Product Code Database
A supercluster is a large group of smaller or ; 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. 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.
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.
Superclusters form massive structures of galaxies, called galaxy filament, "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.
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.
| Einasto Supercluster |
| |
| King Ghidorah Supercluster |
| |
| Laniakea Supercluster |
| |
| Virgo Supercluster |
A 2014 study indicates that the Virgo Supercluster is only a lobe of an even greater supercluster, Laniakea. | |
| 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
In 2014, the newly announced Laniakea Supercluster subsumed the Hydra-Centaurus Supercluster, which became a component of the new supercluster. | |
| Pavo–Indus Supercluster | In 2014, the newly announced Laniakea Supercluster subsumed the Pavo-Indus Supercluster, which became a component of the new supercluster. | |
| Southern Supercluster | Includes Fornax Cluster (S373), Dorado and Eridanus Cluster clouds. | |
| Saraswati Supercluster | Distance = 4 billion light years (1.2 Gigaparsec) Length = 652 Million light-years | The Saraswati Supercluster consists of 43 massive galaxy clusters such as Abell 2361 and has a mass of about and is seen in the Pisces constellation |
| 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 |
| |
| Shapley Supercluster |
|
| Pisces–Cetus Supercluster | SCl 10 | |
| Boötes Supercluster | SCl 138 | |
| Horologium–Reticulum Supercluster |
| |
| Corona Borealis Supercluster |
| |
| 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 |
| |
| 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 |
| Hyperion proto-supercluster | Redshift=2.45 | This supercluster at the time of its discovery in 2018 was the earliest and largest proto-supercluster found to date. | |
| Lynx Supercluster | Redshift=1.27 | Discovered in 1999
(as ClG J0848+4453, a name now used to describe the western cluster, with ClG J0849+4452 being the eastern one),
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.
Nakata, F. (2025). 052184908X, Cambridge University Press. 052184908X Additionally, seven smaller groups of galaxies are associated with the supercluster.
| |
| SCL @ 1338+27 at z=1.1 | Redshift=1.1
Length=70Mpc A rich supercluster with several galaxy clusters was discovered around an unusual concentration of 23 quasar at z=1.1 in 2001. The size of the complex of clusters may indicate a galaxy filament 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 | ||
| SCL @ 1604+43 at z=0.9 | Redshift=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 , | |
| SCL @ 0018+16 at z=0.54 in SA26 | Redshift=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 . | |
| MS 0302+17 | Redshift=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.University of Hawaii, "The MS0302+17 Supercluster", Nick Kaiser. Retrieved 15 September 2009. | ||
|
|
