistant and finally as colleague.
(Montpellier École de Pharmacie) Montpellier, France  
174 YBN
[1826 AD]
3384)
London, England  
173 YBN
[04/07/1827 AD]
6242)
England  
173 YBN
[05/01/1827 AD]
2606) Ohm is the son of a self-taught master mechanic interested in science.
Oh
m draws his own wires.
In 1817, Ohm becomes professor of mathematics at the Jesuits'
College at Cologne.
From 1826 to 1833 Ohm teaches at the Military Academy in
Berlin.
In 1833, Ohm accepts a position at the Polytechnic School of Nürnberg.
In
1841, Ohm is awarded the Copley Medal of the Royal Society of London.
In 1849,
Ohm is appointed a professor at the University of Munich.
Berlin, Germany (written in Cologne?)  
173 YBN
[12/08/1827 AD]
2356)
Chalon-sur-Saône, France  
173 YBN
[1827 AD]
2415)
London, England (presumably)  
173 YBN
[1827 AD]
2425)
Paris, France  
173 YBN
[1827 AD]
2450)
Göttingen, Germany (presumably)  
173 YBN
[1827 AD]
2472) Joseph Louis Gay-Lussac (GAlYUSoK) (CE 1778-1850) invents the "Gay-Lussac
tower" in which oxides of nitrogen arising from the preparation of sulfuric
acid by the lead-chamber process, which formerly escaped into the atmosphere,
are absorbed by passing them up a chimney packed with coke, over which
concentrated sulfuric acid is trickled. This tower and its modifications are
used in many chemically-based industries today.

Paris, France (presumably)  
173 YBN
[1827 AD]
2546) This (naming system) is quickly adopted by other biochemists.
London, England (presumably)  
173 YBN
[1827 AD]
2552) John James Audubon (oDUBoN) (CE 1785-1851), starts publishing "Birds of
America" (4 vol, 1827-38) which when done 11 years later will contain 435
hand-colored plates.

William MacGillivray helped write the accompanying text, "Ornithological
Biography", (5 vol, octavo, 1831-39), and "A Synopsis of the Birds of North
America" (1 vol, 1839), which serves as an index.
The first hint that Audubon's
skills as an artist and naturalist could be combined to make money come in 1810
when Alexander Wilson passes through Louisville, Louisiana, where Audubon is
operating a general store. Wilson is looking for subscribers to his lavishly
illustrated American Ornithology (9 vols; 1808-14).

In 1824 Audubon goes to Philadelphia to find a publisher, but encounters the
opposition of friends of Alexander Wilson, the other pioneer American
ornithologist, with whom Audubon has a bitter rivalry with.

(When published) sets of five plates are sold to subscribers for 2 guineas to
finance the next set. In this way 200 full sets of Birds of America (1827-38)
are published in Britain in 87 parts with 435 plates. (In modern times), full
sets are rarely available for sale and when auctioned are raise at least a
million dollars.
London, England  
173 YBN
[1827 AD]
2553) John James Audubon (oDUBoN) (CE 1785-1851), publishes "Viviparous
Quadrupeds of North America" (2 vols., 1842-1845) and the accompanying text (3
vol., 1846-53) is completed with the aid of Audubon's sons and the naturalist
John Bachman.
Audubon himself completes only about half the drawings in this last work,
Audubon's son contributed the remainder.
London, England  
173 YBN
[1827 AD]
2614) Bright's disease, also called Glomerulonephritis, or Nephritis, is an
inflammation of the structures in the kidney that produce urine: the glomeruli
and the nephrons.

The kidney is an organ found in some invertebrates and all vertebrates that
maintains water balance and expels metabolic wastes.

Bright's subsequent papers on renal (located or relating to the location of the
kidneys) disease are published in a second volume of reports (1831) and in the
first volume of Guy's Hospital Reports of 1836.
London, England  
173 YBN
[1827 AD]
2724) Baer contributes to the Academy at St. Petersburg by establishing an
extensive skull collection.
Baer is responsible for the founding of the Russian
Geographical Society and the Russian Entomological Society, of which Baer is
the first president.

Baer rejects Darwinism. (Surprising for something as simple and logical for
somebody in biology. But then religion is a powerful force against the theory
of evolution.)
Although Baer believes that some very similar animals, such as goats and
antelopes, might be related, Baer is vehemently against the concept expressed
in Darwin's "Origin of Species" that all living creatures might have evolved
from one or a few common ancestors.
(Königsberg now) Kaliningrad, Russia  
173 YBN
[1827 AD]
2745) Charles Babbage (CE 1792-1871), English mathematician, publishes "Tables
of Logarithms" (1827).

Cambridge, England (presumably)  
173 YBN
[1827 AD]
2770) Selenic acid is prepared by oxidation of selenium dioxide with hydrogen
peroxide:
SeO2 + H2O2 → H2SeO4
To obtain the anhydrous acid as a crystalline solid,
the resulting solution is evaporated at temperatures<140 °C in vacuum.
(University of Berlin) Berlin, Germany  
173 YBN
[1827 AD]
2774) Babinet improves the valves of the air-pump, attaining a very high
vacuum.
Babinet constructs a hygrometer and a goniometer (an optical instrument for
measuring crystal angles, as between crystal faces (a compass?)).
Babinet invents the
"Babinet compensator", a double quartz wedge used in the study of elliptically
polarized light. (more info and image)
Babinet studies in Paris at the Ecole
Polytechnique.
In 1820 Babinet is a professor at the Collège Louis le Grand in Paris.
Paris, France  
173 YBN
[1827 AD]
2856) Wöhler studies with the famous Swedish chemist Jöns Jacob Berzelius.
In the first
few years teaching at Göttingen, Wöhler (in parallel with Liebig at Giessen)
pioneers a new pattern of science education and scientific research. Instead of
the traditional lecturing and performing selected demonstrations for them,
Wöhler and Liebig require that all students fulfill a laboratory practice in
which they carry out laboratory manipulations themselves. This innovation is
rapidly adopted throughout Germany and then in other nations and is the basis
of modern laboratory-based university education today.
Wöhler's works on chemistry
are widely used as texts, and include "Outlines of Organic Chemistry" (1840,
tr. 1873).
(Berlin Gewerbeschule (trade school)) Berlin, Germany  
173 YBN
[1827 AD]
2892) (Airy supervises expeditions to (measure the parallax of Venus (relative
to the edge of the Sun?)) when Venus crosses the face of the sun, but the
mission fails because the atmosphere of Venus makes determining the time of
contact difficult.
Airy is the son of a poor farmer, who distinguishes himself
as Senior Wrangler at Cambridge, where Airy is elected fellow of Trinity
College (1824) and appointed professor (1826). (This is an example of how a
poor person through success in education can rise to a well paid employment.)
In 1835 Airy
is appointed Astronomer Royal (director of the Royal Greenwich Observatory),
and holds this post for 46 years.
In September 1845, John Adams comes to Airy, with
news of the position of a new planet, Airy unwisely ignores Adams, and delays
the discovery of planet Neptune.
Greenwich, England (presumably)  
173 YBN
[1827 AD]
2999) Hamilton writes "By a Ray, in this
Essay, is meant a line along which light is
propagated; and by a System of Rays is meant
an infinite number of such lines,
connected by any analytic law, or any common property.
Thus, for example, the rays which
proceed from a luminous point in a medium of uniform
density, compose one system of
rays; the same rays, after being reflected or refracted, compose
another system.
And when we represent a ray analytically by two equations between its three
coordinate
s, the coefficients of those equations will be connected by one or more
relations
depending on the nature of the system, so that they may be considered as
functions of one or
more arbitrary quantities. These arbitrary quantities, which
enter into the equations of the
ray, may be called its Elements of Position,
because they serve to particularise its situation
in the system to which it belongs. And
the number of these arbitrary quantities, or elements
of position, is what I shall take
for the basis of my classification of systems of rays; calling a
system with one
element of position a system of the First Class: a system with two elements
of position,
a system of the Second Class, and so on.". (More clearly explain "elements -
are they variables? dimensions?)

Hamilton writes "
(D) dp + dp' = 0.

This equation (D) is called the Principle of least Action, because it expresses
that if the
coordinates of the point of incidence were to receive any infinitely
small variations consistent
with the nature of the mirror, the bent path (dp + dp') would
have its variation nothing; and if
light be a material substance, moving with a
velocity unaltered by reflection, this bent path
dp + dp' measures what in mechanics
is called the Action, from the one assumed point to the
other. Laplace has deduced
the formula (D), together with analogous formulae for ordinary
and extraordinary
refraction, by supposing light to consist of particles of matter, moving
with certain
determined velocities, and subject only to forces which are insensible at
sensible
distances. The manner in which I have deduced it, is independent of any
hypothesis about
the nature or the velocity of light; but I shall continue to call
it, from analogy, the principle
of least action.".

Hamilton writes "The formula (D) expresses, that if we assume any two points,
one on each ray, (the incident and reflected ray) the
sum of the distances of these
two assumed points from the point of incidence, is equal to
the sum of their
distances from any infinitely near point upon the mirror.".


Hamilton concludes by writing: "The preceding pages contain the execution of
the first part of our plan; being an attempt
to establish general principles respecting
the systems of rays produced by the ordinary re-
flexion of light, at any mirror or
combination of mirrors, shaped and placed in any manner
whatsoever; and to shew that
the mathematical properties of such a system may all be de-
duced by analytic
methods from the form of ONE CHARACTERISTIC FUNCTION: as, in the
application of
analysis to geometry, the properties of a plane curve, or of a curve surface,
may all be
deduced by uniform methods from the form of the function which characterises
its
equation. It remains to extend these principles to other optical systems; to
shew that in every
such system, whether the rays be straight or curved, whether
ordinary or extraordinary, there
exists a Characteristic Function analogous to that
which we have already pointed out for the
case of the systems produced by the
ordinary reflexion of light; to simplify and generalise
the methods that we have given,
for calculating from the form of this function all the other
properties of the
system; to integrate various equations which present themselves in the de-
terminati
on of mirrors, lenses, and crystals satisfying assigned conditions; to
establish some
more general principles in the theory of Systems of Rays, and to
terminate with a brief review of our own results, and of the discoveries of
former writers."
Hamilton is a child prodigy, not only in mathematics, but in languages
too.
At age 17 Hamilton astonishes the royal astronomer in Ireland by communicating
an error found in Laplace's "Celestial Mechanics".
In 1823, Hamilton takes the entrance
examination for Trinity College and (scores highest) of 100 candidates.
(Trinity College, at Dunsink Observatory) Dublin, Ireland  
173 YBN
[1827 AD]
3391)
London, England  
173 YBN
[1827 AD]
3591) Dyar writes in 1848:
"I invented a plan of a telegraph, which should be
independent of day, or night, or weather, which should extend from town to
town, or city to city, without any intermediary agency, by means of an
insulated wire, suspended on poles, and through which I intended to send
strokes of electricity, in such a manner as that the diverse distances of time
separating the divers sparks should represent the different letters of the
alphabet, and stops between the words, &c. This absolute, or this relative,
difference of time between the several sparks I intended to take off from an
electric machine by a little mechanical contrivance, regulated by a pendulum;
while the sparks themselves were intended to be recorded upon a moving, or
revolving, sheet of moistened litmus paper, which by the formation of nitric
acid by the spark in its passage through the paper, would leave {show} a red
spot for each spark. These so-produced red spots, with their relative
interspaces, were, as I have said, taken as an equivalent for the letters of
the alphabet, &c, or for other signs intended to be transmitted, whereby a
correspondence could be kept up through one wire of any length, either in one
direction, or back and forwards, simultaneously or successively. In addition to
this use of electricity I considered that I had, if wanted, an auxiliary
resource in the power of sending impulses along the same wire, properly
suspended, somewhat like the action of a common bell-wire in a house.
Now you will
perceive that this plan is like that known as Morse's telegraph, with the
exception that his is inferior to mine, inasmuch as he and others now make use
of electro-magnetism, in place of the simple spark, which requires that they
should, in order to get dots, or marks, upon paper, make use of mechanical
motions, which require time; whereas my dots were produced by chemical action
of the spark itself, and would be, for that reason, transmitted and recorded
with any required velocity.
In order to carry out my invention I associated myself with
a Mr. Brown, of Providence, who gave me certain sums of money to become my
partner. We employed a Mr. Connel, of New York, to aid in getting the capital
wanted to carry the wires to Philadelphia. This we considered as accomplished;
but, before beginning on the long wire, it was decided that we should try some
miles of it on Long Island. Accordingly I obtained some fine card wire,
intending to run it several times around the Old Union Racecourse. We put up
this wire at different lengths, in curves and straight lines, by suspending it
{with glass insulators} from stake to stake, and tree to tree, until we
concluded that our experiments justified our undertaking to carry it from New
York to Philadelphia. At this moment our agent brought a suit, or summons,
against me for 20,000 dollars, for agencies and services, which I found was
done to extort a concession of a share of the whole project.
I appeared before Judge
Irving, who, on hearing my statement, dismissed the suit as groundless. A few
days after this, our patent agent (for, being no longer able to keep our
invention a secret, we had applied for a patent) came to Mr. Brown and myself
and stated that Mr. Connel had obtained a writ against us, under a charge of
conspiracy for carrying on secret communication from city to city, and advised
us to leave New York until he could settle the affair for us. As you may
suppose, this happening just after the notorious bank-conspiracy trials, we
were frightened beyond measure, and the same night slipped off to Providence.
There I remained some time, and did not return to New York for many months, and
then with much fear of a suit. This is the circumstance which put an end {to
our project}, killing effectually all desire to engage further on such a
dangerous enterprise. I think that, on my return to New York, I consulted
Charles Walker, who thought that, however groundless such a charge might be, it
might give me infinite trouble to stand a suit. From all this the very name of
electric telegraph has given me pain whenever I have heard it mentioned, until
I received your last letter, stimulating me to come out with my claims; and
even now I cannot overcome the painful association of ideas which the name
excites." (This story sounds somewhat unlikely, in particular knowing that
shasiastafb has been kept secret for so long. There is a hint of some kind of
pain being given - perhaps depending on how much Dyar chooses to makes public?
Kind of a bizarre law against "secret messages", perhaps similar to the equally
free info violating espionage laws.)

Beccaria had used an electric spark to decompose the sulphuret of mercury and
recovered the metal. (chronology)

(This shows that clearly by 1827, the technology existed to print images,
although possibly capturing an image might have to wait for selenium.)

(There must be millions of red dot images in the telegraph/telephone company
archives. Why have no people tried to access these and force them to be made
public?)

(The author of the 1884 book "A History of Electric Telegraphy, to the Year
1837" ends a paragraph on page 156 with "Cooke and Morse" which is "cam"era.)

(It is kind of curious that, which this kind of red-dot printer, that the
electro-mechanical system stays in use for so long, at least as far as the
public knows.)
New York City NY (presumably)  
173 YBN
[1827 AD]
4001)
London, England (presumably)  
172 YBN
[02/??/1828 AD]
2857) German chemist, Friedrich Wöhler (VOElR) (CE 1800-1882), is the first to
produce an "organic" (or biotic) compound {molecule} from an "inorganic" (or
abiotic) compound, the compound "urea", which forms crystals when ammonium
cyanate is heated.

Wöhler finds that urea has the same composition as ammonium cyanate, and
Berzelius will call these "isomers". (Isomers must be molecules made of the
same ratio of atoms but in different structure. What explains isomerism?)

Urea is the primary nitrogenous waste of the mammalian body, found in urine.
This is the first experiment to show the theory of vitalism wrong. The theory
of vitalism, first put forward by Stahl, is that organic molecules are
different from inorganic molecules and require a "vital force" to be created.
Berzelius had separates all chemicals (molecules) into organic and inorganic,
depending on if the are created in living tissue or not. Gmelin accepted this,
however Chevreul doubted this erroneous theory.
(In addition, Wöhler
reinforces the idea that life is made of molecules that are no different from
non-living matter in the rest of the universe, This supports the idea that life
was not created by a deity, is magical, or different from a natural process.)

Berzelius eventually concedes. Berzelius and others argue that Ammonium cyanate
is an organic compound. However, Berthelot 25 years later will remove all
doubt.

Wöhler also finds that urea has exactly the same composition as a different
substance, ammonium cyanate.
This discovery is equally important in the history of
isomerism as for vitalism, since, at the time, very few cases of two distinct
compounds having identical compositions are known. Two years after Wöhler's
synthesis of urea, Berzelius defines the concept and introduces the new word
"isomerism".
(Berlin Gewerbeschule (trade school)) Berlin, Germany  
172 YBN
[06/??/1828 AD]
2805) Henry is one of the first great American scientists after Benjamin
Franklin and also the first in America to experiment with electricity in an
important way after Franklin 75 years before.
Henry's life parallels Faraday's
life in many ways.
Henry is from a poor family.
Henry has little schooling, and is forced to
work when young.
At age 13 Henry is apprenticed to a watchmaker.
At age 16
Henry finds a book titled "Lectures on Experimental Philosophy" in a church he
enters through a broken floor board. This inspires him to go to school, and he
enters the Albany Academy. (It shows the possibility of a person simply being
exposed to ideas of science.)
Henry teaches at country schools and tutors on the side to
earn his tuition.
From 1826 to 1832 Henry teaches mathematics and science at
Albany Academy.
In 1832 as a result of his electromagnets, Henry gets hired as professor
of natural philosophy at the College of New Jersey (later Princeton
University).
When Henry comes to Princeton he had been promised at first a
salary of $1000 (a year), which is later raised to $1500 and a house. Henry
remarks, however, that sometimes he receives no more than $600 a year because
the university does not have the funds needed to pay him.
In 1846 Henry is elected
first secretary of the newly formed Smithsonian Institution. Henry makes the
Smithsonian a clearing house of scientific knowledge and encourages scientific
communications on a worldwide scale.
Henry is one of Lincoln's chief technical
advisers during the U.S. Civil War and recommends the building of ironclads
(iron ships).
Henry is one of the founders of the National Academy of Sciences
of the United States and its second president.

(Henry is evidence that people in the USA are catching up at this time in terms
of scientific skills with those in England and the rest of Europe. This
advancing of people in the USA in science will be clear when Pupin is the first
to see thought at Columbia, and of course, with the drain of all Europe's best
minds before and during World War II. {Part of the success of the US may be
that freethinking people flea to the USA for political and religious freedom.
For example, Pupin was an immigrant from Europe. Perhaps this mixing of
cultures, or the advanced view of religious freedom {including no religion}, is
what gives the USA a competitive advantage over other older more settled
nations.}. But this dominance of the USA fails with a resurgence of religion
and violence after World War II in particular with the rise of the murderers of
JFK and the ending of the Moon program. For example, people in the Asian
nations are the first to go public with a walking robot, and are the main
producers of cars, video devices, while the people in the USA and Europe trail
behind, stuck in fanatical religion, hostile to science, and sharing of
information. One exception is the recent rocket plane {star ships one and two,
the X prize, etc.} development in the USA.)

In 1893 the International Electrical Congress agrees to name the standard
electrical unit of inductive resistance the "henry" in honor of Joseph Henry.

The 1911 Encyclopedia Britannica describes Henry as the foremost of American
physicists, by general concession, and a man with a liberality of views, of
generous impulses, of great gentleness and courtesy of manner, combined with
equal firmness of purpose and energy of action.
Albany, NY, USA  
172 YBN
[1828 AD]
2383) (I disagree with the current view that polarization is a wave phenomenon.
I think that polarized light are beams of light particles that have no
horizontal or vertical component (relative to the plane of the polarizing
surface). Materials that polarize probably only allow light in one plane to be
transmitted, reflecting (or absorbing) the rest, so moving two objects at 90
degrees cancels out beams of light moving in any other direction than
i,j,k=(0,0,1). In any event, I think the phenomenon of polarization is a
particle phenomenon, and I view light beams as being beams of particles without
amplitude where frequency is defined by frequency of photons.)

Nicol lectures in natural philosophy at the University of Edinburgh where James
Clerk Maxwell is probably one of Nicol's pupils.
Edinburgh, Scotland (presumably)  
172 YBN
[1828 AD]
2725)
(Königsberg now) Kaliningrad, Russia (presumably)  
172 YBN
[1828 AD]
2859)
(Berlin Gewerbeschule (trade school)) Berlin, Germany  
172 YBN
[1828 AD]
6028)
Paris, France (presumably)  
172 YBN
[1828 AD]
6246)
Pannonhalma, Hungary (presumably)  
172 YBN
[1828 AD]
6256)
Pannonhalma, Hungary (presumably)  
171 YBN
[03/05/1829 AD]
3392) James Anderson transports 15 passengers in a steam road vehicle.

Epping Forest, England  
171 YBN
[03/27/1829 AD]
2844) In 1830, Zantedeschi performs experiments that show that prolonged
exposure to Sun light increases the strength of unpolished permanent magnets.

Here is a translation with many mistakes:
PS. I add in the form of an appendix to the
experience 1. and 2. Of Part 1. Another fact I observed at times in this
month, which is my duty to discuss, because it tends to connect and unite the
different electromagnetic facts that arise. I have taken an iron horse-shoe
magnet that weighs approximately a French pound, that can support a weight of
approximately 4 to 5 pounds, and around each pole I have closely wrapped the
thinnest wire of copper so that, placing the magnet at a distance of 15 to 16
Parisian feet, I can verify/test the other extremity of the wire. Now I take a
multiplier to two magnets, I have looped wire in the same way (that of the
copper surrounded by silk) attached to two well polished small thin copper
plates, in between two wooden rods, in order not to alter the temperature, join
the wires that I have said to be in communication with poles of the magnet, I
have seen that the magnetic needle turns from its natural position declining
towards the east {when} the above pole (of the coil of wire) enters the
magnetic action of the North Pole, and towards the West, if this (the coil)
enters below it, otherwise of that which passes with the ordinary electrical.
The declination was from 8� to 10�. My opinion is that this
phenomenon cannot be ascribed to the electromotive faculty (force), because the
copper is found between two equal and contrary forces. And data also, as I have
been experimenting in the liquids, that the electrical currents, have any
direction; not defeated, like the light and the radiant caloric, would not have
the multiplier give some sign, as it does clearly. It seems therefore that such
effect must be ascribed to the magnetic, and however that the North Pole is
equivalent to the zinc pole of a voltaic apparatus. I hope that others
experimenting with delicate multiplier pins, like with the sideroscope of (M)
Lebaillif (a kind of galvanometer), can obtain greater effects than I heard
when they are at their pleasure. (Interesting to end on the word "pleasure",
perhaps a partially admitted pro-pleasurist.)

(Much of the parallel claims may be due to people of different nations who have
known about the identify of magnetism and electricity for years finally making
it public, perhaps even through remote neuron writing on excluded people or
partial direct-to-brain windows people.)
Pavia, Italy  
171 YBN
[11/19/1829 AD]
2710) Michael Faraday (CE 1791-1867) produce a glass of very high refractive
index that will lead him, in 1845, to the discovery of diamagnetism. Faraday
finds this while completing an assignment from the Royal Society of London to
improve the quality of optical glass for telescopes.

(Royal Institution in) London, England  
171 YBN
[1829 AD]
2495) Thorium is a radioactive silvery white but turns gray or black on
exposure to air (oxygen or nitrogen?). It is about half as abundant as lead and
is three times more abundant than uranium in the Earth's crust. Thorium is
commercially recovered from the mineral monazite and occurs also in thorite and
thorianite. Thorium has been produced in commercial quantities by reduction of
the fluoride (ThF4) and dioxide (ThO2) and by electrolysis of the chloride
(ThCl4).

Thorium's longest-lived isotope, the only one that occurs naturally, is Th 232
with a half-life of 1.41 × 1010 years. Thorium has 26 known radioactive
isotopes, only 12 of which have half-lives greater than 1 sec.

Thorium has atomic number 90; atomic weight 232.038; approximate melting point
1,750°C; approximate boiling point 4,500°C; approximate specific gravity
11.7; valence 4.

At ordinary temperatures thorium has a face-centered cubic crystalline
structure. Thorium is a member of the actinide series in Group 3 of the
periodic table and is sometimes classed as one of the rare-earth metals. When
pure, Thorium metal is stable and resists oxidation, but it is usually
contaminated with small amounts of the oxide, which cause it to tarnish
rapidly. Thorium reacts slowly with water and is attacked only by hydrochloric
acid among the common acids. The finely divided thorium metal readily ignites
when heated, burning with a brilliant white flame; the thorium oxide formed has
the highest melting point of all oxides. Thorium forms numerous compounds with
other elements.

Thorium-232 undergoes natural disintegration and eventually is converted
through a 10-step chain of isotopes to lead-208, a stable isotope; alpha and
beta particles are emitted during this decay. One intermediate product is the
gas radon-220, also called thorium emanation or thoron. Thorium and its decay
products are sometimes used in radiotherapy.Although not a nuclear reactor fuel
itself, thorium-232 can be used in breeder reactors because, on capturing
slow-moving neutrons, (thorium) decays into fissionable uranium-233.
(Because of this)
thorium is expected to become increasingly important for conversion into the
fissionable fuel uranium-233.

Thorium-232 can react with a thermal (slow) neutron to form thorium-233,
emitting (a quantity of photons with gamma frequency).
Stokholm, Sweden (presumably)  
171 YBN
[1829 AD]
2507)
Jena, Germany (presumably)  
171 YBN
[1829 AD]
2575)
(Breslau, Prussia now:)Wroclaw, Poland  
171 YBN
[1829 AD]
2577) Jan (also Johannes) Evangelista Purkinje (PORKiNYA or PURKiNYA) (CE
1787-1869), describes the experimental effects on humans of camphor, opium,
belladonna, and turpentine and the visual images produced by poisoning with
digitalis and belladonna.

(Breslau, Prussia now:)Wroclaw, Poland  
171 YBN
[1829 AD]
2735) From 1816 to 1838 Coriolis is an assistant professor of analysis and
mechanics at the École Polytechnique, Paris.
Paris, France  
171 YBN
[1829 AD]
2761) Thomas Addison (CE 1793-1860), English physician with John Morgan,
publishes "An Essay on the Operation of Poisonous Agents upon the Living Body"
(1829), the first English book on toxicology.

(Guy's Hospital) London, England  
171 YBN
[1829 AD]
2767) In 1802 Lobachevsky lives in Kazan, studying on a government scholarship
at the Gymnasium.
After 1807 Lobachevsky attends Kazan State University, which had been
opened by Tsar Alexander I in 1804.
(At Kazan State University), Lobachevsky's
teachers are German professors invited to the university, in particular the
mathematician Martin Bartels, a friend of Gauss noted for his encyclopedic
knowledge of mathematics.
In 1812 Lobachevsky earns a master's degree from the university.
In 1814
Lobachevsky earns the degree of adjunct of pure mathematics and permission to
teach independently.
From 1816 Lobachevsky is professor extraordinarius.
In 1819 the Kazan
regional board of education institutes a xenophobic (undo fear of all things
foreign in particular people) policy, and the German faculty leaves.
The resulting
shortage of professors leads to a rapid advancement in Lobachevsky's career.
In 1823
Lobachevsky publishes a gymnasium textbook in geometry.
In 1824, Lobachevsky publishes an
algebra textbook.
In 1827 Lobachevsky is rector of (Kazan) University.
Lobachevsky encourages the
dissemination of education in the extensive Kazan district.
In 1830-1831 Lobachevsky is
instrumental in stopping the spread of a virulent cholera epidemic among the
teachers and students of the university by means of a rigid quarantine.
In order to inform
Western scientists about his new ideas, in 1837 Lobachevsky publishes an
article in French ("Geometrie imaginaire") and in 1840 a small book in German
(Geometrische Untersuchungen zur Theorie der Parallellinien). Lobachevsky's
article "Pangeometry" appears in Russian in 1855 and in French in 1856, the
year of his death.
In 1842, Lobachevsky saves the university from a devastating
fire that sweeps through Kazan.
Despite his efficient and devoted service, in 1846 he
was relieved by the government of his posts of professor and rector. No reason
is given.
Carl Friedrich Gauss helps to get Lobachevsky's election as an honorary
member of the Gottingen Scientific Society.
Apart from geometry, Lobachevsky also does
important work in the theory of infinite series, algebraic equations, integral
calculus, and probability.
Kazan, Russia  
171 YBN
[1829 AD]
2771) Eilhardt Mitscherlich (miCRliK) (CE 1794-1863), German chemist, publishes
"Lehrbuch der Chemie, which embodies many original observations, and is a
successful and well regarded textbook of chemistry.

(University of Berlin) Berlin, Germany  
171 YBN
[1829 AD]
2789) German naturalist (Baron von) Friedrich Wilhelm Heinrich Alexander
Humboldt (CE 1769-1859) is funded by Russian Czar Nicolas I to explore lands
owned by Russia in Central Asia and Siberia.

Humboldt is accompanied by another German naturalist, Christian Gottfried
Ehrenberg (IreNBRG) (CE 1795-1876)

Siberia, Russia  
171 YBN
[1829 AD]
2898) Wheatstone shows that every Chladni figure is the resultant of two or
more sets of isochronous parallel vibrations. (chronology)
In 1834 Wheatstone is made
professor of experimental philosophy at King's College, London.
Wheatstone can never
become a lecturer on account of his shyness. Therefore many of Wheatstone's
investigations are first described by Faraday in his Friday evening discourses
at the Royal Institution.
Wheatstone invents the "Playfair cipher", which is based on
substituting different pairs of letters for paired letters in the message.

Wheatstone manufactures musical instruments.
London, England  
171 YBN
[1829 AD]
2946) In 1825, Jacobi converts to Christianity, and a position opens for him at
the University of Berlin.
Asimov relates that because Jacobi is Jewish, it is unusual
that he gets a teaching position at an important school.
(University of Königsberg) Königsberg, Germany  
171 YBN
[1829 AD]
3009) Graham's father is determined that Thomas should enter the ministry and
when Thomas persists with his scientific studies, his father withdraws
financial support.
Graham is the first president of the Chemical Society of London, and
of the Cavendish Society, which Graham founds.
Graham is the first to suggest that
alcohol intended for nondrinking use by adultereated with poison ("denatured
alcohol") to prevent or punish unauthorized drinking. (This seems so
destructive and dangerous. This is like practically arranging a potential
poisoning. What is alcohol denatured with? I think people should rely on
education to lower alcohol addiction without the use of poisons.)
Graham became an
enthusiastic supporter of the atomic theory first suggested by John Dalton.
Grah
am also devised the sand tray for heating flasks. (chronology and more info on
usefulness)
(Mechanics' Institute) Glasgow, Scotland  
171 YBN
[1829 AD]
3107) Galois' collected works are published, in "Journal de Liouville" (1846),
pp. 381-444, about fifty of these pages being occupied by researches on the
resolubility of algebraic equations by radicals. Galois is credited with the
notion of a group of substitutions.

When Galois writes a vigorous article expressing pro-republican views, he is
promptly expelled from the École Normale Supérieure. Subsequently, Galois is
arrested twice for republican activities; Galois is acquitted the first time
but spends six months in prison on the second charge.
In 1815, during the Hundred Days
regime that followed Napoleon's escape from Elba, Galois' father is elected
mayor of the Paris suburb of Bourg-la-Reine.

Augustin-Louis Cauchy loses a memoir on the solvability of algebraic equations
that Galois had submitted in 1829 to the French Academy of Sciences.

Galois fails in two attempts (1827 and 1829) to gain admission to the École
Polytechnique,

Galois is shot and killed by a gun before the age of 21 in a duel.
Paris, France  
171 YBN
[1829 AD]
5985)
Paris, France  
170 YBN
[09/15/1830 AD]
2517) When the Liverpool-Manchester line is nearing completion in 1829, a
competition is held for locomotives; Stephenson's new engine, the Rocket, which
he built with his son, Robert, won with a speed of 36 miles (58 km) per hour.
Eight locomotives, all built in Stephenson's Newcastle works, are used when the
Liverpool-Manchester line opens on Sept. 15, 1830. From this time on, railroad
building spreads rapidly throughout Britain, Europe, and North America, and
George Stephenson continues as the chief guide of the railroad revolution
solving problems such as roadway construction, bridge design, and locomotive
manufacture, in addition to building other railways.
Liverpool (and Manchester), England  
170 YBN
[1830 AD]
1210)
  
170 YBN
[1830 AD]
2527)
Surrey, England (presumably)  
170 YBN
[1830 AD]
2535)
Paris, France (presumably)  
170 YBN
[1830 AD]
2556) In 1830 Lister beings grinding his own lenses and develops techniques
that Lister teaches to optical instrument makers in London.
Lister is the father of the
surgeon Joseph Lister.
london, England (presumbly)  
170 YBN
[1830 AD]
2562) Amici makes microscopes that can examine objects with 6000 times
magnification.

Using an improved micrometer of his own design, Amici makes accurate
measurements of the polar and equatorial diameters of the Sun.

Amici builds lenses, mirrors and spectroscopic prisms for use in telescopes.)

Amici invents a combination of three prisms that is still used in spectroscopy
and is known as the Amici prism.
From 1815 to 1825 Amici is professor of mathematics
at the University of Modena.
In 1831 Amici is invited by the grand duke of
Florence to head the observatory and Museum of Natural History in Florence.
Modena, Italy (presumably)  
170 YBN
[1830 AD]
2573) The English chemist Henry Enfield Roscoe are the first to isolate
vanadium metal in 1867 by hydrogen reduction of vanadium dichloride, VCl2, and
the American chemists John Wesley Marden and Malcolm N. Rich will obtain
vanadium in 99.7 percent purity in 1925 by reduction of vanadium pentoxide,
V2O5, with calcium metal.
Sefström studies under Jöns Berzelius in Stockholm,
graduating in 1813.
Starting in 1820 Sefström teaches chemistry at the School of
Mines.
  
170 YBN
[1830 AD]
2624) Hall's other works include "The Diagnosis of Diseases" (1817) and
"Memoirs on the Nervous System" (1837).
London, England (presumably)  
170 YBN
[1830 AD]
2636) George Peacock (PEKoK) (CE 1791-1858), publishes "Treatise on Algebra"
which attempts to give algebra a logical treatment comparable to Euclid's
"Elements". Peacock (defines) two types of algebra, arithmetical algebra and
symbolic algebra. Peacock describes symbolic algebra as "the science which
treats the combinations of arbitrary signs and symbols by means defined through
arbitrary laws." (and arithmetical algebra as...)

Cambridge, England (presumably)  
170 YBN
[1830 AD]
2746) Charles Babbage (CE 1792-1871), English mathematician, publishes
"Reflections on the Decline of Science in England, and on Some of Its Causes"
(1830, London, B. Fellowes).

This work is directed almost exclusively at the Royal Society. One improvement
Babbage suggests is biannual elections for president as opposed to lifetime
Presidency.

Babbage blames "the party" which governs the Royal Society and not the members,
and near the end of his preface uses the expression "by ratifying it" which may
imply that those who inform the public about the growing number of
technological secrets may be frowned on as "rats", although perhaps this is
simply coincidence.

Cambridge, England (presumably)  
170 YBN
[1830 AD]
2779) In 1817 Mädler graduates from a Gymnasium and teaches in a seminary in
Berlin.
In Berlin Mädler befriends Wilhelm Beer (1797-1850), a banker and amateur
astronomer who owns a private observatory.
Berlin, Germany (presumably)  
170 YBN
[1830 AD]
2802) At age 15 Lyell reads Robert Bakewell's "Introduction to Geology" (1813),
which arouses Lyell's interest in geology.
In 1819, Lyell gets a bachelor's degree from
Exeter College, Oxford.
Lyell joins the Geological Society, becoming its secretary in
1823 and later president for two terms.
In 1825, Lyell is admitted to the bar
(certified to work as a lawyer).
Lyell works as a lawyer intermittently for 3 years.
From May
1828 to February 1829 Lyell explores the geology of Europe.
From 1831 to 1833, Lyell
serves as the first professor of geology at King's College, London.
In 1832 and 1833
Lyell delivers well-received lectures at King's College, London, afterward
resigning the professorship as too time-consuming.
In 1833, Lyell meets Cuvier and Humboldt in
Paris.
The young Darwin is friends with and will be influenced by Lyell.
In the 1840s Lyell
visits America and see many important geological sites.
Lyell's lectures at the Lowell
Institute in Boston attract thousands of people of both genders and every
(income level).
Lyell long objects to church domination of British colleges and helps
to begin educational reform at Oxford university.
Lyell will be one of the first converts
to Darwin's theory of evolution.
Lyell is a strong proponent of the North in
the US Civil War, while most others of the upper class of England were
pro-Southern.
London, England (presumably)  
170 YBN
[1830 AD]
2848) Oxymide is a white crystalline neutral substance (C2O2(NH2)2) obtained by
treating ethyl oxalate with ammonia. Oxymide is the acid amide of oxalic acid.
(Ecole Polytechnique) Paris, France (presumably)  
170 YBN
[1830 AD]
3271) This is an early instance of people using violence because of anger that
machines has taken their jobs. A similar event happens in England with the
Spinning Jenny. The walking robots will ultimately take many jobs away from
humans, but like all technological advances, ultimately the majority benefits
from the increased production of the robots. Ultimately the robots will be
unpaid labor seeding, growing, harvesting, packaging and distributing for to
the humans for less cost while humans get the rewards without having to work,
clean, or do unthinking low-skill labor.
France  
170 YBN
[1830 AD]
4003) Wilhelm Weber is the brother of the noted scientists Ernst Heinrich Weber
and Eduard Friedrich Weber, both of whom worked in anatomy and physiology.

In 1825, with his elder brother Weber publishes a well known treatise on waves,
"Die Wellenlehre auf Experimente gegrundet" ("Wave teachings based on
experiments").
In 1833 With his younger brother, the physiologist Eduard Friedrich Weber
(1806-1871), Weber publishes an investigation into the mechanism of walking.

In 1837, a new King began his reign in Hanover. He suspends the constitution
and this creates vigorous protests from several of the professors at the
University, Weber among them. To punish them, seven Professors are dismissed
from their chairs, and three are even banished from the country. Weber is
forced into retirement for some years.
(University of) Göttingen, Germany  
170 YBN
[1830 AD]
4699)
London, England (guess)  
170 YBN
[1830 AD]
5987) (Louis-)Hector Berlioz (CE 1803-1869), French composer, critic, and
conductor of the Romantic period, composes his "Symphonie fantastique".

Paris, France (presumably)  
169 YBN
[01/03/1831 AD]
2806)
Albany, NY, USA  
169 YBN
[02/17/1831 AD]
2702) The transformer makes use of the important principle of dynamic
electromagnet induction, how moving electrical particles can induce other
electrical particles to move in an unconnected conductor. Static electric
induction was first described in 1753 by John Canton (CE 1718-1772).
Electrostatic induction is how an electrified object can induce an opposite
charge in a second object without touching by being close to the electrified
object.

Faraday reports his production of electric current from magnetism initially on
February 17, 1831, which is reported in the April edition of the "Annals of
Philosophy" under "Proceedings of the Royal Institution" and then gives a more
detailed account which is published on August 29, 1831.

In the spring of 1831 Faraday began working with Charles Wheatstone on the
theory of sound. Faraday is particularly fascinated by the Chladni figures
formed in light powder spread on iron plates when these plates are vibrated by
a violin bow. Faraday observes that such patterns can be induced in one plate
by bowing another plate nearby. According to the Encyclopedia Britannica, this
acoustic induction is apparently what lay behind Faraday's most famous
experiment which results in the discovery of magnetic induction of electrical
current.


Why is there only a change in current and not a similar current as Faraday had
expected? I think the explanation for this is that if a current is made of
photons, or even electrons, or other particles, photon particles spill-out,
outside of the wire and surround it. Current appears to move in a spiral shape
like water going down a drain, and this may reflect the movement of photons
through the atomic structure of metals. This spiral shape is reflected in the
electric field around a wire which current is moving through. The photons
outside the wire are less in quantity and less dense than in the wire. So I
think that as the current in the first wire is initiated, a hole in the battery
is caused, which starts a chain of particles (I think are photons but could be
electrons) moving in a spiral within and around the first wire. These first
photons collide with the coiled wire on the other side, and these photons fill
holes in the second coiled wire which causes the photons to flow in the second
wire, however once these holes or channels are filled (there is no where else
for the photons to go except out as heat), photons simply bounce off (or
replace those lost as heat), until the current in the first wire is stopped and
photons stop bombarding the second wire, as the current trails to an end in the
first wire, the photons end in sequence, which allows the holes or channels in
the second wire to clear with the remaining photons (perhaps because they are
emitted as heat?) photons in the rest of the wire then using these new holes to
move in the opposite direction, temporarily filling the newly emptied channel.
(I'm not sure about what explains the reverse motion, the holes are filled on
one side, and then emptied on the other, and it doesn't circle forever because
it is dissipated as heat. If true a superconductor might sustain the current
longer.)

In this view metals are filled with empty spiral channels that photons fill,
the photons then move through empty holes because of gravity, and perhaps
collision which is electrical current.


Faraday presents his results in a four-part paper read to the Royal Society on
November 24, December 8 and 15, 1831. The paper appears in print in May 1832 in
the "Philosophical Transactions" and forms the first series of Faraday's famous
"Experimental Researches in Electricity".

In the first section Faraday describes the induction of momentary currents
induced in a wire when either an adjacent primary wire is connected and
disconnected to a battery, or when the position of the primary wire carrying a
current is moved relative to the wire. In the second section Faraday describes
the increased inductive effect obtained by inserting iron in the helices of
wire in which current is induced, in addition to how currents are induced from
the movement of permanent magnets when brought near the helices of wire.
Faraday labels the effect of induced current from batteries as "volta-electric
induction" and current induced from magnets as "magneto-electric induction".
Faraday describes an experiment where a needle in the center of an induced
helix remains magnetized after the primary circuit is disconnected. Faraday
dedicates the third section to outlining his concept of an "electro-tonic
state", which Faraday proposes as a "new electrical condition" established in
matter when in the presence of magnets and current-carrying wires.

In his paper, Faraday mentions Ampere's experiments of bring a copper disc near
to a flat spiral, Ampere's repeating Arago's experiments (describe), and
Ampere's finding that every electric current is accompanied by a corresponding
magnetic action at right angles to the current. Faraday goes on to say that he
would be surprised if a good conductor within the sphere of this magnetic
action should not have any current induced through it.

Initially, a number of experiments to cause a current in a second wire from a
first that has a current that Faraday performs fail to produce any current in
the second wire. Faraday rolls 26 feet of 1/20 inch diameter copper wire around
a cylinder of wood (diameter? perhaps an inch) as a helix. Each spiral is
separated from the next by a thin twine so they do not touch. This helix is
covered with calico (cotton cloth which serves as an insulator) and a second
wire and thread wound over the first. In this way 12 helices are layered around
a cylinder of wood. Each alternate coil (the first, third, fifth, seventh,
ninth and eleventh) is connected at each end to form a single helix, and the
second coil is also connected in a similar way. So two helices are closely
intertwined, having the same direction, not touching anywhere, and each
containing 155 feet in length of wire. One helix is connected to a galvanometer
the other to a voltaic batter of 10 pairs of plates four inches square (one of
zinc and double coppers). This experiment fails to produce any movement in the
galvanometer. A similar compound helix with six lengths of copper and six of
soft iron wire containing even more wire, 208 feet per helix, fails to produce
an induced current in the secondary helix in either the copper or iron helix
when current was passed through the other helix. Similar other experiments
fail, however when Faraday uses a battery with 100 pairs of 4 inch square
plates (10 times more than the earlier mentioned 10 pairs of plates (what are
equivalent voltages?)), with each of the two helices 203 feet of copper wire,
and metal contact everywhere prevented by twine, when contact (between the
primary coil and the battery) is made, Faraday reports "a sudden and very
slight effect at the galvanometer" and "also a similar slight effect when the
contact with the battery was broken". But while the voltaic current is
continuing to pass through the one helix, the needle of the galvanometer does
not move, indicating that no current is flowing in the second helix even
though, Faraday observes, current continues to pass through the primary helix,
resulting in heat from the helix. Faraday repeats this experiments with a
battery of 120 pairs of plates, which produces no other effects, but Faraday
notices that the movement of the needle when the battery is connected is always
in one direction, and that the equally slight deflection produced when the
battery disconnected is in the other direction. Faraday describes this flash of
current as being more like that produced by a Leyden jar than by a voltaic
battery. This causes Faraday to wonder if this induced current might magnetize
a steel needle (because Leyden jars must have been used to magnetize needles
and other bars of metal). Faraday substitutes a small hollow helix for the
galvanometer and places a steel needle (in the middle of this new coil that has
replaced the galvanometer in the secondary circuit). When Faraday connects the
battery and primary coil and removes the needle before the battery is
disconnected, Faraday finds that the needle is magnetized. When the battery
contact is first made, and an unmagnetized needle is then put into the center
(touching or insulated?) of the small indicating helix, and the battery then
disconnected, the needle is magnetized to in equal strength as the first, but
with opposite poles. When an unmagnetized needle is put into the indicating
helix, before the battery is connected and remains there until the battery is
disconnected, the needle has little or no magnetism, Faraday concluding that
the first effect must be nearly neutralized by the second. Faraday finds that
the induced current when the battery is connected is larger than when
disconnected and explains this as the possible result of an accumulation at the
poles of the unconnected pile which makes current stronger when first
connected. Faraday states that there is no induced current in the second coil
when the second coil connected from an open circuit after the battery is
connected to the primary coil. Similarly, a needle is not magnetized when the
second circuit is connected after the first, although a needle is magnetized
when the battery is disconnected in the direction of the current induced.
Faraday then stretches several feet of copper wire on a board in the letter W,
with a second similar board with a sheet of thick paper in between the wires of
each. One of these wires is connected to a galvanometer and the other with a
voltaic battery. Faraday finds that when the first wire is moved towards the
second, as the wire approaches the needle is deflected, and when removed the
needle is deflected in the opposite direction. By making the wires approach and
then recede simultaneously with the movement of the needle, the needle moves
(often), but when the wires do not move towards or away from each other, the
galvanometer shows no current. When the wires are brought together the induced
current is in the opposite direction to the inducing current, and when the
wires are receding the induced current is in the same direction as the inducing
current. When the wires remain stationary there is no induced current. (20)
When a small voltaic battery is connected to the secondary circuit so a smaller
current runs through it, and a 100 plate pairs battery is connected to the
primary circuit, the galvanometer needle moved in the usual way, but the
resumed its position measuring the constant current. (21) Faraday concludes
that the induced extra current exert no permanent inducing power on the
existing current. (24) Faraday uses a Leyden jar in place of a batter which
magnetizes an iron needle. (25) Faraday comments that separating the effect
when the charge begins and ends is impossible because the charge happens too
quickly. (have people since confirmed the same effect of current passing both
ways on start and end of charge/current?) (26) Faraday defines the action of a
current from a voltaic battery "volta-electric induction", and views the
property of the secondary wire after the brief initial current, while the
current flows through the primary circuit, as having a peculiar electric
condition. (I think the analogy of an empty spiral channel running through wire
which is filled by (photon) particles from the primary current until full and
then no more particles can enter the channel, or simply replace those particles
already in the channel fits the phenomenon too. (EX) If true, perhaps there is
some way to extract that current temporarily into a second closed loop of wire
(to fill a second, extended coil off the secondary coil while the current is
already flowing in the primary coil)). Faraday titles part 2 "Evolution of
Electricity from Magnetism", using the word Evolution in 1832, (Darwin
formulates the theory of evolution from 1837-1839, and publishes "Origin of
Species" in 1859, perhaps evolution was a code word for the early Lamarkian
evolution theory or perhaps just coincidence. Now of course, the minority of
evolution supporters use the word "evolution" to reveal themselves as
theory-of-evolution supporters usually.)
(27) A welded (how) ring, six inches in
diameter, is made of round 7/8 inch thick soft iron bar. On one side of this
ring Faraday wraps three helices, each with 24 feet of 1/20th inch copper wire,
insulated from the iron and each other. These helices, connected end to end,
occupy about 9 inches in length on the ring. (see image). On the other side of
the ring sixty feet of copper wire in 2 pieces are applied forming helix B in
the same direction as the helices of A, but separated from each other by about
1/2 and inch of uncovered iron. (28) Helix B is connected by copper wire with a
galvanometer 3 feet away. The wires of A are connected to a battery with 10
pairs of plates four inches square. When Faraday connects the battery, the
galvanometer needle is immediately affected, and to a degree far beyond that
produced by a battery of 10 times the power produced by helices without iron.
Again the effect is not permanent and the needle soon returns to rest in its
natural position, similarly when breaking the connection with the battery, the
needle is again powerfully deflected, but in the opposite direction to that
induced when the battery was connected. (Presumably if there is a channel in
the wire, more particles are entering it which shows that the weak current
without the iron bar was not filling it completely but yet no more particles
could enter. Did Faraday try with the wires intertwined? Perhaps the effect is
from the secondary coil being farther away. It seems likely that the extra
particles come from the iron atoms. Similar to an electromagnet, perhaps a
larger channel is created in/extended into the iron bar. Perhaps the particles
in the coil push the particles in the iron along, since they apparently do not
move on their own, or perhaps they do.) (32) Faraday uses the larger 100 paired
plates battery and by using charcoal at the ends of the B helix creates a tiny
spark when the battery connected to A is connected, and a spark is rarely seen
(in the opposite direction?) on breaking contact. (Is charcoal needed, or is an
open circuit enough?) (34) Faraday again comments on how adding a soft iron
cylinder 7/8" thick and 12" long into the coil produces a much larger movement
on the galvanometer, and adds that this makes magnets with more energy,
apparently, than when no iron cylinder is present. (35) Replacing the iron
cylinder with an equal cylinder of copper produces no magnified effect, and
only produces a feeble current similar to a hollow coil. (What other metals
besides iron can be magnetized? Do alloys stop the magnetic (electric field)
properties of iron?) (36) Faraday finds that ordinary permanent magnets can
produce current in the same way as a battery can. Faraday connects two bar
magnets with opposite poles on one end, with the other ends connecting on
either side of an iron cylinder (around the iron cylinder with the helix around
it connected to the galvanometer) which converts it for a time into a magnet
(explain how magnets are created). By connecting and disconnecting one of the
bar magnets, or reversing them, "the magnetism of the iron cylinder can be
destroyed or reversed at pleasure" (and therefore the induced current) (see
figure 2). (37) When making magnetic contact the needle is deflected, however,
quickly resumes its initial position, and on breaking contact the needle is
again deflected, but in the opposite direction. When the magnetic contacts are
reversed, the deflections are reversed. (38) When magnetic contact is made the
deflection indicates an induced current in the opposite direction than the
current (see figure 3) that is used to make a magnet with the same polarity as
the bar magnet. This current is in the opposite direction of the theory
proposed by Ampere as existing in a permanent magnet or as current in an
electromagnet of similar polarity. (Is this because electrons flow from
negative to positive? - so the left-hand rule applies in terms of flow of
electrons from negative to positive.) (This part is not exactly clear to me.)
In figure 3, P is the wire going to the positive pole of the batter (which the
zinc plates face) and the N the negative wire.(39) Faraday finds that when a
cylindrical magnet 3/4" in diameter and 8.5 inches in length is inserted into a
hollow helix connected to a galvanometer, the needle is deflected, and when the
magnet is removed, the needle again is deflected, but in the opposite
direction. The effect is small, but by introducing and withdrawing the magnet
so that the impulse each time should be added to those previously causes the
needle to vibrate through an arc of 180 degrees or more. (41) Faraday finds
that when the magnet is inserted, the needle is deflected in the same
direction, and when withdrawn the needle is deflected in the opposite
direction. (figure 4) (43) Moving the magnet outside the helix has no effect on
the galvanometer needle. (44) Faraday uses a large compound (bar?) magnet owned
by the Royal Society for his experiments. (what kind? How manufactured?) This
magnet is made of 450 bar magnets each 15 inches long, 1 inch wide, and half
inch thick. When a soft iron cylinder 3/4 inch in diameter and 12 inches long
is put across this magnet a force of 100 pounds is required to break the
contact. (see figure 5) (46) When a soft iron cylinder 13 inches long is put
through the compound hollow helix connected to the galvanometer, and the iron
cylinder brought in contact with the two poles of this magnet (figure 5), a
very powerful rush of electricity takes place causing the needle to whirl
around many times (47) before coming to rest. Breaking the magnetic contact
causes the needle to whirl around in the opposite direction with an equal force
as the first. Using an armed (?) loadstone capable of lifting 30 pounds, a frog
leg is powerfully convulsed each time magnetic contact is made, but only after
separating the battery with a blow does the frog leg muscle convulse, which
shows that the more instantaneous the connection or disconnection is the more
powerful the convulsion (and current). (57) These experiments show conclusively
that, although weak and quantity small, permanent magnets can be used to
produce electricity. Faraday thinks that powerful electromagnets can be used to
produce a brighter spark, ignite wires, and by being passed through liquid
chemical action can be produced with such electric current. (58) Faraday
importantly states "The similarity of action, almost amounting to identity (any
difference perhaps because of the difference in direction of current), between
common magnets and either electro-magnets or volta-electric currents, is
strikingly in accordance with and confirmatority of M. Ampere's theory, and
furnishes powerful reasons for believing that the action is the same in both
cases". Faraday defines the words "magneto-electric" or "magnelectric"
induction to describe current induced by permanent, or as he describes ordinary
magnets. (59) Faraday finds the olny difference between volta-electric and
magneto-electric induction as the suddenness of the volta-electric effect and
the larger time required by magneto-electric induction, but states that
circumstances indicate that this difference will disappear with more
investigation. (So Faraday is basically agreeing with the theory put forward by
Ampere that a magnetic field is an electric field caused by electric current in
permanent magnets.)
In the third section "New Electrical State or Condition of Matter",
Faraday hypothesizes about an electro-tonic state, but notes that later
investigations (73,76,77) induce him to think that these phenomena can be fully
explained without any electro-tonic state. (60) Faraday states that when a wire
is subject to induction it resists the formation of an electrical current in
it, where if in a common condition, a current would be produced. (Clearly a
current can still flow through the induced wire, as Faraday has shown. Faraday
most likely means that the magnetic field does not cause a constant current as
would be expected.) (67) Faraday explains that this hypothesized state begins
when the effect of induction starts and ends when the inductive force is
removed. (My own view is that particles fill holes in the iron and when filled
with particles no current flows, however that an additional current flows
during induction makes that seem unlikely. Possibly the lines of particles fill
holes once, and then since not moved, collide with the same filled holes, while
current flowing through from a different source pull a chain of particles. In
fact with a current flowing, possibly more particles from the electric field
might be accepted, but I doubt it since the hole in current is produced at the
battery. But yet, even with a current, the field adds those initial particles.
An alternative explanation is that the field {as a force that originates from
the primary source} causes particles of current to flow. Clearly more particles
of force are produced by the mass of the iron bar, but not that of a copper
bar, which implies that the atomic structure, and not the mass of the iron is
responsible to the addition.)

(77) Faraday recounts an interesting story of M.A. De La Rive who found that a
metallic conductor in a liquid connected to a battery can produce a current in
the fluid after the battery is disconnected and another finding of electricity
of two metals in contact that remains after their separation by M.A. Van Beek.
(78) Faraday describes Ampere's experiment where a disc of copper is suspended
by a silk thread and surrounded by a helix of wire, when a current is sent
through the helix and a strong magnet moved towards the disc, the disc turns at
the moment to take a position of equilibrium, exactly as the helix would have
turned (in response to the magnet) if the helix was free to move. Faraday
cannot reproduce this experiment and explains that this is probably because the
induction effect is too fast or to the power of Ampere's electro-magnet
apparatus. Ampere proposed that "a current of electricity tends to put the
electricity of conductors near which it passes in the same direction" where
Faraday finds that current of electricity produce current in nearby conductors
in the opposite direction, and that this effect is only momentary.

Faraday first experimented in an effort to induce a current from a helix on
November 28, 1825 quoting from his notes: "Experiments on induction by
connecting wire of voltaic battery:-a battery of four troughs, ten pairs of
plates, each arranged side by side- the poles connected by a wire about four
feet long, parallel to which was another similar wire separated from it only by
two thicknesses of paper, the ends of the latter were attached to a
galvanometer:- exhibited no action, &c, &c, &c,-Could not in any way render any
induction evidence from the connecting wire." Faraday then writes that the
cause of failure at that time is now evident. (Presumably that either the
battery was not strong enough for the number of hollow coils used, or that a
soft iron bar was needed to increase the induced current.)(Possibly penis
symbol used by Faraday ":-" I notice because I can imagine the suspicion
created if I used such a symbol. Generally the smartest people understand the
massive injustice done to physical pleasure.)

On his discovery of magneto-electricity Faraday abandons the commercial work
which adds to his small salary, in order to devote all his time for research.
This financial loss is made up in part later by a pension of 300 pounds a year
from the British Government.

James Clerk Maxwell will create "Faraday's law of induction" giving a
mathematical interpretation based on this work.

(Can static electricity induce current?)
(Royal Institution in) London, England  
169 YBN
[06/01/1831 AD]
2835)
Boothia Peninsula,Nunavut, Canada  
169 YBN
[06/01/1831 AD]
2837) Part of the "Carta Marina" of 1539 by Olaus Magnus, depicts the location
of magnetic north vaguely conceived as "Insula Magnetu" (Latin for "Magnetic
Island") off modern day Murmansk. The man holding the rune staffs is the Norse
hero Starkad.

The Scottish explorer, James Clark Ross (CE 1800-1862) will be the first to
reach the North Magnetic Pole in 1831.

Boothia Peninsula,Nunavut, Canada  
169 YBN
[08/??/1831 AD]
2525) Guthrie invents and first manufactured percussion pills, also inventing
the punch lock for exploding them. This lock takes the place of the old flint
lock in firearms, and will be in turn superseded, after Dr. Guthrie's death, by
the percussion cap. In the course of Guthrie's experiments Guthrie sustains
lasting injuries and nearly loses his life from an accidental explosion.

In 1830 Guthrie invents a process for the rapid conversion of potato starch
into molasses, which he published in Silliman's "American Journal of Science,"
to which he contributed occasional papers on scientific subjects.
Sackets Harbor, NY, USA  
169 YBN
[09/??/1831 AD]
2705) The first electrical generator was the static electricity generator of
Guericke, in which mechanical movement is used to create a static electric
potential. In 1663, Volta invented the first constant electricity generator,
the electric battery (voltaic pile), which creates electricity from molecular
combination (chemical reaction), in 1800. Faraday builds the first electrical
generator, which creates constant electric current from mechanical motion in
1831. The electrical generator allows any source of mechanical movement, such
as the force of wind, water, or a steam (coal burning), or gas burning engine
to create a constant stream of electricity.

Faraday reports his experiments which lead to the first electric generator in
part 4 of his famous "Experimental Researches in Electricity".

In Part 4 "Explication of Arago's Magnetic Phenomena", Faraday describes
Arago's experiment (81) in which a plate of copper is revolved close to a
magnetic needle or magnet which is suspended so that it may rotate in a plane
parallel to the plate. (more detail about how suspended? Perhaps from a similar
copper plate with both on different axes. Perhaps new record for Arago's
experiment) When the copper plate is revolved, the magnetic needle or magnet
tends to follow the motion of the plate and similarly if the magnet is
revolved, the plate tends to follow the motion of the magnet. Arago states that
this effect happens with all solids, liquids and even gases. (82) Babbage and
John Herschel repeat this experiment and can only obtain the effect for
excellent conductors of electricity. Babbage and Herschel explain the effect as
magnetism induced in the plate by the magnet, the pole of the magnet causes an
opposite pole in the nearest part of the plate. Arago and Ampere reject this
theory because there is no attraction when the magnet and metal are at rest.
(83) Having already obtained electricity from magnets, Faraday hopes to make
Arago's experiment a new source of electricity. In addition, Faraday intends to
offer the correct interpretation of the magnet following phenomenon found by
Arago. (84) Faraday uses two iron or steel bars about 6x1x1/2 inches in size
connected to the opposite poles of the large magnet of the Royal Society's at
Christie's house. (85) Faraday mounts a disc of copper 12" in diameter and 1/5
inch thick on a brass axis so the disc can rotate either vertically or
horizontally. The edge of this disc is placed between the two magnetic poles
(see figure 7). (86) Faraday uses copper and lead conductors 4x1/3x1/5 inch in
size which contact the edge of the copper disc and are connected to a
galvanometer. (87) Faraday makes his own galvanometer of copper wire covered
with silk coiled into 16-18 turns. Two sewing-needles are magnetized and put
through a stem of dried grass parallel to each other but in opposite directions
about held an inch apart. This system is suspended by a fiber of unspun silk
(see figure 8). The entire instrument is protected in a glass jar. The wires
are shown in the figures as A and B. (88) The edge of the copper disc is
inserted in between the magnetic poles which are 1/2 inch apart. One
galvanometer wire is connected to the brass axis and the other to the conductor
which is held at the edge of the disc at the part between the magnetic poles.
In this position, the galvanometer shows no effect, but the instant the plate
is moved the galvanometer needle moves, and by rotating the copper plate
quickly, the needle can be deflected 90 degrees or more. 89) After more
experimenting Faraday can sustain a permanent deflection of the needle of
nearly 45 degrees by rotating the disk. (90) Faraday writes "Here therefore was
demonstrated the production of permanent current of electricity by ordinary
magnets (57.).". (This is the invention of the first electrical generator {also
called a dynamo}, a device that can convert mechanical movement into a
sustained electrical current.) (91) When the motion of the disc is reversed,
the galvanometer is deflected with equal power but on the opposite side, and
the current of electricity is created in the reverse direction as in the
initial direction. (92) Faraday finds that even when the conductor is placed to
the right or left (see figure 9) of the poles, even as much as 50-60 degrees,
the current is still passed through the galvanometer, but gradually weakens any
farther than 50-60 degrees away from the magnetic poles. (94) Faraday finds
that even if the conductor moves along with the disc, current flows when the
disc is moved. (95) When the galvanometer wires are connected to two conductors
on the edge of the disc, Faraday finds that when in the position in figure 11 a
current is produced, and when shifted in figure 12 a current in the opposite
direction is produced (when turning the disc in either direction?) Faraday
describes this as in figure 11 a strong current at A and a weak current at B,
and the opposite for figure 12. (96) So when the two conductors are equally
distant from the magnetic poles, as in figure 13, no current at the
galvanometer is measured, no matter which direction the disc is rotated. When
the galvanometer is connected to a conductor and the disc axis, then the
galvanometer shows a current according to the direction of disc rotation. (98)
Faraday makes an effort to make sure that these results are independent of the
Earth's magnetism. (This is an interesting point, because, can the Earth's
magnetic field be used against an opposite pole to produce electricity, only
needing one magnet? Probably the Earth field is too weak? State how strong the
Earth magnetic field is. Does this represent particles per volume space per
unit time?) (99) Faraday describes the relation of current of electricity
produced to the magnetic pole and the direction of rotation of the plate.
Faraday uses the terms "marked and unmarked pole". This is an important point.
The marked end is the end with an "N" marked on it. Since we call the arctic
pole of Earth the North pole, the side of a magnet with the letter N, the
"marked" end, is actually a South pole since it points to the North Pole of the
Earth. Particles appear to flow from South Pole to North Pole, so all North
Poles are receivers of particles and South Poles emitters of particles. Placing
a compass over a magnet shows that the compass needle points to the magnet's
South Pole, when the compass is aligned to point to the Earth's North pole. A
compass needle can have its magnetic field reversed by a magnet simply by
changing the field around the needle before the needle has time to move, and so
people should be aware of this too. If the unmarked magnetic pole is under the
edge of the plate and the plate rotated clockwise, the current is positive at
the edge and negative at the center (see figure 15). (In other words particles
flow from the edge of the disk to the center.) (100) If the unmarked magnetic
pole is placed above the disc and the disc rotated clockwise, the electricity
is reversed. (The current flows from the center of the disk to the edge, the
edge being considered the ground and source of electrons.) (101) Faraday states
that the rotating plate is merely another form of the more simple experiment of
passing a piece of metal between the magnetic poles in a rectilinear direction
which produces currents of electricity at right angles to the direction of
motion, reversing when crossing the place of the magnetic pole or poles. This
is shown by the simple experiment: (see figure 16) a piece of copper plate
12x1.5x0.2 inches is placed between the magnetic poles while the two conductors
from the galvanometer are held in contact with the edges of the copper plate.
When the plate is then drawn through in the direction of the arrow the
galvanometer needle is deflected, its unmarked end passing eastward, indicating
that wire A received negative and wire B positive electricity. Since the
unmarked pole of the magnet is above, the result is the same as the effect
obtained by the rotating plate (99). (102) Reversing the motion of the plate
causes the galvanometer needle to be deflected in the opposite direction,
showing an opposite current. (103) To determine the nature of the electrical
current in various parts of the moving copper plate, Faraday connects one
conductor is connected to the copper plate near the pole of the magnet with the
other connected to the end of the copper plate. In figure 17, B gets positive
electricity, but on the opposite side (figure 18) gets negative electricity.
Reversing the motion (figure 19) B gets negative electricity, and (figure 20) B
gets positive electricity. (104) (Figure 21) The same effects are produced when
the plate is not directly aligned with the polar axis of the magnet, although
not as strongly. (105) When the two magnet poles are put together and the
copper plate drawn between the conductors near the plate, there was only little
effect produced. When the poles are separated by the width of a card, the
effect is more, but still small. (106) A copper wire 1/8 inch thick moved
between the conductors and magnet poles produces an effect although not as much
as the plates. (108) (Figure 22) The results are the same when the conductors
are connected to the ends of the copper plate and the plate moved in a
direction transverse to their length. (109) Even simply the wire from the
galvanometer connected to form a complete circuit, passed through between the
magnet poles causes the galvanometer to move. Passing the wire back and forth
to correspond with the vibrations of the needle can cause the needle to be
increased by 20 or 30 degrees on each side. (110) (Figure 23) With the ends of
a plate of metal connected to the galvanometer, and the plate then moved
between the poles from end to end in either direction, no effect is produced on
the galvanometer. Only when the motion is transverse is the needle deflected.
(111) These effects are also obtained with electromagnetic poles, resulting
from the use of copper helices or spirals, either alone or with iron cores. The
directions of the motions are precisely the same, but the action is much
greater when the iron cores are used, than without. (112) When a flat spiral is
passed through long-side first between the poles, a curios action at the
galvanometer results; the needle first moves strongly one way, but then
suddenly stopped, as if the needle struck against some solid obstacle, and
immediately returns. When the spiral is moved up or down the motion of the
needle is the same, suddenly stopping and reversing, but on turning the spiral
around 180 degrees the directions of needle motions are reversed, but still are
suddenly interrupted and inverted. (This is difficult to visualize and I may be
describing it incorrectly.) This double action depends on the halves of the
spiral which is divided by a line passing through it's center perpendicular to
the direction of its motion. So although this effect is curious, it is
explainable to the action of single wires. (113) Faraday writes that although
the experiments with the rotating plate, wires and plates of metal are first
successfully made with the large magnet belonging to the Royal Society, they
were all repeated with a couple of bar magnets two feet long, 1.5 inches wide
and 0.5 inch thick, and by making the galvanometer (87) more delicate.
Ferro-electro-magnets like those of Moll, henry, etc (57) are very powerful. It
is very important when making experiments on different substances that
thermo-electric effects produced by contact of the fingers, etc, be avoided or
accounted for. (114) Faraday describes the relation that holds between the
magnetic pole, the moving wire or metal and the direction of current evolved,
that is, the law that governs the evolution of electricity by magneto-electric
induction, stating that this relation is simple, although difficult to express.
In figure 24, PN represents a horizontal wire passing by a south (marked)
magnetic pole so that the direction of its motion coincides with the curved
line proceeding from below upwards then the current of electricity in the wire
is from P to N. This is also the case no matter what the motion so long as the
wire cuts the magnetic curves in the same direction. By magnetic curves,
Faraday is referring to the lines of force that would be shown by iron filings
or with which a small magnetic needle would form a tangent with. If the wire is
moved in the reverse directions, the electric current is from N to P.
Alternatively, if the wire is in position shown by P' and N' and viewed as
tangent to the curved surface of the cylindrical magnet, the wire moved with
the dotted horizontal curve causes current to flow from P' to N'. (115) This
same relation holds true for the unmarked pole of the magnet but the current
directions are reversed. (116) (Figure 25) So the current of electricity which
is excited in metal when moving in the neighborhood of a magnet depends on the
relation of the metal to the magnetic curves. In figure 25, let AB represent a
cylinder magnet, A is the marked pole and B the unmarked pole. Let PN be a
silver knife-blade resting across the magnet with its edge upward, and with its
marked or notched side towards the pole A, then, no matter what direction the
knife is moved edge first in, either around the marked or unmarked pole, the
current of electricity produced is from P to N, so long as the intersected
curves from A contact the notched side of the knife, and those from B on the
unnotched side. When the knife is moved with its back first, current flows from
N to P. Faraday explains, as if instructing a child that "A little model is
easily constructed, by using a cylinder of wood for a magnet, a flat piece for
the blade, and a piece of thread connecting one end of the cylinder with the
other, and passing through a hole in the blade, for the magnetic curves: this
readily gives the result of any possible direction." (Although I don't
understand how direction is determined readily with this kind of model, and why
not just use a real magnet? Perhaps magnets were expensive at the time?) (177)
In a wire with induced current that passes an electro-magnetic pole, the
direction of the current in the approaching wire is the same with the direction
of current in the side of the spirals nearest, and in a receding wire, the
direction of current is the reverse in the spirals nearest. (need 3D animation)
(118) All these results show that induced electric current is created by
circumferential magnetism, just as circumferential magnetism is created by
electric current. (119) These experiments show that when a piece of metal (and
the same may be true of all conducting matter) is passed before a single pole,
or between opposite poles of a magnet, or near electromagnetic poles,
electrical currents are produced across the metal transverse to the direction
of motion. In Arago's experiments, this transverse direction is in the
direction of the radii of the disc. (Interesting that not in straight lines.)
If the copper disc is viewed like a wheel with many spokes, and these spokes
rotated near the pole, each radius will have a current produced in it as it
passes the pole. (12) Now that the existence of these currents is known,
Arago's phenomena can be viewed without the need to create a magnetic pole in
the copper disk. (121) Faraday states that the effect is the same as the
electro-magnetic rotations which Faraday discovered in 1821 with the invention
of the first electric motor. (Figure 26)
If a wire PN is connected with the
positive and negative ends of a battery, so the positive electricity passes
from P to N, and a marked magnetic pole N is placed near the wire between the
wire and the viewer, the pole will move to the right, and the wire will move to
the left (as shown by the arrows). This is exactly what takes place in the
rotation of a plate beneath a magnetic pole. (Figure 27) Let N be a marked pole
above the circular plate, the plate being rotated in the direction of the
arrow. Immediately currents of positive electricity flow from the central part
in the direction of the radii by the pole to the parts of the circumference (a)
on the other side of that pole, and are therefore exactly in the same relation
to the pole as the current in the wire, and therefore the pole in the same
manner moves to the right. (122) If the rotation of the disc is reversed the
electric currents are reversed and the pole therefore moves to the left. So in
this way the direction of motion is explained. (123) Faraday states that these
currents are discharged or return in the parts of the plate on each side of and
more distant from the place of the pole where the magnetic induction is weaker,
and when collecters are applied a current of electricity is carried away to the
galvanometer, where the deflection there is merely a repetition by the same
current or part of it, of the effect of rotation in the the magnet over the
plate. (Interesting that Faraday addresses the issue of the circuit of current
when not drawn off. This applies to a permanent magnet too, where current must
flow through the center.) (126) The unusual fact that all movement stops when
the magnet and metal are stopped can now be explained because the electrical
currents that cause (and are caused by) the motion stop. (127) This also
explains the finding of Babbage and Herschel (Philosophical Transactions, 1825,
p. 481) who found that when the copper plate is cut, the power of the effect is
diminished, but when the cuts filled with metallic substances, even though
deficient in the power of influencing magnets, the power is restored. (Figure
29) Therefore if a fifth of the outside is cut off a copper plate and then
reattached with the thickness of a paper between, the magnetic currents will
greatly interfered with and the plate probably will lose much of its effect.
Faraday notes that this experiment has been performed by Mr. Christie and is
correct (Philosophical Transactions 1827, p82). (Figure 28) Faraday performs a
similar experiment: when two pieces of thick copper are connected and passed
between the poles of a magnet in a direction parallel to the center edges, a
current is urged through the wires attached to the outer angles, and the
galvanometer is strongly effected, however when a single film of paper is put
between the two copper pieces and the experiment repeated, no effect is
measured. (This would be a nice experiment to repeat.) (I don't understand 128,
"A section of this kind could not interfere much with the induction of
magnetism, supposed to be of the nature ordinarily received by iron." A section
clearly is a cut. Is Faraday claiming that cutting an iron magnet in a similar
way has no effect on the magnetic field's ability to cause current in metals?)
(129) The effect of rotation or deflection of a needle, which Arago obtained
using permanent magnets, and that Ampere obtained by using electromagnets can
be used in this experiment. By using flat spirals of copper wire, through which
electric currents are sent in place of permanent magnetic poles, Faraday is
able to measure the actual induced current of electricity from the plate itself
with the galvanometer (which was apparently too small to measure with permanent
magnets). Faraday finds this effect using a single electromagnet on one side,
and two on opposite sides. (130) The explanation for the rotation in Arago's
experiment of the production of electrical currents, seems clear for all
metals, and perhaps even other conductors, but in terms of glass, resins, and
gases for which it seems impossible that currents of electricity could be
generated in them, experiments Faraday performs convince him that any motion
effect does not happen for non-conducting materials. (132) Copper, iron, tin,
zinc, lead, mercury, and all metals tried by Faraday produce electrical
currents when passed between magnetic poles (the mercury put into a glass tube
for the purpose). The dense carbon placed in coal gas retorts also produce
current, but ordinary charcoal does not. Faraday finds no current in salt
water, sulphuric acid, saline solutions, whether rotated in basin or includes
in tubes and passed between the poles. (133) Faraday states that he has never
been able to produce any sensation on his tongue, heat a fine plantinum wire,
produce a spark, or convulse the limbs of a frog from the electric current
produced through the conductors on the edges of the rotating metal plate. (The
current and voltage must be very small.) (Wasn't Faraday able to feel
electricity and create a spark with the copper disk with both permanent and
electric magnets? Clearly Faraday did measure current with the Galvanometer.)
(134) Faraday states the the electric current in the rotating copper plate only
occupies a small space, moving by the poles and being discharged right and left
at very small distances, but even so, large currents can be drawn off that are
strong enough to pass through narrow wires even 100 feet long; it is evident
that the current existing in the plate itself must be a very powerful one when
the rotation is rapid and the magnet strong. This is also proved by how a
magnet 12 pounds in weight follows the motion of the plate and twists up the
cord from which the magnet is suspended. (135) Faraday makes 2 rough trials
with the intention of constructing magneto-electric (magnet-electric) machines.
In one, a ring cut from a thick copper plate, 1.5 inches wide and 12 inches in
external diameter is mounted to rotate between the poles of a magnet. The inner
and outer edges are amalgamated (covered with mercury?), and the conductors
applied, one to each edge, at the place of the magnetic poles (so that the disk
slides over the stationary conductors). The current evolved does not appear to
be stronger than the current created by the circular plate. (136) In the second
trial, a small thick disk of copper or other metal, half an inch in diameter
are rotated rapidly near the poles, but with the axis of rotation out of the
polar axis. The electricity evolved is collected by conductors applied to the
edges. Currents are created but far smaller than the currents produced by the
circular plate. (137) This last experiment is analogous to those made by Mr.
Barlow with a rotating iron shell, subjected to the magnetic field of the
Earth. (Philosophical Transactions, 1825, p. 317) Messrs. Babbage and Herschel
give the same explanation to the effects of Barlow's experiment as they do for
Arago's experiment. (Philosophical Transactions, 1825, p.485) (Did Barlow
produce a sustained or temporary current from the Earth's magnetic field?)
Faraday notes that the rotation of a copper shell might decide the point and
even throw light on the more permanent, although analogous effects obtained by
Mr. Christie. (138) Faraday uses an iron plate in place of the copper plate
(101) which is passed between the magnetic poles. While the experiments on the
induction of electric currents (9) show no difference between iron and other
metals, the iron plate produces less power than the copper plate in the
rotating plate experiment. Faraday states that with iron, the larger part of
the effect is due to ordinary magnetic action, and that there is no doubt that
Babbage's and Herschel's explanation of Arago's phenomenon is true when iron is
the metal used. (So an opposite magnetic pole is created in the iron disk?)
(139) Faraday comments that Mr. Harris found that bismuth and antimony effect a
suspended magnet disproportionately to their conducting power, but that Faraday
has been able to explain these differences and prove with several metals, the
the effect is based on the order of the conducting power, because Faraday has
produced currents of electricity that are proportionate in strength to the
conducting power of the bodies experimented with.
(Royal Institution in) London, England  
169 YBN
[1831 AD]
2414) Robert Brown (CE 1773-1858) identifies and names the cell "nucleus".

While dealing with the fertilization of flowers, Brown notes the existence of a
structure within the cells of orchids as well as many other plants that brown
terms the "nucleus" of the cell (from the Latin word meaning "little nut").

This description is embedded in a pamphlet which focuses on the sexual organs
of orchids.
London, England (presumably)  
169 YBN
[1831 AD]
2496)
Stokholm, Sweden (presumably)  
169 YBN
[1831 AD]
2608) William C. Redfield (CE 1789-1857), publishes his evidence that storm
winds rotate counterclockwise about a center that moves in the direction of the
prevailing winds. (I think hurricanes rotate counterclockwise in the northern
hemisphere and clockwise in the Southern hemisphere?)

New York, USA (presumably)  
169 YBN
[1831 AD]
2625)
London, England (presumably)  
169 YBN
[1831 AD]
2629) John Frederic Daniell (CE 1790-1845) invents a pyrometer (a device for
measuring relatively high temperatures, such as found in furnaces) Phil.
Trans., 1830). (describe design)
Daniell receives the Rumford Medal of the Royal
Society (in 1832) for his invention of a pyrometer and his papers detailing the
uses for the pyrometer.
London, England (presumably)  
169 YBN
[1831 AD]
2809)
Albany, NY, USA  
169 YBN
[1831 AD]
2889)
(University of Bonn) Bonn, Germany  
169 YBN
[1831 AD]
2895) When little more than 20 years old, Boussingault goes to South America as
a mining engineer on behalf of an English company.
During the insurrection of the
Spanish colonies Boussingault is attached to the staff of General Bolivar, and
travels widely in the northern parts of the continent.
Boussingault is professor of
chemistry at the University of Lyon, and professor of agricultural chemistry at
the Conservatory of Arts and Crafts, Paris (1839-1887).
Lyon, France (presumably)  
169 YBN
[1831 AD]
2919) While in Paris, working under Joseph-Louis Gay-Lussac (1822-1824), Liebig
investigates the dangerous explosive silver fulminate, a salt of fulminic acid.
At the same time, the German chemist Friedrich Wöhler is analyzing cyanic
acid. Liebig and Wöhler realize that cyanic acid and fulminic acid represent
two different compounds that have the same composition, the same number and
kind of atoms, but have different chemical properties. The Swedish chemist,
Jöns Jacob Berzelius refers to such compounds as isomers (from the Greek words
meaning "equal parts"). This shared finding leads to a lifelong friendship and
collaborative research partnership between Liebig and Wöhler.

This finding of isomers shows that the molecule of a compound is more than a
(singular) collection of atoms, but that these atoms have particular (three
dimensional) positions. Kekulé will create a structural formula for molecules.


Liebig creates a laboratory for general student use.

Liebig succeeds in institutionalizing the independent teaching of chemistry,
which German universities had been taught as an adjunct to pharmacy for
apothecaries and physicians.

Liebig determines the oxygen content of the air by quantifying its adsorption
in an alkaline solution of pyrogallol (benzene-1,2,3-triol). (chronology)
Liebig is the son
of a pigment and chemical manufacturer whose shop has a small laboratory.
Liebig publishes
an average of 30 papers a year between 1830 and 1840.
In 1832 Liebig takes over the
"Annalen der Pharmacie" ("Annals of Pharmacy") and renames it in 1840 the
"Annalen der Chemie" ("Annals of Chemistry").
At Giessen, Liebig produces chloroform and
chloral, and discovers hippuric acid.
So many students are drawn to Liebig that he
has to expand his facilities and systematize his training procedures. A
considerable number of his students, some 10 per semester, are from other
nations.
Liebig's former laboratories in Giessen are now the Liebig Museum.
(University of Giessen), Giessen, Germany  
169 YBN
[1831 AD]
2992)
Pavia, Italy (possibly)  
168 YBN
[01/03/1832 AD]
2808)
Albany, NY, USA  
168 YBN
[06/08/1832 AD]
2747) Charles Babbage (CE 1792-1871), English mathematician, publishes
"Economy of Machines and Manufactures" (1832) which is the result of Babbage's
travels through several of the countries of Europe, examining different systems
of machinery. In this work, Babbage describes what is now called the Babbage
principle, which describes certain advantages with division of labor. Babbage
notes that highly skilled, and therefore generally higher paid, workers spend
parts of their job performing tasks that are 'below' their skill level. If the
labor process can be divided among several workers, it is possible to assign
only high-skill tasks to high-skill and high-cost workers and leave other
working tasks to less-skilled and paid workers, which lowers labor costs. This
principle is criticized by Karl Marx who argues that it causes labor
segregation and contributes to alienation. The Babbage principle is an inherent
assumption in Frederick Winslow Taylor's scientific management. (I think the
differences between high and low skill are many times hard to define. It seems
clear that walking robots will fill low skill jobs first, such as picking
fruit, order taking, food serving, cleaning, driving, grocery shopping,
filming, and this would imply that any job which a robot cannot perform is a
higher skill job. We are heading to a society where walking robots perform
almost all of the work, while humans and other species live off the products of
that work. I see full and constant democracy as the future of government and
society. The hope is that the majority will be well informed and educated and
form a civilization full of pleasure and freedom and free of pain and
violence.)

In this work Babbage publishes his finding that the cost of collecting and
stamping a letter for various sums depending on the distance it is to travel
costs more in labor than using some small sum charged independently of
distance. The British government will adopt this practice in 1840.

Cambridge, England (presumably)  
168 YBN
[07/??/1832 AD]
2807)
Albany, NY, USA  
168 YBN
[10/??/1832 AD]
3002) Hamilton describes the confirmation of conical refraction:
"After making
this communication
to the Academy, in October, 1832, I requested Professor Lloyd to examine
the question
experimentally, and to try whether he could perceive any such phenomena in
biaxial crystals,
as my theory of conical refraction had led me to expect. The
experiments of Professor Lloyd,
confirming my theoretical expectations, have
been published by him in the numbers of the
London and Edinburgh Philosophical
Magazine, for the months of February and March, 1833;
and they will be found with
fuller details in the present Volume of the Irish Transactions."


In this paper, Hamilton changes from his earlier neutrality to support the wave
theory: Hamilton writes: " The latter theory was deduced, by my general
methods, from the hypothesis of transver-
sal vibrations in a luminous ether, which
hypothesis seems to have been first proposed by
Dr. Young, but to have been
independently framed and far more perfectly developed by
Fresnel; and from
Fresnel"s other principle, of the existence of three rectangular axes of
elasticity
within a biaxal crystallised medium. The verification, therefore, of
this theory of
conical refraction, by the experiments of Professor Lloyd, must be
considered as affording a
new and important probability in favour of
Fresnel"s views: that is, a new encouragement
to reason from those views, in combining and
predicting appearances."

(Interesting that a single material can have more than one index of refraction.
To me this implies that refraction has to do with crystal and or molecular
structure (and shape) and less to do with kind of material (atom or molecule).
Who first found this?)
(Trinity College, at Dunsink Observatory) Dublin, Ireland  
168 YBN
[12/15/1832 AD]
2448)
Göttingen, Germany (presumably)  
168 YBN
[1832 AD]
2514) Plastic. (Nitrocellulose).

Braconnet creates a flammable product he names "xyloidine" by treating starch,
sawdust, and cotton with nitric acid. Braconnot finds that this material is
soluble in wood vinegar and attempts to make coatings (varnish), films, and
shaped articles from it. (What kind of shaped articles? Solid-plastic
objects?)

This substance may be considered the first polymer or plastic material created
by a chemist.

Henri Bracconet is the first to prepare cellulose nitrate in 1833, by mixing
sawdust cellulose with nitric acid. In 1855 Christian Schönbein, a professor
at Basel University, copies Bracconet's method in treating simple paper made
from wood cellulose with nitrite acid. The result is a transparent, highly
flammable substance, which Schönbein names "cellulose nitrate" and markets as
an explosive. Parkes will use cellulose nitrate as the basis of Parkesine, an
early plastic.
Nancy, France  
168 YBN
[1832 AD]
2528)
Surrey, England (presumably)  
168 YBN
[1832 AD]
2623)
Tilgate Forest, England  
168 YBN
[1832 AD]
2659)
St. Petersburg, Russia  
168 YBN
[1832 AD]
2704) The quantity of electricity required to liberate 23 grams of sodium, or
108 grams of silver, or 32 grams of copper, in other words to liberate the
"equivalent weight" (named by Wollaston) of an element, is named the Faraday.

Faraday invents the voltameter, a device for measuring electrical charges,
which was the first step toward the later standardization of electrical
quantities. The voltameter is not to be confused with the voltmeter which
measures electric potential. The voltameter measures quantity of electricity.
The voltameter is an electrolytic cell and the measurement is made by weighing
the element deposited or released at the cathode in a specified time.
(Royal Institution in) London, England  
168 YBN
[1832 AD]
2717) Antoine-Hippolyte Pixii lives a very short life, only 27 years.
Paris, France  
168 YBN
[1832 AD]
2718) Antoine-Hippolyte Pixii lives a very short life, only 27 years.
Paris, France  
168 YBN
[1832 AD]
2740)
Cambridge, England (presumably)  
168 YBN
[1832 AD]
2773) Nitrobenzene is a poisonous organic compound, C6H5NO2, either bright
yellow crystals or an oily liquid, having the odor of almonds and used in the
manufacture of aniline, insulating compounds, and polishes.
(University of Berlin) Berlin, Germany  
168 YBN
[1832 AD]
2775) John Wycliffe (WIKLIF) (c1330-1384), English theologian, and church
reformer initiates the first complete translation of the Bible into English.

The New Testament seems to have been completed about 1380, the Old Testament
between 1382 and 1384. Exactly how much of it was done by Wyclif's own hand is
uncertain.

About 30 copies of this book have survived. Some are large folio volumes,
written and illuminated in the style of the period. Others are plain copies of
ordinary size, intended for private persons or monastic libraries. Clearly, in
spite of official disfavor and eventual prohibition, Wycliff's Bible is welcome
in many places in England.

Wycliff dies on December 31, 1384 and is buried, but on May 4, 1415 by a decree
of the council of Constance, Wycliff's remains are ordered to be dug up and
burned, an order which is carried out, at the command of Pope Martin V, by
Bishop Fleming in 1428.
Wycliff writes a political treatises on divine and civil
dominion "De dominio divino libri tres and Tractatus de civili dominio", in
which Wycliff states that, as the church is in sin, the church should give up
its possessions and return to evangelical poverty.

Wycliff criticizes the belief in transubstantiation, that the substance of the
bread and wine used in (religious ceremony) is changed into the body and blood
of Christ. As a Realist philosopher, Wycliff criticizes this belief because in
the destruction of the bread and wine, the end of being is involved.

In May 1382, at the synod held at Blackfriars, London, many of his Wycliff's
works are condemned. At Oxford Wycliff's (supporters) also give in, and all
Wycliff's writings are banned.

As an example of the english of this time Wycliff's Bible begins:
"1 In the bigynnyng
God made of nouyt heuene and erthe.
2 Forsothe the erthe was idel and voide, and
derknessis weren on the face of depthe; and the Spiryt of the Lord was borun on
the watris.
3 And God seide, Liyt be maad, and liyt was maad.
4 And God seiy the liyt, that
it was good, and he departide the liyt fro derknessis; and he clepide the
liyt,
5 dai, and the derknessis, nyyt. And the euentid and morwetid was maad, o
daie."


According to the Columbia Encyclopedia, this first and literal translation of
the Latin Vulgate Bible into English is mainly the work of Wycliff's followers,
notably Nicholas Hereford; the smoother revision of c.1395 is directed by
Wyclif's follower John Purvey. In England the Lollards form the link between
Wyclif and the Protestant Reformation. On the Continent Wycliff is a chief
forerunner of the Reformation, through his influence on Jan Huss, the Bohemian
reformer, and through Huss on Martin Luther and the Moravians.
Wycliffe received his
formal education at Oxford University.
In 1361 Wycliff is made rector at Fillingham.
In 1368 Wycliff is
rector at Ludgershall.
In 1369 Wycliffe earns a bachelor of divinity. (presumably from
Oxford)
In 1372 Wycliffe earns a doctor of divinity.
In 1374 Wycliff is rector at Lutterworth.
Wycliff's early
associates himself with the anticlerical party in the nation.
In 1374 Wycliff is sent
to Bruges to represent the English crown in negotiations over payment of
tribute to the Holy See.(notice "Holy See" from Columbia.)
From 1377 Wycliff makes many
vigorous attacks in both Latin and English on orthodox church doctrines,
especially that of transubstantiation. Through his own preaching in the
vernacular at Oxford and London and the teaching of his "poor priests", Wycliff
spreads the doctrine that the Scriptures are the supreme authority over the
church. Wycliff is condemned as a heretic in 1380 and again in 1382, and
Wycliff's followers are persecuted, but Wycliff is not disturbed in his
retirement at Lutterworth, where he dies in 1384.
Oxford, England  
168 YBN
[1832 AD]
2849) Cymene is any of three colorless isomeric liquid hydrocarbons, C10H14,
obtained chiefly from the essential oils of cumin and thyme and used in the
manufacture of synthetic resins.

Cymene is a naturally occurring aromatic organic compound.

Anthrecene, C14H10, is a solid organic compound derived from coal tar.
The molecular
structure of anthracene consists of three benzenelike rings joined side by
side; it is therefore an aromatic compound. Cymene is the first member of the
anthracene series, a group of aromatic hydrocarbons that are structurally
related to it and have the general formula CnH2n−18.
(Ecole Polytechnique) Paris, France (presumably)  
168 YBN
[1832 AD]
2860)
(Berlin Gewerbeschule (trade school)) Berlin, Germany (and (University of
Giessen), Giessen, Germany)  
168 YBN
[1832 AD]
2925) (Baron) Justus von Liebig (lEBiK) (CE 1803-1873), German chemist
discovers chloral, a sedative/hypnotic substance.

(University of Giessen), Giessen, Germany  
168 YBN
[1832 AD]
2947) Carl Gustav Jacob Jacobi (YoKOBE) (CE 1804-1851), German mathematician
discovers hyperelliptic functions.

Jacobi shows that just as elliptic functions can be obtained by inverting
elliptic integrals, hyperelliptic functions can also be obtained by inverting
hyperelliptic integrals.

This thinking leads Jacobi to the theory of Abelian functions, which are
complex functions of several variables. (more info)

(University of Königsberg) Königsberg, Germany  
168 YBN
[1832 AD]
3046) Joseph Liouville (lYUVEL) (CE 1809-1882), French mathematician, creates
his theory of integration in finite terms (1832â€"33). The main goals of
Liouville's work in this period is to decide whether given algebraic functions
have integrals that can be expressed in finite (or elementary) terms.
In analysis
Liouville is the first to deduce the theory of doubly periodic functions
(functions with two distinct periods whose ratio is not a real number) (what
are doubly periodic functions whose two periods ration is real called?) from
general theorems (including his own) (Liouville's theorem) in the theory of
analytic functions of a complex variable (also known as holomorphic functions
or regular functions; a complex-valued function defined and differentiable over
some subset of the complex number plane). (See for related info)

In 1836 Liouville founds and becomes editor of the "Journal des Mathématiques
Pures et Appliquées" ("Journal of Pure and Applied Mathematics").

Altogether, Liouville's publications comprise about 400 memoirs, articles, and
notes.
(École Polytechnique) Paris, France  
168 YBN
[1832 AD]
3343)
(Institut Gaggia) Brussels, Belgium  
168 YBN
[1832 AD]
3910)
Padua, Italy (verify)  
167 YBN
[07/07/1833 AD]
2931) Asimov describes Lenz as being third in investigating electrical
induction behind Faraday and Henry.
(University of St. Petersburg) St. Petersberg, Russia (presumably)  
167 YBN
[11/29/1833 AD]
2932) Lenz's law must be taken into account in the design of electrical
equipment.
(University of St. Petersburg) St. Petersberg, Russia (presumably)  
167 YBN
[1833 AD]
2449) Much of electricity and in particular the telegraph marks a major turn to
secrecy in science, perhaps because of the nature of using technology to record
the private message of people without their knowledge, and the strategic use
that may provide.
(University of) Göttingen, Germany  
167 YBN
[1833 AD]
2555) William Beaumont (BOmoNT) (CE 1785-1853), American surgeon publishes
"Experiments and Observations on the Gastric Juice and the Physiology of
Digestion" (1833), in which Beaumont lists 238 experiments that he does on a
person who survives a gunshot wound that leaves a hole (a fistula) into his
stomach. Beaumont suggests using artificial fistulas (holes) in animals for
further research.
Beaumont is a US Army surgeon.
Alexis St. Martin, a 19-year-old French-Canadian
trapper has a wound from a shotgun blast. As a result of the healing of the
wound, a gastric fistula, or passage, remains which, when pressed with the
finger allows Beaumont to see the activities occurring within St. Martin's
stomach.
Washington DC, USA  
167 YBN
[1833 AD]
2578)
(Breslau, Prussia now:)Wroclaw, Poland  
167 YBN
[1833 AD]
2772) Eilhardt Mitscherlich (miCRliK) (CE 1794-1863), German chemist names
Benzene, after producing it using the distillation of benzoic acid (from gum
benzoin) and lime. Mitscherlich gives the compound the name "benzin".

(University of Berlin) Berlin, Germany  
167 YBN
[1833 AD]
2786)
Paris, France (presumably)  
167 YBN
[1833 AD]
2850) Urethane is a colorless or white crystalline compound, CO(NH2)OC2H5, used
in organic synthesis.

Urethane is not a component of polyurethanes.
(Ecole Polytechnique) Paris, France (presumably)  
167 YBN
[1833 AD]
2901)
(King's College) London, England  
167 YBN
[1833 AD]
2906)
Royal Military Academy, Woolwich, England  
167 YBN
[1833 AD]
2935) (Sir) Richard Owen (CE 1804-1892), English zoologist publishes "Memoir on
the Pearly Nautilus" (London, 1832).

Owen discovers the pearly nautilus which is a mollusk.

In the late 1830s(chronology), Owen distingushes between 'homology' and
'analogy'. Homology is any similarity between characters that is due to their
shared ancestry. An example is that ovaries and testicles are homologous; they
evolve through the same pathway. Analogy is similar structures which evolved
through different developmental pathways, in a process known as convergent
evolution. An example is that the wings of insects, birds and bats are
analogous; they perform the same function but evolved through different
pathways.

Owen is the first to identify the recently extinct moas of New Zealand.

Owen is the first to describe the sponge "Venus' flower basket" or Euplectella
(1841, 1857).
Owen refuses knighthood in 1842 but accepts in 1884.
Owen shows aggressive
animosity for the theory of evolution by natural selection.
Owen writes a very long
anonymous review of Darwin's "Origin of Species" (The Edinburgh Review, 1860)
to discredit Darwin.
(Hunterian museum of the Royal College of Surgeons) London, England  
167 YBN
[1833 AD]
2941) (Sir) Richard Owen (CE 1804-1892), English zoologist publishes
"Descriptive and Illustrated Catalogue of the Physiological Series of
Comparative Anatomy" (5 vol., 1833-40) which is considered to be Owen's
monumental work.

(Hunterian museum of the Royal College of Surgeons) London, England  
167 YBN
[1833 AD]
3003) Lloyd writes: "Here then are two singular and unexpected consequences of
the undulatory theory, not
only unsupported by any phaeomena hitherto noticed, but
even opposed to all the analogies
derived from experience. If confirmed by experiment,
they would furnish a new and almost
convincing proof of the truth of that theory; and
if disproved, on the other hand, it is evident
that the theory must be abandoned or
modified.
Being naturally anxious to submit the theory of waves to this delicate
test, and to ascer-
tain how far these new theoretical conclusions were in accordance
with actual phaenomena,
Professor Hamilton requested me to undertake a series of
experiments with that view. I ac-
cordingly applied myself to this experimental
problem with all the attention which the subject
so well deserved, and have fortunately
succeeded in verifying the first-mentioned species of
conical refraction. I hope
before long to be able to make similar researches on the second*.

The editor comments: "to this direction was made by subsequent trial. The
phaenomenon which presented itself,
* Since we received this paper, we have been
informed by the author that he has now
observed phaenomena corresponding to the
second species of conical refraction, and of which
an account will be given in our
next Number. -Edit."

Lloyd continues: " The mineral I employed in these experiments was
arragonite, which I selected partly on
account of the magnitude of the cone which
theory indicated in this instance, and partly
because the three elasticities in this
mineral have been determined, apparently with great
care, by Professor Rudberg, and
therefore the results of theory could be applied to it at once
without further
examination. The specimen I used was one of considerable size and purity,
procured for
me by Mr. Dollond, and cut with its parallel faces perpendicular to the line
bisectin
g the optic axes. If we suppose a ray of common light to pass in both
directions out
of such a crystal, along the line connecting the two cusps in the
wave, it is evident that it
must emerge similarly at both surfaces: consequently
the ray which passes along this line, and
forms a diverging cone of rays at
emergence at the second surface of the crystal, must arise
from a converging cone
incident upon the first surface. Having therefore nearly ascertained
the direction of the
optic axis by means of the rings, I placed a lens of short focus at the
distance of
its own focal length from the first surface, and in such a position that the
central
rays of the pencil might after refraction pass along the axis. Then looking
through the crystal
at the light of a lamp placed at a considerable distance, I
observed, in the expected direction, a
point more luminous than the space
immediately about it, and surrounded by something like
a stellar radiation. Fearing
that this appearance might have arisen from some imperfection
in the crystal, I examined it
with polarized light, and was happy to find the system of rings
in the same
direction. This was afterwards confirmed by numerous observations on different
parts of
the crystal."

(Perhaps using a lens causes the circular outline. This must be the proof of
the first claim by Hamilton that the incident in the shape of a cone with the
point reaching the surface will be refracted as a cylinder. I think this theory
is based strictly on a transverse wave, and cannot fit an equivalent particle
interval beam, and therefore seems doubtful in my mind.)

Lloyd publishes "Elementary Treatise on the Wave-theory of Light" in 1857 and a
second edition in 1873.

In this work Lloyd describes how crystalline bodies are divided into 3 classes,
with respect to their action of light:
"I Single refracting crystals
II Uniaxal crystals or
those which have one axis of double refraction
III Biaxal crystals or those
which have two such axes"

In this work Lloyd gives his account of confirming the two theoretical
refractions:
"Being naturally anxious to submit the wave theory to this test and to
establish or disprove its new results Sir William Hamilton requested the author
to examine the subject experimentally. The result of this examination has been
to prove the existence of both species of conical refraction. The first case of
conical refraction is that called by Sir William Hamilton external conical
refraction
and was expected to take place as we have seen when a single ray
passes within the crystal in the direction of either of the lines of single ray
velocity
. These lines coincide nearly but not exactly with the optic axes of
the crystal, and in the case of arragonite, the crystal submitted to experiment
contain an angle of nearly 20degrees. The plate of arragonite employed has its
faces perpendicular to the line bisecting the optic axes, consequently the
lines above mentioned were inclined to the perpendicular at an angle of about
10degrees on either side. Let these lines be represented by OM and ON, equally
inclined to the perpendicular OP. A ray of common light traversing the crystal
in the direction OM or MO should emerge in a cone of rays as represented in the
figure, the angle of this cone depending on the relative magnitude of the three
elasticities of the crystal a2 b2 c2. In the case of arragonite this angle is
considerable and amounts to 3degrees very nearly.
A thin metallic plate perforated
with a very minute aperture was placed on each face of the crystal and these
plates were so adjusted that the line connecting the two apertures should
coincide with the line MO or any parallel line within the crystal. The flame of
a lamp was then brought near one of the apertures, and in such a position that
the central part of the beam converging from its several points to the aperture
should have an incidence of 15 or 16degrees. When the adjustment was completed
a brilliant annulus of light appeared on looking through the aperture in the
second surface. (see image) When the aperture in the second plate was ever so
slightly shifted so that the line connecting the two apertures no longer
coincided with the line MO, the phenomenon rapidly changed and the annulus
resolved itself into two separate pencils.
The incident converging cone was also formed
by a lens of short focus placed at the distance of its own focal length from
the surface, and in this case the lamp was removed to a distance and the plate
on the first surface dispensed with. The same experiments were repeated with
the sun's light and the emergent rays were even thrown on a screen and thus the
section of the cone observed at various distances from its summit.
...
The rays that compose the emergent cone are all polarized in different planes.
It was discovered by observation that these planes are connected by the
following law; namely the angle between the planes of polarization of any two
rays of the cone is half the angle between the planes containing the rays
themselves and the axis
. This law was found to be in accordance with theory.
...
(191) The other case of conical refraction called internal conical refraction
by Sir William Hamilton was expected to take place when a single ray has been
incident externally upon a biaxal crystal in such a manner that one of the
refracted rays may coincide with an optic axis (see image). The incident ray in
this case should be divided into a cone of rays within the crystal the angle of
which in the case of arragonite is equal to 1degree 55'. The rays composing
this cone will be refracted at the second surface of the crystal in directions
parallel to the ray incident on the first so as to form a small cylinder of
rays in air whose base is the section of the cone made by the surface of
emergence. This is represented in the annexed diagram in which NO is the
incident ray, aOb the cone of refracted rays within the crystal and aa'b'b the
emergent cylinder.
The minuteness of this phenomenon, and the perfect accuracy
required in the incidence, rendered it much more difficult to observe than the
former. A thin pencil of light proceeding from a distant lamp was suffered to
fall upon the crystal, and the position of the latter was altered with extreme
slowness, so as to change the incidence very gradually. When the required
position was attained, the two rays suddenly spread out into a continuous
circle whose diameter was apparently equal to their former interval. The same
experiment was repeated with the sun's light, and the emergent cylinder was
received on a small screen of silver paper at various distances from the
crystal, and no sensible enlargement of the section was observable on
increasing the distance. The angle of this minute cone within the crystal was
found to agree within very narrow limits with that deduced from theory the
observed angle being 1degree 50' and the theoretical angle 1 degree55'.
The
rays composing the internal cone are all polarized in different planes and the
law connecting these planes is the same as in the case of external conical
refraction."

(My own feeling about double refraction is that (see video) light is reflected
off the crystal plane and this reflected beam causes the second extraordinary
beam being refracted differently after reflection. The example is holding a
plate of glass, such as a slide, and shining a laser beam through it, and
turning the glass slide to see the "extraordinary image" rotate with the slide.
In fact, there may be many surfaces that reflect light inside crystals.)
Lloyd is a
reverend.
(Trinity College) Dublin, Ireland  
167 YBN
[1833 AD]
3004) (Sir) William Rowan Hamilton (CE 1805-1865) publishes "On a General
Method of Expressing the Paths of Light and of the Planets by the Coefficients
of a Characteristic Function" (1833), in which Hamilton attempts to apply his
characteristic function, based on the principle of least action, to mechanics
as well as to light.

(Trinity College, at Dunsink Observatory) Dublin, Ireland  
167 YBN
[1833 AD]
3014) Prior to 1833 when Graham published his work on phosphate compounds, it
was thought that there were two forms of phosphoric acid which produced a
variety of salts. The common form, what we now know is Na2HPO4, gave a yellow
precipitate with silver nitrate and left the solution acidic. The second form
resulted from heating the phosphate salt (Na2HPO4) above 350 degrees C. This
form gave a white precipitate with silver nitrate and a neutral solution.
Graham finds that when crystals of the neutral phosphate are heated, all but
one of the water molecules in the crystal are readily lost (these are the water
of hydration) and the last unit of water is not lost until the temperature is
much higher. The salt that is formed from the pyrophosphate gives the white
precipitate with silver nitrate. The difference between the two phosphate salts
is the one water molecule. Graham then concludes that the water might play the
role of a base in a salt. Continuing in this way Graham determines that there
are really three phosphate salts of sodium (Na3PO4, Na2HPO4, NaH2PO4) as well
as sodium pyrophosphate (Na4P2O7) and sodium metaphosphate (NaPO3).(needs
visual)
(Andersonian Institution) Edinburgh, Scotland  
167 YBN
[1833 AD]
3026) This book is produced with 1,000 francs of financial help from Alexander
von Humboldt, who Asimov describes as the dean of Europe's scientists.

Turning his attention to other extinct animals found with the fishes, Agassiz
publishes in two volumes on the fossil echinoderms of Switzerland (from
1838�42), and later "�tudes critiques sur les mollusques fossiles"
(from 1841�42).

Agassiz's "Contributions to the Natural History of the United States" (4 vols.
1857â€"62) remains uncompleted at his death.
A monograph on the fishes of Brazil
brings Agassiz to the attention of Georges Cuvier. Cuvier supported
catastrophism, and neptunism rejecting Larmarck's theory of evolution. The
supporters of catastrophism seek to try to accommodate the inaccurate creation
story of the Christian Bible, where all species are created at one time.
Agassiz
does not accept Darwin's view of a gradual evolution of species, but, like
Cuvier, considers that there have been repeated separate creations and
extinctions of species, this theory explaining changes and the appearance of
new forms. Agassiz, supporting the theory of catastrophism, views ice ages as
catastrophes (which they were for many species). Agassiz imagines as many as 20
repeated creations.

In 1836 the Wollaston medal is awarded to Agassiz for his work on fossil
ichthyology.

Agassiz pronounces that there are several species of humans, an argument used
by pro-slavery supporters to justify their subjugation of Negroid people as an
inferior species. Asimov states that Agassiz is "firmly convinced of the
inherent inferiority of blacks". This view, that a race of humans is somehow
inferior to another race is erroneous and elitist in my opinion.

Agassiz is the most prominent biologist in the USA to oppose evolution.

In 1859 as professor of zoology and geology at Harvard, Agassiz establishes the
Museum of Comparative Zoology.

(It is difficult when people with bad ethics have contributions to science. The
contributions we love, but their ethics we do not. Such is the case with Louis
Alvarez with his support for the fraudulent single-bullet theory, and numerous
others, even Darwin wrongly believed the Negroid race to be inferior to the
Caucasian race. The history of science is filled with people making science
contributions that have terrible or shockingly inaccurate beliefs or ethics.
What is clear to me is that accurate truths should be accepted no matter how
unpleasant the source, because truth exists independently of the source of
information, something is either true or false based only on physical evidence,
not based on the ethics of the person making the scientific claim. Although,
certainly, poor ethics, a history of dishonesty and/or inaccurate views,
certainly does and no doubt should, effect a person's willingness to explore
the claims of people who are consistently dishonest or inaccurate.)
(University of Neuch�tel) Neuch�tel, Switzerland  
167 YBN
[1833 AD]
3027) Arnold Henry Guyot (GEO) (CE 1807-1884), the person whom Harry Hammond
Hess names flat-topped sea mountains for, studies the structure and movement of
glaciers in Switzerland, spending time testing the new theories of Louis
Agassiz.
(University of Neuch�tel) Neuch�tel, Switzerland  
167 YBN
[1833 AD]
3393) Walter Hancock's (CE 1799-1852) steam bus ("The Enterprise").
By this time several
steam coaches drive the roads in England.

London, England  
167 YBN
[1833 AD]
5989) Of a distinguished intellectual, artistic and banking family in Berlin,
Mendelssohn grows up in a privileged environment (the family converts from
Judaism to Christianity in 1816, taking the additional name "Bartholdy").(Is
seems to me absurd to have a religion, to change religion, or to change your
name when you change religion. But those are all, of course, personal
nonviolent activities that people must be allowed.)

Fanny Mendelssohn Hensel, Felix's older sister, also composes music.
London, England  
166 YBN
[01/01/1834 AD]
1247) Mechanical reaper.


A reaper is any farm machine that cuts grain. Early reapers simply cut the crop
and drop it unbound, but modern machines include harvesters, combines, and
binders, which also perform other harvesting operations.

Cyrus McCormick builds a practical mechanical harvester.

The Roman historian Pliny the Younger (62-113 CE) describes a harvesting
machine that is in use by Celtic people in Gaul in 100 CE, but this machine is
not adapted elsewhere and seems to disappear from use after the year 500.

A patent for a reaper was issued in England to Joseph Boyce in 1800. In 1826
Patrick Bell builds a plane reaper which cuts and gathers wheat with serrated
rotary blades. In the 1830s Jeremiah Bailey of the United States patents a
mower-reaper, and Obed Hussey and Cyrus McCormick both develop reapers with
guards and reciprocating (back-and-forth-moving) cutting blades. McCormick’s
reaper has the several advantages over Hussy's in having a divider to separate
cut and standing grain and a revolving reel to topple the cut grain onto the
rear of the machine, where it can be raked off onto the ground and later tied.
Robert McCormick attempts to build an automatic horse-drawn reaper that can be
mass produced, but abandons the project. However, Robert inspired his son Cyrus
(1809-1884) who invents a practical mechanical harvester in 1831 and patents it
in 1834.

(Note that all moving parts are driven by the movement of the wheel on the
ground, pulled by the horses. Imagine cutting grain by hand with a scythe. In
the future walking robots will probably do almost all the work required in
planting, growing, harvesting, packaging and distributing food to humans.
Walking robots and tiny machines may even target insects that feed on plants
meant for humans.)
Rockbridge County, Virginia, USA  
166 YBN
[1834 AD]
2497) Jöns Jakob Berzelius (BRZElEuS) (CE 1779-1848) reports finding organic
matter, "humic acid", in a meteorite, in "Annalen der physikalisches Chemie".
Such meteorites are called "carbonaceous chondrites".

Stokholm, Sweden (presumably)  
166 YBN
[1834 AD]
2539) Asimov comments that around this time astronomers are moving from
exploring the solar system as Laplace and others had done, and exploring the
outer stars.
Königsberg, (Prussia now:) Germany  
166 YBN
[1834 AD]
2557)
london, England (presumbly)  
166 YBN
[1834 AD]
2570)
Rhône River valley, Switzerland  
166 YBN
[1834 AD]
2622) Gideon Mantell (maNTeL) (CE 1790-1852) buys the skeleton for £25.
Sussex, England (presumably)  
166 YBN
[1834 AD]
2741) In 1842, following repeated failures to obtain funding from the First
Lord of the Treasury, Babbage approaches Sir Robert Peel for funding. Peel
refused, and offers Babbage a knighthood instead which Babbage refuses. Babbage
continues to modify and improve the design of his Analytical Engine for many
years to come.

The principles of the Analytical Engine will be later realized electronically.

It is interesting to think about the electrical engineers perspective on this
clearly all mechanical approach, as clearly electric computers will evolve from
these early mechanical machines. With the invention of walking robots, there is
an integration of electronics (and the nervous system) and mechanical design
(as the muscular system).
Cambridge, England (presumably)  
166 YBN
[1834 AD]
2758) Lovelace has been called the first computer programmer.

Mathematics for Lady Byron, Ada Byron's mother, is first a mode of moral
discipline. Accordingly, Lady Byron arranges a full study schedule for her
child, emphasizing music and arithmetic-music to be put to purposes of social
service, arithmetic to train the mind.
Lovelace goes against traditional Victorian
society by studying mathematics which is a (skill) few women attempt.


Biographers debate the extent of Lovelace's original contributions, with some
holding that the programs were written by Babbage himself. Babbage writes in
his "Passages from the Life of a Philosopher" (1846):
"I then suggested that she add
some notes to Menabrea's memoir, an idea which was immediately adopted. We
discussed together the various illustrations that might be introduced: I
suggested several but the selection was entirely her own. So also was the
algebraic working out of the different problems, except, indeed, that relating
to the numbers of Bernoulli, which I had offered to do to save Lady Lovelace
the trouble. This she sent back to me for an amendment, having detected a grave
mistake which I had made in the process. The notes of the Countess Lovelace
extend to about three times the length of the original memoir. Their author
entered fully into almost all the very difficult and abstract questions
connected with the subject."

Lovelace labels her seven "Notes" with the letters A through G.

"Note A" distinguishes between Babbage's Difference Engine and his Analytical
Engine. This note describes a general purpose computer that will not be
invented for more than 100 years (although much of this technology has been
kept secret from the public and must be investigated). In "Note B", Lovelace
looks at the concept of computer memory and the ability to insert statements to
indicate what is happening to the person looking at the program. This idea is
similar to the current practice of using REM or non-executable remark
statements in a program.

Lovelace expands on a method called "backing" in "Note C". This allows for the
operation cards to be put back in the correct order so that they could be used
again and again like a loop or subroutine. "Note D" is a very complex
explanation of how to write a set of instructions or a program to accomplish a
set of operations. "Note E", Baum a biographer of Lovelace, clearly states
"emphasize the versatility of the Analytical Engine and suggests, in its brief
description of operation cards which designate cycles, modern-day function
keys".

"Note F" explains how the Analytical Engine can solve difficult problems and
eliminate error. This allows for the solving of problems that were prohibitive
due to the constraints of time, labor and funds. Baum also notes that Lovelace
wonders "if the engine might not be set to investigate formulas of no apparent
practical interest … as computers are used today, to find problems rather
than to solve them".

The last and probably the most mathematically complex and most quoted of
Lovelace's notations is "Note G". In this note, Lovelace states what some have
referred to as "Lady Lovelace's Objection" or, in the more modern phrasing,
"garbage in, garbage out". Basically, that the computer's output is only as
good as the information it is given. "Note G" also includes an actual
illustration of how the engine can produce a table of Bernoulli numbers.
Lovelace,
originally Augusta Ada Byron, is the daughter of the notorious English Romantic
poet, Lord Byron.
Five weeks after Lovelace's birth, her mother, Lady Byron, left her
abusive husband and Lady Byron takes control of her daughter's upbringing.
Lovelace is
educated privately by tutors and then self-educated but is helped in her
advanced studies by mathematician-logician Augustus De Morgan, the first
professor of mathematics at the University of London.
De Morgan describes Ada
as "an original mathematical investigator, perhaps of first-rate eminence".

On July 8, 1835, Ada Byron marries William King who is then the eighth Baron
King. In 1838, King becomes the 1st Earl of Lovelace and Ada becomes the
Countess of Lovelace. Ada's husband is 11 years older than she and considered
to be somewhat reserved. He does, however, take pride in his wife's
mathematical talents and supported her endeavors. His approval is quite
fortunate for Ada Byron Lovelace as few women of her station in Victorian
England are encouraged to pursue academic interests of any kind. In fact, those
of the aristocracy consider practicing a profession to be beneath them. For
that reason, Lovelace only signs the initials, "A.A.L." to her "Notes". So
Lovelace is limited by her class status as much as by her gender with regard to
her passion for mathematics.

Lovelace first meets Babbage when she is 18 at a dinner party hosted by Mary
Fairfax Somerville, the 1800s most prominent woman scientist. Despite the fact
that Babbage is 23 years older, Babbage becomes Lovelace's good friend and
intellectual mentor. Lovelace is immediately intrigued when she first sees
Babbage's Difference Engine and plans for the Analytical Engine in 1834.

"ADA", a computer programming language, is named for Ada Lovelace.

Ada Lovelace was bled to death at the age of 36 by her physicians, while trying
to cure her uterine cancer.

Lovelace will not obtain widespread recognition until the historian, Lord B.V.
Bowden, rediscovers her "Notes" in 1952 and has them reprinted the following
year, 110 years after their original publication.
Cambridge, England (presumably)  
166 YBN
[1834 AD]
2787) Cellulose is now known to be the main constituent of cell walls in most
plants, and is important in the manufacture of numerous products with fibrous
components, such as paper, textiles, pharmaceuticals, and explosives.
Paris, France (presumably)  
166 YBN
[1834 AD]
2793) Ernst Heinrich Weber (VABR) (CE 1795-1878), German physiologist
determines that there was a threshold of sensation that must be passed before
an increase in the intensity of any (nervous system) stimulus (such as
different shades of light, or different weights) can be detected. Weber
publishes this finding in "De Tactu" (1834, "Concerning Touch").

Weber describes a terminal threshold for all senses, the maximum stimulus
beyond which no further sensation can be (detected).

Weber formulates what will be called "Weber's law", that the increase in
stimulus necessary to produce an increase in sensation is not fixed but depends
on the strength of the preceding stimulus. (I have doubts about this, but
perhaps.)

This examining of the nervous system will result in Michael Pupin researching
the possibility of seeing what eyes see from behind the brain, which leads to
Pupin successfully seeing what the eye sees, and images the brain produces in
1910.

(University of Leipzig) Leipzig, Germany  
166 YBN
[1834 AD]
2822) Clapeyron emphasizes the fact, already contained in Carnot"s work, that
the efficiency of a reversible engine depends only on the temperatures of the
source and sink. In the introduction to his paper Clapeyron writes that one of
the basic ideas contained in Carnot"s work is that "it is impossible to create
motive power or heat out of nothing", and that from here one can conclude, for
example, that the difference in the heat capacities of a gas is the same for
all gases. (Is it true that all gases absorb the same amount of heat? Because
different gases absorb different frequencies of light.)

This is before the concept of absolute temperature is established. Instead of
absolute temperature, Clapeyron uses the Mariotte-Gay-Lussac law in this form
(see image).

Clapeyron writes the relation (see image) (v super L is volume of liquid, and v
super G is volume of gas, dP over dt is change in pressure over a unit of time,
and C is the number of calories of heat?) where k is the latent heat
vaporization (which he calls latent caloric) per unit volume of vapor.
Clapeyron remarks that k is never infinite but can be zero when both phases
have the same density (critical point).

This equation is essentially the same as (the current form of the equation) if
C is taken as the absolute temperature multiplied by the conversion factor
between heat and mechanical work units. In his paper Clapeyron indicates that
no experimental data are available to determine the value of C except for t =
0. Using the value CP/CV = 1.412 found by Dulong, Clapeyron calculates 1/C to
be 1.41 at 0 °C and therefore the value 386 as the mechanical equivalent kg.m
kcal-1. Although this equation has been determined using a cycle in the
liquid-vapor (transition), it is clear that the same result would be obtained
if the cycle is performed either in the solid-gas or in the solid-liquid
(transitions).
Clapeyron designs and constructs locomotives and metal bridges.
Paris, France  
166 YBN
[1834 AD]
2851) Methanol, once produced by destructive distillation of wood, is now
usually made from the methane in natural gas. Methanol is produced commercially
from a mixture of carbon monoxide (CO) and hydrogen (H2). Methanol is an
important industrial material; its derivatives are used in great quantities for
making a vast number of compounds, among them many important synthetic dyes,
resins, drugs, and perfumes. Methanol is also used in automotive antifreezes,
rocket fuels, and as a solvent. Methanol is flammable and explosive. A
clean-burning fuel, methanol may substitute (in part) for gasoline. Methanol is
also used to denature of ethanol (for sale without the regulations of drinking
alcohol (ethyl alcohol)). A violent poison, methanol causes blindness and
eventually death when drunk. (Perhaps not the best idea to mix with ethyl
alcohol and sell to the public, but prohibition is not known for its logic. It
rings of the vindicative "serves them right" violent nature of many
prohibitionists and conservatives in general.)
(Ecole Polytechnique) Paris, France (presumably)  
166 YBN
[1834 AD]
2853)
(Ecole Polytechnique) Paris, France (presumably)  
166 YBN
[1834 AD]
2890) Johannes Peter Müller (MYUlR) (CE 1801-1858), German physiologist,
publishes "Handbuch der Physiologie des Menschen" (2 vols., 1834-40, "Handbook
of Human Physiology").

This book becomes the leading textbook in human physiology and is revised and
re-published many times.

(University of Berlin) Berlin, Germany  
166 YBN
[1834 AD]
2896)
Lyon, France (presumably)  
166 YBN
[1834 AD]
2899) (Sir) Charles Wheatstone (WETSTON) (CE 1802-1875), English physicist uses
a revolving mirror to measure the speed of electricity in a conductor. (more
info, describe experiment)

The same revolving mirror, by Wheatstone's suggestion, is later used in
measurements of the speed of light.

Wheatstone measures the speed of electricity to be 576,000 miles in a second
(one fluid theory) or 288,000 miles in a second (two fluid theory), and
concludes that "...the velocity of electricity through a copper wire exceeds
that of light through the planetary space.".

The great velocity of electrical transmission suggests the possibility of
utilizing electricity for sending messages.

The mirror's rotation is powered by a cord and pulley in order to count the
exact rate of mirror turning.

In order to measure the velocity of electricity through a wire, Wheatstone uses
0.8km (half a mile) of wire. Wheatstone cuts the wire at the middle, to form a
gap which a spark leaps across, and connects the ends of the wire to the poles
of a Leyden jar filled with electricity. Three sparks are therefore produced,
one at either end of the wire (when the Leyden jar discharges to the two ends
of the wire), and another at the middle (when the electric current has passed
through each of the two segments of wire). (needs visual) Wheatstone mounts a
tiny mirror on the works of a watch, so that the mirror revolves at a high
velocity (800 rotations per second), and observes the reflections of the three
sparks in it. The points of the wire are so arranged that if the sparks are
instantaneous, their reflections appear in one straight line; but the middle
one is seen to lag behind the others, because it is an instant later. The
electricity takes a certain time to travel from the ends of the wire to the
middle. This time is found by measuring the amount of lag, and comparing it
with the known velocity of the mirror. Any difference in time between the
sparks is converted into an angular separation, since the mirror turns slightly
during the tiny interval between the sparks, resulting in slightly displaced
reflections. The smearing of light in the reflected images indicate the
duration of the sparks and their relative displacement gives a value for the
speed of electricity. Having the time, Wheatstone can compare that with the
length of half the wire, and he can find the velocity of electricity. However
experimental or calculation error leads Wheatstone to conclude that this
velocity is 288,000 miles per second, an impossible value as it is faster than
the speed of light.

Until this time, many people had considered the electric discharge to be
instantaneous; but it was afterwards found that its velocity depended on the
nature of the conductor, its resistance, and its electro-static capacity (by
Ohm who uses the same law as Fourier for heat). Michael Faraday (goes on to
show), for example, that the velocity of electric current in an underwater
wire, coated with insulator, is only 144,000 miles per second (232,000 km/s),
or still less. Arago is in Britain for the 1834 Edinburgh meeting of the
British Association for the Advancement of Science and may learn of
Wheatstone's mirror then. Arago suggests to his fellow Academicians using a
rotating mirror to test the speed of light. On the advice of Arago,
Wheatstone's rotating mirror device is used by Léon Foucault and Hippolyte
Fizeau to measure the velocity of light.

William Watson had tried to measure the speed of electricity in 1748.

This experiment is important to electronic telegraphy, (which Wheatstone is
invested in, in England) because the thought is that if electrical propagation
is a diffusion phenomenon, like heat, long distance communication might be
impractical.
(King's College) London, England  
166 YBN
[1834 AD]
2913) Germain Henri Hess (CE 1802-1850), Swiss-Russian chemist, publishes a
chemistry textbook that is the standard for Russia until the textbook by
Mendeléev.
Hess finds that the oxidation of sugars yields saccharic acid.
(University of Saint Petersberg) Saint Petersberg, Russia (presumably)  
166 YBN
[1834 AD]
2916) Antoine Jérôme Balard (BoloR) (CE 1802-1876), French chemist discovers
(1834) discovered dichlorine oxide (Cl2O) and chloric(I) acid (HClO) (a
strongly oxidizing unstable chlorine acid that exists only in solution and as
chlorates).

(Montpellier École de Pharmacie) Montpellier, France  
166 YBN
[1834 AD]
3000)
(Trinity College, at Dunsink Observatory) Dublin, Ireland  
166 YBN
[1834 AD]
3061) Valentin is the first Jewish human to be hired as a professor in a
German-language university (although the University (of Bern) is not in Germany
itself), and the first Jewish person to be granted citizenship of the city of
Bern.
(Breslau now:) Wrocław, Poland (presumably)  
166 YBN
[1834 AD]
3076) Bunsen's father, Christian Bunsen, is chief librarian and professor of
modern philology at the University of Göttingen.
In 1830, Bunsen takes his Ph.D. in
chemistry at the University of Göttingen.
Bunsen never marries.
Bunsen does not allow organic
research in his lab.
Chemists who come to study with Bunsen at Heidelberg include
Adolph Kolbe, Edward Frankland, Victor and Lothar Meyer, Friedrich Beilstein,
Johann Baeyer and Dmitri Mendeleev. Bunsen makes the University of Heidelberg
one of the major world centers of chemical research.

In 1860, Bunsen is awarded the Copley Medal.
In 1877, Bunsen and Kirchhoff receive the
first Davy Medal.
In 1898 the Albert Medal in awarded to Bunsen in recognition of
Bunsen's many scientific contributions to industry.
(University of Göttingen), Göttingen, Germany  
166 YBN
[1834 AD]
3085)
(University of Göttingen), Göttingen, Germany  
166 YBN
[1834 AD]
3272)
New york City, NY, USA  
166 YBN
[1834 AD]
3453)
Wiltshire, England (presumably)  
165 YBN
[01/29/1835 AD]
3459)
(University of Edinburgh) Edinburgh, Scotland  
165 YBN
[02/06/1835 AD]
2810) Henry becomes an unwilling participant in the protracted litigation over
the scope and validity of Morse's patents. Between 1849 and 1852 the defendants
in three infringement suits subpoena Henry in the hopes that his statements
would weaken or invalidate Morse's claims, and Henry's testimony proves crucial
to the Supreme Court's 1854 split decision that strikes down Morse's broadest
claim. Henry claims that he does not want to become a party to this controversy
and that he gives his statement unwillingly, only under subpoena.
Princeton, NJ, USA  
165 YBN
[08/12/1835 AD]
2900)
(King's College) London, England  
165 YBN
[1835 AD]
2420) For this work Biot was awarded the Rumford Medal of the Royal Society in
1840.
Paris, France (presumably)  
165 YBN
[1835 AD]
2498)
Stokholm, Sweden (presumably)  
165 YBN
[1835 AD]
2550) Sedgwick strongly opposes Darwin's theory of evolution, although Sedgwick
is the first to recognize Darwin's talent.

In 1818 Sedgwick is elected to the Woodwardian Chair of Geology (at Cambridge),
a post Sedgwick holds until his death.

In 1829 Sedgwick is president of the Geological Society.
Cambridge, England  
165 YBN
[1835 AD]
2638) In October 1832 Morse returns to the United States from Italy aboard the
packet-ship Sully. On the voyage Morse meet Charles Thomas Jackson, a doctor
and inventor and the two discuss electromagnetism. Morse learns about Ampère's
idea for the electric telegraph. Jackson assured Morse that an electric impulse
can be carried along even a very long wire. Morse later recalls that he reacted
to this news with the thought that "if this be so, and the presence of
electricity can be made visible in any desired part of the circuit, I see no
reason why intelligence might not be instantaneously transmitted by electricity
to any distance." Morse immediately makes some sketches of a device to
accomplish this purpose. Morse's shipboard sketches of 1832 have clearly laid
out the three major parts of the telegraph: a sender which opens and closes an
electric circuit, a receiver which used an electromagnet to (convert the
electronic signal back into mechanical movement), and a code which translates
the signal into letters and numbers. These notes, made aboard the Sully are
still in the Morse papers in the Library of Congress in Washington, D.C..

Morse works for the next 12 years, with the aid of the chemist Leonard Gale,
physicist Joseph Henry, and machinist Alfred Vail to perfect his own version of
the instrument. So many phases of the telegraph, however, have already been
anticipated by other inventors, especially in Great Britain, Germany, and
France, that Morse's originality as the inventor of telegraphy has been
questioned; even the Morse code does not differ greatly from earlier codes,
including the semaphore.

The first telegraphs were in the form of optical telegraphs which include smoke
signals and beacons.

One of the most successful of the visual telegraphs was the semaphore developed
in France by the Chappe brothers, Claude and Ignace, in 1791. This system
consisted of pairs of movable arms mounted at the ends of a crossbeam on
hilltop towers. Each arm of the semaphore could assume seven angular positions
45° apart, and the horizontal beam could tilt 45° clockwise or
counterclockwise. In this manner it was possible to represent numbers and the
letters of the alphabet. Chains of these towers were built to permit
transmission over long distances. The towers were spaced at intervals of 5 to
10 kilometres (3 to 6 miles), and a signaling rate of three symbols per minute
could be achieved. Even from stars in a globular cluster to other stars in the
plane of the Milky Way galaxy, perhaps there are transmitting and receiving
stations because if the message is emitted in all directions, a very intense
light is needed, like a star, we only see a few photons of the many that a star
emits, but if the signals are directed to a specific direction which is much
more efficient, the longer the distance between a sender and receiver the more
complex the calculation of all the many pieces of matter in between that
influence the two points, their positions and velocities, in particular the
sender and receiver positions, and where the receiving object will be when the
photons finally arrive at the receiver. So there probably needs to be
relatively short range relay stations even between star clusters and their
exploring voyagers.

The invention of the voltaic cell in 1800 by Alessandro Volta of Italy helps to
make the electric telegraph (and so many other electric inventions) a reality.

The word telegraphy comes from Greek. "Tele" means distant and "graphein" to
write. So the meaning is "writing at a distance".

This telegraph is believed by many to this day to have been the scientific work
of Joseph Henry, which Morse exploits.
Morse's father Jedediah Morse is a Congregational
Pastor and author of "Geography Made Easy", the first book on geography printed
in the United States.

Morse's mother is the daughter of the man who founded Shrewsbury, New Jersey.

Morse attends Yale from 1808 to 1810, attends lectures on electricity, and
spends a vacation assisting with electrical experiments.
After 1825, Morse settles in New
York City and paints portraits.

As part of a campaign against the licentiousness (sexually unrestrained or
going beyond customary limits nature) of the theater (stage), Morse helps
launch, in 1827, the New York Journal of Commerce, which refuses theater
advertisements.

On 10/02/1832 Morse is hired as the professor of the literature of arts and
design at the University of the City of New York (now New York University),
which had been founded one year earlier. Morse receives no salary and must
depend on fees from his students and the occasional sale of a portrait.
Both Morse and
John Draper are instrumental in introducing the daguerreotype in the United
States.

Morse enters politics, for mayor of New York (City) as a member of the "Native
American" party, a group of anti-Catholic and anti-immigrant people.

Morse does not acknowledge Henry's help.
In 1837 Morse receives a patent on a
telegraph in the USA.

Morse's patent is rejected in England, where a similar device has already been
developed.
In 1854, a U.S. Supreme Court decision established Morse's patent rights.
During the
Civil War, Morse sympathizes with the South, even though he is a Northerner
because of his belief that Negro slavery is justified.

Morse is made a charter member of the Hall of Fame for Great Americans on the
campus of New York University, but the authentically great American Henry is
not elected until 1915.

In his old age Morse is a founder and trustee of Vassar College, donates money
to his alma mater, Yale College; and to churches, theological seminaries, Bible
societies, mission societies, and temperance societies (people that want to
jail those who use alcohol), as well as to poor artists.
New York City, New York, USA  
165 YBN
[1835 AD]
2671) The first railway is constructed in Germany, between Nuremberg and Furth.

Nuremberg (and Furth), Germany  
165 YBN
[1835 AD]
2673)
Bonn, Germany  
165 YBN
[1835 AD]
2736) Gustave Gaspard de Coriolis (KOrYOlES) (CE 1792-1843), French physicist,
publishes "Théorie mathématique des effets du jeu de billiard" (1835,
"Mathematical Theory of the Game of Billiards").

Paris, France  
165 YBN
[1835 AD]
2738) The Coriolis "force", is an example of how a natural cumulative effect of
motion of many particles due to gravity and collision can be described as a
separate distinct force. This is why I prefer to call this an "effect" or
"phenomenon", although "force" is fine, but people should recognize that this
is a cumulative effect of a more fundamental force of gravity.
Paris, France  
165 YBN
[1835 AD]
2796) Adolphe Quetelet (full: Lambert Adolphe Jacques Quetelet) (KeTlA) (CE
1796-1874), Belgian astronomer and statistician applies statistical analysis to
humans.

In 1830, Quetelet is supervisor of statistics for Belgium where he develops
many of the rules governing modern census taking and stimulates statistical
activity in other countries.
For the Dutch and Belgian governments, Quetelet
collects and analyzes statistics on crime, mortality, and other subjects and
devises improvements in census taking.
Quetelet records various measurements of human
properties, for example height and then graphs the results which shows that the
results fit a bell-shaped curve.
Queteley uses these statistics to social phenomena,
and develops the concept of the "average man". In this way Queteley establishes
the theoretical foundations for the use of statistics in social physics or what
is now called sociology. Therefore Queteley is considered by many to be the
founder of modern quantitative social science.

Quetelet publishes this analysis in "Sur l'homme et le développement de ses
facultés, ou essai de physique sociale" (1835, tr Eng 1842, "A Treatise on Man
and the Development of His Faculties").
In 1828 Quetelet is the first director of the Royal
Observatory at Brussels, a position held until his death in 1874.
Brussels, Belgium  
165 YBN
[1835 AD]
2829) Talbot writes: "(In) October, 1833, I was amusing myself on the lovely
shores of the Lake of Como in Italy, taking sketches with a Camera Lucida, or
rather, I should say, attempting to make them; but with the smallest possible
amount of success...
After various fruitless attempts I laid aside the instrument and
came to the conclusion that its use required a previous knowledge of drawing
which unfortunately I did not possess.
I then thought of trying again a method which
I had tried many years before. This method was to take a Camera Obscura and to
throw the image of the objects on a piece of paper in its focus - fairy
pictures, creations of a moment, and destined as rapidly to fade away...
It was
during these thoughts that the idea occurred to me... how charming it would be
if it were possible to cause these natural images to imprint themselves durably
and remain fixed on the paper!"

Talbot describes how he captures a paper negative: ".. I constructed {a camera
obscura} out of a large box, the image being thrown upon one end of it by a
good object-glass fixed at the opposite end. The apparatus being armed with a
sensitive paper, was taken out in a summer afternoon, and placed about one
hundred yards from a building favourably illuminated by the sun. An hour or so
afterwards I opened the box and I found depicted upon the paper a very distinct
representation of the building, with the exception of those parts of it which
lay in the shade. A little experience in this branch of the art showed me that
with a smaller camera obscura the effect would be produced in a smaller time.
Accordingly I had several small boxes made, in which I fixed lenses of shorter
focus, and with these I obtained very perfect, but extremely small pictures
..."
Wiltshire, England (presumably)  
165 YBN
[1835 AD]
2864)
Paris?, France (verify)  
165 YBN
[1835 AD]
2865)
Paris?, France (verify)  
165 YBN
[1835 AD]
2939)
(Hunterian museum of the Royal College of Surgeons) London, England  
165 YBN
[1835 AD]
3017)
(Andersonian Institution) Edinburgh, Scotland  
165 YBN
[1835 AD]
3028) Other achievements of Laurent include discovering anthracene, 1832;
obtaining phthalic acid from napthalene, 1836; and showing that carbolic acid
is phenol, 1841.

The collected papers of Laurent are published posthumously in "Methode de
Chimie" (1854; "Method of Chemistry").

Liebig, Gmelin, and Beilstein come to accept Laurent's view, Wöhler sides with
Berzelius.

Laurent presents three-dimensional models of molecules.

In 1844 Laurent is one of the first chemists to embrace Avogadro's law.
Laurent sees
that chemists must distinguish clearly between atoms, molecules, and
equivalents. Laurent regards the molecules of hydrogen, oxygen, and others as
consisting of two atoms, forming what he calls a "homogeneous compound", which,
by double decomposition, could form "heterogeneous compounds". This provides a
basis for the accurate determination of atomic weights.

In 1892 Laurent's suggestion for naming organic chemicals forms the basis of
the Geneva nomenclature adopted for organic chemistry.
In 1850 Laurent is the
best-qualified candidate for the chair of chemistry at the Collège de France,
but his appointment was vetoed by the Academy of Sciences, some of whose
members are worried by Laurent's radical republican views in the tense
atmosphere of conservative reaction that had set in after the Revolutions of
1848.

Laurent dies of tuberculosis at age 44.

(Perhaps an argument can be made for atoms holding together by the force of
gravity or because of collision. Currently the view is that valence electrons
hold atoms together in molecules, which seems a development of Berzelius' view
of oppositely electrically charged atoms holding together. This may involve how
electrons are gained or lost on atoms, or shared between atoms in a molecule,
for example, where chlorine is thought to have 7 outer orbiting electrons, and
is viewed as more likely to accept an eighth electron, hydrogen is seen as
having only one electron and more likely to donate the electron. If a stable
hydrogen shell is 2 electrons, perhaps adding an electron to hydrogen is a
stable configuration for hydrogen. In this sense, hydrogen might be viewed as
being just an atom that can gain an electron just as easily as lose an
electron, however, the most common form of hydrogen is the single electron
hydrogen and a second electron would cause a negative hydrogen ion which I
don't think has ever been observed. Bromine is under Chlorine and is a similar
single electron accepter, NO2 may also be a similar single electron accepter.
If true, perhaps other molecules show the same property of Hydrogen and
Chlorine being electron accepters. Are there any other known examples that
violate the idea of atoms with opposite electrically balanced outer shells of
atoms (1 electron versus 7, etc) bonding? The current view is that atoms are
electrically neutral unless in the form of ions. The current view is also that
an atom attaches to a molecule based on what makes the number of electrons in
its outer (valence) electron shell most stable.)

(Atoms and molecules are so small, and there are so many pieces of matter put
together, that I think humans should keep an open mind about the physical
structure of atoms without yet or perhaps ever physically seeing all the
objects involved.)
Paris, France (presumably)  
165 YBN
[1835 AD]
3226)
Belgium  
165 YBN
[1835 AD]
3300)
(University of Giessen), Giessen, Germany  
165 YBN
[1835 AD]
3781)
Paris, France (presumably)  
165 YBN
[1835 AD]
3896)
Lodi, Italy (verify)  
165 YBN
[1835 AD]
5982) Nicolò Paganini (CE 1782-1840), Italian violinist and composer, composes
"Moto Perpetuo" ("Perpetual Motion"). (verify)

Parma, Italy  
165 YBN
[1835 AD]
5993)
Paris, France  
164 YBN
[1836 AD]
2579)
(Breslau, Prussia now:)Wroclaw, Poland  
164 YBN
[1836 AD]
2605)
Copenhagen, Denmark  
164 YBN
[1836 AD]
2670)
Göttingen, Germany  
164 YBN
[1836 AD]
2672) Carl August von Steinheil (CE 1801-1870) erects a single insulated wire
on wooden poles parallel to the railway track and uses the rails and Earth as
return conductors. (Was this a telegraph? Was this done with railway and
government participation?)

Göttingen, Germany  
164 YBN
[1836 AD]
2703) In 1836 Michael Faraday observes that the charge on a charged conductor
is located only on its exterior and has no influence on anything enclosed
within it. To demonstrate this fact Faraday builds a room (size?) coated with
metal foil and allows high-voltage discharges from an electrostatic generator
to strike the outside of the room. He uses an electroscope to show that there
is no electric charge present on the inside of the room's walls.

The same effect was predicted earlier by Francesco Beccaria (1716-1781) at the
University of Turin, a student of Benjamin Franklin, who stated that "all
electricity goes up to the free surface of the bodies without diffusing in
their interior substance.". Later, the Belgian physicist Louis Melsens
(1814-1886) applied the principle to lightning conductors. Another researcher
of this concept was Gauss (Gaussian surfaces).

A metal mesh cage also stops photon radio signals.
(Royal Institution in) London, England  
164 YBN
[1836 AD]
2780) This map is the first lunar map to be divided into quadrants.
In 1878, J.F. Julius
Schmidt's lunar map will surpass this map in detail.
Berlin, Germany (presumably)  
164 YBN
[1836 AD]
2813) It is possible that people were murdered with high voltage from this
point on, although an autopsy might reveal burned tissue.
Maynooth, Ireland  
164 YBN
[1836 AD]
2852)
(Ecole Polytechnique) Paris, France (presumably)  
164 YBN
[1836 AD]
2863) Pure acetylene is a colorless gas with a pleasant odor; as prepared from
calcium carbide it usually contains traces of phosphine that cause an
unpleasant garliclike odor.
Pure acetylene under pressure in excess of about 15
pounds per square inch or in liquid or solid form explodes with extreme
violence.

Davy first makes acetylene from a compound produced during the manufacture of
potassium from potassium tartrate and charcoal, which under certain conditions
yields a black compound decomposed by water with considerable violence and the
evolution of acetylene. This compound is afterwards fully investigated by J. J.
Berzelius, who shows it to be potassium carbide. Davy also makes the
corresponding sodium compound and shows that it evolves the same gas. In 1862
F. Wohler will first makes calcium carbide, and find that water decomposes it
into lime and acetylene. Not until 1892 T. L. Wilson in America and H. Moissan
in France independently find that if lime and carbon are fused together at the
temperature of the electric furnace, the lime is reduced to calcium, which
unites with the excess of carbon present to form calcium carbide. The cheap
production of this material and the easy liberation by its aid of acetylene at
once gaives the gas a position of commercial importance.
Edmund Davy is cousin and lab
assistant of Humprey Davy.
Starting in 1813 Edmund Davy is professor of Chemistry at
Cork Institution.
Starting in 1826 Edmund Davy is professor of chemistry at the Royal Dublin
Society.
(Royal Dublin Society) Dublin, Ireland (presumably)  
164 YBN
[1836 AD]
2867)
Auch?, France  
164 YBN
[1836 AD]
2926)
London, England (presumably)  
164 YBN
[1836 AD]
3066) Asa Gray (CE 1810-1888), US botanist, publishes "Elements of Botany"
(1836).
In 1842 Gray if professor of natural history at Harvard University.

In 1851 Gray meets Darwin.

In 1865, Gray donates the thousands of books and plants he has collected at his
own expense to Harvard, and this results in the establishment of the botany
department at Harvard.

On Sept. 5, 1857, Darwin writes Gray a famous letter in which Darwin outlines
his theory of the evolution of species by natural selection.

Gray reviews Darwin's "Origin of Species" (1859) in the "American Journal of
Science", of which Gray is a coeditor.

Gray supports Darwin's theory of evolution in the United States (with Agassiz
opposing) and writes numerous popular botanical books on North American
plants.

Gray boldy supports Darwinism in the United States against the objections of
religious leaders and debates the point vigorously with the antievolutionist
Agassiz. As a prominent religious person, Gray cannot be dismissed as an
atheist (which is stupid anyway, since ultimately the truth of a theory should
be the important thing, not the religious or political beliefs of the source),
and this gives Gray's support more influence. Gray argues that natural
selection is guided by a God, which Darwin disagrees with.
(possibly move to
chronological)
New York City, NY, USA  
164 YBN
[1836 AD]
3070) Schwann is an assistant to the physiologist Johannes Peter Müller
(1834–38) at the University of Berlin.
The last 40 years of Schwann's life he
dedicates to mysticism and religious meditation. (How can people go backwards
like that? In accumulating information, I think most people must get smarter
and more well informed as they age.)

After leaving the influence of Müller, Schwann's productivity practically
ceases; in Belgium Schwann only publishes one paper, on the use of bile.

In 1845 Schwann receives the Copley Medal.
(University of Berlin) Berlin, Germany  
164 YBN
[1836 AD]
3071)
(University of Louvain) Louvain, Belgium (verify)  
164 YBN
[1836 AD]
3590)
London, England (presumably)  
164 YBN
[1836 AD]
3897)
(Charite Hospital) Paris, France  
163 YBN
[06/12/1837 AD]
2647) In this same year Samuel Morse demonstrates an electric telegraph that
produces coded written messages and so the era of electric telegraphy starts in
1837 almost simultaneously in Great Britain and the United States.

(Those people who own the telegraph companies, store and read the telegraph
messages of people, and this informs them of what is going on. This system of
recording public communications is adopted by the telephone companies who
record phone calls, and even extend the system by putting microphones and
cameras to see visible and infrared light, and even deadly lasers inside the
majority of people's houses under the excuse of national security and in the
interest of data collection and crime solving, however, the system is
ultimately used to facilitate violence and protect powerful violent criminal
people. This is done, presumably, in all nations with electrical communications
systems.)
England (presumably) (more specific)  
163 YBN
[07/??/1837 AD]
3995)
Salem, Massachusetts, USA  
163 YBN
[09/04/1837 AD]
2674) Samuel Morse (CE 1791-1872) sends a telegraph message on a wire 550m long
in his classroom. This demonstration results in the partnership of Morse, Gale
and Alfred Vail. Vail's wealthy father finances the development of the
telegraph, including paying for Morse's patent. Alfred Vail builds the
instrument and receives 25% interest in the invention.

New York City, New York, USA  
163 YBN
[10/17/1837 AD]
4008)
St. Petersburg, Russia (presumably)  
163 YBN
[11/16/1837 AD]
3663)
(Royal Institution in) London, England  
163 YBN
[1837 AD]
2435)
Turin, Italy (presumably)  
163 YBN
[1837 AD]
2521)
Paris, France  
163 YBN
[1837 AD]
2580)
(University of Bresslau) Bresslau, Prussia (now: Wroclaw, Poland)|Delivered
before the Congress of Physicians and Scientists in Prague  
163 YBN
[1837 AD]
2602) Boucher de Perthes is the director of the customhouse (a building where
customs and duties are paid or collected and where vessels are entered and
cleared) at Abbeville, near the mouth of the Somme River, and devotes his
leisure to archaeological searches in the Somme valley. (So de Perthes is not
employed in a university, but has a natural interest in science and
archeology.)
Abbeville, France  
163 YBN
[1837 AD]
2626) This research serves as the basis for Hall's theory of reflex action,
which states that the spinal cord is made of a chain of units and that each of
these units functions as an independent reflex (unit which Hall calls an
"arc"); that the function of each arc arises from the activity of sensory and
motor nerves and the segment of the spinal cord from which these nerves
originate; and that the arcs are interconnected, interacting with one another
and the brain to produce coordinated movement. (explain more nature of units -
or arcs, are these nerve ganglions/bundles?) Hall theorizes that reflex actions
such as pulling a finger away from something hot before knowing it is hot, is
from nerve impulses to and from the spinal chord (without going all the way to
the brain).
London, England (presumably)  
163 YBN
[1837 AD]
2630) In the early 1830s, Daniell becomes deeply interested in the work of his
friend Michael Faraday and so turned to electrochemistry for his main research
interest at that time. A major problem with the Volta pile is that it can not
provide current for a sustained period of time. (William) Sturgeon (the
inventor of the electromagnet) worked on the problem and in 1830 produced a
battery with longer life than that of Volta by amalgamating the zinc (to blend
with another metal (which metal?)). Contributing to the major problem with
batteries is a thin film of hydrogen bubbles that forms over the positive
electrode. The thin film of hydrogen causes increased internal resistance of
the battery that reduces the battery's effective electromotive force (voltage).
This process of a thin film of hydrogen collecting on the electrode is known as
polarization. Daniell begins experiments in 1835 in an attempt to improve the
Voltaic battery with its problem of being unsteady and as a weak source of
electrical current. Daniell soon achieves remarkable results. In 1836, Daniell
invents a primary cell in which hydrogen is eliminated in the generation of the
electricity and this solves the problem of polarization. In his laboratory
Daniell learns to alloy the amalgamated zinc of Sturgeon with mercury.
Daniell's battery is the first of the two-fluid class battery and the first
battery that produces a constant reliable source of electrical current over a
long period of time. That is, the power remains constant with this type of
battery upon repeated application without removing the metals which is a source
of weakness in all single fluid batteries. Until now the current of other
batteries rapidly declines. Daniell's placement of a barrier between the copper
and zinc plates stops the hydrogen from forming. The Volta battery (or pile)
emits free hydrogen by the electrolyte which then migrates to the positive
copper pole. The hydrogen accumulates on the pole to form a barrier that soon
stops the flow of the current. Both single fluid and two-fluid batteries use
solutions to create the electricity. Daniell's battery consists of a
cylindrical copper vessel that serves as the passive plate (or pole). A porous
earthenware container or partition that holds a zinc rod or active plate (or
pole) is placed inside the outer copper vessel. The space between the copper
and the porous cup is filled with a solution of copper sulfate which keeps
saturated by crystals of the (copper) salt lying on a perforated shelf. The
porous cup is filled with dilute sulfuric acid. The porous earthenware keeps
the fluids from mixing without stopping the passage of current; the earthenware
barrier allows (hydrogen) ions to move through while the reaction of the cell
is taking place. (The replacement of Zinc for hydrogen in the sulfuric acid is
passed by the transfer of hydrogen, which is small enough to passes through the
barrier and replaces copper in the copper sulfate on the other side.) The
contents of the battery have to be dismantled when not used to stop the
chemical reactions and conserve the metals. The sulfate of copper that is in
contact with the passive plate serves to take up hydrogen. The amalgamated
zinc rod (anode) had a binding screw (to hold a metal wire). The top of the
copper cylinder contains the other binding screw (cathode). The chemical
reaction within the battery consists of a decrease of zinc and an increase of
copper; the zinc crowds out copper from its sulfate so that the copper sulfate
continuously changes into zinc sulfate by replacement. Beard and Rockwell
express the chemical reaction with the equation: Zn + H2SO4 + CuSO4 = ZnSO4 +
H2SO4 + Cu (separate out two equations Zn+H2SO4->ZnSO4+H2 and
H2+CuSO4->H2SO4+Cu) The sulfuric acid is kept in the porous cup to keep the
sulfate of zinc formed from contacting the copper (what purpose does the copper
pole serve? Not a source for copper ions, but as an attractor of zinc ions? It
seems like any conductor/metal would work perhaps). Since copper sulfate
solution is heavy, it remains on the bottom of the cell. Daniell's battery with
modifications has an operating voltage (gives constant electromotive force and
retains a nearly constant internal resistance) of 1.11 volts. Daniell's battery
is called a "constant battery" because it does not evolve gas, and therefore
does not polarize, supplying a constant current. Daniell's battery (makes
possible the measuring of) the unit of electric potential, the volt, just as a
column of mercury does (for the measuring of) the unit of resistance, the ohm.
The Daniell cell still uses the familiar copper and zinc electrodes. The zinc
electrode is put in a cup of unglazed earthenware and bathed in dilute
sulphuric acid. The copper is surrounded by crystals of copper sulphate that
maintain a saturated solution. Instead of releasing hydrogen, the electrons are
furnished to the copper ions in the electrolyte, which plate out as copper
metal on any nearby surface. (This seems a possible confusion between the
movement of electrons and protons, because states that hydrogen combines with
copper sulfate to plate copper at the positive copper pole - perhaps electrons
replace a negative ion or perhaps all current is the proton, the hydrogen
atom.) The purpose of the cup is to keep the solutions separate (the copper
sulfate and sulfuric acid mixture with the zinc sulfate and sulfuric acid
mixture) while allowing electrical conduction by ion migration. If the
solutions mixed, (the) local (mixing) action ruins the battery (explain: with
no barrier, the hydrogen gas builds up?). When the cell (provides) current, the
zinc dissolves (in the sulfuric acid) to form zinc sulphate solution (and
hydrogen is released), (the hydrogen moves through the barrier and replaces the
copper in the copper sulfate) and copper from the copper sulphate plates out on
the (positive) copper electrode. (Perhaps this causes a hole which pulls an
ion, electron or proton from the wire and the object the wires are connected
to, the so-called load. This chain reaction may creates the phenomenon of
electrical current.) (State the official explanation.) No gases are (evolved)
at all (the replacement of Zinc with Hydrogen in the Sulfuric acid causes free
hydrogen but this is quickly reacts with copper sulfate on the other side of
the barrier) (What is the exact order of the above equation? The hydrogen must
be all taken up by the copper sulfate on the other side of the barrier), so the
cell does not polarize. The cell has a fairly large internal resistance, but
this is not a serious defect in view of the small currents required, and
actually proves an advantage in many applications. This large internal
resistance also protects the cell against damage if short circuited. The copper
sulphate even keeps algae (growth) under control. However, the porous cup,
intended to keep the solutions separate, is rendered impervious after a time by
deposition of copper on it as the cell operates. This internal resistance
varies slightly with areas of the copper and zinc plates immersed in the
solutions, distance between the metal plates, and the width and materials of
the walls of the porous cup. The battery's operating voltage depends on the
densities of the copper and zinc sulfate solutions. The operating voltage
increases (to around 1.14 V) by increasing the density of copper sulfate
solution, and the battery's voltage decreases (to around 1.08 V) by increasing
the density of the zinc sulfate solution. (zinc sulfate or sulfuric acid
solution?) When the battery is not in use corrosion of the zinc plates is high
which greatly limits its longevity. Daniell's battery required little
maintenance, and does not give off noxious fumes. The Daniell battery is less
expensive than existing batteries. (Does the zinc electrode get used up or the
zinc in the zinc sulfate? Does copper plating happen on both inside and outside
of earthenware container?) (See diagram below) This combination consists of a
jar of glass or earthenware, F (Fig. 3), about six inches in diameter and eight
or nine inches high. A plate of copper, G, is bent into a cylindrical form, so
as to fit within it, and is provided with a perforated chamber, to contain a
supply of sulphate of copper in crystals, and a strap of the same metal with a
clamp for connecting it to the zinc of the next element. H is a porous cup, as
it is technically termed, made of unglazed earthenware, six or seven inches
high and two inches in diameter, within which is placed the zinc, X. This is
usually of the shape shown in the figure, which is called the "star zinc", but
it is often made in the form of a hollow cylinder, the latter giving greater
power, but being somewhat more difficult to clean. The outer cell is filled
with a saturated solution of sulphate of copper (blue vitriol), and the porous
cell with a solution of sulphate of zinc. A series of three elements connected
together, as usually employed on American lines for a local battery, is shown
at I. Daniell's research into development of constant current cells takes place
at the same time (late 1830s) that commercial telegraph systems begin to
appear. Early telegraph messages are brief and travel short distances. Crude,
weak batteries were sufficient to support the signal. With the increase in
traffic and introduction of Morse sets, stronger currents and more constant
output are required in the batteries. Daniell's copper-depolarized battery
(1836) and Grove"s nitric acid depolarized cell are fortuitous arrivals.
British and American telegraph systems use the Daniell cell exclusively, as it
is the only one capable of being rapidly depolarized. (describe how, I thought
this battery would not become polarized.) Daniell's cells also produced a more
constant output and generated a stronger current than Sand batteries. This is
the "pre-volt" period, when the intensity of pain is used as a measure of a
cell's power. The Daniell cell is widely used in France before the Leclanché
cell is invented in 1868.
In 1837 Daniell is presented the highest award of the
Royal Society, the Copley Medal, for the invention of the Daniell cell.
London, England (presumably)  
163 YBN
[1837 AD]
2646)
New York City, New York, USA  
163 YBN
[1837 AD]
2748) Charles Babbage (CE 1792-1871), English mathematician, responding to the
Bridgewater Treatises, of which there were eight, publishes "The Ninth
Bridgewater Treatise, a Fragment" (1837, John Murray) challenging Hume on
miracles. Babbage titles this work "On the Power, Wisdom and Goodness of God,
as manifested in the Creation", putting forward the thesis that God has the
omnipotence and foresight to create as a divine legislator, making laws (or
programs) which then produced species at the appropriate times, rather than
continually interfering with ad hoc miracles each time a new species was
required. The book is a work of natural theology, and incorporates extracts
from correspondence Babbage had been having with John Herschel on the subject.

Cambridge, England (presumably)  
163 YBN
[1837 AD]
2749) Charles Babbage (CE 1792-1871), English mathematician, decodes
Vigenère's autokey cipher as well as the much weaker cipher that is called
Vigenère cipher today. Babbage's discovery is used to aid English military
campaigns, and is not published until several years later; as a result credit
for the development is instead given to Friedrich Kasiski, a Prussian infantry
officer, who makes the same discovery some years after Babbage. (This clearly
hints that Babbage was in communication with government military employees and
the view of keeping scientific advances secret at the expense of public
education and information is well underway by this time in Great Britain.)
(chronology) (more details about cipher and encryption)

Cambridge, England (presumably)  
163 YBN
[1837 AD]
2765) In 1808 Struve leaves Germany to avoid (involuntary employment)
(conscription) by the Napoleonic armies, and goes first to Denmark and then to
Russia.
In 1813 Struve becomes professor of astronomy and mathematics at the University
of Dorpat (now Tartu, Estonia).
Struve makes substantial contributions to the study of
galactic structure and also is involved in notable geodetic operations such as
the triangulation of Livonia and the measurement of an arc of the meridian.
In
1817 Struve is appointed director of the Dorpat Observatory.
In 1830 Czar Nicholas I set
aside land in the Pulkovo Hills outside St. Petersburg as the site for a new
astronomical observatory and selects Struve for the commission responsible for
its construction.
(For this observatory), Struve buys the largest and best refracting
telescope in the world made by Fraunhofer, a 15 inch objective lens.
Struve is
director of the observatory in Pulkovo for 20 years.
Struve is the first in a
line of 4 astronomers.
Pulkovo, Russia  
163 YBN
[1837 AD]
2777) From 1828-1832, Whewell is professor of mineralogy at Trinity College,
Cambridge.
In 1834 Whewell opposes the admission of Dissenters.
From 1838-1855 Whewell is professor of
moral philosophy at Cambridge.
From 1841-1866 Whewell is college master at Cambridge.
In 1842 Whewell
is made vice chancellor of Cambridge University.
Cambridge, England  
163 YBN
[1837 AD]
2943) Wilhelm Eduard Weber (CE 1804-1891), German physicist publishes
"Resultate aus den Beobachtungen des magnetischen Vereins" (6 vols, 1837-43),
which contains many of Weber's extensive articles edited by Weber and Gauss.

(University of) Göttingen, Germany  
163 YBN
[1837 AD]
3005) (Sir) William Rowan Hamilton (CE 1805-1865) corrects Abel's proof of the
impossibility of solving the general quintic equation (an equation where the
highest power variable is 5) and defends this proof against G. B. Jerrard who
claims to have found a solution.

(Trinity College, at Dunsink Observatory) Dublin, Ireland  
163 YBN
[1837 AD]
3029) As a child, science is considered by the majority in English public
schools to be dehumanizing, and for dabbling in chemistry Darwin is condemned
by his headmaster (and nicknamed "Gas" by schoolmates).
Darwin starts to study "medicine"
((health science)) at Edinburgh University, but the sight of operations on
children with no anesthesia upsets him.
Edinburgh attracts English Dissenters who
are barred from graduating at the Anglican universities of Oxford and
Cambridge, and so the university's radical students expose the teenage Darwin
to the latest Continental sciences.
In 1828, Darwin's father transfers Charles
to Christ's College, Cambridge to prepare for the church.
Inspired by Alexander von
Humboldt's account of the South American jungles in his "Personal Narrative of
Travels", Darwin gladly accepts Reverend John Henslow's suggestion of a voyage
to Tierra del Fuego, at the southern tip of South America, aboard a rebuilt
brig, HMS Beagle, commanded by the 26-year-old captain, Robert Fitzroy.
This voyage is
to survey coastal Patagonia to facilitate British trade and return three
"savages" previously brought to England from Tierra del Fuego and
Christianized.
On the voyage Darwin accumulates a 770-page diary, 1,750 pages of notes, and
draws up 12 catalogs of the 5,436 bones, skins, and carcasses Darwin had
collected during the journey.

According to the Encyclopedia Britannica, Darwin is a typical Victorian in his
racial and sexual stereotyping, thinking women inferior, and although a fervent
abolitionist, considers blacks a lower race.
Darwin witnesses Negro slavery in the
Americas, and passionately is against it.
Darwin believes in a clear style and
doing away with eloquence.
Darwin is wealthy, according to the Encyclopedia
Britannica, by the late 1840s the Darwins had £80,000 invested; Darwin is an
absentee landlord of two large Lincolnshire farms; and in the 1850s plows tens
of thousands of pounds into railway shares.
In 1873, Darwin helps raise
£2,100 to send a fatigued Huxley on holiday.
In 1881, with help from Darwin, the
routinely poor Wallace is added to the Civil List, which gives money to people
who have achieved distinction in the arts.
Darwin has ten children with his wife (and
cousin) Emma Wedgwood.

To people who ask about his religious beliefs, Darwin states that he is an
agnostic (a word coined by Huxley in 1869).
Darwin as an agnostic, is given the
ultimate British accolade of burial in Westminster Abbey, London. (For me being
frozen and preserved for future scientists to reawaken is the ultimate in
preservation and respect.)
London, England (presumably)  
163 YBN
[1837 AD]
3055) In 1827 Rawlinson goes to India as a British East India Company cadet,
and in 1833 Rawlinson and other British officers are sent to Iran to reorganize
the shah's army. In Iran, Rawlinson becomes interested in Persian antiquities,
and deciphering the cuneiform inscriptions at Bisitun becomes his goal.

