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Williamina Fleming

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Williamina Paton Stevens Fleming was a pioneering Scottish astronomer. She played a vital role in organizing how we understand the light from stars. Her work at the Harvard College Observatory helped create systems for naming and grouping celestial objects. Through her research, she cataloged thousands of stars and discovered many deep-sky phenomena. She was also a leader for women in science.

Astronomer Edward Charles Pickering's Harvard computers
Astronomer Edward Charles Pickering's Harvard computers

Fleming's journey into astronomy began under difficult circumstances. Born in Dundee, Scotland, in 1857, she later moved to Boston in 1878. After her husband abandoned her and their son, she worked as a maid. She worked in the home of Professor Edward Charles Pickering. His wife, Elizabeth, noticed Fleming had talents beyond domestic work. In 1879, Pickering hired her for administrative tasks. By 1881, he formally invited her to join the observatory. He taught her how to analyze stellar spectra.

Delegates to the Fourth Conference International Union for Cooperation in Solar Research at Mount Wilson Observatory
Delegates to the Fourth Conference International Union for Cooperation in Solar Research at Mount Wilson Observatory

Fleming became a founding member of the Harvard Computers. This was a group of women hired to perform mathematical classifications. They also edited the observatory's scientific publications. In 1886, the Henry Draper Memorial was started to fund research. This led to the Henry Draper Catalogue project. The goal was to obtain and classify the optical spectra of as many stars as possible. A spectrum is the pattern of light produced by a star. Fleming was placed in charge of this massive project.

To classify stars, Fleming used a method called the Pickering-Fleming system. She used photographic plates rather than observing by hand at night. These plates captured light in the ultraviolet range. This allowed for much more accurate classifications. Fleming's system focused on the amount of hydrogen in a star's spectrum. Stars with the most hydrogen were classified as type A. Those with the second-most hydrogen were type B. This continued through the alphabet. Later, her colleague Annie Jump Cannon reordered these into the Harvard spectral classification. This temperature-based system is still used by astronomers today.

Fleming's research led to many significant discoveries. In 1888, she discovered the Horsehead Nebula. She found it on a telescope-photogrammetry plate. She described it as having a semicircular indentation. She also discovered the first white dwarf star in 1910. Throughout her career, she cataloged more than 10,000 stars. She also identified 59 gaseous nebulae and over 310 variable stars. Additionally, she found 10 novae. In 1898, she became the first woman to serve as Curator of Astronomical Photographs at Harvard.

Fleming was a vocal advocate for women's representation in science. At the 1893 World's Fair in Chicago, she gave a talk. Her speech was titled "A Field for Woman's Work in Astronomy." She promoted the hiring of female assistants. She believed that women could be equals if they were given significant opportunities. She argued that perceived differences between sexes were culturally constructed rather than biological. While early publications sometimes omitted her name, she received proper credit by 1908. She became a U.S. citizen in 1907.

Today, Fleming's legacy is preserved in many ways. There is a Fleming lunar crater on the moon. The asteroid 5747 Williamina is also named after her. Modern librarians are working to preserve her research. They are part of Project PHaEDRA at the Wolbach Library. This project aims to make her notebooks searchable. There are over 2,500 volumes of research from the women computers. Digitizing these materials helps scientists find her specific work. Her notebooks remain a vital link to the history of astronomy.

Astronomer Edward Charles Pickering's Harvard computers
Astronomer Edward Charles Pickering's Harvard computers
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