Visual binary star system in the constellation Ophiuchus
Xi Ophiuchi
Location of ξ Ophiuchi (circled)
Observation dataEpoch J2000 Equinox J2000
Constellation
Ophiuchus
Right ascension
17h 21m 00.37452s [ 1]
Declination
−21° 06′ 46.5710″[ 1]
Apparent magnitude (V)
4.39[ 2]
Characteristics
Spectral type
F2V[ 3]
U−B color index
−0.06[ 4]
B−V color index
+0.41[ 4]
Astrometry Radial velocity (Rv ) −8.73± 0.12[ 1] km/s Proper motion (μ) RA: +265.543 mas /yr [ 1] Dec.: −202.584 mas /yr [ 1] Parallax (π)57.0820± 0.1851 mas [ 1] Distance 57.1 ± 0.2 ly (17.52 ± 0.06 pc ) Absolute magnitude (MV )3.19[ 2]
Details[ 5] A Mass 1.30 M ☉ Radius 1.59± 0.06 R ☉ Luminosity 4.429± 0.035[ 6] L ☉ Surface gravity (log g ) 4.15± 0.10 cgs Temperature 6,611± 80 K Metallicity [Fe/H] −0.27± 0.07 dex Rotational velocity (v sin i ) 20.2± 0.7 km/sAge 916[ 7] Myr
Other designations ξ Oph , 40 Oph , BD −20°4731 , FK5 917 , GC 23423 , GJ 670 , HD 156897 , HIP 84893 , HR 6445 , SAO 185296 , CCDM J17210-2107AB , WDS J17210-2107AB , LTT 6908[ 8]
Database references SIMBAD A B
ξ Oph , Latinized as Xi Ophiuchi , is a visual binary star [ 9] system in the equatorial constellation of Ophiuchus .[ 2] It has a yellow-white hue and is faintly visible to the naked eye with a combined apparent visual magnitude of 4.39.[ 2] The system is located approximately 57.1 light-years (17.5 parsecs ) away from the Sun based on parallax , but is drifting closer with a radial velocity of -9 km/s.[ 1]
The magnitude 4.40[ 10] primary, designated component A, is an ordinary F-type main-sequence star with a stellar classification of F2V.[ 3] It is 916[ 7] million years old and is rotating with a projected rotational velocity of 20 km/s. The star has 1.3 times the mass of the Sun and 1.6 times the Sun's radius .[ 5] It is radiating 4.4[ 6] times the luminosity of the Sun from its photosphere at an effective temperature of 6,611 K.[ 5]
The system is a source of X-ray emission .[ 11] The orbiting companion, component B, is a magnitude 8.9 star at an angular separation of 4.1″ along a position angle of 26° from the primary, as of 2016. A magnitude 10.8 visual companion , component C, lies at a separation of 10.8″ , as of 2004.[ 10]
According to Richard H. Allen's Star Names : Their Lore and Meaning (1899), ξ Oph together with θ Oph formed the Sogdian Wajrik "the Magician", the Khorasmian Markhashik "the Serpent-bitten" and with η Oph the Coptic Tshiō , "the Snake", and Aggia , "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 the Habitable Worlds Observatory .[ 14] As of June 2025[update] , it does not appear in the IAU Catalog of Star Names .[ 15]
References
^ a b c d e f Vallenari, 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 at VizieR .
^ a b c d Anderson, 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
^ a b Gray, 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 .
^ a b Mallama, 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
^ a b c Fuhrmann, 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 .
^ a b Brown, 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 at VizieR .
^ a b David, 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
^ "ksi Oph" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-10-08 .
^ 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 .
^ a b Mason, 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
^ 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 .
^ Allen, R.H. (1899), Star Names: Their Lore and Meaning , p. 297
^ 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.
^ 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.
^ "IAU Catalog of Star Names" . Retrieved 22 February 2025 .