Chenmingite, FeCr2O4 in the CaFe2O4-type Structure, a Shock-induced, High-pressure Mineral in the Tissint Martian Meteorite
Document Type
Article
Publication Date
10-25-2019
Publication Title
American Mineralogist
Volume
104
Issue
10
First page number:
1521
Last page number:
1525
Abstract
Chenmingite (FeCr2O4; 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 (Fe0.752+Mg0.23Mn0.02) (Fe0.752+Mg0.23Mn0.02(Cr1.60Al0.29Fe0.063+Fe0.042+Ti0.02)ς2.01O4. (Cr1.60A l0.29Fe0.063+Fe 0.042+Ti0.02)Σ 2.01 O4. The general and end-member formulas are (Fe,Mg)(Cr,Al)2O4 and FeCr2O4. Synchrotron X-ray diffraction reveals that chenmingite has an orthorhombic Pnma CaFe2O4-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) Å3, 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.
Keywords
Chenmingite; FeCr2O4; High-pressure mineral; Shock-induced phase; Tissint martian meteorite; Shergottite
Disciplines
Astrophysics and Astronomy | Physical Processes | Physical Sciences and Mathematics
Language
English
Repository Citation
Ma, C.,
Tschauner, O.,
Beckett, J. R.,
Liu, Y.,
Greenberg, E.,
Prakapenka, V. B.
(2019).
Chenmingite, FeCr2O4 in the CaFe2O4-type Structure, a Shock-induced, High-pressure Mineral in the Tissint Martian Meteorite.
American Mineralogist, 104(10),
1521-1525.
http://dx.doi.org/10.2138/am-2019-6999