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dc.contributor.authorOostingh, K.
dc.contributor.authorJourdan, Fred
dc.contributor.authorDanisik, Martin
dc.contributor.authorEvans, Noreen
dc.date.accessioned2017-11-20T08:50:00Z
dc.date.available2017-11-20T08:50:00Z
dc.date.created2017-11-20T08:13:30Z
dc.date.issued2017
dc.identifier.citationOostingh, K. and Jourdan, F. and Danisik, M. and Evans, N. 2017. Advancements in cosmogenic <sup>38</sup>Ar exposure dating of terrestrial rocks. Geochimica Et Cosmochimica Acta. 217: pp. 193-218.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/58002
dc.identifier.doi10.1016/j.gca.2017.07.043
dc.description.abstract

© 2017 Elsevier Ltd Cosmogenic exposure dating of Ca-rich minerals using 38 Ar on terrestrial rocks could be a valuable new dating tool to determine timescales of geological surface processes on Earth. Here, we show that advancement in analytical precision, using the new generation multi-collector ARGUSVI mass spectrometer on irradiated pyroxene and apatite samples, allows determination of cosmogenic 38 Ar abundances above background values, as well as discrimination of 38 Ar/ 36 Ar ratios (1s absolute precision of ±0.3%) from the non-cosmogenic background value. Four statistically significant cosmochron ( 38 Ar/ 36 Ar vs 37 Ar/ 36 Ar) diagrams could be constructed for southeast Australian pyroxene samples from the Mt Elephant scoria cone for which a combined apparent exposure age of 313 ± 179 ka (2s) was obtained when using a 38 Ar production rate (Ca) of 250 atoms /g Ca/ yr. This exposure age overlaps within error with the known 40 Ar/ 39 Ar eruption age of 184 ± 15 ka (2s). Although apatite shows much larger 38 Ar abundances than pyroxene, our modelling and analyses of unirradiated apatite suggest that apatite suffers from both natural and reactor-derived chlorogenic as well as natural nucleogenic contributions of 38 Ar. Hence, we suggest that cosmogenic 38 Ar exposure dating on irradiated Ca-rich (and eventually K-rich), but Cl-free, terrestrial minerals is a potential valuable and accessible tool to determine geological surface processes on timescales of a few Ma. Calculations show that with the new generation multi-collector mass spectrometers an analytical uncertainty better than 5% (2s) can be achieved on samples with expected exposure ages of > 4 Ma.

dc.publisherPergamon
dc.relation.sponsoredbyhttp://purl.org/au-research/grants/arc/DP160102427
dc.titleAdvancements in cosmogenic <sup>38</sup>Ar exposure dating of terrestrial rocks
dc.typeJournal Article
dcterms.source.volume217
dcterms.source.startPage193
dcterms.source.endPage218
dcterms.source.issn0016-7037
dcterms.source.titleGeochimica Et Cosmochimica Acta
curtin.departmentDepartment of Applied Geology
curtin.accessStatusFulltext not available


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