Harvard Computers

Harvard Computers refers to a group of women who were employed as "computer" at Harvard University in the early 20th century. This group played a significant role in the field of astronomy, as they were responsible for analyzing astronomical data and cataloging celestial phenomena, particularly at the Harvard College Observatory. The work involved manual calculations and the interpretation of vast amounts of observational data.

Anna Winlock was an American astronomer and a notable figure in 19th-century science. She is best known for her work in the field of astronomy, particularly her contributions to the study of double stars and her involvement with observatory work. Winlock was the daughter of William C. Winlock, an astronomer who worked at the Harvard College Observatory. She played a significant role in the advancement of female participation in scientific fields during a time when such opportunities were limited for women.

Annie Jump Cannon (1863–1941) was an American astronomer known for her significant contributions to the field of stellar classification. She is best known for developing the Harvard Classification Scheme, which categorizes stars based on their temperatures and spectral types. This system uses letters (O, B, A, F, G, K, M) to classify stars, with O being the hottest and M being the coolest.

Antonia Maury (1866–1952) was an American astronomer and a significant figure in the field of astrophysics. She is best known for her contributions to the classification of star spectra and was a pioneer in the study of stellar classification. Maury developed a systematic way to classify stars based on their spectra, proposing enhancements to the classification system that was established by her mentor, Edward C. Pickering, at Harvard College Observatory.

Evelyn Leland does not appear to be a widely recognized figure or concept as of my last knowledge update in October 2021. It is possible that she could be a private individual, a character from a work of fiction, or someone who has gained some form of recognition after that date.

Florence Cushman was a notable figure in the realm of education in the late 19th and early 20th centuries. She is best known for her work as one of the founders of Cushman School, a private institution in Miami, Florida. Established in 1962, the school has a long-standing reputation for providing quality education and fostering a supportive learning environment.

Henrietta Swan Leavitt (1868–1921) was an American astronomer whose work significantly contributed to the field of astrophysics, particularly in understanding variable stars and the measurement of cosmic distances. She is best known for her discovery of the relationship between the luminosity and the periodicity of Cepheid variable stars. Leavitt's research at the Harvard College Observatory involved studying the brightness variations of these stars, which pulsate in regular intervals.

Mary Anna Draper refers to a historical figure who is best known for being the wife of the notable American explorer, activist, and naturalist, William Henry Draper. She is often recognized within the context of her contributions to various social and cultural initiatives during her lifetime in the 19th century.

Muriel Mussells Seyfert appears to be a less widely known figure, and there may be limited publicly available information about her. If you are looking for specific details or context about her, it might be beneficial to provide more information or clarify the context in which you are inquiring about her. If she is a fictional character, a historical figure, or related to a particular field (such as science, art, etc.

Williamina Fleming (1857–1911) was a Scottish astronomer known for her significant contributions to the field of astronomy during the late 19th and early 20th centuries. She worked at the Harvard College Observatory, where she was one of the first women to be appointed to an official position in the field. Fleming played a crucial role in the classification of stars and the development of stellar spectroscopy.