Modeling the Hydrodynamics, Sediment Transport, and Valley Incision of Outlet‐Forming Floods From Martian Crater Lakes

Abstract

AbstractOpen‐basin lakes that have outlets, formed where the stored water breached the basin‐confining topography (e.g., crater rims), have been recognized on Mars for decades. However, the mechanics involved in formation of these outlets has not been studied in detail. Here, we study this outlet formation process through a series of numerical experiments accomplished by adding erosion and sediment transport routines to an existing hydrodynamic simulation, ANUGA. These experiments are consistent with outlets being carved in single flood events, at least if sediment was available throughout outlet formation as in a transport‐limited regime. Peak discharges from these open‐basin lakes, including from Jezero crater, were 104 to 106 m3/s, and the outlet‐forming floods lasted for days to weeks, depending on lake size. Moreover, we find that sediment transport by suspension was likely important during these floods—outlets could not have reached their observed sizes if flow was limited to bedload transport alone. This in turn may explain why small open‐basin lakes are less commonly recognized on Mars, as small lakes had less inherent capacity to transport sediment in suspension and thus incise confining topography catastrophically. Geometry, topographic setting, and earlier fluvial valley development may have played a significant role in influencing the magnitude of outlet‐forming floods and resulting outlet canyon incision.