We present a self-consistent model for the interior of Io, taking the recent Galileo data into account. In this model, Io has a completely molten core, substantially molten mantle, and a very cold lithosphere. Heat from magmatic activity can mobilize volatile compounds such as SO2 in the lithosphere, and the movement of such cryogenic fluids may be important in the formation of surface features including sapping scarps and paterae.
|Publication Subtype||Journal Article|
|Title||A post-Galileo view of Io's interior|
|Contributing office(s)||Astrogeology Science Center|
|Larger Work Type||Article|
|Larger Work Subtype||Journal Article|
|Larger Work Title||Icarus|
|Google Analytic Metrics||Metrics page|