| NGC 177 | |
|---|---|
 NGC 177 as seen in thePan-STARRS 1 Sky Survey. | |
| Observation data (J2000epoch) | |
| Constellation | Cetus |
| Right ascension | 00h 37m 34.3s[1] |
| Declination | −22° 32′ 57″[1] |
| Redshift | 0.012792[1] |
| Distance | 197.73 ± 10.57 Mly (60.625 ± 3.240 Mpc)[1] |
| Apparent magnitude (V) | 14.10[1] |
| Characteristics | |
| Type | SA(r)ab[1] |
| Apparent size (V) | 2.2' × 0.5'[1] |
| Other designations | |
| ESO 474- G 006,MCG -04-02-028,2MASX J00373433-2232573, 2MASXi J0037343-223257, ESO-LV 4740060,PGC 2241.[1] | |
NGC 177 is an unbarredspiral galaxy with a distinct ring structure, located around 200 millionlight-years away in theconstellationCetus. It was discovered in 1886 byFrank Muller.[2]
Media related toNGC 177 at Wikimedia Commons | Thisunbarred spiral galaxy article is astub. You can help Wikipedia byadding missing information. |
