Zeta Canis Majoris

ζ Canis Majoris
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Canis Major
Right ascension 06h20m18.8s
Declination −30°03′48″
Apparent magnitude (V) +3.02
Distance 336 ± 20 ly
(103 ± 6 pc)
Spectral type B2.5V
Other designations
Furud, Phurud, ζ CMa, 1 CMa, HR 2282, HD 44402, CD-30°3038, FK5 240, HIP 30122, SAO 196698, GC 8170, CCDM 06203-3003

Zeta Canis Majoris (ζ CMa, ζ Canis Majoris) is a spectroscopic binary in the constellation Canis Major. It has the traditional name Furud or Phurud, from the Arabic ألفرد al-furud meaning the bright single ones or, perhaps by a transcriber's error, from Al Ḳurūd (ألقرد - al-qird), the Apes, or Al Agribah (أل أغربة), the Raven by Al Sufi, referring to the surrounding small stars with some of those of Columba[1] (ζ CMa, λ CMa, γ Col, δ Col, θ Col, κ Col, λ Col, μ Col and ξ Col)[2]. ζ Canis Majoris is approximately 336 light years from Earth.

The primary component, ζ Canis Majoris A, is a blue-white B-type main sequence dwarf with an apparent magnitude of +3.02. It has an unseen companion, ζ Canis Majoris B. The two stars orbit around their common centre of mass once every 675 days.

References

  1. ^ Allen, R. H. (1963). Star Names: Their Lore and Meaning (Reprint ed.). New York: Dover Publications Inc. p. 130. ISBN 0486210790. http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Canis_Major*.html. Retrieved 2010-12-12. 
  2. ^ Davis Jr., G. A., "The Pronunciations, Derivations, and Meanings of a Selected List of Star Names,"Popular Astronomy, Vol. LII, No. 3, Oct. 1944, p. 14.