The limitations of hibonite as a single-mineral oxybarometer for early solar system processes

作者：Berry Andrew J^*; Schofield Paul F; Kravtsova Antonina N; Miller Laura A; Stephen Natasha R; Walker Andrew M; Soldatov Alexander V; Ireland Trevor R; Geraki K; Mosselmans J Fred W

来源：Chemical Geology, 2017, 466: 32-40.

DOI：10.1016/j.chemgeo.2017.03.031

• Hibonite
• Calcium hexaluminate
• CA6
• CAI
• Oxybarometry
• Solar nebula
• Crystal chemistry
• Oxygen fugacity
• XANES
• FDMNES

The relationships between the composition of hibonite with the general formula CaAl12-2x-yMgxTix4+Tiy3+O19, the oxidation state of Ti (Ti3+/Sigma Ti, where STi = Ti3+ + Ti4+), and oxygen fugacity (fO(2)) were investigated experimentally. It was found that hibonite can be synthesised with a range of Ti3+/Sigma Ti values at constant fO(2) and with a constant Ti3+/Sigma Ti value for a range of fO(2)s. It was also found that if hibonite with the formula CaAl12-yTiy3+O19 (Ti3+/Sigma Ti = 1) is equilibrated with a melt of CAI composition at fO(2)s below the iron-wustite buffer then the resulting hibonite contained Mg, with Mg per formula unit (pfu) similar to 0.8 Ti pfu, and Ti3+/Sigma Ti similar to 0.2, irrespective of the fO(2). These results suggest that the availability of Mg, rather than fO(2), is the key factor that determines Ti3+/Sigma Ti of hibonite. The structures of synthetic samples of hibonite with the general formula CaAl12-2x-yMgxTix4+Tiy3+O19, where 0 <= X < 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+/Sigma Ti. 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+/Sigma Ti, but are instead due to differences in STi, which relate to the petrogenetic history. Crystal chemistry exerts a first order control on the Ti site occupancy and Ti3+/Sigma Ti value of hibonite. As a result, no simple relationship between Ti3+/Sigma Ti and fO(2) should be expected. It is unlikely that hibonite will be useful as an oxybarometer for solar processes without Ti3+/Sigma Ti standards that are compositionally matched to the unknown.

• 出版日期2017-9-5