- Mu Herculis
-
Mu Herculis Aa/B/C
Historical view of the Hercules constellation showing Mu Herculis (μ Her) as one of stars in the hero's elbow.Observation data
Epoch J2000 Equinox J2000Constellation Hercules Right ascension 17h 46m 27.52667s[1] Declination +27° 43′ 14.4379″[1] Apparent magnitude (V) 3.417 ± 0.014[1]/10.35/10.80 Characteristics Spectral type G5 IV[2]/M3.5 V/M4 V U−B color index 0.39/1.01 B−V color index 0.75/1.50 Variable type Periodic Astrometry Radial velocity (Rv) −16.1/-13.7 km/s Proper motion (μ) RA: −291.66[1]/-77.62 mas/yr
Dec.: −749.60[1]/-270.12 mas/yrParallax (π) 120.33 ± 0.16[1] mas Distance 27.11 ± 0.04 ly
(8.31 ± 0.01 pc)Absolute magnitude (MV) 3.80/10.73/11.18 Details Mass 1.00[2]/0.31/0.31 M☉ Radius 1.77 ± 0.07[2]/0.48/0.4 R☉ Luminosity 2.70 ± 0.16[2]/0.005/0.003 L☉ Temperature 5,596 ± 80[2] K Metallicity [Fe/H] 0.21 ± 0.07[2] dex Rotational velocity (v sin i) 20 km/s Age 6.43 ± 0.04[2] Gyr Other designations Mu Herculis is a nearby star system about 27.1 light years from Earth in the constellation Hercules. Its main star, Mu Herculis A is fairly similar to the Sun although more highly evolved with a [[stellar classification of G4 IV. Its mass is about 1.1 times that of the Sun, and it is beginning to expand to become a giant. The secondary component consists of a pair of stars that orbit about each other with a period of 43.2 years.[3] Mu Herculis A and the binary pair B-C are separated by 286 AUs. The stars B-C are separated from each other by 11.4 AUs. Their orbit is quite elliptic (e=0.18) and both stars swing each other between 9.4 and 13.5 AUs.[citation needed]
Contents
Etymology
In the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Marfak Al Jathih Al Aisr, which was translated into Latin as Cubitum Sinistrum Ingeniculi, meaning the left elbow of kneeling man.[4]
In Chinese, 天市左垣 (Tiān Shì Zuǒ Yuán), meaning Left Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states in China which is marking the left borderline of the enclosure, consisting of μ Herculis, δ Herculis, λ Herculis, ο Herculis, 112 Herculis, ζ Aquilae, θ1 Serpentis, η Serpentis, ν Ophiuchi, ξ Serpentis and η Ophiuchi[5]. Consequently, μ Herculis itself is known as 天市左垣三 (Tiān Shì Zuǒ Yuán sān, English: the Third Star of Left Wall of Heavenly Market Enclosure), represent Jiuhe (九河, lit. meaning nine rivers), possibly for Jiujiang, the prefecture-level city in Jiangxi, China, which is the same literally meaning with Jiuhe.[6][7]. From this Chinese title, the name Kew Ho was appeared[8]
Star system
Star A is itself suspected to be a close binary with a low mass stellar or a large substellar companion, probably at 17.2 AUs in an elliptic orbit. Nevertheless the existence of such an object has still not been confirmed.[citation needed]
References
- ^ a b c d e f van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, Bibcode 2007A&A...474..653V, doi:10.1051/0004-6361:20078357
- ^ a b c d e f g Yang, Wuming; Meng, Xiangcun (April 2010), "Models of μ Her with asteroseismic constraints", New Astronomy 15: 367–372, Bibcode 2010NewA...15..367Y, doi:10.1016/j.newast.2009.11.001
- ^ Turner, Nils H. et al. (June 2001), "Search for Faint Companions to Nearby Solar-like Stars using the Adaptive Optics System at Mount Wilson Observatory", The Astronomical Journal (6): 3254–3258, Bibcode 2001AJ....121.3254T, doi:10.1086/321075
- ^ 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
- ^ (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 23 日
- ^ (Chinese) English-Chinese Glossary of Chinese Star Regions, Asterisms and Star Name, Hong Kong Space Museum. Accessed on line November 23, 2010.
