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.
CITATION STYLE
Ollé, M., Barrabés, E., Gómez, G., & Mondelo, J. M. (2015). Transport Dynamics: From the Bicircular to the Real Solar System Problem. In Trends in Mathematics (Vol. 4, pp. 45–48). Springer International Publishing. https://doi.org/10.1007/978-3-319-22129-8_8
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