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Forest Ray Moulton (April 29, 1872 – December 7, 1952) was an American astronomer.[1]

He was born in Le Roy, Michigan, and was educated at Albion College. After graduating in 1894 (A.B.), he performed his graduate studies at the University of Chicago and gained a Ph.D. in 1899. At the University of Chicago he was associate in astronomy (1898–1900), instructor (1900–03), assistant professor (1903–08), associate professor (1908–12), and professor after 1912.[2]

He is noted for being a proponent, along with Thomas Chamberlin, of the Chamberlin-Moulton planetesimal hypothesis that the planets coalesced from smaller bodies they termed planetesimals. Their hypothesis called for the close passage of another star to trigger this condensation, a concept that has since fallen out of favor.

In the first decades of the twentieth century, some additional small satellites were discovered to be in orbit around Jupiter. Dr. Moulton proposed that these were actually gravitationally-captured planetesimals. This theory has become well-accepted among astronomers.

The crater Moulton on the Moon, the Adams-Moulton methods for solving differential equations and the Moulton plane in geometry are named after him.
Writings

He became an associate editor of the Transactions of the American Mathematical Society in 1907 and a research associate of the Carnegie Institution in 1908. Besides various contributions to mathematical and astronomical journals he was the author of:

An Introduction to Celestial Mechanics (1902; second revised edition, 1914)
An Introduction to Astronomy (1905)
Descriptive Astronomy (1912)
Periodic Orbits (1913)
Differential Equations (1930)

References

^ Carlson, A. J. (1953), "FOREST Ray Moulton: 1872–1952.", Science 117 (3047): 545–6, 1953 May 22, doi:10.1126/science.117.3047.545, PMID 13056607
^ New International Encyclopedia

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