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44 Ophiuchi

From Wikipedia, the free encyclopedia
Star in the constellation Ophiuchus
This article is about b Ophiuchi and is not to be confused withβ (Beta) Ophiuchi.
44 Ophiuchi
Location of 44 Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationOphiuchus
Right ascension17h 26m 22.21749s[1]
Declination−24° 10′ 31.1190″[1]
Apparent magnitude (V)4.16[2]
Characteristics
Spectral typekA5hA9mF1III[3]
U−Bcolor index+0.12[4]
B−Vcolor 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]
Distance83.2 ± 0.5 ly
(25.5 ± 0.2 pc)
Absolute magnitude (MV)2.13[2]
Details
Mass1.77[6] M
Radius1.9[7] R
Luminosity13[6] L
Surface gravity (log g)4.15[8] cgs
Temperature7,559[8] K
Metallicity[Fe/H]+0.30[2] dex
Rotational velocity (v sin i)78[6] km/s
Age1.028[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
SIMBADdata

44 Ophiuchi is a single[10]star in theconstellationOphiuchus. It has theBayer designationb Ophiuchi, while44 Ophiuchi is theFlamsteed designation. It is visible to the naked eye as a faint, white-hued star with anapparent 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 heliocentricradial 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 anAm star with astellar classification of kA5hA9mF1III,[3] indicating it has theluminosity class of agiant star with aspectrum that matches an A5 star based on thecalcium K line, and an A9 star from thehydrogen andmetallines. It is around a billion years old[8] with 1.77[6] times themass of the Sun and 1.9[7] times theSun's girth. The star is radiating 13[6] times theSun's luminosity from itsphotosphere at aneffective temperature of 7,559 K.[8] It retains a moderately high rotation rate, showing aprojected rotational velocity of 78 km/s.[6]

References

[edit]
  1. ^abcdefVan 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. ^abcdAnderson, 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. ^abGray, 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. ^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. ^abGontcharov, 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. ^abcdefZorec, 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. ^abAllende 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. ^abcdeDavid, 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. Retrieved2019-06-21.
  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.
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