Vera Roberts Popular Books

Vera Roberts Biography & Facts

Vera Florence Cooper Rubin (; July 23, 1928 – December 25, 2016) was an American astronomer who pioneered work on galaxy rotation rates. She uncovered the discrepancy between the predicted and observed angular motion of galaxies by studying galactic rotation curves. By identifying the galaxy rotation problem, her work provided evidence for the existence of dark matter. These results were later confirmed over subsequent decades. Beginning her academic career as the sole undergraduate in astronomy at Vassar College, Rubin went on to graduate studies at Cornell University and Georgetown University, where she observed deviations from Hubble flow in galaxies and provided evidence for the existence of galactic superclusters. She was honored throughout her career for her work, receiving the Bruce Medal, the Gold Medal of the Royal Astronomical Society, and the National Medal of Science, among others.Rubin spent her life advocating for women in science, and she was known for her mentorship of aspiring female astronomers. Her legacy was described by The New York Times as "ushering in a Copernican-scale change" in cosmological theory. Early life Vera Cooper was born on July 23, 1928, in Philadelphia, Pennsylvania. She was the younger of two sisters. Her parents were Jewish immigrants from Eastern Europe. Pesach Kobchefski, who was born in Vilnius, Lithuania (then part of Poland) and anglicized his name to Philip Cooper, became an electrical engineer and worked at Bell Telephone. He married Rose Applebaum, who was from Bessarabia (in present-day Moldova). They met at Bell, where Rose worked until they married.The Coopers moved to Washington, D.C., in 1938, where 10-year-old Vera developed an interest in astronomy while watching the stars from her window. "Even then I was more interested in the question than in the answer," she remembered. "I decided at an early age that we inhabit a very curious world." She built a crude telescope out of cardboard with her father, and began to observe and track meteors. She attended Coolidge Senior High School, graduating in 1944.Rubin's older sister, Ruth Cooper Burg, was an attorney who later worked as an administrative law judge in the United States Department of Defense. Her father, a mathematically talented electrical engineer, supported her passion by helping her build a telescope Education Rubin was inspired to pursue an undergraduate education at Vassar College – then an all-women's school –, and she was also inspired by Maria Mitchell, who had been a professor in that same college in 1865. She ignored advice she had received from a high school science teacher to avoid a scientific career and become an artist. She graduated Phi Beta Kappa and earned her bachelor's degree in astronomy in 1948, the only graduate in astronomy that year. She attempted to enroll in a graduate program at Princeton, but was barred due to her gender. Princeton would not accept women as astronomy graduate students for 27 more years. Rubin also turned down an offer from Harvard University. She married in 1948, and her husband, Robert Joshua Rubin, was a graduate student at Cornell University.Rubin then enrolled at Cornell University, and earned a master's degree in 1951. During her graduate studies, she studied the motions of 109 galaxies and made one of the first observations of deviations from Hubble flow (how the galaxies move apart from one another). She worked with astronomer Martha Carpenter on galactic dynamics, and studied under Philip Morrison, Hans Bethe, and Richard Feynman. Though the conclusion she came to – that there was an orbital motion of galaxies around a particular pole – was disproven, the idea that galaxies were moving held true and sparked further research. Her research also provided early evidence of the supergalactic plane. This information and the data she discovered was immensely controversial. After she struggled to be allowed to present her work at the American Astronomical Society despite being visibly pregnant, she was summarily rejected and the paper was forgotten.Rubin studied for her Ph.D. at Georgetown University, the only university in Washington, D.C., that offered a graduate degree in astronomy.She was 23 years old and pregnant when she began her doctoral studies, and the Rubins had one young child at home. She began to take classes with Francis Heyden, who recommended her to George Gamow of the neighboring George Washington University, her eventual doctoral advisor. Her dissertation, completed in 1954, concluded that galaxies clumped together, rather than being randomly distributed through the universe, a controversial idea not pursued by others for two decades. Throughout her graduate studies, she encountered discouraging sexism; in one incident she was not allowed to meet with her advisor in his office, because women were not allowed in that area of the Catholic university. Career For the next eleven years, Rubin held various academic positions. She served for a year as an instructor of Mathematics and Physics at Montgomery College. From 1955 to 1965 she worked at Georgetown University as a research associate astronomer, lecturer (1959–1962), and finally, assistant professor of astronomy (1962–1965). She joined the Carnegie Institution of Washington (later called Carnegie Institute of Science) in 1965 as a staff member in the Department of Terrestrial Magnetism. There she met her long-time collaborator, instrument-maker Kent Ford. Because she had young children, she did much of her work from home. In 1963, Rubin began a year-long collaboration with Geoffrey and Margaret Burbidge, during which she made her first observations of the rotation of galaxies while using the McDonald Observatory's 82-inch telescope. During her work at the Carnegie Institute, Rubin applied to observe at the Palomar Observatory in 1965, despite the fact that the building did not have facilities for women. She created her own women's restroom, sidestepping the lack of facilities available for her. She became the first female astronomer to observe there.At the Carnegie Institution, Rubin began work related to her controversial thesis regarding galaxy clusters with Ford, making hundreds of observations using Ford's image-tube spectrograph. This image intensifier allowed resolving the spectra of astronomical objects that were previously too dim for spectral analysis. The Rubin–Ford effect, an apparent anisotropy in the expansion of the Universe on the scale of 100 million light years, was discovered through studies of spiral galaxies, particularly the Andromeda Galaxy, chosen for its brightness and proximity to Earth. The idea of peculiar motion on this scale in the universe was a highly controversial proposition, which was first published in journals in 1976. It was dismissed by leading astronomers but ultimately shown to be valid. The effect is now known as large scale streaming. The pair also briefly studied quasars, which had been discovered i.... Discover the Vera Roberts popular books. Find the top 100 most popular Vera Roberts books.