| NGC 888 | |
|---|---|
NGC 888 imaged by Legacy Surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Horologium |
| Right ascension | 02h 17m 27.1s |
| Declination | −59° 51′ 40″ |
| Redshift | 0.029190±0.000133 |
| Heliocentric radial velocity | 8,751±40 km/s |
| Galactocentric velocity | 8662±40 km/s |
| Distance | 416.7 ± 29.2 Mly (127.76 ± 8.96 Mpc) |
| Apparent magnitude (V) | 13.0 |
| Apparent magnitude (B) | 14.0 |
| Surface brightness | 12.52 |
| Characteristics | |
| Type | E1? pec · E/S0? E |
| Apparent size (V) | 0.8′ × 0.8′ |
| Notable features | Flat-spectrum radio source |
| Other designations | |
| PGC 8743 ESO 115-2 AM 0215-600 | |
NGC 888 is a large and relatively distant elliptical galaxy in the constellation Horologium. Its velocity relative to the cosmic microwave background is 8662±40 km/s, corresponding to a Hubble distance of 127.8±9.0 Mpc. It was discovered by British astronomer John Herschel in 1834.
A redshift-independent distance measurement gives 136.0 Mpc, which is consistent within uncertainties with the Hubble distance.
NGC 888 is classified as a flat-spectrum radio galaxy.
NGC 888 and ESO 115-003 form a galaxy pair. The Hubble distance of ESO 115-003 is 134.65±9.45 Mpc. Considering the uncertainties in the distances, it is possible that the two galaxies form a physical pair.
One supernova has been observed in NGC 888: