Local Supercluster

GPTKB entity

Statements (122)
Predicate Object
gptkbp:instance_of gptkb:microprocessor
gptkbp:bfsLayer 3
gptkbp:bfsParent gptkb:Milky_Way
gptkbp:applies_to the study of dark energy
gptkbp:contains gptkb:Virgo_Cluster
gptkb:Coma_Cluster
gptkb:Triangulum_Galaxy
gptkb:Andromeda_Galaxy
gptkb:Hercules_Cluster
gptkb:Centaurus_Cluster
gptkb:Milky_Way_Galaxy
gptkbp:depicted_in gptkb:physicist
gptkbp:diameter approximately 10 million light-years
gptkbp:discovered_by the 20th century
gptkbp:focuses_on multi-wavelength observations
astronomical research
theoretical astrophysics research
gptkbp:governed_by gptkb:Virgo_Cluster
https://www.w3.org/2000/01/rdf-schema#label Local Supercluster
gptkbp:ingredients around 1000 galaxies
gptkbp:is_a_center_for gptkb:Virgo_Cluster
gptkbp:is_a_site_for star formation
galactic mergers
intense gravitational interactions
gptkbp:is_affected_by cosmic microwave background radiation
cosmic expansion
gptkbp:is_analyzed_in gravitational lensing
gptkbp:is_approximately 10 million light-years in diameter
110 million light-years from Earth
1.5 billion light-years from the center of the Laniakea Supercluster
gptkbp:is_associated_with gptkb:nebula
large-scale cosmic flows
gptkbp:is_characterized_by large-scale structure of the universe
galaxy interactions
galaxy clusters and groups
galaxy clustering patterns
galaxy density variations
galaxy morphology diversity
galaxy redshift distributions
gptkbp:is_connected_to the Shapley Supercluster
other superclusters
other superclusters through filaments
the Bootes Supercluster
the Coma Supercluster
the Hercules Supercluster
the Perseus-Pisces Supercluster
the Pisces-Perseus Supercluster
gptkbp:is_described_as cosmological models
gptkbp:is_essential_for galaxy formation theories
gptkbp:is_explored_in observational astronomy
gptkbp:is_home_to gptkb:the_Sculptor_Group
gptkb:the_Local_Group
over 100 galaxy groups and clusters
many galaxy clusters
the Centaurus Cluster
the Fornax Cluster
the Leo Cluster
gptkbp:is_influenced_by gptkb:Monarch
gptkb:nebula
the expansion of the universe
large-scale cosmic flows
cosmic expansion
the cosmic background radiation
local gravitational effects
gptkbp:is_involved_in galactic interactions
gptkbp:is_known_for gptkb:Virgo_Supercluster
gptkbp:is_located_near gptkb:the_Great_Attractor
gptkbp:is_observed_in X-ray wavelengths
radio wavelengths
various wavelengths of light
gptkbp:is_part_of gptkb:Laniakea_Supercluster
gptkb:the_Local_Group
the Virgo Supercluster
the observable universe
the cosmic web
the universe's large-scale structure
the larger structure of the universe
the large-scale structure of the cosmos
the cosmic web structure
the cosmic structure of the universe
the observable universe's structure
gptkbp:is_studied_in gptkb:spacecraft
gptkb:observatory
astrophysics
understanding cosmic evolution
galaxy formation and evolution
galaxy dynamics
gptkbp:is_subject_to gravitational forces
gptkbp:is_surrounded_by voids
cosmic voids
intergalactic space
gptkbp:key observational astronomy
gptkbp:located_in gptkb:Virgo_constellation
gptkb:supernova_remnants
observable universe
various astronomical phenomena
gptkbp:map gptkb:observatory
galaxy redshift surveys
3 D galaxy surveys
astronomical surveys.
gptkbp:named_after the Virgo constellation
gptkbp:notable_feature the universe's structure
gptkbp:region gptkb:active_galactic_nuclei
high galaxy density
varied galaxy types
contains many bright galaxies
cosmic microwave background radiation is studied
galaxies collide
galaxy clusters are studied
hosts various galaxy clusters
is crucial for understanding dark matter effects
is explored through simulations.
is important for cosmological models
is mapped by telescopes
is rich in galaxy diversity
gptkbp:significance the study of galaxy evolution
understanding cosmic history
understanding large-scale structure of the universe
gptkbp:subject astrophysical simulations
theories of cosmic evolution
gptkbp:surface other superclusters
gptkbp:targets future astronomical surveys