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NGC 3886

In today's article we will explore the fascinating world of NGC 3886, a topic that has captured society's attention for a long time. Whether due to its impact on history, its relevance today or its future potential, NGC 3886 has generated constant interest in different areas and has been the subject of numerous debates and studies. Throughout this article, we will try to analyze different aspects related to NGC 3886, from its origin to its possible implications in the future, with the aim of offering a comprehensive vision of this exciting topic.

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NGC 3886
SDSS image of NGC 3886.
Observation data (J2000 epoch)
ConstellationLeo
Right ascension11h 47m 05.6s[1]
Declination19° 50′ 14″[1]
Redshift0.019667[1]
Heliocentric radial velocity5896 km/s[1]
Distance280 Mly (85 Mpc)[1]
Group or clusterLeo Cluster
Apparent magnitude (V)14.11[1]
Characteristics
TypeS0^-[1]
Size~160,000 ly (49 kpc) (estimated)[1]
Apparent size (V)1.2 x 0.9[1]
Other designations
CGCG 97-147, MCG 3-30-111, PGC 36756, UGC 6760[1]

NGC 3886 is a lenticular galaxy located about 280 million light-years away[2] in the constellation Leo.[3] It was discovered by astronomer Heinrich d'Arrest on May 9, 1864.[4] The galaxy 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 3886. Retrieved 2018-08-09.
  2. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-08-10.
  3. ^ "Revised NGC Data for NGC 3886". spider.seds.org. Retrieved 2018-08-10.
  4. ^ "New General Catalog Objects: NGC 3850 - 3899". cseligman.com. Retrieved 2018-07-17.
  5. ^ "NGC 3886". Retrieved 2018-08-10.
  6. ^ Steinicke, Wolfgang (2010-08-19). Observing and Cataloguing Nebulae and Star Clusters: From Herschel to Dreyer's New General Catalogue. Cambridge University Press. ISBN 978-1-139-49010-8.
  • Media related to NGC 3886 at Wikimedia Commons
  • NGC 3886 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images