CORDIS Project
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This project investigates geological activity on Mars by analyzing the changes in large gullies to determine if they are caused by liquid water or dry frost. It combines remote sensing with fieldwork to understand Martian habitability and inform future missions.
This study will identify and analyse ongoing geological activity across the whole of Mars in the form of the changing morphology of kilometre-scale “classical gullies” (Fig. 1).
From this, we aim to determine whether these changes are caused by the action of liquid water, or dry frost (water or carbon dioxide).
Such a study addresses key questions of ongoing martian habitability, planetary protection (i.e. limiting access for future missions to possible ‘wet’ environments) and current climate. J…
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