日本地球惑星科学連合2016年大会

講演情報

ポスター発表

セッション記号 S (固体地球科学) » S-GC 固体地球化学

[S-GC50] 固体地球化学・惑星化学

2016年5月22日(日) 17:15 〜 18:30 ポスター会場 (国際展示場 6ホール)

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(国立研究開発法人海洋研究開発機構・海底資源研究開発センター)、山下 勝行(岡山大学大学院自然科学研究科)、石川 晃(東京大学大学院総合文化研究科)、飯塚 毅(東京大学)

17:15 〜 18:30

[SGC50-P04] 陽・陰イオン交換樹脂とMC-ICP-MSに基づくMo同位体分析

*後藤 孝介1下田 玄1青木 翔吾2石川 晃2 (1.産業技術総合研究所、2.東京大学大学院総合文化研究科)

キーワード:モリブデン

In the past 15 years, molybdenum stable isotope (δ98/95Mo) has become a valuable tool for assessing plaeo-ocean redox conditions (Arnold et al., 2004 Science; Dahl et al., 2010 PNAS). To measure Mo isotopic compositions in Fe and Mn rich samples, we conducted (1) chemical purification of reference Mn nodules (JMn-1, Nod P-1, and Nod A-1) by two-stage of ion exchange chemistry (AG1X-8 and AG50WX-8)(Barling et al., 2001 EPSL; Gordon et al., 2009 Geology), and (2) isotope measurements of spiked Mo standard solutions (NIST 3134 and Alfa Aesar Specpure standard solution), using multi-collector inductively coupled plasma mass spectrometry (MC-ICP-MS, Thermo Fisher Scientific Neptune) at Geological Survey of Japan. The yields during the column chemistry were better than 95%. Although isobaric interferences on Mo masses are possible from Fe (or Fe argide), Zr, and Ru (Siebert et al., 2001 G-cubed; Malinovsky et al., 2005 Int. J. Mass Spectrom.), their concentrations in the purified samples were comparable to our chemical procedural blank values. The difference in δ98/95Mo between NIST 3134 and the Alfa Aesar standard solution was 0.17 ± 0.14‰. The observed offset was consistent with previously reported values (0.12 ± 0.11‰; Greber et al., 2012 Geostand. Geoanal. Res.). Hence, accurate and high precision Mo isotope measurements of Fe-Mn oxides are possible using the anion and cation exchange resins and MC-ICP-MS. In the presentation, we will also report new δ98/95Mo data of hydrothermal Mn and Fe crusts based on this method.