Supercluster

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 most of them, unlike clusters, expand with the Hubble expansion. The number of superclusters in the observable universe is estimated to be 10 million.[3]

## Contents

* 1 Existence
* 2 List of superclusters
* 2.1 Nearby superclusters
* 2.2 Distant superclusters
* 2.3 Extremely distant superclusters
* 3 Diagram
* 4 See also
* 5 References
* 6 Further reading
* 7 External links

## Existence

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", "hyperclusters",[6] "chains", "strands", "superstructures",[7] "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.[8]

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.[9]

## List of superclusters

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.[10][11]
King Ghidorah Supercluster  |

* z = 0.50-0.64
* Mass = 1 × 1016 solar masses

| The most massive galaxy supercluster discovered until 2023.[12]
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.[13]

Hydra–Centaurus Supercluster |  | SCl 128 \- 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.[13]

Pavo–Indus Supercluster |  |

In 2014, the newly announced Laniakea Supercluster subsumed the Pavo-Indus Supercluster, which became a component of the new supercluster.[13]

Southern Supercluster |  |

Includes Fornax Cluster (S373), Dorado and Eridanus clouds.[14]

Saraswati Supercluster | Distance = 4 billion 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 × 1016 M☉ and is seen in the Pisces constellation

### Nearby superclusters

Galaxy supercluster  | Data  | Notes

|
|

Perseus–Pisces Supercluster |  | SCl 40
Coma Supercluster |  | SCl 117 \- 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=8500–9000 km/s (centre)
* 18 Mpc × 26 Mpc

| (no SCl number) - 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.[15]
Shapley Supercluster |

* z=0.046.(650 Mly away)

| SCl 124 \- The second supercluster found, after the Local Supercluster.

### Distant superclusters

Galaxy supercluster  | Data  | Notes

|
|

Pisces–Cetus Supercluster  |  | SCl 10
Boötes Supercluster  |  | SCl 138
Horologium–Reticulum Supercluster  |

z=0.063 (700 Mly)
Length = 550 Mly
| SCl 48 \+ SCl 49
Corona Borealis Supercluster |

z=0.07[16]
| SCl 158
Columba Supercluster  |  | (no SCl number)
Aquarius Supercluster  |  | SCl 4
Aquarius B Supercluster  |  | SCl 193
Aquarius–Capricornus Supercluster  |  | SCl 189
Aquarius–Cetus Supercluster  |  | SCl 188
Bootes A Supercluster  |  | SCl 150
Caelum Supercluster  |

z=0.126 (1.4 Gly)
| SCl 59
Draco Supercluster |  | SCl 114
Draco–Ursa Major Supercluster  |  | SCl 257
Fornax–Eridanus Supercluster  |  | SCl 53
Grus Supercluster  |  | SCl 197
Leo A Supercluster  |  | SCl 100
Leo–Sextans Supercluster  |  | SCl 91
Leo–Virgo Supercluster  |  | SCl 107
Microscopium Supercluster |  | SCl 174
Pegasus–Pisces Supercluster  |  | SCl 3
Perseus–Pisces Supercluster |  | SCl 40
Pisces–Aries Supercluster  |  | SCl 30
Ursa Majoris Supercluster  |  | SCl 109
Virgo-Coma Supercluster  |  | SCl 111

### Extremely distant superclusters

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.[17][18]
Lynx Supercluster | z=1.27  | Discovered in 1999[19] (as ClG J0848+4453, a name now used to describe the western cluster, with ClG J0849+4452 being the eastern one),[20] 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.[21] Additionally, seven smaller groups of galaxies are associated with the supercluster.[22]
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[23][24]
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″[25]
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 .[26]
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.[27]

## Diagram

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

## See also

* Lists of astronomical objects
* List of largest cosmic structures
* Galaxy
* Galaxy groups and clusters
* Galaxy cluster
* Galaxy filament
* Galaxy group
* Illustris project
* Large-scale structure of the cosmos

