Abstract
The main goal is to give an explanation of transport in the Solar System based in dynamical systems theory. More concretely, we consider as an approximation of the Solar System, a chain of independent Bicircular problems in order to get a first insight of transport in this simplified case. Each bicircular problem (BP) consists of the Sun (S), Jupiter (J), a planet and an infinitesimal mass.
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References
E. Barrabés, G. Gómez, J.M. Mondelo, and M. Ollé, “Transport in the Solar System”. Preprint.
G. Gómez, J. Llibre, R. Martínez, and C. Simó, “Study on orbits near the triangular libration points in the perturbed restricted three-body problem”. Report ESOC 6139/84/D/JS(SC), 1987.
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Ollé, M., Barrabés, E., Gómez, G., Mondelo, J.M. (2015). Transport Dynamics: From the Bicircular to the Real Solar System Problem. In: Corbera, M., Cors, J., Llibre, J., Korobeinikov, A. (eds) Extended Abstracts Spring 2014. Trends in Mathematics(), vol 4. Birkhäuser, Cham. https://doi.org/10.1007/978-3-319-22129-8_8
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DOI: https://doi.org/10.1007/978-3-319-22129-8_8
Publisher Name: Birkhäuser, Cham
Print ISBN: 978-3-319-22128-1
Online ISBN: 978-3-319-22129-8
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