NGC 1032
NGC 1032 is a spiral galaxy that is about 117 million light-years away in the constellation Cetus.
| NGC 1032 | |
|---|---|
 NGC 1032 taken by the Hubble Space Telescope.[1] | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 02h 39m 23.6s[2] |
| Declination | +01° 05′ 38″[2] |
| Redshift | 2694 ± 18 km/s[2] |
| Distance | 117 Million ly |
| Apparent magnitude (V) | 12.64[2] |
| Characteristics | |
| Type | S0/a[2] |
| Apparent size (V) | 3.3′ × 1.1′[2] |
| Other designations | |
| UGC 2147, PGC 10060, CGCG 388-086, MCG +00-07-073, SRGb 149.043, 2MASX J02392368+0105376 [2] | |
In January 2005 SN 2005E, a calcium-rich supernova, was discovered in NGC 1032.[3]
References
- "A spiral disguised". www.spacetelescope.org. Retrieved 14 May 2018.
- "NASA/IPAC Extragalactic Database". Results for NGC 1032. Retrieved 2006-11-11.
- Bishop, David. "Bright Supernovae 2005". Rochester Astronomy.org. Retrieved 21 October 2018.
External links
Media related to NGC 1032 at Wikimedia Commons- NGC 1032 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.