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71 Ophiuchi

From Wikipedia, the free encyclopedia
Giant star in the constellation of Ophiuchus
71 Ophiuchi
Location of 71 Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationOphiuchus
Right ascension18h 07m 18.35888s[1]
Declination+08° 44′ 01.9181″[1]
Apparent magnitude (V)4.64[2]
Characteristics
Spectral typeG8III[3]
U−Bcolor index+0.73[4]
B−Vcolor index+0.97[4]
Astrometry
Radial velocity (Rv)−3.00±0.09[5] km/s
Proper motion (μ)RA: +9.857[1]mas/yr
Dec.: +29.770[1]mas/yr
Parallax (π)13.1352±0.1891 mas[1]
Distance248 ± 4 ly
(76 ± 1 pc)
Absolute magnitude (MV)0.03[2]
Details[6]
Mass2.87±0.09 M
Radius12.55+0.27
−0.34
[1] R
Luminosity88.8±1.5[1] L
Surface gravity (log g)3.00±0.02 cgs
Temperature5,001+70
−52
[1] K
Metallicity [Fe/H]0.10±0.01 dex
Rotational velocity (v sin i)0.32±0.45 km/s
Age400±30 Myr
Other designations
71 Oph,BD+08°3582,GC 24693,HD 165760,HIP 88765,HR 6770,SAO 123140[7]
Database references
SIMBADdata

71 Ophiuchi is a single[8]star in theequatorialconstellation ofOphiuchus. It is visible to the naked eye as a faint, yellow-hued point of light with anapparent visual magnitude of 4.64.[2] The star is located approximately 273 light years away from the Sun based onparallax,[9] and is moving closer with aradial velocity of −3 km/s.[5]

At the estimated age of 400 million years,[6] this is an aginggiant star with astellar classification of G8III,[3] having exhausted the supply of hydrogen at itscore and expanded to around 13[1] times theSun's radius. It is ared clump giant,[10] which means it is on thehorizontal branch and is generating energy throughhelium fusion at its core. The star has 2.9 times themass of the Sun and is radiating 89 times theSun's luminosity from its swollenphotosphere at aneffective temperature of 5,001 K.[6]

References

[edit]
  1. ^abcdefghiBrown, 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.
  2. ^abcAnderson, 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. ^abHoffleit, D.; Warren, W. H. (1995). "VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)".VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H.5050.Bibcode:1995yCat.5050....0H.
  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. ^abJofré, E.; Petrucci, R.; Saffe, C.; Saker, L.; Artur de la Villarmois, E.; Chavero, C.; Gómez, M.; Mauas, P. J. D. (2015). "Stellar parameters and chemical abundances of 223 evolved stars with and without planets".Astronomy & Astrophysics.574: A50.arXiv:1410.6422.Bibcode:2015A&A...574A..50J.doi:10.1051/0004-6361/201424474.S2CID 53666931.Vizier catalog entry
  6. ^abcJofré, E.; et al. (2015). "Stellar parameters and chemical abundances of 223 evolved stars with and without planets".Astronomy & Astrophysics.574: A50.arXiv:1410.6422.Bibcode:2015A&A...574A..50J.doi:10.1051/0004-6361/201424474.S2CID 53666931. A50.
  7. ^"71 Oph".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-06-21.
  8. ^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.
  9. ^Van 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
  10. ^Alves, David R. (August 2000). "K-Band Calibration of the Red Clump Luminosity".The Astrophysical Journal.539 (2):732–741.arXiv:astro-ph/0003329.Bibcode:2000ApJ...539..732A.doi:10.1086/309278.S2CID 16673121.
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