Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
10701437 | Icarus | 2012 | 16 Pages |
Abstract
⺠We numerically simulate fold formation on Europa. ⺠Nominally, fold formation requires larger strains than previously assumed. ⺠Low strain rates and small ice grain sizes enhance fold growth. ⺠Strain can be taken up via thickening of the lithosphere without fold formation. ⺠Uniform thickening offers a partial solution to Europa's apparent strain imbalance.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Michael T. Bland, William B. McKinnon,