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  2. Vera Rubin - Wikipedia

    en.wikipedia.org/wiki/Vera_Rubin

    Vera Florence Cooper Rubin (/ ˈ r uː b ɪ n /; July 23, 1928 – December 25, 2016) was an American astronomer who pioneered work on galaxy rotation rates. [1] [2] She uncovered the discrepancy between the predicted and observed angular motion of galaxies by studying galactic rotation curves.

  3. Vera Rubin, pioneering U.S. dark matter astronomer, dies at 88

    www.aol.com/article/news/2016/12/26/vera-rubin...

    She used galaxies' rotations to discover the first direct evidence of dark matter in the 1970s while working at the Carnegie Institution in Washington. Vera Rubin, pioneering U.S. dark matter ...

  4. Telescope with world’s largest digital camera will be a ‘game ...

    www.aol.com/world-largest-digital-camera-game...

    Under construction since 2015, the telescope is named after pioneering American astronomer Vera Rubin, who died in 2016 and, among other achievements, first confirmed the existence of dark matter ...

  5. Galaxy rotation curve - Wikipedia

    en.wikipedia.org/wiki/Galaxy_rotation_curve

    Such dark-matter-dominated dwarf galaxies may hold the key to solving the dwarf galaxy problem of structure formation. Very importantly, the analysis of the inner parts of low and high surface brightness galaxies showed that the shape of the rotation curves in the centre of dark-matter dominated systems indicates a profile different from the ...

  6. Vera C. Rubin Observatory - Wikipedia

    en.wikipedia.org/wiki/Vera_C._Rubin_Observatory

    The observatory is named after Vera C. Rubin. The name honors Rubin and her colleagues' legacy to probe the nature of dark matter by mapping and cataloging billions of galaxies through space and time. [24] The telescope itself is named the Simonyi Survey Telescope, after private donors Charles and Lisa Simonyi. [26]

  7. Dark matter - Wikipedia

    en.wikipedia.org/wiki/Dark_matter

    It is dark matter composed of constituents with an FSL much smaller than a protogalaxy. This is the focus for dark matter research, as hot dark matter does not seem capable of supporting galaxy or galaxy cluster formation, and most particle candidates slowed early. The constituents of cold dark matter are unknown.

  8. Unafraid of the Dark - Wikipedia

    en.wikipedia.org/wiki/Unafraid_of_the_Dark

    His calculations suggested that there must be more mass in the universe than those apparent in the observable galaxies, and called this dark matter. Initially forgotten, Zwicky's theory was confirmed by the work of Vera Rubin , who observed that the rotation of stars at the edges of observable galaxies did not follow expected rotational ...

  9. Dark Matter May Not Be Invisible After All. This Discovery ...

    www.aol.com/dark-matter-may-not-invisible...

    Dark matter is called ‘dark’ because it’s invisible to us and does not measurably interact with anything other than gravity. It could be interspersed between the atoms that make up the Earth ...