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Carlyle S. Beals
Carlyle Smith Beals, OC FRS (June 29, 1899 – July 2, 1979) was a Canadian astronomer.
Carlyle Smith Beals was born in Canso, Nova Scotia to Rev. Francis H. P. Beals and his wife, Annie Florence Nightingale Smith Beals, on June 29, 1899. He is the brother of artist and educator Helen D. Beals.
Beals received a Bachelor of Arts degree from Acadia University in 1919, specializing in physics and mathematics. Although he wished to continue his studies, he was forced to postpone those plans due to poor health. He taught at a small country school in Nova Scotia during the winter of 1920.
He began his Ph.D. studies in physics at Yale University in 1921, but was forced to return home in the winter of 1921 when his health failed again. He resumed his graduate studies in 1922 at University of Toronto and received a master's degree in Physics in 1923. His master's thesis work on triboluminescence spectra, the frequencies of light generated by breaking chemical bonds, was done under the supervision of John Cunningham McLennan, one of the leading physicists in Canada at the time.
Beals spent one year as the Science Master at the High School of Quebec in Quebec City, before enrolling in a graduate programme in physics in 1924 at the Royal College of Science at Imperial College London. Working under Alfred Fowler, he studied the Zeeman effect and the spectra of palladium, copper, and ionized silver. During this time Beals became acquainted with observational astronomy by using the small observatory in the Royal College of Science building. He received a Ph.D. in 1926.
After obtaining his PhD, Beals returned to Acadia University as an assistant professor of physics, but left one year later for an Assistant Astronomer position at the Dominion Astrophysical Observatory (DAO), Victoria, British Columbia. Beals worked at the Dominion Astrophysical Observatory from 1927 until 1946, becoming Assistant Director of the DAO in 1940.
At the DAO, he studied emission lines in the spectra of hot stars and gas clouds in the interstellar medium. His work established a reliable temperature scale for hotter stars, based on their spectra. He showed that the broad emission lines seen in Wolf-Rayet and P Cygni-type stars were due to strong stellar winds. Beals was the first astronomer to quantitatively measure the ratio of sodium and calcium absorption lines in the interstellar medium (the gas between stars) and the ratio of the two lines in the sodium D doublet. He also found that rather than being uniform, the interstellar medium was clumpy and moved with different velocities.
During his time at the DAO, he developed several astronomical instruments to analyse astronomical spectra, including a self-recording micro-photometer and a high efficiency grating spectrograph.
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Carlyle S. Beals
Carlyle Smith Beals, OC FRS (June 29, 1899 – July 2, 1979) was a Canadian astronomer.
Carlyle Smith Beals was born in Canso, Nova Scotia to Rev. Francis H. P. Beals and his wife, Annie Florence Nightingale Smith Beals, on June 29, 1899. He is the brother of artist and educator Helen D. Beals.
Beals received a Bachelor of Arts degree from Acadia University in 1919, specializing in physics and mathematics. Although he wished to continue his studies, he was forced to postpone those plans due to poor health. He taught at a small country school in Nova Scotia during the winter of 1920.
He began his Ph.D. studies in physics at Yale University in 1921, but was forced to return home in the winter of 1921 when his health failed again. He resumed his graduate studies in 1922 at University of Toronto and received a master's degree in Physics in 1923. His master's thesis work on triboluminescence spectra, the frequencies of light generated by breaking chemical bonds, was done under the supervision of John Cunningham McLennan, one of the leading physicists in Canada at the time.
Beals spent one year as the Science Master at the High School of Quebec in Quebec City, before enrolling in a graduate programme in physics in 1924 at the Royal College of Science at Imperial College London. Working under Alfred Fowler, he studied the Zeeman effect and the spectra of palladium, copper, and ionized silver. During this time Beals became acquainted with observational astronomy by using the small observatory in the Royal College of Science building. He received a Ph.D. in 1926.
After obtaining his PhD, Beals returned to Acadia University as an assistant professor of physics, but left one year later for an Assistant Astronomer position at the Dominion Astrophysical Observatory (DAO), Victoria, British Columbia. Beals worked at the Dominion Astrophysical Observatory from 1927 until 1946, becoming Assistant Director of the DAO in 1940.
At the DAO, he studied emission lines in the spectra of hot stars and gas clouds in the interstellar medium. His work established a reliable temperature scale for hotter stars, based on their spectra. He showed that the broad emission lines seen in Wolf-Rayet and P Cygni-type stars were due to strong stellar winds. Beals was the first astronomer to quantitatively measure the ratio of sodium and calcium absorption lines in the interstellar medium (the gas between stars) and the ratio of the two lines in the sodium D doublet. He also found that rather than being uniform, the interstellar medium was clumpy and moved with different velocities.
During his time at the DAO, he developed several astronomical instruments to analyse astronomical spectra, including a self-recording micro-photometer and a high efficiency grating spectrograph.