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• W3100247756 abstract "A simple rearrangement of the torque free motion Hamiltonian shapes it as a perturbation problem for bodies rotating close to the principal axis of maximum inertia, independently of their triaxiality. The complete reduction of the main part of this Hamiltonian via the Hamilton-Jacobi equation provides the action-angle variables that ease the construction of a perturbation solution by Lie transforms. The lowest orders of the transformation equations of the perturbation solution are checked to agree with Kinoshita's corresponding expansions for the exact solution of the free rigid body problem. For approximately axisymmetric bodies rotating close to the principal axis of maximum inertia, the common case of major solar system bodies, the new approach is advantageous over classical expansions based on a small triaxiality parameter." @default.
• W3100247756 created "2020-11-23" @default.
• W3100247756 creator A5076476638 @default.
• W3100247756 date "2014-02-04" @default.
• W3100247756 modified "2023-09-25" @default.
• W3100247756 title "Short-axis-mode rotation of a free rigid body by perturbation series" @default.
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• W3100247756 doi "https://doi.org/10.1007/s10569-014-9532-0" @default.
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