The discovery of three planets orbiting the PSR 1257 +12 [3], and the possibility of a fourth pla-net, has been an important subject in modern astrophysics in the field of extra-solar planets. Tidal forces are considered in the orbital motion. The classical mechanics equations of the planetary mo-tion were used to obtain the effect of the forces. It was observed how the tides act upon the period, eccentricity, and a precession in the orbits of planets. The precession velocity and the stability condition of the orbits for each planet are also calculated according to the Roche limit.
Keywords: Tidal forces, Roche limit.