1. Celestial Reasonings, Carson City, Nevada 89703, USA
2. US Geological Survey, Flagstaff, Arizona 86001, USA
3. Department of Geological Sciences, Arizona State University, Tempe, Arizona 85287, USA

Correspondence to: Philip R. Christensen³ Correspondence and requests for materials should be addressed to P.R.C. (Email: phil.christensen@asu.edu).

Abstract

The martian polar caps are among the most dynamic regions on Mars, growing substantially in winter as a significant fraction of the atmosphere freezes out in the form of CO₂ ice. Unusual dark spots, fans and blotches form as the south-polar seasonal CO₂ ice cap retreats during spring and summer. Small radial channel networks are often associated with the location of spots once the ice disappears. The spots have been proposed to be simply bare, defrosted ground^{1, 2, 3}; the formation of the channels has remained uncertain. Here we report infrared and visible observations that show that the spots and fans remain at CO₂ ice temperatures well into summer, and must be granular materials that have been brought up to the surface of the ice, requiring a complex suite of processes to get them there. We propose that the seasonal ice cap forms an impermeable, translucent slab of CO₂ ice that sublimates from the base, building up high-pressure gas beneath the slab. This gas levitates the ice, which eventually ruptures, producing high-velocity CO₂ vents that erupt sand-sized grains in jets to form the spots and erode the channels. These processes are unlike any observed on Earth.

MORE ARTICLES LIKE THIS

These links to content published by NPG are automatically generated.