Shear Heating and the Orbital Evolution of Enceladus

Details Shear Heating and the Orbital Evolution of Enceladus Shear Heating and the Orbital Evolution of Enceladus

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1311n&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

Volumetric viscoelastic dissipation depends on eccentricity
e2 and mean motion n5. Shear heating, by contrast,
depends on e3 and n7 and results in longer
eccentricity damping timescales.

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