Boulder Movement on High-Latitude Martian Thermal Contraction Crack Polygons

Mathematics – Logic

Scientific paper

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[5400] Planetary Sciences: Solid Surface Planets, [5422] Planetary Sciences: Solid Surface Planets / Ices, [5462] Planetary Sciences: Solid Surface Planets / Polar Regions, [6225] Planetary Sciences: Solar System Objects / Mars

Scientific paper

Boulders on patterned ground terrain on Mars tend to cluster in cracks (Fig. 1). The precise mechanism for boulder clustering remains unknown but various hypotheses have been proposed. These processes are based on our understanding of patterned ground on Earth but Mars presents a unique situation. We propose the following model (pictured in Figure 2): a) Impact craters or other geological phenomena produce boulders at the surface. b) CO2 frost forms which locks boulders in place. c) The descending temperature wave caused thermal contraction of the underlying polygons. d) The CO2 sublimates releasing the boulders. e) The polygons expand and the boulders experience a net movement towards the polygon edge. Our initial calculations showed that solid CO2 indeed could lock boulders below a size threshold in place and that 5 m diameter polygons contract/expand as much as 5 mm through the year. We now present the results of our detailed analysis of the thermal contraction of polygons and migration of boulders.

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