Star in the constellation Ursa Major
HD 89744 is astar in the northerncircumpolar constellation ofUrsa Major , positioned about 0.4° due south of the bright starTania Australis (μ UMa).[ 13] This object has a yellow-white hue and is dimly visible to the naked eye with anapparent visual magnitude of 5.73.[ 2] The distance to this star has been measured using theparallax method, which locates it 126 light years from theSun . It is drifting closer with aradial velocity of −4.4 km/s.[ 2] There are two knownexoplanets orbiting this star.
At various times the star HD 89744 has been assigned astellar classification of F7V,[ 4] [ 14] F7IV-V,[ 15] and F8IV,[ 5] [ 2] suggesting it is anF-type main-sequence star that isevolving onto thesubgiant branch. It is ~8.4[ 9] billion years old with aninactive chromosphere [ 15] and is spinning with aprojected rotational velocity of 9.3 km/s.[ 10] The star is 2.16[ 8] times the size of the Sun with 1.4[ 7] times the Sun's radius. It is a highmetallicity star, showing a greater abundance of heavier elements than in the Sun. The star is radiating 6.4[ 9] times theluminosity of the Sun from itsphotosphere at aneffective temperature of 6,381 K.[ 7]
This star was identified as a member of theAB Doradus moving group by J. López-Santiago and collaborators in 2006.[ 16] It was later shown that its evolutionary state is incompatible with membership.[ 17]
In 2001, a faint co-moving companion was identified at anangular separation of 63.1″ from the primary.[ 18] This is equivalent to a linearprojected separation of 2,456 AU (0.04 ly ).[ 11] The companion, designated component B, is an L-class (~L0.5)[ 4] brown dwarf [ 18] with a mass of ~0.076 M ☉ .[ 11]
In April 2000, aplanet was discovered usingradial velocity measurements taken atFred Lawrence Whipple Observatory andLick Observatory .[ 14] The orbital parameters were updated in 2006 and 2007 using additional measurements.[ 19] [ 20] A second planet with a much longer period was discovered in 2019.[ 21]
^a b c d Vallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties" .Astronomy and Astrophysics .674 : A1.arXiv :2208.00211 .Bibcode :2023A&A...674A...1G .doi :10.1051/0004-6361/202243940 .S2CID 244398875 . Gaia DR3 record for this source atVizieR .^a b c d e f 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 . ^a b c d Vallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties" .Astronomy and Astrophysics .674 : A1.arXiv :2208.00211 .Bibcode :2023A&A...674A...1G .doi :10.1051/0004-6361/202243940 .S2CID 244398875 . Gaia DR3 record for this source atVizieR .^a b c Scholz, R. -D. (March 2016). "Overlooked wide companions of nearby F stars".Astronomy & Astrophysics .587 : 8.arXiv :1601.01896 .Bibcode :2016A&A...587A..51S .doi :10.1051/0004-6361/201527965 .S2CID 118348424 . A51. ^a b Gray, R. O.; et al. (July 2006). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 parsecs: The Northern Sample I".The Astronomical Journal .132 (1):161– 170.arXiv :astro-ph/0603770 .Bibcode :2006AJ....132..161G .doi :10.1086/504637 .S2CID 119476992 . ^ Pizzolato, N.; et al. (September 2000). "Evolution of X-ray activity of 1-3 Msun late-type stars in early post-main-sequence phases".Astronomy and Astrophysics .361 :614– 628.Bibcode :2000A&A...361..614P . ^a b c d e f Sousa, S. G.; et al. (November 2018). "SWEET-Cat updated. New homogenous spectroscopic parameters".Astronomy & Astrophysics .620 : 13.arXiv :1810.08108 .Bibcode :2018A&A...620A..58S .doi :10.1051/0004-6361/201833350 .S2CID 119374557 . A58. ^a b 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 atVizieR .^a b c d e Metcalfe, Travis S.; Egeland, Ricky (January 2019)."Understanding the Limitations of Gyrochronology for Old Field Stars" .The Astrophysical Journal .871 (1): 6.arXiv :1811.11905 .Bibcode :2019ApJ...871...39M .doi :10.3847/1538-4357/aaf575 .S2CID 119405127 . 39. ^a b Morris, Brett M.; et al. (September 2019)."Stellar Properties of Active G and K Stars: Exploring the Connection between Starspots and Chromospheric Activity" .The Astronomical Journal .158 (3): 16.arXiv :1907.00423 .Bibcode :2019AJ....158..101M .doi :10.3847/1538-3881/ab2e04 .S2CID 195767281 . 101. ^a b c Mugrauer, M.; et al. (2005)."Four new wide binaries among exoplanet host stars" .Astronomy and Astrophysics .440 (3):1051– 1060.arXiv :astro-ph/0507101 .Bibcode :2005A&A...440.1051M .doi :10.1051/0004-6361:20042297 . ^ "HD 89744" .SIMBAD .Centre de données astronomiques de Strasbourg . Retrieved2019-10-14 .^ Sinnott, Roger W.; Perryman, Michael A. C. (1997).Millennium Star Atlas . Vol. 2. Sky Publishing Corporation and the European Space Agency. p. 617.ISBN 0-933346-83-2 . ^a b Korzennik, Sylvain G.; et al. (2000)."A High-Eccentricity Low-Mass Companion to HD 89744" .The Astrophysical Journal Letters .533 (2):L147 – L150 .arXiv :astro-ph/0003045 .Bibcode :2000ApJ...533L.147K .doi :10.1086/312611 .PMID 10770711 . ^a b Wright, J. T. (September 2004). "Do We Know of Any Maunder Minimum Stars?".The Astronomical Journal .128 (3):1273– 1278.arXiv :astro-ph/0406338 .Bibcode :2004AJ....128.1273W .doi :10.1086/423221 .S2CID 118975831 . ^ Lopez-Santiago, J.; et al. (2006)."The Nearest Young Moving Groups" .The Astrophysical Journal .643 (2):1160– 1165.arXiv :astro-ph/0601573 .Bibcode :2006ApJ...643.1160L .doi :10.1086/503183 . ^ Schaefer, G. H.; et al. (2018-05-07)."AB Dor Moving Group Stars Resolved with the CHARA Array" .The Astrophysical Journal .858 (2) 71.Bibcode :2018ApJ...858...71S .doi :10.3847/1538-4357/aaba71 . ^a b Wilson, J. C.; et al. (October 2001). "Three Wide-Separation L Dwarf Companions from the Two Micron All Sky Survey: Gliese 337C, Gliese 618.1B, and HD 89744B".The Astronomical Journal .122 (4):1989– 2000.arXiv :astro-ph/0108424 .Bibcode :2001AJ....122.1989W .doi :10.1086/323134 .S2CID 17789028 . ^ Butler, R. P.; et al. (2006)."Catalog of Nearby Exoplanets" .The Astrophysical Journal .646 (1):505– 522.arXiv :astro-ph/0607493 .Bibcode :2006ApJ...646..505B .doi :10.1086/504701 . ^ Wittenmyer, Robert A.; et al. (2007)."Dynamical and Observational Constraints on Additional Planets in Highly Eccentric Planetary Systems" .The Astronomical Journal .134 (3):1276– 1284.arXiv :0706.1962 .Bibcode :2007AJ....134.1276W .doi :10.1086/520880 . ^a b Wittenmyer, Robert A.; et al. (2019)."Truly eccentric – I. Revisiting eight single-eccentric planetary systems" .Monthly Notices of the Royal Astronomical Society .484 (4):5859– 5867.arXiv :1901.08471 .Bibcode :2019MNRAS.484.5859W .doi :10.1093/mnras/stz290 .