| NGC 4150 | |
|---|---|
Hubble Space Telescope image of NGC 4150 | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 10m 33.655s |
| Declination | +30° 25′ 05.35″ |
| Redshift | 0.000694 |
| Heliocentric radial velocity | 208±5 km/s |
| Distance | 42.60 ± 0.46 Mly (13.06 ± 0.14 Mpc) |
| Apparent magnitude (V) | 11.64 |
| Apparent magnitude (B) | 12.44 |
| Characteristics | |
| Type | SA(r)0^0^ |
| Number of stars | 6.3+3.1 −2.1×109 M☉ |
| Apparent size (V) | 2.3′ × 1.6′ |
| Other designations | |
| 2MASX J12103365+3024053, NGC 4150, LEDA 38742 | |
NGC 4150 is a lenticular galaxy in the constellation of Coma Berenices. It was discovered by German-British astronomer William Herschel on March 13, 1785. This galaxy is located at a distance of 42.6 million light-years (13.06 Mpc) from the Milky Way. It has an apparent visual magnitude of 11.64 and spans an angular size of 2.3′ × 1.6′.
The morphological classification of NGC 4150 is SA00(r)?, indicating this is a lenticular galaxy with possible ring structure. The galaxy is inclined at an angle of 58° with the long axis aligned along a position angle of 148°. It has a significant reservoir of molecular hydrogen that has a mass in the range (3.8 to 6.6)×107 M☉. The core region is kinematically decoupled from the rest of the galaxy, suggesting a recent merger. This minor merger added around 3×108 M☉ to the total mass.