Back NGC 21 Arabic NGC 21 (مجره) ARZ NGC 21 AST NGC 21 Azerbaijani NGC 21 Byelorussian NGC 21 BS NGC 21 Catalan NGC 21 CE NGC 29 Czech NGC 21 Welsh
| NGC 21 | |
|---|---|
 NGC 21/NGC 29 (Sloan Digital Sky Survey) | |
| Observation data (J 2000.0 epoch) | |
| Constellation | Andromeda |
| Right ascension | 00h 10m 46.9s[1] |
| Declination | +33° 21′ 10″[1] |
| Redshift | 0.015911[1] |
| Heliocentric radial velocity | 4770 ± 4 km/s[1] |
| Distance | 234 ± 29 Mly (71.7 ± 8.9 Mpc)[2] |
| Apparent magnitude (V) | +12.8 |
| Absolute magnitude (V) | -20.75[3] |
| Characteristics | |
| Type | SAB(s)bc |
| Apparent size (V) | 1,2′ × 0,59′ |
| Other designations | |
| IRAS 00082+3304, NGC 29, UGC 100, MCG +05-01-048, PGC 767, CGCG 499-066[1] | |
NGC 21 (also known as NGC 29) is a spiral galaxy in the Andromeda constellation. It was discovered by German-British astronomer William Herschel on 26 November 1790. Lewis Swift observed it again in 1885, leading to its double listing in the New General Catalogue.
- ^ a b c d e "NASA/IPAC Extragalactic Database". Results for NGC 0021. Retrieved 2010-05-03.
- ^ "Distance Results for NGC 0021". NASA/IPAC Extragalactic Database. Retrieved 2010-05-03.
- ^ "The galaxy NGC 21".