| Abstract: | The Martian surface shows abundant evidence of water erosion. Liquid water is unstable under present climatic conditions but conditions may have been different in the past. The planet has been volcanically active throughout its history. The combination of water and volcanism must have commonly resulted in hydrothermal environments similar to those in which grow the most primitive terrestrial life-forms. |
| Genre: | Article |
| ProdID: | 70017749 |
| Citation Author: | Carr, M. H. |
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| Citation End Page: | 60 |
| Citation Issue: | 2 |
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| Citation Language: | English |
| Citation Larger Work Title: | Endeavour |
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| Citation Number Of Pages: | 5 |
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| Citation Search Results Text: | Water erosion on mars and its biologic implications; 1996; Article; Journal; Endeavour; Carr, M. H. |
| Citation Start Page: | 56 |
| Citation Volume: | 20 |
| Citation Year: | 1996 |
| Type: | citation/reference |
| Text: | Water erosion on mars and its biologic implications; 1996; Article; Journal; Endeavour; Carr, M. H. |
| URL (THUMBNAIL): | http://pubs.er.usgs.gov/thumbnails/outside_thumb.jpg |
| URL (DIGITAL OBJECT IDENTIFIER): | http://dx.doi.org/10.1016/0160-9327(96)10013-2 |
| Date Other: | Mon, 1 Jan 1996 00:00 -0600 |
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