| Abstract: | Hapke (1989, Icarus 79, 56-74) proposed that the surface of Io is dominantly basaltic with thin coatings of polysulfur oxide, S2O, ad SO,2. However, observations and models of the active volcanism indicate that volatiles such as sulfur and SO2 must be more abundant than envisioned by Hapke. ?? 1990. |
| Genre: | Article |
| ProdID: | 70016241 |
| Citation Author: | McEwen, A. S.; Lunine, J. I. |
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| Citation End Page: | 274 |
| Citation Issue: | 1 |
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| Citation Language: | English |
| Citation Larger Work Title: | Icarus |
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| Citation Number Of Pages: | 7 |
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| Citation Search Results Text: | Comment on "The surface of lo: A new model" by Bruce Hapke; 1990; Article; Journal; Icarus; McEwen, A. S.; Lunine, J. I. |
| Citation Start Page: | 268 |
| Citation Volume: | 84 |
| Citation Year: | 1990 |
| Type: | citation/reference |
| Text: | Comment on "The surface of lo: A new model" by Bruce Hapke; 1990; Article; Journal; Icarus; McEwen, A. S.; Lunine, J. I. |
| URL (THUMBNAIL): | http://pubs.er.usgs.gov/thumbnails/outside_thumb.jpg |
| Date Other: | Mon, 1 Jan 1990 00:00 -0600 |
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