2020
DOI: 10.1038/s41586-020-2676-z
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The lithospheric-to-lower-mantle carbon cycle recorded in superdeep diamonds

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Cited by 32 publications
(23 citation statements)
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“…This is consistent with trace element patterns (Bulanova et al, 2010;Stachel, 2001;Stachel et al, 2005;Thomson et al, 2014;Walter et al, 2008) and heavy oxygen isotopic compositions exhibited by inclusions (Burnham et al, 2015;Ickert et al, 2013;Regier et al, 2020) that support derivation from altered oceanic crust. Indeed, such very heavy oxygen isotopic compositions (δ 18 O from +6‰ to +10‰) are at the extreme end of the seawater altered basalt compositional range and could be derived directly from carbonate melts released from altered oceanic crust (Regier et al, 2020). These sublithospheric diamonds are characterized by isotopically variable, typically light carbon with a composition (δ 13 C as low as −28.7‰) far below that of the average ambient mantle composition in δ 13 C of around −5‰ (Table 1; Bulanova et al, 2010;Palot et al, 2014Palot et al, , 2017Shirey et al, 2019;Walter et al, 2008Walter et al, , 2011.…”
Section: A Subducted Oceanic Slab Source For Sublithospheric Diamond-forming Fluidssupporting
confidence: 84%
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“…This is consistent with trace element patterns (Bulanova et al, 2010;Stachel, 2001;Stachel et al, 2005;Thomson et al, 2014;Walter et al, 2008) and heavy oxygen isotopic compositions exhibited by inclusions (Burnham et al, 2015;Ickert et al, 2013;Regier et al, 2020) that support derivation from altered oceanic crust. Indeed, such very heavy oxygen isotopic compositions (δ 18 O from +6‰ to +10‰) are at the extreme end of the seawater altered basalt compositional range and could be derived directly from carbonate melts released from altered oceanic crust (Regier et al, 2020). These sublithospheric diamonds are characterized by isotopically variable, typically light carbon with a composition (δ 13 C as low as −28.7‰) far below that of the average ambient mantle composition in δ 13 C of around −5‰ (Table 1; Bulanova et al, 2010;Palot et al, 2014Palot et al, , 2017Shirey et al, 2019;Walter et al, 2008Walter et al, , 2011.…”
Section: A Subducted Oceanic Slab Source For Sublithospheric Diamond-forming Fluidssupporting
confidence: 84%
“…Rather, in this examination of the role of carbonate, we are only considering the role of cooler slabs and carbonate in the deeper, altered igneous oceanic crust (Li et al, 2019), especially since it is only the cooler slabs that produce deep seismicity regardless of mechanism (Figures 5a, 6a, and 6b). This association with oceanic crust is cemented further by oxygen isotope measurements on majorite inclusions in sublithospheric diamonds (Burnham et al, 2015;Ickert et al, 2013;Regier et al, 2020). Just as with water in altered peridotite, carbonate in the deeper igneous oceanic crust of hot slabs will be removed shallower than 300 km depths (Figure 5b; e.g., Kerrick & Connolly, 2001), especially if water is infiltrating from cooler, deeper crustal levels (e.g., Gorman et al, 2006;Martin & Hermann, 2018).…”
Section: Correlation Between Carbonate Melting Deep Earthquakes and Deep Diamondsmentioning
confidence: 90%
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“…Carbon-bearing species were assumed to dissolve in a specific order, starting with the leaching of organic carbon and followed by the dissolution of carbonate minerals (see Supplementary Data 2). This assumption is supported by (1) the organic C-rich nature of subduction zone fluids 70 , and the isotopic signature of asthenospheric to transition zone diamonds that is consistent with carbonated igneous oceanic crust, rather than sediments rich in organic carbon, being the dominant source of their carbon 4,71 . Even if some of the organic carbon does not dissolve and eventually graphitizes as the slab experiences higher pressures and temperatures with depth, the available water will dissolve calcite/aragonite instead.…”
Section: Methodsmentioning
confidence: 93%