| NGC 4653 | |
|---|---|
NGC 4653 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 12h 43m 50.9247s |
| Declination | −00° 33′ 40.241″ |
| Redshift | 0.008742±0.000013 |
| Heliocentric radial velocity | 2,621±4 km/s |
| Distance | 131.11 ± 3.59 Mly (40.200 ± 1.100 Mpc) |
| Group or cluster | NGC 4642 Group (LDC 913) |
| Apparent magnitude (V) | 13.4 |
| Characteristics | |
| Type | SAB(rs)cd |
| Size | ~117,800 ly (36.13 kpc) (estimated) |
| Apparent size (V) | 1.77′ × 1.38′ |
| Other designations | |
| IRAS 12412-0017, UGC 7900, MCG +00-33-006, PGC 42847, CGCG 015-009 | |
NGC 4653 is an intermediate spiral galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 2,960±24 km/s, which corresponds to a Hubble distance of 142.4 ± 10.0 Mly (43.66 ± 3.08 Mpc). However, two non-redshift measurements give a closer distance of 131.11 ± 3.59 Mly (40.200 ± 1.100 Mpc). It was discovered by German-British astronomer William Herschel on 11 April 1787.
NGC 4653 is a member of the NGC 4642 Group (also known as LDC 913). This trio of galaxies includes NGC 4642 and NGC 4690. A study published in 2022 claims that NGC 4653 and NGC 4642 form a physical pair, separated by about 50 kpc, and that there is a high probability of a merger in the near future.
Three supernovae have been observed in NGC 4653: