| NGC 6324 | |
|---|---|
NGC 6324 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Ursa Minor |
| Right ascension | 17h 05m 25.4687s |
| Declination | +75° 24′ 26.061″ |
| Redshift | 0.016231±0.000127 |
| Heliocentric radial velocity | 4,866±38 km/s |
| Distance | 232.1 ± 16.4 Mly (71.16 ± 5.04 Mpc) |
| Apparent magnitude (V) | 13.8 |
| Characteristics | |
| Type | Sc |
| Size | ~81,500 ly (25.00 kpc) (estimated) |
| Apparent size (V) | 0.9′ × 0.5′ |
| Other designations | |
| IRAS 17070+7528, 2MASX J17052594+7524267, UGC 10725, MCG +13-12-016, PGC 59583, CGCG 355-025 | |
NGC 6324 is a spiral galaxy in the constellation of Ursa Minor. Its velocity with respect to the cosmic microwave background is 4,825±38 km/s, which corresponds to a Hubble distance of 232.1 ± 16.4 Mly (71.16 ± 5.04 Mpc). It was discovered by German-British astronomer William Herschel on 12 December 1797.
NGC 6324 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
Two supernovae have been observed in NGC 6324: