The behavior of C, H, and S in the solid Earth depends on their oxidation states, which are related to oxygen fugacity (fO 2 ). Volcanic degassing is a source of these elements to Earth's surface; therefore, variations in mantle fO 2 may influence the fO 2 at Earth's surface. However, degassing can impact magmatic fO 2 before or during eruption, potentially obscuring relationships between the fO 2 of the solid Earth and of emitted gases and their impact on surface fO 2 . We show that low-pressure degassing resulted in reduction of the fO 2 of Mauna Kea magmas by more than an order of magnitude. The least degassed magmas from Mauna Kea are more oxidized than midocean ridge basalt (MORB) magmas, suggesting that the upper mantle sources of Hawaiian magmas have higher fO 2 than MORB sources. One explanation for this difference is recycling of material from the oxidized surface to the deep mantle, which is then returned to the surface as a component of buoyant plumes. It has been proposed that a decreasing pressure of volcanic eruptions led to the oxygenation of the atmosphere. Extension of our findings via modeling of degassing trends suggests that a decrease in eruption pressure would not produce this effect. If degassing of basalts were responsible for the rise in oxygen, it requires that Archean magmas had at least two orders of magnitude lower fO 2 than modern magmas. Estimates of fO 2 of Archean magmas are not this low, arguing for alternative explanations for the oxygenation of the atmosphere. /ΣS, oxygen fugacity (fO 2 ), and melt composition (8, 9) and on recent observations that Fe 3+ /ΣFe of subduction-related magmas are only weakly dependent on factors such as crystal−liquid fractionation and degassing (7, 10, 11), the higher Fe 3+ /ΣFe ratios of arc and back-arc basalts relative to MORBs have been attributed by most authors to elevated fO 2 in their mantle sources resulting from addition of oxidized hydrous fluids or silicate melts from subducted slabs (7,11,12). Ocean island basalts (OIBs) are more variable in fO 2 , with Fe 3+ /ΣFe and S 6+ /ΣS ratios that range from lower than to higher than MORBs (4, 13-17), but it is unclear whether these differences relate to variable amounts of ancient, more oxidized subducted material in the mantle sources of OIB (e.g., ref. 18) or to other factors related to differences in the petrogenesis of OIB and MORB magmas [e.g., temperature and pressure of melting (15) /ΣS ratios could change during magmatic differentiation, and these could contribute to the observed variability in fO 2 among basalts erupted at Earth's surface. One possibility is crystal−liquid fractionation: In a system closed to oxygen, olivine and pyroxene crystallization would result in an increase in the Fe 3+ /ΣFe of residual liquids; alternatively, spinel crystallization could decrease this ratio in residual liquids. Degassing is another possibility: Degassing and loss of H 2 can lead to oxidation of residual liquids (19). Likewise, although CO 3 2− species are thought to be the dominant forms of d...