Harvard Computers
The Harvard Computers were a team of women working as skilled workers to process astronomical data at the Harvard College Observatory in Cambridge, Massachusetts, United States. The team was directed by Edward Charles Pickering and, following his death in 1919, by Annie Jump Cannon.
Other computers on the team included Mary Anna Draper, Williamina Fleming, Anna Winlock, and Florence Cushman. Although these women started primarily as calculators, they made significant contributions to astronomy, much of which they published in research articles.
History
In the 19th century, the Harvard College Observatory faced the challenge of working through an overwhelming amount of astronomical data due to improvements in photographic technology. Harvard Observatory's director, Edward Charles Pickering, hired a group of women to analyze the astronomical data recorded on the growing collection of plate negatives. While Pickering was the director of the Harvard Observatory, he hired over eighty women. These women were known as computers.' Although Pickering believed that gathering data at astronomical observatories was not the most appropriate work, it seems that several factors contributed to his decision to hire women instead of men. Among them was that men were paid much more than women, so he could employ more staff with the same budget. This was relevant in a time when the amount of astronomical data was surpassing the capacity of the Observatories to process it. Although some of Pickering's female staff were astronomy graduates, their wages were similar to those of unskilled workers. They usually earned between 25 and 50 cents per hour, more than a factory worker but less than a clerical one. Most of the women depended financially on their friends and family members and lived with coworkers to combat the low wages. Although the wages Pickering provided were low, it was common to pay women less than men during the 20th century and does not discount his advocation for women in astronomy. In describing the dedication and efficiency with which the Harvard Computers, including Cushman, undertook this effort, Edward Pickering said, "a loss of one minute in the reduction of each estimate would delay the publication of the entire work by the equivalent of the time of one assistant for two years." Another reason why Pickering decided to hire women over men was he thought allowing women to conduct astronomical research would show the general public that women were capable of higher thinking and worthy of higher education. The first female computer to be hired at the Harvard Observatory was Anna Winlock. Pickering's first hire was Williamina Fleming six years later in 1881. Together, Fleming and Pickering continued to hire female computers through the twentieth century. At times women offered to work at the observatory for free in order to gain experience in a field that was difficult to get into.The computer position was one of the lower class positions at the observatory due to the pay and little chance for promotion. Under the Henry Draper Memorial project, the women were often tasked with measuring the brightness, position, and color of stars. The goal of the project was to photograph the stars and classify their spectrum. Their work was often segregated from men, so teams of male astronomers would take photographs of the stars in the evening and send them to the women at Harvard for analysis. The work included such tasks as classifying stars by calculating their exact position and movement, predicting the return of comets, and by comparing the photographs to known catalogs and reducing the photographs while accounting for things like atmospheric refraction, parallax, and error in various instruments in order to render the clearest possible image. While the work was repetitive, it still required attention and accuracy. Fleming herself described the work as "so nearly alike that there will be little to describe outside ordinary routine work of measurement, examination of photographs, and of work involved in the reduction of these observations". The work would not have been possible without photographic plate technology.' With such technology, dry, color sensitive plates are used to capture photo visual and photo-red magnitudes. The dry plates allowed for longer exposure over longer time intervals, increasing the accuracy of the photographs and range of stars capable of being photographed. The plate technology allowed the women to classify stars more accurately than before.
The observatory, with the help of computers, made several breakthroughs in classifying and cataloging the stars. One such accomplishment was the Henry Draper Catalogue. Following the death of Henry Draper, Mary Anna Palmer Draper funded the Mount Wilson Observatory. The work on the catalogue was led by Williamina Fleming. Following the initial classifications done by Fleming, Antonia Maury helped place stars in their correct positions and did further research on the spectra of the stars with Pickering. Henrietta Leavitt discovered a relationship between a Cepheid variable’s brightness and its pulsation period. Annie Jump Cannon and her team classified an average of 5,000 stars per month from the years 1912–1915. Florence Cushman helped organize and process the data. The catalog was published between 1918 and 1924. Following the death of Pickering, Cannon took control of the projects. An extension to the original works was published between 1925 and 1936, where over 46,850 stars were classified.
