Thanks to its location at low latitude and close to the terminator in the outbound view of Mercury obtained during MESSENGER\u2019s first fly-by, the Beagle Rupes lobate scarp on Mercury has been particularly clearly imaged. This enables us to interpret it as a component of a linked fault system, consisting of a frontal scarp terminated by transpressive lateral ramps. The terrain bounded by these surface manifestations of faulting is the hanging-wall block of a thrust sheet and must be underlain by a basal decollement (a detachment horizon) constituting the fault zone at depth. The decollement must extend a minimum of 150 km eastwards from the frontal scarp, and at least 400 km if displacement is transferred to features interpreted as out-o...
[1] Insight into the mechanical and thermal structure of Mercury’s early lithosphere has been obtain...
A vast majority of tectonic landforms on Mercury have been formed by compression; extensional landfo...
Volcanic and tectonic implications of the surface morphology of Mercury are discussed. Mercurian sca...
Thanks to its location at low latitude and close to the terminator in the outbound view of Mercury o...
Utilizing Mariner 10 images of Mercury, we derived a digital elevation model to examine the topograp...
Lobate scarps are landforms on Mercury that appear to have formed by thrust faulting and are thought...
Areas of crustal convergence and shortening on Earth, Mars and Venus are often characterized by stru...
At a global scale, Mercury is dominated by contractional features manifested as lobate scarps, wrink...
The Rembrandt basin is crosscut by the largest fault scarp on Mercury, Enterprise Rupes, and a secon...
International audienceBasin-edge lobate scarps are a sub-type of tectonic shortening structure on th...
Lobate scarps on Mercury are generally accepted as being surface expressions of thrust faulting. Thi...
Lobate scarps, thought to be the surface expression of large thrust faults, are the most spectacular...
Lobate scarps on Mercury are generally accepted to be surface expressions of thrust faulting. This i...
[1] Lobate scarps on Mercury are the surface expression of thrust faults and are generally thought t...
In this work we use a mechanical dislocation program to analyze the fault geometries and depths asso...
[1] Insight into the mechanical and thermal structure of Mercury’s early lithosphere has been obtain...
A vast majority of tectonic landforms on Mercury have been formed by compression; extensional landfo...
Volcanic and tectonic implications of the surface morphology of Mercury are discussed. Mercurian sca...
Thanks to its location at low latitude and close to the terminator in the outbound view of Mercury o...
Utilizing Mariner 10 images of Mercury, we derived a digital elevation model to examine the topograp...
Lobate scarps are landforms on Mercury that appear to have formed by thrust faulting and are thought...
Areas of crustal convergence and shortening on Earth, Mars and Venus are often characterized by stru...
At a global scale, Mercury is dominated by contractional features manifested as lobate scarps, wrink...
The Rembrandt basin is crosscut by the largest fault scarp on Mercury, Enterprise Rupes, and a secon...
International audienceBasin-edge lobate scarps are a sub-type of tectonic shortening structure on th...
Lobate scarps on Mercury are generally accepted as being surface expressions of thrust faulting. Thi...
Lobate scarps, thought to be the surface expression of large thrust faults, are the most spectacular...
Lobate scarps on Mercury are generally accepted to be surface expressions of thrust faulting. This i...
[1] Lobate scarps on Mercury are the surface expression of thrust faults and are generally thought t...
In this work we use a mechanical dislocation program to analyze the fault geometries and depths asso...
[1] Insight into the mechanical and thermal structure of Mercury’s early lithosphere has been obtain...
A vast majority of tectonic landforms on Mercury have been formed by compression; extensional landfo...
Volcanic and tectonic implications of the surface morphology of Mercury are discussed. Mercurian sca...