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Annie Jump Cannon (/ ˈ k æ n ə n /; December 11, 1863 – April 13, 1941) was an American astronomer whose cataloging work was instrumental in the development of contemporary stellar classification. [2]
The Annie Jump Cannon Award in Astronomy is awarded annually by the American Astronomical Society (AAS) to a woman resident of North America, who is within five years of receipt of a PhD, for distinguished contributions to astronomy or for similar contributions in related sciences which have immediate application to astronomy.
Annie Jump Cannon was the first female scientist to be recognized for many awards and titles in her field of study. She was the first woman to receive an honorary doctorate from the University of Oxford and the Henry Draper Medal from the National Academy of Sciences, and the first female officer in the American Astronomical Society. Cannon ...
Here, Matlin provides the voice of Annie Jump Cannon, a deaf astronomer at Harvard who, along with Edward C. Pickering, is credited with the creation of the Harvard Classification Scheme, which was the first serious attempt to organize and classify stars based on their temperatures.
This was evident in the achievements accomplished earlier in the century by Williamina Fleming, Antonia Maury, Annie Jump Cannon, and Henrietta Swan Leavitt. However, with Payne's PhD, women entered the mainstream. [37] The trail she blazed into the largely male-dominated scientific community was an inspiration to many.
Later, her colleague Annie Jump Cannon reordered the classification system based on the surface temperature of stars, ... Cannon, Annie J. (November 1911).
Lee was the 2022 recipient of the Annie Jump Cannon Award in Astronomy, of the American Astronomical Society, "for her illuminating work on the formation of stars, debris disks, and planets", [2] and the 2022 recipient of the Professor M. K. Vainu Bappu Gold Medal of the Astronomical Society of India. [3]
It was listed with its variable star designation, W Orionis, in Annie Jump Cannon's 1907 work Second Catalog of Variable Stars. [11] W Orionis is a semiregular variable with an approximately 212‑day cycle. [5] A long secondary period of 2,450 days has also been reported. [12]