History of Cosmology

Lives

Isaac Newton

1642 - 1727

Charles-Joseph Messier

1730 - 1817

Made the Messier catalog of nebulous objects.

William Herschel

1738 - 1822

Built telescopes with large mirrors in England, and was funded by King George III to make the telescopes.

Joseph von Fraunhofer

1787 - 1826

Spectroscopy

Jakes Lick

1796 - 1876

William Parsons, Lord Rosse

1800 - Approx. 1887

Ireland

Margaret and William Huggins

1848 - 1915

amateurs

Jacobus Kapteyn

1851 - 1922

Kapteyn Model

Edward Barnard

1857 - 1923

amateur->pro

George Ellery Hale

1868 - 1938

Solar astronomer and great entrepreneur

Vesto Slipher

1875 - 1969

wacky Mars guy

Albert Einstein

1879 - 1955

Harlow Shapley

1885 - 1972

Cepheids

Events

Clockwork Universe

1687

We live in an infinite, static Universe. Since we are not pulled into a tiny ball, the Universe must be static. The smallest heterogeneity would unbalance everything and cause collapse so God steps in from time to time to re-balance everything.

Could use small telescopes with precise measurements to catalog stars and predict locations.

Law of Universal Gravitation

1687

Newton showed that the effects of gravity are everywhere, not just on Earth. The force of gravitation is measurable. If the mass and location is known, the history and future of a system can be predicted. This set up the idea of the "Clockwork Universe" which gave a sense of universal order.

Discovery of Neptune

1781

Triumph of Newtonian physics. Neptune explained Uranus' problematic orbit.

Herschel's Heavens

1784

Herschel decided to make a model of the Universe (with a lot of assumptions).

Stellar Evolution - Herschel

1800

Herschel saw stars that looked different, and concluded that the Universe must be evolving therefore it cannot be static or stable. If the Universe is not stable, there is chaos.

His mirrors tarnished often which required frequent polishing and reshaping the mirror. Professionals did not want to do this.

Fraunhofer Lines

1820

Mapped the spectrograph of the Sun.

Fransou Aragou

1830

"We can never know the composition of the stars..."

SPIRAL GALAXIES - Lord Rosse

1845

Most powerful telescope (6ft), but it couldn't see anything due to weather. Discovered a spiral, cannibal galaxy who's form implied that it must be in motion. Professionals couldn't see these because they had tiny telescopes. Discovered that the Andromeda galaxy is a spiral.

Stellar Spectrum Analysis

1859

Robert Bunsen and Gustav Kirchfhoff discovered laws of spectrum analysis. Absorption lines are from a hot star surrounded by cooler gas. Spectroscopy led to discovery of the Red Shift. Amateurs measured stellar compositions.

REFLECTING TELESCOPES

Approx. 1860

Potential of reflecting telescopes was known, but professionals didn't want to switch.

Angelo Secchi

Approx. 1860

Amateur, Classified stars based on spectra (first serious spectroscopy)

Huggins look at spectrum of green planetary nebulae

1869

They only found a few elements

Norman Lockyer, Henry Draper analyze composition of the Sun

Approx. 1870 - Approx. 1879

Amateurs, discovered Helium

Photography - Henry Draper

1880

Images of Orion Nebula finally did not depend on the eyesight of the observer. Amateurs did the photography because guiding the telescopes for a long night was a lot of work. It also required knowledge of chemistry and some leisure time to tinker with new ideas.

Crossley Reflector

1880 - 1889

Given to Edward Holden (Director of Lick Observatory) which was then used to get Holden fired. Mounting did not follow the stars.

Amateur Comet photograph

1882

Showed that cameras could be used to make maps.

Lick Observatory

1887

Built on top of Mount Hamilton with the biggest refracting telescope.

Michaelson and Morley - Aether

1887

Search for the speed of light - is it constant?
The Aether was the medium through which light traveled and through which the Universe moves.

Isaac Roberts

1888

Amateur astronomer photographed tilted spiral nebula - is it a solar system? He made the first atlas of nebulae.

Dark lanes in space

1890

Found by Edward Barnard

Harvard Observatory Staff "Computers"

1890

Edward Pickering hired a lot of women to catalog stars.

Lowell Observatory

1894

Interpreted the Mars "canals" as evidence of superior intellect. He saw the veins in his own eyes. He mapped his own eyeball...

Problems with Physics - Roentgen

1895

X-rays not predicted

Problems with Physics - Becquerel

1896

Radioactvity

Problems with Physics - Thompson

1897

Discovered electron which was not predicted by Newtonian physics

Yerkes Observatory

1897

Spectrum of Andromeda Galaxy matches Sun

1899

Is this due to Andromeda being similar to the Sun or to the Solar System?

Spectrum of M31 - Julius Scheiner

1899

1899- He took spectrum of spiral nebula M31. Which he noticed looked like that of the sun. Wondered if it was beginning of new solar system, or is it a universe of sun type stars. Worked with spectroscopy. Studied in Berlin at Potsdam observatory because it was still custom to build them in urban areas even though it wasn't the best option.

Separate island Universes

1900

Spiral galaxies are commonplace. Are each of these separate island universes? If our Milky Way has been replicated, are we not special?

JAMES KEELER

1900

Keeler used the Crossley telescope @Lick instead of the refracting. Took hella pictures and found spiral galaxies everywhere. Proved that reflecting telescopes were important to professionals. Estimated that the Crossley could see 0.5 Million spirals.

Max Planck - UV Catastrophe

1901

Quantum theory (photons) helps avoid (UV catastrophe).

Einstein - Photoelectric Effect

1905

Proved quantum theory of light

Einstein - Brownian Motion

1905

Calculate the size of molecules in a liquid.

Mount Wilson

1905

Astrophysical observatory, good seeing, solar telescopes, reflecting (1917). Cosmology needed big money at this point, good seeing, big telescopes, and showed American industrial power.

Special Relativity & E=mc²

1905

Deals with scenarios of an accelerating frame. We need this for GPS.

Spectrographs of spirals look like the Sun

1909

Lick Observatory

Heber Curtis

1910 - 1920

Responsible for the Crossley. Estimated that more than 1 million spirals could be photographed with the Crossley.

Henrietta Levitt

1912

Since the stars in the Small and Large Magellanic Clouds are roughly the same distance from us, their brightness could be compared and a bunch of Cepheid Variables were found.

Cepheid Variable Stars

1912

These stars have a direct relationship between brightness and period which allows astronomers to calculate the distance to the Cepheids. These are known as standard candles.

Galaxies are receeding

1914 - 1924

Vesto Slipher took 70+ hour exposures and measured galaxy velocities. He was hired by Lowell and worked at Mt Wilson Observatory?

Einstein's Theory of General Relativity

1915

Essay on the theory of Gen. Rel. - gravity is a field.
Space tells matter how to act and matter tells space what shape to be. Light is bent by gravity of the Sun - Eddington's experiment.

Mercury is a Problem. Its orbit does not match the Newtonian predictions, but does match Einstein's equations.

General Relativity exists in an accelerated reference frame - non-Euclidean

Comparing Cepheid brightness to period

1918

Harlow Shapley used Solon Bailey's photographs of globular clusters to determine distances to clusters, and suggested that Cepheids could be pulsating stars. Made a graph of Abs, magnitude vs. period (huge problems).

Shapley's Globular Cluster Distribution

1918

Clusters are located in a spherical halo around the sun therefore they are the edges of the Milky Way. This distribution is much bigger than the Herschel Universe. The Universe/galaxy is 10x bigger than thought. Spiral galaxies must be in our Universe because our galaxy is too big for anything else. Used Levitt's catalog of cepheids to estimate the distance.

Einsteinian Universe

1919

1917: Einstein added a cosmological constant to account for his equations saying the Universe would have to be expanding or contracting. He still believed in a static universe.

Could now build a mathematical model of the Universe.

Repercussions: Einstein upset the entire view of the Universe, it was an era of wanting to believe in someone who could fix everything

The Great Debate

1920

George Hale hosted a series of lectures about the scale of the Universe.
The Kapteyn universe is all there is, and it is relatively small, with the sun close to the center. Shapley's universe is also all there is, but it is immense: remember, I used his term "the big galaxy."​

Heber Curtis (Lick Observatory):
-spiral nebulae were separate galaxies
-believed in the Kapteyn Universe (small galaxies in a big universe)
-Evidence:
-edge-on spirals look like the Milky Way
-other galaxies have solar spectra
-supernovae in other galaxies are similar to ours, but further from us
-slipher's spiral velocities
-Shapley's calibration curve was wrong

Harlow Shapley (Mt Wilson):
-spirals are part of the Milky Way, which is huge
-Calibration curve
-astrophysics theory
-the objects in the spirals are in motion (Adriaan von Maanan)
-- the spirals could not be separate, distant, island universes and had to be part of our own galaxy. Nobody has ever discovered just how van Maanan managed to mis-measure the photographs.

Great Debate was a draw, and not resolved until 1923.

Kapteyn Model of the Universe

1922

Redid Herschel's Universe with new observations and statistics. It was 17 kpc wide which was a small universe, but it seemed reasonable.

The Kapteyn universe is all there is, and it is relatively small, with the sun close to the center. Shapley's universe is also all there is, but it is immense: remember, I used his term "the big galaxy."​

200" reflector telescope

1930 - 1939

Palomar, CA

Einstein flees Germany

1933

Became a US citizen and worked at Princeton (1940)

Leo Szilard - atomic bomb

1934

Szilard realizes Einstein's E=mc2 and understanding of nuclei can be used to make a huge bomb.

Problems with Physics - Rutherford

1937

Gold foil experiment

Nuclear fission

1939

Lise Meitner, Otto Hahn

H to He

1939

Hans Bethe explained the life of stars. (Eddington suggested this in 1914.)

BIG SCIENCE

1940

-Meeting at U Cal Berkeley for 184" cyclotron
-largest physics grant ever

Cyclotron

1940

-was not built in Germany (Great Migration)
-women monitored atomic material

Frisch and Peierls realize bomb could be build

1940

-Gen. Graves got secret funding from the government
-Oppenheimer ran the project

Atom Bomb

August 6, 1945

Results of pure and applied physics.