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Planetary Geosciences

Ganymede (an Icy Moon of Jupiter)

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image of physical analog models of the "grooved" terrain on Ganymede, a large icy moon of Jupiter

Physical analog models of the "grooved" terrain on Ganymede, a large icy moon of Jupiter, indicate that rotational half-graben block faulting may be the process that formed Ganymede's unique surface.

 

For more information about planetary physical analog modeling capabilities at  Southwest Research Institute (SwRI) or how you can contract with SwRI, please contact Danielle Y. Wyrick at dwyrick@swri.org or (210) 522-6837.
 

Contact Information

Danielle Y. Wyrick

Earth and Planetary Science

(210) 522-6837

dwyrick@swri.org

Related Terminology

planetary geology

Ganymede

Eros

planetary sciences

planetary geosciences

structural analysis

Martian crust

geologic investigations

groundwater flow

physical analog modeling

computer modeling

geophysical surveys

geological analyses

terrestrial sites

Ganymede's icy crust

pit chain formation

Mars

Pellas-Ryder award

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Southwest Research Institute® (SwRI®), headquartered in San Antonio, Texas, is a multidisciplinary, independent, nonprofit, applied engineering and physical sciences research and development organization with 11 technical divisions.

October 04, 2011