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53 Ophiuchi

From Wikipedia, the free encyclopedia
Star system in the constellation Ophiuchus
53 Ophiuchi
Observation data
Epoch J2000      Equinox J2000
ConstellationOphiuchus
Right ascension17h 34m 36.69409s[1]
Declination+09° 35′ 12.1005″[1]
Apparent magnitude (V)5.80[2](5.82 + 7.8)[3]
Characteristics
Spectral typeA2 V + A8 IV[4]
Astrometry
53 Oph A
Radial velocity (Rv)−13.9±2.9[5] km/s
Proper motion (μ)RA: +2.126[1]mas/yr
Dec.: −8.530[1]mas/yr
Parallax (π)8.8060±0.0978 mas[1]
Distance370 ± 4 ly
(114 ± 1 pc)
53 Oph B
Proper motion (μ)RA: +1.794[6] mas/yr
Dec.: −8.148[6] mas/yr
Parallax (π)8.8979 ± 0.0413 mas[6]
Distance367 ± 2 ly
(112.4 ± 0.5 pc)
Details
53 Oph Aa
Mass2.50±0.05[7] M
Radius1.7[8] R
Luminosity56.4+5.3
−4.9
[7] L
Surface gravity (log g)3.90[9] cgs
Temperature9,311+173
−170
[7] K
Metallicity [Fe/H]0.21[9] dex
Rotational velocity (v sin i)29[7] km/s
53 Oph B
Radius1.72+0.06
−0.03
[6] R
Luminosity7.74±0.05[6] L
Temperature7,344+124
−152
[6] K
Rotational velocity (v sin i)140[4] km/s
Other designations
f Oph,53 Oph,HD 159480,HIP 85998,HR 6548,WDS J17346+0935[10]
53 Oph A:BD+09°3424,GC 23824,SAO 122526[10]
53 Oph B:BD+09°3423,GC 23823,SAO 122525[11]
Database references
SIMBADdata

53 Ophiuchi is a multiplestar system in theequatorialconstellation ofOphiuchus. It is visible to the naked eye as a faint star with a combinedapparent visual magnitude of 5.80.[3] Located around 370 light years distant from the Sun based onparallax,[1] it is moving closer to the Earth with a heliocentricradial velocity of −14 km/s.[5] As of 2011, the visible components had anangular separation of41.28 along aposition angle of 190°.[12] The primary may itself be a close binary system with a separation of0.3692″ and a magnitude difference of 3.97 at an infrared wavelength of562 nm.[13]

The magnitude 5.82[3] primary, designated component Aa, is anA-type main-sequence star with astellar classification of A2 V.[4] It has 2.5[7] times themass of the Sun and about 1.7[8] times theSun's radius. The star is radiating 56 times theSun's luminosity from itsphotosphere at aneffective temperature of 9,311 K.[7] The widely spaced secondary, designated component B, is a magnitude 7.8[3]A-typesubgiant star with a class of A8 IV.[4]

References

[edit]
  1. ^abcdefBrown, 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. ^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.
  3. ^abcdEggleton, 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. ^abcdLevato, H. (1975), "Rotational velocities and spectral types for a sample of binary systems",Astronomy and Astrophysics,19: 91,Bibcode:1975A&AS...19...91L.
  5. ^abde Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",Astronomy & Astrophysics,546: 14,arXiv:1208.3048,Bibcode:2012A&A...546A..61D,doi:10.1051/0004-6361/201219219,S2CID 59451347, A61.
  6. ^abcdefBrown, 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. ^abcdefZorec, J.; Royer, F.; Asplund, Martin; Cassisi, Santi; Ramirez, Ivan; Melendez, Jorge; Bensby, Thomas; Feltzing, Sofia (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities",Astronomy and Astrophysics,537: A120,arXiv:1201.2052,Bibcode:2012A&A...537A.120Z,doi:10.1051/0004-6361/201117691,S2CID 55586789.
  8. ^abPasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics,367 (2) (Third ed.):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  9. ^abLemke, M. (November 1989), "Abundance anomalies in main sequence A stars. I. Iron and titanium",Astronomy and Astrophysics,225:125–136,Bibcode:1989A&A...225..125L.
  10. ^ab"f Oph".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-06-21.
  11. ^"BD+09 3423".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-06-21.
  12. ^Mason, Brian D.; et al. (August 2011), "Speckle Interferometry at the U.S. Naval Observatory. XVII.",The Astronomical Journal,142 (2): 4,Bibcode:2011AJ....142...46M,doi:10.1088/0004-6256/142/2/46,S2CID 250806722, 46.
  13. ^Horch, Elliott P.; et al. (February 2011), "Observations of Binary Stars with the Differential Speckle Survey Instrument. II. Hipparcos Stars Observed in 2010 January and June",The Astronomical Journal,141 (2): 13,Bibcode:2011AJ....141...45H,doi:10.1088/0004-6256/141/2/45, 45.
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