RCS2 J2327 (also identified as RCS2 J2327-0204) is an extremely massive galaxy cluster. It is located approximately 6.4 billion light-years away in the constellation of Pisces,[2] thus making it one of the farthest clusters away from Earth. Recent studies have shown that the galaxy cluster has the mass of two quadrillion suns, making it the second-most-massive galaxy cluster.[3] The galaxies are known to be distorted by gravitational lensing, which can have the ability to deflect distort, and amplify the light from the objects behind it.[4] It can also be observed in strong lens, weak lens, and microlens[5] and has 85% invisible dark matter.[6]
RCS2 J2327 | |
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Observation data (Epoch ) | |
Constellation(s) | Pisces |
Right ascension | 23h 27m 27.60s[1] |
Declination | −02° 04′ 37.4″[1] |
Redshift | 0.6986[1] |
Distance | 6.4 billion ly |
Other designations | |
ACT-CL J2327.4-0204, PSZ1 G080.66-57.87[1] |
References
edit- ^ a b c d "RCS J2327-0204". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-05-06.
- ^ "Galaxy cluster RCS2 J2327". www.spacetelescope.org. Retrieved 2020-04-27.
- ^ ESO; ESA/Hubble; NASA (2017-12-26). "RCS2 J2327 - A Cluster with the Mass of Two Quadrillion Suns". SciTechDaily. Retrieved 2020-04-27.
- ^ "www.zivilisationen.de - Galaxienhaufen". zivilisationen.de (in German). Retrieved 2020-05-09.
- ^ "An estimate of the total mass of one of the largest known galaxy clusters". 28 December 2017. Retrieved 2020-05-07.
- ^ "Is the cosmic colossus RCS2J2327 heavier than allowed?". phys.org. Retrieved 2020-04-29.