| NGC 3074 | |
|---|---|
NGC 3074 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Leo Minor |
| Right ascension | 09h 59m 41.2437s |
| Declination | +35° 23′ 34.050″ |
| Redshift | 0.017130±0.0000117 |
| Heliocentric radial velocity | 5,135±4 km/s |
| Distance | 259.5 ± 18.2 Mly (79.57 ± 5.58 Mpc) |
| Apparent magnitude (V) | 14.2g |
| Characteristics | |
| Type | SAB(rs)c |
| Size | ~38,700 ly (11.87 kpc) (estimated) |
| Apparent size (V) | 2.3′ × 2.1′ |
| Other designations | |
| IRAS 09567+3537, UGC 5366, MCG +06-22-047, PGC 28888, CGCG 182-054 | |
NGC 3074 is a barred spiral galaxy in the constellation of Leo Minor. Its velocity with respect to the cosmic microwave background is 5,395±18 km/s, which corresponds to a Hubble distance of 259.5 ± 18.2 Mly (79.57 ± 5.58 Mpc). It was discovered by German-British astronomer William Herschel on 28 March 1786.
NGC 3074 is an active galaxy nucleus candidate, 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 3074: