Stereo Imaging, Crater Relaxation, and Thermal Histories of Rhea and Dione

Details Stereo Imaging, Crater Relaxation, and Thermal Histories of Rhea and Dione Stereo Imaging, Crater Relaxation, and Thermal Histories of Rhea and Dione

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2571p&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2571

Computer Science

Scientific paper

We use crater relaxation as a probe for subsurface temperature structure
on satellites of Saturn. Crater relaxation from Cassini DEM crater
profiles is compared with theoretical results. We find Rhea and Dione
were warmer than predicted by our model.

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