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

JA Barrat, B Zanda, F Moynier, C Bollinger…�- …�et Cosmochimica Acta, 2012 - Elsevier
JA Barrat, B Zanda, F Moynier, C Bollinger, C Liorzou, G Bayon
Geochimica et Cosmochimica Acta, 2012Elsevier
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�…
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 1.2g) 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 100ppm per atomic mass unit (amu).
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