Simulating early Mars hydrology with the MARSSIM landform evolution model: New insights from an integrated system of precipitation, infiltration, and groundwater flow

Abstract

The MARSSIM landform evolution model has been used successfully over the past three decades to simulate sediment transport on the surface of Mars. The model relies on an advection–diffusion relation that has been used to describe the difference in scale efficiency and profile concavity in landscapes. Beyond this, MARSSIM has also been used to simulate groundwater flow, eolian transport, and impact cratering. We first describe the history of the model in the published literature, followed by an in-depth analysis of the physical theory on which it is based. We review the successes and limitations of the current model and how these have been addressed. Other parts of the model included in the source code have been rarely used, so we also investigate new applications in these areas. Finally, we propose a modification to the model that would allow for an integrated system of precipitation, infiltration, and groundwater flow, and provide a practical example on a simulated cratered terrain similar to those found in past MARSSIM studies. We find that the introduction of an integrated model has noticeable effects on erosion patterns within the simulation domain compared to cases of either complete infiltration or complete runoff.