| NGC 3408 | |
|---|---|
NGC 3408 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Ursa Major |
| Right ascension | 10h 52m 11.6721s |
| Declination | +58° 26′ 17.272″ |
| Redshift | 0.031582±0.0000107 |
| Heliocentric radial velocity | 9,468±3 km/s |
| Distance | 462.8 ± 32.4 Mly (141.91 ± 9.94 Mpc) |
| Apparent magnitude (V) | 14.3g |
| Characteristics | |
| Type | Sc |
| Size | ~175,800 ly (53.90 kpc) (estimated) |
| Apparent size (V) | 0.85′ × 0.75′ |
| Other designations | |
| IRAS 10490+5842, 2MASX J10521167+5826168, UGC 5977, MCG +10-16-016, PGC 32616, CGCG 291-006 | |
NGC 3408 is a spiral galaxy in the constellation of Ursa Major. Its velocity with respect to the cosmic microwave background is 9,621±11 km/s, which corresponds to a Hubble distance of 462.8 ± 32.4 Mly (141.91 ± 9.94 Mpc). It was discovered by German-British astronomer William Herschel on 8 April 1793.
NGC 3408 is a radio galaxy, i.e. it has giant regions of radio emission extending well beyond its visible structure.
One supernova has been observed in NGC 3408: