# Vera Rubin

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Vera Florence Cooper Rubin (/ˈruːbɪn/; 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. These results were later confirmed over subsequent decades. Her work on the galaxy rotation problem was cited by others as evidence for the existence of dark matter. The Vera C. Rubin Observatory in Chile is named in her honor.
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 Philip Cooper, an electrical engineer at Bell Telephone and Rose Cooper who worked at Bell Telephone until they married. The Coopers moved to Washington, D.C., in 1938, where ten-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.

## 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. She struggled to be allowed to present her work at the American Astronomical Society as she was visibly pregnant and not a member of the society, the talk received - to her recollection - universally negative feedback and the paper was not published.
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 Institution 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 Institution, 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 in 1963 and were a popular topic of research.
Wishing to avoid controversial areas of astronomy, including quasars and galactic motion, Rubin began to study the rotation and outer reaches of galaxies, an interest sparked by her collaboration with the Burbidges. She investigated the rotation curves of spiral galaxies, again beginning with Andromeda, by looking at their outermost material. She observed flat rotation curves: the outermost components of the galaxy were moving as quickly as those close to the center. She further uncovered the discrepancy between the predicted angular motion of galaxies based on the visible light and the observed motion. Her research showed that spiral galaxies rotate quickly enough that they should fly apart, if the gravity of their constituent stars was all that was holding them together; because they stay intact, a large amount of unseen mass must be holding them together, a conundrum that became known as the galaxy rotation problem.
Rubin's results came to be cited as evidence that spiral galaxies were surrounded by dark matter haloes. Rubin's calculations showed that galaxies must contain at least five to ten times more mass than can be observed directly based on the light emitted by ordinary matter. Rubin's results were confirmed over subsequent decades, and became the first persuasive results supporting the theory of dark matter, initially proposed by Fritz Zwicky in the 1930s. This data was confirmed by radio astronomers, the discovery of the cosmic microwave background, and images of gravitational lensing. However, Rubin did not rule out alternative models to dark matter also inspired by her measurements. She and her research were discussed in the 1991 PBS series, The Astronomers.
Another area of interest for Rubin was the phenomenon of counter-rotation in galaxies. Her discovery that some gas and stars moved in the opposite direction to the rotation of the rest of the galaxy challenged the prevailing theory that all of the material in a galaxy moved in the same direction, and provided the first evidence for galaxy mergers and the process by which galaxies initially formed.
Rubin's perspective on the history of the work on galaxy movements was presented in a review, "One Hundred Years of Rotating Galaxies," for the Publications of the Astronomical Society of the Pacific in 2000. This was an adaptation of the lecture she gave in 1996 upon receiving the Gold Medal of the Royal Astronomical Society, the second woman to be so honored, 168 years after Caroline Herschel received the Medal in 1828. In 2002, Discover magazine recognized Rubin as one of the 50 most important women in science. She continued her research and mentorship until her death in 2016.

### Vera C. Rubin Observatory

On December 20, 2019, the Large Synoptic Survey Telescope was renamed the Vera C. Rubin Observatory in recognition of Rubin's contributions to the study of dark matter and her outspoken advocacy for the equal treatment and representation of women in science. The observatory is located a mountain in Cerro Pachón, Chile and observations will focus on the study of dark matter and dark energy. As of 2024, the extremely agile telescope is in place and full operation is expected within the next year

## Legacy

When Rubin was elected to the National Academy of Science, she became the second woman astronomer in its ranks, after her colleague Margaret Burbidge. Rubin never won the Nobel Prize, though physicists such as Lisa Randall and Emily Levesque have argued that this was an oversight. She was described by Sandra Faber and Neta Bahcall as one of the astronomers who paved the way for other women in the field, as a "guiding light" for those who wished to have families and careers in astronomy. Rebecca Oppenheimer also recalled Rubin's mentorship as important to her early career.
Rubin died on the night of December 25, 2016, of complications associated with dementia. The president of the Carnegie Institution, where she performed the bulk of her work and research, called her a "national treasure."
The Carnegie Institution has created a postdoctoral research fund in Rubin's honor, and the Division on Dynamical Astronomy of the American Astronomical Society has named the Vera Rubin Early Career Prize in her honor.
Rubin was featured in an animated segment of the 13th and final episode of Cosmos: A Spacetime Odyssey. An area on Mars, Vera Rubin Ridge, is named after her and Asteroid 5726 Rubin was named in her honor.
On 6 November 2020, a satellite named after her (ÑuSat 18 or "Vera", COSPAR 2020-079K) was launched into space.
Rubin will be honored on a U.S. quarter in 2025 as part of the final year of the American Women quarters program.
On June 2, 2024, Nvidia announced that their next generation of data center accelerators would be named after her, with the CPU named Vera and GPU named Rubin.

### In media

The Verubin Nebula which appears in Season Three of Star Trek: Discovery is named after Rubin.
The Stuff Between the Stars: How Vera Rubin Discovered Most of the Universe is a children's book by Sandra Nickel and Aimee Sicuro.

