CONICET | Buscador de Institutos y Recursos Humanos

Although planets with masses less than 15Mearth have already been detected, the sample is still not large enough and we also have to rely on what we know from our own Solar System, as well as on computational models, to gain a better understanding of the planetary formation process. Our principal aim is to analyse which factors will inﬂuence the formation of these habitable planets. To this end, we developed a simple code which allows us to form a large population of planets and study them statistically, analysing which parameters favor their formation.