<?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. Edward Danielson</dc:contributor>
  <dc:contributor>M. E. Davies</dc:contributor>
  <dc:contributor>D. E. 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>&lt;p&gt;The surface morphology and optical properties of Mercury resemble those of the moon in remarkable detail and record a very similar sequence of events. Chemical and mineralogical similarity of the outer layers of Mercury and the moon is implied; Mercury is probably a differentiated planet with a large iron-rich core. Differentiation is inferred to have occurred very early. No evidence of atmospheric modification of landforms has been found. Large-scale scarps and ridges unlike lunar or Martian features may reflect a unique period of planetary compression near the end of heavy bombardment by small planetesimals.&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1126/science.185.4146.169</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>American Association for the Advancement of Science</dc:publisher>
  <dc:title>Mercury's surface: Preliminary description and interpretation from Mariner 10 pictures</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>