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HD 89307

From Wikipedia, the free encyclopedia
Star in the constellation Leo
HD 89307
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationLeo[1]
Right ascension10h 18m 21.28771s[2]
Declination+12° 37′ 15.9909″[2]
Apparent magnitude (V)7.02[1]
Characteristics
Evolutionary stagemain sequence[2]
Spectral typeG0V[3]
B−Vcolor index0.594±0.003[1]
Astrometry
Radial velocity (Rv)+23.27±0.13[2] km/s
Proper motion (μ)RA: −272.659mas/yr[2]
Dec.: −39.333mas/yr[2]
Parallax (π)31.4134±0.0226 mas[2]
Distance103.83 ± 0.07 ly
(31.83 ± 0.02 pc)
Absolute magnitude (MV)4.57[4]
Details[4]
Mass1.028±0.04 M
Radius1.08+0.01
−0.02
[5] R
Luminosity1.354±0.003[5] L
Surface gravity (log g)4.414±0.10 cgs
Temperature5,950±44 K
Metallicity[Fe/H]−0.15±0.02[1] dex
Rotation23.7 d
Rotational velocity (v sin i)3.21±0.50 km/s
Age5.3+2.7
−2.9
 Gyr
[1]
6.76[4] Gyr
Other designations
BD+13 2237,GC 14140,HD 1835,HIP 50473,SAO 99049,PPM 127289[6]
Database references
SIMBADdata

HD 89307 is astar in theequatorialconstellation ofLeo. It is too faint to be viewed with the naked eye except under ideal conditions, having anapparent visual magnitude of 7.02.[1] The star is located at a distance of 104light-years (32parsecs) from theSun based onparallax, and is drifting further away with aradial velocity of +23 km/s.[2]

This is an ordinaryG-type main-sequence star with astellar classification of G0V.[3] It ischromospherically inactive and appears older than the Sun with arotation period of 23.7 days.[4] The star has about the same mass[4] as the Sun and is 8% larger. It is radiating 1.35[5] times the Sun's luminosity from itsphotosphere at aneffective temperature of 5,950 K.[4]

Planetary system

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In December 2004, using theradial velocity method, it was found to have a long-periodgiant planet inorbit around it.[4] The parameters of HD 89307 b were updated in 2012,[7] and in 2023 its inclination andtrue mass were determined viaastrometry.[8]

The HD 89307 planetary system[8]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(years)
EccentricityInclinationRadius
b2.02+0.27
−0.15
 MJ
3.331+0.052
−0.053
5.991+0.081
−0.078
0.174+0.041
−0.043
72+13
−15
or108+15
−13
°

See also

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References

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  1. ^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. XHIP record for this object atVizieR.
  2. ^abcdefgVallenari, 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.
  3. ^abHarlan, E. A. (September 1969). "MK classifications for F- and G-type stars. I".Astronomical Journal.74:916–919.Bibcode:1969AJ.....74..916H.doi:10.1086/110881.
  4. ^abcdefgFischer, Debra; et al. (2009). "Five planets and an independent confirmation of HD 196885 Ab from Lick Observatory".The Astrophysical Journal.703 (2):1545–1556.arXiv:0908.1596.Bibcode:2009ApJ...703.1545F.doi:10.1088/0004-637X/703/2/1545.S2CID 15524804.
  5. ^abcBrown, 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.
  6. ^"9 Cet".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2021-03-27.
  7. ^Boisse, Isabelle; Pepe, Francesco; Perrier, Christian; Queloz, Didier; Bonfils, Xavier; Bouchy, François; Santos, Nuno C.; Arnold, Luc; Beuzit, Jean-Luc; Dìaz, Rodrigo F.; Delfosse, Xavier; Eggenberger, Anne; Ehrenreich, David; Forveille, Thierry; Hébrard, Guillaume; Lagrange, Anne-Marie; Lovis, Christophe; Mayor, Michel; Moutou, Claire; Naef, Dominique; Santerne, Alexandre; Ségransan, Damien; Sivan, Jean-Pierre; Udry, Stéphane (2012), "The SOPHIE search for northern extrasolar planets V. Follow-up of ELODIE candidates: Jupiter-analogs around Sun-like stars",Astronomy and Astrophysics,545: A55,arXiv:1205.5835,Bibcode:2012A&A...545A..55B,doi:10.1051/0004-6361/201118419,S2CID 119109836
  8. ^abXiao, Guang-Yao; Liu, Yu-Juan; et al. (March 2023). "The Masses of a Sample of Radial-Velocity Exoplanets with Astrometric Measurements".Research in Astronomy and Astrophysics.23 (5).arXiv:2303.12409.Bibcode:2023RAA....23e5022X.doi:10.1088/1674-4527/accb7e.

External links

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