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74 Ophiuchi

From Wikipedia, the free encyclopedia
Star in the constellation Ophiuchus
74 Ophiuchi
Location of 74 Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationOphiuchus
Right ascension18h 20m 52.06435s[1]
Declination03° 22′ 37.7817″[1]
Apparent magnitude (V)4.85[2]
Characteristics
Spectral typeG8III[3]
U−Bcolor index+0.61[4]
B−Vcolor index+0.91[4]
Astrometry
Radial velocity (Rv)+4.35[5] km/s
Proper motion (μ)RA: −7.646[1]mas/yr
Dec.: +12.546[1]mas/yr
Parallax (π)13.7320±0.2060 mas[1]
Distance238 ± 4 ly
(73 ± 1 pc)
Absolute magnitude (MV)0.34[2]
Details
Mass2.38[6] M
Radius10.52+0.32
−1.04
[1] R
Luminosity66.0±1.2[1] L
Surface gravity (log g)2.70[6] cgs
Temperature5,073+271
−76
[1] K
Metallicity [Fe/H]-0.21[6] dex
Rotational velocity (v sin i)0.0[5] km/s
Age1.73[7] Gyr
Other designations
74 Oph,BD+03°3680,FK5 1476,GC 25036,GJ 9615 A,HD 168656,HIP 89918,HR 6866,SAO 123377,CCDM J18209+0323A,WDS J18209+0323A[8]
Database references
SIMBADdata

74 Ophiuchi is a suspectedbinary star[9] in theequatorialconstellation ofOphiuchus, near the border withSerpens Cauda. It is visible to the naked eye as a faint, yellow-hued point of light with a combinedapparent visual magnitude of 4.85.[2] The system is located at a distance of 238 light years from the Sun based onparallax,[1] and is drifting further away with aradial velocity of +4.4 km/s.[5]

The primary member, designated component A, is an aginggiant star with astellar classification of G8III[3] and an estimated age of 1.73[7] billion years. Having exhausted the hydrogen supply at itscore, the star has expanded to 10.5[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 2.4[6] times themass of the Sun and is radiating 66[1] times theSun's luminosity from its swollenphotosphere at aneffective temperature of around 5,073 K.[1]

The magnitude 11.5 secondary, component B, lies at anangular separation of28.1″ from the primary, as of 2008.[9] Avisual companion, component C, is magnitude 12.28 and has a separation of57.9″.[11]

References

[edit]
  1. ^abcdefghijklBrown, 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. ^abHouk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars".Michigan Spectral Survey.5.Bibcode:1999MSS...C05....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. ^abcMassarotti, Alessandro; Latham, David W.; Stefanik, Robert P.; Fogel, Jeffrey (2008)."Rotational and Radial Velocities for a Sample of 761 Hipparcos Giants and the Role of Binarity".The Astronomical Journal.135 (1):209–231.Bibcode:2008AJ....135..209M.doi:10.1088/0004-6256/135/1/209.
  6. ^abcdReffert, Sabine; et al. (2015). "Precise radial velocities of giant stars".Astronomy & Astrophysics.574: A116.arXiv:1412.4634.Bibcode:2015A&A...574A.116R.doi:10.1051/0004-6361/201322360.hdl:10722/215277.S2CID 59334290.Vizier catalog entry
  7. ^abLuck, R. Earle (2015). "Abundances in the Local Region. I. G and K Giants".Astronomical Journal.150 (3). 88.arXiv:1507.01466.Bibcode:2015AJ....150...88L.doi:10.1088/0004-6256/150/3/88.S2CID 118505114.
  8. ^"74 Oph".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-06-26.
  9. ^abEggleton, 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. ^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.
  11. ^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
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