NGC 4605
Galaxy in the constellation Ursa Major
From Wikipedia, the free encyclopedia
NGC 4605 is a dwarf barred spiral galaxy[6] in the constellation Ursa Major, located at a distance of 18.1 ± 0.3 megalight-years from the Milky Way.[5] Physically it is similar in size and in B-band absolute magnitude to the Large Magellanic Cloud.[6] It is a possible member of either the M81 Galaxy Group or the Messier 101 Group.[9]
Right ascension12h 39m 59.381s[2]
Declination+61° 36′ 33.09″[2]
| NGC 4605 | |
|---|---|
| Observation data (J2000 epoch) | |
| Constellation | Ursa Major |
| Right ascension | 12h 39m 59.381s[2] |
| Declination | +61° 36′ 33.09″[2] |
| Redshift | 0.000484±0.000020[3] |
| Heliocentric radial velocity | 143 ± 5 km/s[4] |
| Distance | 18.10 ± 0.33 Mly (5.55 ± 0.10 Mpc)[5] |
| Apparent magnitude (V) | 10.9[4] |
| Absolute magnitude (B) | –18.10[6] |
| Characteristics | |
| Type | SBc[6] or SB(s)c pec[4] |
| Mass/Light ratio | 0.25±0.03[6] M☉/L☉ |
| Apparent size (V) | 6.03′ × 2.45′[7] |
| Other designations | |
| UGC 7831,[8] PGC 42408[4] | |