Physics
Scientific paper
Sep 1972
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972cemec...6..208a&link_type=abstract
Celestial Mechanics, Volume 6, Issue 2, pp.208-213
Physics
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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