Sir William Hunter McCrea FRS (13 December 1904, Dublin – 25 April 1999) [1 ] was an English [2 ] astronomer and mathematician.
Biography [ edit ]
His family moved to
Kent in 1906 and then Derbyshire where he attended Chesterfield Grammar School. His father was a school master at Netherthorpe Grammar School in Staveley. He went to Trinity College, Cambridge in 1923 where he studied Mathematics, later gaining a PhD in 1929 under Ralph H. Fowler. He was later appointed a lecturer of Mathematics at the University of Edinburgh in 1929. He also served as reader and assistant professor at Imperial College London. In 1936 he became head of the mathematics department at the Queen's University of Belfast. After serving in the war, he joined the mathematics department at Royal Holloway College in 1944 (the McCrea Building on Royal Holloway's campus is named after him). In 1965, McCrea created the astronomy centre of the physics department at the University of Sussex.
Discoveries [ edit ]
In 1928, he studied
Albrecht Unsöld's hypothesis, and discovered that three quarters of the Sun is made of hydrogen, and about one quarter is helium, with 1% being other elements. Previous to this many people thought the Sun consisted mostly of iron. After this, people realised most stars consist of hydrogen.
In 1964 he proposed mass transfer mechanism as an explanation of
blue straggler stars. [3 ]
McCrea was president of the
Royal Astronomical Society from 1961–3 and president of Section A of the British Association for the Advancement of Science from 1965–6. He was knighted in 1985. He won the Gold Medal of the Royal Astronomical Society in 1976. McCrea died on 25 April 1999 in Lewes.
References [ edit ]
^ Mestel, L.; Pagel, B. E. J. (2007). "William Hunter McCrea. 13 December 1904 -- 25 April 1999: Elected FRS 1952". Biographical Memoirs of Fellows of the Royal Society 53: 223. doi: 10.1098/rsbm.2007.0005.
^ Mestel, Leon (30 April 1999). "Obituary: Sir William McCrea – The Independent". London . Retrieved . 20 July 2011
^ McCrea, Monthly Notices of the Royal Astronomical Society, 128:147, 1964; Carney, Latham, and Laird, The Astronomical Journal, 129:466–479, 2005; Perets, and Fabrycky, The Astrophysical Journal, 697:1048–1056, 2009