日本地球惑星科学連合2021年大会

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[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-IS14] 水惑星学

2021年6月5日(土) 17:15 〜 18:30 Ch.22

コンビーナ:関根 康人(東京工業大学地球生命研究所)、渋谷 岳造(海洋研究開発機構)、玄田 英典(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)

17:15 〜 18:30

[MIS14-P07] No effective oxychloride formations on Europa's surface inferred from UV/electron irradiation experiments onto salt-ice mixtures

*丹 秀也1、関根 康人1、菊池 崇志2、末松 久幸2、羽馬 哲也3、高橋 嘉夫4 (1.東京工業大学地球生命研究所、2.長岡技術科学大学、3.東京大学先進科学研究機構、4.東京大学大学院理学系研究科地球惑星科学専攻)

キーワード:エウロパ、照射実験、過塩素酸塩

Recent observations of Europa's surface suggest that chlorides (e.g., NaCl, MgCl2·nH2O) exist on Europa's geologically active chaos regions (Fischer et al., 2015; Ligier et al. 2016). Europa's surface is irradiated by high-energy particles, such as electrons, and solar UV light. These irradiations would cause the oxidation of surface materials due to dissociation of H2O ice and subsequent escape of H2 into space. Through the irradiation, chlorides on the surface could be oxidized to form oxychlorides, such as chlorates (e.g., Mg(ClO3)2·6H2O) or perchlorates (e.g., NaClO4, Mg(ClO4)2·6H2O) (e.g., Johnson et al., 2019). However, the oxidation reactions have been poorly investigated based on laboratory experiments.
Here, we perform laboratory experiments to investigate formation of oxychlorides on Europa. We irradiated ~10-keV electron or UV light onto mixtures of H2O ice and chlorides at temperatures of ~120 K using a newly-developed irradiation experimental system. In addition, we irradiated MeV electron onto mixture of H2O ice and chlorides using an electron-beam accelerator, ETIGO-III (Tokuchi et al., 1998). Our results show no significant formations of ClO4 and ClO3 from chlorides regardless of the experimental conditions. The upper limits of conversion efficiency from NaCl to NaClO4 are estimated in our experiments. The estimated upper limits of conversion efficiency are 10-19−10-20 /electron. Considering the upper limits of conversion efficiency, together with the fluxes of electrons or photons on Europa (Paranicas et al., 2009; Clare et al., 2012), an upper limit abundance of NaClO4 are estimated as less than ~2 mol% relative to H2O ice over Europa's surface age (30−100 Myr). Our experimental results and estimations suggest that oxychlorides are minor components as salts and oxidants on Europa's surface.