Halogens in chondritic meteorites and terrestrial accretion

Patricia L. Clay (), Ray Burgess, Henner Busemann, Lorraine Ruzié-Hamilton, Bastian Joachim, James M. D. Day and Christopher J. Ballentine
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Patricia L. Clay: School of Earth and Environmental Sciences, University of Manchester
Ray Burgess: School of Earth and Environmental Sciences, University of Manchester
Henner Busemann: Institute for Geochemistry and Petrology, ETH Zürich, Clausiusstrasse 25
Lorraine Ruzié-Hamilton: School of Earth and Environmental Sciences, University of Manchester
Bastian Joachim: Institute for Mineralogy and Petrography, University of Innsbruck, Innrain 52
James M. D. Day: Scripps Institution of Oceanography, University of California San Diego
Christopher J. Ballentine: University of Oxford, South Parks Road

Nature, 2017, vol. 551, issue 7682, 614-618

Abstract: Halogen abundances in chondrites are 6 to 37 times lower than previously reported, which is consistent with the low abundances of these elements found in Earth.

Date: 2017
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DOI: 10.1038/nature24625

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