- Born:
- December 11, 1863, Dover, Delaware, U.S.
- Died:
- April 13, 1941, Cambridge, Massachusetts (aged 77)
- Subjects Of Study:
- classification
- spectral type
- stellar classification
Annie Jump Cannon
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Who was Annie Jump Cannon?
Annie Jump Cannon (1863–1941) was an American astronomer who specialized in the classification of stellar spectra. As an assistant at the Harvard Observatory, Cannon joined a group known as “Pickering’s Women,” and she devoted her time to recording, classifying, and cataloging the spectra of stars.
In 1901, Cannon simplified existing classification schemes to the classes O, B, A, F, G, K, and M and also divided each class into 10 steps. This became the universally adopted system for classifying stars according to their temperature. Cannon obtained and classified spectra for over 225,000 stars, publishing her work in nine volumes as the Henry Draper Catalogue (1918–24). In her career, she discovered about 300 variable stars and 5 novae.
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What is Annie Jump Cannon famous for in astronomy?
Annie Jump Cannon (1863–1941) was an American astronomer known for her work in stellar classification. As an assistant at the Harvard Observatory, she joined a group known as "Pickering’s Women".
Cannon simplified existing classification schemes and developed the OBAFGKM system, which categorizes stars by temperature. This system was universally adopted and is still in use today. She classified the spectra of over 225,000 stars, published in the Henry Draper Catalogue (1918–24). Cannon also discovered approximately 300 variable stars and five novae.
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What major system did Annie Jump Cannon help create?
Annie Jump Cannon helped create the Harvard system for stellar classification, which is based on a star's surface temperature. Cannon simplified an earlier classification scheme and cataloged the spectra of over 225,000 stars. Her system, which classifies stars by the letters O, B, A, F, G, K, and M, is still in use today.
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How did her classification system help astronomers study stars?
Annie Jump Cannon greatly contributed to astronomy through her stellar classification system. Cannon simplified existing classification methods and organized stars into the spectral classes O, B, A, F, G, K, and M based on temperature. This arrangement, which runs from hottest to coolest, helped astronomers study stars by providing a clear method to determine a star's temperature, chemical composition, and luminosity from its spectrum. Her work led to the classification of over 225,000 stars and was published in the Henry Draper Catalogue. Cannon's classification scheme was universally adopted and remains a fundamental tool in astronomy.
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How has Annie Jump Cannon’s work influenced modern astronomy today?
Annie Jump Cannon's work classifying stellar spectra significantly shaped modern astronomy. Cannon, one of "Pickering’s Women," simplified existing classification schemes and created the OBAFGKM system, which is based on temperature and universally adopted.
Cannon's system enabled astronomers to classify stars by temperature, which was a major influence in the evolution of astronomy from observation to a science with theoretical and philosophical content. Her work led to the classification of over 225,000 stars, published in the Henry Draper Catalogue, and the subsequent cataloging of tens of thousands more. In addition, Cannon discovered around 300 variable stars and 5 novae.
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Annie Jump Cannon (born December 11, 1863, Dover, Delaware, U.S.—died April 13, 1941, Cambridge, Massachusetts) was an American astronomer who specialized in the classification of stellar spectra.
Cannon was the eldest daughter of Wilson Cannon, a Delaware state senator, and Mary Jump. She studied physics and astronomy at Wellesley College, graduating in 1884. For several years thereafter she traveled and dabbled in photography and music. In 1894 she returned to Wellesley for a year of advanced study in astronomy, and in 1895 she enrolled at Radcliffe in order to continue her studies under Edward C. Pickering, who was director of the Harvard College Observatory.
In 1896 Cannon was named an assistant at the Harvard Observatory, becoming one of a group known as “Pickering’s Women.” There, joining Williamina P.S. Fleming and Antonia Maury, she devoted her energies to Pickering’s ambitious project, begun in 1885, of recording, classifying, and cataloging the spectra of all stars down to those of the ninth magnitude. Fleming had initially classified stellar spectra by letter in alphabetic sequence from A to Q, mainly according to the strength of their hydrogen spectral lines. Maury created a new scheme with 22 groups from I to XXII and further added three subdivisions based on the sharpness of the spectral lines. She also placed Fleming’s B stars before the A stars.
In a catalog of 1,122 stars published in 1901, Cannon drastically simplified Fleming’s scheme to the classes O, B, A, F, G, K, and M, and she retained P for planetary nebula and Q for unusual stars. She also added numerical divisions, further dividing each class into 10 steps from 0 to 9 (e.g., the Sun’s spectral type is G2). It was soon realized that Cannon’s scheme actually was classifying stars according to their temperature, and her spectral classifications were universally adopted. She eventually obtained and classified spectra for more than 225,000 stars. Her work was published in nine volumes as the Henry Draper Catalogue (1918–24).
In 1911 Cannon succeeded Fleming as curator of astronomical photographs at the observatory. After 1924 she extended her work, cataloging tens of thousands of additional stars down to the 11th magnitude for the two-volume Henry Draper Extension (1925, 1949). The work was an invaluable contribution to astronomy, bearing strongly on countless other problems and areas of research and exerting major influence on the evolution of the science of astronomy from one of mere observation to one of great theoretical and philosophical content. In the course of her work, Cannon also discovered some 300 variable stars and 5 novae.
Among the numerous honors and awards accorded her were the first honorary doctorate from the University of Oxford to be awarded to a woman (1925) and the Henry Draper Medal of the National Academy of Sciences in 1931. She was also the first woman to become an officer in the American Astronomical Society. In 1933 she established that organization’s Annie Jump Cannon Award, which is given to a North American female astronomer (within five years of receiving a doctorate) for her distinguished contribution to astronomy. It was only in 1938 that she was appointed to the Harvard faculty, when she was named William Cranch Bond Professor of Astronomy. Cannon officially retired from the observatory in 1940 but carried on research until her death the next year.