Near-Surface Heating on Enceladus and the South Polar Thermal Anomaly

Details Near-Surface Heating on Enceladus and the South Polar Thermal Anomaly Near-Surface Heating on Enceladus and the South Polar Thermal Anomaly

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1481r&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

Shear heating along the tiger stripes on Enceladus can enhance
convective upwelling in the underlying ice. Near-surface heating
promotes melting of deep ice, causing regional subsidence, which may
drive TPW, placing the heated region at the pole.

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