Joel Stebbins

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Joel Stebbins
Born (1878-06-30)June 30, 1878
Omaha, Nebraska
Died March 16, 1966(1966-03-16) (aged 87)
Palo Alto, California
Nationality American
Fields astronomy
Institutions University of Wisconsin-Madison
Doctoral advisor William Wallace Campbell

Joel Stebbins (July 30, 1878 – March 16, 1966) was an American astronomer who pioneered photoelectric photometry in astronomy. He was director of the University of Illinois Observatory from 1903 to 1922 where he performed innovative work with the selenium cell.[1] In 1922 he became director of the Washburn Observatory at the University of Wisconsin–Madison where he remained until 1948. After 1948, Stebbins continued his research at Lick Observatory until his final retirement in 1958.

Stebbins brought photoelectric photometry from its infancy in the early 1900s to a mature technique by the 1950s, when it succeeded photography as the primary method of photometry. He used the new technique to investigate eclipsing binaries, the reddening of starlight by interstellar dust, colors of galaxies, and variable stars.

Biography[edit]

Joel Stebbins at the University of Wisconsin about 1925 looking through the photoelectric photometer.

Joel Stebbins was born in Omaha, Nebraska, on March 16, 1878, the son of Charles Stebbins, an office worker at the Union Pacific Railroad and his wife Sara Ann née Stubbs. Stebbins had two sisters, Eunice and Millicent. He attended elementary and high school in Omaha, before entering the University of Nebraska-Lincoln in 1896. He received his Bachelor of Science (BS) degree in 1899, and remained for a year as a graduate student before leaving for the University of Wisconsin, where he studied astronomy at the Washburn Observatory under George G. Comstock.[2]

Stebbins published his first paper, concerning the light curve of Nova Persei with Comstock in 1901. He then received a fellowship from the University of California's Lick Observatory. He earned his Doctor of Philosophy (PhD) degree there under the supervision of William Wallace Campbell, writing a thesis on the spectra of Omicron Ceti. His was only the third PhD to be awarded for astronomy by the University of California. His thesis was subsequently published in the Astrophysical Journal in 1903.[2]

Even before Stebbins received his doctorate, he took a job as an instructor in astronomy at the University of Illinois at Urbana–Champaign. He married May Louise Prentiss, who had been a classmate at the University of Nebraska, in Lincoln on May 27, 1905.[3] They had two children, a son, Robert, and a daughter, Isabelle.[4]

Stebbins began making observations with a polarizing photometer. He examined eclipsing binaries such as Algol. By 1913, Henry Norris Russell had developed the theory of eclipsing binaries, and Stebbins realized that there were many undiscovered ones. He soon found that Beta Aurigae and Delta Orionis were eclipsing binaries. Further discoveries followed.[5]

The development of the photoelectric cell by Jakob Kunz revolutionized astronomical photometry. Kunz’s photoelectric cells were many times more sensitive than what was available commercially and therefore able to detect faint star light. In 1915, Stebbins used the new photometers to examine Beta Lyrae, a more irregular binary system. The new equipment allowed observations of increasingly faint stars. Stebbins work was recognized with the American Academy of Arts and Sciences' Rumford Prize in 1913, and the United States National Academy of Sciences' Henry Draper Medal in 1915.[6]

In 1922, Stebbins relocated to the University of Wisconsin-Madison, where he became the director of the Washburn Observatory in succession to George C. Comstock. Stebbins conducted systematic photometric studies of the O-type and B-type main-sequence stars and globular clusters. In later years, he became interested in cosmic dust.[7] His students included Olin J. Eggen, Charles M. Huffer, Gerald Kron and Albert Whitford.[8]

Stebbins retired from the University of Wisconsin-Madison and the Washburn Observatory in 1948 at the age of seventy, and then went to work at the Lick Observatory, collaborating with Gerald Kron, who had once been his student. They used photometric methods to obtain new values for the luminosity of the Cepheids. This confirmed Walter Baade's extragalactic distance scale.[9]

Having dealt with the bright Cepheids, Stebbins and Kron used photometric techniques to study the Sun, which is orders of magnitude brighter than any other object in the sky. Obtaining an accurate assessment of its stellar color and magnitude. He retired for good at the age of eighty.[9]

In his later years, he suffered from leukaemia. He died at Palo Alto hospital on March 16, 1966. He was survived by his wife May, son Robert and daughter Isabelle.[4] His papers are in the University of Illinois Archives.[10]

Honors[edit]

Awards

Named after him

Notes[edit]

  1. ^ "History of the University of Illinois Observatory and 12" Refractor". Astronomical Society at the University of Illinois. Retrieved February 19, 2011. 
  2. ^ a b Whitford 1978, pp. 293–294.
  3. ^ Whitford 1978, pp. 296–297.
  4. ^ a b Whitford 1978, p. 308.
  5. ^ Whitford 1978, p. 298.
  6. ^ Whitford 1978, pp. 298–300.
  7. ^ Whitford 1978, pp. 300–304.
  8. ^ Kron 1966, p. 217.
  9. ^ a b Whitford 1978, pp. 306–307.
  10. ^ "Joel Stebbins Papers, 1907-23, 1936, 1939, 1957". University of Illinois. Retrieved August 18, 2013. 
  11. ^ "Past Recipients of the Rumford Prize". American Academy of Arts and Sciences. Retrieved February 19, 2011. 
  12. ^ "Henry Draper Medal". National Academy of Sciences. Retrieved February 19, 2011. 
  13. ^ "Past Winners of the Catherine Wolfe Bruce Gold Medal". Astronomical Society of the Pacific. Retrieved February 19, 2011. 
  14. ^ "Winners of the Gold Medal of the Royal Astronomical Society". Royal Astronomical Society. Retrieved February 19, 2011. 
  15. ^ "Grants, Prizes and Awards". American Astronomical Society. Retrieved February 19, 2011. 
  16. ^ "Stebbins C on Moon". United States Geological Survey. Retrieved August 18, 2013. 
  17. ^ "2300 Stebbins (1953 TG2)". Jet Propulsion Laboratory. Retrieved August 18, 2013. 

References[edit]