Evidence for multiple companions to upsilon andromedae

The bright F8 V star upsilon Andromedae was previously reported to have a 4 .6 day Doppler velocity periodicity, consistent with having a Jupiter-mass companion orbiting at 0.059 AU. Follow-up observations by both the Lick and Advanced Fiber-Optic Echelle spectrometer (AFOE) planet survey programs co nfirm this periodicity and reveal additional periodicities at 241 and 1267 days. These periodicities are consistent with Keplerian orbital motion and imply two additional companions orbiting at 0.83 and 2.5 AU, with minimum ( M sin i) masses of 2.0 and 4.6 M-JUP, respectively. Non-Keplerian explanati ons for the observed Doppler velocity variations, including radial and nonr adial pulsations, rotational modulation of surface features, and stellar ma gnetic cycles, are examined. These explanations seem unlikely based on the observed photometric and chromospheric stability of the star. This putative three-planet system is found to be dynamically stable by both analytic tec hniques and numerical simulations. The outer two companions both reside in eccentric orbits, as do all nine known extrasolar planet candidates in dist ant orbits. If real, this multiple-planet system is the first around a main -sequence star, and its study should offer insights into planet formation, planet-planet interactions, and the observed eccentricities of planetary or bits.