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NGC 3851

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!

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NGC 3851
SDSS image of NGC 3851
Observation data (J2000 epoch)
ConstellationLeo
Right ascension11h 44m 20.4s[1]
Declination19° 58′ 51″[1]
Redshift0.021365[1]
Heliocentric radial velocity6405 km/s[1]
Distance300 Mly (92 Mpc)[1]
Group or clusterLeo Cluster
Apparent magnitude (V)15.1[1]
Characteristics
TypeE/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]

See also

References

  1. ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 3851. Retrieved 2018-07-17.
  2. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-07-17.
  3. ^ "Revised NGC Data for NGC 3851". spider.seds.org. Retrieved 2018-07-17.
  4. ^ "New General Catalog Objects: NGC 3850 - 3899". cseligman.com. Retrieved 2018-07-17.
  5. ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2018-07-17.
  6. ^ "Hierarchy catalogue". leda.univ-lyon1.fr. Retrieved 2018-07-17.
  • Media related to NGC 3851 at Wikimedia Commons
  • NGC 3851 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images