In [#1], the authors state in the abstract
The conventional view holds that the oxidation state of a mantle-derived degassed magma reflects its source
From other research that has been conducted, the authors discussed that the oxygen fugacity (the partial pressure of the "non-ideal" oxygen in the presence of the high pressures and temperatures, presumably of the magma itself) was controlled by a pair of redox reactions (their equations 11 and 12):
$$\ce{S_{(melt)}^2- + Fe2^3+O3_{(melt)} <=> SO2_{(gas)} + 6Fe^2+O_{(melt)} + O_{(melt)}^2-}$$ $$\ce{SO4_{(melt)}^2- + 2Fe^2+O_{(melt)} <=> SO2_{(gas)} + Fe2^3+O3_{(melt)} + O_{(melt)}^2-}$$
Their claim is that the change in the $\ce{Fe^3+}$ to $\ce{Fe^2+}$ ratio is due to the top reaction being favored during decompression (due to the equilibrium shift from the changes in pressure).
I get all of that so far, I think. My question is a more fundamental one, being, if this equilibrium (#11) governing the changes in oxidation states becomes more prevalent as the pressure decreases rapidly, what are the governing equations for when the magma is deeper in the earth? Do they favor the bottom equation (#12) instead, or are the reactions at that temperature and pressure completely different?
It's possible I'm missing what the "changing oxidation states" aspect really means. A clarification of that would certainly be appreciated.
Reference:
- Moussallam, Y., Oppenheimer, C., Scaillet, B., Gaillard, F., Kyle, P., Peters, N., & Donovan, A. (2014). Tracking the changing oxidation state of Erebus magmas, from mantle to surface, driven by magma ascent and degassing. Earth and Planetary Science Letters, 393, 200-209. [DOI]