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Supercluster

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A supercluster is a large group of smaller galaxy clusters or galaxy groups;[1] they are among the largest known structures in the universe. The Milky Way is part of the Local Group galaxy group (which contains more than 54 galaxies), which in turn is part of the Virgo Supercluster, which is part of the Laniakea Supercluster, which is part of the Pisces–Cetus Supercluster Complex.[2] The large size and low density of superclusters means that they, unlike clusters, expand with the Hubble expansion. The number of superclusters in the observable universe is estimated to be 10 million.[3]

A map of the superclusters and voids nearest to Earth

Existence

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The existence of superclusters indicates that the galaxies in the Universe are not uniformly distributed; most of them are drawn together in groups and clusters, with groups containing up to some dozens of galaxies and clusters up to several thousand galaxies. Those groups and clusters and additional isolated galaxies in turn form even larger structures called superclusters.

 
The Abell 901/902 supercluster is located a little over two billion light-years from Earth.[4]

Their existence was first postulated by George Abell in his 1958 Abell catalogue of galaxy clusters. He called them "second-order clusters", or clusters of clusters.[5]

Superclusters form massive structures of galaxies, called "filaments", "supercluster complexes", "walls" or "sheets", that may span between several hundred million light-years to 10 billion light-years, covering more than 5% of the observable universe. These are the largest structures known to date. Observations of superclusters can give information about the initial condition of the universe, when these superclusters were created. The directions of the rotational axes of galaxies within superclusters are studied by those who believe that they may give insight and information into the early formation process of galaxies in the history of the Universe.[6]

Interspersed among superclusters are large voids of space where few galaxies exist. Superclusters are frequently subdivided into groups of clusters called galaxy groups and clusters.

Although superclusters are supposed to be the largest structures in the universe according to the Cosmological principle, larger structures have been observed in surveys, including the Sloan Great Wall.[7]

List of superclusters

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Galaxy supercluster Data Notes
Einasto Supercluster
  • z = ~0.25 (3 billion light years )
  • Length = 360 million light years
  • Mass = 2.6 × 1016 solar masses
 Discovered in 2023 by analyzing Sloan Digital Sky Survey images. Claimed to be the most massive galaxy supercluster discovered so far.[8][9]
King Ghidorah Supercluster
  • z = 0.50-0.64
  • Mass = 1 × 1016 solar masses
 The most massive galaxy supercluster discovered until 2023.[10]
Laniakea Supercluster
  • z = 0.000
  • Length = 153 Mpc (500 million light-years)
 The Laniakea Supercluster is the supercluster that contains the Virgo Cluster, Local Group, and by extension on the latter, our galaxy; the Milky Way.[2]
Virgo Supercluster
  • z= 0.000
  • Length = 33 Mpc (110 million light-years)
 It contains the Local Group with our galaxy, the Milky Way. It also contains the Virgo Cluster near its center, and is sometimes called the Local Supercluster. It is thought to contain over 47,000 galaxies.

A 2014 study indicates that the Virgo Supercluster is only a lobe of an even greater supercluster, Laniakea.[11]

Hydra–Centaurus Supercluster It is composed of two lobes, sometimes also referred to as superclusters, or sometimes the entire supercluster is referred to by these other two names
  • Hydra Supercluster
  • Centaurus Supercluster

In 2014, the newly announced Laniakea Supercluster subsumed the Hydra-Centaurus Supercluster, which became a component of the new supercluster.[11]

Pavo–Indus Supercluster

In 2014, the newly announced Laniakea Supercluster subsumed the Pavo-Indus Supercluster, which became a component of the new supercluster.[11]

Southern Supercluster

Includes Fornax Cluster (S373), Dorado and Eridanus clouds.[12]

Saraswati Supercluster Distance = 4000 Million light years (1.2 Gpc)

Length = 652 Million light-years

The Saraswati Supercluster consists of 43 massive galaxy clusters such as Abell 2361 and has a mass of about 2 x 1016 M☉ and is seen in the Pisces constellation

