RESOLVING THE PERICENTER
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 exp...
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| フォーマット: | 論文 |
| 言語: | en_US |
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IOP Publishing
2016
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| オンライン･アクセス: | http://hdl.handle.net/1721.1/100693 https://orcid.org/0000-0002-6142-0653 |