| UGC 3478 | |
|---|---|
UGC 3478 imaged by the Hubble Space Telescope | |
| Observation data (J2000 epoch) | |
| Constellation | Camelopardalis |
| Right ascension | 06h 32m 47.173s |
| Declination | +63° 40′ 25.28″ |
| Redshift | 0.01271338 |
| Heliocentric radial velocity | 3787 ± 150 |
| Distance | 142.10 ± 1.71 Mly (43.567 ± 0.524 Mpc) |
| Apparent magnitude (B) | 13.3 |
| Characteristics | |
| Type | Sb |
| Other designations | |
| IRAS 06280+6342, 2MASX J06324716+6340250, MCG +11-08-054, PGC 19228, CGCG 308-030 | |
UGC 3478 is a spiral galaxy located in the constellation of Camelopardalis. Its velocity with respect to the cosmic microwave background is 3,849±8 km/s, which corresponds to a Hubble distance of 185.2 ± 13.0 Mly (56.77 ± 3.98 Mpc). However, three non-redshift measurements give a closer mean distance of 142.10 ± 1.71 Mly (43.567 ± 0.524 Mpc). The first known reference to this galaxy comes from Part 1 of the Morphological Catalogue of Galaxies, published in 1962, where it is listed as MCG +11-08-054.
UGC 3478 features a growing supermassive black hole (AGN) at its center.