Kappa Canis Majoris
| Observation data Epoch J2000.0 Equinox J2000.0 |
|
|---|---|
| Constellation | Canis Major |
| Right ascension | 06h 49m 50.5s |
| Declination | −32° 30′ 31″ |
| Apparent magnitude (V) | +3.50 |
| Distance | 790 ± 96 ly (242 ± 29 pc) |
| Spectral type | B1.5IVne |
| Other designations | |
Kappa Canis Majoris (κ CMa, κ Canis Majoris) is a star in the constellation Canis Major. It is approximately 790 light years from Earth.
κ Canis Majoris is a blue-white B-type subgiant with a mean apparent magnitude of +3.50. This is a rapidly rotating Be star with 5.9 times the radius of the Sun.[1] It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +3.4 to +3.97.[2] It has become 50% brighter between 1963 and 1978, from magnitude 3.96 or so to 3.52.[3]
Naming
In Chinese, 弧矢 (Hú Shǐ), meaning Bow and Arrow,[4] refers to an asterism consisting of κ Canis Majoris, δ Canis Majoris, η Canis Majoris, HD 63032, HD 65456, ο Puppis, k Puppis, ε Canis Majoris and π Puppis. Consequently, κ Canis Majoris itself is known as 弧矢八 (Hú Shǐ bā, English: the Eighth Star of Bow and Arrow.)[5]
References
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- ↑ 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
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