In this work we use a mechanical dislocation program to analyze the fault geometries and depths associated with a group of prominent lobate scarps in Mercury. We obtain depths of faulting of 30-40 km. This range overlaps with those previously obtained for Discovery Rupes and for two unnamed lobate scarps
Lobate scarps are tectonic structures considered as the topographic expression of thrust faults. For...
Objective of this thesis is the mapping and structural analysis of the H2 quadrangle, “Victoria”, an...
The volcanic plains that fill the Caloris basin, the largest recognized impact basin on Mercury, are...
Utilizing Mariner 10 images of Mercury, we derived a digital elevation model to examine the topograp...
Insight into the mechanical and thermal structure of Mercury's early lithosphere has been obtained f...
[1] Insight into the mechanical and thermal structure of Mercury’s early lithosphere has been obtain...
Lobate scarps are landforms on Mercury that appear to have formed by thrust faulting and are thought...
Lobate scarps, landforms interpreted as the surface manifestation of thrust faults, are widely distr...
Thanks to its location at low latitude and close to the terminator in the outbound view of Mercury o...
The surface of Mercury shows abundant compressive tectonic landforms, including lobate scarps, wrink...
The global tectonics of Mercury is dominated by contractional features mainly represented by lobate ...
The tectonic evolution of Mercury is dominated at a global scale by contractional features such as l...
Basin-edge lobate scarps are a sub-type of tectonic shortening structure on the surface of Mercury t...
Lobate scarps, thought to be the surface expression of large thrust faults, are the most spectacular...
<p>Mercury's tectonic history has been dominated by global contraction as the planet cools and...
Lobate scarps are tectonic structures considered as the topographic expression of thrust faults. For...
Objective of this thesis is the mapping and structural analysis of the H2 quadrangle, “Victoria”, an...
The volcanic plains that fill the Caloris basin, the largest recognized impact basin on Mercury, are...
Utilizing Mariner 10 images of Mercury, we derived a digital elevation model to examine the topograp...
Insight into the mechanical and thermal structure of Mercury's early lithosphere has been obtained f...
[1] Insight into the mechanical and thermal structure of Mercury’s early lithosphere has been obtain...
Lobate scarps are landforms on Mercury that appear to have formed by thrust faulting and are thought...
Lobate scarps, landforms interpreted as the surface manifestation of thrust faults, are widely distr...
Thanks to its location at low latitude and close to the terminator in the outbound view of Mercury o...
The surface of Mercury shows abundant compressive tectonic landforms, including lobate scarps, wrink...
The global tectonics of Mercury is dominated by contractional features mainly represented by lobate ...
The tectonic evolution of Mercury is dominated at a global scale by contractional features such as l...
Basin-edge lobate scarps are a sub-type of tectonic shortening structure on the surface of Mercury t...
Lobate scarps, thought to be the surface expression of large thrust faults, are the most spectacular...
<p>Mercury's tectonic history has been dominated by global contraction as the planet cools and...
Lobate scarps are tectonic structures considered as the topographic expression of thrust faults. For...
Objective of this thesis is the mapping and structural analysis of the H2 quadrangle, “Victoria”, an...
The volcanic plains that fill the Caloris basin, the largest recognized impact basin on Mercury, are...