Sinclair Smith (astronomer)

From Wikipedia, the free encyclopedia
Sinclair Smith
Born24 March 1899 Edit this on Wikidata
Chicago Edit this on Wikidata
Died18 May 1938 Edit this on Wikidata (aged 39)
Pasadena Edit this on Wikidata
Alma mater
OccupationAstronomer Edit this on Wikidata

Sinclair Smith was an American astronomer born on 24 March 1899 in Chicago and died on 18 May 1938 in Pasadena. His observations of the Virgo Cluster were among the first to suggest the existence of dark matter.

Biography[]

In 1906, his parents took him to Italy for two years, then to Indiana, where they lived until 1913, when they moved to California.[1]

As a child, he showed a great interest in mechanical design and drawing. He was hired as a draughtsman for the design of the Mount Wilson Observatory's 100-inch (2.5-metre) Hooker telescope.[1]

He received his bachelor's degree from the California Institute of Technology (Caltech) in 1921, and in 1924, he obtained his Ph.D. for his work with John August Anderson on the exploding wire method, to obtain laboratory spectra at high excitation and ionization energies.[2]

He then spent a year at the Cavendish Laboratory at Cambridge University, and worked at the physics laboratory of the Mount Wilson Observatory for the rest of his life.[1][2]

He died prematurely of cancer at the age of 39.[1]

Publications[]

  • Sinclair Smith (15 January 1924). "Note on Electrically Exploded Wires in High Vacuum". Proceedings of the National Academy of Sciences of the United States of America. 10 (1): 4–5. ISSN 0027-8424.
  • Sinclair Smith; Richard C. Tolman (15 May 1926). "On the Nature of Light". Proceedings of the National Academy of Sciences of the United States of America. 12 (5): 343–347.
  • Sinclair Smith; Richard C. Tolman (15 August 1926). "Remarks on Professor Lewis's Note on the Path of Light Quanta in an Interference Field". Proceedings of the National Academy of Sciences of the United States of America. 12 (8): 508–509.
  • Sinclair Smith (15 May 1930). "The Effect of Low Temperatures on the Sensitivity of Radiometers". Proceedings of the National Academy of Sciences of the United States of America. 16 (5): 373–376.
  • Sinclair Smith (August 1934). "The Spectral Distribution of Stellar Energy Determined with the Radiometer". Publications of the Astronomical Society of the Pacific. 46 (272): 215–216. ISSN 0004-6280.

References[]

  1. ^ a b c d Anderson 1938, p. 232.
  2. ^ a b Trimble 2007, p. 1068.

Appendices[]

Bibliography[]

Biography[]

Other works[]

External links[]

Retrieved from ""