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Samuel A. Mitchell
Samuel Alfred Mitchell was born in Kingston, Ontario on April 29, 1874. This son of John Cook and Sarah Chown Mitchell was the sixth of ten children to grow up in the Mitchell home. At age twelve, undoubtedly to get away from his many siblings, he went off to Kingston Collegiate Institute. From there, he went on to Queen's University where he received his Masters of Arts in mathematics in 1894. While at Queen's University, he was introduced to Reverend James Williamson, known as Uncle Billy, who at eighty years of age found it pleasant to delegate the care of the astronomical instruments to Mitchell which is how he acquired knowledge of the techniques of an astronomical observatory.
Upon encouragement from his math professor, Nathan F. Dupuis, he left in 1895 for The Johns Hopkins University to study math under Simon Newcomb, only to find Newcomb retired. Thomas Craig was the new head of mathematics and Mitchell also began study under Charles Lane Poor, the head of astronomy. Poor was an excellent teacher and Mitchell was inclined to follow astronomy from that point on. Mitchell was awarded an astronomy assistantship for his second year at JHU and continued until he received his PhD in 1898 with his thesis published in the Astrophysical Journal, which included a discussion of the amount of astigmatism of concave grating. While at Hopkins, his astronomy duties consisted of caring for the transit instrument and the clocks in the little observatory behind the physics laboratory, and the 9.5 inch refractor in the dome of the laboratory roof.
Following receipt of his doctoral degree, Mitchell set out for the brand new Yerkes Observatory in Wisconsin where he began work as a research student in 1898. Though he enjoyed his work at Yerkes, he was enticed to move away and became an instructor in astronomy at Columbia University in June 1899. That December he married Milly Gray Dumble, the daughter of Professor E. T. Dumble who was then the State Geologist of Texas. Over the fourteen years he was at Columbia, Mitchell taught undergraduate courses in descriptive astronomy both at Columbia and later for girls from Barnard College, a year long course in geodesy for third year students, which continued into a first semester fourth year course, and a six week summer camp for civil engineers.
In 1900, he took what would be for him the first of ten eclipse expeditions. The May 28, 1900 eclipse took him to Griffin, Georgia with the United States Naval Observatory. Mitchell became a world-renowned authority on solar eclipses through his numerous expeditions, including trips to: Sawah Loento, Sumatra in the Dutch West Indies (May 18, 1901), Daroca, Spain (August 30, 1905), Baker, Oregon (June 8, 1918), San Diego, California (September 10, 1923), Van Vleck Observatory, Middleton, Connecticut (January 24, 1925), Fagernas, Norway (June 29, 1927), Niuafoou or "Tin-Can" Island, Tonga, in the South Pacific Ocean (October 22, 1930) and Magog, Quebec, Canada (August 31, 1932), and Canton (Kanton) Island, Kiribati (June 8, 1937), this time as the scientific leader of a National Geographic Society Expedition. An article entitled "Nature's Most Dramatic Spectacle" by Mitchell appeared in the September 1938 edition of National Geographic Magazine. These ten expeditions allowed him to write Eclipses of the Sun, summarizing his work on solar flash spectra, first published in 1923 and produced through five editions (5th edition, 1951). On the 1918 Oregon eclipse, Mitchell was assisted by Llewelyn G. Hoxton (chair of the University of Virginia Physics Department 1916-1948), and accompanied by the artist Howard Russell Butler, whose paintings of totality graced the old Hayden Planetarium for many years.
Mitchell went back to Yerkes for the summers of 1909, 1910 and 1911 and then returned for a fifteen month sabbatical in 1912 and 1913. Frank Schlesinger first demonstrated the technique of determing stellar parallaxes photographically at Yerkes in 1905, and Mitchell (along with Frederick Slocum) carried out research applying the technique, publishing their results in 1913. At that point, he was offered the directorship at the Leander J. McCormick Observatory at the University of Virginia. Mitchell spent much of his time and energy as director coming up with funds for running the observatory and paying staff and graduate students. Mitchell started the use of photographic plates with the visual 26¼-inch refractor shortly after his arrival at the University of Virginia. He became well known for his work on stellar parallaxes and photometry. Dr. Mitchell was liked by faculty and students alike, known for helping to bring prestige to the University. "Corks and Curls", the yearbook at the University of Virginia, honored Dr. Mitchell by dedicating its 1938 volume to him, saying "Dr. Mitchell typifies the intellectual ideal of the University." He also served as vestryman at St. Paul's Episcopal Church for several years.
Dr. Samuel Mitchell died in Bloomington, Indiana on February 22, 1960 (Science Magazine Obitiuary). His son, Allan C. G. Mitchell (1902-1963) (M.A. Physics, UVa, 1924), was chair of the Indiana University Physics Department from 1938-1963 and pioneered the creation of the IU Cyclotron Facility in 1941 (one of the first in the world), which was dismantled in 1968 to make room for the current facility.
Samuel Mitchell's granddaughter, Alice Mitchell Rivlin, a Senior Fellow in Economic Studies at the Brookings Institution, served as the Vice Chair of the Board of Governors of the Federal Reserve (1996-1999), was the Director of the White House Office of Management and Budget (1994-1996), and was the founding director of the Congressional Budget Office (1975).