NGC 4163

In today's world, NGC 4163 has become a relevant topic that arouses the interest of millions of people around the world. Over time, NGC 4163 has acquired increasing importance in different areas, from technology to culture, politics and society in general. The impact of NGC 4163 is undeniable and its influence is felt in all spheres of daily life. In this article, we will thoroughly explore the phenomenon of NGC 4163 and analyze its relevance in today's world.

NGC 4163
Hubble Space Telescope image of NGC 4163
Observation data (J2000 epoch)
ConstellationCanes Venatici
Right ascension12h 12.9m [1]
Declination36° 10′[1]
Distance2.959 megaparsecs (9.65 Mly)
Apparent magnitude (V)14.5[1]
Characteristics
TypedIrr[1]
Apparent size (V)1.9′ × 1.6′[1]
Other designations
NGC 4167, UGC 7199, PGC 38881, MCG 6-27-26

NGC 4163, also known as NGC 4167, is a dwarf irregular galaxy in the constellation Canes Venatici, about 9.65 million light-years away. It was discovered by William Herschel on April 28, 1785 as NGC 4163. John Herschel discovered it again on March 11, 1831 as NGC 4167. It has a size on the night sky of 1.9 x 1.6, which, at its distance, gives a diameter of 4000 light-years. This galaxy consists of young blue stars.[2] It is a member of the M94 Group.[3][4][5]

References

  1. ^ a b c d e Dunlop, Storm (2005). Atlas of the Night Sky. Collins. ISBN 978-0-00-717223-8.
  2. ^ "NGC 4163".
  3. ^ R. B. Tully (1988). Nearby Galaxies Catalog. Cambridge: Cambridge University Press. ISBN 978-0-521-35299-4.
  4. ^ Fouque, P.; Gourgoulhon, E.; Chamaraux, P.; Paturel, G. (May 1992). "Groups of galaxies within 80 Mpc. II. The catalogue of groups and group members". Astronomy and Astrophysics Supplement Series. 93: 211. Bibcode:1992A&AS...93..211F. ISSN 0365-0138.
  5. ^ Garcia, A. M. (July 1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G. ISSN 0365-0138.
  • Media related to NGC 4163 at Wikimedia Commons


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