NGC 1032
Appearance
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] |
NGC 1032 is a spiral galaxy that is about 117 million light-years away in the constellation Cetus.
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.
- ^ a b c d e f g "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