- ^ Star Name - R.H. Allen p. 238
External links
- Jim Kaler's Stars, University of Illinois: MU HER (Mu Herculis)
- SolStation: Mu Hercules4
Star systems (including brown dwarf systems) within 25–30 light-years from Earth. Pi³ Orionis «Tabit» (26.2 ± 0.2 ly; 1 star) • Chi Draconis (26.22 ± 0.11 ly; 2 stars) • Zeta Tucanae (28.0 ± 0.2 ly; 1 star) • Gamma Leporis (29.3 ± 0.2 ly; 2 stars) • Gamma Pavonis (30.1 ± 0.2 ly; 1 star)‡Mu Herculis (27.4 ± 0.2 ly; 3 stars)Xi Ursae Majoris «Alula Australis» (27.25 ± 0.18 ly; 3 stars, 1 brown dwarf) • Beta Canum Venaticorum «Chara» (27.3 ± 0.2 ly; 1 star) • 61 Virginis (27.8 ± 0.2 ly; 1 star, 3 planets: planet b • planet c • planet d) • Chi¹ Orionis (28.3 ± 0.3 ly; 2 stars) • 41 G. Arae (28.7 ± 0.3 ly; 2 stars) • Beta Comae Berenices (29.9 ± 0.2 ly; 1 star)‡ • Kappa¹ Ceti (29.9 ± 0.2 ly; 1 star)‡ • HR 4523 (30.1 ± 0.2 ly; 2 stars, 1 planet: planet b)‡Groombridge 1830 (29.9 ± 0.2 ly; 1 star)‡Delta Eridani «Rana» (29.5 ± 0.3 ly; 1 star)TW Piscis Austrini (24.9 ± 0.2 ly; 1 star)‡ • Gliese 673 (25.2 ± 0.2 ly; 1 star)‡ • Gliese 884 (26.6 ± 0.3 ly; 1 star) • p Eridani (26.6 ± 0.3 ly; 2 stars) • Gliese 250 (28.4 ± 0.3 ly; 2 stars) • HR 1614 (28.8 ± 0.3 ly; 1 star) • HR 7722 (28.8 ± 0.3 ly; 1 star, 2 planets: planet b • planet c)Gliese 623 (26.2 ± 0.3 ly; 2 stars) • AP Columbae (27.4 ± 0.2 ly; 1 star) • Gliese 185 (27.8 ± 0.4 ly; 2 stars) • Gliese 745 (28.1 ± 0.6 ly; 2 stars) • Gliese 849 (28.6 ± 0.5 ly; 1 star, 1 planet: planet b) • Gliese 433 (29.5 ± 0.5 ly; 1 star, 1 planet: planet b) • Gliese 317 (29.9 ± 5.5 ly; 1 star: Gliese 317; 1 (2?) planets: planet b • planet c?)‡DAGJ 1087 (26.1 ± 0.8 ly; 1 star) • Gliese 915 (26.7 ± 0.3 ly; 1 star) • Gliese 318 (28.7 ± 0.5 ly; 1 star)DCGliese 293 (25.8 ± 0.3 ly; 1 star)DQGJ 2012 (29.5 ± 0.3 ly; 1 star)DZGliese 518 (26.9 ± 0.8 ly; 1 star) • GJ 1276 (27.9 ± 0.2 ly; 1 star) • Gliese 283 (29.7 ± 0.2 ly; 2 stars)SDSS J1416+13 (25.7 ± 5.5 ly; 2 brown dwarfs)‡ • WISE 1647+5632 (28.1 + 9.4/- 5.6 ly; 1 brown dwarf)‡ • 2MASS 0036+1821 (28.6 ± 0.2 ly; 1 brown dwarf)WISE 0254+0223 (19.8 + 7.6/- 4.3 ly; 1 brown dwarf)‡ • WISE 0313+7807 (~26.4 ly; 1 brown dwarf)‡ • UGPS J0521+3640 (26.7 + 3.9/- 3.2 ly; 1 brown