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Published November 15, 2015 | public
Journal Article

Spinel–olivine–pyroxene equilibrium iron isotopic fractionation and applications to natural peridotites

Abstract

Eight spinel-group minerals were synthesized by a flux-growth method producing spinels with varying composition and Fe^(3+)/Fe_(tot) ratios. The mean force constants of iron bonds in these minerals were determined by synchrotron nuclear resonant inelastic X-ray scattering (NRIXS) in order to determine the reduced isotopic partition function ratios (β-factors) of these spinels. The mean force constants are strongly dependent on the Fe^(3+)/Fe_(tot) of the spinel but are independent, or weakly dependent on other structural and compositional parameters. From our spectroscopic data, it is found that a single redox-dependent calibration line accounts for the effects of Fe^(3+)/Fe_(tot) on the β-factors of spinels. This calibration successfully describes the equilibrium Fe isotopes fractionation factors between spinels and silicates (olivine and pyroxenes). Our predictions are in excellent agreement with independent determinations for the equilibrium Fe isotopic fractionations for the magnetite–fayalite and the magnetite–hedenbergite couples. Our calibration applies to the entire range of Fe^(3+)/Fe_(tot) ratios found in natural spinels and provides a basis for interpreting iron isotopic variations documented in mantle peridotites. Except for a few exceptions, most of the samples measured so far are in isotopic disequilibrium, reflecting metasomatism and partial melting processes.

Additional Information

© 2015 Elsevier Ltd. Received 5 December 2014, Accepted 27 July 2015, Available online 12 August 2015. We thank Ian Steele (University of Chicago) for assistance in performing the electron probe analyses and Séverine Bellayer (UMET, ENSCL, Université Lille 1) for additional electron microprobe analysis. Jonathan Giencke (Bruker AXS) performed the XRD analysis. We thank Dr. X.M. Zhao for sharing her data on the peridotites from Yangyuan, North China Craton with us. The thoughtful reviews of three anonymous reviewers and the handling by S. Weyer deeply improved the quality of this work. Use of the Advanced Photon Source, an Office of Science User Facility operated for the U.S. Department of Energy (DOE) Office of Science by Argonne National Laboratory, was supported by the U.S. DOE under Contract No. DE-AC02-06CH11357. This work was supported by an ANR grant (2011JS56 004 01; FrIHIDDA) to MR; grants from NSF Petrology and Geochemistry (EAR1144429), NASA Cosmochemistry (NNX12AH60G), LARS (NNX14AK09G) and FACCTS programs to ND; a Chateaubriand Fellowship to CKS.

Additional details

Created:
August 22, 2023
Modified:
October 18, 2023