The high-pressure, vacancy-stabilized component in clinopyroxenes
Abstract
Motivated by the recent discovery of albitic clinopyroxene, we assess the molar volume systematics of vacancy-stabilized, high-pressure clinopyroxenes. Previous assessments used the Ca-Eskola component M2(Ca0.5□0.5) M1AlTSi2O6 (where □ denotes a vacancy) as an end-member and were limited to compositions with ≤50% vacancies in the M2 site. The discovery of albitic jadeite calls for extension of the solid solution space toward an end-member with entirely vacant M2 sites, M2□M1SiTSi2O6, i.e., silica in the C2/c pyroxene structure. Based on our new and compiled data, we fit a model for volumes of clinopyroxenes in an 11-component subsystem. We tested two different scenarios: ideal mixing and symmetric excess volumes. Ideal mixing is easily rejected, as the correlation between vacancy concentration and volume at standard conditions is clearly nonlinear. The symmetric excess volume model, however, yields an adequate fit to the data when using three excess terms (Hd-En, Hd-Di, and Hd-Jd). The estimated molar volume of the clinopyroxene-structured silica end-member, which has one octahedrally coordinated silicon atom per formula unit, is 60.77 ± 0.75 cm3/mol on a six-oxygen formula basis, slightly smaller than that of coesite (61.73 cm3/mol) but much larger than that of stishovite (41.44 cm3/mol). We also obtained a molar volume of 62.16 ± 0.75 cm3/mol for the Ca-Eskola component, modestly larger than earlier estimates extrapolated with an ideal mixing assumption from natural samples (60.52 ± 0.73 cm3/mol) or experiments (60.87 ± 0.63 cm3/mol). The proposed volume model provides a partial basis for assessing the formation conditions of vacancy-stabilized pyroxenes.
Copyright and License
© 2025 by the Mineralogical Society of America.
Acknowledgement
Synchrotron X-ray diffraction data were collected at HPCAT (Sector 16), Advanced Photon Source (APS), Argonne National Laboratory. HPCAT operations are supported by DOE-NNSA’s Office of Experimental Sciences. The Advanced Photon Source is a U.S. Department of Energy (DOE) Office of Science User Facility operated for the DOE Office of Science by Argonne National Laboratory under Contract No. DE-AC02-06CH11357. We thank two anonymous reviewers for their helpful review comments. We gratefully recognize the efforts of the associate editor, Antonio dos Santos, for his editorial handling.
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Additional details
- United States Department of Energy
- DE-AC02-06CH11357
- Accepted
-
2025-01-29
- Available
-
2025-02-04First online
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)
- Publication Status
- Published