Observatoire De Paris, D.A.N.O.F./URA 1125, 61 Avenue de l'Observatoire, 75014 Paris
Here are presented the calculations concerning the determination of precession-nutation series of Mars. These tables are based on the Kinoshita's method for a rigid Earth. Our results are compared to those of Raesenburg & King, Borderies and Hilton. And so the well-adapted parameters could be determined to describe the planets'rotation (except the Earth) and the effects of Phobos and Deimos on the rotation of Mars are computed.