| NGC 4162 | |
|---|---|
NGC 4162 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 11m 52.5190s |
| Declination | +24° 07′ 25.346″ |
| Redshift | 0.008579±0.000005 |
| Heliocentric radial velocity | 2,572±1 km/s |
| Distance | 118.00 ± 5.96 Mly (36.179 ± 1.828 Mpc) |
| Apparent magnitude (V) | 12.87 |
| Characteristics | |
| Type | (R)SA(rs)bc |
| Size | ~85,800 ly (26.31 kpc) (estimated) |
| Apparent size (V) | 2.3′ × 1.4′ |
| Other designations | |
| IRAS 12093+2423, UGC 7193, MCG +04-29-046, PGC 038851, CGCG 128-051 | |
NGC 4162 is a spiral galaxy in the constellation of Coma Berenices. Its velocity with respect to the cosmic microwave background is 2,878±21 km/s, which corresponds to a Hubble distance of 138.5 ± 9.8 Mly (42.45 ± 2.99 Mpc). However, 19 non-redshift measurements give a closer mean distance of 118.00 ± 5.96 Mly (36.179 ± 1.828 Mpc). It was discovered by German-British astronomer William Herschel on 10 April 1785.
NGC 4162 has an active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
Three supernovae have been observed in NGC 4162: