The Anglo-Australian planet search. XXIII. Two new jupiter analogs
We report the discovery of two long-period giant planets from the Anglo-Australian Planet Search. HD 154857c is in a multiple-planet system, while HD 114613b appears to be solitary. HD 114613b has an orbital period P = 10.5 yr, and a minimum mass msin i of 0.48 M Jup HD 154857c has P = 9.5 yr and msin i = 2.6 M Jup. These new data confirm the planetary nature of the previously unconstrained long-period object in the HD 154857 system. We have performed detailed dynamical stability simulations which show that the HD 154857 two-planet system is stable on timescales of at least 108 yr. These results highlight the continued importance of "legacy" surveys with long observational baselines; these ongoing campaigns are critical for determining the population of Jupiter analogs, and hence of those planetary systems with architectures most like our own solar system.
Item Type | Article |
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Additional information | Robert A. Wittenmyer, et al, 'The Anglo-Australian planet search. XXIII. Two new Jupiter analogs', The Astrophysical Journal, Vol. 783:103 (9pp), first published online 20 February 2014. The version of record is available online at doi:10.1088/0004-637X/783/2/103 © 2014. The American Astronomical Society. All rights reserved. |
Keywords | planets and satellites: detection, planets and satellites: dynamical evolution and stability, planets and satellites: individual (hd 114613, hd 154857), techniques: radial velocities, space and planetary science, astronomy and astrophysics, nuclear and high energy physics |
Date Deposited | 15 May 2025 13:27 |
Last Modified | 31 May 2025 00:10 |
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