HD 143361 b

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HD 143361 b
Discovery
Discovered byMinniti et al.
Discovery dateOctober 29, 2008
Doppler spectroscopy
Orbital characteristics
1.98±0.07 AU
Eccentricity0.193±0.015[1]
1046.2±3.2[1] d
241.2±3.4[1]
Semi-amplitude72.1±1.0[1]
StarHD 143361

HD 143361 b is an extrasolar planet located approximately 194 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 is not known, the true mass is not known. This planet orbits at a distance of 2.0 AU with an orbital eccentricity of 0.18.

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.[2]

References[]

  1. ^ a b c d 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.
  2. ^ 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.

External links[]

Coordinates: Sky map 16h 01m 50.3484s, −44° 26′ 04.335″


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