While much has been written on the ramifications of Newton's dynamics, until now the details of Newton's solution were available only to the physics expert. The Key to Newton's Dynamics clearly explains the surprisingly simple analytical structure that underlies the determination of the force necessary to maintain ideal planetary motion. J. Bruce Brackenridge sets the problem in historical and conceptual perspective, showing the physicist's debt to the works of both Descartes and Galileo. He tracks Newton's work on the Kepler problem from its early stages at Cambridge before 1669, through the revival of his interest ten years later, to its fruition in the first three sections of the first edition of the Principia.
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J. Bruce Brackenridge is Alice G. Chapman Professor of Physics at Lawrence University.
"The Key to Newton's Dynamics is lucid, important, and fills a large gap in the existing literature. Brackenridge is undoubtedly that gifted, patient teacher that one expects from a quality liberal arts college."--Alan E. Shapiro, University of Minnesota
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Zustand: Very Good. This text explains the surprisingly simple analytical structure that underlies the determination of the force necessary to maintain ideal planetary motion. It sets the problem in historical and conceptual perspective, showing Newton's debt to the works of Descartes and Galileo. Num Pages: 330 pages, 5 b&w photographs, 113 figures. BIC Classification: PDX; PHD. Category: (P) Professional & Vocational. Dimension: 227 x 156 x 20. Weight in Grams: 514. Good clean copy with minor shelfwear, remains very good. 1996. paperback. . . . . Artikel-Nr. KTS0036651
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Taschenbuch. Zustand: Neu. Neuware - While much has been written on the ramifications of Newton's dynamics, until now the details of Newton's solution were available only to the physics expert. 'The Key to Newton's Dynamics' clearly explains the surprisingly simple analytical structure that underlies the determination of the force necessary to maintain ideal planetary motion. J. Bruce Brackenridge sets the problem in historical and conceptual perspective, showing the physicist's debt to the works of both Descartes and Galileo. He tracks Newton's work on the Kepler problem from its early stages at Cambridge before 1669, through the revival of his interest ten years later, to its fruition in the first three sections of the first edition of the 'Principia.'. Artikel-Nr. 9780520202177
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