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Titlebook: Dynamics of Comets and Asteroids and Their Role in Earth History; Proceedings of a Wor Shin Yabushita,Jacques Henrard Conference proceeding

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Guangwei Miao,Shuaiqi Wang,Chengyou Cui< 2 AU) where the NEA orbits evolve. Our numerical integrations (over a time span of a few Myr) have shown that: (i) the linear secular resonances with both the inner and the outer planets may play an important role in the dynamical evolution of NEAs; (ii) the apsidal secular resonance with Mars cou
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Guangwei Miao,Shuaiqi Wang,Chengyou Cuie meteoroids in orbit close to the ecliptic. Since 1975 we have also been aware of an apparently massive meteoroidal swarm in probable 7:2 mean motion resonance with Jupiter, seemingly at the heart of the Taurid Complex and connecting therefore with the near-ecliptic system through the so-called Što
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Yinan Fu,Xiaolong Zheng,Peilun Du,Liang Liue Hecuba gap) is investigated. We confirm the proposition made by Ferraz-Mello and collaborators that the great inequality generates secondary resonances which are likely to produce the slow diffusion observed in numerical investigations. We identify, in the restricted three body problem, the freque
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Yinan Fu,Xiaolong Zheng,Peilun Du,Liang Liu 400 asteroids using the Fast Lyapunov Indicator, a method of analysis closely related to the computation of the Lyapunov Characteristic Exponents, but cheaper in computational time. For both regular and chaotic orbits we try to associate the motion to the underlying resonances network. For it we co
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Feng Li,Liang Chen,Yaling Wang,Xiarao Wangencounters with meteor streams. We have made a systematic search of encounter chances (encounter duration and velocity) with the major meteor showers taken from the Kronk’s catalog (1988) for some mission target asteroids and Mars. It is argued that dust clouds much enhanced by stream impacts are on
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Feng Li,Liang Chen,Yaling Wang,Xiarao Wangsions to nuclear wars, and collision with minor bodies (comets and asteroids). Of these three factors, the collision with minor body is the most serious for continuation of civilization of mankind, because, the civilization will be collapsed completely by the collision with a some size minor body.
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Yinan Fu,Xiaolong Zheng,Peilun Du,Liang LiuThe lack of asteroids in the 2/1-resonance is explained by the global stochasticity of the solutions in the Sun-Jupiter-Saturn-asteroid model. The explanation is based on data obtained with Laskar’s frequency map analysis and on simulations showing the decisive influence of Jupiter’s orbit perturbations related to the “Great Inequality”.
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On the Lack of Asteroids in the Hecuba Gap,The lack of asteroids in the 2/1-resonance is explained by the global stochasticity of the solutions in the Sun-Jupiter-Saturn-asteroid model. The explanation is based on data obtained with Laskar’s frequency map analysis and on simulations showing the decisive influence of Jupiter’s orbit perturbations related to the “Great Inequality”.
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