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Virgo Supercluster

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The Virgo Supercluster or Local Supercluster is the supercluster of galaxies that contains the Local Group and with it our galaxy, the Milky Way. It has the pancake-like shape of a flattened disk, with a diameter of about 200 million light years. It contains about 100 groups and clusters of galaxies and is dominated by the Virgo cluster near its center. The Local Group is located near the edge and is drawn towards the Virgo cluster.

By tracking its gravitational effect on the movement of galaxies, one can estimate that the total mass of the Virgo Supercluster is about 1015 solar masses (2 × 1046 kg; see Orders of magnitude (mass)). As its luminosity is far too small for this number of stars, it is thought that a large part of its mass is dark matter.

The entire Virgo Supercluster is being pulled toward a gravitational anomaly known as the Great Attractor, which lies near the Norma cluster.

Clusters of the Virgo Supercluster

Sorted by the number of galaxies they contain with large apparent size:

External links

See also

[[http://encycl.opentopia.com/ edit]]Milky Way
Galactic Core: Center of the Milky Way
Spiral Arms: Carina Arm | Crux Arm | Cygnus Arm | Norma Arm | Orion Arm | Perseus Arm | Sagittarius Arm | Scutum Arm
Location: Universe | Virgo Supercluster | Local Group
Satellite galaxies: Canis Major Dwarf Galaxy | Carina Dwarf | Draco Dwarf | Fornax Dwarf | Large Magellanic Cloud | Leo I | Leo II | Sag DEG | Sculptor Dwarf Galaxy | Sextans Dwarf | Small Magellanic Cloud | Virgo Stellar Stream | Ursa Minor Dwarf

 


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