Are two of the Neptune Trojans dynamically unstable?
Paper
Paper/Presentation Title | Are two of the Neptune Trojans dynamically unstable? |
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Presentation Type | Paper |
Authors | Horner, Jonathan (Author) and Lykawka, Patryk Sofia (Author) |
Editors | Short, Wayne and Cairns, Iver |
Journal or Proceedings Title | Proceedings of the 11th Australian Space Science Conference (ASSC 2011) |
Number of Pages | 12 |
Year | 2012 |
Place of Publication | Canberra, Australia |
ISBN | 9780977574056 |
Web Address (URL) of Paper | http://www.nssa.com.au/11assc/downloads/11ASSC-Proceedings-web.pdf |
Conference/Event | 11th Australian Space Science Conference (ASSC 2011) |
Event Details | 11th Australian Space Science Conference (ASSC 2011) Parent Australian Space Science Conference (ASSC) Delivery In person Event Date 26 to end of 29 Sep 2011 Event Location Canberra, Australia Sydney, Australia |
Abstract | The Neptune Trojans are the most recently discovered population of small bodies in the Solar System. To date, only eight have been discovered, though it is thought likely that the total population at least rivals that of the asteroid belt. Their origin is still the subject of |
Keywords | Neptune Trojans, solar system formation, solar system evolution, centaurs, comets, dynamical methods |
ANZSRC Field of Research 2020 | 510109. Stellar astronomy and planetary systems |
Public Notes | Copyright © 2012 National Space Society of Australia Ltd. No evidence of copyright restrictions preventing deposit of Accepted version. |
Byline Affiliations | University of New South Wales |
Kindai University, Japan | |
Institution of Origin | University of Southern Queensland |
https://research.usq.edu.au/item/q453x/are-two-of-the-neptune-trojans-dynamically-unstable
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