Resonance in the Restricted Problem of Three Bodies
Abstract
A formal solution of the motion of an asteroid whose mean motion is approximately rational with that of Jupiter is developed. The series obtained are extended formally to an arbitrary degree of approximation in powers of the small parameter of the problem: the ratio of the mass of Jupiter to that of the sun. Specific numerical applications have been and will be published separately.
 Publication:

The Astronomical Journal
 Pub Date:
 December 1969
 DOI:
 10.1086/110930
 Bibcode:
 1969AJ.....74.1254G