NGC 7010
Appearance
NGC 7010 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Aquarius |
Right ascension | 21h 04m 39.5s[1] |
Declination | −12° 20′ 18″[1] |
Redshift | 0.028306[1] |
Heliocentric radial velocity | 8,486 km/s[1] |
Distance | 365,344,000 ly |
Apparent magnitude (V) | 14.5[1] |
Characteristics | |
Type | E+ pec [1] |
Size | ~209,420.4 ly [1] |
Apparent size (V) | 1.9 x 1.0[1] |
Other designations | |
NPM1G -12.0537, IC 5082, MCG -2-53-24, PGC 66039[1] |
NGC 7010 is a massive elliptical galaxy located about 365 million light-years from Earth in the constellation Aquarius.[2][3] NGC 7010 was discovered by astronomer John Herschel on August 6, 1823 and was later listed by French astronomer Guillaume Bigourdan as IC 5082.[4]
Physical characteristics
NGC 7010 has broad, plateau shaped shells of stars surrounding it.[5] Its theorized that the shells formed from the accretion of another galaxy.[6]
See also
References
- ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 7010. Retrieved 2017-05-06.
- ^ Rojas, Sebastián García. "Galaxy NGC 7010 Deep Sky Objects Browser". DSO Browser. Retrieved 2017-05-06.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2017-05-06.
- ^ "New General Catalog Objects: NGC 7000 - 7049". cseligman.com. Retrieved 2017-05-08.
- ^ McGaugh, Stacy S.; Bothun, Gregory D. (October 1990). "Stellar populations in shell galaxies" (PDF). The Astronomical Journal. 100: 1073. Bibcode:1990AJ....100.1073M. doi:10.1086/115580. hdl:1903/8712.
- ^ Kojima, Makoto; Noguchi, Masafumi (20 May 1997). "Sinking satellite disk galaxies. I. Shell formation preceded by cessation of star formation". The Astrophysical Journal. 481 (1): 132–156. Bibcode:1997ApJ...481..132K. doi:10.1086/304021.
External links
- Media related to NGC 7010 at Wikimedia Commons
- NGC 7010 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images