Stationary solutions and their characteristic exponents in the restricted three-body problem when the more massive primary is an oblate spheroid

Details Stationary solutions and their characteristic exponents in the restricted three-body problem when the more massive primary is an oblate spheroid Stationary solutions and their characteristic exponents in the restricted three-body problem when the more massive primary is an oblate spheroid

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976cemec..13..137s&link_type=gif

Celestial Mechanics, vol. 13, Mar. 1976, p. 137-149.

Physics

35

Celestial Mechanics, Eigenvalues, Lagrangian Equilibrium Points, Oblate Spheroids, Three Body Problem, Calculus Of Variations, Eigenvectors, Equations Of Motion, Liapunov Functions, Tables (Data)

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