| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10701563 | Icarus | 2012 | 10 Pages |
Abstract
⺠We model Mars 40Ar atmosphere, mantle and crust. ⺠Present atmosphere content cannot be reproduced with Mars' formation model. ⺠This suggests a significant crust past erosion.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
F. Leblanc, E. Chassefière, C. Gillmann, D. Breuer,