Jump to content

12 Lyncis

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Praemonitus (talk | contribs) at 04:00, 29 July 2016 (Identifiers). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

12 Lyncis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Lynx
Right ascension 06h 46m 14.13019s [1]
Declination +59° 26′ 30.0227″ [1]
Spectral typeA3V [1]
Other designations
12 Lyn, BD+59°1015 A, HD 48250, HR 2470, SAO 25939, WDS 06462+5927A

12 Lyncis (12 Lyn) is a star in the constellation Lynx. Its combined apparent magnitude is 4.87. When seen through a telescope, it can be separated into three stars: two very close together of magnitudes 5.4 and 6.0 and a yellow-hued star of magnitude 7.2 a little further away.[2] The orbit of the two brighter stars is not known with certainty, but appears to have a period of somewhere around 700 to 900 years.[3] Parallax indicates the system is 210 ± 10 light years distant from Earth.[4]

References

  1. ^ a b c SIMBAD, Ident=12+Lyncis&submit=SIMBAD+search CCDM J06462+5926AB (accessed 20 November 2012)
  2. ^ Monks, Neale (2010). Go-To Telescopes Under Suburban Skies. New York, New York: Springer Science & Business Media. p. 56. ISBN 9781441968517.
  3. ^ Malkov, O. Yu.; Tamazian, V.S.; Docobo, J.A.; Chulkov, D.A. (2012). "Dynamical Masses of a Selected Sample of Orbital Binaries". Astronomy and Astrophysics. 546: 5. Bibcode:2012A&A...546A..69M. doi:10.1051/0004-6361/201219774. A69.
  4. ^ van Leeuwen, F. (2007). "Validation of the New Hipparcos Reduction". Astronomy and Astrophysics. 474 (2): 653–64. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.