Canes Venatici I Dwarf Galaxy

E486514

Canes Venatici I Dwarf Galaxy is a faint dwarf spheroidal satellite galaxy of the Milky Way located in the constellation Canes Venatici.

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Statements (31)

Predicate Object
instanceOf dwarf spheroidal galaxy
galaxy
satellite galaxy of the Milky Way
absoluteMagnitudeV about −8.6
apparentMagnitudeV ~13.9
belongsTo Local Group NERFINISHED
constellation Canes Venatici NERFINISHED
containsDarkMatter true
declination +33° 33′
discoveredBy Beth Willman NERFINISHED
discoveryMethod Sloan Digital Sky Survey NERFINISHED
discoveryYear 2006
distanceFromEarth ~220 kiloparsecs
~720,000 light-years
galaxyType dwarf spheroidal
halfLightRadius ~550 parsecs
hostGalaxy Milky Way NERFINISHED
isFaint true
isSatelliteOf Milky Way NERFINISHED
luminosity ~2×10^5 times the luminosity of the Sun
massToLightRatio >100 (in solar units)
memberOf Milky Way satellite system
metallicity very metal-poor
otherName CVn I dSph NERFINISHED
Canes Venatici I NERFINISHED
radialVelocity ~31 km/s
rightAscension ~13h 28m
shape spheroidal
starFormationActivity no current star formation
stellarPopulation old
surfaceBrightness very low

Referenced by (1)

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

Milky Way subgroup hasMember Canes Venatici I Dwarf Galaxy