2016
DOI: 10.1038/ngeo2772
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Redox-induced lower mantle density contrast and effect on mantle structure and primitive oxygen

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Cited by 24 publications
(29 citation statements)
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“…For Mg# = Mg/(Mg + Fe) = 90 Bdg representative of the mantle, differences in oxidation state of iron result in a density difference up to ~0.3% (Fig. 4 ), far less than the 1.5–2% redox-induced density contrast required to rapidly separate oxidized materials from reduced materials in the early history of the Earth 20 . Moreover, the spin-transition-induced density increase makes the density contrast of Bdg with different Fe 3+ /ΣFe ratios sharply fade away below the mid-mantle depth (Fig.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…For Mg# = Mg/(Mg + Fe) = 90 Bdg representative of the mantle, differences in oxidation state of iron result in a density difference up to ~0.3% (Fig. 4 ), far less than the 1.5–2% redox-induced density contrast required to rapidly separate oxidized materials from reduced materials in the early history of the Earth 20 . Moreover, the spin-transition-induced density increase makes the density contrast of Bdg with different Fe 3+ /ΣFe ratios sharply fade away below the mid-mantle depth (Fig.…”
Section: Discussionmentioning
confidence: 99%
“…The effects of Fe 2+ and Fe 3+ on incompressibility of Bdg are thought to be opposite 19 . The density contrast between Fe 2+ - and Fe 3+ -dominant Bdg may result in separation of oxidized and reduced materials through mantle convection and leave imprints in geochemical and isotopic compositions 20 . However, in many experimental studies on Bdg, Fe 3+ /∑Fe was not characterized.…”
Section: Introductionmentioning
confidence: 99%
“…5. An astrobiological implication: That the wet and rocky bodies in the solar system smaller than Earth probably have little or no bridgmanite (perovskite) and, therefore, have more reduced mantles may explain the preponderance of methane on some of the moons of Saturn (Wood et al , 2006 ; Bouquet et al , 2015 ; Dorofeeva, 2016 ; Girard et al , 2016; Gu et al , 2016 ), possibly Europa (Zolotov and Kargel, 2009 ) and even early Mars (Wadhwa, 2001 ; Edwards and Ehlmann, 2015 ; Hu et al , 2015 ; Wong et al , 2017b ). The challenge then is to consider the availability of electron acceptors on these other worlds ( e.g.…”
Section: Résumé and Conclusionmentioning
confidence: 99%
“…The formation of materials strongly enhanced in bridgmanite has been indeed linked to primordial processes such as magma‐ocean crystallization [ Elkins‐Tanton , ], since Mg‐rich bridgmanite is the magma‐ocean liquidus phase over a wide pressure range [ de Koker et al ., ; Tateno et al ., ], but a mechanism for subsequent Fe‐enrichment remains elusive. Other viable (primordial) candidates for DDD composition involve foundered CaSiO 3 ‐rich protocrust [ Kawai and Tsuchiya , ] as well as anomalously reduced bridgmanitic materials [ Gu et al ., ].…”
Section: Comparison Of Model Predictions With Seismic Constraintsmentioning
confidence: 99%