Rawlinson's other writings include "A Commentary on the Cuneiform Inscriptions
of Babylonia and Assyria" (1850) and "Outline of the History of Assyria"
(1852).
Behistun, (Persia now) Iran (and England)  
163 YBN
[1837 AD]
3056) The inscription starts:
"1.1) I (am) Darius, the great king, the king of
kings, the king in Persia, the king of countries, the son of Hystaspes, the
grandson of Arsames, the Achaemenide.

1.2) Says Darius the king: My father (is) Hystaspes, the father of Hystaspes
(is) Arsames, the father of Arsames (is) Ariaramnes, the father of Ariaramnes
(is Teispes), the father of Teispes (is) Achaemenes.

1.3) Says Darius the king: Therefore we are called the Achaemenides; from long
ago we have extended; from long ago our family have been kings.

1.4) Says Darius the king: 8 of my family (there were) who were formerly kings;
I am the ninth (9); long aforetime we were (lit. are) kings.

1.5) Says Darius the king: By the grace of Auramazda I am king; Auramazda gave
me the kingdom.

1.6) Says Darius the king: These are the countries which came to me; by the
grace of Auramazda I became king of them; Persia, Susiana, Babylonia, Assyria,
Arabia, Egypt, the (lands) which are on the sea, Sparda, Ionia, , Armenia,
Cappadocia, Parthia, Drangiana, Aria, Chorasmia, Bactria, Sogdiana, Ga(n)dara,
Scythia, Sattagydia, Arachosia, Maka; in all (there are) 23 countries." (and
continues on)
Behistun, (Persia now) Iran (and England)  
163 YBN
[1837 AD]
3998)
(US Military Academy) West Point, NY, USA  
163 YBN
[1837 AD]
6257)
  
162 YBN
[02/22/1838 AD]
2885)
(Royal Institution in) London, England  
162 YBN
[02/??/1838 AD]
2640) Samuel Morse (CE 1791-1872) gives his first public demonstration of his
telegraph for interested members of the United States Congress.

Washington DC, USA  
162 YBN
[07/??/1838 AD]
3618)
(tested on railroad tracks from Nüremburg to Fürth) (Munich University)
Munich, Germany  
162 YBN
[1838 AD]
2499)
Stokholm, Sweden (presumably)  
162 YBN
[1838 AD]
2500)
Stokholm, Sweden (presumably)  
162 YBN
[1838 AD]
2540) Bessel uses a heliometer to make this measurement.
Earlier astronomers trying to
measure parallax had chosen bright stars, supposing that all stars are about
the same size and that the brightest stars are the nearest stars.
By this time the
"proper motion" of different stars is available and offers more reliable
guidance in guessing which stars are most likely to be nearby.

Bessel chooses to observe 61 Cygni, the star known to have the largest proper
motion at the time. After 1 1/2 years of careful observations and laborious
calculations, Bessel separates the star's own motion from the various motions
of the earth and concludes in 1838 that the star was oscillating back and forth
each year by about 3/10 of 1 second of arc.

This calculation of parallax is pivotal in astronomy because it signals the
official end of the dispute (between Sun-centered over Earth-centered theories)
and constitutes the beginning of (calculating the distances to the other
stars).
Königsberg, (Prussia now:) Germany  
162 YBN
[1838 AD]
2639)
New York City, New York, USA  
162 YBN
[1838 AD]
2753)
Cambridge, England (presumably)  
162 YBN
[1838 AD]
2766)
Pulkovo, Russia  
162 YBN
[1838 AD]
2791)
Berlin, Germany  
162 YBN
[1838 AD]
2799) Poiseuille publishes (this equation) in 1846.
Paris, France (presumably) (Berlin, Germany for Hagen)  
162 YBN
[1838 AD]
2803) (Sir) Charles Lyell (CE 1797-1875), Scottish geologist, publishes
"Elements of Geology" (1838), a well-illustrated work, which describes European
rocks and fossils from the most recent to the oldest known at the time.

London, England (presumably)  
162 YBN
[1838 AD]
2814)
Maynooth, Ireland  
162 YBN
[1838 AD]
2815)
Maynooth, Ireland  
162 YBN
[1838 AD]
2854)
(Ecole Polytechnique) Paris, France (presumably)  
162 YBN
[1838 AD]
2891) Johannes Peter Müller (MYUlR) (CE 1801-1858), German physiologist,
publishes "Über den feineren Bau und die Formen der krankhaften Geschwülste"
(1838, "On the Nature and Structural Characteristics of Cancer, and of Those
Morbid Growths Which May Be Confounded with It"), a book on the pathology
((progress over time)) of tumors, which begins to establish pathological
histology as an independent branch of science.

Histology is a branch of biology concerned with the composition and structure
of plant and animal tissues in relation to their specialized functions.

(University of Berlin) Berlin, Germany  
162 YBN
[1838 AD]
2918)
Rotterdam?, Netherlands (presumably)  
162 YBN
[1838 AD]
2934) Schleiden mistakenly believes that new cells bud out of the nucleus.
Schle
iden is one of the first German biologists to accept Darwin's theory of
evolution.
Schleiden is a successful science popularizer in lectures and in articles.

The Encyclopedia Britannica compares the importance of Schleiden's cell theory
to the atomic theory of chemistry.
(University of Jena) Jena, Germany  
162 YBN
[1838 AD]
3006)
(Royal Observatory) Bogenhausen, Germany  
162 YBN
[1838 AD]
3067)
New York City, NY, USA  
162 YBN
[1838 AD]
3157) Remak is barred from teaching by Prussian law, which forbids Jewish
people to be employed as teachers. Remak does his research as an unpaid
assistant in Müller's laboratory and supported himself by his medical
practice. In 1843 Remak petitions directly to Friedrich Wilhelm IV for a
teaching position, but is refused. Finally in 1847, Remak is hired as a
lecturer at the University of Berlin, becoming the first Jewish person to teach
at the University of Berlin. (It's amazing how focused people are on race,
which to me seems unimportant other than working towards racial integration.)
(University of Berlin) Berlin, Germany (presumably)  
162 YBN
[1838 AD]
3386)
?, England  
162 YBN
[1838 AD]
3509)
Berlin, Germany   
162 YBN
[1838 AD]
3589)
London, England  
162 YBN
[1838 AD]
6003)
Paris, France (verify)  
162 YBN
[1838 AD]
6213)
  
161 YBN
[01/09/1839 AD]
2617) Daguerre specializes in painting scenic backdrops for theaters.
Working
with Charles-Marie Bouton Daguerre invents the diorama - a display of paintings
on semitransparent linen that transmit and reflect light - and opens a diorama
in Paris (in 1822).

Niépce, who since 1814 has been trying to create permanent pictures by the
action of sunlight, learns in 1826 of Daguerre's efforts in the same field.
Niépce
and Daguerre became partners in the development of Niépce's heliographic
process from 1829 until the death of Niépce in 1833.

The first permanent photograph from nature was made around 1826 by Nicéphore
Niépce, but this photo is of poor quality and requires about eight hours of
exposure time. The process that Daguerre develops (the daguerreotype process)
required only 20 to 30 minutes. The daguerreotype is the first practical
photograph.

Niepce's heliography depends on the hardening action of sunlight on bitumen and
the subsequent (dissolving) of the (dark unlit) parts of the image. Using this
method on a glass plate, Niépce had obtained and fixed a photograph from the
camera obscura in 1826. But Niepce wants to create a photoengraved plate from
which (paper prints can be copied). This goal leads to Niepce using bitumen on
silver-coated copperplates and then iodizing the silver revealed after
dissolving the unexposed bitumen. The removal of the hardened bitumen produces
a silver-silver iodide image. But Niépce goes no further.

Daguerre (working with Niepce) makes the first permanent image using a pin-hole
camera (a camera obscura, Italian for "dark room") with a lens and a copper
plate with silver salts deposited on it.
Building on his partner Niepce's
foundation, Daguerre discovers the light sensitivity of silver iodide in 1831
but is unable to obtain a visible image. Daguerre discovers in 1835 that the
latent image present on a silver iodide plate exposed for only 20 minutes can
be developed with mercury vapor marks a major advance. Fixing this image is
achieved in 1837, when Daguerre removes the unreduced silver iodide with a
solution of common salt (and water). Having improved Niépce's process,
Daguerre calls this process the daguerreotype (process).

After 20 minute exposures, light portions darken the silver salts and dark
areas leave the light-sensitive layer of silver iodide and bromide (silver
salts) unaffected.
The unchanged salts are then dissolved away with sodium
thiosulfate (a process suggested by John Hershel), and a permanent image is
left behind (on the copper plate?).

By 1840 the Daguerreotype technique will be used to record astronomical images.


Before this the camera obscura or pinhole camera is popular. Sunlight enters a
room through a small opening and is made to fall onto a screen to show a sharp
image of whatever is outside the room. People had inserted a lens in the
pinhole in order to make possible a larger opening and more light without
affecting the sharpness of the focus. (The so-called pin-hole camera, is a
basic thing that all people should see and is very easy to create by simply
making two holes in a cardboard box and looking through one to see light going
through the other hole projected on the back wall which produces the scene
horizontally and vertically backwards. It's interesting that light enters a
tiny hole and shows a large scene. It means that light of many different
directions is entering the hole.)

On January 9, 1839, a full description of the daguerreotype process is
announced at a meeting of the Academy of Sciences by the eminent astronomer and
physicist François Arago. (Does Daguerre patent his invention?)

Daguerre describes the process as consisting of five operations: the polishing
of the (copper) plate; the coating of the plate with iodide of silver by
submitting it for about 20 minutes to the action of iodine vapor; the
projection of the image of the object upon the golden-colored iodized surface;
the development of the latent image by means of the vapor of mercury (how is
the vapor produced?); and, lastly, the fixing of the picture by immersing the
plate in a solution of sodium "hyposulphite" (sodium thiosulphate).

Daguerre's "Historique et description des procedes du daguerreotype et du
diorama" (Paris, 1839) passes through several editions, and is translated into
English. Besides this Daguerre writes an octavo work (paper is in octavo when a
whole single sheet is folded three times to form eight leaves; a book is called
an "octavo" size when made up of sheets folded three times), entitled "Nouveau
moyen de preparer la couche sensible des plaques destinees a recevoir les
images photographiques" (Paris, 1844).

(One question for the excluded historian/scientist is: when did people start
secretly using cameras and microphones to spy on people? It must have been very
recently after the invention, and who did all the spying? Probably the wealthy,
and those who use taxpayer wealth in governments.)
(This process of capturing a permanent
image of light will grow to include moving images by Thomas Edison in 1889, and
in 1910 light that people see will first be captured from behind people's heads
by Michael Pupin making the first "eye image" and the surprising find that the
brain can generate its own images from past memories, what people generally
call "thought". This find will show how similar the brains of all the species
are, having the ability to remember images in their mind. But sadly these will
be kept secret from the public, {as will hearing thought, recording the sounds
people think of, and the technology of sending images, sounds and even
triggering muscle movements remotely to brains} for 9 years and counting.)
(The
box with a hole to only allow a small amount of light in is useful to filter
out large amounts of light from many sources and directions.)
Paris, France  
161 YBN
[01/31/1839 AD]
2834)
Wiltshire, England (presumably)  
161 YBN
[01/??/1839 AD]
3103)
(University of Basel) Basel, Switzerland  
161 YBN
[02/21/1839 AD]
2833)
Wiltshire, England (presumably)  
161 YBN
[02/??/1839 AD]
3100) In his Philosophical Magazine postscript of January 1839, Groves writes
"I should have pursued these experiments further, and with other metals, but
was led aside by some experiments with different solutions separated by a
diaphragm and connected by platinum plates; in many of these I have been
anticipated.
I will however mention one which goes a step further than any hitherto
recorded; and affords, I think, an important illustration of the combination of
gases by platinum.
Two strips of platinum 2 inches long and three-eighths of an inch
wide, standing erect at a short distance from each other, passed, hermetically
sealed, through the bottom of a bell glass; the projecting ends were made to
communicate with a delicate galvanometer; the glass was filled with water
acidulated with sulphuric acid, and both the platina strips made the positive
electrodes of a voltaic battery until perfectly clean, &c; contact with the
battery having been broken, over each piece of platinum was inverted a tube of
gas, four-tenths of an inch in diameter, one of oxygen, the other of hydrogen,
acidulated water reaching a certain mark on the glass so that about half of the
platina was exposed to the gas, and half to the water. The instant the tubes
were lowered so as to expose part of the surface of platinum to the gases, the
galvanometer needle was deflected so strongly as to turn more than half round;
it remained stationary at 15°, the platinum in the hydrogen being similar to
the zinc element of the pile. When the tubes were raised so as to cover the
plates with water, the needle returned slowly to zero; but the instant that the
tubes were lowered again, it was again deflected; if the tubes were changed
with regard to the platina, the deflection was the contrary side.
The action lowered
considerably after the first few minutes, but was in some degree restored every
time the tubes were raised so as to wash the surface of the platina, and again
lowered. After 24 hours, the water had risen half an inch in the tube
containing oxygen. in two other tubes, without platina, but with the same gases
and immersed in acidulated water for the same time, the water had scarcely
perceptibly risen, the effect therefore could not have been due to solution;
the same sheets of platinum were exposed to atmospheres of common air and of
similar gases, i.e. both to oxygen or both to hydrogen, &c, but without
affecting the galvanometer. The platinum in the hydrogen was made the positive,
and that in the oxygen the negative electrode of a single voltaic pair; the
water now rose at the rate of three-eighths of an inch per hour in the hydrogen
tube and proportionally in the oxygen; when the platina was not assisted by a
pair of metals the oxygen was absorbed in more than its relative proportion. I
hope, by repeating this experiment in series, to effect decomposition of water
by means of its composition.".
In an 1845 paper, Grove writes "led me to the result, for
which I have the honour of laying before the Royal Society in this paper.",
which, although it may be a stretch, may imply that "tp" may be telephone
company, or a person with initials TP, although 1845 is an early date for even
telegraph. But more likely, there appears to be subtle sex-based joking in many
Philosophical Transaction papers - some take a positive tone and others a
negative tone. Faraday took a positive tone, Priestley referred to "Canton's
balls", and here "the honour of laying before the Royal Society" has to be a
play on laying as having sex before the Royal Society. But this paper, may also
imply that people might be so intrusive as to inspect a toilet paper. All this
is speculation in an effort to understand the secret inside jokes of wealthy
and educated in London society in 1845.
London, England  
161 YBN
[07/29/1839 AD]
3308) Alexandre Edmond Becquerel is the son of Antoine-César Becquerel
(1788-1878) whom Edmond assists when young and eventually succeeds as director
of the Muséum d'Historie Naturelle in 1878.

Becquerel is interested in fluorescence, where a substance absorbs light of one
wavelength and emits light of a different wavelength. Becquerel's son will
identify (high speed?) electrons (beta particles) emitting from uranium.

People now have nanometer sized photovoltaic devices that can even detect
infrared light and can fly.

(Does Becquerel understand that the effect is light on the metal only, and not
the liquids (although the liquids must serve as carriers of the electrons)?)
(University of Paris) Paris, France  
161 YBN
[1839 AD]
2581) Also in this year, Purkinje creates the planet's first independent
department of physiology at the University of Breslau.
(Breslau, Prussia now:)Wroclaw, Poland  
161 YBN
[1839 AD]
2631) John Frederic Daniell (CE 1790-1845) experiments on the fusion of metals
with a 70-cell battery. Daniell produces an electric arc so rich in ultraviolet
rays that it results in an instant, artificial sunburn.

London, England (presumably)  
161 YBN
[1839 AD]
2660)
Liverpool (and Manchester), England  
161 YBN
[1839 AD]
2684)
Calcutta, India  
161 YBN
[1839 AD]
2711) Michael Faraday (CE 1791-1867) puts forward a new theory of electrical
action. Electricity, whatever it was, causes tensions in matter. When these
tensions snap in a conductor, there is a cyclical repetition of buildup,
breakdown, and buildup of tension that, like a wave, passes along the
substance. In electrochemical processes the rate of buildup and release of
strain is proportional to the chemical affinities of the substances involved.
In Faraday's view the current is not a material flow but a wave pattern of
tensions and their relief. (Did Faraday reject the atomic theory?). In
Faraday's view insulators are materials whose particles can take an
extraordinary amount of strain before snapping. Electrostatic charge in an
isolated insulator is simply a measure of this accumulated strain. Therefore,
according to Faraday, all electrical action is the result of forced strains in
bodies.

(Royal Institution in) London, England  
161 YBN
[1839 AD]
2721) In 1831 Murchison is elected president of the Geological Society of
London.
London, England (presumably)  
161 YBN
[1839 AD]
2730) Herschel also coins the term "snapshot".
London, England (presumably)  
161 YBN
[1839 AD]
2755)
Cambridge, England (presumably)  
161 YBN
[1839 AD]
2762)
(Guy's Hospital) London, England  
161 YBN
[1839 AD]
2800) Lanthanum has the symbol La, atomic number 57, atomic weight 138.91.
Lanthanum, is a metal and the second most abundant element in the rare-earth
group. The naturally occurring element is made up of the isotopes 138La
(0.089%) and 139La (99.91%). 138La is a radioactive positron emitter with a
half-life of 1.1 × 1011 years. Lanthanum occurs associated with other rare
earths in monazite, bastnasite, and other minerals. Lanthanum is one of the
radioactive products of the fission of uranium, thorium, or plutonium.
Lanthanum is the most basic of the rare earths and can be separated rapidly
from other members of the rare-earth series by fractional crystallization.
Large quantities of Lanthanum are separated commercially because it is an
important ingredient in glass manufacture. Lanthanum imparts a high refractive
index to the glass and is used in the manufacture of expensive lenses. The
metal is readily attacked in air and is rapidly converted to a white powder.
Lanthanum becomes a superconductor below about 6 K -449°F) in both the
hexagonal and face-centered crystal forms.
(Caroline Medical Institute) Stockholm, Sweden  
161 YBN
[1839 AD]
2820)
(University of Edinburgh)Edinburgh, Scotland (and observation in Cape Town,
South Africa)  
161 YBN
[1839 AD]
2862) Goodyear patents this process in 1844, but the process is too simple and
like Whitney's cotton gin many people copy it. Goodyear spends all his time
with 60 court cases. Goodyear wins his case in 1852, but dies in debt. When
Goodyear dies in 1860, he leaves his wife and six children $200,000 in debt.

The major use of this rubber will be in automobile tires 50 years after
Goodyear's death.

The Goodyear Tire and Rubber Company (founded 1898) honors Goodyear's name.
Woburn, Massachussetts, USA (presumably)  
161 YBN
[1839 AD]
2866)
Cambridge, England  
161 YBN
[1839 AD]
3030) With a £1,000 Treasury grant, obtained through the Cambridge network,
Darwin hires the best experts and publishes their descriptions of his specimens
in "Zoology of the Voyage of H.M.S. Beagle" (1838-43).
London, England (presumably)  
161 YBN
[1839 AD]
3063) Regnault is an active amateur photographer and introduces the use of
pyrogallic acid as a photographic developer (c. 1845-7). Regnault is one of the
first photographers to use paper negatives. In 1854, Regnault becomes the
founding president of the Société Française de Photographie.

Regnault takes samples of air from different parts of Earth and demonstrates
that all over the Earth, the air contains about 21% oxygen.

Regnault is credited with the invention of the air thermometer. Regnault
introduces the use of an accurate air-thermometer, and compares its indications
with those of a mercury thermometer, determining the (specific heat) of mercury
as a step in the process. Regnault devises a hygrometer in which a cooled metal
surface is used for the deposition of moisture.

Carbon tetrachloride has atomic formula CCl4, colorless, poisonous, liquid
organic compound that boils at 76.8°C. It is toxic when absorbed through the
skin or when inhaled. It reacts at high temperatures to form the poisonous gas
phosgene. Carbon tetrachloride is used in the production of Freon refrigerants,
for example, Freon-12 (dichlorodifluoromethane). Because it is not flammable
and is a good solvent for fats, oils, and greases, carbon tetrachloride is
often used commercially for dry cleaning and for degreasing metals.
Regnault grows up
in poverty struggling to maintain himself and a sister.
Regnault loses much of the
results of his chemical work and his son Henri is killed as a result of the
Franco-German War (1870-1871).
(University of Lyons) Lyons, France  
161 YBN
[1839 AD]
3072) Schwann knows Mathias Schleiden well, and a year after Schleiden, working
at University of Jena, advances the cell theory for plants, Schwann extends it
to animals in his "Microscopical Researches into the Accordance in the
Structure and Growth of Animals and Plants" (1839).

Schwann more clearly states and summarizes the theory. Schwann states that
plants and animals are formed out of cells, that eggs are cells distorted by
the presence of yolk, that eggs grow and develop by constant dividing so that
the developing organism consists of more and more cells, but always of cells.
Schwann refines Bichat's concept of tissues, by differentiating tissues by cell
types. Asimov describes the cell theory as a landmark of biology, comparable to
the atomic theory as a landmark of chemistry.

The Concise Dictionary of Scientific Biography states that Schwann's cell
theory can be regarded as marking the origin in biology of the school of
mechanistic materialism that Brückem, du Bois-Raymond, Helmholtz, and Carl
Ludwig make famous. According to Schwann, the theory that leads from the
chemical molecule to the organism by way of the universal stage of the cell, is
inspired by an intellectual, mechanistic reaction to Müller's vitalism.

Schwann states that the cell theory demonstrates that the great barrier between
the animal and vegetable kingdoms vanishes.

Schwann proposes three generalizations concerning the nature of cells: First,
animals and plants consist of cells plus the secretions of cells. Second, these
cells have independent lives, and third, these lives are subject to the
organism's life. In addition Schwann realizes that the phenomena (or perhaps
purpose or activity?) of individual cells can be placed into two classes:
"those which relate to the combination of the molecules to form a cell. These
may be called plastic phenomena," and those phenomena "which result from
chemical changes either in the component particles of the cell itself, or in
the surrounding cytoblastema (modern cytoplasm). These may be called metabolic
phenomena." With this Schwann coins the term "metabolism," which becomes
generally adopted for the sum total of chemical processes by which energy
changes occur in living things. (The word "metabolism" is somewhat abstract, as
is the term "energy" when applied to living objects. At the basic level there
is a conservation of velocity and mass, however, there needs to be language and
descriptions more specifically adapted to more complex processes that result
from many millions of pieces of matter interacting together in routine ways.)

Schwann classifies tissues into five groups: 1) separate independent cells,
such as blood; 2) compacted independent cells, such as skin; 3) cells whose
walls have coalesced, such as cartilage, bones, and teeth; 4) elongated cells
which have formed fibers, such as tendons and ligaments; and finally, 5) cells
formed by the fusion of walls and cavities, such as muscles and tendons. (what
is the modern classification of cells?)

The first cell is at least 3.8 billion years old and is the basis for all of
life on earth. Everything object alive today is descended from a single
individual cell that divided. Cell structure is old, however, free living DNA
and/or RNA molecules are viewed as the oldest ancestors of living objects.
(University of Louvain) Louvain, Belgium  
161 YBN
[1839 AD]
3075) First nude human photograph.

  
161 YBN
[1839 AD]
3090) John William Draper (CE 1811-1882), English-US chemist makes one of the
earliest daguerreotype portraits (1839).

Draper discovers that by increasing the (diameter) (aperture) of the lens and
reducing its focal length he can drastically reduce exposure time. In December
1840 Draper is using a lens with an f1.4 aperture (focal length 1.4 inches).

Draper reduces the exposure time of photography to under a minute.
Draper founds the
School of Medicine at New York University.
Draper creates a partnership with Samuel Morse,
a colleague at New York University. Morse is the beginning of recording
people's messages to each other, which grows into the telephone company and a
massive microscopic secret visible and thought cameras, microphones, and remote
neuron activation network. So Draper, in particular in New York City the center
of much of this development, must have been a part of that.

In 1876 Draper is elected the first President of the American Chemical Society.

From 1850-1873, Draper is the president of the University of the City of New
York.

Draper's son, Henry Draper (1837-1882) also teaches at the University of the
City of New York.
(New York University) New York City, New York, USA  
161 YBN
[1839 AD]
3099) In 1847 Franklin Leonard Pope describes the Grove battery in "Modern
Practice of the Electric Telegraph: A Handbook for Electricians" like this:
"The most intense and powerful voltaic combination that has yet been discovered
is that of Grove. For many years it was exclusively used for telegraphic
purposes in this country, and is still employed in that capacity to a
considerable extent. Its component parts are shown in Fig. 5, in which A
represents a glass jar or tumbler, about 3 inches in diameter and 4 1/2 inches
high. A thick cylinder of zinc, B, of a size nearly sufficient to fill the
tumbler, is placed within it, and is furnished with a projecting arm, to which
is attached the positive plate of the next element. The porous cup, C, is
placed within the zinc. A thin strip of platina, D, about 2 1/2 inches long and
half an inch in width, is soldered to the end of the zinc arm projecting from
the adjacent cell, and reaches nearly to the bottom of the porous cup.
Setting up a
Grove Battery. It is necessary that the zinc should first be thoroughly
amalgamated. The ordinary zinc of commerce contains particles of lead, iron,
and other impurities, which, when the plate is immersed in dilute acid, form as
it were small batteries upon the surface, which eat away numerous cavities in
the zinc without producing any useful effect. This is prevented by the above
process of amalgamation, which is usually performed by immersing the zincs in a
vessel containing dilute muriatic or sulphuric acid, and then plunging them in
a bath of metallic mercury. After remaining in this for a minute or two they
are taken out and placed in a vat of clean water, where the superfluous mercury
is allowed to drain off. The mercury dissolves a little of the zinc, which
flows over and covers the impurities, and prevents the acid solution from
coming in contact with them.

In putting the Grove battery together, first place the glass tumblers in
position and fill them about half full of a solution composed of one part of
sulphuric acid and twenty to thirty parts water, by measure, thoroughly mixed.
Then place the amalgamated zincs in the tumblers, with the arms turned at right
angles to the line of cells. Fill the porous cups nearly full of strong nitric
acid and place them within the zincs, then turn the zincs around so as to
immerse the platina strips in the nitric acid of the adjoining cell, throughout
the whole series, as shown at T, in Fig. 5.
The strength of the dilute sulphuric
acid solution in this battery should be varied in proportion to the number of
wires worked from it. The less the number of the latter the weaker the solution
may be made.

When in continuous service a Grove battery ought to be taken apart every night,
and the nitric acid from the porous cups emptied into a vessel and kept closed
until morning. The zincs should be removed and placed inverted in a trough of
water, acidulated with sulphuric acid, and in the morning rubbed with a brush,
and the mercury diffused evenly over their surfaces. To every ten parts of the
nitric acid taken from the battery add one part of fresh acid every morning. By
this means a steady and uniform current will be maintained when the battery is
in action. The dilute sulphuric acid requires renewal about twice a week. In
handling this battery great care is required not to injure the connection
between the zinc and the platina. A set of Grove zincs, in continuous service,
will require renewal about once in three months.".

Groves takes a considerable interest in photographic science during the 1840s.
London, England  
161 YBN
[1839 AD]
3102)
London, England  
161 YBN
[1839 AD]
3106)
Bristol, England (presumably)  
161 YBN
[1839 AD]
3137)
Berlin, Germany  
161 YBN
[1839 AD]
3469)
(University of Basel) Basel, Switzerland  
160 YBN
[03/12/1840 AD]
3875)
London, England (presumably)  
160 YBN
[12/17/1840 AD]
3238) The entire paper is this: "The inquiries of the author are directed to
the investigation of the cause of the different degrees of facility with which
various kinds of metal, of different sizes, are heated by the passage of
voltaic electricity. The apparatus he employed for this purpose consisted of a
coil of the wire, which was to be subjected to trial, placed in a jar of water,
of which the change of temperature was measured by a very sensible thermometer
immersed in it; and of a galvanometer, to indicate the quantity of electricity
sent through the wire, which was estimated by the quantity of water decomposed
by that electricity. The conclusion he draws from the results of his
experiments is, that the calorific effects of equal quantities of transmitted
electricity are proportional to the resistance opposed to its passage, whatever
may be the length, thickness, shape, or kind of metal which closes the circuit;
and also that, caeteris paribus, these effects are in the duplicate ratio of
the quantities of transmitted electricity, and, consequently, also in the
suplicate ratio of the velocity of transmission. He also infers from his
researches that the heat produced by the combustion of zinc in oxygen is
likewise the consequence of resistance to electric conduction.".

I think that measuring temperature is difficult, because the temperature is
only measured in the volume of the device doing the measuring. In addition, if,
for example mercury expansion is used as a guide, only photons that mercury
atoms absorb effect the measurement, while those reflected or otherwise not
absorbed by mercury are not counted. So perhaps other liquids or gases might
produce different temperatures in similar locations. EXPER: How does the
expansion of different liquids and gases relate to temperature? Since some must
absorb more photons than others, clearly some expand more than others. For
example, chlorine being yellow, does the absence of yellow frequency photon
absorption change the quantity of expansion relative to clear gases? It would
seem that different materials (solids, liquids, gases) have different rates of
expansion given some constant temperature simply because theoretically they
absorb different frequencies of photons.

(It is fun to speculate about what causes heat emitted from wires electric
current is passed through. I think the collisions between the moving electrons
with other particles, such as metal atoms, causes photons to be knocked loose
to exit the atom. Those photons are then absorbed by surrounding material such
as air and water, etc. and this raises their temperature. I think it has to do
with conservation of velocity ultimately. Velocity is transferred from the
moving electrons to the surrounding medium. The velocity was there perhaps in
orbiting photons, and is released - so instead of moving in circles the photon
then moves in a straight line.)
Joule comes from a wealthy family.
Joule's father is a
brewer, and Joule works in his father's brewery.
Joule has a spine injury that prevents
him from participating in many activities.
Joule's wife dies after only 6 years
of marriage. (how?)
Joule never takes a job and spends his life performing experiments
in his own laboratory at his own expense.
Although not initially received, eventually in
1849 Faraday sponsors Joule to read a paper on his work before the Royal
Society.
In 1850 Joule is elected to the Royal Society.
In 1866 Joule wins the Copley
medal.
Joule remains a brewer all his life and is never a professor.
Broom Hill (near Manchester), England  
160 YBN
[1840 AD]
2563) Giovanni Battista Amici (omECE) (CE 1786-1686) invents the oil-immersion
technique, in which the objective (lower) lens (of a microscope) is immersed in
a drop of oil which is placed on top of the specimen under observation in order
to minimize light aberrations. (So the oil is constant from the specimen to the
lens?)

Florence, Italy (presumably)  
160 YBN
[1840 AD]
2778) William Whewell (HYUuL) (CE 1794-1866), English scholar publishes
"Philosophy of the Inductive Sciences" (1840) which begins with the claim that
"Man is the interpreter of Nature, science is the right interpretation".

Cambridge, England  
160 YBN
[1840 AD]
2827) Ozone is an irritating, pale blue gas that is explosive and toxic, even
at low concentrations.
Ozone is formed naturally in the ozone layer from
atmospheric oxygen by electric discharge or exposure to ultraviolet radiation.
Ozone is a highly reactive oxidizing agent used to deodorize air, purify water,
and treat industrial wastes.

Ozone gas decomposes rapidly at temperatures above 100° C (212° F) or, in the
presence of certain catalysts, at (lower ) temperatures.
At -112 °C, ozone forms a dark blue
liquid. At temperatures below -193 °C, it forms a violet-black solid. Ozone
usually is manufactured by passing an electric discharge through a current of
oxygen or dry air. The resulting mixtures of ozone and original gases are good
enough for most industrial purposes. Purer ozone can be obtained from them by
various methods; for example, on liquefaction, an oxygen-ozone mixture
separates into two layers, of which the denser one contains about 75 percent
ozone. The extreme instability and reactivity of concentrated ozone makes its
preparation both difficult and hazardous.
In 1828 Schönbein joins the faculty of the
University of Basel, in Switzerland.
In 1835, Schönbein is appointed professor of chemistry
and physics at the University of Basel, staying there for the rest of his
life.
Schönbein rejects the atomic theory.
Schönbein (correctly) thinks that Scheele was
wrong in thinking chlorine a compound and Davy correct in proving chlorine to
be an element.

In his lifetime Schönbein produces more than 360 scientific papers.
(University of Basel) Basel, Switzerland  
160 YBN
[1840 AD]
2855)
(Ecole Polytechnique) Paris, France (presumably)  
160 YBN
[1840 AD]
2902)
(King's College) London, England (presumably)  
160 YBN
[1840 AD]
2904)
(King's College) London, England (presumably)  
160 YBN
[1840 AD]
2911) (Sir) Charles Wheatstone (WETSTON) (CE 1802-1875), English physicist
builds a magneto-electrical machine (electric generator) for generating
continuous currents.

(King's College) London, England (presumably)  
160 YBN
[1840 AD]
2914)
(University of Saint Petersberg) Saint Petersberg, Russia (presumably)  
160 YBN
[1840 AD]
2921)
(University of Giessen), Giessen, Germany  
160 YBN
[1840 AD]
2936) (Sir) Richard Owen (CE 1804-1892), English zoologist publishes
"Odontography" (1840-45), a major study of the structure of teeth.

(Hunterian museum of the Royal College of Surgeons) London, England  
160 YBN
[1840 AD]
3051) After studying medicine at Heidelberg and at Bonn, where Henle gets his
doctor's degree in 1832, Henle becomes prosector in anatomy to Johannes Muller
at Berlin. During the six years henle spends in this position he publishes a
large amount of work, including three anatomical monographs on new species of
animals, and papers on the structure of the lacteal system, the distribution of
epithelium in the human body, the structure and development of the hair, the
formation of mucus and pus, and the first descriptions of the structure and
distribution of human epithelial tissue and of the fine structures of the eye
and brain.

Henle recognizes that all inner and outer surfaces of the body are lined with
epithelial tissue. (chronology)

Henle makes numerous microanatomical finds, the best known being Henle's loop,
a part of the kidney tubule. In addition, "Henle's fibers", which are the inner
fibers of photoreceptors, Hassle-Henle bodies.
In 1835 Henle is arrested for
belonging to a radical students' movement, sentenced to seven years in prison,
but soon released. According to Asimov, Henle's liberal views bring him to
trial for treason in Berlin and a short period of imprisonment.
(University of Zürich) Zürich, Germany  
160 YBN
[1840 AD]
3091)
(New York University) New York City, New York, USA  
160 YBN
[1840 AD]
3123) Stas has liberal views, and is openly critical of the part played by the
Christian church in education. (more specific)
(Ecole Polytechnique) Paris, France (presumably)  
160 YBN
[1840 AD]
3230) Du Bois-Reymond works at the University of Berlin (1836–96) under
Johannes Müller, whom he later succeeds as professor of physiology (1858).
Du
Bois-Reymond is an early supporter of evolution.
Du Bois-Reymond's collaboration with
fellow physiologists Hermann von Helmholtz, Carl Ludwig, and Ernst von Brücke
is of great significance in linking animal physiology with physical and
chemical laws. Mijalo Pupin studies under Helmholtz in Berlin, so there is a
clear continuity between this research and the view that Pupin is the first
person to see images stored and generated by the brain remotely using a camera
that detects a specific frequency of radio or microwave light. In addition the
finding of the as of yet unknown P.C. who first remotely makes muscles move.
All of this technology apparently connected with the phone companies of earth.
Du
Bois-Reymond considers the history of science the most important, but most
neglected part of cultural history.
In 1867 Du Bois-Reymond is appointed perpetual
secretary of the Berlin Academy of Sciences.
Du Bois-Reymond serves as
president of both the Physical and the Physiological societies of Germany and
is elected a foreign fellow of the Royal Society of London.

Du Bois-Reymond rejects the theory of vitalism and is a "materialist". Du
Bois-Reymond writes memoirs of some of the materialistic philosophers,
including Voltaire and Denis Diderot.
(University of Berlin) Berlin, Germany  
160 YBN
[1840 AD]
3360)
Leipzig, Germany (presumably)  
160 YBN
[1840 AD]
4004)
(École Polytechnique) Paris, France (presumably)  
159 YBN
[01/01/1841 AD]
2836) (Sir) James Clark Ross (CE 1800-1862), Scottish explorer names Mt.
Erebus, (located on Antarctica) after one of his ships. Mt. Erebus is the
southern-most active volcano known.

Ross publishes "A Voyage of Discovery and Research in the Southern and
Antarctic Regions" (1847).

Boothia Peninsula,Nunavut, Canada  
159 YBN
[01/11/1841 AD]
3600)
London, England  
159 YBN
[11/02/1841 AD]
3246)
Broom Hill (near Manchester), England  
159 YBN
[1841 AD]
2542) Friedrich Wilhelm Bessel (CE 1784-1846), In 1841 Bessel deduces a value
of 1/299 for the ellipticity of the Earth (the amount of elliptical distortion
the Earth's shape departs from a perfect sphere by). The study of the Earth's
size and shape is called "geodesy" ("Geometrics" is an alternative title).

Königsberg, (Prussia now:) Germany  
159 YBN
[1841 AD]
2543) Friedrich Wilhelm Bessel (CE 1784-1846), publishes "Astronomische
Untersuchungen" (1841-42). (more info)

Königsberg, (Prussia now:) Germany  
159 YBN
[1841 AD]
2582) Jan (also Johannes) Evangelista Purkinje (PORKiNYA or PURKiNYA) (CE
1787-1869), improves the stroboscopic viewer of Simon Stampfer and J. A. F.
Plateau with his "Phorolyt" device which is marketed in two sizes as a
scientific toy. In the 1850s Purkinje will produce a disc holding nine posed
photographs of a simple movement intended for projection when his Kinesiskop
viewer is attached to a magic lantern. With this apparatus, in 1861, Purkinje
demonstrates the action of the human heart and the circulation of blood, using
individual photographs of each sequence of the heart's movement. Purkinje's
Kinesiskop discs are used in his lectures throughout the decade; one survives
at the Technical Museum, Prague.

(Breslau, Prussia now:)Wroclaw, Poland  
159 YBN
[1841 AD]
2722)
London, England (presumably)  
159 YBN
[1841 AD]
2750) Charles Babbage (CE 1792-1871), English mathematician, publishes "Table
of the Logarithms of the Natural Numbers from 1 to 108000" (1841, London,
William Clowes and Sons).

Cambridge, England (presumably)  
159 YBN
[1841 AD]
2781)
(Dorpat Observatory) Dorpat (Tartu), Estonia  
159 YBN
[1841 AD]
2903)
(King's College) London, England (presumably)  
159 YBN
[1841 AD]
2948)
(University of Königsberg) Königsberg, Germany  
159 YBN
[1841 AD]
3023)
Newcastle, England  
159 YBN
[1841 AD]
3052)
(University of Zürich) Zürich, Germany  
159 YBN
[1841 AD]
3053)
(University of Heidelberg) Heidelberg, Germany  
159 YBN
[1841 AD]
3077)
(University of Marburg), Marburg, Germany  
159 YBN
[1841 AD]
3128)
Birmingham, England   
159 YBN
[1841 AD]
3158)
(University of Berlin) Berlin, Germany (presumably)  
159 YBN
[1841 AD]
3159)
(University of Berlin) Berlin, Germany (presumably)  
159 YBN
[1841 AD]
3190) Kölliker like Nägeli believes that evolution proceeds in jumps.
Kölliker emphasizes the significance of sudden change in evolution as opposed
to gradual change.
In 1848 with Karl von Siebold, Kölliker founds the
"Zeitschrift für wissenschaftliche Zoologie" ("Journal of Scientific
Zoology").
Kölliker plays an influential role in the development of Würzburg
as a leading center of health science (medical) learning.
(University of Zurich) Zurich, Switzerland  
158 YBN
[03/30/1842 AD]
3171) The use of anesthetic gases in surgery was first proposed by British
chemist Sir Humphrey Davy in 1798, following his observation that inhalation of
nitrous oxide relieves pain.

The idea of using ether came to Long after he had engaged in "ether frolics",
parties at which ether is inhaled for the intoxicating effect.
Long participates in
many ether parties and often notices that participants receive bumps and
bruises but experience no pain.
This suggests to him the possibility of using ether
to provide surgical anesthesia. On March 30, 1842, Long removes a small tumor
from the neck of an etherized patient. When the person operated on regains
consciousness he tells Long that he did not experienced any pain. Long follows
this up in July by painlessly amputating the toe of a young etherized boy. Long
does not publish any report of this use until 1849.

Despite Morton's claims to the discovery and the publicity of his
demonstration, Long is recognized as the first to use ether as an anesthetic
for surgery.

There is one earlier record of the administration of ether, for a tooth
extraction: in January 1842, William Clark gave ether to a patient whose tooth
was then removed by Elijah Pope.
Jefferson, Georgia  
158 YBN
[06/17/1842 AD]
2812) Also in this year Henry traces the influence of induction to surprising
distances, magnetizing needles in the lower story of a house through several
intervening floors by means of electrical discharges in the upper story, and
also by the secondary current in a wire 220 ft. distant from the wire of the
primary circuit.
Princeton, NJ, USA  
158 YBN
[07/04/1842 AD]
5837)
Paris, France (presumably)  
158 YBN
[1842 AD]
2733) The cyanotype method of photography is used by Herschel's friend Anna
Atkins to produce the first photographically illustrated book, and later
employed for decades in the form of the architect's blueprint.
London, England (presumably)  
158 YBN
[1842 AD]
2734)
London, England (presumably)  
158 YBN
[1842 AD]
2751) The British government officially withdraws funding and puts the
incomplete "Difference Engine" of Charles Babbage (CE 1792-1871) in the Science
Museum, where it still is located. Babbage then, using his own money, spends
the rest of his life working on the Analytical Engine, but never finishes it.
Babbage is assisted by Lord Byron's daughter, Ada Augusta, the countess of
Lovelace and an amateur mathematician. In spite of his failure to completely
develop a working machine, Babbage (and Lady Lovelace) are legendary heroes in
the prehistory of the computing age. Babbage is sometimes called "the
grandfather of modern computing".

It is possible that at this time the British military decided to fund and
continue this project secretly.

Cambridge, England (presumably)  
158 YBN
[1842 AD]
2798) The evils of racism, such as slavery, or the race-based murder in Nazi
Germany, will use Retzius' and the actual scientific work of other people to
determine differences between humans, fraudulently for their own bad purposes
(in supporting claims of racial separation, inferiority, etc.).
From 1824-1860
Retzius is a professor of anatomy and physiology at the Karolinska
Medic-Kirurgiska Institutet, Stockholm.
Stockholm, Sweden  
158 YBN
[1842 AD]
2923)
(University of Giessen), Giessen, Germany  
158 YBN
[1842 AD]
2929)
(Prague Polytechnic, now Czech Technical University)Prague, Czech
Republic  
158 YBN
[1842 AD]
2937)
(Hunterian museum of the Royal College of Surgeons) London, England  
158 YBN
[1842 AD]
3031) Charles Robert Darwin (CE 1809-1882), English naturalist, drafts a
35-page sketch of his theory of natural selection.

Downe, Kent, England (presumably)  
158 YBN
[1842 AD]
3054) Oliver Wendell Holmes (CE 1809-1894), United States author and physician,
reads "The Contagiousness of Puerperal Fever" (1843), calling attention to the
contagiousness of puerperal fever (a fever relating to, or occurring during
childbirth or the period immediately following). Holmes' investigation
convinces him that physicians are themselves responsible for carrying the
disease from one patient to another. As a result, Holmes advocates the washing
of hands, changing of clothes, and a twenty-four-hour period between handling
corpses and treating patients. However, Holmes' directions are viewed badly by
some who can not believe that physicians could be the source of disease. Yet,
his protocols offered some response to a pressing public health concern and
questioned the relationship between disease, patients, and physicians. Asimov
states that Holmes figured out that childbed fever is caused by doctors not
washing their hands, and that Holmes takes abuse from doctors who view bloodied
and smelly hands with pride.

Holmes names the process of applying ether as "anesthesia" from the Greek word
for "no feeling".

(Holmes recommends the use of soap in washing hands? What kind of soap?)
At the early
age of 33 Holmes becomes the first dean of Harvard Medical School.
Boston, Massachussetts, USA  
158 YBN
[1842 AD]
3150) As ship's physician on a Dutch merchant ship on a voyage to Java (an
island of Indonesia), Mayer realizes that heat and work are interchangeable,
that the same amount of food can be converted to different proportions of heat
and work, but that the total must be the same.

Mayer send his first paper on the subject to Annalen der Physik (Annals of
Physics) where the editor, Johann Poggendorf, does not acknowledge it. however,
Justus von Liebig publishes the paper "Bemerkungen über die Krafte der
unbelebten Natur" ("Comments on the forces of inanimate nature") in the journal
"Annalen der Chemie und Pharmazie" (Annals of Chemistry and Pharmacy).
Mayer is expelled
(from school) for liberal views.
In 1849 Mayer jumps out a 3 story building in a
failed suicide attempt laming himself permanently.
In 1851 Mayer is (locked) in
a mental institution where primitive and cruel methods prevail, however is
later released.
In 1856 Liebig mistakenly refers to Mayer as dead.
In 1871
Mayer receives the Copley medal.
(I think some people feel sympathy for some people
with potential scientific contributions, and I think the important thing is
feel sympathy for all of life, but clearly distinguishing true and false in
terms of science, throwing away any lies or compromises told to be polite,
popular, or warm, etc and also with no regard to gender, race, religion,
political beliefs, just focusing on what is factually true in your own opinion.
And I think that individual scientific beliefs can be asserted, politely, and
compassionately without disrespecting any person.)
Heilbronn, Germany  
158 YBN
[1842 AD]
3152) A neighbor of Lawes explains that on some local farms bone meal increases
turnip production, while on others bone meal seems to have no effect and this
starts Lawes on his life of experimenting on the chemistry of fertilizers.

(One idea that occurs to me is that very large buildings built up or down into
the earth, could grow many rows of plants inside using electric lights which
would be free of many insects, loss of light and wind. In addition, if not
already, eventually, the cost of space above or below the earth is not as much
as the cost on the surface. Inside growing is going to dominate the future in
my opinion, in particular as humans move into orbit and to the planets of other
stars. Also, totally automated systems, where seeding, watering, harvesting,
packaging and distributing are all done automatically with machines and/or
walking robots.)
Rothamsted, England  
158 YBN
[1842 AD]
3156) Forbes devotes much of his life to an extensive study of mollusks and
starfishes, participating in dredgings and expeditions in the Irish Sea (1834),
France, Switzerland, Germany, Algeria (1836), Austria (1838), and the
Mediterranean (1841–42).

Forbes believes in a creation plan as opposed to evolution.

Forbes completes "History of British Mollusca" (4 vol., 1852) in 1852.
Mediterranean Sea  
158 YBN
[1842 AD]
3179) Over the course of his life, more than two hundred and fifty men from a
dozen different countries come to study under Ludwig. (Sadly, at the time women
are not encouraged to pursue the career of physician, which wastes half of the
potential human resource and talent, in addition to creating a second lower
class of people of half the humans.)

Schmiedeberg under Ludwig's guidance in 1866 discovers the accelerator nerve of
the heart of the frog and the dog, and in 1883, Wooldridge finds centrifugal
fibers to the heart of the dog which alter the blood pressure without changing
the rate of the heart beat. Bowditch the best known of the US physiologists in
1871 working with an excised (frog?) heart and frog manometer (an instrument
for measuring the pressure of a fluid, consisting of a tube filled with a
liquid, the level of the liquid being determined by the fluid pressure and the
height of the liquid being indicated on a scale) shows that the heart muscle
either contracts all together or not at all (referred to as the "all or none"
principle), Luciana and Stienon, study the effects of electrical excitation on
the heart muscle and ascertain a number of facts of theoretical importance to
heart and muscle physiology.
(University of Marburg) Marburg, Germany  
158 YBN
[1842 AD]
3284)
France (presumably)  
158 YBN
[1842 AD]
3475) Thompson is an infant prodigy.
William Thomson's father, James Thomson, is a
textbook writer, who teaches mathematics, first in Belfast and later as a
professor at the University of Glasgow.
From 1890-1894 Thompson is president of the
Royal Society.
Thompson rejects the idea that radioactive atoms are disintegrating, or
that the energy they release (in modern terms the photons) comes from within
the atom.
Thomson also opposes Darwin, remaining "on the side of the angels". (To me
this shows a serious limitation on the depth of his logic skills, understanding
of history and basic education.)
After assisting the successful laying of the transatlantic
cable, Thomson becomes a partner in two engineering consulting firms, which
play a major role in the planning and construction of submarine cables during
the period of massive growth that results in a global network of telegraph
communication. Thomson becomes a wealthy man, owning a 126-ton yacht and a
baronial estate.
Thompson is one of the first to support Faraday's lines of force.
Thompson
introduces Bell's telephone to Great Britain.
In retirement, Thomson spends much of his
time in writing and revising the lectures on the wave theory of light which he
had delivered at Johns Hopkins University, Baltimore, in 1884, but which were
not finally published till 1904.
In his lifetime Thomson produces 661 scientific
publications and 70 patents.
(Cambridge University) Cambridge, England  
158 YBN
[1842 AD]
5991) Chopin is a legendary pianist who only gives approximately 30 public
performances in his entire lifetime.

Chopin is a child prodigy and at eight makes his first public appearance at a
charity concert. Three years later Chopin performs in the presence of the
Russian tsar Alexander I, who is in Warsaw to open Parliament. At seven Chopin
writes a Polonaise in G Minor.
Nohant, France  
157 YBN
[02/03/1843 AD]
2641) Morse buys some 250km of (iron?) wire made by the Stephen & Thomas plant
in New Jersey. The Ohio Railway gives Morse permission to use the railroad's
right-of-way. Initially Morse chooses to run the wire underground, using two
wires enclosed in lead pipes. However, after laying about 15km of wire, work is
stopped because the line fails to operate. Morse reads that Cooke and
Wheatstone have shifted from underground to above ground pole mounting of wire,
Morse decides to mount the wire on poles. Upon advice from Joseph Henry, Morse
decides to use two glass plates on each pole separating the two wires. 500
chestnut tree poles, 7 meters (23 feet) high are erected 60 meters apart.
Number 16 copper wire is used, insulated with cotton thread treated with
shellac and a mixture of beeswax, resin, linseed oil, and asphalt. The battery
in Baltimore consisting of acid cells, provides an 80 volt electricity source.
Before this messages are sent by horse, railways had only started in 1830, and
messages from New York to Washington took a day to deliver and 3 weeks to reach
Chicago.

This starts the telegraph era in the United States, which will last more than
100 years. (Is this the origin of AT&T?)

Although the earliest applications of the telegraph is for railroad traffic
control, the telegraph immediately becomes a vital tool for the transmission of
news around the (planet).
Washington DC, USA  
157 YBN
[06/??/1843 AD]
2394)
Paris, France  
157 YBN
[06/??/1843 AD]
2395)
Paris, France  
157 YBN
[08/21/1843 AD]
3239) Joule begins "It is pretty generally, I believe, taken for granted that
the electric forces which are put into play by the magneto-electrical machine
possess, throughout the whole circuit, the same caloritic properties as
currents arising from other sources. And indeed when we consider heat not as a
substance, but as a state of vibration, there appears to be no reason why it
should not be induced by an action of a simply mechanical character, such, for
instance, as is presented in the revolution of a coil of wire before the poles
of a permanent magnet. At the same time it must be admitted that hitherto no
experiments have been made decisive of this very interesting question; for all
of them refer to a particular part of the circuit only, leaving it a matter of
doubt whether the heat observed was generated, or merely transferred from the
coils
in which the magneto-electricity was induced, the coild themselves
becoming cold. The latter view did not appear untenable without further
experiments, considering the facts which I had already succeeded in proving,
viz. that the heat evolved by the voltaic batter is definite (Phil. Mag. ser.
3. vol. xix. p. 275.) for the chemical changes taking place at the same time;
and that the heat rendered ("Memoirs of the Literary and Philosophical Society
of Manchester", 2nd series, vol. vii. p. 97.) - facts which, among others,
might seem to prove that arrangement only, not generation of heat, takes place
inthe voltaic apparatus, the simply conducting parts of the circuit evolving
that which was previously latent in the battery. And Peltier, by his discovery
that cold is produced by a current passing from bismuth to antimony, had, I
conceived, proved to a great extent that the heat evolved by thermo-electricity
is transferred (the quantity of heat thus transferred is, I doubt not,
proportional to the square of the difference between the temperatures of the
two solders. I have attempted an experimental demonstration of this law, but,
owning to the extreme minuteness of the quantities of heat in question, I have
not been able to arrive at any satisfactory result.") from the heated solder,
no heat being generated. I resolved therefore to endeavor to clear up the
uncertainty with respect to magneto-electrical heat. In this attempt I have met
with results which will, I hope, be worthy the attention of the British
Association.".
(read in Cork, Ireland experiments done in:) Broom Hill (near Manchester),
England  
157 YBN
[10/16/1843 AD]
3001)
(Trinity College, at Dunsink Observatory) Dublin, Ireland  
157 YBN
[12/31/1843 AD]
3603) Alexander Bain (CE 1811-1877), machinist, constructs an earth battery, by
creating current between a plate of zinc and copper buried in the ground. Gauss
and Steinheil had previously done this. (chronology)

London, England (presumably)  
157 YBN
[1843 AD]
1614)
Paris, France  
157 YBN
[1843 AD]
2615) Schwabe makes (1831) the first known detailed drawing of the Great Red
Spot on Jupiter.
Dessau, Germany (presumably)  
157 YBN
[1843 AD]
2616)
Dessau, Germany (presumably)  
157 YBN
[1843 AD]
2794) James Braid (CE 1795-1860), Scottish surgeon uses the word "hypnotism"
instead of "mesmerism" or "animal magnetism", and demonstrates that hypnosis is
achieved by suggestion. Braid's writings prepared the way for investigations
into what will be called the unconscious mind.

In 1841, Braid attends a lecture on animal magnetism (mesmerism) given by
Charles Lafontaine, then performs his own experiments with mesmerism. (This
view of animal magnetism descends from the idea that magnets affect humans, and
perhaps Braid seeks to remove this theoretical relation to the method of
hypnosis.)
Braid rejects the popular belief that the ability to induce hypnosis is
connected with the magical passage of a fluid or other influence from the
operator to the patient. Instead Braid adopts a physiological view that
hypnosis is a kind of nervous sleep, induced by fatigue resulting from the
intense concentration necessary for staring at a bright, inanimate object.

Braid finds that he is able to put a person in a trance-like state resembling
sleep but different in being (partially)-conscious and extraordinarily open to
suggestion. Braid describes this as a suspension of the conscious mind, induced
by having been forced into weariness through repetitive stimuli, and calls this
state "hypnotism" from the Greek word for "sleep".

Braid publishes his findings in his book "Neurypnology" (1843), in which Brain
introduces the term "hypnosis".
brain is mainly interested in the therapeutic possibilities
of hypnosis and reports successful treatment of paralysis, rheumatism, and
aphasia. Brain hopes that hypnosis can be used to cure various seemingly
incurable "nervous" diseases and also to alleviate the pain and (fear) of
patients in surgery.


(some people are more easily brought into this condition, while for others it
is virtually impossible. I wonder if "hypnotist" shows are rigged, and if there
is any truth at all to the phenomenon. Seeing and hearing people's thoughts
might reveal. Perhaps the hypnotic state is simply sleeping, or the part of the
brain that controls sleep is activated, or the part that controls the brain
when awake is made to sleep. )

On aspect of the idea of suggestion is how easily an image, sound sent directly
or invoked by stimulated an already existing memory can influence the decisions
made by a brain. This is shown, in particular, in brains that are unaware that
such images, and sounds are being sent or stimulated in their brain, wrongly
believing that their thoughts cannot be externally changed except through the
usual inputs such as eyes, ears, nose, skin, etc. In some sense, perhaps there
is a component of this principle in the phenomenon of hypnosis. More
interesting is how decisions may possibly be automatically made in the brain
without the owner of the brain having any control over any part of their own
brain. Clearly this has been demonstrated for all muscles, so there is every
reason to believe that this may also be true for the movement of all electrical
currents in the cells of any brain. The future of this technology may result in
a voluntary-only use, more user-controlled and pleasant. Some of those people
may enjoy wisely chosen suggestions and information, for example, of what to
eat, which videos to see, potential dangers, etc.

I think hypnotism is a very experimental and mostly ineffective method,
although I have never seen any real studies done. In this time, even now, with
so much pseudo and experimental science in health, mainly psychology, I doubt
the value of hypnosis, and I doubt many of the theories behind so-called
psychiatric diseases. As always, the key concept is consensual treatment only.
How much of the current view of health will change or has already secretly
radically changed as a result of the secret technology of seeing, hearing,
sending images and sounds to and from brains leaves large unanswered questions
for the future. For example, many of those who claimed to hear voices might not
be forcibly treated, pain might be stopped at the neuron, sleep might be able
to be automatically induced at the neuron, health problems more easily
determined by examining thought images, violent people more easily identified
using thought images as evidence, among many countless other improvements.

Braid's findings are opposed at first, but eventually inspire the development
of the French school of neuropsychiatry.

Manchester, England (presumably)  
157 YBN
[1843 AD]
2801) Erbium has symbol Er, atomic number 68, atomic mass 167.26, melting point
1,529°C, boiling point 2,863°C, relative density 9.05 at 25°C, and valence
+3. Erbium is a soft, malleable, lustrous, silvery metal. Erbium is a member of
the lanthanide series in Group 3 of the periodic table. With other rare earths
Erbium's oxide occurs in the mineral gadolinite, found in Sweden. Natural
erbium is a mixture of 6 stable isotopes; in addition, 10 radioactive isotopes
are known. Erbium does not oxidize in air as rapidly as some of the other
rare-earth metals. Erbia is a rose-colored oxide of erbium and has been used to
a very limited extent in glazes and glass as a coloring agent.

What Mossander calls terbia becomes known as erbia and is shown to contain five
distinct rare earths, now called (made singular) erbium, scandium, holmium,
thulium, and ytterbium. Fairly pure erbium oxide is first isolated in 1905;
fairly pure erbium is isolated in 1934.

Terbium is a soft, silvery-gray metallic rare-earth element, used in x-ray and
color television tubes. Atomic number 65; atomic weight 158.925; melting point
1,356°C; boiling point 3,123°C; relative density 8.229; valence 3, 4.

Terbium does not tarnish rapidly in air. Terbium's oxide, terbia, Tb2O3, is
white; its peroxide, Tb4O7, is dark brown to black. Terbium and its compounds
have limited commercial importance; some minor uses are in lasers,
semiconductor devices, and phosphors for color television picture tubes (like
yttrium they must emit light in red frequencies when collided with electrons).
Mosander discovered Terbium in its oxide form originally naming it "erbia", but
has been known as terbium since 1877.
(Caroline Medical Institute) Stockholm, Sweden  
157 YBN
[1843 AD]
2905) (Sir) Charles Wheatstone (WETSTON) (CE 1802-1875), English physicist,
communicates an important paper to the Royal Society, entitled "An Account of
Several New Processes for Determining the Constants of a Voltaic Circuit" which
contains a description of the balance for measuring the electrical resistance
of a conductor, which still goes by the name of "Wheatstone's Bridge" or
balance, although it was first devised by Samuel Hunter Christie, of the Royal
Military Academy, Woolwich, who published it in the Philosophical Transactions
for 1833. The method was neglected until Wheatstone brings it into notice.

The Christie (or Wheatstone) bridge is an electrical bridge circuit used to
measure resistance. It consists of a common source of electrical current (such
as a battery) and a galvanometer that connects two parallel branches,
containing four resistors, three of which are known. One parallel branch
contains one known resistance and an unknown; the other parallel branch
contains resistors of known resistances. In order to determine the resistance
of the unknown resistor, the resistances of the other three are adjusted and
balanced until the current passing through the galvanometer decreases to zero.

(King's College) London, England (presumably)  
157 YBN
[1843 AD]
2924)
(University of Giessen), Giessen, Germany  
157 YBN
[1843 AD]
3092)
(New York University) New York City, New York, USA  
157 YBN
[1843 AD]
3133)
Singapore (and London, England)  
157 YBN
[1843 AD]
3153)
Rothamsted, England (factory at Deptford Creek, England  
157 YBN
[1843 AD]
3194) In 1841, Kopp becomes Privatdozent (unsalaried lecturer) at the
University of Giessen.
Kopp works under Justus Liebig at the University of Giessen.
(University of Giessen) Geissen, Germany  
157 YBN
[1843 AD]
3201) Hofmann studies law and languages at Giessen. (Which may explain how he
successfully worked in England for a long time)
Hofmann studied under Justus von
Liebig at the University of Giessen and received his doctorate in 1841.
Hofmann
is a co-founder of the German Chemical Society (1867) and serves as its
president from 1868–92.

Hofmann is a windower 3 times. (that seems beyond coincidence, but perhaps are
natural deaths.)
Hofmann is the father of 11 children.
Asimov comments that under Hofmann's
leadership, Germany overtakes England and France in the dye industry, until the
WWI British blockade, when the US will develop a chemical industry.

Hofmann synthesizes new dyes.

Most of Hofmann's 360 major papers grow out of his work with the derivatives of
coal tar and the synthesis of related organic compounds.
(University of Bonn) Bonn, Germany  
157 YBN
[1843 AD]
3231)
(University of Berlin) Berlin, Germany  
157 YBN
[1843 AD]
3232) Emil Heinrich Du Bois-Reymond (DYUBWA rAmON) (CE 1818-1896), German
physiologist publishes "Untersuchungen über thierische Elektricität", 2 vol.
(1848–1884; "Researches on Animal Electricity"), which creates the field of
electrophysiology.
Du Bois-Reymond rarely publishes discoveries in separate papers. The bulk of
his work appeared collectively in this, Du Bois-Reymond's most famous book.

(University of Berlin) Berlin, Germany  
157 YBN
[1843 AD]
3301)
London, England  
157 YBN
[1843 AD]
3326) In 1842, Cayley is the champion student ("Senior Wrangler") of his year.
Cayley
spends 14 years working as a barrister, since he is unwilling to take holy
orders, which at the time is a necessary condition of continuing his
mathematical career at Cambridge. When this requirement is dropped, Cayley is
able to return to Cambridge and in 1863 becomes Sadlerian Professor there.
Cayley has
an extraordinarily prolific career, producing almost a thousand mathematical
papers.
In 1876 Cayley publishes his only book "Treatise on Elliptic
Functions".
Cayley's collected papers are published in 13 volumes (1889–98).
In 1882, Cayley is
awarded the Copley Medal by the Royal Society.
London, England (presumably)  
157 YBN
[1843 AD]
3329)
London, England (presumably)  
157 YBN
[1843 AD]
3899)
(private practice) Paris, France  
157 YBN
[1843 AD]
5990)
Leipsig, Germany (presumably)  
157 YBN
[1843 AD]
6240)
Paterson, New Jersey, USA (presumably)  
156 YBN
[05/01/1844 AD]
2643)
Annapolis, Maryland, USA  
156 YBN
[05/24/1844 AD]
2644)
Washington DC, USA  
156 YBN
[06/20/1844 AD]
3245)
(Oak Field Whalley Range near) Manchester, England (presumably)  
156 YBN
[12/31/1844 AD]
3602)
London, England  
156 YBN
[1844 AD]
2642)
Washington DC, USA  
156 YBN
[1844 AD]
2676)
New York City, New York, USA  
156 YBN
[1844 AD]
2707)
(Royal Institution in) London, England  
156 YBN
[1844 AD]
2708) Michael Faraday performs experiments trying to measure an electromagnetic
current produced by the force of gravity when a metal cylinder is allowed to
fall through a coiled wire but no current is produced.

I think that magnetism can be reduced to electricity (as Ampere concluded too),
and that electricity can be reduced to the effects of gravity, and collision.
In my opinion, the most simple explanation is probably the most accurate one.
In this sense, there is only one force in nature, and other forces are only
larger scale effects of a single force (just as field of grass may look like
one object but is made of many individual plants). I think ultimately that both
the attractive and repulsive forces of electricity are mainly due to particle
collision, and ultimately due to the attractive force of gravity.

(Royal Institution in) London, England  
156 YBN
[1844 AD]
2737) Gustave Gaspard de Coriolis (KOrYOlES) (CE 1792-1843), French physicist,
publishes "Traité de la mécanique des corps solides" (1844, "Treatise on the
Mechanics of Solid Bodies").

Paris, France  
156 YBN
[1844 AD]
2795) Ruthenium has atomic number 44, has the symbol "Ru". Ruthenium is a hard
silver-gray acid-resistant metallic element that is found in platinum ores and
is used to harden platinum and palladium for jewelry and in alloys for
nonmagnetic wear-resistant instrument pivots and electrical contacts. Ruthenium
has an atomic mass of 101.07; melting point 2,310°C; boiling point
3,900°C; specific gravity 12.41; valence 0, 1, 2, 3, 4, 5, 6, 7, 8.

Because of its high melting point, ruthenium is not easily cast; its
brittleness, even at white heat, makes it very difficult to roll or draw into
wires.

Natural ruthenium consists of a mixture of seven stable isotopes: ruthenium-96
(5.54 percent), ruthenium-98 (1.86 percent), ruthenium-99 (12.7 percent),
ruthenium-100 (12.6 percent), ruthenium-101 (17.1 percent), ruthenium-102 (31.6
percent), and ruthenium-104 (18.6 percent). Ruthenium has four allotropic
forms. Ruthenium metal does not tarnish in air at ordinary temperatures and
resists attack by strong acids, even by aqua regia.
St. Petersberg, Russia  
156 YBN
[1844 AD]
2832)
Wiltshire, England (presumably)  
156 YBN
[1844 AD]
2897) Jean Baptiste Joseph Dieudonné Boussingault (BUSoNGO) (CE 1802-1887),
French agricultural chemist publishes "Traitt d'economie rurale" (1844), which
is remodeled as "Agronomie, chimie agricole, et physiologie" (5 vols.,
1860-1874; 2nd ed., 1884).

Paris, France (presumably)  
156 YBN
[1844 AD]
3032) Charles Robert Darwin (CE 1809-1882), English naturalist, expands his
1842 sketch into an essay (which will become) "On the Origin of Species by
Means of Natural Selection", but does not intent to publish it.

Darwin writes a letter to his wife Emma in 1844 asking that, if he dies, she
should pay an editor £400 to publish the work.

Downe, Kent, England  
156 YBN
[1844 AD]
3047)
(École Polytechnique) Paris, France  
156 YBN
[1844 AD]
3048) Grassmann is an accomplished linguist, specializing in Sanskrit
literature. At the age of 53 (around 1862), disappointed with the lack of
interest in his mathematical work, Grassman turns all his efforts to Sanskrit
studies. Grassman translates sanskrit texts, and prepares Sanskrit
dictionaries. Grassman's Sanskrit dictionary on the Rigveda is still widely
used.
(Gymnasium in) Stettin, (Prussia now) Poland  
156 YBN
[1844 AD]
3062)
(University of Bern) Bern, Switzerland  
156 YBN
[1844 AD]
3078)
(University of Marburg), Marburg, Germany  
156 YBN
[1844 AD]
3093) John William Draper (CE 1811-1882), English-US chemist captures one of
the first photographs of specimens under a microscope.

(New York University) New York City, New York, USA  
156 YBN
[1844 AD]
3185) Nägeli accepts evolution but puts forward the erroneous theory of
orthogenesis arguing that some inner push drives evolution in a particular
direction, for example increased size.
Nägeli rejects the paper sent to him by
an obscure monk named Mendel. Asimov describes this as Nägeli's most
far-reaching mistake. When this paper is rediscovered 40 years later, it will
serve as the source of the Mendelian laws of inheritance.
(University of Jena) Jena, Germany  
156 YBN
[1844 AD]
3216) Richard Jordan Gatling (CE 1818-1903), US inventor, adapts the cotton
sowing machine for sowing (seed planting) rice, wheat and other grains, and
establishes factories to manufacture these sowing machines.
Gatling is the son of a
wealthy planter and slave-owner.
With his father Gatling perfects machines to sow cotton and
to thin out cotton plants.
In 1839 Gatling perfects a practical screw propeller
for steamboats, only to find that a patent had been granted to John Ericsson
for a similar invention a few months earlier.
Gatling is well educated and is
successively a school teacher and a merchant, spending all his spare time in
developing new inventions.
Because of an attack of smallpox Gatling becomes interested in
the study of health science and completes a course at the Ohio Medical College,
taking his M.D. degree in 1850.
St. Louis, Missouri  
156 YBN
[1844 AD]
3236) Pettenkofer is most familiar in connection with his work in practical
hygiene, advocating good water, fresh air and proper sewage disposal.
Pettenkofer's attention is drawn to this subject around 1850 by the unhealthy
condition of Munich.
In hygiene, Pettenkofer studies the role of ventilation on health
and how contaminated soil and water spread cholera.
Pettenkofer rejects the
germ theory of disease.

Pettenkofer publishes papers on the preparation of gold and platinum, numerical
relations between the atomic weights of analogous elements, the formation of
aventurine glass, the manufacture of illuminating gas from wood.
According to the
Concise Dictionary of Scientific Biography, in 1850, Pettenkofer anticipates
the periodic law of the elements.
In 1892 Pettenkofer deliberately swallows a virulent
culture of cholera bacteria to show his contempt for the germ theory of
disease, but does not become infected.
In 1901, Pettenkofer buys a gun and
shoots himself in old age because of a painful sore throat.
(University of Würzburg) Würzburg, Germany  
156 YBN
[1844 AD]
3237)
(University of Geissen) Geissen, Germany  
156 YBN
[1844 AD]
3294) Foucault is the son of a publisher in Paris and educated at home due to
delicate health. Foucault abandons medical studies unable to bear the sight of
blood.
Foucault is experimental assistant to Alfred Donne (1801-1878) for three years
in Donne's course of lectures on microscopic anatomy.
Paris, France (presumably)  
156 YBN
[1844 AD]
3898)
(Hotel dieu) Paris, France (verify)  
156 YBN
[1844 AD]
6243) Wells is jailed in New York City for throwing acid at passersby and ends
his own life there in a jail cell. (Perhaps Wells was excluded and remote
neuron writing was used to support an association of nitrous oxide with acts of
violence.)
Hartford, Connecticut, USA (presumably)  
155 YBN
[04/02/1845 AD]
3279)
Paris, France (presumably)  
155 YBN
[04/??/1845 AD]
2839) William Parsons, (3d earl of Rosse) (CE 1800-1867), Irish astronomer is
the first person to recognize the spiral shape of the objects at the time
called nebulae, but now known to be galaxies, like our own Milky Way Galaxy.

Parsons' main aim is to build a telescope as large as those of William Herschel
and to discover the nature of the unresolved nebulae found by William Herschel
to determine if they are only gaseous masses in space or are composed of many
stars, like our own Milky Way, as introduced by Kant in his theory of "world
islands". Even the largest telescopes (like those build by Herschel) were not
able to resolve the nebulae (into their spiral shape or into individual stars).
Herschel had left no details of how to grind large mirrors, and so Parsons has
to rediscover all this for himself. Parsons uses an alloy composed of four
atoms of copper to each atom of tin. This alloy is very brittle. Not until 1839
does Parsons make a 3-inch (8-cm) mirror; this is followed by mirrors of 15
inches (38 cm), 24 inches (61 cm), and 36 inches (91 cm). Parsons' first
36-inch-diameter mirror is made of 16 thin plates soldered to a brass
framework. In 1842, Parsons starts works on his 72-inch (183-cm) massive
mirror. Parsons is only successful on the fifth casting. The mirror weighs 8960
pounds (4064 kg), cost £12,000, and becomes known as the "Leviathan of
Corkstown". The telescope tube is over 50 feet (15 m) long and because of winds
the tube has to be protected by two masonry piers 50 feet high and 23 feet (7
m) apart in which it is supported by an elaborate system of platforms, chains,
and pulleys. The telescope takes 4 people to run it.

In the year 1845, Parsons completes his 72 inch reflector telescope, the
largest on Earth until the 100-inch reflector is installed in 1917 at the Mt.
Wilson Observatory, California.

In April 1845, when Parsons points his new telescope to M51 for the first time,
he discovers that the nebula has a spiral structure. Parsons creates the term
"spiral nebula" and concludes (that the nebula is) an inner rotation of a large
system "pretty well studded with stars".

Parsons will discover 15 spiral galaxies.

The Leviathan is dismantled in 1908.
(Birr Castle) Parsonstown, Ireland  
155 YBN
[08/06/1845 AD]
3248)
(Oak Field, Whalley Range near) Manchester, England  
155 YBN
[09/18/1845 AD]
2713) Faraday holds the belief that all the forces of matter have one common
origin, and are convertible into each other. However, experiments done by
Faraday show no effect of electricity on light particles. A ray of light from
an Argand lamp is polarized in a horizontal plane by reflection from a surface
of glass, and passed through a Nichol's eye-piece revolving on a horizontal
axis. Between the polarizing (glass) mirror and eye-piece, two powerful
electro-magnetic poles are arranged, separated by about two inches. The
direction of the magnet is positioned so that the magnetic lines of force are
parallel to the ray of light. (I think an important note is that although we
call a beam of light a ray, the ray is composed of many billions of individual
rays of light particles, an unimaginably large quantity of very fast moving
particles.) Any transparent substance in between the two poles would have
passing through it the polarized ray of light and the magnetic lines of force
at the same time in the same direction. Faraday first finds an effect in a
glass he created 16 years before called silicated borate of lead. In addition,
the glass illustrates the effect to a larger degree than any other substance
examined. A piece of this glass 2 inches square and 1/5 inch thick is placed
between the poles (not yet magnetized by electric current), and the polarized
light appears extinguished when the eye-piece is turned to the same position as
when there is nothing between the magnetic poles. When sending the current
through its coils, creating the electromagnet, looking through the eye-piece,
immediately the lamp-flame becomes visible, and continues to be visible as long
as the electric current is on. On stopping the electric current, causing the
magnetic force to stop, the light instantly disappears. The battery Faraday
uses is five pairs of Grove's construction (explain), and the electromagnets
have a power such that the poles can each sustain a weight of 56 or more
pounds, so this phenomenon is no seen with a weak magnet. (How many wire turns,
what diameter iron bar?) Faraday finds that when the current is flowing, the
rotating the eyepiece to the right or left will cause it to disappear, and
concludes that the polarized light has been rotated. (2149) Faraday uses the
word "diamagnetic" to mean a body through which lines of magnetic force are
passing. When the marked pole is nearest the observer, the rotation of the ray
is right-handed; the eye-piece needs to be turned to the right-hand, clockwise.
When the poles are reversed, simply by changing the direction of the electric
current, the rotation is also changed and becomes left-handed in equal quantity
as before. When the magnetic lines of force are perpendicular to the glass, no
effects are observed. These results are also obtained with an ordinary steel
horse-shoe magnet with no electric current used, although these results were
feeble. Faraday uses a single magnet pole (see figure 1, a and b are the
positions of the diamagnetic (glass) where the ray of light is perpendicular to
the magnetic pole at P, c and d are at points where the ray is parallel to the
field which is circling around the pole (on the outside, not the lines entering
or emitting from the pole center), the ray is marked by a dotted line. Faraday
notes that if a glass is placed directly at the end of the magnet, no effect is
produced. (I think the curving nature of particles in the field is needed.) So
in position a and b, when light is perpendicular (and probably the magnetic
lines are parallel to rows of atoms), there is no effect, but in positions c
and d when light is parallel (and probably the magnetic lines are perpendicular
to rows of atoms), there is an effect. The rotation of the ray is in proportion
to the length of the "diamagnetic" (the glass). (2163) When Faraday adds more
pieces of glass end to end, the amount of rotation is increased. (So clearly
there is a cumulative effect, the longer the light passes through the atomic
field the more deflected it is. The phenomenon may be like a ball bouncing down
a corridor, and with each 20 reflections, the position of the ball at regular
intervals of time has rotated by a certain quantity.) (2164) The power of
rotating the ray of light increases with the intensity of the magnetic lines of
force (or the intensity of the electric field). (It may be that an atomic
lattice "corridor" is tilted more with a stronger magnetic field.) (2165) In
bodies that have a rotative power of their own such as turpentine, sugar,
tartaric acid, tartrates, etc, the effect of the magnetic force is to add to or
subtract from their specific force. (2176) Flint-glass exhibits the property
but in a less degree, and crown-glass is an even smaller degree. (What can it
mean that a highly refractive material exhibits this property most? Perhaps in
a material that already changes the direction of light significantly, small
changes to the atomic positions are magnified.) (2178) Rock-crystal shows no
effect on the ray. (So clearly the nature of the atomic structure makes a
difference, and it appears that some parts of the atomic structure can be moved
by particles in an electric field in transparent materials.) (2179) Iceland
spar shows no effect. (2184) Water, alcohol and ether all show the effect,
water most, alcohol less, and ether the least. Every liquid substance Faraday
has at hand produce this effect. (I think it shows that the atomic structure is
more easily moved in a liquid than in a solid.) (2186) In gases, Faraday does
not observe this effect in any substance. (Perhaps there constantly moving
structure of the gas atoms removes any kind of permanent order.) (2189) Faraday
finds the same effect for electric current running through a wire on the
polarization angle of the ray of light. (2224) Faraday makes clear that the
magnetic forces do not act on the ray of light directly but only through the
intervention of matter. (Which shows that Faraday does not consider light to be
made of matter.) (2242) Faraday concludes by stating that he hopes to find a
way to use light to evolve electricity and magnetism, but prefers to
investigate and develop real truth through experiment as opposed to suppose
ideas that may or may not be founded on or consistent with fact.
(Like Faraday, I
also share this belief that all forces of matter have one common origin,
however, I think all apparent forces of matter, electromagnetism, the strong
and weak nuclear forces are all cumulative and collective effects of gravity,
just as life itself, with the many complex molecules and naturally selected
forms is complex, but made of the same atomic units functioning by gravity. It
is probably hard to believe that such complexity could result from the simple
principles of an infinite sized and scaled space, matter, time under a single
force of gravity, and modeling the evolution of molecules and life using light
particles and gravity requires massive computer resources and time. We should
definitely keep an open mind when it comes to theories of the universe. In
particular I find that the probability of an infinity of space and matter both
in size and scale causes a mathematical problem with modeling the universe
exactly. In any event, to reduce unnecessary "forces" to a single force seems
logical. The most simple explanation is probably the correct one. instead of
creating dozens of new "forces" that are probably the results of the cumulative
and larger scale effects of a single force. One example I give is that a star
wobbles from the matter orbiting it. From a distance people could say that
there is some "wobbling" force "wobblery" that all stars have besides the force
of gravity that appears to hold the stars together. Perhaps a clearer example
is how a person might see, from a distance an anthill created without ever
seeing individual ants building the anthill, and then create a new force "hill
growthery" which causes hills to arise from the ground over time. So it is, I
think, with electricity {and therefore magnetism} being a collective effect of
gravity, and particle collisions.)
(Royal Institution in) London, England  
155 YBN
[09/??/1845 AD]
3266) Adams is a child prodigy.
Adams refuses knighthood and astronomer royal because of
age.
(Cambridge Observatory) Cambridge, England  
155 YBN
[12/24/1845 AD]
2714) Faraday suspends a bar of glass composed of silicated borate of lead
2x0.5x0.5 inches in size by a long thread. This bar can turn freely by the
slightest force in the horizontal plane and is enclosed in a glass jar to
prevents the movement of air from moving the bar. Two poles of a powerful
electromagnet are placed on each side of the glass bar so the center of the bar
is in the line connecting the poles, which is the line of magnetic force. If
the bar is inclined at 45 degrees to that line of force, then when the battery
is connected, the glass bar will turn to a position at right angles to the line
of force, and if moved will return to that position. A bar of bismuth exhibits
the same phenomenon. While a bar of iron takes a position in the same direction
of the magnetic forces, which is 90 degrees with the direction the bar of
bizmuth takes when subjected to the same magnetic influence. (How do the
dimensions of the bar make a difference? For example, in cube shape, no
difference can be noticed, but when in rectoid a difference is noticed? And
then is it not possible to simply cut the material so that what was once the
long dimension is then the short dimension, the long part extending 90 degrees
from the grain? I think this needs to be verified and explained. If time make a
video of this experiment. Search for videos of this experiment.) Faraday
categorizes these two different kinds of objects as those, like iron usually
called "magnetics", and the other group, like bismuth, obeying a contrary law,
and therefore being called "diamagnetics". The number of magnetics are
extremely limited, consisting only of iron, nickel, cobalt, manganese,
chromium, cerium, titanium, palladium, platinum and osmium. All other bodies,
either solid or liquid are diamagnetic, but with various degrees of intensity.
Some diamagnetics, listed in increasing degree are ether, alcohol, gold, water,
mercury, flint glass, tin, lead, zinc, antimony, phophorus, and bismuth. No
gases, rarefied or condensed are observed to be affected by magnetic forces.
Faraday views gases as occupying a neutral point in the magnetic scale between
magnetic and diamagnetic bodies. (So perhaps a sliver of bizmuth will always
point east and west? Perhaps their movement depends on the direction of current
in them. One in which current flows around the short side, and the other where
the current flows around the long side. Clearly the dimensions of the material
are partially responsible for the effect, because the "grain" of the material
could be in any of 3 dimensions depending on how the material is cut.)
Faraday states
that the material requires an elongated shape for this effect. When the
material is in the form of a cube or sphere they do not turn in any direction,
but the entire object if magnetic, is attracted towards either magnetic pole;
if diamagnetic, the object is repelled from them. (Interesting that there are
objects that are repelled from North and South magnetic poles?) Substances
divided into minute fragments, or fine powder, obey the same law as the larger
masses. This powder moves in lines which Faraday terms "diamagnetic curves", in
contradistinction to the ordinary magnetic curves, which they everywhere
intersect at right angles. (To me this is a major find, that there are
materials that cause different lines of magnetic force.) Faraday writes "These
movements may be beautifully seen by sprinkling bismuth in very fine powder on
paper, and taping on the paper while subjected to the action of a magnet.".
Faraday explains that these lines are the result of the simple law that while
every particle of a magnetic body is attracted, every particle of a diamagnetic
body is repelled, by either pole of a magnet. (Perhaps the diamagnetics align
on separate lines of current, or the current flows through them only in the
long dimension. I want to see the effect before I think more about it.) Faraday
states that these two modes of action stand in the same general antithetical
relation to one another as the positive and negative conditions of electricity,
the northern and southern polarities of ordinary magnetism, or the lines of
electric and of magnetic force in magneto-electricity. (It is important to note
that at this stage in 1845, Faraday, still holds out magnetism as a separate
force of nature, different from electricity. Faraday still describes the
"magnetic force" instead of the "electric force". Although some might interpret
this as simply calling this force the magnetic force, just because it is an
electric force in a permanent magnet as opposed to an electric force created by
a battery. Clearly the modern view is still this distinction between
electricity and magnetism.) Faraday concludes his first paper on the
diamagnetic phenomenon by theorizing that both magnetic and diamagnetic
materials become magnetized when exposed to a magnetic field (Note that on this
occasion, Faraday is using the word "field" instead of magnetic action or
force), each having its axis parallel to the lines of force passing through it,
but the particle of magnetic matter would have its north and south poles
opposite or facing the pole of the inducing magnet, where the diamagnetic
particles would align in the reverse which results in the magnetic particle
being attracted, while the diamagnetic particle being receded. (It's confusing.
Make clearer. I think I doubt the receding claim, are bars of bismuth actually
recede from magnetic poles?) Faraday then states that according to Ampere's
theory (the theory of an electric current causing a magnetic field? Faraday
should be more explicit.) this view would result in currents that are induced
in iron and magnetics parallel to those existing
(Royal Institution in) London, England  
155 YBN
[1845 AD]
2652) The Electric Telegraph Company is formed in England.

The Electric Telegraph Company must store every telegraph, and keep them on
file for wealthy connected people to search through the messages of people they
are interested in. Why do we never hear about this massive telegraph library?
In 1870
the telegraph industry in England is nationalized and becomes part of the
British Post Office.
England  
155 YBN
[1845 AD]
2723) (Sir) Roderick Impey Murchison (mRKiSuN) (CE 1792-1871), Scottish
geologist, publishes "The Geology of Russia in Europe and the Ural Mountains"
(1845).

London, England (presumably)  
155 YBN
[1845 AD]
2828) Nitrocellulose is a pulpy or cottonlike polymer derived from cellulose
treated with sulfuric and nitric acids and used in the manufacture of
explosives, collodion, plastics, and solid monopropellants.

Nitrocellulose is the main ingredient of modern gunpowder. Nitrocellulose is a
fluffy white substance that retains some of the fibrous structure of untreated
cellulose. Nitrocellulose will ignite on brief heating of more than about 150°
C (300° F). When nitrocellulose (breaks apart), it forms products that further
catalyze decomposition and this reaction, if not stopped in time, results in an
explosion (which is when many pieces of matter are quickly given high
velocities in an outward direction, in particular many photons are released in
even visible frequencies).

Nitrocellulose is nitric acid ester of cellulose (a glucose polymer).
Nitrocellulose is usually formed by the action of a mixture of nitric and
sulfuric acids on purified cotton or wood pulp. The quantity of nitration and
degradation (breaking down) of the cellulose (into glucose?) is carefully
controlled in order to obtain the desired product.

When cotton is treated so that nearly all of the hydroxyl groups of the
cellulose molecule are esterified (conversion of an acid into an ester by
combination with an alcohol and removal of a molecule of water), but with
little or no degradation of the molecular structure, the nitrocellulose formed
is called guncotton. Guncotton resembles cotton in its appearance. Extremely
flammable, guncotton explodes when detonated and is used in the manufacture of
explosives. Guncotton is insoluble in such common solvents as water,
chloroform, ether, and ethanol.

If the nitration is not carried to completion (the point at which about two
thirds of the hydroxyl groups are esterified), the soluble cellulose nitrate
pyroxylin is formed.

Less completely nitrated celluloses are called collodion cotton or pyroxylin
and are inferior to guncotton in explosive properties. Collodion with a
nitrogen content of not more than 12 percent is used chiefly for lacquers and
celluloid plastics. Materials with a nitrogen content of about 11.5 percent are
used as artificial silk but have been replaced by other materials such as
viscose rayon. A nitrogen content of 11.5 percent is also used for
manufacturing photographic film until safety film made of cellulose acetate
plastics becomes more popular.
(University of Basel) Basel, Switzerland  
155 YBN
[1845 AD]
2838) Parsons is a wealthy aristocrat. (One of the few who spends on science,
and in particular useful science.)
Parsons is educated at Trinity College, Dublin, and
Oxford University, where he graduates in 1822.
In 1821 Rosse is elected to the House
of Commons as Lord Oxmantown.
Parsons sits in Parliament for 12 years, resigning his seat
in 1834.
In 1841 Parsons inherits his father's earldom and serves as one of the Irish
peers in the House of Lords.
(You can see how even after monarchy, the wealthy somehow
control the "representative" governments.)

In 1845 Parsons is the Irish representative in the House of Lords (in
England?).
In Ireland in the years after 1845 the "potato famine" costs the lives of more
than 1 million people.
During the potato famine, Rosse (pays) back a major portion of
his rents to the farmers.
From 1849 to 1854 Parsons is the president of the
Royal Society.
From 1862 (on) Parsons is the chancellor of the University of Dublin.
(Birr Castle) Parsonstown, Ireland  
155 YBN
[1845 AD]
2922) In Hertfordshire England experiments by Liebig's English pupil J.H.
Gilbert, together with the landowner John Bennet Lawes, lead to the discovery
of superphosphates, which are developed as fertilizers.

In addition extracting the necessary molecules from manure may remove the
unpleasant smell of feces when fertilizing public plants.
(University of Giessen), Giessen, Germany  
155 YBN
[1845 AD]
2933) Siebold founds the "Zeitschrift für wissenschaftliche Zoologie"
("Journal of Scientific Zoology"), which becomes one of the foremost
periodicals for biological research.
(University in) Freiburg, Germany  
155 YBN
[1845 AD]
3151) Julius Robert Mayer (MIR) (CE 1814-1878), German physicist, publishes
"Die organische Bewegung in ihrem Zusammenhang mit dem Stoffwechsel" (1845,
"Organic movement in their connection with the metabolism") in which Mayer
extends the conservation of force to magnetic, electrical and chemical forces.
Mayer describes how plants convert the sun's heat and light into latent
chemical force; animals consume this chemical force as food; the animals then
convert that force to body heat and mechanical muscle force in their life
processes.

Heilbronn, Germany  
155 YBN
[1845 AD]
3202)
(University of Bonn) Bonn, Germany  
155 YBN
[1845 AD]
3227) Kolbe studies chemistry with Friedrich Wöhler at the University of
Göttingen and earns his doctorate in 1843 with Robert Bunsen at the University
of Marburg.

Just before 1860, the German chemist August Kekulé and others develop the the
theory of chemical structure that depends on valence bonds. However, Kolbe
categorically rejects the molecular structural diagrams drawn by Kekulé, and
holds that the classical theory of radicals, in which groups of atoms are held
together by electrostatic forces is sufficient to describe even the most
complex organic molecules, and that therefore the new structural formulas are
overly speculative. However, most other chemists Kolbe's age or younger accept
the structure theory, and this theory is well established around 1870.

In 1874 when Kekulé's former student Jacobus Henricus van't Hoff extends
structural formulas into three dimensions to create the new field of
stereochemistry, Kolbe explodes with anger. Being chief editor of a leading
journal, the "Journal für praktische Chemie", Kolbe often publishes scathing
editorials, and in 1877 Kolbe viciously opposes the young and still unknown
Van't Hoff and the tetrahedral carbon atom proposed by Van't Hoff and Le Bel.
(University of Marburg) Marburg, Germany  
155 YBN
[1845 AD]
3234) Adolph Wilhelm Hermann Kolbe (KOLBu) (CE 1818-1884), German chemist
publishes a "Textbook of Organic Chemistry" (1854–60), which collects
together all the methods of preparing organic compounds.

(University of Marburg) Marburg, Germany  
155 YBN
[1845 AD]
3295)
Paris, France  
155 YBN
[1845 AD]
3362) Virchow bases his view on a mechanistic understanding of vital phenomena
seeing life as the sum of physical and chemical actions and as essentially the
expression of cell activity.

In 1847 Virchow and friend Benno Reinhardt, start a new journal, "Archiv für
pathologische Anatomie und Physiologie, und für klinische Medizin" ("Archives
for Pathological Anatomy and Physiology, and for Clinical Medicine").

In 1848 Virchow denounces social conditions in Silesia, radicalized by his
experiences with the destitute Polish minority of Upper Silesia during the
typhus epidemic of 1848, and fights on the side of the revolutionaries against
the Prussian government, and loses his university position. But Virchow is
hired as professor in the more liberal atmosphere of Bavaria in 1849.

In 1860 Virchow states that "all cells arise from cells" in Latin.

Bismarck challenges Virchow to a duel in 1865. Virchow refuses.

Virchow is elected to the Reichstag in 1880, as a leader of a small German
liberal party which vigorously opposes Bismarck.

Virchow rejects Pasteur's germ theory of disease, and views disease as a civil
war between cells, an anarchy among order, not an invasion from the outside. We
now know that there are diseases of both kinds. (In addition to external
causes, there are congenital (genetic) inherited diseases.) Virchow also thinks
that sociological factors play a significant role in disease.

Virchow rejects Darwin's theory of evolution, and votes for a measure banning
the teaching of Darwin's theory from schools.

Virchow accompanies Schliemann to Troy in 1879 and to Egypt in 1888.

In 1873 Virchow is elected to the Prussian Academy of Sciences.
Virchow declines to be
ennobled as "von Virchow", but in 1894 is created Geheimrat ("privy
councillor").
From his anthropological studies, Virchow is convinced that there are no such
things as "superior races".

In 1892 Virchow receives the Copley medal of the Royal Society.
(Charité Hospital) Berlin, Germany  
155 YBN
[1845 AD]
3363)
(Charité Hospital) Berlin, Germany  
155 YBN
[1845 AD]
3401)
London, England (presumably)  
155 YBN
[1845 AD]
3451) In 1847 Kirchhoff becomes privatdozent (unsalaried lecturer) at the
University of Berlin.
In 1850 Kirchhoff accepts the post of extraordinary professor of
physics at the University of Breslau.
In 1854 he was appointed professor of physics at
the University of Heidelberg, where he joined forces with Bunsen and
(establishes) spectrum analysis.
(University of Königsberg) Königsberg, Prussia (now Germany)
(presumably)  
155 YBN
[1845 AD]
3519)
(School of Pharmacy) Paris, France  
155 YBN
[1845 AD]
3660)
(Gymnasium in) Stettin, (Prussia now) Poland  
154 YBN
[05/??/1846 AD]
3298) For me light interference is a very interesting phenomena. EXPERIMENT: I
think we need to carefully measure the light that goes in and comes out of
interference. Do it all add up? Is mass (energy) conserved? Where does the
light in the dark areas go? in the light areas is the light brighter than the
source when added up? If any light is missing, test for larger particles, such
as electrons, neutrinos, neutrons, protons, other possible composite particles
to verify that no two or more photons are falling together because of their
gravity.
Paris, France  
154 YBN
[08/??/1846 AD]
2930) James Challis (CE 1803-1882), English astronomer observes the planet
Neptune but fails to compare that night's observations with those of the
previous night.

(Cambridge University) Cambridge, England  
154 YBN
[09/03/1846 AD]
3101)
London, England  
154 YBN
[09/23/1846 AD]
3073) In 1821 Alexis Bouvard, of the Paris Observatory, had published a set of
tables of the motion of Uranus. (Tables are different from observations, in
that tables are mathematical predictions of the location of an object over a
period of time.) Within a few years there is a noticeable difference between
the predicted and observed location of Uranus.

Urbain Jean Joseph Leverrier (luVerYA) (CE 1811-1877), French astronomer,
calculates the position of Neptune mathematically from the perturbations of
Uranus. On 09/23/1846, Galle is the first to see planet Neptune, in the first
night of searching at the request of Leverrier names the planet "Neptune", god
of the ocean (supposedly from the planet Neptune's green color). The finding of
a planet from pure calculation is strong evidence in favor of Newton's theory.

John Couch Adams had made the same calculation months earlier with the same
result. Leverrier works out the gravitational accounting of the motions of the
planets in greater detail than ever before. (But it is now accepted that these
motions are partially unpredictable, like the weather on earth, because of the
many atoms of water and their complex movement on earth and even the moving of
many atoms inside planets.) Both Leverrier and Adams has thought that Neptune
would be more distant based on Bode's law.

In the field of celestial mechanics, Le Verrier revises much of the work of
Pierre Simon Laplace.

(At the time) the theory of celestial mechanics centers on the theory that each
planet moves around the sun in an ellipse with minor deviations due to
attractions by the rest of the planets. This is different from running a
simulation forward into time by using a computer to iterate the positions of
all known masses and their mutual forces on each other (that is to calculate
each position for each unit of time given starting positions and velocities
into the future). Leverrier and Laplace before Leverrier use equations which
are supposed to repeat periodically in time, for example, the equation for an
ellipse; these equations are independent of time, since they form a periodic
pattern. This method must make special exceptions to account for the
interaction of other masses in the system. The computations involved are very
complicated, but the results are accurate enough to provide predictions of
considerable accuracy. However, the planet Uranus is the one exception. The
error is in prediction of location of Uranus is 1 minute of arc.

Another contribution of Galle's is that Galle suggests that the parallax of
asteroids be used to determine the scale of the solar system. This will finally
be done and successful, but not until 20 years after Galle dies. (chronology,
may be 4.8)
Berlin, Germany (and Paris, France)  
154 YBN
[09/30/1846 AD]
2998) William Thomas Green Morton (CE 1819-1868), United States dental surgeon,
popularizes the use of ether by giving a successful public demonstration of
ether as an anesthesia during surgery, using ether for a tooth removal
(extraction).

The rural Georgia physician Crawford Long was the first to use ether for
surgery 4 years before, but did not make his findings public until 1849.
In 1844,
the earliest known tooth extraction under anesthesia using nitrous oxide was
performed by US dentist Horace Wells, which Morton witnessed.

Determined to find a more reliable pain-killing chemical than nitrous oxide,
Morton consults his former teacher Boston chemist Charles Jackson (CE
1805-1880). The two discuss the use of ether.

On October 16 Morton successfully demonstrates the use of ether as an
anesthetic, administering ether to a person undergoing a tumor operation.

Morton attempts to obtain exclusive rights to the use of ether anesthesia and
spends the remainder of his life engaged in a costly disagreement with Jackson,
who claims priority in the discovery, despite official recognition going to
Horace Wells and the rural Georgia physician Crawford Long.
(Massachusetts General Hospital) Boston, Massachusetts, USA  
154 YBN
[09/??/1846 AD]
3268) Howe's early years are spent on his father's farm. In 1835 Howe enters
the factory of a manufacturer of cotton-machinery at Lowell, Massachusetts,
where he learns the machinist's trade. Howe is apprenticed in 1838 to an
instrument maker and watchmaker in Boston at whose suggestion Howe turns his
attention to devising a sewing machine. For five years Howe spends all his
spare time in its development.

Howe sends his brother to England to seek a market and there sells his third
machine to William Thomas a manufacturer of corsets, umbrellas, and shoes. This
manufacturer sees the possibilities the sewing machine could have if it can sew
leather for shoes. Howe works with Thomas in London to produce a machine to
stitch leather. The two soon quarrel, however, and Howe is forced to pawn his
model and the patent papers to raise enough money to return back to the USA.
When he
cannot make money from his sewing machine patent, Howe sells the patent rights
in England for £250 ($1,250), and moves to England. Howe works for £5 a week
to perfect his machine for use in sewing leather and similar materials.

When
Howe returns to the U.S., he finds that some manufacturers, including Isaac
Singer, are making and selling sewing machines similar to his. After a five
year legal battle, lasting from 1849 to 1854, Howe's patent rights are
established in 1854, and from then until 1867, when his patent expires, Howe
receives royalties on all sewing machines produced in the United States.
At the height
of his prosperity Howe receives as much as $4,000 a week in royalties.

(Can you imagine had Michael Pupin fought for his patent right to the camera
that sees eyes and brain images? He probably feared being murdered if he pushed
the point in the press or courts.)
Cambridge, Massachussetts, USA  
154 YBN
[10/10/1846 AD]
2824) Triton is the largest of Neptune's moons and has a diameter around 1,680
mi (2,700 km), nearly 80% that of Earth's Moon. Triton is the only large moon
of the solar system to move in a retrograde orbit, opposite the direction of
Neptune's rotation. Triton's orbital period of 5.9 Earth days is the same as
its rotation period and as a result Triton always keeps the same face toward
Neptune. Triton has a very thin atmosphere of nitrogen and methane and a
surface temperature of -390 °F (-235 °C). The surface of Triton is covered
with enormous (sheets) of ice sculpted with fissures, puckers, and
ridge-crossed depressions. Geyser-like plumes will be observed by the Voyager 2
spacecraft and these may be gas venting through fissures when the surface is
warmed by sunlight. Triton appears to have formed elsewhere in the star system
and to have been gravitationally captured by Neptune in the planet's early
history.
In 1839, Lassell describes his home-made 9-inch equatorial reflector to the
Royal Astronomical Society.
Lassell never publishes any drawings of the 24-inch
telescope.
Around 1825 Lassell starts a brewery business, after a seven-year
apprenticeship.
(Starfield Observatory) Liverpool, England  
154 YBN
[10/??/1846 AD]
3022) In 1865 De Morgan helps to found the London Mathematical Society.
De Morgan is
prevented from taking his M.A. degree, or from obtaining a fellowship, by his
conscientious objection to signing the theological tests then required from
masters of arts and fellows at Cambridge.
De Morgan publishes numerous math papers and
textbooks.
(University College) London, England  
154 YBN
[12/12/1846 AD]
3601)
Edinburgh, Scotland  
154 YBN
[1846 AD]
2603)
Abbeville, France (presumably)  
154 YBN
[1846 AD]
2675) After a year of operation the telegraph system is moved from government
owned and opened to ownership by private industry.

(Some people argue that handing over the telegraph to private industry the
telegraph grew faster, and perhaps that is true, however companies are not
democratic (not that government is either), and if a conservative company owns
the telegraph, telephone, and eventually the Pupin technology, liberal
intellectual atheists and non-church going tend to be excluded from use of the
service and the victim of abuse at the hands of conservative religious who own
and have access to the technology. If owned by government, there might be on
occasion the possibility of liberal leadership, as opposed to a company like
AT&T where the owners rarely change, and are generally passed down like
monarchy through inheritance. Either way, ultimately, the majority can control
the vast wire network through government laws, once the public realizes what is
happening with the secrecy and two-tier society that has been created.)

The telegraph companies must store every telegraph recognizing the value of
charging people to see the messages sent by people they are interested in.
However, this routine process must be kept from the public, for fear of the
public becoming angry. What are some of the oldest telegraphs secretly and
systematically stored?

Washington DC, USA  
154 YBN
[1846 AD]
2716) Charles Wheatstone is supposed to give a lecture for the Royal Society,
but at the last second, with the audience already in their seats, Wheatstone
becomes scared and leaves the theater, so Faraday gives this improvised lecture
in which Faraday speculates that light may be a disturbance of electricity and
magnetism.
(Royal Institution in) London, England  
154 YBN
[1846 AD]
2944) The name "Weber" was used for the unit of current for some time, until an
international congress in Paris in 1881 in which Helmholtz, the leader of the
German delegation proposed the name "Ampere" for the unit of current instead of
"Weber" which was accepted.
The magnetic unit, termed a Weber, formerly the Coulomb, is
named after Weber.
A "Weber" is the International System unit of magnetic flux.
One "Weber" is equal to the flux that produces in a circuit of one turn (of
wire) an electromotive force of one volt, when the flux is uniformly reduced to
zero within one second.
A Weber is equivalent to 108 "Maxwell"s, the unit used
in the centimeter-gram-second system.
(University of) Leipzig, Germany  
154 YBN
[1846 AD]
2950)
(University of Tübingen) Tübingen, Germany  
154 YBN
[1846 AD]
2951)
(University of Tübingen) Tübingen, Germany  
154 YBN
[1846 AD]
3084)
(University of Marburg), Marburg, Germany  
154 YBN
[1846 AD]
3108) Probably military people take an interest in developing this explosive,
and the traditions of secrecy in military would make this research unavailable
to the public. (Used for projectiles? propulsion of projectiles or vehicles?)
Torino, Italy (presumably)  
154 YBN
[1846 AD]
3129) This process is used extensively by Goodyear in the United States and
Hancock in England. Elkington and Mason use the process for waterproofing
before selling the patent rights to Macintosh and Company, who became famous
for their waterproofing products.
Birmingham, England (presumably)   
154 YBN
[1846 AD]
3132) Ménard is educated at the Collège Louis-le-Grand and the École Normale
and is a gifted chemist, painter and historian. Ménard is a socialist
republican and is condemned to prison in 1849 for his "Prologue d'une
révolution", which contains radical political opinions and his reminiscences
of the June 1848 insurrections in Paris, in which Ménard played an active
part. Ménard escapes abroad, returning to Paris in 1852.
In 1876 Ménard publishes
"Rêveries d'un païen mystique" ("Reveries of a Mystic Pagan"), which explains
his philosophy.
Paris, France  
154 YBN
[1846 AD]
3240)
Salford, England (presumably)  
154 YBN
[1846 AD]
3327)
London, England (presumably)  
154 YBN
[1846 AD]
3476) At the University of Glasgow where Thomson is the chair of natural
philosophy (later called physics), Thomson creates the first physics laboratory
for students in the British Isles.
(University of Glasgow) Glasgow, Scotland  
153 YBN
[05/05/1847 AD]
3255)
Broom Hill (near Manchester), England  
153 YBN
[07/23/1847 AD]
3331) (Possibly include text of introduction here)

Helmholtz's father is a teacher of philosophy and literature at the Potsdam
Gymnasium, and Helmholtz's mother is descended from William Penn, the founder
of Pennsylvania. (It is interesting that there are lines of descent where
clearly some families have progressed into science farther than others, and
their descendants generally receive science educations as opposed to the
explanations offered by religions, and this effect is amplified over many
generations.)

In 1838, Helmholtz enters the Friedrich Wilhelm Medical Institute in Berlin,
where he receives a free (physician's) education on the condition that he serve
eight years as an army doctor. At the Institute Helmholtz does research under
the greatest German physiologist of the day, Johannes Müller.

Helmholtz learns to play piano while at the Medical Institute.

Helmholtz opposes the "nature philosophy" of Kant and others which views
concepts of time, space, and causation were not products of sense experience
but mental attributes, instead insisting that all knowledge comes through the
senses, and that all science and the universe can and should be reduced to the
laws of classical mechanics, which, for Helmholtz, includes matter, force, and,
later, energy. Müller, whose lab Helmholtz earned his doctorate in, is a
vitalist and is convinced that living processes will never be reduced to the
ordinary mechanical laws of physics and chemistry.

Ernst Brücke, Helmholtz and Karl Ludwig make up the "1847 school" of
physiology whose program reacts sharply against German physiology of previous
decades, in rejecting any explanation of life processes that appeals to
nonphysical vital properties or forces. The Concise Dictionary of Scientific
Biography states that "All of Helmholtz's minor papers published between 1843
and 1847, most of which treat problems of animal heat and muscle contraction,
clearly reflect the mechanistic tenets of the school.".

Heinrich Hertz, who discovers radio waves in 1888, is Helmholtz's pupil.

(Helmholtz is the teacher/mentor of Michael Pupin for a few years, and
Helmholtz's interest and immersion in studies of the sense organs no doubt
inspired Pupin to explore the questions of "can the heat from a human's body
and in particular the brain be seen apart from the background heat?", “can
what a person sees be seen from behind the head?”, "can image a brain creates
be seen outside of the head in different frequencies of light?", “can thought
be somehow heard outside of the head?”, questions perhaps Helmholtz and
others openly asked among themselves. When did hidden microphones start to be
used? After 1890, people probably were using hidden movie cameras. )

In 1873 Helmholtz is award the Copley Medal.

Helmholtz experiences fainting spells throughout his life, on returning from a
lecture tour of the USA, he suffers a concussion from a faint, doesn't recover
and dies 8 weeks later.

Many of Helmholtz's works appear in Hermann von Helmholtz, "Wissenschaftliche
Abhandlungen", "Scientific Papers" (2 vol, 1882,1883).
(Physikalische Gesellschaft) Berlin, Germany  
153 YBN
[10/01/1847 AD]
3215) Mitchell is the first professional woman astronomer in the USA.

As a child Mitchell's interest in astronomy is stimulated by her father, who
encourages her independent use of his telescope.
From 1836 to 1856 Mitchell works as a
librarian during the day and is a regular observer of the skies at night.
In October
1847 Mitchell succeeds in establishing (plotting?) the orbit of a new comet.
(how is this communicated to the public?)
This discovery causes Mitchell's immediate
recognition among people in science.
Mitchell is awarded a gold medal from the King of
Denmark.
The following year Mitchell becomes the first woman elected to the American
Academy of Arts and Sciences.
In 1849 Mitchell is hired as a "computer" by the US
Nautical Almanac Office.
The next year Mitchell is elected to the American Association
for the Advancement of Science.
In 1857 a group of Boston area women (led by Elizabeth
Peabody) present Mitchell with a 5-in. Alvan Clark refractor, with which she
expands her studies of sunspots, planets, and nebulae.
In 1865, Mitchell, reluctantly,
but encouraged by her father, accepts a job at Vassar Female College, which
opens this year in Poughkeepsie, New York.
(Is Mitchell the first female professor
(of astronomy) in the US?)

In 1873 Mitchell helps found the Association for the Advancement of Women and
serves as its president (1875–76).

Asimov comments that Mitchell's contributions to science are moderate, but that
she represents the (highest point) for the oppressed half of the American
population.
Nantucket, Massachusetts, USA  
153 YBN
[1847 AD]
2731)
London, England (presumably)  
153 YBN
[1847 AD]
2754)
Cambridge, England (presumably)  
153 YBN
[1847 AD]
3064) In 1843 Regnault is commissioned by the Government to investigate the
properties of steam and to obtain numerical data that should be of value to
steam engineers. The results are published in 1847, as vol. XXI of the
"Mémoires" of the Academy of Sciences. For this work Regnault wins the Rumford
Medal of the Royal Society of London. (alpha of 1/273 is in this work?)

Also in this year, Regnault publishes a four-volume treatise on Chemistry which
has been translated into many languages. (title = )
(College de France) Paris, France  
153 YBN
[1847 AD]
3094)
(New York University) New York City, New York, USA  
153 YBN
[1847 AD]
3098) Simpson is a child prodigy, and enters the University of Edinburgh at 14,
receiving a medical degree at age 21.
Simpson develops the long obstetrics
forceps that are named for him. Simpson is also known for his writings on
medical history (especially on leprosy in Scotland) and on fetal pathology and
hermaphroditism.
(University of Edinburgh) Edinburgh, Scotland  
153 YBN
[1847 AD]
3110) Until Snow is 14, he is educated at a common day school for poor
families. In 1827, Snow travels to Newcastle - upon - Tyne, 80 miles from his
home, where Snow begins serving a six year apprenticeship in medicine (or
perhaps in the study of illness) under surgeon William Hardcastle. The
apprenticeship includes attending lectures at the Newcastle Infirmary. During
this apprenticeship, Snow became a vegetarian as well as a total abstainer of
alcohol (perhaps a non-drinker of alcohol, nonalcoholian).
London, England  
153 YBN
[1847 AD]
3172) Boole comes from a poor background in the English city of Lincoln.
Boole's father
teaches him math and to make optical instruments. Aside from his father's help
and a few years at local schools, however, Boole is self-taught in
mathematics.
From the age of 16 Boole teaches in village schools in the West Riding of
Yorkshire.
In 1835 Boole opens his own school in Lincoln when he is 20.
In 1844 Boole is
awarded the Royal Society's first gold medal for mathematics for Boole's
pioneering paper on the calculus of operators.

Much of language is defined by our interpretation of the universe. We define
subset objects from a singular universe. For example we create the object
"Star" which is different from the rest of the universe. From the definition of
space and time come the questions what, where, when, if, etc which form the
basis of language. So humans create and move around these objects in our
brains. The objects (nouns) we select in the universe, and their movement
(verbs) define much of human language.
Lincoln, England (presumably)  
153 YBN
[1847 AD]
3180) Ludwig attempts to determine, with greater precision than Harvey had
done, the relation of the movements of the heart and chest to the fluctuations
of pressure of the blood in the veins and arteries. In 1846, Ludwig, while
still at Marburg, studies the relation which exists between the movements of
respiration and the pressure of the blood. Ludwig connects a U shaped manometer
tube partly filled with mercury with an artery (describe how - wrapping around
or injecting in?) but the movements of the column of mercury are so rapid and
complex that the eye fails to retain them. It is then that Ludwig conceives the
idea of placing on the mercury a float carrying a style tipped with a writing
point and of letting this record the movements of the mercury and consequently
of the blood column on a moving surface. The movement of the paper on which the
tracing is written is effected by means of a clockwork. The respiratory
movements are recorded on the same paper at the same time with the oscillations
of the arterial pressure. Therefore the records of these two processes are
written simultaneously and can be readily compared.
(University of Marburg) Marburg, Germany  
153 YBN
[1847 AD]
3213) Semmelweiss is educated at the universities of Pest and Vienna, receives
his doctor's degree from Vienna in 1844 and is appointed assistant at the
obstetric clinic in Vienna.

In July 1865 Semmelweiss is locked into a psychiatric hospital and dies there.
(I always wonder what the person did to be handcuffed by police and taken to a
psychiatric hospital...maybe he grabbed a juicy ass, who knows?!)
(Vienna General Hospital) Vienna, (Austria now:) Germany  
153 YBN
[1847 AD]
3225) Many people mistake a gun "bullet" with a gun "cartridge". The bullet is
the projectile inside the cartridge.
Paris, France  
153 YBN
[1847 AD]
3303)
Paris, France  
153 YBN
[1847 AD]
3473) This paper wins Hofmeister, self-educated, an honorary degree from the
University of Rostock.
In 1863 Hofmeister is given the chair of botany at Heidelberg.
and in 1872 is hired as chair at the University of Tübingen, both unheard of
accomplishments for a self-taught scholar.
Leipzig, Germany (presumably)  
153 YBN
[1847 AD]
3605)
Edinburgh, Scotland  
153 YBN
[1847 AD]
3606)
London, England  
153 YBN
[1847 AD]
5992)
Paris, France (presumably)  
153 YBN
[1847 AD]
6002) Clara Josephine Schumann (CE 1819-1896), German pianist and composer,
composes Piano Trio opus 17.

Shumann wins success as a touring piano virtuoso both before and after she
marries the composer Robert Schumann (1840).

Despite strong objections from her father, she married Schumann in 1840, and
they have eight children between 1841 and 1854.

Leipzig, Germany (verify)  
152 YBN
[03/11/1848 AD]
2843)
(Birr Castle) Parsonstown, Ireland  
152 YBN
[05/22/1848 AD]
3411) Pasteur is the descendant of generations of tanners. His
great-grandfather was an indentured laborer who bought his own freedom.
Pasteur tutors,
but experiences periods of semistarvation from poverty.
In 1848 Pasteur takes side of
the revolutionaries but is politically conservative.
Pasteur shows these (stereo optical
molecular isomers) to Biot.
The finding of stereo optical isomers makes Pasteur
famous at age 26.
Pasteur receives the Rumsford medal for this work.
Pasteur is a very
religious person.
Pasteur rejects the theory of evolution on religious
reasons.

In 1868 Pasteur has a stroke that partially paralyzes him.

In 1888 the Pasteur Institute is established with the help of donations from
all over the earth, including from the governments of Russia, Turkey and
Brazil. It's purpose is originally to treat rabies, and it is now one of the
most recognized and productive centers of biological research on earth. In the
closing paragraphs of his inaugural oration, Pasteur said: "Two opposing laws
seem to me now to be in contest. The one, a law of blood and death opening out
each day new modes of destruction, forces nations always to be ready for the
battle. The other, a law of peace, work and health, whose only aim is to
deliver man from the calamities which beset him. The one seeks violent
conquests, the other, the relief of mankind. The one places a single life above
all victories, the other sacrifices hundreds of thousands of lives to the
ambition of a single individual. The law of which we are the instruments
strives even through the carnage to cure the wounds due to the law of war.
Treatment by our antiseptic methods may preserve the lives of thousands of
soldiers. Which of these two laws will prevail, God only knows. But of this we
may be sure, science, in obeying the law of humanity, will always labor to
enlarge the frontiers of life.".

Asimov comments that nobody except Aristotle and Darwin can compete with
Pasteur for the greatest scientist in the field of biology.
Paris, France  
152 YBN
[08/10/1848 AD]
2879)
London, England (presumably)  
152 YBN
[08/??/1848 AD]
3241)
(read at) Swansea, Wales, England  
152 YBN
[09/16/1848 AD]
2612) Bond builds a home observatory that is the best in the nation.

Hyperion is 370x280x225km (230x174x140 miles), and is largest highly irregular
(nonspherical) body in the solar system. Hyperion's mean density is only about
half that of water ice, suggesting that the moon's interior may be a loose
agglomeration of (water?) ice blocks interspersed with empty space. (I have
doubts, because the meteor impacts imply a solid one-piece object, in
particular the largest impact.)
Hyperion orbits Saturn once every 21.3 Earth days in the
prograde direction at a distance of 1,481,100 km (920,300 miles), between the
orbits of the moons Titan and Iapetus. Hyperion's orbit is unusual in that it
is somewhat eccentric (elongated) yet inclined less than a half degree from the
plane of Saturn's equator.
Hyperion forms a satellite pair with Titan; that is,
the two moons interact gravitationally.

Because of Hyperion's shape and orbit, it does not maintain a stable rotation
around its own fixed axis. Unlike any other known object in the solar system,
Hyperion rotates (unpredictably), changing its rotational characteristics over
timescales as short as a month.

Hyperion is named for one of the Titans of Greek mythology.
Bond is largely
self-educated, and is a watchmaker who becomes interested in astronomy after
observing the solar eclipse of 1806.
In 1815 Bond is sent by Harvard College to
Europe to visit existing observatories and gather data preliminary to the
building of an observatory at Harvard.
In 1839, Bond is appointed the first astronomical
observer at Harvard College in recognition of his efforts.
In 1839 the (Harvard)
observatory is founded. Bond supervises its construction and becomes its first
director.
In 1847 a 15-in. (37.5 cm) telescope, then matched in size by only
one other on Earth, is installed. With this telescope Bond makes elaborate
studies of sunspots, of the Orion nebula, and of the planet Saturn, publishing
his results chiefly in the Annals of the Harvard College Observatory.
In 1851 a photograph
(daguerreotype )of the moon Bond takes is a sensation at the Great Exhibition
in London.
Harvard, Massachussetts, USA ((Starfield Observatory) Liverpool, England)  
152 YBN
[1848 AD]
2561) Slavery is abolished in the French colonies.
French physicist, Dominique François
Jean Arago (oroGO) (CE 1786-1853) as minister of war and navy, appoints the
greatest advocate of ending slavery Victor Schoelcher as undersecretary for the
navy, who the prepares the famous decree that abolishes slavery in the
colonies.
Paris, France (presumably)  
152 YBN
[1848 AD]
2648) The Associated Press is a cooperative news agency (wire service), the
oldest and largest of those in the United States and long the largest and one
of the preeminent news agencies on Earth. The AP is formed in 1848, when six
New York City daily newspapers pooled their efforts to finance a telegraphic
relay of foreign news brought by ships to Boston, the first U.S. port of call
for westbound transatlantic ships.
New York City, NY, USA  
152 YBN
[1848 AD]
2679)
France  
152 YBN
[1848 AD]
2759) Charles Babbage (CE 1792-1871), English mathematician, makes a complete
set of drawings for "Difference Engine 2".

Cambridge, England (presumably)  
152 YBN
[1848 AD]
2811) In this same paper, Henry describes how at a high enough temperature
silver does not evaporate as thought, but sinks into copper metal below it.
Princeton, NJ, USA  
152 YBN
[1848 AD]
2842)
(Birr Castle) Parsonstown, Ireland  
152 YBN
[1848 AD]
3018) Maury describes the gulf stream by saying "there is a river in the
ocean".
Maury is one of the founders of the American Association for the
Advancement of Science.
According to the Concise Dictionary of Scientific Biography, as
head of the U.S. naval Observatory from 1844 to 1861, Maury's poor
qualifications as an astronomer hold back the Earth's greatest observatories.
Being a
Virginian Maury sides with the Confederacy in the outbreak of the US Civil War
in 1861.
In England, Maury takes an active part in organizing an unsuccessful
petition for peace in the United States.
Washington, DC, USA  
152 YBN
[1848 AD]
3068)
(Harvard University) Cambridge, Massachussetts, USA  
152 YBN
[1848 AD]
3191)
(University of Würzburg) Würzburg, Germany  
152 YBN
[1848 AD]
3289) Fizeau substitutes bromine for the iodine used by Daguerre in making
daguerreotypes and this increases the permanency of daguerreotypes. (verify)
With Jean
Foucault, Fizeau performs a series of investigations on the interference of
light and heat.
Most of Fizeau's published works appear in the "Comptes Rendus" and
in the "Annales de physique et de chimie".
Fizeau is the son of a wealthy physician and
professor at the Faculty of Medicine in Paris. Fizeau receives his secondary
education at the Collège Stanislas and starts to study a career as a
physician, but because of poor health has to stop regular attendance of
classes. Upon return to health Fizeau turns his focus to physics.
Fizeau never holds
professorships but is elected to the Academy of Sciences in 1860.
In 1875 Fizeau is
awarded the Royal Society's Rumford medal.
Paris, France (presumably)  
152 YBN
[1848 AD]
3302)
Paris, France  
152 YBN
[1848 AD]
3333)
(Physikalische Gesellschaft) Berlin, Germany  
152 YBN
[1848 AD]
3405)
(University of Göttingen) Göttingen, Germany (presumably)  
152 YBN
[1848 AD]
3477)
(University of Glasgow) Glasgow, Scotland  
152 YBN
[1848 AD]
3478)
(University of Glasgow) Glasgow, Scotland  
152 YBN
[1848 AD]
3497) In later life Bates is considered possibly the greatest authority on
Coleoptera (beetles and weevils).
Brazil, South America  
152 YBN
[1848 AD]
3658)
(University of) Leipzig, Germany  
152 YBN
[1848 AD]
5988) Johann Strauss I (Known as "the Elder.") (CE 1804-1849), Austrian
violinist and composer of waltzes and other works, composes the "Redetzky
March" (1848). His son Johann (1825-1899), known as "the Younger," is sometimes
called "the Waltz King" and is best remembered for his numerous waltzes, such
as "The Blue Danube" (1867).

(It is interesting how different from Mozart and Beethoven's music the march
is. There is, perhaps more focus on percussion and a regular drum beat.
Apparently the march goes back a long way in history.)

(Determine when the march originates and by whom.)

Vienna, Austria (presumably)  
151 YBN
[01/20/1849 AD]
3280) EXPER: For all known substances, use a diffraction grating and computer
interface to analyze for all photon intervals (wavelengths) of light, those
absorbed, reflected, and transmitted. Try various angles of incidence to see if
there is a difference. Make public all findings.

I think there is the remote possibility that light particles of the same
frequency could be colliding off each other and this might explain the dark
areas. Kirchhoff had found that the absorption happens even for unilluminated
sodium - see id3458. EXPERIMENT: In 2D and 3D models do particle beams of the
same or different frequencies from two spherical sources collide more often?
How are distance, intensity, frequency, etc related to number and rate of
collisions?
Paris, France (presumably)  
151 YBN
[01/23/1849 AD]
1252) Blackwell applies to several prominent medical schools but is rejected by
all. Her second round of applications is sent to smaller colleges, including
Geneva College in New York, where she is accepted. According to legend, because
the faculty put the application to a student vote, and the students think her
application is a hoax. Blackwell braves the prejudice of some of the professors
and students to complete her training. She persists, ranking first in her
class.
Geneva, New York, USA  
151 YBN
[03/29/1849 AD]
3507)
(Royal College of Surgeons) London, England  
151 YBN
[05/27/1849 AD]
3299)
Paris, France  
151 YBN
[06/21/1849 AD]
3247) Joule publishes these results as "On the Mechanical Equivalent of Heat"
in the Philosophical Transactions.

Joule opens with two quotes, the first from John Locke, and the second from
Gottfried Leibnitz:
From Locke: "Heat is a very brisk agitation of the
insensible parts of the object, which produces in us that sensation from whence
we denominate the object hot; so what in our sensation is heat, in the object
is nothing but motion." and from Leibnitz: "The force of a moving body is
proportional to the square of its velocity, or to the height to which it would
rise against gravity.". This last quote is interesting to me, because, perhaps
this work is on the path that leads to the use of "energy" as a quantity which
is conserved and equal to 1/2mv2. Joule refers to the "vis-viva" of the heated
water (particles) and defines this property (vis-viva) as being proportional to
the particle velocity squared. I think according to the F=ma law, force of an
object is proportional to the object's mass and acceleration. This idea of
gravity presumes the large mass of the Earth, strictly speaking, a mass that is
pulled away, against the force exerted by a larger mass. But I think this may
be a case of how a person may say, force is proportional to mass, and to mass
squared, and to the square root of mass, and to mass cubed, etc. all true, but
seems apparently unimportant. Although I am not sure and this is certainly open
to other explanations. But beyond that, I don't think force is proportional to
velocity or velocity squared (or cubed, etc), as it is, strictly speaking by
the definition of F=ma defined as proportional only to mass and acceleration.
But again, I'm not entirely clear on this.

My own feeling about the heat convertible to force, force convertible to heat
issue that Faraday rejects, is that these quantities, heat and force, are
composite quantities and strictly speaking the modern view of heat does not
include all possible forces, because it excludes photons of a frequency that
are not absorbed by the heat measuring device, which may account for the
velocity of a force. Are we measuring that small slice of the spectrum in the
microwave and infrared, or the movement of particles in the full spectrum? The
definition of heat, I think needs to be more clearly defined, because, clearly
there are moving particles that are not absorbed by the heat measuring device,
whether that is mercury, water, a skin cell, etc. So is the intention to
measure the average velocity of all particles in some volume of space, or to
measure the average velocity of only those particles that are absorbed by the
substance used to determine the quantity of heat? Ultimately mass and velocity
are conserved, so the velocity of the particles as they do mechanical work, can
be transferred to particles that are heated up, but I think that there may be
large velocities of photons within atoms, which, because they are limited to an
orbit, cannot be measured directly using other atoms, but are observed when the
photon exits the atom and takes a straight line direction. So, it may be, that
there are many hidden velocities in atoms that are revealed when photons are
sent into straight line directions from friction. To conclude, I think that,
there are many velocities of photons in atoms. So a small velocity (an example
is like a neutron in fission) might release a much larger velocity summed over
many released particles than went into some event. The velocities were always
there, but simply not moving in straight lines and not visually observable. So
it's an issue of space, the many resulting velocities were already there, but
confined to a small space. But I think we need to open this debate up and try
to find the clearest and most simple and accurate explanations that everybody
can understand and accept as the best theory currently known.
(Oak Field, Whalley Range near) Manchester, England  
151 YBN
[07/23/1849 AD]
3290) EXPER: Use a device similar to the one used by Fizeau to determine if
long photon interval light beams can be halved. use a diffraction grating to
isolate a single frequency of light from a light source. To detect the light a
grating can also be used, or perhaps an electronic tuned circuit. For a
grating, is the spectral line moved because of the blocking by the spinning
toothed wheel? Is this evidence for the particle theory, or can a wave theory
explain this result?
Paris, France  
151 YBN
[1849 AD]
1026)
  
151 YBN
[1849 AD]
2523) David Brewster (CE 1781-1868) invents the lenticular "stereoscope" where
a person looks at two slightly different pictures, one with each eye, which
gives the illusion of three-dimensional features.

Charles Wheatstone discovered the principle (of the stereoscope) and applied it
as early as 1838 to an instrument, in which the binocular pictures are made to
combine by means of mirrors. Brewster uses of lenses for the purpose of uniting
the dissimilar pictures.

Edinburgh, Scotland  
151 YBN
[1849 AD]
2649) Reuters uses pigeons to cover sections where lines are incomplete.
Reuters' original
name is Israel Beer Josaphat. Reuters is a German-born founder of one of the
first news agencies, which still bears his name. Of Jewish parentage, Reuters
becomes a Christian in 1844 and adopts the name of Reuter.
Paris, France  
151 YBN
[1849 AD]
2732)
London, England (presumably)  
151 YBN
[1849 AD]
2763)
(Guy's Hospital) London, England  
151 YBN
[1849 AD]
3065)
(College de France) Paris, France  
151 YBN
[1849 AD]
3114) Barnard is one of the founders of experimental (health science). Barnard
describes the concept of the internal environment of the organism, which leads
to the current understanding of homeostasis, the self-regulation of vital
processes.
Bernard studies under François Magendie at both the Hôtel-Dieu and the
Collège de France. Magendie notices Bernard's skillful dissections and takes
Bernard on as a research assistant.

Bernard's wife, Fanny, opposes vivisection (the act or practice of cutting into
or otherwise injuring living animals, especially for the purpose of scientific
research) so much that, she joins the newly formed society for the protection
of animals, the SPA, and becomes one of its most vocal members. The two have a
legal separation in 1870.

Bernard rejects evolution. Asimov explains that French biologists, even
Pasteur, reject Darwinism, this is partly from the influence of Lamarck and
Cuvier 50 years before.

At his death Bernard is given a funeral arranged and financed by the
government, the first ever given to a scientist in France.
(Collège de France) Paris, France  
151 YBN
[1849 AD]
3135) William Zinsser manufactures shellac into the USA.

Zinsser is a foreman in a Mainz, Germany, shellac factory, who emigrates from
Germany to the United States in 1848. Zinsser discovers that shellac varnishes
are unknown in America. Working from a home laboratory, Zinsser develops a
product and soon establishes the nation's first bleached shellac manufacturing
plant, William Zinsser & Company, in what is then "far uptown rural
Manhattan".

Shellac is made from the secretions of the tiny lac insect, Laccifer lacca.
Shellac is a natural thermoplastic, a material that is soft and flows under
pressure when heated but becomes rigid at room temperature. Shellac is an
ingredient in many products, including abrasives, sealing wax, hair sprays, and
cake glazes. Shellac is used, along with fine clay or other filler, to mold
phonograph records, but, after the early 1930s, synthetic thermoplastics,
particularly vinyl resins, gradually replace shellac.

In the 1800s many mixtures and compositions are based on shellac, the most
successful being the American ones of Peck, Halvorson, and Critchlow.

Manhattan, NY, USA  
151 YBN
[1849 AD]
3195) Ethylamine is a colorless volatile liquid, C2H5NH2, used in petroleum
refining and detergents and in organic synthesis. Also called ethamine.

Methylamine is a toxic flammable gas, CH3NH2, produced by the decomposition of
organic matter and synthesized for use as a solvent and in the manufacture of
many products, such as dyes and insecticides.

Diethylamine, (C2H5)2NH is a water-soluble, colorless liquid with ammonia
aroma, boiling at 56°C; used in rubber chemicals and pharmaceuticals and as a
solvent and flotation agent.

Trietylamine, (C2H5)3N is a colorless, toxic, flammable liquid with an ammonia
aroma; soluble in water and alcohol; boils at 90°C; used as a solvent,
rubber-accelerator activator, corrosion inhibitor, and propellant, and in
penetrating and waterproofing agents.
In 1845 Wurtz becomes an assistant to
Jean-Baptiste-André Dumas, whom Wurtz succeeds at the School of Medicine in
1852.
In 1858 Archibald Couper apparently anticipates Kekulé in working out the
structure of the carbon atom (more detail) and asks Wurtz to present his paper
to the Académie des Sciences. Wurtz delays and Kekulé publishes. When Couper
protests with Wurtz Couper is expelled from Wurtz's laboratory. (I don't worry
about priority. With the camera-thought network, history will show who was
first, and ultimately the important thing is human progress no matter what the
source. In any event, theoriginator of new ideas should always be honestly
recognized by people.)
In 1875 Wurtz is the first chair of organic chemistry at the
Sorbonne.

Wurtz is one of the founders of the Paris Chemical Society (1858), and its
first secretary and three times serves as its president.
(Ecole de Médicine, School of Medicine) Paris, France  
151 YBN
[1849 AD]
3199) Sainte-Claire Deville also isolates toluene and methyl benzoate from tolu
balsam and investigates other natural products before turning to inorganic
chemistry.

Toluene is a colorless, flammable, toxic liquid hydrocarbon aromatic compound
(C6H5CH3), the methyl derivative of benzene. Found in coal-tar light oil and in
petroleum, toluene is mainly obtained from the processing of petroleum
fractions. It is used as a solvent, diluent (serving to dilute), and thinner;
as an antiknock additive in airplane gasoline; and as a raw material for TNT,
benzoic acid and its derivatives, saccharin, dyes, photographic chemicals, and
pharmaceuticals. Toluene is also called methylbenzene.

Toluene was discovered by Pelletier in 1838 (Ann. chim. phys., 1838, 67, p.
269).

Starting around 1857 Deville studies reversible reactions under a general
theory of dissociation. In the course of this investigation Deville devises the
apparatus known as the "Deville hot and cold tube". Deville discovers
dissociation of heated chemical compounds and their recombination at lower
temperatures. (more info. Is the dissociation between atoms, or between
molecule groups?)
Deville is the son of a wealthy shipowner from the Caribbean island
of St. Thomas.
Sainte-Claire Deville commits suicide at 63.
(University of Besançon) Besançon, France  
151 YBN
[1849 AD]
3229)
Braunschweig, Germany  
151 YBN
[1849 AD]
3319)
(University of Montpellier) Montpellier, France  
151 YBN
[1849 AD]
3479)
(University of Glasgow) Glasgow, Scotland  
150 YBN
[02/??/1850 AD]
3364) Clausius writes "Die Potentialfunktion und das Potential" (1859) and "Die
mechanische Wärmetheorie" (1865–67; tr. "The Mechanical Theory of Heat",
1879).

(So is heat a particle or movement? I think my own opinion is that heat is a
movement due to a particle, but its not clear to me. Is the heat the velocity
of the photon or the photon itself? Without the photon there is no heat, but
without the velocity of a photon there is no heat either, so it is in some
sense both a movement and a particle perhaps. It has to do with the quantity of
free photons too, in particular free photons absorbed. For example you could
hold a dense solid cold object and a less dense warm object. The dense object
clearly has more photons and more velocity within it, but the warm object is
emitting more photons, in particular photons of a frequency that are absorbed
by sensors in the skin.)

(Notice how the heat and work equivalent group never refer to velocity (or
momentum) of particles but only to their vis viva, which is 1/2mv^2.)
Clausius rejects
Helmholtz's explanation of the first law of thermodynamics (the conservation of
energy) in the early 1850s. An interesting example in my mind is that if you
put a mass near a large mass, it's potential energy goes up (because the force
of gravity is large on it), as opposed to putting a mass far away from a large
mass. It just seems like the mass is just a mass and there is no difference
physically in it, no matter where it happens to be located. Faraday stated that
the law of gravity violates the conservation of energy, but I think that it is
preserved because any added acceleration is balanced in an opposite direction,
and in addition, two masses moving closer, results in their moving farther away
from all other masses.

In 1857, Clausius wrongly claims priority for Avogadro's hypothesis of diatomic
molecules and in 1866 for the diatomic nature of the oxygen molecule.
(Royal Artillery and Engineering School) Berlin, Germany  
150 YBN
[05/06/1850 AD]
3281) Jean Bernard Léon Foucault (FUKo) (CE 1819-1868), measures that the
light moves more slowly in water than in air, and that the speed of light is
inversely proportional to the index of refraction of the medium.

Roemer had measured the speed of light and proved light to have a finite
velocity in 1676.

In 1834, Charles Wheatstone had used a rotating mirror powered by (wound up)
clock gears to measure the speed of electricity.

Foucault clearly supports the wave theory of light writing in "Journal des
Débats" on May 15, 1850: "To complete the downfall of this poor theory of
emission...to give it the fatal blow, it was only a matter of performing
{Arago's} famous experiment.".

Foucault and Fizeau both independently perform the same experiment, Foucault
finding success first. Historian William Tobin describes Foucault's experiment:
(see image 1) "Sunlight from a heliostat (a heliostat is an instrument in which
a mirror is automatically moved so that it reflects sunlight in a constant
direction) illuminated a 2-mm square entrance aperture. In its initial form,
the aperture was crossed by a vertical grid of eleven fine platinum wires, but
later Foucault used only a single wire, and this arrangement will be described
since it accords with an engraving which he later published {see image 2}.
Let
us consider the air path first with the spinning mirror stationary. Within a
certain range of azimuth (space in the horizontal or X dimension), this mirror
reflects rays from the wire towards the air-path concave mirro, where an image
is produced owing to a converging lens placed earlier along the optical path.
The concave mirror reflects the rays back towards the platinum wire, where they
would refocus, except that Foucault introduced a beam-splitting glass plate
near the aperture to reflect this final image into an eyepiece. To emphasize a
point already made, because a concave mirror was used, the position of the
image in the eyepiece remained the same whatever the azimuth of the spinning
mirror, though of course no image appears if the azimuth of the spinning mirror
was outside the range that fed rays to the concave mirror. A ruling in the
eyepiece marked the undeviated position of the image {see image 2}.
When the
mirror was spinning, it turned through a certain minuscule angle during the
time it took light to make the tript to the concave mirror and back. The final
image was therefore shifted slightly sideways in the eyepiece. The size of the
deviation depended on how much the spinning mirror had rotated, which in turn
depended on the mirror speed and the delay between the outward and returning
beams. With such a complicated path, Foucault reported that the principal
difficulty was obtaining a sharp image.
The spinning mirror was held in a
barrel-like fixture mounted on a spindle {see image 3}. To turn the spindle,
Foucault adandones his beloved clockwork, which he felt was too
self-destructive at high speeds and did not allow the mirror speed to be varied
ina continuous manner or held constant for sufficiently long. Instead, he
adapted the siren {see image 4} devised by the aged Cagniard-Latour...Foucault
adapted the siren into a 24-bladed turbine driven by steam {see image 3}.
...The
{mirror} needed to be dynamically balanced ... {and} ...then statically
balanced. ...
Foucault first saw the image of the wire deviate on 1850 February
17. He will then have known that the experiment was going to work. However, it
took a further two months to set up the water-path leg of the experiment, in
which the light passed through a 3-m long tube of water. To get a satisfactory
final image it was essential that the windows at the end of the tube had
accurately parallel sides; luckily there was a supplier of optical plates in
Paris, MM. Radiguet and Son. ... Distilled water was surprisingly murky because
of microorganisms; water from the public supply provided much superior
transparency. The final image of the wire was nevertheless very dim - and green
- because of absorption by the long column of water. For this reason, both
Foucault and Fizeau were forced to operate with sunlight, and to increase
throughput, Foucault mounted two glass mirror in the barrel, back to back.
{Foucault uses the new chemical silvering process for these mirrors.}
So as to be able
to see the air- and water-path images simultaneously, Foucault masked the
air-path concave mirror with a screen pierced by a narrow, horizontal slit {see
image 6}. This reduced the path of the air-path image {image 2b}, allowing the
water-path image to be seen dimly flanking it {image 2c}. The experiment
finally worked on April 27, a Saturday. Foucault observed the air- and
water-path deviations successively, and then simultaneously, as in {image 2.d},
where a vertical scratch in the eyepiece marked the position of no deviation.
The rightwards displacement of the image of the wire was greater for the water
path, as illustrated. Further, the ratio of the two deviations was as expected
given the refractive index of water. The emission theory was dead,
incontestably incompatible with the experimental results! Within three hours,
Foucault had had four others peer into the eyepiece and confirm his result....
On
Monday, May 6, Foucault reported to the Academy. The mirror speed was estimated
from the pitch (of sound) of the knocking of the bearings, but was not
accurately determined, which prevented an absolute determination of the
velocity of light. With 600-800 r.p.s., the deviations were 0.2 to 0.3 mm.
Foucault went on to suggest how to make an absolute measurement and adapt the
method to calorific rays using the tiny thermometers devised with Fizeau.
....
Non-scientists wanted to see the image deviate too. Hector Berlioz asked to
bring along three friends."

Foucault publishes this as "Methode générale pour mesurer la vitesse de la
lumière dans l'air et les milieux transparants. Vitesses relatives de la
lumière dans l'air et dans l'eau. Projet d'experience sur la vitesse de
propagation du calorique rayonnant.", ("General method to measure the speed of
light in air and the transparent medium. Relative speeds of light in air and
water. Project experiment on the speed of propagation of radiant heat.").
(verify translation) (Find translation of 1850 paper)

In his paper, Foucault writes (note: this is a Google and babel fish
translation since Foucault's writings, shockingly, considering the importance
to science of these works, have not been translated to English to my knowledge)

"The new experimental method that I propose to evaluate the speed of light
being propagated at small distance, is founded on the use of the rotating
mirror invented by Mr. Wheatstone, and indicated by Mr. Arago, as being able to
be used to attack this kind of question. The rotating mirror associated with a
suitable optical apparatus indeed makes it possible to note, to less than one
thirtieth close, the duration of the double course of the light through a
column of water 3 meters in length, and when it is intended to operate only in
the air, a slight modification of this apparatus permits the attainment of a
degree of precision of which it not is not yet possible to specify the limit. A
third modification, designed to spare much the loss of light, will be useful,
and I've come to understand a note by thermometric indications that the heating
radiation until here inseparable from the light, is propagated with same
speed.".

Foucault continues: "Moreover, taking into account lengths of air and water
crossings, deviations have been substantially proportionate to the refractive
indices. These results show a speed of light in water less than in the air and
accordingly, fully confirm the views of Mr Arago indications of the theory of
undulations.
It should be noted as Mr. Arago said at the meeting that the experiment, in
demonstrating a lower speed in water than in air, is quite crucial and is the
decisive call between the two systems. If we would have found an inverse
result, the theory of Newton would remain sustainable, but that the wave theory
is not possibly reversed, waits until it is possible to constitute ether in
order to explain, whatever is the meaning of the change of speed to the changes
of mediums." (It is interesting that no exploration of a particle theory is
examined. It's no credit to the corpuscular supporters that they never created
a theory to support light particles being slowed in denser mediums, so far as I
know.)

In his "Opticks" (in 1704), Newton had theorized that because the path of light
corpuscles is slanted towards the perpendicular, the distance traveled by the
corpuscles must be shorter, and therefore that the speed of the corpuscles must
be faster in denser mediums. (verify) The accepted view given by corpuscular
supporters is that the parallel component of the velocity of a ray of particles
is unchanged when the particles enter the water, but the perpendicular
component is increased by the attraction of the water. The total velocity of
the particles is therefore increased in water. Nobody, so far as I know, had
any alternative corpuscular theory, in particular that the speed of corpuscles
might be slower and the parallel velocity nonzero because of collision with
atoms in water. Before Newton's corpuscular (or "emission") theory, the view
was that light is like sound, a wave in a medium. This view was supported by
(Grimaldi, Hooke, Huygens, Euler, Thomas Young, Fresnel, and others).

The wave interpretation of light is thought to imply that the movement of light
would be slowed in a denser medium. (verify first to claim light would be
slowed in denser medium - Fresnel in 1821?) Thomas Young determined the
wavelength of light in 1801 and theorized that light is a transverse wave in an
aether medium in 1817, as did Fresnel in 1821, and the corpuscular theory of
light then started to lose popularity.
In the undulatory or wave theory,
wavefronts are deviated but not broken when the enter water. This deviation
shorten the space between wavefronts. Since the same number of wavefronts must
pass per second, their reduced separation results in a lower velocity in water.


Foucault's finding that light is slowed down in denser mediums therefore
supports the wave theory. The corpuscular supporters had never theorized that
collisions of light corpuscles and atoms in the medium might delay the passage
of the corpuscles, and as far as I know, no published paper has ever contested
the wave explanation for light being slower in denser mediums, or offered a
corpuscular alternative. Do any known rebuttals or alternative corpuscular
explanations exist?

Tobin explains that this effect is explained in quantum mechanics by Planck's
equation for the momentum of a photon (momentum=Planck's constant/wavelength).
The photon is interpreted differently from the old corpuscular theory (which
presumed particles of light to be material while the photon is viewed as
nonmaterial or massless). Tobin states that "The component of the photon
momentum perpendicular to the interface does increase as the photon passes into
water, as does the total momentum; but the wavelength is thereby reduced. Since
the frequency is unchanged, the velocity, which equals the product of frequency
and wavelength, is lessened too...". However, I think the delay is because of
photons, as masses, colliding and reflecting off the internal structure of the
atoms of the medium. In addition, I think Planck's equation for momentum, being
dependent on wavelength, cannot represent a single photon. This equation of
momentum can only apply to two or more photons, and I think the photon must
have a mass and momentum of its own. This equation may represent the total
momentum of a beam of sequential photons.
Paris, France (presumably)  
150 YBN
[08/28/1850 AD]
5996) The court opera authorities in Dresen refuse to stage Wagner's opera,
Lohengrin, because they are alienated by Wagner’s projected administrative
and artistic reforms. Wagner's proposals would have taken control of the opera
away from the court and created a national theater whose productions would be
chosen by a union of dramatists and composers. Wagner becomes involved in the
German revolution of 1848–49. Wagner writes a number of articles advocating
revolution and takes an active part in the Dresden uprising of 1849. When the
uprising fails, a warrant is issued for Wagner's arrest and he fleas from
Germany, unable to attend the first performance of Lohengrin at Weimar, given
by his friend Franz Liszt on Aug. 28, 1850.

In 1850-51, in Zürich, Wagner writes his ferociously anti-Jewish "Jewishness
in Music" (some of it an attack on Meyerbeer).
Weimar, Germany  
150 YBN
[08/??/1850 AD]
3893)
Paris, France (presumably)  
150 YBN
[1850 AD]
1134)
(Military School) Brussels, Belgium  
150 YBN
[1850 AD]
2613) In this same year, Bond detects the dark inner ring of Saturn (the Crepe
Ring), which Lassell discovers independently only a few nights later. Johann
Galle had discovered the Crepe (or C) ring in 1838.
(What is the reason that
the rings have different colors?)
Vega is also called Alpha Lyrae. Vega is the
brightest star in the northern constellation Lyra and fifth brightest in the
night sky, with a visual magnitude of 0.03 (in photons). Vega is 25 light-years
away.

Vega is a white main-sequence star of spectral class A0 V indicating that Vega
has a surface temperature of 9600 K (16,800°F).

Compared to the Sun, Vega is approximately 2.9 times larger in diameter, 2.5
times more massive, and 60 times more luminous (emits 60x as many photons).

Vega emits far more radiation at infrared wavelengths than would be expected.
This radiation originates from a shell or disk of particles with a temperature
of 100 K (−280°F) surrounding Vega out to a distance of 1.3 × 1010 km (8 ×
109 mi), twice the radius of the solar system.
Harvard, Massachussetts, USA  
150 YBN
[1850 AD]
2663)
Calcutta, India  
150 YBN
[1850 AD]
2817) In 1830 Melloni takes part in an unsuccessful Italian revolution.
(Melloni measures
the heat effect of moonlight (from a high location on Mount Vesuvius.).)
Naples, Italy  
150 YBN
[1850 AD]
2942)
(Hunterian museum of the Royal College of Surgeons) London, England  
150 YBN
[1850 AD]
3008)
(Royal Observatory) Bogenhausen, Germany  
150 YBN
[1850 AD]
3019)
Washington, DC, USA  
150 YBN
[1850 AD]
3115) In 1850, the Academy of Sciences award Bernard, for the third time, its
prize in Experimental Physiology.
(Collège de France) Paris, France  
150 YBN
[1850 AD]
3116) These findings are published as "Recherches sur le curare". C R hebd Acad
Sci, t.31, 1850, p 533-537. Avec J Pelouze. and "Action du curare et de la
nicotine sur le système nerveux et sur le système musculaire." - C. R. Soc.
Biol., t. 2, 1850 (1851), p. 195.
(Collège de France) Paris, France  
150 YBN
[1850 AD]
3130)
(Elkington and Mason copper smelting plant) Pembrey, South Wales, England  
150 YBN
[1850 AD]
3217) Richard Jordan Gatling (CE 1818-1903), US inventor, invents a
double-acting hemp break (an instrument or machine to break or bruise the woody
part of flax or hemp so that it may be separated from the fiber). (human
powered?)

Indianapolis, Indiana (presumably)  
150 YBN
[1850 AD]
3265)
Tarentum, Pennsylvania, USA  
150 YBN
[1850 AD]
3291)
Paris, France (presumably)  
150 YBN
[1850 AD]
3332)
(University of Königsberg) Königsberg, Germany  
150 YBN
[1850 AD]
3471)
(University College, London) London, England  
150 YBN
[1850 AD]
3488) Frankland receives his doctorate at Marburg under Bunsen in 1949.
In 1851,
Frankland becomes the first professor of chemistry at Owens College,
Manchester.
In 1863, Frankland succeeds Michael Faraday as professor of chemistry at the
Royal Institution of Great Britain, London.
Frankland names his son Percy Faraday
Frankland, presumably in honor of Michael Faraday.
In 1894, Frankland receives the
Copley medal of the Royal Society.
Frankland investigates the chamistry of storage
batteries, publishing 3 papers through the Royal Society on this topic.
Frankland installs electricity into his residence using batteries of his own
design.
Frankland makes many contributions to purification of drinking water.
(Queenwood school) Hampshire, England  
150 YBN
[1850 AD]
3561) Cohn is born in the ghetto of Breslau, the first of three sons of a
Jewish merchant.
Cohn is a child prodigy.
From 1842-1846 Cohn studies at the University of Brelau
(now Wroclaw, Poland), but as a Jewish person, Cohn is barred from the degree
examinations, because the University of Breslau will not grant the doctorate to
a Jewish person. So, in 1847 Cohn gets his doctorate degree from the more
liberal University of Berlin at the age of 19. However, Cohn spends the rest of
his life employed teaching at the University of Breslau.
In 1866, at the
University of Breslau, Cohn founds the first institute for plant physiology.
In 1870 Cohn
founds the journal Beiträge zur Biologie der Pflanzen ("Contributions to the
Biology of Plants") in which the founding papers of modern bacteriology
appear.

In 1876 Robert Koch turns to Cohn for a prepublication appraisal of his work on
the cause of anthrax, a disease of cattle, sheep, and sometimes humans. Cohn
agrees to see the unknown country physician and quickly recognizes Koch as "an
unsurpassed master of scientific research". Cohn’s publishes Koch's paper
which shows that Bacillus anthracis is the agent that causes anthrax, in his
journal Beiträge.

Cohn is an effective popularizer of science.
The Encyclopedia Britannica writes
that perhaps Cohn's greatest achievement is his introduction of the strict and
systematic observation of the life histories of bacteria, algae, and other
microorganisms.
(University of Breslau) Breslau, Lower Silesia (now Wroclaw, Poland)  
150 YBN
[1850 AD]
3580)
  
150 YBN
[1850 AD]
4544)
unknown  
150 YBN
[1850 AD]
4700)
London, England (guess)  
150 YBN
[1850 AD]
5995)
Weimar, Germany (presumably)  
149 YBN
[02/03/1851 AD]
3282) Foucault's first pendulum swings in the cellar of the house he lives in
with his mother. Froment makes this and all later pendulums for Foucault. A
substantial piece of cast iron is fixed into the vaulting to provide a solid
suspension for a 5-kg brass bob hung on a 2-m steel wire. Foucault tells Arago
of his discovery and Arago authorizes Foucault to swing his bob with an 11-,
wire in the Meridian Room of the observatory. The Observatory has a north-south
line set into the floor which can serve as a reference line.

Foucault suspends an iron ball, 2 feet in diameter, from a steel wire more than
67m (220feet) long, under the dome of a large Paris church. The pendulum has a
spike that just clears the floor and makes a line in sand placed on the floor.
In this way, the pendulum appears to draw lines in different direction as the
earth slowly moves relative to the motion of the pendulum. The pendulum swings
a full rotation in 31 hours and 47 minutes, which is the rate to be expected
for the latitude of Paris. This experiment causes great excitement. Heracleides
was the first to suggest that the earth is rotating, 22 centuries before, and
Foucault is the first to demonstrate this fact.

For this demonstration and a similar one using a gyroscope (in 1852), Foucault
receives the Copley Medal of the Royal Society of London in 1855 and is made
physical assistant at the Imperial Observatory, Paris.

Foucault publishes this experiment in 1851 as "Demonstration physique du
mouvement de rotation de la terre au moyen du pendule" ("Physical Demonstration
of the Rotation of the Earth by Means of the Pendulum") presented to the
Academy by Arago.

Foucault writes "The very numerous and important observations which have
hitherto been made upon the pendulum, are especially relative to the time of
its oscillations; those which I propose to relate to the Academy, have
reference principally to the direction of the plane of oscillation, which being
gradually displaced from east to west, gives a sensible proof of the diurnal
motion of the terrestrial globe.
In order to succeed in justifying this
interpretation of a constant result, I will neglect the earth's movement of
translation, which is without effect upon the phenomenon which I wish to
exhibit, and I will suppose the observer to have established at the pole a
pendulum of the greatest simplicity: that is, a compound pendulum composed of a
heavy, homogeneous, and spherical mass, suspended by a flexible thread from a
point absolutely fixed. I will, moreover, suppose at first, that this point of
suspension is exactly in the prolongation of the axis of rotation of the globe,
and the solid masses which support it do not participate in the diurnal
movement. If, under these circumstances, the mass of the pendulum is drawn
aside from its position of equilibrium, and abandoned to the action of gravity
without having any lateral impulse given to it, its center of gravity will pass
through the vertical, and by its acquired velocity will rise upon the other
side of the vertical to a height nearly equal to that whence it came. Arrived
at this point, its velocity dies out, changes its sign, and brings it back,
causing it to pass again through the vertical to a point a little below its
starting point. Thus a movement of oscillation is excited in an arc of a circle
whose plane is clearly determined, to which the inertia of the mass gives an
invariable position in space. If then these oscillations continue for a certain
time, the motion of the earth, which does not cease turning from west to east,
will become sensible by contrast with the immobility of the plane of
oscillation, whose trace upon the ground will appear to have a motion
comfortable to the apparent motion of the heavenly sphere; and if the
oscillations could be continued for twenty-four hours, the trace of their plane
would have executed in that time a complete revolution around the vertical
projection of the point of suspension.
Such are the ideal conditions under which the motion
of rotation of the globe would become evidently accessible to observation. But,
in fact, we are obliged to take our fixed point upon a moving base; the parts
to which the upper end of the pendulum thread is attached cannot be withdrawn
from the diurnal movement, and it might be feared, at first sight, that this
motion, communicated to the thread and to the mass of the pendulum, would alter
the direction of the plane of oscillation. However, theory shews us here no
serious difficulty, and on the other hand, experiment has shewn me that,
provided the thread be round and homogeneous, it may be turned with
considerable rapidity around its axis in either direction, without influencing
sensibly the position of the plane of oscillation, so that the experiment such
as I have described it, must succeed at the pole.

But when we descend to our latitudes, the phenomenon becomes complicated by an
element of considerable difficulty of appreciation, and to which I desire
particularly to call attention of mathematicians.

In proportion as we approach the equator, the plane of the horizon assumes a
position more and more oblique to the axis of the earth, and the vertical, in
place of turning on itself, as at the pole, describes a cone of greater and
greater angle; whence results a retardation in the apparent motion of the plane
of oscillation, a motion which becomes nothing at the equator, and changes its
sign in the other hemisphere. To determine the law according to which this
motion varies in different latitudes, we must have recourse either to analysis
or to mechanical and geometrical considerations, which do not suit the narrow
limits of this note. I must, therefore, confine myself to announcing that the
two methods accord (neglecting certain secondary phenomena) in shewing that the
angular motion of the earth during the same time multiplied by the sine of the
latitude. I then set to work with confidence, and in the following way I
established the reality of the predicted phenomenon as to its direction and
probable amount.".

Foucault concludes: "In conclusion I will present on further remark:
It is, that the
facts observed under these circumstances, accord perfectly with the results
announced by Poisson in a very remarkable memoir, read by him before the
Academy, 14th November, 1837. In this memoir, Poisoon, treating of the motion
of projectiles in the air, and taking into consideration the diurnal movement
of the earth shows, by calculation that in our latitude, projectiles thrown
towards any point, experience a deviation which takes place constantly towards
the right of the observer, standing at the point of departure and looking
towards the trajectory. It appears to me that the mass of the pendulum may be
compared to the projectile, which deviates towards the right while departing
from the observer, and necessarily in the opposite direction in returning
towards its mean plane of oscillation, and indicates its direction.. But the
pendulum possesses the advantage of accumulating the effects, and allowing them
to pass from the domain of theory into that observation.".

An audience of people watches the pendulum. The rope holding the pendulum from
moving is burned off to prevent the effects of cutting. (Perhaps a small
vibration could be amplified over time, but it seems like the original
direction would be maintained. Still a burnt rope might also impart an uneven
motion in some direction since not all of the rope separates at once.)

Pendulums complete a 360 degree circuit in 23 hour 56 minutes at the North or
South Pole, increasing in time to thousands of hours around the equator.

Fifty years before, Laplace wrote in his "Celestial Mechanics" (translated from
French) "Although the rotation of the Earth is now established with all the
certainty available in the physical sciences, a direct proof of this phenomenon
would nevertheless be of interest to mathematicians and astronomers.".

In March 1851, a pendulum is installed in the Paris Panthéon to demonstrate
what Foucault has found. In ancient Greece pantheons were temples dedicated to
all gods. The Panthéon in Paris' Latin Quarter is a former church dedicated to
the cit's patron saint, Saint Genevieve, whose prayers supposedly saved Paris
from Atilla the Hun in the 400s CE. A new building replaced the original
building in 1791. Louis-Napoléon approves the installation of the pendulum.
Foucault comments "Every man, whether converted or not to prevailing ideas
(about the Earth's rotation) remains thoughtful and silent for a few moments,
and generally leaves carrying with him a more insistent and lively appreciation
of our unceasing motion in space.". One magazine reports "Pendulum mania"
spreading like wildfire after this demonstration. (Imagine the response to the
public demonstration of seeing and hearing thought.)

In 1852 Louis-Napoléon gives Foucault 10,000 francs.
Paris, France (presumably)  
149 YBN
[03/??/1851 AD]
2680)
France  
149 YBN
[03/??/1851 AD]
3112) Talbot sues for patent infringement but loses. Archer does not patent
this process, although does patent other inventions.
Archer dies very poor.

At the time, collodion is also sold as finger nail polish after dye is added to
it.
Bloomsbury, London, England (presumably)  
149 YBN
[03/??/1851 AD]
3480)
(University of Glasgow) Glasgow, Scotland  
149 YBN
[05/06/1851 AD]
6250)
New Orleans, Lousiana, USA  
149 YBN
[09/29/1851 AD]
3292)
Paris, France (presumably)  
149 YBN
[10/22/1851 AD]
2726) According to one source, Faraday's introduction of the concept of lines
of force is rejected by most of the mathematical physicists of Europe, since
they assume that electric charges attract and repel each other, by action at a
distance, making such lines unnecessary.

According to the Encyclopedia Britannica, by 1850 Faraday will evolve a
radically new view of space and force. Space is not "nothing", the mere
location of bodies and forces, but a medium capable of supporting the strains
of electric and magnetic forces. The energies of the world are not localized in
the particles from which these forces arise but rather are to be found in the
space surrounding them. Therefore the field theory is created. Maxwell will
admit that the basic ideas for his mathematical theory of electrical and
magnetic fields came from Faraday; his contribution was to mathematize those
ideas in the form of his classical field equations.

James Clerk Maxwell will formulate a mathematical theory of the propagation of
electromagnetic waves from Faraday's theory of lines of force moving between
bodies with electrical and magnetic properties. In 1865, Maxwell theorizes
mathematically that electromagnetic phenomena are propagated as waves through
space (with an aether as a medium) moving at the velocity of light, which will
lay the foundation of radio communication being confirmed experimentally in
1888 by Hertz and developed for practical use by Guglielmo Marconi. (My own
view is that Maxwell theorized that electricity is light waves because the
speeds were similar, and then created a mathematical justification for this
view, with Hertz detecting photons emitted from electric wire, just as photons
are emitted from all atoms. So I think that Maxwell can be credited with the
idea that light is emitted from current and inspiring Hertz, however, I think
the photons emitted from electrical current, are the same as photons emitted
from any object, and Maxwell coincidentally inspired a very powerful concept of
invisible photon detection which would rise into invisible photon
communication.)

James Maxwell will write: "Faraday, in his mind's eye, saw lines of force
traversing all space where the mathematicians saw centres of force attacting at
a distance: Faraday saw a medium where they saw nothing but distance: Faraday
sought the seat of the phenomena in real actions going on in the medium, they
were satisfied that they found it in a power of action at a distance impressed
on the electric fluids.... Faraday's methods resembled those in which we begin
with the whole and arrive at the parts by analysis, while the ordinary
mathematical methods were founded on the principle of beginning with the parts
and building up the whole by synthesis".

I think the mistakes that Faraday make, are 1) not realizing that a electric
(magnetic) field is made of particles, 2) not thinking that those particle in
the electric field are tiny centers of gravity 3) not recognizing that, at tiny
magnifications, many particles may be grouping, colliding and result in the
appearance of a stronger force but may be the result of the accumulated
movements of many particles. This view is the obvious method to apply if
theorizing an argument to entertain the concept of gravity, which apparently
either was not done or not popular. So the idea of "action at a distance" is a
phrase that is applied as a dogma in my opinion, because it implies that an
electric field is just empty space, not chock full of particles and that the
magnetic force, like gravity must emanate from the center of the magnet. It is
maybe a subtle point, but the idea that an electric field is made of material
particles is still not popular.

Had Faraday supported the view of electrical current as a fluid made of
particles, the wave theories of light may not have lasted as long as it has,
and the wave theory of electricity might not have ever been created, saving the
human species more than 100 years of theoretical progress in science.

According to Oxford University Press Philosophy Dictionary states that
Faraday's discovery of electro-magnetic 'lines of force' and view of the atom
as merely a center of force opened up field theory, which itself owns ancestry
to the views of Kant, and especially Boscovich.

Clearly by this time, the corpuscular or emission theory appears to have lost
favor.
(Royal Institution in) London, England  
149 YBN
[11/25/1851 AD]
6258)
Cambridge, Massachussetts, USA  
149 YBN
[11/??/1851 AD]
3544) Riemann was born into a poor Lutheran pastor’s family.
Riemann plans on a
career in the Church in accordance with his father's wishes but changes to
mathematics.
Riemann also teaches course in mathematical physics (at Göttingen).
Riemann dies of
tuberculosis before the age of 40.
(University of Göttingen) Göttingen, Germany  
149 YBN
[1851 AD]
2653) The International Morse Code is adopted.
The American Morse Code is inadequate
for the transmission of much non-English text and so a variant ultimately
becomes known as the International Morse Code is used on all cables, for land
telegraph lines except in North America, and later for wireless telegraphy.
Europe  
149 YBN
[1851 AD]
2681)
St Petersburg, Russia  
149 YBN
[1851 AD]
2756)
Cambridge, England (presumably)  
149 YBN
[1851 AD]
2816) One induction coil of Ruhmkorff in 1851 that is awarded a 50,000-franc
prize in 1858 by Emperor Napoleon III as the most important discovery in the
application of electricity.

