Metal–silicate silicon isotope fractionation in enstatite meteorites and constraints on Earth's core formation

2010 ◽  
Vol 295 (3-4) ◽  
pp. 487-496 ◽  
Author(s):  
Karen Ziegler ◽  
Edward D. Young ◽  
Edwin A. Schauble ◽  
John T. Wasson
2020 ◽  
Vol 117 (16) ◽  
pp. 8743-8749 ◽  
Author(s):  
Rebecca A. Fischer ◽  
Elizabeth Cottrell ◽  
Erik Hauri ◽  
Kanani K. M. Lee ◽  
Marion Le Voyer

Earth’s core is likely the largest reservoir of carbon (C) in the planet, but its C abundance has been poorly constrained because measurements of carbon’s preference for core versus mantle materials at the pressures and temperatures of core formation are lacking. Using metal–silicate partitioning experiments in a laser-heated diamond anvil cell, we show that carbon becomes significantly less siderophile as pressures and temperatures increase to those expected in a deep magma ocean during formation of Earth’s core. Based on a multistage model of core formation, the core likely contains a maximum of 0.09(4) to 0.20(10) wt% C, making carbon a negligible contributor to the core’s composition and density. However, this accounts for ∼80 to 90% of Earth’s overall carbon inventory, which totals 370(150) to 740(370) ppm. The bulk Earth’s carbon/sulfur ratio is best explained by the delivery of most of Earth’s volatiles from carbonaceous chondrite-like precursors.


2021 ◽  
Author(s):  
Carlos Pinilla ◽  
Aldemar De Moya ◽  
Guillaume Morard ◽  
Ségolène Rabin ◽  
Mathieu Roskosz ◽  
...  

2009 ◽  
Vol 288 (1-2) ◽  
pp. 228-234 ◽  
Author(s):  
Anat Shahar ◽  
Karen Ziegler ◽  
Edward D. Young ◽  
Angele Ricolleau ◽  
Edwin A. Schauble ◽  
...  

2021 ◽  
Vol 12 (1) ◽  
Author(s):  
Shoh Tagawa ◽  
Naoya Sakamoto ◽  
Kei Hirose ◽  
Shunpei Yokoo ◽  
John Hernlund ◽  
...  

AbstractHydrogen is one of the possible alloying elements in the Earth’s core, but its siderophile (iron-loving) nature is debated. Here we experimentally examined the partitioning of hydrogen between molten iron and silicate melt at 30–60 gigapascals and 3100–4600 kelvin. We find that hydrogen has a metal/silicate partition coefficient DH ≥ 29 and is therefore strongly siderophile at conditions of core formation. Unless water was delivered only in the final stage of accretion, core formation scenarios suggest that 0.3–0.6 wt% H was incorporated into the core, leaving a relatively small residual H2O concentration in silicates. This amount of H explains 30–60% of the density deficit and sound velocity excess of the outer core relative to pure iron. Our results also suggest that hydrogen may be an important constituent in the metallic cores of any terrestrial planet or moon having a mass in excess of ~10% of the Earth.


2021 ◽  
Vol 569 ◽  
pp. 117059
Author(s):  
Carlos Pinilla ◽  
Aldemar de Moya ◽  
Segolene Rabin ◽  
Guillaume Morard ◽  
Mathieu Roskosz ◽  
...  

Molecules ◽  
2019 ◽  
Vol 24 (7) ◽  
pp. 1415 ◽  
Author(s):  
Wang ◽  
Wei ◽  
Jiang ◽  
Liu ◽  
Lei ◽  
...  

The fundamental advances in silicon isotope geochemistry have been systematically demonstrated in this work. Firstly, the continuous modifications in analytical approaches and the silicon isotope variations in major reservoirs and geological processes have been briefly introduced. Secondly, the silicon isotope fractionation linked to silicon complexation/coordination and thermodynamic conditions have been extensively stressed, including silicate minerals with variable structures and chemical compositions, silica precipitation and diagenesis, chemical weathering of crustal surface silicate rocks, biological uptake, global oceanic Si cycle, etc. Finally, the relevant geological implications for meteorites and planetary core formation, ore deposits formation, hydrothermal fluids activities, and silicon cycling in hydrosphere have been summarized. Compared to the thermodynamic isotope fractionation of silicon associated with high-temperature processes, that in low-temperature geological processes is much more significant (e.g., chemical weathering, biogenic/non-biogenic precipitation, biological uptake, adsorption, etc.). The equilibrium silicon isotope fractionation during the mantle-core differentiation resulted in the observed heavy isotope composition of the bulk silicate Earth (BSE). The equilibrium fractionation of silicon isotopes among silicate minerals are sensitive to the Si–O bond length, Si coordination numbers (CN), the polymerization degrees of silicate unites, and the electronegativity of cations in minerals. The preferential enrichment of different speciation of dissoluble Si (DSi) (e.g., silicic acid H4SiO40 (H4) and H3SiO4− (H3)) in silica precipitation and diagenesis, and chemical weathering, lead to predominately positive Si isotope signatures in continental surface waters, in which the dynamic fractionation of silicon isotope could be well described by the Rayleigh fractionation model. The role of complexation in biological fractionations of silicon isotopes is more complicated, likely involving several enzymatic processes and active transport proteins. The integrated understanding greatly strengthens the potential of δ30Si proxy for reconstructing the paleo terrestrial and oceanic environments, and exploring the meteorites and planetary core formation, as well as constraining ore deposits and hydrothermal fluid activity.


Nature ◽  
2006 ◽  
Vol 444 (7115) ◽  
pp. E1-E1 ◽  
Author(s):  
Qing-zhu Yin ◽  
Stein B. Jacobsen

1993 ◽  
Vol 98 (B2) ◽  
pp. 2075-2089 ◽  
Author(s):  
Rie Honda ◽  
Hitoshi Mizutani ◽  
Tetsuo Yamamoto

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