| NGC 809 | |
|---|---|
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 02h 04m 18.97s |
| Declination | −08° 44′ 07.06″ |
| Redshift | 0.01781±0.00001 |
| Heliocentric radial velocity | 5,292 km/s |
| Distance | 245.14 ± 0.29 Mly (75.16 ± 0.09 Mpc) |
| Apparent magnitude (B) | 14.66 |
| Characteristics | |
| Type | (R)S0^+? |
| Size | ~108,500 ly (33.27 kpc) (estimated) |
| Apparent size (V) | 1.23′ × 0.92′ |
| Other designations | |
| 6dF J0204190-084407, NGC 809, MCG -02-06-023, PGC 7889 | |
NGC 809 is a lenticular galaxy located in the constellation Cetus about 245 million light-years (75 Mpc) away from the Milky Way. It was discovered by the American astronomer Lewis Swift in November 1886. The galaxy is receding from the Milky Way with a line of sight velocity component of 5,292 km/s.
The morphological classification of NGC 809 is (R)S0+:, indicating an outer ring structure (R) around a lenticular galaxy (S0). The galaxy has a miniature central bar structure with weakly-developed spiral arms. There is a very red ring structure that is likely dust rich. This symmetrical ring was probably formed by the impact of a satellite on the central part of the galaxy.
Two supernovae have been observed in NGC 809: