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|Born||November 29, 1889
Marshfield, Missouri, USA
|Died||September 28, 1953
San Marino, California
|Institution||University of Chicago
Mount Wilson Observatory
|Alma mater||University of Chicago
|Known for||Big Bang
Edwin Powell Hubble (November 29, 1889 – September 28, 1953) was born on 29th November, 1889 to an insurance executive in Marshfield, Missouri and moved to Wheaton, Illinois in 1898. In his younger days, he was noted more for his athletic abilities rather than his intellectual genius, although he did earn good grades in every subject, except for spelling. He won seven first places and a third placing in a single high school track meet in 1906. That year he also set a state record for high jump in Illinois.
His studies at the University of Chicago concentrated on mathematics and astronomy which led to a BS degree in 1910. Hubble also became a member of the Kappa Sigma Fraternity and in 1948 was named Kappa Sigma "Man of the Year". He spent the next three years as one of Oxford's first Rhodes Scholars, where he originally studied jurisprudence, before switching his major to Spanish and receiving the MA degree, after which he returned to the United States. Some of his British mannerisms and dress stayed with him all his life, occasionally irritating his more Americanized colleagues.
Returning to the United States he worked as a high school teacher and a basketball coach at New Albany High School in New Albany, Indiana (near Louisville), and practiced law in Kentucky. He served in World War I and quickly advanced to the rank of Major. He returned to astronomy at the Yerkes Observatory of the University of Chicago, where he earned a PhD in 1917 with a dissertation entitled "Photographic Investigations of Faint Nebulae".
In 1919 Hubble was offered a staff position by George Ellery Hale, the founder and director of Carnegie Institution's Mount Wilson Observatory, near Pasadena, California, where he remained until his death. He also served in the US Army at the Aberdeen Proving Ground during World War II. For his work there he received the Legion of Merit. Shortly before his death, Palomar's 200-inch Hale Telescope was completed; Hubble was the first to use it.
He died of a cerebral thrombosis on September 28, 1953, in San Marino, California. His wife, Grace, did not have a funeral for him and never revealed what was done with his body--it was apparently Hubble's wish to have no funeral service and be buried in an unmarked grave, or that he wanted to be cremated. As of now, the whereabouts of his remains are unknown.
 Galaxies exist beyond the Milky Way
Hubble's arrival at Mount Wilson in 1919 coincided roughly with the completion of the 100-inch Hooker Telescope, then the world's largest telescope. Using the Hooker Telescope Hubble identified Cepheid variables (a kind of star; see also standard candle) in several nearby "nebulae" (including the Andromeda Galaxy). His observations in 1923–1924 conclusively proved that these objects were much more distant than previously thought and hence galaxies themselves rather than constituents of the Milky Way. Announced on January 1, 1925, this discovery fundamentally changed mankind's view of the universe.
Hubble also devised a classification system for galaxies, grouping them according to their content, distance, shape, size and brightness.
 Redshift increases with distance
Hubble was generally incorrectly credited with discovering the redshift of galaxies. These measurements and their significance were understood before 1918 by James Edward Keeler (Lick & Allegheny), Vesto Melvin Slipher (Lowell), and Professor William Wallace Campbell (Lick) at other observatories. Combining his own measurements of galaxy distances with Vesto Slipher's measurements of the redshifts associated with the galaxies, Hubble and Milton L. Humason discovered a rough proportionality of the objects' distances with their redshifts. Though there was considerable scatter (now known to be due to peculiar velocities), Hubble and Humason were able to plot a trend line from the 46 galaxies they studied and obtained a value for the Hubble-Humason constant of 500 km/s/Mpc, which is much higher than the currently accepted value due to errors in their distance calibrations. In 1929 Hubble and Humason formulated the empirical Redshift Distance Law of galaxies, nowadays termed simply Hubble's law, which, if the redshift is interpreted as a measure of recession speed, is consistent with the solutions of Einstein’s equations of general relativity for a homogeneous, isotropic expanding space. Although concepts underlying an expanding universe were well understood earlier, this statement by Hubble and Humason led to wider scale acceptance for this view. The law states that the greater the distance between any two galaxies, the greater their relative speed of separation.
