NGC 4324 | |
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Observation data (J2000 epoch) | |
Constellation | Virgo |
Right ascension | 12h 23m 06.2s[1] |
Declination | 05° 15′ 01″[1] |
Redshift | 0.005561[1] |
Heliocentric radial velocity | 1667 km/s[1] |
Distance | 85.4 Mly (26.18 Mpc)[1] |
Group or cluster | Virgo W |
Apparent magnitude (V) | 12.51[1] |
Characteristics | |
Type | SA(r)0+[1] |
Mass | 5.25 × 1011[2] M☉ |
Size | ~66,000 ly (20.2 kpc) (estimated)[1] |
Apparent size (V) | 2.8 x 1.2[1] |
Notable features | Star Forming Ring |
Other designations | |
UGC 07451, VCC 0613, PGC 040179, MCG +01-32-032[1] |
NGC 4324 is a lenticular galaxy[3] located about 85 million light-years away[4] in the constellation Virgo. It was discovered by astronomer Heinrich d'Arrest on March 4, 1862.[5] NGC 4324 has a stellar mass of 5.62 × 1010 M☉, and a baryonic mass of 5.88 × 1010 M☉. The galaxy's total mass is around 5.25 × 1011 M☉.[2] NGC 4324 is notable for having a ring of star formation surrounding its nucleus.[6][7][8] It was considered a member of the Virgo II Groups until 1999, when its distance was recalculated and it was placed in the Virgo W Group.[9][10]
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