Formation of terrestrial planets in eccentric and inclined giant-planet systems

Abstract : The orbits of extrasolar planets are more various than the circular and coplanar ones of the Solar system. We study the impact of inclined and eccentric massive giant planets on the terrestrial planet formation process. The physical and orbital parameters of the giant planets considered in this study arise from n-body simulations of three giant planets in the late stage of the gas disc, under the combined action of Type II migration and planet-planet scattering. At the dispersal of the gas disc, the two- and three-planet systems interact then with an inner disc of planetesimals and planetary embryos. We discuss the mass and orbital parameters of the terrestrial planets formed by our simulations, as well as their water content. We also investigate how the disc of planetesimals and planetary embryos modifies the eccentric and inclined orbits of the giant planets.
Type de document :
Communication dans un congrès
2016DPS..4810501S - American Astronomical Society, DPS meeting #48, id.#105.01 05 held in Pasadena, California 16–21 October 2016, Oct 2016, Pasadena, United States. 48, 2016
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https://hal.archives-ouvertes.fr/hal-01379021
Contributeur : Marie-Paule Pomies <>
Soumis le : mardi 11 octobre 2016 - 09:41:40
Dernière modification le : mercredi 12 octobre 2016 - 01:27:47

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Sotiris Sotiriadis, Anne-Sophie Libert, Sean N. Raymond. Formation of terrestrial planets in eccentric and inclined giant-planet systems. 2016DPS..4810501S - American Astronomical Society, DPS meeting #48, id.#105.01 05 held in Pasadena, California 16–21 October 2016, Oct 2016, Pasadena, United States. 48, 2016. <hal-01379021>

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