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RESOLVING THE PERICENTER
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DOI：10.1088/0004-6256/150/4/127.png)
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Abstract
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The Wisdom-Holman mapping method and its variations have become a mainstay of research in solar system dynamics. But the method is not without its limitations. Rauch & Holman noted that at large eccentricities sufficiently small steps must be taken to resolve the pericenter. In this paper, I explore in more detail what it means to resolve the pericenter.
Keywords:
celestial mechanics
methods: numerical
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ASTRONOMICAL JOURNAL
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ASTRONOMICAL JOURNALIF5.1
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