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Eruption Age of a ~100,000-Year-Old Basalt From ^(40)Ar-^(39)Ar Analysis of Partially Degassed Xenoliths

Gillespie, A. R. and Huneke, J. C. and Wasserburg, G. J. (1984) Eruption Age of a ~100,000-Year-Old Basalt From ^(40)Ar-^(39)Ar Analysis of Partially Degassed Xenoliths. Journal of Geophysical Research B, 89 (B2). pp. 1033-1048. ISSN 0148-0227. https://resolver.caltech.edu/CaltechAUTHORS:20140115-133554905

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Abstract

We have applied ^(40)Ar-^(39)Ar dating, using stepwise thermal extraction of Ar, to five potassium-rich granitic xenoliths and their host basalt from Sawmill Canyon in the Sierra Nevada, California. Previous K/Ar analyses showed the age of the basalt to be roughly 100,000 years or less. The xenoliths, which had accumulated large amounts of radiogenic ^(40)Ar since their crystallization ∼100 m.y. ago, were partially degassed upon their inclusion in the basaltic magma. Ar released from the xenoliths in the laboratory at temperatures substantially below the melting temperature of the basalt, was created since the host magma cooled. Isotopic compositions of Ar released from the xenoliths in several extraction steps at temperatures below ∼900°C were colinear in ^(36)Ar/^(40)Ar versus ^(39)Ar/^(40)Ar diagrams and defined isochrons giving a mean age of degassing of 119,000±7000 (2σ) years. ^(40)Ar extracted at higher temperatures included ancient radiogenic ^(40)Ar that was never diffused from the xenoliths during immersion in the magma. This ^(40)Ar caused an increase in the apparent age for the high-temperature extractions. The high precision of the eruption age determined by this method is comparable to that obtained elsewhere by conventional K/Ar dating of sanidine. ^(40)Ar-^(39)Ar analysis of granitic xenoliths to date young basaltic lava flows may prove to yield results superior to those found from analysis of the lava itself. Establishing the age of eruption of the basalt flow in Sawmill Canyon establishes age limits for two Sierran glaciations which left moraines stratigraphically above and below the lava. Thus the younger glaciation must be Wisconsin; the older must be pre-Wisconsin in age.


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http://dx.doi.org/10.1029/JB089iB02p01033DOIArticle
http://onlinelibrary.wiley.com/doi/10.1029/JB089iB02p01033/abstractPublisherArticle
Additional Information:© 1984 American Geophysical Union. Received March 25, 1983; revised November 15, 1983; accepted November 17, 1983. We thank Glenn Berger and Mark Harrison for their thorough and thoughtful formal reviews. We are grateful to Art Chodos of Caltech for electron microprobe analyses and to Kathleen Baird of JPL for X-ray diffraction analyses. This research was supported by National Science Foundation grants EAR 78-01717 and EAR 79-19997 and by the Jet Propulsion Laboratory, California Institute of Technology, under contract to the National Aeronautics and Space Administration. Contribution 3629 (392) of the Division of Geological and Planetary Sciences, California Institute of Technology.
Funders:
Funding AgencyGrant Number
NSFEAR 78-01717
NSFEAR 79-19997
NASA/JPL/CaltechUNSPECIFIED
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Caltech Division of Geological and Planetary Sciences3629
Lunatic Asylum Lab392
Issue or Number:B2
Record Number:CaltechAUTHORS:20140115-133554905
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20140115-133554905
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:43389
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:15 Jan 2014 22:49
Last Modified:03 Oct 2019 06:07

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