Antonia Maury life and biography

American astronomer Antonia Maury was notable as much for refusing to submit to obscurity as she was for her valuable research. The importance of her work was not fully recognized until late in her life. At the age of 77, Maury was awarded the Annie J. Cannon Prize by the American Astronomical Society.

Maury was a woman ahead of her time. She was driven by her convictions rather than the agenda set by the scientific community. Maury demanded to be acknowledged as the author of her work, a gesture commonly denied to contemporary women scientists. Spending long hours in tedious and painstaking observation of the spectral emissions of stars, she invented her own system of star classification that was ignored as cumbersome by her Harvard contemporaries. However, her system was the stepping stone to discoveries that constitute the very foundation of modern stellar astrophysics.

Antonia Maury was born in Cold-Spring-on Hudson, New York, on March 21, 1866, to a distinguished family She was the older daughter of the Reverend Mytton Maury and his wife Virginia Draper. Her maternal uncle was the respected Harvard astronomer, Henry Draper. Historian and physicist, John William Draper, was her maternal grandfather. Her father's ancestors were French Huguenots, while her mother was descended from Portuguese nobility.

Maury was educated at home with her brother and younger sister until her teenage years. Her father, an Episcopalian minister, was her primary tutor. She went on to study at Vassar and graduated with a bachelor's degree in 1887, earning honors in astronomy and physics.

When Henry Draper died, astronomer Edward Charles Pickering of the Harvard Observatory took over his project of cataloging and classifying stars according to their spectra. The light from a star, when viewed through a prism and magnified appears as a band of colors punctuated by darker bands. These are termed spectral lines, and represent a distinctive fingerprint for each star. Analysis of these lines provides insights into the star's temperature, chemical composition, and motion.

A year after her graduation, Maury joined Pickering's staff of women "computers" to help complete the immense work of observing and classifying stars for the Draper catalog. As director of the Harvard Observatory since 1876, Pickering was the first to include women on his staff, as volunteers and salaried assistants. This, however, appears to have been more an act of economic pragmatism than progressive-mindedness. In spite of the low pay, averaging about $10.50 per week, or about 25 cents an hour, applications from women flooded in from all over the world. Harlow Shapley, a director of the observatory after Pickering, was quoted as saying: "Luckily Harvard College was swarming with cheap assistants; that was how we got things done." The entire job of classifying some 250,000 stars took 40 years to complete. It could not have been accomplished without the group of women whom some alluded to as "Pickering's Harem." Foremost among them were Antonia Maury, Williamina Fleming, and Annie Cannon.

Maury's first assignment for Pickering was to determine the orbital period of the spectroscopic binary, Zeta Ursae Majoris, also called Mizar, first discovered by Pickering in 1887. Binaries are stars that orbit so close to each other that they cannot be detected except by a spectroscope. When examined, the spectral lines regularly shift back and forth as the stars revolve around each other. In 1889, Maury independently discovered the second binary, Beta Aurigae and determined its orbital period. Binaries continued to fascinate Maury throughout her career.

Maury's major assignment for the Draper catalog was to observe a group of selected bright northern stars. These were photographed with a more powerful telescope fitted with additional prisms. As she enlarged and studied the spectra under a microscope, they proved much more complex than had ever been previously realized. Fleming had devised an alphabetical system of classification where stars were grouped into alphabetical categories: OBAFGKM— which was remembered through the mnemonic "Oh Be A Fine Girl, Kiss Me." Maury felt this system to be too simplistic, so she replaced it with her own system of 22 groups based on a sequence of descending temperature.

Within each of these groups, however, Maury noticed that two stars having the same pattern of lines and color were displaying differences in line width and sharpness. She decided to introduce three further subdivisions that recognized these features, believing them to signal some property yet to be discovered.

