CONICET | Buscador de Institutos y Recursos Humanos

We develop a simple model for computing planetary formation based on the core instability model for the gas accretion and the oligarchic growth regime for the accretion of the solid core. In this model several planets can form simultaneously in the disc, a fact that has important implications specially for the changes in the dynamic of the planetesimals and the growth of the cores since we consider the collision between them as a source of potential growth. With this model we consider different initial conditions to generate a variety of planetary systems and analyse them statistically. We explore the different conditions for the generation of habitable planets.