Flat rotation curve of the Andromeda Galaxy (1970)
With Kent Ford; outer stars orbited as fast as inner ones, implying large amounts of unseen mass
Science · Maths, astronomy, medicine & more
1928–2016 · American
Astronomy — galaxy rotation and dark matter
Vera Rubin was an American astronomer at the Carnegie Institution of Washington whose measurements, made with Kent Ford, showed that stars in the outer parts of spiral galaxies orbit as fast as those near the centre. These "flat rotation curves", beginning with the Andromeda Galaxy in 1970, provided the most persuasive early evidence for dark matter. She was also a tireless campaigner for women in science, and the Vera C. Rubin Observatory in Chile is named after her.
Flat rotation curve of the Andromeda Galaxy (1970)
With Kent Ford; outer stars orbited as fast as inner ones, implying large amounts of unseen mass
Flat rotation curves of spiral galaxies as evidence for dark matter (1970s–1980)
Data on dozens of galaxies showed the pattern was universal, making the case for dark matter
Georgetown PhD thesis showing galaxies are clumped, not evenly distributed (1954)
Supervised by George Gamow; an early hint of large-scale structure in the universe
Discovery of counter-rotating stellar disks in galaxy NGC 4550 (1992)
Two populations of stars in the same galaxy orbiting in opposite directions
Bright Galaxies, Dark Matters (1997)
Collection of her essays on astronomy and on women in science