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Yardangs on Mars

Aeolian formation From Wikipedia, the free encyclopedia

Yardangs on Mars
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Yardangs are common in some regions on Mars, especially in the Medusae Fossae Formation. This formation is found in the Amazonis quadrangle and near the equator.[1] They are formed by the action of wind on sand sized particles; hence they often point in the prevailing direction that the winds were blowing when they were formed.[2][3] Yardangs exhibit very few impact craters, indicating that the surface exposed is relatively young and the process of erosion may be active.[4] The easily eroded nature of the Medusae Fossae Formation suggests that it is composed of weakly cemented particles, and was most likely formed by the deposition of wind-blown dust or volcanic ash. Yardangs are parts of rock that have been sand blasted into long, skinny ridges by bouncing sand particles blowing in the wind.[5][6] Layers are seen in parts of the formation. A resistant caprock on the top of yardangs has been observed in Viking,[7] Mars Global Surveyor,[8] and HiRISE photos.[9] Images from spacecraft show that they have different degrees of hardness probably because of significant variations in the physical properties, composition, particle size, and/or cementation.

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Zooming on the yardangs of Mount Sharp with Remote Micro Imager on the Curiosity rover - sol 1994
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