Leo B

E496039

Leo B is a faint dwarf spheroidal galaxy in the constellation Leo and a satellite of the Milky Way, notable for its low luminosity and dark-matter dominance.

All labels observed (1)

Label Occurrences
Leo B canonical 2

How this entity was disambiguated

Statements (25)

Predicate Object
instanceOf dwarf spheroidal galaxy
belongsToGalaxyGroup Local Group
constellation Leo
darkMatterContent dark-matter dominated
discoveryMethod deep imaging surveys
galaxyType dwarf spheroidal
hasProperty gas-poor
high mass-to-light ratio
low stellar mass
low surface brightness
hasStellarPopulation metal-poor stars
old stars
hostGalaxy Milky Way
isGravitationallyBoundTo Milky Way
isNearbyGalaxy true
isPartOf Local Group dwarf galaxies
Milky Way satellite system
isSatelliteOf Milky Way
luminosityCharacteristic low luminosity
morphologicalClass dSph
scientificInterest dark matter studies
evolution of dwarf spheroidal galaxies
galaxy formation in low-mass halos
skyLocation northern celestial hemisphere
visibility faint

How these facts were elicited

Referenced by (2)

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

Leo II otherName Leo B