Asteroids: 2/1 resonance and high eccentricity (Q687257)
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scientific article; zbMATH DE number 429327
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Asteroids: 2/1 resonance and high eccentricity |
scientific article; zbMATH DE number 429327 |
Statements
Asteroids: 2/1 resonance and high eccentricity (English)
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3 November 1993
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The present work consists in a systematic exploration of the dynamics in mean motion resonances and is original in at least three aspects: 1. in developing a general theory, based on the use of action-angle variables, which can be applied to any isolated mean motion resonance in the main asteroid belt; 2. in taking into account also the inclination of the asteroid (three-dimensional model) and avoiding expansions in the eccentricity; 3. in taking into account the secular perturbations introduced by the Jupiter-Saturn system.
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general theory
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action-angle variables
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inclination of the asteroid
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secular perturbations
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Jupiter-Saturn system
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