Xi Serpentis

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Template:Short description

ξ Serpentis
Template:Location mark
Location of ξ Serpentis (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Serpens
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 3.54[2]
Characteristics
Spectral type A9 IIIp Sr[3]
U−B Template:Engvar +0.12[2]
B−V Template:Engvar +0.27[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[4] km/s
Proper motion (μ) RA: −42.10[1] mas/yr
Dec.: −59.94[1] mas/yr
Parallax (π)30.98±0.19 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+1.00[5]
Orbit[6]
Period (P)2.2923 d
Eccentricity (e)0.00
Periastron epoch (T)2419210.191 JD
Semi-amplitude (K1)
(primary)
19.4 km/s
Details
ξ Ser Aa
Mass2.06[7] Template:Solar mass
Radius3.695[8] Template:Solar radius
Luminosity30.6[9] Template:Solar luminosity
Surface gravity (log g)3.55[3] cgs
TemperatureScript error: No such module "val".[7] K
Metallicity [Fe/H]+0.07[3] dex
Rotational velocity (v sin i)54[10] km/s
Age1.03[7] Gyr
ξ Ser Ab
Mass0.18[11] Template:Solar mass
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[12]
Database references
SIMBADdata

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Xi Serpentis, Latinized from ξ Serpentis, is a triple star[11] system in the Serpens Cauda (tail) section of the equatorial constellation Serpens. Based upon an annual parallax shift of 30.98 mas as seen from Earth,[1] it is located 105.3 light years from the Sun. The star system is visible to the naked eye with a base apparent visual magnitude of +3.54.[2] It is moving closer to the Sun and will make perihelion passage at a distance of Script error: No such module "convert". in around 690,000 years.[13]

The inner pair form a single-lined spectroscopic binary with an orbital period of 2.29 days following a circular orbit.[6] The primary, component Aa, has a visual magnitude of 3.54.[14] It is a white-hued G-type giant star with a stellar classification of A9 IIIp Sr.[3] This indicates it is a chemically peculiar Ap star with an abnormal abundance of strontium. The primary has around double the mass of the Sun, while its close companion,[7] component Ab,[14] has only 18% of the Sun's mass.[11]

The third member, component B, is a magnitude 13.0[14] common proper motion companion.[11] As of 2012, it was located at an angular separation of 24 arc seconds along a position angle of 78° from the inner pair.[14] It has about 27% of the Sun's mass and an estimated orbital period of 14,763 years.[11]

Name

In Chinese, Tiān Shì Zuǒ Yuán (Script error: No such module "Lang".), meaning Left Wall of Heavenly Market Enclosure, refers to an asterism which represents eleven old states (and region) in China and which marks the left borderline of the enclosure, consisting of ξ Serpentis, δ Herculis, λ Herculis, μ Herculis, ο Herculis, 112 Herculis, ζ Aquilae, η Serpentis, θ1 Serpentis, ν Ophiuchi and η Ophiuchi.[15] Consequently, the Chinese name for ξ Serpentis itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx), representing the region of Nanhai (南海, lit. meaning southern sea)[16][17]

References

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  5. Script error: No such module "citation/CS1".
  6. a b Script error: No such module "citation/CS1".
  7. a b c d Script error: No such module "citation/CS1".
  8. Script error: No such module "citation/CS1". Xi Serpentis' database entry at VizieR.
  9. Script error: No such module "citation/CS1".
  10. Script error: No such module "citation/CS1".
  11. a b c d e Script error: No such module "citation/CS1".
  12. Template:Cite simbad
  13. Script error: No such module "citation/CS1".
  14. a b c d Script error: No such module "citation/CS1".
  15. Template:In lang 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, Template:ISBN.
  16. Template:In lang AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 23 日 Script error: No such module "webarchive".
  17. Template:In lang English-Chinese Glossary of Chinese Star Regions, Asterisms and Star Name Script error: No such module "webarchive"., Hong Kong Space Museum. Accessed on line November 23, 2010.

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Template:Stars of Serpens