| NGC 6045 | |
|---|---|
Sloan Digital Sky Survey image of NGC 6045. The small, nearby galaxy at left portion of the image is PGC 84720. | |
| Observation data (J2000 epoch) | |
| Constellation | Hercules |
| Right ascension | 16h 05m 07.9s |
| Declination | 17° 45′ 28″ |
| Redshift | 0.033310 |
| Heliocentric radial velocity | 9986 km/s |
| Distance | 137 Mpc (447 Mly) |
| Group or cluster | Hercules Cluster |
| Apparent magnitude (V) | 14.9 |
| Characteristics | |
| Type | SB(s)c |
| Size | ~183,300 ly (56.20 kpc) (estimated) |
| Apparent size (V) | 1.17 x 0.28 |
| Notable features | Warped disk |
| Other designations | |
| PGC 057031, UGC 10177, Arp 71, MCG +03-41-088 | |
NGC 6045 is a barred spiral galaxy located about 450 million light-years away in the constellation Hercules. NGC 6045 was discovered by astronomer Lewis Swift on June 27, 1886 and is a member of the Hercules Cluster. It is also a LINER galaxy.
NGC 6045 is very luminous in both X-ray and infrared light. This high luminosity in both X-ray and infrared has been suggested to be the result of a starburst event in the galaxy. It is thought that starburst events are caused by interactions or mergers with other galaxies. Also, NGC 6045 has a warped disk which may be due to an interaction with the elliptical galaxy NGC 6047 which lies around ~320,000 ly (97 kpc) from the galaxy.