Nearby superclusters

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Galaxy supercluster Data Notes
Perseus–Pisces Supercluster
Coma Supercluster Forms most of the CfA Homunculus, the center of the CfA2 Great Wall galaxy filament
Sculptor Superclusters SCl 9
Hercules Superclusters SCl 160
Leo Supercluster SCl 93
Ophiuchus Supercluster
  • 17h 10m −22°
  • cz=8500–9500 km/s (centre)
  • 18 Mpc x 26 Mpc
 Forming the far wall of the Ophiuchus Void, it may be connected in a filament, with the Pavo-Indus-Telescopium Supercluster and the Hercules Supercluster. This supercluster is centered on the cD cluster Ophiuchus Cluster, and has at least two more galaxy clusters, four more galaxy groups, several field galaxies, as members.[13]
Shapley Supercluster
  • z=0.046.(650 Mly away)
 The second supercluster found, after the Local Supercluster.

Distant superclusters

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Galaxy supercluster Data Notes
Pisces–Cetus Supercluster
Boötes Supercluster SCl 138
Horologium–Reticulum Supercluster
z=0.063 (700 Mly)
Length = 550 Mly
Corona Borealis Supercluster
z=0.07[14]
Columba Supercluster
Aquarius Supercluster
Aquarius B Supercluster
Aquarius–Capricornus Supercluster
Aquarius–Cetus Supercluster
Bootes A Supercluster
Caelum Supercluster
z=0.126 (1.4 Gly)
Draco Supercluster
Draco–Ursa Major Supercluster
Fornax–Eridanus Supercluster
Grus Supercluster
Leo A Supercluster
Leo–Sextans Supercluster
Leo–Virgo Supercluster SCl 107
Microscopium Supercluster SCl 174
Pegasus–Pisces Supercluster SCl 3
Perseus–Pisces Supercluster SCl 40
Pisces–Aries Supercluster
Ursa Majoris Supercluster
Virgo-Coma Supercluster SCl 111

Extremely distant superclusters

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Galaxy supercluster Data Notes
Hyperion proto-supercluster z=2.45 This supercluster at the time of its discovery in 2018 was the earliest and largest proto-supercluster found to date.[15][16]
Lynx Supercluster z=1.27 Discovered in 1999[17] (as ClG J0848 4453, a name now used to describe the western cluster, with ClG J0849 4452 being the eastern one),[18] it contains at least two clusters RXJ 0848.9 4452 (z=1.26) and RXJ 0848.6 4453 (z=1.27) . At the time of discovery, it became the most distant known supercluster.[19] Additionally, seven smaller groups of galaxies are associated with the supercluster.[20]
SCL @ 1338 27 at z=1.1

z=1.1

Length=70Mpc

A rich supercluster with several galaxy clusters was discovered around an unusual concentration of 23 QSOs at z=1.1 in 2001. The size of the complex of clusters may indicate a wall of galaxies exists there, instead of a single supercluster. The size discovered approaches the size of the CfA2 Great Wall filament. At the time of the discovery, it was the largest and most distant supercluster beyond z=0.5[21][22]
SCL @ 1604 43 at z=0.9 z=0.91 This supercluster at the time of its discovery was the largest supercluster found so deep into space, in 2000. It consisted of two known rich clusters and one newly discovered cluster as a result of the study that discovered it. The then known clusters were Cl 1604 4304 (z=0.897) and Cl 1604 4321 (z=0.924), which then known to have 21 and 42 known galaxies respectively. The then newly discovered cluster was located at 16h 04m 25.7s, 43° 14′ 44.7″[23]
SCL @ 0018 16 at z=0.54 in SA26 z=0.54 This supercluster lies around radio galaxy 54W084C (z=0.544) and is composed of at least three large clusters, CL 0016 16 (z=0.5455), RX J0018.3 1618 (z=0.5506), RX J0018.8 1602 .[24]
MS 0302 17

z=0.42

Length=6Mpc

This supercluster has at least three member clusters, the eastern cluster CL 0303 1706, southern cluster MS 0302 1659 and northern cluster MS 0302 1717.[25]

Diagram

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A diagram of Earth's location in the observable Universe and neighbouring superclusters of galaxies. (Alternative image.)

See also

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References

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  1. ^ Cain, Fraser (4 May 2009). "Local Group". Universe Today. Retrieved 6 December 2015.
  2. ^ a b Gibney, Elizabeth (2014-09-03). "Earth's new address: 'Solar System, Milky Way, Laniakea'". Nature. doi:10.1038/nature.2014.15819. ISSN 1476-4687. S2CID 124323774.
  3. ^ "The Universe within 14 billion Light Years". Atlas of the Universe. Retrieved 6 December 2015.
  4. ^ "An Intergalactic Heavyweight". ESO Picture of the Week. Retrieved 12 February 2013.
  5. ^ Abell, George O. (1958). "The distribution of rich clusters of galaxies. A catalogue of 2,712 rich clusters found on the National Geographic Society Palomar Observatory Sky Survey" (PDF). The Astrophysical Journal Supplement Series. 3: 211–288. Bibcode:1958ApJS....3..211A. doi:10.1086/190036.
  6. ^ Hu, F. X.; et al. (2006). "Orientation of Galaxies in the Local Supercluster: A Review". Astrophysics and Space Science. 302 (1–4): 43–59. arXiv:astro-ph/0508669. Bibcode:2006Ap&SS.302...43H. doi:10.1007/s10509-005-9006-7. S2CID 18837475.
  7. ^ Nurmi, P.; Heinamaki, P.; Martinez, V. J.; Einasto, J.; Enkvist, I.; Einasto, P.; Tago, E.; Saar, E.; Tempel, E. (2011-05-09). "The Sloan Great Wall. Morphology and galaxy content". The Astrophysical Journal. 736 (1): 51. arXiv:1105.1632. Bibcode:2011ApJ...736...51E. doi:10.1088/0004-637X/736/1/51. S2CID 119218634.
  8. ^ "Einasto Supercluster: the new heavyweight contender in the universe | Tartu Ülikool". ut.ee. 2024-02-19. Retrieved 2024-03-22.
  9. ^ Sankhyayan, Shishir; Bagchi, Joydeep; Tempel, Elmo; More, Surhud; Einasto, Maret; Dabhade, Pratik; Raychaudhury, Somak; Athreya, Ramana; Heinämäki, Pekka (2023). "Identification of Superclusters and Their Properties in the Sloan Digital Sky Survey Using the WHL Cluster Catalog". The Astrophysical Journal. 958 (1): 62. arXiv:2309.06251. Bibcode:2023ApJ...958...62S. doi:10.3847/1538-4357/acfaeb. ISSN 0004-637X.
  10. ^ Shimawaka, Rhythm; Okabe, Nobuhiro; Shirasaki, Masat; Tanaka, Masayuki (22 November 2022). "King Ghidorah Supercluster: Mapping the light and dark matter in a new supercluster at z = 0.55 using the subaru hyper suprime-cam". Monthly Notices of the Royal Astronomical Society: Letters. 519 (1): L45–L50. arXiv:2211.11970. Bibcode:2023MNRAS.519L..45S. doi:10.1093/mnrasl/slac150. ISSN 1745-3933. S2CID 253761264.
  11. ^ a b c Tully, R. Brent; Courtois, Helene; Hoffman, Yehuda; Pomarède, Daniel (2 September 2014). "The Laniakea supercluster of galaxies". Nature. 513 (7516) (published 4 September 2014): 71–73. arXiv:1409.0880. Bibcode:2014Natur.513...71T. doi:10.1038/nature13674. PMID 25186900. S2CID 205240232.
  12. ^ Mitra, Shyamal (1989). "A Study of the Southern Supercluster". The World of Galaxies. Springer, New York, NY. pp. 426–427. doi:10.1007/978-1-4613-9356-6_65. ISBN 978-1-4613-9358-0. Archived from the original on 9 June 2018. Retrieved 23 September 2020.
  13. ^ Hasegawa, T.; et al. (2000). "Large-scale structure of galaxies in the Ophiuchus region". Monthly Notices of the Royal Astronomical Society. 316 (2): 326–344. Bibcode:2000MNRAS.316..326H. doi:10.1046/j.1365-8711.2000.03531.x.
