Eros (a Near-Earth Asteroid)
Ganymede (an Icy Moon of Jupiter)
Geologic and
Hydrologic Investigations of
Past Surface and Groundwater Flow
Structural Analyses of
the Martian Crust in a Variety of Tectonic Settings
Geophysical Surveys
and Geological Analyses of Terrestrial Sites as Analogs to Mars
Computer Modeling of
Multi-Phase Water Under Martian Conditions
Publications
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SwRI Information
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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. |
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For more information about our planetary geosciences
capabilities, or how you can contract with Southwest Research
Institute (SwRI),
please contact
Danielle Y. Wyrick
at
dwyrick@swri.org or
(210) 522-6837.
planetarygeosciences.swri.org
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Contact Information |
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Danielle Y. Wyrick
Planetary Geosciences
(210) 522-6837
dwyrick@swri.org
planetarygeosciences.swri.org
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Related Terminology |
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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.
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