NGC 2967
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Right ascension09h 42m 03.3401s[1]
Declination+00° 20′ 10.837″[1]
| NGC 2967 | |
|---|---|
NGC 2967 imaged by Legacy Surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Sextans |
| Right ascension | 09h 42m 03.3401s[1] |
| Declination | +00° 20′ 10.837″[1] |
| Redshift | 0.006264±0.00000700[1] |
| Heliocentric radial velocity | 1,878±2 km/s[1] |
| Distance | 76.52 ± 6.16 Mly (23.460 ± 1.889 Mpc)[1] |
| Group or cluster | NGC 2967 group (LGG 182) |
| Apparent magnitude (V) | 12.30[1] |
| Characteristics | |
| Type | SA(s)c[1] |
| Size | ~70,400 ly (21.58 kpc) (estimated)[1] |
| Apparent size (V) | 3.0′ × 2.8′[1] |
| Other designations | |
| IRAS 09394+0033, 2MASS J09420330+0020113, UGC 5180, MCG +00-25-007, PGC 27723, CGCG 007-020[1] | |
NGC 2967 is a spiral galaxy in the constellation of Sextans. Its velocity with respect to the cosmic microwave background is 2,218±24 km/s, which corresponds to a Hubble distance of 106.7 ± 7.6 Mly (32.71 ± 2.32 Mpc).[1] However, five non-redshift measurements give a closer mean distance of 76.52 ± 6.16 Mly (23.460 ± 1.889 Mpc).[2] It was discovered by German-British astronomer William Herschel on 20 December 1784.[3][4]
Supernova
One supernova has been observed in NGC 2967: SN 2010fz (Type Ia, mag. 15.8) was discovered by Berto Monard on 9 July 2010.[7][8]