  14. ^ Postman, M.; Geller, M. J.; Huchra, J. P. (1988). "The dynamics of the Corona Borealis supercluster". Astronomical Journal. 95: 267–83. Bibcode:1988AJ.....95..267P. doi:10.1086/114635.
  15. ^ Miranda, Natalia A. Ramos (October 17, 2018), Scientists in Chile unveil 'A Cosmic Titan' cluster of galaxies, Reuters
  16. ^ Cucciati, O.; Lemaux, B. C.; Zamorani, G.; Le Fevre, O.; Tasca, L. A. M.; Hathi, N. P.; Lee, K-G.; Bardelli, S.; Cassata, P.; Garilli, B.; Le Brun, V.; Maccagni, D.; Pentericci, L.; Thomas, R.; Vanzella, E.; Zucca, E.; Lubin, L. M.; Amorin, R.; Cassara', L. P.; Cimatti, A.; Talia, M.; Vergani, D.; Koekemoer, A.; Pforr, J.; Salvato, M. (2018). "The progeny of a Cosmic Titan: a massive multi-component proto-supercluster in formation at z=2.45 in VUDS". Astronomy & Astrophysics. 619: A49. arXiv:1806.06073. Bibcode:2018A&A...619A..49C. doi:10.1051/0004-6361/201833655. S2CID 119472428.
  17. ^ Rosati, P.; et al. (1999). "An X-Ray-Selected Galaxy Cluster at z = 1.26". The Astronomical Journal. 118 (1): 76–85. arXiv:astro-ph/9903381. Bibcode:1999AJ....118...76R. doi:10.1086/300934. S2CID 2560006.
  18. ^ "Lynx Supercluster". SIMBAD.
  19. ^ Nakata, F.; et al. (2004). "Discovery of a large-scale clumpy structure of the Lynx supercluster at z∼1.27". Proceedings of the International Astronomical Union. 2004. Cambridge University Press: 29–33. Bibcode:2004ogci.conf...29N. doi:10.1017/S1743921304000080 (inactive 1 November 2024). ISBN 0-521-84908-X.{{cite journal}}: CS1 maint: DOI inactive as of November 2024 (link)
  20. ^ Ohta, K.; et al. (2003). "Optical Identification of the ASCA Lynx Deep Survey: An Association of Quasi-Stellar Objects and a Supercluster at z = 1.3?". The Astrophysical Journal. 598 (1): 210–215. arXiv:astro-ph/0308066. Bibcode:2003ApJ...598..210O. doi:10.1086/378690. S2CID 117171639.
  21. ^ Tanaka, I. (2004). "Subaru Observation of a Supercluster of Galaxies and QSOS at Z = 1.1". Studies of Galaxies in the Young Universe with New Generation Telescope, Proceedings of Japan-German Seminar, held in Sendai, Japan, July 24–28, 2001. pp. 61–64. Bibcode:2004sgyu.conf...61T.
  22. ^ Tanaka, I.; Yamada, T.; Turner, E. L.; Suto, Y. (2001). "Superclustering of Faint Galaxies in the Field of a QSO Concentration at z ~ 1.1". The Astrophysical Journal. 547 (2): 521–530. arXiv:astro-ph/0009229. Bibcode:2001ApJ...547..521T. doi:10.1086/318430. S2CID 119439816.
  23. ^ Lubin, L. M.; et al. (2000). "A Definitive Optical Detection of a Supercluster at z ≈ 0.91". The Astrophysical Journal. 531 (1): L5–L8. arXiv:astro-ph/0001166. Bibcode:2000ApJ...531L...5L. doi:10.1086/312518. PMID 10673401. S2CID 14588174.
  24. ^ Connolly, A. J.; et al. (1996). "Superclustering at Redshift z = 0.54". The Astrophysical Journal Letters. 473 (2): L67–L70. arXiv:astro-ph/9610047. Bibcode:1996ApJ...473L..67C. doi:10.1086/310395. S2CID 17697662.
  25. ^ University of Hawaii, "The MS0302 17 Supercluster", Nick Kaiser. Retrieved 15 September 2009.
  • Freedman, Roger; Gellar, Robert M.; Kaufmann, William III (2015). "Galaxies". Universe (10th ed.). New York: W.H. Freedman. ISBN 978-1-319-04238-7.
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