Thick deposits cover broad regions of the Martian mid-latitudes with a smooth mantle;
erosion in these regions creates scarps that expose the internal structure of the mantle. We …

Mars exhibits diverse surface changes at all latitudes and all seasons. Active processes
include impact cratering, aeolian sand and dust transport, a variety of slope processes …

Upon their discovery in 2000, Martian gullies were hailed as the first proof of recent (ie less
than a few million years) flowing liquid water on the surface of a dry desert planet. Many …

Although ice in the Martian midlatitudes is typically covered by a layer of dust or regolith, it is
exposed in some locations by fresh impact craters or in erosional scarps. In both cases, the …

A decade of high-resolution monitoring has revealed extensive activity in fresh Martian
gullies. Flows within the gullies are diverse: they can be relatively light, neutral or dark …

Martian gully landforms resemble terrestrial debris flows formed by the action of liquid water
and have thus been interpreted as evidence for potential habitable environments on Mars …

As consequence of ongoing climate change, permafrost degradation is thought to be
increasingly affecting slope stability in periglacial environments. This is of growing concern …

On Mars, seasonal martian flow features known as recurring slope lineae (RSL) are
prevalent on sun-facing slopes and are associated with salts. On Earth, subsurface …

Evidence for past basal melting of young (late Amazonian‐aged), debris‐covered glaciers in
Mars' mid‐latitudes is extremely rare. Thus, it is widely thought that these viscous flow …

Here we study rocks falling from exposed outcrops of bedrock, which have left tracks on the
slope over which they have bounced and/or rolled, in fresh impact craters (1–10 km in …