The stability of the 2:3 mean motion resonance with Neptune is systematically explored and compared to the observed resonant population. It is shown that orbits with small and moderate amplitudes of the resonant angle are stable over the age of the Solar System. The observed resonant population is d
✦ LIBER ✦
Orbital resonances in the inner neptunian system: I. The 2:1 Proteus–Larissa mean-motion resonance
✍ Scribed by Ke Zhang; Douglas P. Hamilton
- Book ID
- 108138728
- Publisher
- Elsevier Science
- Year
- 2007
- Tongue
- English
- Weight
- 976 KB
- Volume
- 188
- Category
- Article
- ISSN
- 0019-1035
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