Abstract
This chapter derives the general equations for interacting rigid bodies accounting for their rolling motion on each other. The derivation of the non-rolling motions has been given previously, but to accommodating rolling and slipping motion it is necessary to develop a non-holonomic form of the equations of motion. The resulting derivation shows that the key analysis parameters for a collection of grains that gravitationally attract and rest on each other are preserved in this more advanced formulation. The chapter ends with a simple application of these results to a series of bodies that can roll on each other, satisfying a non-holonomic constraint.
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Acknowledgements
This chapter was derived from a set of lectures given at the SDSM 2017 School entitled: “Satellite Dynamics and Space Missions: Theory and Applications of Celestial Mechanics,” held August 28–September 2, 2017, in San Martino al Cimino (VT), Italy. The author acknowledges support from NASA’s SSERVI program (Institute for the Science of Exploration Targets) through institute grant number NNA14AB03A. The author acknowledges Dr. Giulio Baù for his insightful and comprehensive review of this contribution, which greatly helped to improve its discussion and correctness.
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Scheeres, D.J. (2019). Celestial Mechanics of Rubble Pile Bodies. In: Baù, G., Celletti, A., Galeș, C., Gronchi, G. (eds) Satellite Dynamics and Space Missions. Springer INdAM Series, vol 34. Springer, Cham. https://doi.org/10.1007/978-3-030-20633-8_5
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