<?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>Patricio Becerra</dc:contributor>
  <dc:contributor>Shane Byrne</dc:contributor>
  <dc:contributor>Matthew Chojnacki</dc:contributor>
  <dc:contributor>Ingrid J. Daubar</dc:contributor>
  <dc:contributor>Serina Diniega</dc:contributor>
  <dc:contributor>Candice J. Hansen</dc:contributor>
  <dc:contributor>Kenneth E. Herkenhoff</dc:contributor>
  <dc:contributor>Margaret E. Landis</dc:contributor>
  <dc:contributor>Alfred S. McEwen</dc:contributor>
  <dc:contributor>Ganna Portyankina</dc:contributor>
  <dc:contributor>Adomas Valantinas</dc:contributor>
  <dc:creator>Colin M. Dundas</dc:creator>
  <dc:date>2021</dc:date>
  <dc:description>&lt;div class="article-section__content en main"&gt;&lt;p&gt;Mars exhibits diverse surface changes at all latitudes and all seasons. Active processes include impact cratering, aeolian sand and dust transport, a variety of slope processes, changes in polar ices, and diverse effects of seasonal CO&lt;sub&gt;2&lt;/sub&gt;&lt;span&gt;&amp;nbsp;&lt;/span&gt;frost. The extent of surface change has been surprising and indicates that the present climate is capable of reshaping the surface. Activity has important implications for the Amazonian history of Mars: understanding processes is a necessary step before we can understand their implications and variations over time.&lt;/p&gt;&lt;/div&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1029/2021JE006876</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>American Geophysical Union</dc:publisher>
  <dc:title>Active Mars: A dynamic world</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>