Leo Cloud
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Leo Cloud
The Leo II Groups, Leo II Cloud, or simply the Leo Cloud is a galaxy filament consisting of at least 18 galaxy groups. It is located approximately 86 Mly (26 Mpc) from the Solar System. The Leo Cloud in Supergalactic coordinate system, supergalactic SGY coordinates is physically behind the Virgo Cluster. Eventually, over the next Hubble time, the galaxy groups that make up the Leo II Cloud will infall and merge with the Virgo Cluster. The Leo Cloud, along with the Crater Cloud which contains the NGC 4038 Group, is actually the same branch of a larger galaxy filament that extends from the Centaurus Cluster through the Virgo Cluster and continues through the Ursa Major Cluster, known as the Virgo Strand. The Virgo Strand is the main component of the Virgo Supercluster and is made of two branches with the lower branch consisting of the Leo and Crater clouds, while the upper branch is known as the Virgo Southern Extension or Virgo II Groups. The Leo Cloud itself is actually compos ...
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Virgo Supercluster
The Local Supercluster (LSC or LS), or Virgo Supercluster is a formerly defined supercluster containing the Virgo Cluster and Local Group, which itself contains the Milky Way and Andromeda galaxies, as well as others. At least 100 galaxy groups and clusters are located within its diameter of 33 megaparsecs (110 million light-years). 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. The Virgo Supercluster is part of the Pisces–Cetus Supercluster Complex, a galaxy filament. A 2014 study indicates that the Local Supercluster is only a part of an even greater supercluster, Laniakea, a larger group centered on the Great Attractor, thus subsuming the former Virgo Supercluster under Laniakea. Background Beginning with the first large sample of nebulae published by William and John Herschel in 1863, it ...
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