At present the scientists who study Mars are looking forward to the seis- mic study of Mars. As a result of preparing for the experiment, the papers in which seismic elds in the Martian interiors due to marsquakes are modeled [1-4]. In studies [5, 6] an attempt to model the distribution of the dissipative factor of Mars Qμ(l) has been made. The periods of free oscillations of a planet are its important physical characteristics. If during the seismic experiment of mission InSight [4] an event with low enough number of oscillation is recorded, the problem of interior structure of the planet and the distribution of the dissipative factor could be signi cantly moved forward.