HD 143361 b

HD 143361 b is an exoplanet located approximately 224 light-years away in the constellation of Norma, orbiting the 9th magnitude G-type main sequence star HD 143361. This planet has a minimum mass of 3.0 times that of Jupiter. Because the inclination was initially unknown, the true mass was not known. This planet orbits at a distance of 2.0 AU with an orbital eccentricity of 0.18.

HD 143361 b
Discovery[1]
Discovered byMinniti et al.
Discovery dateOctober 29, 2008
Doppler spectroscopy
Orbital characteristics[2]
1.994±0.018 AU
Eccentricity0.1938+0.0047
−0.0046
1042.4±1.1 d
2.8538+0.0031
−0.003
 yr
Inclination55°+22°
−15°
or 125°+15°
−22°
33°+128°
−21°
2455761.5±4.1
240.4°+1.4°
−1.5°
Semi-amplitude72.1±1.0[3]
StarHD 143361
Physical characteristics[2]
Mass4.35+1.2
−0.66
 MJ

    This object was detected using the radial velocity method during an astronomical survey conducted by the Magellan Planet Search Program using the MIKE echelle spectrograph on the 6.5-m Magellan II (Clay) telescope.[1] In 2023, the inclination and true mass of HD 143361 b were determined via astrometry.[2]

    References

    1. Minniti, Dante; et al. (2009). "Low-Mass Companions for Five Solar-Type Stars From the Magellan Planet Search Program". The Astrophysical Journal. 693 (2): 1424–1430. arXiv:0810.5348. Bibcode:2009ApJ...693.1424M. doi:10.1088/0004-637X/693/2/1424. S2CID 119224845.
    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. Jenkins, J. S.; et al. (2017). "New planetary systems from the Calan–Hertfordshire Extrasolar Planet Search". Monthly Notices of the Royal Astronomical Society. 466 (1): 443–473. arXiv:1603.09391. Bibcode:2017MNRAS.466..443J. doi:10.1093/mnras/stw2811. S2CID 18016219.
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