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Pisces–Cetus Supercluster Complex

The Pisces–Cetus Supercluster Complex is a galaxy filament. It includes the Laniakea Supercluster which contains the Virgo Supercluster lobe which in turn contains the Local Group, the galaxy cluster that includes the Milky Way.[1] This filament is adjacent to the Perseus–Pegasus Filament.[2]

Discovery

Astronomer R. Brent Tully of the University of Hawaii’s Institute of Astronomy identified the Complex in 1987.[3]

Extent

The Pisces–Cetus Supercluster Complex is estimated to be about 1.0 billion light-years (Gly) long and 150 million light years (Mly) wide. It is one of the largest structures known in the observable universe, but is exceeded by the Sloan Great Wall (1.3 Gly), Clowes–Campusano LQG (2.0 Gly), U1.11 LQG (2.5 Gly), Huge-LQG (4.0 Gly), and Hercules–Corona Borealis Great Wall (10 Gly), respectively.

The complex comprises about 60 clusters and is estimated to have a total mass of 1018 M.[4] According to the discoverer, the complex is composed of 5 parts:

  1. The Pisces–Cetus Supercluster
  2. The Perseus–Pegasus chain, including the Perseus–Pisces Supercluster
  3. The Pegasus–Pisces chain
  4. The Sculptor region, including the Sculptor Supercluster and Hercules Supercluster
  5. The Laniakea Supercluster, which contains our Virgo Supercluster (Local Supercluster) as well as the Hydra–Centaurus Supercluster.[4]

With its mass of 1015 M, our Virgo Supercluster accounts only for 0.1 percent of the total mass of the complex.

The complex was named after the Pisces–Cetus Superclusters, which are its richest superclusters.

Image

 
The Pisces–Cetus Supercluster Complex is the very long chain of galaxies from the Pisces–Cetus Superclusters, Sculptor Superclusters, the Perseus–Pisces Supercluster and the Laniakea Supercluster. (Shown at the center)

See also

References

  1. ^ Tully, R. B. (1986-04-01). "Alignment of clusters and galaxies on scales up to 0.1 C". The Astrophysical Journal. 303: 25–38. Bibcode:1986ApJ...303...25T. doi:10.1086/164049.
  2. ^ Tully, R. B., Courtois, H., Hoffman, Y & Pomarède, D. Nature 513, 71–73 (2014).
  3. ^ John Noble Wilford (November 10, 1987). "Massive Clusters of Galaxies Defy Concepts of the Universe". The New York Times.
  4. ^ a b Tully, R. Brent (1987-12-01). "More about clustering on a scale of 0.1 C". The Astrophysical Journal. 323: 1–18. Bibcode:1987ApJ...323....1T. doi:10.1086/165803.

External links

pisces, cetus, supercluster, complex, galaxy, filament, includes, laniakea, supercluster, which, contains, virgo, supercluster, lobe, which, turn, contains, local, group, galaxy, cluster, that, includes, milky, this, filament, adjacent, perseus, pegasus, filam. The Pisces Cetus Supercluster Complex is a galaxy filament It includes the Laniakea Supercluster which contains the Virgo Supercluster lobe which in turn contains the Local Group the galaxy cluster that includes the Milky Way 1 This filament is adjacent to the Perseus Pegasus Filament 2 Contents 1 Discovery 2 Extent 3 Image 4 See also 5 References 6 External linksDiscovery EditAstronomer R Brent Tully of the University of Hawaii s Institute of Astronomy identified the Complex in 1987 3 Extent EditThe Pisces Cetus Supercluster Complex is estimated to be about 1 0 billion light years Gly long and 150 million light years Mly wide It is one of the largest structures known in the observable universe but is exceeded by the Sloan Great Wall 1 3 Gly Clowes Campusano LQG 2 0 Gly U1 11 LQG 2 5 Gly Huge LQG 4 0 Gly and Hercules Corona Borealis Great Wall 10 Gly respectively The complex comprises about 60 clusters and is estimated to have a total mass of 1018 M 4 According to the discoverer the complex is composed of 5 parts The Pisces Cetus Supercluster The Perseus Pegasus chain including the Perseus Pisces Supercluster The Pegasus Pisces chain The Sculptor region including the Sculptor Supercluster and Hercules Supercluster The Laniakea Supercluster which contains our Virgo Supercluster Local Supercluster as well as the Hydra Centaurus Supercluster 4 With its mass of 1015 M our Virgo Supercluster accounts only for 0 1 percent of the total mass of the complex The complex was named after the Pisces Cetus Superclusters which are its richest superclusters Image Edit The Pisces Cetus Supercluster Complex is the very long chain of galaxies from the Pisces Cetus Superclusters Sculptor Superclusters the Perseus Pisces Supercluster and the Laniakea Supercluster Shown at the center See also EditEntropy Fossil galaxy group Galaxy group Galaxy cluster Galactic orientation Intracluster medium Large scale structure of the universe List of galaxy groups and clusters Supercluster Timeline of galaxies and large scale structuresReferences Edit Tully R B 1986 04 01 Alignment of clusters and galaxies on scales up to 0 1 C The Astrophysical Journal 303 25 38 Bibcode 1986ApJ 303 25T doi 10 1086 164049 Tully R B Courtois H Hoffman Y amp Pomarede D Nature 513 71 73 2014 John Noble Wilford November 10 1987 Massive Clusters of Galaxies Defy Concepts of the Universe The New York Times a b Tully R Brent 1987 12 01 More about clustering on a scale of 0 1 C The Astrophysical Journal 323 1 18 Bibcode 1987ApJ 323 1T doi 10 1086 165803 External links EditPortals Stars Spaceflight Solar System Science Retrieved from https en wikipedia org w index php title Pisces Cetus Supercluster Complex amp oldid 1170140748, wikipedia, wiki, book, books, library,

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