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  2. Galaxy rotation curve - Wikipedia

    en.wikipedia.org/wiki/Galaxy_rotation_curve

    The rotation curve of a disc galaxy (also called a velocity curve) is a plot of the orbital speeds of visible stars or gas in that galaxy versus their radial distance from that galaxy's centre. It is typically rendered graphically as a plot , and the data observed from each side of a spiral galaxy are generally asymmetric, so that data from ...

  3. Oort constants - Wikipedia

    en.wikipedia.org/wiki/Oort_constants

    The first two examples are used as constraints to the Galactic rotation, for they show the fastest and slowest the Galaxy can rotate at a given radius. The flat rotation curve serves as an intermediate step between the two rotation curves, and in fact gives the most reasonable Oort constants as compared to current measurements.

  4. Modified Newtonian dynamics - Wikipedia

    en.wikipedia.org/wiki/Modified_Newtonian_dynamics

    Modified Newtonian dynamics (MOND) is a theory that proposes a modification of Newton's second law to account for observed properties of galaxies.Its primary motivation is to explain galaxy rotation curves without invoking dark matter, and is one of the most well-known theories of this class.

  5. Galaxy - Wikipedia

    en.wikipedia.org/wiki/Galaxy

    Though the stars and other visible material contained in such a galaxy lie mostly on a plane, the majority of mass in spiral galaxies exists in a roughly spherical halo of dark matter which extends beyond the visible component, as demonstrated by the universal rotation curve concept. [82]

  6. 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. These results were later confirmed over subsequent ...

  7. Wikipedia:Reference desk/Archives/Science/2018 April 24

    en.wikipedia.org/wiki/Wikipedia:Reference_desk/...

    Rotation curve of a typical spiral galaxy: predicted (A) and observed (B). Dark matter can explain the 'flat' appearance of the velocity curve out to a large radius. Models of rotating disc galaxies in the present day (left) and ten billion years ago (right).

  8. File:Galaxy rotation under the influence of dark matter.ogv

    en.wikipedia.org/wiki/File:Galaxy_rotation_under...

    Right: A galaxy with a flat rotation curve that can be explained by the effects of dark matter. Deutsch: Links: Eine Galaxie mit einer Rotationskurve , wie sie durch die Keplerschen Gesetze vorrausgesagt wird, ohne die Annahme, dass Dunkle Materie existiert.

  9. Talk:Galaxy rotation curve - Wikipedia

    en.wikipedia.org/wiki/Talk:Galaxy_rotation_curve

    > A model of galaxy based on a general relativity metric was also proposed, showing that the rotation curves for the Milky Way, NGC 3031, NGC 3198 and NGC 7331 are consistent with the mass density distributions of the visible matter, avoiding the need for a massive halo of exotic dark matter.