Luiz Alberto de Paula in research grants and scholarships supported by FAPESP.
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According to the classical accretion models, giant planets are formed through the planet core formation in the disk of planetesimals. When a core attains a determined (critical) mass, it is capable to capture the residual gas of the protoplanetary disk which will constitute its envelope. Therefore a giant planet is formed. The critical point of this scenario is to adjust the times of the …
The study of planetary migration is the purpose of the present Project. Planet migration is the process by which a planet's orbital radius changes in time. The main agent for causing migration is the gravitational interaction of the young planet with the gaseous disk from which it forms. The already developed models predict two main types of migration, I and II. The first one is character…
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