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Correlations between O^(18)/O^(16) ratios and chemical compositions of tektites

Taylor, Hugh P., Jr. and Epstein, Samuel (1969) Correlations between O^(18)/O^(16) ratios and chemical compositions of tektites. Journal of Geophysical Research, 74 (27). pp. 6834-6844. ISSN 0148-0227. https://resolver.caltech.edu/CaltechAUTHORS:20141107-105624681

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Abstract

The limits of oxygen isotope variation in tektites have been determined by analyzing 33 tektites that cover the widest possible spectrum of chemical compositions. δO^(18) values were obtained for 7 australites (8.9 to 11.0), 4 javaites (9.4 to 10.0), 3 indochinites (9.3 to 10.6), 5 philippinites (9.8 to 10.6), 8 moldavites (10.7 to 11.8), and 6 Ivory Coast tektites (13.0 to 13.6), as well as 2 samples of Darwin glass (14.4 to 14.9). Various tektite groupings based on chemical composition and geographic occurrence all show a systematic increase in O^(18) with decreasing SiO_2 content, similar to that previously found for the bediasites. These systematic correlations must arise either by (1) vapor fractionation of tektite material during impact melting or (2) mixing of a SiO_2-rich igneous component and a low-SiO_2 component formed at a much lower temperature; perhaps the mixing occurred during weathering at the earth's surface or during hydrothermal alteration of silicic igneous rocks either on the earth or the moon.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1029/JB074i027p06834DOIArticle
http://onlinelibrary.wiley.com/doi/10.1029/JB074i027p06834/abstractPublisherArticle
Alternate Title:Correlations between O18/O16 ratios and chemical compositions of tektites
Additional Information:Copyright 1969 by the American Geophysical Union. (Received June 27, 1969.) We are very grateful to Dean R. Chapman and William H. Pinson, Jr., for contributing the samples analyzed in this study. In particular, Dean Chapman suggested that we do further isotopic work on tektites, and he provided carefully selected samples chosen specifically to cover the entire spectrum of chemical compositions and types that he has delineated among the thousands of Australasian tetkites examined by him. We also wish to thank Eugene M. Shoemaker and' Susan Kieffer for supplying the Meteor Crater samples, and we are grateful for stimulating discussions with E. C. T. Chao and L. S. Walter. This work was supported by NASA grant NGR 05-002-085 and Atomic Energy Commission contract AT (04-3)-427, CALT-427-41. Publications of the Division of Geological Sciences, California Institute of Technology, Contribution 1641.
Funders:
Funding AgencyGrant Number
NASANGR 05-002-085
Atomic Energy CommissionAT (04-3)-427
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Caltech Division of Geological Sciences1641
CALT427-41
Issue or Number:27
Record Number:CaltechAUTHORS:20141107-105624681
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20141107-105624681
Official Citation:Taylor Jr., H. P., and S. Epstein (1969), Correlations between O18/O16 ratios and chemical compositions of tektites, J. Geophys. Res., 74(27), 6834–6844, doi:10.1029/JB074i027p06834.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:51432
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:07 Nov 2014 19:20
Last Modified:03 Oct 2019 07:33

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