  Precise radial velocities from the Anglo-Australian Telescope 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.
