Sky science
Mean Motion Resonance
Direct answer
Mean Motion Resonance is an orbital resonance tied to a near-integer ratio of average angular orbital rates.
It couples bodies through commensurate mean motions.
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At a glance
- Found in
- Astronomy & Skywatching
- Related
- Escape Velocity, Orbital Resonance, Lagrange Point, Hill Sphere
It couples bodies through commensurate mean motions.
A scientific orientation to scale, light, or motion; the article supplies the precise definition.
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The story behind Mean Motion Resonance
Celestial mechanicians used perturbation theory to identify resonant terms and stability zones.
A one-minute story
The Wandering Stars
How the moving planets were watched, named and found, and what a transit is.

Why Mean Motion Resonance matters
Mean Motion Resonance explains structured gaps, rings, satellite relations, and protected small-body orbits.
How to read Mean Motion Resonance
Confirm a resonant argument librates before declaring resonance.
Mean Motion Resonance in practice: an example
Jupiter’s resonances help create Kirkwood gaps in the asteroid belt.
Where readings of Mean Motion Resonance go wrong
Mean motion is an average; instantaneous angular speeds can differ strongly.
Sources and editorial method
Research references used for this entry include:
- NASA Science: Solar System Exploration - NASA overview of planets, moons, small bodies, rings, and the structure of the Solar System.
- NASA Science: Universe Glossary - NASA definitions for common stellar, galactic, orbital, and high-energy astronomy terms.
- Source
- The Great Almanac Dictionary
- Category
- Astronomy & Skywatching
- Last updated
- 2026-09-26
Map a mean-motion resonance
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Common questions
What is Mean Motion Resonance?
Mean Motion Resonance is an orbital resonance tied to a near-integer ratio of average angular orbital rates.
What do people get wrong about Mean Motion Resonance?
Mean motion is an average; instantaneous angular speeds can differ strongly.
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