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Solar System Dynamics

Murray, Carl D., Dermott, Stanley F.·2000·Cambridge University Press eBooks

Abstract

The Solar System is a complex and fascinating dynamical system. This is the first textbook to describe comprehensively the dynamical features of the Solar System and to provide students with all the mathematical tools and physical models they need to understand how it works. It is a benchmark publication in the field of planetary dynamics and destined to become a classic. Clearly written and well illustrated, Solar System Dynamics shows how a basic knowledge of the two- and three-body problems and perturbation theory can be combined to understand features as diverse as the tidal heating of Jupiter's moon Io, the origin of the Kirkwood gaps in the asteroid belt, and the radial structure of Saturn's rings. Problems at the end of each chapter and a free Internet Mathematica® software package are provided. Solar System Dynamics provides an authoritative textbook for courses on planetary dynamics and celestial mechanics. It also equips students with the mathematical tools to tackle broader courses on dynamics, dynamical systems, applications of chaos theory and non-linear dynamics.

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Metadata

Authors
Murray, C. D., & Dermott, S. F.
Venue
Cambridge University Press eBooks
Published
2000-02-13
OpenAlex
W1634825185
Cited by
2,856
References
0
FWCI
36.31
Type
book
Language
en
Open access
closed

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CoChat. (2026). Citation check: Solar System Dynamics. https://app.cochat.ai/papers/10.1017/cbo9781139174817
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Murray, C. D., & Dermott, S. F. (2000). Solar System Dynamics. Cambridge University Press eBooks. https://doi.org/10.1017/cbo9781139174817

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.