The HO and CO adsorption properties of phyllosilicate-poor palagonitic dust and smectites under martian environmental conditions
The recent detection of up to ∼10 wt.% water-equivalent H heterogeneously distributed in the upper meter of the equatorial regions of the martian surface and the presence of the 3-μm hydrations feature across the entire planet raises the question whether martian surficial dust can account for this w...
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| Veröffentlicht in: | Icarus (New York, N.Y. 1962) N.Y. 1962), 2009-03, Vol.200 (2) |
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| Hauptverfasser: | , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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| Zusammenfassung: | The recent detection of up to ∼10 wt.% water-equivalent H heterogeneously distributed in the upper meter of the equatorial regions of the martian surface and the presence of the 3-μm hydrations feature across the entire planet raises the question whether martian surficial dust can account for this water-equivalent H. We have investigated the HO and CO adsorption properties of palagonitic dust ( |
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| ISSN: | 0019-1035 1090-2643 |
| DOI: | 10.1016/j.icarus.2008.12.006 |