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Icarus
Volumn 190, Issue 1, 2007, Pages 280-282
The Mars 1:2 resonant population
Author keywords

Asteroids; Celestial mechanics; dynamics; Mars; orbital; Resonances
Indexed keywords

EID: 34547757051     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/j.icarus.2007.05.012     Document Type: Article
Times cited : (11)
References (11)
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  • 5
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    • The high-eccentricity librations of the Hildas
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  • 6
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    • Atlas of the mean motion resonances in the Solar System
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  • 8
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    • Numerous weak resonances drive asteroids toward terrestrial planets orbits
    • Morbidelli A., and Nesvorný D. Numerous weak resonances drive asteroids toward terrestrial planets orbits. Icarus 139 (1999) 295-308
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    • Three-body mean motion resonances and the chaotic structure of the asteroid belt
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    • Nesvorný, D.1    Morbidelli, A.2
  • 10
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    • Regular and chaotic dynamics in the mean-motion resonances: Implications for the structure and evolution of the asteroid belt
    • Bottke W.F., Paolicchi P., Binzel R.P., and Cellino A. (Eds), Univ. of Arizona Press, Tucson
    • Nesvorný D., Ferraz-Mello S., Holman M., and Morbidelli A. Regular and chaotic dynamics in the mean-motion resonances: Implications for the structure and evolution of the asteroid belt. In: Bottke W.F., Paolicchi P., Binzel R.P., and Cellino A. (Eds). Asteroids III (2002), Univ. of Arizona Press, Tucson 379-394
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    • Rubincam, D.P.1

* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.