44The formation process of recent gullies on Mars is currently under debate. This study aims to 45 discriminate between the proposed formation processes: pure water flow, debris flow and dry 46 mass wasting, through the application of geomorphological indices commonly used in 47 terrestrial geomorphology. We used high resolution digital elevation models of Earth and 48Mars to evaluate the drainage characteristics of small slope sections. We have used the data 49 from Earth to validate the hillslope, debris flow and alluvial process domains previously 50 found for large fluvial catchments on Earth, and have applied these domains to gullied and 51 ungullied slopes on Mars. In accordance with other studies our results indicate that debris 52 flow is one of the main processes forming the martian gullies that we studied. The source of 53 the water is predominantly distributed surface melting, not an underground aquifer. We also 54 present evidence that other processes may have shaped martian crater slopes, such as ice 55 assisted creep and solifluction, in agreement with proposed recent martian glacial and 56 periglacial climate. Our results suggest that, within impact craters, different processes are 57 acting on differently oriented slopes, but further work is needed to investigate the potential 58 link between these observations and changes in martian climate. 59 60 61 4