日本地球惑星科学連合2021年大会

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セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS12] 惑星火山学

2021年6月5日(土) 09:00 〜 10:30 Ch.02 (Zoom会場02)

コンビーナ:野口 里奈(新潟大学 自然科学系)、下司 信夫(産業技術総合研究所 活断層・火山研究部門)、諸田 智克(東京大学理学系研究科地球惑星科学専攻)、座長:野口 里奈(新潟大学 自然科学系)、下司 信夫(産業技術総合研究所 活断層・火山研究部門)、諸田 智克(東京大学理学系研究科地球惑星科学専攻)

09:15 〜 09:30

[MIS12-02] Laboratory investigations of salt precipitation upon decompression and degassing of volatile-containing brines: Implication for carbonate mineral formations on Solar system icy bodies

*依田 優大1,2、関根 康人2,3 (1.東京大学理学系研究科地球惑星科学専攻、2.東京工業大学 地球生命研究所、3.金沢大学 環日本海域環境研究センター)

キーワード:氷火山活動、氷天体における塩の形成、減圧過程における脱ガス

Chemical compositions of subsurface oceans on Europa, Ceres, Enceladus and other icy bodies can be constrained based on observations of non-ice materials on the surfaces. Carbonate mineral (i.e., sodium carbonate (Na2CO3)) is indeed found on bright spots of Ceres (De Sanctis et al., 2016), suggesting the presence of carbonate-rich subsurface brine reservoirs and precipitations of the carbonate salts upon cryovolcanic activities. The mineralogical and chemical compositions of the salts would reflect not only the water chemistry of liquid reservoirs, but also eruption dynamics and degassing processes. For instance, the previous experimental studies showed that rapid freezing of brine results in formation of Na2CO3, compared with NaHCO3 precipitation in slow freezing (e.g., Vu et al., 2017; Thomas et al., 2018). In addition to rapid freezing, decompression upon cryovolcanic activities could affect salt precipitations through degassing of dissolved volatiles from brine. However, no experimental studies have been conducted to investigate the effects of rapid decompression and degassing of volatile on salt precipitation.

Here, we perform laboratory experiments to investigate the effect of decompression on salt mineralization. To this end, we newly constructed an experimental system, which can simulate rapid decompression and degassing of volatile from brine. Through evacuation of gas in a vacuum chamber, volatile-containing brine evaporates and subsequently freezes. We collected salt residues after the experiments and analyzed their size and structure using SEM and mineralogical and chemical compositions using both of SEM and micro XRD. We also observed dynamics of eruption using a high-speed camera as a function of dissolved CO2 gas in starting brines.

In the experiments, we find a clear dependence of precipitated mineralogical compositions on speed of decompression. Precipitations of Na2CO3 tend to be suppressed in slow decompression and ineffective degassing, resulting in precipitation of NaHCO3. To form more Na2CO3, rapid decompression and effective degassing are favored. Together with the results of the previous studies (Vu et al., 2017; Thomas et al., 2018), the occurrence of Na2CO3 on the bright spots of Ceres implies that occurrence of explosive eruption of cryomagma with degassing and rapid freezing, rather than effusive eruption.