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dc.contributor.advisorNeish, Catherine
dc.contributor.authorFey, Deirdra
dc.date2015-04
dc.date.accessioned2015-09-08T19:14:56Z
dc.date.available2015-09-08T19:14:56Z
dc.identifier.citationFey, D. (2015, April). Sand Dune Elevations on the Earth, Mars, and Titan. Poster presented at the Northrop Grumman Engineering & Science Student Design Showcase, Florida Institute of Technology, Melbourne, FL.en_US
dc.identifier.urihttp://hdl.handle.net/11141/733
dc.description.abstractSand dunes are observed on many places in the solar system. They are found on bodies with atmospheres and are formed through wind processes. Dunes can tell us about the geological process on the planets they inhabit. Dunes are found on many worlds, including Earth, Mars and Titan. For Titan, the dunes are a major geologic feature, covering most of the equatorial region. Titan’s sand dunes are at a much higher elevation than the rest of the surface. By comparing the dune elevations of Mars and Earth, we hope to determine the reason for the higher than average dune elevations on Titan.en_US
dc.language.isoen_USen_US
dc.titleSand Dune Elevations on the Earth, Mars, and Titanen_US
dc.typeposteren_US


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