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| IC 1185 | |
|---|---|
 IC 1185 captured by
Sloan Digital Sky Survey | |
| Observation data | |
| Constellation | Hercules |
| Right ascension | 241.43 degrees |
| Declination | 17.17 degrees |
| Redshift | 0.034764 |
| Heliocentric radial velocity | 10,440 km/s |
| Distance | 424.5 Mly (130.2 Mpc) |
| Group or cluster | Hercules Cluster |
| Apparent magnitude (V) | 14.89 |
| Surface brightness | 22.7 mag/arcsec |
| Characteristics | |
| Type | Sab |
| Size | 115,000 ly |
| Other designations | |
| PGC 57096, 2MASX J16054464+1743008, GIN 500, WBL 607-022, CGCG 108-134, SDSS J160544.67+174301.4, 2XMM J160544.6+174301, NFP J160544.7+174302, MCG +03-41-110, 2MASS J16054468+1743014, BMW-HRI J160544.5+174303, LEDA 57096 | |
IC 1185 is a type Sab [1] spiral galaxy located in Hercules. [2] [3] It is located 420 million light-years from the solar system and has an approximate diameter of 115,000 light-years. [4] IC 1185 was discovered on June 8, 1888, by astronomer Guillaume Bigourdan [5] and is a member of the Hercules Cluster. [6] [7] IC 1185 has a surface brightness of magnitude 22.7 [2] and presents a double nucleus, which might represent a late stage of galaxy merger. [8]
References
- ^ "Revised IC Data for IC 1185". spider.seds.org. Retrieved 2024-04-30.
- ^ a b Astronomy, Go. "IC 1185 | galaxy in Hercules | IC List | GO ASTRONOMY". Go-Astronomy.com. Retrieved 2024-04-30.
- ^ Ford, Dominic. "IC1185 (Galaxy)". In-The-Sky.org. Retrieved 2024-04-30.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-30.
- ^ "Index Catalog Objects: IC 1150 - 1199". cseligman.com. Retrieved 2024-04-30.
- ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2024-04-30.
- ^ Bakich, Michael E. (2024-01-01). "The Hercules galaxy cluster". Astronomy Magazine. Retrieved 2024-04-30.
- ^ Kollatschny, W.; Fricke, K. J.; Hellwig, J. (1986), Giuricin, G.; Mardirossian, F.; Mezzetti, M.; Ramella, M. (eds.), "Double Nucleus Galaxies", Structure and Evolution of Active Galactic Nuclei: International Meeting Held in Trieste, Italy, April 10–13, 1985, Dordrecht: Springer Netherlands, pp. 605–609, doi: 10.1007/978-94-009-4562-3_58, ISBN 978-94-009-4562-3, retrieved 2024-04-30
| This article is an
orphan, as no other articles
link to it. Please
introduce links to this page from
related articles; try the
Find link tool for suggestions. (April 2024) |
| IC 1185 | |
|---|---|
|
IC 1185 captured by
Sloan Digital Sky Survey | |
| Observation data | |
| Constellation | Hercules |
| Right ascension | 241.43 degrees |
| Declination | 17.17 degrees |
| Redshift | 0.034764 |
| Heliocentric radial velocity | 10,440 km/s |
| Distance | 424.5 Mly (130.2 Mpc) |
| Group or cluster | Hercules Cluster |
| Apparent magnitude (V) | 14.89 |
| Surface brightness | 22.7 mag/arcsec |
| Characteristics | |
| Type | Sab |
| Size | 115,000 ly |
| Other designations | |
| PGC 57096, 2MASX J16054464+1743008, GIN 500, WBL 607-022, CGCG 108-134, SDSS J160544.67+174301.4, 2XMM J160544.6+174301, NFP J160544.7+174302, MCG +03-41-110, 2MASS J16054468+1743014, BMW-HRI J160544.5+174303, LEDA 57096 | |
IC 1185 is a type Sab [1] spiral galaxy located in Hercules. [2] [3] It is located 420 million light-years from the solar system and has an approximate diameter of 115,000 light-years. [4] IC 1185 was discovered on June 8, 1888, by astronomer Guillaume Bigourdan [5] and is a member of the Hercules Cluster. [6] [7] IC 1185 has a surface brightness of magnitude 22.7 [2] and presents a double nucleus, which might represent a late stage of galaxy merger. [8]
References
- ^ "Revised IC Data for IC 1185". spider.seds.org. Retrieved 2024-04-30.
- ^ a b Astronomy, Go. "IC 1185 | galaxy in Hercules | IC List | GO ASTRONOMY". Go-Astronomy.com. Retrieved 2024-04-30.
- ^ Ford, Dominic. "IC1185 (Galaxy)". In-The-Sky.org. Retrieved 2024-04-30.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-30.
- ^ "Index Catalog Objects: IC 1150 - 1199". cseligman.com. Retrieved 2024-04-30.
- ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2024-04-30.
- ^ Bakich, Michael E. (2024-01-01). "The Hercules galaxy cluster". Astronomy Magazine. Retrieved 2024-04-30.
- ^ Kollatschny, W.; Fricke, K. J.; Hellwig, J. (1986), Giuricin, G.; Mardirossian, F.; Mezzetti, M.; Ramella, M. (eds.), "Double Nucleus Galaxies", Structure and Evolution of Active Galactic Nuclei: International Meeting Held in Trieste, Italy, April 10–13, 1985, Dordrecht: Springer Netherlands, pp. 605–609, doi: 10.1007/978-94-009-4562-3_58, ISBN 978-94-009-4562-3, retrieved 2024-04-30