| NGC 3313 | |
|---|---|
 legacy surveys image of NGC 3313 | |
| Observation data (J2000 epoch) | |
| Constellation | Hydra |
| Right ascension | 10h 37m 25.4s[1] |
| Declination | −25° 19′ 10″[1] |
| Redshift | 0.012362[1] |
| Heliocentric radial velocity | 3706 km/s[1] |
| Distance | 55.4 Mpc (181 Mly)[1] |
| Group or cluster | Hydra Cluster |
| Apparent magnitude (V) | 12.38[1] |
| Characteristics | |
| Type | (R')SB(rs)ab[1] |
| Size | ~39.04 kpc (127,300 ly) (estimated)[1] |
| Apparent size (V) | 3.9 × 3.2[1] |
| Other designations | |
| ESO 501-50, AM 1035-250, IRAS 10350-2503, MCG -4-25-44, PGC 31551, UGCA 213[1] | |
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NGC 3313 is a large barred spiral galaxy[2][3] located about 55 megaparsecs (180 million light-years) away in the constellation Hydra.[4] It was discovered by astronomer Ormond Stone in 1886[5][6] and is an outlying member of the Hydra Cluster.[7]
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 3313. Retrieved 2018-06-06.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-06-06.
- ^ "NGC 3313 - SB(r)b". The De Vaucouleurs Atlas of Galaxies. 2017. Retrieved 2018-06-06.
- ^ "Revised NGC Data for NGC 3313". spider.seds.org. Retrieved 2018-06-06.
- ^ Gottlieb, Steve. "Astronomy-Mall: Adventures In Deep Space NGC objects 3001-3999". Astronomy-Mall. Retrieved 2018-04-27.
- ^ "New General Catalog Objects: NGC 3300 - 3349". cseligman.com. Retrieved 2018-05-04.
- ^ Richter, O.-G. (February 1989). "The Hydra I cluster of galaxies. V - A catalogue of galaxies in the cluster area". Astronomy and Astrophysics Supplement Series. 77: 237–256. Bibcode:1989A&AS...77..237R.