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HD 129445 b

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Eccentric Jupiter gas giant exoplanet orbiting the star HD 129445
HD 129445 b
Discovery
Discovered byArriagada et al.
Discovery siteLas Campanas Observatory
Discovery dateJanuary 26, 2010
Detection methodDoppler spectroscopy
Orbital characteristics
Semi-major axis2.984+0.039
−0.054 AU
Eccentricity0.572+0.087
−0.086
Orbital period (sidereal)1802+34
−47 d
4.933+0.093
−0.13 yr
Average orbital speed17
Inclination52°+24°
−19° or 128°+19°
−24°
Longitude of ascending node105°+47°
−74°
Time of periastron2456705+57
−77
Argument of periastron163.8°+8.8°
−8.9°
Semi-amplitude38 ± 6
StarHD 129445
Physical characteristics
Mass2.51+1.1
−0.54 MJ

HD 129445 b is an eccentric Jupiter gas giant exoplanet orbiting the star HD 129445 which was discovered by the Magellan Planet Search Program in 2010. Its minimum mass is 1.6 times Jupiter's, and it takes 5 years to complete one orbit around HD 129445, a G-type star approximately 219 light years away. In 2023, the inclination and true mass of HD 129445 b were determined via astrometry.

References

  1. ^ Arriagada, Pamela; et al. (2010). "Five Long-period Extrasolar Planets in Eccentric orbits from the Magellan Planet Search Program". The Astrophysical Journal. 711 (2): 1229–35. arXiv:1001.4093. Bibcode:2010ApJ...711.1229A. doi:10.1088/0004-637X/711/2/1229. S2CID 118682009.
  2. ^ Xiao, Guang-Yao; Liu, Yu-Juan; et al. (May 2023). "The Masses of a Sample of Radial-Velocity Exoplanets with Astrometric Measurements". Research in Astronomy and Astrophysics. 23 (5): 055022. arXiv:2303.12409. Bibcode:2023RAA....23e5022X. doi:10.1088/1674-4527/accb7e.
  3. "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2020-01-10.
  4. "HD 129445". Universe Guide. 25 January 2015. Retrieved 2020-01-10.
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