11 Canis Minoris

11 Canis Minoris
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Canis Minor
Right ascension 07h 46m 16.20110s[1]
Declination +10° 46 05.7063[1]
Apparent magnitude (V) +5.25
Distance301±7[1] ly
(92±2[1] pc)
Spectral typeA1Vnn[2]
Other designations
11 CMi, BD+11° 1670, FK5 1201, GC 10463, HD 62832, HIP 37921, HR 3008, SAO 97224[3]

11 Canis Minoris is a variable star in the constellation Canis Minor. It is a white A-type main sequence dwarf with an average apparent magnitude of +5.25 and lies approximately 312 light years from Earth.

References

  1. 1 2 3 4 van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.
  2. Cowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal, 74: 375–406, Bibcode:1969AJ.....74..375C, doi:10.1086/110819.
  3. "11 CMi". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-01-26.


This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.