A Forest of Channels on the South Polar Layered Deposits (by Lunar and Planetary Institute)
The sublimation of seasonal carbon dioxide in the Martian polar regions seems to erode connected channels on the underlying surface, as escaping carbon dioxide gas scours the surface beneath the carbon dioxide ice. Such features are fairly common to the south polar region. However, the channel clusters here are unusually even in their spacing. The carbon dioxide gas-driven erosion will exploit pre-existing weakness in the underlying surface, so it’s possible that these features are following joints or fractures that exist in the layered deposits. The regularity of these features may suggest something about the thickness of ground ice deep below the surface. ASU-IPF-3256
