- Theta Centauri
-
θ Centauri Observation data
Epoch J2000.0 Equinox J2000.0Constellation Centaurus Right ascension 14h06m41.3s Declination -36°22′07.3″ Apparent magnitude (V) +2.06 Characteristics Spectral type K0IIIb U−B color index +0.88 B−V color index +1.01 Variable type none Astrometry Radial velocity (Rv) +1.3 km/s Proper motion (μ) RA: -519.29 mas/yr
Dec.: -517.87 mas/yrParallax (π) 53.52 ± 0.79 mas Distance 60.9 ± 0.9 ly
(18.7 ± 0.3 pc)Absolute magnitude (MV) +0.70 Details Mass 4 M☉ Radius 16 R☉ Luminosity 45 L☉ Temperature 4,500 K Other designations Theta Centauri (θ Cen, θ Centauri) is a star in the constellation Centaurus. It is also has the traditional Arabic name Menkent (possibly abbreviation of ألمنكب ألقنتوس - al mankib al-qanturis, meaning "shoulder of the Centaur"). It is an orange K-type giant with an apparent magnitude of +2.06 and is approximately 60.94 light years from Earth.
In Chinese, 庫樓 (Kù Lóu), meaning Arsenal, refers to an asterism consisting of θ Centauri, ζ Centauri, η Centauri, 2 Centauri, HD 117440, ξ1 Centauri, γ Centauri, τ Centauri, D Centauri and σ Centauri.[1] Consequently, θ Centauri itself is known as 庫樓三 (Kù Lóu sān, English: the Third Star of Arsenal.)[2]
References
- ^ (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) 香港太空館 - 研究資源 - 亮星中英對照表, Hong Kong Space Museum. Accessed on line November 23, 2010.
Star systems within 60–70 light-years from Earth with brightest member's absolute magnitude of +8.5 or brighter.Rho Puppis «Tureis» (62.7 ± 0.8 ly; 1 star)Theta Centauri «Menkent» (60.9 ± 0.9 ly; 1 star) • Aldebaran (65.1 ± 1.3 ly; 2 stars) • Epsilon Scorpii «Wei» (65.4 ± 1.1 ly; 1 star) • Alpha Arietis «Hamal» (65.9 ± 1.3 ly; 1 star, 1 planet: planet b)Beta Arietis «Sheratan» (59.6 ± 0.8 ly; 2 stars)‡ • Beta Pictoris (62.9 ± 0.6 ly; 1 star, 1 planet: planet b)Psi Velorum (59.7 ± 1.0 ly; 2 stars)‡ • Mu Virginis (60.9 ± 1.1 ly; 1 star)‡ • Alpha Chamaeleontis (63.5 ± 0.6 ly; 1 star) • Alpha Trianguli «Metallah» (64.1 ± 1.0 ly; 2 stars) • Eta Crucis (64.2 ± 0.6 ly; 2 stars) • Tau Cygni (66.4 ± 0.8 ly; 4 stars) • Theta Draconis (68.3 ± 0.8 ly; 2 stars) • Iota Virginis «Syrma» (69.8 ± 1.3 ly; 1 star)‡Chi Cancri (59.2 ± 1.0 ly; 1 star)‡ • Eta Corvi «Avis Satyra» (59.4 ± 0.7 ly; 1 star)‡ • Delta Equulei «Pherasauval» (60.0 ± 1.0 ly; 2 stars)‡ • Theta Cygni (60.7 ± 0.5 ly; 2 stars) • HR 1249 (62.7 ± 0.9 ly; 1 star) • 1 Centauri (62.8 ± 0.9 ly; 2 stars) • Omicron Aquilae (63.3 ± 0.9 ly; 3 stars) • c (45) Boötis (64.3 ± 1.0 ly; 2 stars) • Alpha Caeli (65.7 ± 0.7 ly; 2 stars) • Kappa Tucanae (66.04 ± 1.2 ly; 4 stars) • Gamma Doradus (66.2 ± 0.7 ly; 1 star) • Sigma² Ursae Majoris (66.7 ± 0.9 ly; 3 stars) • HR 1686 (68.4 ± 0.8 ly; 2 stars, 1 planet: planet b) • B Carinae (69.8 + 5.4/- 4.7 ly; 1 star)‡94 Aquarii (67.6 + 8.3/- 6.6 ly; 2 stars)‡ • Gliese 848.4 (69.4 ± 1.2 ly; 1 star, 1 planet: planet b)‡HD 217107 (64.3 ± 1.0 ly; 1 star, 2 planets: planet b • planet c) • 53 Aquarii (65.5 ± 3.5 ly; 2 stars) • GJ 3255 (67.4 ± 1.5 ly; 1 star, 1 planet: planet b) • 51 Arietis (69.0 ± 1.3 ly; 1 star)‡ • c (16) Cygni (69.8 ± 0.8 ly; 2 stars, 1 planet: planet Bb)‡Epsilon Reticuli (59.5 ± 0.5 ly; 1 star, 1 planet: planet b)‡ • Eta Serpentis «Tang» (61.8 ± 0.9 ly; 1 star) • Nu² Canis Majoris (64.7 ± 0.9 ly; 1 star, 1 planet: planet b)GJ 4130 (62.8 ± 1.1 ly; 2 stars, 1 planet: planet b) • Gliese 710 (63.0 ± 1.8 ly; 1 star) • HD 192263 (64.9 ± 1.5 ly; 1 star, 1 planet: planet b) • GJ 3769 (66.6 ± 1.5 ly; 1 star, 1 planet: planet b) • GJ 3651 (69.5 ± 1.5 ly; 1 star, 1 planet: planet b)‡ • GJ 4291 (70.2 ± 2.0 ly; 1 star, 1 planet: planet b)‡In left column are stellar classes of primary members of star systems. ‡Distance error margin extends out of declared distance interval. Italic are systems possibly located within declared distance interval, but probably not.Stars of Centaurus Bayer Flamsteed Categories:- Bayer objects
- Flamsteed objects
- Centaurus constellation
- K-type giants
- Stars with proper names
- Giant star stubs
Wikimedia Foundation. 2010.