Ruhmkorff is able to improve Callan's two-winding induction spark-coils, on the
basis of the research conducted in Paris by Masson and Breguet in 1842.
  
149 YBN
[1851 AD]
2825) Ariel rotates around Uranus at a mean distance of 191,240 km (118,830
miles) from the center of the planet, taking 2.52 days to complete one orbit.
Like the other large Uranian moons, Ariel rotates synchronously with its
orbital period, keeping the same face toward the planet. Ariel has an average
diameter around 1,160 km (720 miles) and has a density of about 1.67 grams per
cubic cm which is consistent with a composition of roughly equal parts water
ice and rock, perhaps intermixed with a small amount of frozen methane.
The surface of
Ariel has scarps (a line of cliffs produced by faulting or erosion) and long
valleylike formations. These features and the small number of large impact
craters suggests that Ariel has the youngest surface of all of Uranus's major
moons.

Umbriel is the nearest of the five major moons of Uranus and the one having the
darkest and oldest surface of the group. Umbriel orbits Uranus once every 4.144
days at a mean distance of 265,970 km (165,270 miles). Umbriel has a diameter
of 1,170 km (727 miles) and a density of about 1.4 grams per cubic cm. Umbriel
appears to be composed of equal parts water ice and rocky material, intermixed
with small amounts of frozen methane. Umbriel is distinct from the other major
moons of Uranus in having no evidence of past tectonic activity. Its surface is
uniformly covered with impact craters, most of them large, measuring 100-200 km
(60-120 miles) across. Craters of this size could only have been produced early
in the history of the star system, when planetesimal-size impacting bodies
existed.

The name "Ariel" and the names of all four satellites of Uranus then known were
suggested by John Herschel in 1852 at the request of Lassell and named for
characters in Alexander Pope's poem "The Rape of the Lock". Ariel is also the
name of the spirit who serves Prospero in Shakespeare's "Tempest".
Malta  
149 YBN
[1851 AD]
2830) |
Wiltshire, England (presumably)  
149 YBN
[1851 AD]
2952)
(University of Tübingen) Tübingen, Germany  
149 YBN
[1851 AD]
3025)
Dublin, Ireland (presumably)  
149 YBN
[1851 AD]
3154) From 1868-1883, De La Rue investigates the discharge of electricity
through gases by means of a battery of 14,600 chloride of silver cells.
London, England (presumably)  
149 YBN
[1851 AD]
3182)
(University of Zürich) Zürich, Germany  
149 YBN
[1851 AD]
3204)
(Royal College of Chemistry) London, England  
149 YBN
[1851 AD]
3208) Secchi enters the Jesuit order in Rome, studies at the Collegio Romano,
and becomes the director of its observatory in 1849.
Secchi's works include a star
catalog (1867).
(Collegio Romano) Rome, Italy  
149 YBN
[1851 AD]
3273) In 1854 Stokes suggests that the Fraunhofer lines might be caused by
atoms in the outer layers of the Sun that absorb light of certain wavelengths,
however concedes priority to Kirchhoff. Although the first to publish this
theory is Foucault in 1849. In fact, Stokes. himself publishes the English
translation of Foucault's 1849 paper.

The 1911 Encyclopedia Britannica states that Stokes' perhaps best-known
researches are those which deal with the undulatory theory of light. Stokes is
an advocate of the wave theory of light and in the ether as a medium for the
waves of light. To explain how the ether can be rigid but moved, Stokes
suggests that the aether is like wax that is rigid but flows under a slow but
steady force, such as that applied by the orbiting planets. In addition, Stokes
hypothesizes that the planets drag part of the ether along with them because of
friction.

Stokes is among the first to appreciate the importance of the work of James
Joule.

The Royal Society's catalog of scientific papers gives the titles of over a
hundred memoirs by Stokes published to 1883.
Stokes is the youngest son of the
Reverend Gabriel Stokes, rector of Skreen.
In 1849 Stokes is appointed to the
Lucasian professorship of mathematics at Cambridge, but finds it necessary to
supplement his slender income from this post by teaching at the Government
School of Mines in London.
In 1852 Stokes receives the Rumford medal of Royal Society
for his paper on fluorescence (1852) in which Stokes shows how fluorescence can
be used to study the ultraviolet segment of the spectrum.
In 1885 Stokes is President of
the Royal Society (1885-1892). (As President of the Royal Society and supported
of the wave theory for light, clearly the overthrow of the corpuscular theory
originated by Newton was complete in England at this time.)
In 1893 Stokes receives
the Copley medal. (state for what)
Stokes serves as Conservative member in Parliament
for Cambridge University.
A devoutly religious person, Stokes is deeply interested in the
relationship of science to religion. For me, the uselessness of religions is
obvious.
(I am not sure that Stokes' achievements in science justify the awards he
receives. Perhaps this is an example of perhaps a wealthy person, that either
buys awards or is given awards in recognition of monetary contributions to
science or simply for have other wealthy connections. Stokes might have
contributions to science that are not public.)
Cambridge, England  
149 YBN
[1851 AD]
3275)
Cambridge, England  
149 YBN
[1851 AD]
3334)
(University of Königsberg) Königsberg, Germany  
149 YBN
[1851 AD]
3341) EXPER:How fast can CCD chips capture images?
Wiltshire, England (presumably)  
149 YBN
[1851 AD]
3404) Arrest helps Galle find Neptune. Galle reads off the stars he observes
while Arrest checks each with its position against the star chart.
Arrest finds
several (previously unknown) comets.
(Leipzig Observatory) Pleissenburg, Germany (presumably)  
149 YBN
[1851 AD]
3474)
Leipzig, Germany (presumably)  
149 YBN
[1851 AD]
5998) Rigoletto is produced in Venice (after trouble with the censors, a
recurring theme for Verdi) and is a huge success. Hugo's play depicts a king
(Francis I of France) as an immoral and cynical womanizer, something that is
not accepted in Europe during the Restoration period.(verify)
Venice, Italy  
148 YBN
[01/07/1852 AD]
2880) William Robert Grove (CE 1811-1896), British physicist, applies an
induction coil high voltage through an evacuated tube with various gases, and
performs electrolysis on gases.

Grove describes his experiments in "On the Electro-Chemical Polarity of Gases".
London, England (presumably)  
148 YBN
[05/10/1852 AD]
3489)
(Queenwood school) Hampshire, England  
148 YBN
[05/11/1852 AD]
3274) Stokes receives the Rumford medal of Royal Society for this paper.
Cambridge, England  
148 YBN
[1852 AD]
2604) Sabine superintends the establishment of magnetic observatories
throughout the world (and so this provides Sabine with regular access to
Earth's magnetic data).
From 1861-1871, Sabine is president of the Royal Society.
London, England (presumably)  
148 YBN
[1852 AD]
2678) E. P. Smith coins the word "telegram".

(It is interesting how telegram is replaced by phone call, email, vmail, and
perhaps thought-gram or thought-message.)

  
148 YBN
[1852 AD]
2920)
(University of Giessen), Giessen, Germany  
148 YBN
[1852 AD]
2938)
(Hunterian museum of the Royal College of Surgeons) London, England  
148 YBN
[1852 AD]
3086)
(University of Heidelberg), Heidelberg, Germany  
148 YBN
[1852 AD]
3104) Otis' device is demonstrated at the Crystal Palace Exposition in New
York.
In 1854, Otis tests his new design with himself inside. The elevator cable is
cut and it descends safely.
Yonkers, NY, USA  
148 YBN
[1852 AD]
3117) Later in 1869, the Swiss physician Horner additionally observes reduced
sweating in a woman with a tumor invading the sympathetic nerve in the neck.
The complete clinical syndrome is widely called Horner's Syndrome, but in
France is referred to as the Syndrome de Claude Bernard-Horner.

For this work Bernard is awarded his fourth award from the Academy of Sciences
for experimental physiology.
(Collège de France) Paris, France  
148 YBN
[1852 AD]
3192) Rudolf Albert von Kölliker (KRLiKR) (CE 1817-1905), Swiss anatomist and
physiologist, publishes "Handbuch der Gewebelehre des Menschen" (1852; "Manual
of Human Histology"): probably the best early text on histology.

This textbook may be the first good study of histology, the science started 50
years before by Bichat without a microscope.
In this work Kölliker expounds on his
isolating the first smooth muscle cell.

Kölliker shows that nerve fibers are elongated parts of cells, therefore
anticipating the neuron theory, (in which) the neuron is the basic unit of the
nervous system.

(University of Würzburg) Würzburg, Germany  
148 YBN
[1852 AD]
3283)
Paris, France (presumably)  
148 YBN
[1852 AD]
3335)
(University of Königsberg) Königsberg, Germany  
148 YBN
[1852 AD]
3413)
(University of Strasbourg) Strasbourg, France  
147 YBN
[01/19/1853 AD]
3482)
(University of Glasgow) Glasgow, Scotland  
147 YBN
[02/16/1853 AD]
3143) In 1872, Angström is awarded the Rumford medal of the Royal Society.
(University of Uppsala) Uppsala, Sweden  
147 YBN
[1853 AD]
2655)
Vienna, Austria  
147 YBN
[1853 AD]
2689)
Stockholm (and Uppsala), Sweden  
147 YBN
[1853 AD]
2894) During his passage back from London, Borden sees several children on
board ship die after drinking contaminated milk. Because no one yet understands
how to keep milk fresh, spoiled and even poisonous milk is not uncommon.
Visiting the
Shaker community at New Lebanon, N.Y., in 1851, Borden observes sugar making
with airtight pans and decides that milk could be condensed and could remain
wholesome indefinitely.
Borden knows that the Shakers (?) use vacuum pans to preserve fruit,
and he begins experimenting with a similar apparatus in search of a way to
preserve milk.

In 1861 the U.S. government orders 500 pounds of condensed milk for troops
fighting in the Civil War. As the conflict grows, government orders increase,
until Borden has to license other manufacturers to keep up with demand. After
the war, Bordon's New York Condensed Milk Company has a ready-made customer
base in both Union and Confederate veterans.
Bordon teaches school in southern
Mississippi and immigrates to Texas in 1829, where he prepares the first
topographical map of Texas, helps write the first constitution of that state,
is cofounder of the first long-lived Texas newspaper, and lays out the city of
Galveston.
New York City, NY, USA (presumably)  
147 YBN
[1853 AD]
3186)
(University of Freiburg) Freiburg im Bresigau, Germany  
147 YBN
[1853 AD]
3293)
Paris, France (presumably)  
147 YBN
[1853 AD]
3309)
(Conservatoire des Arts et Métiers) Paris, France  
147 YBN
[1853 AD]
3312) The concept of potential energy presumes a set course over a period of
time, where in my view, the forces at each instant need to be recalculated
using the law of gravitation. Actually, I think that simply the mass times the
velocity squared of any particle can be viewed as its potential energy, or
possibly kinetic energy, without any presumptions about future forces (although
because of gravity, there must be forces that change the energy, because
gravity changes the acceleration, and therefore the velocity of the particle,
which in turn changes the potential energy.

One question I have, is, how can the amount of heat emitted from exothermic
chemical reactions be related to energy of the reagents? For example, in a
battery, the energy is related to electric current. Perhaps the initial mass of
the chemicals? So Joule's constant applies to the conversion of electric
current to heat, but I think it depends on wire diameter and other parameters.
(University of Glasgow) Glasgow, Scotland, UK  
147 YBN
[1853 AD]
3468)
(University of Bonn) Bonn, Germany (presumably)  
147 YBN
[1853 AD]
3525) Thomsen is a member of Copenhagen's Municipal Council for 35 years and is
the driving force responsible for the development of Copenhagen's gas, water,
and sewage system.
(Polytekniske Laereanstalt) Copenhagen, Denmark  
147 YBN
[1853 AD]
3538) When a revolution starts in 1847, Cannizzaro returns from his studies in
Pisa to his native Sicily, and takes an active role in fighting on the side of
the republicans, who seek to break the domination of the Italian states by
Austria and the House of Bourbon (rulers of the kingdom of Naples). After the
failure of the revolt in 1849, Cannizzaro flees to Paris.
Cannizaro becomes
vice president of the Italian senate.
In 1891 Cannizzaro receives the Copley medal of
the Royal Society.
(Collegio Nazionale in Alessandria) Piedmont (now part of Italy), Italy  
147 YBN
[1853 AD]
3644) James Clerk Maxwell (CE 1831-1879), Scottish mathematician and physicist,
work in geometrical optics leads to the discovery of the fish-eye lens.

(Cambridge University) Cambridge, England  
147 YBN
[1853 AD]
5999)
Rome, Italy  
147 YBN
[1853 AD]
6247)
Paris, France (presumably)  
146 YBN
[11/08/1854 AD]
2682)
Madrid, Spain  
146 YBN
[11/08/1854 AD]
2683)
Madrid, Spain  
146 YBN
[1854 AD]
2569) Michel Eugéne Chevreul (seVRuL) (CE 1786-1889) publishes a treatise
debunking psychic phenomena entitled "De la baguette divinatoire" (1854).

Paris, France (presumably)  
146 YBN
[1854 AD]
2693)
Melbourne (and Victoria), Australia  
146 YBN
[1854 AD]
2792)
Berlin, Germany  
146 YBN
[1854 AD]
2893)
Greenwich, England (presumably)  
146 YBN
[1854 AD]
2940)
(Hunterian museum of the Royal College of Surgeons) London, England  
146 YBN
[1854 AD]
2945)
(University of) Göttingen, Germany  
146 YBN
[1854 AD]
3111) Snow is called the "father of epidemiology".
London, England  
146 YBN
[1854 AD]
3167) Weierstrass' lectures were published, as "Die Elemente der Arithmetik",
by one of his students in 1872.
(Catholic Gymnasium) Braunsberg, East Prussia  
146 YBN
[1854 AD]
3173) Boole writes "Logic is conversant with two kinds of relations, relations
among things, and relations among facts. But as facts are expressed by
propositions, the latter species of relation may, at least, for the purposes of
Logic, be resolved into a relation among propositions. The assertion that the
fact or event A, is an invariable consequent of the fact or event B, may to
this extent, at least be regarded as equivalent to the assertion that the truth
of the proposition affirming the occurrence of the event B always implies the
truth of the proposition affirming the occurrence of the event A. Instead then
of saying that Logic is conversant with relations among things, and relations
among facts, we are permitted to say that it is concerned with relations among
things, and relations among propositions. Of the former kind of relations we
have an example in the proposition- 'All men are mortal' of the latter kind in
the proposition- 'If the sun is totally eclipsed, the stars will become
visible'. The one expresses a relation between 'men' and 'mortal beings;' the
other between the elementary propositions- 'The sun is totally eclipsed;' 'The
stars will become visible'. Among such relations, I suppose to be included,
those which affirm or deny existence with respect to things, and those which
affirm or deny truth with respect to propositions. Now let those things, or
those propositions among which relation is expressed be termed 'the elements of
the propositions by which such relation is expressed'. Proceeding from this
definition we may then say that i) the premises of any logical argument express
given relations among certain elements, and that the conclusion must express an
implied relation among those elements or among a part of them ie a relation
implied by or inferentially involved in the premises.
(Queen's College) Cork, Ireland  
146 YBN
[1854 AD]
3276) (Sir) George Gabriel Stokes (CE 1819-1903), British mathematician and
physicist, publishes "Stokes' theorem" which describes an equality concerning
the cosines of a normal vector of a surface.
Stokes for several years sets the
Smith's Prize Exam at Cambridge with this proving this theorem as a test
question.

The left hand expression is in two earlier works of Stokes'. Before appearing
in print in 1854, this theorem had already appeared in a letter of William
Thomson to Stokes on July 2, 1850.

This theorem, a theorem by Gauss, and the same theorem by Reimann will be
eventually generalized and unified.

Cambridge, England  
146 YBN
[1854 AD]
3352)
(University of Königsberg) Königsberg, Germany  
146 YBN
[1854 AD]
3365) (My own view on this topic is that there is a larger equation describing
the conservation of velocity. Each atom has a certain quantity of velocity,
which is proportional to the quantity of photons in it. So much of the heat
produced by simple friction, is the release of particles with a velocity that
is simply changing direction out of the atom and into a straight line as a free
photon. The velocity was already there from perhaps some gravitational exchange
far in the past, such as a collision with another photon. It may be that a
photon-photon collision is what causes the photons to be released in simple
friction. So there is a larger, more inclusive equation which includes {sums}
the velocities of all particles involved. For example, velocity of moving
particles in arm and metal file + velocity of particles in piece of metal that
will be freed by passing file scraping on metal => velocity of particles in
metal file + velocity of free photons released from scraped metal ... I am
saying that it is something like that ... that this concept is more complex and
can't be confined to quantity of movement=quantity of heat. But we should
verify all of these claims for all theories as best as possible.)
(Royal Artillery and Engineering School) Berlin, Germany  
146 YBN
[1854 AD]
3423) In writings and public appearances Wallace opposes vaccination, eugenics,
and vivisection while strongly supporting women’s rights, but also believes
in and promotes spiritualism.

Also over the course of his life, Alfred Wallace publishes 21 books, and the
list of his articles, essays, and letters in periodicals totals more than 700
items.

Among Wallace's books are: "The Malay Archipelago: The Land of the Orang-Utan,
and the Bird of Paradise" (1869), "Contributions to the Theory of Natural
Selection (1870), a two-volume "Geographical Distribution of Animals" (1876)
and "Island Life" (1880) which synthesize knowledge about the distribution and
dispersal of living and extinct animals in an evolutionary framework, and
Darwinism (1889) which contains an explanation of natural selection and
Wallace's points of divergence from Darwin.
Wallace wins the Royal Society of
London’s Royal Medal (1868), Darwin Medal (1890; for his independent
origination of the origin of species by natural selection), Copley Medal
(1908), and Order of Merit (1908); the Linnean Society of London’s Gold Medal
(1892) and Darwin-Wallace Medal (1908); and the Royal Geographical Society’s
Founder’s Medal (1892). (Perhaps all these medals are mainly due to Wallace's
public support of the theory of common ancestry and natural selection.)
Malaysia  
146 YBN
[1854 AD]
3472)
(University College, London) London, England  
146 YBN
[1854 AD]
3545)
(University of Göttingen) Göttingen, Germany  
146 YBN
[1854 AD]
3546)
(University of Göttingen) Göttingen, Germany  
146 YBN
[1854 AD]
3551)
(Collège de France) Paris, France  
146 YBN
[1854 AD]
3552) Berthelot is born into a middle-income Parisian family.
Berthelot is the son of a
doctor, and studies medicine at the Collège de France but is more interested
in chemistry, and becomes assistant to Antoine-Jérôme Balard in 1851.
Berthelot is
professor of organic chemistry at the Ecole Supérieure de Pharmacie
(1859–76) and professor of chemistry at the Collège de France
(1864–1907).
In 1860, Berthelot declines German chemist August Kekule’s offer to join the
Karlsruhe Conference, which is organized to reach an agreement on formulas and
atomic weights, because Berthelot wants to return to equivalent weights.

Berthelot unsuccessfully leads the opposition to the atomic conventions put
forward by Cannizzaro.
Berthelot wrongly suggests that the heat emitted by a chemical
reaction is its driving force. However, reversible reactions (shown by
Williamson) show that heat is not the driving force of reactions. Gibbs will
describe "free energy" and "chemical potential" to define the driving force
behind chemical reactions. (As a novice, I feel that simple physical proximity
to each other has to be one part of the drive of reaction, in addition, to
material distribution - atomic structure, particle collisions and
interactions.)
In 1866 Berthelot becomes president of the Chemical Society of Paris.
In 1881
Berthelot becomes a senator.
In 1886 Berthelot enters the cabinet.
In 1889 Berthelot
succeeds Louis Pasteur as secretary of the French Academy of Sciences.

Berthelot is a prolific writer, with some 1,600 published papers and books in
his lifetime.

Scholars of chemical history are greatly indebted to Berthelot for his book
"Les Origines de l'alchimie" (1885) and his "Introduction a l'etude de la
chimie des anciens et du moyen age" (1889), as well as for publishing
translations of various old Greek, Syriac and Arabic treatises on alchemy and
chemistry ("Collection des anciens alchimistes grecs", 1887-1888, and "La
Chimie au moyen age", 1893). Berthelot is also the author of "Science et
philosophie" (1886), which contains a well-known letter to Renan on "La Science
ideale et la science positive", of "La Revolution chimique, Lavoisier" (1890),
of "Science et morale" (1897), and of numerous articles in "La Grande
Encyclopedie", which Berthelot helps to establish.

Berthelot is one of the last chemists to reject Dalton's theory of atoms. He
rejects the theories of chemical atoms and molecular constitutions, which he
considered to be "theories of language", as opposed to his own system of
equivalents, which he views to be "theories of facts" firmly grounded on
empirical evidence.

(Some people may confuse Pierre Eugène Marcellin Berthelot (BARTulO or BRTulO)
(CE 1827-1907) with another French chemist, Claude-Louis Berthollet (BRTOlA)
(CE 1748-1822).)
(Collège de France) Paris, France  
146 YBN
[1854 AD]
3671) Crookes is the oldest of 16 children.
In 1856, having inherited a large fortune
from his father, Crookes devotes himself entirely to scientific work of various
kinds at his private laboratory in London.
Crookes has 10 children.
In 1859 Crookes
founds the Chemical News, which makes him widely known, and Crookes is editor
and owner all his life.
Crookes grows interested in psychic research and
spiritualism.
(private lab) London, England(presumably)  
145 YBN
[01/04/1855 AD]
3650)
Edinburgh, Scotland  
145 YBN
[01/04/1855 AD]
3651) For this paper Maxwell receives the Rumford Medal of the Royal Society of
London.
Edinburgh, Scotland  
145 YBN
[08/08/1855 AD]
2760) Charles Babbage (CE 1792-1871), English mathematician, publishes "On the
Method of Laying Guns in a Battery without exposing the men to the shot of the
enemy."

Another interesting statement by Babbage is "...men of science in Italy might
have made three steps in advance..." which may imply that Babbage and others
are already aware of the possibility of walking robots, and the potential
military advantage such a machine could supply. Perhaps this is just
coincidence, but if not, it also implies that Babbage, for some reason feels
reluctance to openly express the idea of walking machines.

Cambridge, England (presumably)  
145 YBN
[09/??/1855 AD]
3285)
Paris, France (presumably)  
145 YBN
[12/10/1855 AD]
3641) (Possibly put either entire text or above notes here)
(Cambridge University) Cambridge, England  
145 YBN
[1855 AD]
2463)
Tours, France (presumably)  
145 YBN
[1855 AD]
2627) Marshall Hall (CE 1790-1857) introduces (1855) a method of artificial
respiration that was widely applied in cases of drowning.

London, England (presumably)  
145 YBN
[1855 AD]
2632)
London, England (presumably)  
145 YBN
[1855 AD]
2637) George Peacock (PEKoK) (CE 1791-1858), publishes a memoir of Thomas
Young, and edits the first two volumes of the three volume "Miscellaneous
works" (1855, London) of Thomas Young. This is the main source for those
interested in Young's contribution to the transition in popularity from
Newton's corpuscular theory of light to the wave (or undulatory) theory for
light.
These three volumes contain 1. Scientific memoirs. 2. Scientific memoirs
{concluded} Biographies of men of science. 3. Hieroglyphical essays and
correspondence. The articles "Languages" and "Herculaneum", from the Supplement
to the Encyclopaedia Britannica. Lives of eminent scholars (which contains
Young's biographies of scientists).
Cambridge, England (presumably)  
145 YBN
[1855 AD]
2764)
(Guy's Hospital) London, England  
145 YBN
[1855 AD]
3020)
Washington, DC, USA  
145 YBN
[1855 AD]
3021) In 1862 Mallet publishes two volumes, dealing with the Great Neapolitan
Earthquake of 1857 and "The First Principles of Observational Seismology".
Mallet then brings forward evidence to show that the depth below the earth's
surface, where impulse of the Neapolitan earthquake came from, is about 8 or 9
geographical miles.

One of his Mallet's most important essays is that communicated to the Royal
Society (Phil. Trans. clxiii. 147; 1874), entitled "Volcanic Energy: an
Attempt to develop its True Origin and Cosmical Relations" in which Mallet
seeks to show that volcanic heat may be attributed to the effects of crushing,
contortion and other disturbances in the crust of the earth; these disturbances
leading to the formation of lines of fracture, more or less vertical, down
which water moves, and if the temperature generated is sufficient, volcanic
eruptions of steam or lava would follow.
Washington, DC, USA  
145 YBN
[1855 AD]
3024)
(Vesuvius Observatory) Naples, Italy  
145 YBN
[1855 AD]
3082)
(University of Heidelberg) Heidelberg, Germany  
145 YBN
[1855 AD]
3131) In 1866 Parkes founds the Parkesine Company and begins commercial
production of parkesine. However, Parkes's business fails. Daniel Spill. A
talented chemist, and works manager at the Parkesine Company takes over the
company, renaming it the Xylonite Company and markets celluloid as Xylonite and
Ivoride, but goes bankrupt in 1874. However, Spill reopens in a new location in
1875, takes on several partners in 1877 becoming the British Xylonite Company
and they achieve commercial success producing celluloid collars and cuffs.

John Wesley Hyatt of the Hyatt Brothers, in the United States will discover
that nitrate cellulose mixed with camphor creates a much more pliable product.
The Hyatt Brothers will find planet-wide success and bring in the age of modern
plastics.
(Elkington and Mason copper smelting plant) Pembrey, South Wales, England  
145 YBN
[1855 AD]
3139) In 1869, in conjunction with H. P. J. Vogelsang, Geissler proves the
existence of liquid carbon dioxide in cavities in quartz and topaz.
Geissler was
educated as a glass-blower.
Bonn, Germany  
145 YBN
[1855 AD]
3160)
(University of Berlin) Berlin, Germany (presumably)  
145 YBN
[1855 AD]
3163) Ducheene publishes over fifty volumes containing his researches on
muscular and nervous diseases, and on the applications of electricity both for
diagnostic purposes and for treatment.

This work is translated to English by GV Poore in "Selections from the clinical
works of Dr Duchenne (de Boulogne)." (London: The New Sydenham Society, 1883).

In 1838 interest in electrical methods of treatment become popular when
Cerletti and Bini introduce electroconvulsive therapy (Cerletti, 1950). High
voltage electricity on the human nervous system in the crude involuntary
application of "electroshock" or "electroconvulsive" therapy, even
involuntarily still is used in some psychiatric hospitals on unwilling people.
This practice of applying a large voltage to the human nervous system needs to
be stopped if unconsensual, but even if consensual (which I think should be
allowed although I do not advocate), the theories behind it, and the supposed
beneficial results, in particular given the trauma induced, are highly doubtful
in my mind. I compare it to cooking a hotdog with electricity in terms of
precision and overall effect. The wise use of electricity in testing the
functioning of nerves, and stimulating paralyzed muscles (although how much of
this may be replaced by remote or local photon muscle stimulation when the
secret is finally shown to all is unknown) are some beneficial results of the
application of electricity to health science of Duchenne and others.

Quoting from selections of Duchenne's writings:
"...faradisation (applying a high
voltage) of a very wasted muscle in the last stage of atrophy causes no
movement, or only a feeble one, of the limb or part of the limb to which it
belongs, especially when the health antagonising muscles oppose a tonic
resistance to its action. We must not conclude that the contractility of such a
muscle is weakened, the true meaning of such a fact being merely that the
fibres are insufficient for performing the normal work of the muscle."
Duchenne
describes paralysis of the tongue, palate and lips, a disease called
"glosso-labio-laryngeal paralysis" which Duchenne had originally named
"progressive muscular paralysis of the tongue, soft palate, and lips". This
raises the issue of naming conventions, which in my view should be as simple
and accurate as possible. Problems arise when there are many different
languages, and many times Latin is preferred, although Latin is not in common
use anymore.

In describing progressive locomotor ataxy, Duchenne writes "The sexual power in
man sooner or later has manifested considerable change: once it was increased;
in all the others it was weakened or abolished.", and it causes me to wonder if
Duchenne applied so-called faradisation to a penis. Electrical stimulation of
the anus is used to make the penis erect in mammal species, however does direct
electrical stimulation cause the penis to become erect?

In describing lead palsy and "vegtable palsy" Duchenne writes "under the
influence of local faradisation, I noted on the right side that the extensor
communis digitorum, extensor minimi digiti, extensor secundii internodi, and
the extensores carpi radiales, did not contract to a maximum current with moist
rheophores, and even electro-puncture (a needle being plunged into the muscles)
only caused a few fibrillary contractions with the most intense current.".

Duchenne writes about so-called "hyterical paralysis". One interesting case
Cuchenne describes is case number 76 "A girl, aged 24, a baker's assistant,
usually healthy, was in the habit of carrying bread daily to a customer. One
day she found him dead in his bed, and the shock was so great as to cause an
hysterical fit, lasting several hours. After this she remained deprived of
movement, the lower limbs being tetanised, and presenting a well-marked
equino-varus. Her menstruation was suppressed, and she became blind. Certain
senses were strangely perverted. If she were pinched or spoken to on the right
side, she felt and heard on the left.
The contractions of the legs lasted several
years, long after the disappearance of the other troubles, and this persistence
might have caused a fear that they were symptomatic of damage to the cord.
Nevertheless the whole group of symptoms just given made me certain of its
hysterical origin.
This diagnosis was completely justified by her spontaneous and
sudden recovery, only some deformity of the joints, caused by the
long-sustained faulty posture of the feet, remaining."

Duchenne writes on "nervous deafness": "1. The rheophore having been placed in
my own external Auditory meatus (previously half-filled with water), and the
apparatus being at its minimum, I perceived, on the instant that the
intermission of the current took place, a little dry parchment-like sound, a
crackling which I referred to the bottom of the external auditory meatus. When
the intermissions were very rapid the sound resembled a crepitation, or the
noise produced by the wings of a fly flying between a window-pane and the
blind. The intensity of these sounds increased with the force of the current.
2. To the
auditory phenomenon was added a sense of tickling in the bottom of the ear,
proportional to the strength of the current, and absolutely limited to the
point at which the sound seemed to originate.
3. After a certain time, and with a certain
degree of tension of current (voltage), I felt very plainly a tickling of the
right side of my tongue at the junction of the middle and posterior thirds. As
the stength of the current increased, the tickling reached the point of the
tongue, where I then felt a numbness and a disagreeable pricking which was not
actually painful. This experiment is often followed by a numbness, and
sometimes by an over-sensitiveness of the two front thirds of the edge of the
tongue, which persists a considerable time.
4. It seemed also as if my tongue
were dry and rough on the side operated upon.
Such were the phenomena which first
attracted my attention, and which appeared almost in the order I have indicated
in the patients who were submitted to this experiment.
5. I must mention a very
important phenomenon which, often enough, appears when the stimulation is
sufficiently energenetic, viz., the production of a peculiar taste. It was the
last phenomenon to attract my attention, because it is masked byu the tickling
and pricking which accompanies it. It would pass unobserved if attentionwere
not directed to it. Although the taste is feeble, it can be recognized to be of
a metallic kind.
6. Finally, some patients perceived which each intermission a
luminous sensation on the side stimulated.".

Duchenne describes curing asphyxia (absence of respiration) by faradisation of
the skin over the heart.

In a number of cases Duchenne describes faradisation curing problems it seems
doubtful were cured by applying electricity and more likely other causes. In
this sense Duchenne advertises faradisation, as a cure-all, and more than is
likely and accurate. One example is case 118, a child who has a general
paralysis, which lasted about forty-eight hours, and was followed by a complete
loss of voice, and a difficulty in swallowing and breathing...", Duchenne
writes "...The palsy returned many times, but was soon overcome by faradisation
of the phrenic nerves. After faradizing the palate, phrynx, and front of the
neck on a level with the larynx, the child sucked better, and voice came back a
little. he was completely cured in a few sittings.". Case no 119 is another
example, which makes use of the very abstract so-called disease of "neurosis",
Duchenne writing "Case no. 119 - Neurosis marked by a kind of apnea. Cured by
faradising the skin of the praecordia, and by faradising the phrenic nerve.".
In this case, Duchenne describes a young man "of nervous temperament" who has
intervals where he stops breathing for from thirty to sixty seconds.
Paris, France  
145 YBN
[1855 AD]
3196)
(Ecole de Médicine, School of Medicine) Paris, France  
145 YBN
[1855 AD]
3200)
(École Normale Supérieure) Paris, France  
145 YBN
[1855 AD]
3553)
(Collège de France) Paris, France  
145 YBN
[1855 AD]
3564)
(University of Breslau) Breslau, Lower Silesia (now Wroclaw, Poland)  
145 YBN
[1855 AD]
3565)
(University of Breslau) Breslau, Lower Silesia (now Wroclaw, Poland)  
144 YBN
[1856 AD]
2650) The Western Union Telegraph Company is founded.
Western Union must store every
telegraph, and keep them on file for wealthy connected people to search through
the messages of people they are interested in. Why do we never hear about this
massive telegraph library?
Western Union became the dominant telegraph company in the
United States.
Mississippi, USA (and New York)  
144 YBN
[1856 AD]
2654) By 1856 the register in the Morse system is replaced by a sounder
(speaker?), and the code is transcribed (onto paper) directly from the sounds
by the operator.

  
144 YBN
[1856 AD]
2868)
Aurignac?, France  
144 YBN
[1856 AD]
3044) Charles Robert Darwin (CE 1809-1882), tells his friends Lyell and J. D.
Hooker about his theory of evolution. both Lyell and Hooker do not accept
evolution which they are familiar with through Lamarck. On their urging Darwin
starts to write a book on the theory (1856).

Downe, Kent, England (presumably)  
144 YBN
[1856 AD]
3095)
(New York University) New York City, New York, USA  
144 YBN
[1856 AD]
3096)
(New York University) New York City, New York, USA  
144 YBN
[1856 AD]
3097) This work is a In this work, Draper summarizes the history of science,
spending a chapter on the Museum in Alexandria, concluding the chapter with the
murder of Hypatia.

Draper's preface begins: "WHOEVER has had an opportunity of becoming acquainted
with the
mental condition of the intelligent classes in Europe and
America, must have
perceived that there is a great and
rapidly-increasing departure from the public
religious faith, and
that, while among the more frank this divergence is not
concealed,
there is a far more extensive and far more dangerous
secession, private and
unacknowledged.

So wide-spread and so powerful is this secession, that it can
neither be treated
with contempt nor with punishment. It cannot
be extinguished by derision, by
vituperation, or by force. The
time is rapidly approaching when it will give rise
to serious
political results.

Ecclesiastical spirit no longer inspires the policy of the world.
Military fervor in
behalf of faith has disappeared. Its only
souvenirs are the marble effigies of
crusading knights, reposing
in the silent crypts of churches on their tombs.

That a crisis is impending is shown by the attitude of the great
powers toward the
papacy. The papacy represents the ideas and
aspirations of two-thirds of the
population of Europe. It insists
on a political supremacy in accordance with its claims
to a
divine origin and mission, and a restoration of the mediaeval
order of things, loudly
declaring that it will accept no
reconciliation with modern civilization."

Draper concludes: "As to the issue of the coming conflict, can any one doubt?
Whatever
is resting on fiction and fraud will be overthrown.
Institutions that organize impostures
and spread delusions must
show what right they have to exist. Faith must render an
account
of herself to Reason. Mysteries must give place to facts.
Religion must relinquish
that imperious, that domineering
position which she has so long maintained against Science.
There
must be absolute freedom for thought. The ecclesiastic must learn
to keep himself
within the domain he has chosen, and cease to
tyrannize over the philosopher, who,
conscious of his own
strength and the purity of his motives, will bear such
interference
no longer. What was written by Esdras near the
willow-fringed rivers of Babylon,
more than twenty-three
centuries ago, still holds good: 'As for Truth it endureth and is
always
strong; it liveth and conquereth for evermore."'.
(New York University) New York City, New York, USA  
144 YBN
[1856 AD]
3109) In 1860 Bessemer starts his own steel works, using phosphorus-free iron
ore, and sells high-grade steel for one-tenth the prices of the competition. He
grows rich in a very few years.

The invention of the open-hearth (Siemens-Martin) process in the late 1860s
eventually is more popular than the Bessemer process. William Siemens, a German
person living in England revisits an old proposal for using the waste heat
given off by the furnace; directing the fumes from the furnace through a brick
checkerwork, Siemans heats the brick to a high temperature, then used the same
pathway for the introduction of air into the furnace; the preheated air
increases the temperature.
In his youth Bessemer learns metal processing in his father's
type foundry and machine design and chemistry in London.

Bessemer invention of movable stamps for dating deeds and other government
documents.
Before aged 20 Bessemer invents a new way to stamp deeds, which the
British government uses but doesn't compensate Bessemer for.
Bessemer improves a
typesetting machine.
Bessemer manufactures "gold" powder from brass for use in paints.
Bessemer
grows wealthy from his secret brass powder process.
Bessemer retires a rich man in 1873.
Cheltenham, Gloucestershire, England (announcement)  
144 YBN
[1856 AD]
3118)
(Sorbonne) Paris, France  
144 YBN
[1856 AD]
3119)
(Sorbonne) Paris, France  
144 YBN
[1856 AD]
3136) Francois Charles Lepage invents "Bois Durci" (BOE DRSE?), a form of
plastic based on cow's blood.

This is a plastic based on an animal polymer patented in France in 1856 by
Francois Charles Lepage who calims "A New Composition of materials which may be
employed as a substitute for wood, leather, bone, metal and other hard or
plastic substances". Bois Durci is made from blood (from the Paris
slaughterhouses) and powdered wood, mixed with coloring to simulate wood color.
Lepage heats and stirs the mixture until it acquired the 'correct consistency'
and then molds it in a heated mold. The mixture is cured under heat and
pressure to produce a hard, dense, glossy, molding.

Paris, France  
144 YBN
[1856 AD]
3168)
(Industry Institute) Berlin, Germany  
144 YBN
[1856 AD]
3181)
(University of Vienna) Vienna, Austria, Germany  
144 YBN
[1856 AD]
3350)
(University of Bonn) Bonn, Germany  
144 YBN
[1856 AD]
3425) Charles William (Carl Wilhelm) Siemens is the younger brother of Ernst
Wener von Siemens (CE 1816-1892), who after improving the indicator telegraph
of Wheatstone, founds with Halske, in 1847, the company of
"Telegraphenbaunstalt von Siemens & Halske" to manufacture and construct
telegraph systems, eventually expanding to London, St. Petersberg and Vienna.
Charles becomes a partner in Ernst's subsidiary British company.

Siemens designs the cable-laying ship Faraday for laying a new trans-Atlantic
cable in 1874.
London, England (presumably)  
144 YBN
[1856 AD]
3442)
(Tulse Hill)London, England  
144 YBN
[1856 AD]
3457)
Edinburgh, Scotland  
144 YBN
[1856 AD]
3554)
(Collège de France) Paris, France  
144 YBN
[1856 AD]
3607)
(University of Florence, Florence, Italy demonstrates in Froment's workshop)
Paris, France  
144 YBN
[1856 AD]
3774) Perkin is inspired by the lectures of Faraday, as Faraday was once
inspired by the lectures of Davy. After seeing the lectures, Perkins becomes
determined to attend the Royal College of Chemistry.

In 1889 Perkin is awarded the Davy medal.
(Royal College of Chemistry) London, England  
143 YBN
[01/26/1857 AD]
4005)
Paris, France  
143 YBN
[03/24/1857 AD]
3999) Sound recorded mechanically by the sound vibrating a stylus that draws
onto paper.

The phonautograph, an early cylinder sound recording device that records sound
mechanically by drawing the sound vibration shape onto paper. Scott is the
first to record sound using a membrane instead of directly attaching a stylus
to a string, tuning fork or bell.

Leon Scott (Édouard-Léon Scott de Martinville, (CE 1817–1879)) invents the
phonautograph, the earliest known mechanical device for recording and
reproducing sounds including music and speech. This device consists simply of
an ellipsoidal barrel. The sound receiver is open at one end and closed at the
other. From the closed end projects a small tube, with a stretched flexible
membrane across it. In the center of the membrane is a bristle which acts as a
stylus and vibrates with the membrane. In front of the membrane is a horizontal
cylinder wrapped with a sheet of paper and covered with a layer of lampblack
(carbon) which the bristle rests lightly against. Any sound vibrations entering
the ellipsoid are transmitted by the membrane to the stylus, which, when the
cylinder is made to revolve and to advance slowly, describes on the lampblack
surface a wavy line which is a phonographic record of whatever vibrations have
been produced. In 1870 Fleeming Jenkin and Ewing record sounds onto a tin foil
phonograph. The physicist and instrument maker Konig of Paris builds a device
based on Leon Scott's invention, but nothing practical is created until Thomas
Edison constructs a machine in which a receiving funnel is substituted for the
ellipsoid, an iron diaphragm for the membrane, a sharp metallic point for the
bristle, and a tin-foil-covered cylinder in place of the cylinder coated with
lamp-black. With the sound vibrations indented as opposed to traced on the
surface of the cylinder, the machine can be reversed which causes the stylus to
travel over the spiral line indented by the recording point, and the original
sonud is reproduced by the diaphragm.


In January, Scott had deposited his first paper to the Academy of Sciences on
recording sound vibrations to sooted glass plates.

Now in March 1857, Scott deposits the paperwork for a patent on the
phonautograph-the same basic design described in the "Principes de
Phonautographie", but now lays out in greater detail with drawings and a sample
phonautogram and instead of plates of glass uses a hand-cranked cylinder.

This patent is the first to publicly introduce a rotating cylinder to record
sound vibrations. Scott writes:
"The process I have invented-hitherto completely
unknown, and for which I am requesting a patent- consists of fastening a simple
or composite stylus near the center of a thin membrane placed at the end of any
acoustic conduit. This stylus light grazes a substance sensitive to the
lightest friction, such as for example a film of lampblack - a substance
deposited on a glass, a metal, or even a piece of paper or fabric. The
sensitive film passes under the stylus at a regular and determined speed. When
one speaks, sings, or plays an instrument in the presence of the acoustic
conduit, the stylus traces figures or drawings in keeping with the sounds
produced. Afterwards I fix this novel writing by immersion in a liquid
carburet, followed by a bath of albuminous water. I then make prints called
negatives directly, or positive prints indirectly by photography or transfer to
stone, etc.

With the aid of this process and the interchangeable parts of the phonautograph
(fig. 2,3,4,5 of the supporting drawing). I collect the acoustic trace of
speech at a distance- of the song of the coice and of various instruments. I
propose to apply my process to the construction of a divider instrument; to
that of a mathematical tuner for all instruments, of a stenographer for the
voice and of instruments; to the study of the conditions of sonority of various
commercial substances and alloys; and to produce industrial designs for
embroideries, filigrees, jewelry, shades, illustration of books of an entirely
new kind.

The first figure of the plate clearly shows my process in its most extreme
simplicity - a process which is in my mind roughly independent of the number of
thin membranes, of their size, of the form and dimensions of he conduit to
which they have been applied, of the manner of suspension of the phonautograph,
and of the nature of the motor which imparts speed to the sensitive film.".
Scott then goes on to explain each part in particular the addition of the
cylinder. Scott writes:
"dir.-stylus director - Small cylinder of very light material
performated along its axis and glued firmly to the membrane. It is intended to
receive the stylus and to maintain it in a fixed and determined direction.".
Scott describes the use of a motor too writing:
"fig. 6 -sensitive film that passes
under the stylus set in motion by the action of a trumpet at a distance, at a
speed determined by the movement of a pendulum and made uniform by means of a
motor borrowed from clockwork or from the electromagnet - a motor not
represented in the figure.". Scott concludes writing "For greater clarity, I am
appending to the drawing of my apparatuses a print in duplicate of the acoustic
figures of the voice, or the cornet- of drawings I obtain before any
construction of apparatuses and by the only use of the process of figure 1.".
Scott describes the process:
"The manner of proceeding to obtain phonautographic prints
is very simple. A strip of paper is rolled up on the cylinder while being
stretched. This paper, which turns with a nearly uniform speed, is charged with
an even, opaque, exceedingly thin film of lampblack. Towards the center of the
membrane is placed the stylus, of which the end that does the tracing is taken
from a feather of certain birds. This point, so very thin, obeys all the simple
or complex movements of the membrane. In this state the stylus is introduced to
the cylinder in such a manner that it grazes it while remaining fixed in the
direction of its shadt. One makes the sound heard at the opening of the tub or
conduit, the membrane begins vibrating, the stylus follows its movements and
its end traces upon the cylinder, which describes a continuous helix, the
figures of the vibration of the sound produced. They show the number of the
timbre thereof. These figures are large when the sound is intense, microscopic
if it is very weak, spread out if it is low, squeezed together if it is high,
of a regular and straightforward pattern if the timbre is pure, uneven and
somewhat shaky if it is bad or clouded.

Here now is the series of interesting experiments for physicists,
physiologists, instrument makers, {and} lovers of the sciences, which can
already be carried out with the apparatus built as represented in the present
certificate:

1. To write the vibratory movement of any solid to be used as a term of
comparison with the movements of a fluid; to count the number of vibrations
carried out by the solid in a unit of time by means of the marking
chronometer.

2. A tuning fork having been calibrated by means of the preceding experiment to
a determined number of vibrations in a unit of time (500 or 1000 for example),
to count, by causing them to write simultaneously, the number of vibrations
achieved by any agent capable of vibrating 9solid or fluid) in a space of time
as short as one might wish (a few thousandths of a second). Example: to count
and measure the various phases of a noise and the intervals of time contained
between rapid and successive sound phenomena; to test the relative sonority of
metals, alloys, wood, etc.

3. To write the vibrations produced in a membrane by one of more pipes sounding
sumultaneously, to count the number thereof, to show the phases thereof; to
obtain the acoustic figure or diagram of each chord and dissonance; to write
likewise the song of any wind instrument; to show the characteristic timbre of
these instruments; to write the composite movement resulting from the sounds of
two or more instruments playing simultaneously.

4. To write the song of a voice, to measure the extent thereof with the marking
chronometer or the calibrated marking tuning fork; to write the scale of a
singer, to measure the accuracy thereof with the marking tuning fork; to show
the purity or isochronism of the vibrations thereof, as well as the timbre; to
write a melody and transcribe it with the aid of the marking tuning fork; to
write the simultaneous song of two voices and to show the harmony or discord
thereof.

5. To study acoustically the physiological or pathological movements of the
vocal apparatus and of its parts during the various emissions of sound, the
shout, etc; to mark down the characteristic timbre of a given voice;

6. To study the articular voice, the declamation (see in the appended plates a
first application to ordinary writing); to show the syllabic diagrams.

7. To inscribe by the combination of the second method (the flexible stylus)
and the third (the fixing) the movements of the pendulum, of the teetotum or
top, of the magnetized needle, the manner of locomotion of an insect, etc."

Scott describes plate 2 writing:
"...For noting declamation exactly it does not suffice
to mark down above or below the line the longs and the shorts, the fortes and
the pianos, the raisings and lowerings of pitch, the inalations, the breathing,
and the pauses and the explosions; it is necessary to represent clearly and
easily the quantum or mathematical value of each of these modifications.

The phoautographic trace furnishes at present-without one having to be occupied
with articulation- a very simple means of objectively representing the artist's
diction. This trace is a kind of reptile, the coils of which follow all the
modulations or inflections of discorse. It suffices for translating by sight-
except for the articulation - to make the following remarks: the horizontal
distance of the foot of the curves indicates the pitch or tonality; the height
of the same curves the intensity of the voice; the detail of the curves the
timbre; the absence of curves the pauses or silences. The few natural
expressions opposite suffice for understanding this page.

represents the deep voice
the high-pitched voice
a high-pitched voice descending to a deep
one
a deep voice rising to the high-pitched on
an intense voice
an average voice
a weak voice
the
tremolo on the letter r
the cadence on a vowel
the outburst of the voice

So to this rival faithless Hedelmone must have given this diadem! In their
cruel rage, our lions
of the desert, beneath their burning laei,
sometimes tear apart the
trembling traveler-
It would be better for him for their devouring
hunger to scatter the scraps of
his palpitating flesh
than to fall alive into my terrible hands!". Scott
describes plate 3 as the "calibration of a sound by means of the chronometer".



Notice that playing these recordings on paper out loud is not claimed. Playing
recorded - that is permanently stored - sounds out loud will only be known
publicly with the phoneograph of Thomas Edison in 1877 which records the sounds
as impressions into tin foil - although playing live sounds from a microphone
through a wire and out a speaker will be first done publicly by Philip Reiss in
1861.

A recording made on April 9, 1860 of a person singing the words, "Au clair de
la lune, Pierrot repondit" is currently the oldest known sound recording. This
soot-covered paper is converted to audio in 2008, replayed from a digital
scan.

It is disappointing that so few people know about Leon Scott, and so few have a
biography on Scott and the telautograph. It is a combination of the evilness
and fear of those who want to keep technology and science secret together with
the underinformed and/or easily fooled who believe and follow the outlandish
claims of religions and pseudosciences.

There is some confusion about the history of sound recording between Hooke and
Chladni's sand drawings and this first rotating cylinder.

THere is a claim that Wilhelm Weber recorded the sound vibrations of a tuning
fork onto a sooted glass plate in 1830. There is also a claim that Duhamel was
the first to record sound to a sooted glass cylinder in 1840.

Note that this is the first public record of at least the technical possibility
of people, in particular, governments, and telegraph and telephone companies,
accumulating data records of sound, before this, could only be paper records on
which a person wrote or typed the sounds, and of course, photographs, and text
information. It seems very likely that people in governments, in particular
military, and in the telegraph and telephone companies were secretly recording
and playing back sounds before this time, in particular presuming they saw and
heard thought and were doing remote neuron activation in 1810. Is Arthur Korn
the first to apply this pressure writing method to record the intensity of each
dot in an image?

According to one source, Scott succeeds in causing the phonautograph to render
back faint sounds from the blast of two huge organ pipes, three feet from the
instrument.
Paris, France  
143 YBN
[04/??/1857 AD]
3354)
(Royal Institution in) London, England  
143 YBN
[07/17/1857 AD]
3121) Thomas Andrews (CE 1813-1885), Irish physical chemist measure the density
of ozone, and shows that ozone is an allotrope of oxygen, but cannot determine
its composition(chronology for second part).
Ozone was first identified by
Schönbein.

An allotrope is any of two or more forms of the same chemical element. They may
have different arrangements of atoms in crystals of the solid, for example,
graphite and diamond for carbon, or different numbers of atoms in their
molecules, for example, ordinary oxygen (O2) and ozone (O3).

(Queen's College) Belfast, Ireland  
143 YBN
[08/08/1857 AD]
3412)
(University of Lille) Lille, France  
143 YBN
[12/10/1857 AD]
3325) Cayley plays a large role in persuading the University of Cambridge to
admit women as students.
London, England (presumably)  
143 YBN
[12/27/1857 AD]
2873) Plücker writes (translated): "The idea of employing tubes with platinum
electrodes fused into them for observing the electrical discharge through
rarefied gases, instead of the electrical egg, as originally employed by
Ruhmkorff and Quet, may be considered in many respects a happy one. Such tubes,
containing various gases and vapours, are prepared in this city, of the most
different forms, by M. Geissler, and present sometimes an appearance of
incomparable beauty. Geissler's tubes (I give them, and with justice, this name
although the first such tubes were not prepared by him) were tried at the
beginning of this year in the Physical Cabinet: and what more natural than the
thought of approximating such tubes in various ways to the poles of a magnet
during the discharge? Davy had already noticed that the arch of light which he
formed between carbon-points by means of a powerful battery was diverted by the
magnet. Arago had predicted such diversion. In the same way it was possible to
predict generally the nature of the diversion of the electric current in
Geissler's tubes. But on the actual performance of the experiment, in addition
to the phaenomena which were looked for, certain unexpected one presented
themselves; namely, the division of the light-stream, its decomposition at the
negative electrode into an undulating flickering light, and the extension of
the stream from the positive electrode into a brilliantly illuminating fine
point...
This electrolysis of dilute compound gases received complete verification in
subsequent cases. In tubes containing hydriodic acid, the iodine is gradually
deposited. In highly rarified gases this electrolysis by the electric stream,
as it becomes finely divided, often manifests itself suddenly by a remarkable
alteration of colour. Examples of this were furnished by tubes containing
phosphoretted hydrogen and sulphurous acid. The laws of the electrolysis
brought about by the spark of Ruhmkorff's apparatus may, however, be traced in
gases and vapours of ordinary density.
...
In the different Geissler's tubes the light appears of all kinds of colours,
often of a very intense nature, and on analysis with the prism yields variously
modified spectra.
...
The dark bands first observed by Rugmkorff and Quet in the electrical egg
(electric egg electrodes) appear in Geissler's tubes of the most varied shape,
and in some of them with the greatest distinctness. ... In wider tubes the dark
intervals may attain a breadth of 5 millims.; they become narrower if the
electric light passes from a wide tube into a narrower one. They often appear
only after the discharge has passed for a long time through the tube, and then
become gradually better and better defined. ... the discharges of light take
place at intervals, which, if Ruhmkorff's apparatus be employed, depend upon
the rapidity with which the breakings of the current follow one another. The
phaenomena can only consist in an aggregation of matter at definite parts of
the tube which become luminous through the discharge, while the passage of the
electricity from one luminous plate to the other is dark.
...
In the experiments immediately to be described I employed a great upright
horseshoe magnet, to the two limbs of which two heavy armatures were applied, 4
cm thick, 13 cm wide, and 20 cm long. Each of these armatures was rounded
circularly at one end, and the rounded extremities were directed towards one
another, being kept by an interposed brass disc, at a distance of about 4 mm.
...
I placed a tube about 270 mm long, widened in the middle to an ellipsoid ...
This tube contained a trace of phosphorus, and gave a beautiful red light when
the discharge was led through it by means of the two platinum wires fused into
its extremities. ...
In two cases the electrical light-currents were attracted in
the ellipsoid; in the other two they were repelled.
...
A perfectly similarly-shaped tube, containing a small quantity of hydrogen
instead of the trace of phosphorus, showed exactly the same appearances, with
the single exception that the light, instead of being red, was bright violet.
...
The two arcs of light, which were before circular and which bordered the ring
in which the atmosphere of light had become concentrated around the
warmth-pole, assumed the form of magnetic curves.
"
Plücker follows up on January 25, 1858 by stating clearly "In accordance with
the phaenomena described in the latter part of the preceding paper, we may say
that electric light under the circumstances in point is magnetic. Inasmuc h as
such light, which proceeds from one point of the negative electrode in all
directions, is drawn together by the magnet to a luminous magnetic curve
passing through the same point, the original rays behave as iron-filings would
do if we imagine them infinitely fine, perfectly flexible, and attached to the
point of the electrode in opposition to the force of gravitation." (Here the
view is that light particles and electric current particles (later called
electrons) are the same, as opposed to the view that the light particle are
emitted from the electric particles in such arcs.)

On March 30, 1858 Plücker writes "The behavior towards magnetism of that light
which, proceeding from the negative electrode, spreads out in all directions,
is so remarkable that I shall in the first place recur to it again. We can best
illustrate this behaviour by considering the well-known fact, that when iron
filings are strewn upon a piece of stiff paper covering the pole of a magnet,
they arrange themselves in curves which have been called magnetic curves, or
lines of magnetic force. Such curves render the distribution of the power of a
magnet visible even when analysis is unable to determine their form. in every
such curve the separate particles of iron having, under the influence of the
magnet, become themselves little magnets, arrange themselves with their
attracting poles together so as to form a chain. Could we remove the particles
of iron from the influence of gravitation and distribute them through the whole
space surrounding the magnetic pole, then such chains assuming the form of
magnetic curves would traverse the whole magnetic field, and furnish a visible
image of the distribution of the magnetic force. ... The hypotheses
conditioning such a phaenomenon are such as can scarcely by realized; so that
the phaenomenon itslf will probably remain a merely imaginary one. if, however,
in place of the linked iron chain, we suppose rays of magnetic light, the
phaenomenon is converted into one which actually exists. " (EX: It would be
interesting to attach a magnet inside a tube and see the beams of light forms
around the magnetic field.)
Plücker describes a system using lines instead of points
as the fundamental geometric elements.

In 1847 Plücker is made professor of physics at Bonn, and this begins the
record of Plücker's work in physics after a life dedicated to mathematics.
(University of Bonn) Bonn, Germany  
143 YBN
[1857 AD]
2831)
Wiltshire, England (presumably)  
143 YBN
[1857 AD]
2858)
(University of Göttingen) Göttingen, Germany (presumably)  
143 YBN
[1857 AD]
2910) In 1870 the electric telegraph lines of the United Kingdom, worked by
different companies, is transferred to the Post Office, and placed under
Government control. (Perhaps there was a difference of opinion about how the
public's messages are stored. Under government control, the heads, handlers and
controllers of the telegraph service can be replaced by popular opinion unlike
the US system.)
(King's College) London, England (presumably)  
143 YBN
[1857 AD]
3034)
London, England (presumably)  
143 YBN
[1857 AD]
3079) Robert Bunsen (CE 1811-1899), German chemist, publishes his only book
"Gasometrische Methoden" (1857) which brings gas analysis to a new level of
accuracy and simplicity.

In 1838, Bunsen started working with gases, starting with work on the gases
present in the blast furnaces used for making iron. Accompanied by a
collaborator, Lyon Playfair, Bunsen visits England and their results help
iron-masters save fuel. Bunsen and Playfair suggest techniques that can recycle
gases through the furnace and retrieve valuable escaping by-products such as
ammonia. From this work Bunsen goes on to show how to determine the specific
gravity of gases, to measure their absorption by liquids, and their rates of
diffusion. Bunsen perfects the technique of eudiometry, where known volumes of
gas are exploded with oxygen and the amounts of the products measured.

(University of Heidelberg) Heidelberg, Germany  
143 YBN
[1857 AD]
3148)
(Indiana University) Indiana, USA  
143 YBN
[1857 AD]
3218)
Indianapolis, Indiana (presumably)  
143 YBN
[1857 AD]
3286)
Paris, France (presumably)  
143 YBN
[1857 AD]
3366)
(New Polytechnicum) Zurich, Germany  
143 YBN
[1857 AD]
3367)
(New Polytechnicum) Zurich, Germany  
143 YBN
[1857 AD]
3394) Thomas Rickett builds a "road locomotive" (steam engine car).

Buckingham, England  
143 YBN
[1857 AD]
3455)
(University of Heidelberg) Heidelberg, Germany  
143 YBN
[1857 AD]
3508) Bond identifies a number of comets.
Bond dies of tuberculosis at age 29.
(Harvard U) Cambridge, Massachussetts, USA (presumably)  
143 YBN
[1857 AD]
3562)
(Collège de France) Paris, France  
143 YBN
[1857 AD]
3628) Suess advocates bringing in drinking water into Vienna from mountain
springs instead of using disease-filled wells. Suess develops the plan for a
69-mile (112-kilometre) aqueduct (completed in 1873) that brings fresh water
from the Alps to Vienna.

In 1876, Suess supervises the production of the Danube canal which puts an end
to the flooding of the low-lying sections of Vienna.
In 1850 Suess is imprisoned for
being on the side of the liberals during a revolution in 1848. Another source
has Suess imprisoned simply for participating in revolutionary demonstrations
of 1848.
In 1856, Suess is appointed extraordinary professor of paleontology at the
University of Vienna without a doctorate degree.
From 1873 on, Suess spends 30
years in the Austrian legislature.
(University of Vienna) Vienna, Austria (now Germany)  
143 YBN
[1857 AD]
3640) Maxwell's parents married late in life, and his mother is 40 years old at
his birth.
James's unusual mode of dress is how he got the nickname "Dafty" at
Edinburgh Academy, where he enrolled in 1841.
Asimov explains this nickname as being
because talent, for example in math, is some times mistaken for foolishness.
At age 15,
Maxwell submits a paper on curves to the Royal Society of Edinburgh.
In 1871
Maxwell is appointed professor of experimental physics at Cambridge.
According to Asimov,
Maxwell is not a popular lecturer.
Maxwell organizes the Cavendish laboratory
and serves as its director it until his death.
The Encyclopedia Britannica states that
(as director of Cavendish laboratory), Maxwell has few students, but that they
are of the highest quality.
Like Faraday, Maxwell has deep religious beliefs, and has a
childless but happy marriage.
In 1876, Maxwell writes a classic elementary text
in dynamics, "Matter and Motion" (1876).
Maxell and Thomas Huxley are joint scientific
editors of the ninth edition of the Encyclopedia Britannica.
Maxwell publishes
the "Unpublished Electrical Researches of the Hon. Henry Cavendish" (1879).
According to Asimov this work shows that Cavendish was 50 years ahead of his
time.
Maxwell rejects the particle theory for electricity, although Faraday's laws of
electrolysis strongly suggest the particulate nature of electricity (and this
is true also for light, Maxwell viewing light as waves of electromagnetic
radiation carried by the ether).

Maxwell is one of the first to appreciate the work of Gibbs.

Maxwell dies before the age of 50 from cancer.

Over the course of his life, Maxwell wrote four books and about 100 papers.
(Marischal College) Aberdeen, Scotland  
143 YBN
[1857 AD]
3670)
(Ximenian Institute)Florence, Italy  
143 YBN
[1857 AD]
3791)
(Conservatoire des Arts et Métiers) Paris, France  
142 YBN
[01/06/1858 AD]
2881) Gassiot describes his experiments in a January 6, 1858 paper "On the
Stratifications and Dark Band in Electrical Discharges as observed in
Toricellian Vacua.". (I think "stratifications" can be interpreted as
"stripes".) Gassiot writes:
"The striated condition of the electrical discharge in
vacuo that takes place when the terminal wires of Ruhmkorff's inductive coil
are inserted into a well-exhausted receiver, in which a small piece of
phosphorus has been previously placed, was first announced by Mr. Grove in his
communication to the Royal Society, 7th January, 1852; ...
I had, at the time,
the pleasure of witnessing many of these experiments, which are now so well
known to electricians; shortly afterwards I examined the discharge in a
Torricellian vacuum: my apparatus consisted of a glass cylinder 6 inches long,
in which two platinum wires are hermetically sealed about 4 inches apart; the
cylinder forms the upper portion of a barometer, the lower part being made of
the usual sized tubing; the mercury, when at the height of 30 inches, reaches
to within about 6 inches of the cylinder; the mercury was carefully boiled in
the usual manner by M. Negretti, and the apparatus fixed in my laboratory ...
When
the discharge is made with a Ruhmkorff's coil, by connecting the above platinum
wires with the terminals of that apparatus, the cylinder is brilliantly
illuminated with a dense white phosphorescent light, filling the entire vacuum,
the intensity of the light depending on the energy of the battery. The mercury
sinks at each discharge, but not the slightest trace of any transverse bands
can be detected.
The phenomenon of stratifications in the discharge in vacuo were
subsequently observed in Paris by M. Ruhmkorff, who obtained the effect by
using the vapour of alcohol; they were again noticed by Masson, Du Moncel,
Quet, and other continental electricians, who all describe the intense white
light without stratification
produced in the barometrical vacuum.
The Rev. Dr.
Robinson, who has made a series of beautiful experiments with the inductive
coil, says, "Nothing satisfactory has yet been ascertained as to the cause of
the stratification of light. Mr. Grove appears to think that it arises from
some vibration in the metal of the contact breaker, which produces a
fluctuation in the inducing current;...
(Is this due to the alternating current of the
induction coil?)
...
(see figure)
While pursuing my experiments, it occurred to me that an apparatus similar
in some respects to that used by Davy, could without much difficulty be
constructed, which would enable me not only to make experiments in a
Torricellian vacuum, but also with great facility in any gas which does not act
on mercury Plat I. fig. 1 represents this apparatus. In the glass tube, two
platinum wires, a and b, are carefully sealed about 6 inches apart; the tube is
filled with pure mercury. A stopcock, fixed at C, can, by means of a flexible
tube, be connected with an air-pump. When the air is extracted from the ball of
the apparatus, the mercury sinks in the tube, and in this manner the
Torricellian vacuum is formed, the mercury in the tube descending to "d."
...
...the discharge from the coil, when excited by a single cell of Grove's
battery, the upper wire being negative, consisted of eight or ten distinct
stratifications, extending from the positive wire to the dark space, while the
usual blue flame surrounding the intense red, which has the appearance of red
heat, is visible on the negative wire. (The blue flame are actually photons
emitting from charged particles? I don't think this flame must appear like an
ordinary flame from gas or a match.) On reversing the direction of the primary
current by the commutator, the stratifications appear from the upper wire,
while the lower, which is now negative, has the blue and red glow; but in this
case there is aphosphorescent light from the surface of the mercury at d to the
lower wire.
...
In some experiments which I made as far back as October 1854, I noticed a
deposit when the discharge was made from platinum wires sealed in a glass
globe, exhausted by means of the air-pump. I showed the globe to Dr. Faraday,
who kindly tested and examined the deposit, and found it to be finely divided
platinum in the metallic state. (how tested?)...
...it appeared surprising that there
should be so marked a difference in the discharge when, as in some instances,
so very minute a quantity of air (less than 1/6000th of the contents of the
tube) was present.
Mr. Casella, who had made all the glass apparatus already described
(with the exception of the barometer), placed one of his most intelligent
workmen at my disposal;...
Each of these tubes was filled with pure mercury, carefully
boiled; a tube about 34 inches in length being attached to each, also filled
with mercury; the apparatus was inverted into a basin of mercury, thereby
forming the usual barometrical vacuum, and the tubes were then sealed about 4
inches below the lower platinum wire.
...the platinum coating is deposited on the
portion of the tube surrounding the negative wire, but none at or near the
positive.
....
The stratifications are very powerfully affected by a magnet. When the
discharge is made from wire to wire. Plat I. figs 1,2,3 or 7, if a horseshoe
magnet is passed along the tube so as alternately to present the poles to
different contiguous positions of the discharge, it will assume the form of ~
in consequence of its tendency to rotate round the poles in opposite
directions, as the magnet in this position is moved up and down the side of the
tube.
The effect is still more striking if the straight bar of a powerful
electro-magnet is placed close to the ends of the stratifications; they then
tend to rotate in one direction round the north, and in another round the south
pole of the magnet.
When the discharge was first made in the pear-shaped apparatus,
fig. 5 (24.), the mercury being negative and about 2 inches from the end of the
positive wire, the discharge formed nearly a straight line; in this position,
when the pole of a powerful electro-magnet was placed close to the glass vessel
of the apparatus, the discharge was deflected across the pole at right angles,
the discharge being from the positive wire to the negative mercury; if the
magnet presented a northern polarity, the discharge deflected to the right,
when looking from the magnet to the discharge, carrying with it the red spot in
a direct line across the mercury.
...
In this experiment I noticed another effect which I have not seen in any of my
other apparatus. The magnet so divided the electrical discharge, that the rays
producing the fluorescence in the glass tube were all accumulated in the
neighbourhood of the negative terminal, the glass in that part being highly
fluorescent, while the positive portion exhibited little or no signs of this
phenomenon.
I refrain for the present from offering any observations as to the action of
the magnet on the discharge. The intimate relation of magnetic and electric
action has long since been shown; but the curious effect of the power of a
magnet to draw out the stratification from the positive terminal, and in some
instances its powerful action on that portion of the discharge which exhibited
the phosphorescent light in its greatest intensity, are worthy of further
examination."
London, England (presumably)  
142 YBN
[03/12/1858 AD]
3539)
(Collegio Nazionale in Alessandria) Piedmont (now part of Italy), Italy  
142 YBN
[03/15/1858 AD]
3460) After a 10 year career in business Stewart changes to a career in
science.
For this in 1868 Stewart is awarded the Rumford medal of the Royal Society.
Stewart's
textbooks and popularizations of science are widely read.
Stewart writes "The Unseen
Universe" (with Peter Tait, 1875) and many other popular accounts of scientific
discoveries of the time. "The Unseen Universe", is at first published
anonymously, and according to the 1911 Encyclopedia Britannica is intended to
combat the common notion of the incompatibility of science and religion.
(University of Edinburgh) Edinburgh, Scotland  
142 YBN
[03/16/1858 AD]
3581) Kekulé is attacted to chemistry by the teaching of Justus Liebig at the
University of Giessen.
Kekulé has a complete mastery of English and French in addition
to his native German.
In September 1860, Kekulé organizes the First International
Chemical Congress at Karlsruhe.
During Kekulé's long time at the University of Bonn
(1867-1896), he contributes to the rise of organic chemistry and the chemical
industry of Germany. Students of Kekulé come from all over Europe and then
take leading professorships and head industrial laboratories.
Kekulé is ennobled in 1895 by
Emperor William II and can then add "von Stradonitz" to his name.
(University of Heidelberg) Heidelberg, Germany  
142 YBN
[03/30/1858 AD]
2874) Plücker continues: "On discharging Ruhmkorff's apparatus through one of
the tubes before described, not only the intensity, but the colour of the light
is different in different parts of the tube. (Are these different elements?)
The eye perceives, for instance, in one part of the tube red, in another
violet, and in the middle cylinder a fainter colour; so that one would be
inclined to imagine that the ponderable matter which becomes luminous is
differently distributed through the tube. In addition to this, it happens in
many cases that the colour of the electric light undergoes a change in its
passage through the narrow tube on the excitation of the great
electro-magnet...But in all cases, whatever may be the colour-impression
produced on the eye, the distribution of the colours in the spectrum remains
for the same gas entirely of the same kind; it is the intensity of the colours
alone which changes in different degrees in different portions of the spectrum:
so that when the eye ... is at fault, still the nature of the gas or vapour
contained in the tube is unfailingly determined by means of the spectrum."
(University of Bonn) Bonn, Germany  
142 YBN
[07/01/1858 AD]
3033) Richard Owen opposes the theory of evolution by natural selection.
Darwin is gentle,
avoids conflict and spends many years trying to build up evidence before
publishing.
Thomas Huxley calls himself "Darwin's bulldog" and does much of the public
arguing for Darwin.
In Germany, Ernst Haeckel supports evolution against the
opposition of Virchow.
In America Asa Gray supports evolution against the opposition of
Agassiz.
(in France and Italy, Russia, China, India: ? It is interesting how the theory
of evolution clearly divides people into two sides. In my opinion, those who
see the truth of evolution are the smarter and more concerned with truth and
accuracy.)
In 1863 in "The Antiquity of Man", Lyell comes out strongly in favor of
evolution.
Wallace doubts that evolution can apply to humans, but Darwin
accepts this.
Wallace becomes engaged in spiritualism.
Both British prime ministers William
Gladstone and Benjamin Disraeli are both strongly opposed to evolution. (Now
politicians are not even required to express an opinion, and it is an absolute
disgrace on society. Update: recently the question of belief in evolution was
asked of a few United States presidential candidates with a few {Huckabee,
Brownback and Tancredo being examples} openly rejecting evolution.)
(Linnean Society), London, England  
142 YBN
[08/16/1858 AD]
3305)
(Newfoundland to Ireland) Atlantic Ocean  
142 YBN
[08/25/1858 AD]
2974)
(University of Bonn) Bonn, Germany  
142 YBN
[1858 AD]
2826)
(Starfield Observatory) Liverpool, England  
142 YBN
[1858 AD]
3120)
(Sorbonne) Paris, France  
142 YBN
[1858 AD]
3155) In 1851 De La Rue's attention is drawn to a daguerreotype of the moon by
G. P. Bond (or W. C.?), shown at the great exhibition of that year. De La Rue
uses the rapid wet-collodion process and succeeds in obtaining well defined
lunar pictures, which remain unsurpassed until the appearance of the Rutherfurd
photographs in 1865. De La Rue's photograph of the Moon is sharp enough to be
magnified twenty-times. (This magnification must be done with a negative raised
above a photograph exposure paper and light beamed down through the negative
onto the exposure paper.) De La Rue's stereoscopic pictures (formed by
combining two photographs) of the Sun and the Moon create a sensation at the
International Exhibition of 1862 in London.

In 1860 De la Rue took the photoheliograph to Spain for the purpose of
photographing the total solar eclipse which occurs on the 18th of July of that
year. The photographs obtained on that occasion prove beyond doubt the solar
character of the prominences or red flames, seen around the limb of the moon
during a solar eclipse. According to Asimov, this and Schwabe's finding of a
sunspot cycle initiate astrophysics, the study of the composition of the stars
and their physical processes.
(Kew Observatory) Surrey, England  
142 YBN
[1858 AD]
3161) Robert Remak (rAmoK or rAmaK?) (CE 1815-1865), German physician,
publishes the results of his study of the therapeutic effects of electric
current in "Galvanotherapie" and recommends the use of the constant current in
"morbid conditions of the brain accompanied by disordered mental functions".

(Is this the earliest use and or study of the use of electricity for human
health?)

(electricity has many important uses in health, for example, diagnostic testing
of nerves, closing blood vessels, and of course, running machines that analyze
body fluids, however, electroshock or electroconvulsive treatment is an example
of the many experimental and destructive or useless application of electricity
to health care, and reminds us that clear consent in applying health care
procedures is of primary importance in addition to carefully separating
observed clearly measurable truth from unproven highly speculative,
non-physical, or abstract theory. I think there is a fine line between
neurology the science of nerve cells and psychology the study of human behavior
and the brain {the so called "mind"}. For example, the use of electricity to
determine is a nerve cell is working is neurology, but to apply electricity
without a physical explanation is not neurology in my opinion. The most
important point is that there is consent when applying electricity to a body,
in particular a human. I think a clear line should be drawn between the science
of damaged nerve cells versus the science of diseases without any known
physical damage to nerve cells, and I define these two sciences as neurology
and psychology, although again, the most important point is making all health
care whether neurology, psychology or any other ology consensual only as
defined by the Nuremburg laws and basic ethics and logic.)

(University of Berlin) Berlin, Germany (presumably)  
142 YBN
[1858 AD]
3164)
Paris, France  
142 YBN
[1858 AD]
3203)
(Royal College of Chemistry) London, England  
142 YBN
[1858 AD]
3205) Donders uses his own money to establish the polyclinic in Utrecht which
becomes a center for both research and teaching.
(University of Utrecht) Utrecht, Netherlands  
142 YBN
[1858 AD]
3211)
(Collegio Romano) Rome, Italy  
142 YBN
[1858 AD]
3288)
Paris, France (presumably)  
142 YBN
[1858 AD]
3358)
(University of Bonn) Bonn, Germany  
142 YBN
[1858 AD]
3359)
(University of Bonn) Bonn, Germany  
142 YBN
[1858 AD]
3368)
(New Polytechnicum) Zurich, Germany  
142 YBN
[1858 AD]
3395) Because of the liquids in the planets, moons and Sun, in addition to the
effect of smaller masses not accounted for, I think estimating the locations of
the planets and moons will forever be like predicting the weather on planet
Earth, impossible to estimate into the far future. Even into the far future, I
think our descendants will be have to constantly update the latest positions of
the moons, planets, and all the ships in orbit of the Sun to carefully make
sure that the star system remains stable and does not collapse or become
chaotic.

EXPER: Use a computer and the simple Newtonian equation to see how closely the
Sun, planets and moons follow observations from different centuries. Can the
effect of the other planets be seen in the motion of the Sun? When every object
is moving, how can any location be fixed in the universe (in particular some
center point of 0,0,0 for any given time, presuming time to be the same value
everywhere in the universe)? Include the constant loss of mass from the Sun.
Use initial velocities. How do these initial inertial velocities change through
time? For example how is the x,y,z of a planet relative to the Sun or a central
0,0,0 point, changed in the course of a single orbit?
Paris, France  
142 YBN
[1858 AD]
3408)
(Collège de France) Paris, France (presumably)  
142 YBN
[1858 AD]
3415)
(École Normale Supérieure) Paris, France  
142 YBN
[1858 AD]
3481)
(University of Glasgow) Glasgow, Scotland  
142 YBN
[1858 AD]
3501) Huxley is the youngest of the six surviving children of schoolmaster
George Huxley and his wife, Rachel.
In 1845, Huxley discovers a new membrane, now known
as Huxley’s layer, in the human hair sheath.
Huxley teaches natural history at the
Royal School of Mines, giving very popular lectures aimed at lower income
people, and is a popularizer of science.
Huxley's strong belief in public education of
science is expressed in his famous lectures to working men, delivered from 1855
on.
In 1856, Charles Darwin and T.H. Huxley meet, become friends. The two
complement each other well, because the reclusive Darwin needs a public
defender, which Huxley is skilled with.
Huxley praises Darwin's "Origin of Species"
in a review for the London Times (the day after Christmas, 1859); in an article
for the "Westminster Review"; and in a discourse at the Royal Institution ("On
Species and Races, and their Origin").
Huxley popularizes the theory of evolution.
In 1869, Huxley's
team founds the journal "Nature".
As an example of Huxley's popularity, in 1866, as
Huxley gives a talk on blind faith as the ultimate sin, 2,000 people must be
turned away from the crowded hall.
A bequest of £1,000 from a Quaker supporter
finances Huxley’s American (US only?) tour in 1876, in which Huxley gives
talks about the dinosaur ancestry of birds and shows how the succession of
fossil horses in America is “Demonstrative Evidence of Evolution”.
Huxley serves as
president of the Geological Society (1869–71), the Ethnological Society
(1868–71), the British Association for the Advancement of Science (1870), the
Marine Biological Association (1884–90), and the Royal Society (1883–85).
Huxley's
talented daughter Marian was labeled insane after 1882 and died in Paris, under
the care of the renowned neurologist Jean-Martin Charcot, in 1887.
To fill the
demand for science teachers (driven in part by the Education Act of 1870),
Huxley teaches courses at South Kensington for schoolmasters and mistresses,
and from the good performance of the women Huxley is inspired to fight for the
admission of women to universities.
In 1880 Huxley names the class Osteichthyes which are
also called bony fish".
In 1883, a lord chief justice declares that Christianity is no
longer the law of the land in England, with the caveat that while Huxley’s
reverent questioning is now legal, vulgar working-class attacks on Christian
beliefs are still indictable.
Huxley has many nicknames including "Darwin's pit bull", "The
General", "Huxley Eikonoklastes", and "Pope Huxley".
(University of London) London, England (presumably)  
142 YBN
[1858 AD]
3555)
(Collège de France) Paris, France  
142 YBN
[1858 AD]
3557) Berthelot synthetically produces many organic (carbon) compounds such as
methyl alcohol, ethyl alcohol, methane, benzene, and acetylene.
Berthelot is
the first to synthesize organic (carbon) compounds that do not occur naturally,
by combining glycerol with fatty acids that do not naturally occur in fats.
Bert
helot builds a calorimeter to measure the heat of chemical reactions.
Berthelot defines
the terms "exothermic" for reactions that give off heat, and "endothermic" for
reactions that absorb heat.
In 1883, Berthelot publishes the results of a detailed
study on the strength of explosives in a two-volume book. (How many explosives
reactions are then known?)
(Collège de France) Paris, France  
142 YBN
[1858 AD]
3627) With Couper there is a claim of nervous breakdown possibly as result of
priority of Kekule structure priority. I reject the claims of "nervous
breakdown" as too abstract, and the stigma of psychiatric disorder is a massive
injustice directed at many lawful nonviolent people. So I think people should
require specific examples of claims of unusual behavior. Many times, the
so-called unusual behavior is not unusual, or is within the realm of creative
expression, and is completely nonviolent and legal. Perhaps a better expression
would be, was unable to contribute to science because of constant distraction,
etc, a more specific kind of claim, then labeling "nervous breakdown". Perhaps
Couper just became uninterested in chemistry or suffered from some physical
health problem.
(Wurtz's Paris laboratory) Paris, France  
142 YBN
[1858 AD]
3635) Voit is a pupil of the German chemists Justus von Liebig and Friedrich
Wöhler at the University of Munich, where Voit later is professor of
physiology (1863–1908).
In 1862 Voits begins a collaboration with the German chemist Max von
Pettenkofer that leads to productive investigations into metabolism (the
chemical processes occurring within a living cell or organism that are
necessary for the maintenance of life).
(University of Munich) Munich, Germany (presumably)  
142 YBN
[1858 AD]
3775)
(Perkin factory) Greenford Green, England  
142 YBN
[1858 AD]
6001)
(Bouffes-Parisiens theater) Paris, France  
141 YBN
[02/21/1859 AD]
3747)
(Conservatoire des Arts et Métiers) Paris, France  
141 YBN
[08/10/1859 AD]
3754) Kühne succeeds Helmholtz in the chair of physiology at Heidelberg
(1871-1899).
(University of ?) Paris, France  
141 YBN
[08/27/1859 AD]
3264)
(near) Titusville, Pennsylvania, USA  
141 YBN
[09/23/1859 AD]
3074)
Paris, France  
141 YBN
[10/20/1859 AD]
3087) Robert Bunsen (CE 1811-1899), and Gustav Kirchhoff (KRKHuF) (CE
1824-1887) understand that the spectra of light relates to and can be used to
determine the atomic (chemical) composition of a substance and develop the
technique of spectroscopy.

Bunsen (CE 1811-1899), and Kirchhoff (KRKHuF) (CE 1824-1887) build a
spectroscope and develop the technique of spectroscopy.

Bunsen and Kirchhoff (confirm clearly Fraunhofer's view that) each pure
substance has its own characteristic spectrum.

Kirchhoff supports the theory that each element emits and absorbs frequencies
of light at the same specific frequencies.

Kirchhoff recognizes that sodium and potassium exist in the sun's atmosphere,
while lithium does not or does in undetectably small quantity.

Kirchhoff recognizes that temperature of source and absorbing material makes a
difference in absorption of spectral lines.

Kirchhoff and Bunsen develop a spectroscope which allows light to pass through
a narrow slit before reaching a prism. The different wavelengths (or photon
intervals) of light are refracted differently so that numerous images of the
slit are thrown on a scale in different positions and with different colors.

In addition to yielding a unique spectrum for each element (and compound
molecules), the spectroscope has the advantage of definite identification while
only using a minimal amount of sample, on the range of nanograms to micrograms
for elements like sodium and barium respectively. Bunsen and Kirchhoff will use
this technique to quickly identify the two new elements cesium and rubidium.

The Bunsen-Kirchhoff spectroscope, a very important instrument of chemical
analysis is initially built with simple components such as a prism, cigar box,
and two ends of otherwise unusable old telescopes. The spectroscope is an
instrument which will prove to be of tremendous importance in chemical analysis
and the discovery of new elements.

The spectroscope will be used to identify five more new elements. These
included thallium (Crookes, 1861), indium (Reich and Richter, 1863), gallium
(Lecoq de Boisbaudran, 1875), scandium (Nilson, 1879) and germanium (Winkler,
1886). Bunsen's original vision of analyzing the composition of the stars is
realized in 1868 when helium is discovered in the solar spectrum. Draper and
Huggins also use the spectroscope for astronomy.

The Bunsen lamp provides a hot flame of low visible light emission in which
flame spectra can be observed against a minimum of background spectra, which
makes spectrum analysis easier.

In 1859, Bunsen suddenly stops his work with Roscoe, telling Roscoe: "At
present Kirchhoff and I are engaged in a common work which doesn't let us
sleep... Kirchhoff has made a wonderful, entirely unexpected discovery in
finding the cause of the dark lines in the solar spectrum.... thus a means has
been found to determine the composition of the sun and fixed stars with the
same accuracy as we determine sulfuric acid, chlorine, etc., with our chemical
reagents. Substances on the earth can be determined by this method just as
easily as on the sun, so that, for example, I have been able to detect lithium
in twenty grams of sea water."

This work is published as (translated from German) "On Fraunhofer's Lines"
("Uber die Fraunhofer'schen Linien,") in the "Monatsberichte der Koniglich
Preussischen Akademie der Wissenschaften zu Berlin". The two main contributions
of this paper are: 1) recognizing that the elements of any substance can be
determined from the spectrum of an object and 2) identifying elements in the
sun.

Kirchhoff makes the important observation that, to observe an absorption
feature, the source of the light has to be hotter than the absorbing flame.

Kirkkoff report this in "Uber die Fraunhofer'schen Linien" ("On Fraunhofer's
lines").


This finding initiates a new era in the method used to identify new elements.
The first fifty elements discovered, beyond those known since ancient times,
were either the products of chemical reactions or were released by
electrolysis. From 1860 on, the search is on for trace elements detectable only
with the help of specialized instruments like the spectroscope.
(University of Heidelberg), Heidelberg, Germany  
141 YBN
[11/22/1859 AD]
3035) Darwin hates public argument, and Huxley, a good friend, loves public
argument and famously argues in favor of the theory of evolution.

Huxley writes three reviews of "Origin of Species", defends human evolution at
the Oxford meeting of the British Association for the Advancement of Science in
1860 (when Bishop Samuel Wilberforce jokingly asks whether the apes are on
Huxley's grandmother's or grandfather's side), and publishes his own book on
human evolution, "Evidence as to Man's Place in Nature" (1863). Throughout
these struggles Huxley is the leading champion for evolution and for fair play
to natural selection, although Huxley never entirely accepts the theory of
natural selection, although enthusiastic for the theory of evolution, that is
descent from a common ancestor. Herbert Spencer's alternative phrase, "the
survival of the fittest", probably helps to spread a clear appreciation of
Darwin's meaning.
London, England (presumably)  
141 YBN
[11/24/1859 AD]
2928)
Mourillon, Toulon, France  
141 YBN
[12/11/1859 AD]
3456)
(University of Heidelberg), Heidelberg, Germany  
141 YBN
[1859 AD]
2823) Argelander is friends with Frederick William IV, which allows Argelander
to build a new observatory.
In 1863 Argelander founds the "Astronomische
Gesellschaft", (Astronomical Society) the first large international
organization of astronomers. The object of the society is to expand the
collaboration with many observatories.
Bonn, Germany  
141 YBN
[1859 AD]
3183)
(University of Vienna) Vienna, Austria, Germany  
141 YBN
[1859 AD]
3209)
(Collegio Romano) Rome, Italy  
141 YBN
[1859 AD]
3228)
(University of Marburg) Marburg, Germany  
141 YBN
[1859 AD]
3311)
(University of Glasgow) Glasgow, Scotland, UK  
141 YBN
[1859 AD]
3313) Tyndall is descended from William Tyndale, a 1500s translator of the
bible who was burned at the stake as a heretic in 1536.
Tyndall spends his savings on
gaining a Ph.D. from the University of Marburg, Germany (1848–50), but then
struggles to find employment.
In 1853 Tyndall is appointed professor of natural philosophy
at the Royal Institution, London, where he becomes a friend of the much-admired
Michael Faraday, gives many public lectures, and pursues science research.

Tyndall has a successful lecturing tour in America (1872-1873) and receives the
equivalent of several thousands of pounds, but places it in the hands of
trustees for the benefit of American science.

Tyndale helps to inaugurate the British scientific journal "Nature".

Tyndall's respect for Faraday is recorded in his memorial volume called
"Faraday as a Discoverer" (1868).
Suffering from sleeplessness, Tyndall is accidentally
given an overdose of chloral hydrate by his wife and dies the next day.
(Royal Institution) London, England  
141 YBN
[1859 AD]
3328) This paper is very abstract and complex. It examines conic (cones) and
spherical geometry and so appears to be an extension of the so-called
non-Euclidean surface geometry that rose up after Lobechevskii.
London, England (presumably)  
141 YBN
[1859 AD]
3373) Lenoir dies poor.
(This invention shows that a certain amount of engineering
skill, and inventive free thought exists in this time in France, also clearly
in England, Germany, Italy, Western Russia, and the USA (perhaps also China?
South America? Spain?).)
?, France  
141 YBN
[1859 AD]
3536) Carrington, like Joule is the son of a wealthy brewer.
Carrington dies of
a stroke before 50.
(Redhill Observatory) Surrey, England  
141 YBN
[1859 AD]
3543)
(U of Jena) Jena, Germany  
141 YBN
[1859 AD]
3547)
(University of Göttingen) Göttingen, Germany  
141 YBN
[1859 AD]
3714)
(Conservatory of Arts and Crafts) Paris, France  
140 YBN
[01/??/1860 AD]
3461)
(University of Heidelberg), Heidelberg, Germany  
140 YBN
[04/16/1860 AD]
3088) Cesium is a soft, silvery-white ductile metal, liquid at room
temperature, the most electropositive and alkaline of the elements, used in
photoelectric cells and to catalyze hydrogenation of some organic compounds.
Cesium has atomic number 55; atomic weight 132.905; melting point 28.5°C;
boiling point 690°C; density (specific gravity) 1.87; valence 1.

Cesium is the heaviest of the alkali metals in group 1 of the periodic table
(except for francium, the radioactive member of the alkali metal family) and is
the most reactive of the alkali metals. Cesium reacts vigorously with oxygen to
form a mixture of oxides. Cesium does not appear to react with nitrogen to form
a nitride, but does react with hydrogen at high temperatures to form a fairly
stable hydride. Cesium reacts (bonds?) with the halogens, ammonia, and carbon
monoxide. In general, cesium undergoes some of the same type of reactions with
organic compounds as do the other alkali metals (such as Lithium and Sodium),
but is much more reactive. Cesium is not very abundant in the Earth's crust,
there being only 7 parts per million (ppm) present (about half as abundant as
lead). Like lithium and rubidium, cesium is found as a component of complex
minerals and not in relatively pure halide form as are sodium and potassium.
Lithium, rubidium, and cesium frequently occur together in lepidolite ores.

Pure cesium can be prepared by electrolysis of fused cesium cyanide in an inert
atmosphere; the pure metal must be kept under an inert liquid or gas or in a
vacuum to protect it from air and water. Cesium reacts readily with oxygen; it
is sometimes used to remove traces of the gas from vacuum tubes and from light
bulbs. It reacts with ice; it reacts explosively with water to form cesium
hydroxide, the strongest base known. Cesium-137, a waste product of nuclear
reactors, is a radioactive isotope used in the treatment of cancer. Cesium is
found in the mineral pollux. Commercially useful quantities of inexpensive
cesium are now available as a byproduct of the production of lithium metal.

Cesium is first isolated by Carl Sefferburg in 1881 by electrolysis of its
salts.
(University of Heidelberg), Heidelberg, Germany  
140 YBN
[04/??/1860 AD]
3458)
(University of Heidelberg), Heidelberg, Germany  
140 YBN
[09/??/1860 AD]
3540) Also in 1860 Cannizzaro takes part in attacking Naples to make it part of
a unified Italy. This is eleven years after his failed 1847 Sicilian
revolution. This Sicilian revolt, led by Giuseppe Garibaldi, is successful and
leads to the unification of Italy under Victor Emmanuel II. Cannizzaro moves to
Rome and is made a senator. As a moderate liberal, Cannizzaro plays a role in
shaping the new constitution and establishing political reforms.
Karlsruhe, Baden  
140 YBN
[1860 AD]
2694)
Cape Town (and Simon's Town), South Africa  
140 YBN
[1860 AD]
2706) Faraday writes "The Chemical History of a Candle" and this is the first
complete book to be converted into "basic English".
"The Chemical History of a Candle",
is taken from a series of six children's lectures.

In this work Faraday describes atoms, but not light as made of corpuscles, but
simply as "light" and "heat". For example Faraday states "You see it comes to
this - that all bright flames contain these solid particles; all things that
burn and produce solid particles, either during the time they are burning, as
in the candle, or immediately after being burnt, as in the case of the
gunpowder and iron filings - all these things give us this glorious and
beautiful light." and "for what is this bright flame but the solid particles
passing off?" (Presumably Faraday is referring to atoms of carbon.) Faraday
uses the word "particles" to describe atoms and molecules.

(Royal Institution in) London, England  
140 YBN
[1860 AD]
2870) Édouard Armand Isidore Hippolyte Lartet (loRTA) (CE 1801-1871), French
paleontologist publishes "Sur l'ancienneté géologique de l'espèce humaine
dans l'Europe occidentale" (1860; "Antiquity of Man in Western Europe"). Lartet
follows this with "New Researches on the Coexistence of Man and of the Great
Fossil Mamnifers Characteristic of the Last Geological Period" (1861) in 1861.

Paris?,France  
140 YBN
[1860 AD]
2872) Gustav Theodore Fechner (FeKnR) (CE 1801-1887), German physicist
publishes "Elemente der Psychophysik" (1860, 2 vol, "Elements of
Psychophysics"). In this work Fechner develops experimental procedures for
measuring sensations in relation to the physical magnitude of stimuli and
devised an equation to express the theory of the just-noticeable difference,
advanced earlier by Ernst Heinrich Weber. This theory concerns the sensory
ability to discriminate when two stimuli (for example two weights) are just
noticeably different from each other. Later research has shown, however, that
Fechner's equation is applicable within the midrange of stimulus intensity and
then holds only approximately true.

This book claims to describe the "exact science of the functional relations, or
relations of dependency, between body and mind". Pupin's work once made public,
will show that the so-called mind, is much more like a mechanical machine which
stores and retrieves images, than many early primitive religious theories
understood.
Fechner is said to have learned Latin by age 5.

I would say my current views on psychology are:
1) Psychiatric treatments need to be
consensual only
2) People should not be locked in psychiatric hospitals without
consent
3) Consensual-only use of drugs and/or treatments is fine
4) If a person feels that
consensual drug or treatment is curing some problem, than in some sense that is
science in the form of find a solution to some perceived problem for at least
one person through consensual experimentation.
5) People should view much of psychology as
modern day snake-oil cure-all salespeople. All people are prescribed drugs, and
I doubt that most of the drugs given are helpful in solving any believed or
perceived problems.
Leipzig, Germany (presumably)  
140 YBN
[1860 AD]
2990)
London, England  
140 YBN
[1860 AD]
3045) There is a famous debate between Thomas Huxley and Samuel Wilberforce on
human evolution at the Oxford meeting of the British Association for the
Advancement of Science.

According to Isaac Asimov: the Bishop of Oxford, Samuel Wilberforce is primed
with facts by Owen, and when asked if Huxley traces his own descent from the
apes through his father or mother. Before a crowd of 700 Huxley answers that if
given the choice of an ancestor either a miserable ape or an educated man who
could introduce such a remark into a serious scientific discussion, he would
choose the ape.

Oxford, England  
140 YBN
[1860 AD]
3124)
(Ecole Polytechnique) Paris, France (presumably)  
140 YBN
[1860 AD]
3125) Butlerov studies under N.N. Zinin at Kazan university (1844-49), and
teaches there (1852-68), and at St. Petersburg University (1868-85).
Butlerov goes farther
than Kekulé, and is the first to speak of the chemical structure of a
compound. (make clearer)
Butlerov is an eager convert to the new structural theory (of
Kekulé).
Butlerov becomes interested in spiritualism, Mendeléev investigates his
suggestions, and becomes an outspoken critic of (spiritualism) but remains
friends with Butlerov. (Notice Asimov keyword "suggestions". When did people in
Russia first see eyes and hear ears?)
Butlerov creates the first Russian school of
chemists, which includes V. V. Markovnikov, A. M. Zaytsev, A. P. Popov at Kazan
and A. E. Favorski and I. L. Kondakov at St. Petersburg.
(Kazan University) Kazan, Russia  
140 YBN
[1860 AD]
3166)
Paris, France  
140 YBN
[1860 AD]
3174) From 1837 to 1849 Rutherfurd practices law.
From 1858–84 Rutherfurd is a
trustee of Columbia University. A trustee is a member of a board elected or
appointed to direct the funds and policy of an institution.
Rutherfurd gives his instruments
and collections of photographs to Columbia University.
(invented: New York City, NY, USA) (tested:) Laborador, Canada  
140 YBN
[1860 AD]
3177) Between 1854 and 1864 Donati discovers six comets, one of which, first
seen on June 2, 1858, is named after Donati.
Florence, Italy  
140 YBN
[1860 AD]
3416)
(École Normale Supérieure) Paris, France  
140 YBN
[1860 AD]
3532) Pacinotti graduates from the University of Pisa (1861) where his father
is a professor of mathematics and physics.
(University of Pisa) Pisa, Italy  
140 YBN
[1860 AD]
3573) Swan's house is the first house to be lit by electricity. (on Earth?
verify)
In 1881 The House of Commons in Great Britain is lit with Swan lamps.
In 1882 The
British Museum is lit by Swan lamps.
Newcastle, England (presumably)  
140 YBN
[1860 AD]
3642) (To me, temperature, might more accurately be stated as average velocity
of particles over a dimensional space. The quantities {variables} necessary
are: velocity, quantity of particles, mass, space, time. One possible
definition of temperature, in terms of photons {presuming constant velocity and
perfectly elastic collisions}, is defining temperature as the number of photons
moving through some photon sized-point over some period of time. Temperature
and heat would then be a measurement of rate as opposed to velocity (the rate
of accumulated constant velocity photons). But I question the theory that light
always has a constant velocity. Light particles may, perhaps as a result of
some finite distance they can get to each other - creating the maximum
acceleration possible. However, if true, then photon velocities change, but
only very close to other photons.)

(Does Maxwell claim to integrate temperature and heat? To me heat is average
velocity * quantity. Clearly there is a difference between temperature and heat
- since two objects, of different size with the same temperature on contact
with a thermometer, give different temperatures if the thermometer is 10 cm
away in a vacuum. So heat and temperature as identical or different - both
depend on a volume space which involves quantity of particles.)

(It is interesting and a key concept that Maxwell defines temperature as the
velocity of molecules (not for example how often molecules collide, since this
is viewed as perfectly elastic). I think this needs to be taken into the realm
of photons, however. Clearly photons absorbed into an atom, cause the atoms
velocity to increase {photons with infrared frequency in, for example,
sunlight, raise the temperature of mercury and other atoms more than any other
frequency}. EXPERIMENT: Are there materials which expand more with other
frequencies besides the traditional infrared?)

(There is also a major point in my mind that temperature should be defined as
average velocity of all particles, perhaps multiplied by quantity of particles
involved - and so cannot be measured accurately with mercury of other atoms,
since none absorb all frequencies of light. Measurements with mercury are only
partial estimates, and then may be inaccurate if two different objects emit the
same quantity but different frequencies of light.)

(Are all collisions elastic? Since clearly velocity is always conserved. At a
scale larger than the photonic scale, velocity of a single fast moving particle
colliding with other particles is distributed among the many other particles
{for example a drop falling into a pool of water}. The velocity appears to stop
eventually for the one particle, but this velocity is spread among the many
other particles in smaller quantity. One of the great questions in my mind, is
where the return, reverse, mirror velocity come from, when, a ball bounces off
a wall, or water rising up after a drop of water falls into it. Clearly this
reverse velocity must come from somewhere. Is it the original velocity simple
bent into a circle 180 degrees back onto itself? Or is there at some atomic or
photonic level always particles that periodically in their orbiting have an
orbit in this direction which impart this "answer" velocity back? This is
interesting to model on a computer.)

(Either photons maintain constant velocity, and 1)
in the realm of photons temperature has no meaning, since it only relates to a
larger phenomenon of atoms (or the quantity of photons in a finite volume of
space determines temperature), or 2) photons do have variable velocity and
photon velocity also determines temperature.)

(Clearly photons are needed to produce heat so in that sense the caloric theory
of heat as the product of a particle is true - but also the particle's velocity
matters - so then one issue is do photons have the same velocity or different
velocities. Another interesting issue is, how do we define the temperature of,
for example particles compressed together that have small velocities, for
example in the center of a planet or star? Only when space is opened up to them
is there a large release of photons, and therefore heat. I think, we should
then claim that the technical temperature of the inside of stars and planets is
actually cold, relative to the surface, because of pressure - only when space
is made for the particles to flow, does the temperature quickly and vastly
increase. It's an interesting issue.)


(Imagine if Jupiter was a sun that has since lost matter. It is 1000 times
smaller than the sun. How many photons are each losing per second? Then work
backwards and see how Jupiter grows. It cannot be ruled out that the oldest
sediment we see is not the sediment that originated on earth, and that perhaps
any original sediment has long since metamorphasized, presenting the
possibility that the earth may be older (and perhaps far older) than 4.6
billion years. Although it seems clear that multicellular life has only evolved
in the last billion years, and would we not see a more developed life in
ancient sediment if the earth was older? Still I don't think we can rule out
sediment older than 3.6 bya...actually I think the zircon may be evidence of a
finite age since the last molten stage of earth. The best evidence of the
matter of our star system being 4.8 billion year old is the meteorites which do
not extend in age past 5 billion. But then, clearly some matter in the universe
must be older than, for example 100 billion years old. Theoretically, the
conservation of matter requires that no matter ever disappears. Each photon may
be infinitely old, and there may be atoms which are trillions of years old -
but without any clear way of knowing. The best method of aging requires a
sample large enough to determine a ratio of some atom to a smaller atom it
decays to. This ratio is presumed to be constant throughout the sample.)
(King's College) London, England  
140 YBN
[1860 AD]
3720) Newcomb is an infant prodigy.
Newcomb rises to the rank of rear admiral in the
Navy.
Newcomb's revision of the value of the solar parallax published in 1867
remained standard until 1895, when it was superseded by his own revision.
Before and even
after the Wright brothers, Newcomb claims that the hope of heavier-than-air
machines is a vain and foolish one. (Seeing the first metal planes must have
surprised some people.)
As early as 1867 Newcomb suggests the desirability of accurately
determining the velocity of light as a method to obtain a reliable value for
the radius of the earth's orbit. In 1878 Newcomb begins the experiments, for a
while collaborating with Albert Michelson, whose later works far overshadow
Newcomb's efforts.
From 1881-1899, Newcomb annually edits "The American Ephemeris and
Nautical Almanac". An ephemeris is a table giving the coordinates of a
celestial body at a number of specific times during a given period. These
annual books report the predicted positions of sun, planets and the moon (not
other moons or stars), eclipses, and transits for various times of the year in
right ascension and declination, from the perspective of Greenwich, Washington,
geocentric and heliocentric.
Newcomb urges the use of a common system of constants and
fundamental stars by astronomers of all nations.
Newcomb is the author of over 350
scientific papers and a number of popular works on astronomy. (see for list of
works.)

Newcomb publishes a number of mathematical textbooks and several astronomical
books for a popular audience, including Popular Astronomy (1878), The Stars
(1901), Astronomy for Everybody (1902), and his autobiographical Reminiscences
of an Astronomer (1903). He also wrote a novel, His Wisdom, the Defender
(1900), and three books and a large number of articles on economics.
(Nautical Almanac Office) Cambridge, Massachusetts, USA  
140 YBN
[1860 AD]
3776)
(Perkin factory) Greenford Green, England (presumably)  
140 YBN
[1860 AD]
3894)
(Hopital de le Charite) Paris, France  
140 YBN
[1860 AD]
3900)
  
140 YBN
[1860 AD]
4545)
unknown  
140 YBN
[1860 AD]
4546)
unknown  
139 YBN
[02/25/1861 AD]
3089) Rubidium is a soft silvery-white metallic element of the alkali group
that ignites spontaneously in air and reacts violently with water. Rubidium has
atomic number 37; atomic weight 85.47; melting point 38.89°C; boiling point
688°C; specific gravity (solid) 1.532; valence 1, 2, 3, 4.

Rubidium is used in photoelectric cells and as a "getter" in electron tubes to
scavenge the traces of sealed-in gases.

Natural rubidium makes up about 0.01 percent of Earth's crust; it exists as a
mixture of two isotopes: rubidium-85 (72.15 percent) and the radioactive
rubidium-87 (27.85 percent). A large number of radioactive isotopes have been
artificially prepared, from rubidium-79 to rubidium-95.

Rubidium is so reactive with oxygen that Rubidium will ignite spontaneously in
pure oxygen. Rubidium, a metal, tarnishes very rapidly in air to form an oxide
coating, and it may ignite. The oxides formed are a mixture of Rb2O, Rb2O2, and
RbO2. Rubidium reacts with hydrogen to form a hydride which is one of the least
stable of the alkali hydrides. Rubidium does not react with nitrogen. With
bromine or chlorine, rubidium reacts vigorously with flame formation.

Rubidium is extremely reactive and forms numerous compounds, e.g., halides,
oxides, sulfates, and sulfides. Rubidium's salts color a flame red. Rubidium is
not found uncombined in nature but occurs widely distributed in lepidolite (the
major source), carnallite, pollucite, and some rare minerals, and with lithium
in seawater, brines, and natural spring waters. Although rubidium is much more
abundant in the earth's crust than chromium, copper, lithium, nickel, or zinc,
and about twice as abundant in seawater as lithium, rubidium did not become
available commercially until the early 1960s as a byproduct of the manufacture
of lithium chemicals. The metal is obtained by electrolysis or chemical
reduction of the fused chloride.
(University of Heidelberg), Heidelberg, Germany  
139 YBN
[03/??/1861 AD]
3652)
(King's College) London, England  
139 YBN
[04/26/1861 AD]
3726) On his retirement Schiaparelli studied the astronomy of the ancient
Hebrews and Babylonians and writes "L'astronomia nell'antico testamento" (1903;
Astronomy in the Old Testament, 1905).

From his observations of Mercury and Venus, Schiaparelli concludes that they
rotate on their axes at the same rate as they rotate around the Sun, so one
side always faces the Sun. This view is generally accepted until the late
1960s, when radar techniques and space probes give different values.
(chronology and work title)
(Brera Observatory) Milan, Italy  
139 YBN
[04/??/1861 AD]
3653)
(King's College) London, England  
139 YBN
[05/10/1861 AD]
3490)
(St Bartholomew's hospital) London, England (presumably)  
139 YBN
[06/??/1861 AD]
3462)
(University of Heidelberg), Heidelberg, Germany  
139 YBN
[09/??/1861 AD]
3568)
(Scientific Congress) Speyer, Germany  
139 YBN
[10/26/1861 AD]
3997) Microphone, speaker, and telephone. Sound converted to electricity and
back to sound again.
Sound can be sent farther as electric current in a wire than
mechanically in air and travels silently.

(Note that if remote neuron reading and writing is centuries old, then probably
the telephone, microphone, speaker, recording and playing back of sound
happened earlier but was kept secret from the public.)

Johann Philipp Reis (CE 1834-1874) explains the first microphone, speaker and
telephone publicly. These devices convert variations in sound (air pressure)
into variations in electric current, which can be carried over long distances
using metal wire, and then convert the electric current back into sound. The
electromagnet made possible the sending of electric current over long
distances.

Before 1840, the attempts to transmit signals over large distances were not
very successful.

The first microphone, or device that transfers variations in sound to
variations in electric current is demonstrated on October 26, 1861 by Philip
Reiss of Friedrichsdorf, Germany, although it seems very likely that the
microphone was invented earlier but like seeing eyes and thought-images kept
secret from the public for a long time.

Reis, Professor of Natural Philosophy at Friedrichsdorf, neat Frankfort,
demonstrates his apparatus in a meeting room before members of the Physical
Society. Reiss causing melodies to be sung in one part of his apparatus in the
Civic Hospital, a building about 300 feet away with doors and windows closed,
and the same sounds to be reproduced and heard in the meeting room through a
second part of his apparatus.

Reiss models his first telephone transmitter (microphone) after the human ear
(see image). Silvanus Thompson describes Reiss' ear this way:
"The end of the
aperture a was closed by a thin membrane b, in imitation of the human tympanum.
Against the centre of the tympanum rested the lower end of a little curved
lever c d, of platinum wire, which represented the " hammer " bone of the human
ear. This curved lever was attached to the membrane by a minute drop of
sealing-wax, so that it followed every motion of the same. It was pivoted near
its centre by being soldered to a short cross-wire which served as an axis;
this axis passing on either side through a hole in a bent strip of tin-plate
screwed to the back of the wooden ear. The upper end of the curved lever rested
in loose contact against the upper end g of a vertical spring, about one inch
long, also of tin-plate, bearing at its summit a slender and resilient strip of
platinum foil. An adjusting-screw, h, served to regulate the degree of contact
between the vertical spring and the curved lever. The conducting-wires by which
the current of electricity entered and left the apparatus were connected to the
screws by which the two strips of tin-plate were fixed to the ear. In order to
make sure that the current from the upper support of tin should reach the
curved lever, another strip of platinum foil was soldered on the side of the
former, and rested lightly against the end of the wire-axis, as shown in
magnified detail in Fig. 6. If now any words or sounds of any kind were uttered
in front of the ear the membrane was thereby set into vibrations, as in the
human ear. The little curved lever took up these motions precisely as the "
hammer "-bone of the human ear does; and, like the " hammer "-bone, transferred
them to that with which it was in contact. The result was that the contact of
the upper end of the lever was caused to vary. With every rarefaction of the
air the membrane moved forward and the upper end of the little lever moved
backward and pressed more firmly than before against the spring, making better
contact and allowing a stronger current to flow. At every condensation of the
air the membrane moved backwards and the upper end of the lever moved forward
so as to press less strongly than before against the spring, thereby making a
less complete contact than before, and by thus partially interrupting the
passage of the current, caused the current to flow less freely. The sound waves
which entered the ear would in this fashion throw the electric current, which
flowed through the point of variable contact, into undulations in strength. It
will be seen that this principle of causing the voice to control the strength
of the electric current by causing it to operate upon a loose or imperfect
contact, runs throughout the whole of Reis's telephonic transmitters. In later
times such pieces of mechanism for varying the strength of an electric current
have been termed current-regulators or sometimes "tension regulators" {ULSF
note: this kind of device is also called a "pressure regulator" and "pressure
relay").". Reis goes on to develop and improve a variety of different models of
telephone.

Sylanus Thompson describes Reis' first receiver (or "speaker"):
"The first form of
apparatus used by Reis for receiving the currents from the transmitter, and for
reproducing audibly that which had been spoken or sung, consisted of a steel
knitting-needle, round which was wound a spiral coil of silk- covered
copper-wire. This wire, as Reis explains in his lecture " On Telephony," was
magnetised in varying degrees by the successive currents, and when thus rapidly
magnetised and demagnetised, emitted tones depending upon the frequency,
strength, etc., of the currents which flowed round it. It was soon found that
the sounds it emitted required to be strengthened by the addition of a
sounding-box, or resonant- case. This was in the first instance attained by
placing the needle upon the sounding-board of a violin. At the first trial it
was stuck loosely into one of the /-shaped holes of the violin (see Fig. 19) :
subsequently the needle was fixed by its lower end to the bridge of the violin.
These details were furnished by Herr Peter, of Friedrichsdorf, music-teacher in
Garnier's Institute, to whom the violin belonged, and who gave Ileis, expressly
for this purpose, a violin of less value than that used by himself in his
profession. Reis, who was not himself a musician, and indeed had so little of a
musical ear as haidly to know one piece of music from another, kept this violin
for the purpose of a sounding-box. It has now passed into the possession of
Garnier's Institute. It was in this form that the instrument was shown by Reis
in October 1861 to the Physical Society of Frankfort.". Later a cigar box will
substitute for the violin, and then an electro-magnet receiver. Reis writes "
The
apparatus named the 'Telephone,' constructed by me, affords the possibility of
evoking sound- vibrations in every manner that may be desired.
Electro-magnetism affords the possibility of calling into life at any given
distance vibrations similar to the vibrations that have been produced, and in
this way to give out again in one place the tones that have been produced in
another place.". This electromagnet receiver or speaker is the basis of the
telephones of the later receivers of Yates, Asa Gray, and Alexander Bell.

Reis builds his telephone in a workshop behind his house in Friedrichsdorf and
runs a wire to a cabinet in Garnier's Institute. Reis names the instrument
"telephon".

Reiss first publishes a description of his telephone delivered verbally on
October 26 and in writing in December 1861, for the 1860-1861 Annual Report of
the Physical Society of Frankfur-am-Main, in a paper entitled (translated to
English from German) "On Telephony by the Galvanic Current". Reiss writes:
"The
surprising results in the domain of Telegraphy, have already suggested the
question whether it may not also be possible to communicate the very tones of
speech direct to a distance. Researches aiming in this direction have not,
however, up to the present time, been able to show any tolerably satisfactory
result, because the vibrations of the media through which sound is conducted,
soon fall off so greatly in their intensity that they are no longer perceptible
to our senses.
A reproduction of tones at some distance by means of the galvanic
current, has perhaps been contemplated; but at all events the practical
solution of this problem has been most doubted by exactly the very persons who
by their knowledge and resources should have been enabled to grasp the problem.
To one who is only superficially acquanted with the doctrines of Physics, the
problem, if indeed he becomes acquainted with it, appears to offer far fewer
points of difficulty because he does not foresee most of them. Thus did I, some
nine years ago (with a great penchant for what was new, but with only too
imperfect knowledge in Physics), have the boldness to wish to solve the problem
mentioned; but I was soon obliged to relinquish it, because the very first
inquiry convinced me firmly of the impossibility of the solution.
Later, after further
studies and much experience, I perceived that my first investigation had been
very crude and by no means conclusive: but I did not resume the question
seriously then, because I did not feel myself sufficiently developed to
overcome the obstacles of the path to be trodden.
Youthful impressions are, however,
strong and not easily effaced. i could not, in spite of every protest of my
reason, banish from my thoughts that first inquiry and its occasion; and so it
happened that, half without intending it, in many a leisure hour the youthful
project was taken up again, the difficulties and the means of vanquishing them
were weighed,- and yet not the first step towards an experiment taken.
How could a
single instrument reproduce, at once, the total actions of all the organs
operated in human speech ? This was ever the cardinal question. At last I came
by accident to put the question another way: How does our ear take cognizance
of the total vibrations of all the simultaneously operant organs of speech? Or,
to put it more generally: How do we perceive the vibrations of several bodies
emitting sounds simultaneously?
In order to answer this question, we will next see what must
happen in order that we may perceive a single tone.
Apart from our ear, every tone
is nothing more than the condensation and rarefactino of a body repeated
several times in a second (at least seven to eight times). If this occurs in
the same medium (the air) as that with which we are surrounded, then the
membrane of our ear will be compressed toward the drum-cavity by every
condensation, so that in the succeeding rarefaction it moves back in the
oposite direction. These vibrations occasion a lifting-up and falling-down of
the "hammer" (malleus bone) upon the "anvil" (incus bone) with the same
velocity, or, according to others, occasion an approach and a recession of the
atoms of the auditory ossicles, and give rise, therefore, to exactly the same
number of concussions in the fluid of the cochlaea, in which the auditory nerve
and its terminals are spread out. The greater the condensation of the
sound-conducting medium at any given moment, the greater will be the amplitude
of vibration of the membrane and of the "hammer," and the more powerful,
therefore, the blow on the "anvil" and the concussion of the nerves through the
intermediary action of the fluid.
The function of the organs of hearing, therefore,
is to impart faithfully to the auditory nerve, every condensation and
rarefaction occuring in the surrounding medium.The function of the auditory
nerve is to bring to our consciousness the vibrations of matter resulting at
the given time, both according to their number and their magnitude. Here, first
certain combinations acquire a distinct name: here, first the vibrations become
musical tones or discords.
...". Reiss goes on to write:
"As soon, therefore, as it shall be
possible at any place and in any prescribed manner, to set up vibrations whose
curves are like those of any given tone or combination of tones, we shall
receive the same impression as that tone or combination of tones would have
produced upon us.

{Silvanus Thompson comments: This is the fundamental principle, not only of the
telephone, but of the phonograph ; and it is wonderful with what clearness Reis
had grasped his principle in 1861.}

Taking my stand on the preceding principles, I have succeeded in constructing
an apparatus by means of which I am in a position to reproduce the tones of
divers instruments, yes, and even to a certain degree the human voice. It is
very simple, and can be clearly explained in the sequel, by aid of the figure:
{ULSF: see image, figure 25}
In a cube of wood, r s t u v w x, there is a conical
hole, a, closed at one side by the membrane b (made of the lesser intestine of
the pig), upon the middle of which a little strip of platinum is cemented as a
conductor of the current {or electrode}. This is united with the binding-screw,
p. From the binding-screw n there passes likewise a thin strip of metal over
the middle of the membrane, and terminates here in a little platinum wire which
stands at right angles to the length and breadth of the strip.

From the binding-screw, p, a conducting-wire leads through the battery to a
distant station, ends there in a spiral of copper-wire, overspun with silk,
which in turn passes into a return-wire that leads to the binding-screw, n.

The spiral at the distant station is about six inches long, consists of six
layers of thin wire, and receives into its middle as a core a knitting-needle,
which projects about two inches at each side. By the projecting ends of the
wire the spiral rests upon two bridges of a sounding-box. (This whole piece may
naturally be replaced by any apparatus by means of which one produces the
well-known "galvanic tones.")

If now tones, or combinations of tones, are produced in the neighbourhood of
the cube, so that waves of sufficient strength enter the opening a, they will
set the membrane b in vibration. At the first condensation the hammer-shaped
little wire d will be pushed back. At the succeeding rarefaction it cannot
follow the return-vibration of the membrane, and the current going through the
little strip {of platinum} remains interrupted so long as until the membrane,
driven by a new condensation, presses the little strip (coming from p) against
d once more. In this way each sound-wave effects an opening and a closing of
the current.

But at every closing of the circuit the atoms of the iron needle lying in the
distant spiral are pushed asunder from one another. (Muller-Pouillet, '
Lehrbuch der Physik,' see p. 304 of vol. ii. 5th ed.). At the interruption of
the current the atoms again attempt to regain their position of equilibrium. If
this happens then in consequence of the action and reaction of elasticity and
traction, they make a certain number of vibrations, and yield the longitudinal
tone of the needle. {Silvanus Thompson comments that at any single
demagnetisation of the needle, it vibrates and emits the same tone as if it had
been struck or mechanically caused to vibrate longitudinally} It happens thus
when the interruptions and restorations of the current are effected relatively
slowly. But if these actions follow one another more rapidly than the
oscillations due to the elasticity of the iron core, then the atoms cannot
travel their entire paths. The paths travelled over become shorter the more
rapidly the interruptions occur, and in proportion to their frequency. The iron
needle emits no longer its longitudinal tone, but a tone whose pitch
corresponds to the number of interruptions (in a given time). But this is
saying nothing less than that the needle reproduces the tone which was imparted
to the interrupting apparatus
.

Moreover, the strength of this tone is proportional to the original tone, for
the stronger this is, the greater will be the movement of the drum-skin, the
greater therefore the movement of the little hammer, the greater finally the
length of time during which the circuit remains open, and consequently the
greater, up to a certain limit, the movement of the atoms in the reproducing
wire {the knitting needle}, which we perceive as a stronger vibration, just as
we should have perceived the original wave.

Since the length of the conducting wire may be extended for this purpose, just
as far as in direct telegraphy, I give to my instrument the name "Telephon."

As to the performance attained by the Telephone, let it be remarked, that, with
its aid, I was in a position to make audible to the members of a numerous
assembly (the Physical Society of Frankfort-on-the-Main) melodies which were
sung (not very loudly) into the apparatus in another house (about three hundred
feet distant) with closed doors. Other researches show that the sounding-rod
{i.e. the knitting needle} is able to reproduce complete triad chords ("
Dreiklange ") of a piano on which the telephone {i.e. the transmitter} stands;
and that, finally, it reproduces equally well the tones of other
instruments—harmonica, clarionet, horn, organ-pipes, &c., always provided
that the tones belong to a certain range between F and f. {Silvanus Thompson
comments that this range is simply due to the degree of tension of the tympanum
; another tympanum differently stretched, or of different proportions, would
have a different range according to circumstances}

It is, of course, understood that in all researches it was sufficiently
ascertained that the direct conduction of the sound did not come into play.
This point may be controlled very simply by arranging at times a good
shunt-circuit directly across the spiral {i.e. to cut the receiving instrument
out of circuit by providing another path for the currents of electricity},
whereby naturally the operation of the latter momentarily ceases.

Until now it has not been possible to reproduce the tones of human speech with
a distinctness to satisfy everybody. The consonants are for the most part
tolerably distinctly reproduced, but the vowels not yet in an equal degree. Why
this is so I will endeavour to explain.
..." Reiss then concludes:
"...
Whether my views with respect to the curves representing combinations of tones
are correct, may perhaps be determined by aid of the new phonautograph
described by Duhamel. (See Vierordt's ' Physiology,' p. 254.)

There may probably remain much more yet to be done for the utilisation of the
telephone in practice (zur praktischen Verwerthung des Telephons). For physics,
however, it has already sufficient interest in that it has opened out a new
field of labour."
Note that there is some confusion about whether Leon Scott was the
first to record to a cylinder, or Duhamel' with the "Vibrograph". Wilhelm Weber
recorded the sound vibrations of a tuning fork onto a sooted glass plate in
1830. There is a claim that Duhamel was the first to record sound to a sooted
glass cylinder in 1840. It seems clear that Reiss may be referring to Duhamel
to take pressure off of himself for talking about what might be technology
classified as secret by the government military by referring to Duhamel - it
seems clear from the words of Silvanus Thompson that Reiss was murdered by
galvanization at the age of 40. Perhaps Reiss is hinting about the possibility
of recording the sounds for permenant storage.
(see for full translation in
English) (The use of "suggested" in the first sentence and "opened out" in the
last sentence indicate that Reiss clearly understood in 1860 about the secret
of remote muscle movement suggested images and sounds and the massive aparteid
of insiders and outsiders, or included and excluded. Was Reiss an insider or
outsider? Most insiders are not complete insiders, and certainly must be
excluded from seeing many important recordings.)

In 1862, Reis sends Professor Poggendorff a paper on the telephone for the
Annalen Der Physiks and Poggendorff rejects the paper. before this in 1859,
Reis sent a paper to Poggendorff entitled "On the Radiation of Electricity"
which is now lost.

Edison admits in court that he started his investigation into the carbon
telephone by having a translation of Legat's report on Reis' telephone.
Alexander Graham Bell also refers to Reis in his "Researches in Electric
Telephony" read before the American Academy of Sciences and Arts in May 1876,
and the Society of Telegraph Engineers in November 1877, refering to the
original paper in Dingler's 'Polytechnic Journal', and to Kuhn's volume in
Karsten's 'Encyclopaedia' in which diagrams and descriptions of two forms of
Reis's telephone are given. In addition, in his British patent, Bell only
claims "improvements in electric telephony (transmitting or causing sounds for
Telegraphing Messages) and Telephonic Apparatus.".

Reis only lives to 40 years which is a very short life, Silvanus Thompson
writes that a portrait of Reis is "...modelled by the sculptor, A. C. Rumpf,
and "executed galvanoplastically" by G. v. Kress." which implies that Reis was
executed by galvanization. Possibly Reis was an excluded or outsider who
duplicated technology already discovered by insiders, and rather than include
or negotiate with Reis insiders just murdered Reis by galvanization which
stopped Reis' possible capitalization on the telephone, microphone, and/or
speaker. In this way, the insiders already in control of the distribution and
sales of microphones, and speakers could maintain their monopoly or oligopoly
which still exists to this day with the seeing of eyes and hearing of
thoughts.

Some people credit Antonio Meucci, in New York City in 1854.

It seems unusual that Reiss did not also report on the idea of adding a feature
to record sound using the telautograph, and then simply play back recorded
sounds out loud with his receiver/speaker.

Still at the time there is no known method of storing electric current for a
duration of time in wire, and the first permanent storage of electrical
information does not occur at least until Edison's tin foil phonograph. The
recording of the strength of an electronic current will be recorded on to
plastic tape by recording the varying intensity of light in 1923 by Lee De
Forest, and then magnetic tape and disk, and burned by laser into compact disks
and DVDs.
(built in workshop behind Reis's house and cabinet in Garnier's Institute,
Friedrichsdorf, demonstrated before Physical Society) Frankfort, Germany  
139 YBN
[11/07/1861 AD]
3493)
(St. Bartholomew's Hospital) London, England  
139 YBN
[1861 AD]
2651) After the Union Pacific Railroad is finished in 1869, much of the line is
relocated to run along the railroad right-of-way (the land occupied by a
railroad especially for its main line) to facilitate maintenance.
USA  
139 YBN
[1861 AD]
2927) John Ericsson (CE 1803-1889), Swedish-American inventor, builds the
"Monitor", an iron ship.
Ericsson's ironclad Monitor, with the first revolving iron
turret on a naval ship. It fought the CSS Virginia (the former USS Merrimack)
to a draw on March 9, 1862 at the Battle of Hampton Roads.
The Monitor is launched on
January 30, 1862.

Napoleon III had rejected Ericsson's model ironclad warship in 1854.
New York City, NY, USA (presumably)  
139 YBN
[1861 AD]
3015)
(Mint) London, England  
139 YBN
[1861 AD]
3193)
(University of Würzburg) Würzburg, Germany  
139 YBN
[1861 AD]
3214)
(University of Pest) Pest, (Hungary since 1873 is:)Budapest  
139 YBN
[1861 AD]
3320) Loschmidt is the son of peasants, but the village priest recognizes
Loschmidt's talent and pays for his education.
(Vienna RealSchul) Vienna, (now:) Germany  
139 YBN
[1861 AD]
3324)
(Vienna RealSchul) Vienna, (now:) Germany  
139 YBN
[1861 AD]
3417)
(École Normale Supérieure) Paris, France  
139 YBN
[1861 AD]
3486) Broca founds the anthropology laboratory at the École des Hautes
Études, Paris (1858), and the Société d’Anthropologie de Paris (1859), and
then later in life the Revue d’anthropologie (1872), and establishes the
École d’Anthropologie, Paris (1876), becomes its director.

Broca is the first to trepan to treat an abscess (is?) on the brain.
Trepanation is drilling a hole in the skull and is the oldest surgical
procedure known to humans; skulls of Cro-Magnon people estimated to be 40,000
years old have been discovered with circular holes as large as 2 inches in
diameter.

In 1856 when an old skull is unearthed in Neanderthal (a valley near
Düsseldorf in the Rhineland), Huxley and Broca support the theory that the
skull of a primitive human while Virchow thinks it is a congenital skull
malformation.

Broca writes "Mémoires d’anthropologie", 5 vol. (1871–78; "Memoirs of
Anthropology"), among other works.
Much of anthropology at this time involves
skull measurements, following Retzius' distinction among races on the basis of
such measurements.

Broca considers the major human racial groups as separate species.
Broca is appointed a
member of the French senate.
(University of Paris) Paris, France (presumably)  
139 YBN
[1861 AD]
3498)
London, England (presumably)  
139 YBN
[1861 AD]
3499) In 1865 Schultze founds the journal "Archiv für mikroskopische Anatomie"
and serves as its editor until his death.
(University of Bonn) Bonn, Germany  
139 YBN
[1861 AD]
3505) Thomas Henry Huxley (CE 1825-1895), English biologist, denies that human
and ape brains differ significantly, sparking a raging dispute with Richard
Owen that brings human evolution to public attention.

(Royal School of Mines) London, England  
139 YBN
[1861 AD]
3511)
Heidelberg, Germany (presumably)  
139 YBN
[1861 AD]
3541)
(U of Jena) Jena, Germany  
139 YBN
[1861 AD]
3582)
(University of Ghent) Ghent, Belgium  
139 YBN
[1861 AD]
3636)
(University of Munich) Munich, Germany  
139 YBN
[1861 AD]
3645)
(King's College, exhibit at the Royal Institution) London, England  
139 YBN
[1861 AD]
3672) Former KGB agent Alexander Litvinenko was poisoned with thallium in
London. Thallium is frequently referred to as the poison of choice: Only a gram
of the colorless, odorless, water-soluble heavy metal can kill. It is as toxic
as arsenic, and even more so than lead.
(private lab) London, England (presumably)  
139 YBN
[1861 AD]
3779) Solvay invents a system of economy that replaces money with a complex
credit system, which gains the name "technocracy".
(Solvay factory) Charleroi, Belgium  
139 YBN
[1861 AD]
4547)
unknown  
138 YBN
[01/27/1862 AD]
3369) Rudolf Julius Emmanuel Clausius (KLoUZEUS) (CE 1822-1888), German
physicist, publishes his "sixth memoir" on the mechanical theory of heat,
(translated from German) "On the Application of the Theorem of the Equivalence
of Transformations to Interior Work" (1862), in which Clausius concludes that
it is "impossible practically to arrive at the absolute zero of temperature by
any alteration of the condition of a body.". (This is somewhat abstract. In
addition, volume plays an important role in temperature and/or motion
measurement. Absolute zero could be any space free of photons, for example. It
may be possible that theoretically photons packed together in a way unable to
move, in some dense object might be the equivalent of absolute zero over some
volume of space, however, this {no space for photons to move, even in the
densest star or galaxy} is an unlikely phenomenon.)

(New Polytechnicum) Zurich, Germany  
138 YBN
[01/31/1862 AD]
3685) Among lenses made under Clark's direction are the 26-in. lens at the U.S.
Naval Observatory, Washington, D.C.; the 36-in. lens at Lick Observatory,
California; and the 40-in. lens at Yerkes Observatory, Wisconsin, which is the
largest refracting telescope in the world. (still true?)

Over the course of his life Clark will discover 16 double stars.
Clark's father is a
lens grinder who owns an optical shop and Clark also follows in this profession
making telescopes recognized around the planet. The Clarks make some of the
best telescopes of the late 1800s.
Cambridgeport, Massachusetts, USA  
138 YBN
[01/??/1862 AD]
3654)
(King's College) London, England  
138 YBN
[02/??/1862 AD]
3655)
(King's College) London, England  
138 YBN
[02/??/1862 AD]
3743)
(University of Berlin?) Berlin, Germany  
138 YBN
[07/19/1862 AD]
3242) I think this debate about the nature of temperature is interesting. Is
temperature only a measure of mass density per unit space? or is it only
velocity of mass per unit space with no regard to mass quantity? Or is
temperature dependent on both quantity of mass and velocity of mass? It would
seem if higher density = higher temperature, a solid would have a higher
temperature than a liquid or gas, but perhaps the measuring device does not
intercept the moving particles in a solid. In the center of a dense object like
the Sun, perhaps the particles move less or not at all, so is the temperature
colder? Heat depends to some extent on photons absorbed by atoms, so does
temperature relate to velocity of photons absorbed or quantity of photons
absorbed or both or neither? Is a volume of space with no matter required for a
temperature of absolute 0 over that volume or can photons or other matter be
present?

(I think that the lowering of temperature may be from the simple fact that the
molecules are farther apart, and therefore colliding less...perhaps even
distance between molecules/atoms is temperature, I doubt that because then
dense solids would be hotter, etc. It's less average velocity according to
Maxwell. Could be quantity of collisions, but that is doubtful. But clearly
heating water for example, involves more movement/collisions of the molecules.
I think the losing energy because of overcoming a gravitational? or some other
attraction theory is abstract, and needs to be explained in terms of electron
orbits being closer, etc. )
(the more photons per volume the higher the
temperature I think, although it all depends on the detection thermometer
location – how many photons are absorbed by the mercury atoms. In addition
temperature is difficult to measure, and is measured only in the space of the
mercury. How measured? If photons are in a frequency reflected or not absorbed
by the mercury, they are not included in measurement of temperature – if all
were absorbed, temperature would be the equivalent measure of number of
absorbed photons-if all have same velocity, and a measure of average velocity
of absorbed photons-if different velocities)

I think the key to temperature (and heat) is how temperature is measured. For
example, if measured by the size of the volume occupied by mercury or some
other liquid, the mercury absorbing free photons increases the temperature. if
measured by heat detectors in skin, again the principle of how many free
photons are absorbed by molecules in the detector are how heat is measured. How
are very low temperatures measured?
Salford, England (presumably- verify)  
138 YBN
[09/22/1862 AD]
3287)
Paris, France (presumably)  
138 YBN
[11/04/1862 AD]
3219) Philip Van Doren Stern writes that "the definitive work on the subject is
'The Machine Gun', a four-volume work prepared for the (US) Navy Bureau of
Ordnance by Lieutenant Colonel George M. Chinn, lately of the Marine Corps.
(Volumes two and three of this work are classified and not available to the
public)."

A breech-loading weapon is a firearm (a rifle, a gun etc.) in which the bullet
or shell is inserted or loaded at the rear of the barrel, or breech; the
opposite of muzzle-loading. Modern mass produced firearms are breech-loading
(though mortars are generally all muzzle-loaded). Early firearms were almost
entirely muzzle-loading.

The principle of a rapid fire gun is simple, since the powder is in the bullet
casing, all that needs to be automated is loading, igniting (hammering) the
powder, and unloading the empty casing. It would seem faster and less work to
rotate the loading and igniting unit instead of the barrels. Parallellisation
(of gun barrels) speeds the firing process. Perhaps multiple barrels could be
loaded, fired and cleared at the same time increasing the quantity of
projectiles. All moving parts can be made automated electronically. For example
electric motors now turn the barrels of modern Gatling-style machine guns on
airplanes.

In my opinion, some weapons such as explosives and rapid fire guns need to be
carefully monitored and kept from violent people. In particular those in the
United States who planned and carried out 9/11, that did 7/7 in England, the
murderers of John and Robert Kennedy, and any people involved with the murder
or assault of nonviolent people should be not allowed to use guns. Obviously,
first those people, the thousands involved in 9/11, 7/7, the Kennedy murders,
Chandra Levy, James Jay, Nicole Simpson and Ron Goldman, Bonnie Bakley,
JonBenet Ramsey...all the laser murderers...etc...the list is in the thousands,
who have not been punished for their murders of nonviolent people, need to have
their crimes shown to the public, and voted into prison first.
Indianapolis, Indiana (presumably)  
138 YBN
[12/04/1862 AD]
3175)
New York City, NY, USA (presumably)  
138 YBN
[1862 AD]
2861) Pure acetylene is a colorless gas with a pleasant odour; as prepared from
calcium carbide it usually contains traces of phosphine that cause an
unpleasant garliclike odor.
Pure acetylene under pressure in excess of about 15
pounds per square inch or in liquid or solid form explodes with extreme
violence.

Edmund Davy (cousin and lab assistant of Humprey Davy) first made acetylene in
1836 from a compound produced during the manufacture of potassium from
potassium tartrate and charcoal, which under certain conditions yielded a black
compound decomposed by water with considerable violence and the evolution of
acetylene. This compound was afterwards fully investigated by J. J. Berzelius,
who showed it to be potassium carbide. He also made the corresponding sodium
compound and showed that it evolved the same gas, whilst in 1862 F. Wohler
first made calcium carbide, and found that water decomposed it into lime and
acetylene. It was not, however, until 1892 that the almost simultaneous
discovery was made by T. L. Wilson in America and H. Moissan in France that if
lime and carbon be fused together at the temperature of the electric furnace,
the lime is reduced to calcium, which unites with the excess of carbon present
to form calcium carbide. The cheap production of this material and the easy
liberation by its aid of acetylene at once gave the gas a position of
commercial importance.
(University of Göttingen) Göttingen, Germany (presumably)  
138 YBN
[1862 AD]
2884)
(University of Bonn) Bonn, Germany  
138 YBN
[1862 AD]
3037) Charles Robert Darwin (CE 1809-1882), English naturalist, publishes "The
Various Contrivances by which British and Foreign Orchids are Fertilised by
Insects" (1862) in which Darwin shows that orchid's are not "designed" by God
but honed by selection to attract insect cross-pollinators; the petals guided
the bees to the nectaries, and pollen sacs are deposited exactly where the
pollen can be removed by a stigma of another flower.

Downe, Kent, England (presumably)  
138 YBN
[1862 AD]
3146)
(University of Uppsala) Uppsala, Sweden  
138 YBN
[1862 AD]
3165) Duchenne writes (translated from French) "Frontispiece A to this text
volume illustrates the method of electrization that I have used to obtain an
isolated contraction of the facial muscles. The electrodes, held in my right
hand, communicate with my inductior apparatus (this precise apparatus, which I
preferred for these experiments, is better represented in Plate 2b.) via some
conducting wires and are positioned to stimulate the muscles of joy, (I, Plate
1 - muscles on face). The expressive lines of joy would have appeared on the
face of the subject if I had sent current through my apparatus. But I must say
that in this case the laughter is natural! I merely wanted to show a simulation
of one of my electrophysiological experiments in this figure.
These experiments
were not as easy as one might suppose from just looking at this plate. They
required a perfect knowledge of the method, which I invented, for limiting the
electrical excitation to each individual organ.
We should recall the principles
required to perform electrization of the muscles of the face to understand
better the electrophysiological photographs that make up this Album:
(Electricity
produced by an induction apparatus is the only type applicable to this kind of
experiment; I have called it faradism, and its use faradization.)
1. The induction apparatus
must be adapted to these types of experiments. The oscillations of its current
must be rapid and regular enough to avoid the muscle trembling during
contraction; gradation of the current must be very precise and adjusted to suit
the differing excitability of each of the facial muscles.
2. The electrodes should be as
small as possible, so as not to obscure the facial features. They are covered
with a damp material and placed on the motor points. In the face, these motor
points are simplistically the points under which the motor nerves enter the
facial muscles. We see them in Plate 2a, where the motor nerve fibers of the
facial muscles have been dissected with the greatest care, and in which the
sensory nerves (from the Vth Nerve) have been cut away.".

Duchenne spends most of the book trying to equate face muscle contractions with
emotions, however, I think the real value of this work is in displaying
photographically the effects of electricity on contracting muscles on a human
body. This work is so closely related to the science of making muscles move
remotely, which has developed into a massive secret industry, the vast majority
of research being done secretly and still kept secret to this very day.

It is possible that facial expressions were sexually selected or perhaps
increased the ability to survive.
Paris, France  
138 YBN
[1862 AD]
3187)
(University of Geneva) Geneva, Switzerland  
138 YBN
[1862 AD]
3206)
(University of Utrecht) Utrecht, Netherlands  
138 YBN
[1862 AD]
3306)
(École Nationale Supérieure des Mines de Paris) Paris, France  
138 YBN
[1862 AD]
3310) Herbert Spencer (CE 1820-1903), English sociologist, is an early advocate
of the theory of evolution, and popularizes the word "evolution" and the phrase
"survival of the fittest".

Thomas Malthus (CE 1766-1834) was the first to put forward the view, in an
anonymous pamphlet in 1798, that population is limited by food supply and the
theory that feeding poor people only increases their suffering.

In 1851 Spencer published "Social Statics" (reissued in 1955), which contains
in embryo most of his later views, including his argument in favor of an
extreme form of economic and social laissez-faire (an economic doctrine that
opposes governmental regulation of or interference in commerce beyond the
minimum necessary for a free-enterprise system to operate according to its own
economic laws.).

In this year Spencer starts publishing "Synthetic Philosophy", a ten volume
work spread over many years, in which all phenomena are to be interpreted
according to the principle of evolutionary progress.

Spencer enthusiastically elaborates on Darwin's process of natural selection,
applying it to human society. Spencer states "If they are sufficiently complete
to live, they do live, and it is well they should live. If they are not
sufficiently complete to live, they die, and it is best they should die.".
Social Darwinism, or Spencerism, is a view of life which justifies opposition
to social reform on the basis that reform interfered with the operation of the
natural law of survival of the fittest.

In 1884 Spencer argues that people who are unemployable or burdens to society
should be allowed to die rather than be made objects of help and charity. This
leads to a brutal form of might-makes-right philosophy, where the winner claims
to be the fittest. (Asimov says that this philosophy is used in international
relations and as a glorification of war as a means of weeding out the "unfit").
This view justifies racist views where other races or nations can be judged as
"unfit" (and dispensed with). Spencer throws a false claim of science over
brutal practices, and this tends to discredit Darwinism among people who feel
kindness, pity and mercy to be important values. Darwin has nothing to do with
the views of Spencer. (Asimov states that evolution works over millenia, where
social evolution happens over centuries.) (I think this idea of insensitivity
to poor people suffering appeals generally to wealthy people. Clearly
evolution, natural selection is happening to humans, although perhaps people
would say that it is an unnatural selection happening as the result of who has
more money, property, etc. The key idea is that we should end involuntary
suffering, starvation, pain, etc for all living objects as best as possible. I
think ultimately smart humans will create a live that maximizes intellectual
and physical pleasure and minimizes pain for the most if not all species of
Earth.)

Brighton?, England  
138 YBN
[1862 AD]
3375)
Paris, France (presumably)  
138 YBN
[1862 AD]
3517) In 1877, Hoppe-Seyler founds and edits the first journal dedicated to
biochemistry, "Zeitschrift für Physiologische Chemie".
Hoppe-Seyler's student
Miescher identifies the nucleic acids.
(University of Tübingen) Tübingen, Germany  
138 YBN
[1862 AD]
3521)
(University of Tübingen) Tübingen, Germany  
138 YBN
[1862 AD]
3556)
(Ecole Superieure de Pharmacie) Paris, France  
138 YBN
[1862 AD]
3559) Pierre Eugène Marcellin Berthelot (BARTulO or BRTulO) (CE 1827-1907),
French chemist, with Péan de Saint Gilles, Berthellot produces an equation for
the reaction velocity (1862). This is incorrect but inspires Cato Guldberg and
Peter Waage to enunciate the law of mass action (1864).

(Ecole Superieure de Pharmacie) Paris, France  
138 YBN
[1862 AD]
3574)
Newcastle, England (presumably)  
138 YBN
[1862 AD]
3664)
Ecole des Mines, Paris, France (presumably)  
138 YBN
[1862 AD]
3686) In 1858, Wundt becomes an assistant to the physiologist Hermann von
Helmholtz.

This new course comes following the publication of his "Contributions to the
Theory of Sense Perception (1858 – 62)".
(University of Heidelberg) Heidelberg, Germany  
137 YBN
[02/07/1863 AD]
3760) In 1860, Newlands joins Garibaldi's small army which invades the Kingdom
of Naples and joins it to the Kingdom of Italy.
Newlands collected his various papers
in On the Discovery of the Periodic Law (1884).
In 1887 Newlands is awarded the Davy
medal for the paper that 25 years before he could not get published.
(Royal Agricultural Society) London, England  
137 YBN
[02/18/1863 AD]
3427) Huggins spends some time making maps of the terrestrial elements before
moving to the stars, collaborating with William Miller, professor of chemistry
at King's College, London.
In 1856, Huggins builds a private observatory at Tulse Hill,
London.
After 1875 Huggins worked mainly in collaboration with his wife, Margaret
Lindsay Huggins (CE 1848-1915).
Huggins is president of the Royal Society from 1900 to
1905.
(Tulse Hill)London, England  
137 YBN
[05/22/1863 AD]
3731) Wislicenus' father, a Lutheran pastor, is ordered arrested in 1853 for
unorthodox Bible studies, and the family fleas to the USA.
The old and conservative
Kolbe scorns Wislicenus' support for Van't Hoff's 3D method.
(Zurich University) Zurich, Switzerland  
137 YBN
[11/05/1863 AD]
3443)
(Tulse Hill)London, England  
137 YBN
[1863 AD]
2804) In 1865, after a major revision of "the Principles of Geology" Lyell
fully adopts Darwin's conclusions and adds powerful arguments of his own that
win new supporters to Darwin's theory.

Darwin explains Lyell's hesitation in accepting (the theory of natural
selection) stating: "Considering his age, his former views, and position in
society, I think his action has been heroic.".
London, England (presumably)  
137 YBN
[1863 AD]
2869)
(In a cave ) La Madelaine, Perigord, France  
137 YBN
[1863 AD]
3016)
(Mint) London, England  
137 YBN
[1863 AD]
3212)
(Collegio Romano) Rome, Italy  
137 YBN
[1863 AD]
3314) John Tyndall (CE 1820-1893), Irish physicist publishes "Heat as a Mode of
Motion" which explains the theory of heat as molecular vibration according to
the new development of Maxwell. This book goes through many editions.

(Royal Institution) London, England  
137 YBN
[1863 AD]
3351) Alexander Ellis translates this book into English.
(University of Heidelberg) Heidelberg, Germany  
137 YBN
[1863 AD]
3396) Galton is a child prodigy.
Galton is first cousin to Darwin.
The death of Galton's father
in 1844 leaves Galton with a wealthy independence, and he abandons his studying
to be a physician, to travel in Syria, Egypt, and South-West Africa.

Galton tests the efficacy of prayer by statistical methods. (This would be
interesting if Galton finds that it makes no difference, which is what I would
expect, although with the thought-cam net, many humans try to make prayers they
hear in thought come (or cam) true.) (chronology)
Galton wrote 9 books and some 200 papers
on a wide variety of topics.
Under the terms of Galton's will, a eugenics chair
is established at the University of London.
London, England (presumably)  
137 YBN
[1863 AD]
3406)
(University of Giesen) Giesen, Germany (presumably)  
137 YBN
[1863 AD]
3414)
(École Normale Supérieure) Paris, France  
137 YBN
[1863 AD]
3487)
(Freiberg University) Freiberg, Saxony, Germany  
137 YBN
[1863 AD]
3537)
(Redhill Observatory) Surrey, England  
137 YBN
[1863 AD]
3563)
(Ecole Superieure de Pharmacie) Paris, France  
137 YBN
[1863 AD]
3587) Marey writes more than 300 articles and seven books.
Paris, France (presumably)  
137 YBN
[1863 AD]
3665)
Ecole des Mines, Paris, France (presumably)  
137 YBN
[1863 AD]
3693) The father of Alfred, Immanuel Nobel had failed at various business
ventures until moving to St. Petersburg in 1837, where he succeeds as a
manufacturer of explosive mines and machine tools. Alfred's newly prosperous
parents send him to private tutors and Alfred is a competent chemist by age 16
and fluent in English, French, German, and Russian, in addition to Swedish.
Nobel's
father invents a submarine mine, which the Russian government buys in 1842.
While
visiting the USA, Nobel sees the value of explosives in developing the
undeveloped USA.
In 1862, Alfred Nobel builds a small factory to manufacture
nitroglycerin, and at the same time begins research in the hope of finding a
safe way to control nitroglycerin's detonation.

In 1864 Nobel's nitroglycerine producing factory blows up in killing his
brother. The Swedish government refuses to let Nobel rebuild his factory. Nobel
is undaunted and goes on to build several factories to manufacture
nitroglycerin for use with his blasting caps. Nobel hires a barge anchored in
the middle of Lake Mälaren to continue

Nobel will obtained a total of 355 patents.
Paris, France (guess)  
137 YBN
[1863 AD]
3734) Baeyer proposed a "strain" (Spannung) theory that helped explain why
carbon rings of five or six atoms are so much more common than carbon rings
with other numbers of atoms. (chronology)
In 1875, Baeyer succeeds Justus von Liebig as
chemistry professor at the University of Munich, where he sets up an important
chemical laboratory in which many young chemists of future prominence are
trained.
In 1881 the Royal Society of London awards Baeyer the Davy Medal for his work
with indigo.

In 1905 Baeyer wins the Nobel prize in chemistry for his work in synthetic
carbon-based chemistry, and for his synthesis of indigo.

To celebrate his seventieth birthday Baeyer's scientific papers are collected
and published in two volumes (Gesammelte Werke, Brunswick, 1905).
(University of Berlin) Berlin, Germany (presumably)  
136 YBN
[02/23/1864 AD]
3466) It is interesting that the spectra reflected off atoms and molecules is
also characteristic of them, for example the color in the visible spectrum is
different and unique for many objects. In addition, is there spectra for
electron and positron collisions? for proton and antiproton collisions? What do
those spectra look like?
(University of Bonn) Bonn (and Münster), Germany  
136 YBN
[02/??/1864 AD]
3742)
(University of Berlin?) Berlin, Germany  
136 YBN
[03/11/1864 AD]
3691) Guldberg and his brother-in-law Waage, publish these theories in a
pamphlet on this day, 03/11/1864.
Waage is deeply involved in the temperance
(prohibition of alcohol) movement.
Guldberg is the brother-in-law of Waage.
(Academy of Sciences) Cristiania (now Oslo), Norway  
136 YBN
[08/05/1864 AD]
3178)
Florence, Italy  
136 YBN
[09/08/1864 AD]
3428)
(Tulse Hill)London, England  
136 YBN
[10/27/1864 AD]
3657)
(King's College) London, England  
136 YBN
[1864 AD]
2752) Charles Babbage (CE 1792-1871), English mathematician, publishes an
autobiography "Passages from the Life of a Philosopher" (1864,London: Longman).

Cambridge, England (presumably)  
136 YBN
[1864 AD]
2994)
(Polytechnic Institute of Riga) Riga, Latvia (presumably)  
136 YBN
[1864 AD]
3207)
(University of Utrecht) Utrecht, Netherlands  
136 YBN
[1864 AD]
3277) (Sir) George Gabriel Stokes (CE 1819-1903), British mathematician and
physicist, publishes a paper on the absorption spectrum of blood.

Cambridge, England   
136 YBN
[1864 AD]
3410)
(Collège de France) Paris, France (presumably)  
136 YBN
[1864 AD]
3445) Pierre Jules César Janssen (joNSeN) (CE 1824-1907), French astronomer,
establishes that certain dark bands in the solar spectrum are of terrestrial
origin and determines that the intensity of these bands is lessened at high
elevations where the atmosphere is less dense and increased by high humidity.
(verify high humidity chronology)
In 1870, when Paris is besieged during the Franco-German
War, Janssen fleas the surrounded city in a balloon so that he can reach the
path of totality of a solar eclipse in Africa. (His effort is for nothing,
since the eclipse is obscured by clouds.)
(observed in Italy and Switzerland, probably compiled at:) Paris, France
(presumably)  
136 YBN
[1864 AD]
3492)
(Royal Institution) London, England  
136 YBN
[1864 AD]
3502)
London, England  
136 YBN
[1864 AD]
3569)
(Kazan University) Kazan, Russia  
136 YBN
[1864 AD]
3757)
(University of Berlin) Berlin, Germany  
135 YBN
[01/11/1865 AD]
3429)
(Tulse Hill)London, England  
135 YBN
[02/??/1865 AD]
3465)
(University of Uppsala) Uppsala, Sweden  
135 YBN
[04/24/1865 AD]
3370)
(New Polytechnicum) Zurich, Germany  
135 YBN
[08/12/1865 AD]
3548) Lister is the son of Joseph Jackson Lister (CE 1786-1869) who had
invented an achromatic microscope.
Lister receives his formal schooling in two Quaker
institutions, which lay far more emphasis on natural history and science than
do other schools.
In 1885 Lister succeeds Kelvin as president of the Royal Society.
(University of Glasgow) Glagow, Scotland  
135 YBN
[1865 AD]
2633) August Ferdinand Möbius (mOEBEUS) (CE 1790-1868), German mathematician,
discusses the properties of one-sided surfaces in a memoir, which includes the
"Möbius strip", a one-sided and one-edge surface created by joining the ends
of a strip of paper after giving the strip half a twist. This is the beginning
of topology, the branch of mathematics that deals with those properties of
figures that are not altered by deformations without tearing.

Möbius discovered this surface in 1858. The German mathematician Johann
Benedict Listing had discovered it a few months earlier, but Listing did not
publish his discovery until 1861.
Möbius is a descendant of Martin Luther through
his mother.
From 1813 to 1814 Möbius studies theoretical astronomy under Carl
Friedrich Gauss at the University of Göttingen.
Möbius then studies
mathematics at the University of Halle.
In 1816 Möbius obtains a position as a
professor of astronomy at Leipzig.
From 1818 to 1821 Möbius supervises the construction
of the university's observatory, and in 1848 is appointed its director.

Möbius publishes "De Computandis Occultationibus Fixarum per Planetas" (1815;
"Concerning the Calculation of the Occultations of the Planets"), "Die
Hauptsätze der Astronomie" (1836; "The Principles of Astronomy") and "Die
Elemente der Mechanik des Himmels" (1843; "The Elements of Celestial
Mechanics").

In mathematics, Möbius publishes "Der barycentrische Calkul" (1827; "The
Calculus of Centres of Gravity"), in which Möbius introduces homogeneous
coordinates (the extension of coordinates to include a "point at infinity")
into analytic geometry and also deals with geometric transformations, in
particular projective transformations. In the "Lehrbuch der Statik" (1837;
"Textbook on Statics") Möbius gives a geometric treatment of statics, a branch
of mechanics concerned with the forces acting on static bodies such as
buildings, bridges, and dams.
George Peacock PEKoK English mathematician 1791-1858 (he with Babbage, and
John Herschel use the nomenclature of Leibniz, which is better than that of
Newton (for calculus)). (A states that English math had suffered because of the
popularity of Newton). Leipzig, Germany (presumably)  
135 YBN
[1865 AD]
2991)
Berlin, Germany (possibly)  
135 YBN
[1865 AD]
2993) Toepler's influence machine consists of two disks fixed on the same shaft
and rotating in the same direction. Each disk carries two strips of tin-foil
extending nearly over a semi-circle, and there are two field plates, one behind
each disk; one of the plates is positively and the other negatively
electrified. The carriers which are touched under the influence of the positive
field plate pass on and give up a portion of their negative charge to increase
that of the negative field plate; in the same way the carriers which are
touched under the influence of the negative field plate send a part of their
charge to augment that of the positive field plate. In this apparatus one of
the charging rods communicates with one of the field plates, but the other with
the neutralizing brush opposite to the other field plate. So one of the field
plates would always remain charged when a spark is taken at the transmitting
terminals.
(Polytechnic Institute of Riga) Riga, Latvia  
135 YBN
[1865 AD]
3122) (My own opinion on vivisection is generally on the side of the rights of
those species with nervous systems to feel no pain, and to live. Currently, I
vote against jailing, fining or physically stopping those who perform useful
experiments on lower order species, however, my own opinion is against such
experiments. I think the popular opinion must create the official laws that
determine what is and what is not punished. I feel most strongly opposed to
cutting into, drugging, and/or restraining of humans, and I extend this to
primates, although I support consensual experimenting. My feelings are not
absolute, and I think I am interesting in seeing what is happening. I think
there are possibilities of my vote in favor of not punishing those who perform
experiments where there is no pain, damage, or death to any mammals other than
primates. It seems very likely that monkeys, mice, rabbits and other mammals
are currently being injected with deadly viruses, bacteria and protists, having
nerves and muscles severed, and being operated on while still alive. Some of
this experimenting results in scientific gains, and some is not worth the price
of violating the rights of a mammal, amphibian, or fish. I think the public
needs to examine their opinions and the rights of other living objects. The
extremes are, on one side, cutting into, poisoning, etc humans while still
alive for scientific gain, which I think the majority oppose and are willing to
lose any science that might be gained in the interest of human rights, on the
other extreme are those who reject any experimentation on living objects at
all, even including viruses, bacteria, protists and plants. So clearly, we as
individuals should determine where exactly our views are on this issue of
experimenting on living objects.)
(Sorbonne) Paris, France  
135 YBN
[1865 AD]
3126) (My own opinion on vivisection is generally on the side of the rights of
those species with nervous systems to feel no pain, and to live. Currently, I
vote against jailing, fining or physically stoping those who perform useful
experiments on lower order species, however, my own opinion is against such
experiments. I think the popular opinion must create the official laws that
determine what is and what is not punished. I feel most strongly opposed to
cutting into, drugging, and/or restraining of humans, and I extend this to
primates, although I support consensual experimenting. My feelings are not
absolute, and I think I am interesting in seeing what is happening. I think
there are possibilities of my vote in favor of not punishing those who perform
experiments where there is no pain, damage, or death to any mammals other than
primates. It seems very likely that monkeys, mice, rabbits and other mammals
are currently being injected with deadly viruses, bacteria and protists, having
nerves and muscles severed, and being operated on while still alive. Some of
this experimenting results in scientific gains, and some is not worth the price
of violating the rights of a mammal, amphibian, or fish. I think the public
needs to examine their opinions and the rights of other living objects. The
extremes are, on one side, cutting into, poisoning, etc humans while still
alive for scientific gain, which I think the majority oppose and are willing to
lose any science that might be gained in the interest of human rights, on the
other extreme are those who reject any experimentation on living objects at
all, even including viruses, bacteria, protists and plants. So clearly, we as
individuals should determine where exactly our views are on this issue of
experimenting on living objects.)
(Sorbonne) Paris, France  
135 YBN
[1865 AD]
3141)
London, England  
135 YBN
[1865 AD]
3403) Mendel is raised in a rural setting, having a childhood of poverty. As
the son of a peasant, Mendel tends fruit trees for the lord of a manor.
Mendel's
academic abilities are recognized by the local priest, who persuades Mendel's
parents to send him away to school at the age of 11.
Mendel takes the name "Gregor"
upon becoming a monk.
In 1850, Mendel fails an exam—introduced through new
legislation for teacher certification—and is sent to the University of Vienna
for two years. Mendel learns physics and mathematics, working under Austrian
physicist Christian Doppler and mathematical physicist Andreas von
Ettinghausen.
In 1854 mendel is employed as a teacher at the Realschule
(secondary school) in Brünn.
Mendel fails an examination 3 times and so does not
qualify to teach in more advanced schools than the Brünn Realschule.
Mendel reads "Origin
of Species" and writes notes in his copy, but he never mentions Darwin in his
paper.
In 1866 the Prussian army under Otto von Bismarck takes over Austria
(and occupies Brünn).
Mendel keeps careful records of daily weather (as Dalton had
done). (Perhaps Mendel has a systematic mind.)
Darwin dies in 1882 never knowing that
the greatest weakness in his theory has been solved.
(Natural Science Society) Brünn, Austria (now: Brno, the Czech Republic)  
135 YBN
[1865 AD]
3514)
(U of Heidelberg) Heidelberg, Germany  
135 YBN
[1865 AD]
3558) A year later, in 1866 Berthelot enunciates the theory that the production
of mineral oils may conceivably have been due to the action of water and
carbonic acid on acetylides of the alkaline metals and to the subsequent
resolutions of acetylene at a high temperature into other hydrocarbons. (Might
this be important to the evolution of fats and oils {lipids} on earth?)
(Ecole Superieure de Pharmacie) Paris, France  
135 YBN
[1865 AD]
3583)
(University of Ghent) Ghent, Belgium  
135 YBN
[1865 AD]
3637)
(University of Munich) Munich, Germany  
135 YBN
[1865 AD]
3638)
(University of Munich) Munich, Germany  
135 YBN
[1865 AD]
3689) Sachs is an assistant to the physiologist Jan Evangelista Purkinje at the
University of Prague.

Sachs is the first to teach plant physiology at a German university (Prague,
1857-1859).

Among his works are the famous (all translated from German) "Textbook of
Botany" (1868, tr. 1882); "Lectures on Physiology" (1882, tr. 1887); and
"History of Botany" (1875, tr. 1890).
(Agricultural Academy) Poppelsdorf, Germany  
135 YBN
[1865 AD]
3694)
Paris, France (guess)  
135 YBN
[1865 AD]
3702) Mendeléev is the youngest of a family of 14 to 17 children.
Mendeléev's
grandfather brought the first printing press to Siberia and published the first
newspaper.
Mendeléev studies abroad for two years at the University of
Heidelberg, financed by a government fellowship. Instead of working closely
with the prominent chemists of the university, including Robert Bunsen, Emil
Erlenmeyer, and August Kekulé, Mendeléev creates a laboratory in his own
apartment.
Another source has Mendeléev working with Bunsen before establishing his own
lab.
In 1865 Mendeléev is appointed professor of chemical technology at the
University of St. Petersburg.
Mendeléev became professor of general chemistry in 1867 and
continues to teach at the University of St. Petersberg until 1890.
According to
Isaac Asimov, as professor of chemistry at the University of Saint Petersburg
Mendeléev is the most capable and interesting lecturer in Russia.
In the 1870s the
visit of a famous medium to St. Petersburg drew him to publish a number of
harsh criticisms of "the apostles of spiritualism".
In 1876 Mendeléev divorces his wife and
marries a young art student. Another source states that Mendeleev never
divorced and was illegally married a second time.
For his work on the Periodic Law he
was awarded in 1882, at the same time as Lothar Meyer, the Davy medal of the
Royal Society.
In 1899 Mendeleev, as chief of the Chamber of Standard Weights and
Measures (verify), introduces the metric system into Russia.
Mendeléev adheres to
Gerhardt's theories and opposes Berzelius' electrical theory of the formation
of chemical compounds. As a consequence of this, Mendeléev resists Arrhenius'
electrical theory, rejecting the concept of the ion as an electrically charged
molecular fragment, and refusing to recognize the electron. In general,
Mendeléev is opposed to linking chemistry with electricity and prefers
associating chemistry with physics as the science of mass.
In "Popytka khimicheskogo
ponimania mirovogo efira" (1902; "An Attempt Towards a Chemical Conception of
the Ether"), Mendeleev explains radioactivity as movements of ether around
heavy atoms, and tries to classify ether as a chemical element above the group
of inert gases.

In 1905 Mendeleev receives the Copley medal of the Royal Society.

Mendeleev's published works include 400 books and articles, and numerous
unpublished manuscripts are kept in the Dmitry Mendeleyev Museum and Archives
at St. Petersburg State University.

Over the course of his life, five Russian universities elect Mendeleev as an
honorary member, Cambridge and Oxford designate him an honored scholar, and
numerous academies and societies elect him member. Few Russians since have been
able to match Mendeleev's worldwide recognition.
In 1955 a newly identified element, number
101 is named mendelevium.
(St. Petersburg Technological Institute) St. Petersburg, Russia
(presumably)  
135 YBN
[1865 AD]
3709)
(St. Bartholomew's Hospital) London, England  
135 YBN
[1865 AD]
3800) Kovalevski is a student of Haekel and therefore a strong evolutionist.
(St. Petersburg University) St. Petersburg, Russia  
135 YBN
[1865 AD]
3870)
(University of Bonn) Bonn, Germany  
135 YBN
[1865 AD]
4548)
unknown  
134 YBN
[01/11/1866 AD]
3431)
(Tulse Hill)London, England  
134 YBN
[02/08/1866 AD]
3921) Ludwig Edward Boltzmann (BOLTSmoN) (CE 1844-1906), Austrian physicist
reads his paper before the Academy of Vienna entitled "Ueber die mechanische
Bedeutung des zweiten Hauptsatzes der Warmetheorie". This paper opens
(translated from German):
"The identity of the First Law of Thermodynamics with
the principle of vis viva has long been known, on the other hand the Second Law
occupies a peculiarly exceptional position, and its proof is based on methods
which are not only uncertain here and there, but are in no case obvious. The
object of this paper is to furnish a purely analytical and perfectly general
proof of the Second Law of Thermodynamics, as well as to investigate the
corresponding principle in Mechanics.".

