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Titlebook: Dynamics of Planets and Satellites and Theories of Their Motion; Proceedings of the 4 Victor Szebehely Conference proceedings 1978 D. Reide

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书目名称Dynamics of Planets and Satellites and Theories of Their Motion
副标题Proceedings of the 4
编辑Victor Szebehely
视频videohttp://file.papertrans.cn/285/284152/284152.mp4
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Dynamics of Planets and Satellites and Theories of Their Motion; Proceedings of the 4 Victor Szebehely Conference proceedings 1978 D. Reide
描述P. J. MESSAGE University of Liverpool The papers which comprise this volume were presented at Colloquium No. 41 of the International Astronimical Union, which was held in Cambridge, England, from the 17th to the 19th of August, 1976, and had as its subject ‘Dynamics of Planets and Satellites and Theories of their Motion‘. The Colloquium was held just prior to the XVIth General Assembly of the Union (which was held from 24th August to 2nd September, in Grenoble, France) to provide an opportunity for the presentation of research papers on a number of active and lively branches of Celestial Mechanics to a gathering of experts in the field, and for the stimulus of discussion of research problems of interest to participants. A number of papers testify to the progress being made in General Planetary Theory, the theories of motion of the minor planets, the Moon, and the satellites of Jupiter and Saturn, and to significant advances in both the general and restricted gravitational problems of three bodies. The Organizing Committee of the Colloquium was comprised of J. Chapront, R. L. Duncombe, J. Hadjidemetriou, Y. Kozai, B. Morando, J. Schubart, V. Szebehely, and P. J. Message (Chairman).
出版日期Conference proceedings 1978
关键词Anomalie; Libration; Rigid body; Variation; artificial satellite; asteroid; dynamics; earth; gravitation; gra
版次1
doihttps://doi.org/10.1007/978-94-009-9809-4
isbn_softcover978-94-009-9811-7
isbn_ebook978-94-009-9809-4Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1978
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Construction of Planetary Theory by Iterative Proceduree simplicity the case of two mutually disturbing planets is considered. In the original version of the method the perturbations of rectangular planetary coordinates are presented by means of the formal integrals . where index i corresponds to the number of the planet; δX. are perbations of X. coordi
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Qualitative Dynamics of the Sun-Jupiter-Saturn Systemth the models of the restricted and general problems of three bodies are compared with numerical integration. The system is found to be stable in the sense that Saturn will neither interrupt the (perturbed) binary orbit of Jupiter around the Sun, nor will it escape from the system. It is shown that
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A New Approach for the Contruction of Long-Periodic Perturbationse all different influences, e.g. near resonances and is combined with the very precise method of the numerical integration. The truncation to low orders can be avoided which is made by analytical methods in using developments with respect to the small parameters inclinations and eccentricities. For
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Discussion sur les Resultats de Theories Planetaierst nous parlerons ici ne sont que des résultats provisoires. Nous développerons quelques aspects des difficultés que nous avons rencontrées et les conséquences de ces difficultés sur 1’orientation des méthodes utilisées pour résoudre les problèmes suivant qu’il s’agit des planètes intérieures ou des
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Relation of a Contracting Earth to the Apparent Accelerations of the Sun and Moonthe Sun and Moon since it was first developed by Jeffreys in 1920. Allowance for a changing moment of inertia of the Earth enables the discrepancy to be completely removed if a decrease is occurring at a rate of just about the amount already required by the phase-change theory of the nature of the t
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