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More Bright Streaks and Dark Fans
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More Bright Streaks and Dark Fans

December 15, 2007

This caption is part of a December 2007 AGU presentation "Spring at the South Pole of Mars."

The south polar region of Mars is covered every year by a layer of carbon dioxide ice. In a region called the "cryptic terrain," the ice is translucent and sunlight can penetrate through the ice to warm the surface below.

The ice layer sublimates (evaporates) from the bottom. The dark fans of dust seen in this image come from the surface below the layer of ice, carried to the top by gas venting from below. The translucent ice is "visible" by virtue of the effect it has on the tone of the surface below, which would otherwise have the same color and reflectivity as the fans.

Bright streaks in this image are fresh frost. The CRISM team has identified the composition of these streaks to be carbon dioxide.



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