Boltzmann tries to establish a connection between the second law of
thermodynamics ("Heat cannot of itself pass from a colder to a hotter body")
and the mechanical principle of least action ("in all the changes that take
place in
the universe, the sum of the products of each body multiplied by the
distance it moves and by the speed with which it moves is the least that is
possible.").
Boltzmann is a strong supporter of atomism.
According to the Concise Dictionary of
Scientific Biography, Boltzmann engages in bitter debates with those who are
opposed to "materialist" science and prefer empirical theories to atomic models
such as Ernst Mach, Wilhelm Ostwald, Pierre Duhem and George Hehn.
Boltzmann ends his
life by hanging himself.
(University of Vienna) Vienna, Austria (now Germany)  
134 YBN
[05/17/1866 AD]
3430)
(Tulse Hill)London, England  
134 YBN
[07/??/1866 AD]
3304) In 1854, Field is one of the founders of the New York, Newfoundland and
London Telegraph Company, formed to lay a cable across the Atlantic Ocean.
In
1856, Field helps organize a British company, the Atlantic Telegraph Company.
In August
1857 the first of several unsuccessful attempts to lay a cable across the
Atlantic Ocean are made.
Five attempts were made in 1857–58 and the first message
goes the length of the cable on August 16, 1858, but the cable ceases working
three weeks later.
Field promotes other oceanic cables, notably cables from Hawaii to
Asia and Australia.
In 1877 Field resuscitates the New York City elevated train system.

Field dies poor because of shady dealings of some of his financiers.
Atlantic Ocean  
134 YBN
[09/??/1866 AD]
3570)
(Kazan University) Kazan, Russia  
134 YBN
[1866 AD]
2949)
(University of Berlin) Berlin, Germany (presumably)  
134 YBN
[1866 AD]
3007) Johann von Lamont (lomoNT) (CE 1805-1879), Scottish-German astronomer,
publishes a major catalog in six volumes (1866-74) of 34,674 small stars.

(University of Munich) Munich, Germany  
134 YBN
[1866 AD]
3140) Daubrée investigates methods of origin and formation of minerals
performing experiments on the artificial production of minerals and rocks.
(Ecole des Mines {Imperial School of Mines}) Paris, France  
134 YBN
[1866 AD]
3149)
(Indiana University) Indiana, USA  
134 YBN
[1866 AD]
3162) Wunderlich publishes this as "Das Verhalten der Eigenwärme in
Krankheiten." (Leipzig, Verlag von Otto Wigand, 1866).
(Leipzig University) Leipzig, Germany  
134 YBN
[1866 AD]
3267)
(Cambridge Observatory) Cambridge, England  
134 YBN
[1866 AD]
3357) I think it is possible that as a realist and supporter of a mechanical
interpretation (for example anti-vitalism), with this paper Helmholtz tries to
stop the growing popularity of the abstract (and inaccurate in my view)
non-Euclidean interpretation of space. However, it seems clear that Helmholtz
retreats and abandons this effort within a few years. In view of the massive
growth of a non-euclidean interpretation of the universe with the theory of
relativity, it seems a good effort. Helmholtz should have just let his single
paper stand as a historical objection and not tried to smooth over and retreat
from the argument.
(University of Heidelberg) Heidelberg, Germany  
134 YBN
[1866 AD]
3491)
(Royal Institution) London, England  
134 YBN
[1866 AD]
3496)
(Royal College) London, England  
134 YBN
[1866 AD]
3679)
(Sorbonne laboratory) Paris, France  
134 YBN
[1866 AD]
3695)
Paris, France (guess)  
134 YBN
[1866 AD]
3707) Haeckel's literary output is enormous, and at the time of the celebration
of his sixtieth birthday at Jena in 1894 Haeckel had produced 42 works with
13,000 pages, besides numerous scientific memoirs.

Building collections around his own, Haeckel founded both the Phyletic Museum
in Jena and the Ernst Haeckel Haus. The Haus contains Haeckel's books and
archives.
(Zoological Institute) Jena, Germany  
134 YBN
[1866 AD]
3728)
(Brera Observatory) Milan, Italy  
134 YBN
[1866 AD]
3736) In 1874 Lockyer is awarded the Rumsford medal.
(at home, employed at War Office) Wimbledon, England  
134 YBN
[1866 AD]
3744) Allbutt is also a health science historian. Two of his most important
publications are" Diseases of the Arteries, Including Angina Pectoris" (1915)
and "Greek Medicine in Rome" (1921). Allbutt also edits "A System of Medicine",
8 vol. (1896–99).

Allbutt is a commissioner in lunacy (from 1889 to 1892). (The word "lunacy" is
perhaps taken from the Lunar society, which if true would be evidence of an
anti-science belief, since the lunar society included some of the smartest
scientists. Perhaps there was a theory that the moon is linked to delusion or
abnormal behavior. In the 1800s, I think that persecution by religious theory
is largely replaced by persecution by psychology theory.)
(General Infirmary) Leeds, England  
134 YBN
[1866 AD]
3792)
(University of Berlin?) Berlin, Germany  
134 YBN
[1866 AD]
6013)
Vienna, Austria   
133 YBN
[12/19/1867 AD]
3439)
(Tulse Hill)London, England  
133 YBN
[1867 AD]
2821)
(Freiberg University) Freiberg, Saxony, Germany  
133 YBN
[1867 AD]
3147)
(University of Uppsala) Uppsala, Sweden  
133 YBN
[1867 AD]
3176) In 1863 Rutherfurd becomes convinced of the possibility of obtaining
better spectra by using a diffraction
grating instead of prisms. The best fine-ruled plates
existing at the time are those made by Nobertat Greifswald, and largely
employed for studying the phenomena of interference and determinations of
wave-lengths. Rutherfurd determines to prepare some glass plates of this sort
and adapt them to a spectrometer. Nobert had succeeded in ruling a few small
groups of lines on glass as tests for microscopes with about 296 lines to the
millimeter—i. e., at intervals of less than 3.4 microns—while for less
severe test-objects intervals of eighteen microns sufficed; but his method of
ruling these and the diffraction gratings is jealously guarded as a "trade
secret;" so that Rutherfurd needs to devise and test his own methods.
In 1867 Rutherfurd
constructs an elaborate ruling machine in which the plate (holding a glass to
be ruled) is moved by a screw. Rutherfurd uses wedge-shaped edged diamond
points to scratch the glass. By studying the plates, Rutherfurd can
deduce the
nature and amount of the periodic error of the screw and devises means for its
correction. Eventually Rutherfurd's grating are better than those of Nobert.
The toothed wheels for this machine Rutherfurd makes himself, on a dividing
circle more than two feet in diameter, which he buys but refits. In 1870
Rutherfurd makes a grating on glass, with 255 lines to the millimeter. In 1875,
or earlier, Rutherfurd silvers the gratings with a view to their more
convenient spectroscopic use, produces gratings measuring about 16.4
millimeters by 24.5 millimeters and with 11,161 lines at intervals of 680.4 to
the millimeter. Later still, similar gratings are made on speculum metal, in
order to avoid the great wear upon the diamond, and Mr. Chapman, his assistant,
produces a large number of these. According to a biographer B. A. Gould, with
these gratings adjusted for spectroscopic use Rutherfurd obtains, from 1867 on,
visual and photographic results for the study of both solar and stellar light,
which command universal admiration and are not equaled until those of Draper
many years later.
New York City, NY, USA  
133 YBN
[1867 AD]
3184)
(University of Leipzig) Leipzig, Germany  
133 YBN
[1867 AD]
3210)
(Collegio Romano) Rome, Italy  
133 YBN
[1867 AD]
3424)
(around London) ?, England  
133 YBN
[1867 AD]
3434)
(Collegio Romano) Rome, Italy  
133 YBN
[1867 AD]
3446)
(Possibly) Azores {archepelago in Atlantic} or Trani {Apulia, Italy}
(verify)  
133 YBN
[1867 AD]
3485)
(University of Glasgow) Glasgow, Scotland  
133 YBN
[1867 AD]
3506)
(Royal College of Surgeons) London, England  
133 YBN
[1867 AD]
3530) Gramme is an indifferent student, prefering to work with his hands.

In 1856 Gramme begins work in a Paris factory that produces devices for the
infant electrical industry.
Paris, France (presumably)  
133 YBN
[1867 AD]
6004)
Vienna, Austria (presumably)  
133 YBN
[1867 AD]
6014) Petrovich Modest Mussorgsky (CE 1839-1881), Russian composer, composes
"Night on Bald Mountain".

Saint Petersberg, (U.S.S.R. now) Russia (presumably)  
132 YBN
[03/24/1868 AD]
5834)
Newark, New Jersey, USA  
132 YBN
[04/23/1868 AD]
3435)
(Tulse Hill)London, England  
132 YBN
[06/23/1868 AD]
6252)
Milwaukee, Wisconsin, USA  
132 YBN
[07/02/1868 AD]
3432)
(Tulse Hill)London, England  
132 YBN
[07/02/1868 AD]
4020)
(Tulse Hill)London, England (presumably)  
132 YBN
[09/??/1868 AD]
3571)
(Kazan University) Kazan, Russia  
132 YBN
[10/08/1868 AD]
3922)
(University of Vienna) Vienna, Austria (now Germany)  
132 YBN
[11/23/1868 AD]
3648)
?, France  
132 YBN
[1868 AD]
2677)
New York City, New York, USA  
132 YBN
[1868 AD]
3036) Charles Robert Darwin (CE 1809-1882), English naturalist, publishes
"Variation of Animals and Plants under Domestication" (1868), in which Darwin
explores the causes of variation in domestic breeds. Darwin creates his
hypothesis of "pangenesis" to explain the discrete inheritance of traits,
imagining that each tissue of an organism throws out tiny "gemmules", which
pass to the sex organs and permit copies of themselves to be made in the next
generation. But Darwin's cousin Francis Galton fails to find these gemmules in
rabbit blood, and the theory is dismissed.

Downe, Kent, England (presumably)  
132 YBN
[1868 AD]
3080)
(University of Heidelberg) Heidelberg, Germany  
132 YBN
[1868 AD]
3418)
(École Normale Supérieure) Paris, France  
132 YBN
[1868 AD]
3447)
(?), India  
132 YBN
[1868 AD]
3495)
(Royal College) London, England  
132 YBN
[1868 AD]
3510) Erlenmeyer studies at Giessen under Justus von Liebig and at Heidelberg
under Friedrich Kekulé, both German chemists.

Erlenmeye is among the first to adopt structural formulas based on valence,
Frankland's new theory.
(Munich Polytechnic) Munich, Germany  
132 YBN
[1868 AD]
3523)
(Queen's University) Dublin, Ireland  
132 YBN
[1868 AD]
3661) James Clerk Maxwell (CE 1831-1879) publishes "On a method of making a
direct comparison of electrostatic with electromagnetic force; with a note on
the electromagnetic theory of light.".

Glenlair, England  
132 YBN
[1868 AD]
3737)
(at home, employed at War Office) West Hampstead, England  
132 YBN
[1868 AD]
3803) In 1875 Asimov claims Graebe suffers a nervous breakdown, what actually
happens is an interesting mystery. It looks like he lost all his money in the
inflation following WW I, and died penniless.
(University of Berlin) Berlin, Germany  
132 YBN
[1868 AD]
3808)
(University of Vienna) Vienna, Austria (now Germany) (presumably)  
132 YBN
[1868 AD]
3984) Westinghouse is the son of a manufacturer of agricultural implements, so
as a child Westinghouse has access to a machine shop.
At age 15, Westinghouse
designed and constructed a rotary engine.
Westinghouse serves in the union army
in the Civil War.
Westinghouse accumulates his fortune from the invention of the air
brake.
Westinghouse is a prolific inventor obtaining an average of more than a patent
a month during the 1880s.
Over 400 patents are credited to Westinghouse in his
lifetime.
Westinghouse's money is more or less destroyed in the Panic of 1907.
But I
imagine that much was restored in the years after.
Westinghouse dies in New York March
12 1914. He was president of some 30 corporations with a capital of about
$200,000,000, employing more than 50,000 persons.
(Westinghouse Air Brake Company) Pittsburg, PA, USA  
132 YBN
[1868 AD]
4049)
(University of Berlin) Berlin, Germany  
132 YBN
[1868 AD]
6005) According to Encyclopedia Britannica Brahms can be viewed as the
protagonist of the Classical tradition of Joseph Haydn, Mozart, and Beethoven
in a period when the standards of this tradition are questioned or overturned
by the Romantics, and also that in Vienna, Brahms' music suffers constant
attacks by the Wagnerites.
Vienna, Austria (presumably)  
132 YBN
[1868 AD]
6015) Edvard (Hagerup) Grieg (CE 1843-1907), Norwegian composer, composes
"Piano Concerto in A minor" (opus 16).

(Christiania now) Oslo, Norway  
131 YBN
[01/15/1869 AD]
3315)
(Royal Institution) London, England  
131 YBN
[01/30/1869 AD]
4839)
London, England (presumably)  
131 YBN
[02/12/1869 AD]
3356) There is an interesting potential similarity in a capacitor connected to
an inductor with a permanent magnet, in that, perhaps running through the
center of a permanent magnet is a capacitor where particles accumulate, and
then dissipate through the inductor channels that run around the outer layers.
it seems like there are two particle centers at each pole of a permanent
magnet, so perhaps this theory is wrong. beyond that, how does a permanent
magnet, continue to supply particles without losing them to heat as a typical
inductor-capacitor circuit eventually does? Is there some constant supply of
free electrons, like some kind of internal battery, in permanent magnets?

This is a major find, but is not listed in most major sources, is this because
of the nature of electrical oscillations relation to secret thought seeing and
spying technology or lack of science education and understanding on the part of
historians?
(University of Heidelberg) Heidelberg, Germany  
131 YBN
[02/18/1869 AD]
4050)
(University of Berlin) Berlin, Germany  
131 YBN
[03/06/1869 AD]
3703) Dmitri Ivanovich Mendeléev (meNDelAeF) (CE 1834-1907), Russian chemist
publishes his first periodic table of elements.
The problem of inaccurate atomic weights
was solved by Stanislao Cannizzaro. Attempts to organize the chemical elements
by increasing atomic weights had already been made by Alexandre Émile Béguyer
de Chancourtois and by John Alexander Reina Newlands.

Mendeléev, like Newlands and Beguyer de Chancourtois before him, starts to
arrange the elements in order of atomic weight. Immediate he finds an
interesting thing in connection with the property of valence, a concept put
forward 15 years before by Frankland. Mendeléev finds that the first row,
starting with Lithium, has a valence of 1, 2, 3, 4, 3, 2, 1 In this time, 63
elements are known. Mendeléev arranges the elements in rows so that elements
with similar valence fall into a vertical column. These elements also show
similarities in many other chemical properties (like what? appearance?
density?). Mendeléev's table differs from Newlands' table in that Newlands
tried to force all the elements into equal segments containing 6 elements each,
where Mendeléev recognizes that while the first two periods contain seven
elements, the next contain seventeen each.
Asimov writes that for the first time in
the history of science, the work of a Russian scientist is quickly recognized.

Mendeléev states the periodic law "Elements placed according to the value of
their atomic weights present a clear periodicity of properties". (Mendeléev
does not use word atomic "mass"?)
The majority of scientists do not accept Mendeléev's
periodic law; the first textbook on organic chemistry to be based on the law is
published in 1874 by Richter in St. Petersburg.

The periodic table and accompanying observations are first presented to the
Russian Chemical Society on March 6, 1869. Mendeleev's colleague Nikolai
Menshutkin presents his paper because Mendeleev is inspecting dairies in
Tversk. The paper is then published in the first volume of the new society's
journal. This paper is titled "Sootnoshenie svoistv s atomnym vesom elementov"
("The Relation of the Properties to the Atomic Weights of the Elements") in the
"Zhurnal Russkoe Fiziko-Khimicheskoe Obshchestvo" (Journal of the Russian
Chemical Society). That same year, a German abstract of the paper, consisting
of the table and eight comments, is published in "Zeitschrift für Chemie".

In the translated abstract mendeleev writes (translated from a German
translation of Russian):
"On the Relationship of the Properties of the Elements
to their Atomic Weights

By ordering the elements according to increasing atomic weight in vertical rows
so that the horizontal rows contain analogous elements, still ordered by
increasing atomic weight, one obtains the following arrangement, from which a
few general conclusions may be derived.

(see image)

1. The elements, if arranged according to their atomic weights, exhibit an
evident stepwise variation of properties.
2. Chemically analogous elements have either
similar atomic weights (Pt, Ir, Os), or weights which increase by equal
increments (K, Rb, Cs).
3. The arrangement according to atomic weight corresponds
to the valence of the element and to a certain extent the difference in
chemical behavior, for example Li, Be, B, C, N, O, F.
4. The elements
distributed most widely in nature have small atomic weights, and all such
elements are marked by the distinctness of their behavior. They are, therefore,
the representative elements; and so the lightest element H is rightly chosen as
the most representative.
5. The magnitude of the atomic weight determines the properties of
the element. Therefore, in the study of compounds, not only the quantities and
properties of the elements and their reciprocal behavior is to be taken into
consideration, but also the atomic weight of the elements. Thus the compounds
of S and Tl {sic--Te was intended}, Cl and J, display not only analogies, but
also striking differences.
6. One can predict the discovery of many new elements, for
example analogues of Si and Al with atomic weights of 65-75.
7. A few atomic
weights will probably require correction; for example Te cannot have the atomic
weight 128, but rather 123-126.
8. From the above table, some new analogies between
elements are revealed. Thus Bo (?) {sic--apparently Ur was intended} appears as
an analogue of Bo and Al, as is well known to have been long established
experimentally.".

Some historians argue that the periodic system is the result of the efforts of
six scholar with William Odling (CE 1829-1921) taking priority in publishing a
periodic table before Mendeleev.

The major drawbacks of Mendeleev's table are that it has difficulty in
accommodating the rare-earth group and that no provision is made for the
chemically inert elements, helium, neon, argon, krypton, xenon, and radon.

(It seems interesting to me that the order of element rows goes 2 8 8 18 18 32
32, which appears to have a dual nature in growing size, as opposed to a
spherical growth which would, in my view, be a linear or exponential series
such as 2 8 18 32 48 etc. Does this reflect a dual nature of the atom?)

It is surprising but I cannot find an English translation of Mendeleev's
classical 1869 paper.

(I still think there is more to understand about the atoms and the periodic
table, because why does it have a dual nature as opposed to spherical nature?
Are there two parts to every atom that must be completed before going to the
next level? Is the atom made of moving parts, statics parts, or both? Why are
zinc and cadmium a solid, but when we get to mercury it is a liquid. What is
special and different about Technetium, why is it not more like Manganese and
Rhenium (non radioactive), and why is Tc, a radioactive element, in the middle
of nonradioactive elements? Interesting that Copper and Gold are some of the
only non-gray metals, and are both in the same column, but Silver is in between
them, what explains this color difference? Why do the other elements
reflect/absorb different wavelengths of visible light?)

(It is also interesting that there are no valences higher than 7.)
(University of St. Petersburg) St. Petersburg, Russia  
131 YBN
[04/30/1869 AD]
3353) In 1870 Gustav Magnus' death leaves an opening the prestigious chair of
physics at the University of Berlin. Helmholtz and Kirchhoff are the primary
candidates, Kirchhoff is preferred but refuses the post, and Helmholtz accepts,
but Helmholtz requires $4,000 taler a year plus the construction of a new
physics institute to be under his full control, to which Prussia readily agrees
to his terms.
(University of Heidelberg) Heidelberg, Germany  
131 YBN
[06/01/1869 AD]
4006) Edison is the son of a Canadian person whose grandfather was a US Tory
who fled to Canada after the Revolutionary War. Edison's father fled back to
the USA after the Canadian rebellion of 1837.
Edison as a child asks many questions,
is reconized as unusual by neighbors, and a schoolteacher tells his mother that
he is "addled". Furious, Edison's mother takes him out of school and home
schools him, being a teacher by profession.
Edison is a fast reader, and
remembers almost everything he reads.
Edison builds himself a chemical laboratory, and
to get money for chemicals and equipment, he starts to work at the age of 12 as
a newsboy on a train between Port Huron and Detroit, in the state of Michigan.
During the stop at Detroit Edison spends his time in the library (which is
evidence of the value of libraries in contributing to science and general
education on earth).
In 1862, using his small handpress in a baggage car, Edison writes
and prints a weekly newspaper, the "Grand Trunk Herald", which is circulates to
400 railroad employees. This is the first newspaper ever to be printed on a
train.

Edison uses earnings from this paper to make a chemical laboratory in the
baggage car, but a chemical fire starts, and he and his equipment are thrown
off the train.
In 1862 Edison rescues a small boy on the train tracks, and the
grateful father, who has no money, offers to teach Edison telegraphy. As a
telegrapher Edison earns enough money to buy the writings of Faraday which
solidifies his interest in electrical technology.

In 1869 Edison goes to New York City to find employment, and while in a
broker's office waiting to be interviewed, a telegraph machine breaks down,
Edison is the only person there who can fix it, and is promptly offered a
better job than he had expected to get.
Edison sells a stock ticker he builds
for $40,000 to the president of a large Wall Street firm. (Edison wanted to ask
for $5,000 but lacked the courage, and so asked the president to make an
offer.) Edison uses this money to start a firm of consulting engineers, and for
the next six years works in Newark, New Jersey.

Edison works 24 hours a day sleeping in small naps.

From 1870 to 1875 Edison invents many telegraphic improvements: transmitters;
receivers; the duplex (transmits and receives telegraph messages on the same
wire), quadruplex, and sextuplex systems; and automatic printers and tape.

In 1876 Edison creates a laboratory in Menlo Park, New Jersey, 12 miles south
of Newark, the first industrial research laboratory on earth. This lab will be
an invention factory, and Edison eventually has as many as 80 scientists
working for him.

Around 1900 Edison loses all his money in an effort to develop a new method of
dealing with iron ore. (need more info)

When eight thousands attempts to create a new storage battery fail, Edison
famously states "Well, at least we know eight thousands things that don't
work.".

During World War I Edison heads the U.S. Navy Consulting Board and contributes
45 inventions, including substitutes for previously imported chemicals
(especially carbolic acid, or phenol), defensive instruments against U-boats, a
ship-telephone system, an underwater searchlight, smoke screen machines,
antitorpedo nets, turbine projectile heads, collision mats, navigating
equipment, and methods of aiming and firing naval guns. After the war Edison
establishes the Naval Research Laboratory, the only American institution for
organized weapons research until World War II. It seems very likely that Edison
provided other secret products and services to the US military, perhaps like
seeing eye images, thought-sound recordings, remote muscle
movements/galvanizations - remote neuron activation, perhaps wireless
videophone services...and similar secret inventions. Those people interested in
researching secret technologies such as seeing and hearing thought, and sending
images and sounds directly to brains and remote muscle movements should closely
examine all available literature on and about Thomas Edison - in particular
Nature, and other science journal articles on Edison. Clearly Edison must have
been linked and involved in these industries - although it is clear that they
have their origin in England, France, Germany and Italy.

Edison is famous for saying: "Genius is one percent inspiration and 99 percent
perspiration", which expresses skepticism about the power of inspiration.

Edison rejects religion stating: "So far as religion of the day is concerned,
it is a damned fake... Religion is all bunk." and rejects the inaccurate belief
in a "soul" stating: "My mind is incapable of conceiving such a thing as a
soul. I may be in error, and man may have a soul; but I simply do not believe
it.".

Before he dies Edison has patents on 1,300 inventions, more than any other
inventor.

Edison is called the Wizard of Menlo Park.

Asimov describes Edison as the greatest inventor since Archimedes and possibly
of all time. (Although, there remains the secret inventions of seeing eyes and
thought which may be William Wollaston, hearing thought and sounds heard by the
brain, and remote neuron activation, among other potential secret inventions
and inventors.)


(Edison is a fine example of how a poor person can earn money through science,
in particular by using engineering skills to construct devices that make life
better and more convenient for many people - with thoughts of what the future
will look like - and trying to capitalize on those future conveniences.)
(private lab) Menlo Park, New Jersey, USA  
131 YBN
[09/01/1869 AD]
3785) Cleveland Abbe (aBE) (CE 1838-1916), US meteorologist begins sending
daily weather bulletins, taking advantage of telegraphic reports of storms (as
Henry at the Smithsonian Institute had done).

Cincinnati, Ohio, USA  
131 YBN
[12/??/1869 AD]
3626) In 1882, with Mendeleev, Meyer receives the Davy medal for his work in
the development of the periodic law.
(Karlsruhe Poltechnic Institute) Karlsruhe, Baden  
131 YBN
[1869 AD]
2685)
Yokohama, Japan  
131 YBN
[1869 AD]
2997)
Berlin, Germany (possibly)  
131 YBN
[1869 AD]
3127)
(Queen's College) Belfast, Ireland  
131 YBN
[1869 AD]
3316) John Tyndall (CE 1820-1893), Irish physicist is accused of materialism
and atheism after his presidential address at the 1874 meeting of the British
Association for the Advancement of Science in Belfast, when he claims that
cosmological theory belongs to science rather than theology and that matter has
the power within itself to produce life. Although Tyndale is not so prominent
as Huxley in detailed controversy over theological problems, Tyndale plays an
important part in educating the public mind about natural philosophy, dogma and
religious authority.

(Royal Institution) London, England  
131 YBN
[1869 AD]
3397) Galton tries to map the distribution of good looks in England.
(chronology)

Galton, like Darwin wrongly thinks that characteristics of individuals of two
different types will blend, and the offspring will be in an intermediate state.
Mendel will show this to be not true (that specific traits are inherited?
Clearly skin color appears to sometimes blend the quantity of melanin.).
London, England (presumably)  
131 YBN
[1869 AD]
3470)
(University of Bonn) Bonn, Germany (presumably)  
131 YBN
[1869 AD]
3494)
(at home, employed at War Office) West Hampstead, England  
131 YBN
[1869 AD]
3503)
London, England  
131 YBN
[1869 AD]
3504)
(University of London) London, England (presumably)  
131 YBN
[1869 AD]
3531)
Paris, France (presumably)  
131 YBN
[1869 AD]
3718) Young is the first to photograph the sun's corona.
Young write some of the most
popular and useful general astronomy textbooks of this period.
(Dartmouth College) Hanover, New Hampshire, USA  
131 YBN
[1869 AD]
3761) In 1914 Hyatt wins the Perkin medal for celluloid.
Hyatt owns a factory that makes
checkers and dominos.
Albany, NY, USA  
131 YBN
[1869 AD]
3763) Markovnikov is an assistant to Butlerov at Kazan University.
From 1873 on Markovnikov
is at the University of Moscow, where he establishes a new chemistry laboratory
and trains a generation of chemists.
(Kazan University) Kazan, Russia  
131 YBN
[1869 AD]
3804)
(University of Berlin) Berlin, Germany  
131 YBN
[1869 AD]
3927) Miescher is from a distinguished scientific family from Basel in
Switzerland: both his father and uncle, held the chair of anatomy at the
University of Basel.

Miescher dies at age 51 of Tuberculosis.
(University of Tübingen) Tübingen, Germany  
131 YBN
[1869 AD]
6008)
Moscow, (U.S.S.R. now) Russia  
130 YBN
[04/28/1870 AD]
3766) In 1875, Hitzig is named professor at the University of Zurich, and
director of the Bergholzli mental asylum there.
(University of Berlin?) Berlin, Germany  
130 YBN
[08/28/1870 AD]
5997)
Munich, Germany  
130 YBN
[10/05/1870 AD]
3951)
  
130 YBN
[12/30/1870 AD]
3835) Strutt studies sound, water and earthquake waves.

In his first paper, published in 1869, Strutt gives a clear demonstration of
some aspects of the electromagnetic theory of James Clerk Maxwell, in terms of
analogies that the average person could understand. This paper is "On some
Electromagnetic Phenomena considered in connexion with the Dynamical Theory".

In 1877, Strutt publishes the first volume of "The Theory of Sound" (2vol,
1877-8), in which he examines vibrations and the resonance of elastic solids
and gases.

As second Cavendish professor of experimental physics at Cambridge (1879–84),
after James Clerk Maxwell, Rayleigh supervises the precise determination of
electrical standards. Rayleigh helps to establish accurate determination of
absolute units in electricity and magnetism, Rowland in the USA also
contributing. Rayleigh leads a program to redetermine the three electrical
constants, the ohm, the ampere, and the volt which is completed in 1884.

In 1884, Rayleigh performs experiments on the rotation of the plane of
polarized light first found by Faraday.

In 1891 Rayleigh succeeded John Tyndall as professor of physics at the Royal
Institution in London.

In 1904 Strutt wins the Nobel prize in physics, and Ramsay in chemistry. Strutt
donates the money from the award to Cambridge.

In 1905 Strutt is the president of the Royal Society.

In 1908 Strutt is the chancellor of Cambridge University.

Like William James and Oliver Lodge, Strutt grows interested in psychic
research around the turn of the century.

Over the course of his life Rayleigh publishes over 450 scientific papers.

Strutt's papers are published as "Scientific papers (1869-1919)" (1899) (6
vol.).
(private laboratory) Terling Place, England  
130 YBN
[1870 AD]
2687)
  
130 YBN
[1870 AD]
3081)
(University of Heidelberg) Heidelberg, Germany  
130 YBN
[1870 AD]
3361)
(University of Heidelberg) Heidelberg, Germany  
130 YBN
[1870 AD]
3634) Marsh is credited with the discovery of more than a thousand fossil
vertebrates. Marsh publishes major works on toothed birds, gigantic horned
mammals, and North American dinosaurs.
Marsh spends his entire career at Yale University
(1866–99) as the first professor of vertebrate paleontology in the United
States.
In 1866, Marsh persuades his rich uncle to endow the Peabody Natural History
Museum at Yale.
Marsh is a strong supporter of Darwinian evolution.
In 1870 Marsh
organizes the first Yale Scientific Expedition, in which he (with a group of
students) explores the Pliocene (5.3 to 1.8 million years ago) deposits of
Nebraska and the Miocene (23.8 to 5.3 million years ago) deposits of northern
Colorado.
Marsh employs William F. Cody ("Buffalo Bill") as a guide to scour
the western United States for fossils.
A succession of such expeditions follows
throughout the 1870s.
Marsh competes with Cope to find fossils. Together they
find enough bones of ancestral horses to understand the complete line of
descent of the horse.
From 1883-1895, Marsh is the President of the National Academy
of Sciences.
Smoky Hill River, (Western) Kansas, USA  
130 YBN
[1870 AD]
3643)
(family estate) Glenlair, England  
130 YBN
[1870 AD]
3735)
(University of Berlin) Berlin, Germany  
130 YBN
[1870 AD]
3777)
(Perkin factory) Greenford Green, England (presumably)  
130 YBN
[1870 AD]
3778)
(Perkin factory) Greenford Green, England (presumably)  
130 YBN
[1870 AD]
3909)
(University of Breslau) Breslau, Lower Silesia (now Wroclaw, Poland)  
130 YBN
[1870 AD]
4701)
London, England (guess)  
129 YBN
[01/07/1871 AD]
3704)
(University of St. Petersburg) St. Petersburg, Russia  
129 YBN
[01/??/1871 AD]
3659)
(University of) Göttingen, Germany  
129 YBN
[02/??/1871 AD]
3705) Dmitri Ivanovich Mendeléev (meNDelAeF) (CE 1834-1907), Russian chemist
publishes a chemistry textbook "Osnovy khimii" (2 vol., 1868-1871; tr. 1905,
"The Principles of Chemistry"), after finding nothing that he can recommend as
a text upon being appointed chair of chemistry at the University of St.
Petersburg.

According to Asimov this is one of the best chemistry books ever written in
Russian.

(University of St. Petersburg) St. Petersburg, Russia  
129 YBN
[05/10/1871 AD]
3433)
(Tulse Hill)London, England  
129 YBN
[08/??/1871 AD]
3814) (private observatory) Bothkamp, Germany  
129 YBN
[09/08/1871 AD]
3113) Although the Royal Photographic Society awards Maddox the Progress Medal,
its highest honor, Maddox dies in poverty.
Woolston, Southhampton, England  
129 YBN
[11/17/1871 AD]
4160)
Greenwich, England   
129 YBN
[12/??/1871 AD]
3876)
(Helmholtz Lab, U of Heidelberg) Heidelberg, Germany  
129 YBN
[1871 AD]
2657) The term "baud" (used for computer modems), which is a measure of symbols
transmitted per second, is named after Emile Baudot.
France  
129 YBN
[1871 AD]
2662)
  
129 YBN
[1871 AD]
2686)
Yokohama, Japan  
129 YBN
[1871 AD]
3169)
(University of Berlin) Berlin, Germany  
129 YBN
[1871 AD]
3355)
(University of Berlin) Berlin, Germany  
129 YBN
[1871 AD]
3518)
(University of Tübingen) Tübingen, Germany  
129 YBN
[1871 AD]
3526)
(Queen's University) Dublin, Ireland  
129 YBN
[1871 AD]
3542)
(U of Jena) Jena, Germany  
129 YBN
[1871 AD]
3560) (Ecole Superieure de Pharmacie) Paris, France  
129 YBN
[1871 AD]
3575)
Newcastle, England (presumably)  
129 YBN
[1871 AD]
3633)
(Upper Jurasic) Wyoming, USA  
129 YBN
[1871 AD]
3666)
Ecole Normal, Paris, France (presumably)  
129 YBN
[1871 AD]
3924)
(University of Graz) Graz, Austria (presumably)  
129 YBN
[1871 AD]
4059) In his life Meyer publishes 275 papers himself.
In 1897 Meyer kills himself by
drinking prussic acid.
(University of Stuttgart), Stuttgart, Germany (presumably)  
129 YBN
[1871 AD]
4069) Klein serves in Franco-Prussian war.
( University of Göttingen) Göttingen, Germany  
128 YBN
[01/01/1872 AD]
1249)
?  
128 YBN
[1872 AD]
3197) Aldol is an oily colorless liquid obtained by the condensation of two
molecules of acetaldehyde. Aldol contains an alcohol group (-OH) and an
aldehyde group (-CHO). The word "aldol" also refers to any similar aldehyde
containing the group CH3OH–CO–CHOH.
(Ecole de Médicine, School of Medicine) Paris, France  
128 YBN
[1872 AD]
3198)
(Ecole de Médicine, School of Medicine) Paris, France  
128 YBN
[1872 AD]
3317)
(Royal Institution) London, England  
128 YBN
[1872 AD]
3566)
(University of Breslau) Breslau, Lower Silesia (now Wroclaw, Poland)  
128 YBN
[1872 AD]
3630) Dedekind studies advanced mathematics at the University of Göttingen
under the mathematician Carl Friedrich Gauss.
(Technical High School in Braunschweig) Braunschweig, Germany  
128 YBN
[1872 AD]
3732)
(Zurich University) Zurich, Switzerland (presumably)  
128 YBN
[1872 AD]
3748) Draper serves in the Union army as a surgeon.

Henry Draper's father, John William Draper, in 1840 had made the first
photograph of the Moon.

Draper rules his own metal gratings.

For his photography of the transit of Venus in 1874, Congress orders a gold
medal struck in his honour.
Draper's widow establishes the Henry Draper Memorial Fund
at Harvard Observatory, financing the making of the great "Henry Draper
Catalogue of stellar spectra".

(This seems very late for the first photograph of the spectrum of a star, in
particular if people see thought in 1810.)
(City University) New York City, NY, USA  
128 YBN
[1872 AD]
3770) Between 1873 and 1893 Mach develops optical and photographic techniques
for the measurement of sound waves and wave propagation. In 1881 Mach proposes
the use of electric discharges to produce photographs with extremely short
exposure time.
Einstein will refer to the Mach principle, which is Mach's view that
the properties of space have no independent existence but are dependent on the
mass content and mass distribution within it.
(explain more accurately, to me
clearly there is space and matter in space. One great question is: does matter
fill space, or is matter part of space? In other words, does matter move from
space to space, or do the matter and space move together? My own view is that
matter occupies space, and moves from space to space. If matter is a kind of
space, then it is a different kind, and that seem not logical to me.)


According to Asimov, Mach is strongly influenced by the "psychophysics" of
Fechner.

Mach opposes the atomic theory, and most things that are not proven through
direct sensory information.

Mach rejects Einstein's theory of relativity, and plans on writing a book
pointing out its flaws when he dies in 1916.
(Charles University) Prague, Czech Republic  
128 YBN
[1872 AD]
3911)
Berlin, Germany  
128 YBN
[1872 AD]
3923) Another explanation of the second law of thermodynamics, that heat moves
from hot to cold, might be the interpretation that masses tend to move to where
there is more space which can hold them - or basically the view that moving
masses will naturally be collided into more open spaces (unmatter filled
spaces) since there are less spaces for them to exist in, in a volume of more
matter filled space - or in a volume where the matter has a higher velocity
than an equivalent adjacent volume of space. - In this sense, this concept of
the first law - of heat moving toward cold - is the natural result of
gravitation+inertia+collision in a universe of matter-filled-space, empty-space
and time (or simply, matter, space and time).

I think a good effort might be to relate temperature to average velocity (and
perhaps quantity of mass, or average density of mass in a volume of space) as
opposed to average energy - but possibly quantity of mass effects temperature -
then temperature has to do with absorption of mass used for measurement.

It's interesting that lineages can be seen in the history of science how
Boltzmann builds on Maxwell's work, Maxwell built upon Thomsen's who built on
Joule's - in the heat as a mechanical movement group and those whose focus was
thermodynamics, using the concept of vis-viva and then energy to describe the
universe which shadowed any other physics models.
(University of Graz) Graz, Austria (presumably)  
128 YBN
[1872 AD]
3930) Cantor was hospitalized first in 1899 and dies in Halle University's
psychiatric clinic. (try to find exact reason - checked in by self, or did
something unusual?)

The German mathematician Kronecker (who famously said "God made the integers,
and all the rest is the work of man”), strongly opposes Cantor's work and
blocks Cantor's appointment to the faculty at the University of Berlin.
(University of Halle) Halle, Germany  
127 YBN
[02/12/1873 AD]
3336)
Valentia, Ireland  
127 YBN
[1873 AD]
2782)
(Dorpat Observatory) Dorpat (Tartu), Estonia  
127 YBN
[1873 AD]
3049) Hermann Günther Grassmann (CE 1809-1877), German mathematician, writes a
six-part "Wörterbuch zum Rigveda" (1873-1875) which is a complete glossery of
the Rigveda (in German).

(Gymnasium in) Stettin, (Prussia now) Poland  
127 YBN
[1873 AD]
3371) Schliemann learns to read and write fluently between 8 and 13 languages
including Russian and both ancient and modern Greek.
Schlieman makes a fortune at the
time of the Crimean War, mainly as a military contractor.
Schlieman publishes "Ithaka, der
Peloponnes und Troja" ("Ithaca, the Peloponnese, and Troy"), in which he argues
that Hisarlık, in Asia Minor, and not Bunarbashi, a short distance south of
it, is the site of ancient Troy and that the graves of the Greek commander
Agamemnon and his wife, Clytemnestra, at Mycenae, described by the Greek
geographer Pausanias, are not the tholoi (vaulted tombs) outside the citadel
walls but lay inside the citadel.
Schliemann publishes "Troja und seine Ruinen" (1875;
"Troy and Its Ruins").
Hisarlik, Turkey  
127 YBN
[1873 AD]
3409)
(Sorbonne) Paris, France (presumably)  
127 YBN
[1873 AD]
3586) Thomson is originally Wyville Thomas Charles, but changes his name when
knighted.
(University of Edinburgh) Edinburgh, Scotland (presumably)  
127 YBN
[1873 AD]
3662)
Glenlair, England  
127 YBN
[1873 AD]
3753) In 1867 Proctor creates a map of Mars and names the features on Mars
mostly after English astronomers, later Schiaparelli renames them to more
objective, less nationalistic names.

Proctor is a prolific writer and authors many works intended to inform the
public of and popularize astronomy.
London, England (presumably)  
127 YBN
[1873 AD]
3758) In 1910 Waals wins the Nobel prize in physics for his gas equations.

James Clerk Maxwell writes in Nature "The molecular theory of the continuity of
the liquid and gaseous states forms the subject of an exceedingly ingenious
thesis by Mr Johannes Diderik van der Waals, a graduate of Leyden. There are
certain points in which I think he has fallen into mathematical errors, and his
final result is certainly not a complete expression for the interaction of real
molecules, but his attack on this difficult question is so able and so brave,
that it cannot fail to give a notable impulse to molecular science. It has
certainly directed the attention of more than one inquirer to the study of the
Low-Dutch language in which it is written.". (Is "Low Dutch" an insult or
describing a dialect of Dutch?)
(University of Leyden) Leyden, Netherlands  
127 YBN
[1873 AD]
3809)
(in his own home) Vienna, Austria (now Germany) (presumably)  
127 YBN
[1873 AD]
3850) In 1876 Ferrier is a founding member of the Physiological Society.
In 1878,
Ferrier is founding editor of the journal "Brain" still published today.

Ferrier has an important influence on the science of brain surgery in urging
his colleagues to remove cerebral lesions through operation.

In 1882, a lawsuit is brought against Ferrier for cruelty against animals. In
court Ferrier upholds the necessity and value of animal experimentation and
wins the case.

(I think there is definitely a line, in my own opinion, that no species should
be made to endure pain and suffering, and even damage at least to higher order
species. Clearly people accept the painless murder of many species for food and
clothing, where I prefer the alternative of only murdering plants, fungi and
protists for food and clothing. I vote against punishing those involved in
clearly consensual health science experimental treatments.)

(I think the violent laws should extend to all primates, and many mammals. In
particular I think the right to life and to be free from pain should extend to
primates and mammals. Clearly insects can be murdered. I support the cruelty to
animals law in which people are punished for causing prolonged pain in any
species - although I doubt the torture of insects and smaller species would win
a vote of jail-time for the offender.)

(I think for useful scientific research, I doubt a penalty of imprisonment
would win popular support, or even fines, given the common murder of many
species for food. It probably depends on the species, the quantity of pain and
suffering they are made to endure, and the intended results. There are examples
of where experimentation on other species directly leads to increased
understanding and cures. One example, is stem cell research used in purposely
paralyzed mammals which produced significant results that may lead to a cure
for paralysis in all species. In this case, many people may forgive the murder,
assault, or paralyzation of the less evolved species, in order to find cures
that will stop the pain of many others. For example, millions of ova and sperm
die every day, and I see nothing wrong with using the cells of human blastulas
so long as there is no nervous system or pain involved, in particular when
these cells are just going to be thrown away otherwise. I think possibly that
animals caused to be in prolonged pain is avoided generally speaking - Hitzig
gives an example of a dog in pain and how unpleasant it was, in addition to how
it can be avoided. My vote is for free info so everybody can see and determine
for each individual case if the intentional damage is acceptable, should be
stopped, or punished, etc. Clearly unconsensually damaging developed humans
outside of a woman's womb is punishable with jail, and no doubt many apparently
useless or pseudoscientific-based damage of animals would not win popular
support.)
(King's College Hospital and Medical School) London, England   
127 YBN
[1873 AD]
3863) Golgi is the president of the University of Pavia.

In 1906 Golgi and Ramón y Cajal are awarded a Nobel prize for work on the
structure of the nervous system.

Golgi's works are published in "Opera Omnia" (v1-3:1903, v4:1929) in 4 volumes.
(Home for Incurables) Abbiategrasso, Italy  
127 YBN
[1873 AD]
3931) In 1908 Henri Poincaré remarks that later generations would regard
Cantor's set theory "as a disease from which one has recovered.".
(University of Halle) Halle, Germany  
127 YBN
[1873 AD]
3950) It seems clear at this time that people in science were engineering
devices with very small dimensions aided by lens and gears.

Some of Lippmann's colour photographs, specially mounted for viewing at an
angle, are preserved in museums, the finest collection being at the Preus
Museum at Horten, Norway.
University of Heidelberg, Germany  
127 YBN
[1873 AD]
4233)
Norway  
126 YBN
[03/18/1874 AD]
3483) William Thomson (CE 1824-1907) invents a new deep sea sounding method
using piano forte wire.

(University of Glasgow) Glasgow, Scotland  
126 YBN
[09/05/1874 AD]
4134) In 1901 Van't Hoff receives the Nobel prize in chemistry for his work on
solutions, and is the first to receive the Nobel prize for chemistry.
(University of Utrecht) Utrecht, Netherlands  
126 YBN
[11/??/1874 AD]
3992) Le Bel writes (translated from French to English):(read full text with
text scrolling in video)

Le Bel and Van't Hoff jointly receive the Davy Medal in 1893.
(Ecole de Médecine) Paris, France  
126 YBN
[12/08/1874 AD]
3855) Gill is educated in clock-making.
Gill plans and supervised the building of an
observatory for Lord Lindsay at Dun Echt, near Aberdeen (1872-1876).
Mauritius  
126 YBN
[12/08/1874 AD]
3856)
Ascension Island  
126 YBN
[12/08/1874 AD]
3857)
(Royal Observatory) Cape of Good Hope, Africa  
126 YBN
[12/12/1874 AD]
3872)
(Astrophysical observatory) Potsdam, Germany  
126 YBN
[1874 AD]
2656)
New Jersey, USA  
126 YBN
[1874 AD]
2661)
France  
126 YBN
[1874 AD]
3450)
(?), Japan  
126 YBN
[1874 AD]
3527)
(Queen's University) Dublin, Ireland  
126 YBN
[1874 AD]
3780) Boisbaudran comes from a wealthy family of distillers of Cognac in
southwestern France. With independent wealth and excited by the new
spectroscopy of Gustav Kirchhoff, Boisbaudran builds his own laboratory.
(home lab) Cognac, France (presumably)  
126 YBN
[1874 AD]
3795) Cleve disapproves of the young Arrhenius's Ph.D. dissertation, but twenty
years later helps to pick Arrhenius for a Nobel prize for that same
dissertation.
(Technological Institute in Stockholm) Stockholm, Sweden (presumably)  
126 YBN
[1874 AD]
3816)
(private observatory) Bothkamp, Germany  
126 YBN
[1874 AD]
3869) Abney is a prolific author, writing for both specialist practitioners and
amateurs. Abney publishes a number of books to educate the public including his
first book "Chemistry for Engineers" (1870). Abney's second book, "Instruction
in Photography" (1871) becomes a standard text.

Abney's papers in the Royal Society Catalog number over 100, and over 70 in the
"Photographic Journal".
From 1893 to 1897 Abney is successively president of the Royal
Astronomical Society and of the Physical Society.
(School of Military Engineering) Chatham, England   
126 YBN
[1874 AD]
3889) James Geikie (CE 1839-1915), publishes "The Great Ice Age" (CE 1874–84)
which provides evidence that there were several ice ages separated by
nonglacial epochs. Thomas Chrowder Chamberlin (CE 1843-1928) contributes the
chapter on North America and shows that some deposits are composed of at least
three layers. Chamberlin goes on to establish four major ice ages, which are
named the Nebraskan, Kansan, Illinoian, and Wisconsin after the states in which
they are most easily studied.
Chamberlin is the son of a father who left North Carolina
for Illinois because he disapproved of slavery.
Chamberlin reports "Geology of
Wisconsin" (4 vol. 1877–83) which examines the glacial deposits of the state
and the ancient coral reefs.
In 1887 Chamberlin is President of the University of
Wisconsin.
Chamberlin establishes the "Journal of Geology". (chronology)
(Government Geological Survey) Edinburgh, Scotland (and Wisconsin, USA)  
126 YBN
[1874 AD]
4079) Kovalevsky is the daughter of a general, who uses marriage at 18 to go to
Germany, where she is not allowed to attend university lectures, but where
Weierstrass, impressed with her obvious talent, tutors her privately.
In 1868 she entered
into a marriage of convenience with Vladimir Kovalevsky, a young paleontologist
and a translator of Darwin.
Kovalevsky is elected into the Swedish and Russian Academy
of Science. (first female?)
Kovalevsky dies of pneumonia at age 41. (That seems too
young - perhaps neuron written murder?)

According to the Encyclopedia Britannica, Kovalevsky is the first woman in
modern Europe to gain a doctorate in mathematics, the first to join the
editorial board of a scientific journal, and the first to be appointed
professor of mathematics.

Kovalevskaya also gained a reputation as a writer, an advocate of women's
rights.
(University of Göttingen) Göttingen, Germany  
126 YBN
[1874 AD]
4087) In 1909 Braun wins a share of a Nobel prize in physics (with Marconi) for
Braun's improvements to radio technology.

Braun goes to America to testify in a court case about radio patents but, when
the United States enters World War I in 1917, he is detained as an alien and
dies in New York a year later.
(Würzburg University) Würzburg, Germany  
126 YBN
[1874 AD]
4146) Fischer is the assistant of Adolph von Baeyer for some time.
In 1902
Fischer wins a Nobel prize in chemistry for researches in sugar and purines.
Fischer
loses 2 of 3 sons in WW I. (again showing how terrible, destructive, pointless
and stupid war and any violence against nonviolent people is.)
Fischer ends his own
life when suffering from cancer.
(University of Strasbourg) Strasbourg, Germany  
126 YBN
[1874 AD]
5994)
Weimar, Germany (presumably)  
126 YBN
[1874 AD]
6000)
Milan, Italy  
126 YBN
[1874 AD]
6010) In 1876 an extraordinary relationship begins to develop between
Tchaikovsky and Nadezhda von Meck, the widow of a wealthy railroad tycoon which
is an important component of their lives for the next 14 years. A great admirer
of his work, von Meck chooses to become his patroness and eventually arranges a
regular monthly allowance for him which enabled him in 1878 to resign from the
conservatory and devote his efforts to writing music. Although he and his
benefactor agree never to meet, they engage in a voluminous correspondence that
constitutes a remarkable historical and literary record. They frankly exchange
their views on a broad spectrum of issues. In 1890 Tchaikovsky is informed by
Nadezhda von Meck that she is close to financial ruin and can not continue his
allowancem and their correspondence comes to an end.
(Moscow Conservatory) Moscow, (U.S.S.R. now) Russia  
125 YBN
[03/03/1875 AD]
6007)
(Opéra-Comique) Paris, France (verify)  
125 YBN
[03/20/1875 AD]
3674)
(private lab) London, England(presumably)  
125 YBN
[04/27/1875 AD]
3851)
(King's College Hospital and Medical School) London, England  
125 YBN
[04/27/1875 AD]
3852)
(King's College Hospital and Medical School) London, England  
125 YBN
[08/28/1875 AD]
5575) Liverpool, England  
125 YBN
[10/07/1875 AD]
5332)
Bristol, England  
125 YBN
[10/??/1875 AD]
3788) In 1863 Gibbs receives the first doctorate of engineering to be conferred
in the United States (from Yale).
From 1866 to 1869 Gibbs studies in Paris, Berlin,
and Heidelberg, where his teachers are some of the most distinguished
mathematicians and physicists on earth.

Maxwell constructs a model illustrating a portion of Gibb's work and sends a
plaster cast to Gibbs.(chronology)

In 1901 the Copley medal of the Royal Society of London is awarded to Gibbs as
being "the first to apply the second law of thermodynamics to the exhaustive
discussion of the relation between chemical, electrical and thermal energy and
capacity for external work.".
(Yale College) New Haven, Connecticut, USA  
125 YBN
[11/12/1875 AD]
3873)
(Surveyor-General's Office) Calcutta, India  
125 YBN
[1875 AD]
2871)
Paris?,France  
125 YBN
[1875 AD]
3436)
(Tulse Hill)London, England  
125 YBN
[1875 AD]
3520)
(University of Strasbourg) Strasbourg, Germany  
125 YBN
[1875 AD]
3567)
(University of Breslau) Breslau, Lower Silesia (now Wroclaw, Poland)  
125 YBN
[1875 AD]
3673)
(private lab) London, England(presumably)  
125 YBN
[1875 AD]
3798) Cope publishes scientific papers in his teens. (This is perhaps evidence
that people in their teens deserve equal rights.)
cope is independently wealthy.
Cope is a
professor of comparative zoology and botany at Haverford College, Pennsylvania
(1864–67).
Cope serves as paleontologist with the U.S. Geological Survey.
Cope is a Quaker and
refuses to carry a gun, despite the danger from Native American people. When
surrounded by a group of hostile Native American humans, Cope surprises them by
taking out and putting back his false teeth over and over. Once all have a
chance to watch this, they let him go.
Cope competes with Othniel Marsh for
fossils, and between the two they fill in the entire story of the evolutionary
history of the horse.
Cope and Marsh have a bitter feud for credit in being the
first to discover American fossil dinosaurs which damages the reputations of
both men.
According to historian Mark Jaffe, one reason for the hostility between
Cope and Marsh, is that Marsh is a Darwinian and Cope, raised a devout Quaker,
can not accept the absence of divine design in nature. Cope is a leading
exponent of the "Neo-Lamarckian" school of evolution. In the late 1800s,
Neo-Lamarckian evolution is more popular in American than Darwinism. (Although
see above quote which appears to support natural selection and survival of the
fittest.)
Another source states that during the 1860s Marsh and Cope have a friendly
relationship, But when in the 1870's Arthur Lakes and O. W. Lucas discover
dinosaurs in the Southwest United states and begin to ship them to Cope and
Marsh, a harsh rivalry between Marsh and Cope breaks out. Marsh hires Lakes and
Cope hires Lucas, and the bonewar is on. This bonewar lasts until their
deaths.
Similar to Lamarck, Cope wrongly believes in inherited characteristics.
Believing that the movements of animals helps alter and develop the moving
parts, Cope calls this kinetogenesis.
In 1868 Cope attacks Darwin's theory of
natural selection.
Cope publishes the notable, "Reptilia and Aves of North America"
(1869–70) and "The Vertebrata of the Tertiary Formations of the West"
(1883).
Financial difficulties compelled him to accept a position on the faculty of the
University of Pennsylvania (1889–97).
In his life, Cope publishes 1,200 books and papers.

Cope's large collection of fossil mammals is now at the American Museum of
Natural History.
(Read before the American Association for the advancement of Science) Detroit,
Michegan, USA  
125 YBN
[1875 AD]
4172) Not yet twenty-five, Lorentz accepts an appointment as chair of
theoretical physics at the University of Leiden. The Leiden theoretical physics
chair is the first of its kind in the Netherlands, and one of the first in
Europe.

According to the Encyclopedia Britannica Lorentz is a joint winner (with Pieter
Zeeman) of the Nobel Prize for Physics in 1902 for his theory of
electromagnetic radiation, which, confirmed, by the findings of Zeeman, give
rise to Albert Einstein's special theory of relativity.

Lorentz supervises the enclosure of the Zuider Zee, a project to make more
agricultural land out of a shallow basin of the sea.
(University of Leiden) Leiden, Netherlands  
125 YBN
[1875 AD]
6009)
Moscow, (U.S.S.R. now) Russia  
125 YBN
[1875 AD]
6016)
Troldhaugen, Norway  
124 YBN
[02/14/1876 AD]
4036) Both Bell's father and grandfather had studied the mechanics of sound,
and Bell's father was a pioneer teacher of speech to deaf people.
In 1871 Bell goes to
Boston to teach at Sarah Fuller's School for the Deaf, the first such school on
earth. Bell also tutors private students, including Helen Keller. As professor
of vocal physiology and speech at Boston University in 1873, Bell initiates
conventions for teachers of the deaf. Throughout his life Bell continues to
educate the deaf, and founds the American Association to Promote the Teaching
of Speech to the Deaf.

Bell's other two brothers die of Tuberculosis.
Bell falls in love with one of his deaf
pupils.
When Bell refers sadly to Henry of his own lack of electrical know-how, Henry
tell Bell "Get it!".
James Clerk Maxwell expected something far more complex of a
device that can carry a voice.

Bell wins France's "Volta Price", and with the prize money (50, 000 francs,
about $10, 000) starts the Volta Laboratory in Washington, D.C. At the
laboratory Bell and associates work on various projects during the 1880s,
including the photophone, induction balance (metal detector), audiometer, and
phonograph improvements.

Aviation is Bell's primary interest after 1895.
Bell experimentes with hydrofoil
boats and with airplanes as early as the 1890s.

Bell funds Samuel Langley. (plane, bolometer ... all research?) Perhaps
Langley's publication of the heat sensing bolometer was Bell's and other
people's coordinated effort to give the poor excluded victims of remote neuron
activation, seeing, hearing and sending thought images and sounds a better
chance at figuring out how to see thought. In addition, Langley is affiliated
with the US Military - the Langley field being named after Langley.

In 1915 the first transcontinental telephone line is opened, and Bell (in the
East) speaks again to his old assistant Watson. Again Bell says 'Watson please
come here. I want you.', and Asimov comments this time instead of the words
going from one floor to another they went from one coast to the other.

Bell performes studies on longevity. In 1918, Bell examines the familial
transmission of human longevity using genealogical data on about 3,000 members
of the Hyde family in New England. (verify)

In his life Bell has 18 patents and 12 with collaborators. These include 14 for
the telephone and telegraph, 4 for the photophone, 1 for the phonograph, 5 for
aerial vehicles, 4 for hydroairplanes, and 2 for a selenium cell.

(Kind of interesting that Bell's later work involves air planes - perhaps with
great wealth comes a desire to escape the confines and limits of the earth.)
Salem, Massachusetts, USA  
124 YBN
[02/14/1876 AD]
4037) Gray invented a number of telegraphic devices and in 1869 was one of two
partners who founded what will become Western Electric Company. (Perhaps Gray
used the information gathered from telegraphs to learn about Reiss' invention -
or perhaps from secret hidden thought cameras and microphones.)
Chicago, Illinois, USA  
124 YBN
[02/15/1876 AD]
4065) Rowland is the first president of the American Physical Society
(1899–1901).
Rowland dies of diabetes before Frederick Banting figures out how to isolate
insulin, a treatment for diabetes.
There is a funny story about Rowland, in that under
oath, he testifies that he is the greatest living american physicist, and later
explains that he had to say this because he was under oath.
(working for Johns Hopkins University, Baltimore) (University of Berlin)
Berlin, Germany  
124 YBN
[05/01/1876 AD]
3656)
(University of Würzburg) Würzburg, Germany  
124 YBN
[09/??/1876 AD]
3572)
(work done at St. Peterburg University, paper presented at) Warsaw,
Poland  
124 YBN
[1876 AD]
2688)
((Berlin or Frankfurt?))  
124 YBN
[1876 AD]
3038)
Downe, Kent, England (presumably)  
124 YBN
[1876 AD]
3039) Charles Robert Darwin (CE 1809-1882), English naturalist, publishes "The
Different Forms of Flowers on Plants of the Same Species" (1877), which is the
result of work into the way evolution in some species favors different male and
female forms of flowers to facilitate "outbreeding" (as opposed to inbreeding,
that is to facilitate variety of mating partners). According to the
Encyclopedia Britannica Darwin had long been sensitive to the effects of
inbreeding because he was himself married to a Wedgwood cousin, as was his
sister Caroline.

(To me, there is a strong natural inclination towards variety even in human
sexuality. This phenomenon works against monogamy {and some might argue perhaps
against reproducing in small numbers, or perhaps responsible parenting} in that
for some humans sex is better between two people the first time, as opposed to
later sex. In this way, it appears that biologically many humans are designed
to prefer a wide variety of sexual partners, a constant stream of new partners,
as opposed to a single mate for repeated sex throughout life, although the data
on this phenomenon is somewhat abstract and in small quantity.)

Downe, Kent, England (presumably)  
124 YBN
[1876 AD]
3040) Darwin's drawing of a hairy human ancestor with pointed ears leads to a
number of caricatures in newspapers.
Downe, Kent, England (presumably)  
124 YBN
[1876 AD]
3041) Charles Robert Darwin (CE 1809-1882), English naturalist, publishes "The
Expression of the Emotions in Man and Animals" (1872), which is
photographically illustrated to show the continuity of emotions and expressions
between humans and animals.

The goal of this book is to disprove the theory that facial expression are only
in humans.

Downe, Kent, England (presumably)  
124 YBN
[1876 AD]
3042) Charles Robert Darwin (CE 1809-1882), English naturalist, writes his
autobiography (1876-1881). In this work Darwin writes about his dislike of
Christian myths of eternal torment.

Downe, Kent, England (presumably)  
124 YBN
[1876 AD]
3050) Hermann Günther Grassmann (CE 1809-1877), German mathematician,
translates the hymns of the Rig-Veda (into German) in "Rig-Veda. Übersetzt und
mit kritischen Anmerkungen versehen" (1876-77).

The linguistic law reformulated by (and named for) Grassman holds that in
Indo-European bases, especially in Sanskrit and Greek, successive syllables may
not begin with aspirates (in linguistics the "H" sound).

(Gymnasium in) Stettin, (Prussia now) Poland  
124 YBN
[1876 AD]
3069)
(Harvard University) Cambridge, Massachussetts, USA  
124 YBN
[1876 AD]
3484) William Thomson (CE 1824-1907) invents a form of analog computer for
measuring tides in a harbour and for calculating tide tables for any hour, past
or future.

Thomson also invents a mariner's compass.

(University of Glasgow) Glasgow, Scotland  
124 YBN
[1876 AD]
3669) In 1861, Otto builds his first gasoline-powered engine.
In 1864, Otto forms a
partnership with the German industrialist Eugen Langen.
In 1867 Otto and Langen win a
gold medal at the Paris Exposition for an improved engine that they develop
together.
(Gasmotoren-Frabrik Deutz AG) Deutz, Cologne, Germany  
124 YBN
[1876 AD]
3696)
Paris, France (presumably)  
124 YBN
[1876 AD]
3755)
(University of Heidelberg) Heidelberg, Germany  
124 YBN
[1876 AD]
3819) Linde's company also sells solid water ice.
(Technische Hochschule) Munich, Germany  
124 YBN
[1876 AD]
3892) Koch serves as an army surgeon on the Prussian side during the
Franco-Prussian War.
Late in life Koch divorces his wife and marries a much
younger woman, shocking the Victorian society of the time.
Koch trains many prominent
bacteriologists such as Gaffky, Kitasato, Behring and Ehrlich.
(District Medical Officer) Wollstein, Germany  
124 YBN
[1876 AD]
3972)
University of Strasbourg, Strasbourg, Alsace, Germany(now in France)  
124 YBN
[1876 AD]
3986)
Cavendish Laboratory, Cambridge University, Cambridge, England
(presumably)  
124 YBN
[1876 AD]
4094)
(University of Berlin) Berlin, Germany  
124 YBN
[1876 AD]
6022)
Milan, Italy (presumably)  
123 YBN
[04/14/1877 AD]
4111) Berliner supports compulsory (a law?) pasteurizing of milk, which will
ultimately contribute to the health of people in the USA.
Berliner does useful work
on airplane motors. (more specific)

Berliner works as chief inspector for the Bell Telephone Company.

Berliners is a supporter of women equality, and argues that women, given the
opportunities for education equal to men, would equal men in the sciences. In
1908 Berliner founds amd funds the "Sarah Berliner Research Fellowship". Mrs.
Christine Ladd Franklin, the first woman to earn a doctor's degree at Johns
Hopkins University, is a charter member, and Berliner also obtains the
cooperation of the American Association of University Women. The fellowship is
made available for research in physics, chemistry or biology. From 1909 to 1926
awards are given to women each year in those fields as well as in psychology,
physiology, paleontology, geology, nutrition, zoology and related subjects.

Berliner is agnostic and writes a book ("Conclusions") explaining his views,
which is published in 1889.
(own apartment) Washington, DC, USA  
123 YBN
[04/27/1877 AD]
3994)
(private lab) Menlo Park, New Jersey, USA  
123 YBN
[04/27/1877 AD]
4294)
(private lab) Menlo Park, New Jersey, USA  
123 YBN
[06/??/1877 AD]
3879)
(Sorbonne laboratory) Paris, France (verify)  
123 YBN
[07/??/1877 AD]
3749)
(City University) New York City, NY, USA  
123 YBN
[08/11/1877 AD]
3584)
(Naval Observatory) Washington, DC, USA  
123 YBN
[08/17/1877 AD]
3585)
(Naval Observatory) Washington, DC, USA  
123 YBN
[08/28/1877 AD]
4000)
(private lab) Menlo Park, New Jersey, USA  
123 YBN
[09/??/1877 AD]
3729)
(Brera Observatory) Milan, Italy  
123 YBN
[10/11/1877 AD]
3925) (I think an important point is showing how any of these equations are
found to be useful, practical and apply accurately to observable phenomena.)
(University of Graz) Graz, Austria   
123 YBN
[12/02/1877 AD]
3688) When young Cailletet works in his father's ironworks and later is in
charge of the works.

Cailletet invented automatic cameras.
(father's ironworks) Chatillon, France  
123 YBN
[12/22/1877 AD]
3961)
University of Geneva, Switzerland  
123 YBN
[12/24/1877 AD]
4002)
(private lab) Menlo Park, New Jersey, USA  
123 YBN
[12/??/1877 AD]
3619)
Veinna  
123 YBN
[1877 AD]
2690) The first electrical telegraph line in Tientsin (now Tianjin) China is
constructed between the castle of the governor and the city arsenal by students
of the local mining school.

Tientsin (now Tianjin), China  
123 YBN
[1877 AD]
3138)
(Ecole Polytechnique) Paris, France  
123 YBN
[1877 AD]
3318)
(Royal Institution) London, England  
123 YBN
[1877 AD]
3342) Muybridge murders a man who had sex with his wife, but is not convicted.
(This shows how acceptable first degree murder and other violence is at the
time and ironically how unacceptable consensual sex is.)
Sacramento, CA, USA  
123 YBN
[1877 AD]
3349)
Sacramento, CA, USA  
123 YBN
[1877 AD]
3667)
Sorbonne, Paris, France  
123 YBN
[1877 AD]
3756)
(University of Heidelberg) Heidelberg, Germany  
123 YBN
[1877 AD]
3901)
Wollstein, Germany  
123 YBN
[1877 AD]
3928)
Hong Kong (presumably)  
123 YBN
[1877 AD]
3934) At 15, Pfeffer works for his father, who is an apothecary.
Pfeffer's only son is
killed in WWI 2 months before the armistice.
  
123 YBN
[1877 AD]
4039)
Boston and New York, USA  
123 YBN
[1877 AD]
4051)
The Haag, Netherlands (work possibly done at University of Halle-Wittenberg,
Germany)  
123 YBN
[1877 AD]
4055) Lilienthal is trained as a mechanical engineer, and establishes his own
machine shop and flight factory following service in the Franco-German War.

During the early days of the Industrial Revolution, the idea of human flight is
ridiculed. But Lilienthal disregards the social stigma associated with flying
machine inventors and applies himself to the study of aerodynamic forces and
design concepts.

In the 1870s Lilienthal begins to conduct studies of the forces operating on
wings in a stream of air and publishes his results in a book entitled "Der
Vogelflug als Grundlage der Fliegekunst" ("Bird Flight as the Basis of
Aviation").

Between 1891 and 1896, Lilienthal completes some 2,000 flights in at least 16
distinct glider types.

Images of Lilienthal flying through the air aboard his standard glider appear
in newspapers and magazines around the earth and these pictures convince
millions of readers in Europe and the United States that the age of flight is
now.

On August 9, 1896, while testing a glider with a new rudder design, Lilienthal
has a crash which breaks his back, and he dies in a Berlin hospital the next
day.

Otto's brother, Gustav Lilienthal (CE 1849-1933), continues Otto's flight
experiments after his brother's death.

The Wright brothers, also experienced with gliders, will demonstrate that by
mounting an engine (with a propeller) on a glider, it can be converted into an
airplane.
(Weber Company and C. Hoppe machine factory) Berlin, Germany  
123 YBN
[1877 AD]
4056)
Derwitz/Krilow (near Potsdam), Germany  
123 YBN
[1877 AD]
4071) Ivan Petrovich Pavlov (PoVluF) (CE 1849-1936), Russian physicologist
publishes his first work, "Experimental Data Concerning the Accommodating
Mechanism of the Blood Vessels", which deals with the reflex regulation of the
circulation of blood. Pavlov describes the role of the vagus nerve as a
regulator of blood pressure. (chronology - in this 1877 work?)
Pavlov is from a
family of priests but at the theological seminary he reads Darwin's "Origin of
Species" and finds that his natural call is for science and not priesthood.
In 1904 Pavlov
receives the Nobel prize in medicine and physiology.
Asimov writes that Pavlov is
anti-communist (which form of government did Pavlov support?), but the Soviet
government does not punish this, even building him a laboratory in 1935, and
Pavlov is an ornament of Russian science and a showpiece of Soviet toleration.
In 1923,
after returning from his first visit to the United States Pavlov publicly
denounces Communism, stating that the basis for international Marxism is false,
and says "For the kind of social experiment that you are making, I would not
sacrifice a frog's hind legs!". (Notice the potential relation to remote neuron
writing {galvanization} with frog legs.)
In 1927, distressed that his was the only
negative vote in the Academy of Sciences against the newly recommended "red
professors", Pavlov writes to Joseph Stalin, protesting that "On account of
what you are doing to the Russian intelligentsia—demoralizing, annihilating,
depraving them—I am ashamed to be called a Russian!".
(Medico-Chirurgical Academy - renamed in 1881 the Military Medical Academy),
St. Petersburg, Russia  
123 YBN
[1877 AD]
4167)
Bromley, Kent, England  
123 YBN
[1877 AD]
4194) In 1908 Ehrlich wins the Nobel prize in medicine and physiology (shared
with Élie Mechnikov) for Ehrlich's work on immunity and serum therapy.
In 1887 Ehrlich
becomes a teacher at the University of Berlin but is not paid because of the
anti-Jewish feeling at the time – Ehrlich would not renounce his Jewish
upbringing.
Ehrlich's tomb, in a Jewish cemetery in Frankfort, is desecrated by Nazi people
but restored after World War 2.
(Leipzig University) Leipzig, Germany  
122 YBN
[01/11/1878 AD]
3962)
University of Geneva, Switzerland  
122 YBN
[04/29/1878 AD]
3419)
(École Normale Supérieure) Paris, France  
122 YBN
[04/??/1878 AD]
4275)
  
122 YBN
[07/22/1878 AD]
3949) George Darwin is the second son of Charles Darwin.

Darwin's scientific papers are published in five volumes.

(This paper is 93 pages long, and is highly mathematical in the style of
Laplace, Maxwell, and Kelvin, etc. - heavily mathematical and somewhat abstract
analysis rose to popularity around the time of Laplace - while math describes
accurately physical phenomena, the problem is that there are so many particles,
and many times, mathematical quantities are highly generalized, that the
mathematical model may not represent the physical phenomenona.)

(How can we be sure that the motions of the oceans might not speed up the
earth's rotational speed? EX: We need to model the effect of a liquid on the
surface of a spinning sphere. Does the rate of rotation decrease or increase?
Do the simulations result in different results? Use different land masses,
different rates of friction on the ocean floor. It is a very complex model.
Atoms of liquid are difficult to model. I initially accepted this conclusion,
but now have questions, because the number of atoms in the ocean is so large,
friction with the sides of land very uneven, and the possibility of the
rotation speed increasing. For a solid sphere, theoretically there would be no
decelerating or accelerating (except as a result of crustal changes). Adding
water in my novice view seems like it might slow the earth by causing extra
frequencies, that tend to work against the rotation. I can imagine that there
is someway of adding some material to a sphere in a way to make it's rotation
speed up over time. It seems that absent any force increasing rotation, any
rotating body could only slow down over time, yet, somehow bodies around stars
start rotating, it is a collective effect of the seemingly random collisions of
matter I think. Without some external source of acceleration, there would be
no way to increase velocity relative to the Sun, however, acceleration from
gravitation may change since the distance of the earth from the Sun may change.
Other planets and masses may impart accleration on the Earth too. There must be
non-rotating objects in the star system, perhaps some asteroids. Do all
asteroids have one axis rotations? It's a complex simulation. It seems that
without any more collisions, there is no way to add to the velocity of the
earth. But perhaps a push by water could speed it up. I think a good case can
be made for the slowing of all rotating bodies in the star system based on an
absence of any force to accelerate them, although there is nothing but photons
and surface liquid and gas to cause friction (perhaps gravity might add to
rotation of uneven asteroids). If I had to guess, I would guess that the earth
and all other planets are slowly slowing down, and even the sun is slowing down
as it loses matter. If true, then the sun and planets probably were orbiting
faster in the past (and each planet's year was shorter). It is interesting to
think that the earth and other rotating bodies might be slowing down, and
perhaps rotated faster in the past.)
(Trinity College) Cambridge, England  
122 YBN
[07/??/1878 AD]
4158) In 1907 Michelson wins the Nobel prize in physics for his optical
studies. Michelson is the first American to win a Nobel Prize.
From 1923-1927
Michelson is the president of National Academy of Sciences.
(U.S. Naval Academy) Annapolis, Maryland  
122 YBN
[08/01/1878 AD]
4019)
(private lab) Menlo Park, New Jersey, USA  
122 YBN
[10/10/1878 AD]
3878)
(King's College and Institute of Chemistry) London, England  
122 YBN
[12/19/1878 AD]
3105) (Sir) William Robert Grove (CE 1811-1896), British physicist examines the
differences in the spectrum of positive and negative electrodes in vacuum
tubes.

London, England  
122 YBN
[1878 AD]
2995)
(Clapham) London, England (presumably)  
122 YBN
[1878 AD]
3188) Ytterbium is named for Ytterby, a town in Sweden.
Ytterbium is a metallic
chemical element that has symbol Yb, atomic number 70, atomic mass (weight)
173.04, melting point 819°C; boiling point about 1,194°C; relative density
(specific gravity) about 7.0 and valence +2 or +3. Ytterbium is a soft,
malleable, ductile, lustrous silver-white metal. Although ytterbium is one of
the rare-earth metals of the lanthanide series in Group 3 of the periodic
table, in some of its chemical and physical properties ytterbium more closely
resembles calcium, strontium, and barium. Ytterbium exhibits allotropy; at room
temperature a face-centered cubic crystalline form is stable. The Yterrbium
metal tarnishes slowly in air and reacts slowly with water but rapidly
dissolves in mineral acids. Ytterbium forms numerous compounds, some of which
are yellow or green. The oxide (ytterbia, Yb2O3) is colorless. Ytterbium is
widely distributed in a number of minerals, for example, gadolinite, and
monazite. At about this same time C. A. von Welsbach independently discovered
ytterbium and called it aldebaranium.

Ytterbium has little commercial use.

Ytterbium is among the less-abundant rare earths. Ytterbium occurs in minute
amounts in many rare-earth minerals such as xenotime and euxenite and is found
in the products of nuclear fission too. Natural ytterbium consists of seven
stable isotopes.
(University of Geneva) Geneva, Switzerland  
122 YBN
[1878 AD]
3189) Gadolinium is a silvery-white, malleable, ductile, metallic rare-earth
element obtained from monazite and bastnaesite and used in improving
high-temperature characteristics of iron, chromium, and related alloys. Atomic
number 64; atomic weight 157.25; melting point 1,312°C; boiling point
approximately 3,000°C; relative density (specific gravity) from 7.8 to 7.896;
valence 3.

Gadolinium has unusual magnetic properties. At room temperature the metal is
paramagnetic, but it becomes strongly ferromagnetic when cooled. Paramagnetism
and Diamagnetism were first identified by Michael Faraday in 1845.
A paramagnetic
material is a substance in which an induced magnetic field is parallel and
proportional to the intensity of the magnetizing field but is much weaker than
in ferromagnetic materials. (This is somehow different from simply having a
weaker magnetic field at a higher temperature?) Diamagnetic material is a
substance in which has a magnetic permeability less than 1; materials with this
property are repelled by a magnet and tend to position themselves at right
angles to magnetic lines of force. (I think this clearly needs to be shown in
videos. In experimenting with Bismuth metal powder I could not detect any
movement from a small magnet.)

Gadolinium has the highest absorption cross section for thermal neutrons of any
natural isotope of any element (49,000 barns), which suggests its use in
nuclear reactor control rods.
(University of Geneva) Geneva, Switzerland  
122 YBN
[1878 AD]
3372)
Mycenae, Greece  
122 YBN
[1878 AD]
3576)
Newcastle, England (presumably)  
122 YBN
[1878 AD]
3692) Bert is an anticlerical leftist and represents Yonne in the Chamber of
Deputies (1872–86) and serves as minister of education (1881–82) in Léon
Gambetta's Cabinet.
Bert argues for free public education and the separation of
church and state. Bert is one of the most determined enemies of clericalism,
and an ardent advocate of "liberating national education from religious sects,
while rendering it accessible to every citizen.".
(Sorbonne) Paris, France  
122 YBN
[1878 AD]
3716) Langley writes "The New Astronomy" (1884) and "Experiments in
Aerodynamics" (1891).

A unit of radiation equal to 1 calorie per square centimeter is called 1
Langley in his honor. (I think "radiation" is generally defined as light,
electrons, and other particles emited from objects, but it is really too
general to be useful in my opinion.)

Langley Field, Virginia, and the Langley Research Center of NASA are named in
Langley's honor.
(Western University of Pennsylvania now the University of Pittsburg) Pittsburg,
Pennsylvania, USA (presumably)  
122 YBN
[1878 AD]
3721)
(Nautical Almanac Office) Washington, DC, USA  
122 YBN
[1878 AD]
3790) In 1914 Chardonnet is awarded the Perkin medal for rayon.
  
122 YBN
[1878 AD]
3864)
(University of Pavia) Pavia, Italy  
122 YBN
[1878 AD]
3902)
(District Medical Officer) Wollstein, Germany  
122 YBN
[1878 AD]
3964) It is noteworthy, or somewhat unusual, that the reprint of the obituary
of Edward Pickering from Science, by the National Academy of Sciences, has the
first phrase changed from "By the death" to "At the death". Perhaps, it may
mean that Pickering was murdered by galvanization by owners or somebody using
the equipment owned by AT&T (since "At the" - may suggest "AT&T"), if perhaps
insiders were somewhat unhappy about such a galvanization. But perhaps it is
just a typo. Although Pickering was in his late 70s, which is somewhat old.
EB2008 uses the word "utilized", instead of uses, perhaps should be
"utility-ized"?
Harvard College Observatory, Cambridge, Massachusetts, USA  
122 YBN
[1878 AD]
4041)
New Haven, Connecticut, USA  
122 YBN
[1878 AD]
4063)
(University of Zurich), Zurich, Switzerland (presumably)  
122 YBN
[1878 AD]
4083) Sharpey-Schäfer argues for equal opportunities for women in health
science (medicine). (as doctors?)

Schäfer publishes two influential works: Essentials of Histology (1885) and
Endocrine Organs (1916) and founds the important Quarterly Journal of
Experimental Physiology in 1898.
After the tragic death of both his sons in World
War I Schäfer changed his own name to the hyphenated Sharpey-Schäfer taking
the last name of William Sharpey, his anatomy and physiology teacher.
(University College) London, England  
122 YBN
[1878 AD]
4195)
(Charité Hospital) Berlin, Germany  
121 YBN
[03/24/1879 AD]
3797)
(University of Uppsala) Uppsala, Sweden.  
121 YBN
[05/15/1879 AD]
3847)
Paris, France  
121 YBN
[07/22/1879 AD]
3690) Nordenskiöld also writes "Facsimile-atlas to the Early History of
Cartography" (1889) and "Periplus-An Essay on the Early History of Charts and
Sailing Directions" (1897) which lay the foundations of the history of
cartography.
Port Clarence, Alaska  
121 YBN
[08/22/1879 AD]
3681)
(British Association for the Advancement of Science)Sheffield, England  
121 YBN
[10/21/1879 AD]
4007) Thomas Alva Edison (CE 1847-1931), US inventor, creates a light bulb that
burns for 40 continuous hours.

(Sir) Joseph Wilson Swan (CE 1828-1914) had built an electric lamp that uses a
carbon fiber as a filament in 1860.

Edison finds finds that a burned cotton thread can function as a light bulb
filament for more time than other materials.

Edison had spent $50,000 and a year to realize that (the ultraexpensive)
platinum would not work as a filament.

In 1878, when Edison announces that he will solve the problem of producing
light from electricity, illuminating gas stock prices fall.

(private lab) Menlo Park, New Jersey, USA (presumably)  
121 YBN
[11/22/1879 AD]
5653)
(Johns Hopkins University) Baltimore, Maryland, USA  
121 YBN
[12/11/1879 AD]
3441)
(Tulse Hill)London, England  
121 YBN
[12/17/1879 AD]
3874)
(Science and Art Department) South Kensington, England  
121 YBN
[1879 AD]
3550) Abel is born in London, the son of a well-known musician.
Abel develops an early
interest in science after visiting his uncle A. J. Abel, a mineralogist and
pupil of Berzelius.
Abel studies chemistry for six years under A. W. von Hofmann at the
Royal College of Chemistry (established in London in 1845).
In 1852 Abel is appointed
lecturer in chemistry at the Royal Military Academy in Woolwich, succeeding
Michael Faraday, who had held that post since 1829.
In 1854 until 1888 Abel serves as
ordnance chemist at the Chemical Establishment of the Royal Arsenal at
Woolwich, establishing himself as the leading British authority on explosives.

Among Abel's books are - "Handbook of Chemistry" (with C. L. Bloxam), "Modern
History of Gunpowder" (1866), "Gun-cotton" (1866), "On Explosive Agents"
(1872), "Researches in Explosives" (1875), and "Electricity applied to
Explosive Purposes" (1884). Abel also writes several important articles in the
ninth edition of the Encyclopaedia Britannica.
(Royal Arsenal at Woolwich) Woolwich, England  
121 YBN
[1879 AD]
3687) In 1881 Wundt will found the first journal ("Philosophische Studien"
changed to "Psychologische Studien" in 1903) devoted to experimental
psychology.

His later works include "Hypnotismus and Suggestion" (1892), "Outline of
Psychology" (1896) and "Ethnic Psychology" (10 vol., 1900 – 20).
(University of Leipzig) Leipzig, Germany  
121 YBN
[1879 AD]
3719)
(Princeton University) Princeton, New Jersey, USA  
121 YBN
[1879 AD]
3730) Other important work by Stefan involves heat conduction in gases, and in
the theory of mutual magnetic effects of two electric currents. Stefan shows,
in opposition to Ampere and Grassman, that clear results can be achieved only
by means of the Faraday-Maxwell theory of continuous action. (more detail)
(Physical Institute, University of Vienna) Vienna, Austria  
121 YBN
[1879 AD]
3764)
(Moscow University) Moscow, Russia  
121 YBN
[1879 AD]
3782)
(home lab) Cognac, France (presumably)  
121 YBN
[1879 AD]
3796)
(University of Uppsala) Uppsala, Sweden.  
121 YBN
[1879 AD]
3853) For some time Flemming is an assistant to Willy Kuhne at the Institute of
Physiology in Amsterdam.
Flemming serves as physician on the Prussian side in
Franco-Prussion War of 1870.
(University of Kiel) Kiel, Germany  
121 YBN
[1879 AD]
3958)
Johns Hopkins University, Baltimore, Maryland, USA  
121 YBN
[1879 AD]
4064) Frege is an extreme nationalist (and racist) who hates all non-German
races.
According to the 2009 Encyclopedia Britannica: "Frege was, in religion, a
liberal Lutheran and, in politics, a reactionary. He had a great love for the
monarchy and for the royal house of Mecklenburg, and during World War I he
developed an intense hatred of socialism and of democracy, to which he came to
ascribe the loss of the war and the shame of the Treaty of Versailles. A diary
kept at the end of his life reveals, as well, a loathing of the French and of
Catholics and an anti-Semitism extending to a belief that the Jews must be
expelled from Germany."

With no regard to his racial beliefs, Frege's contributinos to science appear
to be somewhat overvalued in some sources - the 2009 Encyclopedia Britannica
has 7 pages on him.
(University of Jena) Jena, Germany  
121 YBN
[1879 AD]
4106)
(École Normale) Paris, France  
121 YBN
[1879 AD]
4183) In 1910 Kossel wins the Nobel prize in physiology and medicine for his
work on proteins and nucleic acids.
(University of Strasbourg) Strasbourg , Germany  
121 YBN
[1879 AD]
4196)
(Leipzig University) Leipzig, Germany (presumably)  
121 YBN
[1879 AD]
4231) According to Asimov, Neisser's attempts at inoculating against syphilis
may actually spread the disease instead. Neisser is accused of having
"maliciously inoculated innocent children with syphilis poison", and a scandal
results. Neisser mistakenly draws on an analogy with the serum therapy that
Behring had used against diphtheria and tetanus. Neisser inoculates young
prostitutes with what is probably highly a infectious serum. (voluntarily?)
(Oskar Simon’s clinic) Breslau, Germany  
120 YBN
[01/01/1880 AD]
4009)
(private lab) Menlo Park, New Jersey, USA   
120 YBN
[02/09/1880 AD]
3420)
(École Normale Supérieure) Paris, France  
120 YBN
[05/??/1880 AD]
3750)
(City University) New York City, NY, USA  
120 YBN
[06/03/1880 AD]
4038) inventors.about.com ends with the sentence "Bell's photophone is
recognized as the progenitor of the modern fiber optics that today transport
over eight percent of the world's telecommunications." - and perhaps this is
analogous to 8% of humans on earth see and hear thought - that amounts to about
480 million people of the 6 billion - and for the USA, 24 million of the 300
million people in the USA are allowed to pay for the service of seeing and
hearing thought. But we can only guess. An earlier estimate from insiders was
10% for the USA - 30 million "insiders" of the 300 million people living in the
USA.
(top of Franklin School) Washington, D. C., USA  
120 YBN
[06/17/1880 AD]
3829)
(Royal Institution) London, England   
120 YBN
[07/03/1880 AD]
4045)
(229 Broadway) New York City, New York, USA  
120 YBN
[09/20/1880 AD]
3845)
(Academy of Sciences) Paris, France  
120 YBN
[09/30/1880 AD]
3751)
(City University) New York City, NY, USA  
120 YBN
[09/??/1880 AD]
3759)
(University of Amsterdam) Amsterdam, Netherlands  
120 YBN
[10/10/1880 AD]
3577)
Newcastle, England (presumably)  
120 YBN
[11/23/1880 AD]
3948) In 1907, Laveran wins a Nobel Prize in physiology and medicine for his
finding concerning protists and disease.
Laveran's publishes many writings.
(Académie de Médecine) Paris, France  
120 YBN
[12/12/1880 AD]
3846)
(Academy of Sciences) Paris, France  
120 YBN
[1880 AD]
2691) The "Imperial Chinese Telegraph Company" (ICT) is founded by the Chinese
merchant Li Hongzhang in cooperation with the government.

(Tientsin (now Tianjin) or Shanghai?), China  
120 YBN
[1880 AD]
3512)
(Munich Polytechnic School) Munich, Germany  
120 YBN
[1880 AD]
3646)
?, France  
120 YBN
[1880 AD]
3768) In 1881 Beilstein is elected to the Russian Imperial Academy of Sciences,
while Mendeléev, Asimov cites as the greater scientist, is rejected. Asimov
claims that Russian science in the 1800s had a strongly pro-German and
anti-Russian orientation.
(University of St. Petersburg) St. Petersburg, Russia  
120 YBN
[1880 AD]
3810) Although close for many years, Breuer and Freud separate in 1896 and
never speak again due partly to quarrels over their work.
(in his own home?) Vienna, Austria (now Germany) (presumably)  
120 YBN
[1880 AD]
3812) Nicolas Camille Flammarion (FlomorEON) (CE 1842-1925), French astronomer
publishes "Astronomie populaire" (1880, tr. 1907; "Popular Astronomy"). Asimov
states that this is the best book of its kind produced in the 1800s.

In 1883 Flammarion creates a private observatory at Juvisy (near Paris) and
continues his studies, especially of double and multiple stars and of the moon
and Mars.
Flammarion also publishes several science fiction novels.
Flammarion writes a
500-page manuscript on the universe at a young age.
Flammarion takes the side of
advanced life and canals on Mars (and that all worlds are inhabited by living
beings).
In 1887, Flammarion founds the French Astronomical Society.
Flammarion's later
studies are on psychical research, on which he wrote many works, among them
"Death and Its Mystery" (3 vol., 1920–21; tr. 1921–23), and "Des Forces
naturelles inconnues" (1865; "Unknown Natural Forces").
Paris?, France  
120 YBN
[1880 AD]
3871)
(Science and Art Department) South Kensington, England  
120 YBN
[1880 AD]
3914)
(University of Jena) Jena, Germany  
120 YBN
[1880 AD]
4012)
(private lab) Menlo Park, NJ, USA   
120 YBN
[1880 AD]
4095)
(University of Berlin) Berlin, Germany  
120 YBN
[1880 AD]
4100) Milne has Japanese wife. (How unusual "touch and sex partner" sounds, but
yet, somewhat accurate.)
(Imperial College of Engineering) Tokyo, Japan  
120 YBN
[1880 AD]
4232)
(Oskar Simon’s clinic) Breslau, Germany (presumably)  
120 YBN
[1880 AD]
4348) Pierre is only 18 years old when he and Jacques discover piezoelectricity
but the brothers apparently do not publish until 1880.
Pierre Curie was run over by a
dray, a low heavy sideless cart, on a Paris street and died instantly in 1906.
Was this perhaps a murder?
(Sorbonne) Paris, France  
120 YBN
[1880 AD]
4549)
unknown  
120 YBN
[1880 AD]
4550)
unknown  
120 YBN
[1880 AD]
4551)
unknown  
120 YBN
[1880 AD]
4552)
unknown  
120 YBN
[1880 AD]
5839) In 1862 Röntgen entered a technical school at Utrecht, and is unfairly
expelled, accused of having produced a caricature of one of the teachers, which
was in fact done by somebody else.
Röntgen publishes 55 scientific papers in his
lifetime.
(University of Giessen) Giessen, Germany  
120 YBN
[1880 AD]
6011)
Moscow, (U.S.S.R. now) Russia (presumably) (verify)  
119 YBN
[01/05/1881 AD]
3608)
London, England (presumably)  
119 YBN
[02/05/1881 AD]
3877) In 1882, Abney is awarded the Rumsford medal for these researches.
(Science and Art Department) South Kensington, England  
119 YBN
[02/??/1881 AD]
3421)
(École Normale Supérieure) Paris, France  
119 YBN
[02/??/1881 AD]
3422)
(École Normale Supérieure) Paris, France  
119 YBN
[04/??/1881 AD]
4256) The son of a bookseller, Thomson enters Owens College, now the Victoria
University of Manchester when only 14 years old.
Asimov states that through
Thomson's direction and inspired teaching England maintains clear leadership in
the field of subatomic physics for the first 3 decades of the 1900s.
In 1906 Thomson
wins the Nobel prize in physics for work on the electon.
Seven of Thomson's research
assistants will win Nobel prizes.

Thomson's son,Sir George Paget Thomson (CE 1892–1975), will discover electron
diffraction, for which he shares the 1937 Nobel Prize for physics with Clinton
J. Davisson (1881–1958), who independently makes the same discovery.

In 1884 there was a transition from Lord Rayleigh, who had succeeded Maxwell,
as Cavendish Professorship of Experimental Physics, to Thomson. This may have
been a somewhat important transition from a wave interpretation of light to a
particle interpretation. According to the Complete Dictionary of Scientific
Biography, Thomson was surprised to be elected, and some of Thomson's
competitors, who included Fitzgerald, Glazebrook, Larmor, Reynolds, and
Schuster, were annoyed. Among the electors were Stokes, William Thomson, W. D.
Niven, and George Darwin.

In the course of his life, Thomson publishes over a hundred scientific papers.
(Trinity College) Cambridge, England  
119 YBN
[10/??/1881 AD]
4010)
(Paris International Exhibition) Paris, France   
119 YBN
[12/15/1881 AD]
3738)
(Solar Physics Observatory) South Kensington, England  
119 YBN
[1881 AD]
3043) Charles Robert Darwin (CE 1809-1882), English naturalist, publishes his
last major work "The Formation of Vegetable Mould, through the Action of Worms,
with Observations on Their Habits" (1881).

Downe, Kent, England (presumably)  
119 YBN
[1881 AD]
3330) Mortillet is a freethinker, takes part in Revolution of 1848 and is
forced to leave France in 1849.
(School of Anthropology) Paris, France  
119 YBN
[1881 AD]
3715)
(Gonville and Caius College, Cambridge University) Cambridge, England  
119 YBN
[1881 AD]
3793) Maxim is the eldest son of a farmer who is a locally notable mechanic,
and is apprenticed at 14 to a carriage maker.
Maxim has an early genius for invention,
and obtains his first patent in 1866, for a hair-curling iron.

Maxim spends time as a professional prize fighter.

For this generator Maxim receives the Legion of Honour from France.

In the 1890s Maxim experimented with airplanes, producing one powered by a
light steam engine that dies rise from the ground. Maxim recognizes that the
real solution to flight is the internal-combustion engine but did not develop
any.

Maxim receives 122 United States patents and 149 British patents.
Paris, France  
119 YBN
[1881 AD]
3907)
(International Medical Congress) London, England  
119 YBN
[1881 AD]
4040)
(Volta Lab) Washington, District of Columbia, USA  
119 YBN
[1881 AD]
4136) In 1886 Halsted is the first professor of surgery at Johns Hopkins
University, and establishes the first separate surgical school in the USA
there.
At Johns Hopkins, halsted develops original operations for hernia, breast
cancer, goitre, aneurysms, and intestinal and gallbladder diseases.
Halsted develops an
addiction to cocaine that requires 2 years to stop. But people of this
draconian age should remember that drug addiction is no reason to be
imprisoned, and certainly not for more than a week until an addiction is
physically gone.
Halsted is particularly noted for his skill in breast amputations.
Halsted sends
his shirts to Paris to have then laundered.
New York City, NY, USA  
119 YBN
[1881 AD]
4157)
(University of Berlin) Berlin, Germany  
119 YBN
[1881 AD]
4349)
(Sorbonne) Paris, France  
118 YBN
[01/12/1882 AD]
4011)
(57 Holborn Viaduct) London, England   
118 YBN
[01/14/1882 AD]
4013)
(Crystal Palace) Syndenham, England   
118 YBN
[02/??/1882 AD]
3996)
(University College) Bristol, England  
118 YBN
[03/24/1882 AD]
3903) In 1905 Koch will win the Nobel Prize in medicine and physiology for
findings relating to tuberculosis.
(Imperial Department of Health) Berlin, Germany  
118 YBN
[03/??/1882 AD]
3752)
(City University) New York City, NY, USA (presumably)  
118 YBN
[05/25/1882 AD]
4066)
(Johns Hopkins University), Baltimore, Maryland, USA  
118 YBN
[07/17/1882 AD]
4825)
(Royal College of Science) Dublin, Ireland  
118 YBN
[09/04/1882 AD]
4014)
(Edison Electric illuminating Company, 255 and 257 Pearl Street), New York
City, NY, USA   
118 YBN
[12/??/1882 AD]
3620)
(Tuft's College) Boston, Massachusetts, USA  
118 YBN
[1882 AD]
3513)
(Munich Polytechnic School) Munich, Germany  
118 YBN
[1882 AD]
3515)
(Munich Polytechnic School) Munich, Germany  
118 YBN
[1882 AD]
3516) Jean Martin Charcot (soRKO) (CE 1825-1893), French physician Charcot
presented a summary of his findings on the phenomenon of mesmerism to the
French Academy of Sciences, where they are favorably received, in this way the
phenomenon of mesmerism (hypnotism) is officially recognized as a real and
legitimate phenomenon.

In his study of muscular atrophy, Charcot described the symptoms of locomotor
ataxia, a degeneration of the dorsal columns of the spinal cord and of the
sensory nerve trunks. He is also first to describe the disintegration of
ligaments and joint surfaces (Charcot’s disease, or Charcot’s joint) caused
by locomotor ataxia and other related diseases or injuries. (chronology)


Charcot uses the techniques of mesmerism (hypnosis) that Braid had introduced,
to treat hysteria. Charcot studies the cure of hysterical disorders
(psychoneuroses). These disorders involve what appear to be physiological
disturbances such as convulsions, paralyses, blindness, deafness, anesthesias,
and amnesias. However, there is no evidence of physiological abnormalities in
psychoneuroses since the root of the problem is psychological (or based on
badly ordered neuron connections, as opposed to physical problems with neurons
or neuron connections themselves). In Charcot's time hysteria is thought to be
a disorder found only in women (the Greek word hysterameans uterus). Charcot
continues to think of hysteria as a female disorder.

One of the major problems for psychology in this time is determining whether
behavioral abnormalities originate in psychological or in physiological
disturbances and, if physiological, where in the central nervous system the
abnormality might be located. Charcot becomes noted for his ability to diagnose
and locate the physiological disturbances of nervous system functioning.
Charcot conducts pioneering research in cerebral localization, the
determination of specific sites in the brain responsible for specific nervous
functions, and discovers miliary aneurysms (dilation of the small arteries
feeding the brain), demonstrating their importance in cerebral hemorrhage.
(How was this done, with electronic devices?)
(To me, hysteria is a questionable disease,
in addition to being somewhat trivial and open to abuse in the form of forced
treatment. People can be frantic, overly excited perhaps, but it usually does
not last in my experience, and is not something that I interpret as an
abnormality or disease, but as a natural, albeit maybe annoying, physical part
of genetic structure or the result of learning.)


(Neurology is an actual science, psychology is a dubious science, but as long
as it is consensual only and not used as an excuse to imprison people {for
which only law is a valid excuse, and then, the dubious theories of psychology
should not serve as the basis for any law in my opinion}, I think psychology
should be legal. The value of psychology is very doubtful to me, but if people
enjoy the drugs, or consensual only treatments of those in psychology I see no
reason to outlaw it, and perhaps there is a beneficial purpose, if people truly
feel they are being helped, as is the case for any drug or substance that
directly harms no other person.)

(Between neurology and psychology there is a fine line, which separates these
two as completely different sciences. I think it is important to be able to
distinguish between the two.)

(Does Charcot forcibly treat? drug? restrain? objecting people?)
Charcot is with
Guillaume Duchenne one of the founders of modern neurology.

In 1862 Charcot establishes a major neurological department at La Salpêtrière
Hospital for nervous and mental disorders.
In 1887 Charcot writes, "What I call psychology
is the rational physiology of the cerebral cortex.". Charcot gives impetus to
the new field (of psychology) with the creation, in 1890, of the Laboratory of
Psychology at the Salpêtrière hospital.

In 1885 one of Charcot's students is Freud who also becomes interested in
treating hysteria with hyponotism.

Charcot’s writings include "Leçons sur les maladies du système nerveux", 5
vol. (1872–83; "Lectures on the Diseases of the Nervous System") and "Leçons
du mardi à la Salpêtrière" (1888; "Tuesday Lessons at the Salpêtrière").
Paris, France  
118 YBN
[1882 AD]
3528)
(University of Copenhagen) Copenhagen, Denmark  
118 YBN
[1882 AD]
3579)
(Owens College) Manchester, England (presumably)  
118 YBN
[1882 AD]
3588)
(College de France) Paris, France (presumably)  
118 YBN
[1882 AD]
3854)
(University of Kiel) Kiel, Germany  
118 YBN
[1882 AD]
3908)
(Imperial Department of Health) Berlin, Germany  
118 YBN
[1882 AD]
3947) According to Asimov, Mechnikov has poor eyesight, and a violent temper.

After his wife dies, Mechnikov tries to end his own life by swallowing a large
dose of opium, but does not die.

Virchow is not impressed after a demonstration of phagocytes.
In 1888 Pasteur invites the
Russian Mechnikov to join the Pasteur Institute which Mechnikov does. (The
French version of Ilya is Élie Metchnikoff.)
In 1895 On Pasteur's death Mechnikov succeeds
Pasteur as director of the Institute.
Mechnikov believes that the natural
lifespan of humans is 150 years and that drinking cultured milk helps a person
attain it.
In 1908 Mechnikov shares a Nobel Prize with Paul Ehrlich for their
researches illuminating the understanding of immunity.

Mechnikov publishes "The Comparative pathology of inflammation" (1892) and
"Immunity in infectious diseases" (1901).

Mechnikov's later years are largely centered studying aging factors in humans
and methods of inducing longevity, which are discussed in "The Nature of Man"
(1904) and "The Prolongation of Human Life" (1910).

One biography of Metchnikoff was made by his wife, Olga Metchnikoff, "Life of
Élie Metchnikoff" (trans. 1921).
(In his own private laboratory) Messina, Italy  
118 YBN
[1882 AD]
3956) Hall initially intended to enter the ministry. Hall is inspired by a
partial reading of Physiological Psychology (1873–74), by Wilhelm Wundt,
generally considered the founder of experimental psychology. Hall then studies
in Germany becoming acquainted with Wundt and the German physicist and
physiologist Hermann von Helmholtz. There Hall discovers the value of the
questionnaire for psychological research. Hall and his students will devise
more than 190 questionnaires which stimulate the field of child development.
(Interesting that psychology started in Germany and spread to other nations.)

In 1878, Hall earns, from Harvard University, the first Ph.D. degree in
psychology in America. (To me this shows the seeds and growth of what in some
sense can be seen as a cancer, until made "strictly-consensual only" health
care, or certainly at least "treatment with no-objection only" health care. The
inaccurate claims of pscyhological disorders have slowed the stopping of
violence - since those who tell the truth about the JFK, MLK, RFK, 9/11 murders
are labeled as "insane", and the murderers continue to live free and unknown by
the majority. In addition the stigma and fear of being labeled with a
psychological disorder has slowed creativity and diversity. Beyond this, the
locking up of humans without trial, injecting with drugs, restraining, and
holding indefinitely all violate the most basic principles of the 1200s habeus
corpus law and many other basic laws and principles.)

Hall pioneers the study of child psychology. (psychology as applied to adults
and children too is in large part a total pseudoscience, as far as I can see.
Perhaps there is value in examining patterns of behavior and certainly
understanding physiological development in humans and other species.)

Hall gives an early impetus and direction to the development of psychology in
the United States and is frequently regarded as the founder of child psychology
and educational psychology. Hall promotes the ideas of Sigmund Freud.

In 1888 Hall helps to establish Clark University in Worcester, Massachusetts,
and becomes the university's president and a professor of psychology. (This
shows how pseudoscience, and involuntary torture was still very respectable in
1889 and is even today.)

(documentation of people in psychology serves more to track the growth and
development of pseudoscience industries, and has little if anything to do with
actual science (for example sciences of health and healing). However, I think,
if voluntary only, psychology, although with fraudulent, highly abstract and
speculative theories rarely based on factual science, may serve as experiment,
mainly in drugs (and other non-violent, voluntary only methods, such as talk,
computer games, etc) might serve to create new drugs that some people enjoy
voluntarily and find helpful in solving abstract ununderstood individually
perceived problems.)

(I think the question for psychology is, who tortured/treated involuntarily and
who did not? and in addition, who subscribed to pseudoscience erroneous
theories? who worked against those aims? I think those in psychology need to
work on a different definition of "voluntary-only experimental
treatment/therapy for unknown disease or unwanted behavior, thoughts or
beliefs". The key idea is "voluntary only".)

(I equate the history of psychology similar to the history of message therapy,
although message therapy probably has less inaccurate claims, and certainly no
involuntary injection or torture. Perhaps a closer comparison is the history of
prisons and treatment of prisoners.)

(Clark, as is the case with many soft-science people appears to me to be highly
over-valued with many biographies, but few actual science contributions, and
possibly undocumented human rights violations such as involuntary drugging,
restraint, electrocution, etc.)

(One interesting book title by Hall: Jesus, the Christ, in the Light of
Psychology (1917). This appears to describe how people have drawn Jesus over
the centuries and how Jesus was protrayed to reflect some belief. Possibly
there are minor anti-religious, or exposing the truth about religions,
contributions there.)

(I think that in the transition from religions to science, much if not all of
psychology will probably fall to the past as more and more people focus on
science and accurate analysis of the universe.)
Johns Hopkins University, Baltimore, Maryland, USA  
118 YBN
[1882 AD]
3965)
Harvard College Observatory, Cambridge, Massachusetts, USA  
118 YBN
[1882 AD]
4015)
(private lab) Menlo Park, New Jersey, USA (presumably)  
118 YBN
[1882 AD]
4061)
(University of Zurich), Zurich, Switzerland (presumably)  
118 YBN
[1882 AD]
4126) Lindemann spends 6 years trying to solve Fermat's last theorem, and in
1907 publishes a very long paper in which he claims to have succeeded, however
there is an error in the beginning.
(University of Freiburg) Freiburg, Germany  
118 YBN
[1882 AD]
4130) Löffler works in the same laboratory with Koch for a period of time.
(Imperial Health Office) Berlin, Germany  
118 YBN
[1882 AD]
4805)
London, England  
118 YBN
[1882 AD]
6029)
Paris, France (guess)  
117 YBN
[01/??/1883 AD]
3733)
(University College Hospital) London, England  
117 YBN
[03/05/1883 AD]
3880)
(Science and Art Department) South Kensington, England  
117 YBN
[03/??/1883 AD]
4070)
(laboratory of brewer Carl Jacobsen) Kopenhagen, Denmark  
117 YBN
[04/09/1883 AD]
3955) Wroblewski endured a six-year exile (in Siberia) for participating in the
January Uprising (1863), an unsuccessful Polish rebellion against Russian
rule..

In 1888, while working on the physical properties of hydrogen, Zygmunt
Wróblewski is heavily burned and dies soon afterwards at a Krakow hospital.
Jagiellonian University, Krakow, Austria (now Poland)  
117 YBN
[05/24/1883 AD]
3683)
(Bakerian Lecture, Royal Society) London, England  
117 YBN
[05/26/1883 AD]
4076) Fleming was the author of more than a hundred scientific papers and
books, including the influential "The Principles of Electric Wave Telegraphy"
(1906) and "The Propagation of Electric Currents in Telephone and Telegraph
Conductors" (1911).
(Edison Electric Light Company) London, England  
117 YBN
[06/06/1883 AD]
4339) In 1903 Arrhenius is awarded the Nobel prize in chemistry.
(Institute of Physics of the Academy of Sciences) Stockholm, Sweden  
117 YBN
[11/15/1883 AD]
4016)
(private lab) Menlo Park, New Jersey, USA  
117 YBN
[1883 AD]
3400)
London, England (presumably)  
117 YBN
[1883 AD]
3407)
(University of Liepzig) Liepzig, Germany (presumably)  
117 YBN
[1883 AD]
3578)
Newcastle, England (presumably)  
117 YBN
[1883 AD]
3629) In 1850 Suess is imprisoned for being on the side of the liberals during
a revolution in 1848. Another source has Suess imprisoned simply for
participating in revolutionary demonstrations of 1848.
In 1856, Suess is appointed
extraordinary professor of paleontology at the University of Vienna without a
doctorate degree.
From 1873 on, Suess spends 30 years in the Austrian
legislature.
(University of Vienna) Vienna, Austria (now Germany)  
117 YBN
[1883 AD]
3699) When World War I starts Weismann renounces all his British honors and
awards.
(University of Freiburg) Freiburg, Germany  
117 YBN
[1883 AD]
3710) In 1872 Daimler becomes technical director in the firm of Nikolaus A.
Otto, the man who had invented the four-stroke internal-combustion engine.
In 1882
Daimler and his coworker Wilhelm Maybach left Otto's firm and started their own
engine-building shop.
In 1890 Daimler founds the Daimler motor company.
in 1899, the Daimler
motor company produces the first Mercedes automobile, which is named for the
daughter of the financier backing Daimler.
(factory) Stuttgart, Germany  
117 YBN
[1883 AD]
3771)
(Charles University) Prague, Czech Republic  
117 YBN
[1883 AD]
3794) (Maxim's shop, Hatton Garden) London, England  
117 YBN
[1883 AD]
3815) More than half of these 4051 stars proof to be of Secchi's first type
(represented by Sirius, Vega, Altair and other bluish-white stars,
characterized by the intensity of the hydrogen lines). (Probably because they
are the brightest and easiest to see.)
(Astrophysical Observatory at Potsdam) Potsdam, Germany  
117 YBN
[1883 AD]
3865)
(University of Pavia) Pavia, Italy  
117 YBN
[1883 AD]
3904)
(Imperial Department of Health) Berlin, Germany  
117 YBN
[1883 AD]
3916)
(University of Liege) Liege, Belgium  
117 YBN
[1883 AD]
3959)
University of Liège, Liège, Belgium  
117 YBN
[1883 AD]
3987) George Westinghouse (CE 1846-1914) US engineer, applies his knowledge of
air brakes to the problem of safely piping natural gas.

Westinghouse develops a system of transporting gases through pipes over long
distances, which makes gas ovens and gas furnaces practical.

This work enables Westinghouse to understand the problems involved in
distributing electrical power.

(Westinghouse Air Brake Company) Pittsburg, PA, USA (presumably)  
117 YBN
[1883 AD]
4044)
(Volta Lab) Washington, District of Columbia, USA  
117 YBN
[1883 AD]
4072)
(Military Medical Academy), St. Petersburg, Russia  
117 YBN
[1883 AD]
4203)
(Physiology Institute) München, Germany  
117 YBN
[1883 AD]
4245) Tesla is from a family of Serbian origin. Tesla's father is an Orthodox
priest; and Tesla's mother is an unschooled but highly intelligent.

The unit of magnetic flux density (symbol B) is named the tesla in Tesla's
honor.
Magnetic flux density is the amount of magnetic flux through a unit area
taken perpendicular to the direction of the magnetic flux. Also called magnetic
induction. Magnetic flux is defined as the quantity of magnetism, being the
total number of magnetic lines of force passing through a specified area in a
magnetic field. (Those lines are presumably lines of particles in my opinion,
however, this is not explicitly stated by authoritative sources.)
(In particle terms,
perhaps the magnetic flux density is the quantity of particles in an electric
current summed over an area of space which includes various mediums - like
metals, and air in addition to the empty space surrounding an electromagnetic
conductor.)

In 1932 Tesla publicly rejects the theory that space can be curved stating in
the New York Herald Tribune:
"I hold that space cannot be curved, for the
simple reason that it can have no properties. It might as well be said that God
has properties. He has not, but only attributes and these are of our own
making. Of properties we can only speak when dealing with matter filling the
space. To say that in the presence of large bodies space becomes curved is
equivalent to stating that something can act upon nothing. I, for one, refuse
to subscribe to such a view ...". (verify) (I reject the curvature of space,
because in particular, surface geometry is actually a subset of Euclidean
geometry, in addition to a simple 4 variable universe seems more logical,
intuitive and simple to me.)

In 1935 Tesla critisizes Einstein's relativity work, calling it a:
"...
magnificent mathematical garb which fascinates, dazzles and makes people blind
to the underlying errors. The theory is like a beggar clothed in purple whom
ignorant people take for a king ... its exponents are brilliant men but they
are metaphysicists rather than scientists ...".

Many sources claim Tesla is insane in later life, but I think people need to
put things into perspective and realize that there is a lot of propaganda and
money put towards the many times completely inaccurate myth that all scientists
are insane (for example, the "nutty professor"), much of this comes from an
anti-science anti-technology group, in particular those trying to preserve
traditional religions. In addition, when people talk about Tesla's unusual
activities, why are these no comparisons to the illogical nature of praying to
a person who died hundreds of years ago before going to sleep as thousands do?
Worshipping relics of the past as if they had supernatural properties...beliefs
in superstitions...horoscopes...fortune telling...palm reading.... or to
worshipping a person who died thousands of years ago every 7 earth
rotations....all activities which are based on very inaccurate and doubtful
theories and beliefs - while perhaps common and popular...they are certainly
not sane in the sense of being logical, accurate, and wise activities. Beyond
this, at least Tesla never resorts to violence - so no matter what inaccurate
beliefs, they never resulted in violence - Tesla and many others labeled with
pseudoscience psychiatric disorders express strong will power and control to
not engage in first-strike violence against non-violent people, while many
so-called sane people show much less restraint.

In later life Tesla breeds pigeons and lavishes his affection on them. (I
wonder how much is beyond simply a hobby and love for birds. I think there is a
tradition to make usual behavior appear unusual if there is a myth about
insanity.)
Tesla fights a long battle with Marconi over priority in the invention of
radio.

Asimov states that the last 25 years of Tesla's life degenerated into wild
eccentricity. (Tesla tries to develop a method of transporting electricity
without wires and would not give up, and Westinghouse eventually stops funding
Tesla.)

While at his Colorado laboratory, Tesla announced that he had received signals
from foreign planets, a statement that is greeted with some skepticism.
Encyclopedia Britannica states that this claim is met with derision in some
scientific journals. This appears to originate from a January 7, 1900 letter,
Tesla writes to the Red Cross stating that he received a message that signaled
"one ... two ... three ...".

Among Tesla's public claims are: 1) communication with other planets, 2) his
assertions that he could split the Earth like an apple, and 3) his claim of
having invented a death ray capable of destroying 10,000 airplanes at a
distance of 250 miles (400 km).
Strasbourg, France  
117 YBN
[1883 AD]
4304) Tsiolkovsky has permanently impaired hearing at age nine as a result of
scarlet fever and four years later his mother dies.
In 1881 Tsiolkovsky works out the
kinetic theory of gases, unaware that Maxwell had already done this 25 years
earlier. (interesting that they both reach the same conclusion that velocity of
particles is heat, while there still exists a potential problem with a constant
velocity for photons {or perhaps x or some smaller particle} which may be the
basis for all matter, although I have doubts about a constant velocity for any
material object, and there are possibilities for a constant velocity for
material particles. I view all particles as material. In addition to velocity,
clearly quantity of space and matter plays a part in my opinion.)
In 1895 Tsiolkovsky's
book "Gryozy o zemle i nebe" (Dreams of Earth and Sky) is published.
In 1896 Tsiolkovsky
publishes an article on communication with inhabitants of other planets and
starts to write his largest and most serious work on astronautics, "Exploration
of Cosmic Space by Means of Reaction Devices", which deals with theoretical
problems of using rocket engines in space, including heat transfer, a
navigating mechanism, heating resulting from air friction, and maintenance of
fuel supply.

Tsiolkovsky writes a science fiction novel "Outside the Earth".
Asimov indicates
Tsiolkovsky is held back by the scientific backwardness of Tsarist Russia.
(there are few people that contribute to science in Russia, but then perhaps
like China there is a language barrier. Some in math, and Mendeleev.)
Twenty-two years
after his death the Soviet government plans to launch the first human-made
satellite, Sputnik 1, on the 100th anniversary of Tsiolkovsky's birth, but is
29 days late.
Tsiolkovsky's grave has the phrase "Mankind will not remain tied to
earth forever".
Borovsk, Russia  
117 YBN
[1883 AD]
4336)
(Steel Works Company) Sheffield, England (presumably)  
117 YBN
[1883 AD]
6025) Léo Delibes (CE 1836-1891), French opera and ballet composer, composes
the opera "Lakmé".

Paris, France (presumably)  
116 YBN
[01/06/1884 AD]
3621) Nipkow studies physiological optics with Hermann von Helmholtz, and
physiological optics and electro-physics with Adolf Slaby.
Berlin, Germany   
116 YBN
[01/11/1884 AD]
3859)
(Royal Observatory) Cape of Good Hope, Africa  
116 YBN
[03/07/1884 AD]
4209) When younger Eastman read in British magazines that photographers make
their own gelatin emulsions. Plates coated with this emulsion remain sensitive
after they are dry and can be exposed at any time later as opposed to wet
plates. Using a formula taken from one of these British journals, Eastman
begins making gelatin emulsions.

Eastman starts his business manufacturing dry plates in April 1880.

Clearly Eastman's work is on the side of bringing captured images to the public
- although these images are mainly only of the visible spectrum and do not
include images or sound recordings of thoughts - Eastman's work clearly brings
these awesome truths many steps closer to the public. How deeply was Eastman
involved in neuron reading and writing? Only the remaining historical secret
movies might tell us. In Eastman's October 5, 1884 patent, eastman uses the
words "tension" and "web", which imply either an awareness of 1810 and the
wireless internet, or perhaps an echoing of neuron writing done to Eastman
without his knowledge.
Eastman is from poor parents, and by working supports himself at
age 14.
Eastman, as head of a large business, introduces sickness benefits,
retirement annuities, and life insurance for his employees, long before these
are popular. Eastman is also one of the first to introduce the idea of profit
sharing as employees incentive.
Eastman gives away half his fortune in 1924 in gifts
totaling more than $75,000,000.
Eastman donates $54 million to the University of Rochester,
and $19 million to the Massachusetts Institute of Technology so that others may
receive the education he never had.
Eastman systematically gives money to the
University of Rochester (especially the medical school and Eastman School of
Music), Massachusetts Institute of Technology, Hampton Institute, Tuskegee
Institute, Rochester Dental Dispensary, and European dental clinics.

Interesting that Eastman donates to education and not religions.

In 1932, Eastman ends his own life at age 77, leaving a note with the words,
"My work is done. Why wait?".

Eastman's house in Rochester, now known as the George Eastman House, has become
a renowned archive and museum of international photography in addition to a
popular tourist site.


(Eastman's death sounds very suspicious. In particular in an era of secret
neuron reading and writing. This was just before world war 2, and perhaps the
message was written by the murderers with the last word "why wait" - perhaps
hinting - this is why people should wait to show and tell the public about
neuron reading and writing and the massive injustice of a two tier planet where
one group of people sees a square with the thought-images above the head of
each person, while the other group of people does not even know such technology
has existed for hundreds of years. In addition, "ww" might be some reference to
William Wollaston who may have been the first to see and/or hear thought images
and sounds, and finally a reference to "world war" and an appeal to nationalism
and secrecy for the ironic cause of national security.

The kodak.com webpage states that Eastman "... was a modest, unassuming man...
an inventor, a marketer, a global visionary, a philanthropist, and a champion
of inclusion." - notice "inclusion" - clearly Eastman brought the average
person closer to seeing inside houses and heads than many people.
(Eastman Dry Plate Company) Rochester, NY, USA  
116 YBN
[04/23/1884 AD]
4206) Charles Parsons is the youngest son of the famous astronomer William
Parsons, 3rd Earl of Rosse.
In retirement Parsons tries unsuccessfully to make
diamonds.
(Clarke, Chapman and Company) Gateshead, England  
116 YBN
[08/10/1884 AD]
4047) In 1910 Wallach is awarded a Nobel in chemistry for his work on
terpenes.
In his life Wallach publishes 126 papers on the terpenes.
At the start of World War I six
of Wallach's assistants are killed in action.
(University of Bonn) Bonn, Germany  
116 YBN
[1884 AD]
3398)
London, England   
116 YBN
[1884 AD]
3787)
(Freiberg School of Mining) Freiberg, Germany  
116 YBN
[1884 AD]
3831)
(Royal Institution) London, England   
116 YBN
[1884 AD]
3905)
Egypt|India (more specific)  
116 YBN
[1884 AD]
3906)
(Imperial Department of Health) Berlin, Germany (presumably)  
116 YBN
[1884 AD]
3926) Perhaps there should be distinguished a difference between a "black
body", an "all color emitting body" and a total reflective body.
(University of Graz) Graz, Austria   
116 YBN
[1884 AD]
4042)
Boston and New York (City?), USA  
116 YBN
[1884 AD]
4080)
(Imperial Health Office) Berlin, Germany  
116 YBN
[1884 AD]
4097) Le Châtelier is the first to translate the work of Gibbs into French.
(École des Mines) Paris, France  
116 YBN
[1884 AD]
4107)
(École Normale) Paris, France  
116 YBN
[1884 AD]
4131)
(Imperial Health Office) Berlin, Germany  
116 YBN
[1884 AD]
4182)
(lab of microbiologist Karl Friedländer ) Berlin, Germany  
116 YBN
[1884 AD]
4184)
(University of Berlin) Berlin, Germany  
116 YBN
[1884 AD]
4185) (University of Berlin) Berlin, Germany  
116 YBN
[1884 AD]
4315)
(General Hospital in Vienna) Vienna, Austria  
115 YBN
[01/30/1885 AD]
3500) Balmer teaches at a girl's school in Basel.
From 1865-1890, Balmer also
lectures on geometry at the University of Basel.
Balmer reports his find at age 60.
(Secondary School) Basel, Switzerland  
115 YBN
[05/23/1885 AD]
4017) It is interesting to note that at this time, there has been no
heavier-than-air vehicle, rockets that go above the earth atmosphere, or
photographs of the earth from orbit.
(private lab) Menlo Park, New Jersey, USA  
115 YBN
[07/27/1885 AD]
4078)
(University College) London, England  
115 YBN
[07/??/1885 AD]
3827)
(father's ironworks) Chatillon, France (presumably)  
115 YBN
[1885 AD]
3711)
(factory) Stuttgart, Germany  
115 YBN
[1885 AD]
3712)
(factory) Stuttgart, Germany  
115 YBN
[1885 AD]
3866)
(University of Pavia) Pavia, Italy  
115 YBN
[1885 AD]
3967)
Harvard College Observatory, Cambridge, Massachusetts, USA  
115 YBN
[1885 AD]
3985) From 1885-1888 Pickering is vice president of the American Society for
Psychical Research and serves on the society's Committee on Thought
Transference. Pickering participates in the statistical analysis of experiments
in telepathy using cards, dice, and numbers, a precursor to the methods later
championed by parapsychology. That the science of seeing, hearing and sending
images and sonuds to and from brains got mixed into psychology is an
interesting phenomenon, because on the negative side, it is more easily
dismissed as outlandish pseudoscience, however, on the positive side, it allows
people to talk publicly about the concept of seeing, hearing and sending images
and sounds to and from brains. After the publication of Kamitani and others in
December, 2008, talking about seeing, hearing and sending images and sounds too
and from brains is entering into non-psychology scientific and public
discussion. Pickering writes: "Possibility of Errors in Scientific Researches,
Due to Thought-Transference." and "Discussion of Returns in Response to
Circular No. 4.". Possibly there are solid hints about the names, dates and
other events surrounding the secrets surrounding the seeing, hearing and
sending images and sounds to and from brains and remote muscle contraction
(galvanization) in these works.
Bostom, Massachusetts, USA  
115 YBN
[1885 AD]
3990) George Westinghouse (CE 1846-1914) US engineer, imports a set of
Gaulard-Gibbs transformers and a Siemens AC generator and creates an AC
electrical distribution system in Pittsburgh.

Perhaps the distribution of gas and electricity led to the distribution of
secret microphones, cameras, neuron activation devices, etc.? Perhaps
Westinghouse served as an alternative neuron zapper to the phone company. In
the biography, "His Life and Achievements" there is no "galvanize", but there
is "camera" and "confederate" in the same sentence.

State how many people receive electricity and/or gas from Westinghouse to show
growth of gas and electricity distribution systems (along with telephone).
There are at least two alternatives in providing people electricity, gas, and
other services: 1) send the electricity or gas to them all from a central
location, or 2) they produce their own electricity and/or gas individually.

(Westinghouse Air Brake Company (presumably)) Pittsburg, PA, USA   
115 YBN
[1885 AD]
4132)
(hygienic laboratory at the First Garrison Hospital) Berlin, Germany  
115 YBN
[1885 AD]
4137)
New York City, NY, USA  
115 YBN
[1885 AD]
4329) Auer's baronal motto is "more light".
(University of Vienna) Vienna  
115 YBN
[1885 AD]
4330)
(University of Vienna) Vienna  
115 YBN
[1885 AD]
4388) Bateson translates Mendel's papers into English.
(St. John’s College) Cambridge, England  
115 YBN
[1885 AD]
4461)
(Royal Observatory of Brusells) Bruselles, Belgium  
114 YBN
[02/23/1886 AD]
4431) Hall's teacher stated that any body that can find a cheap way of making
aluminum would grow rich and famous.

After several failures to interest financial backers, Hall obtains the support
of the Mellon family, and the Pittsburgh Reduction Company (later the Aluminum
Company of America) is formed. In 1890 Hall becomes the company's first vice
president. Hall leaves Oberlin more than $5,000,000 after his death.
(Oberlin (Ohio) College Hall) Oberlin, Ohio, USA  
114 YBN
[04/??/1886 AD]
4415)
(family tannery) Gentilly, France  
114 YBN
[05/03/1886 AD]
3881)
(Science and Art Department) South Kensington, England (verify)  
114 YBN
[06/26/1886 AD]
4139) In 1906 Moissan wins a Nobel prize in chemistry for isolating Fluorine
(winning over Mendeléev by one vote, who Asimov argues, probably deserves the
prize more).
(École Supérieure de Pharmacie) Paris, France  
114 YBN
[07/27/1886 AD]
4096)
(University of Berlin - verify) Berlin, Germany  
114 YBN
[1886 AD]
3145) Gabriel Auguste Daubrée (DOBrA) (CE 1814-1896), French geologist,
categorizes meteorites and gives information on their composition, relationship
to terrestrial rocks, and their change in shape in passing through the Earth
atmosphere in "Météorites et la constitution géologique du globe"
("Meteorites and the Geologic Constitution of the World").

Paris, France  
114 YBN
[1886 AD]
3170)
(University of Berlin) Berlin, Germany  
114 YBN
[1886 AD]
3426) Kronecker is a Jewish professor at the University of Berlin starting in
1861 (even though not a Christian).
(University of Berlin) Berlin, Germany  
114 YBN
[1886 AD]
3625)
(University of Grenoble) Grenoble, France  
114 YBN
[1886 AD]
3632)
Anhalt-Bernburg, Germany  
114 YBN
[1886 AD]
3741)
(Solar Physics Observatory) South Kensington, England (presumably)  
114 YBN
[1886 AD]
3769)
(University of St. Petersburg) St. Petersburg, Russia  
114 YBN
[1886 AD]
3783)
(home lab) Cognac, France (presumably)  
114 YBN
[1886 AD]
3786)
(Freiberg School of Mining) Freiberg, Germany  
114 YBN
[1886 AD]
3799) Krafft-Ebing is professor of psychiatry (Is called psychiatry?) at
Strasbourg (1872), Graz (1873), and Vienna (1889).

Krafft-Ebing is the director of an insane asylum in Graz.
Krafft-Ebing
publishes a textbook on psychiatry that goes through seven editions in his
lifetime. (Is the issue of consent ever raised? For example the view that
psychiatric disorder can be treated without consent? This concept is still
popular - the view that the decision and opinions, in particular the objection
of a person with a psychiatric disorder can be overruled, ignored, etc - is
like the opinion of a lesser species or possessed victim who doesn't know what
is good for themselves.)
Krafft-Ebing performs experiments in hypnosis.
(One interesting view of
psychology is that, the view I have of psychology, is that, consent is
required, or at least objection must be honored. In terms of crime, I view the
reasons why as secondary, as opposed to the modern system which views supposed
root causes as more important than punishment of crimes. So I reject the
approach where a person violating a law goes through a decision branch between
unconsensually to a jail and a hospital, anywhere along the line of the penal
process. In my view it must always be jail only, and then if people want to
consensually only offer health services geared towards reducing the repetition
of another similar crime that if fine. So I basically reject the verdict of
non-responsible because of insanity - although I accept the concept of
different levels of intent and responsibility.)
Graz, Austria  
114 YBN
[1886 AD]
3989) George Westinghouse (CE 1846-1914) US engineer, organizes the
Westinghouse Electric Company.

Westinghouse supports the side of alternating current (as opposed to direct
current supported by Edison).

Westinghouse acquires European patents covering single-phase
alternating-current transmission and buys the patents of Nikola Tesla's AC
motor (in May 1885).

Westinghouse hires Tesla to improve and modify the motor for use in
Westinghouse's power system..

(Do all nations use alternating current?)
(Could have Edison and Westinghouse provided
both AC and DC? There probably were patent limits with AC, although it seems,
like DC too simple and old to be patented.)

(Westinghouse Electric Company) Pittsburg, PA, USA (presumably)  
114 YBN
[1886 AD]
4099) Hans is the brother of Eduard Buchner who will win a Nobel prize.
(University of Munich) Munich, Germany  
114 YBN
[1886 AD]
4135)
(University of Amsterdam) Amsterdam, Netherlands  
114 YBN
[1886 AD]
4168) Petrie theorizes about the origin of the alphabet in "The Formation of
the Alphabet" (1912). His views the origin of the alphabet create strong
opposition.
Nile River Delta, Egypt  
114 YBN
[1886 AD]
4197)
(Charité Hospital) Berlin, Germany (presumably)  
114 YBN
[1886 AD]
4359)
(Columbian University, now George Washington University), Washington, D.C,
USA  
114 YBN
[1886 AD]
6006) (Charles) Camille Saint-Saëns (CE 1835-1921), French composer, pianist
and organist, composes "Le carnaval des animaux" ("The Carnival of The
Animals").

Saint-Saens is outspoken against the music of Claude Debussy and the French
impressionist school.

Austria (verify)  
113 YBN
[02/21/1887 AD]
4122)
London, Ontario, Canada  
113 YBN
[03/04/1887 AD]
3713)
(factory) Stuttgart, Germany  
113 YBN
[03/??/1887 AD]
4285)
(University of Karlsruhe) Karlsruhe, Germany  
113 YBN
[05/02/1887 AD]
3762)
Newark, New Jersey  
113 YBN
[05/??/1887 AD]
4286) (Hertz's full paper:)
Hertz writes in (an English translation) "On An Effect of
Ultra-Violet Light Upon The Electric Discharge":
"In a series of experiments on the effects
of resonance between very rapid electric oscillations which I have carried out
and recently published, two electric sparks were produced by the same discharge
of an induction-coil, and therefore simultaneously. One of these, the spark A,
was the discharge-spark of the induction-coil, and served to excite the primary
oscillation. The second, the spark B, belonged to the induced or secondary
oscillation. The latter was not very luminous; in the experiments its maximum
length had to be accurately measured. I occasionally enclosed the spark B in a
dark case so as more easily to make the observations; and in so doing I
observed that the maximum spark-length became decidedly smaller inside the case
than it was before. On removing in succession the various parts of the case, it
was seen that the only portion of it which exercised this prejudicial effect
was that which screened the spark B from the spark A. The partition on that
side exhibited this effect, not only when it was in the immediate neighbourhood
of the spark B, but also when it was interposed at greater distances from B
between A and B. A phenomenon so remarkable called for closer investigation.
The following communication contains the results which I have been able to
establish in the course of the investigation :—

1. The phenomenon could not be traced to any screening effect of an
electrostatic or electromagnetic nature. For the effect was not only exhibited
by good conductors interposed between A and B, but also by perfect
non-conductors, in particular by glass, paraffin, ebonite, which cannot
possibly exert any screening effect. Further, metal gratings of coarse texture
showed no effect, although they act as efficient screens.

2. The fact that both sparks A and B corresponded with synchronous and very
rapid oscillations was immaterial. For the same effect could be exhibited by
exciting two simultaneous sparks in any other way. It also appeared when,
instead of the induced spark, I used a side-spark (this term having the same
significance as in my earlier paper). It also appeared when I used as the spark
B a side-discharge (according to Riess's terminology), such as is obtained by
connecting one pole of an induction-coil with an insulated conductor and
introducing a spark-gap. But it can best and most conveniently be exhibited by
inserting in the same circuit two induction-coils with a common interrupter,
the one coil giving the spark A and the other the spark B. This arrangement was
almost exclusively used in the subsequent experiments. As I found the
experiment succeed with a number of different induction-coils, it could be
carried out with any pair of sets of apparatus at pleasure. At the same time it
will be convenient to describe the particular experimental arrangement which
gave the best results and was most frequently used. The spark A was produced by
a large Ruhmkorff coil (a, Fig. 18), 52 cm. long and 20 cm. in diameter, fed by
six large Bunsen cells (b) and provided with a separate mercury-break (c). With
the current used it could give sparks up to 10 cm. long between point and
plate, and up to about 3 cm. between two spheres. The spark generally used was
one of 1 cm. length between the points of a common discharger (d). The spark B
was produced by a smaller coil (originally intended for medical use) of
relatively greater current-strength, but having a maximum spark-length of only
1/2-1 cm. As it was here introduced into the circuit of the larger coil, its
condenser did not come into play, and thus it only gave sparks of 1 - 2 mm.
length. The sparks used were ones about 1 mm. long between the nickelplated
knobs of a Riess spark-micrometer (f), or between brass knobs of 5 to 10 cm.
diameter. When the apparatus thus arranged was set up with both spark-gaps
parallel and not too far apart, the interrupter set going, and the
spark-micrometer drawn out just so far as to still permit sparks to pass
regularly, then on placing a plate (p) of metal, glass, etc., between the two
sparks-gaps d and f, the sparks are extinguished immediately and completely. On
removing the plate they immediately reappear.
3. The effect becomes more marked as the
spark A is brought nearer to the spark B. The distance between the two sparks
when I first observed the phenomenon was 1 1/2 metres, and the effect is,
therefore, easily observed at this distance. I have been able to detect
indications of it up to a distance of 3 metres between the sparks. But at such
distances the phenomenon manifests itself only in the greater or less
regularity of the stream of sparks at B; at distances less than a metre its
strength can be measured by the difference between the maximum spark-length
before and after the interposition of the plate. In order to indicate the
magnitude of the effect I give the following, naturally rough, observations
which were obtained with the experimental arrangement shown in Fig. 18 :—

{ULSF: table omitted}

It will be seen that, under certain conditions, the sparking distance is
doubled by removing the plate.

4. The observations given in the table may also be adduced as proofs of the
following statement which the reader will probably have assumed from the first.
The phenomenon does not depend upon any prejudicial effect of the plate on the
spark B, but upon its annulling a certain action of the spark A, which tends to
increase the sparking distance. When the distance between the sparks A and B is
great, if we so adjust the spark-micrometer that sparks no longer pass at B,
and then bring the spark-micrometer nearer to A, the stream of sparks in B
reappears; this is the action. If we now introduce the plate, the sparks are
extinguished; this is the cessation of the action. Thus the plate only forms a
means of exhibiting conveniently and plainly the action of the spark A. I shall
in future call A the active spark and B the passive spark.

5. The efficiency of the active spark is not confined to any special form of
it. Sparks between knobs, as well as sparks between points, proved to be
efficient. Short straight sparks, as well as long jagged ones, exhibited the
effect. There was no difference of any importance between faintly luminous
bluish sparks and brilliant white ones. Even sparks 2 mm. long made their
influence felt to considerable distances. Nor does the action proceed from any
special part of the spark; every part is effective. This statement can be
verified by drawing a glass tube over the spark-gap. The glass does not allow
the effect to pass through, and so the spark under these conditions is
inactive. But the effect reappears as soon as a short bit of the spark is
exposed at one pole or the other, or in the middle. I have not observed any
influence due to the metal of the pole. And in arranging the experiment it is
not of importance that the active spark should be parallel to the passive one.

6. On the other hand, the susceptibility of the passive spark to the action
is to a certain extent dependent upon its form. I could detect no
susceptibility with long jagged sparks between points, and but little with
short sparks between points. The effect was best displayed by sparks between
knobs, and of these most strikingly by short sparks. It is advisable to use for
the experiments sparks 1 mm. long between knobs of 5-10 mm. diameter. Still I
have distinctly recognised the effect with sparks 2 cm. long. Perhaps the
absolute lengthening which such sparks experience is really as great as in the
case of shorter sparks, but at all events the relative increase in length is
much smaller; and hence the effect disappears in the differences which occur
between the single discharges of the coil. I have not discovered any
perceptible influence due to the material of the pole. I examined sparks
between poles of copper, brass, iron, aluminium, tin, zinc, and lead. If there
was any difference between the metals with respect to the susceptibility of the
spark, it appeared to be slightly in favour of the iron. The poles must be
clean and smooth; if they are dirty, or corroded by long use, the effect is not
produced.

7. The relation between the two sparks is reciprocal. That is to say, not
only does the larger and stronger spark increase the spark-length of the
smaller one, but conversely the smaller spark has the same effect upon the
sparklength of the larger one. For example, using the same apparatus as before,
let us adjust the spark-micrometer so that the discharge in it passes over
regularly; but let the discharger be so adjusted that the discharges of the
large coil just miss fire. On bringing the spark-micrometer nearer we find that
these discharges are again produced; but that on introducing a plate the action
ceases. For this purpose the spark of the large coil must naturally be fairly
sensitive; and, inasmuch as long sparks are less sensitive, the effect is not
so striking. If both coils are just at the limit of their sparking distance
complications arise which have probably no connection with the matter at
present under discussion. One frequently has occasion to notice a long spark
being started by other ones which are much smaller, and in part this may
certainly be ascribed to the action which we are investigating. When the
discharge of a coil is made to take place between knobs, and the knobs are
drawn apart until the sparks cease, then it is found that the sparking begins
again when an insulated conductor is brought near one of the knobs so as to
draw small side - sparks from it. I have proved to my entire satisfaction that
the side-discharges here perform the function of an active spark in the sense
of the present investigation. It is even sufficient to touch one of the knobs
with a nonconductor, or to bring a point somewhat near it, in order to give
rise to the same action. It appears at least possible that the function of an
active spark is here performed by the scarcely visible side-discharges over the
surface of the nonconductor and of the point.

8. The effect of the active spark spreads out on all sides in straight lines
and forms rays exactly in accordance with the laws of the propagation of light.
Suppose the axes of both of the sparks used to be placed vertically, and let a
plate with a vertical edge be pushed gradually from the side in between the
sparks. It is then found that the effect of the active spark is stopped, not
gradually, but suddenly, and in a definite position of the plate. If we now
look along the edge of the plate from the position of the passive spark, we
find that the active spark is just hid by the plate. If we adjust the plate
with its edge vertical between the two sparks and slowly remove it sideways,
the action begins again in a definite position, and we now find that, from the
position of the passive spark, the active spark has just become visible beyond
the edge of the plate. If we place between the sparks a plate with a small
vertical slit and move it backwards and forwards, we find that the action is
only transmitted in one perfectly definite position, namely, when the active
spark is visible through the slit from the position of the passive spark. If
several plates with such slits are interposed behind each other, we find that
in one particular position the action passes through the whole lot. If we seek
these positions by trial, we end by finding (most easily, of course, by looking
through) that all the slits lie in the vertical plane which passes through the
two sparks. If at any distance from the active spark we place a plate with an
aperture of any shape, and by moving the active spark about fix the limits of
the space within which the action is exerted, we obtain as this limit a conical
surface determined by the active spark as apex and by the limits of the
aperture. If we place a small plate in any position in front of the active
spark we find, by moving the passive spark about, that the plate stops the
action of the active spark within exactly the space which it shelters from its
light. It scarcely requires to be explained that the action is not only
annulled in the shadows cast by external bodies, but also in the shadows of the
knobs of the passive spark. In fact, if we turn the latter so that its axis
remains in the plane of the active spark, but is perpendicular to it instead of
being parallel, the action immediately ceases.

9. Most solid bodies hinder the action of the active spark, but not all; a
few solid bodies are transparent to it. All the metals which I tried proved to
be opaque, even in thin sheets, as did also paraffin, shellac, resin, ebonite,
and india-rubber; all kinds of coloured and uncoloured, polished and
unpolished, thick and thin glass, porcelain, and earthenware; wood, pasteboard,
and paper; ivory, horn, animal hides, and feathers; lastly, agate, and, in a
very remarkable manner, mica, even in the thinnest possible flakes. Further
investigation of crystals showed variations from this behaviour. Some indeed
were equally opaque, e.g. copper sulphate, topaz, and amethyst; but others,
such as crystallised sugar, alum, calc-spar, and rock-salt, transmitted the
action, although with diminished intensity; finally, some proved to be
completely transparent, such as gypsum (selenite), and above all rock-crystal,
which scarcely interfered with the action even when in layers several
centimetres thick. The following is a convenient method of testing :—The
passive spark is placed a few centimetres away from the active spark, and is
brought to its maximum length. The body to be examined is now interposed. If
this does not stop the sparking the body is very transparent. But if the
sparking is stopped, the spark-gap must be shortened until it comes again into
action. An opaque substance is now interposed in addition to the body under
investigation. If this stops the sparking once more, or weakens it, then the
body must have been at any rate partially transparent; but if the plate
produces no further effect it must have been quite opaque. The influence of the
interposed bodies increases with their thickness, and it may properly be
described as an absorption of the action of the active spark; in general,
however, even those bodies which only act as partial absorbers, exert this
influence even in very thin layers.

10. Liquids also proved to be partly transparent and partly opaque to the
action. In order to experiment upon them the active spark was brought about 10
cm. vertically above the passive one, and between both was placed a glass
vessel, of which the bottom consisted of a circular plate of rock-crystal 4 mm.
thick. Into this vessel a layer, more or less deep, of the liquid was poured,
and its influence was then estimated in the manner above described for solid
bodies. Water proved to be remarkably transparent; even a depth of 5 cm.
scarcely hindered the action. In thinner layers pure concentrated sulphuric
acid, alcohol, and ether were also transparent. Pure hydrochloric acid, pure
nitric acid, and solution of ammonia proved to be partially transparent. Molten
paraffin, benzole, petroleum, carbon bisulphide, solution of ammonium sulphide,
and strongly coloured liquids, e.g. solutions of fuchsine, potassium
permanganate, were nearly or completely opaque. The experiments with salt
solutions proved to be interesting. A layer of water 1 cm. deep was introduced
into the rock-crystal vessel; the concentrated salt solution was added to this
drop by drop, stirred, and the effect observed. With many salts the addition of
a few drops, or even a single drop, was sufficient to extinguish the passive
spark; this was the case with nitrate of mercury, sodium hyposulphite,
potassium bromide, and potassium iodide. When iron and copper salts were added,
the extinction of the passive spark occurred before any distinct colouring of
the water could be perceived. Solutions of sal-ammoniac, zinc sulphate, and
common saltl exercised an absorption when added in larger quantities. On the
other hand, the sulphates of potassium, sodium, and magnesium were very
transparent even in concentrated solution.

11. It is clear from the experiments made in air that some gases permit the
transmission of the action even to considerable distances. Some gases, however,
are very opaque to it. In experimenting on gases a tube 20 cm. long and 2.5 cm.
in diameter was interposed between the active and passive sparks; the ends of
this tube were closed by thin quartz plates, and by means of two side-tubes any
gas could at will be led through it. A diaphragm prevented the transmission of
any action excepting through the glass tube. Between hydrogen and air there was
no noticeable difference. Nor could any falling off in the action be perceived
when the tube was filled with carbonic acid. But when coal-gas was introduced,
the sparking at the passive spark-gap immediately ceased. When the coal-gas was
driven out by air the sparking began again; and this experiment could be
repeated with perfect regularity. Even the introduction of air with which some
coalgas had been mixed hindered the transmission of the action. Hence a much
shorter stratum of coal-gas was sufficient to stop the action. If a current of
coal-gas 1 cm. in diameter is allowed to flow freely into the air between the
two sparks, a shadow of it can be plainly perceived on the side remote from the
active spark, i.e. the action of this is more or less completely annulled. A
powerful absorption like that of coal-gas is exhibited by the brown vapours of
nitrous oxide. With these, again, it is not necessary to use the tube with
quartz-plates in order to show the action. On the other hand, although chlorine
and the vapours of bromine and iodine do exercise absorption, it is not at all
in proportion to their opacity. No absorptive action could be recognised when
bromine vapour had been introduced into the tube in sufficient quantity to
produce a distinct coloration; and there was a partial transmission of the
action even when the bromine vapour was so dense that the active spark
(coloured a deep red) was only just visible through the tube.

12. The intensity of the action increases when the air around the passive
spark is rarefied, at any rate up to a certain point. The increase is here
supposed to be measured by the difference between the lengths of the protected
and the unprotected sparks. In these experiments the passive spark was produced
under the bell-jar of an air-pump between adjustable poles which passed through
the sides of the bell-jar. A window of rock-crystal was inserted in the
bell-jar, and through this the action of the other spark had to pass. The
maximum sparklength was now observed, first with the window open, and then with
the window closed; varying air-pressures being used, but a constant current.
The following table may be regarded as typical of the results :—
{ULSF: table
omitted}
It will be seen that as the pressure diminishes, the length of the spark
which is not influenced only increases slowly; the length of the spark which is
influenced increases more rapidly, and so the difference between the two
becomes greater. But at a certain pressure the blue glow-light (Glimmlicht)
spread over a considerable portion of the cathode, the sparking distance became
very great, the discharge altered its character, and it was no longer possible
to perceive any influence due to the active spark.

13. The phenomenon is also exhibited when the sparking takes place in other
gases than air; and also when the two sparks are produced in two different
gases. In these experiments the two sparks were produced in two small tubulated
glass vessels which were closed by plates of rock-crystal and could be filled
with different gases. The experiments were tried mainly because certain
circumstances led to the supposition that a spark in any given gas would only
act upon another spark in the same gas, and on this account the four
gases—hydrogen, air, carbonic acid, and coal-gas—were tried in the sixteen
possible combinations. The main conclusion arrived at was that the above
supposition was erroneous. It should, however, be added that although there is
no great difference in the efficiency of sparks when employed as active sparks
in different gases, there is, on the other hand, a notable difference in their
susceptibility when employed as passive sparks. Other things being equal,
sparks in hydrogen experienced a perceptibly greater increase in length than
sparks in air, and these again about double the increase of sparks in carbonic
acid and coal-gas. It is true that no allowance was made for absorption in
these experiments, for its effect was not known when they were carried out; but
it could only have been perceptible in the case of coal-gas.

14. All parts of the passive spark do not share equally in the action; it
takes place near the poles, more especially near the negative pole. In order to
show this, the passive spark is made from 1 to 2 cm. long, so that the various
parts of it can be shaded separately. Shading the anode has but a slight
effect; shading the cathode stops the greater part of the action. But the
verification of this fact is somewhat difficult, because with long sparks there
is a want of distinctness about the phenomenon. In the case of short sparks
(the parts of which cannot be separately shaded) the statement can be
illustrated as follows :—The passive spark is placed parallel to the active
one and is turned to right and left from the parallel into the perpendicular
position until the action stops. It is found that there is more play in one
direction than in the other; the advantage being in favour of that direction in
which the cathode is turned towards the active spark. Whether the effect is
produced entirely at the cathode, or only chiefly at the cathode, I have not
been able to decide with certainty.

15. The action of the active spark is reflected from most surfaces. From
polished surfaces the reflection takes place according to the laws of regular
reflection of light. In the preliminary experiments on reflection a glass tube,
50 cm. long and 1 cm. in diameter, was used; this tube was open at both ends,
and was pushed through a large sheet of cardboard. The active spark was placed
at one end so that its action could only pass the sheet by way of the tube. If
the passive spark was now moved about beyond the other end of the tube it was
affected when in the continuation of the tubular space and then only; but in
this case a far more powerful action was exhibited than when the tube was
removed and only the diaphragm retained. It was this latter phenomenon that
suggested the use of the tube; of itself it indicates a reflection from the
walls of the tube. The spark-micrometer was now placed to one side of the beam
proceeding out of the tube, and was so disposed that the axis of the spark was
parallel to the direction of the beam. The micrometer was now adjusted so that
the sparking just ceased; it was found to begin again if a plane surface
inclined at an angle of 45° to the beam was held in it so as to direct the
beam, according to the usual law of reflection, upon the passive spark.
Reflection took place more or less from glass, crystals, and metals, even when
these were not particularly smooth; also from such substances as porcelain,
polished wood, and white paper. I obtained no reflection from a well-smoked
glass plate.

In the more accurate experiments the active spark was placed in a vertical
straight line; at a little distance from it was a largeish plate with a
vertical slit, behind which could be placed polished plane mirrors of glass,
rock-crystal, and various metals. The limits of the space within which the
action was exerted behind the slit were then determined by moving the passive
spark about. These limits were quite sharp and always coincided with the limits
of the space within which the image of the active spark in the mirror was
visible. On account of the feebleness of the action these experiments could not
be carried out with unpolished bodies; such bodies may be supposed to give rise
to diffused reflection.

16. In passing from air into a solid transparent medium the action of the
active spark exhibits a refraction like that of light; but it is more strongly
refracted than visible light. The glass tube used in the reflection experiments
served here again for the rougher experiments. The passive spark was placed in
the beam proceeding out of the tube and at a distance of about 3 0 cm. from the
end farthest from the active spark; immediately behind the opening a
quartz-prism was pushed sideways into the beam with its refracting edge
foremost. In spite of the transparency of quartz, the effect upon the passive
spark ceased as soon as the prism covered the end of the tube. If the spark was
then moved in a circle about the prism in the direction in which light would be
refracted by the prism, it was soon found that there were places at which the
effect was again produced. Now let the passive spark be fixed in the position
in which the effect is most powerfully exhibited; on looking from this point
towards the tube through the prism the inside of the tube and the active spark
at the end of it cannot be perceived; in order to see the active spark through
the tube the eye must be shifted backwards through a considerable distance
towards the original position of the spark. The same result is obtained when a
rock-salt prism is used. In the more accurate experiments the active spark was
again fixed vertically; at some distance from it was placed a vertical slit,
and behind this a prism. By inserting a Leyden jar the active spark could be
made luminous, and the space thus illuminated behind the prism could easily be
determined. With the aid of the passive spark it was possible to mark out the
limits of the space within which was exerted the action here under
investigation. Fig. 19 gives (to a scale of 1/2) the result thus obtained by
direct experiment. The space a b c d is filled with light; the space a' b' c'
d' is permeated by the action which we are considering. Since the limits of
this latter space were not sharp, the rays a' b' and c' d' were fixed in the
following way :—The passive spark was placed in a somewhat distant position,
about c', at the edge of the tract within which the action was exerted. A
screen m n (Fig. 19) with vertical edge was then pushed in sideways until it
stopped the action. The position m of its edge then gave one point of the ray
c' d'. In another experiment a prism of small refracting angle was used, and
the width of the slit was made as small, and the spark placed as far from it as
would still allow of the action being perceived. The visible light was then
spread out into a short spectrum, and the influence of the active spark was
found to be exerted within a comparatively limited region which corresponded to
a deviation decidedly greater than that of the visible violet. Fig. 2 0 shows
the positions of the rays as they were directly drawn where the prism was
placed, r being the direction of the red, v of the violet, and w the direction
in which the influence of the active spark was most powerfully exerted.


I have not been able to decide whether any double refraction of the action
takes place. My quartz-prisms would not permit of a sufficient separation of
the beams, and the pieces of calc-spar which I possessed proved to be too
opaque.

17. After what has now been stated, it will be agreed (at any rate until the
contrary is proved) that the light of the active spark must be regarded as the
prime cause of the action which proceeds from it. Every other conjecture which
is based on known facts is contradicted by one or other of the experiments. And
if the observed phenomenon is an effect of light at all it must, according to
the results of the refraction-experiments, be solely an effect of the
ultra-violet light. That it is not an effect of the visible parts of the light
is shown by the fact that glass and mica are opaque to it, while they are
transparent to these. On the other hand, the absorption-experiments of
themselves make it probable that the effect is due to ultra-violet light.
Water, rock-crystal, and the sulphates of the alkalies are remarkably
transparent to ultra-violet light and to the action here investigated; benzole
and allied substances are strikingly opaque to both. Again, the active rays in
our experiments appear to lie at the outermost limits of the known spectrum.
The spectrum of the spark when received on a sensitive dry-plate scarcely
extended to the place at which the most powerful effect upon the passive spark
was produced. And, photographically, there was scarcely any difference between
light which had, and light which had not, passed through coal-gas, whereas the
difference in the effect upon the spark was very marked. Fig. 21 shows the
extent of some of the spectra taken. In a the position of the visible red is
indicated by r, that of the visible violet by v, and that of the strongest
effect upon the passive spark by w. The rest of the series give the
photographic impressions produced—b after simply passing through air and
quartz, c after passing through coal-gas, d after passing through a thin plate
of mica, and e after passing through glass.

18. Our supposition that this effect is to be attributed to light is
confirmed by the fact that the same effect can be produced by a number of
common sources of light. It is true that the power of the light, in the
ordinary sense of the word, forms no measure of its activity as here
considered; and for the purpose of our experiments the faintly visible light of
the spark of the induction-coil remains the most powerful source of light. Let
sparks from any induction-coil pass between knobs, and let the knobs be drawn
so far apart that the sparks fail to pass; if now the flame of a candle be
brought near (about 8 cm. off) the sparking begins again. The effect might at
first be attributed to the hot air from the flame; but when it is observed that
the insertion of a thin small plate of mica stops the action, whereas a much
larger plate of quartz does not stop it, we are compelled to recognise here
again the same effect. The flames of gas, wood, benzene, etc., all act in the
same way. The nonluminous flames of alcohol and of the Bunsen burner exhibit
the same effect, and in the case of the candle-flame the action seems to
proceed more from the lower, non-luminous part than from the upper and luminous
part. From a small hydrogen flame scarcely any effect could be obtained. The
light from platinum glowing at a white-heat in a flame, or through the action
of an electric current, a powerful phosphorus flame burning quite near the
spark, and burning sodium and potassium, all proved to be inactive. So also was
burning sulphur; but this can only have been on account of the feebleness of
the flame, for the flame of burning carbon bisulphide produced some effect.
Magnesium light produced a far more powerful effect than any of the above
sources ; its action extended to a distance of about a metre. The limelight,
produced by means of coalgas and oxygen, was somewhat weaker, and acted up to a
distance of half a metre; the action was mainly due to the jet itself: it made
no great difference whether the lime-cylinder was brought into the flame or
not. On no occasion did I obtain a decisive effect from sunlight at any time of
the day or year at which I was able to test it. When the sunlight was
concentrated by means of a quartz lens upon the spark there was a slight
action; but this was obtained equally when a glass lens was used, and must
therefore be attributed to the heating. But of all sources of light the
electric arc is by far the most effective; it is the only one that can compete
with the spark. If the knobs of an induction-coil are drawn so far apart that
sparks no longer pass, and if an arc light is started at a distance of 1, 2, 3,
or even 4 metres, the sparking begins again simultaneously, and stops again
when the arc light goes out. By means of a narrow opening held in front of the
arc light we can separate the violet light of the feebly luminous arc proper
from that of the glowing carbons; and we then find that the action proceeds
chiefly from the former. With the light of the electric arc I have repeated
most of the experiments already described, e.g. the experiments on the
rectilinear propagation, reflection, and refraction of the action, as well as
its absorption by glass, mica, coal-gas, and other substances.

According to the results of our experiments, ultra-violet light has the
property of increasing the sparking distance of the discharge of an
induction-coil, and of other discharges. The conditions under which it exerts
its effect upon such discharges are certainly very complicated, and it is
desirable that the action should be studied under simpler conditions, and
especially without using an induction-coil. In endeavouring to make progress in
this direction I have met with difficulties. Hence I confine myself at present
to communicating the results obtained, without attempting any theory respecting
the manner in which the observed phenomena are brought about.".



A summary of Hertz's work "Ueber einen Einfluss des ultravioletten Lichtes auf
die electrische Entladung" ("Influence of Ultra-Violet Light on the Electric
Discharge") reads:
"The author has discovered that ultra-violet radiation favours the
electric discharge between two conductors in a remarkable way. As sources of
such radiation, the sun, burning magnesium, or even ordinary flame, may be
used; but by far the most effective are the electric arc and an induced
electric discharge. To produce the phenomenon, the primary circuits of two
induction coils, a large one (10 cm.) and a smaller one (1 cm.), are joined in
circuit with the same battery (six Bunsens) and interruptor. Perfect
synchronism in the induced discharge is thus secured. The terminals of the
large coil being arranged to give a good spark 1 cm. in length, the two coils
are placed close together, and an opaque screen interposed. The terminals of
the small coil are then drawn apart until sparks just cease to pass. On now
removing the screen the discharge is re-established.

The author describes many experiments to test the nature of the effect. The
influence is not electrical, since non-conducting screens are effective as well
as metal plates. It varies in some inverse ratio with the distance, and is
distinctly produced when the coils are 1 m. apart. In the above experiment, the
larger spark may be either short and dense, or long and zig-zag, and every part
of it is effective. The smaller spark, however, should be short (between knobs)
; the seat of the action upon it appears to be in the neighbourhood of the
cathode or negative pole. The influence is reciprocal; that is, the smaller
spark also favours the larger. The action is propagated in straight lines, like
light, and may be reflected from polished surfaces. It may also undergo
refraction ; but its refrangibility (roughly measured by means of a quartz
prism) is much greater than that of the violet rays. Most solid substances are
opaque to it; amongst these glass, paper, agate, and mica, even in the thinnest
sheets, are noticeable. Amongst crystalline substances, copper sulphate, topaz,
and amethyst are opaque to it; but it is transmitted by sugar, alum, calc-spar,
and rock-salt; transparent gypsum and rock crystal transmit it perfectly.
Amongst liquids, water transmits it freely; sulphuric and hydrochloric acids,
alcohol, and ether, less so; whilst melted paraffin and petroleum, benzene,
bisulphide of carbon, ammonium hydrosulphide, and coloured liquids generally,
stop it completely. Solutions of potassium, sodium, and magnesium sulphates,
are fairly transparent to it; those of mercuric nitrate, sodium thiosulphate,
potassium bromide and iodide, are very opaque. Amongst gases, air, hydrogen,
and carbonic anhydride are very transparent; chlorine, and bromine and iodine
vapours, partially so; and coal-gas and nitric peroxide very opaque.

Even an ordinary candle-flame may produce effects similar to those described,
and may cause the reappearance of sparks between the terminals of an
induction-coil after they have been drawn so far apart that the discharge has
ceased. Similar effects are produced by the luminous flames of gas, wood, and
benzene, and the non-luminous flames of alcohol, carbon bisulphide, and the
Bunsen burner. Incandescent platinum, and the flames of sodium, potassium,
sulphur, and phosphorus, and of pure hydrogen, are without effect. The
effective rays are more refrangible even than the so-called photographic rays;
for the latter are not sensibly absorbed by coal-gas.".

(Possibly - that the effect is not electrical may refer to light not being an
electric phenomenon - and kind of a subtle putting forward of that secret
truth.)
(University of Karlsruhe) Karlsruhe, Germany  
113 YBN
[07/07/1887 AD]
4046) Bell's share of the royalties from the Graphophone finance the Volta
Bureau and the American Association to Promote the Teaching of Speech to the
Deaf (since 1956 the Alexander Graham Bell Association for the Deaf).
(Volta Lab) Washington, District of Columbia, USA  
113 YBN
[07/??/1887 AD]
4159)
(Case School of Applied Science) Cleveland, Ohio, USA  
113 YBN
[09/26/1887 AD]
4112) Émile Berliner (BARlENR) (CE 1851-1929), German-US inventor invents a
flat phonograph record in which the needle vibrates from side to side as
opposed to up and down which Edison's phograph uses.

Berliner's first discs are wax-coated zinc pieces, on which a sound vibration
is carved. The discs are dipped in acid, which burns the pattern into the
metal, and the wax is stripped. On September 26, 1887, Berliner patents his
entire playback apparatus as the "gramophone."

Berliner displays his invention at the Franklin Institute of Philadelphia in
1888, but first markets it in Germany. A toy manufacturer, Kummerer & Reinhardt
of Waltershausen, produces his gramophones. At this time, his gramophone is
turned by hand with a crank. back in the USA, Berliner employs several
musicians to record on his discs, and begins making discs from a new material
composed of shellac, soot, and fur. In 1893, Berliner secures investment from
friends to found the United States Gramophone Company in order to market the
gramophone and control its patent rights. In late 1895, investors contribute
another $25,000 to launch the Berliner Gramophone Company, a manufacturing
enterprise. Initially, sales of this new technology are slow, but when Eldridge
R. Johnson of New Jersey introduces a wind-up spring motor to replace the
tedious hand-crank in 1896, sales improve dramatically. Over the next four
years, nearly 25,000 of these motors are manufactured for the Berliner
Gramophone Company.

The Berliner flat disk will eventually replace Edison's cylinder phonograph,
and amazing that these flat records will last until the compact disk of the
1990s - while clearly much more advanced technology is kept secret by the phone
company and those who routinely read and write to and from neurons.
(own lab) Washington, DC, USA  
113 YBN
[10/12/1887 AD]
4246)
(Tesla's private lab) New York City, NY, USA  
113 YBN
[11/07/1887 AD]
4114) Émile Berliner (BARlENR) (CE 1851-1929), German-US inventor invents a
flat phonograph record in which the needle vibrates from side to side as
opposed to up and down which Edison's phograph uses.

Berliner's first discs are wax-coated zinc pieces, on which a sound vibration
is carved. The discs are dipped in acid, which burns the pattern into the
metal, and the wax is stripped. On September 26, 1887, Berliner patents his
entire playback apparatus as the "gramophone."

