Abstract

Hydrogen defects can strongly affect mechanical and chemical properties of feldspars. To get insight into the behavior of such defects, alkali feldspar and plagioclase of igneous origin were studied combining IR spectroscopy with heating experiments under well-controlled conditions. Near-infrared spectra show that OH groups are the predominant hydrous species in these feldspars but presence of minor amounts of molecular H2O cannot be excluded. Short-term annealing at 400–800 °C produces a small but significant irreversible change in the OH stretching vibration band which is attributed to relaxation of the feldspar structure. Polarized mid-infrared spectra of sanidine, adularia, and plagioclase recorded in situ at temperatures up to 600 °C show reversible shifts of maxima toward higher wavenumber and an overall decrease in integrated intensities. The pleochroic features of the OH vibration bands, i.e., the predominant orientation of OH dipoles along the crystallographic a axis in all feldspars and the additional band component perpendicular to the (010) plane in sanidine are still present in the high-temperature spectra. Different behavior during long-term annealing at high temperature was found for the alkali feldspars and the plagioclases. At 900–1000 °C, the Eifel sanidines rapidly lost about one quarter of the initial water content which is attributed to a weakly bound hydrogen species in the feldspar structure. The remaining hydrogen is very strongly bound and was still detectable in 0.7–0.9 mm thick sections after annealing for 108 days at 1000 °C in air dried by phosphorus pentoxide. In contrast, a 1-mm-thick section of plagioclase completely lost hydrogen during heating in air within 8 days at 1000 °C. After partial dehydration, the pleochroic behavior of the OH absorption bands of the feldspars was basically preserved except that the 3050 cm−1 band of the sanidine, oriented perpendicular to (010), becomes more pronounced than the 3400 cm−1 band, oriented parallel to the a direction. Annealing experiments at 1000 °C under controlled water pressures indicate equilibrium solubilities of several tens of ppm H2O in the plagioclases and more than 100 ppm H2O in the alkali feldspars already at 1 bar water pressure. The variation of the water content with H2O pressure and spectroscopic observations indicates that the water content in the feldspars is determined not only by the water pressure but also by already existing defects. Vacancies on alkali sites (VA1) may accommodate H2O molecules, possibly with subsequent hydrolysis of network bonds to minimize local stress. A likely explanation for the strongly bound hydrogen in the sanidine is a coupled substitution of H+ + Al3+ for Si4+ (AlOH defect) where the protons are located on interstitial sites. This incorporation model is supported by the complete recovery of the defects in H2O vapor after previous proton/alkali exchange in alkali chloride vapor at 1000 °C.

Highlights

  • Feldspar is the most abundant mineral in the earth’s crust

  • A constant hydrogen level was detected at greater depth which is interpreted as the original water content of the feldspars

  • A basic finding of this study is that the water content of igneous feldspars is dependent on water pressure, and on the concentration of pre-existing defects in the feldspar

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Summary

Introduction

Feldspar is the most abundant mineral in the earth’s crust. Knowledge on its kinetic behavior can be helpful for understanding and modeling of rock formation and rock deformation. It is well established that intracrystalline processes in feldspar can be strongly enhanced by dissolved hydrogen species. Strong effects of water on deformation of feldspar minerals or aggregates are evident from several studies (see review of Kohlstedt 2006). Electrical conductivity in plagioclase is enhanced by hydrogen species, probably by contributions of protons to the charge transport (Yang et al 2012). Hydrogen contents in the nominally anhydrous mineral feldspar have found attraction as possible hygrometer for magmas in terrestrial volcanic rocks (Seaman et al 2006; Hamada et al 2011, 2013) and in lunar rocks (Hui et al 2013; Mills et al 2017)

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