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Confined chaotic motion in three-body resonances: trapping of trans-Neptunian material induced by gas-drag

de la Fuente Marcos, R. & de la Fuente Marcos, C. (2008)

Published
Jul 21, 2008
DOI
10.1111/j.1365-2966.2008.13385.x

At a GlanceAI

Gas drag in the protoplanetary disc can trap TNO embryos into Neptune's 3:2 and 2:1 resonances, in a size-selective way.

SummaryAI

Revisiting the idea that gas drag could explain the dominance of the 3:2 resonance, the authors simulate the planar restricted four-body problem with Uranus and Neptune. Trapping occurs into the 3:2, the 2:1 and other resonances, along with corotation resonances that later become pure Lindblad resonances (about 0.5 Myr). Trapping is strongly size selective: the 3:2 dominates for submetric particles, the 2:1 for larger ones. Confined chaotic motion raises both trapping efficiency and eccentricities. Results hold for a more compact planetary configuration too.

Method SnapshotAI

Numerical simulations of the planar restricted four-body problem with gas drag.

BackgroundAI

Resonance capture, dissipative forces, restricted N-body problem.

Expert Review: Confined chaotic motion in three-body resonances: trapping of trans-Neptunian material induced by gas-drag | Marginalia