Abstract
n this paper we consider the two-body problem of a spherical pseudo-rigid body and a rigid sphere. Due to the rotational and "re-labelling" symmetries, the system is shown to possess conservation of angular momentum and circulation. We follow a reduction procedure similar to that undertaken in the study of the two-body problem of a rigid body and a sphere so that the computed reduced non-canonical Hamiltonian takes a similar form. We then consider relative equilibria and show that the notions of locally central and planar equilibria coincide. Finally, we show that Riemann's theorem on pseudo-rigid bodies has an extension to this system for planar relative equilibria.
Original language | English |
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Journal | Celestial Mechanics and Dynamical Astronomy |
Volume | 112 |
Pages (from-to) | 169-190 |
ISSN | 0923-2958 |
DOIs | |
Publication status | Published - 2012 |