Protostars and Planets VI, Heidelberg, July 15-20, 2013
Poster 2B076
From planetesimals to planets
Thiabaud, Amaury (Center For Space and Habitability & Physikalisches Institut, University of Bern)
Marboeuf, Ulysse (Center For Space and Habitability & Physikalisches Institut, University of Bern)
Alibert , Yann (Center For Space and Habitability & Physikalisches Institut, University of Bern & Observatoire de Besançon)
Cabral, Nahuel (Center For Space and Habitability & Physikalisches Institut, University of Bern)
Benz, Willy (Center For Space and Habitability & Physikalisches Institut, University of Bern)
Leya, Ingo (Center For Space and Habitability & Physikalisches Institut, University of Bern)
Mezger, Klaus (Center For Space and Habitability & Institut für Geologie, University of Bern)
Abstract:
Computing the chemical composition of planet is a growing need for planetary formation models
and for the search of habitable planets as they are probably related. Previous works have been investigating the chemical composition of planet, combining dynamical process of planetary formation and chemistry. However, either these studies have only focused on the volatile content of the planets (CO, H2O, CO2, CH4) either the composition of the planets have been determined in a non self-consistent manner.
I We present here results of calculations of chemical compositions of planets with the combination
of a planet formation model for both refractory and volatile compounds. Combination has been
carried self-consistency with the planetary formation model.
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