| NGC 1184 | |
|---|---|
NGC 1184 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Cepheus |
| Right ascension | 03h 16m 45.1631s |
| Declination | +80° 47′ 36.130″ |
| Redshift | 0.007812±0.0000630 |
| Heliocentric radial velocity | 2,342±19 km/s |
| Distance | 109.2 ± 7.8 Mly (33.47 ± 2.38 Mpc) |
| Group or cluster | nest 101283 |
| Apparent magnitude (V) | 13.44 |
| Characteristics | |
| Type | S0/a |
| Size | ~143,100 ly (43.86 kpc) (estimated) |
| Apparent size (V) | 2.8′ × 0.6′ |
| Other designations | |
| 2MASX J03164489+8047358, UGC 2583, MCG +13-03-002, PGC 12174, CGCG 346-002 | |
NGC 1184 is a lenticular galaxy in the constellation of Cepheus. Its velocity with respect to the cosmic microwave background is 2,269±20 km/s, which corresponds to a Hubble distance of 109.2 ± 7.8 Mly (33.47 ± 2.38 Mpc). It was discovered by British astronomer William Herschel on 16 September 1787.
NGC 1184 has a possible 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.
NGC 1184 is member of a small galaxy group known as nest 101283. The other two galaxies in the group are UGC 2519 and UGC 2620.
Two supernovae have been observed in NGC 1184: