| NGC 4346 | |
|---|---|
NGC 4346 (SDSS DR14) | |
| Observation data (J2000 epoch) | |
| Constellation | Canes Venatici |
| Right ascension | 12h 23m 27.970s |
| Declination | +46° 59′ 37.558″ |
| Redshift | 0.002568±0.00009 |
| Heliocentric radial velocity | 798 km/s |
| Distance | 45.9 Mly (14.06 Mpc) |
| Group or cluster | Ursa Major Cluster |
| Apparent magnitude (V) | 11.3 |
| Characteristics | |
| Type | S0 edge-on |
| Apparent size (V) | 3.2′ × 1.3′ |
| Other designations | |
| NGC 4346, UGC 07463, MCG +08-23-016, CGCG 244-009, 1221.0+4716 | |
NGC 4346 is a lenticular galaxy located in the constellation Canes Venatici about 50 million light-years away. It was discovered on April 1, 1788 by the German-British astronomer William Herschel. This formation has an apparent visual magnitude of 11.3 and spans an angular size of 3.2′ × 1.3′. It is a member of the Ursa Major Cluster of galaxies, and is the dominant member of its own sub-group located near the center of the cluster.