NGC 4895 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Coma Berenices |
Right ascension | 13h 00m 17.9s[1] |
Declination | 28° 12′ 08″[1] |
Redshift | 0.028326[1] |
Heliocentric radial velocity | 8492 km/s[1] |
Distance | 330 Mly (100 Mpc)[1] |
Group or cluster | Coma Cluster |
Apparent magnitude (V) | 14.0[1] |
Characteristics | |
Type | SA0 pec[1] |
Size | ~200,000 ly (62 kpc) (estimated)[1] |
Apparent size (V) | 1.8 x 0.6[1] |
Other designations | |
NGC 4896,[2] CGCG 160-249, MCG 5-31-81, PGC 44737, UGC 8113[1] |
NGC 4895 is a lenticular galaxy located 330 million light-years away[3] in the constellation Coma Berenices.[4] The galaxy was discovered by astronomer Heinrich d'Arrest on May 5, 1864[4] and is a member of the Coma Cluster.[5][6][7]
NGC identification
According to Harold Corwin, NGC 4895 is equal to NGC 4896. The NGC designation is usually given to CGCG 160-087[2] which is a member of the Coma Cluster.[8]
See also
References
- 1 2 3 4 5 6 7 8 9 10 "NASA/IPAC Extragalactic Database". Results for NGC 4895. Archived from the original on 2011-05-14. Retrieved 2018-11-11.
- 1 2 "NGC/IC Project Restoration Efforts". ngcicproject.org. Archived from the original on 2018-11-13. Retrieved 2018-11-13.
- ↑ "Your NED Search Results". ned.ipac.caltech.edu. Archived from the original on 2018-11-13. Retrieved 2018-11-11.
- 1 2 "New General Catalog Objects: NGC 4850 - 4899". cseligman.com. Archived from the original on 2018-09-22. Retrieved 2018-11-11.
- ↑ "Detailed Object Classifications". ned.ipac.caltech.edu. Archived from the original on 2018-11-13. Retrieved 2018-11-12.
- ↑ "NGC 4895". Archived from the original on 2018-11-13. Retrieved 2018-11-12.
- ↑ "Hierarchy catalogue". leda.univ-lyon1.fr. Retrieved 2018-11-12.
- ↑ "Detailed Object Classifications". ned.ipac.caltech.edu. Archived from the original on 2018-11-13. Retrieved 2018-11-13.
External links
- Media related to NGC 4895 at Wikimedia Commons
- NGC 4895 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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