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gptkbp:instance_of
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gptkb:Super_GT
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gptkbp:composed_of
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galaxies
galaxy clusters
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gptkbp:contains
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gptkb:NGC_1300
gptkb:NGC_1950
gptkb:NGC_1980
gptkb:Perseus_cluster
gptkb:NGC_1850
gptkb:NGC_1260
gptkb:NGC_1280
gptkb:NGC_1291
gptkb:NGC_1332
gptkb:NGC_1419
gptkb:NGC_1426
gptkb:NGC_1435
gptkb:NGC_1440
gptkb:NGC_1450
gptkb:NGC_1500
gptkb:NGC_1510
gptkb:NGC_1520
gptkb:NGC_1530
gptkb:NGC_1540
gptkb:NGC_1550
gptkb:NGC_1560
gptkb:NGC_1580
gptkb:NGC_1590
gptkb:NGC_1600
gptkb:NGC_1610
gptkb:NGC_1620
gptkb:NGC_1630
gptkb:NGC_1640
gptkb:NGC_1650
gptkb:NGC_1660
gptkb:NGC_1670
gptkb:NGC_1680
gptkb:NGC_1690
gptkb:NGC_1700
gptkb:NGC_1710
gptkb:NGC_1720
gptkb:NGC_1730
gptkb:NGC_1740
gptkb:NGC_1760
gptkb:NGC_1770
gptkb:NGC_1780
gptkb:NGC_1790
gptkb:NGC_1800
gptkb:NGC_1810
gptkb:NGC_1820
gptkb:NGC_1830
gptkb:NGC_1840
gptkb:NGC_1860
gptkb:NGC_1870
gptkb:NGC_1880
gptkb:NGC_1890
gptkb:NGC_1900
gptkb:NGC_1910
gptkb:NGC_1920
gptkb:NGC_1930
gptkb:NGC_1940
gptkb:NGC_1960
gptkb:NGC_1970
gptkb:Pisces_cluster
gptkb:NGC_1340
gptkb:NGC_1350
gptkb:NGC_1373
gptkb:NGC_1380
gptkb:NGC_1275
gptkb:NGC_1316
gptkb:NGC_1365
gptkb:NGC_1399
gptkb:NGC_1404
gptkb:NGC_1460
gptkb:NGC_1470
gptkb:NGC_1480
gptkb:NGC_1490
gptkb:NGC_1570
gptkb:NGC_1990
gptkb:NGC_2000
gptkb:Perseus_Cluster
gptkb:Pisces_Cluster
NGC 1750
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|
gptkbp:diameter
|
approximately 100 million light-years
|
|
gptkbp:discovered_by
|
gptkb:astronomy
|
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gptkbp:distance_from_earth
|
approximately 250 million light-years
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gptkbp:governed_by
|
galaxy clusters
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|
https://www.w3.org/2000/01/rdf-schema#label
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Perseus-Pisces supercluster
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gptkbp:is_affected_by
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cosmic expansion
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gptkbp:is_analyzed_in
|
computer simulations
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gptkbp:is_associated_with
|
galactic evolution
large-scale structure of the Universe
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|
gptkbp:is_characterized_by
|
intergalactic medium
high galaxy density
high velocity dispersions
large-scale gravitational interactions
|
|
gptkbp:is_connected_to
|
gptkb:the_Great_Attractor
other superclusters
other galaxy superclusters
the cosmic web structure
the structure of the universe.
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|
gptkbp:is_considered_as
|
a significant region of the Universe
|
|
gptkbp:is_documented_in
|
gptkb:literature
research papers
astronomical catalogs
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|
gptkbp:is_examined_in
|
observational astronomy
galaxy interactions
dark energy effects
|
|
gptkbp:is_explored_in
|
gptkb:cosmology
astrophysicists
space telescopes
telescopic observations
|
|
gptkbp:is_home_to
|
various astronomical phenomena
multiple galaxy types
various types of galaxies
many galaxies
|
|
gptkbp:is_influenced_by
|
gptkb:dark_matter
gravitational forces
baryonic matter
cosmic microwave background radiation
|
|
gptkbp:is_located_at
|
coordinates in the sky
|
|
gptkbp:is_notable_for
|
its rich galaxy clusters
its role in cosmic evolution
its gravitational lensing effects
|
|
gptkbp:is_noted_for
|
its large scale
|
|
gptkbp:is_observed_in
|
X-ray emissions
cluster dynamics
|
|
gptkbp:is_part_of
|
the Universe
the observable universe
the cosmic web
the large-scale structure of the cosmos
large-scale cosmic structures
the local supercluster complex
|
|
gptkbp:is_related_to
|
the Virgo Supercluster
|
|
gptkbp:is_studied_for
|
galaxy formation
its structure and dynamics
its formation history
|
|
gptkbp:is_studied_in
|
gptkb:astronomy
astrophysics
galaxy cluster research
|
|
gptkbp:is_visible_from
|
optical wavelengths
|
|
gptkbp:located_in
|
gptkb:Laniakea_Supercluster
|
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gptkbp:map
|
gptkb:astronomy
galaxy surveys
|
|
gptkbp:mass
|
over 10^15 solar masses
|
|
gptkbp:part_of
|
the observable universe
|
|
gptkbp:redshift
|
0.023
|