| UGC 477 | |
|---|---|
The low surface brightness (LSB) galaxy UGC 477 imaged by the Hubble Space Telescope | |
| Observation data (J2000 epoch) | |
| Constellation | Pisces |
| Right ascension | 00h 46m 13.1067s |
| Declination | +19° 29′ 23.760″ |
| Redshift | 0.008836 |
| Heliocentric radial velocity | 2649 km/s |
| Distance | 117.52 ± 6.11 Mly (36.033 ± 1.872 Mpc) |
| Apparent magnitude (V) | 14.70 |
| Apparent magnitude (B) | 15.4 |
| Characteristics | |
| Type | Sdm: |
| Size | 100,000 ly (31,000 pc) |
| Apparent size (V) | 1.633′ × 0.490′ |
| Notable features | Low-surface-brightness galaxy |
| Other designations | |
| KPG 015A, MCG +03-03-002, PGC 2699, CGCG 458-004 | |
UGC 477 is a low surface brightness (LSB) galaxy, located in the Pisces constellation. It is located over 110 million light years away. At around 100,000 light years across, it is similar in size to the Milky Way galaxy. The earliest known reference to this galaxy comes from part 2 of the Morphological Catalogue of Galaxies, published in 1964, where it is listed as MCG +03-03-002.
According to I.D. Karachentsev, UGC 477 forms an isolated galaxy pair with NGC 251.