| NGC 662 | |
|---|---|
NGC 662 imaged byPan-STARRS | |
| Observation data (J2000epoch) | |
| Constellation | Andromeda |
| Right ascension | 01h 44m 35.4353s[1] |
| Declination | +37° 41′ 45.165″[1] |
| Redshift | 0.018860[1] |
| Heliocentric radial velocity | 5654 ± 4 km/s[1] |
| Distance | 259.7 ± 18.2 Mly (79.61 ± 5.58 Mpc)[1] |
| Apparent magnitude (V) | 13.0[1] |
| Characteristics | |
| Type | S pec[1] |
| Size | ~89,600 ly (27.48 kpc) (estimated)[1] |
| Apparent size (V) | 0.8′ × 0.5′[1] |
| Other designations | |
| IRAS 01416+3726,2MASX J01443544+3741447,UGC 1220,MCG +06-04-060,PGC 6393[1] | |
NGC 662 is aspiral galaxy in theconstellation ofAndromeda. Its velocity with respect to thecosmic microwave background is 5,397 ± 18 km/s, which corresponds to aHubble distance of 79.6 ± 5.6 Mpc (~260 millionlight-years).[1] It was discovered byFrench astronomerÉdouard Stephan on 22 November 1884.[2]
According to theSimbad database, NGC 662 is aradio galaxy.[3] It features a broadHI line[4] and is classified afield galaxy, meaning it does not belong to thegalaxy group nor acluster and is therefore gravitationally isolated.[5]
Threesupernovae have been observed in NGC 662: