Effect of solar radiation pressure on the motion and stability of the system of two inter-connected satellites when their center of mass moves in a circular orbit

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Circular Orbits, Dynamic Stability, Orbit Perturbation, Radiation Pressure, Solar Radiation, Tethered Satellites, Center Of Mass, Equations Of Motion, Gravitational Fields, Satellite Orbits

Scientific paper

The effect of a perturbative force, solar pressure, on the motion and stability of two cable-connected satellites in the earth's central gravitational field of force has been studied. The osculating plane of the orbit of the center of mass has been supposed to be inclined at a constant angle with the plane of the ecliptic. The particular solutions of the nonlinear, nonhomogeneous and nonautonomous equations of relative motion in three-dimensional cases have been obtained. The particular solution in which the system lies wholly along the radius vector joining the attracting center and the center of mass of the system under the central attracting force alone was found previously to be stable (Singh, 1973). It has been established in the present case too that the same particular solution remains stable if the parameter of the solar pressure lies within a certain limit.

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