| NGC 4570 | |
|---|---|
 SDSS image of NGC 4570. | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 12h 36m 53.4s[1] |
| Declination | 07° 14′ 48″[1] |
| Redshift | 0.005961[1] |
| Heliocentric radial velocity | 1787 km/s[1] |
| Distance | 57.30 Mly (17.569 Mpc)[1] |
| Group or cluster | Virgo Cluster |
| Apparent magnitude (V) | 11.84[1] |
| Characteristics | |
| Type | S0[1] |
| Size | ~70,000 ly (21.46 kpc) (estimated)[1] |
| Apparent size (V) | 3.8 x 1.1[1] |
| Other designations | |
| CGCG 42-178, MCG 1-32-114, PGC 42096, UGC 7785, VCC 1692[1] | |
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NGC 4570 is an edge-on lenticular galaxy located about 57 million light-years away[2] in the constellation Virgo.[3] NGC 4570 was discovered by astronomer William Herschel on April 13, 1784[4] and is a member of the Virgo Cluster.[5][6]
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 4570. Retrieved 2018-02-08.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-02-13.
- ^ "Revised NGC Data for NGC 4570". spider.seds.org. Retrieved 2018-02-13.
- ^ "New General Catalog Objects: NGC 4550 - 4599". cseligman.com. Retrieved 2018-02-04.
- ^ Morelli, L.; Cesetti, M.; Corsini, E. M.; Pizzella, A.; Bontà, E. Dalla; Sarzi, M.; Bertola, F. (2010). "Multiband photometric decomposition of nuclear stellar disks". Astronomy and Astrophysics. 518: A32. arXiv:1004.2190. Bibcode:2010A&A...518A..32M. doi:10.1051/0004-6361/201014285. ISSN 0004-6361. S2CID 16619922.
- ^ "The Virgo Cluster". www.atlasoftheuniverse.com. Retrieved 2018-02-04.