## References

1. ↑ Cain, Fraser (4 May 2009). "Local Group". Universe Today. http://www.universetoday.com/30286/local-group/.
2. ↑ 2.0 2.1 Gibney, Elizabeth (2014-09-03). "Earth's new address: 'Solar System, Milky Way, Laniakea'" (in en). Nature. doi:10.1038/nature.2014.15819. ISSN 1476-4687. https://www.nature.com/articles/nature.2014.15819.
3. ↑ "The Universe within 14 billion Light Years". Atlas of the Universe. http://www.atlasoftheuniverse.com/universe.html.
4. ↑ "An Intergalactic Heavyweight". ESO Picture of the Week. http://www.eso.org/public/images/potw1304a/.
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". The Astrophysical Journal Supplement Series 3: 211–288. doi:10.1086/190036. Bibcode: 1958ApJS....3..211A. https://thesis.library.caltech.edu/1581/1/Abell_go_1957.pdf.
6. ↑ "One of the most distant, massive "hypercluster" of galaxies has been discovered". 15 March 2016. https://www.iac.es/en/outreach/news/one-most-distant-massive-hypercluster-galaxies-has-been-discovered.
7. ↑ Einasto, Maret (2025). "Galaxy Superclusters and Their Complexes in the Cosmic Web". Universe 11 (6): 167. doi:10.3390/universe11060167. Bibcode: 2025Univ...11..167E.
8. ↑ Hu, F. X. (2006). "Orientation of Galaxies in the Local Supercluster: A Review". Astrophysics and Space Science 302 (1–4): 43–59. doi:10.1007/s10509-005-9006-7. Bibcode: 2006Ap&SS.302...43H.
9. ↑ Nurmi, P.; Heinamaki, P.; Martinez, V. J.; Einasto, J.; Enkvist, I.; Einasto, P.; Tago, E.; Saar, E. et al. (2011-05-09). "The Sloan Great Wall. Morphology and galaxy content" (in en). The Astrophysical Journal 736 (1): 51. doi:10.1088/0004-637X/736/1/51. Bibcode: 2011ApJ...736...51E.
10. ↑ "Einasto Supercluster: the new heavyweight contender in the universe | Tartu Ülikool" (in en). 2024-02-19. https://ut.ee/en/content/einasto-supercluster-new-heavyweight-contender-universe.
11. ↑ Sankhyayan, Shishir; Bagchi, Joydeep; Tempel, Elmo; More, Surhud; Einasto, Maret; Dabhade, Pratik; Raychaudhury, Somak; Athreya, Ramana et al. (2023). "Identification of Superclusters and Their Properties in the Sloan Digital Sky Survey Using the WHL Cluster Catalog" (in en). The Astrophysical Journal 958 (1): 62. doi:10.3847/1538-4357/acfaeb. ISSN 0004-637X. Bibcode: 2023ApJ...958...62S.
12. ↑ 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. doi:10.1093/mnrasl/slac150. ISSN 1745-3933. Bibcode: 2023MNRAS.519L..45S. https://academic.oup.com/mnrasl/article-abstract/519/1/L45/6847752?redirectedFrom=fulltext.
13. ↑ 13.0 13.1 13.2 Tully, R. Brent; Courtois, Helene; Hoffman, Yehuda; Pomarède, Daniel (2 September 2014). "The Laniakea supercluster of galaxies". Nature 513 (7516): 71–73. 4 September 2014. doi:10.1038/nature13674. PMID 25186900. Bibcode: 2014Natur.513...71T.
14. ↑ Mitra, Shyamal (1989). "A Study of the Southern Supercluster". The World of Galaxies. New York: Springer. pp. 426–427. doi:10.1007/978-1-4613-9356-6_65. ISBN 1-4613-9358-2. https://link.springer.com/chapter/10.1007/978-1-4613-9356-6_65. Retrieved 23 September 2020.
15. ↑ Hasegawa, T. (2000). "Large-scale structure of galaxies in the Ophiuchus region". Monthly Notices of the Royal Astronomical Society 316 (2): 326–344. doi:10.1046/j.1365-8711.2000.03531.x. Bibcode: 2000MNRAS.316..326H.
16. ↑ Postman, M.; Geller, M. J.; Huchra, J. P. (1988). "The dynamics of the Corona Borealis supercluster". Astronomical Journal 95: 267–83. doi:10.1086/114635. Bibcode: 1988AJ.....95..267P.
17. ↑ Ramos Miranda, Natalia A. (October 17, 2018), Scientists in Chile unveil 'A Cosmic Titan' cluster of galaxies, Reuters, https://www.reuters.com/article/us-space-galaxy/scientists-in-chile-unveil-a-cosmic-titan-cluster-of-galaxies-idUSKCN1MR2RS
18. ↑ Cucciati, O.; Lemaux, B. C.; Zamorani, G.; Le Fevre, O.; Tasca, L. A. M.; Hathi, N. P.; Lee, K-G.; Bardelli, S. et al. (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. doi:10.1051/0004-6361/201833655. Bibcode: 2018A&A...619A..49C.
19. ↑ Rosati, P. (1999). "An X-Ray-Selected Galaxy Cluster at z = 1.26". The Astronomical Journal 118 (1): 76–85. doi:10.1086/300934. Bibcode: 1999AJ....118...76R.
20. ↑ "Lynx Supercluster". SIMBAD. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NAME LYNX SUPERCLUSTER.
21. ↑ Nakata, F. (2004). "Discovery of a large-scale clumpy structure of the Lynx supercluster at z∼1.27". Proceedings of the International Astronomical Union (Cambridge University Press) 2004: 29–33. doi:10.1017/S1743921304000080. ISBN 0-521-84908-X. Bibcode: 2004ogci.conf...29N.
22. ↑ Ohta, K. (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. doi:10.1086/378690. Bibcode: 2003ApJ...598..210O.
23. ↑ Tanaka, I. (2004). "Subaru Observation of a Supercluster of Galaxies and QSOS at Z = 1.1". pp. 61–64. Bibcode: 2004sgyu.conf...61T.
24. ↑ 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. doi:10.1086/318430. Bibcode: 2001ApJ...547..521T.
25. ↑ Lubin, L. M. (2000). "A Definitive Optical Detection of a Supercluster at z ≈ 0.91". The Astrophysical Journal 531 (1): L5–L8. doi:10.1086/312518. PMID 10673401. Bibcode: 2000ApJ...531L...5L.
26. ↑ Connolly, A. J. (1996). "Superclustering at Redshift z = 0.54". The Astrophysical Journal Letters 473 (2): L67–L70. doi:10.1086/310395. Bibcode: 1996ApJ...473L..67C.
27. ↑ University of Hawaii, "The MS0302+17 Supercluster", Nick Kaiser. Retrieved 15 September 2009.

