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4697288 
Journal Article 
Distinct U-238/U-235 ratios and REE patterns in plutonic and volcanic angrites: Geochronologic implications and evidence for U isotope fractionation during magmatic processes 
Tissot, FLH; Dauphas, N; Grove, TL 
2017 
Yes 
Geochimica et Cosmochimica Acta
ISSN: 0016-7037 
213 
593-617 
WOS:000407259200033 
Angrites are differentiated meteorites that formed between 4 and 11 Myr after Solar System formation, when several short-lived nuclides (e.g., Al-26-Mg-26, Mn-53-Cr-53,Hf-182-W-182) were still alive. As such, angrites are prime anchors to tie the relative chronology inferred from these short-lived radionuclides to the absolute Pb-Pb clock. The discovery of variable U isotopic composition (at the sub-permil level) calls for a revision of Pb-Pb ages calculated using an "assumed" constant U-238/U-235 ratio (i.e., Pb-Pb ages published before 2009-2010). In this paper, we report high-precision U isotope measurement for six angrite samples (NWA 4590, NWA 4801, NWA 6291, Angra dos Reis, D'Orbigny, and Sahara 99555) using multi-collector inductively coupled plasma mass-spectrometry and the IRMM-3636 U double-spike. The age corrections range from -0.17 to -1.20 Myr depending on the samples. After correction, concordance between the revised Pb-Pb and Hf-W and MnCr ages of plutonic and quenched angrites is good, and the initial (Mn-53/Mn-55)(0) ratio in the Early Solar System (ESS) is recalculated as being (7 +/- 1) x 10(-6) at the formation of the Solar System (the error bar incorporates uncertainty in the absolute age of Calcium, Aluminum-rich inclusions - CAIs). An uncertainty remains as to whether the Al-Mg and Pb-Pb systems agree in large part due to uncertainties in the Pb-Pb age of CAIs.



A systematic difference is found in the U isotopic compositions of quenched and plutonic angrites of + 0.17%. A difference is also found between the rare earth element (REE) patterns of these two angrite subgroups. The delta U-238 values are consistent with fractionation during magmatic evolution of the angrite parent melt. Stable U isotope fractionation due to a change in the coordination environment of U during incorporation into pyroxene could be responsible for such a fractionation. In this context, Pb-Pb ages derived from pyroxenes fraction should be corrected using the U isotope composition measured in the same pyroxene fraction. (C) 2017 Elsevier Ltd. All rights reserved. 
Angrites; U stable isotopes; Pb-Pb ages; Short-lived chronometers; U stable isotope fractionation