Single crystal 40Ar‐39Ar dating of a Late Quaternary paroxysm on Kos, Greece: Concordance of terrestrial and marine ages
Identifieur interne : 000107 ( Istex/Corpus ); précédent : 000106; suivant : 000108Single crystal 40Ar‐39Ar dating of a Late Quaternary paroxysm on Kos, Greece: Concordance of terrestrial and marine ages
Auteurs : P. E. Smith ; D. York ; Y. Chen ; N. M. EvensenSource :
- Geophysical Research Letters [ 0094-8276 ] ; 1996-10-15.
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Abstract
The late Quaternary plinian eruption forming the Kos Plateau Tuff on the island of Kos, Greece, was one of the largest in the Mediterranean. A precise date for this eruption would significantly improve the chronology of the deep‐sea tephra layer W‐3, because reliable correlation of W‐3 with the KOS Plateau Tuff has been previously established. We have dated sanidine from the eruption at 161.3±1.1 ka using the laser‐fusion single crystal 40Ar‐39Ar technique. This age represents a significant refinement over both conventional and highly precise (Cassignol method) K‐Ar ages, and the 40Ar‐39Ar age is shown to be in remarkably good agreement with the age of W‐3 inferred from recent astronomically calibrated oxygen isotope chronologies.
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DOI: 10.1029/96GL02759
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ISTEX:00828BF71B1D548EA700C8D2FD4AD176C8EA7BF1Le document en format XML
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Smith</name><affiliation><mods:affiliation>Department of Physics, University of Toronto, Toronto, Ontario</mods:affiliation></affiliation></author><author><name sortKey="York, D" sort="York, D" uniqKey="York D" first="D." last="York">D. York</name><affiliation><mods:affiliation>Department of Physics, University of Toronto, Toronto, Ontario</mods:affiliation></affiliation></author><author><name sortKey="Chen, Y" sort="Chen, Y" uniqKey="Chen Y" first="Y." last="Chen">Y. Chen</name><affiliation><mods:affiliation>Department of Physics, University of Toronto, Toronto, Ontario</mods:affiliation></affiliation></author><author><name sortKey="Evensen, N M" sort="Evensen, N M" uniqKey="Evensen N" first="N. M." last="Evensen">N. M. Evensen</name><affiliation><mods:affiliation>Department of Physics, University of Toronto, Toronto, Ontario</mods:affiliation></affiliation></author></analytic><monogr></monogr><series><title level="j" type="main">Geophysical Research Letters</title><title level="j" type="alt">GEOPHYSICAL RESEARCH LETTERS</title><idno type="ISSN">0094-8276</idno><idno type="eISSN">1944-8007</idno><imprint><biblScope unit="vol">23</biblScope><biblScope unit="issue">21</biblScope><biblScope unit="page" from="3047">3047</biblScope><biblScope unit="page" to="3050">3050</biblScope><biblScope unit="page-count">4</biblScope><date type="published" when="1996-10-15">1996-10-15</date></imprint><idno type="ISSN">0094-8276</idno></series></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0094-8276</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Ageof</term><term>Composite isochron</term><term>Eastern mediterranean</term><term>Hilgen</term><term>Isochron</term><term>Isotope</term><term>Keller</term><term>Kelleret</term><term>Late quaternary paroxysm</term><term>Pasteels</term><term>Pleistocene</term><term>Pumice</term><term>Quartz</term><term>Sanidine</term><term>Santorini</term><term>Sapropel</term><term>Stratigraphic</term><term>Tephra</term><term>Thekostuff</term><term>Tuff</term><term>University toronto</term><term>Xenocrystic contamination</term><term>Xenolith</term></keywords><keywords scheme="Teeft" xml:lang="en"><term>Ageof</term><term>Composite isochron</term><term>Eastern mediterranean</term><term>Hilgen</term><term>Isochron</term><term>Isotope</term><term>Keller</term><term>Kelleret</term><term>Late quaternary paroxysm</term><term>Pasteels</term><term>Pleistocene</term><term>Pumice</term><term>Quartz</term><term>Sanidine</term><term>Santorini</term><term>Sapropel</term><term>Stratigraphic</term><term>Tephra</term><term>Thekostuff</term><term>Tuff</term><term>University toronto</term><term>Xenocrystic