HD 89307

From Wikipedia, the free encyclopedia
HD 89307
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Leo
Right ascension 10h 18m 21.28741s[1]
Declination +12° 37′ 15.9920″[1]
Apparent magnitude (V) 7.02[2]
Characteristics
Spectral type G0V[3]
B−V color index 0.594±0.003[2]
Astrometry
Radial velocity (Rv)+23.29±0.19[1] km/s
Proper motion (μ) RA: −272.380[1] mas/yr
Dec.: −39.416[1] mas/yr
Parallax (π)31.2110 ± 0.0511[1] mas
Distance104.5 ± 0.2 ly
(32.04 ± 0.05 pc)
Absolute magnitude (MV)4.57[4]
Details[4]
Mass1.028±0.04 M☉
Radius1.08+0.01
−0.02[1] R☉
Luminosity1.354±0.003[1] L☉
Surface gravity (log g)4.414±0.10 cgs
Temperature5,950±44 K
Metallicity [Fe/H]−0.15±0.02[2] dex
Rotation23.7 d
Rotational velocity (v sin i)3.21±0.50 km/s
Age5.3+2.7
−2.9 Gyr[2]
6.76[4] Gyr
Other designations
BD+13 2237, GC 14140, HD 1835, HIP 50473, SAO 99049, PPM 127289[5]
Database references
SIMBADdata

HD 89307 is a star in the equatorial constellation of Leo. It is too faint to be viewed with the naked eye except under ideal conditions, having an apparent visual magnitude of 7.02.[2] The star is located at a distance of 105 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +23 km/s.[1]

This is an ordinary G-type main-sequence star with a stellar classification of G0V.[3] It is chromospherically inactive and appears older than the Sun with a rotation 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[1] times the Sun's luminosity from its photosphere at an effective temperature of 5,950 K.[4]

Planetary system[]

In December 2004, using the radial velocity method, it was found to have a long-period giant planet in orbit around it.[4]

The HD 89307 planetary system[6]
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b ≥2.00 ± 0.42 MJ 3.34 ± 0.17 2,199 ± 61 0.25 ± 0.09 — —

See also[]

  • List of extrasolar planets

References[]

  1. ^ a b c d e f g h i j 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 at VizieR.
  2. ^ a b c d e 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.
  3. ^ a b Harlan, 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. ^ a b c d e f g Fischer, 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. ^ "9 Cet". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-03-27.
  6. ^ 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

External links[]

Coordinates: Sky map 10h 18m 21.2877s, +12° 37′ 15.990″

Retrieved from ""