Kappa Ursae Majoris
From Infogalactic: the planetary knowledge core
Observation data Epoch J2000.0 Equinox J2000.0 |
|
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Constellation | Ursa Major |
Right ascension | 09h 03m 37.52762s[1] |
Declination | +47° 09′ 23.4890″[1] |
Apparent magnitude (V) | +3.60[2] |
Characteristics | |
Spectral type | A0IV-V + A0V[3] |
Astrometry | |
Distance | 358 ± 20 ly (109 ± 6[1] pc) |
Other designations | |
Database references | |
SIMBAD | data |
Kappa Ursae Majoris (Kappa UMa, κ Ursae Majoris, κ UMa) is a binary star in the constellation Ursa Major. It is approximately 358 light years from Earth and has the traditional names Talitha Australis, Al Kaprah, and Alphikra Australis.
Both components of the binary star are a white A-type main sequence dwarfs. They have apparent magnitudes of +4.2 and +4.4,[citation needed] which gives the system a combined apparent magnitude of +3.60.[2] The orbital period of the binary is 35.6 years (13,007.2 days), and the two stars are separated by 0.18 arcseconds.[4]
Name and etymology
- The traditional name Talitha' (share with ι UMa) comes from the Arabic phrase Al Fiḳrah al Thalitha "the third spring, or leap, of the ghazal".[5] The term Australis meaning "the south side" in Latin.
- In Chinese, 三台 (Sān Tái), meaning Three Steps, refers to an asterism consisting of κ Ursae Majoris, ι Ursae Majoris, λ Ursae Majoris, μ Ursae Majoris, ν Ursae Majoris and ξ Ursae Majoris. Consequently, κ Ursae Majoris itself is known as 三台二 (Sān Tái èr, English: the Second Star of Three Steps) and 上台二 (Shàng Tái èr, English: Star of Second Upper Step).[6]
References
- ↑ 1.0 1.1 1.2 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 2.0 2.1 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 3.0 3.1 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Richard Hinckley Allen :Star Names — Their Lore and Meaning - Ursa Major, the Greater Bear
- ↑ (Chinese) (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 21 日
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