Mitchell, Karl L. and Wilson, Lionel (2003) Mars : a geologically active planet. Astronomy and Geophysics, 44 (4). pp. 16-20. ISSN 1468-4004
Full text not available from this repository.Official URL: http://dx.doi.org/10.1046/j.1468-4004.2003.44416.x
Abstract
Recent and continuing missions to Mars are showing that the Red Planet may be more geologically active than previously thought. Volcanoes and erosion by running water have shaped the surface. And evidence is growing that fluvial and possibly volcanic processes have been active in the very recent past.
| Item Type: | Article |
|---|---|
| Journal or Publication Title: | Astronomy and Geophysics |
| Subjects: | G Geography. Anthropology. Recreation > GE Environmental Sciences |
| Departments: | Faculty of Science and Technology > Lancaster Environment Centre |
| ID Code: | 21406 |
| Deposited By: | ep_ss_importer |
| Deposited On: | 13 Jan 2009 11:05 |
| Refereed?: | Yes |
| Published?: | Published |
| Last Modified: | 26 Jul 2012 15:46 |
| Identification Number: | |
| URI: | http://eprints.lancs.ac.uk/id/eprint/21406 |
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