NGC 3718
| NGC 3718 | |
|---|---|
 NGC 3718 | |
| Observation data (J2000.0 epoch) | |
| Constellation | Ursa Major |
| Right ascension | 11h 32m 34.940s[1] |
| Declination | +53° 04′ 04.18″[1] |
| Redshift | 0.003306[2] |
| Distance | 47.84 ± 8.54 Mly (14.667 ± 2.618 Mpc)[3] |
| Apparent magnitude (V) | 10.61[2] |
| Characteristics | |
| Type | SB(s)a pec[3] |
| Apparent size (V) | 2.940″ × 2.352″[1] |
| Other designations | |
| Arp 214, UGC 6524, MCG+09-19-114, PGC 35616[2] | |
NGC 3718, also called Arp 214, is a galaxy located approximately 52 million light years from Earth in the constellation Ursa Major.[4][2][5] It is either a lenticular or spiral galaxy.[6]
NGC 3718 has a warped, s-shape. This may be due to gravitational interaction between it and NGC 3729, another spiral galaxy located 150,000 light-years away.[7]
NGC 3718 is a member of the Ursa Major Cluster.[8]
References
- ^ a b c Skrutskie, M.; et al. (2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708.
- ^ a b c d "NGC 3718". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 8 December 2017.
- ^ a b "NED results for object NGC 3718". National Aeronautics and Space Administration / Infrared Processing and Analysis Center. Retrieved 8 December 2017.
- ^ Nemiroff, R.; Bonnell, J., eds. (31 August 2006). "Extra Galaxies". Astronomy Picture of the Day. NASA.
- ^ "Best of AOP: NGC 3718". noao.edu.
- ^ "NGC 3718, Spiral Galaxy". kopernik.org.
- ^ http://apod.nasa.gov/apod/ap130803.html
- ^ Tully, R. Brent; Verheijen, Marc A. W.; Pierce, Michael J.; Huang, Jia-Sheng; Wainscoat, Richard J. (December 1996). "The Ursa Major Cluster of Galaxies.I.Cluster Definition and Photometric Data". The Astronomical Journal. 112: 2471. arXiv:astro-ph/9608124. Bibcode:1996AJ....112.2471T. doi:10.1086/118196. ISSN 0004-6256.
External links
Media related to NGC 3718 at Wikimedia Commons
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