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  2. Dark galaxy - Wikipedia

    en.wikipedia.org/wiki/Dark_galaxy

    A dark galaxy is a hypothesized galaxy with no (or very few) stars. They received their name because they have no visible stars but may be detectable if they contain significant amounts of gas. Astronomers have long theorized the existence of dark galaxies, but there are no confirmed examples to date. [1]

  3. Category:Dark galaxies - Wikipedia

    en.wikipedia.org/wiki/Category:Dark_galaxies

    Pages in category "Dark galaxies" The following 7 pages are in this category, out of 7 total. This list may not reflect recent changes. ...

  4. Ultra diffuse galaxy - Wikipedia

    en.wikipedia.org/wiki/Ultra_diffuse_galaxy

    NGC 1052-DF2, an ultra diffuse galaxy. An ultra diffuse galaxy (UDG), or dark galaxy, [1] is an extremely low luminosity galaxy, the first example of which was discovered in the nearby Virgo Cluster by Allan Sandage and Bruno Binggeli in 1984. [a] These galaxies have been studied for many years prior to their renaming in 2015. Their lack of ...

  5. VIRGOHI21 - Wikipedia

    en.wikipedia.org/wiki/VIRGOHI21

    The large gravity of the dark matter halo in this interpretation explains the perturbed nature of the nearby spiral galaxy NGC 4254 and the bridge of neutral hydrogen extending between the two entities. Under this interpretation, VIRGOHI21 would be the first discovery of the dark galaxies anticipated by simulations of dark-matter theories. [3]

  6. Dark matter - Wikipedia

    en.wikipedia.org/wiki/Dark_matter

    Because galaxy-size density fluctuations get washed out by free-streaming, hot dark matter implies the first objects that can form are huge supercluster-size pancakes, which then fragment into galaxies, while the reverse is true for cold dark matter.

  7. Abell 1689 - Wikipedia

    en.wikipedia.org/wiki/Abell_1689

    The very large mass of this cluster makes it useful for the study of dark matter and gravitational lensing. [7] [8] At the time of its discovery in 2008, one of the lensed galaxies, A1689-zD1, was the most distant galaxy found. [9] [10]

  8. Void (astronomy) - Wikipedia

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

    Cosmic voids (also known as dark space) are vast spaces between filaments (the largest-scale structures in the universe), which contain very few or no galaxies. In spite of their size, most galaxies are not located in voids. This is because most galaxies are gravitationally bound together, creating huge cosmic structures known as galaxy filaments.

  9. Galaxy - Wikipedia

    en.wikipedia.org/wiki/Galaxy

    A dark or "ultra diffuse" galaxy is an extremely-low-luminosity galaxy. It may be the same size as the Milky Way, but have a visible star count only one percent of the Milky Way's. Multiple mechanisms for producing this type of galaxy have been proposed, and it is possible that different dark galaxies formed by different means. [102]