Stable stationary solutions for the unrestricted three body problem in the case of first order resonance

Details Stable stationary solutions for the unrestricted three body problem in the case of first order resonance Stable stationary solutions for the unrestricted three body problem in the case of first order resonance

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997kosis..35..559s&link_type=abstract

Kosmicheskie Issledovaniya, vol. 35, p. 559, 560

Computer Science

Three Body Problem, Orbital Resonances (Celestial Mechanics), Solar Orbits, Analytic Functions, Numerical Stability

Scientific paper

The paper provides a summary of the results obtained in an earlier study (Shinkin, 1996) concerned with the unrestricted three body problem for the case of first order resonance and central planet compression. New analytical stationary solutions obtained to third order accuracy with respect to the eccentricities and inclinations of the planet orbits are presented.

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