Astrophysics (Index)About

supercluster

(cluster of galaxy clusters)

A supercluster is a cluster of galaxy groups and clusters. Typical size is several hundred million light-years across, and some 1017 solar masses.

Whether a given supercluster is gravitationally bound is often a subject of repeated analysis, often concluding that particular superclusters are not. Given that, the term indicates "a grouping of clusters, which may or may not be gravitationally bound", which some consider to be of little use, though it is accepted that galaxy clusters are generally gathered in groups rather than spread randomly. A level up from superclusters are galaxy filaments, galaxy walls or galaxy sheets, and supercluster complexes.

The term Local Supercluster has long been used for the Virgo Supercluster, which includes the Local Group (with the Milky Way) as well as the Virgo Cluster and is thought to contain 47,000 galaxies. Laniakea Supercluster has been declared a larger supercluster that includes the Virgo Supercluster, so the term Local Supercluster could be used to mean it instead.


(large scale structures,object type)
Further reading:
https://en.wikipedia.org/wiki/Supercluster
http://www.icc.dur.ac.uk/~tt/Lectures/Galaxies/LocalGroup/Back/nearsc.html
https://dictionary.obspm.fr/index.php?showAll=1&formSearchTextfield=supercluster
PrefixExample  
SClSCl 117general

Referenced by pages:
astronomical quantities
Coma Supercluster
dark matter (DM)
galaxy cloud
galaxy cluster (CL)
galaxy filament
gravitationally bound
Great Attractor
Great Wall
Hydra-Centaurus Supercluster
Laniakea Supercluster
large scale structure (LSS)
Local Group (LG)
Perseus-Pisces Supercluster
Pisces-Cetus Supercluster Complex
Sloan Great Wall (SGW)
velocity dispersion (σ)
Virgo Supercluster
Zel'dovich approximation

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