Geochemistry. William M. White

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with an activity of aqueous Fe2+ of 10−6. For any other activity, the line will be shifted, as illustrated in Figure 3.20. For higher concentrations, the magnetite region will expand, while for lower concentrations it will contract.

Graph depicts the stability regions for magnetite and hematite in equilibrium with an iron-bearing aqueous solution. Thick lines represents a Feaq activity of ten to six, finer lines represents the activities of 10-4 and ten to eight. The latter is dashed.

      Now consider the equilibrium between hematite and Fe2+. We can describe this with the reaction:

equation

      The equilibrium constant (which may again be calculated from ΔGr) for this reaction is 23.79.

      Expressed in log form:

equation

      Using an activity of 1 for Fe2+, we can solve for as:

equation

      For an activity of Fe2+ of 10−6, this is a line with a slope of 3 and an intercept of 17.9. This line represents the conditions under which hematite is in equilibrium with images = 10−6. Again, for any other activity, the line will be shifted as shown in Figure 3.20.

      Finally, equilibrium between hematite and Fe3+ may be expressed as:

equation

      The equilibrium constant expression is:

equation

      For a Fe3+ activity of 10–6, this reduces to:

equation

      Since the reaction does not involve transfer of electrons, this boundary depends only on pH.

      The boundary between predominance of Fe3+ and Fe2+ is independent of the Fe concentration in solution and is the same as eqn. 3.119 and Figure 3.18, namely = 13.

      Examining this diagram, we see that for realistic dissolved Fe concentrations, magnetite can be in equilibrium only with a fairly reduced, neutral to alkaline solution. At pH of about 7 or less, it dissolves and would not be stable in equilibrium with acidic waters unless the Fe concentration were very high. Hematite is stable over a larger range of conditions and becomes stable over a wider range of pH as pε increases. Significant concentrations of the Fe3+ ion (>10−6 m) will be found only in very acidic, oxidizing environments.

Graph depicts the pε and pH of various waters on and near the surface of the Earth.

      Balancing redox reactions for pε–pH diagrams

equation

      The next step is to balance the oxygen. We don't want to use O2 gas to do this. We used O2 at a partial pressure of 1 to define the top boundary for the water stability region. Within the region of stability of water, the O2 concentration will be lower and we don't necessarily know its value. This is usually best done using water:

equation

      Next balance the hydrogen using H+:

equation

      Finally, we use electrons to balance charge:

equation

      As a check, we can consider the valance change of our principal species and be sure that our reaction makes sense. In ammonium, nitrogen is in the 3− state, while in nitrate it is in the 5+ state, a net change of 8. This is just the number of electrons exchanged in the reaction we have written.

      3.11.2 Redox in magmatic systems

      High-temperature geochemists use oxygen fugacity to characterize the oxidation state of systems. Consequently, we want to write redox reactions that contain O2. Thus, equilibrium between magnetite and hematite would be written as:

      (or alternatively, as we wrote in eqn. 3.101) rather than the way we expressed it in eqn. 3.120. We note, however, there is negligible molecular oxygen in magmatic systems, and other species are often responsible for transfer of electrons and O2–. For example, the equilibrium between magnetite and hematite may be mediated by water:

      (3.123)equation

      The

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