Abstract

Molecular hydrogen (H2) released during serpentinization of mantle rocks is one of the main fuels for chemosynthetic life. Processes of H2 production at slow-spreading mid-ocean ridges (MORs) have received much attention in the past. Less well understood is serpentinization at passive continental margins where different rock types are involved (lherzolite instead of harzburgite/dunite at MORs) and the alteration temperatures tend to be lower (<200°C vs. >200°C). To help closing this knowledge gap we investigated drill core samples from the West Iberia margin. Lherzolitic compositions and spinel geochemistry indicate that the exhumed peridotites resemble sub-continental lithospheric mantle. The rocks are strongly serpentinized, mainly consist of serpentine with little magnetite, and are generally brucite-free. Serpentine can be uncommonly Fe-rich, with XMg = Mg/(Mg + Fe) < 0.8, and shows distinct compositional trends toward a cronstedtite endmember. Bulk rock and silicate fraction Fe(III)/∑Fe ratios are 0.6–0.92 and 0.58–0.8, respectively; our data show that 2/3 of the ferric Fe is accounted for by Fe(III)-serpentine. Mass balance and thermodynamic calculations suggest that the sample’s initial serpentinization produced ∼120 to >300 mmol H2 per kg rock. The cold, late-stage weathering of the serpentinites at the seafloor caused additional H2 formation. These results suggest that the H2 generation potential evolves during the transition from continental break-up to ultraslow and, eventually, slow MOR spreading. Metamorphic phase assemblages systematically vary between these settings, which has consequences for H2 yields during serpentinization. At magma-poor rifted margins and ultraslow-spreading MORs, serpentine hosts most Fe(III). Hydrogen yields of 120 to >300 mmol and 50–150 mmol H2 per kg rock, respectively, may be expected at temperatures of <200°C. At slow-spreading MORs, in contrast, serpentinization may produce 200–350 mmol H2, most of which is related to magnetite formation at >200°C. Since, in comparison to slow-spreading MORs, geothermal gradients at magma-poor margins and ultraslow-spreading MORs are lower, larger volumes of low-temperature serpentinite should form in these settings. Serpentinization of lherzolitic rocks at magma-poor margins should produce particularly high amounts of H2 under conditions within the habitable zone. Magma-poor margins may hence be more relevant environments for hydrogenotrophic microbial life than previously thought.

Highlights

  • Serpentinites in the oceanic lithosphere form when mantle peridotite interacts with seawater at temperatures below ∼450°C

  • We applied thermodynamic calculations to track the amounts of H2 that are being produced during serpentinization at magmapoor margins such as the West Iberia margin

  • Hydrogen yields during seawater–peridotite interactions primarily rely on the serpentinization mineral assemblages, which in turn strongly depend on protolith type and alteration temperature

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Summary

Introduction

Serpentinites in the oceanic lithosphere form when mantle peridotite interacts with seawater at temperatures below ∼450°C. Magnetite is most abundant at temperatures of 200–350°C, causing the production of >300 mmol H2 per kg of dunite or harzburgite at these temperatures, but its abundance decreases toward lower temperatures at which Fe is progressively incorporated into Fe-rich brucite (Bach et al, 2006; Klein et al, 2009) At such lower temperatures, Fe(III)-serpentine is the main host for ferric Fe and the total amounts of H2 produced are thought to be much lower (below ∼100 mmol per kg of rock; Klein et al, 2009; Andreani et al, 2013)

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