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72 Ophiuchi

From Wikipedia, the free encyclopedia
Binary star system in the constellation Ophiuchus
72 Ophiuchi
Location of 72 Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationOphiuchus
Right ascension18h 07m 20.98393s[1]
Declination9° 33′ 49.8501″[1]
Apparent magnitude (V)3.73[2] + 14.0[3]
Characteristics
Spectral typeA5 V[4]
U−Bcolor index+0.10[2]
B−Vcolor index+0.12[2]
Astrometry
Radial velocity (Rv)-23.90[5] km/s
Proper motion (μ)RA: -62.17[1]mas/yr
Dec.: +79.66[1]mas/yr
Parallax (π)37.55±0.21 mas[1]
Distance86.9 ± 0.5 ly
(26.6 ± 0.1 pc)
Absolute magnitude (MV)1.58[6]
Details
Mass1.99[7] M
Radius1.9[8] R
Luminosity20[7] L
Surface gravity (log g)4.04[9] cgs
Temperature8,718[9] K
Metallicity [Fe/H]+0.09[6] dex
Rotational velocity (v sin i)65[7] km/s
Age250[9] Myr
Other designations
72 Oph,BD+09°3564,FK5 680,GC 24695,GJ 9615 A,HD 165777,HIP 88771,HR 6771,SAO 123142,CCDM J18073+0934A,WDS J18073+0934A[10]
Database references
SIMBADdata

72 Ophiuchi is abinary star[3] system in theequatorialconstellation ofOphiuchus. It is visible to the naked eye as a faint, white-hued point of light with a combinedapparent visual magnitude of 3.73.[2] It is located approximately 86.9 light years away from the Sun based onparallax,[1] but is moving closer with a heliocentricradial velocity of -23.9 km/s.[5]

As of 2008, the pair had anangular separation of25.[3] According to Gray et al. (2003), the primary component has astellar classification of A5 V,[4] matching anA-type main-sequence star. Cowley et al. (1969) had assigned it to a class of A4 IVs,[11] suggesting it is a sharp-lined (s)subgiant star. The latter class is still in use by some sources.[7][3][12]

The primary is 250[9] million years old with double[7] themass of the Sun and is spinning with a moderateprojected rotational velocity of 65 km/s.[7] It is radiating 20[7] times theluminosity of the Sun from itsphotosphere at aneffective temperature of 8,718 K.[9] It displays aninfrared excess, suggesting adebris disk is orbiting the star with a mean separation of82.96 AU and temperature of 60 K.[13] The system is a source ofX-ray emission,[12] which is most likely coming from the 14th[3] magnitude companion.[12]

There are additionalvisual companions: component C with magnitude 11.5 lies at anangular separation of64 from the primary,[14] while component D, has magnitude 14.8 and separation 24".[15]

This star was once considered part of the obsolete constellationTaurus Poniatovii, the brightest star in it. After theInternational Astronomical Union officially recognised constellations, it was placed in Ophiuchus.[16]

References

[edit]
  1. ^abcdefVan Leeuwen, F. (2007). "Validation of the new Hipparcos reduction".Astronomy and Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.S2CID 18759600.Vizier catalog entry
  2. ^abcdDucati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".CDS/ADC Collection of Electronic Catalogues.2237.Bibcode:2002yCat.2237....0D.
  3. ^abcdeEggleton, 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.
  4. ^abGray, R. O.; et al. (2003). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I".The Astronomical Journal.126 (4): 2048.arXiv:astro-ph/0308182.Bibcode:2003AJ....126.2048G.doi:10.1086/378365.S2CID 119417105.
  5. ^abKharchenko, N. V.; Scholz, R.-D.; Piskunov, A. E.; Röser, S.; Schilbach, E. (2007). "Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ~55000 stars and mean radial velocities of 516 Galactic open clusters and associations".Astronomische Nachrichten.328 (9): 889.arXiv:0705.0878.Bibcode:2007AN....328..889K.doi:10.1002/asna.200710776.S2CID 119323941.
  6. ^abAnderson, 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
  7. ^abcdefgZorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars".Astronomy & Astrophysics.537: A120.arXiv:1201.2052.Bibcode:2012A&A...537A.120Z.doi:10.1051/0004-6361/201117691.S2CID 55586789.Vizier catalog entry
  8. ^Allende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: Masses, radii and effective temperatures".Astronomy and Astrophysics.352:555–562.arXiv:astro-ph/9911002.Bibcode:1999A&A...352..555A.Vizier catalog entry
  9. ^abcdeDavid, 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
  10. ^"72 Oph".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-06-26.
  11. ^Cowley, A.; et al. (April 1969). "A study of the bright A stars. I. A catalogue of spectral classifications".Astronomical Journal.74:375–406.Bibcode:1969AJ.....74..375C.doi:10.1086/110819.
  12. ^abcDe Rosa, R. J.; et al. (July 2011)."The Volume-limited A-Star (VAST) survey - I. Companions and the unexpected X-ray detection of B6-A7 stars".Monthly Notices of the Royal Astronomical Society.415 (1):854–866.arXiv:1103.4363.Bibcode:2011MNRAS.415..854D.doi:10.1111/j.1365-2966.2011.18765.x.S2CID 84181878.
  13. ^Gáspár, András; et al. (2016)."The Correlation between Metallicity and Debris Disk Mass".The Astrophysical Journal.826 (2): 171.arXiv:1604.07403.Bibcode:2016ApJ...826..171G.doi:10.3847/0004-637X/826/2/171.S2CID 119241004.
  14. ^Renson, P.; Manfroid, J. (2009)."Catalogue of Ap, HgMn and Am stars".Astronomy and Astrophysics.498 (3): 961.Bibcode:2009A&A...498..961R.doi:10.1051/0004-6361/200810788.
  15. ^Mason, Brian D.; et al. (2001)."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
  16. ^Ian Ridpath."Taurus Poniatovii".Star Tales. Retrieved2023-11-01.
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