<?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>W.R. Muehlberger</dc:contributor>
  <dc:creator>K. A. Howard</dc:creator>
  <dc:date>1973</dc:date>
  <dc:description>"Wrinkle ridges" in the Taurus-Littrow region along the eastern margin of the Mare Serenitatis appear very fresh and are probably among the youngest on the Moon. They include both mare ridges and similar-looking one-sided scarps. Evidence will be presented here to suggest that these ridges and scarps may be anticlines and thrust faults that resulted from sliding on a d&amp;eacute;collement surface. Alternative interpretations are presented by Scott (part D) and Hodges (part B).</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:language>en</dc:language>
  <dc:publisher>National Aeronautics and Space Administration</dc:publisher>
  <dc:title>Mare ridges and related studies: Part C: lunar thrust faults in the Taurus-Littrow region</dc:title>
  <dc:type>chapter</dc:type>
</oai_dc:dc>