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Collisions of Planetesimals and Formation of Planets

Published online by Cambridge University Press:  27 January 2016

Rudolf Dvorak ,
Thomas I. Maindl ,
Áron Süli ,
Christoph M. Schäfer ,
Roland Speith  and
Christoph Burger
Rudolf Dvorak
Affiliation:
Department of Astrophysics, University of Vienna, Austria email: [email protected]
Thomas I. Maindl
Affiliation:
Department of Astrophysics, University of Vienna, Austria email: [email protected]
Áron Süli
Affiliation:
Eötvös University, Department of Astronomy, Budapest, Hungary
Christoph M. Schäfer
Affiliation:
Institut für Astronomie und Astrophysik, Eberhard Karls Universität Tübingen, Germany
Roland Speith
Affiliation:
Physikalisches Institut, Eberhard Karls Universität Tübingen, Germany
Christoph Burger
Affiliation:
Department of Astrophysics, University of Vienna, Austria email: [email protected]
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Abstract

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We present preliminary results of models of terrestrial planet formation using on the one hand classical numerical integration of hundreds of small bodies on CPUs and on the other hand—for comparison—the results of our GPU code with thousands of small bodies which then merge to larger ones. To be able to determine the outcome of collision events we use our smooth particle hydrodynamics (SPH) code which tracks how water is lost during such events.

Keywords

methods: n-body simulationsmethods: numericalminor planetsasteroidsplanets and satellites: formationsolar system: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S314: Young Stars & Planets Near the Sun , November 2015 , pp. 251 - 252
Copyright
Copyright © International Astronomical Union 2016 

References

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