;
Alberto Abad Medina
[1]
Zaragoza, España
In this paper we generate an analytical theory for the motion of the artificial satellite in which the tesseral model of the planetary potential is considered. We inte- grate the problem by applying the Lie-Deprit method with three consecutive canonical transformations: the elimination of the parallax, the Delaunay normalization and a final double normalization to eliminate the perigee and the node. We apply this the- ory to the 2 × 2, 4 × 4, and 5 × 5 tesseral models and we propagate the motion of the satellite, and also, we present the error of this analytical propagation versus the numerical propagation for a wide range of initial conditions.
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