Periodic solutions of the motion of a rigid body about the center of mass in a central Newtonian field.

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Celestial Mechanics: Periodic Orbits

Scientific paper

The equations of motion of a rigid body about a fixed point in a central Newtonian field are reduced to the equation of plane motion under the action of potential and gyroscopic forces, using the isothermal coordinates on the inertia ellipsoid. The construction of periodic solutions in the neighbourhood of nearly equilibrium points, by using Lyapunov's theorem of the holomorphic integral is obtained and the necessary and sufficient conditions for the stability of the system are given.

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