In this article, we invite you to explore the fascinating world of NGC 3851. Whether you are an amateur or an expert on the subject, you will surely find valuable and entertaining information that will allow you to delve deeper into this exciting topic. From its origins to its most current applications, NGC 3851 offers a wide range of aspects of interest that will undoubtedly awaken your curiosity. Join us on this journey of discovery as we explore the most relevant and surprising aspects of NGC 3851. Get ready to expand your knowledge and enjoy a tour that will undoubtedly awaken your interest in this exciting topic!
| NGC 3851 | |
|---|---|
SDSS image of NGC 3851 | |
| Observation data (J2000 epoch) | |
| Constellation | Leo |
| Right ascension | 11h 44m 20.4s[1] |
| Declination | 19° 58′ 51″[1] |
| Redshift | 0.021365[1] |
| Heliocentric radial velocity | 6405 km/s[1] |
| Distance | 300 Mly (92 Mpc)[1] |
| Group or cluster | Leo Cluster |
| Apparent magnitude (V) | 15.1[1] |
| Characteristics | |
| Type | E/S0[1] |
| Size | ~78,000 ly (24 kpc) (estimated)[1] |
| Apparent size (V) | 0.25 × 0.2[1] |
| Other designations | |
| ARAK 316, CGCG 97-106, MCG 3-30-77, PGC 36516[1] | |
NGC 3851 is an elliptical or lenticular galaxy located about 300 million light-years away[2] in the constellation Leo.[3] It was discovered by astronomer John Herschel on February 24, 1827[4] and is a member of the Leo Cluster.[5][6]