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Conference papers

Dunes on Titan at the Beginning of the Cassini Solstice Mission

Abstract : Dunes on Titan, a dominant land- form comprising 12-20% of the surface, represent the end product of many surface processes acting in for- eign conditions. Winds in a nitrogen-rich atmosphere with Earth-like pressure transport sand that is likely to have been derived from complex organics produced in the atmosphere. These sands then accumulate into large linear dunes in planet-encircling sand seas con- centrated near the equator.
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Submitted on : Tuesday, October 28, 2014 - 6:50:29 PM
Last modification on : Tuesday, November 16, 2021 - 4:48:49 AM
Long-term archiving on: : Friday, April 14, 2017 - 12:26:24 PM


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  • HAL Id : hal-01078380, version 1


J. Radebaugh, R. D. Lorenz, Alice Le Gall. Dunes on Titan at the Beginning of the Cassini Solstice Mission. Third International Planetary Dune Workshop, Lunar and Planetary Institute, Jun 2012, Flagstaff, United States. pp.#7031. ⟨hal-01078380⟩



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