In this thesis, I investigated curvilinear features on the surface of Mercury and the impact of illumination bias upon observations of those features. I also demonstrated their utility with regard to photostratigraphy and suggest areas where BepiColombo will provide beneficial additional data. Basin-edge scarps occur within volcanically-filled impact basins in all areas of the surface of Mercury. Many large impact basins are filled with Smooth Plains (volcanic) units. I hypothesise that fault nucleation occurs on the mechanically weak interface between the base of the volcanic fill units and the original floor of the impact basin. Using crater size-frequency distribution analysis I have established that resolvable deformation of basin-ed...
[Introduction] Studies using MESSENGER data suggest that Mercury’s crust is predominantly a product ...
The 715-km-diameter Rembrandt basin is the largest well-preserved impact feature of the southern hem...
The surface of Mercury shows abundant compressive tectonic landforms, including lobate scarps, wrink...
This thesis addresses the regional geology of the planet Mercury as seen by the MErcury Surface, Spa...
Basin-edge lobate scarps are a sub-type of tectonic shortening structure on the surface of Mercury t...
Most of Mercury's surface is volcanic. Plains were emplaced effusively. Explosive volcanism puncture...
Volcanic and tectonic implications of the surface morphology of Mercury are addressed in two separat...
MESSENGER heralded a new era in our geological understanding of Mercury as a dynamic planet. Geologi...
The Caloris basin (1550 km diameter) is the largest, well-preserved impact feature on Mercury. Its i...
The volcanic plains that fill the Caloris basin, the largest recognized impact basin on Mercury, are...
The formation of large impact basins (diameter D greater than or equal to 300 km) was an important p...
The Caloris basin on Mercury is floored by light-toned plains and surrounded by an annulus of dark-t...
Quadrangle geological maps from Mariner 10 data cover 45% of the surface of Mercury at 1:5M scale. O...
Mercury's geological history has been dominated by global contraction caused by secular cooling of t...
I present the results from the first geological map of the Derain (H-10) quadrangle of Mercury and i...
[Introduction] Studies using MESSENGER data suggest that Mercury’s crust is predominantly a product ...
The 715-km-diameter Rembrandt basin is the largest well-preserved impact feature of the southern hem...
The surface of Mercury shows abundant compressive tectonic landforms, including lobate scarps, wrink...
This thesis addresses the regional geology of the planet Mercury as seen by the MErcury Surface, Spa...
Basin-edge lobate scarps are a sub-type of tectonic shortening structure on the surface of Mercury t...
Most of Mercury's surface is volcanic. Plains were emplaced effusively. Explosive volcanism puncture...
Volcanic and tectonic implications of the surface morphology of Mercury are addressed in two separat...
MESSENGER heralded a new era in our geological understanding of Mercury as a dynamic planet. Geologi...
The Caloris basin (1550 km diameter) is the largest, well-preserved impact feature on Mercury. Its i...
The volcanic plains that fill the Caloris basin, the largest recognized impact basin on Mercury, are...
The formation of large impact basins (diameter D greater than or equal to 300 km) was an important p...
The Caloris basin on Mercury is floored by light-toned plains and surrounded by an annulus of dark-t...
Quadrangle geological maps from Mariner 10 data cover 45% of the surface of Mercury at 1:5M scale. O...
Mercury's geological history has been dominated by global contraction caused by secular cooling of t...
I present the results from the first geological map of the Derain (H-10) quadrangle of Mercury and i...
[Introduction] Studies using MESSENGER data suggest that Mercury’s crust is predominantly a product ...
The 715-km-diameter Rembrandt basin is the largest well-preserved impact feature of the southern hem...
The surface of Mercury shows abundant compressive tectonic landforms, including lobate scarps, wrink...