HD 117207

HD 117207
Observation data
Epoch J2000      Equinox J2000
Constellation Centaurus
Right ascension 13h 29m 21.11291s[1]
Declination −35° 34′ 15.5880″[1]
Apparent magnitude (V) 7.240[2]
Characteristics
Spectral type G7IV-V[3]
B−V color index 0.727±0.014[2]
Astrometry
Radial velocity (Rv)−17.43±0.09[4] km/s
Proper motion (μ) RA: −205.904 mas/yr[1]
Dec.: −71.402 mas/yr[1]
Parallax (π)30.9440 ± 0.0256 mas[1]
Distance105.40 ± 0.09 ly
(32.32 ± 0.03 pc)
Absolute magnitude (MV)4.67[4]
Details[2]
Mass1.053±0.028 M☉
Radius1.074±0.041 R☉
Luminosity1.163+0.002
−0.003[5] L☉
Surface gravity (log g)4.371±0.039 cgs
Temperature5,732±53 K
Metallicity [Fe/H]0.19±0.03 dex
Age4.192±2.274[2] Gyr
Other designations
CPD−34°8913, HD 117207, HIP 65808, SAO 204517[6]
Database references
SIMBADdata

HD 117207 is a star in the southern constellation Centaurus. With an apparent visual magnitude of 7.24,[2] it is too dim to be visible to the naked eye but can be seen with a small telescope. Based upon parallax measurements, it is located at a distance of 105.4 light-years (32.3 parsecs) from the Sun. The star is drifting closer with a radial velocity of −17.4 km/s.[4] It has an absolute magnitude of 4.67.[4]

This object has a stellar classification of G7IV-V,[3] showing blended spectral traits of a G-type main-sequence star and an older, evolving subgiant star. It is around four[2] billion years old with 5%[7] greater mass than the Sun and a 7% larger radius.[5] The star is radiating 1.16 times the luminosity of the Sun from its photosphere at an effective temperature of 5,644 K.[5]

In 2005, a planet was found orbiting the star using the radial velocity method, and was designated HD 117207 b.[8][9] The orbital elements of this planet were refined in 2018, showing an orbital period of 7.18 years, a semimajor axis of 3.79 AU, and an eccentricity of 0.16. The minimum mass of this object is nearly double that of Jupiter. If an inner planet is orbiting the star, it must have an orbital period no greater than 3.46 years to satisfy Hill's criteria for dynamic stability.[2] In 2023, the inclination and true mass of HD 117207 b were determined via astrometry.[10]

The HD 117207 planetary system[10]
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(years) 		Eccentricity Inclination Radius
b 2.106+0.16
−0.089 MJ 		3.773+0.036
−0.035 		7.136+0.034
−0.035 		0.04+0.026
−0.024 		76.6+9.3
−12.0 or 103.4+12.0
−9.3° 		—
  1. ^ a b c d Cite error: The named reference GaiaDR3 was invoked but never defined (see the help page).
  2. ^ a b c d e f g Cite error: The named reference Barbato2018 was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference Gray2006 was invoked but never defined (see the help page).
  4. ^ a b c d Cite error: The named reference Anderson2012 was invoked but never defined (see the help page).
  5. ^ a b c Cite error: The named reference GaiaDR2 was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference Luck2018 was invoked but never defined (see the help page).
  8. ^ Cite error: The named reference Marcy2005 was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference Butler2006 was invoked but never defined (see the help page).
  10. ^ a b Cite error: The named reference Xiao2023 was invoked but never defined (see the help page).