| NGC 1056 | |
|---|---|
NGC 1056 imaged by the Hubble Space Telescope | |
| Observation data (J2000 epoch) | |
| Constellation | Aries |
| Right ascension | 02h 42m 48.2738s |
| Declination | +28° 34′ 26.502″ |
| Redshift | 0.004920±0.00000334 |
| Heliocentric radial velocity | 1,475±1 km/s |
| Distance | 91.16 ± 5.50 Mly (27.950 ± 1.685 Mpc) |
| Apparent magnitude (V) | 13.32 |
| Characteristics | |
| Type | Sa? |
| Size | ~68,100 ly (20.89 kpc) (estimated) |
| Apparent size (V) | 2.3′ × 1.1′ |
| Other designations | |
| IRAS 02398+2821, 2MASX J02424828+2834273, UGC 2183, MCG +05-07-032, Mrk 1183, PGC 10272, CGCG 505-036 | |
NGC 1056 is a spiral galaxy in the constellation of Aries. Its velocity with respect to the cosmic microwave background is 1,257±15 km/s, which corresponds to a Hubble distance of 60.5 ± 4.3 Mly (18.55 ± 1.32 Mpc). However, 10 non-redshift measurements give a much farther mean distance of 91.16 ± 5.50 Mly (27.950 ± 1.685 Mpc). It was discovered by German-British astronomer William Herschel on 26 October 1786.
NGC 1056 is a Seyfert II galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.
NGC 1056 is a galaxy whose nucleus shines in the ultraviolet range, and is thus listed in the Markarian catalogue as Mrk 1183.
One supernova has been observed in NGC 1056: SN 2011aq (Type II, mag. 18) was discovered by the Lick Observatory Supernova Search (LOSS) on 24 January 2011.