日本地球惑星科学連合2016年大会

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セッション記号 M (領域外・複数領域) » M-TT 計測技術・研究手法

[M-TT28] 地球化学の最前線:未来の地球化学を展望して

2016年5月22日(日) 10:45 〜 12:15 A04 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*小畑 元(東京大学大気海洋研究所海洋化学部門海洋無機化学分野)、角野 浩史(東京大学大学院総合文化研究科広域科学専攻相関基礎科学系)、横山 哲也(東京工業大学大学院理工学研究科地球惑星科学専攻)、平田 岳史(京都大学大学院理学研究科地球惑星科学専攻)、角皆 潤(名古屋大学大学院環境学研究科)、高橋 嘉夫(東京大学大学院理学系研究科地球惑星科学専攻)、橘 省吾(北海道大学大学院理学研究院自然史科学専攻地球惑星システム科学分野)、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)、下田 玄(産業技術総合研究所地質調査総合センター)、鍵 裕之(東京大学大学院理学系研究科附属地殻化学実験施設)、横山 祐典(東京大学 大気海洋研究所 高解像度環境解析研究センター)、座長:角野 浩史(東京大学大学院総合文化研究科広域科学専攻相関基礎科学系)、横山 哲也小畑 元(東京大学大気海洋研究所海洋化学部門海洋無機化学分野)

11:00 〜 11:15

[MTT28-08] 大気中水銀同位体分析:手法開発および実大気への適応

★招待講演

*山川 茜1守屋 克哉2吉永 淳2李 远瞩2千葉 仁3山下 勝行3松木 篤4 (1.国立研究開発法人国立環境研究所、2.東京大学、3.岡山大学、4.金沢大学)

キーワード:水銀同位体、マルチコレクター誘導結合プラズマ質量分析計、大気中水銀

Mercury (Hg) is a toxic heavy metal, which exists in various chemical forms in the environmental system. In the atmosphere, Hg exists in three forms (Hg0(g), gaseous elemental Hg (GEM); Hg2+(g), gaseous oxidized Hg compounds; and Hg(p), particulate/aerosol bound Hg). Hg0(g) is the dominant species of atmospheric Hg, accounting for >95% of the total Hg in the atmosphere. Because Hg0(g) is highly volatile and has limited solubility in water, it cannot be easily removed by wet or dry deposition processes. Therefore, the residence time of Hg0(g) in the atmosphere is relatively long (0.5 to 1 years), which allows long-range transport from mercury emission source(s). Conversely, Hg+2(g) and Hg(p) are effectively removed from the atmosphere through wet and dry depositions. Because Hg0(g) deposit upon oxidation to Hg2+(g) far from its emission source(s), deposition on local/regional scales represents a combination of multiple sources of Hg (global, regional, or local; natural or anthropogenic).
Over the last decade, the development of analytical methods of highly precise Hg isotopic measurements demonstrated mass dependent fractionation (MDF) and mass independent fractionation (MIF) of Hg isotopes in environmental samples. MDF of Hg isotopes occur during various natural and industrial Hg transformations. MIF of Hg isotopes is observed during abiotic reduction, photochemical and non-photochemical, and physical and chemical processes. Such processes lead to differences in the Hg isotopic composition of different emission sources, both natural and anthropogenic, and atmospheric processes (i.e., transportation, oxidation/reduction, deposition, and reemission). Therefore, Hg isotopic compositions could be used as a tracer of the sources and processes of atmospheric Hg. In this study, we aimed to develop the methods of collection and pretreatment for isotopic measurement of Hg0(g), and then isotopic composition of Hg0(g) was investigated for various regions in Japan.
To identify potential mercury sources, air mass back trajectories were calculated for each sample using the NOAA HYSPLIT model. We divided the back trajectory patterns observed in the results into three groups of air masses predominantly derived from (1) a marine source derived from the Pacific Ocean, (2) coastal and land sources that probably contain anthropogenic mercury emitted from urban-industrial regions, and (3) continental sources associated with northwesterly flow at higher altitude (>1500 m) and long-range transportation. Although multiple sources were possibly impacted during the 24 hr ambient sampling, we were able to observe a correlation between the back-trajectory types and Hg isotopic composition.