Berliner displays his invention at the Franklin Institute of Philadelphia in
1888, but first markets it in Germany. A toy manufacturer, Kummerer & Reinhardt
of Waltershausen, produces his gramophones. At this time, his gramophone is
turned by hand with a crank. back in the USA, Berliner employs several
musicians to record on his discs, and begins making discs from a new material
composed of shellac, soot, and fur. In 1893, Berliner secures investment from
friends to found the United States Gramophone Company in order to market the
gramophone and control its patent rights. In late 1895, investors contribute
another $25,000 to launch the Berliner Gramophone Company, a manufacturing
enterprise. Initially, sales of this new technology are slow, but when Eldridge
R. Johnson of New Jersey introduces a wind-up spring motor to replace the
tedious hand-crank in 1896, sales improve dramatically. Over the next four
years, nearly 25,000 of these motors are manufactured for the Berliner
Gramophone Company.

The Berliner flat disk will eventually replace Edison's cylinder phonograph,
and amazing that these flat records will last until the compact disk of the
1990s - while clearly much more advanced technology is kept secret by the phone
company and those who routinely read and write to and from neurons.
(own lab) Washington, DC, USA  
113 YBN
[1887 AD]
3083)
(University of Heidelberg) Heidelberg, Germany  
113 YBN
[1887 AD]
3697)
Paris, France(presumably)  
113 YBN
[1887 AD]
3739)
(Solar Physics Observatory) South Kensington, England (presumably)  
113 YBN
[1887 AD]
3772)
(Charles University) Prague, Czech Republic  
113 YBN
[1887 AD]
3957) Granville Stanley Hall (CE 1846-1924), US psychologist, founds the
American Journal of Psychology, the first American journal in the field of
psychology and the second of any significance outside Germany.

Johns Hopkins University (presumably), Baltimore, Maryland, USA  
113 YBN
[1887 AD]
3960)
University of Liège, Liège, Belgium  
113 YBN
[1887 AD]
4027)
(private lab) East Newark, New Jersey, USA (presumably)  
113 YBN
[1887 AD]
4048)
(University of Bonn) Bonn, Germany  
113 YBN
[1887 AD]
4098)
(École des Mines) Paris, France  
113 YBN
[1887 AD]
4219)
(Leiden University) Leiden, Netherlands  
113 YBN
[1887 AD]
4224) Johann Elster and Hans Geitel jointly carry out and publish almost all of
their investigations from 1884 to 1920.
(Herzoglich Gymnasium) Wolfenbüttel, Germany  
113 YBN
[1887 AD]
4341)
(Institute of Physics of the Academy of Sciences) Stockholm, Sweden  
113 YBN
[1887 AD]
4369) Electricity of heart beat measured and recorded.

Augustus Desire Waller (CE 1856-1922) measures the electric potentials of the
heart muscle, finds them to coincide with each heart muscle contraction, and
publishes the first electrocardiograph images.


Waller publishes his findings with images in an 1887 report, "A Demonstration
on Man of Electromotive Changes Accompanying the Heart's Beat". This is the
first published account of human electrocardiography.

Waller uses zinc covered by leather and moistened with salt-water to measure
the electricity.

Waller records the electrical activity of the living mammalian heart from the
body surface and in some of the recordings associates that recording with the
mechanical apex beat. While some of the recording devices are of Waller's own
devising Waller primarily uses the Lippmann capillary electrometer which
consists largely of a mercury column supporting a column of dilute sulphuric
acid. With the passage of minute electric currents through the instrument, the
mercury column fluctuates. A light transilluminating the fluctuating level of
the mercury meniscus surface projects the mercury column's movements. This
discovery that cardiac mechanical activity is associated with the generation of
minute electrical currents which Waller names "electrogram" defines the
remainder of Waller's career, as well as being the beginning of a search in the
physiologic community for better techniques for their detection and recording.
To record the light beam photographically Waller devises a technique of slowly
moving a glass photographic plate past the light beam at a constant speed,
using a spring motor driven toy train. Willem Einthoven will improve on the
Waller electrograms with a more robust and sensitive string galvanometer.
Einthoven initially drops the photographic plates at a controlled speed, in a
gravity and then later in a motor driven track.

Waller writes:
"IF a pair of electrodes (zinc covered by chamois leather and moistened
with brine) are strapped to the front and back of the chest, and connected with
a Lippmann's capillary electrometer, the mercury in the latter will be seen to
move slightly but sharply at each beat of the heart'. If the movements of the
column of mercury are photographed on a travelling plate simultaneously with
those of an ordinary cardiographic lever a record is obtained as under (fig. 1)
in which the upper line h.h. indicates the heart's movements and the lower line
e.e. the level of the mercury in the capillary. Each beat of the heart is seen
to be accompanied by an electrical variation.

The first and chief point to determine is whether or no the electrical
variation is physiological, and not due to a mechanical alteration of contact
between the electrodes and the chest wall caused by the heart's impulse. To
ascertain this point accurate time-measurements are necessary; a physiological
variation should precede the movement
of the heart, while this could not be the case if
the variation were due to altered contact. Fig. 2 is an instance of such
time-measurements taken at as high a speed of the travelling surface as may be
used without rendering the initial points of the curves too indeterminate. It
shews that the electrical phenomenon begins a little before the cardiographic
lever begins to
rise. The difference of time is however very small, only about .025", and this
amount must further be diminished by .01" which represents the "lost time" of
the cardiograph. The actual difference is thus no greater than .015", and the
record is therefore, although favourable to the physiological interpretation,
not conclusively
satisfactory.

We know, from the experiment of the secondary contraction made by Helmholtz' on
voluntary muscle, by Kolliker and Muller and by Donders on the heart, that the
negative variation of muscle begins before its visible movement, and the
current of action of the heart begins before the commencement of the heart's
contraction. For muscle the time-difference given is 1/200", for the heart
(rabbit) 1/70"; for the frog's heart the rheotome observations of Marchand are
to the effect that the variation begins .01" to .04" after excitation, while
the contraction does not begin until .11" to .33". The capillary electrometer
may with advantage be employed to measure this time-difference, the
electrical and
the mechanical events being simultaneously recorded.
This I carried out on voluntary and
upon cardiac muscle with the same instrument as that which I employed for the
human heart, and thus ascertained that its indications are trustworthy in this
capacity.

In all these cases the antecedence of the electrical variation is clear and
measurable. In the case of the excised kitten's heart the time-difference is
about .05" with a length of contraction of about 2", i.e. the interval
between the
electrical and the mechanical event is increased in the sluggishly acting
organ. In the case of the human heart the time difference appears to be about
.015" with a length of systole of .35"-a value which corresponds with that
obtained by Donders for the rabbit's heart in situ by the method of the
secondary contraction, viz.
1/70" (the length of systole being presumably about
1/3").

That a true electrical variation of the human heart is demonstrable, may
further be proved beyond doubt by leading off from the body otherwise than from
the chest wall. If the two hands or one hand and one foot be plunged into two
dishes of salt solution connected with the two sides of the electrometer, the
column of mercury will be seen to move at each beat of the heart, though less
than when electrodes are strapped to the chest. The hand and foot act in this
case as leading off electrodes from the heart, and by taking simultaneous
records of these movements of the mercury and of the movements of the heart it
is seen that the former correspond with the latter, slightly preceding them and
not succeeding them, as would be the case if they depended upon pulsation in
the hand or foot. This is unquestionable proof that the variation is
physiological, for there is here of course no possibility of altered contact at
the chest wall, and any mechanical alteration by arterial pulsation could only
produce an effect .15" to .20" after the
cardiac impulse. A similar result is
obtained if an electrode be placed in the mouth while one of the extremities
serves as the other leading off electrode. The electrical variation precedes
the heart's beat as in the
other cases mentioned.

In conclusion it will be well to allude to the difficulties which arise in the
interpretation of the character of the electrical variation of the human
heart.

By mere inspection of the electrometer it is often most difficult to determine
the direction of very rapid movements of the mercury, and photography must be
employed. But even then, owing to the small amplitude of movement, it is still
difficult to say whether the variation consists of two movements, and whether
each movement indicates a single or a double variation in the same direction.
Differences in the position of the electrodes also give rise to differences of
the apparent variation. Thus with the following position of the electrodes (Hg
electrode over the apex beat, H2So4 electrode on the right side of the back)
the variation as watched through the microscope appears usually
nN, and changes to SN
if the Hg electrode be shifted to the sternum. If the Hg electrode is on the
back and the H2So4 electrode over the apex beat, the variation appears to be sS
and to become nS when the H2So4 electrode is shifted away from the apex beat.
The variations accompanying the heart's beat observed as carefully as possible
(without
the aid of photography) on a healthy person with different positions of the
leading off electrodes were as follows. It is to be remarked that the direction
of variation as observed in this series is not such as to indicate
negativity of the
cardiac electrode but the reverse.

{ULSF: table omitted}

It is on account of these sources of doubt that I have not thought it advisable
at this stage to attempt a definite interpretation of the character of the
variation, which although as shewn, especially by the experiments
illustrated in figs. 6
and 7, is certainly physiological, may nevertheless be physically complicated
by the conditions of demonstration on the human body.".
(St. Mary's Hospital) London, England  
112 YBN
[01/10/1888 AD]
4023) Le Prince disappears in 1890 and is never heard from again, perhaps he
was murdered to stop his priority to a patent claim on moving pictures?
New York City, NY, USA (presumably)  
112 YBN
[02/02/1888 AD]
3840)
(Strutt Laboratory) Terling, England  
112 YBN
[02/02/1888 AD]
4288)
(University of Karlsruhe) Karlsruhe, Germany  
112 YBN
[02/??/1888 AD]
4287)
(University of Karlsruhe) Karlsruhe, Germany  
112 YBN
[04/??/1888 AD]
4289)
(University of Karlsruhe) Karlsruhe, Germany  
112 YBN
[05/03/1888 AD]
3971)
Institute of Plant Physiology at the University of Prague, Prague,
Austria  
112 YBN
[09/08/1888 AD]
6260) Smith was Vice President of the Men's League for Women Suffrage.
Bridgeton, New Jersey, USA  
112 YBN
[09/??/1888 AD]
3833)
(Royal Institution) London, England   
112 YBN
[11/??/1888 AD]
4290)
(University of Karlsruhe) Karlsruhe, Germany  
112 YBN
[12/13/1888 AD]
4291)
(University of Karlsruhe) Karlsruhe, Germany  
112 YBN
[1888 AD]
3402)
Belfast, Ireland  
112 YBN
[1888 AD]
3631)
(Technical High School in Braunschweig) Braunschweig, Germany  
112 YBN
[1888 AD]
3745) Waldeyer-Hartz's name originally is just Waldeyer.
(University of Berlin) Berlin, Germany  
112 YBN
[1888 AD]
3801)
(faculte Libre des Sciences of Lyons) Lyons, France  
112 YBN
[1888 AD]
3813) Nicolas Camille Flammarion (FlomorEON) (CE 1842-1925), French astronomer
publishes "L'atmosphère: météorologie populaire" (second edition? first is
1872? 1888; "The Atmopshere: Popular Meterology"), which includes the famous
"flat earth" woodcut drawing (p. 163). (verify)

Juvisy (near Paris), France (presumably)  
112 YBN
[1888 AD]
3817)
(Astrophysical Observatory at Potsdam) Potsdam, Germany  
112 YBN
[1888 AD]
3826) In 1875, Dewar is made a professor at the University of Cambridge, and in
1877 at the Royal Institution in London, and holds both posts throughout his
life.

In his early career Dewar writes papers on measurement of high temperatures,
for example, on the temperature of the sun and of the electric spark, others on
electro-photometry and the chemistry of the electric arc.(describe more with
original papers) With Professor J. G. Kendrick, of Glasgow, Dewar investigates
the physiological action of light, and examines the changes which take place in
the electrical condition of the retina under the influence of light. (perhaps
trying to see thought/what eye sees from behind head?) With Professor G. D.
Liveing, a colleague at Cambridge, Dewar begins in 1878, a long series of
spectroscopic observations, the later part which are devoted to the
spectroscopic examination of various gaseous constituents separated from
atmospheric air by the aid of low temperatures; and Dewar is joined by
Professor J. A. Fleming, of University College, London, in the investigation of
the electrical behavior of substances cooled to very low temperatures. (finding
a decrease in electrical resistance at low temperatures?)

From 1892-1893 Dewar and Fleming measures the electrical resistance of metals
under very cold temperatures and confirm that the resistance of many metals is
decreased by a decrease in temperature.

Dewar publishes many papers, just over 100 in the
Proceedings of the Royal Society of London.

The Concise Dictionary of Scientific Biography states that "Dewar was a superb
experimentalist; he published no theoretical papers.".
(Royal Institution) London, England (presumably)  
112 YBN
[1888 AD]
3915)
(University of Bonn) Bonn, Germany  
112 YBN
[1888 AD]
3935)
(University of Giessen) Giessen, Germany  
112 YBN
[1888 AD]
4025)
(College de France) Paris, France (presumably)  
112 YBN
[1888 AD]
4067)
(Johns Hopkins University) Baltimore, Maryland, USA  
112 YBN
[1888 AD]
4073)
(Military Medical Academy), St. Petersburg, Russia  
112 YBN
[1888 AD]
4108)
(Dutch Yeast and Spirit Factory) Delft, Netherlands  
112 YBN
[1888 AD]
4118) Beginning in 1883, Lodge becomes interested in psychic
research—telepathy, telekinesis, and communication with the dead—an
interest that is intensified after his son’s death and his own retirement in
1919. On two occasions Lodge serves as president of the Society for Psychical
Research. Perhaps Lodge was either excluded from movies beamed in front of his
eyes or did get movies in front of his eyes and worked to try to make neuron
reading and writing public.

Lodge writes a book about photon (wireless) communication in "Signalling across
space without wires: Being a description of the work of Hertz and His
Successors".
(University College) Liverpool, England  
112 YBN
[1888 AD]
4179) According to the Encyclopedia Britannica, Ostwald believes that
thermodynamics is the fundamental theory of science and has roughly two themes
in his philosophy. First Ostwald asserts the primacy of energy over matter
(matter being only a manifestation of energy) in opposition to widespread
scientific materialism. Ostwald reformulates older concepts of dynamism dating
back to Gottfried Leibniz of the 1600s with the principles of thermodynamics to
form a new metaphysical interpretation of the world that he names
"energetics".(I think thermodynamics is inaccurate and violates the principle
of conservation of matter and motion, and support a material universe - the
concept of energy is also only a generalization in my view, because mass and
motion cannot be converted into each other or exchanged in the view I support.)
Secondly Ostwald asserts a form of positivism in the sense of rejecting
theoretical concepts that are not strictly founded on empirical grounds.
Ostwald is
considered one of the primary founders of modern physical chemistry. Physical
chemistry is defined as the branch of chemistry that deals with the
interpretation of chemical phenomena and properties in terms of the underlying
physical processes, and with the development of techniques for their
investigation.
In 1887 Ostwald with friend Van't Hoff establish the first journal exclusively
for physical chemistry "Zeitschrift für physikalische Chemie" (Journal of
Physical Chemistry).
Ostwald has Gibbs' work translated into German.
In 1909 Ostwald wins
the Nobel prize in chemistry for his work on catalysis. (unclear )
Ostwald
rejects atom theory until Perrin analyzes Brownian motion, when a clearly
visible phenomenon can be easily measured.

In 1889 Ostwald starts republishing famous historical science papers in his
series "Klassiker der exakten Wissenschaften" ("Classics of the Exact
Sciences"), with more than 40 books published during the first four years.
Ostwald is
the first exchange professor at Harvard University and gives a series of
lectures (1905–06).
In 1902 Ostwald creates a journal dedicated to the philosophy of
science.
Ostwald views both war and traditional religion as wasting energy and dedicates
himself to the international peace movement and serves as president of the
Deutscher Monistenbund, a scientistic quasi-religion founded by the German
zoologist and evolutionary proponent Ernst Haeckel.

Ostwald's house is turned into a museum after his death.
In his life Ostwald
wrote 45 books and many booklets, about 500 scientific papers, some 5,000
reviews, and more than 10,000 letters.
(University of Leipzig) Leipzig, Germany  
112 YBN
[1888 AD]
4193) Roux is an assistant at Pasteur's laboratory in Paris and is director
from 1904 until his death in 1933.
(Pasteur Institute) Paris, France  
112 YBN
[1888 AD]
4210)
(Eastman Dry Plate Company) Rochester, NY, USA (presumably)  
112 YBN
[1888 AD]
4350)
(Sorbonne) Paris, France  
112 YBN
[1888 AD]
4390) Fridtjof Nansen (noNSeN) (CE 1861-1930), Norwegian explorer and five
other people are the first to cross Greenland by land, taking six weeks to
travel from the eastern shoe to the inhabeted western shore.

On 04/08/1895 Nansen
reaches 86°14' latitude, very near the north pole.
In 1922 Nansen is awarded the
Nobel Peace prize for caring for prisoners of war, those suffering in famines,
the displaced and persecuted.
Greenland  
112 YBN
[1888 AD]
4412)
(Würzburg University) Würzburg, Germany  
112 YBN
[1888 AD]
4448) Paschen is ousted from the presidency of a scientific association by the
pro-Nazi Stark.
Paschen survives WW II and sees the defeat of the Nazis but loses his
house and possessions in a bombing raid in 1943.
(University of Strasbourg) Strasbourg , Germany  
112 YBN
[1888 AD]
6021) Erik (Alfred Leslie) Satie (CE 1866-1925), French composer, composes
"Gymnopédies".

Paris, France (presumably)  
111 YBN
[01/20/1889 AD]
4057) Eötvös is one of the founders of the Hungarian Mathematical and
Physical Society.
(given at Hungarian Academy of Sciences, at the time worked at University of
Budapest) Budapest, Hungary  
111 YBN
[02/16/1889 AD]
211) Dr. John A McWilliam reports in the British Medical Journal his
experiments in which application of an electrical impulse to the hearts of
animals and recommends electric shock as a way of stimulating a feeble or
stopped heart into beating. McWilliam also shows that electrical stimulation
can result in a stronger heart beat.

McWilliam writes:
"... Such a mode
of excitation seems to be available in the form of a
periodic series
of single induction shocks sent through the heart at approximately
the normal rate
of cardiac action. A single induction shock
readily causes a beat in an inhibited
heart, and a regular series
of induction shocks (for example, sixty or seventy per
minute)
gives a regular series of heartbeats at the same rate. Never on
any occasion have
I seen fibrillar contraction excited by such a mode of stimulation. In order to
elucidate more fully the influence
of a series of induction shocks upon the inhibited
heart, I
have frequently (in the dog, cat, and rabbit) performed such
experiments
as the following. The animal being chloroformed, and
means being taken to preserve,
as far as possible, the normal temperature,
the thorax and pericardial sac were laid open;
artificial
respiration was kept up through a cannula introduced into the
trachea. The heart
was inhibited by stimulation of the vagus
nerve in the neck, and then a periodic
series of induction shocks
(regulated by a metronome) was applied to the apex of the
ven- tricles. Contraction of the autricles and ventricles was recorded
by an adaptation
of the graphic method; a blood-pressure tracin
was simultaneously made in the usual
manner. In this way I
was able to obtain an accurate record of the various
changes, while
at the same time some further information was obtained by direct
inspection
of the heart. A series of single induction shocks excites
a corresponding series of
cardiac beats; the ventricular contraction
precedes the auricular contraction when the
exciting
shocks are applied to the ventricles. Each systole causes the ejet:-
tion of a
considerable amount of blood into the aorta and pulmonary
artery, and a marked rise of
the blood-pressure at each
beat. The mean pressure is raised from the low point to
which it
had fallen ...
Such a method, it seems to me, is the only rational and
effective
one for stimulating by direct means the action of a heart which
has been suddenly
enfeebled or arrested in diastole by causes of a
temporary and transient
character. Of course, at the same time,
the expedient of artificial respiration must
by no means be neglected,
but, on the contrary, most sedulously attended to.".

(Note that McWilliam uses the phrase "borne in mind", which probably implies
that he gets D2B and to go public with this may have been a collective D2B
decision.)
(Perhaps a similar electrical stimulation could cause the lung muscles to
work.)
(University of Aberdeen) Aberdeen, Scotland  
111 YBN
[03/12/1889 AD]
6255)
Kansas City, Missouri, USA  
111 YBN
[03/14/1889 AD]
3844)
(Royal College of Science) Dublin, Ireland  
111 YBN
[04/09/1889 AD]
4211)
(Eastman Dry Plate Company) Rochester, NY, USA  
111 YBN
[04/27/1889 AD]
3805) In 1862 Dutton joins the Union army, reaching the rank of major in 1890.
Washington, D.C., USA.   
111 YBN
[05/02/1889 AD]
4117) FitzGerald greatly advances the development of technical education in
Ireland.
FitzGerald is one of the initial group, which includes Heaviside, Hertz, and
Lorentz, that takes Maxwell’s electromagnetic theory seriously and begins to
explore its consequences. FitzGerald extends Maxwell's electromagnetic theory
of light to try to explain light reflection and refraction in terms of waves in
an ether medium, in his paper "Electromagnetic Theory of the Reflection and
Refraction of Light" (1878).

In 1878 FitzGerald publishes a short note on "On the Theory of Muscular
Contraction" which ends with the word "tension".
Dublin, Ireland  
111 YBN
[06/03/1889 AD]
4834)
(University of Glasgow) Glasgow, Scotland  
111 YBN
[06/21/1889 AD]
4021) Motion picture camera and projector. Moving images captured and stored on
plastic film and projected onto a screen. The moving images are played together
with sound from a phonograph.

William Friese-Greene (CE 1855-1921), makes thin sheets of celluloid, which he
then cuts into a series of narrow strips, and joins them together, sensitized.
Friese-Greene then takes a series of photographs taken at about thirty photos
per second. He prepares similar celluloid transparencies from these negatives
and exhibits these at the Crystal Palace in 1889.

William Friese-Greene and Mortimor Evans patent (number 10,131) the first known
plastic film strip moving picture camera and projector. This is the first known
perforated celluloid film used for recording and projecting images of moving
objects. It seems clear that, if images of thought were seen in 1810, that
capturing and projecting moving images occurred much earlier, but was kept
secret from the public and not immediately published.

A few months earlier in the USA, the George Eastman company had filed a patent
for celluloid photo-sensitized roll film for still image capture on April 09,
1889. Two years earlier in the USA Hannibal Goodwin had patented
photo-sensitized celluloid roll film.

A report on the perforated celluloid film camera is published in the British
"Photographic News" on February 28 1890. On 18 March, Friese-Greene sends a
clipping of the story to Thomas Edison, whose laboratory had been developing a
motion picture system known as the Kinetoscope. The report is reprinted in
"Scientific American Supplement" on April 19, 1890. (Find full documents of
patent, "Friese-Greene" book only has part and there is no mention of plastic
or celluloid - but it is clearly a film roll camera - although Marey had
accomplished this in 1888.)

In June 1889 Friese-Greene wrote to Edison describing his camera. On November
15, 1889 issue of the "Optical Magic Lantern Journal" prints an illustration
and technical description of Friese-Greene's celluloid movie camera using the
word "transparencies", and including the information that "...When the
reproduction of speech is also desired this instrument is used in conjunction
with the phonograph". The "Daily News" publishes an article about the invention
on December 6, 1889. (find both articles if possible) The Bath Photographic
Society holds the first public show of motion-pictures taken on celluloid in
the rooms of the Bath Literary and Scientific Society on February 25, 1890. In
April 1890, the "Scientific American Supplement" carries an article on the
Friese-Greene camera.

According to at least one source, this is the first practical moving image
capturing and playing camera.

The Scientific American Supplement article does not explicitly state that this
is a celluloid, transparent or plastic film camera. The article concludes "Mr.
Greene stated to the meeting that the latern had been invented by an
acquantance of his in the west of England. By an improvement upon that latern,
now in the course of manufacture, Mr. Greene hopes to be able to reproduce upon
the screen, by means of photographs taken with his machine camera, stret scenes
full of life and motion; also to represent a man making a speech, with all the
changes in his countenance, and, at the same time, to give the speech itself in
the actual tones of the man's voice by means of a loud-speaking phonograph.".
This article also uses the word "render" which is a very early use of the
secret keyword "render" in 1890, this keyword may imply that people and other
moving objects are currently rendered in three-dimensions in real-time by
computers - as hard as that is to believe. In fact, it seems so difficult to
accept, that this must be viewed as highly speculative, but it might fit if
people saw thought in October 1810. In particular thinking of the precise
pin-point accuracy needed for galvanically contracting a muscle by activating a
single or small quantity of neurons in a moving object.

In November 1910, a US court will rule that Friese-Greene's patent has priority
over that over that of Edison's. In a biography of Friese-Greene the author
writes "Many people, and most Americans, gave Edison credit for inventing the
motion-picture camera, though none of Edison's biographer's seem to have
attached much importance to it. But the "Encyclopedia Britannica", of which the
tenth edition was sold over here by "The Times" in 1902, gave the credit to
Edison in edition after edition.". Perhaps this is because Friese-Green did
not really sell and widely distribute the moving camera as Edison did and
clearly Marey in France had a working film roll camera, although with paper
film, before Friese-Greene (see ) in 1888. It seems clear that there are always
several people of each nation working on the same technological advance like
the motion picture film camera

Friese-Greene writes an article in 1889 describing how he captures an image
from his eye - by looking at an arc light for a few seconds and then exposing a
photographic plate to his eye, then using a microscope to confirm that the
image of the arc light is captured on the photographic plate. This is very
close to talking about capturing images from behind the head of what the eyes
see, and thought-images.

In 1888 Étienne Jules Marey (murA) (CE 1830-1904) used a roll of sensitized
paper to capture images of moving objects, with an electromagnetic film
stopping device to avoid blurry images.

It should be noted that "Nature" magazine for 1889 and 1890 list nothing about
Friese-Green's device of 1889, and only mention Edison's work on the
phonograph, and an article about Muybridge's photographs of the galloping horse
that refers to Marey.

For excluded outsiders, there are many questions about the life of
Friese-Greene. Was he an outsider who figured out that people had kept seeing
eyes and thought a secret, to be enjoyed by only a twisted elite few? Or was
Friese-Greene an insider (insofar as an insider is defined as at least
regularly seeing and hearing thoughts...at least at the consumer "insider"
level) that worked with other insiders to bring some small progressive
technology to the public? Was this plastic film movie camera at this time, far
outdated, behind the phone company and government secret electronic microscopic
camera with electronic digital storage media, what was the nature of the
storage being used by those who see thought at this time? Clearly the cameras
and microphones were "wireless" using low frequency photons to transmit
ultimately to a large storage device, presumably at the phone company and
secret military buildings. The one biographical book on Friese-Greene writes
that Friese-Green "did SEE", but it seems unlikely, and more likely that
Friese-Greene spent his entire life as an outsided excluded person with most of
the rest of the public.
(Piccadilly) London, England  
111 YBN
[06/21/1889 AD]
4024) The full text of the article contains numerous hints and is as follows:
"PHOTOGRAPH
S MADE WITH THE EYE.
(Read before the London and Provincial Photographic
Association.)

By way of preface to the subject I am about to bring before you to-night, may I
ask if you have ever seen anything with your eyes shut? And when I say with
your eyes shut, do not mistake me and run away with the notion that I am in any
way referring to any imaginary mental vision one can conjure up in the dark.
For instance, look at an object that is fairly illuminated, steadily for a few
seconds, then suddenly close your eyes, and a similar object can be seen. I do
not attempt to explain this, though it is evidently governed by some law; and
it leads me at last, after no end of failures, to the discovery which is one of
the subjects of my paper to-night, namely, that you can obtain a photograph
with the human eye if you have a light strong enough and a plate sensitive
enough. After no end of failures, I obtained an impression with the aid of an
electric arc lamp, 2,000 candle-power, which I have at my place, 92 Piccadilly,
for taking photographs. I looked at the arc light for fifteen seconds, then
switched the light off and exposed a very quick plate (a plate coated in
different layers, which makes it much more sensitive), and held it to my eye
for a minute or more. On developing it I found a spot, which pleased me very
much. If you put the spot under a powerful microscope you can see the image of
the arc. I have, obtained marks with the magnesium flash-light, but they are
not so good as with the electric arc ; in fact, there is nothing definite about
them.

I have my flash-light here, so if any of you would like to try the experiment,
I shall be very pleased to watch the proceedings, for I begin to value my eyes
more than I did at first, because after one experiment I did at Piccadilly, I
had a black spot hovering about the retina for some days. With Mr. Debenham's
advice, and that of others, I have come to the conclusion that it is dangerous
; and the black spot did not go off until I put a piece of red glass before the
arc light and looked at it for two minutes, which seemed to counterbalance the
effect I shall not try it many more times, for, after all, sight is very
precious. I have only chanced one eye always, but it may affect the other, so I
intend to be careful.

I may say, here, just one or two things with regard to the eye. It is by it we
alone can judge, not only of its own perfection, but also of the comparative
value of any given optical combination. It is endowed with considerable freedom
of motion ; and no doubt we shall have to go to the eye for many optical
points. I may here say the retina is a transparent substance composed of nerve
fibres spread out into a thin layer, and corresponding to the ground-glass of
the camera. The retina receives the picture from the object in front, and being
connected with the optic nerve behind, the picture is conveyed to the brain. 1
believe if one could analyze them, there are salts in the retina corresponding
to those used in photography, though probably of a much more sensitive nature ;
and the electric magnetic effect of light conducts to the brain, where there is
always an alkali and acid to develop, and the atom deposit in the cells can be
called at will to answer our memory. Perhaps I am going a little too far, both
for myself and others who may think in a similar way, also for those who do not
think in the same way ; but there is no harm in giving you my thoughts, as it
seems to me we like dabbling in ideas that are a perpetual mystery. But now to
offer some suggestions with regard to the picture produced by the eye. Can it
be reflected from the retina, from the cornea, or from the back surface of the
lens ? Is there a kind of phosphorescence which can affect a photographic plate
? Is it some kind of electric phenomena, and our latent image a galvanic action
? Of course, these suggestions are very wild ; for I must confess although I
discovered the effect, I cannot explain it, and the more I try to do so the
more ignorant I feel. It may lead to something important as time rolls on.
Photography is now making huge strides ; its history becomes a clueless
labyrinth of confusion and uncertainty ; it has vigorous health and plenty of
practical and mental ingenuity always at hand, which affords ample proof of the
earnestness with which experimental investigators work. Experimenters should
work out their internal nature, with the aid of experiments]of things contained
in the varied world around them, then they will have something original to tell
us, and be continually adding atoms to the progress of our fascinating art. I
know, for my own part, I have formed a love and veneration for
photography—with all its worry, disappointments, etc.—which has almost the
nature of a passion ; 'every act of seeing leads to consideration,
consideration to reflection, reflection to combination, and combination to
ideas which ought to be worked out with method and system, then we shall be
sure to discover something quite new and original, especially if we work
earnestly and patiently.

Friese Greene.".
(London and Provincial Photographic Association) London, England  
111 YBN
[08/30/1889 AD]
3973)
Technische Hochschule, Karlsruhe, Germany  
111 YBN
[11/12/1889 AD]
3966)
Harvard College Observatory, Cambridge, Massachusetts, USA  
111 YBN
[11/28/1889 AD]
3818)
(Astrophysical Observatory at Potsdam) Potsdam, Germany  
111 YBN
[1889 AD]
3399)
London, England (presumably)  
111 YBN
[1889 AD]
3549)
London, England (presumably)  
111 YBN
[1889 AD]
3701)
(University of Freiburg) Freiburg, Germany  
111 YBN
[1889 AD]
3765)
(Moscow University) Moscow, Russia  
111 YBN
[1889 AD]
3953)
Sorbonne, University of Paris, Paris, France (presumably)  
111 YBN
[1889 AD]
4074)
(Military Medical Academy), St. Petersburg, Russia  
111 YBN
[1889 AD]
4081) Heaviside is almost entirely self-taught.
Heaviside is forced to publish his papers at
his own expense because of their unorthodoxy. (Perhaps also because of his lack
of doctorate degree and no formal education.)

Heaviside publishes "Electrical Papers" in 1892, in which he makes use of an
unusual calculatory method called operational calculus, now better known as the
method of Laplace transforms, to study transient currents in networks.
According to Encyclopedia Britannica, Heaviside's early results are not
recognized, possibly because the papers are written using his own notation.

A year later in 1893, Heaviside publishes his "Electromagnetic Theory"
(1893–1912).
London, England (presumably)  
111 YBN
[1889 AD]
4090) In 1913 Richet wins a Nobel prize in medicine and physiology for work on
anaphylaxus.

In later years Richet grows interested in telepathy and extrasensory
perception. (Probably Richet's work in this area might provide some
whistleblowing information to people who have been excluded, which may be as
many as 90% of the humans on earth. What kind of research into neuron reading
and writing did Richet discuss and perform? How far did he get to reading from
or writing to neurons? Was he an excluded or included? Was he trying to expose
it?)
(University of Paris) Paris, France  
111 YBN
[1889 AD]
4128) Ramón y Cajal is born in a poverty stricken and isolated village in
Navarre, the son of a barber-surgeon.
In 1906 Ramón y Cajal shares the Nobel prize for
medicine and physiology with Golgi.
Ramón y Cajal wrote some 20 books and 250
scientific papers.
Among Ramón y Cajal's many books concerning nervous structure is
"Estudios sobre la degeneración y regeneración del sistema nervioso", 2 vol.
(1913–14; "The Degeneration and Regeneration of the Nervous System") and the
classic "Histology" (tr. 1933).

Ramón y Cajal determined that Spain should have a place on the scientific and
intellectual stage. He succeeds in founding a Spanish school of histology.

It is rare to see a person (Ramon y Cajal is one person - people might think
because of the "y" that this is two people) in Spain credited for science
advances, and perhaps this is because, like much of South America, the terrible
influence of the followers of Jesus who have tended to frown upon science,
learning and all things positive, logical and pleasureful, although no evidence
exists that Jesus was opposed to science, learning or consensual pleasure - and
there were contemporary and earlier scientists like Thales, Anaxagoras,
Archimedes, Euclidos, etc - so plenty to comment on - the view may have been
one of either not informed of these people's written works, or informed but not
caring enough to comment or leave any record expressing any opinion of science
or earlier or contemporary scientists. A similar problem exists in Arab nations
because of similar views of many in Islam. It is interesting to note any
comments Muhammad had about earlier and contemporary scientists. Only a few
years after Muhammad, Al-Razi criticizes Islam and religion in general.
(University of Barcelona) Barcelona, Spain  
111 YBN
[1889 AD]
4225)
(Herzoglich Gymnasium) Wolfenbüttel, Germany  
111 YBN
[1889 AD]
4277)
(Robert Koch’s laboratory) Berlin, Germany  
111 YBN
[1889 AD]
4278)
(Robert Koch’s laboratory) Berlin, Germany  
111 YBN
[1889 AD]
4342)
(Institute of Physics of the Academy of Sciences) Stockholm, Sweden  
111 YBN
[1889 AD]
4396) In 1905 Lenard is awarded the Nobel prize in physics for studies of
cathode rays in open air.

In August 1914 Lenard is swept along by the wave of patriotism and nationalism.
Most scientists eventually find their way back to a more sober view, but Lenard
persists in his position of supernationalism.

Lenard is openly anti-Semitic and supports the Nazi doctrines, one of only 2
important scientists, the other being Stark. Lenard denounces "Jewish science",
perhaps forgetting his debt to Hertz who is of Jewish descent. Lenard denounces
Einstein and the theory of relativity purely on racial grounds and advances no
scientific arguments of merit (of which there are in my view more than one, for
example that space dilation is taken from an excuse to save the ether theory,
that photons are probably the basis of all matter, but obviously never on
racial grounds.) Lenard rejects the theory of quantum mechanics too. Lenard
knows Hitler personally and coaches Hitler on the racial interpretation of
physics. This will help Hitler to ignore progress in physics, in particular in
atomic research, and fail to develop the atomic bomb, despite the German people
initially leading the field.

For an examination of Hertz and Lenard's relationship see "Heinrich Hertz and
Philipp Lenard: Two Distinguished Physicists, Two Disparate Men".
(The rise of Nazism
and nationalism is Germany stopped the solid lead in science they had, and most
science was geared towards war and destruction, and based on fraudulent false
theories.)

(Perhaps Lenard represents the terrible transistion from the wise days of
Bunsen, Kirckhoff, Helmholtz, Rontgen, and Hertz, to the war-based views that
perhaps lead to or are popular up to and including the time of World Wars 1 and
2.)
(University of Heidelberg) Heidelberg, Germany  
111 YBN
[1889 AD]
4439) Nernst says that Roentgen should have patented the X ray and got money
from it.
In 1893 Nernst publishes a textbook on theoretical chemistry which makes
use of the thermodynamic ideas of people such as Ostwald.
Both Nernst's sons die in WW
I.
In 1920 Nernst wins the Nobel prize in chemistry for his third law of
thermodynamics.
Two of Nernst's daughters marry Jewish people and his last years are spent in
disfavor because this is a considerable crime under Nazi rule in Germany
(Nernst dies in November 1941).
( University of Leipzig) Leipzig, Germany  
111 YBN
[1889 AD]
4521)
(Massachusetts Institute of Technology) Boston, Massachusetts, USA  
111 YBN
[1889 AD]
6031)
(U.S. Marines) Washington, District of Columbia, USA  
110 YBN
[02/??/1890 AD]
4223)
(University of Lund) Lund, Sweden  
110 YBN
[06/11/1890 AD]
3974)
University of Heidelberg, Heidelberg, Germany  
110 YBN
[09/04/1890 AD]
4301)
(Lick Observatory) Mount Hamilton, CA, USA  
110 YBN
[11/15/1890 AD]
3243)
New York City, NY, USA  
110 YBN
[12/17/1890 AD]
4458) Steinmetz has a hunchback which his father and grandfather also had.
Steinmetz
joins a student socialist club at the University of Breslau, which was banned
by the government after becoming affiliated with the German Social Democrats.
When some of his fellow party members are arrested, Steinmetz takes over the
editorship of the party newspaper, “The People's Voice.” One of the
articles Steinmetz writes is considered inflammatory, the police began a
crackdown on the paper, and Steinmetz has to leave Breslau (1888).

Steinmetz builds generators capable of producing electricity at extremely high
potential (voltage), high enough to make large lightning bolts. Steinmetz's
last major project working at the General Electric Company, is designing a
generator that produces a discharge of 10,000 amperes and more than 100,000
volts, equivalent to a power of more than 1,000,000 horsepower for 1/100,000 of
a second.

Steinmetz holds 200 patents for electrical inventions.
(Rudolf Eickemeyer's company) New York City, USA  
110 YBN
[12/26/1890 AD]
4123) The Union Sulphur Company, of which Frasch is president, becomes the
earth's leading sulfur-mining company.
Cleveland, Ohio, USA  
110 YBN
[1890 AD]
3740) The 1911 Encyclopedia Britannica state that Lockyer's "The Meteoritic
Hypothesis" (1890) propounds a comprehensive scheme of cosmical evolution,
which has evoked more dissent than approval.
(Solar Physics Observatory) South Kensington, England (presumably)  
110 YBN
[1890 AD]
3807) In 1876 James switches professions from physiology to psychology, a
science in its infancy. James views psychology as an experimental science based
on physiology and not as a vague form of philosophy.

In later life James is interested in "psychic research", which has grown
fashionable at the turn of the century. (what does "psychic research" mean?
research into how the brain functions? ultimately this interest must have
resulted in the work of Pupin, the student of Hemholtz who was very interested
in the senses, and perhaps tried to see thought.)

In 1907 James publishes "Pragmatism: A New Name for Some Old Ways of Thinking"
in which he supports an idea of reality based only on experience. It is
interesting how this universe interpreted only by sensed theory plays out into
the 1900s. The popular view is summed many times with the question: if nobody
can hear a tree fall, does it actually fall? To me the answer is yes, because I
believe in an external universe, even without humans, but the other view is
that the universe does not exist without the viewer. It is interesting that
this view seems so closely linked to George Berkeley is his efforts to disprove
the theory of gravity and atheism of Newton by appealing to all space, time and
motion as being relative as opposed to absolute, and then to Mach whose work
inspires Einstein who accepts the non-euclidean theory and space-dilation. So
are these simply mistakes that the majority and in particular wealthy people
believe and propagate or is there something more to it? Is it just a
coincidence and piecing together of theories through out history that many of
these theories seem to be found together or a directed effort at inaccuracy and
misinformation? I don't know if it is just mistaken beliefs or systematic
deception. I probably lean towards honest mistaken views, with an element of
natural selection, as inaccurate, abstract and complex ideas appeal to the
majority who have been tricked by the obviously inaccurate claims of
religions.

It is amazing how over-valued this person is - even with no serious science
contributions - there is a lot of data documented about this person. What a
terribly misplaced focus - and so it is on all of psychology. For some as of
yet unexplained reasons, psychology rose up and has found enormous popularity
among average people. I think it has to do with people being easily tricked by
abstract terminology, by authority, and abstract theories about health and
because they never receive a basic history of science. It's stomach turning to
see this kind of misplaced popularity - but this is typical of the centuries
under Christianity and in particular the secret of seeing, hearing and sending
images and sounds and remote neuron activation where murderers hold vast wealth
and power and the honest are murdered and persecuted. Documenting some of this
is important for the story of the rise of pseudosciences, and popular mistaken
beliefs.

(My current appraisal of psychology is that 1) there needs to be the stringent
requirement of consent-only incarceration and treatment, and at least
no-treatment-when-objection and 2) some parts of psychology may be viewed as a
science, which I would describe as a science that seeks to cure diseases
perceived with no known physiological cause, or in the realm of healing people
with perceived problems through talking - in a similar way that teaching the
history of science may have a healing effect in a person's brain and mind.
Unfortunately, the unconsensual abuse of many millions of people will, I think,
always leave an unpleasant association with psychology. If consensual only,
clearly the popularity of psychology would go down as would the money earning
potential of those in psychology. People would still seek consensual psychology
or psychiatric health services. I think it very well may be that psychology
falls to be similar to seeing a psychic, astrologer, tribal witchdoctor, or
herbologist, and so-called homeopathic health. science. It seems clear that
psychology has found a space where physiology does not accommodate - in
perceived problems where there is no physical explanation or cause, or a person
simply wants to talk toa somebody. Definitely there is a focus on the science
of the "mind" as something different from anatomy or physiology of the brain.
in some sense the mind, in a physical sense is how the brain is wired - the
connections the owner of the brain makes. My own feeling is that, with
certainly, I will never need and certainly never buy the services of a person
in psychology. Then thinking beyond this, I don't think there is anybody who
really should buy psychology services - but of course, if consensual and it
helps a person according to their own view, I see nothing wrong with that, and
I think it can be called science when consent and is experimentally shown to
improve a person according to their own view. Possibly psychology should be
defined only as "Science of the mind". It is amazing how this science has been
used, I think, unlike any other science to violate and torture people's bodies.
Perhaps because when the issue is the mind, as opposed to the brain, a person
can question all the words and writings of another person as being
unrepresentative of their "sane" mind and so the wants of one person can
therefore be set aside and replaced by the wants of a different person. It is
the total loss of a person's right to decide for themselves, to own property,
to reject health care operations, etc.)
(Harvard University) Cambridge, Massachusetts, USA  
110 YBN
[1890 AD]
3968)
Harvard College Observatory, Cambridge, Massachusetts, USA  
110 YBN
[1890 AD]
4138)
(Johns Hopkins Medical School) Bartimore, Maryland, USA  
110 YBN
[1890 AD]
4166)
Lynn, Massachusetts, USA  
110 YBN
[1890 AD]
4169)
Tel Hasi, Palestine  
110 YBN
[1890 AD]
4173)
(University of Leiden) Leiden, Netherlands  
110 YBN
[1890 AD]
4200) In 1901 Behring wins the first Nobel prize in physiology and medicine.
(Robert Koch Institute of Hygiene) Berlin, Germany  
110 YBN
[1890 AD]
4241) Freud praises cocaine highly, which supposedly contributes to a wave of
cocaine addiction in Europe.
In 1886 Freud enters private practice as a neurologist.
In 1938 one
month after the Nazi occupation of Austria, the 82 year old Freud is taken to
safety in London where he will spend the last year of his life, dying of cancer
of the jaw.
(private practice at the Vienna Institute for Child Diseases and teaching at
the University of Vienna) Vienna, Austria (presumably)  
110 YBN
[1890 AD]
4293) Thomson founds a company that merges with Edison's company to form
General Electric in 1892.
By the end of his life Thomson holds some 700 patents and
has received many awards.
Lynn, Massachusetts, USA  
110 YBN
[1890 AD]
4487) In 1913 Werner wins the Nobel prize in chemistry for his coordination
theory.
(Polytechnikum) Zurich, Switzerland  
110 YBN
[1890 AD]
6020) (Achille-)Claude Debussy (1862-1918), French composer, composes "Clair de
Lune" ("Moonlight", in "Suite bergamasque", 1890–1905).

The title refers to a folk song that was the conventional accompaniment of
scenes of the love-sick Pierrot in the French pantomime. The name comes from
Paul Verlaine's poem of the same name which also refers to 'bergamasques' in
its opening stanza, and should not be confused with "Au clair de la lune" a
traditional song and the first publicly known recorded song. (verify)

Paris, France (presumably)  
109 YBN
[01/15/1891 AD]
4257)
(Trinity College) Cambridge, England  
109 YBN
[01/30/1891 AD]
4186)
(University of Berlin) Berlin, Germany  
109 YBN
[03/17/1891 AD]
3610)
Cleveland, Ohio, USA  
109 YBN
[03/26/1891 AD]
3522) After graduation from Trinity College, Dublin, in 1848 Stoney works as an
assistant to the astronomer, Lord Rosse, at his observatory at Parsonstown
until 1853 when Stony is appointed professor of natural philosophy at Queen's
College, Galway.
In 1857-1893 Stoney becomes secretary of the Queen’s University in
Dublin.
(Queen's University) Dublin, Ireland  
109 YBN
[04/25/1891 AD]
4247)
(Tesla's private lab) New York City, NY, USA  
109 YBN
[05/20/1891 AD]
4018) Edison will greedily try to claim priority on the process of
"cinematography", but loses in court because of earlier patents by Le Prince,
and Friese-Greene.
(private lab) West Orange, New Jersey, USA  
109 YBN
[11/??/1891 AD]
4292)
(University of Bonn) Bonn, Germany  
109 YBN
[12/10/1891 AD]
3822)
(Royal Institution) London, England (presumably)  
109 YBN
[1891 AD]
3639)
(University of Munich) Munich, Germany  
109 YBN
[1891 AD]
3746)
(University of Berlin) Berlin, Germany  
109 YBN
[1891 AD]
3832)
(Royal Institution) London, England   
109 YBN
[1891 AD]
3918)
(University of Bonn) Bonn, Germany  
109 YBN
[1891 AD]
3952) In 1908, Lippmann will win the Nobel prize in physics for his method of
color photography.
University of Paris, Sorbonne Laboratories of Physical Research, Paris,
France  
109 YBN
[1891 AD]
3963)
Cracow Academy, Crakow, Austria (now Poland)  
109 YBN
[1891 AD]
3969) 1903 Pickering is the first to publish a photographic map of the entire
sky.
Arequipa, Peru  
109 YBN
[1891 AD]
3993)
(Ecole de Médecine) Paris, France  
109 YBN
[1891 AD]
4147)
(University of Würzburg ) Würzburg , Germany  
109 YBN
[1891 AD]
4171)
Tell El-Amarna, Egypt  
109 YBN
[1891 AD]
4239) In 1881, working for Edison, Acheson, had installed the first electric
lights in Italy, Belgium, and France.
(Carborundum Company) Monongahedla City, Pennsylvania, USA  
109 YBN
[1891 AD]
4242)
Greenland  
109 YBN
[1891 AD]
4417)
(University of Heidelberg) Heidelberg, Germany  
109 YBN
[1891 AD]
4488)
(Polytechnikum) Zurich, Switzerland  
109 YBN
[1891 AD]
6030)
Michoacán, Mexico (verify)  
108 YBN
[05/??/1892 AD]
3624)
(Needles Lighthouse) Alum Bay  
108 YBN
[05/??/1892 AD]
4399)
(University of Bonn) Bonn, Germany  
108 YBN
[07/??/1892 AD]
4363)
(Pasteur Institute) Paris, France  
108 YBN
[08/17/1892 AD]
6259)
Chicago, Illinois, USA  
108 YBN
[08/??/1892 AD]
3834)
(Royal Institution) London, England   
108 YBN
[09/03/1892 AD]
4316) In 1889 Barnard begins to photograph the Milky Way with large-aperture
lenses, revealing much new detail.

In the 1890s Barnard sees craters on Mars, when the sun is in a good position
to cast shadows on Mars, but does not publish thinking it could be an illusion,
but his observation is correct.

In the course of his life, Barnard discovers 16 comets.

Barnard and Hale are the first to realize that the dark patches in the Milky
Way are clouds of obscuring gas and dust. (but what specifically are they
composed of? Hydrogen and Helium? perhaps ice chunks of water and other
molecules?) (chronology)
(Lick Observatory) Mt. Hamilton, California, USA  
108 YBN
[12/??/1892 AD]
4140)
(Academy of Sciences) Paris, France  
108 YBN
[1892 AD]
3623) Preece attended graduate studies at the Royal Institution of Great
Britain, London, under Michael Faraday.
Preece encourages Guglielmo Marconi by obtaining
assistance from the Post Office in furthering Marconi’s work. Preece also
introduces into Great Britain the first telephones, patented by Alexander
Graham Bell.
London, England (presumably)  
108 YBN
[1892 AD]
3700)
(University of Freiburg) Freiburg, Germany  
108 YBN
[1892 AD]
3823)
(Royal Institution) London, England (presumably)  
108 YBN
[1892 AD]
3867)
(University of Pavia) Pavia, Italy  
108 YBN
[1892 AD]
3932)
(University of Halle) Halle, Germany  
108 YBN
[1892 AD]
3933)
(University of Halle) Halle, Germany  
108 YBN
[1892 AD]
4174)
(University of Leiden) Leiden, Netherlands  
108 YBN
[1892 AD]
4236)
(Cross and Bevan's private business) New Court, Lincoln's Inn, England  
108 YBN
[1892 AD]
4306)
Kaluga, Russia (presumably)  
108 YBN
[1892 AD]
4310) In 1920 Sharrington is President of the Royal Society.
Sherrington publishes
text-books and papers on neurophysiology.
In 1932 Sharrington with Edgar Adrian, win the Nobel
Prize in medicine and physiology.
Sherrington lives to 95.
(Brown Institution Animal Hospital) London, England  
108 YBN
[1892 AD]
4326) Diesel is a pacifist and internationalist.
Diesel is funded by a St. Louis brewer and the
first diesel engine is built in the United States.
In 1913 Diesel disappears from the
deck of the mail steamer "Dresen" while on the way to London and is presumed to
have drowned. Perhaps neuron writing - one of the list of millions and millions
of neuron writing victims - the murderers probably never punished or even seen
by the public.
(Carle von Linde firm) Berlin, Germany  
108 YBN
[1892 AD]
4360)
(Columbian University, now George Washington University), Washington, D.C,
USA  
108 YBN
[1892 AD]
4397)
(University of Heidelberg) Heidelberg, Germany  
108 YBN
[1892 AD]
4446)
(St. Petersburg University) Saint Petersburg, Russia  
108 YBN
[1892 AD]
6012)
Klin (outside Moscow), (U.S.S.R. now) Russia (presumably)  
107 YBN
[03/04/1893 AD]
3841)
(Strutt Home Laboratory) Terling, England  
107 YBN
[04/17/1893 AD]
4161)
(Clark University) Worcester, Massachusetts, USA  
107 YBN
[04/18/1893 AD]
4393)
(Edison's company) West Orange, N.J., USA  
107 YBN
[05/03/1893 AD]
3888)
(Science and Art Department) South Kensington, England (verify)  
107 YBN
[07/??/1893 AD]
4459)
(International Electrical Congress) Chicago, Illinois, USA  
107 YBN
[09/05/1893 AD]
3244)
Indianapolis, Indiana (guess)  
107 YBN
[1893 AD]
3220)
Hartford, Connecticut, USA (presumably)  
107 YBN
[1893 AD]
3449) From 1891-1893 Janssen erects an observatory on Mount Blanc.
(Mount Blanc Observatory) Mount Blanc, France  
107 YBN
[1893 AD]
3668)
Sorbonne, Paris, France  
107 YBN
[1893 AD]
3811) Josef Breuer (BROER) (CE 1842-1925), Austria physician, and Sigmund Freud
publish ("On the psychical mechanism of hysterical phenomena: preliminary
communication", 1893) which becomes the foundation of psychoanalysis. This is
published in book form as "Studien über Hysterie" ("Studies on Hysteria") in
1895.

Breuer and Freud write:
"A chance observation has led us, over a number of years, to
investigate a great variety of different forms and symptoms of hysteria, with a
view to discovering their precipitating cause - the event which provoked the
first occurence, often many years earlier, of the phenomenon in question. In
the great majority of cases it is not possible to establish the point of origin
by a simple interrogation of the patient, however thoroughly it may be carried
out. This is in part because what is in question is often some experience which
the patient dislikes discussing; but principally because he is genuinely unable
to recollect it and often has no suspicion of the causal connection between the
precipitating event and the pathological phenomenon. As a rule it is necessary
to hypnotize the patient and to arouse his memories under hypnosis of the time
at which the symptom made its first appearance; when this has been done, it
becomes possible to demonstrate the connection in the clearest and most
convincing fashion.
This method of examination has in a large number of cases produced
results which seem to be of value from a theoretical and a practical point of
view.".

Here is a modern definition of "hysteria":
"The term 'hysteria' has been in use for over
2,000 years and its definition has become broader and more diffuse over time.
In modern psychology and psychiatry, hysteria is a feature of hysterical
disorders in which a patient experiences physical symptoms that have a
psychological, rather than an organic, cause; and histrionic personality
disorder characterized by excessive emotions, dramatics, and attention-seeking
behavior.".

(I think it is obvious that "hysteria" is hardly a disease, or if a problem, at
the very least certainly not a serious problem.)
Although close for many years, Breuer
and Freud separate in 1896 and never speak again due partly to quarrels over
their work.
(in his own home?) Vienna, Austria (now Germany)  
107 YBN
[1893 AD]
3861) Dorothea Klumpke Roberts (CE 1861-1942) is the first woman to earn a PhD
at the University of Paris.

(University of Paris) Paris, France  
107 YBN
[1893 AD]
3917)
(University of Zurich) Zurich, Switzerland  
107 YBN
[1893 AD]
3988) George Westinghouse (CE 1846-1914) US engineer, wins contracts for
supplying alternating current (AC) electricity for the Chicago World's Fair and
Niagara Falls, which is a large victory for AC electricity in the USA.

(Westinghouse Electric Company) Pittsburg, PA, USA  
107 YBN
[1893 AD]
4116)
(University College) Liverpool, England (presumably)  
107 YBN
[1893 AD]
4187)
(University of Berlin) Berlin, Germany  
107 YBN
[1893 AD]
4379) In 1896 Finsen establishes a Light Institute in Copenhagen.
In 1903
Finsen wins the Nobel Prize in medicine and physiology.
In 1904 Finsen dies at age 43.
(cause? a says failing health)
  
107 YBN
[1893 AD]
4421) Henry Ford (CE 1863-1947) US industrialist builds his first working
gasoline engine.
Ford is a machinist's apprentice at age 16.
Ford admires Hitler, and is
openly anti-Jewish. Asimov claims that Ford was incredibly shrewd in business,
but stupid in intellectual matters. (probably from religion.)
(Detroit Edison Company) Detroit, Michigan, USA  
107 YBN
[1893 AD]
4427) According to Asimov, Baekeland planned to ask $50,000 and go down to
$25,000 but Eastman made an offer first.
Baekeland graduates high school at 16, and
gets a doctor's degree at 21.
In 1924 Baekeland is the president of American
chemical society.
(Baekeland's business) New York City, NY, USA  
107 YBN
[1893 AD]
4432) In 1911 Wein wins a Nobel prize in physics for his work on black body
radiation.
(University of Berlin) Berlin, Germany  
107 YBN
[1893 AD]
4440)
( University of Göttingen) Göttingen, Germany  
107 YBN
[1893 AD]
4449)
(University of Hannover) Hannover , Germany  
107 YBN
[1893 AD]
4489)
(Polytechnikum) Zurich, Switzerland  
107 YBN
[1893 AD]
6017)
(National Conservatory) New York City, New York, USA  
106 YBN
[01/19/1894 AD]
3828)
(Royal Institution) London, England   
106 YBN
[04/14/1894 AD]
2996) M. Bonetti invents an influence machine (static electricity generator).

This machine is based on the Wimhurst design but uses sectorless disks and sets
of several brushes in the neutralizer bars. The idea of a sectorless machine,
can be traced back to Holtz and Poggendorff, by 1869. In this configuration,
output is taken at the front disk only, combs (that do not touch the disk) are
used instead of (contact) brushes in the neutralizer bars, and a different
driving system is used.

  
106 YBN
[05/??/1894 AD]
4092) According to the Dictionary of Scientific Biography, Righi discovered and
described magnetic hysteresis in 1880, a few months before Warburg, who is
credited with the discovery, and Righi also patented a microphone using
conductive powder and a loudspeaker. Magnetic hysterisis is the lagging of the
magnetization of ferromagnetic material, such as iron, behind variations of the
magnetizing field.

Righi is a prolific writer, writing more than 130 papers before 1900.
(Institute of Physics, University of Bologna) Bologna, Italy  
106 YBN
[07/25/1894 AD]
3611) In 1916 Jenkins helps found the Society of Motion Picture Engineers,
later renamed the Society of Motion Picture and Television Engineers (SMPTE),
and is elected as the organization's first president.
Washington, D.C., USA.   
106 YBN
[10/??/1894 AD]
4258) A possible pro-sexual reference, in the Faraday style, may be found when
Thomson writes "The method I employed is as follows :- ...". Notice the "ass
follows" then the universal penis and testicles symbol ":-". The funniness is
that the method Thomson employs is his penis. The sentence kind of jumps out of
the page and that gives it humor too. But it's speculation.
(Trinity College) Cambridge, England  
106 YBN
[1894 AD]
2692)
Tianjin (and Shanghai), China  
106 YBN
[1894 AD]
3144)
(University of Basel) Basel, Switzerland  
106 YBN
[1894 AD]
3913)
Hong Kong  
106 YBN
[1894 AD]
3919)
(University of Bonn) Bonn, Germany  
106 YBN
[1894 AD]
3929)
London, England (presumably)  
106 YBN
[1894 AD]
4085)
(University College) London, England  
106 YBN
[1894 AD]
4110)
(Royal Observatory) Greenwich, England  
106 YBN
[1894 AD]
4115)
(Royal Institution) London, England  
106 YBN
[1894 AD]
4204)
(University of Berlin) Berlin, Germany  
106 YBN
[1894 AD]
4220) In 1887 Takamine founds the chemical fertilizer industry in Japan when he
builds the first super-phosphate factory in Tokyo, the Tokyo Artificial
Fertilizer Company.
(Takamine and this time may mark the beginning of the rise of
Japanese modern science and technology which will greatly advance, in
particular with the computer, image and sound and data capture and storage,
robot, and vehicle industries.)
(His private laboratory) Tokyo, Japan (presumably)  
106 YBN
[1894 AD]
4226)
(Herzoglich Gymnasium) Wolfenbüttel, Germany  
106 YBN
[1894 AD]
4237)
(Cross and Bevan's private business) New Court, Lincoln's Inn, England  
106 YBN
[1894 AD]
4279)
Hong Kong  
106 YBN
[1894 AD]
4305)
Kaluga, Russia  
106 YBN
[1894 AD]
4311)
(Brown Institution Animal Hospital) London, England  
106 YBN
[1894 AD]
4318)
Java  
106 YBN
[1894 AD]
4333) A book of Tyndall's popular essays on science turns him from liberal arts
to physics.
In 1890 Pupin joins the faculty of Columbia.
Pupin's autobiography "From Immigrant To
Inventor" wins the Pulitzer Prize in 1924. (Does this FITI have a meaning of
fight-eye?)
(Columbia University) New York City, NY, USA  
105 YBN
[01/31/1895 AD]
3842) Both Ramsay and Rayleigh win a Nobel award in 1904 for the discovery of
argon.

Ramsay blows his own glass instruments.
According to the Encyclopedia Britannica, Ramsay's
discovery of the noble gases makes him the most famous chemist in Britain.
(Own Laboratory) Terling, England  
105 YBN
[03/06/1895 AD]
4351)
(Sorbonne) Paris, France  
105 YBN
[03/26/1895 AD]
4141)
(University College) London, England  
105 YBN
[04/??/1895 AD]
4032)
New York City, NY, USA (presumably)  
105 YBN
[05/05/1895 AD]
4345) In December 1905 Popov is ordered by the governor of St. Petersburg to
take repressive measures against student political disturbances. Popov refuses,
and this event severely affects his health. Popov dies soon afterward. (It
looks like Popov was probably murdered - in particular only aged around 47.)
(University of St. Petersburg) St. Petersberg, Russia  
105 YBN
[05/13/1895 AD]
4534) In 1927 Wilson wins the Nobel prize in physics for the cloud chamber.
(Sidney Sussex College, Cambridge University) Cambridge, England  
105 YBN
[05/29/1895 AD]
3820)
(Munich Thermal Testing Station) Munich, Germany  
105 YBN
[06/20/1895 AD]
4450)
(University of Hannover) Hannover , Germany  
105 YBN
[11/05/1895 AD]
3936) Members of the New Jersey State government try to create a law banning
the use of X rays in opera glasses to protect women's privacy.
In 1896 Roentgen
shares the Rumford medal with Lenard.
In 1901 Roentgen wins the first Nobel
prize in physics.
Roentgen rejects offer of ennoblement and the right to add "von"
before his last name.
Roentgen dies in somewhat poor finances from the
hyper-inflation that followed World War I.
The unit of X-ray dosage is called the
roentgen.
(University of Würzburg) Würzburg, Germany  
105 YBN
[12/28/1895 AD]
4031)
Paris, France (presumably)  
105 YBN
[1895 AD]
3529)
(University of Copenhagen) Copenhagen, Denmark  
105 YBN
[1895 AD]
3722)
(Nautical Almanac Office) Washington, DC, USA  
105 YBN
[1895 AD]
3954)
Sorbonne, University of Paris, Paris, France (presumably)  
105 YBN
[1895 AD]
3991) Interesting that Baumann dies so closely to the year of his big
discovery. In the "Science" obituary, the death is described using the word
"suggestion" which is a key word, "baumann was actively engaged in the solution
of many probelms suggested by this last great discovery when, after an illness
of only two days, death put an end to a brief but brilliant career.".
(University of Freiberg) Freiberg, Germany  
105 YBN
[1895 AD]
4029)
(Edison's Black Maria Studio) West Orange, New Jersey, USA  
105 YBN
[1895 AD]
4175)
(University of Leiden) Leiden, Netherlands  
105 YBN
[1895 AD]
4176)
(University of Leiden) Leiden, Netherlands  
105 YBN
[1895 AD]
4188)
(University of Marburg) Marburg, Germany  
105 YBN
[1895 AD]
4201) Jules Henri Poincaré (PwoNKorA) (CE 1854-1912), French mathematician
develops the theory of topology in his "Analysis Situs" (1895). Analysis Situs
is the name for the theory of topology (also known as surface geometry) at the
time.
Before this Poincaré had worked on celestial mechanics, the three-body
problem. This is before computers, and equations can take days to calculate and
plot. Now calculating the mutual effect, moving, and plotting millions of
points according to Newton's law of gravity may take only seconds.

In examining the positions of celestial orbits Poincaré discovers that even
small changes in the initial conditions can produce large, unpredictable
changes in the resulting orbit. This idea of a small change in initial
conditions causing largely different results relates to what is now called
chaos theory. Poincaré summarizes his new mathematical methods in astronomy in
"Les Méthodes nouvelles de la mécanique céleste", 3 vol. (1892, 1893, 1899;
"The New Methods of Celestial Mechanics").

In 1905, Poincaré writes a paper on the motion of the electron, which,
according to the Encyclopedia Britannica, with other papers of his at this
time, comes close to anticipating Albert Einstein's discovery of the theory of
special relativity. But Poincaré never takes the decisive step of combining
space and time into space-time.

Poincaré does theoretical work on tides and rotating fluid spheres which
support the work of G. H. Darwin.

Poincaré's first cousin Raymond Poincaré is President of France during World
War I.
(University of Paris) Paris, France  
105 YBN
[1895 AD]
4208) Hampson also published two volumes of science for the public: "Radium
Explained" (1905) and "Paradoxes of Science"(1906).
London, England (presumably)  
105 YBN
[1895 AD]
4243)
Greenland  
105 YBN
[1895 AD]
4302)
(Allegheny Observatory) Pittsburgh, Pennsylvania, USA  
105 YBN
[1895 AD]
4420) In 1947 Walden publishes an important history of chemistry.
(Riga Polytechnical School) Riga, Latvia  
105 YBN
[1895 AD]
4513) Sabine does not get a doctorate degree before teaching.
(Harvard University) Cambridge, Massachussets, USA  
105 YBN
[1895 AD]
4703) In 1919 Bordet wins the Nobel prize in medicine and physiology for work
on complement fixation.
Bordet holds out against the theory of viruses, thinking the
bacteriophages identified by Twort are not living organisms but only toxins,
that is non-living chemicals.
Bordet contributes significantly to the foundation of
serology, the study of immune reactions in body fluids.
(Pasteur Institute) Paris, France  
105 YBN
[1895 AD]
4717) Perrin supports the De Gaulle (anti-Nazi) government in France from the
USA after France fell to the Nazism.

(For the pronounciation of Perrin's last name is "PeraN" correct? because I
don't think there is an "a" sound in the French language - but perhaps there
was adapted from England for English words, for example.)
(École Normale) Paris, France  
105 YBN
[1895 AD]
4810)
(Sorbonne) Paris, France  
105 YBN
[1895 AD]
4826) In 1894 Marconi reads an article about the electromagnetic waves
uncovered by Hertz eight years earlier, and realizes that radio waves might be
used in signaling, and by the end of the year is ringing a bell at a distance
of thirty feet.
In 1895 Marconi sends a signal from his house to his garden,
and later over a mile and a half.
In 1896 The Italian government is uninterested (in
Marconi's radio message sending) and Marconi goes to England (his mother is
Irish and speaks perfect English) where he sends a signal nine miles.
In 1897 in Italy
Marconi sends a signal from land to a warship 12 miles.
In 1898 in England, Marconi
sends a signal 18 miles.
1899 Marconi uses the word "rendered" in a paper on wireless
telegraphy.
In 1904 a demonstration of radio operation is very popular at the St, Louis
World's Fair.
(How would have seeing and hearing thought been? That would have
been popular.)
In 1909 Marconi shares the Nobel Prize in physics with Braun. (Mainly
Marconi developed the process Hertz first found, but Marconi must have made
some improvements, and transmitting a signal over the Atlantic Ocean is
important.)
Marconi is in charge of Italy's radio service during World War I.
Marconi
enthusiastically supports Mussolini's Fascist government.
Marconi is sent as a
delegate to the peace conference of World War I in Paris (1919) and there signs
the peace treaties with Austria and with Bulgaria.
From 1921 on Marconi uses his steam
yacht "Elettra" as home, laboratory, and mobile receiving station in
propagation experiments. (Interesting that perhaps being at sea he wanted to be
able to detect people or particle devices trying to move close to him, although
this would require underwater sensors too.)
In 1929 Marconi is created marchese and
nominated to the Italian senate.
In 1930 Marconi is chosen president of the Royal
Italian Academy.

(It's not clear if Marconi was aware of neuron reading and writing before going
public with his radio communication devices. Being from a wealthy family
implies that Marconi is somehow selected by the insider group to bring wireless
particle communication to the public. This also implies that the Marconi family
may have been a secret provider of radio service already - and simply extend it
to the public at small "phony" planned increments demonstrating devices they
were surpassed long before.)

(Possibly something started the public release of wireless communication.
Joseph Henry, Ampere, Faraday, Edison and others had already publicly described
electric induction to communicate signals from one wire to another. But
clearly, to bring particle (wireless) message sending to the masses instead of
keeping it for an elite few must have required some kind of volitility inside
the group maintaining the secret telegraph and neuron reading/writing networks
- which ultimately is the telegraph and telephone companies, and presumably the
military part of governments.)

Accoring Answers Biographies Marconi is educated by private tutors and attended
the Livorno (Leghorn) technical institute for a short time. In his 1899 paper,
Marconi cites help from assistants. This may imply possibly that Marconi
supervised wireless work done by others without actually assembling devices
himself, in particular as a wealthy person most likely involved in ownership,
development and administration of neuron reading and writing. Possibly Marconi
was some kind of counter to AT&T because the initials att are used by Marconi
in 1899 and by others in biographies of Marconi. An alternative theory is that
Marconi was a subset of AT&T to make them not appear too large.]

(The view from those who control neuron reading and writing must be an
incredibly interesting view - and is somewhat difficult to imagine for those
who do not see people's thought screens. It seems clear that these people are
familiar with most of the typical thought images that people have, and how to
minimally activate certain neurons in any humans brain to get them to move and
make decisions that those neuron writers want them to make. In particular, the
view must have been terrible during the World Wars. Clearly those humans in the
telecommunications had the best view of all the eyes and thoughts - and perhaps
even used neuron writing to advance the poor people employed in the militaries.
Perhaps even some part of the wars were fought virtually by humans controlling
computers, which in turn fight against each other using poor humans in the
armies more or less as unthinking pawn on a chess board - absolutely
controlling their every movement. It's not clear how advanced the particle beam
technology was and is, but clearly, it has rendered and continues to render and
track many objects on earth in real-time.)
(father’s estate) Bologna, Italy  
104 YBN
[01/24/1896 AD]
3941)
(City and Guilds Technical College) Finsbury, England  
104 YBN
[01/26/1896 AD]
3939)
(Reale Istituto Veneto di science) Veneto, Italy  
104 YBN
[02/10/1896 AD]
3938)
Renfrew, England  
104 YBN
[02/12/1896 AD]
4334)
(Columbia University) New York City, NY, USA  
104 YBN
[02/22/1896 AD]
3940)
Philadelphia, Pennsylvania, USA (presumably)  
104 YBN
[02/24/1896 AD]
4150) Henri Becquerel is a member of a scientific family extending through
several generations, the most notable being his grandfather Antoine-César
Becquerel (1788–1878), his father, Alexandre-Edmond Becquerel (1820–1891),
and his son Jean Becquerel (1878–1953).
Becquerel's father, Alexandre Edmond Becquerel did
important work with fluorescence.
In 1903 Becquerel shares the Nobel prize in physics with
the Curies.
(École Polytechnique) Paris, France  
104 YBN
[03/02/1896 AD]
4151)
(École Polytechnique) Paris, France  
104 YBN
[03/03/1896 AD]
4535)
(Sidney Sussex College, Cambridge University) Cambridge, England  
104 YBN
[03/09/1896 AD]
3937)
(University of Würzburg) Würzburg, Germany  
104 YBN
[03/18/1896 AD]
4276)
(Private Lab) New York City, NY, USA (presumably)  
104 YBN
[03/25/1896 AD]
4152)
(École Polytechnique) Paris, France  
104 YBN
[04/06/1896 AD]
4335)
(Columbia University) New York City, NY, USA  
104 YBN
[04/23/1896 AD]
4033)
(Koster and Bial's Music Hall) New York City, NY, USA  
104 YBN
[04/??/1896 AD]
4445) Carver was the son of a slave woman owned by Moses Carver.
In 1865 slavery
outlawed in the USA.
In 1889 Carver is the first black person to attend Simpson
College in Indianola, Iowa.
After graduating from Simpson, Carver graduates from Iowa
State Agricultural College at the head of his class.
In 1892 Carver earns a
master's degree and joins the staff of Iowa State Agricultural College.
In 1896
Carver accepts a job for $1500 a year plus room and board, turning away other
offers with more money, to be a professor at Tuskegee Institute, in Alabama, a
black college founded by Booker T. Washington, to help young black people get a
higher education which Booker T. Washington himself had been unable to find.
In
1939 Carver is awarded the Roosevelt medal.

Late in his career Carver declines an invitation to work for Thomas A. Edison
at a salary of more than $100,000 a year. Presidents Calvin Coolidge and
Franklin D. Roosevelt visit him, and his friends included Henry Ford and
Mohandas K. Gandhi. In 1931 Joseph Stalin invites Carver to superintend cotton
plantations in southern Russia and to make a tour of the Soviet Union, but
Carver refuses.

In 1953 the plantation on which Carver was born is made a national monument.

Asimov describes Carver as a "chemical Burbank", developing not new plant
varieties but new plant products.
Asimov explains that Carver serves as an
example of the use of educating people of every race.

(It is interesting how people see things differently and appear to have
different callings perhaps based mostly on their education, upbringing or
surroundings, but perhaps somethings are genetic.)

(This story of Carter and Booker T too are wonderful and inspirational stories,
that I think would be nice to see on the big screen, or even television, but as
of yet, no.)
(Tuskegee University) in Tuskegee, Alabama, USA  
104 YBN
[05/06/1896 AD]
3717)
Potomac River, Washington DC, USA  
104 YBN
[05/12/1896 AD]
4340)
New York City, NY, USA (presumably)  
104 YBN
[05/19/1896 AD]
4715)
Llewellyn Park, New Jersey, USA   
104 YBN
[06/02/1896 AD]
4337) In 1917 Bose founds and becomes director of the Bose Research Institute,
Calcutta.
Bose is the first Indian to be elected a fellow of the Royal Society.
(Presidency College) Calcutta, India  
104 YBN
[06/02/1896 AD]
4827)
(father’s estate) Bologna, Italy  
104 YBN
[06/11/1896 AD]
4728) Rutherford was one of a dozen children as the son of a wheelwright
(builds and repairs wheels) and small-scale farmer.

Rutherford has a scholarship to New Zealand University.
Rutherford gets a scholarship to
Cambridge University. The first place winner refuses the scholarship in order
to stay in New Zealand and get married. In addition, the University of
Cambridge had recently changed its rules to allow graduates of other
institutions to earn a Cambridge degree after two years of study and completion
of an acceptable research project. The news reaches Rutherford on his father's
farm and he throws down his spade and says “That's the last potato I'll
dig.”, postpones his marriage and leaves for England.
In 1908 Rutherford win
the Nobel Prize in chemistry for the theory of radioactive disintegration of
elements, for determining the nature of alpha particles, for the theory of the
nuclear atom.

Zinc sulfide containing a trace of radium is used on watch faces to create
luminous figures that can be seen at night, but the women painting the figures
absorb traces of radium and get serious, slowly fatal cases of radiation
sickness. This is stopped once the dangers of radioactivity are made clear. (I
guess a radioactive atom may stay in the body continuously emitting photons
that cause mutation. There still needs to be some way of flushing them out of
the system. Maybe if they stay together they could be traced and surgically
removed, but possibly if charged they could be removed with a strong magnetic
field. If uncharged, maybe they could be charged somehow and then pulled out
with a strong magnetic field. Maybe some could be flushed out with a large
blood draining and transfusion/filtering based on radioactivity.)
Rutherford is the President
of the Royal Society from 1925-1930.
In 1933 Rutherford is strongly anti-Nazi and helps to
arrange help for Jewish scientists forced out of Germany, but does not help
Haber because Rutherford feels Haber's development of gas warfare was too
terrible.
In 1933 Rutherford wrongly calls doubts that the vast energy of the
atomic nucleus as revealed in radioactivity can someday be controlled, calling
the idea “moonshine”. Rutherford dies 2 years before the find of uranium
fission by Hahn.
Rutherford doubts Einstein's theory of relativity. (State
Rutherfords quotes if any.)
At McGill University Rutherford welcomes increasing
numbers of research students to his laboratory, including women at a time when
few females study science. For example, Rutherford's first graduate student is
a woman, Harriet Brooks, and Rutherford publishes a paper with Brooks.
Rutherford and William Pope write in "The Times" of London, in December 1920:
"For
our part, we welcome the presence of women in our laboratories on the ground
that residence in this University is intended to fit the rising generation to
take its proper place in the outside world, where, to an ever increasing
extent, men and women are being called upon to work harmoniously side by side
in every department of human affairs.".

Rutherford also actively contributes to using radioactivity to show that the
rocks of earth are far older than Kelvin's estimate of millions of years. (cite
papers)
(Cambridge University) Cambridge, England   
104 YBN
[06/11/1896 AD]
4737)
(Cambridge University) Cambridge, England   
104 YBN
[07/25/1896 AD]
3278)
Cambridge, England   
104 YBN
[09/02/1896 AD]
4828)
Slisbury Plain, England  
104 YBN
[11/25/1896 AD]
4153)
(École Polytechnique) Paris, France  
104 YBN
[11/??/1896 AD]
4165)
(Lick Observatory) Mt. Hamilton, California, USA  
104 YBN
[11/??/1896 AD]
4259)
(Cambridge University) Cambridge, England  
104 YBN
[12/10/1896 AD]
3698) From his explosives and from oil fields in Russia that he owns, Nobel
amassed a vast fortune. Nobel traveled widely and was a committed pacifist.

Although Nobel is unpopular, and viewed as the inventor of horrible tools of
war, Nobel actually thinks that his explosives would outlaw war by making it
too horrible.

The Encyclopedia Britannica explains that in 1888 Alfred's brother Ludvig had
died while staying in Cannes, France. The French newspapers reported Ludvig's
death but confused him with Alfred, and one paper has the headline "Le marchand
de la mort est mort" ("The merchant of death is dead."), and perhaps from this
Alfred Nobel established the prizes in his will to avoid this kind of
posthumous reputation suggested by this premature obituary. The awards Nobel
creates reflect his lifelong interest in the fields of physics, chemistry,
physiology, and literature. There is evidence that his friendship with the
prominent Austrian pacifist Bertha von Suttner inspires him to establish the
prize for peace.

The Nobel Institute in Sweden is named for Alfred Nobel.

Element 102 is first isolated at the Nobel Institute in Sweden in 1958 and is
named nobelium.

(I think a good idea for an award is one which awards those who popularize
science, full and constant democracy, stopping violence and torture, freeing
the unjustly imprisoned in hospitals and prisons, promoting tolerance of
consensual sexuality and nudity, promoting history of science, complete free
information, for invention in mechanics, electronics, robotics, transportation,
basically all those topics I have explained and desire for the Photon award.

I wonder how the secret camera-thought network affects the award decision. The
Nobel prize is not democratically decided as I would like the Photon award to
be. But I wouldn't doubt that many awards reflect a popular opinion. Some
winners, I think have not made serious contributions to science. Any awards for
theories or procedures of psychology, like Moniz and the lobotomy, will be
viewed as perhaps not the best choice. In particular in physics, since the rise
of non-Euclidean theory, almost all physics theories awarded will probably be
thought clearly to have no scientific value 500 years from now. In particular
theories about a big bang, expanding universe, background radiation, time
dilation, black holes in space-time, nuclear forces, quarks, light as an
electromagnetic wave, and similar theories, I think are doubtful or highly
speculative. Many of these awards appear to go to wealthy, mainstream people in
science, supporting mainstream theories. It is true that many new advances in
science probably require expensive technology. Clearly those developing secret
technology are not being recognized. Whoever first saw images from eyes has
never been recognized with a prize, so far as I know. The seeing and sending of
brain images has gone unrecognized, and may now contribute to secret behind the
thought curtain arrangements, but we excluded can only guess. On a positive
note, there have been many people who have won Nobel awards who probably did
deserve them and generally these and many other awards greatly advance science
on earth.)
(dies at) San Remo, Italy|(will, and awards are in)Stockholm, Sweden  
104 YBN
[12/12/1896 AD]
3444)
(Johns Hopkins University) Baltimore, Maryland, U.S.A.  
104 YBN
[12/29/1896 AD]
4759) Around 1932 Cannon will elaborate on an elaboration of Claude Bernard’s
concept of the constancy of the milieu intérieur by developing the concept of
“homeostatis” (as a result of his work studying hemorrhagic and traumatic
shock among wounded people in World War I). Homeostatis is the effort by the
body to maintain a stable internal environment despite fluctuations of the
outside environment. Hormones are primarily responsible for this effect, in
particular adrenalin.
(this needs specific examples, otherwise it is too general.)

Cannon identifies the compound secreted from nerve endings (particularly
influenced by adrenalin) which he names “sympathin” (because the nerve
endings belong to what is called in this time the sympathetic nervous system).
(chronology)
(Harvard Medical School) Cambridge, Massachusetts, USA  
104 YBN
[1896 AD]
4052)
(University of Amsterdam) Amsterdam, Netherlands  
104 YBN
[1896 AD]
4170)
Thebes, Egypt  
104 YBN
[1896 AD]
4240)
(Carborundum Company) Monongahedla City, Pennsylvania, USA  
104 YBN
[1896 AD]
4328) In 1929 Eijkman with Fred Hopkins, wins the Nobel prize in physiology and
medicine.
Javanese Medical School in Batavia (now Jakarta) (presumably)  
104 YBN
[1896 AD]
4343)
(Stockholms Högskola {now the University of Stockholm}) Stockholm,
Sweden  
104 YBN
[1896 AD]
4381) In 1920 Guillaume is awarded the Nobel prize for "invar".
(International Bureau of Weights and Measures) Sèvres, France  
104 YBN
[1896 AD]
4422)
(Detroit Edison Company) Detroit, Michigan, USA  
104 YBN
[1896 AD]
4494)
(Mareseilles University) Mareseilles, France  
104 YBN
[1896 AD]
5499)
(University of Jena) Jena, Germany  
104 YBN
[1896 AD]
6019)
Munich, Germany  
103 YBN
[01/07/1897 AD]
4262)
(University of Königsberg) Königsberg, Germany  
103 YBN
[01/??/1897 AD]
4460) In 1902 Zeeman and Lorentz are awarded the Nobel prize in physics.
(University of Leiden) Amsterdam, Netherlands  
103 YBN
[03/10/1897 AD]
3942)
(University of Würzburg) Würzburg, Germany  
103 YBN
[03/15/1897 AD]
4536)
(Sidney Sussex College, Cambridge University) Cambridge, England  
103 YBN
[04/30/1897 AD]
4260)
(Cambridge University) Cambridge, England  
103 YBN
[05/27/1897 AD]
3437)
(Tulse Hill)London, England  
103 YBN
[07/19/1897 AD]
4730)
(Cambridge University) Cambridge, England   
103 YBN
[08/20/1897 AD]
4296) Ross wins the 1902 Nobel prize in physiology and medicine.
  
103 YBN
[09/02/1897 AD]
4250)
(Private Lab) New York City, NY, USA  
103 YBN
[1897 AD]
3802)
(Ecole Polytechnique) Paris, France  
103 YBN
[1897 AD]
3912)
Calcutta, India  
103 YBN
[1897 AD]
4088) Electric display (Oscilloscope).

Oscilloscope demonstrated publicly. This leads to the first television, and in
some sense is the first television.

(Electronic images-images stored in electronic format as changes in electric
current can now be publicly displayed.) The first image to be displayed on an
oscilloscope (also called "Braun", or "Cathode Ray" Tube) is by Boris Rosing of
Russia.

(Is this the first use of an electromagnet to move an electron beam in a vacuum
tube? Did Plucker use electromagnets?)
(Physikal Institute) Strassburg, France  
103 YBN
[1897 AD]
4093) According to the Dictionary of Scientific Biography, Righi discovered and
described magnetic hysteresis in 1880, a few months before Warburg, who is
credited with the discovery, and Righi also patented a microphone using
conductive powder and a loudspeaker. Magnetic hysterisis is the lagging of the
magnetization of ferromagnetic material, such as iron, behind variations of the
magnetizing field.

Righi is a prolific writer, writing more than 130 papers before 1900.
(Institute of Physics, University of Bologna) Bologna, Italy  
103 YBN
[1897 AD]
4105)
(University of Groningen) Groningen, Netherlands  
103 YBN
[1897 AD]
4207) Charles Parsons is the youngest son of the famous astronomer William
Parsons, 3rd Earl of Rosse.
In retirement Parsons tries unsuccessfully to make
diamonds.
(The Parsons Marine Steam Turbine Co., Ltd., ) Wallsend on Tyne, England  
103 YBN
[1897 AD]
4222) In 1912 Sabatier shares the Nobel prize for chemistry with Victor
Grignard.
(University of Toulouse) Toulouse, France  
103 YBN
[1897 AD]
4297)
(Johns Hopkins University) Baltimore, Maryland, USA  
103 YBN
[1897 AD]
4307)
Kaluga, Russia  
103 YBN
[1897 AD]
4313)
(University of Liverpool) Liverpool, England  
103 YBN
[1897 AD]
4346)
(University of St. Petersburg) St. Petersberg, Russia (presumably)  
103 YBN
[1897 AD]
4433)
(technical college in Aachen) Aachen, Germany  
103 YBN
[1897 AD]
4441)
( University of Göttingen) Göttingen, Germany  
103 YBN
[1897 AD]
4469) Gomberg's family flees Russia when Moses' father is accused of
anti-Tsarist activity, and settle in Chicago.
(University of Heidelberg) Heidelberg, Germany  
103 YBN
[1897 AD]
4503)
(University of Munich?) Munich, Germany  
103 YBN
[1897 AD]
4522) The Yerkes telescope is completed which is supervised by George Ellery
Hale (CE 1868-1938) and funded by Charley Yerkes a wealthy US street-car
company owner. This is the largest refracting telescope, 40 inches, yet built.
Hale convinced Yerkes to fund this telescope.

Williams Bay, Wisconsin, USA  
103 YBN
[1897 AD]
4712) Claude produces liquid chlorine for use in poison gas attacks during
World War I.
Claude produces inert gases in quantity.
Claude supplies Ramsey with liquid
air in Ramsay's search for inert gases.
In 1945 Claude spends 5 years in prison for
supporting the Vichy government in France, which was considered a tool of the
Nazis.
(Compagnie Francaise Houston-Thomson) Paris, France  
103 YBN
[1897 AD]
4793)
(private lab) London, England(presumably)  
103 YBN
[1897 AD]
6032)
(Europe and ship crossing) Atlantic ocean  
103 YBN
[1897 AD]
6033)
(49th Austro-Hungarian Regiment) Sarajevo, (Austria-Hungary now)Bosnia
(verify)  
102 YBN
[04/12/1898 AD]
4352) Curie's mother is the principle of a girl's school and her father is a
physics teacher, but her mother dies of tuberculosis and her father loses his
job.
In 1891 Curie leaves Poland after saving enough money and enters the Sorbonne
in Paris. (How does Curie learn French?)
Curie lives a frugal life, fainting in
class from hunger at one point.
Marie had placed first on the women’s agrégation in
physics (15 August 1896).
In 07/25/1895 Marie Sklodowska and Pierre Curie (after his
piezoelectricity find) married in a civil ceremony both being anti-clerical,
with no wedding dress or rings, but instead buy two bicycles for transportation
on their honeymoon trip.
Pierre abandons his own research and joins Marie as a
willing and admiring assistant for the last 7 years of his life.
In 1903 the Curies
and Henri Becquerel share the Nobel prize in physics for their work in
radioactive radiations. The Curies are too ill to make the trip to Stockholm.

In 1906 Pierre is killed in a traffic accident with a horse-drawn vehicle.
Marie takes over Pierre's position at the Sorbonne and is the first woman to
ever teach there. (Asimov comments that this is remarkable in the notoriously
conservative world of French science.)

Marie is not elected into the august French Academy, losing by one vote because
she is a woman.

In 1911 Marie wins the Nobel prize in chemistry for identifying two unknown
elements.

During WWI Marie drives an ambulance.

The Curie's daughter Iréne Joliot-Curie, son-in-law Frédéric Joilot-Curie,
and neighbor Perrin all will win Nobel prizes.

In 1934 Marie Curie dies of leukemia (a form of cancer in the leukocyte-forming
cells of the body) from overexposure to radioactive radiation. (This makes
clear how radiation (mainly photons in gamma and X ray wavelengths can be used
as a terrible weapon to kill living objects.)

Asimov describes Marie Curie as the greatest woman scientist that ever lived.

(Asimov typed that Marie Curie comments on the vast energies poured out
continuously from a material such as radium, but the source of this energy will
remain a mystery until Einstein in 1905 shows how mass can be converted into
energy. t: To me this is not correct, because this is an example of photons,
electrons and possibly helium nuclei emitting from atoms due to a natural
process that probably results from gravity. I reject the idea of photons as
energy, and here clearly the word "energy" was applied to matter (photons). I
don't see how e=mc^2 which I view as meaningless, because energy does not
relate to anything real, is needed to explain why photons emit constantly from
radioactive atoms. Updating this with my current view - I would say that the
concept of energy is simply a combination - the product of mass and motion -
and I still reject the idea that matter and motion are interchangable.)

The story of Marie Curie is, like that of George Carver, very inspirational and
interesting. It shows that females can succeed in science. But as of yet, this
amazing story has never been made for the large screen or even television which
is truly stupid.
(École de Physique et Chimie Sorbonne) Paris, France  
102 YBN
[04/12/1898 AD]
4693)
(Cambridge University) Cambridge, England   
102 YBN
[04/??/1898 AD]
3868)
(University of Pavia) Pavia, Italy  
102 YBN
[05/02/1898 AD]
4380)
(Business: TH. Goldschmidt) Essen-on-the-Ruhr, Germany  
102 YBN
[05/10/1898 AD]
3824)
(Royal Institution) London, England (presumably)  
102 YBN
[06/03/1898 AD]
4142)
(University College) London, England  
102 YBN
[06/13/1898 AD]
4143)
(University College) London, England  
102 YBN
[07/01/1898 AD]
4255)
(Tesla's private lab) New York City, NY, USA  
102 YBN
[07/18/1898 AD]
4353)
(École de Physique et Chimie Sorbonne) Paris, France  
102 YBN
[07/18/1898 AD]
4354)
(École de Physique et Chimie Sorbonne) Paris, France  
102 YBN
[09/01/1898 AD]
4731)
(Cambridge University) Cambridge, England   
102 YBN
[09/08/1898 AD]
4144)
(University College) London, England  
102 YBN
[10/29/1898 AD]
4689)
(Sidney Sussex College, Cambridge University) Cambridge, England  
102 YBN
[12/??/1898 AD]
4261)
(Cambridge University) Cambridge, England  
102 YBN
[1898 AD]
3524) After graduation from Trinity College, Dublin, in 1848 Stoney works as an
assistant to the astronomer, Lord Rosse, at his observatory at Parsonstown
until 1853 when Stony is appointed professor of natural philosophy at Queen's
College, Galway.
In 1857-1893 Stoney becomes secretary of the Queen’s University in
Dublin.
Dublin, Ireland (presumably)  
102 YBN
[1898 AD]
3723)
(John's Hopkins University ?) Washington, DC, USA  
102 YBN
[1898 AD]
4109) Martinus Willem Beijerinck (BIRiNK) (CE 1851-1931), Dutch botanist
theorizes that the infectious agent from the tobacco mosaic disease identified
by Dmitry I. Ivanovsky in 1892, is a new kind of infectious agent, which he
named "contagium vivum fluidum", meaning that it is a live, reproducing
organism that differs from other organisms.

Beijerinck is led by several observations to conclude that the tobacco mosiac
agent is a unique type of pathogen. First, he finds that sap from plants
infected with tobacco mosaic disease does not lose infectivity after passage
through a filter impervious to microorganisms. In addition the agent can be
precipitated by alcohol, a property not normally associated with living
organisms. Second, Beijerinck observes that a filtered extract from infected
plants can diffuse in a solid agar medium. To Beijerinck this means that the
agent had to be "fluid" or non-particulate, since the capacity to diffuse is
then believed to be a means of distinguishing molecular substances from larger,
supposedly nondiffusing particles and cells. Third, he notes that the pathogen
is unable to reproduce outside the host and seems to multiply only in parts of
the plant undergoing rapid cell division. Reluctant to accept the idea of an
actively self-reproducing molecule, he suggests that replication might occur
passively by incorporation of the pathogen into the reproductive machinery of
the host cell. On the basis of these observations, Beijerinck concludes that
tobacco mosaic disease is caused by a contagium vivum fluidum. a term coined to
convey his concept of a living infectious agent in fluid (noncellular) form.

Beijerinck publishes his conclusion that tobacco mosaic disease is caused by an
infective agent that is not bacterial calling the disease agent a "filterable
virus" (virus is Latin for "poison"). Beijerinck presses out the juice of
diseased tobacco leaves, and passes it through a porcelain filter that can
remove any known bacterium, and finds that the resulting liquid can still
infect a healthy plant, and that this infected plant can then be used to infect
other plants. Beijerinck concludes that whatever the infecting germ is, that it
grows and multiplies. Earlier, Pasteur, finding no causative agent for rabies,
speculated that there are germs too small to see with a microscope. Ivanovsky
had observed that the tobacco mosaic disease can be transmitted by a filtered
liquid, but thought the disease is bacterial. Beijerinck is the first to name
this new class of disease agent, but the work of Stanley will show that viruses
are not liquid but are individual units (particles).

Beijerinck believes that the liquid is alive, and there is a debate whether a
virus is living. In my view, anything connected to DNA and/or RNA I would
describe as a form of life - even if not apparently alive.
(Dutch Yeast and Spirit Factory) Delft, Netherlands  
102 YBN
[1898 AD]
4125) An explosion while working with nitrogen and sulfur destroys sight in one
of Demarçay's eyes.
(personal lab) Paris, France  
102 YBN
[1898 AD]
4133)
(University of Greifswald) Greifswald, Germany  
102 YBN
[1898 AD]
4228)
(Herzoglich Gymnasium) Wolfenbüttel, Germany  
102 YBN
[1898 AD]
4280)
(Institute for Infectious Diseases) near Tokyo, Japan (presumably)  
102 YBN
[1898 AD]
4312)
(University of Liverpool) Liverpool, England  
102 YBN
[1898 AD]
4331)
(University of Vienna) Vienna (presumably)  
102 YBN
[1898 AD]
4434)
(technical college in Aachen) Aachen, Germany  
102 YBN
[1898 AD]
4514)
(Harvard University) Cambridge, Massachussets, USA  
102 YBN
[1898 AD]
4698) Electromagnetic writing and reading of data. Sound recorded and played
back magnetically.
(Copenhagen Telephone Company) Copenhagen, Denmark  
102 YBN
[1898 AD]
4704)
(Pasteur Institute) Paris, France  
101 YBN
[03/03/1899 AD]
4900)
(Marconi Company) London, England (verify)  
101 YBN
[03/17/1899 AD]
4319) Like Lowell, Pickering says that he saw signs of life on the planet by
observing what he supposes are oases in 1892. Pickering also claims to observe
signs of life on the Moon. By comparing descriptions of the Moon from Giovanni
Riccioli's 1651 chart onward, Pickering thinks that he has detected changes
that could be due to the growth and decay of vegetation.

There may be anaerobic bacteria, I would not be surprised, and how interesting
if there is not one cell of life of any kind on the moon of earth. If not now,
there certainly would be anaerobic bacteria living there very soon after humans
live there.


William Pickering also calculates the orbit of a possible trans-Neptunian
planet with results close to Lowell's.

Both William and Edward Pickering, I think, are examples of decent scientists
who spoke more truth, but generally lost to bad people who have more money and
power - mostly the controllers of the neuron reading and writing networks - and
whoever tries to sell relativity and any fraudulent or less accurate theories
in order to purposely mislead the public, to stop women's legal equality, and
supports other bad similar views.
(Harvard College Observatory) Cambridge, Massachussetts, USA  
101 YBN
[03/27/1899 AD]
4829)
South Foreland, England and Wimereux, France  
101 YBN
[04/18/1899 AD]
4089)
(Physics institute at Strasbourg) Strasbourg, France  
101 YBN
[05/01/1899 AD]
4455)
(University College Dublin) Dublin, Ireland  
101 YBN
[05/11/1899 AD]
4690)
(Sidney Sussex College, Cambridge University) Cambridge, England  
101 YBN
[05/??/1899 AD]
4885)
London, England (presumably)  
101 YBN
[08/??/1899 AD]
4491) Wilbur and his brother Orville bicycle, glide, and build an airplane
together.
Several years after the first flight the US government is not interested in the
airplane. (Unlike neuron reading and writing, the motorized airplane happily
becomes public knowledge and on the open market - although, like helicopters,
the sale of and usage are highly restricted.)
In 1908 Wilbur Wright takes the plane to
France.
In 1912 Wilbur Wright dies of typhoid fever.

Both brothers are sons of a minister, do not use tobacco, alcohol, don't marry
and always wear business suits even in the machine shop.

Orville in later life explains that in their home "there was always much
encouragement to children to pursue intellectual interests; to investigate
whatever aroused curiosity.", and in a less-nourishing environment, Orville
believed, "our curiosity might have been nipped long before it could have borne
fruit.".

Both brothers only have high school educations.

(Some time in the future flying cars will probably outnumber land only vehicle.
But the design will probably be an adapted helicopter for earth, and probably
hydrogen thrust vehicles for the moon.)
08/1899|Dayton, Ohio  
101 YBN
[09/13/1899 AD]
4732)
(McGill University) Montreal, Canada   
101 YBN
[09/??/1899 AD]
4739)
(École de Physique et Chimie Sorbonne) Paris, France  
101 YBN
[10/03/1899 AD]
4830)
New York City, NY, USA   
101 YBN
[10/03/1899 AD]
4831)
New York City, NY, USA   
101 YBN
[11/20/1899 AD]
4376)
(École de Physique et Chimie Sorbonne) Paris, France  
101 YBN
[11/22/1899 AD]
4733)
(McGill University) Montreal, Canada   
101 YBN
[12/11/1899 AD]
4374)
(École Polytechnique) Paris, France  
101 YBN
[12/??/1899 AD]
4265)
(British Association Meeting) Dover, England   
101 YBN
[1899 AD]
3724)
(John's Hopkins University ?) Washington, DC, USA  
101 YBN
[1899 AD]
3727)
(John's Hopkins University ?) Washington, DC, USA  
101 YBN
[1899 AD]
3825)
(Royal Institution) London, England (presumably)  
101 YBN
[1899 AD]
3891) Thomas Chrowder Chamberlin (CE 1843-1928), US geologist, argues against
William Thomson's theory that the Earth is only 100 million years old, arguing
that there were several ice ages which goes against Thomson's argument that a
single ice age is evidence of uniform cooling.

(University of Chicago), Chicago, Illinois, USA  
101 YBN
[1899 AD]
4154)
(École Polytechnique) Paris, France  
101 YBN
[1899 AD]
4177)
(University of Leiden) Leiden, Netherlands  
101 YBN
[1899 AD]
4347)
(University of Chicago) Chicago, illinois, USA  
101 YBN
[1899 AD]
4364)
(University College) London, England  
101 YBN
[1899 AD]
4391)
(Cape Observatory) South Africa  
101 YBN
[1899 AD]
4423) Henry Ford (CE 1863-1947) US industrialist founds a company (the Detroit
Automobile Company) to manufacture cars he designs.

Eli Whitney had introduced the manufacture of standardized parts a century
earlier.

(Detroit Automobile Company) Detroit, Michigan, USA  
101 YBN
[1899 AD]
4425) English chemists William Henry Perkin, Jr. (1860-1929) and Frederic
Stanley Kipping (CE 1863-1949) publish one of he first textbooks dedicated
strictly to organic chemistry.
This book remains the standard organic textbook for 50
years.

(Find image of Kipping)

(Heriot-Watt College, Edinburgh) Edinburgh, Scotland  
101 YBN
[1899 AD]
4472)
(Moscow State University) Moscow, Russia  
101 YBN
[1899 AD]
4473)
(Moscow State University) Moscow, Russia  
101 YBN
[1899 AD]
4533)
( University of Göttingen) Göttingen, Germany  
101 YBN
[1899 AD]
4720) Pope leave school at 15, is an assistant to Kipping, and becomes a
professor at the University of Manchester at 1901.
During WWI Pope develops methods
for producing large quantities of mustard gas.
(Institute of the Goldsmiths’ Company) New Cross, England  
101 YBN
[1899 AD]
4836) Debierne is friends of the Curies and is associated with their work.
(Sorbonne) Paris, France  
101 YBN
[1899 AD]
6046)
(George R. Smith College for Negroes) Sedalia, Missouri, USA (presumably)  
100 YBN
[01/18/1900 AD]
4372)
(École de Physique et Chimie Sorbonne) Paris, France  
100 YBN
[03/05/1900 AD]
4373)
(École de Physique et Chimie Sorbonne) Paris, France  
100 YBN
[03/26/1900 AD]
4155) A Google translation of Becquerel's work is all I can find:
"The part of
radiation from radium déviable by a magnetic field
is open to different experiences,
from which I quote the
following on rays that pass through the black paper
"I °
deviation in the magnetic gap. In order to investigate whether
air exerted a
significant influence on the propagation speed
radiation in question, I prepared the
experience of my deviation -
ence in a vacuum. I did not observe any noticeable
difference with this
that obtained in air.

The experiment was conducted in the following way a glass tube,
closed at one end and
connected by another, through a tube
lead, with a trunk to mercury, was placed
horizontally between
poles of an electromagnet and normally in a field. In this tube,
side of
a little phosphoric acid to dry air, was placed a
small photographic plate,
horizontal, wrapped in black paper;
on the plate was placed in a small bowl lead omm,
94 thick -
sor, containing the active ingredient collected in a hole about imm
diamete
r hole in a card kept below by paper
black and above by a very thin foil. In these
con -
ditions, the material can remain for several hours on the plate without
veil, and
only gives. impression directly beneath the
source, through the lead.

"It is now more or less completely in a vacuum tube, then
is passed through the
electromagnet currents that also maintains
constant as possible. Rays back on the
photographic plate
by the magnetic field impressed it on one side of the source.
After ten
minutes of installation, it interrupts the current;
Leaving the return air is then
passed to the electromagnet a neck -
rant equal to the first, during the same
time, but in the opposite direction of
to reject the impression the other side of
the source and can thus
compared to the same test the effects obtained in vacuum and
in air
atmospheric pressure.

"We operated with pressures'] mm, 2mm, of omm i mercury
and the almost absolute vacuum.
In all cases, the two impressions,


all the board below the source of an impression due to rays which
are reduced. If it
has, in space, on the path of rays, various
screens, their shadow is reproduced in the
plate, showing that the rays
normal field is reduced below the source itself, and
that
oblique rays are back on the field axis through the source.
Finally, if, next to the
horizontal plate, there is a plaque ver -
tical plan which extends above and
below the first,
obtains a section of the trajectories of all rays which meet and
we
recognize that they are back on the axis that passes through the source.
"It reflects
all the appearance assimilating the radiation
ing into question the cathode rays, and
considering the radiation
tion as subject to forces that seek the negative electrical
masses
tions across the magnetic field with great speed. In these
conditions, the
trajectories of rays normal to a uniform field is
circles passing through the
source, tangential to the original direction of
radiation and these circles have
equal radius R, whose value is
inversely proportional to the intensity of the
field. The rays emitted nor -
mally to a photographic plate parallel to the
magnetic field
return cut it normally, and produce an impression
maximum intensity. The rays
emitted tangentially to the plate re -
come on themselves tangentially to it and
produce no
printing.

For an oblique direction of propagation, making with the axis of
field angle x,
the trajectory is a helix which winds on a cy -
Lindre sinx radius R, having an
axis parallel to the axis of the field, and
tangential component of the trajectory
at the start. The helix is wound in the
sense of movement clockwise if the
propagation takes place
in the direction of the field, and in reverse if the
propagation takes place in a direction
otherwise.

i> These results, known for cathode rays, apply to
déviables rays of radium. The
location of maximum impressions on the plate
Photography is horizontal instead of
intersections with this
Plan rays whose directions are original in a vertical plane
paralle
l to the field. This place is an arc of an ellipse whose semi-axes
2R is the direction
perpendicular to the field, and the other would
Shooting for the direction of the
axis, but the rays do not reach this point.
All trajectories of these rays have the
same length TCR.
"The place of intersection with a plane normal to the axis of the
scope,
trajectories of oblique rays whose original elements are in
plane through the axis
is a curve whose starting point is on the axis
through the source, and whose tangent
at the origin is the intersection
two planes at an angle equal to "> d is the distance from
the plane to the source,
and R is the radius of the circular path described above.
Experience
verify this theoretical value.

In a magnetic field equal to 4OO ° CGS units were obtained
for R values close to 3mm,
7.

"40 dispersion in the magnetic field. It follows from the form of
trajectories
that, in the experiment described earlier this Note, if the
radiation was
homogeneous, the impressions should be arcs
Ellipse intense toward the outer edge
and diffuse toward the inner edge.
Even with a radiant source of very small diameter
arcs of el -
Lipsius are very diffuse outward, and the diffusion increases when,
decreas
ing the magnetic field increases the value of 2R. This dif -
merger appears to be
attributable to a dispersion of the magnetic field
tion, the beam of radiation which
my previous experiences ( ')
had already reported heterogeneity.

"If we have the photographic plate wrapped in paper
black, and placed parallel to the
field, displays of various kinds, such
a strip of aluminum omm, i thick, a strip of
copper
omm, O85, output in these screens consists of elliptical arcs shifted
against each
other. In a field of approximately 2400 units, and
another screen without the black
paper, the elliptical arc is in the minor axis
region of maximum intensity about 2R
= 12 ™ 2. Under the aluminum
2R = i6mm 5. Under the copper, the value of R 2 is
approximately twice that
obtained without the screen and these numbers are given
here only as an indi -
tion.

The impressions are the kinds of absorption spectra showing
that most rays deflected by
the magnetic field are the most
easily arrested under these conditions. But if,
instead of placing the screen
aluminum on the photographic plate is placed near the
source,
although the rays pass through successively aluminum and
black paper, the
elliptical arc obtained on the plate has the same position
if there was no aluminum. It
seems that aluminum, a very small
(2IO)

distance from the source is transparent to certain rays, and that the
stops when
they traveled in the air a distance of 2cm. I return -
drai shortly on these
phenomena.

"5 Considerations electrostatic deflection. - The facts
newly exposed part of the
show that radiation
Radium is quite similar to cathode rays, or
masses of negative
electricity carried with great speed. We
has been able to recognize the existence
of these electrical charges. He
But could we find himself in the presence of
masses of material
excessively low, carrying loads also very low,
too small to be easily
identified, but such that
report - the mass of the load was a significant order of
magnitude
in a magnetic field. We know that if v is the speed, intensity H
field and p the
radius of curvature of the trajectory, we must have
- V = H p. However, we found for
H = 4000, p = o0, we have
e

therefore approximately - v = i5oo. It should be noted that this number
is the same
order of magnitude as those found for
cathode rays by J.-J. Thomson ((), by W. Wien
(*) and
Mr. Lenard (3) which gave values of - v varying from io3o to 1273,
with values of
v between o, 67.10 'and 0.81. io10.
These masses must undergo movement in an electric
field
intensity F, a deviation 9 = F1 = F? is the length of
iooo y ° m

- V *

e

path in the field. We know we could not get far
no electrostatic deflection for
rays of radium. Maybe
Therefore it is that field employees were not sufficiently
intense.
It is reduced to this point assumptions, if we accept as
likely that the speed v
is, as the cathode rays of
the magnitude of the speed of light, such as in
the
experiments of Lenard, a quarter of that speed, we see that for
out on a journey of
icm deviation 0 of a few degrees or

6 to 0.20 io = i, 4> should make at least one electric field
2.iot2 units or a
potential difference of 20,000 volts between two pla -
Castles remote icm; should
therefore, for a deflection electromagnet
significant static, employing different potentials
equal to or greater
nal to those that cause explosive discharge between conductors
in the air,
which can be achieved in a vacuum, and does not appear
have been done so far. We can
not say anything until we have completed
experience in electric fields of the order of
magnitude of those
which were used for the study of cathode rays. "
(École Polytechnique) Paris, France  
100 YBN
[03/26/1900 AD]
4375)
(École Polytechnique) Paris, France  
100 YBN
[04/09/1900 AD]
4371)
(chemistry laboratory of the École Normale) Paris, France  
100 YBN
[04/12/1900 AD]
4429) Cannon is the oldest daughter of Wilson Cannon, a Delaware state senator,
and Mary Jump.

In 1896 Cannon joins the staff at Harvard University, during a time before even
having the right to vote, as a women, in the United States before 1920.

Jump is the first women to be awarded an honorary doctorate from the University
of Oxford (1925), is awarded the Henry Draper Medal of the National Academy of
Sciences (1931) and is also the first woman to become an officer in the
American Astronomical Society.
(Harvard College Observatory) Cambridge, Massachussetts, USA  
100 YBN
[05/03/1900 AD]
3675)
(private lab) London, England(presumably)  
100 YBN
[06/??/1900 AD]
3843)
(Own Laboratory) Terling, England  
100 YBN
[07/02/1900 AD]
3784) In 1906 Zeppelin builds an airship that has a speed of 30 mi (48 km) per
hr.
In 1928 is the first flight of the most successful dirigible, the Graf
Zeppelin, (Graf is German for count). This ship will go around the earth in
1929.
In 1937, the Hindenburg (a large Hydrogen filled directable balloon), bearing a
swastika, goes down in flames over New Jersey (which greatly lowers the
popularity of these vehicles).
Lake Constance, Germany  
100 YBN
[07/17/1900 AD]
4833)
London, England  
100 YBN
[08/27/1900 AD]
4205) James Carroll (CE 1854-1907), English-US physician on this day Carroll,
working in Cuba, as second in command to Reed in the now-famous commission sent
to Cuba to study yellow fever, doubting the theory of Carlos Finlay that a
mosquito acts as the vector in yellow fever, allows an infected mosquito to
bite his arm. Four days later Carroll has the first experimental case of yellow
fever. Carroll nearly dies, and acquirs a heart disease from which he will die
a few years later.

Lazear a fellow investigator will die from the disease.

A year before in 1899 Reed and Carroll had disproved Sanarelli’s theory that
Bacillus icteroides is the specific agent in yellow fever.

Cuba  
100 YBN
[10/19/1900 AD]
4327) Planck has considerable ability in music, and is an excellent performer
on the piano and organ. For example, Planck commissions the construction of a
harmonium with 104 tones in each octave.

According to the Encyclopedia Britannica, Planck is the first prominent
physicist to champion Einstein's special theory of relativity (1905). Planck
states that "The velocity of light is to the Theory of Relativity as the
elementary quantum of action is to the Quantum Theory; it is its absolute
core.". In 1914 Planck and the physical chemist Walther Hermann Nernst succeed
in bringing Einstein to Berlin. (It is interesting that Planck may be largely
responsible for the rise of the theory of relativity - perhaps larger neuron
forces and wealth were influential - only the phone comapny and government eye
and thought videos will show some century. Perhaps Planck and Einstein were
corpuscularists, non-believers in aether theory- but had to compromise - but it
seems unlikely given the unwavering support for the space and time-dilation of
Fitzgerald and Lorentz. in addition both apparently viewed light as
non-material - at least publicly.)

According to Asimov, Planck accepts Einstein's theory of relativity, but
rejects the quantum theory as applied to the photoelectric effect.
In 1918 Planck
receives the Nobel prize in physics for the quantum theory. Einstein and Bohr
will receive the Nobel a few years later.
In 1930 Planck becomes president of the
Kaiser Wilhelm Society of Berlin and it is renamed the Max Planck Society.
Planc
k never lends his voice to the Hitler regime.
In 1937 Planck intercedes
personally with Hitler on behalf of Jewish colleagues, unsuccessfully, and is
forced to resign his presidency of the Max Planck Society as a result, but will
be restored after WW II.
Planck's house is destroyed by allied bombing in WW
II.
Planck is rescued by allies while in flight during the last days of confusion
before the Nazi's final defeat.
Planck loses a son in WW I, 2 daughters in
childbirth, and his son Erwin, executed in 1944, accused of taking part in a
plot against Hitler's life.
(University of Berlin) Berlin, Germany  
100 YBN
[1900 AD]
3858)
Cape of Good Hope, Africa  
100 YBN
[1900 AD]
3860) (Sir) David Gill (CE 1843-1914), Scottish astronomer proposes that the
nations of the world join together and create an atlas of all the stars. The
Director of the Paris Observatory, Admiral Ernest Mouchez, suggestes that a
meeting should be held in Paris and this initiates the "Carte du Ciel"
project.

The Carte du Ciel project requires that all of the sky be photographed down to
the 14th magnitude on standard sized photographic plates.

Cape of Good Hope, Africa  
100 YBN
[1900 AD]
3890) Thomas Chrowder Chamberlin (CE 1843-1928), US geologist, together with
Moulon raise the theory Buffon had advanced 150 years before, that a star once
passed close to our star and that matter from both stars cooled into small
fragments, which then condensed into planets (as opposed to Laplace's theory
that planets formed simply from gravitational collapse). This is the
"planetesimal hypothesis".

Chamberlin and Moulin publish their work in "The Two Solar Families" (1928),
independently of a similar work by British astronomer Sir James Jeans.

According to the Oxford Dictionary of Scientists, the planetesimal hypothesis
has little support today as cannot account for the distribution of angular
momentum in the solar system.

(Does this presume that no objects form from gravitational collapse? Does this
view presume that gas does not accumulate and contract into stars and planets
as is thought for endo-nebuli? As it stands I doubt this theory exclusively,
but I can accept that stars collide. I think that planets probably can form as
a result of gravitation and collision of matter around a star.)

The current view is that planets and other orbiting objects formed from a cloud
of matter that condensed under gravity. in my view, these kinds of collisions
must happen, and how often could be calculated. Initially I am guessing that
collisions between stars are far more rare than time moving without any
star-star collision.

(This is an interesting theory and there need to be more simulations of the
accumulation of matter in star systems. These are massive and time consuming
simulations, star systems take billions of years to evolve, perhaps there is no
faster way to model this process. In addition, since modeling photons, atoms or
smaller objects would take too long, people generally model millions of
collective pieces of matter.)

(University of Chicago) Chicago, Illinois, USA  
100 YBN
[1900 AD]
4053)
(University of Amsterdam) Amsterdam, Netherlands  
100 YBN
[1900 AD]
4058)
(University of Halle) Halle, Germany  
100 YBN
[1900 AD]
4189)
(University of Marburg) Marburg, Germany  
100 YBN
[1900 AD]
4215)
(Eastman Kodak Company) New York City, NY, USA  
100 YBN
[1900 AD]
4303)
(Lick Observatory) Mount Hamilton, CA, USA  
100 YBN
[1900 AD]
4384) In 1925 Hopkins wins the Nobel prize in medicine and physiology with
Eijkman for enunciating what will ater be known as the "vitamin concept".
From 1930-1935
Hopkins is president of the Royal Society.
(Cambridge University) Cambridge, England   
100 YBN
[1900 AD]
4395)
  
100 YBN
[1900 AD]
4426)
(University College, Nottingham, now Nottingham University) Nottingham,
England  
100 YBN
[1900 AD]
4465)
(Army Medical School) Netley, England  
100 YBN
[1900 AD]
4470)
(University of Michigan) Ann Arbor, Michigan  
100 YBN
[1900 AD]
4478) Fessenden holds 500 patents at the time of his death, second only to
Edison.
Fessenden works for Edison in the 1880s and Edison's greatest rival
Westinghouse from 1890-1892.
(AM works by having a regular periodic sine wave, for example
one at 10 million cycles per second, and adding in a source signal. At the
receiving station the 10 million cycles per second sine wave is subtracted
leaving the source signal.)

(Clearly amplitude modulation must have been recognized much earlier - for
people to have started neuron reading and writing in at least 1810. Perhaps
Feesenden was a person excluded from the technology who reinvented it, or was
included and purposely allowed to release the truth about amplitude modulation
to the public.)

(Amplitude modulation is so simple an idea, that it occurs naturally in any
object that emits a periodic frequency of particles, which is pretty much all
matter. For example, sounds reaching the ear may impart an amplitude modulation
- which is a strength modulation - a quantity of particle modulation to any
regular interval signal emitted from the nerves of the ear portion of the
brain.)

(Probably amplitude modulation of wired recording of sound was the first
instance of listening to hidden microphones.)
(Western University of Pennsylvania, now the University of Pittsburgh)
Pittsburg, Pennsylvania, USA  
100 YBN
[1900 AD]
4504)
(Mikhail Artillery Academy ) St. Petersburg, Russia  
100 YBN
[1900 AD]
4725) During World War I, Grignard creates methods for producing phosgene, a
poisonous gas, and for detecting the first traces of mustard gas.
In 1912 Grignard
wins the Nobel Prize in chemistry with Paul Sabatier.
(University of Lyons) Lyons, France  
100 YBN
[1900 AD]
4806) Schwarzschild attended a Jewish primary school in Frankfurt, Germany. (At
the time were schools separated by race? Were Jewish children prevented from
attending non-all Jewish schools?)
Schwarzschild volunteers for military service in 1914
at the beginning of World War I and is sent home in 1916 with a rare skin
disease from which he dies. (Possibly murdered?)
(University of Munich) Munich, Germany (presented, but photos captured in
Vienna, Austria)  
100 YBN
[1900 AD]
6018)
Saint Petersberg, (U.S.S.R. now) Russia (presumably)  
100 YBN
[1900 AD]
6024) Jean Sibelius (original name Johan Julius Christian Sibelius) (CE
1865-1957), Finnish composer, the most noted symphonic composer of Scandinavia,
composes around this time.

Helsinki, Finland  
99 YBN
[01/01/1901 AD]
4252)
(University of Kansas) Kansas, USA  
99 YBN
[01/23/1901 AD]
4485)
Boston, Massachusetts, USA  
99 YBN
[02/07/1901 AD]
4119) Many people from the United States die in the Spanish-American War not
because of weapons but because of disease.
Some doctors actually allow themselves to be
bitten by mosquitoes to see if they get yellow fever. William Lazear does and
dies.
(Pan American Medical Congress) Habana, Cuba  
99 YBN
[02/14/1901 AD]
6342) Rollins publishes this a "X-Light Kills" in the "Boston Medical and
Surgical Journal".
Boston, Massachusetts, USA  
99 YBN
[03/02/1901 AD]
4435)
(Wurzburg University) Wurzburg, Germany  
99 YBN
[04/19/1901 AD]
4266) (Royal Institution) London, England  
99 YBN
[05/??/1901 AD]
4028)
(private lab) West Orange, New Jersey, USA (presumably)  
99 YBN
[10/27/1901 AD]
6026) Sergey (Vasilyevich) Rachmaninoff (CE 1873-1943), composer who is the
last great figure of the tradition of Russian Romanticism, composes his second
piano concerto.

(Somehow I don't think the melodrama will stop any time soon.)

Moscow, (U.S.S.R. now) Russia  
99 YBN
[12/12/1901 AD]
4832)
Poldhu, Cornwall, England to St. John’s, Newfoundland  
99 YBN
[12/31/1901 AD]
4120)
(Society of American Bacteriologists) Chicago, Illinois, USA  
99 YBN
[1901 AD]
4054)
(University of Amsterdam) Amsterdam, Netherlands  
99 YBN
[1901 AD]
4124)
(personal lab) Paris, France  
99 YBN
[1901 AD]
4148)
(University of Berlin) Berlin, Germany  
99 YBN
[1901 AD]
4156)
(École Polytechnique) Paris, France  
99 YBN
[1901 AD]
4221)
(his private laboratory) Clifton, New Jersey, USA  
99 YBN
[1901 AD]
4227)
(Herzoglich Gymnasium) Wolfenbüttel, Germany  
99 YBN
[1901 AD]
4357) Pierre Curie (CE 1859-1906), French chemist confirms Becquerel's finding
that radium can induce skin burns in a dangerous experiment whose danger was
unknown at the time.

Curie measures the heat given off by radium as 140 calories per
gram per hour. This is the first indication of the huge energy (that is large
quantity of mass and motion) available inside the atom.

(There must be a huge number of photons (and composite particles) inside atoms
and the number of atoms in a piece of material that is small compared to the
size of a human. ).

(Sorbonne) Paris, France  
99 YBN
[1901 AD]
4499) Despite his scientific achievements, Perrine and his office become a
target for nationalist politicians and Perrine is attacked verbally by deputies
in the Argentine Congress. In 1931 Perrine is barely missed by a sniper’s
bullet and in 1933 the Argentine Congress passes legislation removing authority
from the director of the observatory. (There are clearly parallels for me in
living in Orange County.)

In 1936 Perrine is forced into retirement (from the Argentine National
Observatory in Córdoba) by Argentine "rightests".
(Lick Observatory) Mount Hamilton, California, USA  
99 YBN
[1901 AD]
4515) In 1930 Landsteiner wins the Nobel prize in medicine and physiology for
identifying blood groups.
(Pathological-Anatomical Institute) Vienna  
99 YBN
[1901 AD]
4705)
(Institut Antirabique et Bacteriologique, in 1903 the Institut Pasteur du
Brabant) Brussells, Belgium  
99 YBN
[1901 AD]
4711)
Dolgoe Village, Orlovskaya guberniya, Russia  
99 YBN
[1901 AD]
4787) De Forest grows up in Alabama, and his father, a minister, had moved to
Alabama in 1879 to serve as a principal of a school for black people. The
family is ostracized for this and young Lee finds his friends only amoung black
children.

De Forest's father wants him to enter the ministry but De Forest wants to go
into science.
De Forest's Ph.D. dissertation is probably the first in the USA that
relates to radio (Hertzian) waves.

De Forest is indicted in 1912 but later acquitted of federal charges of using
the postal system to defraud by seeking to promote a "worthless device"—the
Audion tube.
During the 1930s De Forest develops Audion-diathermy machines. Diathermy
is the heating of body tissues due to their resistance to the passage of
high-frequency electromagnetic radiation, electric current, or ultrasonic
waves.
During World War II De Forest works on military research at the Bell Telephone
Laboratories.
De Forest has more than 300 patents, the last when he is 84 years old.

(To broadcast photons in with radio frequencies, only a large current is
needed, and a larger transmitting antenna. Clearly the conversion of sound to
electric current had been done already with the invention of the telephone. The
triode can simply amplify weak electronic current signals, which is useful
perhaps in amplifying the weak AM signals at the receiving end. A signal may
start with very dense photons, but as the distance from the source transmitter
increases the quantity of photons decreases by the square of the distance. So
only far fewer photon beams reach distant receivers, which must take those weak
voltages and currents created by the photon beams and amplify them to play
through a speaker. State what kinds of speakers are in use at the time.)


(Was DeForest excluded from direct to neuron reading and writing?)

(It is interesting that DeForest is one of those people who actively tried to
bring radio communication to the public. This is interesting in light or what
must have been the, already by this time, thriving secret particle
communication (wireless) neuron reading and writing networks.)
(Western Electric Company) Chicago, Illinois, USA  
99 YBN
[1901 AD]
5510)
(University of Göttingen) Göttingen, Germany  
99 YBN
[1901 AD]
6023) From 1905 to 1908 Elgar is the University of Birmingham’s first
professor of music.
Malvern, Worcestershire, England (presumably)  
99 YBN
[1901 AD]
6253)
  
98 YBN
[02/15/1902 AD]
4091)
(Société de Biologic) Paris, France (presumably)  
98 YBN
[02/??/1902 AD]
4835)
(US ship Philadelphia) Atlantic Ocean (presumably)  
98 YBN
[03/17/1902 AD]
4398) The interpretation of this relationship of light and electricity is
provided in 1905 by Albert Einstein’s hypothesis of light quanta in applying
the quantum theory of Planck to light.

(I think a light quantum can be interpreted as a mass multiplied by it's
velocity or perhaps its velocity squared. There could be two quanta, one that
is mv, and another that is mv2, and others that are mv3, m2v2, etc.)

This finding persuades people in science that atoms contain electrons as part
of their structure.

Lenard shows that only certain wavelengths of light bring about electron
emission. Lenard shows that for any particular wavelength, electrons of fixed
energies (that having a fixed product of mass and velocity) are given off.
Increasing the intensity of light increases the number of electrons but not
their individual energy. Lenard is the first to suppose that the atom is mostly
made of empty space when he tries to explain this phenomenon. Ernest Rutherford
will establish this a few years later. Lenard proposes a model of the atom in
which the atom is made from "dynamids", units of positive and negative charge.
This will be soon replaced by the nuclear atom of Ernest Rutherford.


(what device does Lenard use to create light of many different specific
frequencies? Lenard probably filters incandescent light from carbon electrodes.
I think there is some amount of photoelectric effect in all photons that
collide with atoms, and that perhaps photons are, or are closely related to
electrons and only show electric effect when in metals or atom lattices. Show
and explain exactly how Lenard finds only certain frequencies cause electron
emission.)

(how was this electron energy measured, with what devices? is this measured as
electric potential?)

(Show how Leonard determines the velocity of electricity - is this simply
measured by electric potential? This again presumes that the speed of
electricity is faster for a higher potential and slower for a lower potential,
which I can accept - but I don't know if that is the majority view.)

(State paper, and translate) (presumably)
(University of Kiel) Kiel, Germany  
98 YBN
[03/28/1902 AD]
4857)
(Harvard University) Cambridge, Massachussets, USA  
98 YBN
[03/??/1902 AD]
4734) Soddy is profoundly disturbed by World War I and “enraged” by the
death of Moseley.
In 1921 Soddy wins the Nobel Prize in chemistry for finding isotopes.
(McGill University) Montreal, Canada   
98 YBN
[04/28/1902 AD]
4235)
(Observatoire de météorologie dynamique {Dynamic Meteorology
Observatory})Trappes, France  
98 YBN
[05/27/1902 AD]
4735)
(McGill University) Montreal, Canada   
98 YBN
[05/??/1902 AD]
4338)
(Royal Institution) London, England  
98 YBN
[10/17/1902 AD]
4253)
(Columbia University) New York City, NY, USA  
98 YBN
[10/17/1902 AD]
4254)
(Columbia University) New York City, NY, USA  
98 YBN
[10/27/1902 AD]
3983)
University of Nancy, Nancy, France (presumably)  
98 YBN
[11/10/1902 AD]
4736)
(McGill University) Montreal, Canada   
98 YBN
[11/19/1902 AD]
4738)
(McGill University) Montreal, Canada   
98 YBN
[1902 AD]
3609) The book "Trailblazer to Television", is a book written by Arthur Korn's
wife Elizabeth and daughter-in-law Terry, after his death, and published by
Scribner's Sons, who also publish the "Dictionary of Scientific Biography". So
like Harper Brothers, Scribner, clearly are informers to the public in these
secretive and terrible times. There are some interesting hints in this book:
The second sentence of the preface uses the word "eye". On page 6 "Arthur's
mother was only a dim image in his mind.". On page 45: "'Yes.' She beamed.".
München, Germany  
98 YBN
[1902 AD]
3821)
(Munich Thermal Testing Station) Munich, Germany (presumably)  
98 YBN
[1902 AD]
4062)
(University of Heidelberg) Heidelberg, Germany (presumably)  
98 YBN
[1902 AD]
4082)
London, England (presumably)  
98 YBN
[1902 AD]
4180)
(University of Leipzig) Leipzig, Germany  
98 YBN
[1902 AD]
4181)
(University of Leipzig) Leipzig, Germany  
98 YBN
[1902 AD]
4365)
(University College) London, England  
98 YBN
[1902 AD]
4394)
(Harvard University) Cambridge, Massachussets, USA  
98 YBN
[1902 AD]
4457) In 1925, Zsigmondy wins the Nobel prize in chemistry for work on
colloids.
(private research) Jena?, Germany (verify)  
98 YBN
[1902 AD]
4480)
(National Electric Signalling Company) Brant Rock, Massachusetts, USA  
98 YBN
[1902 AD]
4713)
(Compagnie Francaise Houston-Thomson) Paris, France  
98 YBN
[1902 AD]
4714)
(Compagnie Francaise Houston-Thomson) Paris, France (presumably)  
98 YBN
[1902 AD]
4721)
(Municipal School of Technology) Manchester, England  
98 YBN
[1902 AD]
4766) Russell's parents died by the time he is four, and his grandfather John
Russell raises him. This grandfather had been prime minister of Great Britain
from 1846-1852, and 1865-1866. His grandfather dies in 1878 and his grandmother
raises him.
Russell supports women's suffrage. (more specific, right to
vote?))
Russell's published views on sex are used by people in the clergy and the
Hearst press to arouse a storm of disapproval against Russell, and a state
court order withdraws his appointment (job) on the staff of the City College of
New York.
In 1916 Russell publishes a leaflet protesting against the harsh treatment
of a conscientious objector and is prosecuted on a charge of making statements
likely to prejudice recruiting for and discipline in the armed services, and
fined £100. The Council, the governing body of Trinity, then dismisses Russell
from his lectureship, and Russell breaks all connection with the college by
removing his name from the books. In 1918 another article of Russell's is
judged seditious, and Russell is sentenced to imprisonment for six months.
After the war, however, in 1925 the college invites Russell to give the Tarner
lectures and from 1944 until his death Russell is again a fellow of the
college.

In 1950 Russell is awarded the Nobel Prize in literature.
In 1961 Russell is jailed again
in England. (explain)
Russell lives until 1970 and reaches 97 years old.
(Cambridge University) Cambridge, England   
98 YBN
[1902 AD]
4784) In 1912 Carrel wins the Nobel Prize for Physiology or Medicine for
developing a method of suturing blood vessels.
In 1935 Carrel publishes a book, "Man,
the Unknown", with authoritarian views about the planet run by an intellectual
elite.

Carrel writes in "Man, the Unknown":
"Criminality and insanity can be prevented only by a
better knowledge of man, by eugenics, by changes in education and in social
conditions. Meanwhile, criminals have to be dealt with effectively. Perhaps
prisons should be abolished. They could be replaced by smaller and less
expensive institutions. The conditioning of petty criminals with the whip, or
some more scientific procedure, followed by a short stay in hospital, would
probably suffice to insure order. Those who have murdered, robbed while armed
with automatic pistol or machine gun, kidnapped children, despoiled the poor of
their savings, misled the public in important matters, should be humanely and
economically disposed of in small euthanasic institutions supplied with proper
gases. A similar treatment could be advantageously applied to the insane,
guilty of criminal acts.".

In the 1936 preface to the German edition of his book, Alexis Carrel added a
praise to the eugenics policies of the Third Reich, writing that:

"(t)he German government has taken energetic measures against the
propagation of the defective, the mentally diseased, and the criminal. The
ideal solution would be the suppression of each of these individuals as soon as
he has proven himself to be dangerous."

Also in this book, Carrel supports the concept of telepathy writing:
"CLairvoyance and
telepathy are a primary datum of scientific observation. Those endowed with
this power grasp the secret thoughts of other individuals without using their
sense organs. They also perceive events more or less remote in space and time.
This quality is exceptional. It develops in only a small number of human
beings. but many possess it in a rudimentary state. ...
The reading of thoughts
seems to be related simultaneously to scientific, esthetic, and religious
inspiration, and to telepathy. Telepathic communications occur frequently. ".

(notice att-and to telepathy. In addition, this may be a cover used by those
who receive videos direct-to-neuron - to mislead those excluded by thinking
that occurances of people saying what they are thinking must be this 'latent'
ability.)

Carrel views homosexuality as a disease in writing: "...Homosexuality
flourishes. Sexual morals have been cast aside. ...".
Carrel works with the Vichy
government and when France is liberated Carrel is dismissed from his posts, but
but died before a trial is arranged. A similar occurance may happen for
accessories who helped cover-up the truth about how Frank Fiorini killed JFK,
Thane Cesar killed RFK, 9/11 and all other murders.
(University of Lyons) Lyons, France  
98 YBN
[1902 AD]
6047)
Saint Louis, Missouri, USA (presumably)  
97 YBN
[03/17/1903 AD]
3676)
(private lab) London, England(presumably)  
97 YBN
[03/23/1903 AD]
4492)
Dayton, Ohio  
97 YBN
[03/23/1903 AD]
4493)
Kill Devil Hills, North Carolina, USA  
97 YBN
[05/14/1903 AD]
4263)
(Yale University) New Haven, Connecticut, USA   
97 YBN
[05/19/1903 AD]
3970)
Harvard College Observatory, Cambridge, Massachusetts, USA  
97 YBN
[05/28/1903 AD]
3677)
(private lab) London, England(presumably)  
97 YBN
[05/28/1903 AD]
3830)
(Royal Institution) London, England (presumably)  
97 YBN
[06/??/1903 AD]
4893) In 1917 Barkla wins a Nobel Prize in physics for work on X rays.
(University College) Liverpool, England  
97 YBN
[07/17/1903 AD]
3438) Huggins may be hinting about secret sending of images to brains with this
sentence:
"...has already thrown many beams of suggestive light into the very obscure
regions of the constitution of matter." in 1903. It could be knowledge of the
secret research that has not yet produced anything. Working with spectra, and
wealthy, Huggins was certainly in a position to know and understand. By this
time the CRT is public, and so probably the electric camera has already been
invented. The electric camera must be quickly integrated into the microphone
networks of the phone and telegraph companies. This implies already by 1903
that people were either sending images, or actively trying to, and Huggins had
access to see or hear about this secret research. All this is before even World
War I or II, to think of how many lives would have been saved had they shared
with the public these science and technology advances instead of hording them
for many decades still to come even now.

In fact, much of Huggins and other scientists writing can be used as a
measurement device to determine when people first saw eyes. For example, in
1897 Huggins writes that Airy said "It seems to me a case of 'Eyes and No
Eyes'.". The use of the word "eyes", "suggest", "beam", "ears", "thought", and
many others, all can be weighted to find a curve from historical documents. In
particular from honest and wise sources. Simply examining the papers of major
indicators such as Huggins, Henry Crew, and others. First a good hinter must be
determined, before their writings are evaluated for clear secret technology
hinting. Even then, it is very difficult to solidly conclude anything other
than...it is very likely that by this time people were seeing eyes. Seeing eyes
from behind the head in infrared is one of those science breakthroughs that you
either know about because somebody told you or you have no idea. It is
generally an all or none type of knowledge. There might be a small period of
time before the actual technology where people are actively experimenting
trying to see eyes, etc. I have to think that period must be brief, but some
science breakthroughs do take decades until possible.
(Tulse Hill)London, England  
97 YBN
[07/28/1903 AD]
4145) Soddy is profoundly disturbed by World War I and “enraged” by the
death of Moseley.
In 1921 Soddy wins the Nobel Prize in chemistry for finding isotopes.
(University College) London, England  
97 YBN
[11/23/1903 AD]
4264)
(Cambridge University) Cambridge, England   
97 YBN
[11/??/1903 AD]
4026)
(private lab) West Orange, New Jersey, USA (presumably)  
97 YBN
[12/??/1903 AD]
4462)
(Tokyo University) Tokyo, Japan  
97 YBN
[1903 AD]
4075)
(Military Medical Academy), St. Petersburg, Russia  
97 YBN
[1903 AD]
4127)
(University of Madrid) Madrid, Spain  
97 YBN
[1903 AD]
4308) Konstantin Eduardovich Tsiolkovsky (TSYULKuVSKE) (CE 1857-1935), Russian
physicist starts a series of articles which thoroughly describe the theory of
rocketry for an aviation magazine.

Kaluga, Russia (presumably)  
97 YBN
[1903 AD]
4368) In 1924 Einthoven wins the Nobel prize in medicine and physiology.
(University of Leiden) Leiden, Netherlands  
97 YBN
[1903 AD]
4756) Schaudinn dies at age 34. (state how if known)
(German-Austrian zoological station) Rovigno (now Rovinj, Yugoslavia)  
97 YBN
[1903 AD]
4768) Tsvet died when only 47. (Probably neuron'd)
(University of Warsaw) Warsaw, Poland  
96 YBN
[02/14/1904 AD]
4837)
(Sorbonne) Paris, France (presumably)  
96 YBN
[03/17/1904 AD]
4894)
(University of Liverpool) Liverpool, England  
96 YBN
[06/18/1904 AD]
4500)
(Lick Observatory) Mount Hamilton, California, USA  
96 YBN
[06/29/1904 AD]
4707)
(Mining Engineering and Chemistry company) New Haven, Conneticut, USA   
96 YBN
[09/08/1904 AD]
4401) In 1915 Bragg wins the Nobel prize in physics with his son (Laue won in
1914).
In 1925 Bragg writes about science for the public in "Concerning the Nature of
Things", and "The universe of light", helping to popularize science.
In 1935 Bragg is
elected president of the Royal Society.
(University of Adelaide) Adelaide, Australia  
96 YBN
[1904 AD]
3448)
(observatory of Meudon) Paris, France  
96 YBN
[1904 AD]
3615)
Paris, France (presumably)  
96 YBN
[1904 AD]
3647)
France  
96 YBN
[1904 AD]
3708)
(Zoological Institute) Jena, Germany  
96 YBN
[1904 AD]
3975)
Technische Hochschule, Karlsruhe, Germany  
96 YBN
[1904 AD]
4077)
(University College) London, England  
96 YBN
[1904 AD]
4084)
(Edinburgh University) Edinburgh, Scotland  
96 YBN
[1904 AD]
4101)
(University of Groningen) Groningen, Netherlands  
96 YBN
[1904 AD]
4102)
(University of Groningen) Groningen, Netherlands  
96 YBN
[1904 AD]
4178)
(University of Leiden) Leiden, Netherlands  
96 YBN
[1904 AD]
4198)
(Serum Institute) Frankfurt, Germany  
96 YBN
[1904 AD]
4202)
(University of Paris) Paris, France  
96 YBN
[1904 AD]
4218) William Crawford Gorgas (GoURGuS) (CE 1854-1920), US army surgeon, helps
to completely end both malaria and yellow fever in Panama by destroying the
mosquito populations. This will make the building of the Panama Canal
(completed in 1914) possible.

Panama  
96 YBN
[1904 AD]
4229)
(Herzoglich Gymnasium) Wolfenbüttel, Germany  
96 YBN
[1904 AD]
4366)
(University College) London, England  
96 YBN
[1904 AD]
4377)
(École de Physique et Chimie Sorbonne) Paris, France  
96 YBN
[1904 AD]
4382)
(International Bureau of Weights and Measures) Sèvres, France  
96 YBN
[1904 AD]
4400)
(University of Chicago) Chicago, illinois, USA  
96 YBN
[1904 AD]
4402)
(University of Adelaide) Adelaide, Australia  
96 YBN
[1904 AD]
4413)
(Würzburg University) Würzburg, Germany  
96 YBN
[1904 AD]
4447)
(Potsdam Observatory) Potsdam, Getmany  
96 YBN
[1904 AD]
4463) In 1929 Harden wins the Nobel prize in chemistry with Euler-Chelpin for
work in fermentation.
(Lister Institute of Preventive Medicine) London, England   
96 YBN
[1904 AD]
4757)
(Institute for Protozoology at the Imperial Ministry of Health) Berlin,
Germany  
96 YBN
[1904 AD]
4873) Kettering is the son of a farmer.
In 1909 Kettering founds the Dayton Engineering
Laboratories Company (Delco), which eventually merges with other companies to
form General Motors.
In 1919 Kettering becomes the head of the General Motors
Research Corporation.
(National Cash Register Company) Dayton, Ohio, USA  
96 YBN
[1904 AD]
4920) In 1903 Nieuwland is ordained a priest.
In 1904 Nieuwland receives his Doctor's
degree from a Catholic University.

(It is rare after the 1700s to see religious people ordained as priests make
contributions in science, so Nieuwland is truly an exception. Nieuwland is
evidence that even those (under the influence and burden of religions) who
believe the lies of religions can make contributions in science.)
(Catholic University of America), Washington, D.C, USA  
96 YBN
[1904 AD]
5099)
Düsselsorf, Germany (presumably)  
96 YBN
[1904 AD]
5779)
(University of Manchester) Machester, England  
96 YBN
[1904 AD]
6100) "Give my regards to Broadway" is released (written by George M. Cohan).
New York City, New York, USA (presumably)  
96 YBN
[1904 AD]
6343)
  
95 YBN
[01/05/1905 AD]
4501)
(Lick Observatory) Mount Hamilton, California, USA  
95 YBN
[01/30/1905 AD]
4267)
(Cambridge University) Cambridge, England   
95 YBN
[03/17/1905 AD]
4928) Einstein drops out of high school following the invitation of the teacher
who said “You will never amount to anything, Einstein.”.

Einstein goes to Italy for a vacation to avoid qualifying for military
service.

Einstein graduates from college in Switzerland.

In 1901 Einstein gets a job as a junior official in the patent office in Berne,
Switzerland.

In 1905 Einstein earns a Ph.D.

In 1909 Einstein gets a low paying job as professor at the University of
Zürich.

In 1913 Einstein gets a high paying job as professor at the Kaiser Wilhelm
Physical Institute in Berlin, thanks to Planck, who is greatly impressed with
Einstein's work. (Probably Planck in particular supported Einstein's use of
Planck's theory to explain the photoelectric effect. This also shows Planck to
honorably be not anti-Jewish.)

After World War I starts, Einstein as a Swiss citizen does not have to serve.
When many German scientists sign a nationalistic pro-war proclamation, Einstein
is one of the few to sign a counterproclamation calling for peace.

In 1930 Einstein visits California to lecture at the California Institute of
Technology and is still there when Hitler comes to power.

Einstein accepts a job as professor in Princeton, New Jersey at the Institute
for Advanced Studies, a private, academic, non-degree granting institution
founded in 1930 in Princeton, New Jersey. Students are postdoctorate or senior
scholars who conduct independent, intensive research through any of the
institute's four schools. It is not affiliated with any other academic
institution but has an informal relationship with Princeton University.

(Einstein does believe in a god), and states in objecting to Heisenberg's
uncertainty principle that “God may be subtle, but He is not malicious.”.

In 1930 Bohr proves Einstein's argument against Heisenberg's uncertainty
principle that time and energy can be simultaneously determined with complete
accuracy wrong. (I think exact positions and times may always be impossible,
although I can see an all integer universe perhaps, at least in terms of space,
the smallest space being the size of a photon. But I reject the idea of
probability being anything other than a useful tool, and I reject the idea of
particles being created or destroyed. My view is that particles have a real
location and velocity even if a completely accurate description of what that
location or velocity is impossible. In other words, particles occupy space and
move through space, they do not appear simply because particles in an observer
interact with them. )

Einstein is persuaded by Szilard to write a letter to US President Franklin D.
Roosevelt, urging him to put into effect a gigantic research program designed
to develop a nuclear bomb. (Clearly FDR and others routinely watched people in
their houses, saw and heard thoughts, and probably routinely got updated motion
pictures from Einstein's thoughts beamed onto their brain through neuron
reading and writing.) The result of this is the Manhattan Project (named for
the location of its origin at Columbia University, although it would later move
to the University of Chicago) which in six years develops the first atomic
bomb.

Einstein rejects Heisenberg's principle of uncertainty because he cannot
accept that the universe could be run by chance. (I reject the idea of chance
too, but I also reject the idea of any kinds of gods.)

Einstein opposes McCarthyism (which is the persecution of those suspected of
supporting Communism) in the early 1950s.

Einstein spends the last decades of his life unsuccessfully searching for a
theory that will explain both gravitation and electromagnetic phoenomena (the
unified field theory).

Element 99 is named Einsteinium in Einstein's honor.

Asimov states that no scientist was as revered in his own time since Newton.

(To credit Einstein, I think his efforts in the interest of peace are good, his
intermediate interpretation of the photo electric effect is a contribution to
science. For criticisms: I wish Einstein had used his popularity and wealth to
make a movie about the history of science (to bring science to the public),
exposed the seeing and hearing of thought -as a note Einstein wrote a preface
to Sinclair Lewis' German edition of the book "Mind Radio" about telepathy. I
wish Einstein had fully explained the situation of science more, sponsored a
history of science movie for the public, had expressed doubts and flaws in his
theory, had entertained the idea of a photon as matter, had explain the GToR
with simple examples many times over for all to see and make it simple and
clear to understand what his theory is. He could have rejected religion and the
theory of the existence of gods, promoted free info, questioned copyright,
secrecy, spoken out against violence, for full democracy, not the
representative democracy, against prohibition or drugs, alcohol and prostition,
etc.)

(I can only really credit Einstein with an intermediate explanation of the
photoelectric effect, the Borwnian motion equation, and for a creative but
untrue interpretation and equations describing the universe. The combining of
space and time into space-time, which Minkowski is credit with, is creative,
but clearly time is the same throughout all of space. E=mc2 is meaningless as
far as I can see since, or at best a useful combination of mass and motion -
however, the implication that mass and motion can be interchanged is an error
in my view. I credit Einstein with rejecting the light as a wave theory and
heading back towards Newton's corpuscular interpretation. My view of the
theories of relativity, both special and general, are that they are completely
wrong, inaccurate, unsalvageable, but a creative math and geometry that does
not apply to the universe, mainly because time-dilation and space-dilation are
wrong, non-Euclidean geometry does not apply to the universe in the view I
support, a photon is a piece of matter and the basis of all matter (both of
which Einstein never stated publicly).)

(Clearly something must explain Einstein's extreme popularity, in my view, the
scientific achievements do not justify the popularity Einstein received and
still receives. The two achievements I think are moving a step closer to
viewing light as a particle, and an equation to estimate the size and number of
molecules. In my view the theories of relativity are completely inaccurate and
of no value, if only because time and space dilation is false. In my view
Einstein is one of the most over-valued scientists of history. Perhaps his
appearance, or wit, or being Jewish which served as an iconic opposition hero
to the rising anti-Jewish views popular in Nazi Germany explain his popularity.
Perhaps wealthy people embraced his views. Perhaps the neuron reading and
writing owners supported his abstract theories as being useful in removing the
public's interest in science or feeling of being able to make contributions to
science and therefore keeping them away from realizing the truth about neuron
reading and writing, or trying to accomplish neuron reading and writing
technology by themselves. Perhaps many people who would be critics of
Einstein's theory of relativity in favor of a more accurate truth felt
overwhelmed and unqualified to debate or criticize with such complex math
involved. Another reason may be that so few people, at this time, know enough
about the history of science, or science itself to care. There were critics, in
particular William Pickering, Herbert Dingle, and Charles Lane Poor, however,
the critics clearly have not won yet.)

(Over the course of Einstein's life, he publishes many papers. todo: determine
how many papers Einstein published.)
Bern, Switzerland  
95 YBN
[03/30/1905 AD]
4502)
(Lick Observatory) Mount Hamilton, California, USA  
95 YBN
[05/01/1905 AD]
4740)
(McGill University) Montreal, Canada   
95 YBN
[05/01/1905 AD]
4741)
(McGill University) Montreal, Canada   
95 YBN
[06/30/1905 AD]
4929)
Bern, Switzerland  
95 YBN
[09/27/1905 AD]
4930)
Bern, Switzerland  
95 YBN
[09/??/1905 AD]
4251)
(Nettie Stevens) Bryn Mawr University, Bryn Mawr, Pennsylvania, PA, USA (E. B.
Wilson) Columbia University, NY City, NY, USA  
95 YBN
[11/05/1905 AD]
4823) In 1919 Stark wins the Nobel prize in physics.
Stark fully supports Hitler and his
racial theories. Asimov states that Stark is one of few scientists of note who
supports Hitler. Stark terms Sommerfeld and Heisenberg “white Jews”.

Stark eventually rejects both quantum and relativity theories.

In 1947 Stark is
sentenced to 4 years in prison by a denazification court. Asimov comments this
is a far milder punishment than if Stark was the judge. I wonder what crimes
Stark is charged with. This raises the issue of who can be imprisoned for
violent crimes, and can a person be imprisoned for unknowlingly or even
knowlingly voting for a murderer? The debate of jailing people who plan, pay
for, or actively coverup violence is a battle of free speech and trade versus
how much responsibility a person has for some violence. 9/11 is a perfect
example of how this principle applies. In the USA, most people view accessory
to murder before the fact as requireing the same punishment as a first degree
murder, and being an accessory to murder after the fact as deserving a few
years in jail, so most people in the USA currently take the view against the
idea that non-violent involvement with a murder is protected by free speech and
support the idea of punishment for all those people involved in violence and in
particular for all those people involved with premeditated murder of nonviolent
people, even those who simply fund, order or somehow knowingly participate
before, during or after the actual murder or murders. For example, I doubt
seriously that those who voted for President George Bush, who presided over the
9/11 mass murders, should be imprisoned for any length of time - even those who
knew of his plans to murder, but I think certainly this point is open to
debate. For myself, I tend to support the side of free thought and speech, but
I can see given the extreme and widespread violence voting to imprison any and
all people directly involved in violence against nonviolent innocent people -
certainly at the level of conpiracy to commit murder, accessory to murder
before and/or after the fact- although some might view those as protected
under a strict interpretation of freedom of speech.
(University of Göttingen) Göttingen, Germany  
95 YBN
[11/21/1905 AD]
6103) (Possibly) earliest recording of popular Scottish song "Auld Lang Syne".
"Auld Lang Syne" is a Scots poem written by Robert Burns in 1788 and set to the
tune of a traditional folk song (Roud # 6294). It is well known in many
countries, especially in English-speaking nations. "Auld Lang Syne" is
traditionally used to celebrate the start of the New Year at the stroke of
midnight. By extension, it is also sung at funerals, graduations, and as a
farewell or ending to other occasions.

New York City, New York, USA  
95 YBN
[11/27/1905 AD]
4436)
(Wurzburg University) Wurzburg, Germany  
95 YBN
[1905 AD]
4034)
(private studio) Brighton, England (presumably)  
95 YBN
[1905 AD]
4234) Percival Lowell (CE 1855-1916), US astronomer theorizes that a planet
beyond Neptune is responsible for discrepancies in the motion of Uranus that
are not resolved by the finding of Neptune, calling this planet "Planet X". 15
years after Lowell's death Tombaugh will identify the planet which will be
named Pluto, although now Pluto is not considered a planet by the majority of
astronomers Does Pluto have enough mass to explain the discrepancy Lowell found
in Uranus' orbit?

In 1894 Lowell establishes an observatory in Arizona.

(Massachusetts Institute of Technology) Boston, Massachusetts, USA  
95 YBN
[1905 AD]
4282)
(University of Copenhagen) Copenhagen, Denmark (presumably)  
95 YBN
[1905 AD]
4283)
(University of Copenhagen) Copenhagen, Denmark (presumably)  
95 YBN
[1905 AD]
4300)
(Sorbonne) Paris, France  
95 YBN
[1905 AD]
4370)
Meteor Crater, Arizona  
95 YBN
[1905 AD]
4389)
(St. John’s College) Cambridge, England  
95 YBN
[1905 AD]
4464)
(Lister Institute of Preventive Medicine) London, England   
95 YBN
[1905 AD]
4708)
(Mining Engineering and Chemistry company) New Haven, Conneticut, USA   
95 YBN
[1905 AD]
4758)
(Institute for Protozoology at the Imperial Ministry of Health) Berlin,
Germany  
95 YBN
[1905 AD]
4760) Langevin popularizes Einstein's theories for the French public as
Eddington does for the English and US public. (To me this implies that
Langevin, like Einstein, was more in the Lorentz camp than in the Michelson
corpuscular camp. The Lorentz camp, in my view, is possibly some kind of
light-as-a-wave-in-an-aether, keep-neuron-reading-and-writing-and
other-science-findings-secret-from-the-public half of scientists. Many viewed
Einstein's theory of relativity as being an advance because of the supposed
view of light as being particulate that Einstein had at least first supported,
however the adoption of Fitzgerald and Lorentz's unlikely space and time
contraction and dilation theory puts most if not all of relativity in the
light-as-a-wave-in-aether view - that light is massless and not material.)
Lange
vin is the great-great-grandnephew of Pinel on his mother's side.
Langevin is an
outspoken anti-Nazi and is imprisoned (under the puppet Vichy regime), but
escapes to Switzerland, is restored to his post in 1944, and lives to see
France free again.

Langevin's daughter Hélène, is imprisoned in Auschwitz and on her return,
both have seats in the Assemblée Consultative as members of the Communist
Party.
(École Municipale de Physique et Chimie) Paris, France  
95 YBN
[1905 AD]
4771) in 1926 Amundsen flies a dirigible from Spitsbergen to Alaska passing
over the North Pole. Amundsen had failed on 3 previous attempts.

In June 1928 Amundsen dies in a flight (in an air plane?) over the Arctic in a
search for survivors of a shipwreck.
Herschel Island, Yukon  
95 YBN
[1905 AD]
4815)
(National Bureau of Standards) Washington D.C., USA  
94 YBN
[01/13/1906 AD]
5502)
(University of Göttingen) Göttingen, Germany (presumably)  
94 YBN
[01/17/1906 AD]
4898)
(University of Liverpool) Liverpool, England  
94 YBN
[02/09/1906 AD]
4901)
(University of Liverpool) Liverpool, England  
94 YBN
[04/17/1906 AD]
3806)
Washington, D.C., USA.  
94 YBN
[06/??/1906 AD]
4268)
(Cambridge University) Cambridge, England   
94 YBN
[07/20/1906 AD]
4743)
(McGill University) Montreal, Canada   
94 YBN
[12/21/1906 AD]
4788)
(De Forest Radio Telephone Company) New York City, New York, USA  
94 YBN
[12/24/1906 AD]
4479) Fessenden holds 500 patents at the time of his death, second only to
Edison.
Fessenden works for Edison in the 1880s and Edison's greatest rival
Westinghouse from 1890-1892.
(AM works by having a regular periodic sine wave, for example
one at 10 million cycles per second, and adding in a source signal. At the
receiving station the 10 million cycles per second sine wave is subtracted
leaving the source signal.)

(Clearly amplitude modulation must have been recognized much earlier - for
people to have started neuron reading and writing in at least 1810. Perhaps
Feesenden was a person excluded from the technology who reinvented it, or was
included and purposely allowed to release the truth about amplitude modulation
to the public.)

(Amplitude modulation is so simple an idea, that it occurs naturally in any
object that emits a periodic frequency of particles, which is pretty much all
matter. For example, sounds reaching the ear may impart an amplitude modulation
- which is a strength modulation - a quantity of particle modulation to any
regular interval signal emitted from the nerves of the ear portion of the
brain.)

(Probably amplitude modulation of wired recording of sound was the first
instance of listening to hidden microphones.)
(National Electric Signaling Company and General Electric?) Brant Rock,
Massachusetts, USA  
94 YBN
[12/24/1906 AD]
4796)
(University of Copenhagen, and at the Urania Observatory in Frederiksberg)
Copenhagen, Denmark (verify)  
94 YBN
[12/24/1906 AD]
4797)
(University of Copenhagen, and at the Urania Observatory in Frederiksberg)
Copenhagen, Denmark (verify)  
94 YBN
[12/27/1906 AD]
4710)
(Yale University) New Haven, Connecticut, USA   
94 YBN
[1906 AD]
3920)
(University of Bonn) Bonn, Germany  
94 YBN
[1906 AD]
4035)
(private lab) Southwick, Sussex, England  
94 YBN
[1906 AD]
4103)
(University of Groningen) Groningen, Netherlands  
94 YBN
[1906 AD]
4314)
(Yale University) New Haven, Connecticut, USA   
94 YBN
[1906 AD]
4355) Marie Sklodowska Curie (KYUrE) (CE 1867-1934) is the first women to teach
at the Sorbonne.

(École de Physique et Chimie Sorbonne) Paris, France  
94 YBN
[1906 AD]
4385)
(Cambridge University) Cambridge, England   
94 YBN
[1906 AD]
4419)
(University of Heidelberg) Heidelberg, Germany  
94 YBN
[1906 AD]
4442)
( University of Berlin) Berlin, Germany  
94 YBN
[1906 AD]
4471)
(Robert Koch Institute for Infectious Diseases) Berlin, Germany  
94 YBN
[1906 AD]
4706)
(Institut Pasteur du Brabant) Brussells, Belgium  
94 YBN
[1906 AD]
4722) In 1911 Ricketts gets typhus while working with it and dies.

(Asimov uses “contracts typhus”, maybe murdered by muscle contraction?
Even so, there are dangers with working closely with infrectious bacteria,
viruses, and protists.)
(University of Chicago) Chicago, illinois, USA  
94 YBN
[1906 AD]
4868) Diels' two sons are killed on the eastern front in World War II. (what
were' Diels' opinions of Nazism?) Diels' home and laboratory are destroyed in
bombing raids.
(University of Berlin) Berlin, Germany  
93 YBN
[04/03/1907 AD]
4763)
(McGill University) Montreal, Canada   
93 YBN
[05/??/1907 AD]
4269)
(Cambridge University) Cambridge, England   
93 YBN
[06/13/1907 AD]
4897)
(Trinity College) Cambridge, England  
93 YBN
[07/09/1907 AD]
4950) In 1953 Staudinger wins the Nobel Prize in chemistry.
(University of Strasbourg) Strasbourg, Germany  
93 YBN
[07/30/1907 AD]
4938) In 1914 Laue wins the Nobel Prize in physics "for his discovery of the
diffraction of X-rays by crystals".
Laue champions Albert Einstein’s theory of
relativity, does research on the quantum theory, the Compton effect (change of
wavelength in light under certain conditions), and the disintegration of atoms.

In 1939 in Switzerland Laue denounces Hitler's policy of refusing to allow
Germans to accept Nobel Prizes.
In 1943 Laue resigns from the University of Berlin in
protest against the Nazis.
In 1960 Laue dies in an automobile accident at age
81. (with seatbelt? because of age?)
( University of Berlin) Berlin, Germany  
93 YBN
[09/14/1907 AD]
6254)
Canton, Ohio, USA  
93 YBN
[09/21/1907 AD]
4709)
(Yale University) New Haven, Connecticut, USA   
93 YBN
[11/13/1907 AD]
354)
  
93 YBN
[11/26/1907 AD]
6263)
Petrograd, Russia  
93 YBN
[12/04/1907 AD]
4931)
(Moskau Ingenieure-Hochschule {Moscow Engineering School}) Moscow, Russia?
(verify)  
93 YBN
[1907 AD]
4149)
(University of Berlin) Berlin, Germany  
93 YBN
[1907 AD]
4386)
(Cambridge University) Cambridge, England   
93 YBN
[1907 AD]
4416)
(Societe Electro Metallurgique Francaise) Froges, Isere, France
(presumably)  
93 YBN
[1907 AD]
4438) Einstein was a pupil of Minkowski.
Minkowski dies at age 44.
(Neuron/particle beam murder?)
(University of Göttingen) Göttingen, Germany  
93 YBN
[1907 AD]
4456)
(Zurich Polytechnikum) Zurich, Switzerland  
93 YBN
[1907 AD]
4516)
(Pathological-Anatomical Institute) Vienna  
93 YBN
[1907 AD]
4764)
(Sorbonne) Paris, France  
93 YBN
[1907 AD]
4884) In 1928 Windaus wins the Nobel prize in chemistry for studies on
cholesterol (steroid) structure, and showing the connection between steroids
and vitamins. The sterols are complex alcohols.
Although Windaus is not a supporter of
the Hitler regime, Windaus is allowed to continue his work because of the
reputation he had established.
(University of Freiburg) Freiburg, Germany  
92 YBN
[03/26/1908 AD]
5881)
(University College) London, England (presumably)  
92 YBN
[05/30/1908 AD]
4902)
(University of Liverpool) Liverpool, England  
92 YBN
[06/06/1908 AD]
3616)
London, England  
92 YBN
[06/18/1908 AD]
4742)
(University of Manchester) Manchester, England  
92 YBN
[06/18/1908 AD]
4744)
(University of Manchester) Manchester, England  
92 YBN
[06/20/1908 AD]
4523)
(Mount Wilson Observatory) Pasadena, California, USA  
92 YBN
[06/27/1908 AD]
4190) In 1894 Kamerlingh Onnes establishes the Cryogenic Laboratory at Leiden
University.
In 1912 Kamerlingh Onnes is awarded the Rumford medal.
In 1913 Kamerlingh Onnes wins
the Nobel prize in physics for liquefying helium.
(Leiden University) Leiden, Netherlands  
92 YBN
[08/12/1908 AD]
4451)
(University of Tübingen) Tübingen , Germany  
92 YBN
[09/24/1908 AD]
3617)
(Hotel Cecil) London, England (presumably)  
92 YBN
[12/09/1908 AD]
4960) In 1946 Bridgman wis the Nobel prize in physics.
Bridgman writes thoughtful books
on the nature of physics. (hints about thoughts?)
In 1961 Bridgman is incurably and
painfully ill, Bridgman shoots himself to death, writing a note stating that it
was indecent of society to turn its back and force him to end his life without
help or sympathy. (Neuron writing could have ended the pain. Stopping pain
should be the focus of research. Maybe some way of disabling the pain nerve
cells in the nerves or brain. In addition, probably a legal and consentual
lethal injection would be much less painful.)
(Harvard University) Cambridge, Massachussets, USA  
92 YBN
[1908 AD]
3836)
(Royal Institution) London, England (presumably)  
92 YBN
[1908 AD]
4212)
(Eastman Kodak Company) New Jersey, USA (presumably)  
92 YBN
[1908 AD]
4214)
(The Eastman Company) Rochester, NY, USA  
92 YBN
[1908 AD]
4238)
Paris, France (presumably)  
92 YBN
[1908 AD]
4344)
(Nobel Institute for Physical Chemistry) Stockholm, Sweden  
92 YBN
[1908 AD]
4378) German inventor Hermann Anschütz-Kaempfe (CE 1872-1931) develops the
first workable gyrocompass. A device which, once properly aligned, always
points to true north.