In the later years of the program, following the publication of the catalog, several women joined and continued to make contributions. Margaret Walton Mayall contributed to the classification of stellar spectra. She later went on to lead the American Association of Variable Star Observers. Helen Sawyer Hogg specialized in cataloging variable stars within globular clusters. Her work helped lay the foundation for understanding stellar evolution and the structure of the universe. Cecilia Payne-Gaposchkin proved that stars are composed primarily of hydrogen and helium. Muriel Mussells Seyfert discovered three new ring nebulae on photographic plates, expanding the catalog of known planetary nebulae.
Notable members
Mary Anna Palmer Draper
was an American astronomer who helped found the Mount Wilson Observatory.Draper was the widow of Dr. Henry Draper, an astronomer who died before completing his work on the chemical composition of stars. She was very involved in her husband's work and wanted to finish his classification of stars after he died. Mary Draper quickly realized the task facing her was far too daunting for one person. She had received correspondence from Mr. Pickering, a close friend of hers and her husband's. Pickering offered to help finish her husband's work, and encouraged her to publish his findings up to the time of his death. Draper agreed to give Pickering the plates her husband had been working on, but took them to Harvard University herself since the plates were very small. While at the university, Draper met the Harvard Observatory's current computers and was able to observe some of the observatory's current projects. After some deliberation and much consideration, Draper decided in 1886 to donate money and a telescope of her husband's to the Harvard Observatory in order to photograph the spectra of stars. She had decided this would be the best way to continue her husband's work and erect his legacy in astronomy. She was very insistent on funding the memorial project with her own inheritance, as it would carry on her husband's legacy. She was a dedicated follower of the observatory and a great friend of Pickering's. In 1900, she funded an expedition to see the total solar eclipse occurring that year.
File:Astronomer Edward Charles Pickering's Harvard computers.jpg|thumb|Harvard Computers at work, circa 1890, including Henrietta Swan Leavitt seated, third from left, with magnifying glass, Annie Jump Cannon, Williamina Fleming standing, at center, and Antonia Maury
Williamina Fleming
was a Scottish immigrant astronomer who helped with the photographic classification of stellar spectra.Fleming had no prior relation to Harvard, as she was a Scottish immigrant working as Pickering's housemaid. Her first assignment was to improve an existing catalog of stellar spectra, which later led to her appointment as head of the ‘’Henry Draper Catalogue’’ project. Fleming went on to help develop a classification of stars based on their hydrogen content, as well as play a major role in discovering the strange nature of white dwarf stars. Williamina continued her career in astronomy when she was appointed Harvard's Curator of Astronomical Photographs in 1899, also known as Curator of the Photographic Plates. At the age of 42, Fleming became the first woman at the observatory to hold a title of such nature. She remained the only woman curator until the 1950s. Her work also led to her becoming the first female American citizen to be elected to the Royal Astronomical Society in 1907. Throughout her career, Fleming was able to classify 10,000 spectra and found over 50 nebulae and over 300 stars. Fleming did not retire from working at the observatory, as she died at age 54 from pneumonia.
Antonia Maury
was an American astronomer who worked on calculating the orbit of a spectroscopic binary.Maury was the niece of Henry Draper, and after recommendation from Mrs. Draper, was hired as a computer at the age of 22. She was a graduate from Vassar College with honors in physics, astronomy, and philosophy. Pickering was uncomfortable paying the average computer salary to someone with Antonia Maury's achievements, but ultimately ended up hiring her. Maury was first tasked with the spectral measurement of some of the brightest stars. Pickering then tasked Maury with reclassifying some of the stars after the publication of the Henry Draper Catalog. In 1889, Maury studied images of Mizar and found out that it was actually two stars based on two K-lines that became visible for the star every few weeks. Antonia took it upon herself to improve and redesigned the system of classification which was later adopted by the International Astronomical Union. Maury left the observatory in 1891 to begin teaching at the Gilman School in Cambridge Massachusetts. Later, Maury would return to the observatory in 1893 and 1895 to publish many of her observations of stellar spectra. Her work was finished with the help of Pickering and the computing staff and was published in 1897. Maury would return to Harvard College Observatory in 1918 as an adjunct professor. During this time, Maury's work began to be published under her own name due in part to the director Harlow Shapely. She would remain at the observatory until she retired in 1948.