// Workers AI · dad joke modeWhat did NGC 254 say to NGC 253? You're one galaxy behind.
| NGC 254 | |
|---|---|
 DECam image of NGC 254 | |
| Observation data (J2000 epoch) | |
| Constellation | Sculptor |
| Right ascension | 00h 47m 27.595s[1] |
| Declination | −31° 25′ 18.11″[1] |
| Redshift | 0.005434[2] |
| Heliocentric radial velocity | 1629[2] |
| Distance | 55.8 Mly (17.10 Mpc)[2] |
| Apparent magnitude (V) | 11.82[1] |
| Apparent magnitude (B) | 11.62[1] |
| Characteristics | |
| Type | (R)SA(rl)0+[3] |
| Apparent size (V) | 2.6′ × 1.7′[4] |
| Other designations | |
| MCG-05-03-005, PGC 2778 | |
NGC 254 is a lenticular galaxy located in the constellation Sculptor. It was discovered by John Herschel in 1834.[4] It is in a galaxy group with NGC 134.[3]
NGC 254 is an example of a ring galaxy, a galaxy with a ring,[3] and in this case, no central bar. Across the entire galaxy disk, there is a disk of ionized gas rotating in the direction opposite the stellar disk's rotation.[3] This situation may have arose when a retrograde-orbiting satellite galaxy accreted onto the galaxy itself, some 1 billion years ago.[3]
See also
[edit]References
[edit]- 1 2 3 4 "NGC 254". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 12 February 2017.
- 1 2 3 "NASA/IPAC Extragalactic Database". Results for NGC 254. Retrieved 2 September 2016.
- 1 2 3 4 5 Katkov, Ivan Yu.; Kniazev, Alexei Yu.; Sil'Chenko, Olga K.; Gasymov, Damir (2022). "Star formation in outer rings of S0 galaxies. IV. NGC 254: A double-ringed S0 with gas counter-rotation". Astronomy & Astrophysics. 658: A154. arXiv:2112.03289. Bibcode:2022A&A...658A.154K. doi:10.1051/0004-6361/202141934. S2CID 245728982.
- 1 2 "New General Catalog Objects: NGC 250–299". cseligman.com. Retrieved 12 February 2017.
External links
[edit]
Media related to NGC 254 at Wikimedia Commons
.jpg){kind=small} | This lenticular galaxy article is a stub. You can help Wikipedia by adding missing information. |