Lifting Grains by the Transient Low Pressure in a Martian Dust Devil

Abstract

Lifting dust and sand into the thin Martian atmosphere is a challenging problem. Atmospheric pressure excursions within dust devils have been proposed to support lifting. We verify this idea in laboratory experiments. Pressure differences up to a few Pa are applied along particle layers of 50 to 400 $\mu \mathrm{m}$. As samples we used glass beads of $\sim$50 $\mu \mathrm{m}$ diameter and irregular basalt grains of $\sim$20 $\mu \mathrm{m}$ in size. The total ambient pressure of air was set to 600 Pa. Particles are ejected at pressure differences as low as 2.0 $\pm$ 0.8 Pa. In the case of glass beads, the ejected grains returning to the particle bed can trigger new particle ejections as they reduce cohesion and release the tension from other grains. Therefore, few impacting grains might be sufficient to sustain dust lifting in a dust devil at even lower pressure differences. Particle lift requires a very thin, $\sim$100 $\mu \mathrm{m}$, low permeability particle layer on top of supporting ground with larger pore space. Assuming this, our experiments support the idea that pressure excursions in Martian dust devils release grains from the ground.

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• Dust aerosol, clouds, and the atmospheric optical depth record over 5 Mars years of the Mars Exploration Rover mission
• Sticking Properties of Silicates in Planetesimal Formation Revisited
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Cited by in corpus (2)

• Lifting of Tribocharged Grains by Martian Winds
• Thermal Creep on Mars: Visualizing a Soil Layer under Tension