Journal Article10.1029/2022jb024365
High‐Pressure Melting Curve of FeH: Implications for Eutectic Melting Between Fe and Non‐Magnetic FeH
9
TL;DR: In this paper , the authors examined the melting curve of non-magnetic FeH between 43 and 152 GPa by a combination of laser-heated diamond-anvil cell techniques and synchrotron X-ray diffraction analyses.
read more
Abstract: While hydrogen could be an important light alloying element in planetary iron cores, phase relations in the Fe-FeH system remain largely unknown at high pressures and temperatures (P-T). A speculative Fe-H2 phase diagram has been proposed assuming continuous solid solution between Fe and FeH and eutectic melting between FeH and H2. Recent studies revealed that stoichiometric FeH becomes non-magnetic above ∼40 GPa, which might affect its melting behavior. Here we examined the melting curve of non-magnetic FeH between 43 and 152 GPa by a combination of laser-heated diamond-anvil cell techniques and synchrotron X-ray diffraction (XRD) analyses. The melting temperature was determined by employing the appearance of additional hazy XRD signals upon quenching temperature as a melting criterion. We also performed thermodynamic modeling, which well reproduces the change in the curvature of FeH melting curve upon the loss of magnetism and extrapolates the experimental constraints to inner core pressures. The XRD data showed that non-magnetic FeH melts congruently at temperatures higher than the known eutectic melting curve for FeHx (x > 1). Combined with the fact that the endmembers exhibit different crystal structures, these results indicate that Fe and non-magnetic FeH form a eutectic system. The dT/dP slope of the FeH melting curve is comparable to that for Fe, suggesting that the eutectic liquid composition of FeH0.42 (Fe + 0.75 wt% H) previously estimated at ∼40 GPa changes little with increasing pressure.
read more
Chat with Paper
AI Agents for this Paper
Find similar papers on Google Scholar, PubMed and Arxiv
Write a critical review of this paper
Analyze citations of this paper to find unaddressed research gaps
Citations
Real-time (nanoseconds) determination of liquid phase growth during shock-induced melting
TL;DR: In this article , the authors investigated the time-dependent growth of the molten phase in shock-compressed germanium and found that the characteristic time for melting in shockcompressed Germanium decreases from ~7.2 nanoseconds at 35 gigapascals to less than 1 nanoscond at 42 gigapasals.
Mineralogy of Planetary Cores
None Guido Posern
- 01 Jan 2023
TL;DR: In this article , the authors reviewed the core compositions and structures of Mercury, Venus, Earth, and Mars as they are currently understood and summarized the phase relations in the iron-dominant core systems at high P-T and discussed the role of light elements during core evolution.
Superionic iron hydride shapes ultralow-velocity zones at Earth’s core–mantle boundary
Yu Zhang,Wenzhong Wang,Yunguo Li,Zhongqing Wu +3 more
TL;DR: First-principles simulations reveal that superionic iron hydride, formed by water-iron reaction, is stable at Earth's core-mantle boundary, explaining ultralow-velocity zones (ULVZs) through accumulation and density differences with the ambient mantle.
References
•Journal Article
R: A language and environment for statistical computing.
TL;DR: Copyright (©) 1999–2012 R Foundation for Statistical Computing; permission is granted to make and distribute verbatim copies of this manual provided the copyright notice and permission notice are preserved on all copies.
410.8K
SGTE data for pure elements
TL;DR: In this article, the authors present the data for the condensed phases of 78 elements as currently used by SGTE (Scientific Group Thermodata Europe) as a sound basis for the critical assessment of thermodynamic data, thereby, perhaps, limiting unnecessary duplication of effort.
4.6K
A low mass for Mars from Jupiter's early gas―driven migration
Kevin J. Walsh,Alessandro Morbidelli,Sean N. Raymond,Sean N. Raymond,David P. O'Brien,Avi Mandell +5 more
TL;DR: Simulation of the early Solar System shows how the inward migration of Jupiter to 1.5 au, and its subsequent outward migration, lead to a planetesimal disk truncated at 1’au; the terrestrial planets then form from this disk over the next 30–50 million years, with an Earth/Mars mass ratio consistent with observations.
1.3K
A model for alloying in ferromagnetic metals
Mats Hillert,Magnus Jarl +1 more
TL;DR: In this paper, a mathematical representation of the magnetic specific heat, recently suggested by Inden, was applied to iron in an evaluation of the difference in Gibbs energy between the fcc and bcc states.
1K
Melting of Iron at Earth’s Inner Core Boundary Based on Fast X-ray Diffraction
TL;DR: In this article, the melting temperature of iron at the inner core boundary is estimated to be 6230 ± 500 kelvin with a possible partial melting of the mantle at the core-mantle boundary.
595