Annotation
А canonical system of differential equations for а disturbed motion of the threebody stellar problem has been obtained. An analytical method of solution with consideration for the third and fourth order terms in the Hamiltonian of the problem has been developed. Secular parts of angular variables g1 and g2 in the arguments of cosines have been introduced as the new variables.
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
N.A. Solovaya
Sternberg State Institute of Astronomy
Sternberg State Institute of Astronomy
Science News of the Faculty of Physics, Lomonosov Moscow State University
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