NGC 4309

Galaxy in the constellation Virgo From Wikipedia, the free encyclopedia

NGC 4309 is a lenticular galaxy located about 55 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer Christian Peters in 1881[3] and is a member of the Virgo Cluster.[4][5]

Right ascension12h 22m 12.3567s[2]
Declination+07° 08 39.632[2]
Redshift0.003479±0.0000111[2][2]
Quick facts Observation data (J2000 epoch), Constellation ...
NGC 4309
NGC 4309 imaged by the Vera C. Rubin Observatory
Observation data (J2000 epoch)
ConstellationVirgo[1]
Right ascension12h 22m 12.3567s[2]
Declination+07° 08 39.632[2]
Redshift0.003479±0.0000111[2][2]
Heliocentric radial velocity1,043±3 km/s[2] km/s[2]
Distance66.7 ± 4.8 Mly (20.44 ± 1.48 Mpc)[2]
Group or clusterVirgo Cluster
Apparent magnitude (V)13.6[2]
Characteristics
TypeSAB0^+(r)[2]
Size~63,600 ly (19.50 kpc) (estimated)[2]
Apparent size (V)2.01′ × 0.91′[2]
Other designations
VCC 0534, HOLM 382A, IRAS 12196+0725, UGC 7435, MCG +01-32-025, PGC 40051, CGCG 042-051[2]
Close

NGC 4309 is classified as an AGN[6] and has undergone ram-pressure stripping.[7]

Globular clusters

Within a distance of 160,000 ly (50 kpc) from NGC 4309 exists a population of 162 globular clusters that surround the galaxy.[8]

See also

References

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