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  2. Great Debate (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Great_Debate_(astronomy)

    Later in the 1920s, Edwin Hubble showed that Andromeda was far outside the Milky Way by measuring Cepheid variable stars, proving that Curtis was correct. [6] It is now known that the Milky Way is only one of as many as an estimated 200 billion (2 × 10 11) [7] to 2 trillion (2 × 10 12) or more galaxies in the observable universe.

  3. US 708 - Wikipedia

    en.wikipedia.org/wiki/US_708

    US 708 is a hyper-velocity class O subdwarf in Ursa Major, in the halo of the Milky Way Galaxy. One of the fastest-moving stars in the galaxy , the star was first surveyed in 1982. [ 3 ] [ 4 ] [ 5 ]

  4. Sombrero Galaxy - Wikipedia

    en.wikipedia.org/wiki/Sombrero_Galaxy

    The Sombrero Galaxy (also known as Messier Object 104, M104 [4] or NGC 4594) is a peculiar galaxy of unclear classification [6] in the constellation borders of Virgo and Corvus, being about 9.55 megaparsecs (31.1 million light-years) [2] from the Milky Way galaxy.

  5. Dark matter - Wikipedia

    en.wikipedia.org/wiki/Dark_matter

    The hypothesis of dark matter has an elaborate history. [18] [19] In the appendices of the book Baltimore lectures on molecular dynamics and the wave theory of light where the main text was based on a series of lectures given in 1884, [18] Lord Kelvin discussed the potential number of stars around the Sun from the observed velocity dispersion of the stars near the Sun, assuming that the Sun ...

  6. Stellar density - Wikipedia

    en.wikipedia.org/wiki/Stellar_density

    The locations within the Milky Way that have the highest stellar density are the central core and the interior of globular clusters. A typical mass density for a globular cluster is 70 M Sun pc −3 , which is 500 times the mass density near the Sun. [ 2 ] In the solar neighborhood, the stellar density of a star cluster must be greater than 0. ...

  7. Small Magellanic Cloud - Wikipedia

    en.wikipedia.org/wiki/Small_Magellanic_Cloud

    The Small Magellanic Cloud (SMC) is a dwarf galaxy near the Milky Way. [5] Classified as a dwarf irregular galaxy, the SMC has a D 25 isophotal diameter of about 5.78 kiloparsecs (18,900 light-years), [1] [3] and contains several hundred million stars. [5] It has a total mass of approximately 7 billion solar masses. [6]

  8. Extragalactic astronomy - Wikipedia

    en.wikipedia.org/wiki/Extragalactic_astronomy

    Galaxies in the 1995 Hubble Deep Field. Extragalactic astronomy is the branch of astronomy concerned with objects outside the Milky Way galaxy. In other words, it is the study of all astronomical objects which are not covered by galactic astronomy.

  9. Great Attractor - Wikipedia

    en.wikipedia.org/wiki/Great_Attractor

    Approximately 400 elliptical galaxies are moving toward the Great Attractor beyond the Zone of Avoidance caused by the Milky Way galaxy light. Intense efforts to work through the difficulties caused by the occlusion by the Milky Way during the late 1990's identified the Norma Cluster at the center of the Great Attractor region. [1]