| NGC 1015 | |
|---|---|
| NGC 1015 imaged by the Hubble Space Telescope [1] | |
| Observation data (J2000 [2] epoch) | |
| Constellation | Cetus |
| Right ascension | 02h 38m 11.565s [2] |
| Declination | −01° 19′ 07.02″ [2] |
| Redshift | 0.008797 [2] |
| Heliocentric radial velocity | 2625.7km/s [2] |
| Apparent magnitude (B) | 12.8 [2] |
| Characteristics | |
| Type | Sb [2] |
| Other designations | |
| 6dFGS gJ023811.6-011907, HIPASS J0238-01, LEDA 9988, 2MASX J02381156-0119070, MCG+00-07-066, SDSS J023811.55-011907.5, UGC 2124, UZC J023811.5-011908, Z 388-75, Z 0235.6-0132, [PVK2003] 039.54833 -01.31778 [2] | |
NGC 1015 is a barred spiral galaxy, at a distance of 118 million light years in the constellation of Cetus (The Whale). [1] It was discovered by German astronomer Wilhelm Tempel on 27 December 1875. [3]
One supernova has been observed in NGC 1015. SN 2009ig (Type Ia, mag. 17.5) was discovered by the Lick Observatory Supernova Search (LOSS) on 20 August 2009. [4] [5] [6] It got as bright as magnitude 13, making it the brightest supernova of 2009. [7]