Thermal and Orbital Evolution of Tethys as Constrained by Surface Observations

Details Thermal and Orbital Evolution of Tethys as Constrained by Surface Observations Thermal and Orbital Evolution of Tethys as Constrained by Surface Observations

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1968c&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

We determine conditions for the orbit and internal structure of Tethys
to account for the high heat flux associated with the formation of
Ithaca Chasma. We suggest that a subsurface ocean was present at some
point in Tethys' history.

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