Today, UGC 11105 is a topic that generates great interest and debate in society. For years, UGC 11105 has been the object of study, analysis and reflection by experts and scientists in different areas. Its relevance has been reflected in numerous studies, conferences and publications that seek to understand its impact and scope in different contexts. UGC 11105 is a topic that crosses borders and reaches people of different ages, genders, cultures and nationalities, generating an enriching dialogue that allows us to understand it from different perspectives. In this article, we will delve into the world of UGC 11105, exploring its origin, evolution and consequences in today's society. Through interviews, analysis and testimonies, we will give a voice to those who have been impacted by UGC 11105 and delve into its global implications.
UGC 11105 | |
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![]() Hubble Space Telescope image of UGC 11105 | |
Observation data (J2000 epoch) | |
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 | 109 Mly (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 as PGC 61361, is a relatively nearby spiral galaxy located 109 million light-years (33.4 Mpc) away in the Hercules constellation.[2][3] The galaxy is outshone by bright stars in the foreground.[3] From the perspective on Earth, the Sun 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 possible active galactic nucleus candidate, according to SIMBAD.[1]
One supernova has been observed in UGC 11105: SN 2019pjs (type II, mag. 17.3).[4]