High-resolution images of the martian surface at scales of a few meter
s show ubiquitous erosional and depositional eolian landforms. Dunes,
sandsheets, and drifts are prevalent and exhibit a range of morphology
, composition (inferred from albedo), and age (as seen in occurrences
of different dune orientations at the same location). Steep walls of t
opographic depressions such as canyons, valleys, and impact craters sh
ow the martian crust to be stratified at scales of a few tens of meter
s. The south polar layered terrain and superposed permanent ice cap di
splay diverse surface textures that may reflect the complex interplay
of volatile and non-volatile components, Low resolution regional views
of the planet provide synoptic observations of polar cap retreat, con
densate clouds, and the lifecycle of local and regional dust storms.