A distinct ripple-formation regime on Mars revealed by the morphometrics of barchan dunes - Nature Communications

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A distinct ripple-formation regime on Mars revealed by the morphometrics of barchan dunes - Nature Communications
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How Mars' thin and turbulent atmosphere leads to curiously sized dunes NatureComms

Sand mobilized by wind forms decimeter-scale impact ripples and decameter-scale or larger dunes on Earth and Mars. In addition to those two bedform scales, orbital and in situ images revealed a third distinct class of larger meter-scale ripples on Mars.

Using an artificial neural network, we characterize the morphometrics of over a million isolated barchan dunes on Mars and analyze how their size and shape vary across Mars’ surface. We find that the size of Mars’ smallest dunes decreases with increasing atmospheric density with a power-law exponent predicted by hydrodynamic theory, similarly to meter-size ripples, tightly bounding a forbidden range in bedform sizes.

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