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intermediate

Exploring the 7:4 mean motion resonance—I: Dynamical evolution of classical transneptunian objects

Lykawka, Patryk Sofia & Mukai, Tadashi (2005)

Published
Sep 1, 2005
DOI
10.1016/j.pss.2004.12.015

At a GlanceAI

The 7:4 resonance in the classical belt is weakly chaotic and keeps exciting and mixing TNO orbits to this day.

SummaryAI

Motivated by a density gap and color anomalies near the 7:4 resonance (a about 43.7 au), the authors follow almost 10,000 test particles under the four giant planets for the age of the Solar System. The resonance is weakly chaotic: most resonant particles get their eccentricities and inclinations pumped, stable locking is rare, and particles typically escape after reaching e about 0.2, on 10^8-10^9 yr timescales. Only 12-15% of real 7:4 TNOs are expected to be retained, and classical objects near the resonance keep evolving and mixing until today.

Method SnapshotAI

Numerical integration of test particles over 4-5 Gyr with a chaotic diffusion experiment.

BackgroundAI

Mean-motion resonances and chaotic diffusion.