Published October 1, 2019 | Version Supplemental Material
Journal Article Open

Chenmingite, FeCr_2O_4 in the CaFe_2O_4-type structure, a shock-induced, high-pressure mineral in the Tissint martian meteorite

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon Jet Propulsion Lab
  • 3. ROR icon University of Chicago

Abstract

Chenmingite (FeCr_2O_4; IMA 2017-036) is a high-pressure mineral, occurring as micrometer- to submicrometer-sized lamellae within precursor chromite grains along with xieite and Fe,Cr-rich ulvöspinel next to shock-induced melt pockets, from the Tissint martian meteorite. The composition of type chenmingite by electron probe analysis shows an empirical formula of (Fe^(2+)_(0.75)Mg_(0.23)Mn_(0.02)) (Cr_(1.60)Al_(0.29)Fe^(3+)_(0.06)Fe^(2+)_(0.04)Ti_(0.02))_(Σ2.01)O_4. The general and end-member formulas are (Fe,Mg)(Cr,Al)_2O_4 and FeCr_2O_4. Synchrotron X-ray diffraction reveals that chenmingite has an orthorhombic Pnma café_2O_4-type (CF) structure with unit-cell dimensions: a = 9.715(6) Å, b = 2.87(1) Å, c = 9.49(7) Å, V = 264.6(4) Å^3, and Z = 4. Both chenmingite and xieite formed by solid-state transformation of precursor chromite under high pressure and high temperature during the Tissint impact event on Mars. The xieite regions are always in contact with melt pockets, whereas chenmingite lamellae only occur within chromite, a few micrometers away from the melt pockets. This arrangement suggests that chenmingite formed under similar pressures as xieite but at lower temperatures, in agreement with experimental studies.

Additional Information

© 2019 Mineralogical Society of America. Manuscript received February 14, 2019; Manuscript accepted July 6, 2019; Manuscript handled by Ian Swainson. We thank Ross Angel and four anonymous reviewers for their constructive reviews. SEM, EBSD, and EPMA analyses were carried out at the Caltech GPS Division Analytical Facility, which is supported, in part, by NSF Grants EAR-0318518 and DMR-0080065. O.T. acknowledges support by NSF EAR-1838330. GSECARS is supported through DOE Award DESC0005278, and NSF award EAR-1128799 and -0318518, DE-FG02-94ER14466, and DMR-0080065. The Advanced Photon Source, a DOE Office of Science User Facility is operated by Argonne National Laboratory under Contract No. DEAC02-06CH11357.

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Additional details

Additional titles

Alternative title
Chenmingite, FeCr2O4 in the CaFe2O4-type structure, a shock-induced, high-pressure mineral in the Tissint martian meteorite

Identifiers

Eprint ID
99060
Resolver ID
CaltechAUTHORS:20191003-141403801

Funding

NSF
EAR-0318518
NSF
DMR-0080065
NSF
EAR-1838330
Department of Energy (DOE)
DE-SC0005278
NSF
EAR-1128799
NSF
EAR-0318518
Department of Energy (DOE)
DE-FG02-94ER14466
NSF
DMR-0080065
Department of Energy (DOE)
DEAC02-06CH11357

Dates

Created
2019-10-03
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field