Geomorphic Tests of the Geyser and Dust Devil Models for Triton's Plumes

Physics

Scientific paper

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Dust Devils, Geyser, Plumes, Triton

Scientific paper

The Voyager Neptune Encounter in 1989 revealed plumes rising over Triton's southern hemisphere with diameters that range between tens of meters and 1.5 km to an altitude of 8 km whereupon their plumes are blown at least 100 km to the west. The plumes, in conjunction with dark surface streaks, have been explained as either nitrogen geysers developed by a solid-state greenhouse mechanism in the polar nitrogen ice or as dust devil thermal vortices forming over and entraining material from darker surface patches. This examination explored both models from a geomorphic perspective to identify and test relevant predictions of each mechanism that should be visible in available imagery.

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