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1.
Science ; 325(5936): 64-7, 2009 Jul 03.
Artigo em Inglês | MEDLINE | ID: mdl-19574385

RESUMO

The Wet Chemistry Laboratory on the Phoenix Mars Lander performed aqueous chemical analyses of martian soil from the polygon-patterned northern plains of the Vastitas Borealis. The solutions contained approximately 10 mM of dissolved salts with 0.4 to 0.6% perchlorate (ClO4) by mass leached from each sample. The remaining anions included small concentrations of chloride, bicarbonate, and possibly sulfate. Cations were dominated by Mg2+ and Na+, with small contributions from K+ and Ca2+. A moderately alkaline pH of 7.7 +/- 0.5 was measured, consistent with a carbonate-buffered solution. Samples analyzed from the surface and the excavated boundary of the approximately 5-centimeter-deep ice table showed no significant difference in soluble chemistry.


Assuntos
Ânions , Cátions , Marte , Percloratos , Fenômenos Químicos , Meio Ambiente Extraterreno , Concentração de Íons de Hidrogênio , Oxirredução , Solubilidade , Astronave , Temperatura , Água
2.
Science ; 325(5936): 61-4, 2009 Jul 03.
Artigo em Inglês | MEDLINE | ID: mdl-19574384

RESUMO

Carbonates are generally products of aqueous processes and may hold important clues about the history of liquid water on the surface of Mars. Calcium carbonate (approximately 3 to 5 weight percent) has been identified in the soils around the Phoenix landing site by scanning calorimetry showing an endothermic transition beginning around 725 degrees C accompanied by evolution of carbon dioxide and by the ability of the soil to buffer pH against acid addition. Based on empirical kinetics, the amount of calcium carbonate is most consistent with formation in the past by the interaction of atmospheric carbon dioxide with liquid water films on particle surfaces.


Assuntos
Carbonato de Cálcio , Marte , Dióxido de Carbono , Precipitação Química , Meio Ambiente Extraterreno , Temperatura Alta , Concentração de Íons de Hidrogênio , Astronave , Água
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