NGC 1250
From Infogalactic: the planetary knowledge core
NGC 1250 | |
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250px
SDSS image of NGC 1250.
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Observation data (J2000 epoch) | |
Constellation | Perseus |
Right ascension | 03h 15m 21.1s[1] |
Declination | 41° 21′ 20″[1] |
Redshift | 0.020061[1] |
Helio radial velocity | 6014 km/s[1] |
Distance | 276 Mly (84.5 Mpc)[1] |
Group or cluster | Perseus Cluster |
Type | S0^0[1] |
Apparent dimensions (V) | 2.1 x 0.9[1] |
Apparent magnitude (V) | 13.96[1] |
Other designations | |
UGC 02613, MCG +07-07-040, PGC 012098[1] | |
NGC 1250 is an edge-on lenticular galaxy located about 275 million light-years away[2] in the constellation Perseus.[3] It was discovered by astronomer Lewis Swift on Oct 21, 1886.[4] NGC 1250 is a member of the Perseus Cluster.[5]
See also
External links
- NGC 1250 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 Lua error in package.lua at line 80: module 'strict' not found.
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