Literature DB >> 34168164

Behavior of light elements in iron-silicate-water-sulfur system during early Earth's evolution.

Riko Iizuka-Oku1, Hirotada Gotou2, Chikara Shito3, Ko Fukuyama3,4, Yuichiro Mori3, Takanori Hattori5, Asami Sano-Furukawa5, Ken-Ichi Funakoshi6, Hiroyuki Kagi3.   

Abstract

Hydrogen (H) is considered to be one of the candidates for light elements in the Earth's core, but the amount and timing of delivery have been unknown. We investigated the effects of sulfur (S), another candidate element in the core, on deuteration of iron (Fe) in iron-silicate-water system up to 6-12 GPa, ~ 1200 K using in situ neutron diffraction measurements. The sample initially contained saturated water (D2O) as Mg(OD)2 in the ideal composition (Fe-MgSiO3-D2O) of the primitive Earth. In the existence of water and sulfur, phase transitions of Fe, dehydration of Mg(OD)2, and formation of iron sulfide (FeS) and silicates occurred with increasing temperature. The deuterium (D) solubility (x) in iron deuterides (FeDx) increased with temperature and pressure, resulting in a maximum of x = 0.33(4) for the hydrous sample without S at 11.2 GPa and 1067 K. FeS was hardly deuterated until Fe deuteration had completed. The lower D concentrations in the S-containing system do not exceed the miscibility gap (x <  ~ 0.4). Both H and S can be incorporated into solid Fe and other light elements could have dissolved into molten iron hydride and/or FeS during the later process of Earth's evolution.

Entities:  

Year:  2021        PMID: 34168164     DOI: 10.1038/s41598-021-91801-3

Source DB:  PubMed          Journal:  Sci Rep        ISSN: 2045-2322            Impact factor:   4.379


  7 in total

1.  Early solar system. Early accretion of water in the inner solar system from a carbonaceous chondrite-like source.

Authors:  Adam R Sarafian; Sune G Nielsen; Horst R Marschall; Francis M McCubbin; Brian D Monteleone
Journal:  Science       Date:  2014-10-30       Impact factor: 47.728

2.  Low core-mantle boundary temperature inferred from the solidus of pyrolite.

Authors:  Ryuichi Nomura; Kei Hirose; Kentaro Uesugi; Yasuo Ohishi; Akira Tsuchiyama; Akira Miyake; Yuichiro Ueno
Journal:  Science       Date:  2014-01-16       Impact factor: 47.728

3.  Hydrogen partitioning into molten iron at high pressure: implications for Earth's core

Authors: 
Journal:  Science       Date:  1997-12-05       Impact factor: 47.728

4.  Site occupancy of interstitial deuterium atoms in face-centred cubic iron.

Authors:  Akihiko Machida; Hiroyuki Saitoh; Hidehiko Sugimoto; Takanori Hattori; Asami Sano-Furukawa; Naruki Endo; Yoshinori Katayama; Riko Iizuka; Toyoto Sato; Motoaki Matsuo; Shin-ichi Orimo; Katsutoshi Aoki
Journal:  Nat Commun       Date:  2014-09-26       Impact factor: 14.919

5.  Hydrogenation of iron in the early stage of Earth's evolution.

Authors:  Riko Iizuka-Oku; Takehiko Yagi; Hirotada Gotou; Takuo Okuchi; Takanori Hattori; Asami Sano-Furukawa
Journal:  Nat Commun       Date:  2017-01-13       Impact factor: 14.919

6.  Interstitial hydrogen atoms in face-centered cubic iron in the Earth's core.

Authors:  Daijo Ikuta; Eiji Ohtani; Asami Sano-Furukawa; Yuki Shibazaki; Hidenori Terasaki; Liang Yuan; Takanori Hattori
Journal:  Sci Rep       Date:  2019-05-08       Impact factor: 4.379

7.  Hexagonal Close-packed Iron Hydride behind the Conventional Phase Diagram.

Authors:  Akihiko Machida; Hiroyuki Saitoh; Takanori Hattori; Asami Sano-Furukawa; Ken-Ichi Funakoshi; Toyoto Sato; Shin-Ichi Orimo; Katsutoshi Aoki
Journal:  Sci Rep       Date:  2019-08-23       Impact factor: 4.379

  7 in total

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