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Hydra–Centaurus Supercluster

The Hydra–Centaurus Supercluster (SCl 128), or the Hydra and Centaurus Superclusters, also known as Hydra–Centaurus concentration, was a previously defined supercluster in two parts, which prior to the identification of Laniakea Supercluster in 2014 is the closest neighbour of the former Virgo Supercluster. Its center is located about 39 Mpc (127 Mly)…

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Declination
−33° 18′ 00″
Distance
~39–69.4 Mpc (127–226 Mly)
Parent structure
Laniakea Supercluster
Redshift
0.016000 (4,797 km/s)
Right ascension
13h 14m 00.0s

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Hydra–Centaurus Supercluster

Nodes30
Edges29
Triples5
Avg. degree1.93
Density0.066667
Components1

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Hydra–Centaurus Supercluster

Top relations

Declination · 1
Hydra–Centaurus Supercluster → −33° 18′ 00″
Distance · 1
Hydra–Centaurus Supercluster → ~39–69.4 Mpc (127–226 Mly)
Parent structure · 1
Hydra–Centaurus Supercluster → Laniakea Supercluster
Redshift · 1
Hydra–Centaurus Supercluster → 0.016000 (4,797 km/s)
Right ascension · 1
Hydra–Centaurus Supercluster → 13h 14m 00.0s

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Important terminology

supercluster centaurus mpc filament laniakea mly hydra cluster wall known antlia clusters also puppis around distance part cloud pp 2014

Entity relationships Subject–Predicate–Object triples

SubjectPredicateObjectConfidenceSrc
Hydra–Centaurus SuperclusterDeclination−33° 18′ 00″1.00infobox
Hydra–Centaurus SuperclusterDistance~39–69.4 Mpc (127–226 Mly)1.00infobox
Hydra–Centaurus SuperclusterParent structureLaniakea Supercluster1.00infobox
Hydra–Centaurus SuperclusterRedshift0.016000 (4,797 km/s)1.00infobox
Hydra–Centaurus SuperclusterRight ascension13h 14m 00.0s1.00infobox

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