| NGC 5056 | |
|---|---|
NGC 5056 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 13h 16m 12.3527s |
| Declination | +30° 57′ 01.239″ |
| Redshift | 0.018653±0.000005 |
| Heliocentric radial velocity | 5,592±1 km/s |
| Distance | 208.31 ± 10.46 Mly (63.867 ± 3.207 Mpc) |
| Group or cluster | [M98j] 192 |
| Apparent magnitude (V) | 13.7 |
| Characteristics | |
| Type | Scd |
| Size | ~135,800 ly (41.65 kpc) (estimated) |
| Apparent size (V) | 1.7′ × 1.0′ |
| Other designations | |
| IRAS 13138+3112, UGC 8337, MCG +05-31-166, PGC 46180, CGCG 160-173 | |
NGC 5056 is a spiral galaxy in the constellation of Coma Berenices. Its velocity with respect to the cosmic microwave background is 5,839±17 km/s, which corresponds to a Hubble distance of 280.9 ± 19.7 Mly (86.13 ± 6.03 Mpc). However, 39 non-redshift measurements give a closer mean distance of 208.31 ± 10.46 Mly (63.867 ± 3.207 Mpc). It was discovered by German-British astronomer William Herschel on 13 March 1785.
NGC 5056 is listed as having an active galactic nucleus.
According to Abraham Mahtessian, NGC 5056 and NGC 5065 form a pair of galaxies, known as [M98j] 192.
One supernova has been observed in NGC 5056: