Precise radial velocities from the Anglo-Australian Telescope (AAT) confirm the presence of a rare short-period planet around the K0 giant HD 121056. An independent two-planet solution using the AAT data shows that the inner planet has P = 89.1 ± 0.1 days, and m sin i = 1.35 ± 0.17 MJup. These data also confirm the planetary nature of the outer companion, with m sin i = 3.9 ± 0.6 MJup and a = 2.96 ± 0.16 AU. HD 121056 is the most-evolved star to host a confirmed multiple-planet system, and is a valuable example of a giant star hosting both a short-period and a long-period planet.
CITATION STYLE
Wittenmyer, R. A., Wang, L., Liu, F., Horner, J., Endl, M., Johnson, J. A., … Carter, B. D. (2015). The pan-pacific planet search. II. Confirmation of a two-planet system around HD 121056. Astrophysical Journal, 800(1). https://doi.org/10.1088/0004-637X/800/1/74
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