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Dynamical architectures of planetary systems induced by orbital migration

By Ewa Szuszkiewicz and John C. B. Papaloizou

Abstract

The aim of this talk is to present the most recent advances in establishing plausible planetary system architectures determined by the gravitational tidal interactions between the planets and the disc in which they are embedded during the early epoch of planetary system formation. We concentrate on a very well defined and intensively studied process of the disc-planet interaction leading to the planet migration. We focus on the dynamics of the systems in which low-mass planets are present. Particular attention is devoted to investigation of the role of resonant configurations. Our studies, apart from being complementary to the fast progress occurring just now in observing the whole variety of planetary systems and uncovering their structure and origin, can also constitute a valuable contribution in support of the missions planned to enhance the number of detected multiple systems.Comment: 10 pages with 5 figures, pdflatex, to appear in the proceedings of the conference "Extra-solar Planets in Multi-body Systems: Theory and Observations"; eds. K. Gozdziewski, A. Niedzielski and J. Schneider, EAS Publication Serie

Topics: Astrophysics - Earth and Planetary Astrophysics
Publisher: 'EDP Sciences'
Year: 2009
DOI identifier: 10.1051/eas/1042034
OAI identifier: oai:arXiv.org:0911.1555

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