Joel Stebbins with his invention: the Photoelectric Photometer, circa 1925 |
His
early administration was marked with many changes: the Observatory was
integrated in the Mathematics Department as the Division of Astronomy
and had no operating budget. After spending eight dollars out of his own
pocket, Stebbins convinced the Board of Trustees to create the first
budget for the Observatory: $750. In addition, the curriculum was
expanded from three classes to nine classes, including Astronomy for
Engineers, Observational Astronomy, Seminar and Thesis. Most of the
classes, taught by Stebbins and an instructor, required weekly use of
the Observatory's facilitates.
Early
on, Stebbins used the popular Pickering visual program to survey stars
in search of undetected eclipsing binary stars. Later in 1904, he began
the estimates of the relative magnitudes of 107 double stars,
duplicating the work of astronomer E.C. Pickering in 1878.It was during
Stebbins' photometric project when he first realized the need for a new
method of photometry. In the summer of 1905, Stebbins was married and he
soon found a source of inspiration for a new photometer. He provided
the following account at a dinner of the American Astronomical Society
in 1957:
“The
photometric program went along well enough for a couple of years until
we got a bride in our household, and then things began to happen. Not
enjoying home alone, she (May Stebbins) found that if she came to the
observatory and acted as recorder, she could get me home earlier. She
wrote down the numbers as the observer called them, but after some
nights of recording a hundred readings to get just one magnitude, she
said it was pretty slow business. I responded that someday we would do
this by electricity. That was a fatal remark. Thereafter she would often
prod me with the question: "When are you going to change to
electricity?" It happened that within a two or three months the
department of physics gave an open house, and one of the exhibits was in
charge of a young instructor F.C. Brown. He showed how when he turned
on a lamp to illuminate a selenium cell, a bell would ring; when the
lamp was off, the bell would stop. Here was the idea; why not turn a
star on to a cell on a telescope and measure the current?” (Stebbins, Early Photometry, 507)
This friendship with F.C Brown soon led to the development of a selenium cell photometer, which ultimately led to the discovery of five new eclipsing binary stars, constructed a light curve for the Moon, determined the mid-eclipse time of the 24 July, 1907 lunar eclipse and determined the magnitude of Comet Halley in May, 1910. However, Stebbins was not happy with the photometer. The cells were not very sensitive, only stars brighter than the third magnitude could be studied. They also had a narrow spectral response, were not readily available, were difficult to work with and the characteristics varied from one cell to another. The solution to Stebbins' problems was found in physicist Jakob Kunz.
Kunz,
in partnership with Stebbins, developed and installed a photoemissive
photocell instead of a selenium based one. This worked fabulously. Kunz
and Stebbins remained friends and continued to develop better cells for
the photometer. Using the photometer, they even succeeded in measuring
the brightness of the solar corona from the eclipse on 9 June, 1918.
Professor
Stebbins left Illinois in September 1922 when he was offered the
directorship of Washburn Observatory. Stebbins continued to improve and
apply the photometer there where he enlisted the help of A. Whitford who
developed a thermonic amplifier, C. M. Huffer, an Illinois math
graduate who had taken a class with Stebbins at Illinois, and G. Kron at
Mt. Hamilton who worked with photomultiplier tubes. Stebbins remained
at the forefront of astronomical photometry until his death in 1966.
_________________________________________________________________________________
Works Cited:
Joel Stebbins Papers, courtesy of the University of Illinois Archives Series No. 15/3/21, Box 1.
Stebbins,
Joel. (1910)The Measurement of the Light of Stars with a Selenium
Photometer. With An Application to the Variations of ALGOL. The Astrophysical Journal, Vol. 32 (3)
The Color Sensibility of Selenium Cells. The Astrophysical Journal. University of Chicago Press. 27(3). April 1908.
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