Martian Stepped Fans: Analysis of the apron and associated channel

Mathematics – Logic

Scientific paper

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1821 Floods, 1825 Geomorphology: Fluvial (1625), 1856 River Channels (0483, 0744), 5415 Erosion And Weathering, 5419 Hydrology And Fluvial Processes

Scientific paper

Martian stepped fans have a distinctive terraced profile and are often fed by deep, first order canyons with small drainage basins. Using flume experiments, we find that distinct terraces form as a fan deposits into a crater basin filling with water. Terrace preservation implies no long-term deposition at a stable water level and an inactive fluvial system during water drainage. Based on scaling from our experiments, we estimate that the formation time for Martian stepped-fans and channel erosion is on the order of decades and conclude that stepped fans on Mars likely formed during a single, basin-filling event driven by a short-lived, intense hydrologic cycle. The estimated discharge rates are comparable to some of the largest rivers on Earth and these rates highlight the challenges of determining the water source.

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