Star in the constellation Ophiuchus
44 Ophiuchi Location of 44 Ophiuchi (circled)
Observation dataEpoch 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−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] 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 theconstellation Ophiuchus . It has theBayer designation b 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 andmetal lines . 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]
^a b c d e f 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 ^a b c d 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 ^a b 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 . ^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 ^a b 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 . ^a b c d e f 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 ^a b 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 ^a b c d e 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 ^ "b Oph" .SIMBAD .Centre de données astronomiques de Strasbourg . Retrieved2019-06-21 .^ 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 . ^ 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.