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Loading contentA mean-motion resonance in which a body completes three orbits for every two of Jupiter's, stabilising the Hilda group in the outer main belt.
A mean-motion resonance in which a body completes three orbits for every two of Jupiter's, stabilising the Hilda group in the outer main belt.
2 modelled members.
The namesake of the Hilda group, whose members orbit in a 3:2 mean-motion resonance with Jupiter in the outer main belt.
A group of outer-belt asteroids held in a 3:2 orbital resonance with Jupiter, tracing a distinctive triangular pattern over time.
Facts on this topic will be cited from these primary and reference sources.
Mission data, planetary science, space telescopes, and public-domain imagery.
Most NASA-produced imagery is in the public domain; individual items are checked for usage terms before publication.
Orbital data, ephemerides, and small-body parameters for planets, asteroids, and comets.