| NGC 6862 | |
|---|---|
NGC 6862 imaged by the Dark Energy Camera | |
| Observation data (J2000 epoch) | |
| Constellation | Telescopium |
| Right ascension | 20h 08m 54.5801s |
| Declination | −56° 23′ 30.300″ |
| Redshift | 0.014026±0.0000170 |
| Heliocentric radial velocity | 4,205±5 km/s |
| Distance | 197.3 ± 13.8 Mly (60.48 ± 4.24 Mpc) |
| Group or cluster | NGC 5084 group (LGG 429) |
| Apparent magnitude (V) | 13.44 |
| Characteristics | |
| Type | SB(rs)b |
| Size | ~136,500 ly (41.86 kpc) (estimated) |
| Apparent size (V) | 1.6′ × 1.1′ |
| Other designations | |
| ESO 186- G 002, IRAS 20049-5632, 2MASX J20085482-5623318, PGC 64168 | |
NGC 6862 is a barred spiral galaxy in the constellation of Telescopium. Its velocity with respect to the cosmic microwave background is 4,100±9 km/s, which corresponds to a Hubble distance of 197.3 ± 13.8 Mly (60.48 ± 4.24 Mpc). It was discovered by British astronomer John Herschel on 9 July 1834.
NGC 6862 is a Seyfert II galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.
NGC 6862 is a member of the ESO 185-54 group (also known as LGG 429). This group contains nine galaxies, including NGC 6848, NGC 6855, NGC 6867, IC 4935, IC 4950, IC 4952, IC 4963, and ESO 185-54.
One supernova has been observed in NGC 6862: