| NGC 4330 | |
|---|---|
NGC 4330 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 12h 23m 17.1775s |
| Declination | +11° 22′ 04.990″ |
| Redshift | 0.005214 |
| Heliocentric radial velocity | 1563 ± 3 km/s |
| Distance | 91.3 ± 6.5 Mly (27.99 ± 1.99 Mpc) |
| Group or cluster | M87 group (LGG 289) |
| Apparent magnitude (V) | 12.4 |
| Characteristics | |
| Type | Scd? |
| Size | ~105,800 ly (32.43 kpc) (estimated) |
| Apparent size (V) | 4.5′ × 0.9′ 4.5' x 0.9' |
| Other designations | |
| IRAS 12207+1138, 2MASX J12231724+1122047, UGC 7456, MCG +02-32-020, PGC 40201, CGCG 070-039, VCC 630 | |
NGC 4330 is a spiral galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 1898 ± 24 km/s, which corresponds to a Hubble distance of 27.99 ± 1.99 Mpc (~112 million light-years). However, a dozen non-redshift measurements give a much closer distance of 19.642 ± 1.559 Mpc (~64.1 million light-years). The galaxy was discovered by Irish engineer Bindon Stoney on 14 April 1852.
One supernova has been observed in NGC 4330: SN 2024phz (Type II, mag. 17.669) was discovered by ATLAS on 11 July 2024.
According to A.M. Garcia, NGC 4330 is a member of the M87 group (also known as LGG 289). This group contains at least 96 members.
NGC 4330 is also listed as catalog number VCC 0630, a member of the Virgo Cluster.