Hurowitz, J. A. and Tosca, N. J. and McLennan, S. M. and Schoonen, M. A. A. (2007) Production of hydrogen peroxide in Martian and lunar soils. Earth and Planetary Science Letters, 255 (1-2). pp. 41-52.
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Abstract
Freshly ground basaltic minerals produce sufficient quantities of hydrogen peroxide (H2O2) when immersed in solution to explain the oxidizing characteristics of Martian soil samples collected by the Viking landers. H2O2 production occurs as a result of reactions between water and defects at the surface of mechanically pulverized minerals, analogous to carcinogenic quartz dusts. Our results also indicate that dehydroxylation of mineral surfaces results in increased H2O2 production, a highly relevant finding for dusts on the airless surface of the Moon. Reactive, pulverized minerals are important on planetary bodies where impact processes have generated fine-grained basaltic dusts, and may pose a significant health risk to astronauts visiting planetary surfaces where impacts have generated such materials. B) 2006 Elsevier B.V. All rights reserved.
| Item Type: | Article |
|---|---|
| Subjects: | 01 - Climate Change and Earth-Ocean Atmosphere Systems |
| Divisions: | 01 - Climate Change and Earth-Ocean Atmosphere Systems |
| Journal or Publication Title: | Earth and Planetary Science Letters |
| Volume: | 255 |
| Page Range: | pp. 41-52 |
| Depositing User: | Sarah Humbert |
| Date Deposited: | 17 Dec 2009 12:55 |
| Last Modified: | 23 Jul 2013 09:56 |
| URI: | http://eprints.esc.cam.ac.uk/id/eprint/1239 |
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