<?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:creator>J. B. Plescia</dc:creator>
  <dc:date>1987</dc:date>
  <dc:description>&lt;p&gt;The southern hemisphere of Ariel, a satellite of Uranus, can be divided into several terrain types. Data on the size-frequency distribution of craters for those different terrain types indicate that these terrains formed over a relatively short period of time. Much information on Ariel's geological history can be gained from these data.&amp;nbsp;&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1038/327201a0</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>Springer Nature</dc:publisher>
  <dc:title>Geological terrains and crater frequencies on Ariel</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>