Transport dynamics : from the bicircular to the real solar system problem
Ollé, Mercè (Universitat Politècnica de Catalunya. Departament de Matemàtica Aplicada I)
Barrabés Vera, Esther (Universitat de Girona. Departament d'Informàtica i Matemàtica Aplicada)
Gómez, Gerard (Universitat de Barcelona. Departament de Matemàtica Aplicada i Anàlisi)
Mondelo González, José María (Universitat Autònoma de Barcelona. Departament de Matemàtiques)
Imprint: |
Cham, etc : Birkhäuser, cop. 2015 |
Description: |
4 pàg. |
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. |
Rights: |
Tots els drets reservats. |
Language: |
Anglès |
Series: |
Trends in mathematics. Research perspectives CRM Barcelona ; 4 |
Document: |
Capítol de llibre ; recerca ; Versió acceptada per publicar |
Subject: |
Periodic orbit ;
Solar system ;
Circular orbit ;
Invariant manifold ;
Body problem |
Published in: |
Extended Abstracts Spring 2014, part 1- Hamiltonian Systems and Celestial Mechanics, 2015, p. 17-21, ISBN 9783319221298 |
DOI: 10.1007/978-3-319-22129-8_8
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Record created 2020-05-04, last modified 2023-02-15