The team used a wind tunnel in the Planetary Aeolian Laboratory at NASA's Ames Research Center to establish threshold wind speeds at which grains would start to move on Titan. They found that the threshold was higher than predicted from models based on terrestrial systems. (Credit: Chris Ford/Flickr)

moons

It takes stronger wind to move Titan’s dunes

Vast dunes march across the surface of Saturn’s largest moon, Titan, as they do across the Sahara.

New research from a refurbished NASA wind tunnel reveals the physics of how particles move in Titan’s methane-laden winds. The findings, published in Nature, could help to explain why Titan’s dunes form in the way they do.

“Conditions on Earth seem natural to us, but models from Earth won’t work elsewhere,” says Bruce White, professor of mechanical and aerospace engineering at the University of California, Davis, and a coauthor of the study. “This paper gives us the thresholds to work out what models for Titan would look like.”

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Earth’s dunes are made of silica sand, while Titan’s dunes, revealed by the Cassini space probe, are made of coated grains of crystalline water. Titan’s atmosphere is 95 percent nitrogen, 5 percent methane, and about half again as thick as that of Earth.

When a fluid flows over a layer of particles, there is a threshold speed at which the particles start to move. On Earth, air blowing over sand will start to kick up grains when it reaches a wind speed of about four meters [about 13 feet] per second. But flowing water, which is closer in density to silica, will move sand at much lower speeds.

White and colleagues used a wind tunnel in the Planetary Aeolian Laboratory at NASA’s Ames Research Center to establish threshold wind speeds at which grains would start to move on Titan. They found that the threshold was higher than predicted from models based on terrestrial systems.

They were able to reconcile their experiments with the models by allowing for the low ratio of density between particles and atmosphere on Titan.

Particle flows

The new results should help in understanding atmospheric forces on other icy moons and planets with very thin or thick atmospheres, such as Neptune’s moon Triton, Pluto, or on comets.

The findings can also help us better understand movement of particles in fluids in general. Particle flows are important in a wide range of situations, including coal-mine or grain-elevator dust explosions, environmental pollution, and lubricants.

For White, it’s a return to work he did almost 40 years ago, before joining the faculty at UC Davis. After completing his doctoral research at Iowa State University on the physics of Martian dust storms, White helped the late Ron Greeley at NASA Ames build a wind tunnel for research on Mars and Venus, which became known as the Planetary Aeolian Laboratory. The facility was mothballed in the mid-1980s, but recently refurbished by a group led by Devon Burr at the University of Tennessee-Knoxville, who is first author of the paper.

“It’s very pleasing to be able to hand this on to a new generation of researchers,” White says.

Other coauthors of the paper contributed from Johns Hopkins University; SETI Institute, Mountain View; Arizona State University; and University of Tennessee-Knoxville. NASA supported the work.

Source: UC Davis

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