Up for auction "Astronomer" Ira Sprague Bowen Hand Signed 3X5 Card.
ES-272A
Ira Sprague Bowen
(December 21, 1898 – February 6, 1973) was an American physicist and astronomer.
In 1927 he discovered that nebulium was not really a chemical
element but instead doubly ionized oxygen. Bowen was born in Seneca Falls, New York in 1898 to Philinda
Sprague and James Bowen. Due to frequent moves of his family he was home
schooled until the death of his father in 1908. From that point on he attended
the Houghton College where his mother worked as
teacher. After graduation from high school in 1915 Bowen stayed at the junior
college of Houghton College and later joined Oberlin
College from which he graduated in 1919. During the time at Oberlin
College Bowen did some research on the properties of steel together with the
scientist Robert Hadfield. The results were published in
1921. Bowen started studying physics at
the University of Chicago in fall 1919.
Already in 1921 Bowen took a position in the research group of Robert Andrews Millikan. He was assigned
to do ultraviolet spectroscopy of chemical elements. Millikan was persuaded by George Ellery Hale to move to the California Institute of Technology
in 1921 and Bowen moved with him. The contact with Hale enabled Bowen also to
work at the Mount Wilson Observatory and the Palomar Observatory. Bowen gave lectures on
general physics at Caltech and did research on cosmic rays and followed his
studies on UV spectroscopy. He also did calculations on spectra for the light
elements of the periodic table. With that data and the inspiration from a
chapter on gaseous nebula and the emission of radiation at low density in the
book Astronomy by Henry Norris Russell, Raymond Smith Dugan and John Quincy Stewart he achieved his best known
discovery. The green emission lines of the Cat's Eye Nebula
at 4959 and 5007 Ångström were discovered by William
Huggins in 1864. Because no known element was showing these emission
lines in the experiment it was concluded in the late 1890s that a new element
was responsible for that lines, it was called nebulium.
Bowen was able to calculate the forbidden transitions of doubly ionized oxygen to be exactly where
the lines had been found. The low probability for collisions in the nebula made
it impossible for the oxygen to get from the excited stated to the ground state
and so the forbidden transitions were the main path for the relaxation. Bowen
published his findings in 1927 and concluded that nebulium was not really a chemical
element. Bowen was the first director of the Palomar Observatory, serving from 1948 to 1964.
Before his retirement in 1964 and even afterwards Bowen was involved in the improvement
of the optical design of several large optical instruments, for example the
100 inch Irenee duPont at the Las Campanas Observatory. He is also known
in the context of meteorology for the introduction of the Bowen ratio,
which quantifies the ratio of sensible to latent heat over an evaporating
surface.