Lambda Herculis
| Observation data Epoch J2000 Equinox J2000 |
|
|---|---|
| Constellation | Hercules |
| Right ascension | 17h 30m 44.3099s[1] |
| Declination | +26° 06′ 38.323″[1] |
| Apparent magnitude (V) | 4.402[2] |
| Characteristics | |
| Spectral type | K4III[2] |
| U−B color index | +1.68[3] |
| B−V color index | +1.44[3] |
| Astrometry | |
| Radial velocity (Rv) | −26.51[4] km/s |
| Proper motion (μ) | RA: +18.39[1] mas/yr Dec.: +16.78[1] mas/yr |
| Parallax (π) | 8.88 ± 0.64[1] mas |
| Distance | 370 ± 30 ly (113 ± 8 pc) |
| Details | |
| Surface gravity (log g) | 1.89[5] cgs |
| Temperature | 4,070[5] K |
| Metallicity | ![\begin{smallmatrix}\left[\frac{Fe}{H}\right]\ =\ -0.04\end{smallmatrix}](/w/images/math/f/e/a/fea17f0f17cf0b9a80cae2deefdb18aa.png) [5] |
| Rotational velocity (v sin i) | 8[6] km/s |
| Other designations | |
Lambda Herculis (λ Her, λ Herculis) is a star in the constellation Hercules. It has the traditional name Maasym ("wrist").
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 λ Herculis, δ Herculis, μ Herculis, ο Herculis, 112 Herculis, ζ Aquilae, θ1 Serpentis, η Serpentis, ν Ophiuchi, ξ Serpentis and η Ophiuchi.[7] Consequently, λ Herculis itself is known as 天市左垣二 (Tiān Shì Zuǒ Yuán èr, English: the Second Star of Left Wall of Heavenly Market Enclosure), represent the state Zhao (or Chaou (趙)).,[8][9] together with 26 Capricorni and 27 Capricorni ("m Capricorni" in R.H.Allen version[10]) in Twelve States (asterism).
Structure
Lambda Herculis belongs to spectral class K3.5III and has apparent magnitude +4.4. It is approximately 370 light years from Earth.
In 1783, English astronomer William Herschel found that the Solar System is, as a whole, moving in a direction close to the position in the sky of Lambda Herculis.[11]
References
<templatestyles src="Reflist/styles.css" />
Cite error: Invalid <references> tag; parameter "group" is allowed only.
<references />, or <references group="..." /><templatestyles src="Asbox/styles.css"></templatestyles>
 |
This giant-star-related article is a stub. You can help Wikipedia by expanding it. |
- ↑ 1.0 1.1 1.2 1.3 1.4 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 2.0 2.1 2.2 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.
- ↑ 5.0 5.1 5.2 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ (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.
- ↑ (Chinese) English-Chinese Glossary of Chinese Star Regions, Asterisms and Star Name, Hong Kong Space Museum. Accessed on line November 23, 2010.
- ↑ Star Names - R.H.Allen p.142
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
