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74 Ophiuchi
Location of 74 Ophiuchi (circled)
Observation data
Epoch J2000       Equinox J2000
Constellation Ophiuchus
Right ascension 18h 20m 52.06435s [1]
Declination 03° 22′ 37.7817″ [1]
Apparent magnitude (V) 4.85 [2]
Characteristics
Spectral type G8III [3]
U−B color index +0.61 [4]
B−V color 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
SIMBAD data

74 Ophiuchi is a suspected binary star [9] in the equatorial constellation of Ophiuchus, near the border with Serpens Cauda. It is visible to the naked eye as a faint, yellow-hued point of light with a combined apparent visual magnitude of 4.85. [2] The system is located at a distance of 238  light years from the Sun based on parallax, [1] and is drifting further away with a radial velocity of +4.4 km/s. [5]

The primary member, designated component A, is an aging giant star with a stellar classification of G8III [3] and an estimated age of 1.73 [7] billion years. Having exhausted the hydrogen supply at its core, the star has expanded to 10.5 [1] times the Sun's radius. It is a red clump giant, [10] which means it is on the horizontal branch and is generating energy through helium fusion at its core. The star has 2.4 [6] times the mass of the Sun and is radiating 66 [1] times the Sun's luminosity from its swollen photosphere at an effective temperature of around 5,073 K. [1]

The magnitude 11.5 secondary, component B, lies at an angular separation of 28.1″ from the primary, as of 2008. [9] A visual companion, component C, is magnitude 12.28 and has a separation of 57.9″. [11]

References

  1. ^ a b c d e f g h i j k l 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.
  2. ^ a b c 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
  3. ^ a b Houk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars". Michigan Spectral Survey. 5. Bibcode: 1999MSS...C05....0H.
  4. ^ 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
  5. ^ a b c Massarotti, 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. ^ a b c d Reffert, 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. ^ a b Luck, 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. Retrieved 2019-06-26.
  9. ^ a b 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.
  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