| 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. ?? Published by Elsevier Inc. |
| Genre: | Article |
| ProdID: | 70027254 |
| Citation Author: | Keszthelyi, L.; Jaeger, W. L.; Turtle, E. P.; Milazzo, M.; Radebaugh, J. |
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| Citation End Page: | 286 |
| Citation Issue: | 1 |
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| Citation Language: | English |
| Citation Larger Work Title: | Icarus |
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| Citation Number Of Pages: | 16 |
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| Citation Search Results Text: | A post-Galileo view of Io‘s interior; 2004; Article; Journal; Icarus; Keszthelyi, L.; Jaeger, W. L.; Turtle, E. P.; Milazzo, M.; Radebaugh, J. |
| Citation Start Page: | 271 |
| Citation Volume: | 169 |
| Citation Year: | 2004 |
| Type: | citation/reference |
| Text: | A post-Galileo view of Io‘s interior; 2004; Article; Journal; Icarus; Keszthelyi, L.; Jaeger, W. L.; Turtle, E. P.; Milazzo, M.; Radebaugh, J. |
| URL (THUMBNAIL): | http://pubs.er.usgs.gov/thumbnails/outside_thumb.jpg |
| URL (DIGITAL OBJECT IDENTIFIER): | http://dx.doi.org/10.1016/j.icarus.2004.01.005 |
| Date Other: | Thu, 1 Jan 2004 00:00 -0600 |
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