Hydra–Centaurus Supercluster

E123841

The Hydra–Centaurus Supercluster is a massive nearby concentration of galaxy clusters that forms one of the dominant structures in our cosmic neighborhood and serves as a major component of the larger Laniakea Supercluster.

All labels observed (6)

How this entity was disambiguated

Statements (44)

Predicate Object
instanceOf galaxy supercluster
large-scale structure of the Universe
alsoKnownAs Hydra–Centaurus
Hydra–Centaurus Supercluster
surface form: Hydra–Centaurus complex
connectedTo Pavo–Indus–Telescopium supercluster region
Shapley Supercluster via large-scale filaments
contains Abell 1060
Abell 3526
Abell 3627
Centaurus Cluster
Centaurus Wall
Hydra–Centaurus Supercluster self-linksurface differs
surface form: Great Attractor mass concentration

Hydra Cluster
Hydra Wall
Norma Cluster
Pavo–Indus filament
coordinateSystem described in supergalactic coordinates
cosmologicalContext used to study large-scale structure formation
used to study peculiar velocity fields in the local Universe
discoveredBy extragalactic astronomers in late 20th century
distanceFromEarth approximately 150–200 million light-years
environment overdense region relative to cosmic mean matter density
hasGravitationalEffectOn nearby galaxy flows within Laniakea
hasRole major mass concentration influencing local galaxy motions
hasSignificance dominant overdensity in the local Universe
key anchor of the Laniakea Supercluster definition
hasSubstructure galaxy groups and filaments
multiple Abell galaxy clusters
influences motion of the Milky Way
peculiar velocities of galaxies in the Local Group
isComponentOf gravitational basin of Laniakea Supercluster
isDynamicallyConnectedTo Great Attractor region
isNeighborOf Pavo–Indus–Telescopium supercluster region
surface form: Pavo–Indus Supercluster region

Virgo Supercluster
surface form: Virgo Supercluster region
isPartOf cosmic web
locatedIn constellation Centaurus
constellation Hydra
local cosmic neighborhood
nearby Universe
mass on the order of 10^16 solar masses (approximate)
partOf Laniakea Supercluster
redshift approximately 0.01–0.03
studiedUsing X-ray observations of galaxy clusters
redshift surveys

How these facts were elicited

Referenced by (6)

Full triples — surface form annotated when it differs from this entity's canonical label.

Laniakea Supercluster contains Hydra–Centaurus Supercluster
Laniakea Supercluster contains Hydra–Centaurus Supercluster
this entity surface form: Great Attractor region
Laniakea Supercluster centerOfMassRegion Hydra–Centaurus Supercluster
this entity surface form: Great Attractor
Laniakea Supercluster includes Hydra–Centaurus Supercluster
this entity surface form: Pavo–Indus filament
Hydra–Centaurus Supercluster alsoKnownAs Hydra–Centaurus Supercluster
this entity surface form: Hydra–Centaurus complex
Hydra–Centaurus Supercluster contains Hydra–Centaurus Supercluster self-linksurface differs
this entity surface form: Great Attractor mass concentration