DURING SOUTHERN WINTER, carbon dioxide gas
condenses onto the
polar cap as a thin slab of translucent CO2 ice. When the Sun rises in
spring, the ice sublimates from the bottom of the layer, and the
growing gas pressure lifts the slab off the ground. Gas then breaks
through the slab in places, erupting in jets that carry dust scavenged
from under the slab. The jets leave dark dust marks on the surface of
the ice cap. TES made polar cap temperature measurements that led to
the development of the model for the jets. Click on the image to
download a larger version (5.6 MB).
Arizona State University/Ron Miller
Kieffer, H.H., P.R. Christensen, and T.N. Titus, CO2 jets formed by sublimation beneath translucent slab ice in Mars' seasonal south polar cap, Nature, 442, 793-796, 2006