日本地球惑星科学連合2014年大会

講演情報

口頭発表

セッション記号 S (固体地球科学) » S-GC 固体地球化学

[S-GC56_30PM2] 固体地球化学・惑星化学

2014年4月30日(水) 16:15 〜 17:45 415 (4F)

コンビーナ:*下田 玄(産業技術総合研究所地質調査総合センター)、鈴木 勝彦(独立行政法人海洋研究開発機構・地球内部ダイナミクス領域)、山下 勝行(岡山大学大学院自然科学研究科)、座長:山下 勝行(岡山大学大学院自然科学研究科)、下田 玄(産業技術総合研究所地質調査総合センター)

17:30 〜 17:45

[SGC56-P04_PG] 天然多結晶ダイヤモンド(カルボナド)のオスミウム同位体比測定の試み

ポスター講演3分口頭発表枠

*白石 智子1仙田 量子2鍵 裕之1角野 浩史1鈴木 勝彦2 (1.東京大学大学院理学系研究科附属地殻化学実験施設、2.独立行政法人海洋研究開発機構地球内部ダイナミクス領域)

キーワード:carbonado, TIMS, Os isotope, diamond

The origin of natural polycrystalline diamond, carbonado, has long been enigmatic. Carbonado is characterized as high porosity, no genetic relations to kimberlites, light carbon isotope ratio, and lack of mantle-derived mineral inclusions. Based on these observations, several hypotheses about the origin of carbonado have been proposed: transformation of subducted organic carbon into diamond in a cold slab (Robinson, 1978); shock metamorphism of organic carbon by meteorite impact (Smith and Dawson, 1985); radiation-induced diamond formation by spontaneous fission of uranium in crustal environment (Ozima et al., 1991); formation in an interstellar environment (Garai et al., 2006); crystallization from C-O-H fluid in cratonic upper mantle (Ishibashi et al., 2012). However, no conclusive evidence has been provided to settle a controversy about the origin of carbonado. In this study, we first tried to measure Os isotopic composition of carbonados collected from placer deposits in the Central African Republic in order to identify its origin.
Natural samples have a wide variety of Os isotopic ratios, 187Os/188Os, depending on their origin because 187Re, the parent nuclide of radiogenic 187Os, is a mildly incompatible element during mantle melting whereas Os is a strongly compatible element. 187Os/188Os ratio of upper continental crust ranges from 1.0 to 1.4 (Peucker-Ehrenbrink and Jahn, 2001), whereas that of primitive upper mantle is about 0.13 (Meisel et al., 1996). Os isotopic ratio of the micro diamond crystal itself can reflect the environment where diamond grains crystallized. Carbonado is a porous aggregate of micrometer-size diamond crystals and original chemical characteristics of the grain boundaries could be heavily altered after the diamond growth.
This study was designed to determine Os isotopic ratios within diamond crystals of carbonados and in the grain boundaries separately. Two-step sample chemical leaching was carried out by Carius tube method (Shirey and Walker, 1995). First, carbonado samples were crushed to submillimeter grains and were sealed in a Carius tube with spike solutions and inverse aqua regia (HCl + 3 HNO3). The solution was heated at 220℃ for 24 hours. This procedure was for extract Os in the grain boundaries. Second, the residue of solid samples was heated in a vacuum chamber to convert diamond to graphite. A graphitized sample was decomposed in acid solution in the same way as the first leaching process. The second process was to extract Os within diamond grains. Osmiums in the both solutions were purified with the solvent extraction (Cohen and Waters, 1996) and microdistillation (Roy-Barman, 1993). Osmium isotopic compositions of the samples were determined using thermal ionization mass spectrometry (TIMS). Blank levels of Carius tubes and inverse aqua regia solutions prepared from several chemical regents were checked. As a result, a quartz glass tube was found to have the lowest blank level compared with other glass tubes made from borosilicate glass.
In the presentation, we will report preliminary results of Os isotopic ratios of the carbonado, which have the potential for a decisive evidence to close the debate on the origin of carbonado.