| NGC 4118 | |
|---|---|
| | |
| Observation data (2000.0 epoch) | |
| Constellation | Ursa Major |
| Right ascension | 12h 07m 52.9s [1] |
| Declination | 43° 06′ 39″ [1] |
| Redshift | 0.002126 [1] |
| Heliocentric radial velocity | 637 km/s [1] |
| Distance | 39 Mly (11.9 Mpc) [1] |
| Apparent magnitude (V) | 15.6 [1] |
| Absolute magnitude (B) | -15.44 [1] |
| Characteristics | |
| Type | S0+ [1] |
| Size | ~8,100 ly (2.48 kpc) (estimated) [1] |
| Apparent size (V) | 0.70 × 0.41 [1] |
| Other designations | |
| CGCG 215-030, MCG +07-25-028, PGC 038507 [1] | |
NGC 4118 is a dwarf lenticular galaxy [2] located approximately 63 million light-years away [3] in the constellation Canes Venatici. It was discovered April 20, 1857 by R. J. Mitchell. [4] NGC 4118 is a star forming dwarf galaxy, [5] and is connected to the galaxy NGC 4111, along with the nearby NGC 4117, by disturbed H I from NGC 4111. [6]
NGC 4118 is a companion of the galaxy NGC 4117, [7] [8] with both galaxies being members of the NGC 4111 Group [9] [10] which is part of the Ursa Major Cloud. [11]