Geochemistry of CI chondrites: Major and trace elements, and Cu and Zn Isotopes

被引：329

作者：

Barrat, J. A. ^{[1
,2
]}

Zanda, B. ^{[3
]}

Moynier, F. ^{[4
]}

Bollinger, C. ^{[1
,2
]}

Liorzou, C. ^{[1
,2
]}

Bayon, G. ^{[5
]}

机构：

[1] UBO IUEM, CNRS UMR Domaines Ocean 6538, F-29280 Plouzane, France

[2] Univ Europeenne Bretagne, Rennes, France

[3] Museum Natl Hist Nat, CNRS UMR 7202, Lab Mineral & Cosmochim Museum, F-75005 Paris, France

[4] Washington Univ St Louis, Dept Earth & Planetary Sci, McDonnell Ctr Space Sci, St Louis, MO 63130 USA

[5] IFREMER, Dept Geosci Marines, F-29280 Plouzane, France

来源：

GEOCHIMICA ET COSMOCHIMICA ACTA | 2012年 / 83卷

关键词：

SOLAR-SYSTEM ABUNDANCES; RARE-EARTH-ELEMENTS; CARBONACEOUS CHONDRITES; MANTLE DIFFERENTIATION; GEOLOGICAL-MATERIALS; TAGISH LAKE; METEORITES; SAMPLES; COPPER; ZINC;

D O I：

10.1016/j.gca.2011.12.011

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

In order to check the heterogeneity of the CI chondrites and determine the average composition of this group of meteorites, we analyzed a series of six large chips (weighing between 0.6 and 1.2 g) of Orgueil prepared from five different stones. In addition, one sample from each of Ivuna and Alais was analyzed. Although the sizes of the chips used in this study were "large", our results show evidence for minor chemical heterogeneity in Orgueil, particularly for alkali elements and U. After removal of one outlier sample, the spread of the results is considerably reduced. For most of the 46 elements analyzed in this study, the average composition calculated for Orgueil is in very good agreement with previous CI estimates. This average, obtained with a "large" mass of samples, is analytically homogeneous and is suitable for normalization purposes. Finally, the Cu and Zn isotopic ratios are homogeneously distributed within the CI parent body with a spread of less than 100 ppm per atomic mass unit (amu). Published by Elsevier Ltd.

引用

页码：79 / 92

页数：14

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