The general form of the equations of motion in the photogravitational restricted two-body problem

Statistics – Computation

Scientific paper

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Celestial Mechanics, Equations Of Motion, Gravitational Effects, Orbital Mechanics, Two Body Problem, Comets, Computational Astrophysics, Coordinates, Differential Equations, Field Theory (Physics)

Scientific paper

The motion of a body in the field of an attractive force and a repulsive force due to a gravitating and radiating point (a sphere) is considered. The general form of the differential equations of the translational-rotational motion of the body are obtained in the framework of the restricted two-body problem. The equations can be applied in photogravitational celestial mechanics, stellar dynamics, and comet dynamics.

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