Messier 77

E591822

Messier 77 is a bright barred spiral galaxy and active galactic nucleus located in the constellation Cetus, known as one of the nearest and most studied Seyfert galaxies.

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Statements (44)

Predicate Object
instanceOf Seyfert galaxy
barred spiral galaxy
activityType Seyfert type II nucleus
alsoKnownAs Arp 37 NERFINISHED
M77 NERFINISHED
NGC 1068 NERFINISHED
apparentMagnitudeV 8.9
arpNumber 37
bestSeenIn autumn months from northern hemisphere
cataloguedBy Charles Messier NERFINISHED
constellation Cetus NERFINISHED
declination −00° 00′ 48″
diameter about 170000 light-years
discoverer Pierre Méchain NERFINISHED
discoveryDate 1780
distanceFromEarth about 14.4 megaparsecs
about 47 million light-years
galaxyType barred spiral galaxy
hasClassification radio-quiet AGN
hasDustStructure circumnuclear dust torus
hasFeature bright active nucleus
prominent central bar
strong emission lines in spectrum
well-defined spiral arms
hasStarFormation enhanced circumnuclear starburst region
hostGalaxyOf supermassive black hole
isOneOf best-studied active galactic nuclei
nearest Seyfert galaxies
isTargetFor amateur astronomers
professional observatories
locatedIn local universe
messierNumber 77
morphologicalType (R)SA(rs)b
ngcNumber 1068
observedIn X-ray wavelengths
infrared wavelengths
optical wavelengths
radio wavelengths
partOf Cetus constellation region NERFINISHED
radialVelocity 1137 km/s
redshift 0.003793
rightAscension 02h 42m 40.7s
supermassiveBlackHoleMass about 10 million solar masses
visibleIn small telescopes

Referenced by (2)

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

Cetus containsDeepSkyObject Messier 77
Cetus containsGalaxy Messier 77