Published November 2017 | Version v1
Journal article

Temperature-induced iron oxidation in bafertisite Ba2Fe42+Ti2(Si2O7)2O2(OH)2F2: X-ray diffraction and Mössbauer spectroscopy study

  • 1. St. Petersburg State University, University Emb. 7/9, Institute of Earth Sciences (Russian Federation)
  • 2. Russian Academy of Sciences, Vinogradov Institute of Geochemistry, Siberian Branch (Russian Federation)
  • 3. St. Petersburg State University, Universitetskaya nab. 7/9, Resource Center (Russian Federation)

Description

The high-temperature behavior of bafertisite was studied by combination of techniques in order to characterize the temperature-induced iron oxidation associated with deprotonation of an octahedral layer. The chemical formula of bafertisite from Darai-Pioz alkaline complex (Tajikistan) determined by electron-microprobe analyzes and Mössbauer spectroscopy is Ba 2.11(Fe2.702+Fe0.173+Mn 1.09Zr 0.04Na 0.03) (Ti 1.96Nb 0.07)(Si 2O7)2O2(OH 1.29 O 0.65F0.06)F2. In situ high-temperature powder X-ray diffraction revealed abrupt shift of reflections to the high-angle region and reduction of their intensity at T > 525 C. The Mössbauer spectroscopy studies indicated that the crystal structure of bafertisite contains Fe in octahedral sites as predominantly ferric ions with Fe 3+/ ΣFe = 0.06, whereas bafertisite annealed at T = 600 C has Fe in the same position with Fe 3+/ ΣFe up to 0.39. The differential scanning calorimetry and thermogravimetric analyzes reveal the occurrence of a broad exothermic effect at T ∼ 537 C associated with the mass loss corresponding to deprotonation. Since in the studied sample of bafertisite, Fe 2+apfu strongly prevails over OH apfu, the stoichiometric (charged-balanced) high-temperature oxidized modification cannot be obtained. In the paper, the high-temperature behavior of bafertisite is discussed and compared to that of astrophyllite.

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Publishing Information

Journal Title
Hyperfine Interactions
Journal Volume
238
Journal Issue
1
Journal Page Range
p. 1-12
ISSN
0304-3843
CODEN
HYINDN

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