Fluid–rock interactions in the shallow Mariana forearc: carbon cycling and redox conditions
Взаимодействие флюидов и горных пород в мелководной зоне преддуги Мариан: циркуляция углерода и редоксные условия
2019-06-24
SCID: 54.1/tjsmpcc3
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Mariana forearccarbonate vein precipitatesoxically precipitated aragonite and calciteslab-derived fluid temperatures (130–300 °C)subduction channel carbonates
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Abstract (AI)
Abstract. Few data exist that provide insight into processes affecting the long-term carbon cycle at shallow forearc depths. To better understand the mobilization of C in sediments and crust of the subducting slab, we investigated carbonate materials that originate from the subduction channel at the Mariana forearc (< 20 km) and were recovered during International Ocean Discovery Program Expedition 366. Calcium carbonates occur as vein precipitates within metavolcanic and metasedimentary clasts. The clasts represent portions of the subducting lithosphere, including ocean island basalt, that were altered at lower blueschist facies conditions and were subsequently transported to the forearc seafloor by serpentinite mud volcanism. Euhedral aragonite and calcite and the lack of deformation within the veins suggest carbonate formation in a stress-free environment after peak metamorphism affected their hosts. Intergrowth with barite and marked negative Ce anomalies in carbonate attest the precipitation within a generally oxic environment, that is an environment not controlled by serpentinization. Strontium and O isotopic compositions in carbonate (87Sr∕86Sr = 0.7052 to 0.7054, δ18OVSMOW = 20 to 24 ‰) imply precipitation from slab-derived fluids at temperatures between ∼130 and 300 ∘C. These temperature estimates are consistent with the presence of blueschist facies phases such as lawsonite coexisting with the carbonates in some veins. Incorporated C is inorganic (δ13CVPDB = −1 ‰ to +4 ‰) and likely derived from the decarbonation of calcareous sediment and/or oceanic crust. These findings provide evidence for the mobilization of C in the downgoing slab at depths of < 20 km. Our study shows for the first time in detail that a portion of this C forms carbonate precipitates in the subduction channel of an active convergent margin. This process may be an important asset in understanding the deep carbon cycle since it highlights that some C is lost from the subducting lithosphere before reaching greater depths.
Key Findings
1
A portion of slab-derived carbon precipitates as carbonate in the subduction channel before reaching greater depths, implying pre-subduction-lithosphere carbon loss affects the deep carbon cycle.
2
Calcium carbonates (aragonite and calcite) occur as stress-free vein precipitates within metavolcanic and metasedimentary clasts recovered from the Mariana forearc (<20 km).
3
Carbon incorporated in the veins is inorganic (δ13C VPDB = −1‰ to +4‰) and likely derived from decarbonation of calcareous sediment and/or oceanic crust, demonstrating carbon mobilization from the downgoing slab at <20 km depth.
4
Isotopic data (87Sr/86Sr = 0.7052–0.7054, δ18O VSMOW = 20–24‰) indicate carbonate precipitation from slab-derived fluids at ~130–300 °C.
5
Negative Ce anomalies and barite intergrowths indicate carbonate precipitation occurred in a generally oxic environment not controlled by serpentinization.
Research Object
Carbonate vein precipitates within metavolcanic and metasedimentary clasts from the shallow Mariana forearc subduction channel
Research Subject
Mobilization, precipitation conditions, and carbon sourcing/redox context of inorganic carbon in those carbonate veins (temperature, isotopic composition, Ce anomalies, oxic vs serpentinization-controlled environment) indicating C loss from the downgoing slab at <20 km depth
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2019-06-24
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