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Status: Unchecked ×Keyword: resonance damping ×Clear all

2 claims from 1 paper

1. Physics and Astronomy › Astro and Planetary Science

   Migration of giant planets in low-viscosity discs

   Griveaud · 2024

   A thesis simulating giant-planet migration in low-viscosity gas discs, from Jupiter and Saturn to four or five planets, and testing whether the results could lead to the Solar System's Nice Model instability.

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   1. UncheckedIn low-viscosity discs, simulated Jupiter and Saturn sit in a 2:1 resonance and migrate inwards, rather than a 3:2 resonance with outward migration.“Précédemment en résonance de mouvement moyen 3:2 et en migration vers l'extérieur, elles sont maintenant dans une résonance 2:1 et migrent vers l'intérieur.”
   2. UncheckedIn a thin (and therefore cold) low-viscosity disc, the four giant planets reverse their outward migration, according to this thesis's simulations.“Nous trouvons également que dans un disque mince (donc froid), les quatre géantes inversent leur migration vers l'extérieur.”