Titlebook: Applications of Modern Dynamics to Celestial Mechanics and Astrodynamics; Proceedings of the N Victor Szebehely (L.B. Meaders Professor of

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書目名稱Applications of Modern Dynamics to Celestial Mechanics and Astrodynamics影響因子(影響力)




書目名稱Applications of Modern Dynamics to Celestial Mechanics and Astrodynamics影響因子(影響力)學科排名




書目名稱Applications of Modern Dynamics to Celestial Mechanics and Astrodynamics網絡公開度




書目名稱Applications of Modern Dynamics to Celestial Mechanics and Astrodynamics網絡公開度學科排名




書目名稱Applications of Modern Dynamics to Celestial Mechanics and Astrodynamics被引頻次




書目名稱Applications of Modern Dynamics to Celestial Mechanics and Astrodynamics被引頻次學科排名




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書目名稱Applications of Modern Dynamics to Celestial Mechanics and Astrodynamics年度引用學科排名




書目名稱Applications of Modern Dynamics to Celestial Mechanics and Astrodynamics讀者反饋




書目名稱Applications of Modern Dynamics to Celestial Mechanics and Astrodynamics讀者反饋學科排名

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A Qualitative Study of Stabilizing and Destabilizing Factors in Planetary and Asteroidal Orbitswith a comet, on the generation of instability may be important for the resonances 1/3, 3/5,…. On the other hand, particular Hamiltonian perturbations exist which stabilize an unstable resonant system.

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Perturbations in Stellar Pathsh whom I never entered into scientific discussion, but whom I joined in a chambermusic evening in Swarthmore, Pennsylvania, on June 5, 1938. There we were: Arnold Dresden, piano; Einstein, violin; my brother Jaap, violoncello; and myself, viola (see my articles in the . (1979), 300, 273; and in . (1

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Some Aspects of Motion in the General Planar Problem of Three Bodies; in Particular in the Vicinity f motion in the vicinity of periodic solutions associated with a small-integer commensurability, extending to the general problem the approach used earlier in the restricted problem of three bodies in the plane (Message, 1966, where is given references to earlier investigations of the restricted cas

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Regularization of the Singularities of the N-Body Problem(implying infinitesimal masses)..For rectilinear motions the binary collisions are not Easton-regularizable (because all neighboring motions have such a collision) but they are Siegel-regularizable and thus the problem can be handled with the usual picture of rectilinear motions and their invariable

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1389-2185 tly the dynamical behavior of artificial satellites and space probes. The underlying mathematical and dynamical principles are, of course, the same for Celestia978-94-009-7795-2978-94-009-7793-8Series ISSN 1389-2185

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Applications of Modern Dynamics to Celestial Mechanics and AstrodynamicsProceedings of the N

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Cytokines and Endocrine Functionh whom I never entered into scientific discussion, but whom I joined in a chambermusic evening in Swarthmore, Pennsylvania, on June 5, 1938. There we were: Arnold Dresden, piano; Einstein, violin; my brother Jaap, violoncello; and myself, viola (see my articles in the . (1979), 300, 273; and in . (1