Cetus dSph

E563945

Cetus dSph is a faint dwarf spheroidal galaxy in the constellation Cetus that is a satellite of the Milky Way and notable for its old, metal-poor stellar population.

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Statements (44)

Predicate Object
instanceOf dwarf spheroidal galaxy
discoveredBy Alan Whiting NERFINISHED
George Hau NERFINISHED
Mike Irwin NERFINISHED
discoveryYear 1999
hasAbsoluteMagnitudeV ~−11.3
hasAlternativeName Cetus dSph galaxy NERFINISHED
Cetus dwarf
Cetus dwarf spheroidal galaxy NERFINISHED
hasApparentMagnitudeV ~14.5
hasCoordinateEpoch J2000
hasDarkMatterDominance high
hasDeclination −11°
hasDistanceFromEarth_ly ~2600000
hasDistanceFromMilkyWayCenter_ly ~2600000
hasDominantStellarPopulationAge_Gyr >10
hasEnvironment isolated Milky Way satellite
hasGalaxyColor red
hasGalaxyMorphologicalType dSph
hasGalaxyType early-type dwarf
hasGasContent gas-poor
hasGlobularClusters none known
hasHalfLightRadius_pc ~300
hasHeliocentricRadialVelocity_km_s ~−87
hasKinematicProperty pressure-supported
hasLuminosityClass dwarf
hasMetallicity_Fe_H ~−1.9
hasNeutralHydrogenContent very low
hasObservationWavelength near-infrared
optical
hasRightAscension 00h 26m
hasShape spheroidal
hasStarFormationActivity quiescent
hasStarFormationHistory early burst followed by long quiescence
hasStellarPopulation metal-poor
old
hasStellarPopulationGradient present
hasSurfaceBrightness low
locatedInConstellation Cetus NERFINISHED
memberOf Local Group NERFINISHED
satelliteOf Milky Way NERFINISHED
studiedFor ancient stellar populations
dark matter content in dwarf spheroidals
dwarf galaxy evolution

Referenced by (1)

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