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.
Even before Stebbins received his doctorate, he took a job as an instructor in astronomy at the University of Illinois at Urbana–Champaign and director of the University of Illinois Observatory. He married May Louise Prentiss, who had been a classmate at the University of Nebraska, in Lincoln on June 27, 1905.[3] They had two children, a son, Robert, and a daughter, Isabelle.[4]
Stebbins began making observations with a polarizing photometer. Frustrated by its use, he worked with F.C. Brown to develop a photometer based on a selenium cell. Beginning in 1907, Stebbins began the first measurements using the selenium cell photometer first on the moon and then later, as the sensitivity of the instrument was improved, on variable stars. He examined eclipsing binaries such as Algol starting in 1910. 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] The University of Illinois Observatory has been designated a National Historic Landmark based on the significance of Stebbins' and Kunz's work.
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]
Stebbins also contributed to ornithology, with his pioneering paper, with E.A. Fath, The Use of Astronomical Telescopes in Determining the Speeds of Migrating Birds.[10]
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] Some of his papers are in the University of Illinois Archives,[11] but most of his correspondence and scientific papers are preserved in the University of Wisconsin-Madison Archives.
[12]
Some of his correspondence, related especially to his early and later days at Lick Observatory, resides in the Mary Lea Shane Archive of Lick Observatory, which is held at the archives of the University of California-Santa Cruz.[13]