dwarf)‡ • 2MASS 0727+1710 (29.6 ± 0.6 ly; 1 brown dwarf)‡ • CFBDS J005910.90-011401.3 (30.1 + 1.5/- 1.3 ly; 1 brown dwarf)‡ • WISE 2313-8037 (30.3 ± 1.3 ly; 1 brown dwarf)‡ • WISE 0458+6434 (34.2 ± 4.6 ly; 2 brown dwarfs)‡WISE 0410+1502 (23.2 + 5.2/- 12.7 ly; 1 brown dwarf)‡In left column are stellar classes of primary members of star systems. ‡Distance error margin extends out of declared distance interval. Bold are systems containing at least one component with absolute magnitude of +8.5 or brighter. Italic are systems possibly located within declared distance interval, but probably not. Nearest bright star systems Star systems within 30 light-years from Earth with brightest member's absolute magnitude of +8.5 or brighter. 0–10 ly → Sirius (8.58 ± 0.03 ly; 2 stars)Solar System (0 ly; 1 star, 8 planets) • Alpha Centauri (4.365 ± 0.007 ly; 3 stars: Alpha¹ Centauri • Alpha² Centauri • Proxima Centauri (4.242 ± 0.002 ly))Altair (16.69 ± 0.04 ly; 1 star)Procyon (11.44 ± 0.02 ly; 2 stars)Tau Ceti (11.905 ± 0.007 ly; 1 star) • Sigma Draconis «Alsafi» (18.77 ± 0.02 ly; 1 star) • Eta Cassiopeiae «Achird» (19.39 ± 0.05 ly; 2 stars) • e (82 G.) Eridani (19.71 ± 0.02 ly; 1 star, 3 planets: planet b • planet c • planet d) • Delta Pavonis (19.92 ± 0.02 ly; 1 star)Epsilon Eridani (10.480 ± 0.003 ly; 1 star, 2 planets: planet b • planet c) • 61 Cygni (11.40 ± 0.02 ly; 2 stars) • Epsilon Indi (11.81 ± 0.01 ly; 1 star, 2 brown dwarfs) • Groombridge 1618 (15.87 ± 0.04 ly; 1 star) • Omicron² (40) Eridani «Keid» (16.25 ± 0.02 ly; 3 stars) • 70 Ophiuchi (16.64 ± 0.07 ly; 2 stars) • 33 G. Librae (19.12 ± 0.08 ly; 3 stars, 1 brown dwarf) • 36 Ophiuchi (19.40 ± 0.05 ly; 3 stars) • Gliese 783 (19.62 ± 0.04 ly; 2 stars)Pi³ Orionis «Tabit» (26.2 ± 0.2 ly; 1 star) • Chi Draconis (26.22 ± 0.11 ly; 2 stars) • Zeta Tucanae (28.0 ± 0.2 ly; 1 star) • Gamma Leporis (29.3 ± 0.2 ly; 2 stars) • Gamma Pavonis (30.1 ± 0.2 ly; 1 star)‡Beta Hydri (24.4 ± 0.1 ly; 1 star) • Mu Herculis (27.4 ± 0.2 ly; 3 stars)Xi Boötis (22.1 ± 0.2 ly; 2 stars) • Xi Ursae Majoris «Alula Australis» (27.25 ± 0.18 ly; 3 stars, 1 brown dwarf) • Beta Canum Venaticorum «Chara» (27.3 ± 0.2 ly; 1 star) • 61 Virginis (27.8 ± 0.2 ly; 1 star, 3 