| UGC 1775 | |
|---|---|
 UGC 1775 by Sloan Digital Sky Survey | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 02h 18m 26.4s[1] |
| Declination | +05° 39′ 14″[1] |
| Redshift | 0.030381 ± 0.000002 [1] |
| Heliocentric radial velocity | 9,108 ± 1 km/s[1] |
| Distance | 395 ± 28 Mly (121 ± 8.5 Mpc)[1] |
| Apparent magnitude (V) | 13.8 |
| Characteristics | |
| Type | S? [1] |
| Apparent size (V) | 1.5′ × 1.5′[1] |
| Notable features | Collisional ring |
| Other designations | |
| Arp 10, VV 362, MCG +01-06-062, IRAS 02158+0525, PGC 8802 | |
UGC 1775 or Arp 10 is a ring galaxy in the constellation Cetus. The galaxy lies about 400 million light years away from Earth, which means, given its apparent dimensions, that UGC 1775 is approximately 220,000 light years across.[1] The galaxy is included in Halton Arp's Atlas of Peculiar Galaxies in the galaxies with split arms category.