US inventor, Elmer Ambrose Sperry (CE 1860-1930), also invents a gyroscopic
compass. A gyroscopic compass uses the fact that a turning gyroscope maintains
it plane of rotation and resists being turned out of that plane. A gyroscope is
mounted on gimbals on a ship so that the ship's movements can not move the
gyroscope out of it's plane, and so the compass can identify north and south
correctly. This is the first improvement to the compass (or new compass design)
in 1000 years. This compass is first used on board the battleship "Delaware" in
1911 and is adopted immediately by the US navy.

If you try to tip a spinning gyroscope, it will turn to one side in a
predictable way - called "precession." In the same way, the force of a spinning
gyrostabilizer pushes a rolling ship in the opposite direction from the push of
the waves. Sperry invents a motion sensor, a motor to amplify the effect of
the sensor on the gyroscope, and an automatic feedback and control system. All
work together to make a much more effective gyrostabilizer.

Perry extends the gyro principle to guidance of torpedoes, to gyropilots for
the steering of ships and for stabilizing airplanes, and finally to a ship
stabilizer.
(needs visual. How is the gyroscope spun? How does the gyroscope stay spinning?
does it have to or can people routinely give it a spin to find north?)
(GPS,
particle communication with satellites probably has replaced most location
determining equipment on more vehicles on and around earth.)

Starting in 1894 Sperry makes electric automobiles powered by his patented
storage battery.
Kiel, Germany (presumably)  
92 YBN
[1908 AD]
4424)
(Detroit Automobile Company) Detroit, Michigan, USA  
92 YBN
[1908 AD]
4474) During 1902-1904 Miller works with Morley to confirm the Michelson-Morley
results.
Repeating the measurement by himself on Mt. Wilson, California, between 1921
and 1926, Miller finds a positive effect corresponding to an apparent relative
motion of the earth and the ether of some ten kilometers per second in the
plane of the interferometer. Though this velocity is about 70 percent less than
expected, Miller puts forward this result as a evidence against Einstein’s
theory of relativity, which Miller rejects to the end of his life.

Miller rejects Einstein's theories that arise out of the Michelson-Morley
experiment and continues to search for evidence of an "ether-drift", which
would disprove relativity. (Note that I don't think that evidence for ether
would disprove relativity, which grew from the Fitzgerald-Lorentz attempt to
save the ether theory. So evidence against an aether, in addition to evidence
against the supposed space contraction/dilation claimed by George FitzGerald,
and applied to time by Hendrik Lorentz, would probably do more to disprove the
claims of the theory of relativity. Beyond that, evidence disputing the claim
of light having a constant velocity, like the Pound-Rebka experiment would
perhaps do more to directly dismantle the theories of relativity or at least
the light as a constant velocity massless particle theory.)

See also for descriptions of Miller's efforts.
(Case School of Applied Science) Cleveland, Ohio, USA  
92 YBN
[1908 AD]
4517)
(Royal-Imperial Wilhelminen Hospital) Vienna  
92 YBN
[1908 AD]
4527) One result of Leavitt's work on stellar magnitudes is her discovery of
some 2,400 variable stars, more than half of all variable stars known even by
1930. Variable stars need to have their intensities compared over time. In
addition Leavitt discovers 4 novas. (nova as in exonebula?)
Like her colleague Annie
Cannon, Leavitt is extremely deaf. (Neuron writing may cure deafness for some
people, but is being withheld and selfishly horded by terrible people.)
(Harvard College Observatory) Cambridge, Massachussetts, USA  
92 YBN
[1908 AD]
4531)
(Fridericiana Technische Hochschule) Karlsruhe, Germany  
92 YBN
[1908 AD]
4718)
(École Normale) Paris, France  
92 YBN
[1908 AD]
4723)
(University of Chicago) Chicago, illinois, USA  
92 YBN
[1908 AD]
4773) Early in his career, Willstätter works on the structure of alkaloids and
throws light on such important compounds as cocaine, which he synthesizes in
1923, and atropine.
In 1915 Willstätter wins the Nobel Prize in chemistry for work on
plant pigments.
In the 1920s Willstätter claims to have isolated active
enzymes with no trace of protein, and this view is widely accepted until Sumner
and Northrop demonstrate that enzymes are proteins in 1930.
In 1924, being a Jewish
person Willstätter resigns his post at Munich in protest against anti-Semitic
pressures. Willstätter continues his work privately, first in Munich and, from
1939, in Switzerland.
(Eidgenössische Technische Hochschule) Zurich, Switzerland  
92 YBN
[1908 AD]
4813) Coolidge with Langmuir develops the first successful submarine-detection
system during World War I.
During World War II, Coolidge is involved in atomic
bomb research in Hanford, Washington.
Coolidge is a distant cousin of US President Calvin
Coolidge.
Coolidge lives to 101.
(Research Laboratory of the General Electric Company) Schenectady, New York, in
1900.  
91 YBN
[02/08/1909 AD]
4428)
(announced at: American Chemical Society lecture) New York City, NY, USA
(presumably)  
91 YBN
[04/06/1909 AD]
4244)
Greenland  
91 YBN
[05/??/1909 AD]
4903)
(University of Liverpool) Liverpool, England  
91 YBN
[07/12/1909 AD]
4475)
(Pasteur Institute in Tunis) Tunis, Tunisia  
91 YBN
[09/??/1909 AD]
4729) Jean Baptiste Perrin (PeraN, PeriN or PeroN) (CE 1870-1942), French
physicist, determines the "corpuscular mass" of an atom of hydrogen writing
(translated from French):
"...Lastly, the mass of one of the identical corpuscles which
carry the negative electricity of the cathode-rays or of the B-rays is itself
obtained accurately, since it is known that it is 1775 times smaller than that
of the atom of hydrogen (Classen). This corpuscular mass, the latest element of
matter revealed to man, is thus
c=0.805 x 10-27.
...
Lastly, even the diameter of the corpuscle can be arrived at, if it is
supposed, with Sir J. J. Thomson, that all its inertia is of electromagnetic
origin, in which case its diameter is given by the equation

D=4/3 e2/mV2 ,

where V signifies the velocity of light, m the mass of the corpuscle and e its
charge, that is to say 4.1 x 10-10. From this there results for D the value
0.33 x 10-12, a value enormously smaller than the diameter of the smallest
atoms. ...".

(This is perhaps as close as any person has publicly tried to determine the
mass of a particle of light, or some basic particle that is thought to be the
basis of all matter, that is, to express matter in terms of number of light
particles, or smallest known particles.)

Perrin gives early evidence of microscopic neuron reader and writer devices
writing (translated to English):
"..The singular phenomenon discovered by Brown {ULSF:
Brownian motion} did not attract much attention. It remained, moreover, for a
long time ignored by the majority of physicists, and it may be supposed that
those who had heard of it thought it analogous to the movement of the dust
particles, which can be seen dancing in a ray of sunlight, under the influence
of feeble currents of air which set up small difference of pressure or
temperature. When we reflect that this apparent explanation was able to satisfy
even thoughtful minds, we ought the more to admire the acuteness of those
physicists, who have recognised in this, supposed insignificant, phenomenon a
fundamental property of matter. ...". The statistical probability of finding
the word "thought" three times in the same paragraph and "dust particles"
implies that this is a historical reference indicating that microscopic secret
camera, and neuron reading and writing devices have already been created by
1909. Looking through the rest of the work, there is very little use of the
word "thought" in any other part. The French part in question reads:
"... Le
phénomène singulier découvert par Brown n'attira pas beaucoup l'attention.
Il resta
d'ailleurs longtemps ignoré de la plupart des physiciens, et l'on peut
supposer que ceux qui en avaient entendu parler le croyaient analogue au
mouvement des poussières qu'on voit danser dans un rayon de Soleil sous
l'action des faibles courants d'air que provoquent de petites différences de
pression ou de température. Si l'on comprend que cette apparente explication
aitpu satisfaire même des esprits réfléchis, on doit admirer d'autant plus
la pénétration des physiciens qui ont su distinguer une propriété
fondamentale de la matière dans le phénomène qu'on pensait insignifiant.
...". Note that "croyaient" is "thought", "réfléchis" is "thoughtful"
("esprits réfléchis" is "thoughtful minds") and third "pensait" is "thought".
(École Normale, University of Paris) Paris, France  
91 YBN
[10/23/1909 AD]
4508)   
91 YBN
[1909 AD]
4113)
Washington, DC, USA  
91 YBN
[1909 AD]
4284)
(University of Copenhagen) Copenhagen, Denmark (presumably)  
91 YBN
[1909 AD]
4332)
(University of Vienna) Vienna (presumably)  
91 YBN
[1909 AD]
4466)
(Army Medical School) Netley, England  
91 YBN
[1909 AD]
4506)
(Carlsberg Laboratory, University of Copenhagen) Copenhagen, Denmark  
91 YBN
[1909 AD]
4532) In 1915 Haber directs the use of the poison gas chlorine and the far
worse Mustard gas in 1917.
In 1919 Haber wins the Nobel prize in chemistry for
haber process of converting Nitrogen from the air into the more usable ammonia
(ammonia synthesis).
Haber tries to isolate gold from seawater but fails.
Haber is Jewish
and is forced to leave his post even after helping in WW I.
(Fridericiana Technische Hochschule) Karlsruhe, Germany  
91 YBN
[1909 AD]
4694)
(Rockefeller Institute for Medical Research) New York City, New York, USA  
91 YBN
[1909 AD]
4719)
(École Normale) Paris, France  
91 YBN
[1909 AD]
4724)
Mexico City, Mexico  
91 YBN
[1909 AD]
4841) Bosch directs a huge ammonia plant at Oppau that is still under
construction when World War I starts.
In 1931 Bosch wins the Nobel prize in chemistry
for his investigations of the type of high-pressure reactions that make it
possible to produce ammonia from nitrogen (gas).
Bosch lives under the Nazis
but does not bow to Nazi principles, for example openly honoring Haber, after
Haber's exile.
(BASF) Oppau, Germany  
91 YBN
[1909 AD]
4872) Stock dies after fleeing from the advancing Russian army to a small town
on the Elbe River.
  
91 YBN
[1909 AD]
4889) In 1927 Wieland wins the Nobel Prize in chemistry for describing the
structure of steroids.
Wieland is openly anti-Nazi during World War II, and
some of his student are involved in the 1944 treason trials. Wieland protects
Jewish humans in his laboratory and in 1944 testifies on behalf of students who
are accused of treason. (verify)
(University of Munich) Munich, Germany  
91 YBN
[1909 AD]
4899)
(Marconi Company) London, England (verify)  
90 YBN
[04/??/1910 AD]
4199)
(announced at the Congress for International Medicine, Wiesbaden, Germany, but
work performed at Serum Institute) Frankfurt, Germany  
90 YBN
[08/??/1910 AD]
4320)
(Harvard College Observatory) Cambridge, Massachussetts, USA (presumably)  
90 YBN
[09/??/1910 AD]
4403)
(University of Adelaide) Adelaide, Australia (presumably)  
90 YBN
[09/??/1910 AD]
4418)
(University of Leeds) Leeds, England  
90 YBN
[10/31/1910 AD]
4273)
(Cambridge University) Cambridge, England   
90 YBN
[11/28/1910 AD]
4509)
(University of Chicago) Chicago, illinois, USA  
90 YBN
[1910 AD]
4230)
(Herzoglich Gymnasium) Wolfenbüttel, Germany  
90 YBN
[1910 AD]
4281)
(University of Zagreb) Zagreb, Croatia  
90 YBN
[1910 AD]
4356)
(École de Physique et Chimie Sorbonne) Paris, France  
90 YBN
[1910 AD]
4409)
(University of Manchester) Manchester, England  
90 YBN
[1910 AD]
4476) In 1926 Morgan publishes "The Theory of the Gene" which establishes and
extends the Mendelian scheme.
In 1933 Morgan wins the Nobel prize in medicine and
physiology.
In the Soviet Union, under the influence of Lysenko a believer in the acquired
characteristics theory, Morganism is virtually a dirty word.
From 1927-1931
Morgan is president of the National Academy of Sciences.
(Columbia University) New York City, NY, USA  
90 YBN
[1910 AD]
4779) Nevil Vincent Sidgwick (CE 1873-1952), English chemist publishes a book
specializing in the organic chemistry of nitrogen (perhaps "chemistry of carbon
and nitrogen compounds" might be more simplified) and will expand it into a
two-volume work in 1947.

(Oxford University) Oxford, England  
90 YBN
[1910 AD]
4807)
(Astrophysical Observatory) Potsdam, Germany   
90 YBN
[1910 AD]
4844) In 1920 Krogh wins the Nobel prize in physiology and medicine.
In 1940 when Denmark
is occupied by the Nazis, Krogh is forced to go underground and then to escape
to Sweden. Krogh returns to Denmark after the war.
(University of Copenhagen) Copenhagen, Denmark (presumably)  
90 YBN
[1910 AD]
4952)
(University of Karlsruhe) Karlsruhe, Germany  
90 YBN
[1910 AD]
4961)
(Harvard University) Cambridge, Massachussets, USA  
90 YBN
[1910 AD]
5021) In 1973 Frisch shares the Nobel Prize for medicine and physiology.
(Munich Zoological Institute) Munich, Germany  
90 YBN
[1910 AD]
6098) "Let Me Call You Sweetheart" is written (music by Leo Friedman and lyrics
by Beth Slater Whitson).

  
90 YBN
[1910 AD]
6099) "America The Beautiful" is published (music by: Samuel A. Ward, words by:
Katharine Lee Bates).

(Colorado College) Colorado Springs, Colorado, USA  
89 YBN
[01/??/1911 AD]
4321)
?  
89 YBN
[03/07/1911 AD]
4745)
(University of Manchester) Manchester, England   
89 YBN
[03/20/1911 AD]
5064)
(Imperial College of Science and Technology) London, England  
89 YBN
[03/??/1911 AD]
3945)
New York City, NY   
89 YBN
[04/19/1911 AD]
4691)
(Sidney Sussex College, Cambridge University) Cambridge, England  
89 YBN
[04/28/1911 AD]
4192)
(Leiden University) Leiden, Netherlands  
89 YBN
[04/??/1911 AD]
4746) On learning that Ernest Marsden found that alpha particles are reflected
by more than 90 degrees by atoms in gold foil, Rutherford’s is often quoted
as having said: “It was almost as incredible as if you fired a fifteen-inch
shell at a piece of tissue paper and it came back and hit you.”.
(University of Manchester) Manchester, England   
89 YBN
[06/12/1911 AD]
3977)
Sorbonne, University of Paris, Paris, France  
89 YBN
[06/15/1911 AD]
4874)
(Dayton Engineering Laboratories Co) Dayton, Ohio, USA  
89 YBN
[06/21/1911 AD]
5778)
Prague, Czechlslovakia  
89 YBN
[06/??/1911 AD]
3944) Perhaps it is no coincidence that this may be just over 100 years from
the first seeing of eyes and internal images produced by the brain, presumably
by William Wollaston in October 24, 1810.
New York City, NY   
89 YBN
[07/07/1911 AD]
4799)
Potsdam, Germany  
89 YBN
[07/??/1911 AD]
3946)
New York City, NY   
89 YBN
[11/13/1911 AD]
4270)
(Cambridge University) Cambridge, England   
89 YBN
[12/14/1911 AD]
4772)
South Pole  
89 YBN
[1911 AD]
3976)
Sorbonne, University of Paris, Paris, France  
89 YBN
[1911 AD]
4358) Reid is the great-grandnephew of George Washington on his mother's side.
( Johns Hopkins University) Baltimore, Maryland, USA  
89 YBN
[1911 AD]
4477)
(Columbia University) New York City, NY, USA  
89 YBN
[1911 AD]
4498) Andrew Ellicott Douglass (CE 1867-1962), US astronomer develops a system
of dendrochronology (chronology based on tree ring patterns), by noticing that
the tree ring patterns have similar patterns, the width of the rings relating
to the pattern of growth of a tree during wetter and drier seasons. When
viewing a cross section of a tree, for certain species of trees, wide rings are
produced during wet years, and narrow rings are produced during dry years. In
this way Douglass works out a pattern covering many centuries. In Arizona many
dead trees are well preserved because of the dry air. The patterns are
different based on the region, and Douglass makes maps of different regions,
finding that each tree fits into a certain chronological period of a regional
map. This is the first of the sensitive dating methods which will produce
Libby's carbon-14 method.

By the late 1920s Douglass will have sequenced of over a thousand tree rings
with six thin rings, presumably records of a severe drought, correlated with
the end of the 1200s. In 1929 Douglass finds some trees that contain the six
thin rings and a further 500 in addition. This takes him to the 700s and over
the years Douglass manages to get as far as the first century. Modern scholars
have taken tihs timeline going back almost to 5000 BCE.

(Lowell Observatory) Flagstaff, Arizona, USA  
89 YBN
[1911 AD]
4798)
Potsdam, Germany  
89 YBN
[1911 AD]
4846) In 1917 Weismann helps to get the Balfour Declaration put forth, which
agrees to the reestablishment of a Jewish national state in Palestine. But the
Balfour Declaration will not implemented until 1948 after the barbarity of
Hitler and his followers.
In 1948 Weismann is the first president of Israel,
and is one of the very few research scientists to serve as head of a state.
(University of Manchester) Manchester, England   
89 YBN
[1911 AD]
4851) In 1936 Dale and Loewi share Nobel prize in medicine and physiology.
In 1940-1945
Dale is president of the Royal Society.
(Wellcome Physiological Research Laboratories) London, England  
89 YBN
[1911 AD]
4890)
(University of Munich) Munich, Germany  
89 YBN
[1911 AD]
4908)
(University of Glasgow) Glasgow, Scotland  
89 YBN
[1911 AD]
4936) In 1928 Richardson wins the Nobel Prize in physics.
(Princeton University) Princeton, New Jersey, USA  
89 YBN
[1911 AD]
4937) In 1966 Rous shares the Nobel Prize for medicine and physiology.
(Rockefeller Institute, now called Rockefeller University) New York City, New
York, USA  
89 YBN
[1911 AD]
4986) Hess has a Jewish wife and leaves Austria shortly before Hitler's
invasion of Austria.
After WW II, Hess measures radioactive fallout from nuclear bombs,
and strongly opposes nuclear tests.
Victor Franz Hess|(CE 1883-1964)  
89 YBN
[1911 AD]
5093)
(Faculté des Sciences de Paris - University of Paris) Paris, France  
88 YBN
[01/05/1912 AD]
5301)
Frankfort-on-the-Main, Germany  
88 YBN
[03/03/1912 AD]
4528)
(Harvard College Observatory) Cambridge, Massachussetts, USA  
88 YBN
[04/20/1912 AD]
4918) (1927 Russell publishes an astronomy text (book) that is the first to
shift the main emphasis from the solar system and celestial mechanics to the
stars and astrophysics.)
(Princeton University) Princeton, New Jersey, USA.  
88 YBN
[05/04/1912 AD]
4939) In 1914 Laue wins the Nobel Prize in physics.
Laue champions Albert Einstein’s
theory of relativity, does research on the quantum theory, the Compton effect
(change of wavelength in light under certain conditions), and the
disintegration of atoms.
In 1939 in Switzerland Laue denounces Hitler's policy
of refusing to allow Germans to accept Nobel Prizes.
In 1943 Laue resigns from the
University of Berlin in protest against the Nazis.
In 1960 Laue dies in an
automobile accident at age 81. (with seatbelt? because of age?)
(University of Munich) Munich, Germany  
88 YBN
[05/06/1912 AD]
4271) (Sir) Joseph John Thomson (CE 1856-1940), English physicist, publishes a
paper "The Unit Theory of Light" in which he rejects the idea that light is
made of constant and invariable units.

(Possibly Thomson rejects the theory publicly in word, in order to offset the
publication of an article discussing a particle theory for light.)

(EX: I think a major experiment, is trying to detect even a tiny portion of
light particles reflecting off each other - it seems like an obvious
experiment. It is mysterious why I have never heard of this kind of experiment
being done - focused lasers aimed at each other with detectors on the sides
trying to pick up photons that may have reflected off other photons. This could
also be done in a vacuum container.)

(Cambridge University) Cambridge, England   
88 YBN
[06/07/1912 AD]
4692)
(Sidney Sussex College, Cambridge University) Cambridge, England  
88 YBN
[07/01/1912 AD]
4861)
(Percival Lowell's observatory) Flagstaff, Arizona, USA  
88 YBN
[07/16/1912 AD]
5203)
(University College) London, England  
88 YBN
[08/??/1912 AD]
4274)
(Cambridge University) Cambridge, England   
88 YBN
[10/??/1912 AD]
4912)
(University of Glasgow) Glasgow, Scotland (verify)  
88 YBN
[11/11/1912 AD]
4404) William Lawrence Bragg enters the University of Adelaide at age 15, and
graduates age 18.
In 1915 both Bragg father and son share the Nobel prize for
physics.
Bragg is interested in lecturing on science to young people.
(Cavindish Laboratory, Cambridge University) Cambridge, England  
88 YBN
[11/??/1912 AD]
5096)
(Columbia University) New York City, New York, USA  
88 YBN
[12/12/1912 AD]
4816)
(National Bureau of Standards) Washington D.C., USA  
88 YBN
[12/20/1912 AD]
4862)
(Percival Lowell's observatory) Flagstaff, Arizona, USA  
88 YBN
[1912 AD]
4298)
(Johns Hopkins University) Baltimore, Maryland, USA  
88 YBN
[1912 AD]
4383) Alfred North Whitehead (CE 1861-1947), English mathematician and
philosopher , in collaboration with Bertrand Russell (CE 1872-1970), publishes
“Principia Mathematica", in which he tries to build up mathematics from
symbolic logic. Gödel will show that there are unresolvable paradoxes in any
system of logic, such as the statement Russell creates about a set containing
all sets of which it is not a member being a member of itself.

(in my view there is no need for a logical basis to math, math simply is, and
needs no explanation or logical foundation. In someway, math can be applied to
the universe, but also to imaginary phenomena.)

(There are many logical apparent errors - for example the statement "can we be
certain that there is no certainty" - a statement which cannot be either true
or false, because if true it would be proven false, if false, then proven
true.)

(Trinity College) Cambridge, England  
88 YBN
[1912 AD]
4454)
(University of Tübingen) Tübingen , Germany  
88 YBN
[1912 AD]
4495)
(Mareseilles University) Mareseilles, France  
88 YBN
[1912 AD]
4697) (University of Innsbruck) Innsbruck, Austria  
88 YBN
[1912 AD]
4789)
(De Forest Radio Telephone Company) New York City, New York, USA
(presumably)  
88 YBN
[1912 AD]
4791)
(University of Leeds) Leeds, England  
88 YBN
[1912 AD]
4845)
(University of Copenhagen) Copenhagen, Denmark  
88 YBN
[1912 AD]
4891)
(University of Munich) Munich, Germany  
88 YBN
[1912 AD]
4892)
(University of Munich) Munich, Germany  
88 YBN
[1912 AD]
4913)
(University of Glasgow) Glasgow, Scotland  
88 YBN
[1912 AD]
4941)
Greenland  
88 YBN
[1912 AD]
4993)
(Lister Institute of Preventive Medicine) London, England   
88 YBN
[1912 AD]
4994) In 1936 Debye wins the Nobel Prize in chemistry for dipolar moments in
particular.
In 1935 as director of the Kaiser Wilhelm Institute for Physics in Berlin,
Debye renames it the Max Planck Institute.
In 1939 The Nazi government orders Debye to
become a citizen, he refuses and moves to the Netherlands.
In 1940 two months before the
Netherlands is invaded by Hitler, Debye leaves for the United States and stays
there. (Perhaps he knew from the cam-thought net?)
(University of Göttingen) Göttingen, Germany  
88 YBN
[1912 AD]
5001) (Technical University at Hannover) Hannover, Germany  
88 YBN
[1912 AD]
6104) "When Irish Eyes Are Smiling" is published. "When Irish Eyes Are Smiling"
is written by Chauncey Olcott and George Graff, Jr., set to music composed by
Ernest Ball, for Olcott's production of "The Isle O' Dreams", and Olcott sings
the song in the show.

New York City, New York, USA (guess)  
88 YBN
[1912 AD]
6262)
(Metropolitan Opera House) New York City, New York, USA  
87 YBN
[01/17/1913 AD]
4405)
(University of Leeds) Leeds, England  
87 YBN
[01/27/1913 AD]
4272)
(Cambridge University) Cambridge, England   
87 YBN
[02/18/1913 AD]
4909)
(University of Glasgow) Glasgow, Scotland  
87 YBN
[04/05/1913 AD]
5005) In 1920 in Copenhagen, Bohr heads an institute for atomic studies that is
funded by the Carlsberg brewery. And this institute is a magnet for theoretical
physicists, Asimov describing it as almost a new Alexandria.
In 1922 Bohr wins the Nobel
Prize in physics for his “electron shell” theory. Bohr will donate his
Nobel Prize to Finnish war relief.
In 1933 when Hitler comes to power in
Germany, Bohr helps to get many Jewish physicists to safety.
In 1943 Bohr escapes from
Denmark to Sweden, Hitler had invaded Denmark in 1940. Before leaving Denmark
Bohr dissolves the gold Nobel medals of Franck and Laue in a bottle of acid to
keep them safe (after the war the gold will be precipitated and the medals
recast]. From Sweden Bohr will help to arrange the escape of nearly every
Danish Jewish person from death in Hitler's poison gas chambers.
On 10/06/1943
Bohr is flown from Denmark in a tiny plane to England and nearly dies from lack
of oxygen.
Bohr will work on the atomic bomb project at Los Alamos until 1945.
Bohr's
desire to share the secret of the atomic bomb with other allies in order to
secure international control causes Winston Churchill to nearly order Bohr to
be arrested. (It seems likely that Bohr wanted to go public with neuron reading
and writing.)
In 1957 Bohr wins the Atoms for Peace award.
(University of Manchester) Machester, England  
87 YBN
[04/07/1913 AD]
4406) William Henry Bragg will state in 1920 that “The outbreak of war,
practically put a stop to the work with the spectroscope , ...", and this may
reflect the general development of science, in particular, how much is allowed
to reach the public. it may very well be that the two world wars greatly
reduced the progress of science, from the perspective of public knowledge.
(University of Leeds) Leeds, England  
87 YBN
[04/07/1913 AD]
6245)
Chicago, Illinois, USA  
87 YBN
[05/09/1913 AD]
4814)
(Research Laboratory of the General Electric Company) Schenectady, New York, in
1900.  
87 YBN
[05/28/1913 AD]
4932)
(Federal Institute of Technology) Zurich, Switzerland  
87 YBN
[05/29/1913 AD]
6035)
(Théâtre des Champs Élysées) Paris, France  
87 YBN
[06/21/1913 AD]
4408)
(Cavindish Laboratory, Cambridge University) Cambridge, England  
87 YBN
[07/18/1913 AD]
4800)
Potsdam, Germany  
87 YBN
[07/30/1913 AD]
4407)
(University of Leeds) Leeds, England  
87 YBN
[10/20/1913 AD]
4863)
(Percival Lowell's observatory) Flagstaff, Arizona, USA  
87 YBN
[10/29/1913 AD]
5067) Armstrong studies electrical engineering under Pupin at Columbia.
Lee De
Forest, the inventor of the triode, the first electric switch and vacuum tube
amplifier, sues Armstrong over who owns the rights for the regenerative
circuit. Armstrong will lose this case after 14 years and two appeals to the
Supreme Court, but Asimov says that the scientific community felt that
Armstrong should have won.
In 1954 Armstrong apparently jumped to his death from his
apartment window. According to Asimov Armstrong thought there was a conspiracy
against him. (This could be a murder, the nanocameras probably show the truth.)
Yonkers, New York City, New York, USA  
87 YBN
[11/05/1913 AD]
4824)
(Physical Institute of Technology) Aachen, Germany  
87 YBN
[11/27/1913 AD]
4911)
  
87 YBN
[12/04/1913 AD]
4910)
(University of Glasgow) Glasgow, Scotland  
87 YBN
[12/??/1913 AD]
5039) World War I starts and Moseley enlists as a lieutenant of the Royal
Engineers. Rutherford tries to get Moseley reassigned to scientific labors but
fails. On 06/13/1915 Moseley ships out to Turkey and two months later is killed
at Gallipoli. Asimov states that Moseley definitely would have won a Nobel
prize as Siegbahn did who carried on Moseley's work. (Possibly murdered for
being a corpuscularist or just random, perhaps his eye image and thought-sound
recordings may show? Being a corpuscularist, Moseley could have potentially
been a powerful force as he aged had he not been murdered. Moseley
unquestionably would have won a Nobel prize.)
(University of Manchester) Machester, England  
87 YBN
[1913 AD]
4030) Thomas Alva Edison (CE 1847-1931) introduces to the public a kinetophone
different from the earlier version of 1895. This time, the sound is made to
synchronize with a motion picture projected onto a screen instead of in the
kinetophone box. A celluloid cylinder record measuring 5 1/2" in diameter is
used for the phonograph. Synchronization is achieved by connecting the
projector at one end of the theater and the phonograph at the other end with a
long pulley. Nineteen talking pictures are produced in 1913 by Edison, but by
1915 Edison abandons sound motion pictures. Breaks in the film cause the motion
picture to get out of step with the phonograph record.

New York City, NY, USA (presumably)  
87 YBN
[1913 AD]
4129)
(University of Madrid) Madrid, Spain  
87 YBN
[1913 AD]
4361)
(University of Wisconsin) Wisconsin, USA  
87 YBN
[1913 AD]
4496)
(Mareseilles University) Mareseilles, France  
87 YBN
[1913 AD]
4507) In 1914 Richards receives the Nobel prize in chemistry for his atomic
weight determinations the first chemist in the United States to be so honored.
(Harvard University) Cambridge, Massachussets, USA  
87 YBN
[1913 AD]
4727)
(Technische Hochschule) Hannover, Germany  
87 YBN
[1913 AD]
4811)
Paris, France  
87 YBN
[1913 AD]
4849) Michaelis, being of Jewish ancestry, is denied the opportunity to
participate fully in the education of future German scientists and physicians.
(Berlin Municipal Hospital) Berlin, Germany  
87 YBN
[1913 AD]
4942) Schaefer and Vonnegut will develop methods to create rain working in
Langmuir's lab at General Electric.

Langmuir develops high vacuum tubes which are needed for radio broadcasting.

Langmuir creates a theory of catalysis based on the formation of gas films on
platinum wires.

Langmuir receives 63 patents and publishes over 200 papers and reports between
1906 and 1956.

In 1932 languir wins the Nobel prize chemistry for his work on surface
chemistry.
(General Electric Company) Schenectady, New York, USA  
87 YBN
[1913 AD]
4963) Geiger participates briefly in Germany's abortive attempt to develop an
atomic bomb during World War II.
In 06/1945 Geiger flees the Russian occupation
to Potsdam and dies there two months after the atomic bomb explodes over
Hiroshima.
(Physikalisch-Technische Reichsanstalt) Berlin, Germany  
87 YBN
[1913 AD]
5019) In 1922 Hill wins the Nobel Prize in medicine and physiology shared with
Meyerhof.
(University of Cambridge) Cambridge, England  
87 YBN
[1913 AD]
5057)
(University of Freiburg) Freiburg, Germany  
87 YBN
[1913 AD]
5083)
(University of Manchester) Manchester, England  
86 YBN
[02/??/1914 AD]
4747)
(University of Manchester) Manchester, England   
86 YBN
[04/02/1914 AD]
5235) Chadwick will spend the years of World War I in a civilian internment
camp in Ruhleben.
(Physikalisch-Technische Reichsanstalt) Charlottenburg, Germany  
86 YBN
[04/20/1914 AD]
5676)
(Sorbonne, University of Paris) Paris, France  
86 YBN
[04/??/1914 AD]
5107)
(University of Oxford) Oxford, England  
86 YBN
[05/??/1914 AD]
4762)
(University of Manchester) Manchester, England   
86 YBN
[05/??/1914 AD]
5085)
(University of Manchester) Manchester, England  
86 YBN
[05/??/1914 AD]
5879)
(University of Manchester) Manchester, England  
86 YBN
[07/28/1914 AD]
4792)
Berlin, Germany (verify)  
86 YBN
[07/??/1914 AD]
4879)
(Mount Wilson Observatory) Pasadena, California, USA  
86 YBN
[07/??/1914 AD]
4973)
(Princeton University) Princeton, New Jersey, USA (verify)  
86 YBN
[08/13/1914 AD]
5007) After World War II, Shapley is active in the cause of civil liberties and
peace.
Shapley clashes frequently with people such as Senator Joseph McCarthy.
(Mount Wilson Solar Observatory) Mount Wilson, California, USA  
86 YBN
[08/??/1914 AD]
5109)
(University of Manchester) Manchester, England  
86 YBN
[1914 AD]
4497)
(Mareseilles University) Mareseilles, France  
86 YBN
[1914 AD]
4785)
(The Rockefeller Institute for Medical Research) New York City, New York,
USA  
86 YBN
[1914 AD]
4852)
(Wellcome Physiological Research Laboratories) Herne Hill, England  
86 YBN
[1914 AD]
4962) In 1925 Franck wins the Nobel Prize in physics shared with Gustav Hertz.
In 1933
Franck resigns his university position in protest against the policies of the
new Nazi government.
In 1934 Franck is forced to flee Hitler's anti-Jewish Nazi Germany.
Franck first joins Bohr in Copenhagen, then goes to the USA.
Franck works on
the atomic bomb project in the USA, and strenuously opposes dropping the atomic
bomb on Japan favoring a demonstration before representatives of the United
Nations instead, in the hope this would encourage a ban of the bomb instead of
its use.




(Hertz works with Franck to establish the quantized nature of the atom's
internal structure.) (needs specifics and I think there are some.)
-Hertz is severely
wounded in World War I fighting on the German side.
-1925 Nobel prize in
physics shared with Franck.
-1934 Hertz is forced to resign his job because he
is of Jewish descent, but remains in Germany through World War II and
survives.
-n
(University of Berlin) Berlin, Germany  
86 YBN
[1914 AD]
4965) Goddard is the only child of a bookkeeper, salesman, and machine-shop
owner .
In 1898 young Goddard’s imagination was fired by the H.G. Wells
space-fiction novel War of the Worlds, then serialized in the Boston Post.

Over the course of his life, Goddard accumulates 214 patents.
Only during World
War II does the US government finance Goddard and then to design small rockets
to help navy planes take off from carriers.
Nazi Germany will develop rockets,
and the captured German rocket experts explain with surprise that they had
learned almost everything they know about rockets from Goddard.
In 1960 the US
Government issues a grant of one million dollars for the use of Goddard's
patents, half to the Goddard's estate and half to the Guggenheim Foundation.

(It seems possible that much of Goddard's work may still be secret. Was Goddard
actually secretly funded by the US Government? Perhaps no since the 1 million
dollar settlement for patent use in 1960.)

(Did Goddard receive neuron written windows?)
(Clark University) Worcester, Massachusetts, USA  
86 YBN
[1914 AD]
4977) Spiral "nebulae" recognized to be other galaxies.

(Sir) Arthur Stanley Eddington (CE 1882-1944), English astronomer and physicist
suggests that spiral nebulas are galaxies in "Stellar movements and the
structure of the universe".

Eddington writes:
"If the spiral nebulae are within the stellar system, we have no
notion what their nature may be. That hypothesis leads to a full stop. It is
true that according to one theory the solar system was evolved from a spiral
nebula, but the term is here used only by a remote analogy with such objects as
those depicted in the Plate. The spirals to which we are referring are, at any
rate, too vast to give birth to a solar system, nor could they arise from the
disruptive approach of two stars; we must at least credit them as capable of
generating a star cluster.

If, however, it is assumed that these nebulae are external to the stellar
system, that they are in fact systems coequal with our own, we have at least an
hypothesis which can be followed up, and may throw some light on the problems
that have been before us. For this reason the "island universe" theory is much
to be preferred as a working hypothesis; and its consequences are so helpful as
to suggest a distinct probability of its truth. ——

If each spiral nebula is a stellar system, it follows that our own system is a
spiral nebula. The oblate inner system of stars may be identified with the
nucleus of the nebula, and the star clouds of the Milky Way form its spiral
arms. There is one nebula seen edgewise (Plate IV) which makes an excellent
model of our system, for the oblate shape of the central portion is well-shown.
From the distribution of the Wolf-Rayet stars and Cepheid Variables, believed
to belong to the more distant parts of the system, we infer that the outer
whorls of our system lie closely confined to the galactic plane; in the nebula
these outer parts are seen in section as a narrow rectilinear streak. The
photograph also shows a remarkable absorption of the light of the oblate
nucleus, where it is crossed by the spiral arms. We have seen that the Milky
Way contains dark patches of absorbing matter, which would give exactly this
effect. Moreover, quite apart from the present theory, a spiral form of the
Milky Way has been advocated. Probably there is more than one way of
representing its structure by means of a double-armed spiral; but as an example
the discussion of C. Easton11 may be taken, which renders a very detailed
explanation of the appearance. His scheme disagrees with our hypothesis in one
respect, for he has placed the Sun well outside the central nucleus, which is
situated according to his view in the rich galactic region of Cygnus.

The two arms of the spiral have an interesting meaning for us in connection
with stellar movements. The form of the arms—a logarithmic spiral—has not
as yet given any clue to the dynamics of spiral nebulae. But though we do not
understand the cause, we see that there'is a widespread law compelling matter
to flow in these forms.

It is clear too that either matter is flowing into the nucleus from the spiral
branches or it is flowing out from the nucleus into the branches. It does not
at present concern us in which direction the evolution is proceeding. In either
case we have currents of matter in opposite directions at the points where the
arms merge in the central aggregation. These currents must continue through the
centre, for, as will be shown in the next chapter, the stars do not interfere
with one another's paths. Here then we have an explanation of the prevalence of
motions

to and fro in a particular straight line; it is the line from • which the
spiral branches start out. The two starstreams and the double-branched spirals
arise from the same cause.".
(Cambridge University) Cambridge, England   
86 YBN
[1914 AD]
5040) Joseph Stalin will support Lysenko's rejection of Mendelism and Vavilov
will be arrested on 08/06/1940 and sentenced to death, although this will be
reduced to 10 years.
During World War II Vavilov will be evacuated to Saratov where he
will die from maltreatment in 1943.
(Agricultural Higher School) Moscow, Russia  
86 YBN
[1914 AD]
5088)
(Lick Observatory) Mount Hamilton, California, USA  
86 YBN
[1914 AD]
5179)
(University of Zurich) Zurich, Switzerland  
86 YBN
[1914 AD]
6034)
(93rd Highlanders, British army) Scotland, UK (verify)  
85 YBN
[01/25/1915 AD]
4043)
New York City and San Francisco, USA  
85 YBN
[01/??/1915 AD]
4410)
(University of Leeds) Leeds, England (and Cambridge University) Cambridge,
England  
85 YBN
[01/??/1915 AD]
4864)
(Percival Lowell's observatory) Flagstaff, Arizona, USA  
85 YBN
[06/04/1915 AD]
4748)
(Royal Institution) London, England   
85 YBN
[09/15/1915 AD]
4510)
(University of Chicago) Chicago, illinois, USA  
85 YBN
[11/??/1915 AD]
4840) Goldberger marries a Gentile (non-Jewish person), and Asimov comments
that this is when mixed race marriages are uncommon.
(US Public Health Service) Washington, DC, USA (verify)  
85 YBN
[12/01/1915 AD]
4881)
(Mount Wilson Observatory) Pasadena, California, USA  
85 YBN
[12/03/1915 AD]
4995)
(University of Göttingen) Göttingen, Germany  
85 YBN
[12/04/1915 AD]
4917)
(Brown Institution) London, England  
85 YBN
[1915 AD]
4392)
(Cape Observatory) South Africa  
85 YBN
[1915 AD]
4777)
(London University) London, England  
85 YBN
[1915 AD]
4817) (University of Chicago) Chicago, illinois, USA  
85 YBN
[1915 AD]
4818)
(University of Chicago) Chicago, illinois, USA  
85 YBN
[1915 AD]
4878)
(Mount Wilson Observatory) Pasadena, California, USA  
85 YBN
[1915 AD]
4933)
( Berlin’s Kaiser Wilhelm Institute for Physics) Berlin, Germany  
85 YBN
[1915 AD]
4934)
(Berlin’s Kaiser Wilhelm Institute for Physics) Berlin, Germany  
85 YBN
[1915 AD]
4970)
(Clark University) Worcester, Massachusetts, USA  
85 YBN
[1915 AD]
6048) First Jazz composition in print, Jelly Roll Morton's "Jelly Roll Blues".

Ferdinand Joseph LaMothe (1885-1941), known professionally as Jelly Roll
Morton, US ragtime and early jazz pianist, bandleader and composer, composed
"Jelly Roll Blues" around 1905, and this composition is the first jazz
arrangement in print (1915), introducing more musicians to the New Orleans
style.

(verify)

(Will Rossiter) Chicago, Illinois, USA (where published)   
84 YBN
[01/13/1916 AD]
4808)
Berlin, Germany (published), Russia (written)  
84 YBN
[01/26/1916 AD]
4855) Lewis is an early supporter of Einstein's 1905 theory of relativity.
In 1917 Lewis
creates a compilation of entropy data and creates an empirical verification of
Nernst’s third law.
To me, without trying to sound rude, both these examples show
how Lewis apparently accepted a large portion of inaccurate, abstract
scientific theories.
(University of California at Berkeley) Berkeley, California, USA  
84 YBN
[01/26/1916 AD]
4856)
(University of California at Berkeley) Berkeley, California, USA  
84 YBN
[02/08/1916 AD]
4880)
(Mount Wilson Observatory) Pasadena, California, USA  
84 YBN
[02/24/1916 AD]
4809)
Berlin, Germany (published), Russia (written)  
84 YBN
[11/27/1916 AD]
4437)
(Wurzburg University) Wurzburg, Germany  
84 YBN
[11/??/1916 AD]
4982)
(Cambridge University) Cambridge, England   
84 YBN
[1916 AD]
4086)
(Edinburgh University) Edinburgh, Scotland  
84 YBN
[1916 AD]
4317)
(Yerkes Observatory University of Chicago) Williams Bay, Wisconsin, USA  
84 YBN
[1916 AD]
4511)
(University of Chicago) Chicago, illinois, USA  
84 YBN
[1916 AD]
4530) Sommerfeld publishes an influential work that goes through a number of
editions in the 1920s, "Atombau und Spektrallinien" (Atomic Structure and
Spectral Lines).
Sommerfeld, although not Jewish, opposes the Fascism and
anti-Jewishness in Germany after WW I, and in 1940 Sommerfeld is denounced and
forced into retirement, but survives WW2.
Sommerfeld is killed at age 83 by an
automobile.
  
84 YBN
[1916 AD]
4776)
(Pasteur Institute) Paris, France  
84 YBN
[1916 AD]
4944)
(General Electric Company) Schenectady, New York, USA  
84 YBN
[1916 AD]
5013) In 1950 Kendall, Hench, and Reichstein share the Nobel Prize in medicine
and physiology.
(Mayo Foundation) Rochester, Minnesota, USA  
84 YBN
[1916 AD]
5023) In 1924 Siegbahn wins the Nobel Prize in physics for his development of
X-ray spectroscopy.
(University of Lund) Lund, Sweden  
83 YBN
[03/03/1917 AD]
4529)
(Harvard College Observatory) Cambridge, Massachussetts, USA  
83 YBN
[04/15/1917 AD]
4945)
(General Electric Company) Schenectady, New York, USA  
83 YBN
[06/??/1917 AD]
4702) In 1937 Honda wins the Cultural Order of the Rising Sun, an equivalent
award to the Nobel prize. (Is this prize only for those in Japan? How much
money is the award?)

Relation to the Honda Soichiro of Honda motor?
(Tokyo Imperial University) Tokyo, Japan  
83 YBN
[07/28/1917 AD]
4769)
(Lick Observatory) Mount Hamilton, California, USA  
83 YBN
[09/??/1917 AD]
4865)
(Percival Lowell's observatory) Flagstaff, Arizona, USA  
83 YBN
[10/18/1917 AD]
5025) Curtis is famous for debating Harlow Shapley in 1920, Curtis taking the
more accurate "island universe" theory against Shapley who takes the view that
the spiral nebulae are part of our galaxy.
(Lick Observatory) Mount Hamilton, California, USA  
83 YBN
[1917 AD]
4295) In 1927 Wagner von Jauregg is awarded a Nobel prize for physiology and
medicine.
(One of a number of dubious people to win the Nobel prize - Moniz for the
involuntary lobotomy being another.)

The Oxford Dictionary of Scientists reports that Wagner von Jauregg finds it
difficult to obtain an academic post in orthodox medicine, and so turns to
psychiatry in 1883 and in 1889 succeeds Krafft-Ebbing as professor of
psychiatry at the University of Graz. (kind of funny - in stating that
psychiatry is not an orthodox health science - I think if strictly consent-only
it could possibly be called a highly experimental science, but with many fields
of science, in particular because of the neuron reading/writing secret, the
theoretical basis behind experiments is many times highly inaccurate and
unlikely.)
(University of Vienna Hospital for Nervous and Mental Diseases) Vienna,
Austria  
83 YBN
[1917 AD]
4524) A 100-inch reflecting telescope is completed on Mount Wilson, planned and
supervised by George Ellery Hale (CE 1868-1938), and funded by the wealthy Los
Angeles hardware business owner John D. Hooker. This will remain the largest
telescope on earth for 40 years.

Hale has for a third time built the largest telescope on earth.

(Mount Wilson Observatory) Pasadena, California, USA  
83 YBN
[1917 AD]
4716)
(unknown) Paris, France (presumably, verify)  
83 YBN
[1917 AD]
4761) Langevin earns his Ph.D. under Curie.
(Collège de France) Paris, France (presumably)  
83 YBN
[1917 AD]
4765) (read and show full paper)
(University of Leiden) Leiden, Netherlands  
83 YBN
[1917 AD]
5026) Köhler is outspoken in his criticism of Adolf Hitler’s government and
goes to the United States in 1935. (perhaps an outsider - unaware of neuron
reading and writing, as millions are?)
(Prussian Academy of Sciences at Tenerife) Canary Islands  
83 YBN
[1917 AD]
6049) The first recording of a jazz musical composition is made by the
"Original Dixieland Jass Band", a New Orleans, Dixieland Jazz band. Their
"Livery Stable Blues" is the first jazz single issued.

The band consists of five musicians who previously had played in the Papa Jack
Laine bands, a diverse and racially integrated group of musicians who played
for parades, dances, and advertising in New Orleans. In late 1917 the spelling
of the band's name is changed to "Original Dixieland Jazz Band".

(verify)
New Orleans, Louisiana, USA (presumably)  
83 YBN
[1917 AD]
6097) "Over There" is written and recorded (by George M. Cohan during World War
I).

New York City, New York, USA (presumably)  
82 YBN
[03/16/1918 AD]
4923) In 1902 Meitner becomes interested in science when she reads of the
Curies' identifying radium.
Emil Fischer makes Meitner promise never to enter
laboratories where males are working at first.
In 1938 when the Nazis take over
Austria, Meitner, being Jewish, is forced to leave. Through the help of Debye
and Coster, Meitner enters the Netherlands without a
visa. Meitner then goes to
Bohr in Denmark and Bohr helps her get a job with Siegbahn.
In 1966 Meitner is awarded a
share of the Fermi Award issued by the Atomic Energy Commission, and is the
first woman to win the award.
Meitner never married.

In 1945 Hahn wins the 1944 Nobel prize in chemistry "for his discovery of the
fission of heavy nuclei". Fortunately the Nazis do not recognize the potential
destruction possible from uranium fission.
In 1946-1960 Hahn is the president of the
West German Max Planck Society.
(Institut für Chemie in Berlin-Dahlem) Berlin, Germany  
82 YBN
[04/??/1918 AD]
5008) The Sun is determined to be in the outer part of our galaxy.

Harlow Shapley (CE 1885-1972), US astronomer, determines that the sun is in the
outer part of a galaxy by measuring the position of globular clusters using the
variable-star method to determine the distance of variable stars within each
globular cluster. Between 1915 and 1920 Shapley uses the 100-inch telescope at
Mount Wilson to study the globular clusters, which are very dense groups of
stars, some containing as many as a million stars each. At this time 100 such
clusters are known. Shapley finds that the globular clusters are all
concentrated in the direction of Sagittarius, one-third of the clusters are
found within the boundaries of Sagittarius. In 1914 Shapley worked out the
variable star distance measuring method worked out by Henrietta Swan Leavitt a
few years earlier, and applied the period-luminosity curve to the variable
stars in each globular cluster. From the period and apparent brightness of
these variable stars, Shapley calculates their distances. Shapley finds that
the clusters are distributed roughly in the shape of a sphere around a center
in Sagittarius. It seems logical to Shapley that these globular clusters are
centered around the center of our galaxy. Shapley calculates this center to be
50,000 light years away. Oort will later reduce this to 30,000 light years.
This is a much larger estimate than all previous estimates. Astronomers from
Herschel to Kapteyn thought the sun was near the center of the galaxy, because
the Milky Way is equally bright in all directions. Shapley explains that dark
dust clouds block the bright center and allow only a view of stars near us, and
outside the plane of the galaxy. Radio astronomy will confirm that the bright
center of the Milky Way is hidden behind clouds of matter. At first, according
to Asimov, there was bitter opposition to this view of the galaxy. Just as
Aristarchos and Copernicus had moved the earth from the center of the universe,
Shapley moved the sun from the center of the galaxy.

Shapley writes in an article titled "Remarks on the Arrangement of the Sidereal
Universe" in Astrophysical Journal:
" Introduction.—A fairly definite conception of
the arrangement of the sidereal system evolves naturally from the observational
work discussed in the preceding Contributions. We find, in short, that globular
clusters, though extensive and massive structures, are but subordinate items in
the immensely greater organization which is dimly outlined by their positions.
From the new point of view our galactic universe appears as a single, enormous,
allcomprehending unit, the extent and form of which seem to be indicated
through the dimensions of the widely extended assemblage of globular clusters.
The fundamental nature of the galactic plane, in the dynamical structure of all
that we now recognize as the sidereal universe, is manifested by the
distribution of clusters in space. Near this plane lie the celestial objects
that we customarily study. The open clusters, the diffused and planetary
nebulae, the naked-eye stars, most variables, the objects that define and
compose the star streams—all of these appear to be far within a relatively
narrow equatorial region of the greater galactic system, a region in which
globular clusters are not found. The Orion nebula and even the Magellanic
clouds are miniature organizations in this general scheme, and undoubtedly are
dependents of the Galaxy.

The adoption of such an arrangement of sidereal objects leaves us with no
evidence of a plurality of stellar "universes." Even the remotest of recorded
globular clusters do not seem to be independent organizations. The hypothesis
that spiral nebulae are separate galactic systems now meets with further
difficulties.
...
3. Relation of present interpretation to earlier hypotheses.—In order to show
where the earlier working hypotheses stand with respect to the interpretation
now offered, it may be of interest to note the development, during the course
of this work on clusters and variable stars, of the ideas concerning the
relation of globular clusters to the galactic organization. Until the last year
or so most students of stellar problems believed rather vaguely that the sun
was not far from the center of the universe, and that the radius of the
galactic system was of the order of iooo parsecs. From the earlier
observational data Seeliger and Newcomb derived a fairly central position for
the sun. Hertzsprung in 1906 estimated the "Dimensionen" of the visible Milky
Way system to be of the order of 2000 parsecs, and some years later Walkey,
from consideration of extensive distributional data, estimated a distance of
about seventeen hundred parsecs for the galactic main stream. In 1914,
referring to the apparently lens-shaped sidereal system, Eddington wrote,
"There is little evidence as to the sun's position with respect to the
perimeter of the lens; all that we can say is that it is not markedly
eccentric"; and the diameter of the whole system (possibly excluding the
peripheral ring of galactic clouds) was placed at some two or three thousand
parsecs, with emphasis on the uncertainty. For a later computation Eddington
assumed the distance of the Milky Way to be 2000 parsecs.

The work on the hypothetical parallaxes of Cepheids and O-type stars by
Hertzsprung, and of eclipsing binaries and Cepheids by Professor Russell and
the writer, began to give concrete numerical expression to the distances of
remote galactic objects, and in 1914 we have the statement: "Our 'universe' of
stars must be some thousands of light-years in diameter," but the computed
radius of 2500 parsecs was reduced to 1200 by allowing for a presumably
reasonable and necessary scattering of light in space. The necessity for such a
correction seems now definitely to have vanished, but the general conception of
the size of the stellar system has not materially changed.
....
5. The Milky Way and its asymmetry; regions of maximum star
density.-—According to the present view of the galactic system the phenomenon
of the Milky Way is largely an optical one. Although the existence of local and
occasionally very extensive condensations of Milky Way stars is not denied, the
conception of a narrow encircling ring is abandoned. The Milky Way girdle is
chiefly a matter of star depth, and its long recognized weakness between
longitudes 90° and 180° is now taken to be a reflection of the eccentric
position of the sun.

On the basis of the third and fourth diagrams of the seventh paper we estimate
provisionally that the limit of the Galaxy is three times greater in longitude
325° than in the opposite direction. This does not require an impossible
difference of stellar density in the two directions, even if there is a
considerable condensation toward the center. A star of a given absolute
luminosity situated in the galactic plane would appear less than two and a half
magnitudes fainter at the boundary of the system beyond the center than at the
opposite point, which is nearest the sun. The remarkable one-sidedness of the
Milky Way has been little considered heretofore in works on stellar
distribution. Nort, in studying the Harvard map, has made an important
beginning by showing that the star density is four or five times greater in the
direction of the southern star clouds than in some of the shallower galactic
regions of the north.

The surpassing stellar density in the direction now assigned to the center of
the galactic system is particularly remarked by Chapman and Melotte1 in their
study of the Franklin-Adams plates. They state that one plate with center in a
= 18h, δ= — 30°

covers the Sagittarius region of the Southern Milky Way, and the star clouds on
limited portions of it are so thick that in the case of twelve out of the

twenty-five areas counted on it, it was found impossible to count every star
shown; the images of the faintest stars in these regions merged into one
another forming a continuous gray background. On every other plate of the
Franklin-Adams series even the faintest star images shown were separate and
distinct, and the counts included all stars visible. The extreme richness of
the Sagittarius region may be judged of, then, when it is noticed that the
incomplete counts on it show far more stars than are found in any other part of
the Milky Way.

The fathoming of the sidereal universe need not long depend on globular
clusters alone. If the nearest part of its boundary in the general direction of
Auriga and Gemini is not more distant than 30,000 parsecs, no stars in that
locality with absolute magnitude of zero or brighter will be fainter than the
apparent magnitude 17.5. B -type stars will therefore contribute in future
measurement of the extent of the system; and the Cepheid variables fainter than
the fourteenth magnitude will in time be fully as valuable as the globular
clusters in outlining the diameter and contour of the equatorial segment. As a
ready qualitative check of the direction and distance of the center, the blue
stars in the Milky Way should persist to a fainter magnitude in the southern
sky than in the direction of the anti-center.

The possibly ellipsoidal form of the system of globular clusters is indicated
in Fig. 1, which gives a projection on the galactic plane of the 60 clusters
for which R sin/3< 15,000 parsecs. If the elongation be accepted as a real characteristic of the stars also, it is evident that the apparently densest star regions, depending on the faintness of the stars involved in the estimate, may he in a longitude differing considerably from that of the center. The general direction of the galactic center is clearly toward the dense star clouds of Sagittarius and Scorpio; but the adopted galactic longitude, 325°, and the corresponding equatorial co-ordinates of the center, 0 = 17*5, S =—30°, are necessarily approximate.

The statistical center derived by Charlier from B-type stars is in Carina, in
longitude 236°, a result referring entirely to the local group (within 500
parsecs of the sun) and not influenced by the arrangement of the general
system. Stromberg, from bright stars

of the redder spectral types, finds the dynamical center in longitude 257°.
Nort,1 using stars to the eleventh magnitude on the Harvard map of the sky,
gets farther outside the bounds of the local cluster and obtains a maximum
stellar density in the Milky Way between longitudes 280° and 290°; he finds a
density but one-fifth as great in longitude 120°, the direction of the
anti*center. Chapman
270° Scorpio
and Melotte, working to the still fainter limit of the
FranklinAdams plates, find in the clouds of Sagittarius the only region too
dense for counting.

This progressive increase of the longitude of maximum star density from 236°
to 325° (with the increasing predominance of the general system over the local
group), and the appearance to be expected of the star clouds in the directions
of the two centers, are
both in striking agreement with Gould's observations of the
brightness of the Milky Way:1

Its brightest portion is unquestionably in Sagittarius {the galactic center};
that in Carina {the local center} being slightly inferior to this as regards
intrinsic brilliancy, although far more magnificent and impressive on account
of the great number of bright stars with which it is there spangled.
...".



A parsec is a unit of astronomical length based on the distance from Earth at
which stellar parallax is one second of arc and is equal to 3.258 light-years,
3.086 × 1013 kilometers, or 1.918 × 1013 miles.

(Interesting to think that our Galaxy may somehow relate to atomic
structure-for example our galaxy may be an atom or photon at some larger
scale.)

(there must be many phenomena around Sagittarius being in the direction of the
rest of the Milky Way Galaxy).

(It is interesting that the Milky Way must extend completely around the
earth.)

In modern times, about 150 globular clusters have been identified in the Milky
Way Galaxy.
(Mount Wilson Solar Observatory) Mount Wilson, California, USA  
82 YBN
[06/21/1918 AD]
6199) Electronic read and write memory.

This is the first use of the electric switch as memory. This is the first
publicly known electronic reading and writing, electronic memory, which with
transistors develops into memory chips (ROM, RAM, EPROM, EEPROM, Flash, etc).
Unlike laser (optical) reading and writing (CDs, DVDs), and magnetic reading
and writing (cassette tapes, VCR tapes, hard disks), the only moving parts are
electrons so electronic memory uses less electricity, but is not as permanent
and does not last as long as laser and magnetic recording.

William Henry Eccles and Frank Wilfred Jordan describe this circuit in a patent
filed in England entitled "Improvements in Ionic Relays". They write:
The relay is
designed to produce a large and permanent change in the current flowing in an
electrical circuit by means of a small electrical stimulus received from
outside. In its simplest form it consists of two three-electrode ionic tubes
with resistances. it is well-known that when the potential of the grid
electrode relative to the filament is increased and decreased within certain
limits, the current that can be sent through the tube from anode to filament by
means of a battery of constant voltage increases and decreases correspondingly.
In what follows the circuit comprising the space in the tube between anode and
filament, the external conductors and the source of E.M.F. will be called the
plate circuit and the current flowing in it the plate current. The circuit
comprising the space in the tube between the grid and the filament, external
conductors and a source of E.M.F. will be called the grid circuit and the
current flowing in it the grid current.
The principle of the relay is most easily
explained when two tubes, each with resistances and battery in its plate
circuit and with a resistance and battery in its grid circuit, are used and
interconnected in the following manner:-
The electrical stimulus from outside which it
is desired to detect is applied in the grid circuit of the first tube so as to
make the grid transiently more positive in potential relative to the filament.
This causes an increase of current in the plate circuit of the first tube and
consequently an increase of the potential difference between the terminals of
the plate circuit resistance. This increased potential difference is
transferred to the grid circuit of the second tube in such a manner the the
grid becomes more negative than before relative to its filament. Consequently
the plate current of the second tube decreases and the potential difference
between the terminals of its plate circuit resistance decreases also. This
decrease of potential difference is now transferred to the grid circuit of the
first tube in such a manner that it tends to make the grid more positive
relative to the filament. The result of these processes is that a positive
stimulus from outside given to the grid of the first tube initiates a chain of
changes, which result finally in the plate current of the first tube attaining
the highest value possible under the E.M.F. of its battery and the plate
current of the second tube falling to its lowest possible value. This condition
persists after the disappearance of the initial stimulus. In the initial
condition with the two-tube arrangement just described the plate current of the
first tube is made very small and that of the second tube large; after the
reception of the outside stimulus on the grid of the first tube the final
condition is a large plate current in the first tube and a small plate current
in the second tube. Either the decreases or the increases of plate current can
be used for indicating. In order to restore the initial conditions it is
necessary to interrupt for an instant the linkage between the tubes or to stop
the operation of one or both of the tubes, as for instance by dimming its
filament.
in the above described arrangements only two tubes have been used.
More than two tubes may be used, and when, more than two are used inductance
and capacity transformers may be utilised as essential parts between tubes in
addition to resistances.
...".
(City and Guilds Technical College) London, UK  
82 YBN
[10/??/1918 AD]
5880)
(University of Glasgow) Glasgow, Scotland  
82 YBN
[11/10/1918 AD]
4974)
(Aberdeen Proving Ground) Aberdeen, Maryland, USA  
82 YBN
[1918 AD]
4430)
(Harvard College Observatory) Cambridge, Massachussetts, USA  
82 YBN
[1918 AD]
4443)
( University of Berlin) Berlin, Germany  
82 YBN
[1918 AD]
4978)
(Cambridge University) Cambridge, England   
82 YBN
[1918 AD]
4979)
(Cambridge University) Cambridge, England   
82 YBN
[1918 AD]
5002) With the rise of the Nazi Party, Hevesy, who was of Jewish descent,
leaves Germany for Copenhagen in 1934.
The Nazis occupy Denmark in 1940, and in 1942
Hevesy escapes to Sweden.
In 1943 Hevesy wins the Nobel Prize in chemistry.
In 1959 Hevesy
wins the Atoms for Peace Award.
(University of Budapest) Budapest, Hungary  
82 YBN
[1918 AD]
5070) In 1959 Heyrovský wins a Nobel prize in chemistry.
(Charles University) Prague, Czechoslovakia  
82 YBN
[1918 AD]
6027)
(St. Paul’s Girls’ School or Morley College) London, England  
81 YBN
[02/08/1919 AD]
5068)
Paris, France  
81 YBN
[04/??/1919 AD]
4749)
(University of Manchester) Manchester, England  
81 YBN
[04/??/1919 AD]
4750) Atomic transmutation. Humans change atoms of nitrogen into atoms of
oxygen (transmutation) by colliding accelerated alpha particles with nitrogen
gas.

Ernest Rutherford (CE 1871-1937), British physicist, changes atoms of nitrogen
into atoms of oxygen (transmutation) by colliding accelerated alpha particles
with nitrogen gas.

Rutherford publishes this in a paper with the phrase "Light Atoms" in the title
which implies that light particles are atomic in nature.


Rutherford is the first to change one element into another, by using helium
nuclei to push out protons (Hydrogen) from nitrogen converting it to oxygen.
Rutherford sends alpha particles through a cylinder that can be filled with
various gases. He observes that oxygen lowers the number of scintillations
(illuminated dots on a luminescent screen), and concludes that the gas absorbs
some of the alpha particles before they reach the zinc sulfide screen. When the
cylinder is filled with hydrogen, very bright scintillations appear, and
Rutherford concludes that alpha particles knock forward the single proton
nucleus of the hydrogen atom, which then collide with the screen and cause the
bright scintillations. However, Rutherford finds that when nitrogen gas is in
the cylinder, the alpha particle scintillations are reduced but occasional
scintillations of the hydrogen kind appear. Rutherford concludes that the alhpa
particles are knocking protons out of the nitrogen atoms, and what remains has
to be oxygen. Rutherford is therefore the first to change one element into
another. This was a dream of the alchemists.

Asimov claims that this is the first "nuclear reaction". however, I think that
simple combustion can only be the complete separation of an atom into light
particles, or certainly a large portion of the atom including light particles
in the so-called nucleus are emitted in a typical combustion. Asimov states
that because only one atom in around 300,000 interacts with nuclei, this is not
a very practical form of transmutation. However it seems clear that
transmutation of atoms is extremely important, and clearly a large part of
secret research has been focused on the goal of greatly increasing the quantity
of atomic conversions. In particular, to convert common atoms like silicon and
iron into more useful atoms like Hydrogen, Oxygen and Nitrogen. This progress,
like most of neuron reading and writing, sadly remains currently secret. If no
such research has occured and is occuring this would seem extremely stupid and
short sighted.

By 1924 Rutherford will have knocked protons out of the nuclei of most of the
lighter elements.

This is a very rich source of research, and it seems clear that many people
must have developed this method of transmutation, trying to make it economical
(perhaps recycling the alpha particles, certainly trying many many more, trying
solids, trying other particles. Fermi will use neutrons to transmutate atoms.
One very important invention is a machine/process that can convert the common
abundant atoms of moons and planets into more useful atoms in particular
hydrogen and oxygen. In this way, all the silicon, aluminum, iron, the most
common elements on planets and moons, (for example on the earth moon) can be
converted into oxygen and hydrogen for use as fuel, to breathe, and for water.
To some extent converting these into nitrogen too is of value, and no doubt
phosphorus. Although Fermi finds that all such elements are radioactive. I
can't believe over 80 years of experimenting, the vast majority of which is
completely secret, people did not find, methods to create oxygen in bulk,
probably using any radioactivity to simply heat water to create electricity,
all contained and completely safe for everything outside the chamber.

Rutherford writes in his paper titled "Collision of α Particles with Light
Atoms":
"It has been shown in paper I. that a metal source, coated with a deposit of
radium C, always gives rise to a number of scintillations on a zinc sulphide
screen far beyond the range of the α particles. The swift atoms causing these
scintillations carry a positive charge and are deflected by a magnetic field,
and have about the same range and energy as the swift H atoms produced by the
passage of α particles through hydrogen. These "natural" scintillations are
believed to be due mainly to swift H atoms from the radioactive source, but it
is difficult to decide whether they are expelled from the radioactive source
itself or are due to the action of α particles on occluded hydrogen.

The apparatus employed to study these "natural" scintillations is the same as
that described in paper I. The intense source of radium C was placed inside a
metal box about 3 cm. from the end, and an opening in the end of the box was
covered with a silver plate of stopping power equal to about 6 cm. of air. The
zinc sulphide screen was mounted outside, about 1 mm. distant from the silver
plate, to admit of the introduction of absorbing foils between them. The whole
apparatus was placed in a strong magnetic field to deflect the beta rays. The
variation in the number of these "natural" scintillations with absorption in
terms of cms. of air is shown in fig. 1, curve A. In this case, the air in the
box was exhausted and absorbing foils of aluminium were used. Then dried oxygen
or carbon dioxide was admitted into the vessel, the number of scintillations
diminished to about the amount to be expected from the stopping power of the
column of gas.

A surprising effect was noticed, however, when dried air was introduced.
Instead of diminishing, the number of scintillations was increased, and for an
absorption corresponding to about 19 cm. of air the number was about twice that
observed when the air was exhausted. It was clear from this experiment that the
α particles in their passage through air gave rise to long-range
scintillations which appeared to the eye to be about equal in brightness to H
scintillations. A systematic series of observations was undertaken to account
for the origin of these scintillations. In the first place we have seen that
the passage of α particles through nitrogen and oxygen gives rise to numerous
bright scintillations which have a range of about 9 cm. in air. These
scintillations have about the range to be expected if they are due to swift N
or O atoms, carrying unit charge, produced by collision with α particles. All
experiments have consequently been made with an absorption greater than 9 cm of
air, so that these atoms are completely stopped before reaching the zinc
sulphide screen.

It was found that these long-range scintillations could not be due to the
presence of water vapour in the air; for the number was only slightly reduced
by thoroughly drying the air. This is to be expected, since on the average the
number of additional scintillations due to air was equivalent to the number of
H atoms produced by the mixture of hydrogen at 6 cm. pressure with oxygen.
Since on the average the vapour pressure of water in air was not more than 1
cm., the effects of complete drying would not reduce the number by more than
one sixth. Even when oxygen and carbon dioxide saturated with water vapour at
20° C. were introduced in place of dry air, the number of scintillations was
much less than with dry air.

It is well known that the amount of hydrogen or gases containing hydrogen is
normally very small in atmospheric air. No difference was observed whether the
air was taken directly from the room or from outside the laboratory or was
stored for some days over water.

There was the possibility that the effect in air might be due to liberation of
H atoms from the dust nuclei in the air. No appreciable difference, however,
was observed when the dried air was filtered though long plugs of cotton wool,
or by storage over water for some days to remove dust nuclei.

Since the anomalous effect was observed in air, but not in oxygen, or carbon
dioxide, it must be due either to nitrogen or to one of the other gases present
in atmospheric air. The latter possibility was excluded by comparing the
effects produced in air and in chemically prepared nitrogen. The nitrogen was
obtained by the well-known method of adding ammonium chloride to sodium
nitrite, and stored over water. It was carefully dried before admission to the
apparatus. With pure nitrogen, the number of long-range scintillations under
similar conditions was greater than in air. As a result of careful experiments,
the ratio was found to be 1.25, the value to be expected if the scintillations
are due to nitrogen.

The results so far obtained show that the long-range scintillations obtained
from air must be ascribed to nitrogen, but it is important, in addition, to
show that they are due to collision of α particles with atoms of nitrogen
through the volume of the gas. In the first place, it was found that the number
of the scintillations varied with the pressure of the air in the way to be
expected if they resulted from collision of α particles along the column of
gas. In addition, when an absorbing screen of gold or aluminium was placed
close to the source, the range of the scintillations was found to be reduced by
the amount to be expected if the range of the expelled atom was proportional to
the range of the colliding α particles. These results show that the
scintillations arise from the volume of the gas and are not due to some surface
effect in the radioactive source.

In fig. 1 curve A the results of a typical experiment are given showing the
variation in the number of natural scintillations with the amount of absorbing
matter in their path measured in terms of centimetres of air for α particles.
In these experiments carbon dioxide was introduced at a pressure calculated to
give the same absorption of the α rays as ordinary air. In curve B the
corresponding curve is given when air at N.T.P. is introduced in place of
carbon dioxide. The difference curve C shows the corresponding variation of the
number of scintillations arising from the nitrogen in the air. It was generally
observed that the ratio of the nitrogen effect to the natural effect was
somewhat greater for 19 cm. than for 12 cm. absorption.

In order to estimate the magnitude of the effect, the space between the source
and screen was filled with carbon dioxide at diminished pressure and a known
pressure of hydrogen was added. The pressure of the carbon dioxide and of
hydrogen were adjusted so that the total absorption of α particles in the
mixed gas should be equal to that of the air. In this way it was found that the
curve of absorption of H atoms produced under these conditions was somewhat
steeper than curve C of fig. 1. As a consequence, the amount of hydrogen mixed
with carbon dioxide required to produce a number of scintillations equal to
that of air, increased with the increase of absorption. For example, the effect
in air was equal to about 4 cm. of hydrogen at 12 cm. absorption. For a mean
value of the absorption, the effect was equal to about 6 cm. of hydrogen. This
increased absorption of H atoms under similar conditions indicated either that
(1) the swift atoms from air had a somewhat greater range than the H atoms, or
(2) that the atoms from air were projected more in the line of flight of the α
particles.

While the maximum range of the scintillations from air using radium C as a
source of α rays appeared to be about the same, viz. 28 cm., as for H atoms
produced from hydrogen, it was difficult to fix the end of the range with
certainty on account of the smallness of the number and the weakness of the
scintillations. Some special experiments were made to test whether, under
favourable conditions, any scintillations due to nitrogen could be observed
beyond 28 cm. of air absorption. For this purpose a strong source (about 60 mg.
Ra activity) was brought within 2.5 cm. of the zinc sulphide screen, the space
between containing dry air. On still further reducing the distance, the screen
became too bright to detect very feeble scintillations. No certain evidence of
scintillations was found beyond a range of 28 cm. It would therefore appear
that (2) above is the more probable explanation.

In a previous paper (III.) we have seen that the number of swift atoms of
nitrogen or oxygen produced per unit path by collision with α particles is
about the same as the corresponding number of H atoms in hydrogen. Since the
number of long-range scintillations in air is equivalent to that produced under
similar conditions in a column of hydrogen at 6 cm. pressure, we may
consequently conclude that only one long-range atom is produced for every 12
close collisions giving rise to a swift nitrogen atom of maximum range 9 cm.

It is of interest to give data showing the number of long-range scintillations
produced in nitrogen at atmospheric pressure under definite conditions. For a
column of nitrogen 3.3 cm. long, and for a total absorption of 19 cm. of air
from the source, the number due to nitrogen per milligram of activity is .6 per
minute on a screen of 3.14 sq. mm. area.

Both as regards range and brightness of scintillations, the long-range atoms
from nitrogen closely resemble H atoms, and in all probability are hydrogen
atoms. In order, however, to settle this important point definitely, it is
necessary to determine the deflexion of these atoms in a magnetic field. Some
preliminary experiments have been made by a method similar to that employed in
measuring the velocity of the H atom (see paper II.). The main difficulty is to
obtain a sufficiently large deflexion of the stream of atoms and yet have a
sufficient number of scintillations per minute for counting. The α rays from a
strong source passed through dry air between two parallel horizontal plates 3
cm. long and 1.6 mm. apart, and the number of scintillations on the screen
placed near the end of the plates was observed for different strengths of the
magnetic field. Under these conditions, when the scintillations arise from the
whole length of the column of air between the plates, the strongest magnetic
field available reduced the number of scintillations by only 30 per cent. When
the air was replaced by a mixture of carbon dioxide and hydrogen of the same
stopping power for α rays, about an equal reduction was noted. As far as the
experiment goes, this is an indication that the scintillations are due to H
atoms; but the actual number of scintillations and the amount of reduction was
too small to place much reliance on the result. In order to settle this
question definitely, it will probably prove necessary to employ a solid
nitrogen compound, free from hydrogen, as a source, and to use much stronger
sources of α rays. In such experiments, it will be of importance to
discriminate between the deflexions due to H atoms and possible atoms of atomic
weight 2. From the calculations given in paper III., it is seen that a
collision of an α particle with a free atom of mass 2 should give rise to an
atom of range about 32 cm. in air, and of initial energy about .89 of that of
the H atom produced under similar conditions. The deflexion of the pencil of
these rays in a magnetic field should be about .6 of that shown by a
corresponding pencil of H atoms.

Discussion of results.
From the results so far obtained it is difficult to avoid the
conclusion that the long-range atoms arising from collision of α particles
with nitrogen are not nitrogen atoms but probably atoms of hydrogen, or atoms
of mass 2. If this be the case, we must conclude that the nitrogen atom is
disintegrated under the intense forces developed in a close collision with a
swift α particle, and that the hydrogen atom which is liberated formed a
constituent part of the nitrogen nucleus. We have drawn attention in paper III.
to the rather surprising observation that the range of the nitrogen atoms in
air is about the same as the oxygen atoms, although we should expect a
difference of about 19 per cent. If in collisions which give rise to swift
nitrogen atoms, the hydrogen is at the same time disrupted, such a difference
might be accounted for, for the energy is then shared between two systems.

It is of interest to note, that while the majority of the light atoms, as is
well known, have atomic weights represented by 4n or 4n+3 where n is a whole
number, nitrogen is the only atom which is expressed by 4n+2. We should
anticipate from radioactive data that the nitrogen nucleus consists of three
helium nuclei each of atomic mass 4 and either two hydrogen nuclei or one of
mass 2. If the H nuclei were outriders of the main system of mass 12, the
number of close collisions with the bound H nuclei would be less than if the
latter were free, for the α particle in a collision comes under the combined
field of the H nucleus and of the central mass. Under such conditions, it is to
be expected that the α particle would only occasionally approach close enough
to the H nucleus to give it the maximum velocity, although in many cases it may
give it sufficient energy to break its bond with the central mass. Such a point
of view would explain why the number of swift H atoms from nitrogen is less
than the corresponding number in free hydrogen and less also than the number of
swift nitrogen atoms. The general results indicate that the H nuclei, which are
released, are distant about twice the diameter of the electron (7x10-13 cm.)
from the centre of the main atom. Without a knowledge of the laws of force at
such small distances, it is difficult to estimate the energy required to free
the H nucleus or to calculate the maximum velocity that can be given to the
escaping H atom. It is not to be expected, a priori, that the velocity or range
of the H atom released from the nitrogen atom should be identical with that due
to a collision in free hydrogen.

Taking into account the great energy of motion of the α particle expelled from
radium C, the close collision of such an α particle with a light atom seems to
be the most likely agency to promote the disruption of the latter; for the
forces on the nuclei arising from such collisions appear to be greater than can
be produced by any other agency at present available. Considering the enormous
intensity of the force brought into play, it is not so much a matter of
surprise that the nitrogen atom should suffer disintegration as that the α
particle itself escapes disruption into its constituents. The results as a
whole suggest that, if α particles--or similar projectiles--of still greater
energy were available for experiment, we might expect to break down the nucleus
structure of many of the lighter atoms.

I desire to express my thanks to Mr. William Kay for his invaluable assistance
in counting scintillations.".
(University of Manchester) Manchester, England  
81 YBN
[05/26/1919 AD]
4966)
(Clark University) Worcester, Massachusetts, USA  
81 YBN
[05/29/1919 AD]
4980)
Príncipe Island, West Africa  
81 YBN
[05/??/1919 AD]
3882)
New York City, NY (presumably)  
81 YBN
[06/08/1919 AD]
3849)
Syracuse, NY  
81 YBN
[08/??/1919 AD]
4905) In 1922 Aston wins the Nobel Prize in chemistry for for his discovery of
a large number of isotopes (atoms of the same element that differ in mass),
using a mass spectrometer, and for formulating the “whole number rule” that
isotopes have masses that are integer values of the mass of the hydrogen atom.

Aston recognizes the possibility of using the energy in the atom (which
Rutherford did not) and in his Nobel speech he speaks of the dangers involved
in such an eventuality. (see specifics.) Rutherford publicly doubted the use of
energy from atoms calling it "moonshine", however, Rutherford appears to have
hinted about atomic fission explosives as early as 1915.

Aston leaves much of his large estate to Trinity College.
(Cavendish Laboratory, Cambridge University) Cambridge, England  
81 YBN
[09/12/1919 AD]
4790)
(De Forest Phonofilm Corporation) New York City, New York, USA  
81 YBN
[11/??/1919 AD]
4163)
(University of Chicago) Chicago, Illinois, USA  
81 YBN
[12/30/1919 AD]
6095)
(University of Budapest) Budapest, Hungary  
81 YBN
[1919 AD]
4452)
(University of Tübingen) Tübingen , Germany  
81 YBN
[1919 AD]
4906)
(Cavendish Laboratory, Cambridge University) Cambridge, England  
81 YBN
[1919 AD]
4943)
(General Electric Company) Schenectady, New York, USA  
81 YBN
[1919 AD]
4997) In 1922 Meyerhof wins the Nobel Prize in medicine and physiology shared
with Hill.
In 1938 Meyerhof leaves Nazi Germany for France.
In 1940 after France falls to
Nazi Germany Meyerhof moves to the USA.
(University of Kiel) Kiel, Germany  
81 YBN
[1919 AD]
5022) Starting in 1911, Frisch conditions bees to relate the color black to
locations for food, showing that the conditioned bees fly to a black location
instead of a location emitting ultraviolet light (which bees can see but humans
cannot).

Frisch finds that bees communicate the distance and direction of a food supply
to other members of the colony by two types of rhythmic movements or dances:
circling and wagging. The circling dance indicates that food is within 75 m
(about 250 feet) of the hive, while the wagging dance indicates a greater
distance. Frisch finds that a bee's sense of smell is similar to that of
humans. Frisch also shows that bees are unable to distinguish between certain
shapes, that they have a limited range of color perception, but can see light
of shorter wavelength than humans.

(What is the proof of this - somehow matching the motions to some particular
food source?)
(Munich Zoological Institute) Munich, Germany  
81 YBN
[1919 AD]
5043) In 1933 Stern leaves Germany when Hitler comes to power.
Stern moves to
the USA, and is professor of physics at Carnegie Institute of Technology (now
Carnegie-Mellon university) in Pittsburgh, PA.
In 1943 Stern wins the Nobel Prize
in physics for work on molecular beams.
(The number of people leading the field in
particle physics that leave Germany on the rise of Hitler is amazing. Clearly
the people in Germany had a strong particle physics program (as did England),
and must have completely lost that advantage with the rise of Hitler. The
particle beam technology clearly is massive, in particular with the neuron
reading and writing flying nano devices.)
(University of Frankfurt) Frankfurt, Germany  
81 YBN
[1919 AD]
5071) Muller is part Jewish descent and leaves Germany with the rise of Hitler
and goes to Russia on the invitation of Vavilov.
In 1937 Muller leaves Russia after
openly opposing Lysenko's views on genetics.
In 1955 Muller joins Einstein and 6 other
scientists in a plea to outlaw nuclear bombs.
Like Galton, Muller promotes
eugenics to improve the “genetic health” of the human species.
(Rice Institute) Houston, Texas   
80 YBN
[01/??/1920 AD]
4914)
(University of Aberdeen) Aberdeen, Scotland  
80 YBN
[02/28/1920 AD]
4819)
(University of Chicago) Chicago, illinois, USA  
80 YBN
[04/19/1920 AD]
4322)
Jamaica  
80 YBN
[04/26/1920 AD]
4770)
(Lick Observatory) Mount Hamilton, California, USA  
80 YBN
[06/03/1920 AD]
4751)
(Cambridge University) Cambridge, England   
80 YBN
[12/01/1920 AD]
5110)
(Washington University) Saint Louis, Missouri, USA  
80 YBN
[1920 AD]
4309)
Kaluga, Russia (presumably)  
80 YBN
[1920 AD]
4411)
(University of Manchester) Manchester, England  
80 YBN
[1920 AD]
4453)
(University of Tübingen) Tübingen , Germany  
80 YBN
[1920 AD]
4553)
unknown  
80 YBN
[1920 AD]
4554)
unknown  
80 YBN
[1920 AD]
4555)
unknown  
80 YBN
[1920 AD]
4556)
unknown  
80 YBN
[1920 AD]
4557)
unknown  
80 YBN
[1920 AD]
4877)
(DuPont's Redpath Laboratory) Parlin, New Jersey  
80 YBN
[1920 AD]
4921)
(Notre Dame University) Notre Dame, Indiana, USA  
80 YBN
[1920 AD]
4922) In 1934 Whipple wins the Nobel Prize in medicine sharing with Minot and
Murphy for the cure for pernicious anemia. (How common is anemia? Perhaps
common because many people lose blood when injured, still how quickly can liver
work to cure anemia? Perhaps there has been some more specific finds about why
liver works to cure anemia since then.)
(University of California) San Francisco, California, USA  
80 YBN
[1920 AD]
4959)
(Technical Academy in Dresden) Dresden, Germany  
80 YBN
[1920 AD]
5041)
(University of Saratov) Saratov, Russia (presumably)  
80 YBN
[1920 AD]
5044)
(University of Frankfurt) Frankfurt, Germany  
80 YBN
[1920 AD]
5045)
(University of Frankfurt) Frankfurt, Germany  
80 YBN
[1920 AD]
5084)
  
80 YBN
[1920 AD]
5119) Baade is an enemy alien being German in the USA during World War II, but
is allowed to do non-war related science such as astronomy.
Baade takes
advantage of the war-time blackout in Los Angeles to capture photographs using
the 100-inch (2.5 m) reflecting telescope on Mount Wilson.
Over the course of his life
Baade locates over 300 variable stars (cephids) in the Andromeda Galaxy.
(University of Hamburg's Bergedorf Observatory) Hamburg, Germany  
80 YBN
[1920 AD]
5180)
(University of Zurich) Zurich, Switzerland  
80 YBN
[1920 AD]
6063) Al Jolson records the George Gershwin (CE 1898-1937) and Irving Caesar
song "Swanee".

New York City, New York, USA (probably)  
79 YBN
[01/21/1921 AD]
4924)
(Kaiser-Wilhelm-Instute fur Chemie) Berlin, Germany  
79 YBN
[02/26/1921 AD]
4752)
(Cambridge University) Cambridge, England   
79 YBN
[02/??/1921 AD]
4162) This is reported on the front page of the New York Times. Perhaps
michelson or others paid for it, or it may show the early popularity and
respectability of the Nobel Prize.
(Mount Wilson Observatory) Pasadena, California, USA  
79 YBN
[03/21/1921 AD]
5238)
(Lowell Observatory) Flagstaff, Arizona, USA  
79 YBN
[03/??/1921 AD]
5157)
(Cambridge University) Cambridge, England  
79 YBN
[04/26/1921 AD]
5239)
(Mount Wilson) Mount Wilson, California, USA  
79 YBN
[07/??/1921 AD]
4866)
(Percival Lowell's observatory) Flagstaff, Arizona, USA  
79 YBN
[09/26/1921 AD]
5051) In 1929 Raman is knighted by the British government.
In 1930 Raman wins the Nobel
Prize in physics.
In 1947 Raman is the Director of Raman Research institute at Bangalore
in India.
Raman is the first Asian human (human living in India, China, or
Russia?) to get a Nobel Prize.
Raman trains more than 500 young Indian people in
science and education in an effort to build up scientific research and
education in India.
(University of Calcutta) Calcutta, India  
79 YBN
[09/??/1921 AD]
4783) In 1936 Loewi with Sir Henry Dale, receive the Nobel Prize for Physiology
or Medicine for their discoveries relating to the chemical transmission of
nerve impulses.
In 1938 Loewi is placed under arrest (for being Jewish) when the Nazi's
invade Austria, but he is allowed to leave the country if he gives his Nobel
Prize money to the Nazis.
Loewi moves to England and then in 1940 to the USA.
(University of Graz) Graz, Austria  
79 YBN
[11/14/1921 AD]
5092) Best, as a graduate student, works a summer with Banting to isolate
insulin.
Best's aunt had recently died of diabetes and this serves as a
motivation.

In 1923 Banting is awarded an annuity by the Canadian Parliament and the
Banting Research Foundation is established for him.

In 1923 Banting and Macleod share the Nobel prize in medicine and physiology,
the first Nobel Prize to be awarded to Canadian people. Banting is furious that
the prize is shared with Macleod who had merely given then laboratory space,
and not with Best who had done his fair share of the labor. Banting has to be
persuaded to accept the prize, and gives half his share of the money to Best.
(University of Toronto) Toronto, Canada  
79 YBN
[1921 AD]
4068) Although having only a high school education, Burbank is profoundly
influenced by the books of Charles Darwin, especially "The Variation of Animals
and Plants Under Domestication". At the age of 21 Burbank purchases a 17-acre
(7-hectare) tract near Lunenberg, Mass., and begins a 55-year plant-breeding
career. After about a year he had developed the Burbank potato, which was
introduced to Ireland to help combat the blight epidemics. By selling the
rights to this potato he made $150, which he used to travel to California,
where three of his brothers had already settled. In Santa Rosa, Burbank
establishes a nursery garden, greenhouse, and experimental farms that will
become famous throughout the earth.

Burbank believes in inheritance by acquired characteristics and lectures on
this at Stanford University in his later years even after the rediscovery of
Gregor Mendel's principles of heredity in 1901 which Burbank is aware of.
Lysenko, also a plant breeder will support this erroneous view 50 years later.


Burbank's work with plants convinces him that the key to good breeding is
selection and environment, like many others of this time, try to apply his
concepts to human society. The product of his thinking on this subject is first
published in 1907 as "The Training of the Human Plant". This book reveals
Burbank's firm belief in the then-discredited theory of the inheritance of
acquired characteristics, so unlike most eugenists of the period, Burbank
stresses education and a good environment generally as the best way to remake
human society. (Clearly environment influences reproduction, although there are
no acquired characteristics.)

In his life Burbank developes more than 800 new strains and varieties of
plants, including 113 varieties of plums and prunes, 20 of which are still
commercially important, especially in California and South Africa; 10
commercial varieties of berries; and more than 50 varieties of lilies, in
addition to publishing a number of books describing his methods.
Santa Rosa, California, USA  
79 YBN
[1921 AD]
4387)
(Cambridge University) Cambridge, England   
79 YBN
[1921 AD]
4518)
(The Hague) Netherlands  
79 YBN
[1921 AD]
4854)
(Columbia University) New York City, NY, USA  
79 YBN
[1921 AD]
4955)
(St Mary's Hospital) London, England  
78 YBN
[01/26/1922 AD]
5103) De Broglie's great-great-grandfather died on the guillotine during the
French Revolution. (So clearly De Broglie must be somewhat wealthy. Of course,
truth exists independently of wealth. I wonder what was the crime. It would be
interesting to see the thought-images and nano-flying dust cams - in the French
Revolution were the wealthy punished for their involvement in secret violence -
like 9/11, the Kennedy killings, etc or were many nonviolent and unfairly
murdered?)
During WW I De Broglie is stationed in the Eiffel Tower as a radio engineer.
In 1929 De
Broglie wins the Nobel Prize in physics.
(brother Maurice's lab) Paris, France (verify)  
78 YBN
[02/06/1922 AD]
4323)
Luxor, Egpyt  
78 YBN
[03/01/1922 AD]
5163) In 1966 Mulliken wins the Nobel Prize in chemistry "for his fundamental
work concerning chemical bonds and the electronic structure of molecules by the
molecular orbital method".
(University of Chicago) Chicago, Illinois, USA  
78 YBN
[03/03/1922 AD]
4324)
Menton, France  
78 YBN
[04/28/1922 AD]
4325)
Mandeville, Jamaica  
78 YBN
[05/19/1922 AD]
3612)
Washington, D.C., USA.   
78 YBN
[05/27/1922 AD]
5197)
(Geophysical Institute) Bergen, Norway  
78 YBN
[05/??/1922 AD]
4104)
(University of Groningen) Groningen, Netherlands  
78 YBN
[08/01/1922 AD]
4820) In 1944 Erlanger and Gasser share the Nobel prize in medicine and
physiology.
(Notice that the Nobel committee is drawing attention to scientific analysis of
the nervous system - a massive, but secret enterprise - and then near the end
of WW2 when clearly the Nazi's were certain to lose.)

(Erlanger's only son dies before he does - how?)
(Washington University) Saint Louis, Missouri, USA  
78 YBN
[11/??/1922 AD]
3883)
New York City, NY (presumably)  
78 YBN
[12/09/1922 AD]
5111)
(Washington University) Saint Louis, Missouri, USA  
78 YBN
[12/13/1922 AD]
5108) Compton is the son of Presbyterian minister who was Dean of Wooster
College. (State how the Presbyterian followers of Jesus differ from other
followers of Jesus.)
In 1927 Compton shares a Nobel Prize in physics with
Charles Wilson.
Compton is one of the top scientists in the Manhattan Project that
develops the atomic bomb. Asimov states that Compton remained on the best of
terms with the (US) military.
Compton directs the research on methods of
producing plutonium.
Compton approves the use of the atomic bomb over Japan.
Like Millikan,
Compton is an outspokenly religious scientist.
(Washington University) Saint Louis, Missouri, USA  
78 YBN
[1922 AD]
3978)
School of Mines, Saint-Etienne, France (presumably)  
78 YBN
[1922 AD]
4362)
(Johns Hopkins University) Baltimore, Maryland, USA  
78 YBN
[1922 AD]
4444)
( University of Berlin) Berlin, Germany  
78 YBN
[1922 AD]
4467)
(Victoria Observatory) Victoria, British Colombia  
78 YBN
[1922 AD]
4490)
(Johns Hopkins University), Baltimore, Maryland, USA  
78 YBN
[1922 AD]
4726)
(Mount Wilson Observatory) Pasadena, California, USA  
78 YBN
[1922 AD]
4875)
(Dayton Engineering Laboratories Co) Dayton, Ohio, USA  
78 YBN
[1922 AD]
4940)
Ur (modern Iraq)  
78 YBN
[1922 AD]
4951)
  
78 YBN
[1922 AD]
5047) Friedmann dies of typhoid fever while still in his thirties.
(Academy of Sciences) Petrograd, Russia  
77 YBN
[01/02/1923 AD]
5003)
(University of Copenhagen) Copenhagen, Denmark  
77 YBN
[02/27/1923 AD]
4996)
(University of Zurich), Zurich, Switzerland  
77 YBN
[05/04/1923 AD]
5004)
(University of Copenhagen) Copenhagen, Denmark  
77 YBN
[06/14/1923 AD]
3613)
Washington, D.C., USA.   
77 YBN
[09/06/1923 AD]
4842)
(BASF) Ludwigshafen-on-the-Rhine, Germany  
77 YBN
[09/10/1923 AD]
5104) De Broglie's great-great-grandfather died on the guillotine during the
French Revolution. (So clearly De Broglie must be somewhat wealthy. Of course,
truth exists independently of wealth. I wonder what was the crime. It would be
interesting to see the thought-images and nano-flying dust cams - were the
wealthy punished for their involvement in secret violence - like 9/11, the
Kennedy killings, etc?)
During WW I De Broglie is stationed in the Eiffel Tower as a
radio engineer.
In 1929 De Broglie wins the Nobel Prize in physics.
(brother Maurice's lab) Paris, France (verify)  
77 YBN
[12/29/1923 AD]
5058) Electronic camera and image display. This electric camera is a "scanning"
electric camera. Later the CCD (charge-coupled device) will allow a
two-dimensional area (frame) of light to be captured very quickly.[]

(and radio frequency light particle (wireless) sending and receiving of images
(television)?)

Vladimir Kosma Zworykin (ZWoURiKiN) (CE 1889-1982) Russian-US electrical
engineer, invents the first publicly known electronic scanning camera, the
"iconoscope".

Zworykin's device focuses an image on a screen made up of many small tiny
potassium hydride droplets which act as photoelectric cells, each insulated,
which develops a charge that depends on the intensity of the light on each drop
of metal. An electron beam moved with an electromagnetic field is scans in
parallel lines over the screen, discharging the photoelectric cells and
producing an electrical signal. Then to draw the scanned image to another
screen, Zworykin uses the cathode-ray tube invented in 1897 by Karl Ferdinand
Braun. The tube (which Zworykin calls a ‘kinescope’) has an electron beam
focused by electromagnetic fields to illuminate a small spot on a fluorescent
screen. The beam is then deflected by the fields in parallel lines across the
screen, and the intensity of the beam varies according to the intensity of the
signal. In this way it was possible to reconstruct the electrical signals into
an image. In 1923 an early version of this system is made and Zworykin manages
to transmit a simple picture (a cross). By 1929 Zworykin is able to demonstrate
a better version suitable for practical use.

In 1848, Lord Kelvin had published "Theory of Electric Images", although a
mathematical paper, this implies that capture and storage of images
electronically was clearly in full progress by 1848. In this sense Kelvin
should probably be credited. There is no much question in my mind that clearly
by 1909 as indicated by Jean Perin, there are already microscopic flying
dust-sized neuron readers and writer, camera, microphone, light particle
transmitting and receiving devices. This may imply that the first electronic
scanning electronic camera was secretly invented in 1823 since the 100 year
anniversary may have been the agreement point between two sides, or perhaps
even a 200 year point.

In his December 29,1923 patent entitled "Television System", Zworykin writes:
"...
My invention relates, in general, to television systems.

One of the objects of my invention is to provide a system for enabling a person
to see distant moving objects or views by radio.

Another object of my invention is to eliminate synchronizing devices
heretofore employed in television systems.

Still another object of my invention is to, provide a system for
broadcasting, from a central point, moving pictures, scenes from plays, or
similar entertainments.

The above and other objects of my invention will be explained more fully
hereinafter with reference to the accompanying drawings forming a part of this
specification.

Referring now to the drawings,

Figure 1 is a diagram of a station for broadcasting motion pictures or other
visual indications, and may be considered the television transmitter.

Fig. 2 is a diagram of a receiving station for receiving the scenes
broadcasted from the transmitting station.

Fig. 3 is a fragmentary view of an alternative arrangement for the
transmitting station.

Fig. 4 shows an arrangement whereby the control of the transmitting and the
receiving stations may be exercised from a central station; and
Fig. 5 shows the
circuits of the transmitting station when a central station is used.
Both of
these stations are shown by means of concentional circuit and apparatus
diagrams in sufficient detail to enable the invention to be readily explained
and understoof.
Any visual indications may be broadcasted by the transmitting set 1
consisting of apparatus and circuits and be received by the receiving set 2
consisting of apparatus and circuits.
The apparatus of the transmitting set 1 comprises
an antenna system 3 which is so tuned that it may oscillate at two separate and
distinct frequencies. The oscillating circuit including the antenna 3 is
connected on one side by means of a transformer 4 to the plate circuit of an
amplifier triode 5. The grid of the amplifier 5 is connected threough a
transformer 6 to the plate circuits of modulator triodes 7 and 9. An oscillator
triode 9 is connected through a transformer 10 to the grid circuit of the
modulator triodes 8 and 8. The above arrangement comprises what is known as an
ordinary "push-and-pull" transmitting arrangement.
...

The light from the image placed before the lens 37 is so varied that, upon the
focusing of this light upon the photoelectric globules 36 of the composite
plate 32, electron emission of varying intensity by these particles takes place
in accordance with the light from the object placed before the lens 37. This
electron emission may be considered a species of conduction between the
photoelectric globules 36 and the grid 39. This phenomena is intensified by the
argon vapor that fills the container 33 as a result of the ionization of the
vapor.

In view of the fact that the aluminum oxide plate 35 is an insulator, there is
no connection existing between the grid 39 and the aluminum plate 34, even
though the photoelectric globules emit electrons. When the cathode beam strikes
a particular point upon the aluminum foil, it is of sufficient intensity to
penetrate it, as well as the aluminum oxide. The action of the cathode ray on
the aluminum oxide in its path, particularly In the presence of the gas, is to
produce a conductive connection between the aluminum plate 34 and the
particular globule or globules of potassium hydride in the path of the cathode
ray. The electrons emitted by these globules are therefore subjected to the
field produced by the battery 42 acting across the conductive part of the
aluminum oxide. The amount of the emission will depend upon the degree of
illumination of these globules. The current flowing in the circuit is dependent
upon the electron emission from the globule or globules covered by the cathode
beam. This current is amplified by means of the amplifier triode 12. The
current from the grid 39 to the grid of the tube 12 is so small that no grid
leak is necessary fur the tube 12 although one may be supplied if desired. The
output of 53 the amplifier 12 now pauses the modulator triodes 7 and 8 to
transmit, through the transformer 6, the high-frequency oscillations, generated
by the oscillator triode 9, modulated in accordance with the current in the
amplifier triode 12 which, In turn, is governed by the intensity of the light
focused upon the particular spot at which the cathode ray is located. The
intensity of this electron stream is of course, governed by the intensity of
the light from the object.
...
When the cathode beam in the cathode-ray tube of the transmitter is in a
certain particular position, the oscillatory current generated by the
oscillator 9 is modulated In accordance with the intensity of the light falling
upon that particular point. This modulated current is radiated by the antenna 3
and received by the antenna 51 at the receiving station. At this particular
point, the cathode beam in the cathode-ray tube 55 will be in the same relative
position as the cathode beam at the sending station. By the action of the grid
14, the intensity of the cathode ray reaching the fluorescent screen at this
particular point is varied in accordance with the light from the image at the
transmitting station.

Thus, for every particular point on the image, the carrier current radiated by
the antenna 3 is modulated whereby the potential on the grid 54 of the
receiving cathode-ray tube 55 is varied, as is, also, the intensity of
fluorescence of the particular point upon the fluorescent screen 60.

As the whole area of the composite plate 32 at the transmitting station and the
fluorescent screen 60 at the receiving station is covered by the cathode beams
in & of a second, the image of the object will be displayed on the screen 60
during jfe of a second. However,.as the frequency of the oscillation of the
generator 23 is 18 cycles per second, the picture will be transmitted twice and
will remain on the screen 60 during A of a 28 second. Thus, due to the
persistency of vision phenomena, any movement of the object before the lens 37
will be properly transmitted and recorded upon the fiuorescent screen 60 and
will appear thereupon as a moving image.

Of course, in place of transmitting the image of actual objects, it is entirely
possible to send moving pictures, as all that is necessary is to pass the
pictures before the lens §7 at the required rate and a replica of them will
appear on the screen 60. In order to place these pictures before a large
audience, it is, of course, possible to intensify and focus them upon an
ordinary screen by means of any well known optical system.

The operation of the system when the apparatus used in Pig. 3 is employed at
the transmitting station is very similar to that already described. The cathode
beam covers the area of the fluorescent screen 75 under the influence of the
magnetic and electrostatic fields. When the beam is at one particular point,
the light from that spot will traverse the film 78, lens 77 and photoelectric
cell 76.

The variation of current of the photoelectric cell 76 causes the carrier
frequency to be modu- ®° lated in accordance with the current flow which is
directly proportional to the intensity of light from the fiuorescent spot that
reaches the photoelectric cell. As this condition occurs for each „
particular point on the picture, the whole picture will be transmitted in the
manner described. The method of reproduction is the same as has been explained
in conjunction with Figs. 1 and 2.
...
It will be seen that this arrangement permits a number of transmitting
stations to transmit pictures or visual indications with only one central
station for generating the synchronizing frequency.

It is, of course, apparent, that any number of receiving stations may receive
the image broadcasted in a manner similar to that described.

My Invention is not limited to the particular arrangement of apparatus
illustrated but may be variously modified without departing from the spirit and
scope thereof, as set forth in the appended claims.
...".

This is the first wireless television system, or wireless image and sound
communication system. Invisible light particles with radio frequency send
images and sounds to receivers which redraw the images on a screen and replay
the sounds through a speaker. Television will surpass sound-only radio, movies,
books, magazines and newspapers, and physical pleasure, as the most popular
form of entertainment for the public. But this will be surpassed when neuron
reading and writing goes public, and humans send and receive images and sounds
directly to and from their brain using similar cameras, transmitters and
receivers. There was and is, of course, a very secret history and scientific
development of camera, microphones, and neuron reading and writing particle
beam transmitting and receiving devices. One focus of this secret development
is on miniturization of these devices, and another focus is on the movement of
these devices. Clearly the devices are extremely small, and move by flying and
hovering in space. Currently neuron reading and writing, that is receiving
video square windows directly to brain to appear before the human eyes is very
widespread, with clearly millions of people paying to receive videos. In
addition, the subject of the videos has changed from scripted theater and stage
productions to watching other people, in particular good-looking, and popular
people. Currently watching people in their homes, for most people, without
their knowledge that they, and the images and sounds in their mind, are being
seen and heard by many people, and that even the images in their thoughts can
be seen, and not only seen, but written and drawn on too. It seems clear that
neuron reading and writing, and the microscopic devices that are used to see,
hear, transmit and receive images and sounds will eventually go public, but it
is not clear when this will happen.]

In 1940 Zworykin will invite James Hillier to join his research group at RCA,
and it is at RCA that Hillier will construct the electron microscope.


(Is this the first radio transmitting and receiving of an image, and or 30
images a second moving images?)

(Interesting the analogy of television to telephone, in particular in light of
the concept of sending and receiving images to and from brains using particle
beams. The view is that the television camera and screen is similar to a
telephone but for pictures in addition to sounds.)

(A major question is when is image storage electronic? image storage initially
started on glass plates, and then on paper, then on plastic film, then in
semiconductor metal.)

(Kind of interesting that the the electronic circuit is from the dots, through
the gas, to an aluminum plate.)

(Davisson at AT&T Bell Labs also patents a similar electron beam device, but
apparently AT&T has so far, not gone public with their massive microscopic
network.)

(It seems that possibly, given AT&T's massive network, that Westinghouse
somehow must have been in conflict with, or somehow been challenging AT&T in
going public with the electronic scanning camera and wireless image sending and
receiving. Clearly Westinghouse won, and the public won whatever conflict must
have occured.)

(From here, a major question is: how is this device miniturized? For this,
electronic integrated circuits will be able to quickly scan each
light-sensitive dot, and emit this image serially to a receiver.)
(for Westinghouse Electric Corporation, Pittsberg, PA, USA) Haddenfield, New
Jersey, USA  
77 YBN
[1923 AD]
4216)
(Eastman Kodak Company) NJ, USA  
77 YBN
[1923 AD]
4775) Euler-Chelpin is distantly related to the famous mathematician Euler.
In 1929
Euler-Chelpin shares the 1929 Nobel Prize for Chemistry with Sir Arthur Harden
for work on the role of enzymes in the fermentation of sugar.
Although Euler-Chelpin
became a Swedish citizen in 1902 he served Germany in both world wars.
(University of Stockholm) Stockholm, Sweden  
77 YBN
[1923 AD]
4858) Gilbert Newton Lewis (CE 1875-1946), US chemist with Merle Randall
publishes “Thermodynamics and the Free Energy of Chemical Substances”,
which more than any other book, clarifies and expands Gibbs' chemical
thermodynamics for students. In this book Lewis replaces the concept of
“concentration” with “activity” which is more useful in working out
rates of reactions and questions of equilibria than the older
“concentration”. This modifies and makes more accurate Guldberg and
Waage's law of mass action. (All of this needs more specific info, I think
thermodynamics may be inaccurate and too abstract to be of use, but clearly
accurately describing rates of reactions is a real and useful thing.).

(University of California at Berkeley) Berkeley, California, USA  
77 YBN
[1923 AD]
4927) Brønsted's firm opposition to Nazism during World War II won him
election to the Danish Parliament in 1947, but illness prevents him from taking
his seat.
(University of Copenhagen) Copenhagen, Denmark  
77 YBN
[1923 AD]
4967)
(Clark University) Worcester, Massachusetts, USA  
77 YBN
[1923 AD]
4987) (Kaiser Wilhelm Institute for Biology) Berlin, Germany  
77 YBN
[1923 AD]
4989)
(University of California at Berkeley) Berkeley, California, USA  
77 YBN
[1923 AD]
5000) Svedberg wins the 1926 Nobel Prize in chemistry.
(University of Uppsala) Upsala, Sweden  
77 YBN
[1923 AD]
5042) (University of Kristiania) Kristiania (now Oslo), Sweden (presumably)  
77 YBN
[1923 AD]
5078) (Sir) Harold Jeffreys (CE 1891-1989), English astronomer establishes that
the large gas giant planets Jupiter, Saturn, Uranus, and Neptune have cold
surface temperatures and are not still warm from interior heat, and devises
early models of their planetary structure.

(Works with Jeans on the tidal hypothesis for the origin of the earth, which
increases the age of the earth to billions from the estimate of tens of
millions of Helmholtz and Kelvin.)

(Determine if Jeffreys means surface of outer atmosphere or liquid or solid
surface temperature. A Jupiter probe measured high temperatures descending into
the clouds of Jupiter.)

(I think there must be something similar to a terrestrial planet inside each of
the gas giant planets.)

(Q: Look at their density and estimate how much is solid, liquid and gas. Are
the insides of these terrestrial planets molten red hot liquid metal? D=m/v If
the mass of the Jovian planet is used with the density of earth to determine
the volume of this density, and then from that volume to simply determine
radius from V=4/3pi r^3, I performed this simple calculation and Jupiter would
have a terrestrial 6 times the radius of earth.
mass of jupiter 318x that of earth.
1.8986x10^27kg volume=1.43x10^15 km^3 1,321 earths
radius of earth 6,371km,
vol=1.08321x10^12 km^3
D=m/v V=4/3pir^3
D(earth)=5.5e12 kg/km^3
D=m/v
5.5e12 kg/km^3=1.8986x10^27kg/v
v=3.452 x 10^14 km^3
V=4/3pi r^3
3.452 x 10^14 km^3=4.19
r^3
r=43,517 km
radius of earth 6,371km
Jupiter would be 6.83 times the radius of earth. 7x
the radius of earth - and a large terretrial inside is probably true for the
other Jovianic-terrestrial planets.

Vjupiter= 1.43x10^15 km^3
1.43x10^15 km^3=4.19 r^3
RadiusJupiter=71,492 (69,883)

This would put the surface 43,517/69,883 = 38 percent below the clouds,
26,366km below the clouds.
)

( Maybe they are cooled and only emit a small amount of infrared if any. The
terrestrial nature of the moons of the gas giant planets I think is evidence
that some dense matter (metals) formed local groupings in the outer star
system. Either the moons formed around Jupiter or were captured. I think the
ring of Jupiter is evidence that matter does compress into moons around
planets. The constant gravitational attraction of the large planet might argue
for the moons being formed in isolation and then captured. It would be
interesting to think we are looking at what used to be planets. Perhaps the
density of each moon indicates its origin. Q: Does the density linearly
increase as the moon is closer to the planet or are they more or less random?
Can it be argued that a denser moon was probably formed closer to the sun than
a less dense moon? )
(Cambridge University) Cambridge, England  
76 YBN
[01/29/1924 AD]
5204)
(Institute of Physical and Chemical Research) Tokyo, Japan  
76 YBN
[02/12/1924 AD]
6036)
(Aeolian Concert Hall) New York City, New York, USA  
76 YBN
[06/07/1924 AD]
5075) (University of Giessen) Giessen, Germany (presumably)  
76 YBN
[06/07/1924 AD]
5076)
(University of Giessen) Giessen, Germany (presumably)  
76 YBN
[06/13/1924 AD]
4975) Like Schrödinger, Born leaves German as soon as Hitler comes to power,
moving to Cambridge in 1933.

In 1954 Born wins the Nobel Prize in physics for work on quantum mechanics with
Bothe.
(University of Göttingen) Göttingen, Germany  
76 YBN
[07/02/1924 AD]
5139)
(University of Dacca) East Bengal, India  
76 YBN
[08/??/1924 AD]
4753)
(Cambridge University) Cambridge, England   
76 YBN
[08/??/1924 AD]
4896)
Chicago, Illinois, USA  
76 YBN
[12/17/1924 AD]
5199) Asimov states that Blackett's strong support of Watson-Watt helps to
develop radar which saves Britain in World War II. (However, it seems clear
that light particle technology has been developed to so extreme an advanced
state, that the continued secret of, for example, neuron reading and writing,
in my view is simply extremely evil, without much question in my mind - to
exclude millions of humans from even knowing, seeing what it looks like, etc...
just absolutely shocking on the level of auschwitz, that average people can be
so inhuman.)

The Nobel Prize in Physics 1948 is awarded to Patrick M.S. Blackett "for his
development of the Wilson cloud chamber method, and his discoveries therewith
in the fields of nuclear physics and cosmic radiation".
(University of Cambridge) Cambridge, England  
76 YBN
[1924 AD]
3614)
Cleveland, OH, (to NYC, NY), USA  
76 YBN
[1924 AD]
4525)
(Mount Wilson Observatory) Pasadena, California, USA  
76 YBN
[1924 AD]
4696) For this work, in 1935 Spemann wins the Nobel prize in medicine and
physiology.
(University of Freiburg) Breisgau, Germany  
76 YBN
[1924 AD]
4981)
(Cambridge University) Cambridge, England   
76 YBN
[1924 AD]
5010) In 1934 Minot shares the Nobel Prize in medicine and physiology with
Whipple and Murphy.
(Collis P. Huntington Memorial Hospital, Harvard University) Cambridge,
Massachusetts, USA (presumably)  
76 YBN
[1924 AD]
5027)
(University of Cambridge) Cambridge, England  
76 YBN
[1924 AD]
5118) A student of Dart's, Josephine Salmons, in the summer of 1924, had
brought Dart a fossil collected from a limestone mine at Taung, Bechuanaland.
Dart names the species the skull belongs to, "Australopithecus africanus",
meaning southern African ape, and declares this species to be intermediate
between apes and humans.

Dart and Broom then begin a systematic search and uncover a number of other
fossils to confirm the existence of the Australopithecus.

The Leakys, Donald Johannsen and others will show that Australopithicines
walked on two legs.

Most people accept that a single australopithecus is a direct ancestor of all
sapiens. (Verify)
(University of Witwatersrand) Johannesburg, South Africa  
76 YBN
[1924 AD]
6039) Giacomo Puccini (CE 1858-1924), Italian composer, composes the opera
"Turandot" with the famous "Nessum Dorma".

Viareggio, Italy (presumably)  
76 YBN
[1924 AD]
6064) Al Jolson records the famous song "California, Here I Come", a song
written for the 1921 Broadway musical "Bombo", starring Al Jolson. The song is
written by Buddy DeSylva and Joseph Meyer, with Jolson often listed as a
co-author.

(Brunswick) Dubuque, Iowa, USA (possibly)  
75 YBN
[01/01/1925 AD]
5060) Spiral nebulae proven to be other galaxies containing stars and to be
very far away.

US astronomer, Edwin Hubble (CE 1889-1953) shows that M31 (Andromeda) contains
stars, and uses the period of a variable star in M31 to show that it is very
far away (930,000 light-years).

Hubble using the largest telescope at this time, a 100-inch telescope on Mount
Wilson is the first to identify individual stars in the Andromeda “nebula”
(later known to be a galaxy), and finding variable stars, using the
period-luminosity law of Shapley and Leavitt, Hubble calculates that Andromeda
is 800,000 light years away, eight times the distance of the farthest
identifiable star in our own galaxy, and so there is no question that the
Andromeda nebula is located outside of our own galaxy. Hubble calculates other
spiral nebulae to be even farther, billions of light years away, and so in this
way Hubble starts to study of the universe beyond our own galaxy. Hubble calls
these nebulae outside of our galaxy “extragalactic nebulae”, and Shapley
will later suggest that they be called galaxies, recognizing that our own
galaxy is only one of many.

Apparently Hubble's original 1925 paper has not survived, but a summary appears
in the "Publications of the Astronomical Society of the Pacific". This paper
was read for Hubble on January 1, 1925 at the Annual Astronomical Society
meeting.
Hubble writes in "Cepheids in Spiral Nebulae":
"Messier 31 and 33, the only spirals that
can be seen with the naked eye, have recently been made the subject of detailed
investigations with the 100-inch and 60-inch reflectors of the Mount Wilson
Observatory. Novae are a common phenomenon in M31 and Duncan has reported three
variables within the area covered by M33. With these exceptions there seems to
have been no definite evidence of actual stars involved in spirals. Under good
observing conditions, however, the outer regions of both spirals are resolved
into dense swarms of images in no way differing from those of ordinary stars. A
survey of the plates made with the blink-comparator has revealed many variable
among the stars, a large proportion of which show the characteristic
light-curve of the Cepheids.
Up to the present time some 47 variables, including
Duncan's three, and one true nova have been found in M33. For M31, the numbers
are 36 variables and 46 novae, including the 22 novae previously discovered by
Mount Wilson observers. Periods and photographic magnitudes have been
determined for 22 Cepheids in M33 and 12 in M31. Others of the variables are
probably Cepheids, judging from their sharp rise and slow decline, but some are
definitely not of this type. One in particular, Duncan's No. 2 in M33, has been
brightening fairly steadily with only minor fluctuations since about 1906. It
has now reached the 15th magnitude and has a spectrum of the bright line B
type.
...
Shapley's period-luminosity curve for Cepheids, as given in his study of
globular clusters, is constructed on a basis of visual magnitudes. It can be
reduced to photgraphic magnitudes by means of his relation between period and
colour-index, given in the same paper, and the result represents his original
data. The slope is of the order of that for spirals, but is not precisely the
same. In comparing the two, greater weight must be given to the brighter
portion of the curve for the spirals, because of the greater reliability of the
magnitude determinations. When this is done, the resulting values of M-m are
-21.8 and -21.9 for M31 and M33 respectively. These must be corrected by half
the average ranges of the Cepheids in the two spirals, and the final values are
then on the order of -22.3 for both nebulae. The corresponding distance is
about 285,000 parsecs* {ULSF: original footnote: *Equal to 930,000
light-years}. The greatest uncertainty is probably in the zero-point of
Shapley's curve.
The results rest on three major assumptions: (1) The variables are
actually connected with the spirals; (2) There is no serious amount of
absorption due to amorphous nebulosity in the spirals; (3) The nature of
Cepheid variation is uniform throughout the observable portion of the universe.
As for the first, besides the weighty arguments based on analogy and
probability, it may be mentioned that no Cepheids have been found on the
several plates of the neighboring selected areas Nos. 21 and 45, on a special
series of plates centred on BD+35°207, just midway between the two spirals,
nor in ten other fields well distributed in galactic latitude, for which six or
more long exposures are available. The second assumption is very strongly
supported by the small dispersion in the period-luminosity curve for M33. In
M31, in spite of the somewhat larger dispersion, there is no evidence of an
absorption-effect to be measured in magnitudes.
These two spirals are not unique.
Variables have also been found in M81, M101, and N.G.C. 2403, although as yet
sufficient plates have not been accumulated to determine the nature of their
variation.".

(Hubble's writing sounds kind of pro-sex with "naked" and "covered" in the
first paragraph.)
(It must have been confusing until Shapley made the name change from
extra-galactic nebulae to galaxy, because there are nebulae like the gas cloud
in Orion that are not "extra-galactic nebulae".)

(Show the actual calculations of distance if possible. How does the
magnification of the telescope, and size of image enter into the equations?)
(Mount Wilson) Mount Wilson, California, USA  
75 YBN
[01/16/1925 AD]
5233) The 1945 Nobel Prize in Physics is awarded to Wolfgang Pauli "for the
discovery of the Exclusion Principle, also called the Pauli Principle".
(Institute fur Theoretische Physik) Hamburg, Germany  
75 YBN
[02/21/1925 AD]
5105)
(King's College) London, England  
75 YBN
[03/19/1925 AD]
6065)
New York City, New York, USA (probably)  
75 YBN
[04/04/1925 AD]
4754)
(Cambridge University) Cambridge, England   
75 YBN
[05/18/1925 AD]
4882)
(Mount Wilson Observatory) Pasadena, California, USA  
75 YBN
[06/06/1925 AD]
5024)
(University of Uppsala) Uppsala, Sweden  
75 YBN
[07/13/1925 AD]
5059)
(Westinghouse Electric Corporation)   
75 YBN
[09/05/1925 AD]
5112)
(University of Chicago) Chicago, Illinois, USA  
75 YBN
[10/22/1925 AD]
5292) Dr. Julius Edgar Lilienfeld was a German scientist who worked at the
University of Leipzig before immigrating to the U.S. in the 1920's (due to the
increasing persecution of Jews in Germany). Lilienfeld operated the first large
scale hydrogen liquification facility in Germany.

It may be that Lilienfeld was aware of neuron reading and writing in Germany,
but then when excluded, or persecuted because of being jewish, he went to the
USA, and in the USA, perhaps he was also excluded from neuron reading and
writing, as a German immigrant, and so felt no fear or reason not to patent and
go public with some technology he had learned about as an insider. I can only
guess, it would be interesting to see the actual story as told by the flying
dust cameras and neuron thought image and sound readers.
Brooklyn, New York City, New York, USA  
75 YBN
[11/16/1925 AD]
5282) As a youth after WW I, Heisenberg engaged in street fights with
Communists in Munich. (Here, Heisenberg clearly shows no interest in stopping
violence, or support for laws against violence.)

In 1932, the Nobel Prize in Physics is awarded to Werner Heisenberg "for the
creation of quantum mechanics, the application of which has, inter alia, led to
the discovery of the allotropic forms of hydrogen". ("inter alia" is Latin for
"among other things") The theory of a quantum was originated by Max Planck.
Quantum atomic theory which views atomic motions as controlled by integral
quanta of energy and momenta was formulated by Niels Bohr in 1913.

In his life Heisenberg publishes over 500 independent works, of which some 100
may be considered original scientific contributions. The others concern
philosophical, cultural political, and popular subjects.

(I think I need to look more closely at exactly what Heisenberg was claiming,
but to me I think we can model the universe using integers although it is
almost useless for practical purposes. I think even if humans forever have have
uncertainty in knowing where and what velocity, matter exists in certain exact
locations with exact velocities.)

Asimov states that Heisenberg is one of the few top notch scientists who find
themselves able to work under the Nazis. Heisenberg accepts high positions
under the Nazis, although refusing them might mean being murdered. However, in
1937 Heisenberg receives a call to join the University of Munich. Thereupon the
official SS journal publishes an article signed by Stark that calls Heisenberg
a "white Jew" and the "Ossietzky of physics".

During WW2 Heisenberg is in charge of German research on the atomic bomb. The
war ends before they are successful.

After WW 2 Heisenberg moves to West Germany.
(University of Göttingen) Göttingen, Germany  
75 YBN
[11/20/1925 AD]
5254)
(Instituut voor Theoretische Natuurkunde) Leyden, Netherlands  
75 YBN
[11/??/1925 AD]
4802)
New York City, NY, USA  
75 YBN
[11/??/1925 AD]
4803)
(University of Milan)Milan, Italy  
75 YBN
[12/24/1925 AD]
4512)
(California Institute of Technology) Pasadena, California, USA  
75 YBN
[1925 AD]
4299)
(Johns Hopkins University) Baltimore, Maryland, USA  
75 YBN
[1925 AD]
4990)
Central Asia  
75 YBN
[1925 AD]
5017) In 1947 Robinson wins the Nobel Prize in chemistry.
From 1945-1950 Robinson is the
President of the Royal Society.
(University of Oxford) Oxford, England  
75 YBN
[1925 AD]
5065) Vannevar Bush (CE 1890-1974), US electrical engineer, and colleagues at
MIT build a machine that can solve differential equations. (Kelvin had worked
out the theory for such a machine 50 years earlier and Babbage had tried to
build a computer 100 years before). According to Asimov, this is the first
analog computer. The first electronic computer (Eniac) will be built in 1946
(using vacuum tubes as electric switches). Computers will greatly speed
mathematical calculation and universe modeling. For example, the calculations
to a work out (an average, or year's worth of) the orbit of planet Mars, which
took Kepler 4 years to calculate, can be done in 1964 in 8 seconds, and pi can
be calculated to 10,000 places in a few hours.

Bush designs a series of mechanical calculators, termed "differential
analyzers", that are initially useful for simulating the operations of electric
power grids.

(Show and explain how these machines work. Do they use any electricity? If not
using electricity, I don't think they should be called "analog" computers.)

(Clearly electronic computers go back into the 1800s, but how far back, like
neuron reading and writing, is unknown. There is something a little absurd in
the statement: "Bush designed a series of mechanical calculators, termed
differential analyzers, that were initially useful for simulating the
operations of electric power grids," - because they have electricity but are
publicly using mechanical calculators? In particular given 200 years of neuron
reading and writing.)
While still at MIT, he cofounded a successful radio tube company:
Raytheon.
(Massachusetts Institute of Technology) Cambridge, Massachusetts, USA  
74 YBN
[01/26/1926 AD]
6264)
(Royal Institution) London, England  
74 YBN
[02/07/1926 AD]
5272) In 1922 Fermi gets a doctorate degree a few months before Benito
Mussolini seizes power in Italy.
In 1938 the Nobel Prize in Physics is awarded to
Enrico Fermi "for his demonstrations of the existence of new radioactive
elements produced by neutron irradiation, and for his related discovery of
nuclear reactions brought about by slow neutrons". Fermi is anti-fascist and at
the Nobel Prize ceremony does not wear the Fascist uniform or give the Fascist
salute, and the controlled Italian press castigates Fermi for these omissions.
Fermi's wife is Jewish and as Hitler's influence becomes more pronounced in
Italy, anti-Jewish laws are passed. From Stockholm, where Fermi accepts the
prize, he and his family sail to the United States. Bohr had hinted to Fermi
that he would win the prize and so Fermi prepared for this trip to the USA.
Fermi becomes a professor of physics at Columbia University.

(In Fermi's Nobel Prize speech he concludes by giving thanks to other people
who had not already been mentioned, which may be a play on the German word for
people which is "menchun", but maybe I am reading into this too much. Was
Fermi's speech in English?)

Fermi approves the use of the fission bomb over Japan.

Fermi opposes the development of the more deadly H-bomb (fusion bomb).

Fermi dies of a stomach cancer never seeing uranium fission used for
non-explosive uses in electric reactors by Rickover and Hinton.

Element 100 discovered the year after Fermi's death is named in his honor.

(Dying so young at age 53, perhaps somebody slipped him some radioactive atoms
in his food, or he had some on his body which entered his mouth.)

(Ernest Lawrence and Fermi, both born around the same time, had unusually early
deaths - which may be an indication of the rise of first strike violent people
with particle beam supremecy - clearly the violent had control in the USA
through much of the 1950s, certainly in 1963 and as the controlled demolition
of 9/11 shows to the present day.)

(Fermi represents the first international scientist making internationally
recognized scientific contributions from Italy since, perhaps, Volta around
1800. What explains this scientific silence?)
(University of Florence) Florence, Italy  
74 YBN
[02/??/1926 AD]
5875) In 1983, the Nobel Prize in Physiology or Medicine is awarded to Barbara
McClintock "for her discovery of mobile genetic elements".
(Cornell University) Ithaca, New York, USA  
74 YBN
[03/06/1926 AD]
5165)
(University of Göttingen) Göttingen, Germany  
74 YBN
[03/16/1926 AD]
4968)
(Aunt Effie's Farm) Auburn, Massachusetts, USA  
74 YBN
[03/18/1926 AD]
5063) In 1932 Adrian wins the Nobel Prize for physiology and medicine shared
with Sherrington.
In 1950 Adrian is President of Royal Society.
(Clearly this relates to neuron
reading and writing. Perhaps this is viewed as helping the public to create
neuron reading devices.)
(University of Cambridge) Cambridge, England  
74 YBN
[06/02/1926 AD]
5038) In 1946 Sumner wins the Nobel Prize in chemistry shared with Northrup and
Stanley.
(Cornell University) Ithaca, New York, USA  
74 YBN
[06/17/1926 AD]
5187) Iréne Joliot-Curie is the elder daughter of Pierre and Marie Curie.
Both
Iréne and Frédéric are raised without religion (and therefore probably
without seeing and hearing thought).
In 1925 Langevin recommends Frédéric to be an
assistant to Marie Curie.
Iréne marries Frédéric Joliot, and both are atheists.
(Interesting that Joliot shares his last name with Curie for himself too.)
In 1931
The Joliot-Curies work together on radioactivity.
In November 1935, Frédéric
Joliot and Irène Curie are awarded the Nobel Prize in chemistry for “their
synthesis of new radioactive elements.".
Marie Curie had died the year before.
In 1936, the
Joliot-Curies take a stand on the side of Republican Spain.
To slow neutrons for
uranium fission, Frederic Joliot, obtains about six tons of uranium oxide from
the Belgian Congo, and orders form Norway the only sizable stock of heavy water
then existing. The heavy water arrives safely in Paris even though World War II
has begun, but there is too little time before the invasion of France for it to
be used there. Joliot decides to remain in France but has Halban and Kowarski
carry the precious substance with them to England to continue the group’s
investigations.

Asimov relates the story of how the Joliot-Curies smuggle a quantity of heavy
water (the only sizable quantity on earth) necessary for atomic bomb research
out of France and the grasp of the Nazis. The Joliot-Curies also hide their
uranium, reclaim it after the war, and it is used to build France's first
nuclear reactor in 1948.

In May 1944, Irène and their children take refuge in Switzerland, and
Frédéric lives in Paris under the name of Jean-Pierre Gaumont. His laboratory
at the Collège de France, at which he organizes the production of explosives,
serves as an arsenal during the battle for the liberation of Paris. In
recognition, Frederic is designated a commander of the Legion of Honour with a
military title and is decorated with the Croix de Guerre.

In 1942 Frederic joins the then clandestine Communist party.

Frédéric Joliot-Curie is an admitted Communist, having joined the party
during World War II after the Nazis had executed Langevin's son-in-law, and
because of this is removed from his position as head of the French atomic
energy commission in 1950. (To me, although I do not support Communism, it's
similar to religion, it is simply a belief, a philosophy, it is well within the
realm of free thought, non-violent belief and disagreement. In my opinion,
nobody should be jailed for their philosophy so long as they are nonviolent.)

In April 1950, during the climax of the cold war and anticommunism, Prime
Minister Georges Bidault removes Frederic without explanation from his position
as high commissioner, and a few months later Irène is also deprived of her
position as commissioner in the Commissariat à l’Energie Atomique. (It seems
like there was somehow a resurgence of Nazism, or that form of radical
so-called conservatism, clearly an anti-science group.)

In 1951 Frédéric Joliot-Curie is awarded with the Stalin Peace Prize, and
remains an outspoken Communist for the rest of his life. (Stalin's vicious rule
should have been a clue to the faulty structure of Communism, certainly in
Russia; how it collapsed into a vicious long-lasting undemocratic monarchy. The
view I have which seems inevitable to me, is the future of full democracy
without religion, the representative system moving towards a full democracy and
religions falling to the past.)

In 1954 Iréne Joliot-Curie's application for membership in the American
Chemical Society is rejected because of the society's disapproval of her
politics (Asimov explains that Iréne Joliot-Curie was active in movements
considered Communist-influenced).
Iréne Joliot-Curie dies of leukemia like Marie after years of work
with radiation.

(Frédéric Joliot-Curie recognizes that in uranium fission neutrons are
produced, and begins work on an explosive chain reaction, but the war
interrupts his work. Asimov comments that Joliot-Curie may have built the first
atomic bomb had France not been invaded in 1940.)

(Somewhat unusual to have died so young and within 2 years of each other.)

(It seems a distinct possibility that the Curies may simply have been murdered
with particle beams, perhaps the thought-screen movies will answer that
question.)

(The Joliot-Curies are an interesting story of a futuristic couple; life
without religion and full of science is certainly the future, although
Communism is clearly a failure and full democracy seems the inevitable future.
It seems clear that many people viewed Communism as the opposite end of the
spectrum to the 2000 year powerful Christianity, so it's clear why people in
favor of science and opposed to the supernatural claims of religion would
gravitate to the Communist side, but clearly people can have atheism and full
democracy too, for example, many founders of the representative democracy in
the USA were vocal critics of religions.)

(It is very interesting to see that atoms can just be changed by beams of
particles. This must lead to systematic conversion, and there must be many
thousands of interesting transmutations secretly recorded. Perhaps some of
these are public but hidden. Systematically converting aluminum into oxygen and
hydrogen would be very useful in living independently on other planets where
aluminum is common. The other key idea is building up a proton from photons. It
is interesting that many of the products of neutron and alpha particle
bombardment remain radioactive. I guess perhaps many isotope atoms are unstable
and decay, but why wouldn't stable isotopes be made? Clearly some stable
isotopes must be made in these particle collisions. Why isn't the stable
isotope the rule instead of the exception? Find all the +n +p +a +b reactions
and examine as many as possible. Since radioactivity is mostly helium,
electrons and high frequency light particles, it seems clear that all of those
particles can be put to use, perhaps in heating water, or other materials.
Clearly, there must be some very fascinating science that has been kept secret
in the field of nuclear physics and engineering.)
(Radium Institute) Paris, France  
74 YBN
[06/26/1926 AD]
5131) In 1926 Noddack and Tacke marry and continue work on rhenium.
(University of Berlin) Berlin, Germany  
74 YBN
[08/02/1926 AD]
5267) The Nobel Prize in Physics 1939 is awarded to Ernest Lawrence "for the
invention and development of the cyclotron and for results obtained with it,
especially with regard to artificial radioactive elements".

During WW2 Lawrence is in Oak Ridge in one of the less successful attempts to
separate quantities of uranium-235 from ordinary uranium, to be included into
the “atomic pile” being built in Chicago by Fermi.
Like Compton, Lawrence
approves of the use of the atomic bomb against Japanese cities and has no
concern about the social aspects of the new weapon.
In 1957 Lawrence wins the
Fermi award, the highest scientific honor the US can offer.
In 1961 after Lawrence's
death, element 103 is named Lawrencium in his honor.

Lawrence was sent by President Dwight Eisenhower to Geneva in 1958 to
participate in nuclear test ban negotiations with the Soviet Union, but
Lawrence became sick and had to be rushed back to California, where he died.
(Sloan Laboratory, Yale University) New Haven, Connecticut, USA  
74 YBN
[12/14/1926 AD]
5146) In 1949 Giauque wins the Nobel Prize in chemistry "for his contributions
in the field of chemical thermodynamics, particularly concerning the behaviour
of substances at extremely low temperatures".
(University of California) Berkeley, California, USA  
74 YBN
[1926 AD]
4871)
(University of Leiden) Leiden, Netherlands  
74 YBN
[1926 AD]
4976) Like Schrödinger, Born leaves German as soon as Hitler comes to power,
moving to Cambridge in 1933.

In 1954 Born wins the Nobel Prize in physics for work on quantum mechanics with
Bothe.
(University of Göttingen) Göttingen, Germany  
74 YBN
[1926 AD]
5032) In 1928 Hitler comes to power and Schrödinger, although not Jewish,
moves to his native Austria. Schrödinger once interferes with storm troopers
bent on a pogrom, and is nearly killed.
In 1933 Schrödinger shares the Nobel
Prize in physics with Dirac.
In 1938 Austria is absorbed by Nazi Germany and
Schrödinger moves to England.
In 1956 Schrödinger returns to Vienna to live
out the rest of his life.
(University of Zürich) Zürich, Switzerland  
74 YBN
[1926 AD]
5072)
(University of Texas) Austin, Texas, USA  
74 YBN
[1926 AD]
5156)
(Uppsala University) Uppsala, Sweden  
74 YBN
[1926 AD]
6050) Louis Armstrong (CE 1901-1971), US trumpeter and one of the most
influential artists in jazz history, records "Heebie Jeebies". This is among
the first recordings with scat singing (improvised vocal jazz using
non-sensical words). So popular is the recording the group becomes the most
famous jazz band in the USA even though they as yet have not performed live to
any great degree. Young musicians across the country, black and white, are
turned on by Armstrong’s new type of jazz. (verify)

New York City, New York, USA (presumably)  
73 YBN
[03/03/1927 AD]
4957) Davisson joined the Bell Telephone Laboratory (then Western Electric) in
1917 and remains there until his retirement in 1946.
In 1937, the Nobel Prize in
Physics is awarded jointly to Clinton Joseph Davisson and George Paget Thomson
"for their experimental discovery of the diffraction of electrons by crystals".
(What role did Thomson play in the discovery?)
(Bell Telephone Laboratories) New York City, New York, USA  
73 YBN
[03/06/1927 AD]
4767) Bertrand Arthur William Russell (CE 1872-1970), 3d Earl English
mathematician and philosopher publishes "Why I am not a Christian", which
criticizes the religion formed around Jesus and the belief that any God
exists.

(Russell does not make the argument, which I think is the best in my mind, as
to why to reject the theory of Gods controlling nature, and that is that for
centuries there was only polytheism, long before monotheism, so if we reject
Poseidon ruling the seas, and Venus all aspects of love, why not reject the
theory of the existance of any God existing in the universe or controlling
nature?)

(National Secular Society, South London Branch, at Battersea Town Hall) London,
England  
73 YBN
[03/28/1927 AD]
5284)
(University of Copenhagen) Copenhagen, Denmark  
73 YBN
[04/14/1927 AD]
5236) Oort is Kapteyn's last student.
After the Nazis occupy the Netherlands, the Leiden
observatory is closed.
(Observatory) Leiden, Netherlands  
73 YBN
[04/19/1927 AD]
4946)
(General Electric Company) Schenectady, New York, USA  
73 YBN
[05/05/1927 AD]
5306) Wigner works with Fermi and Szilard in Chicago to develop a nuclear bomb.

Wigner helps to design the nuclear installations at Hanford, Washington. (State
what kind of installation.)
In 1960 Wigner wins the Atoms for Peace award.
The Nobel Prize in Physics
1963 is divided, one half awarded to Eugene Paul Wigner "for his contributions
to the theory of the atomic nucleus and the elementary particles, particularly
through the discovery and application of fundamental symmetry principles",the
other half jointly to Maria Goeppert-Mayer and J. Hans D. Jensen "for their
discoveries concerning nuclear shell structure".
(Institute fur Theoretische Physik) Berlin, Germany  
73 YBN
[05/21/1927 AD]
5291) In 1925 Lindbergh buys his own plane and becomes an airmail pilot.
In the 1930s
Lindbergh fights against the US entering WW II.
  
73 YBN
[05/24/1927 AD]
5100) George P. Thomson is the son of J. J. Thomson.
In 1927 Thomson shares the
Nobel prize in physics with Davisson.
(University of Aberdeen) Aberdeen, Scotland  
73 YBN
[06/16/1927 AD]
4907)
(Cavendish Laboratory, Cambridge University) Cambridge, England  
73 YBN
[06/30/1927 AD]
5232) In 1933 as a Jewish human, London leaves Germany.
(University of Zurich) Zurich, Switzerland  
73 YBN
[08/01/1927 AD]
5114)
(University of Chicago) Chicago, Illinois, USA  
73 YBN
[08/26/1927 AD]
5756) Griffith is killed working in his laboratory in London during an air-raid
in 1941.
(Ministry of Health) London, England (verify this is in London at the
time)  
73 YBN
[09/03/1927 AD]
5106)
(King's College) London, England  
73 YBN
[11/04/1927 AD]
5101)
(University of Aberdeen) Aberdeen, Scotland  
73 YBN
[12/12/1927 AD]
5113)
(University of Chicago) Chicago, Illinois, USA  
73 YBN
[12/13/1927 AD]
4870) The Nobel Prize in Chemistry 1950 is awarded jointly to Otto Paul Hermann
Diels and Kurt Alder "for their discovery and development of the diene
synthesis".
(Christian Albrecht University) Kiel, Germany  
73 YBN
[1927 AD]
4519)
(Rockefeller Institute, now called Rockefeller University) New York City, New
York, USA  
73 YBN
[1927 AD]
4520)
(Rockefeller Institute, now called Rockefeller University) New York City, New
York, USA  
73 YBN
[1927 AD]
4780)
(Oxford University) Oxford, England  
73 YBN
[1927 AD]
4821)
(Washington University) Saint Louis, Missouri, USA  
73 YBN
[1927 AD]
4847) Moniz is the University of Lisbon’s first professor of neurology
(1911–44).
(University of Lisbon) Lisbon, Portugal  
73 YBN
[1927 AD]
4869)
(Christian Albrecht University) Kiel, Germany  
73 YBN
[1927 AD]
4886)
(University of Göttingen) Göttingen, Germany  
73 YBN
[1927 AD]
4947) In 1949 Hess shares the Nobel Prize for physiology or medicine with Egas
Moniz (the first to perform lobotomies on humans).
(University of Zurich), Zurich, Switzerland  
73 YBN
[1927 AD]
4998)
(Chou Kou Tien) Peking, China  
73 YBN
[1927 AD]
5089) (Mount Wilson) Mount Wilson, California, USA  
73 YBN
[1927 AD]
5143) In 1922 Lemaître is ordained a priest.

(Perhaps a religious person would prefer that the universe have a moment of
creation. The idea of an infinitely old and large universe perhaps seems
illogical because people feel that all things must have a beginning and end. I
can not rule out that the universe does not have a beginning or end, but it
seems doubtful to me, and in addition, clearly the universe must be so large
that there will forever be a majority of the universe that we will never be
able to see one light particle from because of the physical limitation on our
size, and the speed in which we can move. Just knowing the reality of how we
can't possibly see it all, is a good enough argument to presume that the rest
goes on indefinitely. Some might argue that this universe is a tiny particle in
some other universe. The size of the universe in terms of scale, or
magnification, must also be infinite. The universe is probably the one thing
that advanced life will never be able to explain fully because nobody can
possibly see it all, and can only see what must be an extremely small part of
the universe.)
(University of Louvain) Louvain, Belgium  
73 YBN
[1927 AD]
5185)
(Electronic Phenomena Laboratory of the Petrograd Physical-Technical
Radiological Institute) (Petrograd now) Leningrad, Russia (presumably)  
73 YBN
[1927 AD]
5530) Ley is a consultant for the science fiction movie "Frau im Mond".
Ley is
strongly anti-Nazi and in 1935 moves to the USA.

In 1940 Von Braun joins the Nazi party.
In 1942 Von Braun is briefly imprisoned until
Hitler is persuaded that the rocket program cannot continue without him.
At the
close of World War II, von Braun and many colleagues go westward to surrender
to the US. Von Braun's arm is broken when his driver falls asleep at the week
and smashes the car.
In 1947 Von Braun is allowed to return to Germany to marry his
eighteen-year-old second cousin.
On 01/31/1958 Von Braun is the leader of the group at
Huntsville, Alabama that puts the US's first satellite (Explorer I) into orbit.
Asimov states that they may have been first, but were hindered by Eisenhower
and the Soviet Sputnik is first by 4 months.
In 1962 Von Braun's team begins
construction on the Saturn 5 rocket that will carry people to the moon.

(I think the ex-Nazi's should have been hired only as consultants, not as
supervisors. it seems absurd that people in the US could not quickly learn and
develop rockets. Depending on their crimes, they probably should have been
allowed to return to Germany. It should have been put to popular vote as all
things should be. Simply building missiles that are used to murder during war,
I don't think is a major crime if a crime at all, it's like those who
manufacture knives used by other people to murder. Racism is clearly evil and
inaccurate, but is nonviolent and within the realm of freedom of thought.)

(It's interesting that this rocket group probably would have developed one of
the early moon cities, had violent people not taken over Germany in 1935 and
World War 2 occured, and had, instead, the rocket group been free to follow
their own interests.)
(Berlin Institute of Technology) Berlin, Germany  
73 YBN
[1927 AD]
5720)
  
72 YBN
[01/??/1928 AD]
5240)
(Mount Wilson) Mount Wilson, California, USA  
72 YBN
[02/16/1928 AD]
5052) In 1929 Raman is knighted by the British government.
In 1930 Raman wins the Nobel
Prize in physics.
In 1947 Raman is the Director of Raman Research institute at Bangalore
in India.
Raman is the first Asian human (human living in India, China, or
Russia?) to get a Nobel Prize.
Raman trains more than 500 young Indian people in
science and education in an effort to build up scientific research and
education in India.
(University of Calcutta) Calcutta, India  
72 YBN
[02/??/1928 AD]
4801)
New York City, NY, USA  
72 YBN
[03/07/1928 AD]
5256) In the 1920s by using X-ray "diffraction", Pauling determines the
three-dimensional arrangement of atoms in several important silicate and
sulfide minerals. Pauling will also use electron "diffraction" to determine the
structure of some substances.

In 1954 Pauling wins the Nobel Prize in Chemistry "for his research into the
nature of the chemical bond and its application to the elucidation of the
structure of complex substances".

In 1958 Pauling and his wife present an appeal for a test ban to the United
Nations in the form of a document signed by 9,235 scientists from 44 countries.
In 1960 Pauling is called upon to defend his actions regarding a test ban
before a congressional subcommittee and refuses to reveal the names of those
who had helped him collect signatures.
In 1962 Pauling wins the Nobel Peace
Prize. Pauling is outspoken against nuclear testing and for nuclear
disarmament. Pauling is the second person after Marie Curie to win two Nobel
Prizes.

Pauling publishes reprts stating that when taken in large enough quantities
(megadoses), vitamin C helps the body fight off colds and other diseases, and
later that vitamin C is useful in treating cancer, however, investigations at
the Mayo Clinic involving human cancer patients do not corroborate Pauling’s
results. (To me this casts doubts on Pauli's valence theory, and the critical
perception of people in the quantum physics field. It seems possible that
Pauling had never heard of neuron writing and was possibly a victim of neuron
writing by the extreme violent criminals who killed JFK, and own so much of the
neuron writing infrastructure, in an effort to discredit liberal anti-war and
perhaps pro-democracy views.)
(California Institute of Technology) Pasadena, California  
72 YBN
[03/28/1928 AD]
5293)
Brooklyn, New York City, New York, USA  
72 YBN
[04/30/1928 AD]
5164)
(Washington Square College, New York University) New York City, New York, USA
  
72 YBN
[07/11/1928 AD]
5789) Alexander Lippisch (CE 1894-1976) builds and tests "Ente" (English:
"Duck"), the first aircraft to fly using rocket power. The plane has two black
powder rocket engines.

(It seems very likely that much of this research has, like remote neuron
reading and writing, artificial muscle running and jumping robots, etc - been
kept secret for many decades - it seems likely that there may even be very
advanced development on the moon, mars and around the other planets - if not,
there certainly should be by now - given 200 years of neuron reading and
writing.)
Wasserkuppe, Germany (verify)  
72 YBN
[07/22/1928 AD]
5830) In 1933, Ascheim and Zondek have to leave their duties and finally
Germany during National Socialism because they are Jewish.
(Aus der Universitats-Frauenklinik der Charite zu Berlin) Berlin, Germany  
72 YBN
[08/02/1928 AD]
5345) Gamow is the grandson of tsarist general, and son of a teacher.
In 1934
Gamow moves to the USA.
(I seriously doubt much of Gamow's work. Asimov calls him a
first-rate scientist, but without trying to sound mean or unpleasant, in my own
view, I think much of Gamow's work is simply inaccurate. Perhaps he was paid a
first-rate to mislead the neuron excluded. And this work is in the spirit of
mathematical abstraction (and some might say deception, since a major embrace
of secrecy and corruption happened in 1810 and later that was a terrible turn
for life on earth) that is so characteristic of the 1900s. In my view, and I
think any unbiased historian must agree, science completely flew off into an
erroneous direction with space-dilation, the big-bang theory, background
radiation, etc. We may find, as more thought-images reach the public, that much
of this pseudo-science corruption originates simply in the minds of the neuron
owners.)
(University of Göttingen) Göttingen, Germany  
72 YBN
[08/??/1928 AD]
3884)
New York City, NY (presumably)  
72 YBN
[12/28/1928 AD]
5294)
Cesarhurst, New York City, New York, USA  
72 YBN
[1928 AD]
4213)
(Eastman Kodak Company) NJ, USA (presumably)  
72 YBN
[1928 AD]
4468)
(Victoria Observatory) Victoria, British Colombia  
72 YBN
[1928 AD]
4876)
(General Motors Corporation) Dayton, Ohio, USA (verify)  
72 YBN
[1928 AD]
4915) In 1929 Jeans publishes “The Universe Around Us” and in 1934
“Through Space and Time” both of which explain astronomy to the public.

Jeans puts forward the idea that a star came close to our sun and pulled out
matter from the sun that formed into a cigar shape, the larger part forming the
Jovian planets, the smaller parts forming the terrestrial and smaller planets
beyond the gas giant planets.

Jeans doubts the nebular hypothesis of the solar system by Laplace, because the
planets contain 98 percent of the angular momentum of the solar system (the sun
rotates slowly while the planets orbit quickly). (Actually, as far as I can see
this is incorrect and the opposite of the actual physical truth. If the star
system was all connected, all the planets would orbit in the same time the sun
rotates which is only 20 earth days or something. The Sun rotates faster than
any object going around it. So the planets orbit the Sun much slower than the
sun rotates around it's own axis, indicating that the planets if anything trail
behind the rotation of the sun. The spiral shape of spiral galaxies is also an
example of this, the spiral portion on the outside drags behind the faster
rotating center. I am surprised that Jeans and Asimov miss this simple point.
In addition, it seems very likely that in simple Newtonian gravitation models,
randomly distributed masses can fall into rotation. Without question, any mass
that falls into and is captured by a larger group of masses takes an elliptical
orbit around the larger mass, so this is a simple explanation for why matter
tends to orderly orbit a central larger mass.)
(Mount Wilson Observatory) Pasadena, California, USA  
72 YBN
[1928 AD]
4956) The Nobel Prize in Physiology or Medicine 1945 was awarded jointly to Sir
Alexander Fleming, Ernst Boris Chain and Sir Howard Walter Florey "for the
discovery of penicillin and its curative effect in various infectious
diseases".
(St Mary's Hospital) London, England  
72 YBN
[1928 AD]
4984) Haworth works on atomic bomb project in WW II.
In 1937 Haworth wins a Nobel
Prize in chemistry shared with Karrer.
(St. Andrews University) St. Andrews, Scotland  
72 YBN
[1928 AD]
5033) With the rise of the Nazi movement, Paneth goes to England and takes a
position as guest lecturer at the Imperial College of Science and Technology,
London.
Königsberg, Germany  
72 YBN
[1928 AD]
5132) Szent-Györgyi deliberately wounds himself to get out of the Austrian
army during WW I.
In 1937 Szent-Györgyi wins the Nobel Prize in medicine and
physiology.
During WW II, Szent-Györgyi is active in the anti-Nazi
underground.
Szent-Györgyi speaks out against war.
(University of Szeged) Szeged, Hungary  
72 YBN
[1928 AD]
5222) The Nobel Prize in Physiology or Medicine 1961 is awarded to Georg von
Békésy "for his discoveries of the physical mechanism of stimulation within
the cochlea".
(Hungarian Telephone System Research Laboratory) Budapest, Hungary  
72 YBN
[1928 AD]
5709)
Manhattan, New York, New York City, USA  
72 YBN
[1928 AD]
6101) "I Wanna Be Loved By You" is written by Herbert Stothart and Harry Ruby,
with lyrics by Bert Kalmar, for the 1928 musical "Good Boy". The song is first
performed in late 1928 by Helen Kane, who became known as the 'Boop-Boop-a-Doop
Girl' because of her baby-talk, scat-singing tag line to that song. This
version was recorded right when Kane's popularity starts to reach its peak, and
becomes her signature song. Two years later, a cartoon character named Betty
Boop is modeled after Kane.

(Notice the lyric "I know what's on my mind.".)

New York City, New York, USA (guess)  
72 YBN
[1928 AD]
6265)
London, England (verify)  
72 YBN
[1928 AD]
6266)
(General Electric, WGY) Schenectady, New York, USA   
72 YBN
[1928 AD]
6267)
London, England (verify)  
71 YBN
[01/14/1929 AD]
5147)
(University of California) Berkeley, California, USA  
71 YBN
[01/17/1929 AD]
5061)
(Mount Wilson) Mount Wilson, California, USA  
71 YBN
[01/31/1929 AD]
4958)
(Bell Telephone Laboratories) New York City, New York, USA  
71 YBN
[02/23/1929 AD]
5383)
(Phys.-Techn. und Polytechn. Institut) Leningrad, (Soviet Union now)
Russia  
71 YBN
[04/22/1929 AD]
4781) Berger's first subject in these experiments is his young son.

Berger is reportedly disturbed by Nazism and commits suicide by hanging himself
on June 1, 1941, however, nobody should trust any report of suicide in the
neuron reading and writing secret years, in particular somebody who went public
with anything relating to neuron reading and writing.
(University of Jena) Jena, Germany  
71 YBN
[04/26/1929 AD]
5476)
(Norwich Research, Inc.) Norwich, Connecticut, USA  
71 YBN
[05/10/1929 AD]
5445) In 1986, the Nobel Prize in Physics is divided, one half awarded to Ernst
Ruska "for his fundamental work in electron optics, and for the design of the
first electron microscope",the other half jointly to Gerd Binnig and Heinrich
Rohrer "for their design of the scanning tunneling microscope".
(Technischen Hochschule/Technical University) Berlin, Germany  
71 YBN
[07/28/1929 AD]
5361) In 1935 Herzberg leaves Germany and moves to Canada after the rise of
Hitler. Although not of Jewish background, his surname is commonly
misidentified as Jewish and his wife is Jewish.

The Nobel Prize in Chemistry 1971 is awarded to Gerhard Herzberg "for his
contributions to the knowledge of electronic structure and geometry of
molecules, particularly free radicals".

Herzberg is noted for his extensive work on the technique and interpretation of
the spectra of molecules. Herzberg determines the properties of many molecules,
ions, and radicals and also contributes to the use of spectroscopy in astronomy
(for example in detecting hydrogen in space).

Herzberg uses spectral analysis to show the relationship of the spectra to the
molecular structure of gases, in particular simple two-atom molecules of
hydrogen, oxygen, nitrogen, and carbon monoxide. Herzberg detects the presence
of atom groupings that are intermediates in chemical reactions. (chronology)
(more specific:
which molecules? and their significance.)
(University of Göttingen) Göttingen, Germany  
71 YBN
[07/??/1929 AD]
4969) Robert Hutchings Goddard (CE 1882-1945), launches the first
instrument-carrying rocket near Worcester, Massachusetts. This is a larger
rocket than Goddard's first rocket (using a few thousand dollars of funding
from the Smithsonian Institute). This rocket carries a barometer, a
thermometer, and a small camera to photograph the proceedings This rocket goes
faster and higher than the first rocket. Like Langley before him, The New York
Times ridicules Goddard's efforts. The noise of this second rocket brings calls
to the police, and officials order Goddard to stop launching rockets. Goddard
then creates an experimental station for launching rockets near Roswell, New
Mexico, using $50,000 from Daniel Guggenhein who is pursuaded by Charles
Lindbergh. Here Goddard will built large rockets and develop many of the ideas
that are now standard in rocketry. Goddard designs combustion chambers, and
developed the first pumps suitable for rocket fuels, self-cooling rocket
motors.

(TODO: Chronology on fuel pump and self-cooling rocket)

(how are the photos captured? How many images?).
(TODO: Give specifics about NY
Times ridicule)
Worchester, Massachusetts, USA  
71 YBN
[07/??/1929 AD]
4972)
Worchester, Massachusetts, USA  
71 YBN
[08/26/1929 AD]
5211)
(California Institute of Technology) Pasadena, California, USA  
71 YBN
[08/??/1929 AD]
5136) In 1943 Doisy wins the Nobel Prize in medicine and physiology with Dam
for vitamin K composition.
(St. Louis University) St. Louis, Missouri, USA  
71 YBN
[09/13/1929 AD]
5358) Forssmann is captured by the USA in World War II and spends time in a
prison camp.
In 1956, the Nobel Prize in Physiology or Medicine is awarded jointly to
André Frédéric Cournand, Werner Forssmann and Dickinson W. Richards "for
their discoveries concerning heart catheterization and pathological changes in
the circulatory system".
(Chirurgischen Abteilung des Augusta Viktoria-Heims zu Eberswalde)  
71 YBN
[11/14/1929 AD]
5318) 1936 Director of Kaiser Wilhelm Institute for Biochemistry at Berlin.
The Nobel
Prize in Chemistry for 1939 is divided equally between Adolf Friedrich Johann
Butenandt "for his work on sex hormones" and Leopold Ruzicka "for his work on
polymethylenes and higher terpenes". However, like Domagk and Kuhn, Butenandt
is forced by the Nazi government to refuse the award until 1949.
(University of Göttingen) Göttingen, Germany  
71 YBN
[1929 AD]
4695)
(Rockefeller Institute for Medical Research) New York City, New York, USA  
71 YBN
[1929 AD]
4850)
(Johns Hopkins University) Baltimore, Maryland, USA  
71 YBN
[1929 AD]
4919)
(Mount Wilson Observatory) Pasadena, California, USA  
71 YBN
[1929 AD]
4935) Schmidt drinks alcohol regularly, and his last year is in a psychiatric
hospital. (For what activity?)
(Hamburg Observatory) Bergedorf, Germany  
71 YBN
[1929 AD]
4954) In 1930 Fischer wins the Nobel Prize in chemistry "for his researches
into the constitution of haemin and chlorophyll and especially for his
synthesis of haemin".
Fischer kills himself in dispair after air raids on Munich
destroyed his laboratory.
  
71 YBN
[1929 AD]
5144) In 1945 Virtanen wins the Nobel prize in chemistry "for his research and
inventions in agricultural and nutrition chemistry, especially for his fodder
preservation method".
(Biochemical Research Institute at Helsinki) Helsinki, Finland  
71 YBN
[1929 AD]
5287)
(Oxford Univerity) Oxford, England (presumably)  
71 YBN
[1929 AD]
5371)
(University of Giessen) Giessen, Germany (presumably)  
71 YBN
[1929 AD]
6055)
Los Angeles, California, USA (verify)  
71 YBN
[1929 AD]
6066) "Singin' In The Rain" (lyrics by Arthur Freed and music by Nacio Herb
Brown) recorded.

Hollywood, California, USA (probably)  
70 YBN
[01/??/1930 AD]
5178)
(Cornell University) Ithaca, New York, USA  
70 YBN
[02/14/1930 AD]
5353) In 1943 Oppenheimer is placed in charge of the laboratories at Los
Alamos, New Mexico, where the first atomic bomb is designed and constructed,
amd near where it is first exploded.
Oppenheimer approves the use of the fission bomb
over Japan.
Oppenheimer is reluctant to develop the more destructive hydrogen bomb.
In 1954
Oppenheimer is labeled "a loyal citizen but not a good security risk" by the
Atomic Energy Commission. The testimony of Teller who is in favor of developing
the H-bomb helps to convict Oppenheimer of this charge and Oppenheimer is
denied access to classified information. Henry Smyth a commissioner strongly
dissents.
In 1963 Oppenheimer wins the Fermi award which President Kennedy intends to
award personally, but Kennedy is murdered and President Johnson gives the
award. In the controversy that followed, Congress lowers the award from $50,000
to $25,000.

(To die so young and given neuron writing, it seems likely that oppenheimer was
probably murdered as many people were in the 1960s. Perhaps even many mindless
vicious idiot neuron consumers who observed applauded and must pay to see
bizarre and violent and no doubt many sex-related videos beamed to their eyes.
It seems possible that given 200 years of a secret neuron network that high
paid sex actors are used as a ruse for the violent to murder their enemies
under the guise of blaming some other person in the "heat of sexual passion".
Or perhaps there is no sexual element, just cold-blooded, everybody clothed,
military murdering.)

http://prola.aps.org/abstract/PR/v38/i9/p1787_1
range of neutrons and electrons – measure velocity, frequency?
(California Institute of Technology) Pasadena, California  
70 YBN
[02/18/1930 AD]
4795)
(University of Jena) Jena, Germany  
70 YBN
[02/18/1930 AD]
5398) Tombaugh's family is too poor to send him to college.
The news of Pluto will be
announced on March 13, 1930 the 75 anniversary of Lowell's birth.
For finding
Pluto, Tombaugh is awarded with a scholarship to the University of Kansas and
gets his bachelor's degree and a masters.
(Lowell Observatory) Flagstaff, Arizona, USA  
70 YBN
[02/??/1930 AD]
5009)
(Harvard College Observatory) Cambridge, Massachusetts, USA  
70 YBN
[04/04/1930 AD]
5220) Theiler never has any academic degrees. (including MD?)

The Nobel Prize in Physiology or Medicine 1951 is awarded to Max Theiler "for
his discoveries concerning yellow fever and how to combat it".
(Harvard University) Cambridge, Massachusetts, USA   
70 YBN
[05/06/1930 AD]
5102)
(University of Aberdeen) Aberdeen, Scotland  
70 YBN
[06/03/1930 AD]
5369) In 1938 the Mussolini regime falls under Hitler's thumb and Rossi is
forced to leave Italy.
(Physikalisch-Technische Reichsanstalt) Charlottenburg, Germany  
70 YBN
[06/17/1930 AD]
5403) When World War II starts in 1939 Godel fleas Europe with his wife, taking
the trans-Siberian railway across Asia, sailing across the Pacific Ocean, and
then taking another train across the United States to Princeton, N.J., where,
with the help of Einstein, Godel is hired at the newly formed Institute for
Advanced Studies (IAS).

In 1949 Gödel shows that Einstein’s theory of general relativity allows for
the possibility of time travel. (To me this shows perhaps creativity, but a
willingness to develop fraudulent or highly unlikely theories of physics of the
universe.)
(University of Wien) Vienna, (Austria now) Germany  
70 YBN
[07/19/1930 AD]
5020)
(Mount Hamilton) Santa Clara County, California, USA  
70 YBN
[08/19/1930 AD]
5177) The Nobel Prize in Physics 1951 is awarded jointly to Sir John Douglas
Cockcroft and Ernest Thomas Sinton Walton "for their pioneer work on the
transmutation of atomic nuclei by artificially accelerated atomic particles".

In 1961 Cockcroft wins the "Atoms for Peace" award.
(Cambridge University) Cambridge, England  
70 YBN
[10/10/1930 AD]
5268)
(University of California) Berkeley, California, USA  
70 YBN
[10/10/1930 AD]
5269)
(University of California) Berkeley, California, USA  
70 YBN
[10/23/1930 AD]
5077)
(University of Berlin) Berlin, Germany  
70 YBN
[11/15/1930 AD]
5212)
(University of Leeds) Leeds, England  
70 YBN
[12/04/1930 AD]
5234)
(Physical Institute of the Federal Institute of Technology) Zürich,
Switzerland  
70 YBN
[1930 AD]
4505)
(Universal Oil Products Company) Chicago, ILlinois, USA  
70 YBN
[1930 AD]
4804)
New York City, NY, USA (verify)  
70 YBN
[1930 AD]
4999)
(Chou Kou Tien) Peking, China (presumably)  
70 YBN
[1930 AD]
5031) Houssay had fallen out with the dictator of Argentina, Juan Domingo
Péron.
In 1943 Houssay is dismissed from his university post along with 150
other educators for taking too firm a pro-US stand at a time when Péron is
flirting with the German Nazis. (Interesting that Argentina is where many
Nazi's fled at the end of WW II, Klaus von Barbie being one notable, and also
Fritz Thiessan, a funder of Prescott Bush.)(Firing 150 educators shows the
anti-science view of Péron, which is typical of the extreme part of the other
side (the monarchistic, military dictatorship, violent, evil side). So many
things for me can simply be reduced to those that do violence versus those for
stopping violence.)
In 1947 Houssay shares the Nobel prize in medicine and
physiology with Coris. The controlled Argentinian press, instead of celebrating
the first Nobel Prize to a South American person, complains that the award is
politically motivated as a blow to Péron. Houssay responds that one must not
confuse little things (Péron) with big things (the Nobel Prize).
In 1955 when Péron
is driven into exile, Houssay is reinstated.

