日本地球惑星科学連合2014年大会

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セッション記号 S (固体地球科学) » S-MP 岩石学・鉱物学

[S-MP47_1AM1] 鉱物の物理化学

2014年5月1日(木) 09:00 〜 10:45 422 (4F)

コンビーナ:*奥寺 浩樹(金沢大学理工学域自然システム学系)、興野 純(筑波大学大学院生命環境科学研究科地球進化科学専攻)、座長:鎌田 誠司(東北大学大学院理学研究科)、興野 純(筑波大学大学院生命環境科学研究科地球進化科学専攻)

10:00 〜 10:15

[SMP47-05] Fe3S, FeO, 天然アルマンディンの放射光メスバウア測定

*鎌田 誠司1平尾 直久2浜田 麻希3鈴木 那奈美1大谷 栄治1大石 泰生2増田 亮4三井 隆也5 (1.東北大・理、2.高輝度光科学研究センター、3.金沢大学理工学研究域自然システム学系、4.京都大学原子炉実験所、5.日本原子力研究開発機構)

キーワード:地球核, マントル, メスバウア, Fe3S, FeO

The Earth's core is considered to be composed of an iron alloy with light elements since its density is smaller than that of pure iron under core conditions (e.g., Birch, 1964; Dubrovinsky et al., 2000). Although there are many candidates for these elements, such as H, C, O, Si, and S, sulfur in particular has been considered as one of the most plausible candidates. This is because it is depleted in the mantle, suggesting that it exists in the Earth's core (Murthy and Hall, 1970), and iron sulfides are found universally in iron meteorites, i.e., analogues of the Earth's core. Although the content of sulfur in the Earth's core is not known precisely, the sulfur content in the core is estimated to be at least a few wt% based on cosmic element abundances (McDonough, 2003) and high pressure partitioning experiments (e.g., Hillgren et al., 2000).Since sulfur is one of the most plausible light elements, a compressibility and phase diagram in the Fe-FeS system has been studied (e.g., Campbell et al., 2007; Chen et al., 2007; Fei et al., 2000; Kamada et al., 2010; Li et al., 2001; Seagle et al., 2006). According to previous studies, Fe3S is stable from 21 GPa and at least up to 200 GPa. Therefore, Fe3S can be one of a candidate of the inner core materials. In addition, a synchrotron Mössbauer spectroscopy (SMS) and X-ray emission spectroscopic studies on Fe3S revealed a spin transition and magnetic transition between 20 and 25 GPa (Lin et al., 2004; Shen et al., 2003). It also showed an abnormal evolution of a and c axes with increasing pressure (Chen et al., 2007).Synchrotron Mössbauer spectroscopy is a good probe of a small sample under high pressure to investigate magnetic properties and electronic states of Fe of core and mantle minerals. An energy domain Mössbauer spectroscopic system has been recently developed at the BL10XU, SPring-8. We have measured Mössbauer spectra from Fe3S and FeO under high pressure and a natural almandine at ambient pressure.A powder mixture was made from 57Fe (96.63%, ISOFLEX) and FeS (99.9%, RAREMETALLIC co., LTD.) with a ratio of Fe:S=75.0:25.0 (in at%). A foil was made from the mixture by a cold compression using a diamond anvil cell (DAC) and loaded into a sample chamber. 57Fe enriched Fe3S was synthesized from the powder mixture in a DAC at 30 GPa and 1350 K. The synthesis of Fe3S was confirmed by X-ray diffraction patterns at BL10XU, SPring-8. 57FeO was made by reducing from 57Fe2O3 (ISOFLEX) at ambient pressure and high temperature. A pellet was made from 57FeO powder and loaded into a sample chamber of a DAC. We also measured Mössbauer spectra of a natural almandine (Py15.7Alm78.6Gros4.4Sp1.3, Idaho, USA). The energy of used X-ray for Mössbauer spectroscopy was 14.4125 keV.We have measured Mössbauer spectra of Fe3S during decompression at 5, 15, 20, 25, and 30 GPa and room temperature at BL10XU and BL11XU. At BL10XU, those of FeO and the almandine were obtained at 200 GPa and ambient pressure, respectively. The magnetic transition in Fe3S was observed between 20 and 25 GPa, which is consistent with Lin et al. (2004). We observed doublet peaks from FeO. An evidence of Fe3+ in the almandine was not detected in this study. We will report the results of the Mössbauer spectra based on the newly developed system at BL10XU, SPring-8.