{"title":"氧化镁在铁液中的混相","authors":"Leslie Insixiengmay , Lars Stixrude","doi":"10.1016/j.epsl.2025.119242","DOIUrl":null,"url":null,"abstract":"<div><div>We explore phase equilibria on the MgO-Fe join as a prototype of lithophile-core interaction in terrestrial planets. Our density functional theory simulations are based on a phase coexistence method: fluids of initially pure MgO and Fe compositions are allowed to establish a dynamic equilibrium across a near-planar interface. Methods for analyzing the composition and other properties of the two coexisting phases show that MgO behaves as a component, with indistinguishable Mg and O concentrations in Fe-rich and oxide-rich phases. The phase diagram is well described as that of a symmetric regular solution, a picture confirmed by independent one-phase determinations of the enthalpy, entropy, and volume of mixing. The critical temperature, above which there is complete miscibility across the MgO-Fe join is 7000 K at 68 GPa, and 9000 K and 172 GPa. The rate of MgO exsolution from the Fe-rich liquid on cooling is similar to that found in previous experimental studies, and is too small to drive a dynamo.</div></div>","PeriodicalId":11481,"journal":{"name":"Earth and Planetary Science Letters","volume":"654 ","pages":"Article 119242"},"PeriodicalIF":4.8000,"publicationDate":"2025-02-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"MgO miscibility in liquid iron\",\"authors\":\"Leslie Insixiengmay , Lars Stixrude\",\"doi\":\"10.1016/j.epsl.2025.119242\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>We explore phase equilibria on the MgO-Fe join as a prototype of lithophile-core interaction in terrestrial planets. Our density functional theory simulations are based on a phase coexistence method: fluids of initially pure MgO and Fe compositions are allowed to establish a dynamic equilibrium across a near-planar interface. Methods for analyzing the composition and other properties of the two coexisting phases show that MgO behaves as a component, with indistinguishable Mg and O concentrations in Fe-rich and oxide-rich phases. The phase diagram is well described as that of a symmetric regular solution, a picture confirmed by independent one-phase determinations of the enthalpy, entropy, and volume of mixing. The critical temperature, above which there is complete miscibility across the MgO-Fe join is 7000 K at 68 GPa, and 9000 K and 172 GPa. The rate of MgO exsolution from the Fe-rich liquid on cooling is similar to that found in previous experimental studies, and is too small to drive a dynamo.</div></div>\",\"PeriodicalId\":11481,\"journal\":{\"name\":\"Earth and Planetary Science Letters\",\"volume\":\"654 \",\"pages\":\"Article 119242\"},\"PeriodicalIF\":4.8000,\"publicationDate\":\"2025-02-04\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Earth and Planetary Science Letters\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0012821X2500041X\",\"RegionNum\":1,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"GEOCHEMISTRY & GEOPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Earth and Planetary Science Letters","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0012821X2500041X","RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
摘要
我们探索了MgO-Fe连接上的相平衡,作为类地行星中亲石-核相互作用的原型。我们的密度泛函理论模拟基于相共存方法:允许初始纯MgO和Fe成分的流体在近平面界面上建立动态平衡。分析两相的组成和其他性质的方法表明,MgO作为一种组分,在富铁相和富氧相中Mg和O的浓度没有区别。相图很好地描述为对称正则解的相图,这是由独立的单相焓、熵和混合体积的测定所证实的。临界温度为7000 K (68 GPa)和9000 K (172 GPa)。在冷却过程中,富铁液体中氧化镁的析出速率与之前的实验研究中发现的速率相似,但它太小,无法驱动发电机。
We explore phase equilibria on the MgO-Fe join as a prototype of lithophile-core interaction in terrestrial planets. Our density functional theory simulations are based on a phase coexistence method: fluids of initially pure MgO and Fe compositions are allowed to establish a dynamic equilibrium across a near-planar interface. Methods for analyzing the composition and other properties of the two coexisting phases show that MgO behaves as a component, with indistinguishable Mg and O concentrations in Fe-rich and oxide-rich phases. The phase diagram is well described as that of a symmetric regular solution, a picture confirmed by independent one-phase determinations of the enthalpy, entropy, and volume of mixing. The critical temperature, above which there is complete miscibility across the MgO-Fe join is 7000 K at 68 GPa, and 9000 K and 172 GPa. The rate of MgO exsolution from the Fe-rich liquid on cooling is similar to that found in previous experimental studies, and is too small to drive a dynamo.
期刊介绍:
Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.