| NGC 712 | |
|---|---|
Pan-STARRS image of NGC 712 | |
| Observation data ( J2000 epoch) | |
| Constellation | Andromeda |
| Right ascension | 01h 53m 08.4s [1] |
| Declination | 36° 49′ 11″ [1] |
| Redshift | 0.017779 [1] |
| Heliocentric radial velocity | 5330 km/s [1] |
| Distance | 230 Mly (69 Mpc) [1] |
| Group or cluster | Abell 262 |
| Apparent magnitude (V) | 13.77 [1] |
| Characteristics | |
| Type | S0 [1] |
| Size | ~100,000 ly (32 kpc) (estimated) [1] |
| Apparent size (V) | 1.3 x 1.0 [1] |
| Other designations | |
| MCG 6-5-35, PGC 6988, UGC 1352 [1] | |
NGC 712 is a lenticular galaxy located 230 million light-years away [2] in the constellation Andromeda. It was discovered by astronomer John Herschel in October 1828 [3] and is a member of Abell 262. [4] [5] [6] [7]
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 712. Retrieved 2018-12-28.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-12-28.
- ^ "New General Catalog Objects: NGC 700 - 749". cseligman.com. Retrieved 2018-11-21.
- ^ Garcia, A. M. (1993-07-01). "General study of group membership. II - Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47–90. Bibcode: 1993A&AS..100...47G. ISSN 0365-0138.
- ^ Giuricin, Giuliano; Marinoni, Christian; Ceriani, Lorenzo; Pisani, Armando (2000-11-01). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". The Astrophysical Journal. 543 (1): 178–194. arXiv: astro-ph/0001140. Bibcode: 2000ApJ...543..178G. doi: 10.1086/317070. ISSN 0004-637X. S2CID 9618325.
- ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2018-12-29.
- ^ "NGC 712". sim-id. Retrieved 2018-12-29.
- NGC 712 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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.jpg){kind=small} | This lenticular galaxy article is a stub. You can help Wikipedia by expanding it. |
| NGC 712 | |
|---|---|
|
Pan-STARRS image of NGC 712 | |
| Observation data ( J2000 epoch) | |
| Constellation | Andromeda |
| Right ascension | 01h 53m 08.4s [1] |
| Declination | 36° 49′ 11″ [1] |
| Redshift | 0.017779 [1] |
| Heliocentric radial velocity | 5330 km/s [1] |
| Distance | 230 Mly (69 Mpc) [1] |
| Group or cluster | Abell 262 |
| Apparent magnitude (V) | 13.77 [1] |
| Characteristics | |
| Type | S0 [1] |
| Size | ~100,000 ly (32 kpc) (estimated) [1] |
| Apparent size (V) | 1.3 x 1.0 [1] |
| Other designations | |
| MCG 6-5-35, PGC 6988, UGC 1352 [1] | |
NGC 712 is a lenticular galaxy located 230 million light-years away [2] in the constellation Andromeda. It was discovered by astronomer John Herschel in October 1828 [3] and is a member of Abell 262. [4] [5] [6] [7]
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 712. Retrieved 2018-12-28.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-12-28.
- ^ "New General Catalog Objects: NGC 700 - 749". cseligman.com. Retrieved 2018-11-21.
- ^ Garcia, A. M. (1993-07-01). "General study of group membership. II - Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47–90. Bibcode: 1993A&AS..100...47G. ISSN 0365-0138.
- ^ Giuricin, Giuliano; Marinoni, Christian; Ceriani, Lorenzo; Pisani, Armando (2000-11-01). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". The Astrophysical Journal. 543 (1): 178–194. arXiv: astro-ph/0001140. Bibcode: 2000ApJ...543..178G. doi: 10.1086/317070. ISSN 0004-637X. S2CID 9618325.
- ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2018-12-29.
- ^ "NGC 712". sim-id. Retrieved 2018-12-29.
- NGC 712 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
| Stars |
| ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| |||||||||||||
|
Star clusters |
| ||||||||||||
| Nebulae |
| ||||||||||||
| Galaxies |
| ||||||||||||
| |||||||||||||
| |||||||||||||
|
| This lenticular galaxy article is a stub. You can help Wikipedia by expanding it. |