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The aim of this work is to provide an analytical model to characterize theequilibrium points and the phase space associated with the singly-averageddynamics caused by the planetary oblateness coupled with the solar radiationpressure perturbations. A two-dimensional differential system is derived byconsidering the classical theory, supported by the existence of an integral ofmotion comprising semi-major axis, eccentricity and inclination. Under thesingle resonance hypothesis, the analytical expressions for the equilibriumpoints in the eccentricity-resonant angle space are provided, together with thecorresponding linear stability. The Hamiltonian formulation is also given. Themodel is applied considering, as example, the Earth as major oblate body, and asimple tool to visualize the structure of the phase space is presented.Finally, some considerations on the possible use and development of theproposed model are drawn.

Phase space description of the dynamics due to the coupled effect of the planetary oblateness and the solar radiation pressure perturbations