Boulders form from a variety of geological processes, which their size, shape, and
orientation may help us better understand. Furthermore, they represent potential hazards to …

The seasonal deposition and sublimation of CO2 constitute a major element in the Martian
volatile cycle. Here, we propose to use the shadow variations of the ice blocks at the foot of …

Polygonal terrain on Mars can form via thermal contraction and subsequent fracturing of the
permafrost layer and covers much of the surface poleward of∼ 60°. In similar terrains on …

Boulders are ubiquitous on rocky planets and provide valuable information about planetary
processes. The abundance, size, and distribution of boulders offer insights into the primary …

Boulder occurrence at the southern polar regions of the Moon was analysed to see
connections between optical, radio, spectral, and topography-related roughness datasets …