Canes Venatici II Galaxy

GPTKB entity

Statements (54)
Predicate Object
gptkbp:instance_of gptkb:galaxy
gptkbp:contains_star yes
ongoing
gptkbp:diameter about 1,000 light-years
gptkbp:discovered_by K. M. C. Lee
gptkbp:discovery_year gptkb:2006
gptkbp:distance_from_earth approximately 200,000 light-years
gptkbp:has_color B-V = 0.8
gptkbp:has_features irregular shape
gptkbp:has_luminosity low luminosity
https://www.w3.org/2000/01/rdf-schema#label Canes Venatici II Galaxy
gptkbp:included galaxy catalogs
gptkbp:investigates stellar populations
gptkbp:is_affected_by tidal interactions
gptkbp:is_analyzed_in stellar evolution
gptkbp:is_associated_with gptkb:Canes_Venatici_I_Galaxy
gptkbp:is_connected_to the Local Group of galaxies
other dwarf galaxies
gptkbp:is_considered_as a satellite galaxy
gptkbp:is_examined_in galactic dynamics
gptkbp:is_influenced_by gravitational forces
gptkbp:is_inhabited_by star clusters
gptkbp:is_known_for its low surface brightness
gptkbp:is_located_near Ursa Major constellation
gptkbp:is_noted_for its faintness
its irregular morphology
gptkbp:is_observed_in gptkb:Hubble_Space_Telescope
radio telescopes
infrared wavelengths
ground-based telescopes
gptkbp:is_part_of gptkb:Laniakea_Supercluster
gptkb:Ring_of_Honor
cosmic web
the Local Volume
the Milky Way's satellite system
the cosmic structure
Virgo III group
the Virgo cluster
gptkbp:is_related_to dwarf spheroidal galaxies
gptkbp:is_studied_for dark matter research
galaxy formation theories
gptkbp:is_studied_in astrophysics
galactic archaeology
gptkbp:is_visible_from no
gptkbp:lighting low
gptkbp:located_in Canes Venatici constellation
gptkbp:map galaxy surveys
gptkbp:mass old stars
approximately 10 million solar masses
gptkbp:metallicity low metallicity
gptkbp:part_of gptkb:Local_Group
gptkbp:redshift 0.0023
gptkbp:scientific_classification gptkb:spiral_galaxy
gptkbp:type gptkb:spiral_galaxy