Introduction: Today, liquid water is generally unstable on the surface of Mars. However, Mars’ surface pressures can vary widely depending on elevation, with atmospheric pressures reaching >10 mb in lowlying features like Lyot Crater (~-7000 m; [1,2]) compared to its average surface pressure of 6.1 mb. The effect of these higher pressures may have been recorded in gully system morphology [2]. This study examines two gullied craters at different elevations to investigate the effect of altitude on gully morphology. These sites include Moni Crater (47.01°S 18.77°E; ~1140 m elevation) and a ~13-km unnamed crater in Utopia Planitia (“N Crater”, 48.44°N 89.39°E; ~-4600 m elevation).

Comparison of elevation on martian gully morphology at crater gully sites

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Comparison of elevation on martian gully morphology at crater gully sites