Turning solar systems into extrasolar planetary systems

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• Davies, M (Lund)
• Thursday 20 August 2009, 10:40-11:00
• Seminar Room 1 Newton Institute.

If you have a question about this talk, please contact Mustapha Amrani.

Dynamics of Discs and Planets

Many stars are formed in some form of cluster or association. These environments can have a much higher number density of stars than the field of the galaxy. Such crowded places are hostile environments: a large fraction of initially single stars will undergo close encounters with other stars or exchange into binaries. We describe how such close encounters and exchange encounters will affect the properties of a planetary system around a single star. We define singletons as single stars which have never suffered close encounters with other stars or spent time within a binary system. It may be that planetary systems similar to our own solar system can only survive around singletons. Close encounters or the presence of a stellar companion will perturb the planetary system, leading to strong planet-planet interactions, often leaving planets on tighter and more eccentric orbits. Thus, planetary systems which initially resembled our own solar system may later more closely resemble the observed extrasolar planetary systems.

This talk is part of the Isaac Newton Institute Seminar Series series.

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