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|Observation data (J2000 epoch)|
|Right ascension||10h 37m 12.5s|
|Declination||−27° 41′ 05″|
|Distance||117 Mly (a)|
140 million ly (b)
|Apparent magnitude (V)||+12.5|
|Apparent size (V)||2′.6 × 1′.7|
|Notable features||galaxy overlapping another|
NGC 3314 is a pair of overlapping spiral galaxies between 117 and 140 million light-years away in the constellation Hydra. This unique alignment gives astronomers the opportunity to measure the properties of interstellar dust in the face-on foreground galaxy (NGC 3314a). The dust appears dark against the background galaxy (NGC 3314b). Unlike interacting galaxies, the two components of NGC 3314 are physically unrelated. It[clarification needed] was discovered in April 1999.
In a March 2000 observation of the galaxies, a prominent green star-like object was seen in one of the arms. Astronomers theorized that it could have been a supernova, but the unique filtering properties of the foreground galaxy made it difficult to decide definitively.
Both galaxies are members of the Hydra Cluster.
- ^ Keel, Bill; Frattare, Lisa. "NGC 3314 Variable Object". heritage.stsci.edu. Retrieved 2015-11-05.
- ^ 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.
- Media related to NGC 3314 at Wikimedia Commons
- "Hubble Spies Galaxy Silhouettes". ScienceDaily. 25 September 2008. Retrieved 25 March 2018.
- Nemiroff, R.; Bonnell, J., eds. (7 May 2005). "NGC 3314: When Galaxies Overlap". Astronomy Picture of the Day. NASA. Retrieved 25 March 2018.
- NGC 3314 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- "NGC 3314". SIMBAD. Centre de données astronomiques de Strasbourg.