planets: planet b • planet c • planet d) • Chi¹ Orionis (28.3 ± 0.3 ly; 2 stars) • 41 G. Arae (28.7 ± 0.3 ly; 2 stars) • Beta Comae Berenices (29.9 ± 0.2 ly; 1 star)‡ • Kappa¹ Ceti (29.9 ± 0.2 ly; 1 star)‡ • HR 4523 (30.1 ± 0.2 ly; 2 stars, 1 planet: planet b)‡Mu Cassiopeiae «Marfak-West» (24.6 ± 0.2 ly; 2 stars) • Groombridge 1830 (29.9 ± 0.2 ly; 1 star)‡Delta Eridani «Rana» (29.5 ± 0.3 ly; 1 star)Gliese 892 (21.34 ± 0.04 ly; 1 star) • HR 753 (23.5 ± 0.2 ly; 3 stars) • Gliese 667 (23.6 ± 0.1 ly; 3 stars, 1 planet: planet Cb) • Gliese 33 (24.3 ± 0.2 ly; 1 star) • 107 Piscium (24.4 ± 0.2 ly; 1 star) • TW Piscis Austrini (24.9 ± 0.2 ly; 1 star) • Gliese 673 (25.2 ± 0.2 ly; 1 star) • Gliese 884 (26.6 ± 0.3 ly; 1 star) • p Eridani (26.6 ± 0.3 ly; 2 stars) • Gliese 250 (28.4 ± 0.3 ly; 2 stars) • HR 1614 (28.8 ± 0.3 ly; 1 star) • HR 7722 (28.8 ± 0.3 ly; 1 star, 2 planets: planet b • planet c)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 likely not. Total about 50 (47–52) systems. Stars of Hercules Bayer α (Rasalgethi) • β (Kornephoros) • γ • δ (Sarin) • ε (Cujam) • ζ (Rutilicus) • η • θ • ι • κ (Marfik) • λ (Maasym) • μ • ν • ξ • ο (Atia) • π • ρ • σ • τ • υ • φ • χ • ω (Kajam) • b • c • d • e • f • g • h • i • k • l • m • n • o • q • r • s • t • u • w • x • y • z • AFlamsteed 1 (χ) • 2 • 4 • 5 (r) • 6 (υ) • 7 (κ, Marfik) • 8 • 9 • 10 • 11 (φ) • 13 • 14 • 16 • 19 • 20 (γ) • 21 (o) • 22 (τ) • 24 (ω, Kajam) • 25 • 27 (β, Kornephoros) • 28 (n) • 29 (h) • 30 (g) • 31 • 32 • 33 • 34 • 35 (σ) • 36 • 37 (m) • 38 • 39 • 40 (ζ, Rutilicus) • 41 • 42 • 43 (i) • 44 (η) • 45 (l) • 46 • 47 (k) • 48 • 49 • 50 • 51 • 52 • 53 • 54 • 56 • 57 • 58 (ε, Cujam) • 59 (d) • 60 • 61 • 63 • 64 (α, Rasalgethi) • 65 (δ, Sarin) • 67 (π) • 68 (u) • 69 (e)• 70 • 72 (w) • 73 • 74 • 75 (ρ) • 76 (λ, Maasym) • 77 (x) • 78 • 79 • 82 (y) • 83 • 84 • 85 (ι) • 86 (μ) • 87 • 88 (z) • 89 • 90 (f) • 91 (θ) • 92 (ξ) • 93 • 94 (ν) • 95• 96 • 97 • 98 • 99 (b) • 100 • 101 • 102 • 103 (ο, Atia) • 104 (A) • 105 • 106 • 107 (t) • 108 • 109 • 110 • 111 • 112 • 113Nearby WISE 1738+2732 • WISE 1741+2553List This binary or multiple star system-related article is a stub. 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