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Osmium isotopes in Ivory Coast tektites: Confirmation of a meteoritic component and rhenium depletionThe sensitive negative thermal ionization mass spectrometry method was used for the measurement of concentrations and isotopic ratios of osmium and rhenium in four Ivory Coast tektites. These tektites have crustal major and trace element composition, as well as large negative epsilon(sub Nd)(-20) and positive epsilon(sub Sr)(+260 to +300) which are characteristic for old continental crust. Os concentrations ranging from 0.09 to 0.30 ppb were found, clearly much higher than average crustal values, Os-187/Os-186 ratios of about 1.2-1.7, and low Re-187/Os-186 ratios. These results show unambiguously the existence of a meteoritic component (on the order of 0.06%) in the Ivory Coast tektites. Low Re abundances are the result of fractionation of Re during the impact.
Document ID
19940011848
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Koeberl, Christian
(Wien Univ. Austria)
Shirey, Steven B.
(Carnegie Institution of Washington DC., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1993
Publication Information
Publication: Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 2: G-M
Subject Category
Astrophysics
Accession Number
94N16321
Funding Number(s)
PROJECT: FWF PROJ. P9026-GEO
OTHER: NSF EAR-92-18847
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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