contamination</term><term>Xenolith</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract">The late Quaternary plinian eruption forming the Kos Plateau Tuff on the island of Kos, Greece, was one of the largest in the Mediterranean. A precise date for this eruption would significantly improve the chronology of the deep‐sea tephra layer W‐3, because reliable correlation of W‐3 with the KOS Plateau Tuff has been previously established. We have dated sanidine from the eruption at 161.3±1.1 ka using the laser‐fusion single crystal 40Ar‐39Ar technique. This age represents a significant refinement over both conventional and highly precise (Cassignol method) K‐Ar ages, and the 40Ar‐39Ar age is shown to be in remarkably good agreement with the age of W‐3 inferred from recent astronomically calibrated oxygen isotope chronologies.</div></front></TEI><istex><corpusName>wiley</corpusName><keywords><teeft><json:string>sanidine</json:string><json:string>ageof</json:string><json:string>santorini</json:string><json:string>isochron</json:string><json:string>keller</json:string><json:string>sapropel</json:string><json:string>tephra</json:string><json:string>tuff</json:string><json:string>stratigraphic</json:string><json:string>pumice</json:string><json:string>isotope</json:string><json:string>hilgen</json:string><json:string>kelleret</json:string><json:string>thekostuff</json:string><json:string>xenolith</json:string><json:string>pleistocene</json:string><json:string>pasteels</json:string><json:string>university toronto</json:string><json:string>quartz</json:string><json:string>late quaternary paroxysm</json:string><json:string>eastern mediterranean</json:string><json:string>xenocrystic contamination</json:string><json:string>composite isochron</json:string></teeft></keywords><author><json:item><name>P. E. Smith</name><affiliations><json:string>Department of Physics, University of Toronto, Toronto, Ontario</json:string></affiliations></json:item><json:item><name>D. York</name><affiliations><json:string>Department of Physics, University of Toronto, Toronto, Ontario</json:string></affiliations></json:item><json:item><name>Y. Chen</name><affiliations><json:string>Department of Physics, University of Toronto, Toronto, Ontario</json:string></affiliations></json:item><json:item><name>N. M. Evensen</name><affiliations><json:string>Department of Physics, University of Toronto, Toronto, Ontario</json:string></affiliations></json:item></author><articleId><json:string>96GL02759</json:string></articleId><language><json:string>eng</json:string></language><originalGenre><json:string>article</json:string></originalGenre><abstract>The late Quaternary plinian eruption forming the Kos Plateau Tuff on the island of Kos, Greece, was one of the largest in the Mediterranean. A precise date for this eruption would significantly improve the chronology of the deep‐sea tephra layer W‐3, because reliable correlation of W‐3 with the KOS Plateau Tuff has been previously established. We have dated sanidine from the eruption at 161.3±1.1 ka using the laser‐fusion single crystal 40Ar‐39Ar technique. 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E.</forename><surname>Smith</surname></persName><affiliation>Department of Physics, University of Toronto, Toronto, Ontario</affiliation></author><author xml:id="author-0001"><persName><forename type="first">D.</forename><surname>York</surname></persName><affiliation>Department of Physics, University of Toronto, Toronto, Ontario</affiliation></author><author xml:id="author-0002"><persName><forename type="first">Y.</forename><surname>Chen</surname></persName><affiliation>Department of Physics, University of Toronto, Toronto, Ontario</affiliation></author><author xml:id="author-0003"><persName><forename type="first">N. 