NASA’s Mars Perseverance Rover: Searching for Sand Transport

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NASA’s Mars Perseverance Rover: Searching for Sand Transport
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NASA’s Mars Perseverance Rover is currently stopped for sampling at Skinner Ridge rock. An important aspect of Perseverance’s mission is sampling activities, and therefore the rover’s strategic path is developed around sampling stops. During these stops, the rover must remain stationary for at least

. An important aspect of Perseverance’s mission is sampling activities, and therefore the rover’s strategic path is developed around sampling stops. During these stops, the rover must remain stationary for at least twelve sols in order to conduct proximity science and activities related to abrasion and coring. However, there is another advantage to staying in one place for such a long time.

Sampling stops provide rare opportunities to perform “change detection” experiments, which are used to monitor aeolian — or wind-driven — transport of sand. The fundamental idea behind change detection is straightforward: to search for wind-induced movement of sand, compare identical images of the surface acquired at different times. The relative intensity and direction of the winds that were blowing in the interval between the two photos may be inferred from these observations.

The Mars Perseverance rover is not the first spacecraft to perform this type of imaging experiment. In fact, change detection experiments have been conducted since the earliest missions sent to Mars, stretching back for many decades. Theories developed before robotic exploration predicted that contemporary Martian winds would rarely, if ever, be capable of transporting sand.

Developing models that can effectively explain and predict aeolian activity on Mars is critical for interpreting the planet’s climatic and geologic history. It’s also essential for mitigating risks to landed spacecraft and future human explorers. Surface missions enable scientists to study ongoing aeolian activity in greater detail and with higher spatiotemporal resolution than can be achieved from orbit, which is necessary for reconciling the discrepancy between theory and observation.

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