Celestial hemisphere:  Northern  ·  Constellation: Coma Berenices (Com)  ·  Contains:  NGC 4839  ·  NGC 4848  ·  NGC 4874  ·  NGC 4889  ·  NGC 4895  ·  NGC 4908  ·  NGC 4921  ·  NGC 4926
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Abell 1656 Galaxy Cluster, Jeff Weiss
Abell 1656 Galaxy Cluster
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Abell 1656 Galaxy Cluster

Getting plate-solving status, please wait...
Abell 1656 Galaxy Cluster, Jeff Weiss
Abell 1656 Galaxy Cluster
Powered byPixInsight

Abell 1656 Galaxy Cluster

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Description

4.2hr LRGB

Also known as the Coma Cluster, Abell 1656 is a large galaxy cluster of over 1000 identified galaxies, 450 of which are identified by PI image solver in this image. It's mean distance is 320 MLY and the central region is dominated by two giant ellipticals, NGC 4874 and NGC 4889. Predominantly elliptical (old) galaxies, this galaxy cluster produces large amounts of hot X-ray emitting gas and dark matter.    This object is very interesting because it is the cluster from which Fritz Zwicky concluded in the 1930's that the galaxies' rotational fall off was far too slow for the observed matter distribution and inferred the existence of dark matter, inventing the term 50 years ahead of his time. This cluster is now accepted to have 90% of its mass in dark matter.

CORRECTION: Actually Zwicky's 1930's conjecture (and naming of "dark matter") was NOT based on flattening rotational velocity but on an insufficient stellar luminance calculation.  (12/12/14)

North is up. There is actually a quasar QSO [HB89] 1256+280 that is 11.3 +- 1.0 billion light years away in this image, far beyond the Abel 1656 galaxies. Follow the link above to see it.

D.A.R.C. Observatory, Mercey Hot Springs , CA May-June 2014

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  • Abell 1656 Galaxy Cluster, Jeff Weiss
    Original
  • Abell 1656 Galaxy Cluster, Jeff Weiss
    C
  • Abell 1656 Galaxy Cluster, Jeff Weiss
    D
  • Final
    Abell 1656 Galaxy Cluster, Jeff Weiss
    E

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Abell 1656 Galaxy Cluster, Jeff Weiss