We present new precision radial velocities and a three-planet Keplerian orbit fit for the V = 8.5 , G5 V star HIP 14810 .
We began observing this star at Keck Observatory as part of the N2K Planet Search Project . Wright et al .
( 2007 ) announced the inner two planets to this system , and subsequent observations have revealed the outer planet planet and the proper orbital solution for the middle planet .
The planets have minimum masses of 3.9 , 1.3 , and 0.6 \mbox { M } _ { \mbox { Jup } } and orbital periods of 6.67 , 147.7 , and 952 d , respectively .
We have numerically integrated the family of orbital solutions consistent with the data and find that they are stable for at least 10 ^ { 6 } yr. Our photometric search shows that the inner planet does not transit .