Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
10701676 | Icarus | 2012 | 10 Pages |
Abstract
⺠We model the long-term dynamical evolution of the Haumea collisional family. ⺠25-45% of family members will be lost over 3.5 Gyr of orbital evolution. ⺠We apply these loss rates to proposed family formation models. ⺠We compare our dynamically evolved families to current observations.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Kathryn Volk, Renu Malhotra,