- Delta Boötis
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δ Boötis Observation data
Epoch J2000 Equinox J2000Constellation Boötes Right ascension 15h 15m 30.163s Declination +33° 18′ 53.401″ Apparent magnitude (V) 3.47 Characteristics Spectral type G8IIIFe-1 U−B color index 0.66 B−V color index 0.95 R−I color index 0.51 Variable type Variable star Astrometry Radial velocity (Rv) -12.3 km/s Proper motion (μ) RA: 84.84 mas/yr
Dec.: -110.57 mas/yrParallax (π) 27.94 ± 0.61 mas Distance 117 ± 3 ly
(35.8 ± 0.8 pc)Absolute magnitude (MV) 4.42 Details Mass 1.1 M☉ Radius 1.1 R☉ Luminosity 1.2 L☉ Temperature 5,000–6,000 K Rotation < 19 km/s Other designations Database references SIMBAD data Data sources: Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)Database references SIMBAD data Delta Boötis (δ Boo, δ Boötis) is a binary star in the constellation Boötes. It is approximately 117 light years from Earth. The primary component is a yellow G-type giant with an apparent magnitude of +3.46. Its companion is a yellow G-type main sequence dwarf with an apparent magnitude of +8.7.
Sometimes, this star is called by the name Princeps, meaning prince or prime in Latin[1].
In Chinese, 七公 (Qī Gōng), meaning Seven Excellencies, refers to an asterism consisting of δ Boötis, 42 Herculis, τ Herculis, φ Herculis, χ Herculis, ν1 Boötis and μ1 Boötis.[2] Consequently, δ Boötis itself is known as 七公七 (Qī Gōng qī, English: the Seventh Star of Seven Excellencies.)[3]
About 3800 AU apart, the two take about 120,000 years to orbit each other.
References
- ^ Constellations of Word - Boötes (Princeps)
- ^ (Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.
- ^ (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 26 日
Categories:- Variable star stubs
- Multiple star stubs
- Flamsteed objects
- Henry Draper Catalogue objects
- HIP objects
- Bayer objects
- Boötes constellation
- Binary stars
- G-type giants
- G-type main sequence stars
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