Construction of Approximate Solution of Equations for Disturbed Motion of a Satellite of a Spheroidal Planet

Details Construction of Approximate Solution of Equations for Disturbed Motion of a Satellite of a Spheroidal Planet Construction of Approximate Solution of Equations for Disturbed Motion of a Satellite of a Spheroidal Planet

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..767m&link_type=abstract

Astronomicheskii Zhurnal, Vol.60:4, P. 767, 1983

Astronomy and Astrophysics

Astronomy

Scientific paper

The disturbed motion of a satellite of a spheroidal planet under the action of nonautonomous potential disturbances is considered. An additional fictitious degree of freedom is added, as well as a corresponding pair of adjoint canonical variables. Then, the extended Hamiltonian system of equations obtained in relation to Euler's orbital elements is solved by the Delaunay-von Zeipel method of canonical transformations.

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