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Polar and Planetary

St. Elias
Field Work
Mission Science
Geophysical Modeling

A Distinctive Approach to Polar and Planetary Geophysics

Scientists at the University of Texas Institute for Geophysics (UTIG) employ space-based, airborne, land-based, and marine geophysical methods to better understand ice sheet evolution, climate, and geologic processes in the polar regions. Our scientists devise and implement investigations that use cutting edge tools and field campaigns to monitor current oceanographic, glacial, and ice sheet processes, to determine past rates of polar geological evolution, and to predict how elements of the polar Earth system will evolve in the future.

By taking a distinctively geophysical approach to studying planetary systems, UTIG scientists are building the scientific and technical foundations to lead the next generation of geophysical planetary missions, instruments, and discoveries. UTIG researchers study planetary systems via the tools of terrestrial analog field programs, geophysical modeling, and mission science. With a breadth of research areas ranging from planetary ionospheres to planetary cores, including a strong focus on the cryosphere/hydrosphere, impacts, and deep interior, UTIG specializes on problems relating to Mars, icy satellites, and giant planets.

UTIG researchers seamlessly transfer technologies, tools, and approaches from polar science to bring new insights to planetary exploration. This interplay between expeditionary polar science and planetary missions and data analysis also allows planetary discoveries and technologies to feed back into the development of new tools and new understandings of Earth system processes.

Learn more about our researchers and students studying polar regions and planetary systems.

 

 

 

Institute for Geophysics

J.J. Pickle Research Campus,
Building 196
10100 Burnet Road (R2200)
Austin, TX 78758-4445

Phone: 512-471-6156
Fax: 512-471-2370

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