Horologium-Reticulum Supercluster
The Horologium-Reticulum Supercluster, is a massive supercluster spanning around 550 million light-years. It has a mass of around 10 solar masses, similar to that of the Laniakea Supercluster, which houses the Milky Way. It is centered on coordinates right ascension 03 19 and declination −50° 02′, and spans an angular area of 12° × 12°.
The nearest part of the supercluster is 700 million light-years away from Earth, while the far end of it is 1.2 billion light-years. It is visible in the constellations Horologium and Eridanus. The Horologium Supercluster has about 5,000 galaxy groups (30,000 giant galaxies and 300,000 dwarf galaxies). It includes the galaxy cluster Abell 3266.
See also
- Abell catalog
- Large scale structure of the universe
- List of Abell clusters
- List of superclusters
- List of largest galaxy superclusters
References
- ^ "The Horologium Supercluster". www.atlasoftheuniverse.com. Retrieved 2018-11-04.
- ^ Fleenor, Matthew C.; Rose, James A.; Christiansen, Wayne A.; Hunstead, Richard W.; Johnston-Hollitt, Melanie; Drinkwater, Michael J.; Saunders, William (September 2005). "Large-Scale Velocity Structures in the Horologium-Reticulum Supercluster". The Astronomical Journal. 130 (3): 957–967. arXiv:astro-ph/0505361. Bibcode:2005AJ....130..957F. doi:10.1086/431972. S2CID 13839289.
- ^ "The Horologium Supercluster". www.atlasoftheuniverse.com. Retrieved 2018-11-04.
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