## Further reading

* Freedman, Roger; Gellar, Robert M.; Kaufmann, William III (2015). "Galaxies". Universe (10th ed.). New York: W. H. Freedman. ISBN 978-1-319-04238-7.

## External links

* Overview of local superclusters
* The Nearest Superclusters
* Universe family tree: Supercluster

* v
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Galaxies

Morphology|

* Disc
* Lenticular
* barred
* unbarred
* Spiral
* anemic
* barred
* flocculent
* grand design
* intermediate
* Magellanic
* unbarred
* Dwarf galaxy
* elliptical
* irregular
* spheroidal
* spiral
* Elliptical galaxy
* cD
* Irregular
* barred
* Peculiar
* Ring
* Polar

Structure|

* Active galactic nucleus
* Bar
* Bulge
* Dark matter halo
* Disc
* Disc galaxy
* Halo
* corona
* Galactic center
* Galactic plane
* Galactic ridge
* Interstellar medium
* Protogalaxy
* Spiral arm
* Supermassive black hole

Active nuclei|

* Blazar
* LINER
* Markarian
* Quasar
* Radio
* X-shaped
* Relativistic jet
* Seyfert

Energetic galaxies|

* Lyman-alpha emitter
* Luminous infrared
* Starburst
* blue compact dwarf
* pea
* faint blue
* Hot dust-obscured

Low activity|

* Low surface brightness
* Ultra diffuse
* Dark galaxy

Interaction|

* Field
* Galactic tide
* Cloud
* Groups and clusters
* group
* cluster
* Brightest cluster galaxy
* fossile group
* Interacting
* merger
* Jellyfish
* Satellite
* Stellar stream
* Superclusters
* Walls
* Voids and supervoids
* void galaxy

Lists|

* Galaxies
* Galaxies named after people
* Largest
* Nearest
* Polar-ring
* Ring
* Spiral
* Groups and clusters
* Large quasar groups
* Quasars

* Superclusters
* Voids

See also|

* Extragalactic astronomy
* Galactic astronomy
* Galactic coordinate system
* Galactic empire
* Galactic habitable zone
* Galactic magnetic fields
* Galactic orientation
* Galactic quadrant
* Galaxy color–magnitude diagram
* Galaxy formation and evolution
* Galaxy rotation curve
* Illustris project
* Intergalactic dust
* Intergalactic stars
* Intergalactic travel
* Population III stars

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