Planetary science: Martian debris flows from 'recent' running water

Evidence that running water caused frequent debris flows on Mars is reported in a paper published in Nature Communications. Although there is no running water there now, it is thought that sufficient water was flowing in the last million years to cause these frequent flows, suggesting a much more dynamic environment until relatively recently.

Mars is currently very cold and dry and its thin atmosphere makes liquid water at its surface exceptionally rare. However, recent discoveries of extensive gully systems incised into slopes suggest that they were carved by the flow of liquid water. Tjalling de Haas and colleagues investigate a crater that has a maximum age of one million years and calculate the debris flow size and the volumes of water that must have been present. They suggest that centimetres of liquid water existed in the catchment areas resulting in frequent debris flows. The authors think that the melting must have occurred in cyclical periods of warmer climate related to changes in the planet’s orbit.

The results of the study imply that much larger volumes of snow and ice must have existed within the catchment areas than previously imagined. They also suggest that Martian slopes oriented like the one studied were extremely active environments, with Earth-like debris flow frequencies in the geologically very recent past.