The Earth's Core Formation Process

2019 ◽  
pp. 41-101
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

Icarus ◽  
1987 ◽  
Vol 69 (2) ◽  
pp. 239-248 ◽  
Author(s):  
Shigeru Ida ◽  
Yoshitsugu Nakagawa ◽  
Kiyoshi Nakazawa

2017 ◽  
Vol 461 ◽  
pp. 128-139 ◽  
Author(s):  
M.A. Bouhifd ◽  
V. Clesi ◽  
A. Boujibar ◽  
N. Bolfan-Casanova ◽  
C. Cartier ◽  
...  

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 ◽  
...  

2010 ◽  
Vol 295 (3-4) ◽  
pp. 487-496 ◽  
Author(s):  
Karen Ziegler ◽  
Edward D. Young ◽  
Edwin A. Schauble ◽  
John T. Wasson

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