| NGC 6047 | |
|---|---|
SDSS image of NGC 6047. | |
| Observation data (J2000 epoch) | |
| Constellation | Hercules |
| Right ascension | 16h 05m 09.0s |
| Declination | 17° 43′ 48″ |
| Redshift | 0.031262 |
| Heliocentric radial velocity | 9,372 km/s |
| Distance | 131.4 Mpc (429 Mly) |
| Group or cluster | Hercules Cluster |
| Apparent magnitude (V) | 14.55 |
| Characteristics | |
| Type | E+, cD |
| Size | ~170 kly (52 kpc) (estimated) |
| Apparent size (V) | 1′.1 x 0′.8 |
| Notable features | radio jet |
| Other designations | |
| CGCG 108-111, DRCG 34-62, 4C +17.66, PKS 1602+178, MCG +3-41-87, PGC 57033 | |
NGC 6047 is an elliptical galaxy located about 430 million light-years away in the constellation Hercules. It was discovered by astronomer Lewis Swift on June 27, 1886. NGC 6047 is a member of the Hercules Cluster.
NGC 6047 has a peculiar morphology which suggests it has undergone a recent merger. It may be interacting with NGC 6045 which lies around ~320,000 ly (97 kpc) away. NGC 6047 has two radio jets and is classified as a FR I radio galaxy. The jets appear to have a Z-shaped structure.