{"title":"Study on magnetite oxidation using synchrotron X–ray diffraction and X–ray absorption spectroscopy: Vacancy ordering transition in maghemite (γ–Fe2O3)","authors":"Ibuki Kinebuchi, A. Kyono","doi":"10.2465/jmps.210304","DOIUrl":null,"url":null,"abstract":"The oxidation process from magnetite to hematite through maghemite was investigated by X – ray di ff raction (XRD) and X – ray absorption spectroscopic techniques. The XRD pattern of magnetite heated at 100 °C for 3 h showed small re fl ections of maghemite with partially ordered distribution of vacancy (space group P 4 1 32 or P 4 3 32). Thereafter, the XRD pattern of magnetite heated at 250 °C for 3 h exhibited extra re fl ections corresponding to the tetragonal maghemite with fully ordered distribution of vacancy (space group P 4 1 2 1 2 or P 4 3 2 1 2). Di ff raction peaks of hematite occurred from the magnetite heated at 250 °C, in which maghemite and hematite coexisted with magnetite. Di ff raction peaks of magnetite subsequently disappeared at 300 °C. Instead, maghemite and hematite dominated the XRD pattern, but the amount of maghemite reduced from 300 °C. The maghemite completely disappeared at 500 °C, and hematite fi nally dominated the XRD pattern. Rietveld fi tting results clearly showed that the a lattice parameter and site occupancy factor of Fe at the octahedral site continuously decreased at the temperatures from 25 to 300 °C. The X – ray absorption near edge structure (XANES) result showed that the Fe 3+ / Σ Fe increased up to 300 °C and remained constant until 500 °C, indicating that Fe 2+ in oxidized magnetite was completely oxidized to Fe 3+ at 300 °C. Furthermore, the intensities of radial structure function (RSF) peaks at 1.7 and 3.1 Å corresponding to the Fe – O bonds in octahedral site and the Fe – Fe interaction between the octahedral sites reduced continuously from 25 to 300 °C. The fi tting results of the fi rst shells indicated that the coordination number and site occupancy factor at the octahedral site continuously decreased at the temperature range from 25 to 300 °C, which were approximately consistent with those of Rietveld fi tting analysis. The a lattice parameter of the oxidized magnetite displayed a linear trend between stoichiometric magnetite and stoichiometric maghemite with a relationship of a = 0.0985 x + 8.3397 ( x = Fe 2+ /Fe 3+ ). It was clearly con fi rmed that during the magnetite oxidation, Fe was continuously removed from the octahedral sites, which resulted in the formation of maghemite with partially ordered distribution of vacancy. Just after magnetite oxidation was completed, the vacancy ordering further progressed by the di ff usion of Fe 3+ within the structure, leading to the formation of maghemite with fully ordered distribution of vacancy.","PeriodicalId":51093,"journal":{"name":"Journal of Mineralogical and Petrological Sciences","volume":"1 1","pages":""},"PeriodicalIF":0.9000,"publicationDate":"2021-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"5","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Mineralogical and Petrological Sciences","FirstCategoryId":"89","ListUrlMain":"https://doi.org/10.2465/jmps.210304","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"MINERALOGY","Score":null,"Total":0}
引用次数: 5
Abstract
The oxidation process from magnetite to hematite through maghemite was investigated by X – ray di ff raction (XRD) and X – ray absorption spectroscopic techniques. The XRD pattern of magnetite heated at 100 °C for 3 h showed small re fl ections of maghemite with partially ordered distribution of vacancy (space group P 4 1 32 or P 4 3 32). Thereafter, the XRD pattern of magnetite heated at 250 °C for 3 h exhibited extra re fl ections corresponding to the tetragonal maghemite with fully ordered distribution of vacancy (space group P 4 1 2 1 2 or P 4 3 2 1 2). Di ff raction peaks of hematite occurred from the magnetite heated at 250 °C, in which maghemite and hematite coexisted with magnetite. Di ff raction peaks of magnetite subsequently disappeared at 300 °C. Instead, maghemite and hematite dominated the XRD pattern, but the amount of maghemite reduced from 300 °C. The maghemite completely disappeared at 500 °C, and hematite fi nally dominated the XRD pattern. Rietveld fi tting results clearly showed that the a lattice parameter and site occupancy factor of Fe at the octahedral site continuously decreased at the temperatures from 25 to 300 °C. The X – ray absorption near edge structure (XANES) result showed that the Fe 3+ / Σ Fe increased up to 300 °C and remained constant until 500 °C, indicating that Fe 2+ in oxidized magnetite was completely oxidized to Fe 3+ at 300 °C. Furthermore, the intensities of radial structure function (RSF) peaks at 1.7 and 3.1 Å corresponding to the Fe – O bonds in octahedral site and the Fe – Fe interaction between the octahedral sites reduced continuously from 25 to 300 °C. The fi tting results of the fi rst shells indicated that the coordination number and site occupancy factor at the octahedral site continuously decreased at the temperature range from 25 to 300 °C, which were approximately consistent with those of Rietveld fi tting analysis. The a lattice parameter of the oxidized magnetite displayed a linear trend between stoichiometric magnetite and stoichiometric maghemite with a relationship of a = 0.0985 x + 8.3397 ( x = Fe 2+ /Fe 3+ ). It was clearly con fi rmed that during the magnetite oxidation, Fe was continuously removed from the octahedral sites, which resulted in the formation of maghemite with partially ordered distribution of vacancy. Just after magnetite oxidation was completed, the vacancy ordering further progressed by the di ff usion of Fe 3+ within the structure, leading to the formation of maghemite with fully ordered distribution of vacancy.
期刊介绍:
The Journal of Mineralogical and Petrological Sciences (JMPS) publishes original articles, reviews and letters in the fields of mineralogy, petrology, economic geology, geochemistry, planetary materials science, and related scientific fields. As an international journal, we aim to provide worldwide diffusion for the results of research in Japan, as well as to serve as a medium with high impact factor for the global scientific communication
Given the remarkable rate at which publications have been expanding to include several fields, including planetary and earth sciences, materials science, and instrumental analysis technology, the journal aims to encourage and develop a variety of such new interdisciplinary scientific fields, to encourage the wide scope of such new fields to bloom in the future, and to contribute to the rapidly growing international scientific community.
To cope with this emerging scientific environment, in April 2000 the journal''s two parent societies, MSJ* (The Mineralogical Society of Japan) and JAMPEG* (The Japanese Association of Mineralogists, Petrologists and Economic Geologists), combined their respective journals (the Mineralogical Journal and the Journal of Mineralogy, Petrology and Economic Geology). The result of this merger was the Journal of Mineralogical and Petrological Sciences, which has a greatly expanded and enriched scope compared to its predecessors.