Back Coma-superswerm Afrikaans عنقود الذؤابة الفائق Arabic Supercúmul de Coma Catalan Coma-Superhaufen German Supercúmulo de Coma Spanish Coma superparv Estonian Superamas de la Chevelure de Bérénice French Supergugus Coma ID Superammasso della Chioma Italian かみのけ座超銀河団 Japanese
| Coma Supercluster | |
|---|---|
 A map of the Coma Supercluster | |
| Observation data (Epoch ) | |
| Constellation(s) | Coma Berenices |
| Major axis | 6 Mpc (20 Mly) |
| Minor axis | 6 Mpc (20 Mly) |
| Distance | 92 Mpc (300 Mly) |
The Coma Supercluster (SCl 117) is a nearby supercluster of galaxies comprising the Coma Cluster (Abell 1656) and the Leo Cluster (Abell 1367).
Located 300 million light-years from Earth,[1] it is in the center of the Great Wall and a part of the Coma Filament.[2] The Coma Supercluster is the nearest massive cluster of galaxies to our own Virgo Supercluster.[3]
It is roughly spherical, about 20 million light-years in diameter and contains more than 3,000 galaxies. It is located in the constellation Coma Berenices. Being one of the first superclusters to be discovered, the Coma Supercluster helped astronomers understand the large scale structure of the universe.
- ^ "Superclusters - A Review of the Universe". Retrieved 1 January 2016.
- ^ 'Astronomy and Astrophysics' (ISSN 0004-6361), vol. 138, no. 1, Sept. 1984, pp. 85-92. Research supported by Cornell University "The Coma/A 1367 filament of galaxies" 09/1984 Bibcode:1984A&A...138...85F
- ^ "The Cosmic Distance Scale". Retrieved 1 January 2016.