Hubble, Edwin (Powell) (1889-1953)US astronomer who studied extragalactic nebulae and demonstrated them to be galaxies like our own. He found the first evidence for the expansion of the universe, in accordance with the cosmological theories of Georges Lemaître and Willem de Sitter, and his work led to an enormous expansion of our perception of the size of the universe.
Hubble was born in Marshfield, Missouri, on 20 November 1889. He went to high school in Chicago and then attended the University of Chicago where his interest in mathematics and astronomy was influenced by George Hale and Robert Millikan. After receiving his bachelor's degree in 1910, he became a Rhodes scholar at Queen's College, Oxford, where he took a degree in jurisprudence in 1912. When he returned to the USA in 1913, he was admitted to the Kentucky Bar, and he practised law for a brief period before returning to Chicago to take a research post at the Yerkes Observatory 1914-17.
In 1917 Hubble volunteered to serve in the US infantry and was sent to France at the end of World War I. He remained on active service in Germany until 1919, when he was able to return to the USA and take up the earlier offer made to him by Hale of a post as astronomer at the Mount Wilson Observatory near Pasadena, where the 2.5-m/100-in reflecting telescope had only recently been made operational. Hubble worked at Mount Wilson for the rest of his career, and it was there that he carried out his most important work. His research was interrupted by the outbreak of World War II, when he served as a ballistics expert for the US War Department. He was awarded the Gold Medal of the Royal Astronomical Society in 1940, and received the Presidential Medal for Merit in 1946. He was active in research until his last days, despite a heart condition, and died in San Marino, California, on 28 September 1953.
While Hubble was working at the Yerkes Observatory, he made a careful study of nebulae, and attempted to classify them into intra- and extragalactic varieties. At that time there was great interest in discovering what other structures, if any, lay beyond our Galaxy. The mysterious gas clouds, known as the smaller and larger Magellanic Clouds, which had first been systematically catalogued by Charles Messier and called ‘nebulae’, were good extragalactic candidates and were of great interest to Hubble. He had been particularly inspired by Henrietta Leavitt's work on the Cepheid variable stars in the Magellanic Clouds; and later work by Harlow Shapley, Henry Russell, and Ejnar Hertzsprung on the distances of these stars from the Earth had demonstrated that the universe did not begin and end within the confines of our Galaxy. Hubble's doctoral thesis was based on his studies of nebulae, but he found it frustrating because he knew that more definite information depended upon the availability of telescopes of greater light-gathering power and with better resolution...