NGC 167
Spiral galaxy in the constellation Cetus
From Wikipedia, the free encyclopedia
NGC 167 is a spiral galaxy located approximately 172 million light-years from the Solar System[2] in the constellation Cetus. It was discovered in 1886 by Francis Preserved Leavenworth.[4]
| NGC 167 | |
|---|---|
NGC 167 with DECam | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 00h 35m 23.1s[1] |
| Declination | −23° 22′ 30″[1] |
| Redshift | 0.012812[1] |
| Distance | 172 Mly[2] |
| Apparent magnitude (V) | 13.98[1] |
| Characteristics | |
| Type | Sbc[3] |
| Apparent size (V) | 1.0' × 0.7'[1] |
| Other designations | |
| PGC 2122[1] | |