In 1886, Harvard College Observatory director Edward C. Pickering had a monumental task. Funded by Anna Palmer Draper as a memorial to her late husband, the observatory was creating a photographic map of the night sky's brighter stars. Using a new technique, a single glass plate could capture the spectra of hundreds of stars at once. From Massachusetts and, within a few years, a new southern station in Peru, the observatory began collecting an unprecedented flood of data. The collection eventually grew into a massive archive of hundreds of thousands of plates, each a ghostly image packed with faint stellar fingerprints. But Pickering faced a huge problem: how to analyze them all? He needed a team to meticulously identify, measure, and classify every single star in this vast new archive of the heavens.

Annie Jump Cannon and the Harvard Computers
Annie Jump Cannon and the Harvard 'Computers' classified hundreds of thousands of stars, creating a system astronomers still use today.
A Catalogue of Starlight
Frequently Asked Questions
What was the Henry Draper Catalogue?
It was a massive nine-volume list published between 1918 and 1924, containing the spectral classifications of over 225,000 stars. The work was done almost entirely by astronomer Annie Jump Cannon at the Harvard College Observatory.
What is the OBAFGKM stellar classification system?
It is a system created by Annie Jump Cannon to organize stars based on their temperature. The sequence runs from the hottest, blue O-type stars to the coolest, red M-type stars, and became the international standard for astronomy.
Why were the women at Harvard called 'Computers'?
In the late 19th and early 20th centuries, a 'computer' was a job title for a person who performed mathematical calculations. The team of women at the Harvard College Observatory meticulously analyzed data from photographic plates, so they were called the Harvard Computers.
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