GSTDTAP  > 气候变化
DOI10.1029/2019GL082591
Hydrogen Limits Carbon in Liquid Iron
Hirose, Kei1,2; Tagawa, Shoh2; Kuwayama, Yasuhiro2; Sinmyo, Ryosuke2; Morard, Guillaume3; Ohishi, Yasuo4; Genda, Hidenori1
2019-05-28
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2019
卷号46期号:10页码:5190-5197
文章类型Article
语种英语
国家Japan; France
英文摘要

Melting experiments were performed on the Fe-C-H system to 127 GPa in a laser-heated diamond anvil cell. On the basis of in situ and ex situ sample characterizations, we found that the solubility of carbon in liquid Fe correlates inversely with hydrogen concentration at similar to 60 GPa and similar to 3500 K, indicating that liquid Fe preferentially incorporates hydrogen rather than carbon under conditions with abundant C and H. While large amounts of both C and H may have been delivered to the growing Earth, C-poor/H-rich metals were likely added to the protocore in the late stages of core formation. We also obtained a melting curve of Fell(x )(x > 1) far beyond the pressure range in earlier determinations. Its liquidus temperature was found to be 2380 K at 135 GPa, lower than those of Fe alloyed with the other possible core light elements. Relatively low core temperature is thus supported by the presence of hydrogen.


Plain Language Summary Both carbon and hydrogen are possible major light elements in the core but estimation of their abundance in the core as well as in the bulk Earth is difficult because of their high volatility. In addition, the property of hydrogen-bearing iron alloys has been the least studied. Here we performed melting experiments on Fe-C-H to 127 GPa, close to the pressure at the top of the Earth's core. Our main finding is that hydrogen limits the solubility of carbon in liquid Fe; the carbon content correlates inversely with hydrogen concentration in molten Fe coexisting with diamonds at similar to 60 GPa and similar to 3500 K. Recent planet formation theories suggest that large amounts of C and H were delivered to the growing Earth. In the late stages of core formation, liquid metals preferentially incorporating hydrogen rather than carbon may have added to the protocore. We also found that hydrogen decreases the melting temperature of Fe remarkably. The melting temperature of FeHx (x > 1) is only about 2380 K at the core-mantle boundary; lower than those of Fe-Fe3S eutectic and Fe alloyed with the other possible core light elements.


领域气候变化
收录类别SCI-E
WOS记录号WOS:000471237500021
WOS关键词HIGH-PRESSURE ; PHASE-RELATIONS ; OUTER CORE ; MELTING EXPERIMENTS ; FE ; SYSTEM ; GPA ; CONSTRAINTS ; ALLOYS ; SI
WOS类目Geosciences, Multidisciplinary
WOS研究方向Geology
引用统计
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/183384
专题气候变化
作者单位1.Tokyo Inst Technol, Earth Life Sci Inst, Tokyo, Japan;
2.Univ Tokyo, Dept Earth & Planetary Sci, Tokyo, Japan;
3.Sorbonne Univ, Museum Natl Hist Nat, UMR CNRS 7590, IMPMC, Paris, France;
4.Japan Synchrotron Radiat Res Inst, Sayo, Hyogo, Japan
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GB/T 7714
Hirose, Kei,Tagawa, Shoh,Kuwayama, Yasuhiro,et al. Hydrogen Limits Carbon in Liquid Iron[J]. GEOPHYSICAL RESEARCH LETTERS,2019,46(10):5190-5197.
APA Hirose, Kei.,Tagawa, Shoh.,Kuwayama, Yasuhiro.,Sinmyo, Ryosuke.,Morard, Guillaume.,...&Genda, Hidenori.(2019).Hydrogen Limits Carbon in Liquid Iron.GEOPHYSICAL RESEARCH LETTERS,46(10),5190-5197.
MLA Hirose, Kei,et al."Hydrogen Limits Carbon in Liquid Iron".GEOPHYSICAL RESEARCH LETTERS 46.10(2019):5190-5197.
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