NGC 60
Spiral Galaxy in the constellation Pisces
| NGC 60 | |
|---|---|
 NGC 60 (SDSS DR14) | |
| Observation data (2000.0 epoch) | |
| Constellation | Pisces |
| Right ascension | 00h 15m 58.28s |
| Declination | −00° 18′ 12.7″ |
| Redshift | 0.039452[1] |
| Heliocentric radial velocity | 11,827 ± 27 km/s[1] |
| Distance | ~500 Mly (Redshift-based) |
| Apparent magnitude (V) | 14.85 |
| Characteristics | |
| Type | Sc |
| Apparent size (V) | 1'.30 × 1'.20 |
| Other designations | |
| UGC 150, MCG 0-1-48, ZWG 382.37, PGC 1058 | |
NGC 60 is an Sc type spiral galaxy in the Pisces constellation. NGC 60 is noticed for its unusually distorted spiral arms, which are commonly due to gravitational effects of neighboring galaxies, but there are no galaxies around NGC 60 to allow this.[2]
One supernova has been observed in NGC 60: SN 2023zba (type IIP, mag. 18.8).[3]
References
External links
Media related to NGC 60 at Wikimedia Commons- NGC 60 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- SEDS: NGC 60
- RCSED: NGC 60
