日本地球惑星科学連合2019年大会

講演情報

[J] ポスター発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS11] 水惑星学

2019年5月28日(火) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 8ホール)

コンビーナ:関根 康人(東京工業大学地球生命研究所)、臼井 寛裕(東京工業大学地球生命研究所)、福士 圭介(金沢大学環日本海域環境研究センター)、渋谷 岳造(海洋研究開発機構)

[MIS11-P07] 室内実験および熱力学計算に基づいた還元的環境下におけるコンドライトの水変成プロセスの解明

*菊池 早希子1渋谷 岳造1 (1.海洋研究開発機構)

キーワード:コンドライト、サポナイト、ピロータイト

The presence of hydrous minerals in chondrites have been considered as an important evidence for the former presence of liquid water in parent bodies. However, the detailed evolutionary history of parent bodies (e.g., temperature fluid composition and water/rock ratio) are still poorly constrained, because the alteration processes of chondritic rock are not well defined and very few relevant experimental data are available. Here we investigate alteration process of chondrites by experiments simulating reactions between synthetic chondrite (mixtures of olivine, pyroxene, glass, Femetal, and troilite) and NH3-containing solutions at 25 and 80 °C under anoxic conditions. We also compared the experimental results with those predicted from thermodynamic calculations to understand the equilibrium and kinetic conditions of chondrite-water interaction.
The experiments up to 7 months showed that the water-rock reactions caused a series of mineral alterations and production of H2(aq), especially at 80 °C. X-ray diffraction analysis revealed that the formation of pyrrhotite was notable during the first few days in the experiment, which was likely resulted from the dissolution of troilite. In contrast, precipitation of saponite was evident after 100 days in the experiment, which was probably caused by the dissolution of Si-rich glass in the synthetic chondrites. Transmission electron microscope observation revealed that the saponite and secondary Si-rich amorphous phases densely covered the surface of the original olivine, glass, pyroxene, and troilite. These results imply that amorphous silica precipitated after the formation of pyrrhotite, followed by the precipitation of saponite. A part of these mineral assemblages obtained from our experiment was inconsistent with those predicted from the thermodynamic equilibrium calculations, suggesting that some metastable alteration minerals occur in the chondrite-water system before the complete equilibrium is achieved.