On Non-Stationary Problems of Celestial Mechanics

1979

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DOI 10.1017/s0074180900012493
Data confidence 70 medium
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Abstract

Some non-stationary problems of celestial mechanics can be described in an inertial system of right-angled coordinates with gravitational potential of the form: where is a sufficiently arbitrary function of time and is the meaning of in the initial epoch For example, in a two-body problem of variable mass we have: