Theory of the Trojan asteroids,IV |
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Authors: | Boris Garfinkel |
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Affiliation: | (1) Yale University Observatory, New Haven, Conn., USA |
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Abstract: | In a previous publication (1977) the author has constructed a family () of long-periodic orbits in the Trojan case of the restricted problems of three bodies. Here he constructs the domain of the analytical solution of the problem of the motion, excluding the vicinity of thecritical divisor which vanishes at the exact commensurability of the natural frequencies 1 and 2. In terms of thecritical masses mj(2), or the associatedcritical energies j2(m), is the intersection of the intervals ofshallow resonance, of the form. Inasmuch as the intervals |2–j2|<j ofdeep resonance aredisjoint, it follows that (1) the disjointed family () embraces the tadpole branch, 021, lying in: and (2) despite the clustering of j2(m) atj=, the family () includes, for 2=1, an asymptoticseparatrix that terminates the branch in the vicinity of the Lagrangian pointL3.In a similar manner, the family () can be extended to the horseshoe branch 1<222. |
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