Forest Ray Moulton

Forest Ray Moulton

Early Life and Education:

  • Born: April 29, 1872, in Le Roy, Michigan (USA)
  • Parents: Belah G. Moulton and Mary C. Moulton
  • Siblings: Had seven brothers and a sister, with five brothers becoming listed in Who's Who in America
  • Education:
    • Albion College (1892-1894)
    • University of Chicago (1895-1899), where he earned his Ph.D. in astronomy under the guidance of Thomas Chrowder Chamberlin (a noted geologist)

Scientific Career:

  • Known for his contributions to celestial mechanics and planetary astronomy.
  • Collaborated with Thomas Chrowder Chamberlin to develop the Chamberlin-Moulton planetesimal hypothesis, which proposed a theory for the formation of the solar system involving a near-collision between the Sun and another star, leading to the ejection of material that formed the planets. (While not the accepted theory today, it was a significant contribution to the field at the time)
  • Played a key role in the development of numerical integration techniques, particularly Moulton's method, which is still used in ballistics and celestial mechanics calculations.
  • His work on ballistics was crucial during World War I.
  • Mentored prominent astronomers like Edwin Hubble (considered the "father of modern cosmology") and Walter Bartky.
  • Became a leading figure in American mathematical astronomy and held positions at the University of Chicago and the University of Pennsylvania.
  • Served as the Permanent Secretary and then Administrative Secretary of the American Association for the Advancement of Science (AAAS) from 1937 to 1948.

Other Achievements and Recognition:

  • Published several introductory books on astronomy and a celebrated text on celestial mechanics.
  • Elected to the National Academy of Sciences in 1910, a prestigious honor recognizing distinguished and ongoing achievements in scientific research.
  • Brother, Harold G. Moulton, became a noted economist.

Death and Legacy:

  • Died: December 7, 1952, in Wilmette, Illinois (USA) at the age of 80.
  • Remembered as a significant contributor to the fields of celestial mechanics, planetary astronomy, and numerical integration techniques.
  • His work on the Chamberlin-Moulton hypothesis, while not the current accepted theory, laid groundwork for further understanding of the solar system's formation.


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