The Anglo-Australian planet search. XXII : Two new multi-planet systems
We report the detection of two new planets from the Anglo-Australian Planet Search. These planets orbit two stars each previously known to host one planet. The new planet orbiting HD 142 has a period of 6005 +/- 427 days, and a minimum mass of 5.3 M-Jup. HD 142c is thus a new Jupiter analog: a gas-giant planet with a long period and low eccentricity (e = 0.21 +/- 0.07). The second planet in the HD 159868 system has a period of 352.3 +/- 1.3 days and m sin i = 0.73 +/- 0.05 M-Jup. In both of these systems, including the additional planets in the fitting process significantly reduced the eccentricity of the original planet. These systems are thus examples of how multiple-planet systems can masquerade as moderately eccentric single-planet systems.
Item Type | Article |
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Additional information | Robert A. Wittenmyer, et al, 'The Anglo-Australian planet search XXII. Two new multi-planet systems', The Astrophysical ournal, Vol 753 (2) : 169, 2012. The version of record is available online at doi:10.1088/0004-637X/753/2/169. © 2012. The American Astronomical Society. All rights reserved. |
Date Deposited | 15 May 2025 12:29 |
Last Modified | 30 May 2025 23:52 |
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