UGC 426

E459105

UGC 426 is a dwarf elliptical satellite galaxy of the Andromeda Galaxy, more commonly known as Messier 110 (M110).

All labels observed (1)

Label Occurrences
UGC 426 canonical 3

How this entity was disambiguated

Statements (48)

Predicate Object
instanceOf astronomical object
dwarf elliptical galaxy
satellite galaxy
absoluteMagnitudeV approximately -16.5
alternateName M110
Messier 110
NGC 205
angularSize approximately 21 arcminutes by 11 arcminutes
apparentMagnitudeV approximately 8.9
bestSeenIn small telescopes
catalog Messier catalogue
NGC
PGC
UGC
contains dust lanes
gas
globular clusters
declination +41° 41′ 07″
discoveredBy Giovanni Battista Hodierna
discoveryYear before 1654
distanceFromEarth approximately 0.83 megaparsecs
approximately 2.7 million light-years
hasEnvironment dense tidal field of Andromeda Galaxy
hasMessierNumber M110
hasNGCNumber NGC 205
hasNucleus central stellar concentration
hasPGCNumber PGC 2557
hasStarFormation low current star formation rate
hasStellarPopulation intermediate-age stars
old stars
isBrighterThan most dwarf spheroidal satellites of Andromeda
isCompanionOf Andromeda Galaxy
isOneOf brightest dwarf companions of Andromeda Galaxy
isVisibleFrom Northern Hemisphere
locatedIn constellation Andromeda
mass on the order of 10^9 solar masses
memberOf Local Group
morphologicalType dE5
orbitsWithin Andromeda subgroup of the Local Group
linked to: Andromeda subgroup
radialVelocity approximately -241 km/s
recoveredBy Charles Messier
recoveryYear 1773
redshift approximately -0.000804
rightAscension 00h 40m 22s
satelliteOf Andromeda Galaxy
Messier 31
linked to: Andromeda Galaxy
showsEvidenceOf tidal interaction with Andromeda Galaxy
surfaceBrightness low

How these facts were elicited

Referenced by (3)

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

M110 catalogueDesignation UGC 426
NGC 205 alsoKnownAs UGC 426
Messier 110 alsoKnownAs UGC 426