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Keyword: resonant trapping ×Clear all

2 claims from 1 paper

1. Physics and Astronomy › Astro and Planetary Science

   Constraints on resonant-trapping for two planets embedded in a protoplanetary disc

   Pierens and Nelson · Astronomy and Astrophysics · 2008

   Simulations of a Jupiter-mass planet with an outer body of varying mass in a protoplanetary disc show that the outer body's mass decides whether it diverges, is trapped at the gap edge, or enters resonance.

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   1. UncheckedFor outer bodies below 3.5 Earth masses, the giant planet migrates faster than the outer body, so the two planets drift apart rather than into resonance.“For planets with mass < 3.5 M_E the type II migration rate of the giant exceeds the type I migration rate of the outer body, resulting in divergent migration.”
   2. UncheckedIn the paper's disc simulations, outer bodies of 3.5 to 20 Earth masses become trapped at the edge of the gap a giant planet opens, due to corotation torques.“Outer bodies with masses in the range 3.5 < m_o < 20 M_E become trapped at the edge of the gap formed by the giant planet, because of corotation torques.”