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    The Perihelion of Mercury

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    File(s)
    TR161.pdf (2.183Mb)
    Date
    1972
    Author
    Moore, Ramon E.
    Greenspan, Donald
    Publisher
    University of Wisconsin-Madison Department of Computer Sciences
    Metadata
    Show full item record
    Abstract
    Local finite Taylor series expansion is shown to be an efficient numerical method for the study of the n-body problem. Application is made to the accurate determination of the motion of the perihelion of Mercury according to Newtonian celestial mechanics.
    Permanent Link
    http://digital.library.wisc.edu/1793/57768
    Type
    Technical Report
    Citation
    TR161
    Part of
    • CS Technical Reports

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