IANSOct 11, 2017 18:38:05 IST
The fact that we see active sand dunes on Mars today requires that sand particles must be resupplied to replace the grains that are lost over time.
The Martian region spotted by MRO exhibits dark material that is being eroded from dark layers in the bedrock of a semicircular depression near the boundary of the Southern highlands and the Northern lowlands.
Downslope lineations support the notion that these dark sediments are derived locally, and did not accumulate here by coincidence because of the winds, NASA said while releasing the photo on 10 October.
The grains of sand that make up sand dunes on Earth and Mars have a hazardous existence because of the way that they travel.
Wind-blown sand is lifted above the surface of each planet before crashing onto the ground and bouncing in a sequence of repeated hops, a process called saltation.
Sand grains can also roll along the ground as they are blown by the wind, and they are also jostled by other sand gains that are similarly flying across the surface.
All of these repeated impacts tend to wear down the sand grains, smoothing them into a more spherical shape and breaking off small fragments that supply the vast dust deposits of Mars.
This process (known as comminution) ultimately destroys sand grains and limits the length of time that the particles exist.
The regions identified by MRO could be one source from where sand particles get their resupply to replace the grains that are lost over time.
Launched in 2005, MRO is on a search for evidence that water persisted on the surface of Mars for a long period of time to provide a habitat for life
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