HD 181433 c

HD 181433 c is an extrasolar planet located approximately 87 light-years away[4] in the constellation of Pavo, orbiting the star HD 181433. This planet is at least 0.64 times as massive as Jupiter and takes 962 days to orbit the star at an orbital distance of 1.76 astronomical units (AU), or 263 gigametres (Gm). The orbit is eccentric, however, and ranges from 1.27 AU (190 Gm) at periastron to 2.25 AU (337 Gm) at apastron.[3] François Bouchy et al. have published a paper detailing the HD 181433 planetary system in Astronomy and Astrophysics.[1]

HD 181433 c
Discovery
Discovered byBouchy et al.[1]
Discovery siteLa Silla Observatory, Chile[2]
Discovery dateJune 16, 2008[2]
Doppler spectroscopy[2]
Orbital characteristics
Apastron2.25 AU (337 million km)
Periastron1.27 AU (190 million km)
1.76 AU (263 million km)[3]
Eccentricity0.28 ± 0.02[3]
962 ± 15[3] d
2.63 y
20.0
2,453,235 ± 7.3[3]
21.4 ± 3.2[3]
StarHD 181433

    References
    1. Bouchy, François; Mayor, Michel; Lovis, Christophe; Udry, Stéphane; Benz, Willy; Bertaux, Jean-Loup; Delfosse, Xavier; Mordasini, Christoph; Pepe, Francesco; Queloz, Didier; Ségransan, Damien (2009). "The HARPS Search for Southern Extra-solar Planets. XVII. Super-Earth and Neptune-mass Planets in Multiple Planet Systems HD 47186 and HD 181433". Astronomy and Astrophysics. 496 (2): 527–31. arXiv:0812.1608. Bibcode:2009A&A...496..527B. doi:10.1051/0004-6361:200810669. S2CID 117778593.
    2. "A Trio of Super-Earths" (Press release). ESO. 2008-06-16. Archived from the original on 2008-10-07. Retrieved 2008-10-02.
    3. Schneider, J. "Notes for Planet HD 181433 c". The Extrasolar Planets Encyclopaedia. Retrieved 2008-10-02.
    4. van Leeuwen, F. (2007). "HIP 95152". Hipparcos, the New Reduction: The Astrometric Catalogue. Retrieved 2008-10-02.


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