We follow the evolution of distributions of real and fictitious asteroids, initially placed in the vicinity of the 12:7 mean motion resonance with Jupiter. Our results show that, besides the well-known example of 522-Helga, other stable chaotic asteroids could, in principle, exist in this region of
β¦ LIBER β¦
Chaos in the 3 : 1 mean-motion resonance revisited
β Scribed by F. Varadi; W.M. Kaula
- Book ID
- 108366059
- Publisher
- Elsevier Science
- Year
- 1999
- Tongue
- English
- Weight
- 411 KB
- Volume
- 47
- Category
- Article
- ISSN
- 0032-0633
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We have shown, in previous publications, that stable chaos is associated with medium/high-order mean motion resonances with Jupiter, for which there exist no resonant periodic orbits in the framework of the elliptic restricted three-body problem. This topological "defect" results in the absence of t