Title of article
A post-Galileo view of Ioʹs interior
Author/Authors
Keszthelyi، نويسنده , , Laszlo and Jaeger، نويسنده , , Windy L. and Turtle، نويسنده , , Elizabeth P and Milazzo، نويسنده , , Moses and Radebaugh، نويسنده , , Jani، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2004
Pages
16
From page
271
To page
286
Abstract
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.
Keywords
IO , volcanism , interiors
Journal title
Icarus
Serial Year
2004
Journal title
Icarus
Record number
2372930
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