| NGC 4329 | |
|---|---|
Image of NGC 4329 by PanSTARRS. | |
| Observation data (J2000 epoch) | |
| Constellation | Corvus |
| Right ascension | 12h 23m 20.7s |
| Declination | −12° 33′ 31″ |
| Redshift | 0.014153 |
| Heliocentric radial velocity | 4243 km/s |
| Distance | 144 Mly (44.2 Mpc) |
| Apparent magnitude (V) | 14.5 |
| Characteristics | |
| Type | E+ |
| Size | ~62,100 ly (19.03 kpc) (estimated) |
| Apparent size (V) | 2.4 x 1.4 |
| Other designations | |
| PGC 040212, MCG -02-32-009 | |
NGC 4329 is an elliptical galaxy located 144 million light-years away in the constellation Corvus. The galaxy was discovered by astronomer John Herschel on March 9, 1828. NGC 4329 is host a supermassive black hole with an estimated mass of 3.1×108 solar masses. NGC 4329 is a member of a group of 5 galaxies known as [T2015] nest 100478. NGC 4329 is the brightest member of this group and the group includes the galaxies IC 785, IC 786, MCG-02-32-006, and LEDA 170189. The redshift of NGC 4329 places it in the within the bounds of the Hydra-Centaurus supercluster.