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Symplectic maps for the n-body problem

Wisdom, Jack, Holman, Matthew·1991·The Astronomical Journal

Abstract

The present study generalizes the mapping method of Wisdom (1982) to encompass all gravitational n-body problems with a dominant central mass. The rationale for the generalized mapping method is discussed as well as details for the mapping for the n-body problem. Some refinements of the method are considered, and the relationship of the mapping method to other symplectic integration methods is shown. The method is used to compute the evolution of the outer planets for a billion years. The resulting evolution is compared to the 845 million year evolution of the outer planets performed on the Digital Orerry using standard numerical integration techniques. This calculation provides independent numerical confirmation of the result of Sussman and Wisdom (1988) that the motion of the planet Pluto is chaotic.

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Metadata

Authors
Wisdom, J., & Holman, M.
Venue
The Astronomical Journal
Published
1991-10
Volume
102
Pages
1528
ISSN
0004-6256 (ISSN-L)
OpenAlex
W1976860825
Cited by
1,196
References
0
FWCI
11.49
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Symplectic maps for the n-body problem. https://app.cochat.ai/papers/10.1086/115978
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Wisdom, J., & Holman, M. (1991). Symplectic maps for the n-body problem. The Astronomical Journal. https://doi.org/10.1086/115978

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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.