Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
10705564 | Planetary and Space Science | 2005 | 12 Pages |
Abstract
Lastly, by analyzing orbital properties of classical TNOs (42AU99.63% confidence level. Furthermore, more massive classical bodies are anomalously present at a<43.5AU, a result statistically significant and apparently not caused by observational biases. This feature would provide a new constraint for transneptunian belt formation models.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Patryk Sofia Lykawka, Tadashi Mukai,