| タイトル | Chemistry and Mineralogy of Antarctica Dry Valley Soils: Implications for Mars |
| 本文（外部サイト） | http://hdl.handle.net/2060/20110008124 |
| 著者（英） | Tamppari, L, K.; Smith, P. H.; McKay, C. P.; Morris, R. V.; Graff, T. G.; Quinn, J. E.; Golden, D. C.; Archer, P. D., Jr.; Ming, D. W.; Kounaves, S. P.; Douglas, S.; Zent, A. P. |
| 著者所属（英） | NASA Johnson Space Center |
| 発行日 | 2011-03-07 |
| 言語 | eng |
| 内容記述 | The Antarctic Dry Valleys (ADV) comprise the largest ice-free region of Antarctica. Precipitation almost always occurs as snow, relative humidity is frequently low, and mean annual temperatures are about -20 C. The ADV soils have previously been categorized into three soil moisture regimes: subxerous, xerous and ultraxerous, based on elevation and climate influences. The subxerous regime is predominately a coastal zone soil, and has the highest average temperature and precipitation, while the ultraxerous regime occurs at high elevation (>1000 m) and have very low temperature and precipitation. The amounts and types of salts present in the soils vary between regions. The nature, origin and significance of salts in the ADV have been previously investigated. Substantial work has focused on soil formation in the ADVs, however, little work has focused on the mineralogy of secondary alteration phases. The dominant weathering process in the ADV region is physical weathering, however, chemical weathering has been well documented. The objective of this study was to characterize the chemistry and mineralogy, including the alteration mineralogy, of soils from two sites, a subxerous soil in Taylor Valley, and an ultraxerous soil in University Valley. The style of aqueous alteration in the ADVs may have implications for pedogenic processes on Mars. |
| NASA分類 | Geophysics |
| レポートNO | JSC-CN-22848 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
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