Mu Herculis
Appearance
Coordinates: 17h 46m 27.52667s, +27° 43′ 14.4379″
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 J2000 | ||
---|---|---|
Constellation | Hercules | |
μ Her Aab (μ1 Her) | ||
Right ascension | 17h 46m 27.52667s[1] | |
Declination | +27° 43′ 14.4379″[1] | |
Apparent magnitude (V) | 3.417 ± 0.014[1] | |
μ Her BC (μ2 Her) | ||
Right ascension | 17h 46m 25.079s[2] | |
Declination | +27° 43′ 01.45″[2] | |
Apparent magnitude (V) | 10.2 / 10.7[3] | |
Characteristics | ||
μ Her Aab | ||
Spectral type | G5IV[4] / M4V[5] | |
U−B color index | +0.40[6] | |
B−V color index | +0.76[6] | |
μ Her BC | ||
Spectral type | M3.5V[7] | |
U−B color index | +1.00[6] | |
B−V color index | +1.50[6] | |
Absolute magnitude (MV) | +10.26[11] | |
Position (relative to μ Her Aab)[12] | ||
Component | μ Her BC | |
″ | ||
Semi-amplitude (K1)(primary) | 1.12 ± 0.10 km/s | |
Argument of periastron (ω)(secondary) | 172.85 ± 0.64° | |
Details | ||
μ Her Aa | ||
Gyr | ||
μ Her Ab | ||
Mass | 0.32[5] M☉ | |
μ Her B | ||
dex | ||
μ Her C | ||
Mass | 0.39[13] M☉ | |
HIP 86974.[15] | ||
Database references | ||
SIMBAD | μ Her Aab | |
μ Her BC |
Mu Herculis (μ Herculis) is a nearby quadruple
spectrum of this star has served as one of the stable anchor points by which other stars are classified.[16] Its mass is about 1.1 times that of the Sun,[8]
and it is beginning to expand to become a giant.
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.[17]
In
Chinese name for μ Herculis itself is 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.[19][20] From this Chinese title, the name Kew Ho appeared.[21]
Star system
Mu Herculis is a quadruple star system. The brightest star is a well-studied
spectral type of M4V and a mass of 0.32 M☉.[5]
This pair is also known as Mu1 Herculis.
The secondary component, also known as Mu2 Herculis,[12] consists of a pair of stars that orbit about each other with a period of about 43 years.[22] Mu Herculis A and the binary pair B-C are separated by some 35 arcseconds.[15] The stars B and C, which orbit each other, are separated from each other by 1.385 arcseconds, and have a slightly eccentric orbit, at 0.1796.[3]
See also
References
- ^ S2CID 18759600
- ^ Bibcode:2003yCat.2246....0C.
- ^ a b c "Sixth Catalog of Orbits of Visual Binary Stars". United States Naval Observatory. Archived from the original on 1 August 2017. Retrieved 23 March 2017.
- S2CID 119121800
- ^ S2CID 43403927.
- ^ Bibcode:1986EgUBV........0M.
- S2CID 53135130.[permanent dead link]
- ^ S2CID 119480210.
- ^ S2CID 17350617.
- .
- S2CID 9719725.
- ^ a b "* mu.02 Her". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 24 May 2017.
- ^ a b "Multiple Star Catalog". Archived from the original on 2018-12-03. Retrieved 2018-12-02.
- ^ .
- ^ a b "* mu. Her". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 24 May 2017.
- Bibcode:1993AAS...183.1710G, archived from the originalon 2019-06-25, retrieved 2012-02-04
- ISBN 978-986-7332-25-7.
- ^ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 23 日
- ^ (in Chinese) English-Chinese Glossary of Chinese Star Regions, Asterisms and Star Name Archived 2010-08-10 at the Wayback Machine, Hong Kong Space Museum. Accessed on line November 23, 2010.
- ^ Star Name - R.H. Allen p. 238
- doi:10.1086/321075
External links
- Jim Kaler's Stars, University of Illinois: MU HER (Mu Herculis)
- SolStation: Mu Herculis 4