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HD 89744

Coordinates:Sky map10h 11m 10.5621s, +41° 13′ 46.308″
From Wikipedia, the free encyclopedia
Star in the constellation Ursa Major
HD 89744
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationUrsa Major
A
Right ascension10h 22m 10.5619s[1]
Declination+41° 13′ 46.310″[1]
Apparent magnitude (V)5.73[2]
B
Right ascension10h 22m 14.8721s[3]
Declination+41° 14′ 26.514″[3]
Characteristics
Evolutionary stageMain sequence
Spectral typeF7V[4] or F8IV[5]
B−Vcolor index0.531±0.003[2]
Astrometry
A
Radial velocity (Rv)−4.35±0.12[2] km/s
Proper motion (μ)RA: −120.285(42)mas/yr[1]
Dec.: −138.171(50)mas/yr[1]
Parallax (π)25.9334±0.0436 mas[1]
Distance125.8 ± 0.2 ly
(38.56 ± 0.06 pc)
Absolute magnitude (MV)2.83[6]
B
Proper motion (μ)RA: −119.215(647) mas/yr[3]
Dec.: −140.390(457) mas/yr[3]
Parallax (π)26.0070 ± 0.4713 mas[3]
Distance125 ± 2 ly
(38.5 ± 0.7 pc)
Details
A
Mass1.37±0.09[7] M
Radius2.16+0.06
−0.01
[8] R
Luminosity6.38±0.02[9] L
Surface gravity (log g)4.27±0.05[7] cgs
Temperature6,381±43[7] K
Metallicity [Fe/H]0.30±0.03[7] dex
Rotation~9 days[9]
Rotational velocity (v sin i)9.3[10] km/s
Age8.4[9] Gyr
B
Mass0.076[11] M
Other designations
BD+41°2076,GJ 9326,HD 89744,HIP 50786,HR 4067,WDS J10222+4114[12]
A:HD 89744A
B:Gaia DR3 804745827531820288,HD 89744B,2MASS J10221489+4114266
Database references
A
SIMBADdata
Exoplanet Archivedata
ARICNSdata
B
SIMBADdata

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 of63.1 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]

Planetary system

[edit]

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]

The HD 89744 planetary system[21]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b>8.35±0.18 MJ0.917±0.009256.78±0.020.677±0.003
c(unconfirmed)>5.36±4.57MJ8.3±1.86,974±2,1610.29±0.12

See also

[edit]

References

[edit]
  1. ^abcdVallenari, 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.
  2. ^abcdefAnderson, 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.
  3. ^abcdVallenari, 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.
  4. ^abcScholz, 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.
  5. ^abGray, 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.
  6. ^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.
  7. ^abcdefSousa, 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.
  8. ^abBrown, 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.
  9. ^abcdeMetcalfe, 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.
  10. ^abMorris, 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.
  11. ^abcMugrauer, 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.
  12. ^"HD 89744".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-10-14.
  13. ^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.
  14. ^abKorzennik, 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.
  15. ^abWright, 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.
  16. ^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.
  17. ^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.
  18. ^abWilson, 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.
  19. ^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.
  20. ^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.
  21. ^abWittenmyer, 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.


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