Orbital Evolution in Resonance Lock.I.The Restricted 3-Body Problem
R. S. Gomes (1997)
- Published
- Nov 1, 1997
- Journal
- The Astronomical Journal · Vol. 114
- DOI
- 10.1086/118637
At a GlanceAI
Studies orbital evolution under resonance lock in the restricted three-body problem, clarifying dynamics of mean-motion resonant trapping.
SummaryAI
The work examines how a small body’s orbit can evolve while remaining locked in a mean-motion resonance within the restricted three-body problem. By focusing on “resonance lock,” it frames resonant trapping as a driver of long-term orbital change rather than a static configuration. This helps interpret how resonances can shape the architecture and transport processes of small-body populations in planetary systems.
Method SnapshotAI
The study uses theoretical analysis within the restricted three-body problem framework focused on mean-motion resonance dynamics.
BackgroundAI
Celestial mechanics with emphasis on the restricted three-body problem and mean-motion resonances.