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Xi Ophiuchi

From Wikipedia, the free encyclopedia
Visual binary star system in the constellation Ophiuchus
Xi Ophiuchi
Location of ξ Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationOphiuchus
Right ascension17h 21m 00.37452s[1]
Declination−21° 06′ 46.5710″[1]
Apparent magnitude (V)4.39[2]
Characteristics
Spectral typeF2V[3]
U−Bcolor index−0.06[4]
B−Vcolor index+0.41[4]
Astrometry
Radial velocity (Rv)−8.73±0.12[1] km/s
Proper motion (μ)RA: +265.543mas/yr[1]
Dec.: −202.584mas/yr[1]
Parallax (π)57.0820±0.1851 mas[1]
Distance57.1 ± 0.2 ly
(17.52 ± 0.06 pc)
Absolute magnitude (MV)3.19[2]
Details[5]
A
Mass1.30 M
Radius1.59±0.06 R
Luminosity4.429±0.035[6] L
Surface gravity (log g)4.15±0.10 cgs
Temperature6,611±80 K
Metallicity [Fe/H]−0.27±0.07 dex
Rotational velocity (v sin i)20.2±0.7 km/s
Age916[7] Myr
Other designations
ξ Oph,40 Ophiuchi,BD−20°4731,FK5 917,GC 23423,HD 156897,HIP 84893,HR 6445,SAO 185296,CCDM J17210-2107AB,WDS J17210-2107AB,LTT 6908[8]
Database references
SIMBADdata

ξ Oph,Latinized asXi Ophiuchi, is a visualbinary star[9] system in theequatorialconstellation ofOphiuchus.[2] It has a yellow-white hue and is faintly visible to the naked eye with a combinedapparent visual magnitude of 4.39.[2] The system is located approximately 57.1light-years (17.5parsecs) away from the Sun based onparallax, but is drifting closer with aradial velocity of -9 km/s.[1]

The magnitude 4.40[10] primary, designated component A, is an ordinaryF-type main-sequence star with astellar classification of F2V.[3] It is 916[7] million years old and is rotating with aprojected rotational velocity of 20 km/s. The star has 1.3 times themass of the Sun and 1.6 times theSun's radius.[5] It is radiating 4.4[6] times theluminosity of the Sun from itsphotosphere at aneffective temperature of 6,611 K.[5]

The system is a source ofX-ray emission.[11] The orbiting companion, component B, is a magnitude 8.9 star at anangular separation of35 along aposition angle of 27° from the primary, as of 2015. A magnitude 10.8visual companion, component C, lies at a separation of10.8″, as of 2004.[10]

According to Richard H. Allen'sStar Names: Their Lore and Meaning (1899), ξ Oph together withθ Oph formed theSogdianWajrik "the Magician", the KhorasmianMarkhashik "the Serpent-bitten" and withη Oph theCopticTshiō, "the Snake", andAggia, "the Magician".[12] The name Aggia for this star appears in a 1971 NASA list of star names[13] and in a 2023 list of target stars for theHabitable Worlds Observatory.[14] As of April 2025[update], it does not appear in theIAU Catalog of Star Names.[15]

References

[edit]
  1. ^abcdefVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  2. ^abcdAnderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5): 331.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.S2CID 119257644.Vizier catalog entry
  3. ^abGray, R. O.; Corbally, C. J.; Garrison, R. F.; McFadden, M. T.; Bubar, E. J.; McGahee, C. E.; O'Donoghue, A. A.; Knox, E. R. (2006). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 pc--The Southern Sample".The Astronomical Journal.132 (1):161–170.arXiv:astro-ph/0603770.Bibcode:2006AJ....132..161G.doi:10.1086/504637.S2CID 119476992.
  4. ^abMallama, A. (2014). "Sloan Magnitudes for the Brightest Stars".The Journal of the American Association of Variable Star Observers.42 (2): 443.Bibcode:2014JAVSO..42..443M.Vizier catalog entry
  5. ^abcFuhrmann, K.; Chini, R.; Kaderhandt, L.; Chen, Z. (2017)."Multiplicity among Solar-type Stars".The Astrophysical Journal.836 (1): 139.Bibcode:2017ApJ...836..139F.doi:10.3847/1538-4357/836/1/139.
  6. ^abBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  7. ^abDavid, Trevor J.; Hillenbrand, Lynne A. (2015). "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets".The Astrophysical Journal.804 (2): 146.arXiv:1501.03154.Bibcode:2015ApJ...804..146D.doi:10.1088/0004-637X/804/2/146.S2CID 33401607.Vizier catalog entry
  8. ^"ksi Oph".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-10-08.
  9. ^Eggleton, P. P.; Tokovinin, A. A. (September 2008)."A catalogue of multiplicity among bright stellar systems".Monthly Notices of the Royal Astronomical Society.389 (2):869–879.arXiv:0806.2878.Bibcode:2008MNRAS.389..869E.doi:10.1111/j.1365-2966.2008.13596.x.S2CID 14878976.
  10. ^abMason, Brian D.; et al. (200)."The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog".The Astronomical Journal.122 (6): 3466.Bibcode:2001AJ....122.3466M.doi:10.1086/323920.Vizier catalog entry
  11. ^Haakonsen, Christian Bernt; Rutledge, Robert E. (September 2009). "XID II: Statistical Cross-Association of ROSAT Bright Source Catalog X-ray Sources with 2MASS Point Source Catalog Near-Infrared Sources".The Astrophysical Journal Supplement.184 (1):138–151.arXiv:0910.3229.Bibcode:2009ApJS..184..138H.doi:10.1088/0067-0049/184/1/138.S2CID 119267456.
  12. ^Allen, R.H. (1899),Star Names: Their Lore and Meaning, p. 297
  13. ^Rhoads, Jack W. (November 15, 1971),Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars(PDF), Jet Propulsion Laboratory, California Institute of Technology.
  14. ^Mamajek, Eric; Stapelfeldt, Karl (January 2023).NASA Exoplanet Exploration Program (ExEP) Mission Star List for the Habitable Worlds Observatory (2023)(PDF) (Report).arXiv:2402.12414. JPL CL#23-0611.
  15. ^"IAU Catalog of Star Names". Retrieved22 February 2025.
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