<?xml version='1.0' encoding='utf-8'?>
<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>L. Edgar</dc:contributor>
  <dc:contributor>J.C. Bridges</dc:contributor>
  <dc:contributor>A. Williams</dc:contributor>
  <dc:contributor>J. Williams</dc:contributor>
  <dc:contributor>A. Ollila</dc:contributor>
  <dc:contributor>O. Forni</dc:contributor>
  <dc:contributor>N. Mangold</dc:contributor>
  <dc:contributor>N. Lanza</dc:contributor>
  <dc:contributor>V. Sautter</dc:contributor>
  <dc:contributor>S. Gupta</dc:contributor>
  <dc:contributor>D. Blaney</dc:contributor>
  <dc:contributor>B. Clark</dc:contributor>
  <dc:contributor>G. Clegg</dc:contributor>
  <dc:contributor>G. Dromart</dc:contributor>
  <dc:contributor>O. Gasnault</dc:contributor>
  <dc:contributor>J. Lasue</dc:contributor>
  <dc:contributor>S. Le Mouélic</dc:contributor>
  <dc:contributor>Richard Léveillé</dc:contributor>
  <dc:contributor>E. Lewin</dc:contributor>
  <dc:contributor>K. Lewis</dc:contributor>
  <dc:contributor>S. Maurice</dc:contributor>
  <dc:contributor>Marion Nachon</dc:contributor>
  <dc:contributor>H. Newsom</dc:contributor>
  <dc:contributor>D. Vaniman</dc:contributor>
  <dc:contributor>R. C. Wiens</dc:contributor>
  <dc:creator>Ryan Bradley Anderson</dc:creator>
  <dc:date>2014</dc:date>
  <dc:description>&lt;div data-canvas-width="40.49933333333333"&gt;The "Shaler" outcrop in Gale crater is approximately 0.7 m thick and &amp;gt;20 m long, and exhibits multiple well-exposed platy and cross-stratified facies [1] interpreted to be primarily fluvial sandstone deposits. The outcrop is a part of the upper Glenelg member in the Yellowknife Bay (YKB) stratigraphic section [2]. Curiosity first encountered the "Shaler" outcrop on sol 121 of the mission, and returned to the outcrop on sols 309- 324. &lt;/div&gt;&lt;div data-canvas-width="40.49933333333333"&gt;The rugged nature of the outcrop and short time available for analysis limited opportunities for contact science, but ChemCam’s ability to remotely collect compositional and textural observations resulted in a large data set from Shaler. ChemCam conducted analyses of 29 non-soil targets at Shaler, 26 of which used laser-induced breakdown spectroscopy (LIBS) for a total of 9,180 spectra. Three observations used only the remote micro-imager (RMI). Each of the 26 LIBS targets were analyzed at between 5 and 25 points, providing a measure of the target homogeneity and in some cases transecting fine strata.&amp;nbsp;&lt;/div&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:language>en</dc:language>
  <dc:publisher>Lunar and Planetary Institute</dc:publisher>
  <dc:title>ChemCam results from the Shaler Outcrop in Gale Crater, Mars</dc:title>
  <dc:type>text</dc:type>
</oai_dc:dc>