This discovery was the first observational support for the Big Bang theory which had been proposed by Alexander Friedmann in 1922. The observed velocities of distant galaxies, taken together with the cosmological principle appeared to show that the Universe was expanding in a manner consistent with the Friedmann-Lemaître model of general relativity. In 1931 Hubble wrote a letter to the Dutch cosmologist Willem De Sitter expressing his opinion on the theoretical interpretation of the redshift-distance relation:
- "... we use the term 'apparent velocities' in order to emphasize the empirical feature of the correlation. The interpretation, we feel, should be left to you and the very few others who are competent to discuss the matter with authority."
Today, the 'apparent velocities' in question are considered to be artifacts of a coordinate transformation that occurs in an expanding space. Light traveling through stretching space will experience a Hubble-type redshift, a mechanism different from the Doppler effect.
In the 1930s Hubble was involved in determining the distribution of galaxies and spatial curvature. These data seemed to indicate that the universe was flat and homogeneous, but there was a deviation from flatness at large redshifts. According to Allan Sandage,
- "Hubble believed that his count data gave a more reasonable result concerning spatial curvature if the redshift correction was made assuming no recession. To the very end of his writings he maintained this position, favouring (or at the very least keeping open) the model where no true expansion exists, and therefore that the redshift "represents a hitherto unrecognized principle of nature."
There were methodological problems with Hubble's survey technique that showed a deviation from flatness at large redshifts. In particular the technique did not account for changes in luminosity of galaxies due to galaxy evolution.
Earlier, in 1917, Albert Einstein had found that his newly developed theory of general relativity indicated that the universe must be either expanding or contracting. Unable to believe what his own equations were telling him, Einstein introduced a cosmological constant (a "fudge factor") to the equations to avoid this "problem". When Einstein heard of Hubble's discovery, he said that changing his equations was "the biggest blunder of [his] life".
 Other discoveries
 Nobel Prize
Hubble spent much of the later part of his career attempting to have astronomy considered an area of physics, instead of being its own science. He did this largely so that astronomers - including himself - could be recognized by the Nobel Prize Committee for their valuable contributions to astrophysics. This campaign was unsuccessful for a long time. The Nobel Prize Committee eventually decided that astronomical work would be eligible for the physics prize. Unfortunately for Hubble, this occurred in 1953 some months after his death. The Nobel Prize is never awarded posthumously.
- Bruce Medal in 1938.
- Gold Medal of the Royal Astronomical Society in 1940.
- Medal of Merit for outstanding contribution to ballistics research in 1946--ARP
Named after him
- ^ For the record, these were discus, hammer throw, pole vault, standing and running high jump, shot put, mile-relay. The third-placing was for broad jump.
- ^ This had actually been observed by Vesto Slipher in the 1910s, but the world was largely unaware. Ref: Slipher (1917): Proc. Amer. Phil. Soc., 56, 403.
- ^ Distance determination in astronomy continues to be an active area of research, see the article on cosmic distance ladder for more details.
- ^ http://www.astronomycafe.net/anthol/expan.html
- ^ http://antwrp.gsfc.nasa.gov/diamond_jubilee/1996/sandage_hubble.html
- ^ http://www.pbs.org/wnet/hawking/strange/html/strange_cosmo.html
- Christianson, Gale; Edwin Hubble: Mariner of the Nebulae Farrar Straus & Giroux (T) (New York, August 1995.)
- Hubble E.P., The Observational Approach to Cosmology (Oxford, 1937.)
- Hubble E.P., The Realm of the Nebulae (New Haven, 1936.)
- Hubble, A relation between distance and radial velocity among extra-galactic nebulae, Proceedings of the National Academy of Sciences Volume 15 (1929)
 See also
- Expansion of the universe
- Hubble Space Telescope
- Cosmic distance ladder
 External links
- Time 100 Profile
- Astronomy at the University of Louisville - Photographs of Edwin Hubble at New Albany High School.
- Edwin Hubble bio - Written by Allan Sandage
- O'Connor, John J..; Edmund F. Robertson "Edwin Hubble". MacTutor History of Mathematics archive.
|NAME||Hubble, Edwin Powell|
|SHORT DESCRIPTION||American astronomer|
|DATE OF BIRTH||20 November 1889|
|PLACE OF BIRTH||Marshfield, Missouri|
|DATE OF DEATH||28 September 1953|
|PLACE OF DEATH||San Marino, California|