MSc. Thesis Overview

 

My current research involves investigating the interaction between magmatic intrusions (dikes or sills) and subsurface ice on Mars.  Mars is the only planet other than Earth known to have had a long-term dynamic hydrological cycle, and there is abundant geologic evidence that the Martian surface has been substantially modified by the action of liquid water and ice.  However, present-day temperatures and atmospheric conditions on Mars do not allow for the occurrence of liquid water on the surface.  The interaction between volcanism and ice is a unique process on Earth that results in the formation of distinct volcanic edifices.  Likewise, research shows that there is an important spatial and temporal relationship between volcanism and ice on Mars.  Since ground ice is the largest, most plausible, prospective reservoir for H₂O on Mars, it is the most likely candidate for interaction with volcanism.