44 Ophiuchi

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44 Ophiuchi
Ophiuchus constellation map.svg
Red circle.svg
Location of 44 Ophiuchi (circled)
Observation data
Epoch J2000       Equinox J2000
Constellation Ophiuchus
Right ascension 17h 26m 22.21749s [1]
Declination −24° 10 31.1190 [1]
Apparent magnitude  (V)4.16 [2]
Characteristics
Spectral type kA5hA9mF1III [3]
U−B color index +0.12 [4]
B−V color index +0.28 [4]
Astrometry
Radial velocity (Rv)−37.20 [5] km/s
Proper motion (μ)RA: +0.10 [1] mas/yr
Dec.: −118.18 [1] mas/yr
Parallax (π)39.22±0.24  mas [1]
Distance 83.2 ± 0.5  ly
(25.5 ± 0.2  pc)
Absolute magnitude  (MV)2.13 [2]
Details
Mass 1.77 [6]   M
Radius 1.9 [7]   R
Luminosity 13 [6]   L
Surface gravity (log g)4.15 [8]   cgs
Temperature 7,559 [8]   K
Metallicity [Fe/H]+0.30 [2]   dex
Rotational velocity (v sin i)78 [6]  km/s
Age 1.028 [8]   Gyr
Other designations
b Oph, 44 Oph, CD−24°13337, FK5 1457, GC 23597, GJ 9591, HD 157792, HIP 85340, HR 6486, SAO 185401 [9]
Database references
SIMBAD data

44 Ophiuchi is a single [10] star in the constellation Ophiuchus. It has the Bayer designation b Ophiuchi, while 44 Ophiuchi is the Flamsteed designation. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 4.16. [2] The distance to this object is approximately 83.2  light years based on parallax. [1] It is drifting closer to the Earth with a heliocentric radial velocity of -37.2 km/s, [5] and is predicted to come within 30 light-years around 585,000 years from now. [11]

This is an Am star with a stellar classification of kA5hA9mF1III, [3] indicating it has the luminosity class of a giant star with a spectrum that matches an A5 star based on the calcium K line, and an A9 star from the hydrogen and metal lines. It is around a billion years old [8] with 1.77 [6] times the mass of the Sun and 1.9 [7] times the Sun's girth. The star is radiating 13 [6] times the Sun's luminosity from its photosphere at an effective temperature of 7,559 K. [8] It retains a moderately high rotation rate, showing a projected rotational velocity of 78 km/s. [6]

References

  1. 1 2 3 4 5 6 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
  2. 1 2 3 4 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. 1 2 Gray, R. O.; Corbally, C. J.; Garrison, R. F.; McFadden, M. T.; Bubar, E. J.; McGahee, C. E.; O'Donoghue, A. A.; Knox, E. R. (2006). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 pc--The Southern Sample". The Astronomical Journal. 132 (1): 161–170. arXiv: astro-ph/0603770 . Bibcode:2006AJ....132..161G. doi:10.1086/504637. S2CID   119476992.
  4. 1 2 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. 1 2 Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv: 1606.08053 . Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. S2CID   119231169.
  6. 1 2 3 4 5 6 Zorec, 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
  7. 1 2 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
  8. 1 2 3 4 5 David, 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
  9. "b Oph". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-06-21.
  10. 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.
  11. Bailer-Jones, C. A. L. (March 2015). "Close encounters of the stellar kind". Astronomy & Astrophysics. 575: 13. arXiv: 1412.3648 . Bibcode:2015A&A...575A..35B. doi:10.1051/0004-6361/201425221. S2CID   59039482. A35.