### Awards and honors

* Member, National Academy of Sciences (elected 1981)
* Member, Pontifical Academy of Sciences
* Member, American Philosophical Society
* Gold Medal of the Royal Astronomical Society (1996)
* Weizmann Women & Science Award (1996)
* Gruber International Cosmology Prize (2002)
* Catherine Wolfe Bruce Gold Medal of the Astronomical Society of the Pacific (2003)
* James Craig Watson Medal of the National Academy of Sciences (2004)
* Richtmyer Memorial Award
* Dickson Prize for Science
* National Medal of Science (1993)
* Adler Planetarium Lifetime Achievement Award
* Jansky Lectureship before the National Radio Astronomy Observatory
* Henry Norris Russell Lectureship, American Astronomical Society (1994)
* Honorary doctorates from Harvard University, Yale University, Smith College, Grinnell College, and Princeton University (2005)

## Personal life

Vera Cooper Rubin was married to Robert Joshua Rubin from 1948 until his death in 2008. She had children while undertaking her graduate studies at Cornell, and she continued to work on her research while raising their young children. All four of their children earned PhDs in the natural sciences or mathematics: David (born 1950), is a geologist with the U.S. Geological Survey; Judith Young (1952–2014), was an astronomer at the University of Massachusetts; Karl (born 1956), is a mathematician at the University of California at Irvine; and Allan (born 1960), is a geologist at Princeton University. Rubin's children recalled later in life that their mother made a life of science appear desirable and fun, which inspired them to become scientists themselves.
Motivated by her own battle to gain credibility as a woman in a field that was dominated by male astronomers, Rubin encouraged girls interested in investigating the universe to pursue their dreams. Throughout her life, she faced discouraging comments on her choice of study but persevered, as she was supported by family and colleagues. In addition to encouraging women in astronomy, Rubin was a force for greater recognition of women in the sciences and for scientific literacy.
She, alongside Burbidge, advocated for more women to be elected to the National Academy of Sciences (NAS), selected for review panels, and represented in academic searches. She said that despite her struggles with the NAS, she continued to be dissatisfied with the low number of women who were elected each year, and she further said it was "the saddest part of [her] life".
Rubin was Jewish, and she shared that she saw no conflict between science and religion. In an interview, she said: "In my own life, my science and my religion are separate. I'm Jewish, and so religion to me is a kind of moral code and a kind of history. I try to do my science in a moral way, and, I believe that, ideally, science should be looked upon as something that helps us understand our role in the universe."

## Publications
### Books

* Rubin, Vera (1997). Bright Galaxies, Dark Matters. Masters of Modern Physics. Woodbury, New York City: Springer Verlag/AIP Press. ISBN 978-1563962318.
* Alan Lightman, Roberta Brawer (1992). Origins: The Lives and Worlds of Modern Cosmologists. Harvard University Press. ISBN 9780674644717.

### Articles

The following are a small selection of articles selected by the scientists and historians of the CWP project (Contributions of 20-th Century Women to Physics), as being representative of her most important writings; Rubin published over 150 scientific papers.
* Rubin, Vera; Ford, W. Kent Jr. (1970). "Rotation of the Andromeda Nebula from a Spectroscopic Survey of Emission Regions". The Astrophysical Journal. 159: 379ff. Bibcode:1970ApJ...159..379R. doi:10.1086/150317. S2CID 122756867.
* Rubin, Vera; Roberts, M. S.; Graham, J. A.; Ford Jr., W. K.; Thonnard, N. (1976). "Motion of the Galaxy and the Local Group Determined from the Velocity Anisotropy of Distant Sc I Galaxies. I. The Data". The Astronomical Journal. 81: 687. Bibcode:1976AJ.....81..687R. doi:10.1086/111942.
* Rubin, Vera; Roberts, M. S.; Graham, J. A.; Ford Jr., W. K.; Thonnard, N. (1976). "Motion of the Galaxy and the Local Group Determined from the Velocity Anisotropy of Distant Sc I Galaxies. II. The Analysis for the Motion". The Astronomical Journal. 81: 719ff. Bibcode:1976AJ.....81..719R. doi:10.1086/111943.
* Rubin, Vera; Thonnard, N.; Ford, Jr., W. K. (1980). "Rotational Properties of 21 SC Galaxies With a Large Range of Luminosities and Radii, From NGC 4605 (R=4kpc) to UGC 2885 (R=122kpc)". The Astrophysical Journal. 238: 471ff. Bibcode:1980ApJ...238..471R. doi:10.1086/158003.
* Rubin, Vera; Burstein, D.; Ford, Jr., W. K.; Thonnard, N. (1985). "Rotation Velocities of 16 SA Galaxies and a Comparison of Sa, Sb, and SC Rotation Properties". The Astrophysical Journal. 289: 81ff. Bibcode:1985ApJ...289...81R. doi:10.1086/162866.
* Rubin, Vera; Graham, J. A.; Kenney, J.D. P. (1992). "Cospatial Counterrotating Stellar Disks in the Virgo E7/S0 Galaxy NGC 4550". The Astrophysical Journal. 394: L9 – L12. Bibcode:1992ApJ...394L...9R. doi:10.1086/186460.
* Rubin, Vera (1995). "A Century of Galaxy Spectroscopy". The Astrophysical Journal. 451: 419ff. Bibcode:1995ApJ...451..419R. doi:10.1086/176230. The abstract of this is also generally available.