The seismic experiment is going on Mars [1, 2].The seismic experiment is to insert some corrections to the model distribution of the dissipative function. At present the knowledge of the model dissipative factor of Martian interiors is of importance for the interpretation of seismic recordings. The values of the dissipative factor of Martian interiors were discussed from physical point of view in [3], where the distribution Qμ in PREM was taken as a trial one. In [4] assuming that on the P–Т plane, the areotherms and the geotherm are rather close, we took the four-layers piecewise constant distribution Qμ(l) from QLM9 model [5] up to the depth of l = 670 km as a trial zero approximation, and adapted it to the conditions of Martian interiors. In the present study we calculate the correction, which the third- and higher-order tide introduce into the estimate of Q factor for Mars.