KKR 03
From Wikipedia, the free encyclopedia
Right ascension14h 07m 10.7s[1]
Declination+35° 03′ 37″[1]
| KKR 03 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Canes Venatici |
| Right ascension | 14h 07m 10.7s[1] |
| Declination | +35° 03′ 37″[1] |
| Redshift | 0.000211[2] |
| Heliocentric radial velocity | 63.3 ± 1.8 km/s (39.3 ± 1.1 mi/s)[2] |
| Distance | 6.4 million ly (1.97 million pc)[1] |
| Apparent magnitude (V) | 15.68[3] |
| Absolute magnitude (V) | −10.85[3] |
| Characteristics | |
| Type | dIrr[2] |
| Size | 980 ly (300 pc)[1] |
| Other designations | |
| LEDA 166185, PGC 166185, [KK98a] 140501.5+351809, [KK98a] 230, [KKR99] 384.4, [KKR99] 3, 11HUGS 367, MAPS-NGP O_271_0183623 | |
KKR 03 is a dwarf irregular galaxy located 6.4 million light-years (1.97 million parsecs) away from Earth.[1] It has an absolute magnitude of −10.85[3] and lies on the inner edge of the M94 Group.[4]
