• Mosselmans, J. Fred W.
• Ireland, Trevor R.
• Soldatov, Alexander V.
• Geraki, K.
• Schofield, Paul F.
• Kravtsova, Antonina N.
• Stephen, Natasha R.
• Walker, Andrew M.

Abstract

<p>The relationships between the composition of hibonite with the general formula CaAl_12-2x-yMg_xTi⁴⁺ _xTi³⁺ _yO₁₉, the oxidation state of Ti (Ti³⁺/ΣTi, where ΣTi = Ti³⁺ + Ti⁴⁺), and oxygen fugacity (fO₂) were investigated experimentally. It was found that hibonite can be synthesised with a range of Ti³⁺/ΣTi values at constant fO₂ and with a constant Ti³⁺/ΣTi value for a range of fO₂s. It was also found that if hibonite with the formula CaAl_12-yTi³⁺ _yO₁₉ (Ti³⁺/ΣTi = 1) is equilibrated with a melt of CAI composition at fO₂s below the iron-wüstite buffer then the resulting hibonite contained Mg, with Mg per formula unit (pfu) ~ 0.8 Ti pfu, and Ti³⁺/ΣTi ~ 0.2, irrespective of the fO₂. These results suggest that the availability of Mg, rather than fO₂, is the key factor that determines Ti³⁺/ΣTi of hibonite. The structures of synthetic samples of hibonite with the general formula CaAl_12-2xMg_xTi⁴⁺ _xO₁₉, where 0 ≤ X &lt; 1, were determined by Rietveld refinement of X-ray powder diffraction data. The predominant site occupied by Ti⁴⁺ was found to change from M2 to M4 with increasing Ti content. The range of Ti concentrations over which the site occupancy changed corresponds to that observed in meteoritic hibonite. This change in the Ti⁴⁺ site produces changes in the Ti K-edge XANES spectra, particularly in the intensity of the pre-edge feature, for constant Ti³⁺/ΣTi. The observed dependence of the pre-edge on the Ti⁴⁺ site was reproduced by ab initio simulations of the XANES spectra. The XANES spectra of natural hibonite with variable Ti content from the Murchison carbonaceous chondrite closely match the spectra of the synthetic samples with similar Ti contents. These differences in the spectra of meteoritic hibonite could be misinterpreted as being due to changes in Ti³⁺/ΣTi, but are instead due to differences in ΣTi, which relate to the petrogenetic history. Crystal chemistry exerts a first order control on the Ti site occupancy and Ti³⁺/ΣTi value of hibonite. As a result, no simple relationship between Ti³⁺/ΣTi and fO₂ should be expected. It is unlikely that hibonite will be useful as an oxybarometer for solar processes without Ti³⁺/ΣTi standards that are compositionally matched to the unknown.</p>

Topics

• impedance spectroscopy
• mineral
• simulation
• Oxygen
• melt
• iron