// Workers AI · dad joke modeWhy did NGC 417 go to therapy? It had a stellar issue.
| NGC 417 | |
|---|---|
 legacy surveys image of NGC 417 | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 01h 11m 05.5s[1] |
| Declination | −18° 08′ 54″[1] |
| Redshift | 0.042223[1] |
| Heliocentric radial velocity | 12,658 km/s[1] |
| Distance | 534.90 Mly (164.000 Mpc)[1] |
| Apparent magnitude (V) | 15.13[1] |
| Absolute magnitude (V) | -22.46[1] |
| Characteristics | |
| Type | SAB0−[1] |
| Apparent size (V) | 0.6' × 0.5'[1] |
| Other designations | |
| ESO 541- G 024, MCG -03-04-019, 2MASX J01110557-1808534, 2MASXi J0111055-180854, ESO-LV 5410240, 6dF J0111055-180854, PGC 4237.[1] | |
NGC 417 is a lenticular galaxy of type SAB0− located in the constellation Cetus. It was discovered in 1886 by Francis Leavenworth. It was described by Dreyer as "extremely faint, extremely small, round."[2]
References
[edit]- 1 2 3 4 5 6 7 8 9 10 "NASA/IPAC Extragalactic Database". Results for NGC 0417. Retrieved September 2, 2016.
- ↑ "New General Catalog Objects: NGC 400 - 449". Cseligman. Archived from the original on February 5, 2017. Retrieved February 12, 2017.
External links
[edit]
Media related to NGC 417 at Wikimedia Commons
.jpg){kind=small} | This lenticular galaxy article is a stub. You can help Wikipedia by adding missing information. |