We present precision radial velocity ( RV ) datasets from Keck-HIRES and from Lick Observatory ’ s new Automated Planet Finder Telescope and Levy Spectrometer on Mt . Hamilton that reveal a multiple-planet system orbiting the nearby , slightly evolved , K-type star HD 141399 . Our 91 observations over 10.5 years suggest the presence of four planets with orbital periods of 94.35 , 202.08 , 1070.35 , and 3717.35 days and minimum masses of 0.46 , 1.36 , 1.22 , and 0.69 M _ { J } respectively . The orbital eccentricities of the three inner planets are small , and the phase curves are well sampled . The inner two planets lie just outside the 2:1 resonance , suggesting that the system may have experienced dissipative evolution during the protoplanetary disk phase . The fourth companion is a Jupiter-like planet with a Jupiter-like orbital period . Its orbital eccentricity is consistent with zero , but more data will be required for an accurate eccentricity determination .