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Communication Dans Un Congrès Année : 2012

Dunes on Titan at the Beginning of the Cassini Solstice Mission

Résumé

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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hal-01078380 , version 1 (28-10-2014)

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  • HAL Id : hal-01078380 , version 1

Citer

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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