Delta Canis Majoris
Epoch J2000 Equinox J2000
|Right ascension||07h 08m 23.48608s|
|Declination||−26° 23′ 35.5474″|
|Apparent magnitude (V)||1.824|
|Spectral type||F8 Ia|
|U−B color index||+0.584|
|B−V color index||+0.691|
|Variable type||Alpha Cygni|
|Radial velocity (Rv)||34.3 ± 0.9 km/s|
|Proper motion (μ)||RA: –3.12 mas/yr
Dec.: +3.31 mas/yr
|Parallax (π)||2.03 ± 0.38 mas|
|Distance||approx. 1,600 ly
(approx. 490 pc)
|Absolute magnitude (MV)||–6.86|
|Mass||16.9 ± 1.6 M☉|
|Radius||215 ± 66 R☉|
|Surface gravity (log g)||1.00 ± 0.14 cgs|
|Temperature||6,390 ± 150 K|
|Metallicity [Fe/H]||0.24 dex|
|Rotational velocity (v sin i)||25 km/s|
Delta Canis Majoris (δ CMa, δ Canis Majoris) is a star in the constellation Canis Major. It has the traditional name Wezen, Wesen, or Wezea. It is a yellow-white F-type supergiant with an apparent magnitude of +1.83. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.
Delta Canis Majoris is the third brightest star in the constellation after Sirius and Adhara, with an apparent magnitude of +1.83, and is white or yellow-white in colour. Lying about 10 degrees south southeast of Sirius, it only rises to about 11 degrees above the horizon at the latitude of the United Kingdom. The open cluster NGC 2354 is located only 1.3 degrees east of Delta Canis Majoris. As with the rest of Canis Major, Wezen is most visible in winter skies in the northern hemisphere, and summer skies in the southern. In Bayer's Uranometria, it is in the Great Dog's hind quarter.
History and naming
The traditional name, Wezen, is derived from the medieval Arabic وزن al-wazn, which means "weight" in modern Arabic. The name was for one of a pair of stars, the other being Hadar, which has now come to refer to Beta Centauri. It is unclear whether the pair of stars was originally Alpha and Beta Centauri or Alpha and Beta Columbae. In any case, the name was somehow applied to both Delta Canis Majoris and Beta Columbae. Richard Hinckley Allen muses that the name alludes to the difficulty the star has rising above the (northern hemisphere) horizon. Astronomer Jim Kaler has noted the aptness of the traditional name given the star's massive nature.
In Chinese, 弧矢 (Hú Shǐ), meaning Bow and Arrow, refers to an asterism consisting of δ Canis Majoris, η Canis Majoris, HD 63032, HD 65456, ο Puppis, k Puppis, ε Canis Majoris, κ Canis Majoris and π Puppis. Consequently, δ Canis Majoris itself is known as 弧矢一 (Hú Shǐ yī, English: the First Star of Bow and Arrow.)
In the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Thalath al Adzari (تالت ألعذاري - taalit al-aðārii), which was translated into Latin as Tertia Virginum, meaning the third virgin. This star, along with ε CMa (Adhara), η CMa (Aludra) and ο2 CMa (Thanih al Adzari), were Al ʽAdhārā (ألعذاري), the Virgins.
Wezen is a supergiant of class F8 with a radius around 237 times that of the Sun. Its surface temperature is around 5,818 K, and it weighs around 17 solar masses. Its absolute magnitude is –6.87, and it lies around 1,600 light years away. It is rotating at a speed of around 28 km/s, and hence may take a year to rotate fully. Only around 10 million years old, Wezen has stopped fusing hydrogen in its core. Its outer envelope is beginning to expand and cool, and in the next 100,000 years it will become a red supergiant as its core fuses heavier and heavier elements. Once it has a core of iron, it will collapse and explode as a supernova.
If Wezen were as close to Earth as Sirius is, it would be as bright as a half-full moon.
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- Davis, J. et al. (October 2007). "The Emergent Flux and Effective Temperature of δ Canis Majoris". Publications of the Astronomical Society of Australia 24 (3): 151–158. arXiv:0709.3873. Bibcode:2007PASA...24..151D. doi:10.1071/AS07017.
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- Kaler, James B. "Wezen". Stars website. University of Illinois. Retrieved 28 May 2010.
- 弧矢 (Hú Shǐ) is westernized into Koo She. R.H. Allen had opinion that Koo She refers to the asterism including δ Velorum and ω Velorum. AEEA opinion is, δ Velorum is member of 天社 (Tiān Shè), meaning Celestial Earth God's Temple asterism and ω Velorum is not member of any asterisms. 天社 (Tiān Shè) is westernized into Tseen She and R.H.Allen used the term Tseen She for Chinese name of η Carinae. See Richard Hinckley Allen: Star Names — Their Lore and Meaning: Argo Navis and (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 17 日.
- (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 17 日
- Knobel, E. B. (June 1895). "Al Achsasi Al Mouakket, on a catalogue of stars in the Calendarium of Mohammad Al Achsasi Al Mouakket". Monthly Notices of the Royal Astronomical Society 55: 429. Bibcode:1895MNRAS..55..429K. doi:10.1093/mnras/55.8.429.
- Allen, R. H. (1963). Star Names: Their Lore and Meaning (Reprint ed.). New York: Dover Publications Inc. p. 130. ISBN 0-486-21079-0. Retrieved 2010-12-12.
- ε CMa as Aoul al Adzari or Prima Virginum (the first virgin), ο2 CMa as Thanih al Adzari or Secunda Virginum (the second virgin) and δ CMa as Thalath al Adzari or Tertia Virginum (the third virgin). η CMa should be Rabah al Adzari or Quarta Virginum (the fourth virgin) consistently, but it was given by the name Aludra, meaning the virgin (same meaning with Adhara (ε CMa) or Al ʽAdhārā)
- Davis J, Booth AJ, Ireland MJ, Jacob AP, North JR, Owens SM, Robertson JG, Tango WJ, Tuthill PG, J.; Booth, A. J.; Ireland, M. J.; Jacob, A. P.; North, J. R.; Owens, S. M.; Robertson, J. G.; Tango, W. J.; Tuthill, P. G. (2007). "The Emergent Flux and Effective Temperature of Delta Canis Majoris". Publications of the Astronomical Society of Australia 24 (3): 151. arXiv:0709.3873. Bibcode:2007PASA...24..151D. doi:10.1071/AS07017.
- Ridpath, Ian; Tirion, Will (2003). The Monthly Sky Guide. Cambridge University Press. p. 16. ISBN 0-521-53306-6.
- "Astronomy of the Brazilian Flag". FOTW Flags Of The World website.