Thrust Faulting on Venus: Tectonic Modeling of the Vedma Dorsa Ridge Belt
Abstract
Quantitative modeling of thrust faulting in the Vedma Dorsa ridge belt requires fault displacements of 1-2 km, a faulted layer thickness of 10-20 km, and a fault dip of 25-30 degrees.
- Publication:
-
17th Meeting of the Venus Exploration Group (VEXAG)
- Pub Date:
- November 2019
- Bibcode:
- 2019LPICo2193.8021M