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. © 2014. The American Astronomical Society. All rights reserved.
CITATION STYLE
Wittenmyer, R. A., Horner, J., Tinney, C. G., Butler, R. P., Jones, H. R. A., Tuomi, M., … Wright, D. (2014). The Anglo-Australian planet search. XXIII. Two new jupiter analogs. Astrophysical Journal, 783(2). https://doi.org/10.1088/0004-637X/783/2/103
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