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ReportsDetection of Perchlorate and the Soluble Chemistry of Martian Soil at the Phoenix Lander Site![]()
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 ~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 ~5-centimeter-deep ice table showed no significant difference in soluble chemistry.
1 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
2 Department of Chemistry, Tufts University, Medford, MA 02155, USA. 3 SETI Institute, NASA Ames Research Center, Moffett Field, CA 94035, USA. 4 Invensys Process Systems, Foxboro, MA 02035, USA. 5 Astromaterials Research and Exploration Science Directorate, NASA Johnson Space Center, Houston, TX 77058, USA. 6 Department of Earth Sciences, University of Bristol, Wills Memorial Building, Bristol BS8 1RJ, UK. 7 Department of Earth and Space Sciences, University of Washington, Seattle, WA 98195, USA. 8 Space Science Institute, Boulder, CO 80301, USA. 9 Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA. 10 Department of Physics, University of Texas at Dallas, Richardson, TX 95080, USA.
* To whom correspondence should be addressed. E-mail: michael.h.hecht{at}jpl.nasa.gov
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Science. ISSN 0036-8075 (print), 1095-9203 (online)