Investigating Late Amazonian Volcanotectonic Activity on Olympus Mons, Mars Using Flank Vents and Arcuate Graben

Olympus Mons is the largest volcano on Mars. Previous studies have focused on large scale features on Olympus Mons, such as the basal escarpment, summit caldera complex and aureole deposits. My objective was to identify and characterize previously unrecognized and unmapped small scale features to understand the volcanotectonic evolution of this enormous volcano.