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Dynamics of trans-Neptunian objects near the 3/1 mean-motion resonance with Neptune

Alves-Carmo, Alan J. et al. (2023)

Published
Sep 1, 2023
DOI
10.1051/0004-6361/202244982

At a GlanceAI

Stability maps in the resonant angle show TNOs near the 3/1 resonance can be highly inclined; Kozai islands vanish with all giant planets.

SummaryAI

The authors study detected TNOs near Neptune's 3/1 resonance, first with a semi-analytic three-body model of the coplanar secular dynamics, then with surface sections and stability maps for the non-averaged problem. Maps computed in terms of the resonant angle prove a powerful tool. Objects near the 3/1 can have very high inclinations; in the three-body problem many could also be stable outside the resonance thanks to a Kozai resonance, but with all four giant planets the Kozai regions disappear and only the 3/1 region (e below about 0.5) survives.

Method SnapshotAI

Semi-analytic secular model, surfaces of section, stability maps, full N-body checks.

BackgroundAI

Hamiltonian treatment of resonances, Kozai mechanism, chaos indicators.