On a New Form for the Differential Equations of Relative Motion of the Three-Body Problem

Physics

Scientific paper

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Scientific paper

A new method for the development of the disturbing function of the three-body problem is outlined in this paper. A special process is devised to get the distance Δ between two planetsP 1 andP 2 in terms of their heliocentric distances. It is then shown that the differential equations of relative motion of this problem can be brought in an homogeneous set of differential equations.

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