<?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>M. J. S. Belton</dc:contributor>
  <dc:contributor>G. E. Danielson</dc:contributor>
  <dc:contributor>M. E. Davies</dc:contributor>
  <dc:contributor>D. Gault</dc:contributor>
  <dc:contributor>B. Hapke</dc:contributor>
  <dc:contributor>B. O'Leary</dc:contributor>
  <dc:contributor>R.G. Strom</dc:contributor>
  <dc:contributor>V. Suomi</dc:contributor>
  <dc:contributor>N. Trask</dc:contributor>
  <dc:creator>B. C. Murray</dc:creator>
  <dc:date>1974</dc:date>
  <dc:description>Mercury has a heavily cratered surface containing basins up to at least 1300 kilometers diameter flooded with mare-like material. Many features are closely similar to those on the moon, but significant structural differences exist. Major chemical differentiation before termination of accretion is implied.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1126/science.184.4135.459</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>American Association for the Advancement of Science</dc:publisher>
  <dc:title>Mariner 10 pictures of Mercury: First results</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>