Maury's system brought her into direct conflict with Pickering, who saw no need for the entire project to fall behind schedule so that she could carry out her painstakingly meticulous width and sharpness measurements. Maury was always inclined to solve problems or puzzles that she encountered, and tended to fall behind the schedule that Pickering set for data collection. Finally, the original thinker in Maury could no longer endure Pickering's tunnel vision. She left his group in 1892 without completing the study.

One person did take notice of Maury's classification. Although less than fluent in the English language, the noted Danish astrophysicist Ejnar Hertzprung objected strongly to the omission of Maury's classification in the completed catalog. He wrote: "In my opinion the separation by Antonia Maury of the c-and ac stars is the most important advancement in stellar classification since the trials by Vogel and Secchi. To neglect the c-properties in solar spectra, I think, is nearly the same thing as if the zoologist, who had detected the deciding differences between a whale and a fish, would continue in classifying them together."

Maury's work was vital in Hertzprung's formulation which came to be known as the Hertzprung-Russel diagram. This opened the door to an entirely new level of understanding the characteristics and evolution of stars. In 1905, Hertzprung had noticed that some red stars were very bright, while others seemed faint. He was sure that these two types of stars would show differences in their spectra. Of all the catalogs published, only Maury's classification provided the distinction that he was looking for.

Although Pickering continued to downplay the importance of Maury's work, her contribution to spectral analysis was finally acknowledged in 1922. That year, the International Astronomical Union modified its official classification system based on Annie Cannon's system to include the prefix c-to a certain spectral type defined by narrow and sharp lines.

After leaving the Harvard Observatory, Maury continued to work intermittently on the project. Pickering urged her to complete the work or agree to turn it over to someone else. Though she was eager to finish, both for the sake of her reputation and to honor the memory of her late uncle, Maury had one basic condition: she would have to be acknowledged unambiguously as its author. In a letter to Pickering, she said: "I do not think it is fair that I should pass the work into other hands until it can stand as work done by me. I worked out the theory at the cost of much thought and elaborate comparison and I think that I should have full credit for my theory of the relations of the star spectra and also for my theories in regard to Beta Lyrae."

Pickering wrote back somewhat coldly that it was the regular practice of the Observatory to acknowledge authors of "particular portions." Maury would not settle for the standard acknowledgement. In the end, she got her wish. Her catalog, appearing in volume 28 of the Harvard Annals in 1897 was the first issue to have the name of a woman on the title page. Maury's study was based on some 4,800 photographs. 681 northern stars were classified according to her system.

Although Maury did not return to Harvard for over a decade after the publication of her catalog, she continued to research spectroscopic binary stars. She turned her attention to the complex spectroscopic binary, Beta Lyrae, investigating it over many years. Maury is said to have examined close to 300 spectra of this star. She published her conclusions in a treatise published in the Harvard Annals in 1933.

Maury held various teaching positions in the 1890s. She taught first at the Gilman School in Cambridge, Massachusetts and later at Miss Mason's school in Tarrytown, New York. She also delivered lectures on astronomy at Cornell and elsewhere, both to professional audiences and laypersons. She returned to Harvard in 1918 as an adjunct professor. Pickering died in 1919 and Maury found herself able to work better with his successor, Harlow Shapley. She continued to examine the puzzling spectra of Beta Lyrae until her official retirement in 1948.

Maury was also an accomplished ornithologist and a passionate conservationist who fought to save western redwood forests when they were being fed to sawmills to meet the wartime lumber requirements. She was a member of the American Astronomical Society, the Royal Astronomical Society, and the National Audubon Society. For several years after her retirement, Maury was curator of the Draper Park Museum at Hastings-on Hudson. She died on January 8, 1952, at a hospital in Dobbs Ferry, New York.

Cecilia Payne-Gaposchkin, who began work at the Harvard Observatory in 1923, discussed her impressions of Maury: "Of course, I only knew her when she was old. I was very fond of her, but she just talked and talked and talked and talked. You couldn't do any work because she wanted to talk so much. It was just she needed an outlet; she needed to discuss. Nobody had ever listened to her, nobody had ever responded to her scientific questionings, I think."

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