Annotation
A method involving variation of arbitrary constants is used to solve the differetial equations for intermediate non-Kepler motion. A new system of canonical variables is introduced which is convenient for studying perturbations of this motion.
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
A.A. Orlov
Department of Stellar Mechanics and Gravimetry
Department of Stellar Mechanics and Gravimetry