EXPANSION OF THE DISTURBING FUNCTION FOR HIGH ECCENTRICITY AND LARGE-AMPLITUDE OF LIBRATION

dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T15:21:00Z
dc.date.available2014-05-20T15:21:00Z
dc.date.created2014-05-20T15:21:00Z
dc.date.issued1994-12-01
dc.identifierCelestial Mechanics & Dynamical Astronomy. Dordrecht: Kluwer Academic Publ, v. 60, n. 4, p. 387-400, 1994.
dc.identifier0923-2958
dc.identifierhttp://hdl.handle.net/11449/32195
dc.identifier10.1007/BF00692023
dc.identifierWOS:A1994PZ60800001
dc.identifier5483476857978177
dc.description.abstractFollowing some ideas, developed by Woltjer (1928), Message (1989), Yokoyama (1988, 1989) and Duriez (1990) an expansion of the disturbing function is given for high values of the eccentricity and large amplitude of libration. The classical expansion can be obtained as a particular case of the present model. Several asteroids with high eccentricity and large amplitude of libration are tested and the results are much better than those obtained from the classical theory.
dc.languageeng
dc.publisherKluwer Academic Publ
dc.relationCelestial Mechanics & Dynamical Astronomy
dc.relation2.121
dc.relation1,092
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.subjectDISTURBING FUNCTION
dc.subjectHIGH ECCENTRICITY
dc.subjectLIBRATION
dc.subjectRESONANCES
dc.subjectASTEROIDS
dc.titleEXPANSION OF THE DISTURBING FUNCTION FOR HIGH ECCENTRICITY AND LARGE-AMPLITUDE OF LIBRATION
dc.typeArtículos de revistas


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