Perseus–Pisces Supercluster: Difference between revisions
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{{Infobox |
{{Infobox galaxy cluster |
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| name = Perseus-Pisces [[Supercluster]] |
| name = Perseus-Pisces [[Supercluster]] |
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| image = |
| image = Supercúmulo Perseo Piscis.gif |
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| caption = A map of the Perseus-Pisces Supercluster |
| caption = A map of the Perseus-Pisces Supercluster |
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| credit = |
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| other_names = |
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| ⚫ | The ''' |
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| ⚫ | The '''Perseus–Pisces Supercluster''' ('''SCl 40''') is one of the [[List of largest cosmic structures|largest known structures]] in the [[universe]]. Even at a distance of 250 million [[light-year]]s, this chain of [[galaxy cluster]]s extends more than 40° across the northern winter sky. The [[Perseus (constellation)|Perseus]]–[[Pisces (constellation)|Pisces]] Supercluster is one of two dominant concentrations of [[Galaxy|galaxies]] (the other being the [[Local supercluster]]) in the nearby universe (within 300 million light years). This supercluster also borders a prominent void, the [[Taurus Void]], and is part of the [[Perseus–Pegasus Filament]] which stretches for roughly a billion [[light year]]s.<ref>'Astrophysical Journal', Part 1 ({{ISSN|0004-637X}}), vol. 299, Dec. 1, 1985, p. 5-14. "A possible 300 megaparsec filament of clusters of galaxies in Perseus-Pegasus" ''12/1985'' {{bibcode|1985ApJ...299....5B}}</ref> |
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==Clusters== |
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The main clusters of the Perseus–Pisces Supercluster are [[Abell 262]], [[Abell 347]], and [[Abell 426]]. |
The main clusters of the Perseus–Pisces Supercluster are [[Abell 262]], [[Abell 347]], and [[Abell 426]]. |
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* [[List of Abell clusters]] |
* [[List of Abell clusters]] |
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* [[Supercluster]] |
* [[Supercluster]] |
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==References== |
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<references /> |
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==External links== |
==External links== |
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{{Sky|01|50|00|+|36|00|00|250000000}} |
{{Sky|01|50|00|+|36|00|00|250000000}} |
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{{DEFAULTSORT:Perseus-Pisces Supercluster}} |
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[[Category:Perseus-Pisces Supercluster| ]] |
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[[Category:Pisces–Cetus Supercluster Complex]] |
[[Category:Pisces–Cetus Supercluster Complex]] |
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{{supercluster-stub}} |
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Latest revision as of 05:05, 18 October 2024
| Perseus-Pisces Supercluster | |
|---|---|
 A map of the Perseus-Pisces Supercluster | |
| Observation data (Epoch ) | |
| Constellation(s) | Perseus, Pisces |
| Right ascension | 01h 50m |
| Declination | +36° 00′ |
| Distance | 76.7 Mpc (250 Mly) |
The Perseus–Pisces Supercluster (SCl 40) is one of the largest known structures in the universe. Even at a distance of 250 million light-years, this chain of galaxy clusters extends more than 40° across the northern winter sky. The Perseus–Pisces Supercluster is one of two dominant concentrations of galaxies (the other being the Local supercluster) in the nearby universe (within 300 million light years). This supercluster also borders a prominent void, the Taurus Void, and is part of the Perseus–Pegasus Filament which stretches for roughly a billion light years.[1]
Clusters
[edit]The main clusters of the Perseus–Pisces Supercluster are Abell 262, Abell 347, and Abell 426.
See also
[edit]References
[edit]- ^ 'Astrophysical Journal', Part 1 (ISSN 0004-637X), vol. 299, Dec. 1, 1985, p. 5-14. "A possible 300 megaparsec filament of clusters of galaxies in Perseus-Pegasus" 12/1985 Bibcode:1985ApJ...299....5B
External links
[edit]
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