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Virgo Supercluster

formerly defined galactic supercluster containing the Virgo Cluster and the Local Group

Key facts

Constellation s: Virgo & Coma Berenices ( Virgo Cluster )
Right ascension: 12 31
Declination: +12 ° 24 ′
Number of galaxies: 47,000+
Parent structure: Laniakea Supercluster
Major axis: 147 Mly (45 Mpc )
Minor axis: ≈26.1 Mly (8 Mpc )
Redshift: Doppler shift
Distance: 55.62 ± 8.395 Mly (17.053 ± 2.574 Mpc ) ( Virgo Cluster )
Binding mass: ~ 1.48 × 10 M ☉
Luminosity specify: 3 × 10 L ☉ (total)

via Wikipedia infobox

Article

The Virgo Supercluster (Virgo SC) or Local Supercluster (LSC or LS) is a supercluster of galaxies containing the Virgo Cluster and Local Group. The latter contains the Milky Way and Andromeda galaxies, among others. The Virgo Supercluster is roughly centered on the Virgo Cluster, with the Local Group located near one edge and revolving around its center.

At least 100 galaxy groups and clusters are located within the supercluster diameter of 45 megaparsecs (147 million light-years; 1.39×10 kilometres). The Virgo Supercluster is one of about 10 million superclusters in the observable universe, with the main body of the supercluster, the Virgo Strand, connecting the Hydra-Centaurus and the Perseus–Pisces Superclusters. It is part of the Pisces–Cetus Supercluster Complex, a very large galaxy filament.