Interactions between a massive planet and a disc

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics

Scientific paper

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Two-page contribution to "Pathways towards habitable planets". An extended version of this note will be soon published in ApJ

Scientific paper

We analyse the potential migration of massive planets forming far away from an inner planetary system. For this, we follow the dynamical evolution of the orbital elements of a massive planet undergoing a dissipative process with a gas disc centred around the central sun. We use a new method for post-Newtonian, high-precision integration of planetary systems containing a central sun by splitting the forces on a particle between a dominant central force and additional perturbations. In this treatment, which allows us to integrate with a very high-accuracy close encounters, all gravitational forces are integrated directly, without resorting to any simplifying approach. After traversing the disc a number of times, the planet is finally trapped into the disc with a non-negligible eccentricity

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