| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8144209 | Planetary and Space Science | 2012 | 6 Pages |
Abstract
ⶠWe model the topography of a group of lobate scarps in Mercury. ⶠDepths of faulting obtained through our models are between 30 and 39 km. ⶠSurface heat flows calculated from these depths of faulting are of 19-39 mW mâ2. ⶠOur results are consistent with predictions of thermal history models in Mercury.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Isabel Egea-González, Javier Ruiz, Carlos Fernández, Jean-Pierre Williams, Álvaro Márquez, Luisa M. Lara,