Abstract

AbstractThe occurrence of the quartz‐carbonate alteration assemblage (listvenite) in ophiolites indicates that ultramafic rock represents an effective sink for dissolved CO2. However, the majority of earlier studies of ultramafic rock carbonation had to rely on the surface exposure of reaction textures and field relationships. Here we present the first observations on ultramafic rock alteration obtained from the 300 m deep BT1B drill hole, ICDP Oman Drilling Project, allowing for a continuous and high‐resolution investigation. Hole BT1B recovered continuous drill core intersecting surface alluvium, 200 m of altered ultramafic rock comprising mainly listvenite and minor serpentinite bands at 90 and 180 m depth, and 100 m of the underlying metamorphic sole. Textural evidence suggests that the carbonation of fully serpentinized harzburgite commenced by non‐equilibrium growth of spheroidal carbonate characterized by sectorial zoning resulting from radially oriented low‐angle boundaries. In the serpentinite, carbonate spheroids are composed of alternating magnesite cores and dolomite rims, whereas texturally similar carbonate in the listvenite is composed of Fe‐rich magnesite cores and Ca‐Fe‐rich magnesite rims. The distinct compositions and mineral inclusions indicate that the carbonation extent was controlled by fluid accessibility resulting in the simultaneous formation of limited carbonate in the serpentinite bands and complete carbonation in the listvenite parts of BT1B. The presence of euhedral magnesite overgrowing spheroidal carbonate in the listvenite suggests near‐equilibrium conditions during the final stage of carbonation. The carbonate clumped isotope thermometry constrains carbonate crystallization between 50 °C and 250 °C, implying repeated infiltration of reactive fluids during ophiolite uplift and cooling.

Highlights

  • Alteration of the oceanic lithosphere by hydrothermal fluids is the primary driver of the hydrosphere–lithosphere volatile exchange and has significant consequences for rock physical properties and planetary-scale element fluxes

  • We present the first observations on ultramafic rock alteration obtained from the 300 m deep BT1B drill hole, International Continental Scientific Drilling Project (ICDP) Oman Drilling Project, allowing for a continuous and high-resolution investigation

  • Altered ultramafic rocks consisting of the magnesite–quartz assemblage are termed listvenite and represent the end-product of CO2-fluid driven mafic and ultramafic rock alteration as almost the entire inventory of Mg and Ca cations is incorporated into carbonate minerals (Halls & Zhao, 1995)

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Summary

Introduction

Alteration of the oceanic lithosphere by hydrothermal fluids is the primary driver of the hydrosphere–lithosphere volatile exchange and has significant consequences for rock physical properties and planetary-scale element fluxes. More recently investigated listvenite from Wadi Mansah is characterized by magnesite as the dominant carbonate mineral consistent with peridotite alteration predominately driven by influx of CO2 (Falk & Kelemen, 2015). In addition to the carbonated ultramafic basal section, the Samail ophiolite comprises a complete sequence of oceanic lithosphere from the upper mantle through to the continental crust all of which have recently been subject to comprehensive drilling and subsequent analysis of rock core, logging, hydrological and microbial sampling in the course of the Oman Drilling Project (OmanDP, ICDP Exp. 5057) (Kelemen et al, 2020; Kelemen et al, 2014). To better constrain the conditions and reaction pathways driving complete peridotite carbonation at large scale, here we present the first results of microstructural investigation and carbonate clumped isotope thermometry on samples recovered from Hole BT1B of the OmanDP. Reaction textures are assessed across scales ranging from hand specimen to the nanoscale constraining critical reaction parameters and chemical equilibration during natural, large-scale ultramafic rock carbonation

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