| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10705528 | Planetary and Space Science | 2005 | 13 Pages |
Abstract
In the transneptunian classical region (42AU10°. Taking into account those particles still locked in the resonance at the end of the simulations, we determined a retainability of 12-15% for real 7:4 resonant transneptunian objects (TNOs). Lastly, our results demonstrate that classical TNOs associated with the 7:4 mean motion resonance have been evolving continuously until present with non-negligible mixing of populations.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Patryk Sofia Lykawka, Tadashi Mukai,