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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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書(shū)目名稱Dynamics of Comets and Asteroids and Their Role in Earth History
副標(biāo)題Proceedings of a Wor
編輯Shin Yabushita,Jacques Henrard
視頻videohttp://file.papertrans.cn/285/284036/284036.mp4
圖書(shū)封面Titlebook: Dynamics of Comets and Asteroids and Their Role in Earth History; Proceedings of a Wor Shin Yabushita,Jacques Henrard Conference proceeding
描述The last decade of this century has seen a renewed interest in the dynamics and physics of the small bodies of the Solar System, Asteroids, Comets and Meteors. New observational evidences such as the discovery of the Edgeworth-Kuiper belt, refined numerical tools such as the symplectic integrators, analytical tools such as semi-numerical perturbation algorithms and in general a better understanding of the dynamics of Hamiltonian systems, all these factors have converged to make possible and worthwhile the study, over very long time spans, of these "minor" objects. Also the public, the media and even some political assell}blies have become aware that these "minor" objects of our planetary environnement could become deadly weapons. Apparently they did have a role in Earth history and a role more ominous than "predicting" defeat (or victory, why not?) to batches of credulous rulers. Remembering what may have happened to the dinosaurs but keeping all the discretion necessary to avoid creating irrational scares, it may not be unwise or irrelevant to improve our knowledge of the physics and dynamics of these objects and to study in particular their interactions with our planet.
出版日期Conference proceedings 1998
關(guān)鍵詞Cloud; Orbit; Planet; Solar System; Tide; celestial bodies; solar; hydrogeology
版次1
doihttps://doi.org/10.1007/978-94-017-1321-4
isbn_softcover978-90-481-5081-6
isbn_ebook978-94-017-1321-4
copyrightSpringer Science+Business Media Dordrecht 1998
The information of publication is updating

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Feng Li,Liang Chen,Yaling Wang,Xiarao Wangly the .m-sized component, and thus they should be looked for at the encounter times from the spacecraft for the forward scattered lights, namely at large solar phase angles. We also compare statistically encounter conditions between all the showers given in Kronk and possible unknown streams that are likely to be of periodic-comet origin.
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