Abstract
dc:description.abstractTo find Planet Nine, we use N-body simulations to find the true anomaly of Planet Nine that would render distant KBOs the most stable. We obtain an interval of 162-198°matching the intervals given by Medvedev & Vavilov (2016) of 176-184° and Brown & Batygin (2016) of 180°. According to our results, Planet Nine should reside in the constellation Lepus.
Degree
thesis:*- Department dc:contributor.department
- Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences.
- Grantor dc:publisher
- Massachusetts Institute of Technology
- Year dc:date.issued
- 2017
Author and committee
dc:creator, dc:contributor.*- Author dc:creator
-
- Downey, Brynna G
- Advisor dc:contributor.advisor
-
- Jack Wisdom.
Subjects
dc:subject × 1Rights
dc:rights- Statement dc:rights
-
- MIT theses are protected by copyright. They may be viewed, downloaded, or printed from this source but further reproduction or distribution in any format is prohibited without written permission.
- Licence dc:rights.uri
- Language dc:language.iso
- eng
Identifiers
dc:identifier.*- Handle dc:identifier.uri
- http://hdl.handle.net/1721.1/114095
- OAI identifier oai:identifier
- oai:dspace.mit.edu:1721.1/114095