| NGC 178 | |
|---|---|
HST image of NGC 178 | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 00h 39m 08.392s |
| Declination | −14° 10′ 22.25″ |
| Redshift | 0.004863 |
| Heliocentric radial velocity | 1454.4 km/s |
| Distance | 67 Mly (20.6 Mpc) |
| Apparent magnitude (V) | 12.6 |
| Apparent magnitude (B) | 13.6 |
| Characteristics | |
| Type | SB(s)m |
| Size | 25 to 30 kly |
| Apparent size (V) | 1.85′ × 0.85′ |
| Other designations | |
| 2MASX J00390839-1410222, IC 39, MCG -02-02-078, PGC 2349 | |
NGC 178 is a Magellanic spiral galaxy in the constellation of Cetus. The compiler of the New General Catalogue, John Louis Emil Dreyer noted that NGC 178 was "faint, small, much extended 0°, brighter middle". It was discovered on November 3, 1885, by Ormond Stone.
Due to its high rate of star formation NGC 178 is a starburst galaxy. It is forming new stars at a rate of 0.55 M☉ per year. The peculiar morphology of this galaxy may be a sign of it being a galaxy merger.