Vera Rubin
Revision for “Vera Rubin” created on November 17, 2015 @ 11:09:15
Vera Rubin
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Vera Rubin (1928- ) is an astronomer who has done pioneering work on galaxy rotation rates. Her contribution to astronomy was the discovery of the discrepancy between the predicted angular motion of galaxies and the observed motion, by studying galactic rotation curves. Rubin is currently a research astronomer at the Carnegie Institution of Washington. She is a member of the US National Academy of Sciences and the Pontifical Academy of Sciences.
<div id="toc"> <h2>Table of Contents</h2> <ul> <li class="toclevel-1"><a href="#w_early-life-and-education"><span class="tocnumber">1</span> <span class="toctext">Early life and education</span></a></li> <li class="toclevel-1"><a href="#w_discoveries"><span class="tocnumber">2</span> <span class="toctext">Discoveries</span></a></li> <li class="toclevel-1"><a href="#w_prizes-and-distinctions"><span class="tocnumber">3</span> <span class="toctext">Prizes and distinctions</span></a></li> <li class="toclevel-1"><a href="#w_see-also"><span class="tocnumber">4</span> <span class="toctext">See also</span></a></li> <li class="toclevel-1"><a href="#w_sources"><span class="tocnumber">5</span> Referen<span class="toctext">ces</span></a></li> </ul> </div> <h2 id="w_early-life-and-education">Early life and education</h2> Rubin (ne Cooper) was born in Philadelphia, Pennsylvania on July 23, 1928. She graduated from Vassar College in 1948 with a bachelors degree in Astronomy. She then tried to enroll at Princeton but never received their graduate catalogue as women there were not allowed in the graduate astronomy programme until 1975. She went instead, with her new husband Bob Rubin, a physicist, to Cornell University, where she completed a Master’s degree in 1951. Her master’s thesis was severely criticised when presented to the American Astronomical Society: Rubin suggested that galaxies might be rotating around an unknown center, not just expanding out as described in the big bang theory. There was no scientific theory to explain this finding and she was severely criticised. Despite this she went on to complete a PhD at Georgetown University in 1954. Again, her disseration was ignored and criticised; her findings were later validated. By the late 1970s, after Rubin and her colleagues had observed dozens of spirals, it was clear that something other than the visible mass was responsible for the stars’ motions. Analysis showed that each spiral galaxy is embedded in a spheroidal distribution of dark matter — a “halo.” The stars’ response to the gravitational attraction of the matter produces the high velocities. As a result of Rubin’s groundbreaking work, it has become apparent that more than 90% of the universe is composed of dark matter. During the 1970s, Rubin and collaborators Ford, Norbert Thonnard, and John Graham were among the first astronomers to examine the systemic velocities of galaxies to see if there are large-scale motions of galaxies, superposed on the general expansion of the universe. Their early work, and more recent work by others, suggests that such motions exist. |