<?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>Noel O. Velasco</dc:contributor>
  <dc:contributor>Axel K. Schmitt</dc:contributor>
  <dc:contributor>Heather A. Bleick</dc:contributor>
  <dc:contributor>Mark E. Stelten</dc:contributor>
  <dc:creator>Jorge A. Vazquez</dc:creator>
  <dc:date>2014</dc:date>
  <dc:description>&lt;p&gt;Application of &lt;sup&gt;238&lt;/sup&gt;U-&lt;sup&gt;230&lt;/sup&gt;Th disequilibrium dating of accessory minerals with contrasting stabilities and compositions can provide a unique perspective on magmatic evolution by placing the thermochemical evolution of magma within the framework of absolute time. Chevkinite, a Th-rich accessory mineral that occurs in peralkaline and metaluminous rhyolites, may be particularly useful as a chronometer of crystallization and differentiation because its composition may reflect the chemical changes of its host melt. Ion microprobe&amp;nbsp;&lt;sup&gt;128&lt;/sup&gt;U-&lt;sup&gt;230&lt;/sup&gt;Th dating of single chevkinite microphenocrysts from pre- and post-caldera La Primavera, Mexico, rhyolites yields model crystallization ages that are within 10's of k.y. of their corresponding K-Ar ages of ca. 125 ka to 85 ka, while chevkinite microphenocrysts from a post-caldera Yellowstone, USA, rhyolite yield a range of ages from ca. 110 ka to 250 ka, which is indistinguishable from the age distribution of coexisting zircon. Internal chevkinite-zircon isochrons from La Primavera yield Pleistocene ages with ~5% precision due to the nearly two order difference in Th/U between both minerals. Coupling chevkinite &lt;sup&gt;238&lt;/sup&gt;U-&lt;sup&gt;230&lt;/sup&gt;Th ages and compositional analyses reveals a secular trend of Th/U and rare earth elements recorded in Yellowstone rhyolite, likely reflecting progressive compositional evolution of host magma. The relatively short timescale between chevkinite-zircon crystallization and eruption suggests that crystal-poor rhyolites at La Primavera were erupted shortly after differentiation and/or reheating. These results indicate that &lt;sup&gt;238&lt;/sup&gt;U-&lt;sup&gt;230&lt;/sup&gt;Th dating of chevkinite via ion microprobe analysis may be used to date crystallization and chemical evolution of silicic magmas.&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1016/j.chemgeo.2014.10.020</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>Elsevier</dc:publisher>
  <dc:title>238U-230Th dating of chevkinite in high-silica rhyolites from La Primavera and Yellowstone calderas</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>