| UGC 11105 | |
|---|---|
.jpg) Hubble Space Telescope image of UGC 11105 | |
| Observation data (J2000epoch) | |
| Constellation | Hercules |
| Right ascension | 18h 04m 36.08s[1] |
| Declination | +21° 38′ 16.2″[1] |
| Redshift | 0.007418[1] |
| Heliocentric radial velocity | 2216 ± 4 km/s[1] |
| Distance | 109Mly (33.4 Mpc) |
| Apparent magnitude (B) | 15.7[1] |
| Characteristics | |
| Type | Sdm[2] |
| Size | ~81,100 ly (24.87 kpc) (estimated) |
| Other designations | |
| PGC 61361,UGC 11105,MCG +04-42-024, CGCG 141-047 | |
UGC 11105, also known asPGC 61361, is a relatively nearbyspiral galaxy located 109 millionlight-years (33.4Mpc) away in theHercules constellation.[2][3] The galaxy is outshone by brightstars in the foreground.[3] From the perspective onEarth, theSun is 14 thousand trillion times brighter as compared to UGC 1105, if we to calculate the apparent magnitude for both objects.[3] It is a possibleactive galactic nucleus candidate, according toSIMBAD.[1]
Onesupernova has been observed in UGC 11105: SN 2019pjs (type II, mag. 17.3).[4]
