In this article we will explore the fascinating world of NGC 3925, a topic that has piqued the interest of many people over the years. NGC 3925 has been the subject of numerous studies and research, and its relevance has remained over time. From its origins to its impact on today's society, NGC 3925 has left a significant mark on different aspects of daily life. Through this article, we will delve into the different aspects that make NGC 3925 such a relevant and interesting topic, examining its evolution over time and its influence in different areas. Get ready to immerse yourself in the exciting universe of NGC 3925!
NGC 3925 | |
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![]() SDSS image of NGC 3925. | |
Observation data (J2000 epoch) | |
Constellation | Leo |
Right ascension | 11h 51m 20.9s[1] |
Declination | 21° 53′ 21″[1] |
Redshift | 0.026482[1] |
Heliocentric radial velocity | 7939 km/s[1] |
Distance | 370 Mly (113 Mpc)[1] |
Apparent magnitude (V) | 15.3[1] |
Characteristics | |
Type | SAB0/a[1] |
Size | ~128,000 ly (39.3 kpc) (estimated)[1] |
Apparent size (V) | 0.65 x 0.45[1] |
Other designations | |
PGC 037078, MCG +04-28-071[1] |
NGC 3925 is a barred[2] lenticular galaxy[3][2] and a ring galaxy[2] located about 370 million light-years away[3] in the constellation Leo. It was discovered by astronomer Heinrich d'Arrest on February 19, 1863.[4]
NGC 3925 is classified as a "PAS galaxy" because it contains mostly old stars, with no observable star formation activity. NGC 3925 is also a member of the Coma Supercluster.[5]