Equations of Motion of the Elliptical Restricted Problem of Three Bodies with Variable Masses

Astronomy and Astrophysics – Astronomy

Scientific paper

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Celestial Mechanics, Stellar Dynamics, Time

Scientific paper

The differential equations of motion of the elliptical restricted problem of three bodies with variable masses are derived with the help of Meshcherskii's transformation. Here we see that these equations of motion differ from the equations of motion of the elliptical restricted problem of three bodies with constant mass only by a factor Δ=(β2-γα).

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