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Abell 1656/Coma-cluster/Ngc4889, Jens Andersen Dolmer

Abell 1656/Coma-cluster/Ngc4889

Getting plate-solving status, please wait...
Abell 1656/Coma-cluster/Ngc4889, Jens Andersen Dolmer

Abell 1656/Coma-cluster/Ngc4889

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Description

The Coma Galaxy Cluster, listed as Abell 1656, is a regular cluster more than 350 million light years away from earth in the constellation of Coma Berenices, near the north galactic pole. It is estimated that over 1000 galaxies are part of the Coma Cluster, making it very rich. Coma is nearly spherical and  is consisting mainly of elliptical and highly-flattened eliptical galaxies. These galaxies have been estimated to be approximately 15 billion years old. Along with the Leo Cluster (Abell 1367), it is one of the two major clusters comprising the Coma Supercluster.
Two giant elliptical galaxies, NGC 4889 and NGC 4874, dominate the foreground of Coma. Like other galaxy clusters, Coma's center consists of a diffuse cloud of hot gas which emits x-rays and is held by the cluster's gravity.
The central part of the Coma Berenices cluster covers a roughly circular area about 1 1/2 degrees across. That’s nine times the area of a full moon, which is about 1/2 a degree across. However, the full cluster may extend farther, and numerous other galaxy clusters are in the same area of the sky.

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Abell 1656/Coma-cluster/Ngc4889, Jens Andersen Dolmer