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A precise date for this eruption would significantly improve the chronology of the deep‐sea tephra layer W‐3, because reliable correlation of W‐3 with the KOS Plateau Tuff has been previously established. We have dated sanidine from the eruption at 161.3±1.1 ka using the laser‐fusion single crystal <hi rend="superscript">40</hi>Ar‐<hi rend="superscript">39</hi>Ar technique. This age represents a significant refinement over both conventional and highly precise (Cassignol method) K‐Ar ages, and the <hi rend="superscript">40</hi>Ar‐<hi rend="superscript">39</hi>Ar age is shown to be in remarkably good agreement with the age of W‐3 inferred from recent astronomically calibrated oxygen isotope chronologies.</p></abstract><textClass><classCode scheme="http://psi.agu.org/taxonomy5/8400">Volcanology</classCode><classCode scheme="http://psi.agu.org/taxonomy5/9300">Geographic Location</classCode><classCode scheme="http://psi.agu.org/taxonomy5/9600">Information Related to Geologic Time</classCode></textClass><langUsage><language ident="EN"></language></langUsage></profileDesc></teiHeader></istex:fulltextTEI><json:item><extension>txt</extension><original>false</original><mimetype>text/plain</mimetype><uri>https://api.istex.fr/document/00828BF71B1D548EA700C8D2FD4AD176C8EA7BF1/fulltext/txt</uri></json:item></fulltext><metadata><istex:metadataXml wicri:clean="Wiley, elements deleted: body"><istex:xmlDeclaration>version="1.0" encoding="UTF-8" standalone="yes"</istex:xmlDeclaration><istex:document><component type="serialArticle" version="2.0" xml:lang="en" xml:id="grl9636"><header><publicationMeta level="product"><doi>10.1002/(ISSN)1944-8007</doi><issn type="print">0094-8276</issn><issn type="electronic">1944-8007</issn><idGroup><id type="product" value="GRL"></id></idGroup><titleGroup><title type="main" xml:lang="en" sort="GEOPHYSICAL RESEARCH LETTERS">Geophysical Research Letters</title><title type="short">Geophys. 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E.</givenNames> <familyName>Smith</familyName></personName></creator><creator creatorRole="author" xml:id="grl9636-cr-0002" affiliationRef="#grl9636-aff-0001"><personName><givenNames>D.</givenNames> <familyName>York</familyName></personName></creator><creator creatorRole="author" xml:id="grl9636-cr-0003" affiliationRef="#grl9636-aff-0001"><personName><givenNames>Y.</givenNames> <familyName>Chen</familyName></personName></creator><creator creatorRole="author" xml:id="grl9636-cr-0004" affiliationRef="#grl9636-aff-0001"><personName><givenNames>N. 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This age represents a significant refinement over both conventional and highly precise (Cassignol method) K‐Ar ages, and the <sup>40</sup>Ar‐<sup>39</sup>Ar age is shown to be in remarkably good agreement with the age of W‐3 inferred from recent astronomically calibrated oxygen isotope chronologies.</p></abstract></abstractGroup></contentMeta></header></component></istex:document></istex:metadataXml><mods version="3.6"><titleInfo lang="en"><title>Single crystal 40Ar‐39Ar dating of a Late Quaternary paroxysm on Kos, Greece: Concordance of terrestrial and marine ages</title></titleInfo><titleInfo type="alternative" contentType="CDATA" lang="en"><title>Single crystal 40Ar‐39Ar dating of a Late Quaternary paroxysm on Kos, Greece: Concordance of terrestrial and marine ages</title></titleInfo><name type="personal"><namePart type="given">P. 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A precise date for this eruption would significantly improve the chronology of the deep‐sea tephra layer W‐3, because reliable correlation of W‐3 with the KOS Plateau Tuff has been previously established. We have dated sanidine from the eruption at 161.3±1.1 ka using the laser‐fusion single crystal 40Ar‐39Ar technique. This age represents a significant refinement over both conventional and highly precise (Cassignol method) K‐Ar ages, and the 40Ar‐39Ar age is shown to be in remarkably good agreement with the age of W‐3 inferred from recent astronomically calibrated oxygen isotope chronologies.</abstract><relatedItem type="host"><titleInfo><title>Geophysical Research Letters</title></titleInfo><titleInfo type="abbreviated"><title>Geophys. Res. 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|texte= Single crystal 40Ar‐39Ar dating of a Late Quaternary paroxysm on Kos, Greece: Concordance of terrestrial and marine ages
}}
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