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<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>Nicolas Mangold</dc:contributor>
  <dc:contributor>Olivier Forni</dc:contributor>
  <dc:contributor>Agnes Cousin</dc:contributor>
  <dc:contributor>Jeremie Lasue</dc:contributor>
  <dc:contributor>Susanne Schröder</dc:contributor>
  <dc:contributor>Roger C. Wiens</dc:contributor>
  <dc:contributor>Dawn Y. Sumner</dc:contributor>
  <dc:contributor>Cecile Fabre</dc:contributor>
  <dc:contributor>Katherine M. Stack</dc:contributor>
  <dc:contributor>Ryan B. Anderson</dc:contributor>
  <dc:contributor>Diana L. Blaney</dc:contributor>
  <dc:contributor>Samuel M. Clegg</dc:contributor>
  <dc:contributor>Gilles Dromart</dc:contributor>
  <dc:contributor>Martin Fisk</dc:contributor>
  <dc:contributor>Olivier Gasnault</dc:contributor>
  <dc:contributor>John P. Grotzinger</dc:contributor>
  <dc:contributor>Sanjeev Gupta</dc:contributor>
  <dc:contributor>Nina Lanza</dc:contributor>
  <dc:contributor>Stephane Le Mouelic</dc:contributor>
  <dc:contributor>Sylvestre Maurice</dc:contributor>
  <dc:contributor>Scott M. McLennan</dc:contributor>
  <dc:contributor>Pierre-Yves Meslin</dc:contributor>
  <dc:contributor>Marion Nachon</dc:contributor>
  <dc:contributor>Horton E. Newsom</dc:contributor>
  <dc:contributor>Valerie Payre</dc:contributor>
  <dc:contributor>William Rapin</dc:contributor>
  <dc:contributor>Melissa Rice</dc:contributor>
  <dc:contributor>Violaine Sautter</dc:contributor>
  <dc:contributor>Allan H. Treiman</dc:contributor>
  <dc:creator>Laetitia Le Deit</dc:creator>
  <dc:date>2016</dc:date>
  <dc:description>&lt;p&gt;The Mars Science Laboratory rover &lt;i&gt;Curiosity&lt;/i&gt; encountered potassium-rich clastic sedimentary rocks at two sites in Gale Crater, the waypoints Cooperstown and Kimberley. These rocks include several distinct meters thick sedimentary outcrops ranging from fine sandstone to conglomerate, interpreted to record an ancient fluvial or fluvio-deltaic depositional system. From ChemCam Laser-Induced Breakdown Spectroscopy (LIBS) chemical analyses, this suite of sedimentary rocks has an overall mean K&lt;sub&gt;2&lt;/sub&gt;O abundance that is more than 5 times higher than that of the average Martian crust. The combined analysis of ChemCam data with stratigraphic and geographic locations reveals that the mean K&lt;sub&gt;2&lt;/sub&gt;O abundance increases upward through the stratigraphic section. Chemical analyses across each unit can be represented as mixtures of several distinct chemical components, i.e., mineral phases, including K-bearing minerals, mafic silicates, Fe-oxides, and Fe-hydroxide/oxyhydroxides. Possible K-bearing minerals include alkali feldspar (including anorthoclase and sanidine) and K-bearing phyllosilicate such as illite. Mixtures of different source rocks, including a potassium-rich rock located on the rim and walls of Gale Crater, are the likely origin of observed chemical variations within each unit. Physical sorting may have also played a role in the enrichment in K in the Kimberley formation. The occurrence of these potassic sedimentary rocks provides additional evidence for the chemical diversity of the crust exposed at Gale Crater.&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1002/2015JE004987</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>American Geophysical Union</dc:publisher>
  <dc:title>The potassic sedimentary rocks in Gale Crater, Mars, as seen by ChemCam Onboard &lt;i&gt;Curiosity&lt;/i&gt;</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>