NGC 550
Spiral galaxy in the constellation Cetus
From Wikipedia, the free encyclopedia
NGC 550 is a spiral galaxy in the constellation Cetus. It is estimated to be about 300 million light-years from the Milky Way[3] and has a diameter of approximately 110,000 light years. The German-British astronomer William Herschel discovered it on 8 October 1785.[4][5][6]
| NGC 550 | |
|---|---|
SDSS image of NGC 550 | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 01h 26m 42.560s[1] |
| Declination | +02° 01′ 20.52″[1] |
| Redshift | 0.019560[2] |
| Heliocentric radial velocity | 5807 km/s[2] |
| Distance | 303.7 Mly (93.10 Mpc)[3] |
| Apparent magnitude (B) | 15.0[2] |
| Characteristics | |
| Type | SB(s)a?[3] |
| Other designations | |
| UGC 1021, MCG +00-04-146, PGC 5374[2] | |
One supernova has been observed in NGC 550: SN 1961Q (type unknown, mag. 17.2) was discovered by Milton Humason on 30 November 1961.[7][8]
