NGC 5102

E501818

NGC 5102 is a lenticular galaxy in the constellation Centaurus, notable for its relatively nearby distance and membership in the Centaurus A/M83 galaxy group.

All labels observed (1)

Label Occurrences
NGC 5102 canonical 1

How this entity was disambiguated

Statements (49)

Predicate Object
instanceOf galaxy ⓘ
lenticular galaxy ⓘ
absoluteMagnitudeV ~−18 ⓘ
angularSize ~8.7 × 2.8 arcmin ⓘ
apparentMagnitudeB ~10.4 ⓘ
apparentMagnitudeV ~9.9 ⓘ
bulge prominent bulge ⓘ
catalog New General Catalogue ⓘ
color overall blue-green visual appearance in images ⓘ
constellation Centaurus ⓘ
coordinateSystem equatorial coordinate system (J2000) ⓘ
declination −36° 38′ (approx) ⓘ
discovery discovered in the 19th century ⓘ
discoveryCataloger John Louis Emil Dreyer (cataloged in NGC) ⓘ
disk lens-like stellar disk ⓘ
distanceFromEarth ~11 Mly ⓘ
~3.3 Mpc ⓘ
dustContent contains some dust lanes and patches ⓘ
environment member of a loose galaxy group environment ⓘ
galaxyGroup Centaurus A Group ⓘ
Centaurus A/M83 Group ⓘ
gasContent relatively gas-poor ⓘ
groupDominantGalaxy Centaurus A (NGC 5128) ⓘ
linked to: NGC 5128
hemisphere southern celestial hemisphere ⓘ
HIContent contains relatively little neutral hydrogen ⓘ
HubbleSequencePosition early-type disk galaxy ⓘ
interactionStatus no strong current tidal interaction signatures ⓘ
locationRelativeToMilkyWay in the nearby universe outside the Local Group ⓘ
majorAxisAngularSize ~8.7 arcmin ⓘ
mass on the order of 10^10 solar masses ⓘ
minorAxisAngularSize ~2.8 arcmin ⓘ
morphologicalType S0 ⓘ
SA0- ⓘ
NGCNumber 5102 ⓘ
nucleus hosts a compact nuclear region ⓘ
otherDesignation ESO 270-17 ⓘ
HIPASS J1321-36 ⓘ
PGC 46668 ⓘ
radialVelocity ~468 km/s ⓘ
redshift ~0.0009 ⓘ
researchUse used as a laboratory for studying lenticular galaxy evolution ⓘ
rightAscension 13h 21m (approx) ⓘ
spectralFeatures shows absorption-line dominated spectrum with some emission regions ⓘ
starburstHistory evidence for past central starburst ⓘ
starFormationActivity low current star formation rate ⓘ
stellarPopulation dominantly intermediate-age and old stars ⓘ
supermassiveBlackHolePresence likely hosts a central massive black hole ⓘ
surfaceBrightness relatively high central surface brightness ⓘ
visibility observable with small amateur telescopes ⓘ

How these facts were elicited

Referenced by (1)

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