Phase equilibria and liquid lines of descent in alkali basalts at one atmosphere and the role of oxygen fugacity
摘要
This study presents new experimental data on the effect of oxygen fugacity (fO2) and bulk composition on phase equilibria and liquid lines of descent in alkali basalts. Crystallisation experiments were performed at one atmosphere, in the temperature range 1220–1050 °C and at fO2 conditions corresponding to fayalite–magnetite–quartz (FMQ) equilibrium and the following log-unit deviations from this equilibrium: FMQ-1, FMQ + 1.5 and FMQ + 3. Experiments were grouped into two series, those on primitive compositions (9.9–11.9 wt% MgO; total alkali 3.1–5.3 wt%), and those on evolved compositions (5.1–5.8 wt% MgO; total alkali 5.7–8.6 wt%). Experiments on primitive compositions produce assemblages of olivine, clinopyroxene and spinel, with plagioclase present in less silica-undersaturated compositions. Experiments on evolved compositions produce similar assemblages, though olivine is often absent at higher fO2. Whitlockite is present at low temperature, plus occasional Fe-Ti oxides. Nepheline is only observed in the most silica-undersaturated composition at low temperature. Mineral compositions and stability are strongly controlled by bulk composition and redox conditions. High MgO bulk contents favour the early appearance of olivine, while the appearance of clinopyroxene is dictated by both MgO and CaO contents. Increasing silica-undersaturation produces assemblages dominated by clinopyroxene and a high melt fraction at any given temperature, promoting alkali enrichment during melt evolution. Oxidising conditions enhance the crystallisation of spinel and other Fe-Ti oxides, in which both silica and alkalis are incompatible, through increased melt Fe3+/ΣFe. This promotes more modest enrichments in Na2O and K2O with respect to SiO2 as crystallisation proceeds, with the effect strongest where bulk concentrations of FeOtot are high and P2O5 are low. It follows that fO2 exerts a stronger control over the liquid lines of descent of more primitive liquids than evolved ones. We combine our results with those from the literature to calibrate new models for both