<?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>R. M. Batson</dc:contributor>
  <dc:contributor>H. E. Holt</dc:contributor>
  <dc:contributor>E. C. Morris</dc:contributor>
  <dc:contributor>J. J. Rennilson</dc:contributor>
  <dc:contributor>E. A. Whitaker</dc:contributor>
  <dc:creator>Eugene Merle Shoemaker</dc:creator>
  <dc:date>1969</dc:date>
  <dc:description>&lt;div class="article-section__content en main"&gt;&lt;p&gt;Surveyor 7, the last spacecraft of the Surveyor series, landed about 30 km north of the rim crest of Tycho, one of the most prominent and well-known features in the southern part of the moon. About 21,000 pictures were transmitted during two lunar days of operation. At the Surveyor 7 site, the cumulative size-frequency distribution of craters 13 cm to 3 meters in diameter follows closely the distribution of craters observed at the other Surveyor sites in the lunar maria. This distribution of small craters is believed to be a steady-state distribution.&lt;/p&gt;&lt;/div&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1029/JB074i025p06081</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>American Geophysical Union</dc:publisher>
  <dc:title>Observations of the lunar regolith and the Earth from the television camera on Surveyor 7</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>