The dynamics of objects in the inner edgeworth-kuiper belt
Objects in 3:2 mean motion resonance with Neptune are protected from close encounters with Neptune by the resonance. Bodies in orbits with semi-major axis between 39.5 and about 42 AU are not protected by the resonance; indeed due to overlapping secular resonances, the eccentricities of orbits in th...
| Autores principales: | Jones, D.C., Williams, I.P., Melita, M.D. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_01679295_v97_n3-4_p435_Jones |
| Aporte de: |
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