Resonances in the asteroid and trans–Neptunian belts: A brief review
Tabaré Gallardo (2018)
- Published
- Aug 1, 2018
- Journal
- Planetary and Space Science · Vol. 157
- DOI
- 10.1016/j.pss.2018.03.007
At a GlanceAI
Concise 2018 review summarizing mean-motion resonances shaping asteroid and trans-Neptunian belt dynamics.
SummaryAI
The article provides a brief, field-oriented overview of how mean-motion resonances structure and drive the dynamics of both the asteroid belt and the trans-Neptunian region. By synthesizing results across these two populations, it highlights resonance-related behaviors (e.g., trapping, transport, and long-term stability) as a unifying framework for interpreting observed orbital distributions. As a review, it is useful for quickly orienting readers to the main resonance concepts, key resonant populations, and the role resonances play in Solar System evolution.
Method SnapshotAI
Narrative literature review synthesizing prior theoretical, numerical, and observational work on mean-motion resonances.
BackgroundAI
Celestial mechanics basics, especially mean-motion resonances and small-body dynamics in the Solar System.