Abstract

Solid-earth processes act as both sources and sinks for atmospheric O<sub>2</sub>. They act as sinks by introducing reduced minerals and gases to the earth9s surface that can remove O<sub>2</sub> from the atmosphere and ocean. They act as sources by exporting organic carbon and sedimentary pyrite to the mantle via subduction. Here we examine the relative sizes of igneous source and sinks of O<sub>2</sub> for the modern earth to determine their magnitudes and if they are in balance today. We find that igneous sinks for O<sub>2</sub> remove 1.83×10<sup>12</sup> mol O<sub>2</sub>/yr (±0.43, 1σ) while subduction indirectly releases 1.56×10<sup>12</sup> mol/O<sub>2</sub> yr (±0.33, 1σ). This indicates that today igneous O<sub>2</sub> sinks are balanced by solid earth sources. We propose this balance is achieved by negative feedbacks associated with either low-temperature hydrothermal sinks for O<sub>2</sub>, which are sensitive to deep-ocean O<sub>2</sub> concentrations, or the amount of organic carbon and pyrite buried in sediments and subducted, which are sensitive to dissolved O<sub>2</sub> concentrations. We also explore how igneous sinks for O<sub>2</sub> may have varied in the Neoproterozoic when atmospheric O<sub>2</sub> concentrations are thought to have been lower and the deep ocean anoxic. We find that despite these changes, the igneous O<sub>2</sub> sink was essentially the same as today: 1.78×10<sup>12</sup> (±0.43, 1σ) mol O<sub>2</sub>/yr. We explore how this sink would change as the deep ocean accumulated sulfate, became oxygenated, and began oxidizing oceanic crust such that there was an increase in the subduction flux of oxidants to the subarc mantle. We propose that significant changes to the O<sub>2</sub> cycle, both in terms of positive and negative feedbacks could occur during these transitions. For example, accumulation of sulfate in the deep ocean would increase the oxidation state of high-temperature hydrothermal fluids, decreasing the size of this O<sub>2</sub> sink and thus promoting an increase in atmospheric O<sub>2</sub>. In contrast, the oxygenation of the deep ocean would have allowed hydrothermally derived H<sub>2</sub>S to react with and consume O<sub>2</sub> instead of being titrated out via reactions with dissolved Fe<sup>2+</sup>. Additionally, deep-ocean oxygenation would have initiated the oxidation of oceanic crust at low temperatures, creating new sinks for O<sub>2</sub>. Finally, the oxidation of the subarc mantle via subduction of newly oxidized sediments and altered oceanic crust would have increased the oxygen fugacity of arc volcanic gases, decreasing their overall demand for O<sub>2</sub>, allowing yet more O<sub>2</sub> to accumulate in the atmosphere. We place these changes into a conceptual framework and discuss their potential impact on the history of atmospheric and marine O<sub>2</sub> concentrations from the Neoproterozoic to late Paleozoic.

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