Houssay publishs over 600 scientific papers and several books.
(University of Buenos Aires School of Medicine) Buenos Aires, Argentina  
70 YBN
[1930 AD]
5079) Northrop's father was killed in a laboratory explosion when he was a
zoology instructor at Columbia University.
In 1946 Northrop wins the Nobel Prize in
chemistry, shared with Sumner and Stanley.
(Rockefeller Institute of Medical Research) New York City, New York, USA  
70 YBN
[1930 AD]
5160) In 1956 Semenov shares the Nobel Prize in chemistry with Hinshelwood.
Semenov is the first Soviet citizen to win a Nobel Prize.
(Electronic Phenomena Laboratory of the Petrograd Physical-Technical
Radiological Institute) (Petrograd now) Leningrad, Russia  
70 YBN
[1930 AD]
5173)
(Pic du Midi Observatory) Bigorre, France  
70 YBN
[1930 AD]
5176) When the Nazis invade, Hassel publishes in Scandinavian journals instead
of the more widely-read German journals.

From 1943 to 1945 the Nazis keep Hassel in jail with other faculty members of
the University of Oslo.

The Nobel Prize in Chemistry 1969 is awarded jointly to Derek H. R. Barton and
Odd Hassel "for their contributions to the development of the concept of
conformation and its application in chemistry".
(University of Oslo) Oslo, Norway  
70 YBN
[1930 AD]
6069) "I Got Rhythm" (music by George Gershwin, lyrics by Ira Gershwin) is
published.

New York City, New York, USA (probably)  
69 YBN
[02/17/1931 AD]
5257)
(California Institute of Technology) Pasadena, California  
69 YBN
[05/29/1931 AD]
5299) The Nobel Prize in Physics 1933 is awarded jointly to Erwin Schrödinger
and Paul Adrien Maurice Dirac "for the discovery of new productive forms of
atomic theory".
In 1932 Dirac is made Lucasian Professor of Mathematics at Cambridge.
  
69 YBN
[06/11/1931 AD]
5260)
(California Institute of Technology) Pasadena, California  
69 YBN
[09/10/1931 AD]
5446) Ernst August Friedrich Ruska (CE 1906-1988), German electrical engineer,
and Max Knoll (CE 1897-1969) build the first electron microscope, using
magnetic fields to focus electron beams similar to how a lens focuses light
beams. Ruska will go on, as others like Hillier do to make the electron
microscope practical. De Broglie had theorized that electrons posses a wave
aspect and Davisson had demonstrated this. (The view I support is that the
wavelength of electron beams relates to the distance between electrons, and
that electrons are particles and are probably not wave objects.) The claim is
that shorter the wavelength of light, the greater the magnification, and
electron waves are much shorter than waves of light.

This microscope can only magnify an object 16x. In 1933 Ruska builds an
electron microscope that for the first time gives higher magnification than a
light microscope.

Ruska's microscope is a "transmission electron microscope" (TEM). The
transmission electron microscope works on the same principle as an optical
microscope but uses electrons in the place of light and electromagnets in the
place of glass lenses. Development of the transmission electron microscope will
be quickly followed in 1935 by the development of the "scanning electron
microscope" (SEM) by Max Knoll. (verify)

In a later 1932 paper, (translated from German with Google) "The Electron
Microscope", Knoll and Ruska write for an abstract: "The main electron-optical
imaging systems and their suitability for the larger electron-rendered object
image, are given and discussed. The general conditions for error-free images
that define and limit the resolving power are given. A magnetic electron cold
cathode for high-speed electrons and the design of magnetic lenses are
described and several photomicrographs are reproduced. The methods of electron
microscope and imaging systems suitable for an ion microscope are discussed.".

In 1858 John Peter Gassiot (CE 1797-1877) had used a magnetic field to change
the direction of the beam caused by a high voltage through a vacuum tube.

In 1897 Karl Braun had invented the oscilloscope showing that a beam of
electrons can be moved by electromagnetic fields to draw an electronic
picture.

(Translate and read relevent parts of 1931 paper.)

(I doubt the claim that wavelength relates to magnification, because I think
magnification has more to do with the precision of the size of the focused
beam. The more precise the beam can be positioned, the higher the
magnification.)

(EX: Can a lens focus electron beams?)
(Zworykin's em appears perhaps later in
1939)
(Might the light particle provide even higher resolution, being smaller than
the electron?)
(In theory it might be possible to simply send a square of electrons and
record the image reflected, however, the electrons would have to be released in
the same quantity and interval, and maintain a straight line all the way to the
target. If electron beams, the beams would need to all be of equal strength.
Possibly a single electron source in the center that emits a sphere of
electrons might be able to record a reflected picture.)

(It seems likely that the electron microscope was secretly discovered earlier,
given the secret of neuron reading and writing. If true then Ruska would be
either an excluded who figured it out, or a spokesperson for making the
electron microscope public.)

(Determine correct paper. The paper of 09/10/1931 appears to be the first to
use the world "mikroskop")

(The future path for the electron microscope is clear - to make it much smaller
and less expensive so all average people can access an electron microscope for
examining objects around them.)
(Technischen Hochschule/Technical University) Berlin, Germany  
69 YBN
[10/03/1931 AD]
5161) In 1937 Carothers kills himself with cyanide at the age of 41. (It seems
possible that this was a neuron written suicide of an outsider, that is, a
person that had never heard of neuron reading and writing.)
( E.I. du Pont de Nemours & Company) Wilmington, Delaware, USA  
69 YBN
[10/13/1931 AD]
5319)
(University of Göttingen) Göttingen, Germany  
69 YBN
[11/29/1931 AD]
5213)
(University of Leeds) Leeds, England  
69 YBN
[11/29/1931 AD]
5214)
(University of Leeds) Leeds, England  
69 YBN
[12/05/1931 AD]
5125) In 1934 Urey wins the Nobel Prize in chemistry "for his discovery of
heavy hydrogen".

During World War II he was in charge of the separation of isotopes in the
atomic-bomb project. Urey's research also led to a large-scale method of
obtaining deuterium oxide (heavy water) for use as a neutron moderator in
reactors.

(It seems likely that some of Urey's work must be secret. It seems possible
that the Manhattan project followed Urey, or Urey followed the project, from
Columbia to Chicago. Of particular value is the idea of separating bulk matter
into valuable atoms. This will be a major process of the future - simply taking
an asteroid and separating it into useful components.)

Urey is against war, against nuclear power, and denounced Senator Joseph
McCarthy at a time when it was dangerous to do so.

(I see so-called "nuclear" power, as being probably the similar to simply
combustion in atoms releasing light particles. Ultimately, matter is going to
provide everything life of any star needs, and so the ultimate source of fuel,
oxygen, water, etc - is going to be from some method of extracting the light
particles from accumulated matter. So, I think the big process is going to be
seperating down big chunks of matter into useful atoms, - many being separated
into light particles in the process. In the short term, I think alcohol and
methane from waste recycling are likely answers to replacing fossil fuel
combustion. In addition, radioactive sources, and controlled uranium fission is
a fine choice for electricity. Nuclear waste can be atomically converted to
source light particles. Ultimately, all atoms can be converted to photons and
therefore completely used to move other objects.)
(Bureau of Standards) Washington, D. C. (and Columbia University) New York
City, New York, USA  
69 YBN
[12/16/1931 AD]
5370)
(University of Florence) Florence, Italy  
69 YBN
[12/19/1931 AD]
5288)
(Princeton University) Princeton, New Jersey, USA  
69 YBN
[12/28/1931 AD]
5188)
(Radium Institute) Paris, France (presumably)  
69 YBN
[12/??/1931 AD]
6060) "All of Me" is written and recorded (written by: Gerald Marks and Seymour
Simons).
  
69 YBN
[1931 AD]
4964)
(University of Tübingen) Tübingen, Germany  
69 YBN
[1931 AD]
4991)
Augsburg, Germany  
69 YBN
[1931 AD]
5054) In 1937 Karrer wins the Nobel prize in chemistry shared with Haworth.
(Chemical Institute) Zürich, Switzerland  
69 YBN
[1931 AD]
5251) The Nobel Prize in Chemistry 1938 is awarded to Richard Kuhn "for his
work on carotenoids and vitamins", however, Kuhn has to wait until end of World
War II to claim the award because of Hitler's refusal to allow German people to
accpet Nobel prizes after Carl von Ossietzky, in a Nazi concentration camp.

Ossietzky was a German pacifist and journalist who is imprisoned (in 1932) for
articles exposing the secret rearmament in Germany. After Adolf Hitler's rise
to power in 1933, Ossietzky is sent to the Sonnenburg concentration camp.
Suffering from tuberculosis, he is removed (1936) to a prison hospital shortly
before the announcement that he has been awarded the 1935 Nobel Peace Prize.
The German government then protests and bars all Germans from future acceptance
of a Nobel Prize. Still imprisoned, Ossietzky dies two years later.
(Kaiser Wilhelm-Institut fur Medizinische Forschung, Institut fur Chemie)
Heidelberg, Germany  
69 YBN
[1931 AD]
6053)
(Lincoln Tavern) Chicago, Illinois, USA (verify)  
69 YBN
[1931 AD]
6057)
Montclair, New Jersey  
68 YBN
[02/17/1932 AD]
5086)
(Cavendish Lab University of Cambridge) Cambridge, England  
68 YBN
[02/23/1932 AD]
5181)
(Cavendish Laboratory, Cambridge University) Cambridge, England  
68 YBN
[02/??/1932 AD]
5062)
(Mount Wilson) Mount Wilson, California, USA  
68 YBN
[03/01/1932 AD]
5342) The Nobel Prize in Physiology or Medicine 1967 is awarded jointly to
Ragnar Granit, Haldan Keffer Hartline and George Wald "for their discoveries
concerning the primary physiological and chemical visual processes in the eye".
(University of Pennsylvania) Philadelphia, Pennsylvania, USA  
68 YBN
[04/16/1932 AD]
5182)
(Cavendish Laboratory, Cambridge University) Cambridge, England  
68 YBN
[04/23/1932 AD]
5053)
(Massachusetts Institute of Technology)   
68 YBN
[04/29/1932 AD]
5385)
(Bell Telephone Laboratories) New York City, New York, USA  
68 YBN
[04/30/1932 AD]
5244) On April 12, 1933 Krebs is among the numerous Jewish people who are
dismissed from their academic posts in accordance with the newly decreed law
for the reform of the civil service. The Rockefeller Foundation, which had
already supported Krebs’s work in Freiburg through a grant to Thannhauser,
offers Kreb a one–year fellowship at Cambridge in England.

The Nobel Prize in Physiology or Medicine 1953 is divided equally between Hans
Adolf Krebs "for his discovery of the citric acid cycle" and Fritz Albert
Lipmann "for his discovery of co-enzyme A and its importance for intermediary
metabolism".
(University of Freiburg) Freiburg, Germany  
68 YBN
[05/08/1932 AD]
5386) In 1928 Jansky starts working for Bell Telephone Laboratories.
(Bell Telephone Laboratories) New York City, New York, USA  
68 YBN
[05/09/1932 AD]
5167)
(University of Pittsburgh) Pittsburgh, Pennsylvania, USA  
68 YBN
[06/07/1932 AD]
5286)
(University of Leipsig) Leipsig, Germany  
68 YBN
[06/15/1932 AD]
5183)
(Cavendish Laboratory, Cambridge University) Cambridge, England  
68 YBN
[06/??/1932 AD]
4883)
(Mount Wilson Observatory) Pasadena, California, USA  
68 YBN
[07/02/1932 AD]
5158)
(Wadham College) Oxford, England  
68 YBN
[08/02/1932 AD]
5380) In 1936, the Nobel Prize in Physics is divided equally between Victor
Franz Hess "for his discovery of cosmic radiation" and Carl David Anderson "for
his discovery of the positron".
(California Institute of Technology) Pasadena, California  
68 YBN
[08/02/1932 AD]
5381) In 1936, the Nobel Prize in Physics is divided equally between Victor
Franz Hess "for his discovery of cosmic radiation" and Carl David Anderson "for
his discovery of the positron".
(California Institute of Technology) Pasadena, California  
68 YBN
[08/21/1932 AD]
5200)
(Cavendish Laboratory, University of Cambridge) Cambridge, England  
68 YBN
[10/23/1932 AD]
5377) In 1935 Wildt moves from Germany to the USA.
(University of Göttingen) Göttingen, Germany  
68 YBN
[1932 AD]
4217)
(Eastman Kodak Company) NJ, USA  
68 YBN
[1932 AD]
4887)
(University of Göttingen) Göttingen, Germany  
68 YBN
[1932 AD]
4888)
(University of Göttingen) Göttingen, Germany  
68 YBN
[1932 AD]
4948)
(University of Zurich), Zurich, Switzerland  
68 YBN
[1932 AD]
4971)
(Clark University) Worchester, Massachusetts, USA  
68 YBN
[1932 AD]
4988)
(Kaiser Wilhelm Institute for Cell Physiology) Berlin, Germany  
68 YBN
[1932 AD]
5080)
(Rockefeller Institute of Medical Research) New York City, New York, USA  
68 YBN
[1932 AD]
5155) In 1939 Domagk wins the Nobel Prize in physiology and medicine "for the
discovery of the antibacterial effects of prontosil".
Domagk is jailed for a
week because Hitler was enraged in 1935 when the Nobel committee award the
Nobel Prize for Peace to Karl von Ossietzky, a German in a concentration camp.
Hitler refuses to allow German citizens to accept Nobel prizes. Domagk is
forced to withdraw his acceptance. In 1947 Domagk will visit Stockholm and
accept the prize.
(I. G. Farbenindustrie) Wuppertal-Elberfeld, Germany  
68 YBN
[1932 AD]
5324) The Nobel Prize in Physiology or Medicine 1955 is awarded to Hugo
Theorell "for his discoveries concerning the nature and mode of action of
oxidation enzymes".
(Uppsala University) Uppsala, Sweden  
68 YBN
[1932 AD]
5333) At age 6 Neumann can divide two eight digit numbers in his head.
In 1928
Von Neumann first writes about game theory and subsequently will develop game
theory. Game theory works out the best stratagies to follow in simple games,
such as coin matching. However, the principles will apply to more complicates
games such as business, war, and even scientific research can be viewed as a
game of humans trying to win against the challanges of the universe.
Von Neumann helps to
construct giant computers which perform high speed calculations that help the
production of the H-bomb and in reducing the H-bomb to a size small enough to
be fired by missile. (Perhaps Von Neumann was involved with microscopic flying
neuron reading and writing camera radio devices?)
In 1930 Von Neumann leaves Europe to
work in Princeton. (Perhaps an early view of the rise of anti-Jewish views? Von
Neumann was the son of a well-to-do Jewish banker according to the Complete
Dictionary of Scientific Biography.)

In 1954 Von Neumann testifies for Oppenheimer when Oppenheimer, who opposed the
development of the H-bomb, was being investigated. Teller testifies against
Oppenheimer.
In 1956 Von Neumann wins the Fermi award.
(Princeton University) Princeton, New Jersey, USA  
68 YBN
[1932 AD]
6261)
(BASF) Ludwigshafen, Germany  
67 YBN
[01/30/1933 AD]
5115)
(University of Chicago) Chicago, Illinois, USA  
67 YBN
[02/08/1933 AD]
5247) The Nobel Prize in Physiology or Medicine 1967 is awarded jointly to
Ragnar Granit, Haldan Keffer Hartline and George Wald "for their discoveries
concerning the primary physiological and chemical visual processes in the eye".
(Perhaps this was a push to go public or generate some public research with
neuron reading and writing.)
(Oxford Univerity) Oxford, England  
67 YBN
[03/27/1933 AD]
5201)
(Cavendish Laboratory, University of Cambridge) Cambridge, England  
67 YBN
[03/??/1933 AD]
4164)
Irvine, CA, USA  
67 YBN
[04/10/1933 AD]
5189)
(Radium Institute) Paris, France (presumably)  
67 YBN
[04/12/1933 AD]
5148)
(University of California) Berkeley, California, USA  
67 YBN
[05/22/1933 AD]
5190)
(Radium Institute) Paris, France (presumably)  
67 YBN
[06/16/1933 AD]
5278)
(Cavendish Lab University of Cambridge) Cambridge, England  
67 YBN
[07/30/1933 AD]
5069)
New York City, New York, USA  
67 YBN
[08/01/1933 AD]
4985)
(Federal Institute of Technology) Zurich, Switzerland and (Birmingham
University) Birmingham, England  
67 YBN
[08/06/1933 AD]
5435) In the summer of 1933, the Nazis had come to power in Germany and the
National Research Council insisted that Wald, who is Jewish, must return to the
United States.

In 1967, the Nobel Prize in Physiology or Medicine is awarded jointly to Ragnar
Granit, Haldan Keffer Hartline and George Wald "for their discoveries
concerning the primary physiological and chemical visual processes in the
eye".

In 1969, Wald’s life changes dramatically after he delivers a speech at the
Massachusetts Institute of Technology called "A Generation in Search of a
Future" (Wald, 1969). This speech, which criticizes the U.S. war in Vietnam and
the nation’s buildup of nuclear weapons, is published in periodicals around
the planet earth, and it propels Wald into the limelight of social activism.
(University of Zurich) Zurich, Switzerland  
67 YBN
[10/07/1933 AD]
5474)
(Bartol Research Foundation of the Franklin Institute, University of Delaware)
Newark, Delaware, USA  
67 YBN
[12/12/1933 AD]
5447)
(Technischen Hochschule/Technical University) Berlin, Germany  
67 YBN
[1933 AD]
3885)
New York City, NY (presumably)  
67 YBN
[1933 AD]
4778)
(Cambridge University) Cambridge, England   
67 YBN
[1933 AD]
4812)
(Tesla's private lab) New York City, NY, USA (verify)  
67 YBN
[1933 AD]
4822)
(Washington University) Saint Louis, Missouri, USA  
67 YBN
[1933 AD]
4859)
(University of California at Berkeley) Berkeley, California, USA  
67 YBN
[1933 AD]
4983)
(Cambridge University) Cambridge, England   
67 YBN
[1933 AD]
5273)
(University of Rome) Rome, Italy (presumably)  
67 YBN
[1933 AD]
5281)
(University of Rome) Rome, Italy (presumably)  
67 YBN
[1933 AD]
6067) "The Gold Diggers' Song (We're in the Money)" is recorded (lyrics by Al
Dubin, music by Harry Warren).

(Warner Brothers Studio) Burbank, California, USA  
66 YBN
[01/15/1934 AD]
5191)
(Radium Institute) Paris, France (presumably)  
66 YBN
[01/15/1934 AD]
5192)
(Radium Institute) Paris, France  
66 YBN
[01/22/1934 AD]
5413)
(Rockefeller Institute of Medical Research) New York City, New York, USA  
66 YBN
[02/10/1934 AD]
5202)
(Cavendish Laboratory, University of Cambridge) Cambridge, England
(presumably)  
66 YBN
[02/24/1934 AD]
5184)
(Cavendish Laboratory, Cambridge University) Cambridge, England  
66 YBN
[03/17/1934 AD]
4755)
(Cambridge University) Cambridge, England   
66 YBN
[03/19/1934 AD]
5210)
(Mount Wilson Observatory) Mount Wilson, California, USA  
66 YBN
[03/25/1934 AD]
5274)
(University of Rome) Rome, Italy (presumably)  
66 YBN
[04/11/1934 AD]
5320)
(Institute der Technische Hochschule) Danzig-Langfuhr, Germany (Austria)  
66 YBN
[04/14/1934 AD]
5279)
(Cavendish Lab University of Cambridge) Cambridge, England (presumably)  
66 YBN
[05/??/1934 AD]
5275)
(University of Rome) Rome, Italy  
66 YBN
[06/07/1934 AD]
4853)
(National Institute For Medicine) Hampstead, London  
66 YBN
[06/28/1934 AD]
5205) When the Nazis came into power in 1933, Szilard goes to Vienna and, in
1934, to London, where he joins the physics staff of the medical college of St.
Bartholomew’s Hospital.

In 1939 when the uranium fission found by Hahn is announced by Meitner, Szilard
understands that this chain-reaction is practical. Szilard convinces physicists
in the USA not to publish their work in particle physics to avoid giving the
Nazi's any ideas. And also in 1939, Wigner, Teller and Szilard (all Hungarian
refugees) persuade Einstein to send his famous letter (written by Szilard) to
President Franklin D. Roosevelt, and this sets in motion the Manhattan Project
that will prepare the first nuclear bomb.

(I doubt that any "letter" was necessary, and this story of Szilard and
Einstein's letter is probably irrelevent to the development of atomic
explosives in the USA. Because clearly FDR and many others must have received
direct-to-neuron video messages. Certainly no letter was necessary, FDR clearly
received thought-mail, or thought-messages by this time, and it was enough to
make a concerted effort to send a video-message to FDR's brain to get a message
through, but perhaps a formal letter would increase the importance of the
message.)

Szilard is one of the large group of scientists that advocate using the bomb
over an uninhabited territory as a demonstration. The military, and some
scientists such as Compton disagree and Harry Truman decided to explode a
nuclear bomb over Hiroshima and Nagasaki.

(Detonating the bomb over an uninhabited territory is by far the more humane
decision. I think for sure, a second bomb is too murderous. It is a tough
debate. I think a person needs to calculate how much time is involved in
creating another bomb. I think in some way, the nuclear bomb over Japan was
felt to be a justified payback for the first strike invasion of Pearl Harbor.
In any event, the nuclear bombs did bring the war to a quick end. Everybody
should see the neuron images and make their own determination. With war, a
minority of wealthy dictators brutally send young poor people to their death
without any choice. Probably no large scale violent conflicts would ever have a
chance to start if we had a planet of full and constant democracy, and full and
total free information.)

Szilard labors to ban nuclear warfare and even nuclear testing.
(I reject a
test ban on nuclear testing, except for exploding nuclear bombs on, in or in
the atmosphere of earth. For example, I see nothing wrong with a safe atomic
bomb explosion far from the earth in space, perhaps out near the orbit of
Jupiter or Neptune. But this will probably wait for many decades until humans
are moving between the planets. The debate about using uranium fission in space
will be a heated one, but one that eventually will fall to those who want to
build faster ships. Maybe some more acceptable form of propulsion will be found
such as anti-protons...anyway we look at it, clearly nuclear atom separation
uranium fission, or some other fission or fusion is probably going to be the
fastest form of propulsion. Possibly gravitational acceleration may result in a
similar velocity using the large mass of the sun, and Jupiter. )

In 1946 Szilard is appointed to the chair of biophysics at the University of
Chicago, where he remained until his death. (Perhaps for some reason Szilard
was forced to leave particle physics?)

In 1959 Szilard wins the Atoms for Peace award.
(It seems unlikely that a person
secretive about fission would not be secretive about hearing thought, but
maybe, with the fall of the Nazis, reflecting on their rise and abuses of the
innocent excluded unaware of the advance of the technology, Szilard supported
going public with neuron reading and writing.)

(I think always the case is that, there should be a worry about allowing
violent people, in particular first degree murderers have access to ideas of
mass destruction, but the case is less strong for seeing and hearing thoughts,
the telephone, etc, non-destructive technology. Ultimately, violence should be
exposed and stopped, and secrecy, I think, tends to increase the chances of
violent people getting away with violence, and the spiraling out of control of
unseen, unstopped violence on earth, the controlled demolition of of the World
Trade Center buildings on 09/11/2001 and subsequent massive coverup by many
thousands of people is a prime example of where secrecy and misinformation can
have very violent, risky, destructive consequences which threaten survival of
life of earth. But how far should people go to keep information out of the
hands of murderers?)

In 1964 Szilard hypothesizes about the influence living objects might have on
the physics of the universe in his paper "On the decrease of entropy in a
thermodynamic system by the intervention of intelligent beings".
(Claremont Haynes & Co) London, England  
66 YBN
[07/11/1934 AD]
4248)
(Hotel New Yorker) New York City, NY, USA  
66 YBN
[07/11/1934 AD]
5367) In 1970, the Nobel Prize in Physiology or Medicine is awarded jointly to
Sir Bernard Katz, Ulf von Euler and Julius Axelrod "for their discoveries
concerning the humoral transmittors in the nerve terminals and the mechanism
for their storage, release and inactivation".
(Karolinischen Institues) Stockholm, Sweden  
66 YBN
[08/09/1934 AD]
4867)
(Percival Lowell's observatory) Flagstaff, Arizona, USA  
66 YBN
[08/18/1934 AD]
5087) Goldhaber moves from German with the advent of Hitler and in 1938 moves
to the USA.
(Cavendish Lab University of Cambridge) Cambridge, England  
66 YBN
[09/10/1934 AD]
5208)
(St. Bartholmew's Hospital) London, England  
66 YBN
[09/17/1934 AD]
5206)
(St. Bartholmew's Hospital) London, England  
66 YBN
[09/17/1934 AD]
5388)
  
66 YBN
[11/14/1934 AD]
5196)
(Radium Institute) Paris, France  
66 YBN
[11/17/1934 AD]
5452) In 1949, the Nobel Prize in Physics is awarded to Hideki Yukawa "for his
prediction of the existence of mesons on the basis of theoretical work on
nuclear forces". Yukawa is the first Japanese person to win a Nobel Prize.

(I think this theory is highly speculative and in my view is not proven, and
there are many other theories. I think this theory of a nuclear force will
ultimately be proven false. These awards are probably a reflection of a
majority of people in science, and if the majority buy into some theory and
pursue it for decades, it appears to be legitimate, and therefore is awarded.)

(Determine if Yukawa has any recorded comments about Pearl Harbor, Hirohito,
Hiroshima, Hitler, Nazism.)
(Osaka Imperial University) Osaka, Japan  
66 YBN
[11/26/1934 AD]
5207)
(St. Bartholmew's Hospital) London, England  
66 YBN
[12/04/1934 AD]
5126)
(Columbia University) New York City, New York, USA  
66 YBN
[12/??/1934 AD]
5531)
(Kummersdorf Army Proving Grounds) Kummersdorf, Germany  
66 YBN
[1934 AD]
4904)
  
66 YBN
[1934 AD]
5011)
(Columbia University) New York City, New York, USA  
66 YBN
[1934 AD]
5035)
(University of Utrecht) Utrecht, Netherlands (check)  
66 YBN
[1934 AD]
5036)
(Federal Institute of Technology) Zurich, Switzerland (presumably)  
66 YBN
[1934 AD]
5048) The phase-contrast microscope, slightly changes the phase of diffracted
light compared with direct light so that objects in a cell take on color and
objects within the cell become clear without staining, and therefore without
killing the cell.

While studying the flaws that occur in some diffraction gratings because of the
imperfect spacing of engraved lines, Zernicke discovers the phase-contrast
principle. This uses the fact that light passing through bodies with a
different refractive index from the surrounding medium has a different phase.
The microscope contains a plate in the focal plane, which causes interference
patterns and thus increases the contrast. For instance, it can make living
cells observable without killing them by staining and fixing. The method of
phase contrast also allows the detail in transparent objects or on metal
surfaces to be observed.

(More details about how microscope works)

(The phase of light or any beam of particles is a very interesting topic. One
question is: how do detectors understand that 2 beams are actually the same
frequency when they both have different starting times/points (and are
therefore out of phase)? In electronics the resonant frequency of the
inductor-capacitor circuit simply accumulates particles - and only works for a
specific frequency of light. In addition, what is the effect of two out of
phase particle beams? Can this explain the interference patterns of an
interferometer? What is happening there at the particle level? For example a
single tiny beam of white light is made of single beams of other frequencies
but appears white to a detector in a human eye. This detector sees a specific
color wavelength, no matter when that beam starts. What does a beam made of
individual out of phase same frequency beams appear like to a detector? Like a
single wavelength beam? Like a higher wavelength beam? )

(Explain how the light phase is changed in a phase-contrast microscope, show
images of phase-contrast microscopes.)

(Explain how this is interpreted in the light-as-a-material-particle view.)
(University of Groningen) Groningen, Netherlands  
66 YBN
[1934 AD]
5141) In 1922 Oberth has his dissertation on rocket design rejected when trying
for a Ph.D. at Heidelberg.
In 1940 Oberth becomes a German citizen. (Was Oberth opposed to
Hitler's brutal views and many others of the Nazi society?)
Oberth works with von Braun
at Peenemunde (building rockets such as the V-2).
  
66 YBN
[1934 AD]
5154)
(Duke University) Durham, North Carolina, USA(verify)  
66 YBN
[1934 AD]
5276)
(University of Rome) Rome, Italy (presumably)  
66 YBN
[1934 AD]
5356) The Nobel Prize in Physics 1958 is awarded jointly to Pavel Alekseyevich
Cherenkov, Il´ja Mikhailovich Frank and Igor Yevgenyevich Tamm "for the
discovery and the interpretation of the Cherenkov effect".
(Lebedev Institute of Physics) Moscow, (Soviet Union now) Russia  
66 YBN
[1934 AD]
6070) "On the Good Ship Lollipop" (music by Richard A. Whiting, lyrics by
Sidney Clare, sung by Shirley Temple) is recorded in the 1934 movie "Bright
Eyes".

(Sam Fox Publishing Company) New York City, USA (possibly)  
65 YBN
[01/01/1935 AD]
5492) Chandrasekhar is the nephew of Sir Chandrasekhara Venkata Raman, who won
the Nobel Prize for Physics in 1930.

Chandrasekhar is asked or feels it necessary to add a note in the beginning of
the book and a footnote to Albert Michelson's chapter on relativity in the 1968
(also in the 1962?) reprint of Michelson's "Studies in Optics" (1927) which
reads: "In describing these ideas bearing on special relativity, Professor
Michelson adopts a cautious attitude, sometimes giving the impression of
skepticism. Such an attitude was justifiable at the time in view of the
revolutionary character of the theory. However, at the present time the
experimental basis for special relativity is so wide and the theoretical
ramifications so many that there can no longer be any doubt about its validity.
In chapter xiv reference is also made to the 'generalized theory of
relativity.' However, this theory represents a development along somewhat
different lines and except in a very general way does not bear on the subject
matter of these two chapters. The foundations of the general theory (unlike
those of the special theory) are still in the process of change and
evolution.". This is a perfect example of the bizarre and authoritarian
enforcement of the dogma of relativity and time-dilation- most likely due to
pressure placed on those in science by owners of direct-to-neuron writing
devices in order to maintain an absolutely ignorant uneducated non-scientific
barefoot agrarian-society 1400s public.
(University of Cambridge) Cambridge, England  
65 YBN
[01/01/1935 AD]
5501)
(University of Cambridge) Cambridge, England  
65 YBN
[01/26/1935 AD]
5133)
(University of Szeged) Szeged, Hungary  
65 YBN
[02/26/1935 AD]
5098)
Daventry, England  
65 YBN
[02/??/1935 AD]
5162)
(E.I. du Pont de Nemours & Company) Wilmington, Delaware, USA  
65 YBN
[04/08/1935 AD]
5145) In 1940 Dam stays in the USA when the Nazis invade Denmark.
In 1943 Dam wins the
Nobel Prize in medicine and physiology with Doisy.
(University of Copenhagen) Copenhagen, Denmark  
65 YBN
[05/16/1935 AD]
5374)
(National Physical Laboratory) Teddington, Middlesex, England  
65 YBN
[05/31/1935 AD]
5532)
(Mescalero Ranch) Roswell, New Mexico, USA  
65 YBN
[06/05/1935 AD]
5436)
(Kaiser Wilkelm-Institut fur medizinische Forschung, Heidelberg, Germany and
University of Chicago) Chicago, Illinois, USA  
65 YBN
[06/26/1935 AD]
5215) In 1933, being a German-Jewish scientist, Schoenheimer emigrates to the
USA.
In 1941 Schoenheimer kills himself.
(Columbia University) New York City, New York, USA  
65 YBN
[07/11/1935 AD]
4249)
(Hotel New Yorker) New York City, NY, USA  
65 YBN
[07/12/1935 AD]
5016)
(University of Chicago) Chicago, Illinois, USA  
65 YBN
[07/28/1935 AD]
5357) In 1946, the Nobel Prize in Chemistry is divided, one half awarded to
James Batcheller Sumner "for his discovery that enzymes can be crystallized",
the other half jointly to John Howard Northrop and Wendell Meredith Stanley
"for their preparation of enzymes and virus proteins in a pure form".
(The Rockefeller Institute for Medical Research) Princeton, New Jersey,
USA  
65 YBN
[07/31/1935 AD]
5252)
(Kaiser Wilhelm-Institut fur Medizinische Forschung, Institut fur Chemie)
Heidelberg, Germany  
65 YBN
[08/28/1935 AD]
5507)
(Cavendish Lab University of Cambridge) Cambridge, England  
65 YBN
[08/28/1935 AD]
5509)
(Cavendish Lab University of Cambridge) Cambridge, England  
65 YBN
[10/22/1935 AD]
5451) (Notice the submission date of 2 days before 10/24- a day that may have
neuron reading and writing significance.)
(Technischen Hochschule/Technical University) Berlin, Germany
(presumably)  
65 YBN
[10/28/1935 AD]
5095)
(Gonville and Caius College University of Cambridge) Cambridge, England  
65 YBN
[11/19/1935 AD]
5498)
(University College) London, England  
65 YBN
[11/23/1935 AD]
5456) In 1957, the Nobel Prize in Physiology or Medicine is awarded to Daniel
Bovet "for his discoveries relating to synthetic compounds that inhibit the
action of certain body substances, and especially their action on the vascular
system and the skeletal muscles".
(Pasteur Institute) Paris, France  
65 YBN
[??/?/1935 AD]
5508)
(University of Rome) Rome, Italy  
65 YBN
[1935 AD]
4786)
(The Rockefeller Institute for Medical Research) New York City, New York,
USA  
65 YBN
[1935 AD]
5014)
(Mayo Foundation) Rochester, Minnesota, USA  
65 YBN
[1935 AD]
5037)
(Federal Institute of Technology) Zurich, Switzerland (presumably)  
65 YBN
[1935 AD]
5055)
(Chemical Institute) Zürich, Switzerland  
65 YBN
[1935 AD]
5081)
(Rockefeller Institute of Medical Research) New York City, New York, USA  
65 YBN
[1935 AD]
5094)
(Institut d’Optique) Paris, France  
65 YBN
[1935 AD]
5166) The Nobel Prize in Physiology or Medicine 1947 is divided, one half
jointly to Carl Ferdinand Cori and Gerty Theresa Cori, née Radnitz "for their
discovery of the course of the catalytic conversion of glycogen" and the other
half to Bernardo Alberto Houssay "for his discovery of the part played by the
hormone of the anterior pituitary lobe in the metabolism of sugar".
(Washington University) Saint Louis, Missouri, USA  
65 YBN
[1935 AD]
5325)
(Uppsala University) Uppsala, Sweden  
65 YBN
[1935 AD]
6037)
New York City, New York, USA (verify)  
64 YBN
[01/??/1936 AD]
6319) Humason started as a janitor at the Mount Wilson observatory, and was the
assistant of Hubble.
(Mount Wilson) Mount Wilson, California, USA  
64 YBN
[02/13/1936 AD]
5457)
(Pasteur Institute) Paris, France  
64 YBN
[03/11/1936 AD]
5496) In 1934 Katz leaves Germany for Britain.

In 1970, the Nobel Prize in Physiology or Medicine is awarded jointly to Sir
Bernard Katz, Ulf von Euler and Julius Axelrod "for their discoveries
concerning the humoral transmittors in the nerve terminals and the mechanism
for their storage, release and inactivation".
(University College) London, England  
64 YBN
[03/28/1936 AD]
5346)
(George Washington University) Washington, D.C., USA  
64 YBN
[05/27/1936 AD]
5134) Szent-Györgyi isolates flavones that can change the permeability of
capillaries, in other words how easily substances can pass through the
capillary walls. It is not clear if these are vitamins, but for some time are
called “vitamin P”.

Szent-Gyorgyi writes:
"VARIOUS chemical and clinical observations have led to the
assumption that ascorbic acid is accompanied in the cell by a substance of
similar importance and related activity. In absence of both substances, the
symptoms of lack of ascorbic acid (scurvy) prevail and conceal symptoms of the
deficiency of the second substance. In the lack of suitable experimental
animals or conditions, progress was dependent on spontaneous pathological
conditions, caused or influenced by this second factor.
In collaboration with L.
Armentano and A. Bensath, we have dounf that in certain pathological
conditions, characterised by an increased permeability or fragility of the
capillary wall, ascorbic acid is ineffective, while the condition can readilyu
be cured by the administration of extracts of hungarian red pepper ('vitapric')
or lemon juice. The extracts were effective in cases of decreased resistance of
the capillary wall toward whole blood (vascular type of haemorrhagic purpura)
as well as in cases in which the capillary wall showed an increased
permeability towards plasma protein only (various septic conditions). The
extracts were fractinoated. The active substance was found in the end in a
fraction consisting of preactivcally pure flavon or flavonol glycoside. 40 mgm.
of this fraction given daily intravenously to man restored in a fortnight
regularly the normal capillary resistance. Spontaneous bleeding ceased, the
capillary walls lost their fragility towards pressure differences and no more
plasma protein left the vascular system on increased venous pressure.
These
results suggest that this great group of vegtable dyes, the flavons or
flavonols, also play an important role in animal life, and that the dyes are of
vitamin nature. The group is not to be confused with the yellow dye, discovered
by one of us and termed 'flaves' (like cytoflave), which dye forms the
prosthetic group of Warburg's yellow enzyme and has later been renamed by R.
Kuhn 'flavins'. We propose to give the name 'vitamin P' to the substance
responsible for the action on vascular permeability.
...".
(University of Szeged) Szeged, Hungary  
64 YBN
[05/28/1936 AD]
5563) In March 1952 Turing is prosecuted for homosexuality, then a crime in
Britain, and sentenced to 12 months of hormone "therapy".

Turing dies of potassium cyanide, which is ruled a suicide but could have been
an accident. (Could have been murder - only the dust-sized camera images would
reveal if true.)

(Much of the public views on computers and artificial intelligence is of little
value - in particular because nobody imagined that flying and walking cameras,
seeing thought-images and hearing thought-sounds, and artificial muscle robots
would be a common occurance. Knowing and seeing these things vastly changes the
view on what thought is, and how truth can be viewed as more of a sensory match
phenomenon, and a three space dimension and 1 time dimension problem. But
beyond that - my own preference is for the practical application of logic in
developing walking robots that can clean, cook, drive, etc - provide productive
support for humans.)
(Princeton University) Princeton, New Jersey, USA  
64 YBN
[06/22/1936 AD]
5137)
(St. Louis University) St. Louis, Missouri, USA  
64 YBN
[07/15/1936 AD]
5359) In 1970, the Nobel Prize in Physics is divided equally between Hannes
Olof Gösta Alfvén "for fundamental work and discoveries in magnetohydro-
dynamics with fruitful applications in different parts of plasma physics" and
Louis Eugène Félix Néel "for fundamental work and discoveries concerning
antiferromagnetism and ferrimagnetism which have led to important applications
in solid state physics".
(University of Strasbourg) Strasbourg, France  
64 YBN
[07/23/1936 AD]
5270)
(University of California) Berkeley, California, USA  
64 YBN
[08/08/1936 AD]
5479)
(The Central Pathological Laboratory and the Hospital for Epilepsy and
Paralysis) Maida Vale, United Kingdom  
64 YBN
[08/10/1936 AD]
5540)
(Princeton University) Princeton, New Jersey, USA  
64 YBN
[08/14/1936 AD]
5344)
(Jackson Laboratory) Bar Harbor, Maine, USA  
64 YBN
[08/17/1936 AD]
5336)
(Columbia University) New York City, New York, USA  
64 YBN
[1936 AD]
3979)
  
64 YBN
[1936 AD]
4486) Broom wrongly believes that with the human species evolution has come to
an end and the evolution of humans represents the sixth and final day of
creation as in Genesis.
Sterkfontein, Transvaal, South Africa  
64 YBN
[1936 AD]
4848)
(University of Lisbon) Lisbon, Portugal  
64 YBN
[1936 AD]
5012)
(Columbia University) New York City, New York, USA  
64 YBN
[1936 AD]
5028)
(University of Illinois) Urbana, Illinois  
64 YBN
[1936 AD]
5116) Haldane is an assistant to his father at age 8.
Haldane is an outspoken
atheist.
In the 1930s Haldane supports Communism, helps refugees from Nazi Germany, but
then leaves the Communist party, although remains a Marxist, becoming
disillusioned at the rise of Lysenko under Stalin.
(University College) London, England  
64 YBN
[1936 AD]
5117)
(University College) London, England  
64 YBN
[1936 AD]
5140) In 1935 the Soviet government establishes a biochemical institute in
Oparin's honor in Moscow.
In 1946 Oparin becomes the director of the biochemical
institute in Moscow.
Moscow, (Soviet Union) Russia  
64 YBN
[1936 AD]
5422)
(Rockefeller Institute of Medical Research) New York City, New York, USA  
64 YBN
[1936 AD]
5722)
  
64 YBN
[1936 AD]
6041)
Moscow, (U.S.S.R. now) Russia (presumably)  
63 YBN
[01/25/1937 AD]
5300) In 1947 Tiselius is made Vice-president of Nobel Foundation. (Doesn't
this cause a conflict of interest in his award? Perhaps he abstained.)

The Nobel Prize in Chemistry of 1948 is awarded to Arne Tiselius "for his
research on electrophoresis and adsorption analysis, especially for his
discoveries concerning the complex nature of the serum proteins".
(University of Uppsala) Uppsala, Sweden  
63 YBN
[02/18/1937 AD]
5453)
(Osaka Imperial University) Osaka, Japan  
63 YBN
[03/01/1937 AD]
5245)
(University of Sheffield) Sheffield, England  
63 YBN
[03/17/1937 AD]
5471)
(Rothamsted Experimental Station) Harpenden, Hertfordshire, England  
63 YBN
[03/18/1937 AD]
5221)
(Rockefeller Foundation) New York City, New York, USA  
63 YBN
[04/??/1937 AD]
6268)
(British Thomson-Houston works) Rugby, England  
63 YBN
[05/14/1937 AD]
5548)
(Kaiser-Wilhelm-Instute fur Chemie in Berlin-Dahlem) Berlin, Germany  
63 YBN
[05/22/1937 AD]
5515)
(Siemens and Halske) Berlin, Germany  
63 YBN
[06/30/1937 AD]
5364) In the summer of 1938, during his second visit to Berkeley, Segré learns
that, because of his Jewish origins, his professorship at Palermo has been
revoked by Benito Mussolini’s government. At Lawrence’s invitation, Segré
becomes a research associate at the Radiation Laboratory at Berkeley.

In 1938 Segré is removed from his Palermo post by Italy's Fascist government
while in the USA, and Segré stays in the USA.

In 1959, the Nobel Prize in Physics is awarded jointly to Emilio Gino Segrè
and Owen Chamberlain "for their discovery of the antiproton".
(Royal University) Polermo, Italy  
63 YBN
[07/06/1937 AD]
6051)
Hollywood, California, USA (verify)  
63 YBN
[07/09/1937 AD]
5046)
(Carnegie institute of Technology) Pittsburgh, Pennsylvania, USA  
63 YBN
[09/??/1937 AD]
5449)
(University of Saskatchewan) Saskatoon, Saskatchewan, Canada  
63 YBN
[09/??/1937 AD]
5525) At fifteen Reber is active with ham radio.
Reber fails to bounce radio signals
off the moon, but the Army Signal Corps will succeed at this after World War
II. (Clearly light from the Sun is reflected off the moon all the way to our
eye, so any frequency of light can be reflected off the moon, Jupiter, and any
other visible object. The key is that a very large initial signal is needed so
that enough particles reflect back in the direction of the receiver.)
In 1947
Reber gives his radio telescope to the National Bureau of Standards.

In his later years Reber speaks out on what he sees as problems with relativity
theory and big-bang cosmology. Reber believes that much of the redshift
observed in the spectra of distant galaxies is due to the forward scattering of
light as it moves through space.
Wheaton, Illinois, USA  
63 YBN
[12/03/1937 AD]
5142) (Institute for Physical Problems, Academy of Sciences) Moscow, (Soviet Union)
Russia  
63 YBN
[1937 AD]
3622)
New York City NY, USA   
63 YBN
[1937 AD]
4843)
(Carnegie Institution of Washington) Cold Spring Harbor, N.Y., USA  
63 YBN
[1937 AD]
5029)
(University of Illinois) Urbana, Illinois  
63 YBN
[1937 AD]
5030)
(University of Illinois) Urbana, Illinois  
63 YBN
[1937 AD]
5151) The Nobel Prize in Physics 1958 is awarded jointly to Pavel Alekseyevich
Cherenkov, Il´ja Mikhailovich Frank and Igor Yevgenyevich Tamm "for the
discovery and the interpretation of the Cherenkov effect".
(Moscow University) Moscow, (Soviet Union) Russia  
63 YBN
[1937 AD]
5174)
(Observatory) Meudon, France  
63 YBN
[1937 AD]
5223) In 1932 Lipmann leaves Germany to Denmark to move away from the growth of
the Nazi movement.
In 1939 Lipmann moves from Denmark to the USA.

The Nobel Prize in Physiology or Medicine 1953 is divided equally between Hans
Adolf Krebs "for his discovery of the citric acid cycle" and Fritz Albert
Lipmann "for his discovery of co-enzyme A and its importance for intermediary
metabolism".
(Carlsberg Foundation) Copenhagen, Denmark  
63 YBN
[1937 AD]
5229)
(California Institute of Technology) Pasadena, California  
63 YBN
[1937 AD]
5266)
(University of Wisconsin) Madison, Wisconsin, USA  
63 YBN
[1937 AD]
5348)
(George Washington University) Washington, D.C., USA (presumably)  
63 YBN
[1937 AD]
6040)
Frankfurt/Main, Germany (first performance)  
62 YBN
[01/31/1938 AD]
5216) The Nobel Prize in Physics 1944 is awarded to Isidor Isaac Rabi "for his
resonance method for recording the magnetic properties of atomic nuclei".
(Columbia University) New York City, New York, USA  
62 YBN
[03/30/1938 AD]
5253)
(Kaiser Wilhelm-Institut fur Medizinische Forschung, Institut fur Chemie)
Heidelberg, Germany  
62 YBN
[04/12/1938 AD]
4794)
(University of Jena) Jena, Germany  
62 YBN
[04/??/1938 AD]
6271)
(E. I. duPont de Nemours & Company) WIlmington, Delaware, USA  
62 YBN
[06/01/1938 AD]
5544) Seaborg does work in connection with preparing plutonium for use in the
atomic bomb at the University of Chicago.
In 1951 the Nobel Prize in Chemistry is
awarded jointly to Edwin Mattison McMillan and Glenn Theodore Seaborg "for
their discoveries in the chemistry of the transuranium elements".
Seaborgium is
named in Seaborg's honor, making him the only person for whom a chemical
element is named during his lifetime.
(University of California) Berkeley, California, USA  
62 YBN
[06/16/1938 AD]
5382)
(California Institute of Technology) Pasadena, California  
62 YBN
[06/22/1938 AD]
5448)
(Berliner Medizinischen Gesellschaft/Berlin Medical Society) Berlin,
Germany  
62 YBN
[09/01/1938 AD]
5354)
(University of California) Berkeley, California, USA  
62 YBN
[09/01/1938 AD]
5355)
(University of California) Berkeley, California, USA  
62 YBN
[09/07/1938 AD]
5418) In 1933 Bethe leaves Germany for England when Hitler comes to power.
In 1935
Bethe accepts a post at Cornell University in the USA.
Bethe was engaged in the
development of the atomic bomb.

In 1967 the Nobel Prize in Physics is awarded to Hans Bethe "for his
contributions to the theory of nuclear reactions, especially his discoveries
concerning the energy production in stars".
(Kaiser Wilhelm Institute) Berlin, Germany (and Cornell University) Ithaca, New
York, USA  
62 YBN
[10/07/1938 AD]
6059)
(Metro-Goldwyn-Mayer Studios) Los Angeles, California, USA  
62 YBN
[10/25/1938 AD]
5352) In 1933 Elsasser leaves Germany with the rise of Hitler.
In 1936 Elsasser moves
to the USA.
(California Institute of Technology) Pasadena, California  
62 YBN
[11/24/1938 AD]
5464) In 1957 the Nobel Prize in Chemistry is awarded to Todd "for his work on
nucleotides and nucleotide co-enzymes".

(Determine what molecule Todd actually isolated.)
(Lister Institute) London, England  
62 YBN
[12/17/1938 AD]
5339)
(Cambridge University) Cambridge, England  
62 YBN
[12/22/1938 AD]
4926)
(Kaiser-Wilhelm-Instute fur Chemie in Berlin-Dahlem) Berlin, Germany  
62 YBN
[1938 AD]
4782)
  
62 YBN
[1938 AD]
4860)
(University of California at Berkeley) Berkeley, California, USA  
62 YBN
[1938 AD]
5056)
(Chemical Institute) Zürich, Switzerland  
62 YBN
[1938 AD]
5090)
(Mount Wilson) Mount Wilson, California, USA  
62 YBN
[1938 AD]
5533)
Peenemünde, Germany  
62 YBN
[1938 AD]
6077) "God Bless America", written by Irving Berlin (CE 1888-1989) in 1918 and
revised by him in 1938, sung by Kate Smith is recorded.

New York City, New York, USA (guess)  
62 YBN
[1938 AD]
6102) "Thanks for the Memory" with music composed by Ralph Rainger and lyrics
by Leo Robin is released. It is introduced in the 1938 film "The Big Broadcast
of 1938" by Shep Fields and His Orchestra with vocals by Bob Hope and Shirley
Ross.

(There may be many analogies to the secret of remote neuron reading and
writing. "It was fun while it lasted", "no harm done", "thoughts")

Los Angeles, California, USA (probably)  
61 YBN
[01/06/1939 AD]
5484)
(Stanford University) Stanford, California, USA  
61 YBN
[01/16/1939 AD]
4925) Frisch is a science writer on atomic physics for the public.
In 1933 when Hitler
comes to power, Frisch moves to England.
(Academy of Sciences) Stockholm, Sweden (Meitner), (University of Copenhagen),
Copenhagen, Denmark (Frisch)  
61 YBN
[01/19/1939 AD]
5658)
(University of Toronto) Toronto, Canada  
61 YBN
[01/30/1939 AD]
5193)
(Laboratoire de Chimie Nucleaire, College de France) Paris, France  
61 YBN
[02/18/1939 AD]
5493)
(Carnegie Institute of Washington) Washington, D. C, USA  
61 YBN
[03/08/1939 AD]
5194)
(Laboratoire de Chimie Nucleaire, College de France) Paris, France  
61 YBN
[03/20/1939 AD]
5347)
(George Washington University) Washington, D.C., USA  
61 YBN
[04/07/1939 AD]
5195)
(Laboratoire de Chimie Nucleaire, College de France) Paris, France  
61 YBN
[04/14/1939 AD]
5425)
(Merck and Company, Inc) Rahway, New Jersey, USA  
61 YBN
[04/17/1939 AD]
5255)
(Hospital of The Rockefeller Institute for Medical Research) New York City, New
York, USA  
61 YBN
[04/30/1939 AD]
5835)
(Westinghouse Electric Corporation) Mansfield, Ohio, USA  
61 YBN
[06/28/1939 AD]
5006)
(Princeton University) Princeton, New Jersey, USA  
61 YBN
[07/15/1939 AD]
5461) The Atomic Energy Commission pays Dunning $30,000 in lieu of patent
royalties.
(I wonder if the neuron reading and writing inventor, since not publicly
recognized, might have earned much more money from the public if the public was
told about their discovery.)
In 1936 Dunning builds Columbia University's first cyclotron.
(Columbia University) New York City, New York, USA  
61 YBN
[07/31/1939 AD]
5511) Alvarez works on radar and the atomic bomb during WW II.

Alvarez flies with the mission that drops the first atomic bomb—which is of
the original uranium shotgun design—on Hiroshima, releasing his
parachute-borne blast detectors from an accompanying B-29.

After the first Soviet atomic bomb is detected in September 1949, Alvarez and
Edward Teller, successfully advocate the development of a hydrogen bomb, over
the opposition of the General Advisory Committee (GAC) of the Atomic Energy
Commission, chaired by Robert Oppenheimer. (It seems possible that the hydrogen
bomb, in theory is a fraud, basically being simply a larger fission bomb - but
only the neuron transactions at the time, and more honest science will show the
truth. It seems unlikely that very much more light particles would be emitted
from hydrogen, which is a very low mass atom.)

In 1964, Alvarez patents a variable-power spherical lens, which allows for
variable-power spectacles that can be focused quickly and easily for near and
distant vision. (It seems possible that an artificial muscle lens could be
useful for a similar purpose, Possibly an electric motor lens could be helpful
too.)

In 1968, the Nobel Prize in Physics is awarded to Luis Alvarez "for his
decisive contributions to elementary particle physics, in particular the
discovery of a large number of resonance states, made possible through his
development of the technique of using hydrogen bubble chamber and data
analysis".

(Alvarez is notorious for doing experiments, I think with a ladder and
flour-filled skull, to supposedly prove that JFK was shot from behind and that
such a skull will fall forward when shot from behind. Later the camera-thought
net will show that Alvarez may have taken a large amount of money or supported
the Nazi-like killers of JFK, the Republicans, and so therefore worked to sell
the lie of Oswald to the excluded public. This is a definitely black mark on
his career, and calls into doubt much of his scientific work.)


(I don't think that there has ever been a more obvious example of corrupted and
dishonest claims published as "science" than the case of Luis Alvarez. Clearly
all of the work of Alvarez is highly suspect, since he openly served as an
active accessory to murder in the case of John Kennedy.)

(Then the Nobel prize is again clearly political - their statement begins with
"For his decisive contributions" which clearly implies "DC", which at the time
was under the control of the violent criminals who killed JFK, MLK, and has
just murdered Robert Kennedy a few months earlier. This shows again, that the
Nobel prize, many times, is the product of political pressure, and great
wealth, as opposed to actual science. In particular looking at Alvarez's sparse
and very potentially non-existant contributions to actual science.)

(Interesting that Alvarez takes out a number of patents, for radio echo
detection, a stablized zoom binocular, range finding device for a cart... and
given the neuron secret and doubts of being the first to develop technological
innovations, in addition to the limited time of the patent - I think it shows
an element of monetary greed, intellectual possessiveness - in particular when
so much information is written to our neurons from external sources - to claim
something as your own is - somewhat arrogant and unlikely to be true. There is
also the element of a person playing some gambling game to strike it rich by
having that chip on the correct number - given the years of protracted patent
trials - the corrupted neuron court system - patenting anything is worthless, I
think except perhaps to bring secret technology to the public in the form of a
public patent.)

(Looking at the thought-transactions of the time involving Alvarez is one way
of determining the validity of his scientific claims.)
(University of California) Berkeley, California, USA  
61 YBN
[08/27/1939 AD]
6269)
Marienehe, Germany  
61 YBN
[10/30/1939 AD]
5387) In 1933 Bloch leaves Germany when Hitler comes to power.
In 1934 Bloch moves to
the USA.
In 1952 the Nobel Prize in Physics is awarded jointly to Felix Bloch and
Edward Mills Purcell "for their development of new methods for nuclear magnetic
precision measurements and discoveries in connection therewith".
From 1954-1955 Bloch
serves as the first director-general of CERN, the multinational laboratory for
nuclear science at Geneva.
(Stanford University) Stanford, California, USA  
61 YBN
[1939 AD]
5138)
(St. Louis University) St. Louis, Missouri, USA  
61 YBN
[1939 AD]
5175)
(Observatory) Meudon, France  
61 YBN
[1939 AD]
5219) The Nobel Prize in Physiology or Medicine 1948 is awarded to Paul Müller
"for his discovery of the high efficiency of DDT as a contact poison against
several arthropods".
(Laboratory of the J.R. Geigy Dye-Factory Co.) Basel, Switzerland  
61 YBN
[1939 AD]
5248) The Nobel Prize in Physiology or Medicine 1967 is awarded jointly to
Ragnar Granit, Haldan Keffer Hartline and George Wald "for their discoveries
concerning the primary physiological and chemical visual processes in the eye".
(Perhaps this was a push to go public or generate some public research with
neuron reading and writing.)
(The Caroline Institute) Stockholm, Sweden (presumably)  
61 YBN
[1939 AD]
6056)
New York City, New York, USA (verify)  
60 YBN
[01/??/1940 AD]
5545)
(University of California) Berkeley, California, USA  
60 YBN
[02/01/1940 AD]
5246)
(University of Sheffield) Sheffield, England  
60 YBN
[02/29/1940 AD]
5579)
(University of California) Berkeley, California, USA  
60 YBN
[03/03/1940 AD]
5462)
(Columbia University) New York City, New York, USA  
60 YBN
[05/27/1940 AD]
5455) In 1951, the Nobel Prize in Chemistry is awarded jointly to Edwin
Mattison McMillan and Glenn Theodore Seaborg "for their discoveries in the
chemistry of the transuranium elements".
(University of California) Berkeley, California, USA  
60 YBN
[05/28/1940 AD]
5285)
(Westinghouse Research Laboratories) East Pittsburgh, Pennsylvania, USA  
60 YBN
[05/??/1940 AD]
5590)
England  
60 YBN
[06/14/1940 AD]
5568)
(Physico Technical Institute and Radium Institute) Leningrad, (U.S.S.R. now)
Russia  
60 YBN
[06/21/1940 AD]
5554)
(University of California) Berkeley, California, USA  
60 YBN
[07/16/1940 AD]
5365)
(University of California) Berkeley, California, USA  
60 YBN
[07/19/1940 AD]
5262) The Nobel Prize in Chemistry 1955 is awarded to Vincent du Vigneaud "for
his work on biochemically important sulphur compounds, especially for the first
synthesis of a polypeptide hormone".
(Cornell University Medical College) New York City, New York, USA  
60 YBN
[08/24/1940 AD]
5217) The Nobel Prize in Physiology or Medicine 1945 is awarded jointly to Sir
Alexander Fleming, Ernst Boris Chain and Sir Howard Walter Florey "for the
discovery of penicillin and its curative effect in various infectious
diseases".

In 1960 Florey is president of the Royal Society.
(University of Oxford) Oxford, England  
60 YBN
[08/29/1940 AD]
5438) In 1933 Goldmark moves to the USA.
After Goldmark becomes a vice president of
CBS in 1950, he develops the scanning system that allows the U.S. Lunar Orbiter
spacecraft (launched in 1966) to relay photographs 238,000 miles (380,000
kilometres) from the Moon of Earth to the planet Earth.
In 1971 Goldmark retired from
CBS to form his own company, Goldmark Communications Corporation.
(Columbia Broadcasting System, Inc.) New York City, New York, USA  
60 YBN
[11/13/1940 AD]
5524) Kerst worked at Los Alamos, New Mexico (CE 1943-45).
(General Electric Company) Scotia, New York, USA  
60 YBN
[12/02/1940 AD]
5439)
(Columbia Broadcasting System, Inc.) New York City, New York, USA  
60 YBN
[12/05/1940 AD]
5416)
(Oxford Univerity) Oxford, England  
60 YBN
[1940 AD]
4953) Karman establishes the theory of aeronautics.
Karman is largely responsible for the
California Institute of Technology's emergence as a top aeronautical research
center.
Karman is the son of professor of education who was knighted by Emperor
Francis Joseph I of Austria-Hungary for his reorganization of Hungarian
education.
(Guggenheim Aeronautic Laboratory) Pasadena, California, USA  
60 YBN
[1940 AD]
5423)
( University of Cincinnati) Cincinnati, Ohio, USA (presumably)  
60 YBN
[1940 AD]
5433)
  
60 YBN
[1940 AD]
5463)
Philadelphia, Pennsylvania, USA  
60 YBN
[1940 AD]
6078) "When You Wish upon a Star", written by Leigh Harline and Ned Washington
for Walt Disney's 1940 adaptation of Pinocchio, is recorded. The original
version of the song is sung by Cliff Edwards in the character of Jiminy Cricket
and is heard over the opening credits and again in the final scene of the film.
The song has since become the theme song to The Walt Disney Company.

Los Angeles, California, USA (presumably)  
59 YBN
[01/02/1941 AD]
6058)
(Decca Studios) Hollywood, California, USA  
59 YBN
[01/15/1941 AD]
5674) In 1936 Woodward gets a Ph.D. at age 20, and in 1938 is a postdoctoral
fellow on the faculty of Harvard at 21.
In 1950 Woodward becomes a full
professor at 33.
In 1964 Woodward wins the National Medal of Science Award.
In 1965
Robert B. Woodward wins the Nobel Prize in Chemistry "for his outstanding
achievements in the art of organic synthesis".
(Harvard University) Cambridge, Massachusetts, USA   
59 YBN
[01/23/1941 AD]
5580)
(University of California) Berkeley, California, USA  
59 YBN
[02/15/1941 AD]
6052)
New York City, New York, USA (verify)  
59 YBN
[02/24/1941 AD]
5283)
(University of California) Berkeley, California, USA  
59 YBN
[03/07/1941 AD]
5547)
(University of California) Berkeley, California, USA  
59 YBN
[03/22/1941 AD]
5271) The Nobel Prize in Physiology or Medicine 1966 is divided equally between
Peyton Rous "for his discovery of tumour-inducing viruses" and Charles Brenton
Huggins "for his discoveries concerning hormonal treatment of prostatic
cancer".
(University of Chicago) Chicago, Illinois, USA  
59 YBN
[05/07/1941 AD]
6074)
(RCA Victor's Bluebird) New York City, New York, USA  
59 YBN
[05/09/1941 AD]
6073) The song "God Bless the Child" (written by Billie Holiday and Arthur
Herzog, Jr. in 1939) is recorded.

(Part of me thinks that I should not include religious songs - because they are
not lyrically advances, and by promoting religions, in some sense, moving us
back to an out-house era- which is what many in the in-house might prefer.)

New York City, New York, USA  
59 YBN
[05/28/1941 AD]
5477)
(Polaroid Corporation) Cambridge, Massachusetts, USA  
59 YBN
[10/08/1941 AD]
5331) The Nobel Prize in Physiology or Medicine 1958 is divided, one half
jointly to George Wells Beadle and Edward Lawrie Tatum "for their discovery
that genes act by regulating definite chemical events" and the other half to
Joshua Lederberg "for his discoveries concerning genetic recombination and the
organization of the genetic material of bacteria".
(Stanford University) Stanford, California, USA  
59 YBN
[1941 AD]
5049) In 1952 Waksman wins the Nobel prize in medicine and physiology and gives
the prize money to a research foundation at Rutgers.
(Rutgers University) New Brunswick, New Jersey, USA  
59 YBN
[1941 AD]
5066) (Royal Observatory in Greenwich) Greenwich, England  
59 YBN
[1941 AD]
5149) In 1935 Minkowski leaves Nazi Germany for the USA with the help of Baade.
(Mount Wilson) Mount Wilson, California, USA  
59 YBN
[1941 AD]
5153) In 1956 Cournand shares the Nobel prize for physiology and medicine with
D. W. Richards, and Forssmann "for their discoveries concerning heart
catheterization and pathological changes in the circulatory system".
(Bellevue Hospital) New York City, New York, USA (Cournand)  
59 YBN
[1941 AD]
5224)
(Cornell University) Ithaca, New York, USA (presumably)  
59 YBN
[1941 AD]
5362)
(University of Saskatchewan) Saskatoon, Saskatchewan, Canada  
58 YBN
[02/16/1942 AD]
5529) In 1934 Bloch leaves Nazi Germany for Switzerland.
In 1936 Bloch moves to the USA.
In 1964
the Nobel Prize in Physiology or Medicine is awarded jointly to Konrad Bloch
and Feodor Lynen "for their discoveries concerning the mechanism and regulation
of the cholesterol and fatty acid metabolism".
(Columbia University) New York City, New York, USA  
58 YBN
[03/12/1942 AD]
5428) In 1969, the Nobel Prize in Physiology or Medicine is awarded jointly to
Max Delbrück, Alfred D. Hershey and Salvador E. Luria "for their discoveries
concerning the replication mechanism and the genetic structure of viruses".
(RCA Research Laboratories) Camden, New Jersey, USA  
58 YBN
[05/08/1942 AD]
5526)
Wheaton, Illinois, USA  
58 YBN
[05/29/1942 AD]
6071) The song "White Christmas" (written by Irving Berlin, 1940), sung by Bing
Crosby is recorded.

(It's amazing to me how people can still feel warm and fuzzy about Christmas
and Christianity in general, given the history of burning and torturing people.
Then interesting that this Christian song is written by a Jewish person who is
probably not Christian- but then Jesus, the founder of Christianity was Jewish.
We don't for example, see many Christian people showing enough tolerance to
write songs celebrating the customs of other religions. Perhaps I should focus
away from the songs based on the following of Jesus, but perhaps this reminds
people about the reality of the terrible influence on the lives of people on
earth, with the views that pleasure is bad, that its ok to lie, and to believe
ridiculously false claims of supernatural events.)

(Decca Records) New York City, New York, USA (probably)  
58 YBN
[07/??/1942 AD]
5363)
(University of Saskatchewan) Saskatoon, Saskatchewan, Canada  
58 YBN
[07/??/1942 AD]
5378)
(Princeton University) Princeton, New Jersey, USA  
58 YBN
[10/20/1942 AD]
5546)
(University of California) Berkeley, California, USA  
58 YBN
[10/??/1942 AD]
5534)
Peenemünde, Germany  
58 YBN
[11/04/1942 AD]
5289) Kaj Aage Gunnar Strand (CE 1907-2000) working under Peter Van de Kamp (CE
1901-1995), Dutch-US astronomer, claim to detect the first planet of a
different star (exoplanet). Small changes in the relative movement of the 61
Cygni system show the existence of a nonluminous mass eight times the mass of
Jupiter. This planet is detected at Sproul Observatory under the direction of
Van de Kamp.

Strand writes in the article "61 Cygni as a Triple System", in the
"Publications of the Astronomical Society of the Pacific":
"Extensive photographic
observations of high accuracy taken
at the Potsdam, Lick, and Sproul observatories
have revealed
perturbations in the orbital motion of 61 Cygni which are
caused by a third,
invisible member revolving around one of
the two visual components.
The only solution which
will satisfy the observed motions
gives the remarkably small mass of 1/60 that of the
sun or 16
times that of jupiter. With a mass considerably smaller than
the smallest
known stellar mass (Kruger 60 B = 0.14 0), the
dark companion must have an
intrinsic luminosity so extremely
low that we may consider it a planet rather than a
star. Thus
planetary motion has been found outside the solar system.
An extensive
investigation of the motion in the large orbit
is being carried out at the Sproul
Observatory. Though not
yet completed, the following dynamical elements represent
closely the
observed arc: P = 720 yrs., c = 0.40, a = 24".554,
T = 1690. These elements, together
with a parallax of 0".294,
give a total mass, Ma + Mb + Mc = 1.12 0.
The relative motion
of the perturbed component with re-
spect to the center of mass of itself and the
invisible component,
C, has the following dynamical elements : P = 4.9 yrs., e = 0.7,
a =
0".020 +- 0".003 (m.e.), T = 1942.0.
Since only the positions of A and B relative to
each other
are known, no decision can be made regarding which of the two
components
C is attached to. This is, however, of minor im-
portance for the determination of
the mass of C because A and B
C are nearly equal in mass. Using the masses
derived below we
obtain in either case, Mc : 0.016 0, hence C is revolving in
an
orbit with a semi—major axis of approximately 0".70 or 2.4
astronomical units. On
account of the orbit’s large eccentricity,
C, at periastron, is only 0.7 A.U.
from its visible companion.
The two visible components have visual magnitudes of 5.57
and
6.28 and spectra of type K6 and M0. With a parallax of
0".294 and reductions of
-0.80 and -1.2 mag. to bolometric
magnitudes we obtain the absolute bolometric magnitudes
of
7.1 and 7.4. From Eddington’s mass-luminosity curve the
masses are Ma = 0.58 0
and Mb = 0.55 0, hence the total
mass of the system is 1.15 0, practically identical
with the
value for the mass derived from the dynamical elements and
the same parallax.
Since
the total range in the radial velocity of the visual
components caused by the
invisible companion amounts to
about 1 km/sec, spectroscopic observations can
hardly be ex-
pected to reveal to which component C is attached.
The interpretation of the
observed motion in the small orbit
as the motion of the effective center of
light of two luminous
components with respect to their common center of gravity has
to be
rejected since the small orbit would require components
with nearly equal luminosity (Δm
= 0.10 at the most) to give
possible masses. This, however, would give a total mass
of no
less than 1.50 0 from Eddington’s curve or 0.38 0 in excess
of the total mass
found from the dynamical elements.
The photographic observations used in establishing
the per-
turbation are given below for the equinox of 2000 and with
corrections for the
perspective effect and proper motion to the
mean epoch 1930. If no perturbation is
accounted for, the
median mean error as computed from the residuals is increased
from 0".006
to 0".010.
A great part of the preliminary computations for the large
orbit was done by
Miss Virginia Burger who also made the
second complete set of measures of the
Sproul plates. I am
indebted to Dr. H. M. Jeffers for the use of the photographic
plates taken
at the Lick Observatory in 1942.".

This claim of a planet orbiting 61 Cygni is rejected in 1978.

(Make clear that this motion is detected from the measurement of photos of the
stars that captured visible light of the entire star, and not from the observed
movement of spectral lines from Doppler shift.)
(Sproul Observatory, Swartmore University), Swarthmore, Pennsylvania, USA  
58 YBN
[11/04/1942 AD]
5290)
(Sproul Observatory, Swartmore University), Swarthmore, Pennsylvania, USA  
58 YBN
[11/20/1942 AD]
5263)
(Cornell University Medical College) New York City, New York, USA  
58 YBN
[12/02/1942 AD]
5277)
(University of Chicago) Chicago, Illinois, USA  
58 YBN
[1942 AD]
5441)
(K. E. M. Medical College) Lucknow, India  
58 YBN
[1942 AD]
6038)
New York City, New York, USA (presumably)  
58 YBN
[1942 AD]
6042)
New York City, New York, USA (presumably)  
58 YBN
[1942 AD]
6043)
  
58 YBN
[1942 AD]
6054) Dizzy Gillespie (CE 1917-1993) composes "A Night In Tunesia". (verify)

Gillespie also records "Salt Peanuts" this year.

New York City, New York, USA (presumably)  
58 YBN
[1942 AD]
6079) "(There'll Be Bluebirds Over) The White Cliffs of Dover" (written by by
Walter Kent and Nat Burton, sung by Vera Lynn) is recorded.

  
57 YBN
[01/11/1943 AD]
5120)
(Mount Wilson Observatory) Mount Wilson, California, USA  
57 YBN
[05/14/1943 AD]
5264)
(Merck and Company, Inc.) Rahway, New Jersey, USA  
57 YBN
[05/25/1943 AD]
5578)
(University of Pennsylvania) Philadelphia, Pennsylvania, USA  
57 YBN
[09/??/1943 AD]
5280)
(University of Birmingham) Birmingham, England  
57 YBN
[11/01/1943 AD]
4916)
(Rockefeller Institute, now called Rockefeller University) New York City, New
York, USA  
57 YBN
[1943 AD]
4949)
(University of Zurich), Zurich, Switzerland  
57 YBN
[1943 AD]
5050)
(Rutgers University) New Brunswick, New Jersey, USA  
57 YBN
[1943 AD]
5399) In 1965, the Nobel Prize in Physics is awarded jointly to Sin-Itiro
Tomonaga, Julian Schwinger and Richard P. Feynman "for their fundamental work
in quantum electrodynamics, with deep-ploughing consequences for the physics of
elementary particles".

(I have a lot of doubts about this "QED" work, in particular am calling for all
thought-screen and relevent eye images to be released to the public to
determine what the neuron insider story was.)
(Tokyo Bunrika University) Tokyo, Japan  
57 YBN
[1943 AD]
5488)
Paris, France  
56 YBN
[04/25/1944 AD]
5454)
(Lebedev Institute of Physics) Moscow, (Soviet Union now) Russia  
56 YBN
[04/27/1944 AD]
5121)
(Mount Wilson Observatory) Mount Wilson, California, USA  
56 YBN
[05/08/1944 AD]
5527)
Wheaton, Illinois, USA  
56 YBN
[05/13/1944 AD]
5481) In 1952, the Nobel Prize in Chemistry is awarded jointly to Archer John
Porter Martin and Richard Laurence Millington Synge "for their invention of
partition chromatography".

(There is a remote possibility that relating this finding to "wool" is somehow
related to early images from the electron microscope Ernst Ruska paper in the
early 1930s of burned cotton fiber - a play on the word "woll" which may haev
been related to Wollaston and neuron writing - but it's very speculative from
an excluded perspective.)
(Wool Industries Research Association) Torridon, Headingley, Leeds, UK  
56 YBN
[07/03/1944 AD]
5414) In 1933 Chain sees the inevitable when Hitler comes to power and leaves
Germany to England.
(Rockefeller Institute of Medical Research) New York City, New York, USA  
56 YBN
[07/08/1944 AD]
5429) In 1969, the Nobel Prize in Physiology or Medicine is awarded jointly to
Max Delbrück, Alfred D. Hershey and Salvador E. Luria "for their discoveries
concerning the replication mechanism and the genetic structure of viruses".
(Indiana University) Bloomington, Indiana, USA  
56 YBN
[07/17/1944 AD]
5186)
(University of Michigan) Ann Arbor, Michigan, USA  
56 YBN
[08/21/1944 AD]
5389)
(McDonald Observatory, Mount Locke) Fort Davis, Texas, USA  
56 YBN
[11/08/1944 AD]
5675)
(Harvard University) Cambridge, Massachusetts, USA   
56 YBN
[11/11/1944 AD]
5227) The Nobel Prize in Physiology or Medicine 1974 is awarded jointly to
Albert Claude, Christian de Duve and George E. Palade "for their discoveries
concerning the structural and functional organization of the cell".
(Rockefeller Institute of Medical Research) New York City, New York, USA  
56 YBN
[12/19/1944 AD]
5209)
(University of Chicago) Chicago, illinois, USA  
56 YBN
[1944 AD]
5405)
(Columbia University) New York City, New York, USA  
56 YBN
[1944 AD]
6075) Bing Crosby records the song "I'll Be Seeing You" (written by Irving
Kahal and Sammy Fain in 1938).

(Possibly this relates to seeing direct to brain windows and how people always
watch their mates for most of their lives.)

New York City, New York, USA (guess)  
56 YBN
[1944 AD]
6076) Woody Guthrie (CE 1912-1967) records his folk song "This Land Is Your
Land" (written in 1940).

Guthrie tires of the radio overplaying Irving Berlin's "God Bless America", the
lyrics, which he thinks are unrealistic and complacent. Partly inspired by his
experiences during a cross-country trip and his distaste for "God Bless
America", Guthrie pens his most famous song, "This Land Is Your Land", in
February 1940, and subtitles it "God Blessed America." The melody is adapted
from an old gospel song "Oh My Loving Brother", best known as "When The World's
On Fire", sung by the country group The Carter Family.

New York City, New York, USA (presumably)  
55 YBN
[04/15/1945 AD]
5303)
(Iowa State College) Iowa, USA  
55 YBN
[06/30/1945 AD]
5334)
(Princeton University) Princeton, New Jersey, USA  
55 YBN
[06/??/1945 AD]
5699)
(University of Utrecht) Utrecht, Netherlands  
55 YBN
[07/13/1945 AD]
5426)
(Merck and Company, Inc) Rahway, New Jersey, USA  
55 YBN
[07/16/1945 AD]
5311)
(Alamogordo Test Range) Jornada del Muerto (Journey of Death) desert, New
Mexico, USA  
55 YBN
[08/31/1945 AD]
5692) In 1958, the Nobel Prize in Chemistry is awarded to Frederick Sanger "for
his work on the structure of proteins, especially that of insulin".

Sanger wins part of a second Nobel prize when in 1980, the Nobel Prize in
Chemistry is divided, one half awarded to Paul Berg "for his fundamental
studies of the biochemistry of nucleic acids, with particular regard to
recombinant-DNA",the other half jointly to Walter Gilbert and Frederick Sanger
"for their contributions concerning the determination of base sequences in
nucleic acids".
(Cambridge University) Cambridge, England  
55 YBN
[10/08/1945 AD]
6272) Microwave oven.

Dr. Percy Spencer, who had conducted research on radar vacuum tubes for the
military during World War II, recognizes the ability of microwave light to cook
food while working for Raytheon. Spencer finds that, when confined to a metal
enclosure, high-frequency radio light penetrates and excites certain type of
molecules, such as those found in food. Microwave light is strong enough to
cook food but not strong enough to alter its genetic structure or to make it
radioactive.

Raytheon patents the technology and soon develops microwave ovens capable of
cooking large quantities of food. Because manufacturing costs render them too
expensive for most consumers, these early ovens are used primarily by hospitals
and hotels that can afford them (initially at $3,000 US). By the late 1970s,
however, many companies will develop microwave ovens for home use, and the cost
will come down. Today, microwaves are a standard household appliance.

The basic design of a microwave oven is simple. The oven electronics are
located on the exterior casing, to which the oven cavity is bolted. A front
panel allows the user to program the microwave, and the door frame has a small
window to enable the food to be seen while it is cooking. Near the top of the
steel oven cavity is a magnetron—an electronic tube that produces
high-frequency microwave oscillations—which generates the microwave frequency
light particles. The microwave light particles are funneled through a metal
waveguide and into a stirrer fan, also positioned near the top of the cavity.
The fan distributes the microwave light evenly within the oven. Some
manufacturers use dual stirrer fans located on opposite walls to direct
microwaves to the cavity, while others use entry ports at the bottom of the
cavity, allowing microwaves to enter from both the top and bottom. In addition,
many ovens rotate food on a turntable.

(read relevant parts of patent.)

(It seems likely that this discovery, that microwave frequencies of light
particles can be used to remotely heat objects, was known many years earlier,
and was made public at this time for some reason, perhaps to sell microwave
ovens or because many neuron owners and consumers want to be able to use
microwave ovens in public. It is obvious how strong microwave beams can be used
to remotely and invisibly hurt or even murder a living object.)

(It's interesting that some microwave light must exit through the transparent
part of the glass, but it must be so small a quantity that it does not have any
heating effect on the human face.)

(Describe more how microwave frequencies of light are produced from alternating
current.)
(Raytheon Manufacturing Company) Newton, Massachusetts, USA  
55 YBN
[11/20/1945 AD]
5368)
(Karolinischen Institues) Stockholm, Sweden  
55 YBN
[11/30/1945 AD]
5549)
(University of California) Berkeley, California, USA  
55 YBN
[12/24/1945 AD]
5565) In 1952, the Nobel Prize in Physics is awarded jointly to Felix Bloch and
Edward Mills Purcell "for their development of new methods for nuclear magnetic
precision measurements and discoveries in connection therewith".
(Massachusetts Institute of Technology) Cambridge, Massachusetts, USA  
55 YBN
[1945 AD]
5312)
(Argonne Laboratory) Argonne, Illinois  
55 YBN
[1945 AD]
5410)
(Princeton University) Princeton, New Jersey, USA  
54 YBN
[01/10/1946 AD]
5528)
Fort Monmouth, New Jersey, USA  
54 YBN
[02/??/1946 AD]
5459)
(University of Pennsylvania) Philadelphia, Pennsylvania, USA  
54 YBN
[05/27/1946 AD]
5411)
(Princeton University) Princeton, New Jersey, USA  
54 YBN
[06/01/1946 AD]
5472) During the late 1950s, Libby and physicist Edward Teller, are both
prominent advocates of nuclear weapons testing, oppose Linus Pauling’s
petition for a ban on nuclear weapons. Libby builds a fallout shelter at his
house, an event that is widely publicized.

In 1960, the Nobel Prize in Chemistry is awarded to Willard F. Libby "for his
method to use carbon-14 for age determination in archaeology, geology,
geophysics, and other branches of science".
(University of Chicago) Chicago, Illinois, USA  
54 YBN
[06/14/1946 AD]
6072) "The Christmas Song" (commonly subtitled "Chestnuts Roasting on an Open
Fire") or, as it was originally subtitled, "Merry Christmas to You" (written by
Mel Tormé and Bob Wells in 1944) is recorded by Nat King Cole.

(WMCA Radio Studios) New York City, New York, USA  
54 YBN
[06/24/1946 AD]
5430) Delbrück leaves Germany after Hitler comes to power.
In 1937 Delbrück moves to
the USA.

In 1969, the Nobel Prize in Physiology or Medicine is awarded jointly to Max
Delbrück, Alfred D. Hershey and Salvador E. Luria "for their discoveries
concerning the replication mechanism and the genetic structure of viruses".
(Washington University) Saint Louis, Missouri, USA  
54 YBN
[07/15/1946 AD]
5373)
(U. S. Naval Research Laboratory) Washington, D. C., USA  
54 YBN
[08/22/1946 AD]
5697) In 1974, the Nobel Prize in Physics is awarded jointly to Sir Martin Ryle
and Antony Hewish "for their pioneering research in radio astrophysics: Ryle
for his observations and inventions, in particular of the aperture synthesis
technique, and Hewish for his decisive role in the discovery of pulsars".
(Cambridge University) Cambridge, England  
54 YBN
[08/??/1946 AD]
5314)
(University of Chicago) Chicago, illinois, USA  
54 YBN
[09/13/1946 AD]
5349)
(George Washington University) Washington, D.C., USA  
54 YBN
[09/17/1946 AD]
5742) In 1958, the Nobel Prize in Physiology or Medicine is divided, one half
jointly to George Wells Beadle and Edward Lawrie Tatum "for their discovery
that genes act by regulating definite chemical events" and the other half to
Joshua Lederberg "for his discoveries concerning genetic recombination and the
organization of the genetic material of bacteria".
(Yale University) New Haven, Connecticut, USA  
54 YBN
[10/10/1946 AD]
3848)
(White Sands proving area) New Mexico, USA  
54 YBN
[11/13/1946 AD]
5419)
(General Electric Research Laboratory) Schenectady, New York, USA  
54 YBN
[12/21/1946 AD]
5537)
(University of Rome) Rome, Italy  
54 YBN
[12/25/1946 AD]
5307)
(Now: Kurchatov Institute of Atomic Energy) Moscow, Russia (Soviet Union)  
54 YBN
[1946 AD]
5018)
(University of Oxford) Oxford, England  
54 YBN
[1946 AD]
5483)
  
53 YBN
[01/08/1947 AD]
5340)
(Imperial College of Science and Technology) London, England  
53 YBN
[01/09/1947 AD]
5443) In 1930 Zinn moves to the USA.
In 1939 Zinn is one of the US physicists that
confirm Meitner's theory of uranium fission.
Zinn is recruited by Enrico Fermi for the
Manhattan Project, and at the University of Chicago, Zinn is the person that
withdraws a control rod from the atomic pile, releasing the earth’s first
self-sustaining nuclear reaction. Zinn later supervises the dismantling of the
pile and its removal to the Argonne National Laboratory (near Chicago), of
which Zinn is the director of (1946–56).

In 1942 Zinn is the person that withdraws the control rod (a single rod?) in
the first nuclear reactor and makes it self sustaining.)

Zinn works on the development of the nuclear bomb.
Zinn becomes director of the
Argonne National Laboratories in Chicago.
Chicago, Illinois, USA  
53 YBN
[01/10/1947 AD]
5404)
(Harvard University) Cambridge, Massachusetts, USA   
53 YBN
[01/10/1947 AD]
5581) In 1951 Lovell supervises the construction of a 250-foot steerable radio
telescope at Jodrell Bank Experimental Station. This construction takes 6
years. The turret rack of a battleship is used to turn the dish. This telescope
is used to track Sputnik I using radio reflection (radar).

Cambridge radio astronomers under Antony Hewish discover pulsars, but are
limited to observing them only for the few minutes each day that the pulsars
are on the Cambridge meridian. The steerable Jodrell Bank telescope can observe
objects for as long as they are above the horizon. Of the 50 pulsars discovered
in the northern hemisphere before 1972, 27 are detected at Jodrell Bank.

Read more: http://www.answers.com/topic/bernard-lovell#ixzz1Ht46Okvj
(University of Manchester: Jodrell Bank) Cheshire, England  
53 YBN
[01/27/1947 AD]
5335)
(Argonne Laboratory) Argonne, Illinois, USA  
53 YBN
[02/07/1947 AD]
5337)
(Argonne Laboratory) Argonne, Illinois  
53 YBN
[02/08/1947 AD]
5338) The 1950 Nobel Prize in Physics is awarded to Cecil Powell "for his
development of the photographic method of studying nuclear processes and his
discoveries regarding mesons made with this method".

Powell is the founder of the Pugwash Movement, which supports peace and
scientific cooperation among all nations.

(To me, it seems like there can be many particles of different mass with more
or less photons in them, from the size of a photon on up (although clearly at
some point, a single collection of photons is probably not possible and divides
into two orbiting masses.) The finding of particles with charge is also a
specific thing. Are there particles of identical mass but one has a charge and
the other does not? Perhaps charge is the result of a range of mass for a
particle. These charged particles must not be part of atoms so how are they
produced? Can they be routinely produced in particle accelerators? If so, state
how. If they are produced by atoms in collisions might they be part of atoms?
or perhaps they are arranged at the time of the collision. If produced from
particles, might they be part of those particles? or again, made at the time of
the collision? Are there positive and negative muons and pions? What are the
other characteristics of these particles, and how are they deduced? If charged,
can they be substituted for electrons or protons in atoms?)
(what shape might a photon
be? a sphere, or a cube? some other shape? If a sphere, that has implications:
it means that there will always be empty space between photons, where a cube
allows the possibility of photons packed together with no empty space between.)
(University of Bristol) Bristol, England  
53 YBN
[02/17/1947 AD]
5478)
(Polaroid Corporation) Cambridge, Massachusetts, USA  
53 YBN
[03/17/1947 AD]
5588)
(General Electric Research Laboratory) Schenectady, New York, USA  
53 YBN
[06/18/1947 AD]
5402) In 1955, the Nobel Prize in Physics is divided equally between Willis
Eugene Lamb "for his discoveries concerning the fine structure of the hydrogen
spectrum" and Polykarp Kusch "for his precision determination of the magnetic
moment of the electron".
(Columbia University) New York City, New York, USA  
53 YBN
[06/26/1947 AD]
5550)
(University of California) Berkeley, California, USA  
53 YBN
[08/31/1947 AD]
5582)
(University of Manchester: Jodrell Bank) Cheshire, England  
53 YBN
[08/31/1947 AD]
5583)
(University of Manchester: Jodrell Bank) Cheshire, England  
53 YBN
[10/14/1947 AD]
5603)
(over Rogers Dry Lake) Edwards, California, USA  
53 YBN
[10/16/1947 AD]
5589)
(Johns Hopkins University) Silver Spring, Maryland, USA   
53 YBN
[12/20/1947 AD]
5543)
(University of Manchester) Manchester, England  
53 YBN
[1947 AD]
5225) Lipmann had discovered the new coenzyme in 1945.

While working on the role of phosphate in cell metabolism, Lipmann discovers
that a heat-stable factor is acting as a carrier of acetyl (CH3CO–) groups.
It can not be replaced by any other known cofactor. Lipmann eventually isolates
and identifies what he terms ‘cofactor A’, or CoA (the A stands for
acetylation), showing it to contain pantothenic acid (vitamin B2). Lipmann also
realizes that the two-carbon compound in the Krebs cycle that joins with
oxaloacetic acid to form citric acid is in fact acetyl CoA. The coenzyme will
soon be shown to have wider application than the Krebs cycle, when in 1950
Feodor Lynen finds that it plays a key role in the metabolism of fats.

Lipmann shows that coenzyme A contains vitamin B (panthothenic acid) and is the
reason vitamin B is required by a body to survive because it is needed for
digestion of molecules in food.
(Harvard University) Cambridge, Massachusetts, USA   
53 YBN
[1947 AD]
5241) Gabor leaves Germany for England with the coming to power of Hitler.
The Nobel
Prize in Physics 1971 is awarded to Dennis Gabor "for his invention and
development of the holographic method".
(Research Laboratory, British Thomson-Houston Co., Ltd.) Rugby, England  
53 YBN
[1947 AD]
5360)
(University of Grenoble) Grenoble, France  
53 YBN
[1947 AD]
5390)
(McDonald Observatory, Mount Locke) Fort Davis, Texas, USA  
53 YBN
[1947 AD]
5465)
(University of Cambridge) Cambridge, England  
53 YBN
[1947 AD]
5721)
  
52 YBN
[01/15/1948 AD]
5500)
(University of Cambridge) Cambridge, England  
52 YBN
[02/16/1948 AD]
5391)
(McDonald Observatory, Mount Locke) Fort Davis, Texas, USA  
52 YBN
[02/18/1948 AD]
5350)
(George Washington University) Washington, D.C., USA  
52 YBN
[03/10/1948 AD]
3337)
(Associated Electrical Industries) Aldermaston, Berkshire, England  
52 YBN
[03/12/1948 AD]
5538)
(University of California) Berkeley, California, USA  
52 YBN
[04/16/1948 AD]
5417) In 1930 Goeppert-Mayer moves to the USA.

In 1963, the Nobel Prize in Physics is divided, one half awarded to Eugene Paul
Wigner "for his contributions to the theory of the atomic nucleus and the
elementary particles, particularly through the discovery and application of
fundamental symmetry principles",the other half jointly to Maria Goeppert-Mayer
and J. Hans D. Jensen "for their discoveries concerning nuclear shell
structure".
(Argonne Laboratory) Argonne, Illinois  
52 YBN
[04/16/1948 AD]
5427)
(Merck and Company, Inc) Rahway, New Jersey, USA  
52 YBN
[06/17/1948 AD]
5295) Brattain works on the magnetic detection of submarines. (more detail. How
can submarines be detected magnetically? Would that not require a massive
magnet?)
Brattain, Bardeen and Shockley are all employees of Bell Laboratories (and so
must be fully aware of and receivers of neuron reading and writing
direct-to-brain windows.).

The Nobel Prize in Physics 1956 was awarded jointly to William Bradford
Shockley, John Bardeen and Walter Houser Brattain "for their researches on
semiconductors and their discovery of the transistor effect".

Bardeen will win a portion of a second Nobel prize in 1972 with Leon Cooper and
J. Robert Schrieffer for developing the theory of superconductivity (1957).

In the 1970s Shockley implies that genetic factors in intelligence are the
reason for the innate mental inferiority of black people, which is greeted by a
storm of disapproval by many people. Shockley writes in an article "Race and
Heredity": "...If my recommended research on such students confirms my estimate
of one I.Q. point increase for each 1 percent increase of Caucasian ancestry,
we must dismally predict that elimination of prejudice will not remedy the
tragic disadvantages of our black minority and must search for other solutions.
...". Shockley writes in "Race and Heredity": "...Within the last month or so,
the Idaho Legislature passed a sterilization law for mental defectives who,
after being sterilized, would then be permitted to leave institutions and
return to public life. Obviously, the representatives of the
American public are
prepared to take action. I doubt if the public feels that any
individual has a
right to produce children if the probability is high that a child will
never be
self-supporting. Although passed by 40 votes to 2 in the Idaho House,
this law passed
by only 18 to 16 in the Senate and was vetoed by the Governor.
I conjecture that lack of
knowledge of probably well-established facts on inheritance
of mental retardation has lead
to an unwise outcome. ...". (This is exactly what the Nazis believed and
carried through. Think of how easy it is to label a human a "mental defective"
- in particular with all the psychological labels in use today and the ease of
locking lawful people into psychiatric hospitals for 72 hour observation and
unconsensual treatments of druggings and restraints. Notice "outcome" in
near-perfect elitist neuron-speak. Note the emphasis that the post-steralized
people get to go free - apparently this time, at least initially, they won't be
euthanized. Perhaps AT&T and Stanford were not aware of these thoughts and
views of Shockley when they hired and maintained him for years, but then as
outsiders, unlike insiders, we have no idea who shares similar views around
us.)

In 1980 Shockley contributes some of his 72 year old sperm cells for the
purpose of freezing them for eventual use in the insemination of women of high
intelligence.

(The transistor must have been invented in the 1800s if not 1700s, for neuron
reading and writing to be invented in 1810. The transistor clearly helped in
the telephone company's efforts to put at least one microphone and camera (and
of course, telephone line) in every house. The transistor may have lowered the
size of perhaps the microphone, the photon capturing devices, the light
particle transmitters and receivers. Clearly some even smaller technology was
invented that has not been made public. The main aspect of the camera-thought
net is storage in my opinion. Because this is tremendous amounts of data. And
for that magnetic tape was the major product for decades. What replaced
magnetic tape was probably CDs and DVDs, but even now magnetic plastic tape is
still used. Perhaps something like flash drives with no mechanical moving parts
are ultimately the smallest and fastest storage. The mystery of where the
cameras, microphones, infrared thought seeing and sending devices are is a
great mystery, and their size too. It seems likely that these devices are
dust-sized or smaller, many probably hover and fly, and are completely
wireless, but many are probably stationary too. Perhaps ultimately they write
there data to the phone wires to send images and audio data back to the phone
company buildings, but probably many millions of invisible light particle
streams are the main method of information movement. Outside of this, very very
little is known by those of us in the excluded. These devices are clearly
powered by photons and need no wires. But it seems likely that the telephone
wire is used or was used in the past. It may be that tiny devices are necessary
to enter into the human body to precisely pinpoint neurons, but clearly simply
flying micrometer sized cameras and microphones can provide a lot of valuable
information and could fly or even drift into and out of buildings without being
detected. Probably much of this technology of sending and receiving devices and
information into and from people's houses with cameras, microphone, thought
seeing and sending was developed at Bell Labs. These devices can be used to
trigger sadness, happiness, crying, laughing, beam images, sounds, smells,
feelings (touch sensation and heat and pain sensations), muscle movement,
directly and have evolved to an amazing complexity and all secretly without the
public ever knowing. )
(As an relevent aside, the touch, heat and pain neurons
and associated sensations all evolved and contributed to an organism's chance
of survival.)
(Bell Telephone Laboratories) Murray Hill, New Jersey, USA  
52 YBN
[06/18/1948 AD]
5440)
(Columbia Broadcasting System, Inc.) New York City, New York, USA  
52 YBN
[07/13/1948 AD]
5704) Born in Vienna, Gold became a refugee from the Austrian Anschluss (the
political union of Nazi Germany and Austria in 1938).
(Cambridge University) Cambridge, England  
52 YBN
[07/29/1948 AD]
5400) In 1965, the Nobel Prize in Physics is awarded jointly to Sin-Itiro
Tomonaga, Julian Schwinger and Richard P. Feynman "for their fundamental work
in quantum electrodynamics, with deep-ploughing consequences for the physics of
elementary particles".

(I have a lot of doubts about this "QED" work, in particular am calling for all
thought-screen and relevent eye images to be released to the public to
determine what the neuron insider story was.)
(Harvard University) Cambridge, Massachusetts, USA   
52 YBN
[08/03/1948 AD]
5647)
(Cambridge University) Cambridge, England  
52 YBN
[09/27/1948 AD]
5644) In 1961, the Nobel Prize in Physics is divided equally between Robert
Hofstadter "for his pioneering studies of electron scattering in atomic nuclei
and for his thereby achieved discoveries concerning the structure of the
nucleons" and Rudolf Ludwig Mössbauer "for his researches concerning the
resonance absorption of gamma radiation and his discovery in this connection of
the effect which bears his name".
(Princeton University) Princeton, New Jersey, USA  
52 YBN
[09/27/1948 AD]
5645)
(Stanford University) Stanford, California, USA  
52 YBN
[10/02/1948 AD]
5326) Leakey is the son of a Christian missionary person, born and raised in
Kenya, then one of Britain's colonies.

"Consul" is the name of a popular chimp in the London zoo at this time.

(From the work of the Leakeys is much of the evidence that humans originated in
East Africa.)
Rusinga Island, Lake Victoria, Kenya, Africa  
52 YBN
[1948 AD]
4526) The 200-inch reflecting telescope on Palomar Mountain is completed.

In 1929 George Ellery Hale (CE 1868-1938), US astronomer had received a grant
from the Rockefeller foundation to build the Palomar telescope, a 200-inch
reflector, named "the Hale telescope". The Mount Palomar observatory also has a
48-inch camera of the kind invented by Schmidt. Hale does not live to see the
telescope completed in 1948 after 15 years of work, which WW 2 adds delays to.
The Soviet Union will build a 600 centimeter (236 inch) reflecting telescope
which is larger.

(Really amazing that so many major telescopes were all built by the influence
of Hale with the wealthy business people funding.)

(Palomar Observatory) Palomar Mountain, California, USA  
52 YBN
[1948 AD]
4774) Duggar enters the University of Alabama at age 14.
Duggar discovers
aureomycin at age 76.
(American Cyanamid Company) Ontario, Canada (presumably)  
52 YBN
[1948 AD]
5015)
(Mayo Foundation) Rochester, Minnesota, USA  
52 YBN
[1948 AD]
5159) The 1950 Nobel Prize in medicine and physiology is awarded jointly to
Edward Calvin Kendall, Tadeus Reichstein and Philip Showalter Hench "for their
discoveries relating to the hormones of the adrenal cortex, their structure and
biological effects".
  
52 YBN
[1948 AD]
5168)
(Boston Children's Hospital) Boston, Massachusetts, USA  
52 YBN
[1948 AD]
6273)
Nyon, Switzerland  
51 YBN
[01/28/1949 AD]
5169) The Nobel Prize in Physiology or Medicine 1954 is awarded jointly to John
Franklin Enders, Thomas Huckle Weller and Frederick Chapman Robbins "for their
discovery of the ability of poliomyelitis viruses to grow in cultures of
various types of tissue".

(verify original paper, read relevent parts)
(Boston Children's Hospital) Boston, Massachusetts, USA  
51 YBN
[02/02/1949 AD]
5494)
(Columbia University) New York City, New York, USA  
51 YBN
[03/??/1949 AD]
5375)
(Stanford University) Stanford, California, USA  
51 YBN
[04/??/1949 AD]
5135)
(Muscle Research at the Marine Biological Station) Woods Hole, Massachusetts.
USA  
51 YBN
[05/01/1949 AD]
5392)
(McDonald Observatory, Mount Locke) Fort Davis, Texas, USA  
51 YBN
[05/09/1949 AD]
5401) In 1965, the Nobel Prize in Physics is awarded jointly to Sin-Itiro
Tomonaga, Julian Schwinger and Richard P. Feynman "for their fundamental work
in quantum electrodynamics, with deep-ploughing consequences for the physics of
elementary particles".

(When we see all the thought-screen images and floating micro-meter camera
videos of history - probably our views of science will be changed in very large
ways - mostly we will see massive and widespread corruption and dishonesty.)
(Cornell University) Ithaca, New York, USA  
51 YBN
[06/26/1949 AD]
5122)
(Mount Wilson Observatory) Mount Wilson, California, USA  
51 YBN
[07/27/1949 AD]
6270)
Hatfield, England  
51 YBN
[08/01/1949 AD]
5406)
(Columbia University) New York City, New York, USA  
51 YBN
[08/06/1949 AD]
5198) The Nobel Prize in Chemistry 1967 is divided, one half awarded to Manfred
Eigen "for their studies of extremely fast chemical reactions, effected by
disturbing the equlibrium by means of very short pulses of energy",the other
half jointly to Ronald George Wreyford Norrish and George Porter "for their
studies of extremely fast chemical reactions, effected by disturbing the
equlibrium by means of very short pulses of energy".
(University of Cambridge) Cambridge, England  
51 YBN
[08/29/1949 AD]
5308)
Semipalatinsk, Russia (Soviet Union)  
51 YBN
[10/10/1949 AD]
5539)
(University of Rochester) Rochester, New York, USA  
51 YBN
[11/17/1949 AD]
5495)
(Columbia University) New York City, New York, USA  
51 YBN
[11/23/1949 AD]
5434) In 1957 Whipple heads the optical tracking system of the USA, where
observers trace comets and asteroids.
(Harvard University) Cambridge, Massachusetts, USA   
51 YBN
[11/24/1949 AD]
5228) The Nobel Prize in Physiology or Medicine 1960 is awarded jointly to Sir
Frank Macfarlane Burnet and Peter Brian Medawar "for discovery of acquired
immunological tolerance".
(Walter and Eliza Hall Institute of Medical Research) Melbourne,
Australia  
51 YBN
[11/25/1949 AD]
5258)
(California Institute of Technology) Pasadena, California  
51 YBN
[12/23/1949 AD]
5475)
(University of Chicago) Chicago, Illinois, USA  
51 YBN
[1949 AD]
5343)
(Johns Hopkins University) Baltimore, Maryland, USA  
51 YBN
[1949 AD]
5458)
(Istituto Superiore di Sanita/Superior Institute of Health) Rome, Italy  
51 YBN
[1949 AD]
5466)
(University of Cambridge) Cambridge, England  
51 YBN
[1949 AD]
5467) In 1964 the Nobel Prize in Chemistry is awarded to Dorothy Crowfoot
Hodgkin "for her determinations by X-ray techniques of the structures of
important biochemical substances".
(Oxford University) Oxford, England  
50 YBN
[01/13/1950 AD]
5237)
(Observatory at Leiden) Leiden, Netherlands  
50 YBN
[01/23/1950 AD]
5551)
(University of California) Berkeley, California, USA  
50 YBN
[03/07/1950 AD]
5127)
(University of Chicago) Chicago, Illinois, USA  
50 YBN
[03/15/1950 AD]
5552)
(University of California) Berkeley, California, USA  
50 YBN
[03/15/1950 AD]
5553)
(University of California) Berkeley, California, USA  
50 YBN
[03/22/1950 AD]
5393)
(Palomar Observatory) Mount Palomar, California, USA   
50 YBN
[04/17/1950 AD]
5687) Aage Bohr is the son of Niels Bohr.

In 1975, the Nobel Prize in Physics is awarded jointly to Aage Niels Bohr, Ben
Roy Mottelson and Leo James Rainwater "for the discovery of the connection
between collective motion and particle motion in atomic nuclei and the
development of the theory of the structure of the atomic nucleus based on this
connection".
(Columbia University) New York City, New York, USA  
50 YBN
[04/21/1950 AD]
5592)
(Johns Hopkins University) Silver Spring, Maryland, USA   
50 YBN
[04/26/1950 AD]
5542)
(University of Bristol) Bristol, England  
50 YBN
[05/??/1950 AD]
5480)
(Burden Neurological Institute) Bristol, England  
50 YBN
[08/02/1950 AD]
5773)
(University of Birmingham) Birmingham, England  
50 YBN
[08/??/1950 AD]
5696) In 1969, the Nobel Prize in Chemistry is awarded jointly to Derek H. R.
Barton and Odd Hassel "for their contributions to the development of the
concept of conformation and its application in chemistry".
(Harvard University) Cambridge, Massachusetts, USA   
50 YBN
[09/11/1950 AD]
5555)
(University of California) Berkeley, California, USA  
50 YBN
[10/12/1950 AD]
5395)
(Yerkes Observatory, University of Chicago) Williams Bay, Wisconsin, USA  
50 YBN
[10/16/1950 AD]
5259)
(California Institute of Technology) Pasadena, California  
50 YBN
[10/??/1950 AD]
5564)
(University of Manchester) Manchester, England  
50 YBN
[11/08/1950 AD]
5556)
(University of California) Berkeley, California, USA  
50 YBN
[1950 AD]
5297) The Nobel Prize in Physics 1966 is awarded to Alfred Kastler "for the
discovery and development of optical methods for studying Hertzian resonances
in atoms". According to Asimov, Townes had won in 1964 for his work on the
maser, and there was some dissatisfaction in France over the ignoring of
Kastler.
(Ecole Normale Superieure) Paris, France  
50 YBN
[1950 AD]
5298) The Nobel Prize in Physiology or Medicine 1965ias awarded jointly to
François Jacob, André Lwoff and Jacques Monod "for their discoveries
concerning genetic control of enzyme and virus synthesis".
(Institut Pasteur) Paris, France  
50 YBN
[1950 AD]
5379) In 1933 Chargaff moves to Paris on the coming of Hitler.
In 1935 Chargaff moves
to the USA.
(Columbia University) New York City, New York, USA  
50 YBN
[1950 AD]
5394)
(Yerkes Observatory) Williams Bay, Wisconsin, USA  
49 YBN
[03/??/1951 AD]
5460)
(Remington Rand) Philadelphia, Pennsylvania, USA  
49 YBN
[05/05/1951 AD]
5664)
(U. S. Naval Research Laboratory) Washington, D. C., USA  
49 YBN
[05/08/1951 AD]
5097)
(California Institute of Technology) Pasadena, California  
49 YBN
[06/05/1951 AD]
5482)
(National Institute for Medical Research) Mill Hill, London, UK  
49 YBN
[06/14/1951 AD]
5566)
(Harvard University) Cambridge, Massachusetts, USA   
49 YBN
[07/26/1951 AD]
5504) In 1964, the Nobel Prize in Physiology or Medicine is awarded jointly to
Konrad Bloch and Feodor Lynen "for their discoveries concerning the mechanism
and regulation of the cholesterol and fatty acid metabolism".
(University of Munich {Munchen}) Munich, Germany  
49 YBN
[08/27/1951 AD]
5516)
(Kaiser-Wilhelm Institute for Physical Chemistry and Electrochemistry)
Berlin-Dahlem, Germany  
49 YBN
[09/14/1951 AD]
5150)
(Palomar Observatory) Mount Palomar, California, USA   
49 YBN
[10/??/1951 AD]
5505)
(University of Munich {Munchen}) Munich, Germany (presumably)  
49 YBN
[11/11/1951 AD]
6274)
Los Angeles, California, USA[  
49 YBN
[11/29/1951 AD]
5610)
(US Department of Energy Nevada Proving Grounds) Nye County, Nevada, USA  
49 YBN
[12/13/1951 AD]
5313) The Nobel Prize in Physiology or Medicine for 1963 is awarded jointly to
Sir John Carew Eccles, Alan Lloyd Hodgkin and Andrew Fielding Huxley "for their
discoveries concerning the ionic mechanisms involved in excitation and
inhibition in the peripheral and central portions of the nerve cell membrane".
(Universities of Otago, Dunedin, and Australian National University, Canberra)
Canberra, Australia  
49 YBN
[12/20/1951 AD]
5444)
Arco, Idaho (verify)  
49 YBN
[1951 AD]
3338)
  
49 YBN
[1951 AD]
3339)
(University of Liverpool) Liverpool, England  
49 YBN
[1951 AD]
5091) (Mount Wilson) Mount Wilson, California, USA  
49 YBN
[1951 AD]
5129) After a few months of returning from Berkeley to Germany Hitler assumes
power and Simon resigns in June 1933 and accepts the invitation of F. A.
Lindemann (later Lord Cherwell) to work at the Clarendon Laboratory, Oxford,
where a small helium liquefaction plant has been set up by one of Simon’s
former co-workers. K. Mendelssohn.
(Clarendon Laboratory, Oxford University) Oxford, England  
49 YBN
[1951 AD]
5152)
Volga region, (Soviet Union) Russia  
49 YBN
[1951 AD]
5226)
(Harvard University) Cambridge, Massachusetts, USA   
49 YBN
[1951 AD]
5302)
  
49 YBN
[1951 AD]
5876)
(Carnegie Institute of Washington) Cold Spring Harbor, New York, USA  
48 YBN
[03/10/1952 AD]
5584) Andrew Huxley is the grandson of T. H. Huxley.

In 1963, the Nobel Prize in Physiology or Medicine is awarded jointly to Sir
John Carew Eccles, Alan Lloyd Hodgkin and Andrew Fielding Huxley "for their
discoveries concerning the ionic mechanisms involved in excitation and
inhibition in the peripheral and central portions of the nerve cell membrane".
(University of Cambridge) Cambridge, England  
48 YBN
[03/15/1952 AD]
5562) In 1979 the Nobel Prize in Chemistry is awarded jointly to Herbert C.
Brown and Georg Wittig "for their development of the use of boron- and
phosphorus-containing compounds, respectively, into important reagents in
organic synthesis".
(University of Chicago) Chicago, Illinois, USA  
48 YBN
[03/21/1952 AD]
5655)
(Bell Telephone Laboratories) Murray Hill, New Jersey, USA (presumably in New
Jersey)  
48 YBN
[03/22/1952 AD]
5570)
(University of California) Berkeley, California, USA  
48 YBN
[03/24/1952 AD]
5698) In 1973, the Nobel Prize in Chemistry is awarded jointly to Ernst Otto
Fischer and Geoffrey Wilkinson "for their pioneering work, performed
independently, on the chemistry of the organometallic, so called sandwich
compounds".
(Harvard University) Cambridge, Massachusetts, USA and (Technischen Hochschde)
Munich, Germany  
48 YBN
[04/02/1952 AD]
5743)
(University of Wisconsin) Madison, Wisconsin, USA and (Istituto Sicroterapico
Milanese) Milan, Italy  
48 YBN
[04/04/1952 AD]
5677)
(Harvard University) Cambridge, Massachusetts, USA   
48 YBN
[04/09/1952 AD]
5431)
(Carnegie Institute of Washington) Cold Spring Harbor, Long Island, New York,
USA  
48 YBN
[04/14/1952 AD]
5541)
(University of Chicago) Chicago, illinois, USA  
48 YBN
[05/19/1952 AD]
5218) The Nobel Prize in Chemistry 1963 is awarded jointly to Karl Ziegler and
Giulio Natta "for their discoveries in the field of the chemistry and
technology of high polymers".
(Max-Planck-Institute for Coal Research), Mulheim-Ruhr, Germany  
48 YBN
[06/12/1952 AD]
5757) In 1960, the Nobel Prize in Physics is awarded to Donald A. Glaser "for
the invention of the bubble chamber".
(University of Michigan) Ann Arbor, Michigan, USA  
48 YBN
[07/16/1952 AD]
5693) In 1958, the Nobel Prize in Chemistry is awarded to Frederick Sanger "for
his work on the structure of proteins, especially that of insulin".

Sanger wins part of a second Nobel prize when in 1980, the Nobel Prize in
Chemistry is divided, one half awarded to Paul Berg "for his fundamental
studies of the biochemistry of nucleic acids, with particular regard to
recombinant-DNA",the other half jointly to Walter Gilbert and Frederick Sanger
"for their contributions concerning the determination of base sequences in
nucleic acids".
(Cambridge University) Cambridge, England  
48 YBN
[07/19/1952 AD]
5442) In 1942, B. B. Bhatia had reported that the roots, leaves and juice of
the Rauwolfia serpentina plant lowers blood pressure.

Robert Wallace Wilkins (CE 1906-2003), US physician, and others will confirm
that this drug does lower blood pressure in the 1950s. Reserpine is the first
of the tranquilizers. The tranquilizers have an advantage over earlier
sedatives, like barbiturates in producing a calming effect without lowering
alertness or causing sleep.

(This drug will also be used to cure "neurosis", which is a very abstract label
often applied to perfectly healthful normal humans. In addition the
non-consensual drugging of people labeled with neurological disorders is wrong
in my view.)
(Ciba Aktiengesellschaft) Basel, Switzerland  
48 YBN
[08/13/1952 AD]
6061) The song "Hound Dog" recorded. "Hound Dog" is written by Jerry Leiber and
Mike Stoller and originally recorded by Willie Mae "Big Mama" Thornton.
Los Angeles, California, USA  
48 YBN
[08/??/1952 AD]
5591)
(Coast Guard Cutter ship   
48 YBN
[11/01/1952 AD]
5470) As a student Teller loses his right foot in a streetcar accident.
(Perhaps neuron writing is responsible for this.)
Teller leaves Germany when Hitler
came to power in 1933.
Teller works on the uranium fission bomb in Los Alamos, New
Mexico.

When others, such as Oppenheimer are not supportive of the development of the
hydrogen-fusion bomb (the H-bomb), Teller is one that strenuously is in favor
of such development.

At the U.S. government hearings held in 1954 to determine whether Oppenheimer
is a security risk, Teller testifies about his former chief: "...his actions
frankly appeared to me confused and complicated…I would personally feel more
secure if public matters could rest in other hands.". After the hearings,
Oppenheimer’s security clearance is revoked. Although Teller's testimony is
not the decisive factor in the decision to remove Oppenheimer's security
clearance, many prominent US nuclear physicists never forgive Teller for what
they view as his betrayal of Oppenheimer. (It seems somewhat trivial to me -
people should feel free to give their honest opinions - people can see and hear
thought now - it seems dishonest say something other than what you think and
believe.)

Teller opposes the 1963 Nuclear Test Ban Treaty, which bans nuclear weapons
testing in the atmosphere. (While testing in the earth atmosphere is clearly a
bad idea, testing of uranium fission chain reactions far away from earth to
propel ships I see as inevitable.)
(Elugelab Island in the Enewatak Atoll of the) Marshall Islands, Pacific
Ocean  
48 YBN
[12/01/1952 AD]
5782)
(University of Warsaw) Warsaw, Poland  
48 YBN
[1952 AD]
5123)
(Mount Wilson Observatory) Mount Wilson, California, USA  
48 YBN
[1952 AD]
5128)
(University of Chicago) Chicago, Illinois, USA  
48 YBN
[1952 AD]
5407)
(Columbia University) New York City, New York, USA  
48 YBN
[1952 AD]
5670) In 1980 the Nobel Prize in Physiology or Medicine is awarded jointly to
Baruj Benacerraf, Jean Dausset and George D. Snell "for their discoveries
concerning genetically determined structures on the cell surface that regulate
immunological reactions".
(Centre National de Transfusion Sanguine) Paris, France. (presumably)  
47 YBN
[02/13/1953 AD]
5786)
(University of Chicago) Chicago, Illinois, USA  
47 YBN
[02/26/1953 AD]
5396)
(Yerkes Observatory, University of Chicago) Williams Bay, Wisconsin, USA  
47 YBN
[02/26/1953 AD]
5397)
(Yerkes Observatory, University of Chicago) Williams Bay, Wisconsin, USA  
47 YBN
[03/28/1953 AD]
5643)
(University of Pittsburgh) Pittsburgh, Pennsylvania, USA  
47 YBN
[04/02/1953 AD]
5660) Watson entered the University of Chicago at age 15.
Wilkins had worked at the
University of California on the atomic bomb during World War II.
(State what war
reseach the universities were involved in during World War 2.)
In 1968 Watson
publishes "The Double Helix", an account of his DNA research.

Rosalind Franklin dies of cancer age 37 four years before Watson, Crick and
Wilkins are awarded the Nobel Prize. (It seems extremely unusual for a woman of
37 years old to die - perhaps she was murdered by remote galvanization.)

Asimov states that "Her own contribution to the double-helix structure of
nucleic acids has been consistently underestimated and some blame it on the
anti-woman prejudices of the English scientific establishment.". (Excluding and
oppressing women is not smart, in particular since that is rejecting half of
potential scientific contributors and allies.)

In 1980 Crick advances the idea of the seeding of life on planets, including
possibly earth from DNA of other star systems similar to the earlier theory of
Arrhenius.

In early 2007 Watson’s own genome is sequenced and made publicly available on
the Internet. Watson is the second person in history to have a personal genome
sequenced in its entirety. In October of the same year, Watson sparks
controversy by making a public statement referring to the idea that the
intelligence of Africans might not be the same as that of other peoples and
that intellectual differences between geographically separated peoples might
arise over time as a result of genetic divergence. Watson’s remarks are
immediately denounced as racist. Though he denies this charge, Watson resigns
from his position at Cold Spring Harbor and announces his retirement less than
two weeks later. On October 27, 2007 in a statement given to The Associated
Press, Dr. Watson states, “I cannot understand how I could have said what I
am quoted as having said. There is no scientific basis for such a belief.”
(Perhaps it was external neuron writing - many may wonder when there is not
external neuron writing involved in our thought processes.)
(Cavendish Laboratory, University of Cambridge) Cambridge, England  
47 YBN
[05/29/1953 AD]
5700)
Mount Everest, border between Nepal and the Tibet Autonomous Region of
China.  
47 YBN
[06/19/1953 AD]
5124)
(Mount Wilson Observatory) Mount Wilson, California, USA  
47 YBN
[07/09/1953 AD]
5690) In 1995, the Nobel Prize in Physics is awarded "for pioneering
experimental contributions to lepton physics" jointly with one half to Martin
L. Perl "for the discovery of the tau lepton" and with one half to Frederick
Reines "for the detection of the neutrino".

A lepton is any particles that participate in the supposed "weak nuclear
interaction", including the electron, the muon, and their associated
neutrinos.

From 1944 to 1959 Reines is a group leader at the Los Alamos Scientific
Laboratory, concerned with the physics and effects of nuclear explosions.

Cowan is on the faculty of the Catholic University of America in Washington, DC
from 1958 until his death in 1974.
(Los Alamos Scientific Laboratory, University of California) Los Alamos, New
Mexico, USA  
47 YBN
[07/12/1953 AD]
5781)
Bagneres de Bigorre, France  
47 YBN
[08/12/1953 AD]
5309)
Semipalatinsk, Russia (Soviet Union)  
47 YBN
[08/21/1953 AD]
5758)
(University of Chicago) Chicago, Illinois, USA  
47 YBN
[09/28/1953 AD]
5783)
(Institute for Advanced Study) Princeton, New Jersey, USA  
47 YBN
[09/30/1953 AD]
5671)
(Centre National de Transfusion Sanguine) Paris, France.  
47 YBN
[10/03/1953 AD]
5646) The Nobel Prize in Physiology or Medicine 1960 was awarded jointly to Sir
Frank Macfarlane Burnet and Peter Brian Medawar "for discovery of acquired
immunological tolerance".
(University College, University of London) London, England  
47 YBN
[10/22/1953 AD]
5351)
(George Washington University) Washington, D.C., USA  
47 YBN
[11/16/1953 AD]
5701) In 1976, the Nobel Prize in Chemistry is awarded to William Lipscomb "for
his studies on the structure of boranes illuminating problems of chemical
bonding".
(University of Minnesota) Minneapolis, Minnesota, USA  
47 YBN
[1953 AD]
5172)
(Harvard University) Cambridge, Massachusetts, USA (presumably)  
47 YBN
[1953 AD]
5669) Shklovskii is interested in the search for advanced life of other stars,
as are Sagan and Drake.

(Apparently Shklovsky suggested that a moon of Mars may be hollow - determine
what is the origin of this.)
(Moscow University) Moscow, U. S. S. R. (now Russia) (presumably)  
46 YBN
[01/21/1954 AD]
5230)
Thames River, Connecticut, USA  
46 YBN
[02/15/1954 AD]
6080) "Shake, Rattle and Roll" (by Charles E. Calhoun aka Jesse Stone in 1954)
is recorded by Big Joe Turner.

("Rattle" in this song may relate to telling about direct-to-brain windows.
That a woman should be in the kitchen is, kind of a backward - woman as a
servant- view. Then to know that Bill Haley and none other than Elvis more
famously cover this song.)

New York City, New York, USA  
46 YBN
[02/23/1954 AD]
5766) In the last days of WW2 the Nazis draft children and Eigen is briefly in
an antiaircraft gun crew.

In 1967 the Nobel Prize in Chemistry is divided, one half awarded to Manfred
Eigen "for their studies of extremely fast chemical reactions, effected by
disturbing the equlibrium by means of very short pulses of energy",the other
half jointly to Ronald George Wreyford Norrish and George Porter "for their
studies of extremely fast chemical reactions, effected by disturbing the
equlibrium by means of very short pulses of energy".

Eigen is not to be confused with and not the originator of an Eigenfunction,
Eigenstate, or Eigenvalue of mathematics and Schroedinger's wave functions.
"Eigen" in German means "own" and "eigenwert" means "intrinsically worth".
(more details)
(Max-Planck-Institut fur physikalische Chemie) Gottingen, Germany  
46 YBN
[03/05/1954 AD]
5586) In 1936 Perutz leaves Austria for England.
Perutz is interned as an enemy alien
during World War II.
In 1962 the Nobel Prize in Chemistry is awarded jointly to Max
Ferdinand Perutz and John Cowdery Kendrew "for their studies of the structures
of globular proteins".
(Cavendish Laboratory, University of Cambridge) Cambridge, England  
46 YBN
[03/30/1954 AD]
5503)
(University College) London, England  
46 YBN
[04/12/1954 AD]
6062)
(Pythian Temple studios) New York City, New York, USA  
46 YBN
[04/28/1954 AD]
5265)
(Cornell University Medical College) New York City, New York, USA  
46 YBN
[04/28/1954 AD]
5577)
(Carnegie Institute of Washington) Washington, D. C, USA  
46 YBN
[05/05/1954 AD]
5649) In 1948 Townes moves from Bell labs and joins the faculty at Columbia
University.

In 1964, the Nobel Prize in Physics is divided, one half awarded to Charles
Hard Townes "for fundamental work in the field of quantum electronics, which
has led to the construction of oscillators and amplifiers based on the
maser-laser principle",the other half jointly to Nicolay Gennadiyevich Basov
and Aleksandr Mikhailovich Prokhorov "for fundamental work in the field of
quantum electronics, which has led to the construction of oscillators and
amplifiers based on the maser-laser principle".

(Possibly the maser is not an invention, as much as it is an optimization of
the phenomenon of luminescence, or the regular frequencies that various atoms
and molecules emit absorbed light particles at.)
(Columbia University) New York City, New York, USA  
46 YBN
[06/10/1954 AD]
5691) Matthias moves from Germany to Switzerland when Hitler gains control of
Germany.
Matthias works at Bell Labs.
In 1961 Matthias works at the University of
California.
(Bell Telephone Laboratories) Murray Hill, New Jersey, USA  
46 YBN
[06/27/1954 AD]
5310)
Obninsk, Russia (Soviet Union)(verify)  
46 YBN
[07/05/1954 AD]
6081) Elvis Presley records his first single "That's All Right" (written and
originally performed by blues singer Arthur Crudup).

(Sun Records) Memphis, Tennessee, USA  
46 YBN
[07/06/1954 AD]
5520) In 1972, the Nobel Prize in Chemistry is divided, one half awarded to
Christian B. Anfinsen "for his work on ribonuclease, especially concerning the
connection between the amino acid sequence and the biologically active
conformation",the other half jointly to Stanford Moore and William H. Stein
"for their contribution to the understanding of the connection between chemical
structure and catalytic activity of the active centre of the ribonuclease
molecule".
(The Rockefeller Institute for Medical Research) New York City, New York,
USA  
46 YBN
[08/09/1954 AD]
5571)
(University of California) Berkeley, California, USA  
46 YBN
[08/17/1954 AD]
5594)
(University of Iowa) Iowa City, Iowa, USA  
46 YBN
[08/23/1954 AD]
5678)
(Harvard University) Cambridge, Massachusetts, USA   
46 YBN
[08/23/1954 AD]
5679)
(Harvard University) Cambridge, Massachusetts, USA   
46 YBN
[10/21/1954 AD]
5250)
(Kyoto University) Kyoto, Japan  
46 YBN
[12/10/1954 AD]
5315) The Nobel Prize in Chemistry 1963 was awarded jointly to Karl Ziegler and
Giulio Natta "for their discoveries in the field of the chemistry and
technology of high polymers". Natta is the first Italian to be awarded the
Nobel Prize for chemistry.
(Polytechnic of Milan) Milan, Italy  
46 YBN
[1954 AD]
4414)
(Moscow University) Moscow, Russia  
46 YBN
[1954 AD]
5170)
(Boston Children's Hospital) Boston, Massachusetts, USA (presumably)  
46 YBN
[1954 AD]
5322)
(Max Planck Institute) Munich, Germany  
46 YBN
[1954 AD]
5323)
(Worchester Foundation for Experimental Biology) Shrewsbury, Massachusetts,
USA  
45 YBN
[02/18/1955 AD]
5686) In 1974, the Nobel Prize in Physiology or Medicine is awarded jointly to
Electron-microscopists Albert Claude, Christian de Duve and George E. Palade
"for their discoveries concerning the structural and functional organization of
the cell".
(University of Louvain) Louvain, Belgium  
45 YBN
[02/26/1955 AD]
5661)
(Birkbeck College) London, England  
45 YBN
[04/07/1955 AD]
5384) In 1959 the Nobel Prize in Physiology or Medicine is awarded jointly to
Severo Ochoa and Arthur Kornberg "for their discovery of the mechanisms in the
biological synthesis of ribonucleic acid and deoxyribonucleic acid". It seems
clear that Marianne Grunberg-Manago should have had an equal share of the prize
with Ochoa.
(New York University) New York City, New York, USA  
45 YBN
[04/15/1955 AD]
5727)
(Carnegie Institute of Washington) Washington, D. C., USA  
45 YBN
[04/18/1955 AD]
5558)
(University of California) Berkeley, California, USA  
45 YBN
[06/17/1955 AD]
5491) Fraenkel-Conrat leaves Germany with the rise of Hitler.
(University of California) Berkeley, California, USA  
45 YBN
[06/20/1955 AD]
5557)
(University of California) Berkeley, California, USA  
45 YBN
[06/24/1955 AD]
5304)
(Iowa State College) Iowa, USA  
45 YBN
[08/20/1955 AD]
5468)
(Oxford University) Oxford, England  
45 YBN
[08/22/1955 AD]
5710) In 1977, the Nobel Prize in Physiology or Medicine is divided, one half
jointly to Roger Guillemin and Andrew V. Schally "for their discoveries
concerning the peptide hormone production of the brain" and the other half to
Rosalyn Yalow "for the development of radioimmunoassays of peptide hormones".
(Veterans Administration Hospital) Bronx, New York, USA  
45 YBN
[09/14/1955 AD]
6082) Little Richard records "Tutti-Frutti", (written by Little Richard and
Dorothy LaBostrie).

(Cosimo Matassa's studio) New Orleans, Louisiana, USA  
45 YBN
[10/24/1955 AD]
5366) Chamberlain worked on the Manhattan Project, a U.S. research project that
produced the first atom bombs.
(University of California) Berkeley, California, USA  
45 YBN
[11/03/1955 AD]
6096) "The Great Pretender" released (written by Buck Ram, performed by "The
Platters").

(Notice that this song has a verse and a bridge but no chorus. Notice too how
"pretending" is characteristic of those who must pretend that the do not see or
hear thought.)

Los Angeles, California, USA (guess)  
45 YBN
[11/15/1955 AD]
5567) With Soviet forces occupying Romania after World War 2, Palade leaves.
In 1974
the Nobel Prize in Physiology or Medicine is awarded jointly to Albert Claude,
Christian de Duve and George E. Palade "for their discoveries concerning the
structural and functional organization of the cell".
(Rockefeller Institute of Medical Research) New York City, New York, USA  
44 YBN
[01/04/1956 AD]
5305)
(Iowa State College) Iowa, USA  
44 YBN
[01/16/1956 AD]
5316)
(Polytechnic of Milan) Milan, Italy  
44 YBN
[01/23/1956 AD]
5762)
(University of Illinois) Champaign, Illinois, USA  
44 YBN
[02/18/1956 AD]
5760)
(Cambridge University) Cambridge, England  
44 YBN
[03/??/1956 AD]
5688) In 1959, the Nobel Prize in Physiology or Medicine is awarded jointly to
Severo Ochoa and Arthur Kornberg "for their discovery of the mechanisms in the
biological synthesis of ribonucleic acid and deoxyribonucleic acid".
(Washington University) Saint Louis, Missouri, USA  
44 YBN
[04/10/1956 AD]
5680)
(Harvard University) Cambridge, Massachusetts, USA   
44 YBN
[04/16/1956 AD]
6083)
(Chess Records) Chicago, Illinois, USA (presumably)  
44 YBN
[04/23/1956 AD]
5761) In the late 1960s O’Neill turned his attention to the feasibility of
space colonization. He designs a kilometre-long sealed cylinder, to be built
primarily of processed lunar materials and powered by solar energy, capable of
sustaining a human colony indefinitely at a point in space between the Earth
and the Moon. In his book The High Frontier (1978) O'Neill suggests that space
colonies might be the ultimate solution to such terrestrial problems as
pollution, overpopulation, and the energy shortage.
(Princeton University) Princeton, New Jersey, USA  
44 YBN
[04/??/1956 AD]
5082)
(Mount Wilson) Mount Wilson, California, USA  
44 YBN
[04/??/1956 AD]
5777) In 1944 Gell-Mann enters Yale on his 15th birthday.
Gell-Mann works under Fermi at
the University of Chicago.
In 1956 at 26 Gell-Mann is a full professor at the California
Institute of Technology.

In 1969, the Nobel Prize in Physics is awarded to Murray Gell-Mann "for his
contributions and discoveries concerning the classification of elementary
particles and their interactions". (This is a very theoretical contribution to
be awarded an entire Nobel prize for.) (Note that Gell-Mann's Nobel lecture
"Symmetry and Currents in Particle Physics" is apparently not published
anywhere.)
(Institute for Advanced Study) Princeton, New Jersey, USA  
44 YBN
[04/??/1956 AD]
6275)
San Carlos, California, USA (presumably)  
44 YBN
[06/22/1956 AD]
5723) Yang actively seeks out Fermi for his graduate work.
In 1957, the Nobel Prize
in Physics is awarded jointly to Chen Ning Yang and Tsung-Dao (T.D.) Lee "for
their penetrating investigation of the so-called parity laws which has led to
important discoveries regarding the elementary particles". This is the first
people of Chinese birth to win a Nobel prize. (Without any intent to be rude or
racist but simply honest, I have to put this Nobel prize choice up towards the
top of the most abstract, useless, highly theoretical, corrupt, and most likely
false so-called science contribution the Nobel Prize committee has ever
recognized. But clearly behind Egas Moniz's award - there are many others to
chose from. There are many useful physics applications that help life on earth
constantly being uncovered - in particular in product innovations and secret
neuron, transmutation and robot research - to name a few. But I do support the
effort of the Nobel committee to explore and award the science contributions of
people of non-European race, in the interest of racial variety, harmony and
equality.)
(Columbia University) New York City, New York, USA and (Brookhaven National
Laboratory) Upton, New York, USA  
44 YBN
[07/02/1956 AD]
6105) "Don't Be Cruel" is recorded by Elvis Presley and written by Otis
Blackwell in 1956.

New York City, New York, USA  
44 YBN
[07/06/1956 AD]
5702) In 1943 Bloembergen gets his master's degree at the University of
Utrecht, but in the same year the Nazis occupy the Netherlands and shut down
the Dutch universities.

In 1981, the Nobel Prize in Physics is divided, one half jointly to Nicolaas
Bloembergen and Arthur Leonard Schawlow "for their contribution to the
development of laser spectroscopy" and the other half to Kai M. Siegbahn "for
his contribution to the development of high-resolution electron spectroscopy".
(Harvard University) Cambridge, Massachusetts, USA   
44 YBN
[07/24/1956 AD]
5572)
(University of California) Berkeley, California, USA  
44 YBN
[10/25/1956 AD]
5424)
( University of Cincinnati) Cincinnati, Ohio, USA  
44 YBN
[11/16/1956 AD]
5573)
(University of California) Berkeley, California, USA  
44 YBN
[12/03/1956 AD]
5703)
(Bell Telephone Laboratories) Murray Hill, New Jersey, USA  
44 YBN
[1956 AD]
5130)
(Clarendon Laboratory, Oxford University) Oxford, England  
44 YBN
[1956 AD]
5261) Calder Hall is build under the guidance of (Baron) Christopher Hinton (CE
1901-1983).

The first uranium fission electricity generating plant is started in 1954 in
Obninsk in the Soviet Union.

(This structure uses the heat from uranium fission to heat water and uses the
steam to drive a generator which creates electric current. How is this current
stored? Describe how electrical power stations actually work, perhaps they just
create a continuous voltage difference with end users houses. How are changing
demands met? Are there temporary holding batteries, or are more electricity
producing devices turned on when more electricity is in use?))

In 1954 the first nuclear power plant was built in the Soviet Union.

(Show internal diagram of nuclear plant. Why is the traditional concrete
cylinder shape used? Does it serve a purpose? Is it necessary? It seems an
unnecessary waste.)
(Are there other designs beside uranium fission that can produce
more heat/free particle motion than is put in? Clearly burning trash and
containing all waste products in a closed vessel is one simple method of
producing heat and therefore electricity.)
(Calder Hall) Sellafield, England  
44 YBN
[1956 AD]
5317)
(University of Boston) Boston, Massachusetts, USA  
44 YBN
[1956 AD]
5408)
(Columbia University) New York City, New York, USA  
44 YBN
[1956 AD]
6248)
(The Boots Company) England  
43 YBN
[01/13/1957 AD]
6084) Elvis Presley records "All Shook Up" (written by Otis Blackwell).

(Possibly some lyrics have to do with remote neuron writing for example -
"please don't ask me what's on my mind".)

(Notice that this song contains a "bridge" {'Please don't ask what's on my
mind...'} although no chorus. Describe the history of the "bridge", which is
usually a "third" part besides the verse and chorus. I think the bridge goes
back at least to the 1920s and 1930s pop/show songs- for example "Swanny" has
possibly a bridge. In the 1950s popular music in the USA was mostly a verse, a
solo and maybe a chorus - with no bridge. But the bridge becomes a standard
part of most of the progressive - in terms of structure- pop music by the end
of the 1950s I think- verify.)
(Radio Recorders) Hollywood, California, USA  
43 YBN
[01/15/1957 AD]
5724)
(Columbia University) New York City, New York, USA and (National Bureau of
Standards) Washington, D. C., USA  
43 YBN
[01/16/1957 AD]
5711) Surprising that there is no Nobel Prize for this.
(Harvard University, Massachusetts General Hospital) Boston, Massachusetts, USA
  
43 YBN
[04/05/1957 AD]
5517)
(Pennsylvania State University) University park, Pennsylvania, USA  
43 YBN
[04/24/1957 AD]
5668) Chubb, Friedman, Kreplin, and Kupperian report as an abstract:
"A rocket
instrumented to measure Lyman alpha and X-rays
wasf ired while a smallf lare was in
progresso n June2 0, 1956.T he
rocket reached peak altitude about ten minutes
after the flare was
first seen visually. An unusually high X-ray flux was observed
extending
to a short wavelength limit of 3A. Although the flare
was still visible in Ha, Lyman
alpha was not appreciably different
from normal.".

(Solar flares appear to me to be openings in the crust of the star where high
densities of light particles escape. In this view, solar flares are like
volcanos, but perhaps molten liquid volcanos. Pehaps it is similar to a hot
chili or spaghetti sauce where air bubbles escape.)
(U. S. Naval Research Laboratory) Washington, D. C., USA  
43 YBN
[04/??/1957 AD]
6110) The Kingsmen release their version of Richard Berry's song "Louie Louie".

(Northwestern, Inc., Motion Pictures and Recording) Portland, Oregon, USA  
43 YBN
[05/03/1957 AD]
6085) "Jailhouse Rock" (written by Jerry Leiber and Mike Stoller, sung by Elvis
Presley) is recorded.

(Note that this song has eletric guitar. Note also that there are also lyrics
that relate to same-gender romantic relationships, "Number 47 said to number 3,
you're the cutest jail-bird I ever did see", which indicates a progressive view
in the US. Note "Nix" may relate to "Nixon". Note that the media format is a 45
rpm plastic record.)

(Radio Recorders) Hollywood, California, USA (presumably)  
43 YBN
[05/27/1957 AD]
6107) "That'll Be The Day" is released (written by Buddy Holly, Jerry Allison,
Norman Petty).

(This could relate to the neuron secret - "lie" is a keyword, - and after
hundreds of years of the lie, most people may believe that seeing and hearing
thought may never go public. Even that might have been enough to galvanize
Holly's plane.)

Clovis, New Mexico, USA (recorded)  
43 YBN
[07/08/1957 AD]
5296) The Nobel Prize in Physics 1972 was awarded jointly to John Bardeen, Leon
Neil Cooper and John Robert Schrieffer "for their jointly developed theory of
superconductivity, usually called the BCS-theory". This is the second Nobel
Prize Bardeen has won a part of, the first time for developing the first
semiconductor transistor - while Lilienfeld, the inventor of the first
solid-state transistor receives no share of a single prize.
(The Nobel prize
committee, I think has somewhat short vision in awarding the same person a
second time, in particular for something so apparently insignificant,
nonpractical and speculatively theoretical.)
(University of Illinois) Urbana, Illinois, USA  
43 YBN
[09/19/1957 AD]
5611)
(US Department of Energy Nevada Proving Grounds) Nye County, Nevada, USA  
43 YBN
[10/04/1957 AD]
5486)
(Baikonur Cosmodrome at Tyuratam, 370 km southwest of the small town of
Baikonur) Kazakhstan (, Soviet Union)  
43 YBN
[10/10/1957 AD]
5689)
(Washington University) Saint Louis, Missouri, USA  
43 YBN
[10/11/1957 AD]
5740) In 1973, the Nobel Prize in Physics is divided, one half jointly to Leo
Esaki and Ivar Giaever "for their experimental discoveries regarding tunneling
phenomena in semiconductors and superconductors, respectively" and the other
half to Brian David Josephson "for his theoretical predictions of the
properties of a supercurrent through a tunnel barrier, in particular those
phenomena which are generally known as the Josephson effects".
(Tokyo Tsushin Kogyo, Limited) Shinagawa, Tokyo, Japan  
43 YBN
[10/23/1957 AD]
5432) In 1944, Leloir, in conflict with the president, Juan Peron, goes into
exile in the United States.

In 1970, Luis Leloir is awarded the Nobel Prize in Chemistry "for his discovery
of sugar nucleotides and their role in the biosynthesis of carbohydrates", and
is the first Argentinian person to be awarded the Nobel Prize.
(INSTITUTIO DE INVESTIGACIONES BIOQUIMICAS) Buenos Aires, Argentina, South
America  
43 YBN
[10/23/1957 AD]
5659)
(Western Reserve University) Cleveland, Ohio, USA  
43 YBN
[11/03/1957 AD]
5487)
(Baikonur Cosmodrome) Tyuratam, Kazakhstan (, Soviet Union)  
43 YBN
[12/??/1957 AD]
4895)
Chicago, Illinois, USA  
43 YBN
[1957 AD]
5409)
(Columbia University) New York City, New York, USA  
43 YBN
[1957 AD]
5506) Calvin spent two years two years on the Manhattan Project (the atomic
bomb).

In 1961, the Nobel Prize in Chemistry 1961 is awarded to Melvin Calvin "for his
research on the carbon dioxide assimilation in plants".
(University of California) Berkeley, California, USA  
43 YBN
[1957 AD]
6086) Danny & the Juniors record the song "At the Hop" (written by Arthur
Singer, John Medora and David White).

(Three and four-part vocal harmony, popular in the 1940s and 50s mostly passes
out of popularity by 1960. The Beatles use two-part vocal harmony in many songs
written during the 1960s.)

  
43 YBN
[1957 AD]
6106) "Wake Up Little Susie" written by Felice and Boudleaux Bryant, and
performed by "The Everly Brothers" is published.

New York City, New York, USA (presumably)  
42 YBN
[01/06/1958 AD]
6087) Chuck Berry writes and records "Johnny B. Goode".

(Chess Studios) Chicago, Illinois, USA  
42 YBN
[01/09/1958 AD]
5772) In 1961, the Nobel Prize in Physics is divided equally between Robert
Hofstadter "for his pioneering studies of electron scattering in atomic nuclei
and for his thereby achieved discoveries concerning the structure of the
nucleons" and Rudolf Ludwig Mössbauer "for his researches concerning the
resonance absorption of gamma radiation and his discovery in this connection of
the effect which bears his name".
(Institut fur Physik im Max-Planck-Institut fur medizinische Forschung
{Institute of Physics at the Max Planck Institute for Medical Research})
Heidelberg, Germany  
42 YBN
[01/31/1958 AD]
5593)
(Johns Hopkins University) Silver Spring, Maryland, USA   
42 YBN
[03/06/1958 AD]
6088) The Everly Brothers record "All I Have to Do Is Dream" (written by
husband and wife Felice and Boudleaux Bryant).
(RCA Studio) Nashville, Tennessee, USA  
42 YBN
[04/28/1958 AD]
5607)
(85 nm NE of) Enewetak Atoll, Marshall Islands, Pacific Ocean  
42 YBN
[05/01/1958 AD]
5608)
(National Academy of Science and American Physical Society joint meeting)
Washington, D. C., USA  
42 YBN
[05/??/1958 AD]
5321)
(Max Planck Institute) Munich, Germany  
42 YBN
[06/06/1958 AD]
5559)
(University of California) Berkeley, California, USA  
42 YBN
[06/06/1958 AD]
5561)
(University of California) Berkeley, California, USA  
42 YBN
[07/??/1958 AD]
5521)
(The Rockefeller Institute for Medical Research) New York City, New York,
USA  
42 YBN
[08/01/1958 AD]
5450)
(Technischen Hochschule/Technical University) Berlin, Germany  
42 YBN
[08/01/1958 AD]
5606)
(Johnson Island) Pacific Ocean  
42 YBN
[08/03/1958 AD]
5231)
North Pole  
42 YBN
[08/26/1958 AD]
5650)
(Bell Telephone Laboratories) Murray Hill, New Jersey, USA  
42 YBN
[09/29/1958 AD]
5651)
(Columbia University) New York City, New York, USA  
42 YBN
[10/08/1958 AD]
195) Swedish Doctor Dr. Rune Elmqvist develops the first fully internal (fully
implantable) pacemaker.
(Elema-Schnander) Sweden  
42 YBN
[11/14/1958 AD]
5535)
(Florida State University) Tallahassee, Florida, USA  
42 YBN
[1958 AD]
6044)
Hollywood, California, USA (verify)  
42 YBN
[1958 AD]
6068) "He's Got the Whole World in His Hands", a spiritual song that is written
by Obie Phillis, a Cherokee Native American person, written while serving in
WWII. The song makes the popular song charts in a 1958 version by English
singer Laurie London with the Geoff Love Orchestra.

(Capitol Records) Hollywood, California ,USA (possibly, or possibly in
England)  
41 YBN
[01/03/1959 AD]
5596)
(Baikonur Cosmodrome) Tyuratam, Kazakhstan (was Soviet Union)  
41 YBN
[01/27/1959 AD]
5672)
  
41 YBN
[02/14/1959 AD]
5595)
(State University of Iowa) Iowa City, Iowa, USA  
41 YBN
[02/18/1959 AD]
6089) Ray Charles writes and records "What'd I Say".

(Is the first popular recording with amplified (electric) piano?)
New York City, New York, USA (guess)  
41 YBN
[03/03/1959 AD]
5732) From 1949 to 1984 Anderson worked at Bell Telephone Laboratories in
Murray Hill, New Jersey. (So clearly Anderson must have seen thought-screens
and regularly received direct-to-brain windows.)

In 1977, the Nobel Prize in Physics is awarded jointly to Philip Warren
Anderson, Sir Nevill Francis Mott and John Hasbrouck van Vleck "for their
fundamental theoretical investigations of the electronic structure of magnetic
and disordered systems".
(to me this seems, overvaluing a theory that may not be entirely
accurate, and is of limited practical importance currently.)
(Bell Telephone Laboratories) Murray Hill, New Jersey, USA  
41 YBN
[04/??/1959 AD]
5787)
(National Radio Astronomy Observatory) Green Bank, West Virginia, USA  
41 YBN
[05/01/1959 AD]
5536)
(Florida State University) Tallahassee, Florida, USA  
41 YBN
[07/17/1959 AD]
5327)
Olduvai Gorge, Tanganyika Territory, Africa  
41 YBN
[07/22/1959 AD]
5489)
Paris, France  
41 YBN
[09/14/1959 AD]
5597)
(Baikonur Cosmodrome) Tyuratam, Kazakhstan (was Soviet Union)  
41 YBN
[10/18/1959 AD]
5598)
(Baikonur Cosmodrome) Tyuratam, Kazakhstan (was Soviet Union)  
41 YBN
[11/05/1959 AD]
191) A device inside the body controlled remotely. An artificial heart
pacemaker is remotely controlled with radio.
(Yale University School of Medicine) New Haven, New Jersey, USA  
41 YBN
[11/??/1959 AD]
5767)
(University of Chicago) Chicago, Illinois, USA  
41 YBN
[12/07/1959 AD]
5372) Bruno Benedetto Rossi (CE 1905-1994) Italian-US physicist, and Riccardo
Giacconi publishes the first report of an x-ray telescope, 60 years after
x-rays were first made public by Rontgen in 1895.

In 1896 Seneca Egbert had detected x-rays in sunlight. So the Sun, moon, and
bright stars and planets could have been examined for x-ray light without any
magnification. But it seems unlikely that reflecting and or refracting x-ray
light is so difficult. Karl Manne Georg Siegbahn (SEGBoN) (CE 1886-1978),
Swedish physicist, reflected and refracted x-rays with glass in 1925.

In October 1962 Rossi et. al, will report observing x-ray sources from outside
the solar system.

Giacconi and Rossi report in an article "A 'Telescope' for Soft X-Ray
Astronomy" in the "Journal of Geophysical Research":
"With the development of artificial
satellites
it has become possible to observe soft X rays
from extraterrestrial sources. The
purpose of
this note is to describe the design of an X-ray
'telescope' and to analyze
some of its characteristics.
The instrument consists of one or several
paraboIic mirrorso n whicht he X
rays impinging
at nearly grazing angles undergo total reflection.
The possibility of using optics of
this type has
been discussed in the past in connection with
X-ray microscopy
(Kirkpatrick and Pattee,1 957;
Trurnit, 1946). These discussionhsa ve remained
of purely
theoreticailn terest,o wingt o the difficulty
of constructinsgu fficientlya ccuratem
irrors
of the extremely small physical dimensions required.
These difficulties, however, are
greatly
reduced in the construction of large mirrors.
Let us consider first a narrow section of
a
parabolic mirror whose plane is at the distance
from the focus of the paraboloid, F
(Fig. 1).
Rays parallel to the axis are concentratedb y
the mirror into a point at F.
It can be shown
that, on a first approximation, a parallel beam
of rays, forming a small
angle, a, with the axis,
are concentratedo n a circle in the focal plane
whose center is at
F and whose radius is R =
Thus, a detector of radius R in the focal plane
will record
all rays striking the mirror and forming
with the axis angles less than R/1.
In the actual
design of the instrument it is
necessary to consider two limitations: (1) for
each
wavelength, and for each material, the
angle of the incident rays with the
reflecting
surface must be smaller than a certain value,
0, so that the reflection coefficient
will be of the
order of unity; (2) in general, the design of the
satellite will impose
an upper limit to the distance,
l, between the detector and the outer edge
of the mirror.
The problem
is to obtain the maximum area
of collection consistent with these limitations.
Figure 2
illustrates two possible solutions
...
Table 1 gives numerical values of these
quantities for silver mirrors and for X rays
of
about 10 A wavelength. The maximum angle
of incidence, •, has been set equal to 2
ø, correspondingt
o a minimum coefficiento f reflection
of 50 per cent. In Figure 3, the efficiencyo f
light
collection for different wavelengths is plotted.
Utilizing Table 1, we may estimate the
minimum
detectable intensity of X rays. The main
source of background is cosmic radiation,
whose
omnidirectional intensity in outer space is of the
ordero f 2 particles/cm2 s ec.W
e believe,h owever,
that it is possible to design a detector whose
efficiency is 10 • times
higher for X rays than
for cosmic-ray particles. Then we see that the
minimum detectable
intensity is of the order of
10 -• quantum/cm • sec for an angular resolution
of 10 -•
radian.
The prime advantages of the instrument are
the large area of collection, the high
resolution,
and the large signal-to-noiser atio. Among the
obvious applications are a detailed
analysis of
the distribution of X-ray sources on the solar
disk and the solar corona,
and a search for weak
X-ray sourcesf,o r examplei n the Crab Nebula.
We are at present
consideringt he possibility,
originally suggested y Wolter (1952) for microscopes,
of using multiple
total reflections to
construct image-forming X-ray telescopes.".

(Kind of shocking that x-rays were identified in 1895 but are supposedly not
used in astronomy until 1960 65 years later. And what technical difficulty is
involved? Simply putting a metal plate over the photographic plate in the
telescope.)

(From the figures and text, it's not clear what the difference between this
telescope design and a simple reflecting telescope design is.)
(Massachusetts Institute of Technology) Cambridge, Massachusetts, USA  
40 YBN
[01/23/1960 AD]
4992)
Marianas Trench of the Pacific Ocean  
40 YBN
[02/13/1960 AD]
5587)
(Cavendish Laboratory, University of Cambridge) Cambridge, England  
40 YBN
[03/09/1960 AD]
5774)
(Harvard University) Cambridge, Massachusetts, USA   
40 YBN
[04/14/1960 AD]
6142) Sam Cooke releases "Wonderful_World".

(This song contains a good and smart pro-science, pro-education message.)

  
40 YBN
[04/19/1960 AD]
5665)
(U. S. Naval Research Laboratory) Washington, D. C., USA  
40 YBN
[04/22/1960 AD]
5768) Theodore Harold Maiman (CE 1927-2007), US physicist invents the first
laser (light amplification by stimulated emission of radiation). Townes the
inventor of the maser had predicted that the maser principle could be applied
to wavelengths of light even as short as those of visible light. Maiman makes
use of the three-level principle worked out by Bloembergen and designs a ruby
cylinder with its ends carefully polished flat and parallel and covered with
silver coatings. Light is fed into the ruby cylinder from a flash lamp and the
ruby emits monochromatic (of a single wavelength) and coherent (all the beams
in a single direction) light. These coherent beams of light can travel
thousands of miles without spreading very far apart, and can be focused into so
small a space as to deliver energy (or light particle density) with the
temperature equivalent of the surface of the sun.

The laser has found numerous practical uses, ranging from delicate surgery to
measuring the distance between the Earth and the Moon.

The first large-scale application for lasers is the laser scanner for automated
checkout in supermarkets, which develops in the mid-1970s and becomes common a
few years later. Compact disc audio players and laser printers for personal
computers soon follow.

The first claim of a successful x-ray laser is by Ilyukhin et al in 1977.

Maimon publishes this first in "Physical Review Letters" as "Optical and
Microwave-Optical Experiments in Ruby". He writes:
" Several recent papers have
reported optical and microwave-optical measurements in ruby (Cr+++ in Al2O3).
We wish to report here some new experiments concerning the fluorescent
relaxation processes in this crystal. Reported here also are the first
observations of ground-state population changes in ruby due to optical
excitation and the detection of optical absorption between two excited states
in this crystal.
The predominant processes which ensue in a fluorescent material when
it is irradiated at an appropriate wavelength are shown in Fig. 1. W13 is the
induced transition probability per unit time due to an exciting radiation and
the Smn are decay rates which incclude both radiative and nonradiative
processes. In this crystal S21 is easily obtained from the decay rate of the
fluorescent level (2E) after an exciting source is turned off. The lifetime for
this process is about 5 msec. Varsanyu, Wood, and Schawlow have further
demonstrated that this lifetime is almost entirely due to spontaneous emission,
i.e., S21 is approximately the Einstein A coefficient A21.
An approximate value
for the rate S32 was obtained in the following way. A crystal of ruby was
irradiated with 5600A radiation causing absorption into the lower band
(4A2-4F2). The sample used was a one-centimeter cube cut from a boule of
standard pink ruby supplied by the Linde Company, with a concentration of
approximately 0.05 weight percent of Cr2O3 to Al2O3. Two components of
radiation re-emitted from the crystal were observed in a direction
perpendicular to the exciting beam: that due to re-emission of the incoming
radiation (spontaneous decay from 4F2) and fluorescence (spontaeous decay from
2E). The intensity of the first component is proportional to hv31N3A31, where
A31 is the A coefficient for 4F2-4A2 and is calculated from measurements of
absorption coefficient and line width for this transition (A31 ~3x105/sec).
Similarly the fluorescent intensity is proportional to hv21N2A21. Bby a
measurement of the ratio of these two components and the use of an auxiliary
condition applicable to steady=state condirions N2S21=N3S32 and also the use of
the approximation S21=A21, we find S32 ~2x107/sec.
A measurement of fluorescent quantum
efficiency, i.e., the number of fluorescent quanta emitted compared to the
number absorbed by the crystal frmo the exciting beam, yielded a value near
unity. This result reconfirms the evidence that the life of level 2 is near
radiative and also implies that S32>>S31. The experiment was not accurate
enough to yield a precise value byt does indicate that the nonradiative process
(S31-A31) < 4x106/sec.
Calculations utilizing the previous results indicated that
population changes in the ground state of ruby due to optical excitation would
be easily observed. This conclusion was verified in the following experiments.
A ruby crystal was mounted between parallel silvered plates to form a microwave
cavity resonant at the ground-state zero-field splitting (11.3 kMc/sec). About
half the cavity losses were due to magnetic absorption as evidenced by an
increase in vacity Q when a small magnet was brough near the ruby. The
reflection coefficient of the cavity was monitored on an oscilloscope while a
short pulse (200 usec) of light from a flash tube irradiated the crystal. The
magnitude of the microwave magnetic absorption was observed to decrease
abruptly and then return to equilibrium with a time constant of about 5 msec
(see Fig. 2). We attribute this effect to temporary depletion of this ground
state population with subsequent decay back from the fluorescent level. The
experiment was performed at room temperature where the thermal relaxation times
in the ground state of ruby are the order of a microsecond; in the time scale
of the experiment, therefore, boltzmann equilibrium in these levels is
maintained.
A repetition of the above experiment at liquid helium temperatures is being
planned. At this temperature we would expect to be able to observe directly any
preferential depopulation of the ground sublevels due to polarized light and
also any preferential repopulation of these levels since the thermal
relatzations times would then be 30-100 msec.
To verify further the depletion of
ground-state population observed in the previous experiment an independent
measurement was made. A beam of monochromatic light of wavelength 4100 A was
transmitted through a ruby crystal and partially absorbed due to the transition
4A2-4F1. When the intense pulse of radiation at 5600 A was turned on, the 4100A
radiation passing through the crystal absruptly increased and subsequently
decayed in about 5 msec just as the microwave signal in the previous
experiment. This result was expected since the temporary reduction in
ground-state population caused the crystal to become more transparent to the
4100A radiation until the fluorescent level decayed to normal. In both
experiments a population change of about 3% was estimated.
An unexpected result was
observed when the probe wavelength was changed from 4100 A to 3600 A. In this
case a decrease in light intensity emerging from the crystal was observed. This
implies that the crystal became more absorbing even thought the ground-state
population was decreased. We can explain this last effect when it is realized
that 3600A radiation can cause transitions from the fluorescent level (2E) to a
high lying charge transfer band (not shown in the figure). Consequently, we
conclude that we were observing transitions between two excited optical states.
The fact that the abruptly increased 3600A absorption also decayed with a
5-msec time constant is consistent with and strengthens the above conclusion.
..
.".

In his April 1961 patent application "Ruby Laser Systems". Maimon writes:
"This
invention relates to the generation, amplification, and utilization of
electromagnetic waves in the infrared, visible and. ultraviolet portion of the
spectrum, and more specifically to lasers and laser systems. A laser, the term
being an acronym for light amplification by stimulated emission of radiation,
is a device capable of generating or amplifying coherent light. The principle
of operation is similar to that of a maser and is therefore also referred to as
an optical maser.

Much effort has been expended in the fields of electronics and physics in
attempts to generate or amplify coherent light. Such an achievement, it was
known, would make available a vast new region of the electromagnetic spectrum
for a multitude of purposes including communications and metrology
(measurements) applications. Such coherent light would have the properties of
being monochromatic and of having its component waves propa gating in phase
with each other. Thus, as at radio or microwave frequencies, a great deal of
energy could be concentrated at or extremely near to a single frequency and be
utilized in methods analogous to those at radio frequencies.

Ordinary techniques of generating or amplifying electromagnetic waves,
including microwave maser techniques, cannot be extended usefully into the
optical frequencies because such techniques require components, such as maser
cavities, for supporting wave oscillations which must have physical dimensions
of the order of a wavelength. Obviously, such components can neither be
manufactured nor meaningfully utilized at optical frequencies where the
wavelengths are of the order of atomic dimensions. When it is attempted to use
cavities which have dimensions corresponding to a large number of wavelengths,
many modes arc supported, coherence is degraded, and impracticably large
sources of pumping power arc required.

A laser has been proposed by Schawlow and Townes, sec United States Patent No.
2,929,922, issued March 22, 1960, which suggests using as the negative
temperature medium certain gaseous state materials such as alkali metal vapors.
Such materials may be shown to have energy levels in their atomic systems
corresponding to appropriate optical frequencies for absorbing optical pump
energy to invert the population from the stable equilibrium state and thus
provide the material with what is known as a negative temperature or excited,
nonequilibrium state. Then by stimulation or spontaneous relaxation the atomic
system falls back to Its normal equilibrium state by one or more steps emitting
energy of certain optical frequencies.

Such proposed gaseous state devices are of great interest as theoretical models
and represent significant academic advances, however, they have not been shown
to provide a net generation or amplification of light. In addition, the
structure of gaseous state systems is complex and requires the maintenance of
critical vapor pressures and temperatures. Impurities in the gas is another
very serious problem. The inter-atomic spacing of the gas severely limits the
efficiency of coupling between the stimulated

emission and a coherent wave propagating through the medium. In addition, the
frequency of operation of any given gas laser may be effectively tuned only by
Stark or Zeeman effects which can provide a tuning range of only

g approximately 5X1010 cycles per second. Further, the construction of a gas
cell is extremely critical in that the end plates must be highly reflective and
perfectly parallel so that the many reflections required because of the low
density gaseous material will be accomplished.

j0 It is therefore an object, of the present invention to provide an operable,
low noise. ;fficient laser.

It is another object to provide a laser which is mechanically stable and of
noncritical construction.

It is another object to provide a laser which operates

15 at room temperature or cryogenic temperatures for additional simplicity and
even greater flexibility in design parameters.

It is another object to provide a laser which does not require critical vacuum
or vapor pressure techniques and 20 which operates in a medium of high
dielectric constant.

It is another object to provide a laser capable of much higher power handling.

It Is another object to provide a laser which is tunable over aproximately a 5x
1011 cycles per second range. 25 It is another object to provide an optical
radar system utilizing the advantages of a laser.

Briefly, these and other objects are achieved in accordance with the present
invention in a system including a solid state negative temperature medium. 80
In one example a segment of solid state active laser material such as a
cylindrical ruby (Ala03 doped with Cra03) rod with reflecting coating at each
end is coaxially placed in a helical flash lamp. White light or, predominantly,
the green and blue components thereof, is absorbed 36 by the ruby, and red
light is emitted therefrom and coupled out of the system through a hole in the
reflective coating at one end of the rod. The reflecting coatings provide a
regeneration related to the coupling between the reflecting wave, traveling
back and forth many times, and 40 the emitting atoms. In other words, a
resonating, standing wave is provided which derives energy from the negative
temperature dielectric. Thus the rod may be considered as a resonator having
different Q's for different modes of oscillation. The mode having the highest Q
46 corresponds to waves traveling nearly parallel to the rod axis since it
supplies the highest degree of regeneration. This effect causes the output to
be an extremely parallel beam so that it propagates immense distances without
spreading. Inherent in the regeneration process is the 60 coherent
amplification of an extremely narrow band of frequencies, thus providing a
monochromatic output. Additional discussion of principles of operation, of
further objects and advantages, including uses, and of other examples will be
presented below in connection with a 68 description of the accompanying
drawings in which:

FIG. 1 is an energy level diagram for the atoms of a substance exhibiting laser
properties;

FIQ.2 is a schematic diagram illustrating optical pumping of negative
temperature laser material; fl0 FIG. 3 is a schematic diagram of means for
optically pumping the laser material with sunlight energy;

FIG. 4 is a schematic diagram of one embodiment of the present invention which
utilizes a helical gas-filled flash tube for optical pumping of the laser
material;

FIG. 5 is a diagram of an alternative embodiment utilizing a hollow gas-filled
cylinder for optical pumping of th; laser material;

FIG. 6 is another embodiment of the present invention 70 which utilizes a
hollow cylindrical gas-filled optical pumping means which is radially separated
from the active laser material by a fluorescent material;
FIG. 7 is an energy level
diagram illustrating the method of operation of the embodiment of FIG. 6;

FIG. 8 is a schematic diagram of an embodiment of the invention in which the
active laser material is a hollow cylinder surrounding a cylindrical gas-filled
flash tube, the entire assembly being surrounded by a second hollow cylinder of
coolant of a high index of refraction;

FIG. 9 is a cut-away view of an embodiment of the present invention in which
the laser material is refrigerated;

FIG. 10 is a diagram of a segment of laser material; FIG. 11 is a diagram of a
coated segment of laser material;

FIG. 12 is a diagram of a segment of laser material which is surrounded by a
coolant having a high index of refraction;

FIG. 13 is a schematic diagram of a portion of a laser system illustrating the
use of an interferometer;

FIGS. 14 and 15 are schematic diagrams illustrating additional types of
interferometers;

FIGS. 16 and 17 are diagrams of a laser system in which the optical pump
utilizes an exploding wire; and

FIG. 18 is a schematic diagram of a practical colidar system utilizing a
laser.

The laser to be herein below described utilizes the interaction of
electromagnetic radiation with a material having an appropriate set of discrete
energy levels. Consider, for example, a pair of such levels with energies Ei
and E3 where E3 is greater than Ej. An electromagnetic wave of frequency

= ——

where h is Planck's constant, coupled to the system stimulates both absorption
and emission. In other words, atoms in (he lower level make transitions to the
upper level, each absorbing energy E=»>ji and similarly upper level atoms arc
stimulated downwardly, each of these giving up energy to the wave by radiating
a like quantum of energy. The net absorption of the radiating wave interacting
with the system is proportional to Ni-Nj where Ni and N3 arc respectively the
number of atoms in these two levels. Since in thermal equilibrium Ni is greater
than N3 the indicated difference is positive and a wave propagating the length
of the material is attenuated.

