| dc.contributor.author | Wisdom, Jack | |
| dc.date.accessioned | 2016-01-05T00:42:50Z | |
| dc.date.available | 2016-01-05T00:42:50Z | |
| dc.date.issued | 2015-09 | |
| dc.date.submitted | 2015-06 | |
| dc.identifier.issn | 1538-3881 | |
| dc.identifier.issn | 0004-6256 | |
| dc.identifier.uri | http://hdl.handle.net/1721.1/100693 | |
| dc.description.abstract | 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. | en_US |
| dc.language.iso | en_US | |
| dc.publisher | IOP Publishing | en_US |
| dc.relation.isversionof | http://dx.doi.org/10.1088/0004-6256/150/4/127 | en_US |
| dc.rights | Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. | en_US |
| dc.source | IOP Publishing | en_US |
| dc.title | RESOLVING THE PERICENTER | en_US |
| dc.type | Article | en_US |
| dc.identifier.citation | Wisdom, Jack. “RESOLVING THE PERICENTER.” The Astronomical Journal 150, no. 4 (September 29, 2015): 127. © 2015 The American Astronomical Society | en_US |
| dc.contributor.department | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences | en_US |
| dc.contributor.mitauthor | Wisdom, Jack | en_US |
| dc.relation.journal | The Astronomical Journal | en_US |
| dc.eprint.version | Final published version | en_US |
| dc.type.uri | http://purl.org/eprint/type/JournalArticle | en_US |
| eprint.status | http://purl.org/eprint/status/PeerReviewed | en_US |
| dspace.orderedauthors | Wisdom, Jack | en_US |
| dc.identifier.orcid | https://orcid.org/0000-0002-6142-0653 | |
| mit.license | PUBLISHER_POLICY | en_US |
