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.