In a substance with a third energy level Ej higher than either of the other two
levels, energy can be supplied to the system by a radiating wave of frequency

If other parameters, and, in particular, relaxation times, in the material arc
suitably related, an inverted population will be produced such that N3 is
greater than Ht; then the net interaction with a radiating wave of frequency
1-3, is emission and the wave is amplified. Also, by providing a feedback
mechanism oscillation can be produced.

Visible light covers the electromagnetic spectrum approximately 4x10'* cycles
per second, that is, red light to approximately 7.5xlOu cycles per second which
is violet light. In substance as described above with energy levels such that
*n lies in this frequency range can therefore amplify or generate visible
light.
Referring specifically to FIG. 1 an energy level diagram is illustrated for the
atoms of a material such as AljOj which may exhibit laser action in accordance
with the present invention. Level 1 may be considered the ground slate
corresponding to Ei and region 3 in the relatively high energy state
corresponding to E3 which is actually a broadband of energy levels rather than
a discrete energy level. The atoms, or ions, as the case may be, are excited or
pumped from the level 1 to the region 3 by means of an optical pumping source
having the energies or frequencies i-ji corresponding to the diffcrenco between
the energy of level 1 and those of the levels throughout region

53,115

4

3. Because of the broadness of region 3, doping atoms, which for exampie may be
the chromium atoms, may accept pumping energy over a correspondingly broad
band. The atoms thus excited may then decay from the

5 region 3 back to the ground state or, alternatively, they may decay to level
2 corresponding to E3 and thence to level 1. The latter course is definitely
the favored one and the atoms in decaying to level 2 do not emit energy. In
other words, it is a radiationless thermal type of transitu tion which funnels
the energy distributed in the board region 3 into the very narrow region 2. The
energy level 2 is in fact a single energy level, or may in the presence of a
magnetic field be a doublet, and the atoms of this state of excitation will
emit the correspondingly discrete frc

15 quency »31 corresponding to the difference between level 2 and level 1 that
is Er-^-i when they are appropriately stimulated or triggered to do so.
Further, when an appropriate stimulation does occur, the atoms in the
particular segment of laser material will fall together or emit

20 their radiated energy coherently with each other and with the stimulating
wave. Thus it may be seen that the mechanism is a funneling of energy from a
broadband incoherent source into a discrete frequency that is monochromatic
coherent radiation.

25 Referring to FIG. 2, there is shown a schematic representation of the
mechanism of optically pumping the atoms such as those of chromium in a ruby
rod 10. A light pump 12 emits a high intensity "white" light or, in this
example, it may be broadly green, toward the ruby rod

30 10. The broadband light thus radiated includes at least some light in the
frequency range *31. This light is absorbed by the ruby rod and causes the
doping atoms to be excited in the energy state represented by region 3 of the
diagram of FIG. 1. This excitation is equivalent

35 to an inversion of the population of the chromium atoms as discussed above.
The excited atoms then relax by thermal processes down to the level 2 and may
remain there until stimulated to fall to the level 1 thereby emitting the
desired monochromatic light of frequency v2]. This stimu

40 lation may be by an external source of radiation at frequency yllt or it may
be triggered spontaneously as by optical noise. When the energy at frequency
»3t is emitted from the atoms in the ruby rod 10 it causes a wave to propagate
through the rod and if the wave is parallel

45 to the axis it may reflect repeatedly from the ends of the rod. If the rod
is of an appropriate length a standing wave 14 may be set up. In either event
the repeated reflections through the material stimulate the emission of
substantially all the atoms from level 2 to their ground

50 state level 1. The emission of the enrcgy at frequency v2i combines in phase
with the stimulating wave 14 thus adding coherently with it. This energy may
then be coupled out of the rod as a beam 16 which is monochromatic at frequenvy
v3I and which is traveling or prop

55 agating in a direction parallel to the axis of the ruby rod 10.

FIG. 3 illustrates an example of the invention in which the light pump 12 of
FIG. 2 is the sun or some other source of parallel "white" light. The lens 18
focuses the

60 light so that it is of relatively high intensity in a region 20 where an
element of active laser material 22 is disposed. An auxiliary mirror 24 may
further intensify the light in the region of the laser material. The mirror 24
may be a spherical reflector which merely sends the un

65 absorbed, pumping light back through the focal point of the lens 18 and
thence through the laser material 22 a second time.

Referring to FIG. 4, an embodiment of the invention is shown in which an active
laser rod 26 is disposed

70 coaxially within a helical gas-filled flash tube 28. The ends of the rod 26
may be suitably plated as by a partial coating of silver in order to provide
the rcptitive reflections of the monochromatic emitted light. The system of
stimulation is so efficient that a plating 26 which will provide

75 approximately 10 percent reflection is adequate. One end
of the rod 30 has a
nonreflective opening 32 in the end plating to provide unobstructed passage of
the coherent monochromatic beam 34 as shown. A power supply 36 provides the
flashing energy for the tube 28. An outer enclosing cylinder 38 is provided
which has a very highly 6 reflecting inner surface for reflecting the pumping
energy repeatedly through the rod 26 for improved efficiency of the system as
compared with operation when the light energy of the tube 28 is permitted to
radiate indefinitely in all directions causing only a fraction of its energy to
1Q pass through the rod 26.

Referring to FIG. 5, a rod of active laser material 40 is shown which again has
reflectively coated ends 42, 44 wilh an opening 46 in the plating 44 to permit
passage of the laser output beam 48. The light pump in this example 15 is a
hollow cylinder 50 which is coaxially disposed about the rod 42 with the radial
space therebetween being filled with a flashing gas 52. Appropriate electrodes
54 and 56 at opposite ends of the cylinder 50 are energized by a power supply
58 to cause the gas 52 to emit high intensity 20 "while" light when desired.
Again, the inner surface of the cylinder 50 is highly reflective for added
efficiency of the light pump mechanism.

FIG. 6 illustrates an embodiment of the invention in which a rod 60 of active
laser material similar to rods 26 25 and 42 is disposed coaxially within a
hollow flash tube 62. The radial space between the rod 60 and the flash tube 62
is filled with a fluorescent material 64, such as fluorescein. The fluorescent
material efficiently absorbs the "white" light emitted by the flash tube 62 and
re-emits predomi- 30 nantly green light which is more efficiently absorbed by
the laser rod 60. Thus, as illustrated in FIG. 7, the broadband "while" light
66 is directed into the fluorescein which re-emits incoherent green light
predominantly in the region 3 of ihe material discussed in cpnneclion with 3a
tlie description of FIG. 1. Thus the fluorescein effectively funnels ihe
"white" light into green light which energy is further funneled and
subsequently emitted as a single frequency or monochromatic light by the laser
material, as indicated by the heavy vector 68 between lever 2 and 40 level 1 of
FIG. 7. Again in FIG. 6 the inner surface of the cylinder surrounding the tube
62 may be highly polished for even greater efficiency of pumping.

Referring to FIG. 8 there is illustrated an example of the invention in which
the active laser material is in the 45 form of a hollow cylinder 70 within
which is coaxially disposed a cylindrical flash tube 72, Thus when the flash
tube is energized, substantially all of its pumping radiation is emitted in a
radial direction and must therefore pass through the laser material. The laser
material 70 is 50 in turn coaxially surrounded by a cylinder 74 filled with a
coolant 76. The coolant 76 may be chosen to have a high index of refraction for
the advantages and purposes discussed below. Cylinder 74 may have a highly
polished internal surface for reflecting energy of the flash tube 72 55 back
through the laser material 70.

Referring to FIG. 9, an embodiment of the invention is shown in which the laser
material is refrigerated to liquid nitrogen temperatures for the purpose of
making its output beam even more purely monochromatic be- 60 cause the line
width of the laser transition (frequency v3l) is much sharper in most solids at
low temperature. A rod 78 of active laser material has plated ends 80 and 82
with a coupling hole 84 in the upper end for emitting the laser beam 86. The
opposite end of the rod Is mounted on a 65 thermally conductive rod 88 which
may be of copper or sapphire. The major portion of the rod 88 is immersed in
liquid nitrogen 90 within a Dewar flask 92. A hollow cylindrical flash tube 94
is disposed coaxially about the »0 laser rod 78 and is energized from a power
supply 96 through a set of annular electrodes 98 disposed at opposite ends of
the gas tube 94. A further hollow cylinder is disposed coaxially about the
flash tube 94 and is filled with a coolant 102 to cool the flash tube 94. 75

FIG. 10 illustrates schematically a segment of laser material 104 for purposes
of illustrating internal reflections of the stimulating wave when the segment
is not coated but is merely surrounded by material of a low index of
refraction, such as air. A ray of energy 106 is shown as propagating parallel
with the axis of the rod and therefore never reflects against the side of the
segment 104. A ray 108, however, has a radial component of direction and
reflects, as shown, off the side boundaiy of the segment 104. Such reflections
cause two deleterious effects. One is that the effective length of the
resonating segment is greater than that for an axially traveling ray such as
106. Thus the ray 108 may represent a component of energy at a frequency
slightly different from the desired or designed frequency of operation.
Secondly, the ray 108, if it finds its way out of the coupling hole HO of the
segment 104, will cause a spreading of the beam thereby detracting from the
otherwise extremely narrow beam of the laser and contributing to its
noncoherence. A ray 112 propagating in a direction even further removed from
that of the axis of the segment may obviously reverberate substantially
endlessly through the segment causing by its interference with the desired
energy a decrease in the coherence and narrowness of bandwidth of the laser
output.
....
FIG. 13 illustrates a system in accordance with the present invention which
utilizes an interferometer for providing even greater coherence and narrow
bandwidth. In this embodiment a rod 136 of active laser material does not have
coated ends but rather has prisms 138 and 140 coupled to each end of the rod
136. An additional pair of mirrors or prisms 142 and 144 are disposed so that a
ray of light 146 which is axially directed through the rod 136 may propagate
along the closed path determined by the reflecting surfaces of the 4 mirrors.
Disposed between the mirrors 142 and 144 is an interferometer 148 which may be
a Fabry-Perot interferometer. The interferometer comprises a pair of parallel
plates 150 and 152, the distance between which may be adjusted to "tunc" the
regenerative circuit for the ray 146. Thus a ray of the proper wavelength will
resonate between the parallel plates 150, 152 while waves of other frequencies
will be dissipated and lost in the interferometer.
...
FIG. 14 illustrates another type of interferometer in which the active laser
segment 160 does not have reflective ends. Instead, mutually parallel plates
162 and 164 arc disposed perpendicularly to the axis of the segment 160 which
is the desired direction of propagation. The plates may be disposed at some
distance from the laser material; the greater the distance and the smaller
their size the more the system discriminates against nonparallel light rays 166
and 168. Again the desired energy may be coupled out of the system through a
small opening in the reflective plate 164 to provide a laser output beam 170.

FIG. 15 illustrates the use of an interferometer similar in some respects to
the device of FIG. 14. In this example one of the reflective plates 172 may be
placed directly on the active laser segment 174 while the other reflective
plate 176 may be axially disposed at some distance from the segment 174. As
shown, the nonparallel ray 178 will not be re-reflected between the two
reflective plates 172 and 176 thereby minimizing its deleterious effects on the
monochromatic output beam 180.

FIGS. 16 and 17 illustrate methods of optically pumping the active laser
segment 182 by a source 184 of broadband light which is disposed some distance
from the laser segment. In each case the output beam 186 of the laser is
directed out of the rod-shaped laser segment in a direction parallel to the
axis of the rod. In FIG. 16 two
parabolic reflectors 189 and 190 are directed
toward each other so that the light source 184 at the focal point of reflector
189 emits a substantially parallel beam of pumping light 188 which is collected
by the parabolic reflec

5 tor 190 and focused to pass through the laser segment 182. The parabolic
surfaces 189 and 190 may be parabolic cylindrical surfaces as shown or they may
be paraboloidal surfaces of revolution symmetrically disposed about the line
joining their respective foci.

10 FIG. 17 illustrates an elliptical system for reflecting the energy from the
light source 184 to the laser segment 182 wherein the source 184 is disposed at
one focus of an ellipse while the laser segment 182 is disposed at the opposite
focus; hence, the elliptical surface 192 reflects

15 substantially all of the energy radiating from the source 184 and refocuses
it through the laser segment 182. The elliptical surface 192 may be an
elliptical cylindrical surface or it may be an ellipsoid.

The light source 184 in either of the above examples

20 may make use of exploding wire phenomenon in which an extremely high current
at low voltage is sent through a wire thereby exploding and vaporizing it. The
light energy emitted by this phenomena may be extremely intense "white" light.
Alternatively, the source 184 may

25 be other conventional light sources such as gas-filled flash tubes, or
carbon arc lamps. An advantage of the systems depicted in FIGS. 16 and 17 is
that the light source and the active laser material may be independently
handled and cooled due to their spacing from each other.

30 Referring to FIG. 18, there is illustrated a practical application of a
laser in a colidar optica! radar system. "Colidar" is an acronym for coherent
light ranging. A laser unit 200 is the colidar transmitter and includes an
active laser segment 202. Surrounding the segment 202

35 is a gas-filled flash tube 204 which is pulsed from a pump power supply 206.
A synchronizer 208 triggers the pump power supply which in turn fires the flash
tube 204 and the laser 200 transmits a beam 210 of monochromatic coherent light
toward a target 212, the range to which

40 is to be determined. The synchronizer trigger also triggers the horizontal
sweeps of a pair of oscillographs 214 and 216. A sample of the laser output is
determined by a photoelectric cell 218 which is coupled to the oscillograph 214
and presented on the face thereof as a "transmitter"

45 pulse 220 to indicate the time at which the laser output pulse was
transmitted. The laser beam 210 is reflected off a target 212 and a minute
portion thereof is received as a parallel beam 210' by the colidar receiver
222. The received beam 210 impinges upon a parabolic reflector

50 224 and is focused into a photoelectric cell 226. The electrical cell of the
protoelectric cell 226 is coupled to the receiver oscillograph 216 where it is
presented on the face thereof as a "receiver" pulse 228. The time difference
between the pulses 220 and 228 on the two oscillographs

85 is, of course, a direct indication of the range from the colidar system to
the target 212. The two oscillographs 214 and 216 may alternatively be a dual
trace, single oscillograph tube or, as in conventional radar "B-scope"
presentation, be displayed with a single horizontal trace.

00 The advantages of such a ranging system which may obviously be extended to
other forms of radar, such as plan position indicator types, include the fact
that the transmitted beam Is extremely narrow and may be sent over great
distances with very little beam spreading. Also

65 the wavelength is so small that extremely high resolution is obtained. It
may also be seen that it is substantially impossible to jam a laser radar
system because the jamming equipment would have to be placed precisely in

^Q line with the transmitter and the target would have to be directed at the
receiver and would have to be at precisely the proper optical frequency in
order to interfere with the laser receiver. For further improvements in this
regard optical filters 230 may be placed in the receiver 222 to 75 discriminate
not only against deliberate jamming but also

against the minute amount of optical noise at the operating frequency.

There has thus been disclosed a laser system in which the active laser
substance is solid state and which provides coherent monochromatic
amplification and generation of electromagnetic wave energy in the optical or
visible spectrum. The invention is effectively an efficient device which is
mechanically stable and which may be operated at room temperature without
complex vacuum or vapor pressure techniques. The invention as disclosed also is
capable of tuning over a 5X1011 cycles per second range and may handle high
powers for practical optical radar and communications utilization. In addition,
because it provides light which can be focused extremely precisely, the laser
opens new possibilities in the investigation of basic properties of mater, as
well as in medicine where objects or very minute portions thereof can bo
selectively sterilized or vaporized.

What is claimed is:

1. A three energy level laser comprising: a ruby having atoms exhibiting a
first energy level corresponding to a ground atomic state, a substantially
discrete second energy level above said ground stale and third energy- levels
defining a relatively broadband absorption third region extending above said
second level; a pumping source of broadband light energy optically coupled to
said ruby for illuminating it and exciting atoms thereof to exhibit excitation
at said third energy levels from whence they decay without substantial
radiation loss to said discrete second energy level so as to establish a
population inversion between said discrete second energy level and said ground
state;

interferometer means optically coupled to said ruby and tuned to the frequency
corresponding to that of the energy difference between said second energy level
and said first energy level for reflecting light energy of said frequency
repeatedly through portions of said ruby to generate a coherent light beam;

and coupling means for extracting the monochromatic

coherent light beam from said ruby.
2. A three energy level ruby laser system,
comprising:
a ruby having atoms exhibiting a first energy level cor-
responding to a ground
atomic state, a substantially
discrete second energy level above said ground state
and third energy
levels defining a relatively broad-
band absorption third region extending above said
second
level;

broadband optical pumping means directly coupled to
said ruby for exciting atoms
of said ruby from said
first energy level to said third energy levels from
which
radiationless energy transition of said atoms
takes place to said second energy level
to establish
a population inversion between said second energy
level and said ground state; and
light
-resonating means coupled to and forming a re-
generative optical path through said
ruby to stimulate
radiant energy transitions of said atoms from said
second energy level
toward said ground state to pro-
duce a coherent monochromatic light beam having a
freq
uency substantially corresponding to the energy
difference between said ground state
and said second
energy level.". (read entire patent?)

(more detail: is one side half-silvered? what is entered into the ruby? what is
a flash lamp and how does it work? What are the wavelengths of the flash lamp?
Are there other materials that emit single wavelengths of photons? Who invents
the CO2 maser/laser? what other lasers exist? What can lasers/masers cut
through? How small can these dangerous lasers be? Ultimately the photons in
electricity are converted/distributed into densely packed beams so an initial
number of photons needs to be high. Explain more detail about how lasers work.
Show schematics. The maser was clearly a major invention, and the adaption of
laser also important, as this is a new kind of device with many valuable uses.
In addition, this creates the fastest and most deadly hand-held weapon ever
built of earth (surpassing the metal-bullet gun as a light particle is faster
than a lead projectile).)

(Might the regularly of the frequency and direction have anything to do with
the regular atomic structure of crystals? Bragg's law shows that light
particles clearly reflect off of atomic crystal planes.)

(Describe how the laser principle is different from fluorescence, and from an
LED.)

(Describe how lasers and masers are made dense enough to cut through materials
- is frequency of laser/maser important or is density/intensity more important?
Is size of device important? Can there be hand-held, and dust-sized lasers and
masers?)

(Note that the Encyclopedia Britannica mention of lasers for "delicate surgery"
conjures also the "gross and undelicate murder".)

(Many scientists that publish fall into two groups - those with numerous
publications and those with sparse publications. Maimon is one with sparse
publicatinos. Many times, but not always, those with numerous publications are
mathematical theoreticians who publish a lot of abstract theories - many if not
all of which are false and inaccurate. These many-hundreds-of-published-papers
people many times are the "darlings" of wealthy propagandists who pay them to
mislead the public - Gamow being one that comes to mind. Alternatively, for
example there are those in chemistry and biology who publish many new small
findings, which are valid and honest science. Because of the neuron secret,
most astronomy and physics in particular is mostly fraud or describes
inventions actually realized many decades before.)

(It seems unlikely, as is the case for Townes and the maser, that Maimon is not
the actual first inventor of the laser. Was this published with AT&T's approval
or against AT&T's wishes?)

(Notice "ensue" - like perhaps there was some law suit involved or threatened
lawsuit?)

(Perhaps there is some relationship between the rate light particles can be
absorbed by atoms in the crystal and the rate they can be emitted, or perhaps
this is a rate of reflection phenomenon where many light particles arrive at
different frequencies but are converted to regular frequencies by reflection.)

(Notice "decayed" - perhaps echoing a word in the thought-audio of JFK or a
hope for a science-dominated decade - that was sadly cut short only 3 years
later - and eventually the traditional antiscience secrecy, superstition and
violence returned.)

(Determine if these rubys are grown and how they are manufactured.)

(Note that one design uses a fluorescent gas light to stimulate the ruby
light.)

(Describe the different known lasers and their inventors and uses.)

(Is the CO2 laser the most destructive laser known? Is it a maser since it is
mostly infrared light?)

(So can it be said that the laser frequency is one of a fluorescent emission
frequency of light?)

(State how the ruby's red appearance in white light is a result of this
absorption of various frequencies and reflection and/or emission of red
frequency light.)
(Hughes Research Laboratories) Malibu, California  
40 YBN
[04/??/1960 AD]
5073)
(University of London) London, England  
40 YBN
[06/29/1960 AD]
5681)
(Harvard University) Cambridge, Massachusetts, USA   
40 YBN
[07/05/1960 AD]
5775) In 1973, the Nobel Prize in Physics is divided, one half jointly to Leo
Esaki and Ivar Giaever "for their experimental discoveries regarding tunneling
phenomena in semiconductors and superconductors, respectively" and the other
half to Brian David Josephson "for his theoretical predictions of the
properties of a supercurrent through a tunnel barrier, in particular those
phenomena which are generally known as the Josephson effects".
(General Electric Research Laboratory) Schenectady, New York, USA  
40 YBN
[08/12/1960 AD]
5485) At Bell Telephone Laboratories, Pierce develops a klystron-oscillator,
which is used in US radar receivers. The klystron-oscillator was first publicly
described by Russell and Sigurd Varian in 1939.

Pierce writes science fiction under the pseudonym J. J. Coupling.

In 1948 Arthur C. Clarke is the first to propose the concept of satellites
orbiting the earth and acting as reflectors for radio waves. Such satellites
make world-wide communications as simple as a telephone call.

In 1948 Pierce coins the term "transistor" to describe the new solid-state
device invented at Bell Laboratories.

(Clearly, being at AT&T Bell Labs, Pierce must have been involved in the
development of flying dust-sized neuron reader and writer devices. In one paper
Pierce states in the introduction that he can't talk about most technology
because it is classified as government secret information.)
(Launchpad 17) Cape Canaveral, Florida, USA  
40 YBN
[09/01/1960 AD]
5512) (It seems possible that around the 1950s, there arose a clearly new
direction in science which I would describe as a kind of "lose the public"
philosophy, and "who can create the most complex and abstract paper?" - like a
transistion from the more conservative philosophy where all doubts must be
thoroughly explored, and all possible explanations examined - as was the
tradition for Rutherford, and other scientists, for the most part - this new
view is more of - like an "artistic" science, where scientists are like Picasso
- creating abstract art which is labeled priceless purely by the association of
the creator to the art, with no regard for accuracy, or honesty. This is
characteristic of the radical and unlikely claims of relativity which rose in
the 1920s but Einstein's large-scale US popularity occured in the 1950s. I
think you can see a clear transition from careful and conservative statements
which must pass the scrutiny of all other scientists, to a kind of
massive-funded steam-engine thundering off into some useless direction full of
petrified passangers too scared to tell the truth to the conductor or owners,
and this smoke-screen serves as some kind of aether-cloud to fool the public
and remove any element of logic from the people of earth. Alvarez, et al
papers, I think, mark a clear begining of this ultra-abstract, very hard to
follow paper. Clearly, there is an unending string of inaccurate abstract
mathematical theoretical papers - those of Clausius, Gibbs, Maxwell, etc., but
always the experimentalists tend to stay on the conservative line, staying
close to the observed physical phenomena. It may be that the neuron network
took on a different form after WW2 - one of a more "rendered fake news stories"
fascism - like Stalin's erasing the photos of Trotsky, and Life publishing the
altered Oswald photo. It's like humans have reached this stage where - even the
journal publishers themselves are corrupting science and delaying truth from
reaching the public - and simply producing loads of - what is mostly garbage -
all because of direct-to-brain windows and the loss of traditional controls on
information - except for the slave-like excluded who fund their lives and
journals - the journals would otherwise be viewed as videos direct-to-brain and
would not be so full of lies.)
(University of California) Berkeley, California, USA  
40 YBN
[09/09/1960 AD]
5747) Glashow and Weinberg are classmates at the Bronx high School of Science
and as undergraduates at Cornell university.

In 1979, the Nobel Prize in Physics is awarded jointly to Sheldon Lee Glashow,
Abdus Salam and Steven Weinberg "for their contributions to the theory of the
unified weak and electromagnetic interaction between elementary particles,
including, inter alia, the prediction of the weak neutral current".
(University of Copenhagen) Copenhagen, Denmark  
40 YBN
[09/09/1960 AD]
5748)
(University of Copenhagen) Copenhagen, Denmark  
40 YBN
[09/15/1960 AD]
5798)
(Jet Propulsion Laboratory, California Institute of Technology) Pasadena,
California  
40 YBN
[09/16/1960 AD]
5652)
(Harvard University) Cambridge, Massachusetts, USA  
40 YBN
[09/??/1960 AD]
5707) In 1978, the Nobel Prize in Chemistry is awarded to Peter Mitchell "for
his contribution to the understanding of biological energy transfer through the
formulation of the chemiosmotic theory".
(University of Edinburgh) Edinburgh, Scotland, U.K.  
40 YBN
[10/15/1960 AD]
6090) The Miracles song "Shop Around" (written by Smokey Robinson and Berry
Gordy) is released.
(Hitsville USA) Detroit, Michigan, USA  
40 YBN
[10/24/1960 AD]
5415)
(Rockefeller Institute of Medical Research) New York City, New York, USA  
40 YBN
[12/28/1960 AD]
5705) Jacob is badly wounded serving with the Free French forces in WW II, and
receives a 90% disability
pension.

In 1965, the Nobel Prize in Physiology or Medicine is awarded jointly to
François Jacob, André Lwoff and Jacques Monod "for their discoveries
concerning genetic control of enzyme and virus synthesis".

In 1970 Monod publishes "Chance and Necessity" in which he insists that chance
is the architext of all things. (Monod is probably atheist then.)
(Pasteur Institute) Paris, France  
40 YBN
[12/30/1960 AD]
5654)
(Bell Telephone Laboratories) Murray Hill, New Jersey, USA  
40 YBN
[12/30/1960 AD]
5769)
(Bell Telephone Laboratories) Murray Hill, New Jersey, USA  
40 YBN
[12/??/1960 AD]
5412)
(Princeton University) Princeton, New Jersey, USA  
40 YBN
[1960 AD]
5685) In 1975, the Nobel Prize in Chemistry is divided equally between John
Warcup Cornforth "for his work on the stereochemistry of enzyme-catalyzed
reactions" and Vladimir Prelog "for his research into the stereochemistry of
organic molecules and reactions".
(National Institute for Medical Research) Mill Hill, London, UK  
39 YBN
[02/13/1961 AD]
5741)
(Imperial College) London, England and (California Institute of Technology)
Pasadena, California, USA  
39 YBN
[04/12/1961 AD]
5601)
Saratovskaya oblast, Russia (was U.S.S.R.)  
39 YBN
[04/13/1961 AD]
5560)
(University of California) Berkeley, California, USA  
39 YBN
[05/19/1961 AD]
5612)
Planet Venus  
39 YBN
[05/20/1961 AD]
5673) In 1958 Kendrew founds the "Journal of Molecular Biology".

In 1962, the Nobel Prize in Chemistry is awarded jointly to Max Ferdinand
Perutz and John Cowdery Kendrew "for their studies of the structures of
globular proteins".
(Cavendish Laboratory, University of Cambridge) Cambridge, England (and the
Royal Instutition, London)  
39 YBN
[07/??/1961 AD]
6092) The song "Tossin' and Turnin"' (written by Ritchie Adams and Malou Rene,
sung by Bobby Lewis) is released.
  
39 YBN
[08/03/1961 AD]
5765) In 1968 the Nobel Prize in Physiology or Medicine is awarded jointly to
Robert W. Holley, Har Gobind Khorana and Marshall W. Nirenberg "for their
interpretation of the genetic code and its function in protein synthesis".
(National Institutes of Health) Bethesda, Maryland, USA  
39 YBN
[09/??/1961 AD]
6091) "Hit the Road Jack" (written by Percy Mayfield) sung by Ray Charles.

New York City, New York, USA (guess)  
39 YBN
[10/16/1961 AD]
5242)
(University of Michigan) Ann Arbor, Michigan, USA  
39 YBN
[10/16/1961 AD]
5718) In 1968, the Nobel Prize in Physiology or Medicine is awarded jointly to
Robert W. Holley, Har Gobind Khorana and Marshall W. Nirenberg "for their
interpretation of the genetic code and its function in protein synthesis".
(Cornell University) Ithaca, New York, USA  
39 YBN
[12/30/1961 AD]
5663)
(Cavendish Lab University of Cambridge) Cambridge, England  
39 YBN
[1961 AD]
3340)
(University of California, Berkeley) Berkeley, CA, USA  
39 YBN
[1961 AD]
5706)
(Pasteur Institute) Paris, France  
39 YBN
[1961 AD]
5788)
(SETI conference) Green Bank, West Virginia, USA  
38 YBN
[01/05/1962 AD]
5792)
(Chester Beatty Research Institute, Institute of Cancer Research: Royal Cancer
Hospital) London, England  
38 YBN
[01/??/1962 AD]
5657)
(RCA Laboratories) Princeton, New Jersey, USA  
38 YBN
[03/27/1962 AD]
6094) "Return to sender" (written by Winfield Scott and Otis Blackwell, and
sung by Elvis Presley) is recorded.

(The phrase "return to sender" also may very smartly be resonate with the
meaning of "fire back the neuron writing to the sender".)

(Radio Recorders) Hollywood, California, USA  
38 YBN
[05/04/1962 AD]
5796)
(University of British Columbia) Vancouver, British Columbia, Canada  
38 YBN
[06/08/1962 AD]
5802) In 1973, the Nobel Prize in Physics is divided, one half jointly to Leo
Esaki and Ivar Giaever "for their experimental discoveries regarding tunneling
phenomena in semiconductors and superconductors, respectively" and the other
half to Brian David Josephson "for his theoretical predictions of the
properties of a supercurrent through a tunnel barrier, in particular those
phenomena which are generally known as the Josephson effects".

(I have a lot of doubts, but perhaps this superposition of oscillating currents
is a real phenomenon. If based on the Cooper electron-pairs theory, I have
doubts. The work seems highly mathematical and theoretical - which is usually
too generalized and therefore different from the many more particle actual
phenomena.)
(Cavendish Laboratory, University of Cambridge) Cambridge, England  
38 YBN
[06/16/1962 AD]
5662)
(King's College) London, England  
38 YBN
[06/30/1962 AD]
5682)
(Harvard University) Cambridge, Massachusetts, USA (and CHAS. PFIZER AND CO.,
INC, Groton, Connecticut, USA)   
38 YBN
[09/24/1962 AD]
5656)
(General Electric Research Laboratory) Schenectady, New York, USA  
38 YBN
[09/??/1962 AD]
6093) "Green Onions" is written and recorded by Booker T. & the M.G.s.

(Since this song is simply 1-4-5 blues, the thrill is probably the new sounding
hammond electric organ and the new sounding electric guitar - in particular
with a more distorted/rougher sounded.)

Memphis, Tennessee, USA  
38 YBN
[10/12/1962 AD]
5376) Bruno Benedetto Rossi (CE 1905-1994) Italian-US physicist, at MIT and
Riccardo Giacconi, Herbert Gursky and Frank Paolini from the American Science
and Engineering in Cambridge, Massachusetts publish the first report of x-ray
sources from outside the solar system, 67 years after x-rays were first made
public by Rontgen in 1895.

Less than 3 years earlier, Rossi and Giacconi had published a report about the
first publicly known x-ray telescope, but this x-ray astronomy is done using a
rocket and Geiger detectors.

In a letter "Evidence for X Rays from Sources Outside the Solar System", in the
journal "Physical Review", Rossi et al write:
" Data from an Aerobee rocket carrying
a payload consisting of three large area Geiger counters have revealed a
considerable flux of radiation in the night sky that has been identified as
consisting of soft c rays.
The entrance aperture of each Geiger counter consisted
of seven individual mica windows comprising 20 cm2 of area placed into one face
of the counter. Two of the counters had windows of about 0.2-mil mica, and one
counter had windows of 1.0-mil mica. The sensitivity of these detectors for x
rays was etween 2 and 8 A, falling sharply at the extremes due to the
transmission of the filling gas and the opacity of the windows, respectively.
The mica was coated with lamp-black to prevent ultraviolet light transmission.
The three detectors were disposed symmetrically around the longitudinal axis of
the rocket, the normal to each detector making an angle of 55° to that axis.
Thus, during flight, the normal to the detectors swept through the sky, at a
rate determined by the rotation of the rocket, forming a cone of 55° with
respect to the longitudinal axis. no mechanical collimation was used to limit
the field of view of the detectors. Also included in the payload was an optical
aspect system similar to the one developed by Kupperian and Kreplin. The axes
of the optical sensors were normal to the longitudinal axis of the rocket. Each
Geiger counter was placed in a well formed by an anticoincidence scintillation
counter designed to reduce the cosmic-ray background. The experiment was
intended to study fluorescence x rays produced on the lunar surface by x rays
from the sun and to explore the night sky for other possible sources. On the
basis of the known flux of solar x rays, we had estimated a flux from the moon
of about 0.1 to 1 photon cm-2sec-1 in the region of sensitivity of the counter.

The rocket launching took place at the White Sands Missile Range, New Mexico,
at 2359 MST on June 18, 1962. The moon was one day past full and was in the sky
about 20° east of south and 35° above the horizon. The rocket reached a
maximum altitude of 225 km and was above 80 km for a total of 350 seconds. The
vehicle traveled almost due north for a distance of 120 km. Two of the Geiger
counters functioned properly during the flight; the third counter apparently
arced sporadically and was disregarded in the analysis. The optical aspect
system functioned correctly. The rocket was spinning at 2.0 rps around the
longitudinal axis. From the optical sensor data it is known that the spin axis
of the rocket did not deviate from the vertical by more than 3°; for purposes
of analysis, the spin axis is taken as pointing to zenith. The angle of
rotation of the rocket corresponds with the azimuth ...
...
From Fig. 2 we see
that the main apparent source is in the vicinity of the galactic center at the
G. T. azimuthal angle of about 195°. We also see that the trace of the G.T.
axis lies close to the galactic equator for a value of the azimuthal angle neat
40°, which is the region where the background radiation is recorded with
greater intensity. This apparent maximum of the background radiation is the
general region of the sky where two peculiar objects-Cassiopeia A and Cygnus A-
are located. It is perhaps significant that both the center of the galaxy where
the main apparent source of x rays lies, and the region of Cassiopeia A and
Cygnus A where there appears to be a secondary x-ray source, are also regions
of strong radio emission. ...
With this one experiment it is impossible to
complete define the nature and origin of the radiation we have observed. Even
though the statistical precision of the measurement is high, the numerical
values for the derived quantities and angle are subject to large variation
depending on the choice of assumptions., However, we believe that the data can
best be explained by indentifying the bulk of the radiation as soft x rays from
sources outside the solar system. Syncrotron radiation by cosmic electrons is a
possible mechanism for the production of these x-rays. Ordinary stellar sources
could also contribute a considerable fraction of the observed radiation.
...".

(Determine if the moon reflects x-ray light from the Sun. Perhaps some is
absorbed by atoms on the moon, but it seems likely that, like visible light,
much is reflected.)

(Note that the paper is received in October.)

(Note that a rocket is used to detect x-rays but not the x-ray telescope
proposed by Rossi 2 years earlier.)
(Massachusetts Institute of Technology) Cambridge, Massachusetts, USA  
38 YBN
[10/26/1962 AD]
6201) Laser writing and reading of data. Data is written and read from plastic
film. Reading data with light particles is better than reading data
mechanically, like using the arm of a phonograph player, because only light
particles touch the recorded surface.
(Winston Research Corporation) Los Angeles, California, USA  
38 YBN
[10/26/1962 AD]
6212) Elvis Presley records "Riding the Rainbow".
  
38 YBN
[11/??/1962 AD]
5666)
(U. S. Naval Research Laboratory) Washington, D. C., USA  
38 YBN
[1962 AD]
3981)
RCA Labs, Princeton, New Jersey, USA  
38 YBN
[1962 AD]
5171)
(Harvard University) Cambridge, Massachusetts, USA  
38 YBN
[1962 AD]
5328)
Fort Ternan, Kenya, Africa  
38 YBN
[1962 AD]
5490)
(off coast of) Marseilles, France  
38 YBN
[1962 AD]
5794)
(Biochemical Research Laboratory, Bulgarian Academy of Sciences) Sofia,
Bulgaria (verify)  
37 YBN
[02/25/1963 AD]
5249)
(The Caroline Institute) Stockholm, Sweden  
37 YBN
[03/04/1963 AD]
5750)
(Wilson and Palomar Observatories, Carnegie institute of Washington and
California Institute of Technology) Pasadena, California, USA  
37 YBN
[03/16/1963 AD]
5785)
(California Institute of Technology) Pasadena, California  
37 YBN
[04/26/1963 AD]
5736) In 1979, the Nobel Prize in Physiology or Medicine is awarded jointly to
Allan M. Cormack and Godfrey N. Hounsfield "for the development of computer
assisted tomography".
(Tufts University) Medford, Massachusetts, USA  
37 YBN
[06/16/1963 AD]
5602)
(Baikonur Cosmodrome) Tyuratam, Kazakhstan (was Soviet Union)  
37 YBN
[07/01/1963 AD]
6109) The Beatles record "She Loves You".

(EMI Studios) London, England  
37 YBN
[07/20/1963 AD]
5730)
(NASA Ames Research Center) Moffett Field, California, USA and (Stanford
University) Palo Alto, California, USA  
37 YBN
[08/05/1963 AD]
5609)
Moscow, (Soviet Union) Russia  
37 YBN
[10/17/1963 AD]
6108) The Beatles record "I Want to Hold Your Hand".

(EMI Studios) London, England  
37 YBN
[12/??/1963 AD]
5694)
(Deutsches Wollforschungsinstitut - German Wool Research Institute) Aachen,
Germany and (University of Pittsburgh) Pittsburgh, Pennsylvania, USA  
36 YBN
[01/04/1964 AD]
5780)
(California Institute of Technology) Pasadena, California  
36 YBN
[02/11/1964 AD]
5784)
(Brookhaven National Laboratory) Upton, New York, USA  
36 YBN
[02/26/1964 AD]
5437)
(Harvard University) Cambridge, Massachusetts, USA  
36 YBN
[04/04/1964 AD]
5330)
Olduvai Gorge, Africa  
36 YBN
[05/11/1964 AD]
6113) The Beach Boys release "I Get Around".

(Western Studios) Hollywood, California, USA  
36 YBN
[06/19/1964 AD]
5749)
(University of Copenhagen) Copenhagen, Denmark  
36 YBN
[07/10/1964 AD]
5726) In the mid-1940s while Fitch is a member of the U.S. Army, he is sent to
Los Alamos, N.M., to work on the Manhattan Project. (To me this clearly implies
very likely governmental dishonesty and corruption of science. Probably Fitch
was called upon by people in government and neuron owners to feed false
information to the public in the constant effort to remove the public's belief
that they can understand science and that the universe is logical and
consistent.)

In 1980, the Nobel Prize in Physics is awarded jointly to James Watson Cronin
and Val Logsdon Fitch "for the discovery of violations of fundamental symmetry
principles in the decay of neutral K-mesons". (This award choice to me seems
highly fraudulent. In addition, this is just after the election of the
Republicans in the USA and the murder of John Lennon - clearly a rise and peak
of evil on earth.)

(This is a theory, and I think more caution should be shown for theories, and
more reward for experimental finds or useful instrument creations. Very few
people criticize complex math, most are intimidated by it, and cannot spend the
time necessary to try and understand it. But I think the burden of explaining
clearly is on the theorist, and should be presumed as theory until you are
convinced of it's accuracy. In addition, all major skepticism and rejections of
a theory should be heard.)
(Princeton University) Princeton, New Jersey, USA  
36 YBN
[07/15/1964 AD]
5770) Patel publishes this in "Physical Review" as "Continuous-Wave Laser
Action on Vibrational-Rotational Transitions of CO2". For an abstract Patel
writes: "We have obtained cw laser action on a number of rotational transitions
of the Σu+-Σg+ vibrational band of CO2 around 10.4 and 9.4μ. The laser
wavelengths are identified as the P-branch rotational transitions from P(12) to
P(38) for the 00°1-10°0 band and from P(22) to P(34) for the 00°1-02°0
band. Strongest laser transition occurs at 10.6324μ (vacuum). A cw power
output of about 1 mW has been measured. All these laser transitions can also be
made to oscillate under pulsed discharge conditions with a small increase in
the peak laser power output. No R-branch transitions have been seen to
oscillate either under cw or pulsed discharge conditions. The wavelength
measurements are in reasonable agreement with earlier measurement of the bands
in absorption, but there are slight differences. These are ascribed to possible
pressure-dependent frequency shift effects. A study has been made of the time
dependence of the laser output under pulsed excitation, and some conclusions
about possible excitation processes are given. Theoretical interpretation given
earlier for laser action on vibrational-rotational transitions is discussed in
a generalized form. The theory is applicable to both the linear polyatomic
molecules and the diatomic molecules.". Patel describes the apparatus by
writing: " The experimental setup used in the CO2 laser experiments consisted
of a far-infrared optical maser similar to the one described in Ref. 6. The
quartz discharge tube (see Fig. 1 of Ref. 6) was 25.4 mm i.d. and 5 m long. The
optical resonator cavity was formed with a pair of near-confocal silicon
mirrors, which were coated with vacuum-deposited aluminum for high reflectivity
in the infrared. Coupling of energy out from the cavity was obtained by either
(a) making the aluminum coating on one of the mirrors partially transparent or
(b) leaving a small (1.0 mm diam) area uncoated at the center of the output
mirror. (The relative advantages of the two techniques have been discussed in
Ref. 7). It was found that the second method was generally more satisfactory,
and the results reported in this paper were obtained with that method. As such
there was no additional wavelength-discriminating device (such as dielectric
mirror coatings capable of giving high reflectivity in a narrow region of
wavelengths) intentionally introduced in the optical cavity. ...Discharge in
CO2 was produced by using dc excitation. (In a limited number of cases, high
current pulses of 1-usec duration were also used for investigation of the CO2
optical maser.).
...".

The carbon dioxide (CO2) molecular laser has become the laser of choice for
many industrial applications, such as cutting and welding.

The carbon-dioxide laser, which can generate kilowatts of continuous power, is
the most powerful commercial gas laser.

(Determine if the CO2 laser is the most potentially destructive laser ever made
public.)
(Bell Telephone Laboratories) Murray Hill, New Jersey, USA  
36 YBN
[07/24/1964 AD]
6112) British pop band The Zombies release "She's Not There".

One of the song's most distinctive features is Argent's electric piano sound;
the instrument used was a Hohner Pianet.

(This could be interpreted as being about remote neuron writing done to
excluded by an AT&T computer that mimics a female voice, and perhaps sends
images of females to excluded and how excluded chase after the pretend woman-
who they can't possibly ever meet. In addition, it could be an actual female
that is coerced or for some sex-based reason sends audio and images from
herself via AT&T's wireless neuron writing network to excluded - as a "tease",
in particular to arouse the insider neuron consumer and owner males.)

England  
36 YBN
[08/??/1964 AD]
6111) Roy Orbison releases the song "Oh, Pretty Woman".

(Monument Records) Nashville, Tennessee, USA  
36 YBN
[09/24/1964 AD]
5746) In 1979, the Nobel Prize in Physics is awarded jointly to Sheldon Lee
Glashow, Abdus Salam and Steven Weinberg "for their contributions to the theory
of the unified weak and electromagnetic interaction between elementary
particles, including, inter alia, the prediction of the weak neutral current".
Salam is the first Pakistani and the first Muslim scientist to win a Nobel
Prize. (This seems highly theoretical, in particular given the view that all
matter is simply made of light particles. In particular imagining what
corruption may exist given many decades of secret remote neuron reading and
writing. The experimental side of physics appears to take second place to the
theoretical side with the Nobel prize.)
(Imperial College) London, England  
36 YBN
[10/08/1964 AD]
5569) Flerov announces the formation of an isotope of element 104, the most
massive element formed to this date, and suggests the name "kurchatovium" in
honor of Kurchatov, but in 1969, Albert Ghiorso and a group at Berkeley will
report not being able to confirm the Dubna experiments and claim a positive
identification of element 104 using a separate method and suggest the name
"rutherfordium".
(Joint Institute for Nuclear Research, Laboratory of Nuclear Reactions) Moscow,
(U.S.S.R. now) Russia  
36 YBN
[12/17/1964 AD]
5585) In 1975, the Nobel Prize in Physiology or Medicine is awarded jointly to
David Baltimore, Renato Dulbecco and Howard Martin Temin "for their discoveries
concerning the interaction between tumour viruses and the genetic material of
the cell".
(The Salk Institute For Biological Studies) San Diego, California, USA  
36 YBN
[12/??/1964 AD]
5497)
(La Salpetriere), Paris, France  
36 YBN
[1964 AD]
3980) Liquid Crystal Display.

A Liquid Crystal Display (LCD) uses much less electricity, weighs much less,
and can be much thinner than a Cathode Ray Tube (CRT) display.

George Heilmeier (CE 1936-) in RCA Labs, uses a DC voltage of several volts to
change the color of a liquid crystal cell. This is the first publicly known
liquid crystal display device.

This device is based on the "William domain" effect published by Richard
William of RCA in 1962, in which an electric field applied to a liquid crystal
cell causes regular patterns of lines which he calls "domains".
RCA Labs, Princeton, New Jersey, USA  
36 YBN
[1964 AD]
5803)
(Boston University) Bostom, Massachusetts, USA (presumably)  
35 YBN
[01/08/1965 AD]
5719)
(Cornell University) Ithaca, New York, USA  
35 YBN
[02/15/1965 AD]
5744) In 1976, the Nobel Prize in Physiology or Medicine is awarded jointly to
Baruch S. Blumberg and D. Carleton Gajdusek "for their discoveries concerning
new mechanisms for the origin and dissemination of infectious diseases".
(Institute for Cancer Research) Philadelphia, Pennsylvania, USA and (U.S.
National Institutes for Health) Maryland, USA   
35 YBN
[03/29/1965 AD]
5731)
(NASA Ames Research Center) Moffett Field, California, USA  
35 YBN
[05/13/1965 AD]
5797) Penzias' family, being Jewish, leaves Germany 10 weeks after Hitler takes
control.

In 1978, the Nobel Prize in Physics is divided, one half awarded to Pyotr
Leonidovich Kapitsa "for his basic inventions and discoveries in the area of
low-temperature physics",the other half jointly to Arno Allan Penzias and
Robert Woodrow Wilson "for their discovery of cosmic microwave background
radiation".

In 2006, the Nobel Prize in Physics is awarded jointly to John C. Mather and
George F. Smoot "for their discovery of the blackbody form and anisotropy of
the cosmic microwave background radiation" using the COBE satellite.
(Bell Telephone Laboratories, Inc.) Crawford Hill, Holmdel, New Jersey,
USA  
35 YBN
[06/05/1965 AD]
5714)
(Yale University) New Haven, Connecticut, USA and (Cambridge University)
Cambridge, England  
35 YBN
[07/14/1965 AD]
5615) The first ship from Earth to reach planet Mars, and to return images of
the surface, Mariner 4.

These represent the first images of another planet ever returned from deep
space.
Planet Mars  
35 YBN
[08/12/1965 AD]
5420) In 1941 Prelog escapes from Yugoslavia to Switzerland when the Nazi army
invades Yugoslavia.

In 1975, the Nobel Prize in Chemistry is divided equally between John Warcup
Cornforth "for his work on the stereochemistry of enzyme-catalyzed reactions"
and Vladimir Prelog "for his research into the stereochemistry of organic
molecules and reactions".
(Eidgenossische Technische Hochschule) Zurich, Switzerland  
35 YBN
[09/02/1965 AD]
5713)
(University of Wisconsin) Madison, Wisconsin, USA  
35 YBN
[09/25/1965 AD]
6115) The Rolling Stones release "Get Off of My Cloud".

The song has a similar structure as "Louie Louie": 1-4-5-4, in this case E A B
A.
(Possibly there is a play on the remote neuron writing - for example - 'stop
writing to our heads.')

(RCA Studios) Hollywood, California, USA  
35 YBN
[10/20/1965 AD]
6117) The Beatles record the song "We Can Work Out".

(There may be a play on the idea of a direct-to-brain windows female dating or
having a relationship with an excluded male which must be very rare. It's rare
also to see a statement against fighting or indirectly violence.)

(EMI Studios) London, England  
35 YBN
[10/??/1965 AD]
6114) James Brown releases "I Got You (I Feel Good)".

(Criteria Recording Studios) Miami, Florida, USA  
35 YBN
[1965 AD]
5712) In 1968, the Nobel Prize in Physiology or Medicine is awarded jointly to
Robert W. Holley, Har Gobind Khorana and Marshall W. Nirenberg "for their
interpretation of the genetic code and its function in protein synthesis".
(University of Wisconsin) Madison, Wisconsin, USA (verify)  
35 YBN
[1965 AD]
6276)
  
34 YBN
[01/27/1966 AD]
5648)
(Harvard University) Cambridge, Massachusetts, USA   
34 YBN
[02/03/1966 AD]
5616)
Moon of Earth  
34 YBN
[02/19/1966 AD]
5728) In 1976, the Nobel Prize in Physiology or Medicine is awarded jointly to
Baruch S. Blumberg and D. Carleton Gajdusek "for their discoveries concerning
new mechanisms for the origin and dissemination of infectious diseases".

Over his years working amongst the tribes of the South Seas, he adopted 57
kids, bringing them to a new life in Washington DC. In 1997 Gajdusek pleaded
guilty to child abuse involving the sexual molestation of a teenaged boy and
served one year in prison.
(National Institute of Health) Bethesda, Maryland, USA  
34 YBN
[03/01/1966 AD]
5613) The first ship from Earth to impact a different planet, "Venera 3"
impacts the surface of Venus.
Planet Venus  
34 YBN
[04/04/1966 AD]
5599)
(Baikonur Cosmodrome) Tyuratam, Kazakhstan (was Soviet Union)  
34 YBN
[10/10/1966 AD]
6116) The Beach Boys release "Good Vibrations".

(It's somewhat rare to hear a cello in a pop song. Violins were in many pop
songs of the late 1950s and since, but cello is not introduced as a major
component until the Beatles "Strawberry Fields" and "I am the Walrus". State
where violins enter into mainstream pop of the USA. This song also features the
"electro-theremin" instrument.)
Los Angeles, California, USA (presumably)  
34 YBN
[10/24/1966 AD]
5793) In 1980, the Nobel Prize in Chemistry is divided, one half awarded to
Paul Berg "for his fundamental studies of the biochemistry of nucleic acids,
with particular regard to recombinant-DNA",the other half jointly to Walter
Gilbert and Frederick Sanger "for their contributions concerning the
determination of base sequences in nucleic acids".
(Harvard University) Cambridge, Massachusetts, USA   
34 YBN
[11/03/1966 AD]
6121) Jefferson Airplane records "Somebody to Love".

(One thing that is clear is that wealthy violent and dishonest people use their
wealth and neuron writing to influence popular music. For an excluded, it's
hard to know where this happened. One typical example may be John Lennon's "Out
the Blue" which contains a possible homicidal suggestion "...you came to
me...and blew away life's misery..."- probably neuron written onto Lennon's
brain by wealthy conservatives. The popularity of "Hey Joe" and "I Shot the
Sheriff"- probably conservatives who prefer and insist on associating black
people with violence against women and police. "Down By The River (I shot my
lady)" onto the brain of the anti-Nixon Neil Young. Mostly the writing is meant
to mislead the public who repeatedly hear popular songs many times in their
life. Many of us know the feeling of humming a song, having no idea how the
song got into our head, that we suddenly realize has lyrics that are clearly
not to our advantage. Very fast computers analyze and can easily spin human
thought into their desired directions - mostly which is to protect their
direct-to-neuron secret empire, to protect the murderers (Frank Fiorini, Thane
Cesar, the 9/11 killers being easily recognized examples) of many thousands of
non-violent lawful people. For people who understand about neuron writing,
which are few among excluded, you can protect yourself to a certain extent by
realizing that the sounds or feeling in your mind is sent there by violent
criminals trying to mislead the many fine people who may watch your eyes and
hear your thought-audio, and so to counter it with a positive and more helpful
message. The neuron writing is many times very subtle and difficult to detect,
othertimes it seems somewhat obvious. Because so many people listen to
mass-marketed pop music, wealthy people buy ads in the music - and many times
the ads are bought from AT&T neuron services to be neuron written onto an
artist- not bought from or paid to the actual artist - who may be excluded and
completely unaware of direct-to-brain windows. Think of more likely examples of
direct to brain writing. For myself there are some clear examples - two being
"Is It Dead?", "How Will They Take Me?"- clearly the desired impression is
anything relating to suicide and homicide - but after becoming aware of this -
I changed the theme of many of my songs to "stop violence, teach science",
"lock up the violent, free the nonviolent", "brain imaging machine", etc. So
the majority of my early works, in particular, those after I attained some
popularity, are heavily neuron writing influenced in mostly a negative way. It
may even be that many of the songs that we think are original are neuron
written there. many of us constantly feel our muscles moved remotely and so you
have to add up the possibilities of what the view of those on the other side
is. I could place this comment on any song - I don't know if the lyrics of this
song were influenced by neuron writing - but it wouldn't surprise me - for some
violent JFK killers to see some young talented kids in the Bay area - become
worried about the love, science/education and truth movement- and try to
influence it in a variety of ways - by making them appear to be drug addicts,
perverted/sex crazed, for hippies to be associated with violence, with
depression, sadness, despair - not confidence, not sobriety, not anti-violence,
etc. So - many times the original message is a positive and good message - the
violent neuron writers taking only half of a song or a word here or there. The
first lyric in this song is nice "When the truth is found to be lies" - which
applies to all the thousands of lies - the red shift, expanding universe, 19
hijackers, the JFK, RFK murders, that people are far from figuring out seeing
and hearing thought, etc....just thousands of lies passed off as the truth to
the majority of the planet...or religious claims...because eventually people
have to find out the truth.)

San Francisco, California, USA (presumably)  
34 YBN
[12/19/1966 AD]
5799)
(Harvard University) Cambridge, Massachusetts, USA and (University of Maryland)
College Park, Maryland, USA and (National Biomedical Research Foundation)
Silver Springs, Maryland, USA   
34 YBN
[12/19/1966 AD]
5800)
(Harvard University) Cambridge, Massachusetts, USA   
33 YBN
[01/01/1967 AD]
6120) The Doors release "Break on Through (to the Other Side)".

The song also appears as track one on the band's debut album. Elektra Records'
censors objected to the drug use implied by the line "she gets high", which is
repeated in the middle section of the song (after the line "everybody loves my
baby"). The original album version and all reissues until the 1990s have the
word "high" deleted, with Morrison singing "she gets" four times before a final
wail. Live versions and more recent, remastered releases have the full line
portion restored.

(I wonder if the idea of breaking through to the other side relates to those
who do receive direct-to-brain windows and those who do not. For example did
Morrison and the other Doors get direct-to-brain windows? If yes, then what
they saw and wrote about must be influenced by what they saw in their eyes. The
keyboard sounds is very nice and fuzzy - or perhaps that is a guitar -
determine what kind of keyboard.)

Sunset Sound Studios, Los Angeles, California, USA  
33 YBN
[01/13/1967 AD]
6125) The Rolling Stones release "Let's Spend the Night Together".

(There may be a hint about remote neuron writing with "don't worry what's on
your mind.")

  
33 YBN
[02/03/1967 AD]
6119) Jimi Hendrix records "Purple Haze".

(This may mark the beginning of distorted guitar and the dominate role of the
distorted guitar in pop and rock music. This may be viewed as the beginning of
rock or hard rock music. Jimi Hendrix was one of the many people, like Elvis,
John Lennon, JFK, MLK, RFK, indirectly or directly murdered at a young age by
remote neuron writer owners and consumers. The intro is somewhat unusual and
creative. Hendrix's voice sounds a lot like a saxophone. 1967 was a very
prolific year for music.)

(De Lane Lea and Olympic Studios) London, England  
33 YBN
[02/13/1967 AD]
6123) The Beatles release "Strawberry Fields Forever".

(This song, All you need is love, I am the walrus, all represent a change from
strictly traditional pop music with few instruments to a more orchestral type
composition. This year 1967 may represent some kind of planetary high point -
which apparently somewhat collapsed - perhaps with the murder of MLK and RFK in
1968. Because science has been a minority next to religions, it seems like evil
{violence and dishonesty} will have the upper hand for many centuries more
probably.)

(EMI Studios) London, England  
33 YBN
[02/24/1967 AD]
5715)
(University of Wisconsin) Madison, Wisconsin, USA  
33 YBN
[04/03/1967 AD]
6202)
(Gauss Electrophysics, Inc), Santa Monica, California, USA  
33 YBN
[06/01/1967 AD]
6150) The Beatles release "Sgt. Pepper's Lonely Hearts Club Band".

(EMI Studios) London, England  
33 YBN
[06/25/1967 AD]
6122) The Beatles record "All You Need Is Love".

(This period of song writing and recording by the Beatles introduces are larger
focus on the traditional orchestral string instruments which adds a much
fuller, richer and more professional, sophisticated sound. This is like a
mixing of old-world classical with new age guitar-based vocal pop.)

(Olympic and EMI studios) London, England  
33 YBN
[07/03/1967 AD]
5683)
(Harvard University) Cambridge, Massachusetts, USA (and Cornell University,
Ithaca, New York, USA)   
33 YBN
[11/24/1967 AD]
6124) The Beatles release "I am the Walrus".

(Probably there is neuron writing in this song - for example trying to
associate police with pigs, and what might be misinterpreted as an anti-police
message - the goal being to try and turn the large unified police group away
from enjoying or having a positive view of the Beatles. From the violent people
perspective - they probably felt and feel that they need to somehow lower the
popularity of the Beatles and they did this by trying to make them say things
that play on popular mistaken beliefs about them or their views. The snare drum
sounds nice - perhaps recorded twice or some kind of electronic effect?
Determine what effect was used.)

(EMI Studios) London, England  
33 YBN
[12/03/1967 AD]
5725)
(University of Cape Town and Groote Schuur Hospital) Cape Town, South
Africa  
33 YBN
[1967 AD]
3982)
RCA Labs, Princeton, New Jersey, USA  
33 YBN
[1967 AD]
4558)
unknown  
33 YBN
[1967 AD]
5341) In 1980 the Nobel Prize in Physiology or Medicine 1980 is awarded jointly
to Baruj Benacerraf, Jean Dausset and George D. Snell "for their discoveries
concerning genetically determined structures on the cell surface that regulate
immunological reactions".
(Oak Ridge national Laboratory) Oak Ridge, Tennessee, USA  
33 YBN
[1967 AD]
5845)
(Texas Instruments) Dallas, Texas, USA  
33 YBN
[1967 AD]
6118) Aretha Franklin records a version of Otis Redding's song "Respect".

  
33 YBN
[1967 AD]
6344)
  
32 YBN
[01/25/1968 AD]
5755) In 1978, the Nobel Prize in Physiology or Medicine is awarded jointly to
Werner Arber, Daniel Nathans and Hamilton O. Smith "for the discovery of
restriction enzymes and their application to problems of molecular genetics".
(University of Geneva) Geneva, Switzerland  
32 YBN
[02/09/1968 AD]
5739) In 1974, the Nobel Prize in Physics is awarded jointly to Sir Martin Ryle
and Antony Hewish "for their pioneering research in radio astrophysics: Ryle
for his observations and inventions, in particular of the aperture synthesis
technique, and Hewish for his decisive role in the discovery of pulsars".
(Cavendish Laboratory, University of Cambridge) Cambridge, England  
32 YBN
[02/27/1968 AD]
5759) Charpak’s family moves from Poland to Paris when he is seven years old.
During World War II Charpak serves in the resistance and is imprisoned by Vichy
authorities in 1943. In 1944 he is deported to the Nazi concentration camp at
Dachau, where he remains until the camp is liberated in 1945.

In 1992, the Nobel Prize in Physics is awarded to Georges Charpak "for his
invention and development of particle detectors, in particular the multiwire
proportional chamber".
(CERN) Geneva, Switzerland  
32 YBN
[03/11/1968 AD]
5754)
(Harvard University) Cambridge, Massachusetts, USA   
32 YBN
[04/16/1968 AD]
5745)
(The Institute for Cancer Research) Philadelphia, Pennsylvania, USA  
32 YBN
[11/16/1968 AD]
5808)
(G. D. Searle and Co.) Skokie, Illinois, USA  
32 YBN
[11/21/1968 AD]
6126) Jimi Hendrix releases "Crosstown Traffic".

(Record Plant Studios) New York City, New York, USA  
32 YBN
[12/24/1968 AD]
5604)
Moon of Earth  
32 YBN
[1968 AD]
5243)
(Massachusetts Institute of Technology) Cambridge, Massachusetts, USA
(presumably)  
31 YBN
[03/07/1969 AD]
6129) The Who record "I'm Free".

  
31 YBN
[03/21/1969 AD]
5776) In 1972, the Nobel Prize in Physiology or Medicine is awarded jointly to
Gerald M. Edelman and Rodney R. Porter "for their discoveries concerning the
chemical structure of antibodies".

Edelman writes "Neural Darwinism" (1987), which may have information about the
neuron owner unnatural selection of who gets direct-to-brain windows and who
doesn't, which results in an unnecessary genocide of those who the owners of
AT&T view as troublesome - which usually implies that they are very ethical and
honest, non-racist, fair-minded, etc.
(The Rockefeller University) New York City, New York, USA  
31 YBN
[04/??/1969 AD]
5576)
(Albert Einstein College of Medicine) Bronx, New York, USA  
31 YBN
[07/11/1969 AD]
6161) David Bowie releases "Space Oddity".
(Trident Studios) London, England  
31 YBN
[07/21/1969 AD]
655)
Moon of Earth  
31 YBN
[07/28/1969 AD]
5795)
(Cambridge University) Cambridge, England  
31 YBN
[09/15/1969 AD]
5753) In 1978, the Nobel Prize in Physiology or Medicine is awarded jointly to
Werner Arber, Daniel Nathans and Hamilton O. Smith "for the discovery of
restriction enzymes and their application to problems of molecular genetics".
(Johns Hopkins University, School of Medicine) Baltimore, Maryland, USA  
31 YBN
[09/26/1969 AD]
6128) The Beatles release "Here Comes The Sun".
(EMI, Olympic and/or Trident Studios) London, England  
31 YBN
[10/10/1969 AD]
5469)
(Oxford University) Oxford, England  
31 YBN
[10/29/1969 AD]
5733) In 1939 Guillemin with his family fleas Poland with the Nazi invasion.

In 1977, the Nobel Prize in Physiology or Medicine is divided, one half jointly
to Roger Guillemin and Andrew V. Schally "for their discoveries concerning the
peptide hormone production of the brain" and the other half to Rosalyn Yalow
"for the development of radioimmunoassays of peptide hormones".
(Baylor University) Houston, Texas, USA  
31 YBN
[11/07/1969 AD]
6127) Led Zeppelin releases "Whole Lotta Love".

(Olympic Studios) London, England  
31 YBN
[1969 AD]
5840)
(Waseda Univerity) Tokyo, Japan  
31 YBN
[1969 AD]
5841)
  
31 YBN
[1969 AD]
5851) The ARPAnet (Advanced Research Projects Agency NETwork), the research
network funded by the U.S. Advanced Research Projects Agency (ARPA) is started
in 1969. The software is developed by Bolt, Beranek and Newman (BBN), and
Honeywell 516 minicomputers are the first hardware devices used as packet
switches. ARPAnet starts with four sites including two University of California
campuses (Santa Barbara and Los Angeles), the Stanford Research Institute and
the University of Utah. In late 1972, the ARPAnet is demonstrated at the
International Conference on Computers in Washington, DC. This is the first
public demonstration of packet switching. Over the next decade, ARPAnet grows,
and in 1983 with more than 300 computers connected, the cmomunication protocol
is changed to TCP/IP. In that same year, the unclassified military Milnet
network is split off from ARPAnet. As TCP/IP and gateway technologies mature,
the ARPAnet becomes known as "the Internet" and "the Net." Starting in 1987,
the National Science Foundation begins developing a high-speed backbone between
its supercomputer centers. Intermediate networks of regional ARPAnet sites are
formed to connect to the backbone, and commercial as well as non-profit network
service providers are formed to handle the operations. In 1995, commercial
Internet service providers take control of the major backbones, and the
Internet grows exponentially.

(Clearly the direct-to-brain windows network has been operating for at least
200 years - how much of this network makes use of the phone company wires, if
at all, is unknown to we who are excluded, and no doubt to many direct-to-brain
consumers.)
(University of California at Los Angeles) Los Angeles, California, USA and
(Stanford Research Institute) Stanford, California, USA and (University of
California Santa Barbara) Santa Barbara, California, USA, and (University of
Utah) Salt Lake City, Utah, USA  
30 YBN
[01/29/1970 AD]
5836) A CCD is an electronic memory that can be charged by light. CCDs can hold
a charge corresponding to variable shades of light, which makes them useful as
imaging devices for cameras, scanners, and fax machines.

Willard S. Boyle (CE 1924-2011) and George E Smith (CE 1930- ), at Bell labs,
invent the first Charge Coupled Device (CCD). They report this in the journal
"Bell System Technical Journal" as "Charge Coupled Semiconductor Devices". As
an abstract they write:
" In this paper we describe a new semiconductor device
concept. Basically, it consists of storing charge in potential wells created at
the surface of a semiconductor and moving the charge (representing information)
over the surface by moving the potential minima. We discuss schemes for
creating, transferring, and detecting the presence or absence of the charge.
In
particular, we consider minority carrier charge storage at the Si-SiO2
interface of a MOS capacitor. This charge may be transferred to a closely
adjacent capacitor on the same substrate by appropriate manipulation of
electrode potentials. Examples of possible applications are as a shift
register, as an imaging device, as a display device, and in performing logic.".
A second paper is published by Amelio, Tompsett, and Smith immediately
following the first paper, and is titled "Experimental Verification of the
Charge Coupled Device Concept". As an abstract they write:
" Structures have been
fabricated consisting of closely spaced MOS capacitors on an n-type silicon
substrate. By forming a depletion region under one of the electrodes, minority
carriers (holes) may be stored in the resulting potential well. This charge may
then be transferred to an adjacent electrode by proper manipulation of
electrode potentials. The assumptikno that this transfer will take place in
reasonable times with a small fractional loss of charge is the basis of the
charge coupled devices described in the preceding paper. To test this
assumption, devices were fabricated and measurements made. Charge transfer
efficiencies greater than 98 percent for transfer times less than 100 nsec were
observed.".

Before the CCD, AT&T released the "Picturephone" which was a videophone
system, built in 1956. The Picturephone could transmit an image once every two
seconds. By 1964 AT&T released the "Mod 1", a videophone which was shown at the
New York World's fair, and the public was invited to place video calls between
special exhibits at Disneyland and the New York World's Fair.

Smith describes the process that lead to the CCD in his 2009 Nobel Prize
lecture. He states:
"...First, the semiconductor analogy of the magnetic bubble is
needed. The electric
dual is a packet of charge. The next problem is how to store this
charge
in a confined region. The structure which came to mind, of course, was the
simple
MOS capacitor shown in Figure 3. Charge can be introduced into this
depletion region
with the amount of charge stored being the magnitude of
the signal. To understand
this better, a plot of electron energy vs. distance into
the structure is shown in
Figure 4. As charge is introduced into the depletion
region, the potential at the surface
rises until the maximum allowable
charge is reached. Any further charge added will flow
into the substrate.
The last problem was to shift the charge from one site to another,
thereby
allowing manipulation of the information. This is solved by simply placing
the MOS
capacitors very close together as shown in Figure 5, one with charge
and the second
empty. In order to pass the charge from one to the next, one
simply applies a more
attractive voltage to the second, causing its depletion
region to overlap the first and
the charge to flow along the surface to the
silicon-silicon dioxide interface of
the second capacitor.
The original structure using this mechanism to make a shift register
is shown
in Figure 6. Many MOS capacitors are placed closely together in a row and
connect
ed to a three phase voltage source. The top figure shows the storage
phase with Va
applied to one set of electrodes and a smaller rest voltage Vb
applied to the
other two. One site has charge and the other has none. The
second figure shows the
transfer phase where a larger voltage, Vp, is applied
to the adjacent plates to
transfer charge from one to the next. The last two
show resetting the voltages to
the initial state with the charge information
shifted by one site. This is continued to an
output device at the end of the
row in order to read the stored information. Many
other storage and transfer
schemes are possible. The charge can be injected into the
device electrically
at the beginning of the row making a shift register or supplied by light
incident
on a structure with empty cells. Then the amount of charge which accumulates
by the
absorption of photons is determined by the intensity of the
light, and the
resulting charge pattern can then be read out in shift register
fashion after a suitable
integration time.
This completed the basic invention. It should be stressed that the
basic unit
of information in the device was a discrete packet of charge and not the
voltages
and currents of circuit based devices. The CCD is indeed a functional
device and not a
collection of individual devices connected by wires.
Finally, it was decided to go
ahead and fabricate a device to show experimental
feasibility. In less than a week, masks
were made and devices were
fabricated and tested. This first simple structure is
shown in Figure 7. Charge
was introduced in the first MOS capacitor by thermal
generation and then
transferred to the output by applying voltages to the plates
where it was detected
by pushing the charge into the substrate and measuring the
substrate
current.
The first device was very crude but charge transfer was successfully
demonstrated
and this was followed by the first integrated structure, which is shown
in Figure 8.
This device had a three-phase metallization and diffused input
and output
successfully demonstrating that it could be operated as a serial
memory, the first
driving force of the invention. It is no surprise that we tried
to use the eight bit
CCD as a linear scanning imaging device and the first
rather crude image is shown in
Figure 9.
Following the initial experiments, it was evident that the main problem
with
the device was charge transfer inefficiency, the inability to transfer all of
the
charge from one element to the next. The main reason for this was the trapping
of charge
in traps at the silicon-silicon dioxide interface, see Figure 10.
The trapped
electrons would emit at a later time causing smearing of the image.
So Bill and I got
together again and invented the buried channel CCD,
which placed the stored charge
in the interior of the semiconductor where
there was relatively little trapping. The
structure is shown in Figure 11 where
a lightly doped n layer has been added to the
original structure. Once the
layer has been depleted by transferring the electrons
to the output diode,
the resulting potential is shown. Electrons in the channel region
will now
accumulate in the valley created in the interior of the silicon and kept
away
from the surface traps.
A period of rapid development followed both at Bell Labs and
other companies.
One major activity was to make an area imaging device for video
applications.
Many different schemes were devised. The one we chose for
the Picturephone
application is shown schematically in Figure 12. Linear
CCDs are formed side by side
and split into an imaging and storage area.
During a frame time, the image is taken
in the upper region and then transferred
rapidly to the lower where it is read out a line
at a time by the serial
readout while the next frame is being taken. The chip that we
made for the
Picturephone is shown in Figure 13 along with a self-contained
experimental
camera. Successful testing of the device is shown in Figure 14.
...".

(Part of the importance of the CCD is not that it is a variably charged
capacitor, but that there are many capacitors in a small area, which allows
many dots - that is many light beams - of an image to be captured and
permanently recorded.)

(It seems interesting that nobody ever talks about, simply measuring the
differences in resistance caused by varying amounts of light - basically the
photoelectric effect - where there is light the resistance is less. Probaly
this is to mislead the public from the simplicity of these devices.)

(The CCD and electronic images will allow cameras to become very small - in
particular if no image is needed to be stored but instead if the image can
simply be transmitted wirelessly to a stationary receiver that stores all the
transmitted images.)

(It is interesting that the video phone as a device which connects to a phone
port may never actually be realized - because programs like Skype have made
video phone calling over the wired computer and wireless cell phone the
apparent path to video communications until direct-to-brain windows is made
public and available to all people.)
(Bell Telephone Laboratories) Murray Hill, New Jersey, USA  
30 YBN
[02/02/1970 AD]
5518)
(Pennsylvania State University) University Park, Pennsylvania, USA  
30 YBN
[05/??/1970 AD]
6131) Three Dog Night release their version of Randy Newman's "Mama Told Me Not
To Come".

The keyboard used in this song is a Wurlitzer electric piano.

  
30 YBN
[06/02/1970 AD]
5801) In 1975, the Nobel Prize in Physiology or Medicine is awarded jointly to
David Baltimore, Renato Dulbecco and Howard Martin Temin "for their discoveries
concerning the interaction between tumour viruses and the genetic material of
the cell".
(Massachusetts Institute of Technology) Cambridge, Massachusetts, USA and
(University of Wisconsin) Madison, Wisconsin, USA  
30 YBN
[06/10/1970 AD]
6151) Edwin Starr releases the song "War".

(Hitsville USA - Studio A) Detroit, Michigan, USA  
30 YBN
[06/16/1970 AD]
5716) Har Gobind Khorana (CE 1922-), Indian-US chemist, and team synthesize the
first artificial gene, a yeast gene.

Khorana and team publish this in "Nature" as "Total Synthesis of the Gene for
an Alanine Transfer Ribonucleic Acid from Yeast". They write as an abstract:
"by exploiting the natural ability of polynucleotides to align by base pairing
and using polynucleotide kinase and ligase, chemically synthesized segments
have been combined into a double stranded DNA corresponding to the gene for the
earliest characterized tRNA.". They conclude by writing:
" The priciples used in
present work are such that they allow "welding" of bihelical DNAs to one
another. We hope that these principles will permit studies of the punctuation
marks on DNA by addition of appropriate deoxypolynucleotide sequences at either
end of the synthetic gene. The same principle could be used eventually to add
the synthetic gene to other genomes such as those of the transducing phages.
While all these possibilities belong to the future, the present results
nevertheless seem to give an encouraging start. ...".

Later on August 31, 1970 Khorana, et al will publish details on how a
polynucleotide ligase to join two DNA molecules together. Khorana et al publish
this in the "Proceedings of the National Academy of Sciences" as "Studies on
Polynucleotides, C. A Novel Joining Reaction Catalyzed by the T4-Polynucleotide
Ligase". For an abstract they write:
"Abstract. The polynucleotide ligase isolated
from T4-infected Escherichia coli
was previously shown to bring about repair of
breaks in the single strands of bihelical
DNA. The present work shows that the enzyme can
also catalyze the
joining of DNA duplexes at their base-paired ends. This novel
reaction occurs
-hen the deoxynucleoside at a 5'-end carries a phosphate group and the
complementary
deoxynucleoside opposite to it carries a 3'-hydroxyl group. The
consequence is the
lengthening of the original duplex to form dimers or oligomers
depending upon whether one
or both ends are base-paired.".
(University of Wisconsin) Madison, Wisconsin, USA  
30 YBN
[09/08/1970 AD]
5574)
(University of California) San Francisco, California, USA  
30 YBN
[09/13/1970 AD]
6345) The Santa Ana, California, "Register" prints a photo of a thought screen.
Santa Ana, California, USA  
30 YBN
[09/24/1970 AD]
5600)
(80 km SE of the city of) Dzhezkazgan, Kazakhstan (was U.S.S.R.)  
30 YBN
[12/15/1970 AD]
5617)
Planet Venus  
30 YBN
[12/??/1970 AD]
6134) Gordon Lightfoot releases "If You Could Read My Mind" which strongly
hints about remote neuron reading.

(Perhaps there is a play on -if you could read my mind 'what a tail' - for
example you would see many buttocks' on people's thought-screens. Did Lightfoot
receive direct-to-brain windows? If no, then he perhaps accidentally hinted
about a massive secret industry, but if yes, then he may have been labeled a
"rat" for his care and concern for the human species. "Wishing well" may relate
to "William Wollaston" - but neuron reading may go back much longer - perhaps
even to the 1300s.)

  
30 YBN
[1970 AD]
5842)
  
30 YBN
[1970 AD]
6130) Crosby, stills, Nash and Young release their version of Joni Mitchell's
song "Woodstock".

  
30 YBN
[1970 AD]
6149) Black Sabbath release "Paranoid".

(This song represents the beginning of heavy metal music.)

  
29 YBN
[01/01/1971 AD]
5519)
(Pennsylvania State University) University Park, Pennsylvania, USA  
29 YBN
[01/15/1971 AD]
1133) Lithium iodine battery. Inventor Wilson Greatbatch will adapt this
battery by 1972 for use in pacemakers. The lithium iodine batter has a long
lifetime of 10 years and is used in pacemakers.
(Catalyst Research Corporation) Baltimore, Maryland, USA  
29 YBN
[01/??/1971 AD]
5523) Wheeler, is the son of librarians, and first becomes interested in
science as a boy reading scientific articles.
Wheeler helps develop the hydrogen bomb at
Los Alamos, New mexico (CE 1949–51).
(Princeton University) Princeton, New Jersey, USA  
29 YBN
[04/19/1971 AD]
5667)
(Baikonur Cosmodrome) Tyuratam, Kazakhstan (was Soviet Union) (verify)  
29 YBN
[05/06/1971 AD]
5734)
(V.A. Hospital and Tulane University School of Medicine) New Orleans,
Louisiana, USA  
29 YBN
[05/06/1971 AD]
5735)
(V.A. Hospital and Tulane University School of Medicine) New Orleans,
Louisiana, USA  
29 YBN
[05/28/1971 AD]
6132) John Lennon records the song "Imagine" which is released October 11,
1971.

In June Elvis will record "There is no God But God".

(This song helps for people to learn the truth about the mistaken beliefs of
the religions. 1971 must have been a year in which goodness made a comeback
from 1967-68 when MLK and RFK were successfully murdered. But in 1977 Elvis
dies most likely as a result of particle murder, and John Lennon will be
murdered by an excluded {presumably} who is remotely neuron written on in 1980.
These deaths may have been some kind of retaliation by wealthy people invested
in organized religions, or perhaps just some anti-popular, anti-democracy,
anti-truth violent wealthy people.)
  
29 YBN
[06/09/1971 AD]
6133) Elvis records "There is no God but God".

Months earlier John Lennon had recorded the song "Imagine".

(Notice the play on the phrase "there is no god" and then as if this was spoken
by a "butt(ocks) god". It is really an interesting phenomenon. Because Elvis
must have been somewhat worldly, wealthy, well-informed - probably received
direct-to-brain windows. But realized that most people are excluded, and very
strong believers in Christianity. So, as has the case for many of the earth's
best song writers, there was a double-meaning which pleases conservatives and
also has an underlying joke that pleases educated liberal minded people.
William Byrd even clearly does this as early as the 1500s.)

(RCA Studio B) Nashville, Tennessee, USA  
29 YBN
[07/15/1971 AD]
5421)
(Eidgenossische Technische Hochschule) Zurich, Switzerland  
29 YBN
[11/09/1971 AD]
5838)
(Bell Telephone Laboratories) Holmdel, New Jersey, USA  
29 YBN
[11/14/1971 AD]
5618) U.S. "Mariner 9" is the first ship from earth to orbit another planet
(Mars).

The Mariner 9 mission results in a global mapping of the surface of Mars,
including the first detailed views of the martian volcanoes, Valles Marineris,
the polar caps, and the satellites Phobos and Deimos. It also provides
information on global dust storms, the triaxial figure of Mars, and the
variable gravity field.
Planet Mars  
29 YBN
[11/27/1971 AD]
5619) Ship impacts Mars (Soviet "Mars 2").

The Soviet Mars 2 and 3 orbiters send back a large volume of data covering the
period from December 1971 to March 1972, although transmissions continue
through August. It is announced that Mars 2 and 3 have completed their missions
by 22 August 1972, after 362 orbits completed by Mars 2 and 20 orbits by Mars
3. The probes send back a total of 60 pictures. The images and data reveal
mountains as high as 22 km, atomic hydrogen and oxygen in the upper atmosphere,
surface temperatures ranging from -110 C to +13 C, surface pressures of 5.5 to
6 mb, water vapor concentrations 5000 times less than in Earth's atmosphere,
the base of the ionosphere starting at 80 to 110 km altitude, and grains from
dust storms as high as 7 km in the atmosphere. The data enables creation of
surface relief maps, and gives information on the martian gravity and magnetic
fields.

The descent module is separated from the orbiter on November 27, 1971 about 4.5
hours before reaching Mars. After entering the atmosphere at approximately 6
km/sec, the descent system on the module malfunctions, possibly because the
angle of entry is too steep. The descent sequence does not operate as planned
and the parachute does not deploy. The lander impacts Mars at high velocity.
Mars 2 is the first human-made object to reach the surface of Mars.
Planet Mars  
29 YBN
[11/??/1971 AD]
5844)
(Intel Corporation) Santa Clara, California, USA  
29 YBN
[12/02/1971 AD]
5620)
Planet Mars  
29 YBN
[1971 AD]
5843)
  
29 YBN
[1971 AD]
5852)
  
28 YBN
[01/21/1972 AD]
5708) Benacerraf, is born in the Venezuelan capital of Caracas, is brought up
in France and moves to the USA in 1940.

In 1980 the Nobel Prize in Physiology or Medicine is awarded jointly to Baruj
Benacerraf, Jean Dausset and George D. Snell "for their discoveries concerning
genetically determined structures on the cell surface that regulate
immunological reactions".
(Harvard University) Cambridge, Massachusetts, USA   
28 YBN
[04/17/1972 AD]
6160) Elton John releases "Rocket Man".

  
28 YBN
[04/??/1972 AD]
6136) Billy Preston relases the song "Outa-Space".

(1972 introduces the funky sound of the Hohner clavinet electric piano to the
majority of the public.)

  
28 YBN
[07/15/1972 AD]
5621)
Planet Mars  
28 YBN
[07/31/1972 AD]
5751) Proteins are synthesized by adding DNA to bacteria.

US biochemist, Paul Berg (CE 1926- ), creates a technique to recombine DNA
fragments.

In 1970, Har Gobind Khorana (CE 1922- ) and team had used a polynucleotide
ligase to join two DNA molecules.

Berg uses the techniques of Nathans and Hamilton Smith to cut nucleic acid
molecules at specific places and then developed methods for attaching segments
of the molecule to the DNA of a virus or plasmid, which can then enter
bacterial or animal cells. The foreign DNA is incorporated into the host and
causes the synthesis of proteins that are not ordinarily found there. One of
the earliest practical results of recombinant technology is the development of
a strain of bacteria containing the gene for producing the mammalian hormone
insulin.

This allows the creation of a bacteria that can produce useful molecules such
as insulin by simply sewing in the DNA code that produces the insulin protein
into a bacteria, allowing the bacteria to multiply exponentially and then
isolate all the insulin produced. This technology may lead to microorganisms
that can clean oil spills, or concentrate certain minerals from the sea.
Ultimately this technology of genetic modification may lead to species,
including humans that do not age and can grow replacement body parts. One
dangerous aspect is that new viruses, bacteria and protists might be created
for which the human immune system has no natural defense for and so some of
this research is regulated and certain aspects of genetic modification, for
example in food sources, is opposed by many humans. Since this time, the
dangers have been found to be exaggerated and some relaxation of controls has
taken place.

Paul Berg, David A. Jackson, and Robert H. Symons publish this in "Proccedings
of the National Academy of Sciences" as "Biochemical Method for Inserting New
Genetic Information into DNA of
Simian Virus 40: Circular SV40 DNA Molecules
Containing Lambda Phage Genes and the Galactose Operon of Escherichia coli".
For an abstract they write:
"We have developed methods for covalently
joining duplex DNA
molecules to one another and have
used these techniques to construct circular dimers
of
SV40 DNA and to insert a DNA segment containing lambda
phage genes and the galactose
operon of E. coli into SV40
DNA. The method involves: (a) converting circular
SV40 DNA to a
linear form, (b) adding single-stranded
homodeoxypolymeric extensions of defined composition
and length to
the 3' ends of one of the DNA strands with
the enzyme terminal deoxynucleotidyl
transferase (c)
adding complementary homodeoxypolymeric extensions
to the other DNA strand,
(d) annealing the two DNA molecules
to form a circular duplex structure, and (e) filling
the gaps
and sealing nicks in this structure with E. coli
DNA polymerase and DNA ligase to
form a covalently
closed-circular DNA molecule.". In their paper they write:
"Our goal is to
develop a method by which new, functionally
defined segments of genetic information can be
introduced into
mammalian cells. It is known that the DNA of the transforming
virus SV40 can
enter into a stable, heritable, and
presumably covalent association with the
genomes of various
mammalian cells (1, 2). Since purified SV40 DNA can also
transform cells
(although with reduced efficiency), it seemed
possible that SV40 DNA molecules, into
which a segment of
functionally defined, nonviral DNA had been covalently
integrated, could
serve as vectors to transport and stabilize
these nonviral DNA sequences in the cell
genome. Accordingly,
we have developed biochemical techniques that are
generally applicable for
joining covalently any two DNA
molecules. Using these techniques, we have
constructed
circular dimers of SV40 DNA; moreover, a DNA segment
containing X phage genes and the
galactose operon of Escherichia
coli has been covalently integrated into the circular
SV40 DNA
molecule. Such hybrid DNA molecules and others
like them can be tested for their
capacity to transduce foreign
DNA sequences into mammalian cells, and can be used to
determ
ine whether these new nonviral genes can be expressed
in a novel environment. ...
DISCUSSION
The methods described in this report for the covalent joining
of two SV40 molecules and
for the insertion of a segment
of DNA containing the galactose operon of E. coli into
SV40
are general and offer an approach for covalently joining any
two DNA molecules
together. With the exception of the fortuitous
property of the RI endonuclease, which
creates convenient
linear DNA precursors, none of the techniques used
depends upon any unique
property of SV40 and/or the Xdvgal
DNA. By the use of known enzymes and only minor
modifications
of the methods described here, it should be possible
to join DNA molecules even if they
have the wrong combination
of hydroxyl and phosphoryl groups at their termini. By
judicious
use of generally available enzymes, even DNA
duplexes with protruding 5'- or
3'-ends can be modified to
become suitable substrates for the joining reaction.
One
important feature of this method, which is different
from some other techniques that can
be used to join unrelated
DNA molecules to one another (16, 19), is that here the
joining
is directed by the homopolymeric tails on the DNA. In
our protocol, molecule A and
molecule B can only be joined
to each other; all AA and BB intermolecular joinings and
all
A and B intramolecular joinings (circularizations) are prevented.
The yield of the desired
product is thus increased,
and subsequent purification problems are greatly reduced.
For some
purposes, however, it may be desirable to insert
Xdvgal or other DNA molecules at
other specific, or even random,
locations in the SV40 genome. Other specific
placements
could be accomplished if other endonucleases could be found
that cleave the SV40
circular DNA specifically. Since pancreatic
DNase in the presence of Mn2+ produces
randomly
located, double-strand scissions (17) of SV40 circular DNA
(Jackson and Berg, in
preparation), it should be possible to
insert a DNA segment at a large number of
positions in the
SV40 genome.
...".

A year later, in July 1973, Stanley N. Cohen, Annie C. Y. Chang, Herbert W.
Boyer, and Robert B. Helling publish a method of constructing biologically
functional bacterial plasmids in vitro which are inserted into E. coli by
transformation (conjugation).

In Science (July 26, 1974) Paul Berg and others publish a letter describing the
dangers of the uncontrolled practice of recombinant DNA experiments. Berg
consequently proposea an absolute voluntary moratorium on certain types of
experiment and strict control on a large number of others. An international
conference is held in Asilomar, California, followed by the publication of
strict guidelines by the National Institutes of Health in 1976. Berg writes:
"Recent
advances in techniques for
the isolation and rejoining of segments
of DNA now permit
construction of
biologically active recombinant DNA
molecules in vitro. For example,
DNA
restriction endonucleases, which generate
DNA fragments containing cohesive
ends especially
suitable for rejoining,
have been used to create new
types of biologically functional
bacterial
plasmids carrying antibiotic resistance
markers (1) and to link
Xenopus laevis ribosomal DNA
to
DNA from a bacterial plasmid. This
latter recombinant plasmid has been
shown to replicate
stably in Escherichia
coli where it synthesizes RNA that is
complementary to X. laevis
ribsomal
DNA (2). Similarly, segments of
Drosophila chromosomal DNA have
been incorporated into
both plasmid
and bacteriophage DNA's to yield hybrid
molecules that can infect and
replicate in E.
coli (3).
Several groups of scientists are now
planning to use this technology to
create
recombinant DNA's from a
variety of other viral, animal, and
bacterial sources.
Although such experiments
are likely to facilitate the solution
of important theoretical and
practical
biological problems, they would
also result in the creation of novel
types of infectious
DNA elements
whose biological properties cannot be
completely predicted in advance.
There is serious
concern that some of
these artificial recombinant DNA molecules
could prove biologically
hazardous.
One potential hazard in current
experiments derives from the need to
use a bacterium like
E. coli to clone
the recombinant DNA molecules and
to amplify their number. Strains of
E.
coli commonly reside in the human
intestinal tract, and they are capable
of exchanging
genetic information with
other types of bacteria, some of which
are pathogenic to man.
Thus, new
DNA elements introduced into E. coli
might possibly become widely
disseminated
among human, bacterial,
plant, or animal populations with unpredictable
effects.
Concern for these emerging capabilities
was raised by scientists attending
the 1973 Gordon Research
Conference
on Nucleic Acids (4), who requested
that the National Academy of
Sciences give consideration
to these
matters. The undersigned members of
a committee, acting on behalf of and
with the
endorsement of the Assembly
of Life Sciences of the National Research
Council on this matter,
propose
the following recommendations.
First, and most important, that until
the potential hazards of such
recombinant
DNA molecules have been better
evaluated or until adequate methods
are developed for
preventing their
spread, scientists throughout the world
join with the members of this
committee
in voluntarily deferring the following
types of experiments.
- Type 1: Construction of new,
autonomously
replicating bacterial plasmids
that might result in the introduction
of genetic determinants for
antibiotic
resistance or bacterial toxin
formation into bacterial strains that do
not at present
carry such determinants;
or construction of new bacterial plasmids
containing combinations of
resistance
to clinically useful antibiotics
unless plasmids containing such combinations
of antibiotic resistance
determinants
already exist in nature.
i Type 2: Linkage of all or segments
of the DNA's from oncogenic or
other
animal viruses to autonomously
replicating DNA elements such as bacterial
plasmids or other viral
DNA's.
Such recombinant DNA molecules
might be more easily disseminated to
bacterial populations in
humans and
other species, and thus possibly increase
the incidence of cancer or other
diseases.
Second, plans to link fragments of
animal DNA's to bacterial plasmid
DNA or bacteriophage
DNA should be
carefully weighed in light of the fact
that many types of animal cell
DNA's
contain sequences common to RNA
tumor viruses. Since joining of any
foreign DNA to a
DNA replication
system creates new recombinant DNA
molecules whose biological properties
cannot be
predicted with certainty,
such experiments should not be undertaken
lightly.
Third, the director of the National
Institutes of Health is requested to give
immediate
consideration to establishing
an advisory committee charged with
(i) overseeing an experimental
program
to evaluate the potential biological
and ecological hazards of the above
types of recombinant
DNA molecules;
(ii) developing procedures which will
minimize the spread of such molecules
within human
and other populations;
and (iii) devising guidelines to be
followed by investigators working
with
potentially hazardous recombinant
DNA molecules.
Fourth, an international meeting of
involved scientis,ts
from all over the
world should be convened early in the
coming year to review
scientific progress
in this area and to further discuss
appropriate ways to deal with the
potential
biohazards of recombinant
DNA molecules.
...".


(In the view that some unknown virus may be created - it seems clear that micro
and nanotechnology has reached a startling state of development, although
secretly, and that the possibility may exist if not already that humans may
destroy viruses using microscopic or nano-meter sized remotely or self moved
devices.)

(My own feeling is generally of less fear of genetic modification, but I think
the main concern should be securing life on the moon and mars, and after that
probably we will see much more open and experimental genetic experimentation.
The nature of the current modification is similar to natural selection, and in
particular a bacteria simply producing a new known harmless protein seems to me
of little if any risk. For example, I view GMO rice as not risky, but I think
there is a very tiny risk involved in eating all GMO organisms, just like there
is for GMO from natural selection.)

(Could people not simply produce proteins directly from DNA with the correct
M-RNA, T-RNA, ribosomes, amino acids, etc. without the need for bacteria
cells?)
(Stanford University Medical Center) Stanford, California, USA  
28 YBN
[10/02/1972 AD]
5522)
(Rockefeller University) New York City, New York, USA  
28 YBN
[11/??/1972 AD]
6135) Stevie Wonder releases the song "Superstition".

(This introduces the public to the famous sound of the "clavinet" electric
piano made by Hohner. Billy Preston will use the clavinet on many of his songs,
and the clavinet is typically used on many funk recordings.)

New York City, New York, USA  
28 YBN
[12/??/1972 AD]
6138) The O'Jays release "Love Train".

  
28 YBN
[1972 AD]
5074)
(University of London) London, England (presumably)  
28 YBN
[1972 AD]
5790) In 1976, the Nobel Prize in Physics is awarded jointly to Burton Richter
and Samuel Chao Chung Ting "for their pioneering work in the discovery of a
heavy elementary particle of a new kind". (It seems like there is an misplaced
focus on particle collision experiments - that really probably should be on
other more useful and practical science contributions - like neuron reading and
writing, artificial muscle robots, moving life to other planets, teaching the
public the history of science, useful bulk transmutations which will help
humans adapt to life on other planets and moons, etc.)
(Stanford University Stanford Linear Accelerator Center {SLAC}) Stanford,
California, USA  
27 YBN
[03/28/1973 AD]
6153) Led Zeppelin releases "The Ocean".
  
27 YBN
[03/??/1973 AD]
6137) Stevie Wonder releases "You Are the Sunshine of My Life".

  
27 YBN
[04/??/1973 AD]
6170) The Wailers record the Bob Marley and Peter Tosh song "Get Up, Stand Up".

(Harry J. Studios) Kingston, Jamaica  
27 YBN
[07/18/1973 AD]
5752)
(Stanford University School of Medicine) Stanford, California, USA and
(University of California) San Francisco, California, USA  
27 YBN
[10/??/1973 AD]
6157) The O'Jays release "For the Love of Money".

(Give the history of the phaser and wah pedal, both included in this song.)

(Sigma Sound Studios) Philadelphia, Pennsylvania, USA  
27 YBN
[12/03/1973 AD]
5622)
Planet Jupiter  
27 YBN
[1973 AD]
5684) Vitamin B-12 is synthesized by a sequence of more than 100 reactions.

(Determine chronology better.)
(Harvard University) Cambridge, Massachusetts, USA (and Federal Institute of
Technology in Zürich, Switzerland)  
26 YBN
[03/29/1974 AD]
5614)
Planet Mercury  
26 YBN
[07/??/1974 AD]
6139) The Average White Band releases "Pick Up the Pieces".

  
26 YBN
[11/12/1974 AD]
5791) In 1976, the Nobel Prize in Physics is awarded jointly to Burton Richter
and Samuel Chao Chung Ting "for their pioneering work in the discovery of a
heavy elementary particle of a new kind". (It seems like there is an misplaced
focus on particle collision experiments - that really probably should be on
other more useful and practical science contributions - like neuron reading and
writing, artificial muscle robots, moving life to other planets, teaching the
public the history of science, useful bulk transmutations which will help
humans adapt to life on other planets and moons, etc.)
(Stanford University Stanford Linear Accelerator Center {SLAC}) Stanford,
California, USA and (Massachusetts Institute of Technology) Cambridge,
Massachusetts, USA and (Brookhaven National Laboratory) Upton, New York,
USA  
26 YBN
[12/??/1974 AD]
6140) Labelle releases "Lady Marmalade".

(This song makes use of a cowbell.)

  
26 YBN
[1974 AD]
5846) Personal computer.
The Altair 8800, is a microcomputer kit introduced in late 1974
from Micro Instrumentation and Telemetry Systems (MITS). It sold for $400 and
used an 8080 microprocessor. In 1975, it was packaged with the Microsoft MBASIC
interpreter written by Paul Allen and Bill Gates. Although computer kits were
advertised earlier by others, an estimated 10,000 Altairs were sold, making it
the first commercially successful microcomputer.

The Altair 8800 has 256 bytes of memory. (ROM or RAM?)

(Clearly soon, we should see low cost walking robots - the rest of the computer
body.)

Read more: http://www.answers.com/topic/altair#ixzz1NoJknHXS
(Micro Instrumentation and Telemetry Systems) Albuquerque, New Mexico, USA
(verify)  
26 YBN
[1974 AD]
5896)
(Xerox Palo Alto Research Center) Palo Alto, California, USA  
25 YBN
[02/11/1975 AD]
6143) KC and the Sunshine Band release "Get Down Tonight".
  
25 YBN
[03/19/1975 AD]
5717)
(Massachusetts Institute of Technology) Cambridge, MAssachusetts, USA and
(University of Wisconsin) Madison, Wisconsin, USA  
25 YBN
[04/??/1975 AD]
6141) Chicago releases "Old Days".

(By the 1970s, much of professional popular music contains added layers of
strings - in particular violins, which give songs a more professional
sophisticated sound and more subtle depth. This song makes nice use of violin
accents. The more variety a song has, the longer a person can listen to it
before being bored with it- because they start to recognize more subtle parts
of the recording the more times they listen to it. For a song with only 4
instruments, it does not take a lot of time until everything has been heard and
recognized.)
  
25 YBN
[10/20/1975 AD]
5623) The first ship to orbit and land on Venus, and transmit the first image
from the surface of another planet (Soviet "Venera 9").

The orbiter fulfills its communications mission while photographing the
planet's atmosphere in UV light and conducting other investigations. The lander
transmits data from Venus' surface for 53 minutes, including taking a 180°
panorama of the rocky Venusian surface. Illumination at the surface was said to
be as bright as Moscow on a cloudy day in June. Gamma ray measurements indicate
that the probe landed on a basaltic surface. Temperature at the surface is
found to be 460°C (860°F); atmospheric pressure was 90 times that of Earth.
Planet Venus  
25 YBN
[1975 AD]
6371) External object moved by thought.
  
24 YBN
[01/26/1976 AD]
5513)
(University of California) Berkeley, California, USA  
24 YBN
[03/10/1976 AD]
1122) Lithium ion battery.
M. S. Whittingham publishes this in the journal "Science" as
"Electrical Energy Storage and Intercalation Chemistry". As an abstract he
writes:
"The electrochemical reaction of layered titanium disulfide with lithium
giving the
intercalation compound lithium titanium disulfide is the basis of a new
battery
system. This reaction occurs very rapidly and in a highly reversible manner at
ambi
ent temperatures as a result of structural retention. Titanium disulfide is one
of
a new generation of solid cathode materials.".

Intercalation of molecules is the insertion of additional material between the
parts of an existing series.
(Exxon Research and Engineering Company) Linden, New Jersey, USA  
24 YBN
[03/19/1976 AD]
6144) The Doobie Brothers release "Takin' To The Streets".

(Warner Brothers Studios) North Hollywood, California, USA  
24 YBN
[03/??/1976 AD]
5763) Rubbia, McIntyre and Cline describe this in "Proceedings of International
Neutrino Conference" as "Producing Massive Neutral Intermediate Vector
Bosons with
Existing Accelerators". They write as an abstract:
"We outline a scheme of searching for
the massive
weak boson (M = 50 - 200 Gev/c2 ). An antiproton source
is added either to the
Fermilab or the CERN SPS machines
to transform a conventional 400 GeV accelerator into
a
pp colliding beam facility with 800 GeV in the center of
mass (Eeq = 320,000 GeV).
Reliable estimates of production
cross sections along with a high luminosity make
the scheme
feasible.". In their paper they write:
"The past ten years have seen remarkable
progress in the understanding
of weak interactions. First there is the experimental
discovery
of 6S = 0 weak neutral currents,l which when contrasted with
the previous limits on
~S = 1 neutral current decay processes2
leads to the suggestion of additional hadronic
quantum numbers in
nature. 3 Strong evidence now exists for new hadronic quantum
numbers
that are manifested either directly4,5 or indirectly.6 The experimental
discoveries are
complemented by the theoretical progress of
unified gauge theories. 7 ,8 These
developments lead to the expectation
that very massive intermediate vector bosons (50 - 100
Gev/c2 )
may exist in nature. 7 ,8 The search for these massive bosons require
three
separate elements to be successful: a reliable physical
mechanism for production, very
high center of mass energies, and an
unambiguous experimental signature to observe
them. In this note
we outline a scheme which satisfies these requirements and that
could
be carried out with a relatively moqest program at existing proton
accelerators.
We first turn to the production process. We concentrate on
neutral bosons because
of the extremely simple experimental signature
and because production is largely
dominated by a single
production resonant pole in the particle-antiparticle cross
section.
The best production reaction would of course be:
...
where a sharp resonance peak is expected for 2Ee + = 2Ee - = M. In the
Breit-Wigner
approximation near its maximum we get:
(2 )
where f + - i , f are the partial width to
the initial e e state and the
total width, respectively. The decay widths into e+e-
(and ~+~-)
pairs can be calculated in the first order of the semi-weak coupling
constant: f
e+e ± =ru+~- = 1.5 x 10-7 ~ (GeV). For M = 100 GeV,
r e+e - ~ 150 MeV, which is
surprisingly large. The total width is
related to the above quantity by the
branching ratio Be+e - = fe+e-/f
which is unknown. Crude guesses based on quark models
suggest
Be+e - ~ 1/10, giving r = 1.5 GeV or f/2E = 1.5% for M = 100 Gev/c2 •
At the peak
of the resonance, a(e+e - + W0 , 2E = M) = 3n*2 B. ~
~
2.10- 31 cm2 • Neutrino experiments9 have found that ~ > 20 Gev/c2 •
Therefore,
if ~ - ~, the neutral intermediate boson is out of
reach of existing e+e - storage
r~. ngs.
A more realistic production process is the one initiated by
proton-antiproton
collisions:
p + p + we + (hadrons)
which, according to the quark (parton) picture, proceeds by a
reaction
analog to (1), except that now incoming e+ and e- are replaced with
q and q. Strong
support to the idea that Wls are directly coupled to
spin 1/2 point-like
constituents comes from neutrino experimentslO
and from semi-leptonic hadron decays.ll
Furthermore neutrino experiments
provide the necessary structure functions and have set
limits9
(~ 20 GeV) on any nonlocality in the parton form factor. The main
difference with
respect to e+e - ~.s that now the kinematics is largely
smeared out by the internal
motion of q's and q's.
...
We note that calculations of W- production in proton-proton collisions
are very uncertain
in contrast to the present one due to the apparent
small antiparton {ULSF: typo?}
content in the nucleon and the unknown distributions
of this component.
...
We now briefly outline the scheme of transforming an existing
proton accelerator into
high luminosity pp colliding beamsl7 using
standard vacuum (p ~ 10-7 Torr) and the
separate function magnet
system. The main elements are (1) an extracted proton beam to
produce
an intense source of antiprotons at 3.5 GeV/c, and (2) a small ring
of magnets and
quadrupoles that guides and accumulates the p beam,
(3) a suitable mechanism for
damping the transverse and longitudinal
phase spaces of the p beam (either electron
cooling18 or stochastic
cooling19 ), (4) an R.F. system that bunches the protons in the
main
ring and in the cooling ring, (5) transport of the "cooled" R.F.
bunched p beam back
to the main ring for injection and acceleration.
A long straight section of the main ring is
used as pp interaction
region. A schematic drawing of these elements for the FNAL
accelerator
is presented in Fig. 1. The main parameters of the scheme are
summarized in Table
I.
The luminosity for two bunches colliding head-on is estimated
using the relation
L = NpNp- $/a
where
Np and Np are the number of protons and antiprotons circulating
in the machine,
respectively, ~ is the revolution frequency and ~ 15
the effective area of
interaction of the two beams. Np is taken as
1012 protons in one R.F. bunch. The
value of N is limited by the
p
maximum allowed beam-beam tune shift (Np = 1012 for ~v = 0.01). We
have verified
the longitudinal stability of the bunch, the phase area
growth due to R.F. noise,
the transverse wall instability, the headtail
effect and non-linear resonances,
including those arising from
beam-beam interactions. None of these effects appears
to be important.
...
The production of antiprotons at 3.5 GeV is done with protons
from the same accelerator
and with an overall efficiency -pip ~ 4 x 10-6 .
In order to reach Np = 3 x 1010
we need 750 pulses with 10 l3ppp.
About 10 seconds must elapse between puls~s in order
to clear away
the freshly injected antiprotons. 2l Therefore the formation of piS
would
take of the order of few hours.
..."

At CERN, protons are accelerated in a linear accelerator, booster, and proton
synchroton (PS) up to 27 GeV. These protons hit a heavy target (Be). At the
target many particle-antiparticle pairs are released. Some of the antiprotons
are caught in the antiproton cooler (AC) and stored in the antiproton
accumulator (AA). From there they are transferred to the low energy antiproton
ring (LEAR) where experiments take place.

(Describe also how antiprotons are produced. Determine what the proton target
that creates antiprotons is - is it beryllium? Determine how thick the Be is.
State if reflected or transmitted particles are captured.)
Rubbia's father was an
electrical engineer at the local telephone company in Gorizia, Italy, so most
likely Rubbia receives direct-to-brain windows.

In 1984, the Nobel Prize in Physics is awarded jointly to Carlo Rubbia and
Simon van der Meer "for their decisive contributions to the large project,
which led to the discovery of the field particles W and Z, communicators of
weak interaction". (The existence of a W and Z particle, as being a unifying
particle of fundamental forces seems doubtful to me - I can accept that
particles of such masses exist, but doubt that they have anything to do with
particle decay. Knowing that all matter is probably made of light particles,
and that neuron reading and writing has been kept secret for more than 200
years adds a lot of doubt to most modern physics claims.)
(Harvard University) Cambridge, Massachusetts, USA and (University of
Wisconsin) Madison, Wisconsin, USA   
24 YBN
[05/??/1976 AD]
6147) Steve Miller releases the song "Fly Like An Eagle".

  
24 YBN
[07/20/1976 AD]
5624)
Planet Mars  
24 YBN
[11/30/1976 AD]
5695)
(Cambridge University) Cambridge, England  
24 YBN
[12/??/1976 AD]
6145) Heatwave release the song "Boogie Nights".

(Describe the effects used in this recording.)

  
24 YBN
[1976 AD]
5329)
Laetoli, Tanzania, Africa  
23 YBN
[01/??/1977 AD]
5847)
(Commodore International) West Chester, Pennsylvania, USA (verify)  
23 YBN
[01/??/1977 AD]
6152) Heart releases the song "Barracuda".

The song is an aggressive hard rock number notable for a galloping guitar riff
which has often been compared to that of Led Zeppelin's "Achilles Last Stand"
and is noted for its use of natural harmonics, particularly in the intro where
the harmonics are bent using the tremolo arm of the guitar.

  
23 YBN
[05/03/1977 AD]
6148) The Eagles release "Life In the Fast Lane".

(Determine if this is the first use of phaser. It's interesting that this
guitar riff is similar to the famous riff of "Walk This Way", but distinctly
different, and both are released in the same year.)

  
23 YBN
[05/19/1977 AD]
5771)
(P. N. Lebedev Physics Institute, USSR Academy of Sciences) Moscow, USSR (now
Russia)  
23 YBN
[12/13/1977 AD]
6146) The Bee-Gees release "Stayin' Alive".

(Disco, to some extent marks the beginning of the use of synthesized drums as
opposed to the standard drum set. In addition, violin accenting, which become
popular starting in the 1970s is a nice edition to this song.)

(Château d'Hérouville,)Hérouville, France  
23 YBN
[1977 AD]
5738)
  
23 YBN
[1977 AD]
6045)
Los Angeles, California, USA (verify)  
23 YBN
[1977 AD]
6277)
(University of Illinois at Chicago) Chicago, Illinois, USA  
23 YBN
[1977 AD]
6312) Self-driving car.

The first common road driving autonomous car is the Intelligent Vehicle of the
Tsukuba Mechanical Engineering Laboratory which tests a car in 1977 that can
follow roads for up to 50 meters at speeds up to 30 km/h.
(Tsukuba Mechanical Engineering Lab) Japan  
22 YBN
[05/15/1978 AD]
5831)
(The Rockefeller University) New York City, New York, USA  
22 YBN
[07/25/1978 AD]
5810)
(General Hostpial) Oldham, UK  
22 YBN
[10/27/1978 AD]
6154) Gloria Gaynor releases "I Will Survive".

  
21 YBN
[01/15/1979 AD]
6203) (This method of laser burning makes lasers that can burn widely
available, although using them as a weapon is beyond the skills of the average
person. The publication of the maser also opened the possibility of people in
the public developing maser weapons, but probably the nanotechnology is so
advanced that the biggest danger is still, as has been for many centuries,
violent people who already have access to the nanotechnology, who apparently
cannot be even shown to the public and certainly not stopped, 9/11, the Kennedy
murders, and so many other millions of murders being obvious examples.)
Eindhoven, Netherlands  
21 YBN
[03/05/1979 AD]
5630)
Planet Jupiter  
21 YBN
[07/09/1979 AD]
5633)
Jupiter  
21 YBN
[08/??/1979 AD]
6155) "The Sugarhill Gang" release "Rapper's Delight" which uses the bass and
guitar melody from Chic's "Good Times".

(This song marks the beginning of modern rap music. Describe rap more -
basically the vocal is mostly monotone and not singing.)

(Sugar Hill Studios) Englewood, New Jersey, USA  
21 YBN
[09/01/1979 AD]
388) Ship from Earth, the U.S. "Pioneer 11", passes and sends close images of
planet Saturn.

Pioneer 11 flies to within 13,000 miles of Saturn and takes the first close-up
pictures of the Saturn. Instruments locate two previously undiscovered small
moons and an additional ring, chart Saturn's magnetosphere and magnetic field
and determine that its planet-size moon, Titan, is too cold for life. Flying
underneath the ring plane, Pioneer 11 sends back images of Saturn's rings. The
rings, which normally appear bright when observed from Earth, appeared dark in
the Pioneer pictures, and the dark gaps in the rings seen from Earth appear as
bright rings.
Planet Saturn  
21 YBN
[09/01/1979 AD]
5625)
Planet Saturn  
21 YBN
[09/07/1979 AD]
6158) Buggles releases "Video Killed The Radio Star".

  
21 YBN
[1979 AD]
6156) Chic releases "Good Times".
  
21 YBN
[1979 AD]
6159) The Talking Heads release "Life During Wartime".

Written about life in New York City during the late nineteen seventies, this
song describes life in an impoverished metropolis. Byrne describes life in New
York as a metaphor for WWII-era civilians and argues against the concept that
life there is bohemian by saying, 'This ain't no party. This ain't no disco.
This ain't no foolin' around.' The wartime imagery is taken further by images
of having to stand away from windows for fear of being shot and people living
on the street long beyond the thought of having food to eat.

(The line "this ain't no disco" has a comedic sense of truth when applied to
this dim era of the direct-to-brain secret, expanding universe, mass secret
neuron murders, although perhaps that was not the original intent.)

  
20 YBN
[06/06/1980 AD]
5514)
(University of California) Berkeley, California, USA  
20 YBN
[09/12/1980 AD]
6189) (IBM Zurich Research Laboratory) Ruschlikon, Zurich, Switzerland
(presumably)  
20 YBN
[11/12/1980 AD]
5631)
Planet Saturn  
19 YBN
[05/11/1981 AD]
6162) George Harrison releases "All Those Years Ago".

  
19 YBN
[08/05/1981 AD]
5634)
Saturn  
19 YBN
[08/12/1981 AD]
5848)
(International Business Machines) Boca Raton, Florida, USA  
19 YBN
[11/12/1981 AD]
5805)
(Launch Pad 39A) Merritt Island, Florida, USA  
18 YBN
[03/01/1982 AD]
5626)
Planet Venus  
18 YBN
[04/09/1982 AD]
5729) In 1997, the Nobel Prize in Physiology or Medicine is awarded to Stanley
B. Prusiner "for his discovery of Prions - a new biological principle of
infection".
(University of California) San Francisco, California, USA  
18 YBN
[04/30/1982 AD]
6188)
In 1986 , the Nobel Prize in Physics is divided, one half awarded to
Ernst Ruska "for his fundamental work in electron optics, and for the design of
the first electron microscope",the other half jointly to Gerd Binnig and
Heinrich Rohrer "for their design of the scanning tunneling microscope".
(IBM Zurich Research Laboratory) Ruschlikon, Zurich, Switzerland  
18 YBN
[10/01/1982 AD]
5806)
(Sony Corporation) Japan (presumably)  
18 YBN
[10/08/1982 AD]
5807)
(Institut fur Kernphysik, Technische Hochschule Darmstadt) Darmstadt, Federal
Republic of Germany (now Germany)  
18 YBN
[1982 AD]
5853)
  
18 YBN
[1982 AD]
6164) Thomas Dolby releases "She Blinded Me with Science".

  
18 YBN
[1982 AD]
6166) Alan Parsons Project releases "Eye in the Sky" which hints about the
secret of remote neuron reading.

  
17 YBN
[02/14/1983 AD]
6163) Michael Jackson releases "Beat It".

  
17 YBN
[06/13/1983 AD]
5627)
Planet Neptune  
17 YBN
[10/25/1983 AD]
5811)
(Yale University) New Haven, Connecticut, USA  
17 YBN
[1983 AD]
5764)
(CERN) Geneva, Switzerland  
16 YBN
[01/12/1984 AD]
5809)
(University of Basel) Basel, Switzerland and (Indiana University) Bloomington,
Indiana, USA  
16 YBN
[03/10/1984 AD]
5814) In 1996 Ian Wilmut, Keith Campbell and team at Scotland's Roslin
Institute will clone a sheep (Dolly) from a nucleus of an adult somatic cell.

Steen Malte Willadsen and Robert A. Godke publish this in the journal
"Veterinary Record" as "A simple procedure for the production of identical
sheep twins". For an abstract they write:
"Eggs were collected surgically on day 6, 7
or 8 from 18 Jacob ewes mated to a Welsh mountain ram. Thirty one (86 per cent)
of the 36 eggs ovulated were recovered and of these 27 (87 per cent) had
developed normally. All ovulated eggs were collected from 14 of the ewes. One
(or more) normally developing morula or blastocyst was collected from 16 of the
ewes. While the ewes remained under general anaesthesia each embryo was divided
into two 'half' embryos with a thin glass needle. One monozygotic pair of
'half' embryos was retransferred to the embryo donor. The two ewes from which
no normal embryos had been recovered were used as recipients for surplus
bisected embryos from two other donors. Two of the 18 ewes returned to oestrus.
The remaining 16 went to term producing, in all, eight pairs of identical
twins, one pair of non-identical twins and seven single lambs.".
(AFRC Institute of Animal Physiology) Cambridge, UK  
16 YBN
[06/25/1984 AD]
5815)
(University of California) Berkeley, California, USA  
16 YBN
[08/31/1984 AD]
6190)
(IBM Zurich Research Laboratory, Switzerland, presented in) Prague,
Czechoslovakia  
16 YBN
[10/04/1984 AD]
5812)
(University of Arizona) Tuscon, Arizona, USA and (Jet Propulsion Laboratory)
Pasadena, California, USA  
16 YBN
[11/16/1984 AD]
5813)
(University of Leicester) Leicester, UK  
16 YBN
[1984 AD]
5854)
  
15 YBN
[01/28/1985 AD]
5825)
(Service d'Endocrinologie et des Maladies de la Reproductio) Bicetre,France and
(INSERM U 3 Hôpital de Bicêtre) Bicêtre, France and (CNRS 105), Paris ,
France  
15 YBN
[02/18/1985 AD]
5821)
(Technische Universitat Munchen) Garching, Germany and (Institut Laue-Langevin)
Grenoble, France  
15 YBN
[09/20/1985 AD]
5804) The first stage of the process is to heat DNA containing the required
genetic segment in order to unravel the helix. Primers can then be added to
mark out the target sequence. If, then, the enzyme DNA polymerase together with
a number of free bases are added, two copies of the target sequence will be
produced. These two copies can then be heated, separated, and once more produce
two further copies each. The cycle, lasting no more than a few minutes, can be
repeated as long as supplies last, doubling the target sequence each time. With
geometric growth of this kind, more than 100 billion copies can be made in a
few hours.
Mullis patents this process as "Process for amplifying nucleic acid
sequences." in 1985.

Mullis and Faloona describe this process in a 1987 paper in the journal
"Methods in Enzymology" as "Specific synthesis of DNA in vitro via a
polymerase-catalyzed chain reaction". They write:
"We have devised a method whereby a
nucleic acid sequence can be
exponentially amplified in vitro. The same method can
be used to alter the
amplified sequence or to append new sequence information to
it. It is
necessary that the ends of the sequence be known in sufficient detail
that
oligonucleotides can be synthesized which will hybridize to them, and
that a small
amount of the sequence be available to initiate the reaction. It
is not necessary
that the sequence to be synthesized enzymatically be
present initially in a pure
form; it can be a minor fraction of a complex
mixture, such as a segment of a
single-copy gene in whole human DNA.
The sequence to be synthesized can be present
initially as a discrete
molecule or it can be part of a larger molecule. In either case,
the product
of the reaction will be a discrete dsDNA molecule with termini
corresponding
to the 5' ends of the oligomers employed.
Synthesis of a 110-bp fragment from a larger
molecule via this procedure,
which we have termed polymerase chain reaction, is depicted
in
Fig. 1. A source of DNA including the desired sequence is denatured in
the
presence of a large molar excess of two oligonucleotides and the four
deoxyribonucleo
side triphosphates. The oligonucleotides are complementary
to different strands of the
desired sequence and at relative positions
along the sequence such that the DNA
polymerase extension product
of the one, when denatured, can serve as a template for
the other, and
vice versa. DNA polymerase is added and a reaction allowed to
occur.
The reaction products are denatured and the process is repeated until the
desired
amount of the l l0-bp sequence bounded by the two oligonucleotides
is obtained.
During the first and each
subsequent reaction cycle extension of each
oligonucleotide on the original template
will produce one new ssDNA
molecule of indefinite length. These "long products" will
accumulate in a
linear fashion, i.e., the amount present after any number of
cycles will be
linearly proportional to the number of cycles. The long products
thus
produced will act as templates for one or the other of the oligonucleotides
during subsequent
cycles and extension of these oligonucleotides by polymerase
will produce molecules of a
specific length, in this case, 110 bases
long. These will also function as templates
for one or the other of the
oligonucleotides producing more 110-base molecules.
Thus a chain reac-
tion can be sustained which will result in the accumulation of a
specific
110-bp dsDNA at an exponential rate relative to the number of cycles.
Figure 2
demonstrates the exponential growth of the 110-bp fragment
beginning with 0.1 pmol of a
plasmid template. After 10 cycles of polymerase
chain reaction, the target sequence was
amplified 100 times. The
data have been fit to a simple exponential curve (Fig.
2B), which assumes
that the fraction of template molecules successfully copied in each
cycle
remains constant over the 10 cycles. ...
Amplification of this same 110-bp
fragment
starting with I /zg total human DNA (contains approximately 5 × 10 -19
mol of the
target sequence from a single-copy gene) produced a 200,000-
fold increase of this
fragment after 20 cycles. This corresponds to a calculated
yield of 85% per cycle.~ This
yield is higher than that in the first
example in which the target sequence is
present at a higher concentration.
It is likely that when the target DNA is present in high
concentrations,
rehybridization of the amplified fragments occurs more readily than their
hybridizatio
n to primer molecules.
...
The polymerase chain reaction has thus found immediate use in developmental
DNA diagnostic
procedures L3 and in molecular cloning from
genomic DNA2; it should be useful
wherever increased amounts and relative
purification of a particular nucleic acid
sequence would be advantageous,
or when alterations or additions to the ends of a sequence
are
required.
We are exploring the possibility of utilizing a heat-stable DNA polymerase
so as to avoid
the need for addition of new enzyme after each
cycle of thermal denaturation; in
addition, it is anticipated that increasing
the temperature at which the priming and
polymerization reactions take
place will have a beneficial effect on the specificity
of the amplification."
In 1993, the Nobel Prize in Chemistry is awarded "for contributions to
the developments of methods within DNA-based chemistry" jointly with one half
to Kary B. Mullis "for his invention of the polymerase chain reaction (PCR)
method" and with one half to Michael Smith "for his fundamental contributions
to the establishment of oligonucleotide-based, site-directed mutagenesis and
its development for protein studies".
(Cetus Corporation) Emeryville, California, USA  
15 YBN
[12/06/1985 AD]
5816)
(Lanxide Technology Corporation) Newark, Delaware, USA  
14 YBN
[01/24/1986 AD]
5628)
Planet Uranus  
14 YBN
[04/17/1986 AD]
5824) In 1987, the Nobel Prize in Physics is awarded jointly to J. Georg
Bednorz and K. Alexander Müller "for their important break-through in the
discovery of superconductivity in ceramic materials".
(IBM Zurich Research Laboratory) Ruschlikon, Switzerland  
14 YBN
[1986 AD]
567) Cyndi Lauper releases "True Colors".
  
14 YBN
[1986 AD]
5818)
(Peking University) Perking, China (presumably)  
14 YBN
[1986 AD]
5855)
  
13 YBN
[02/06/1987 AD]
5819) Chu was employed by AT&T early in his career. (Perhaps this gave Chu an
advantage in receiving direct-to-brain windows.)
(University of Alabama) Huntsville, Alabama, USA and (University of Houston)
Houston, Texas, USA  
13 YBN
[07/14/1987 AD]
5820)
(University of Michigan) Ann Arbor, Michigan, USA  
13 YBN
[12/14/1987 AD]
5817)
(University of Victoria) Victoria, Canada and (University of British Columbia)
British Columbia, Canada  
12 YBN
[12/14/1988 AD]
6194)
(University of California at Berkeley), Berkeley, California, USA  
12 YBN
[1988 AD]
4621) Information Society releases "What's On Your Mind (Pure Energy)".
  
12 YBN
[1988 AD]
5856)
  
11 YBN
[01/18/1989 AD]
6205)
(University of Minnesota) Minneapolis, Minnesota, USA  
11 YBN
[08/25/1989 AD]
5629) A ship from Earth, the U.S. "Voyager 2", reaches planet Neptune and
transmits the first close images of Neptune, its moons and rings.

In the summer of 1989, NASA's Voyager 2 becomes the first spacecraft to observe
the planet Neptune, its final planetary target. Passing about 4,950 kilometers
(3,000 miles) above Neptune's north pole, Voyager 2 makes its closest approach
to any planet since leaving Earth 12 years earlier. Five hours later, Voyager 2
passes about 40,000 kilometers (25,000 miles) from Neptune's largest moon,
Triton, the last solid body the spacecraft will have an opportunity to examine.
Planet Neptune  
11 YBN
[1989 AD]
6216) Neil Young releases "Keep On Rockin' In The Free World".
  
10 YBN
[01/17/1990 AD]
6191)
(IBM Research Division, Almaden Research Center) San Jose, California,
USA  
10 YBN
[01/29/1990 AD]
6278)
(AT&T Bell Labs) Holmdel, New Jersey, United States  
10 YBN
[02/14/1990 AD]
5632)
Outside star system  
10 YBN
[04/25/1990 AD]
5828)
Earth Orbit (Launched from Launch Pad 39B) Merritt Island, Florida, USA  
10 YBN
[06/11/1990 AD]
5826) SRY is an abbreviation for "sex-determining region of Y chromosome", it
also has the other name: "testis-determining gene". SRY is a gene on the Y
chromosome in humans that encodes a DNA-binding protein (240 amino acids) that
induces differentiation of Sertoli cells in the developing gonad so that they
produce and secrete anti-Müllerian hormone, which causes regression of female
internal genitalia. It also induces Leydig cells to secrete the androgen
necessary for development of male genitalia. The DNA-binding domain (≈80
amino acids) is homologous with that of HMG proteins. Many mutations in the
gene cause familial XY gonadal dysgenesis (i.e. a female phenotype in the
presence of X and Y chromosomes).

Peter N. Goodfellow and team publish this in "Nature" as "A gene from the human
sex-determining region encodes a protein with homology to a conserved
DNA-binding motif". As an abstract they write:
"A search of a 35-kilobase region of
the human Y chromosome necessary for male sex determination has resulted in the
identification of a new gene. This gene is conserved and Y-specific among a
wide range of mammals, and encodes a testis-specific transcript. It shares
homology with the mating-type protein, Mc, from the fission yeast
Schizosaccharomyces pombe and a conserved DNA-binding motif present in the
nuclear high-mobility-group proteins HMG1 and HMG2. This gene has been termed
SRY (for sex-determining region Y) and proposed to be a candidate for the
elusive testis-determining gene, TDF.". (Read more relevent parts.)
(Human Molecular Genetics Laboratory, Imperial Cancer Research Fund) London, UK
(and two other locations)  
10 YBN
[12/20/1990 AD]
6346)
( Abteilung Biophysik der Universitat Ulm) Ulm, Germany  
10 YBN
[1990 AD]
5849)
(Dycam Inc) Ventura Blvd, Woodland Hillsa, California, USA (verify)  
10 YBN
[1990 AD]
6217) C + C Music Factory release "Gonna Make You Sweat (Everybody Dance Now".
  
9 YBN
[10/29/1991 AD]
5635)
Asteroid Gaspra  
9 YBN
[10/29/1991 AD]
5636)
Asteroid Gaspra (Ida encounter must occur later)  
9 YBN
[1991 AD]
5857)
  
8 YBN
[1992 AD]
5859)
  
7 YBN
[1993 AD]
5858)
  
5 YBN
[02/24/1995 AD]
5822)
(Fermi National Accelerator Laboratory) Batavia, Illinois, USA  
5 YBN
[12/07/1995 AD]
396)
Jupiter  
5 YBN
[12/07/1995 AD]
5637)
Planet Jupiter  
5 YBN
[1995 AD]
5850)
(Ricoh) Tokyo, japan (verify)  
5 YBN
[1995 AD]
6325) Natalie Merchant releases the song "Carnival". The lyric "Have I been
blind?" may relate to how many people who are excluded from seeing thought are
in some sense "blind" compared to those who do receive see the thought-screen
with remote neuron reading and writing (direct-to-brain windows).
  
4 YBN
[05/15/1996 AD]
5827)
(Pfizer Central Research) Sandwich, Kent, UK (verify earliest date)  
4 YBN
[08/??/1996 AD]
6165) R. Kelly releases "I Can Believe I Can Fly".

  
4 YBN
[11/25/1996 AD]
186)
  
4 YBN
[11/25/1996 AD]
5829)
(University of Edinburgh, Roslin Institute), Roslin Midlothian, UK  
1 YBN
[09/15/1999 AD]
3887)
(University of California, Berkeley) Berkeley, CA, USA  
1 YBN
[09/20/1999 AD]
5833)
(Washington University School of Medicine) St. Louis, Missouri, USA  
0 YAN
[01/01/0 AD]
55)
  
0 YAN
[01/01/0 AD]
161)
  
0 YAN
[01/01/0 AD]
229)
  
0 YAN
[01/01/0 AD]
230)
  
0 YAN
[01/01/0 AD]
231)
  
0 YAN
[01/01/0 AD]
233)
  
0 YAN
[01/01/0 AD]
294)
  
0 YAN
[01/01/0 AD]
325)
  
0 YAN
[01/01/0 AD]
427)
  
0 YAN
[01/01/0 AD]
445)
  
0 YAN
[01/01/0 AD]
536)
  
0 YAN
[01/01/0 AD]
569)
  
0 YAN
[01/01/0 AD]
595)
  
0 YAN
[01/01/0 AD]
596)
  
0 YAN
[01/01/0 AD]
623)
  
0 YAN
[01/01/0 AD]
674)
  
0 YAN
[01/01/0 AD]
690)
  
0 YAN
[01/01/0 AD]
707)
  
0 YAN
[01/01/0 AD]
740)
  
0 YAN
[01/01/0 AD]
799)
  
0 YAN
[01/01/0 AD]
1069)
  
0 YAN
[01/01/0 AD]
1297)
  
0 YAN
[01/01/0 AD]
1585)
  
0 YAN
[01/01/0 AD]
1772)
  
0 YAN
[01/01/0 AD]
5034)
  
0 YAN
[01/01/0 AD]
5473)
  
0 YAN
[01/01/0 AD]
6311)
  
0 YAN
[02/14/2000 AD]
5638)
Asteroid Eros  
0 YAN
[12/05/2000 AD]
5823)
(Celera Genomics) Rockville, Maryland, USA (and 13 other locations)  
0 YAN
[0 AD]
3706)
Manchester, England  
0 YAN
[0 AD]
3789)
  
0 YAN
[0 AD]
4367) Eduard Buchner's brother Hans Buchner also has achievements in science.
Eduard
Buchner is killed by a grenade wound on the Romanian front fighting for the
Central Powers, which is a terrible waste of an person with science skills and
achievements, just as Moseley died in WW I on the Allied side.
(University of Tübingen) Tübingen, Germany  
0 YAN
[0 AD]
5919) Girolamo Frescobaldi (CE 1583-1643), Italian composer and organist
composes in this time. Johann Sebastian Bach will own a copy of Frescobaldi's
"Fiori musicali" (1635) and learn from it.

(Saint Peter's cathedral) Rome, Italy  
1 YAN
[02/12/2001 AD]
5639)
Asteroid Eros  
1 YAN
[06/28/2001 AD]
6192)
(Hitachi) Japan  
1 YAN
[07/27/2001 AD]
6200) Millimeter scale rotational wing flying device.
Miki and Shimoyama publish this
in the "Journal of Microelectromechanical Systems" as "Dynamics of a
microflight mechanism with magnetic rotational wings in an alternating magnetic
field". As an abstract they write:
"Dynamics of a three-dimensionally movable
microflight mechanism were analyzed both theoretically and experimentally. The
microflight mechanism is composed of magnetic rotational wings that rotate and
generate thrust in an alternating magnetic field and a body with magnetic
anisotropy that contributes to attitude control. The device consisted of
2.5-mm-long wings weighing 3.5 mg which were fabricated with MEMS technology. A
wing rotational frequency of 500 Hz provided enough thrust for liftoff.
Experimental data obtained through high-speed camera images show good agreement
with theory and also quantify the magnetic anisotropy of the microflight
mechanism, which cannot be estimated theoretically. Simultaneous actuation and
attitude control by an external magnetic field presented herein, which
culminated in simplification and small weight of the device and thus the
successful flight, is applicable to other MEMS devices.".
(University of Tokyo) Tokyo, Japan  
1 YAN
[12/??/2001 AD]
6218) Ted Huntington records the "Stop Violence, Teach Science" group of songs.
Irvine, California, USA  
2 YAN
[02/16/2002 AD]
6332) Much of this work is done by teams of people in Massachussets, from
Harvard, MIT, and the company MicroCHIPS Inc. Robert Farra and team publish
this in the journal "Science Translational Medicine" as "First-in-Human Testing
of a Wirelessly Controlled Drug Delivery Microchip". As an abstract they
write:
"The first clinical trial of an implantable microchip-based drug delivery
device is discussed. Human parathyroid hormone fragment {hPTH(1-34)} was
delivered from the device in vivo. hPTH(1-34) is the only approved anabolic
osteoporosis treatment, but requires daily injections, making patient
compliance an obstacle to effective treatment. Furthermore, a net increase in
bone mineral density requires intermittent or pulsatile hPTH(1-34) delivery, a
challenge for implantable drug delivery products. The microchip-based devices,
containing discrete doses of lyophilized hPTH(1-34), were implanted in 8
osteoporotic postmenopausal women for 4 months and wirelessly programmed to
release doses from the device once daily for up to 20 days. A computer-based
programmer, operating in the Medical Implant Communications Service band,
established a bidirectional wireless communication link with the implant to
program the dosing schedule and receive implant status confirming proper
operation. Each woman subsequently received hPTH(1-34) injections in escalating
doses. The pharmacokinetics, safety, tolerability, and bioequivalence of
hPTH(1-34) were assessed. Device dosing produced similar pharmacokinetics to
multiple injections, and had lower coefficients of variation. Bone marker
evaluation indicated that daily release from the device increased bone
formation. There were no toxic or adverse events due to the device or drug, and
patients stated that the implant did not impact quality of life.".

(Determine if earlier devices could be controlled somehow through the skin-
"first intrabody remote control device".)

(I wonder how practical this is because I can't imagine that many doses would
fit in a microchip. Determine how many doses can fit in the device. Doses are
very small= 40 μg. These devices deliver 20 doses. At least one fails to
deliver the drugs.)

(The real importance may be the public report of a remote controlled particle
communication device positioned inside a human body.)
(CCBR-SYNARC) Denmark  
3 YAN
[04/04/2003 AD]
6195)
(University of California at Berkeley), Berkeley, California, USA  
3 YAN
[08/??/2003 AD]
6326) Ted Huntington records the "Complete Freedom of All Information" group of
songs.
Irvine, California, USA  
4 YAN
[01/15/2004 AD]
5640)
Planet Mars  
4 YAN
[06/17/2004 AD]
6204)
(Massachusetts Institute of Technology) Cambridge, Massachusetts, USA  
4 YAN
[07/01/2004 AD]
5641) The U.S. "Cassini" is the first ship to orbit the planet Saturn.
Planet Saturn  
4 YAN
[11/29/2004 AD]
5832)
(Chosun University) Kwangju, South Korea  
4 YAN
[2004 AD]
6327) U2 releases the song "Vertigo".
  
5 YAN
[01/14/2005 AD]
5642) The European Space Agency (E.S.A.) "Huygens" Titan probe is the first
ship to soft-land on a moon of a planet besides earth, landing on Titan, a moon
of Saturn.
Planet Saturn, moon Titan  
7 YAN
[08/??/2007 AD]
1652)
Kenya, Africa  
7 YAN
[10/31/2007 AD]
6187)
(University of California) Berkeley, California, USA  
8 YAN
[05/24/2008 AD]
6168) Ted Huntington releases a version of "Journey To Centauri".
Irvine, California, USA  
8 YAN
[12/10/2008 AD]
3886)
(Collaboration between researchers at two Japanese Universities, two research
Institutes, and ATR Computational Neuroscience Laboratories) Kyoto, Japan  
9 YAN
[10/12/2009 AD]
6207) Laser is microscopic in two dimensions. This laser is 30 micrometers long
and 8 micrometers high (state width).
(Institute for Quantum Electronics) Zurich, Switzerland  
10 YAN
[10/15/2010 AD]
6169) Ted Huntington releases a group of songs titled "Freedom of Speech" which
includes the song "Neuron Writing".

Irvine, California, USA  
10 YAN
[2010 AD]
6167) Many "9/11 truth" songs are produced around this time.

  
11 YAN
[05/02/2011 AD]
6196) Camera is microscopic in two-dimensions. The camera’s diameter is 990
um, the first video camera on Earth with a diameter smaller than 1 mm. The
camera image sensor ship measures 660x660um with resolution 45K pixels.

A few days later on May 13, 2001, Gill and team publish details about a
microscopic camera sensor chip without the need for a lens.

(Note that this camera is microscopic in only 2 dimensions. A microscopic
camera in 3 dimensions probably must use remote particle communication. Perhaps
if the micrometer camera had a wireless device next to it- it could technically
be called the first microscopic camera.)
(Medigus Ltd. and Tower Semiconductor Ltd) Omer, Israel  
11 YAN
[05/08/2011 AD]
6286)
(Mayo Clinic College of Medicine) Rochester, Minnesota, USA  
11 YAN
[07/08/2011 AD]
255)
(Massachusetts Institute of Technology) Cambridge, Massachusetts, USA  
11 YAN
[09/22/2011 AD]
6211)
(University of California) Berkeley, California, USA  
11 YAN
[10/10/2011 AD]
6214)
(Massachusetts Institute of Technology) Cambridge, Massachusetts, USA  
11 YAN
[11/18/2011 AD]
6336)
(IBM Research–Zurich) Rüschlikon, Switzerland  
15 YAN
[2015 AD]
276)
  
15 YAN
[2015 AD]
332)
  
15 YAN
[2015 AD]
6193) Microscopic wireless camera and microphone. This camera uses particle
communication to reduce its size.
  
18 YAN
[2018 AD]
6208)
  
20 YAN
[2020 AD]
337) Remote neuron writing using microscopic devices in neurons is shown
publicly. Microscopic devices enter the human body by the lung, enter the blood
circulation which connects directly to all cells, and position themselves as
human-made cell organelles. External devices communicate with the intracellular
devices to make the neuron cell fire. Using this method, muscles can be
remotely contracted, and images and sounds can be sent directly to brain
(direct-to-brain windows/direct-to-brain videos).

This technology allows humans to communicate by sending and receiving
thought-images and thought-sounds with each other without the need to move
muscles to talk.

Direct neuron writing was accomplished in 1678, and presuming remote neuron
reading and writing was actually discovered in 1310, this means that 710 years
passes before remote neuron writing is demonstrated to the public.
  
20 YAN
[2020 AD]
4559)
unknown  
20 YAN
[2020 AD]
6197) Remote controlled microscopic flying device.

Perhaps this may be published by Berkeley, since they have a history of the
first micromotors and nanomotors or perhaps Japan. It seems likely that this
has already been achieved, given that micromotors, in particular, appear to
function just like any regular motor.
  
25 YAN
[2025 AD]
365)
  
25 YAN
[2025 AD]
680)
  
25 YAN
[2025 AD]
6198) Remote controlled microscopic flying camera.

Perhaps this may be published by the University of California at Berkeley,
since they have a history of the first micromotors and nanomotors. It seems
likely that this has already been achieved, given that micromotors, in
particular, appear to function just like any regular motor.
  
25 YAN
[2025 AD]
6375) Microscopic wireless laser.
  
30 YAN
[2030 AD]
791) Bipedal robots start replacing humans in most low-skill jobs (fast-food,
fruit and vegetable picking, etc).

Many humans will be unemployed, replaced by more efficient, more predictable,
less expensive humanoid robots. However, the majority of humans will probably
vote for a basic standard of living (eradicating starvation, etc) for all
humans at least in developed nations. The development of low-cost humanoid
robots, will change the paradigm of life for humans, no longer will they need
to work or get a job to survive.
  
40 YAN
[2040 AD]
366) Artificial muscle bipedal robot, lighter and more electrically efficient,
than motor robots. Artificial muscles work like human muscles and are much
lighter than electromagnetic motors. These robots are much lighter and more
electrically efficient.

Two leg walking robots that use artificial muscles are mass produced and
available for public to buy. These robots are much lighter weight than the
electromagnetic motor robots, because the artificial muscle fibers move just as
much weight but are much lighter.

These robots do simple work like cleaning, cooking, driving, shopping- routine
tasks that humans do not want to do.
unknown  
40 YAN
[2040 AD]
4561)
unknown  
40 YAN
[2040 AD]
4562)
unknown  
40 YAN
[2040 AD]
4563)
unknown  
40 YAN
[2040 AD]
6206)
  
50 YAN
[2050 AD]
790) Humans walk around with robot servants. These robots record the owner's
daily activities, and perform simple tasks like cleaning floors, dusting,
vacuuming, washing dishes and clothes, security camera, etc.
  
50 YAN
[2050 AD]
4564)
unknown  
50 YAN
[2050 AD]
4565)
unknown  
50 YAN
[2050 AD]
4566)
unknown  
50 YAN
[2050 AD]
6300) Bacteria identified and destroyed by micro or nanometer scale particle
device inside an animal body.
By 2100 all bacteria and even viral diseases can be
stopped by nanometer scale devices.
unknown  
55 YAN
[2055 AD]
6302) Cancer cell growth stopped by microscopic devices.

Microscopic particle communication devices identify and destroy cancer cells
inside an animal body.
unknown  
58 YAN
[2058 AD]
6303) Cancer caused by microscopic particle device inside an animal body.
unknown  
60 YAN
[2060 AD]
4567)
unknown  
60 YAN
[2060 AD]
6301) Virus identified and destroyed by microscopic devices inside an animal
body.
unknown  
80 YAN
[2080 AD]
4568)
unknown  
100 YAN
[2100 AD]
367)
  
100 YAN
[2100 AD]
793) Helicopter-cars form a second line of traffic above the streets. Flying
cars travel over the already exiting roads because of sound level.

Flying cars are the popular alternative to ground cars because of 1)
improvements to safety {emergency landing chutes, airbags, and thrusters), 2)
need to speed, street-level roads are slow and overcrowded 3) lower cost.

These cars are basically low flying, low-noise helicopters with ground driving
abilities built in.

The cars are completely autopilot using cameras and particle distance sensors.
  
100 YAN
[2100 AD]
794)
  
100 YAN
[2100 AD]
4569)
unknown  
100 YAN
[2100 AD]
4570)
unknown  
100 YAN
[2100 AD]
4575)
unknown  
100 YAN
[2100 AD]
4613) All bacteria and viruses conquered. Microscopic devices can identify and
destroy all known bacteria and viruses anywhere inside or outside of the body.
End of
disease caused by bacteria and viruses when caught early enough.
unknown  
120 YAN
[2120 AD]
4571)
unknown  
120 YAN
[2120 AD]
4584)
unknown  
130 YAN
[2130 AD]
4572) Ship lands on an asteroid.
unknown  
140 YAN
[2140 AD]
687)
  
140 YAN
[2140 AD]
4573)
unknown  
150 YAN
[2150 AD]
659)
  
150 YAN
[2150 AD]
4574)
unknown  
150 YAN
[2150 AD]
4576)
unknown  
150 YAN
[2150 AD]
4592) Humans land on Mars.
unknown  
150 YAN
[2150 AD]
6304) Nucleic Acid changed by remote control microscopic devices. This leads to
repair, regrowth and reshaping of damaged cells with microscopic devices.
unknown  
170 YAN
[2170 AD]
4577)
unknown  
180 YAN
[2180 AD]
4594) Humans live on Mars.
unknown  
190 YAN
[2190 AD]
4578)
unknown  
200 YAN
[2200 AD]
792) Robots and other machines have replaced humans in most manual labor tasks
(driving, cleaning, food planting, harvesting, preparing and serving).

In addition, robots dominate the most dangerous parts of law enforcement and
personal security.

Physical pleasure for money, previously outlawed for nearly a century, becomes
the main human-dominated occupation, while robots are very natural and skilled,
the human touch may be preferred for many physical pleasure services.
  
200 YAN
[2200 AD]
795)
  
200 YAN
[2200 AD]
4581)
unknown  
200 YAN
[2200 AD]
6305)
  
210 YAN
[2210 AD]
4582)
unknown  
220 YAN
[2220 AD]
4583)
unknown  
240 YAN
[2240 AD]
4585)
unknown  
250 YAN
[2250 AD]
4586)
unknown  
250 YAN
[2250 AD]
4587)
unknown  
250 YAN
[2250 AD]
4588)
unknown  
250 YAN
[2250 AD]
4589)
unknown  
250 YAN
[2250 AD]
4590)
unknown  
250 YAN
[2250 AD]
4591)
unknown  
260 YAN
[2260 AD]
4593)
unknown  
275 YAN
[2275 AD]
661)
  
280 YAN
[2280 AD]
4595)
unknown  
280 YAN
[2280 AD]
4596)
unknown  
280 YAN
[2280 AD]
4597)
unknown  
280 YAN
[2280 AD]
4598)
unknown  
290 YAN
[2290 AD]
4599)
unknown  
300 YAN
[2300 AD]
4600)
unknown  
300 YAN
[2300 AD]
4601)
unknown  
300 YAN
[2300 AD]
4602)
unknown  
300 YAN
[2300 AD]
4603)
unknown  
310 YAN
[2310 AD]
4604)
unknown  
320 YAN
[2320 AD]
4605)
unknown  
325 YAN
[2325 AD]
781) The majority of humans in developed nations do not believe that any Heaven
or Hell exists.
  
340 YAN
[2340 AD]
4606)
unknown  
350 YAN
[2350 AD]
4607)
unknown  
350 YAN
[2350 AD]
4608)
unknown  
350 YAN
[2350 AD]
4609)
unknown  
350 YAN
[2350 AD]
4610)
unknown  
400 YAN
[2400 AD]
4611)
unknown  
400 YAN
[2400 AD]
4612)
unknown  
420 YAN
[2420 AD]
779)
  
500 YAN
[2500 AD]
683) The removal and conversion of the Venus atmosphere project is started.

This is the first major "removal of gas atmosphere" engineering work of humans.
Eventually the gas surrounding all planets will be removed and consumed.

After most of the gas is removed, and the surface of the planet cools down,
Oxygen and nitrogen gas will be released to create a new atmosphere.

This project removes the Carbon from the atmosphere and converts it to H2, O2.
This process may be done by thousands of surface (and/or low orbit) machines
working in parallel. There is so much gas on Venus, that this process may take
1000 years or more.

Based on a conversion rate of 1km3/day conversion by 1000 machines.

Probably much of the carbon will be used as hydrogen and oxygen for fuel, air,
water and food for humans around Venus, some might eventually be converted into
oxygen and nitrogen and put back into the atmosphere, but some may be sent back
to Earth or stored as big blocks of carbon. Perhaps the stage of filling the
atmosphere of Venus with Nitrogen and Oxygen gas will start only after the
entire atmosphere of Venus is removed.

Presuming a total mass of Venus atmosphere around 4.8 x 1020 kg, if 1 machine
can convert 100,000 kg of atmosphere a day, and 100,000 machines are operating
every day, it would take 131 million years to convert all the atmosphere of
Venus. But perhaps enough can be converted within 1000 years or less to allow
humans to live on the surface.

Another possibility is that the atmosphere could be "darkened" by adding some
matter to prevent light particles reaching the surface, however this might also
stop light particles from the surface exiting.

(Determine quantity of atoms in and mass of Venus atmosphere, and more accurate
estimate of complete conversion. Use Charles' and Avogadro's laws (using Number
of atoms, Pressure, Temperature, Volume).)
  
500 YAN
[2500 AD]
686) End of death by aging.
Using genetic editing, humans grow and develop to age 20,
and then hold that body shape indefinitely, dying only from physical
destruction. Humans now live for thousands of years. This causes the human
population to grow at an extremely rapid pace.

An alternative view has microscopic genetic editing allowing humans to age
extremely slowly and live for millions of years with very little change.

Each new human created by reproduction may be an "improved model", with new
advanced features, and biological problems and useless DNA removed. This may
also just be a reflection of creativity and experimentation, as humans
experiment with an endless combination of possibilities. This shifts the focus
to the problem of how to feed and house the rapidly increasing quantity of
humans. This will make the exploration of other planets and in particular other
stars to be an absolute requirement, in particular for humans who want to
reproduce but are not allowed to because of the extremely limited resources on
Earth and the human home star. Humans will probably reach a steady state
equilibrium, living for thousands of years. A very few will die in accidents,
and their matter will be recycled, and a new human can then take their place
using the resources they would have used. If humans are not wise, there may be
terrible struggles because the need for food greatly outweighs the tiny supply
of food. Ultimately, however, there is more than enough matter and space in the
universe, for all of life, the problem is simply reaching it.

This end of the physical effects of aging, may create a new existence of finite
resources and careful monitoring of human reproduction, in particular if humans
fail to quickly collect other stars. There is only new matter being emitted
from the star, more dense matter will need to come from mining the matter
orbiting other stars. At this point, the matter orbiting the Sun will continue
to increase as a result of more living objects capturing and using sun light to
reproduce. More light particles emitted from the sun will be captured and
staying in orbit around the Sun (in the form of new living objects), that
otherwise would have escaped to other parts of the universe. So in an
interesting occurrence, matter from the Sun, is for the first time, being
captured and held in orbit around the Sun - as a massive matter transfer from
the Sun to the receivers that form a growing sphere around it. Perhaps most
matter will be imported from other stars. For many centuries, humans will be
able to continue living forever, and even be able to reproduce growing off the
mass emitted from the Sun. But clearly, a time will come when perhaps all the
light emitted from the Sun will be captured, perhaps by the distance of Jupiter
or even closer, and so again, the requirement for living objects, in particular
those in outer locations, to move to other stars will be obvious. As in all
historical examples of explorers moving to an undeveloped "new world", the
journey to the other stars will be a harsh and long journey, but as always
historically, there will be much more freedom and space for those who
successfully arrive at the other stars alive.

Eventually, there will be no more uninhabited stars, and the galaxy will reach
the stage of being a globular galaxy. At the stage of a galaxy where all stars
are inhabited, and none are left to claim, there must be basically equilibrium
systems where all matter (minus the light that escape into the space beyond) is
recycled, and very few new living objects can be made...it may be the same old
crew of living objects for millions and millions of years unless they happen to
die. I can see a gruesome view of possibly purposely ending the lives of some
everliving living objects to feed others in a globular galaxy or cluster that
is losing more matter than taking in.

Perhaps making new humans will be outlawed (although sex may still be
acceptable), and only those ever living humans will exist around the star for
century after century. Long lived organisms ads a different aspect to
evolution, for example now, the current cycle of aging to death has some
advantages, because if there is a bad tradition, those who started it may die
and the bad tradition may stop, but in the same way, a good tradition may be
lost and forgotten. With the same organisms ever-living, living all the time
without aging, the movie freezes, and the star system is stuck with the values
of those people, never to change, or only to change very slowly. Still, I
doubt things would be dull, because of the distance and time involved in moving
between stars. There have to be major differences that evolve between people
separated by the great distance between stars.

This greatly increases the population of humans and the rate at which the
population increases. Before this the population was doubling every 40 years,
now the population doubles every 5 years. This makes all later estimates
unclear because this so greatly changes the number of humans and greatly
increases the rate (by necessity) of expansion of humans to the other stars.

The descendants of humans will be competing against living objects that have
probably adapted through natural selection to be far better at survival than
our descendants, in particular because they have. been competing on a larger
scale against more other living objects.
  
500 YAN
[2500 AD]
774)
  
500 YAN
[2500 AD]
776) All people in developed nations no longer attend religious services at
least once a month.
  
550 YAN
[2550 AD]
4615)
unknown  
570 YAN
[2570 AD]
4616)
unknown  
600 YAN
[2600 AD]
4617)
unknown  
650 YAN
[2650 AD]
4618)
unknown  
650 YAN
[2650 AD]
4619) Humans create atoms from light particles. Photon fusion. The reverse of
separating atoms into light particles.

This process may involve focusing light particles to form larger particles,
like electrons, and protons, which can then be collided together to form larger
atoms.

Although it seems logical that somewhere in the universe light particle must
fuse to form larger compound particles, it may be that a more efficient method
may exist such as adding light particles to an atom to cause the atom to create
a new electron, or proton. Perhaps adding light particles to an electron may
cause the electron to divide into two electrons, or perhaps electrons can be
fused together to form protons.

Building atoms may require extreme precision and timing of how to make pieces
of matter group together without dividing the accumulated cluster of matter
into smaller pieces. At first this will probably be more of a theoretical and
scientific achievement and not practical, the more practical process being
separating larger atoms into smaller more useful atoms - like converting Iron
and Silicon into Hydrogen, Oxygen and Nitrogen.

Possibly this may only occur in volumes of large density, and the realization
will simply be that, yes this occurred, but it is of little or no practical
value since getting desired atoms from existing atoms is faster and easier. For
example, there might be some molten object which is bombarded by light
particles, cooled and then the number of atoms determined to be larger than
started with.
unknown  
700 YAN
[2700 AD]
4620) Humans orbit Saturn.
unknown  
701 YAN
[2701 AD]
4560) Humans land on a moon of Saturn.
unknown  
750 YAN
[2750 AD]
4622) Ship reaches other star (Alpha Centauri). First close up pictures of
planets of a different star.

Smaller ships land on all the planets and moons of Centauri.

Robots start mining and building to prepare for the many millions of humans
that will eventually arrive.

Some ships will return matter from Centauri back to Earth.

Bipedal robots land ships and walk around on the surface of the planets and
moons of the three stars of Centauri. This is perhaps 400 years after setting
out from the star of Earth. The ship must travel with a velocity greater than
1% the speed of light to reach Centauri within 400 years. The robots mine the
matter of the planets, build new ships, perform biological and chemical
analysis, sending all information back to the humans of Earth. Probably the
robots will find lots of bacteria which will provide proof that nucleic acids
molecules like DNA and RNA, and even more evolved cells like bacteria and
viruses are common throughout the universe, found on most planets of every
star. Seeing close-up images of planets of a different star will create a large
amount of excitement in the humans on Earth and perhaps boost their confidence
and interest in exploration.
unknown  
765 YAN
[2765 AD]
6209)
Alpha Centauri  
800 YAN
[2800 AD]
24)
  
800 YAN
[2800 AD]
780)
  
800 YAN
[2800 AD]
782)
  
800 YAN
[2800 AD]
4623)
unknown  
800 YAN
[2800 AD]
4624)
unknown  
800 YAN
[2800 AD]
4625)
unknown  
800 YAN
[2800 AD]
4626)
unknown  
800 YAN
[2800 AD]
4627)
unknown  
800 YAN
[2800 AD]
4628)
unknown  
850 YAN
[2850 AD]
4580)
unknown  
900 YAN
[2900 AD]
29) Ship impacts the surface of Jupiter. First image of the surface of Jupiter.
Surface found to be molten liquid, and six times the diameter of Earth, making
Jupiter the second largest solid body of this star system after the Sun.

Perhaps the surface of Jupiter will be found to be molten liquid metal, mostly
iron, silicon and the other most abundant atoms. Because of the high
temperature, perhaps the first image of the surface of Jupiter without any
filter will have to wait until all the gases are removed from the atmosphere of
the planet, and the planet cool enough for the surface to solidify.
unknown  
900 YAN
[2900 AD]
775)
unknown  
900 YAN
[2900 AD]
4629)
unknown  
900 YAN
[2900 AD]
4630)
unknown  
900 YAN
[2900 AD]
4632)
unknown  
950 YAN
[2950 AD]
4633) Humans penetrate the surface of Saturn. As expected, the diameter of
Saturn is 4 times that of Earth (verify) and is molten metal like Jupiter.
unknown  
1,000 YAN
[3000 AD]
4631)
unknown  
1,000 YAN
[3000 AD]
4634)
unknown  
1,000 YAN
[3000 AD]
4635) Ship impacts the surface of Uranus. The diameter is found to be around 3
times that of earth (verify) and is molten metal.
unknown  
1,000 YAN
[3000 AD]
4636) Ship impacts surface of Neptune. Like Uranus, the diameter is found to be
around 3 times that of earth (verify) and is molten metal.
unknown  
1,150 YAN
[3150 AD]
4638)
unknown  
1,200 YAN
[3200 AD]
4614)
Neptune  
1,200 YAN
[3200 AD]
4637)
unknown  
1,200 YAN
[3200 AD]
4639)
unknown  
1,300 YAN
[3300 AD]
777) The majority of humans in traditionally undeveloped nations are not
religious.
  
1,350 YAN
[3350 AD]
4640)
unknown  
1,400 YAN
[3400 AD]
4643) Motion of planet Mars and moons of Mars controlled by orbiting ships.
unknown  
1,500 YAN
[3500 AD]
684)
  
1,500 YAN
[3500 AD]
4642)
unknown  
1,600 YAN
[3600 AD]
4641) Motion of Venus controlled by orbiting ships.
unknown  
1,800 YAN
[3800 AD]
681) Earth Moon population reaches maximum possible (250 trillion).
  
1,800 YAN
[3800 AD]
4645) Motion of Jupiter controlled by orbiting ships.
unknown  
1,800 YAN
[3800 AD]
4655)
Jupiter  
1,900 YAN
[3900 AD]
682)
  
1,900 YAN
[3900 AD]
4647)
unknown  
2,000 YAN
[4000 AD]
4644)
Jupiter  
2,000 YAN
[4000 AD]
4646)
unknown  
2,000 YAN
[4000 AD]
4648)
unknown  
2,100 YAN
[4100 AD]
4649)
unknown  
2,100 YAN
[4100 AD]
4650)
unknown  
2,200 YAN
[4200 AD]
4651)
unknown  
2,200 YAN
[4200 AD]
4652)
unknown  
2,200 YAN
[4200 AD]
4653)
unknown  
2,300 YAN
[4300 AD]
778) All humans in traditionally undeveloped nations are not religious.
  
2,300 YAN
[4300 AD]
4657)
unknown  
2,500 YAN
[4500 AD]
4579) This is based on a conversion rate of 1km3/day conversion by 1000
machines.
  
2,500 YAN
[4500 AD]
4654)
unknown  
2,500 YAN
[4500 AD]
4659) Humans land on surface of Saturn.
unknown  
2,500 YAN
[4500 AD]
4660) Humans land on surface of Uranus.
unknown  
2,500 YAN
[4500 AD]
4661)
unknown  
2,500 YAN
[4500 AD]
4662)
unknown  
2,500 YAN
[4500 AD]
6171)
  
2,600 YAN
[4600 AD]
4663) Atmosphere of Saturn consumed.

The gases in the atmosphere of Saturn are completely consumed. This begins the
emitting of Nitrogen, Oxygen, Carbon Dioxide and other gases to create a warm
temperature on the surface of Saturn. Robots mine the surface of Saturn
exporting the precious matter to the inner star system.
unknown  
2,600 YAN
[4600 AD]
4665) Humans land on and live on the surface of Neptune.
unknown  
2,600 YAN
[4600 AD]
5605) The air of Uranus is completely consumed. This begins the converting of
surface solid atoms into nitrogen, oxygen, and other gases which are released
around Uranus to make an Earth-like atmosphere. This is temporary until most of
the matter of Uranus has been mined and completely separated into its source
photons by consumption as water, food, fuel, building materials, etc. Robots
extract solid matter, mostly metal, from the surface of Uranus which is shipped
back to Earth, Mars and Jupiter for consumption. Much of these ships and robots
are probably owned by humans that live closer to the star.
unknown  
2,700 YAN
[4700 AD]
4666)
unknown  
2,700 YAN
[4700 AD]
4667) The atmosphere (all the free gases) of Neptune consumed. The native gases
will be replaced with oxygen, nitrogen, CO2, and other molecules. The
temperature will be maintained to be similar to Earth temperatures.
Neptune  
2,800 YAN
[4800 AD]
685)
  
2,800 YAN
[4800 AD]
4669)
unknown  
3,000 YAN
[5000 AD]
679)
  
3,000 YAN
[5000 AD]
4656)
Jupiter  
3,000 YAN
[5000 AD]
4668)
unknown  
3,000 YAN
[5000 AD]
4670)
unknown  
3,000 YAN
[5000 AD]
6177)
unknown  
3,100 YAN
[5100 AD]
4664)
Uranus  
3,100 YAN
[5100 AD]
4671)
unknown  
3,200 YAN
[5200 AD]
4673)
unknown  
3,200 YAN
[5200 AD]
6173)
Neptune  
3,500 YAN
[5500 AD]
6176)
Mars  
4,000 YAN
[6000 AD]
4674)
Centauri  
4,000 YAN
[6000 AD]
4675)
unknown  
4,500 YAN
[6500 AD]
4676)
unknown  
9,000 YAN
[11000 AD]
4680)
unknown  
10,000 YAN
[12000 AD]
4681)
unknown  
11,000 YAN
[13000 AD]
4682)
unknown  
12,000 YAN
[14000 AD]
4683)
unknown  
15,000 YAN
[17000 AD]
678)
  
25,000 YAN
[27000 AD]
4677)
unknown  
45,000 YAN
[47000 AD]
4679)
unknown  
50,000 YAN
[52000 AD]
4658) All asteroids in between Mars and Jupiter have been converted into more
humans, fuel and food.
  
55,000 YAN
[57000 AD]
4672) Planet Mercury completely filled with living objects. The matter of
planet Mercury is completely used as fuel and food by life of the earth star.
Mercury now functions as a massive ship. In the absence of an external supply,
it may be that Mercury becomes hollow and ultimately divides into many smaller
ships.
unknown  
60,000 YAN
[62000 AD]
6175) Mars is filled with living objects. There is no more molten material
inside the planet Mars.
Mars  
65,000 YAN
[67000 AD]
6174) Earth is completely filled with living objects.

There is no more molten material inside the Earth. All the molten compressed
matter was extracted, cooled and consumed as building materials, fuel, food,
etc. Earth is completely filled with tunnels, rooms, and living objects. The
inside is connected to the surface by many passages. The sphere of Earth is
held together by metal support structures, and functions as a giant ship. Earth
and the other planets will perhaps function as giant metal ships for a long
time. Possibly the inside of the Earth will be devoid of life, life preferring
to live in orbiting ships. In that case, probably the humans on the surface
would be relocated, and the molten surface of Earth slowly consumed from the
top down. With only light particles from the Sun, matter imported from outer
planets, and other stars, as a source of new matter, the Earth and other
completely developed smaller inner planets have to consume more internal
matter, perhaps hollowing or dividing planets into smaller pieces.
Earth  
70,000 YAN
[72000 AD]
4684)
unknown  
90,000 YAN
[92000 AD]
6210)
unknown  
100,000 YAN
4678)
unknown  
130,000 YAN
100)
  
185,000 YAN
6178) All planets of Sirius consumed.
Sirius  
205,000 YAN
6317)
Sirius  
630,000 YAN
106)
  
100,000,000 YAN
4685) All stars in the Milky Way Galaxy belong to a globular cluster.

It seems safe to presume that by 100 million years from now, all stars in the
Milky Way Galaxy will belong to a globular cluster.
unknown  
20,000,000,000 YAN
4686)
unknown  
30,000,000,000 YAN
4687)
unknown  
40,000,000,000 YAN
4688)
unknown  
"Universe, Life, Science, Future" is published under the GNU license, except where otherwise indicated or determined to be fair use, copyrighted, public domain, CC, GDFL or other license.
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