日本地球惑星科学連合2014年大会

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[U-05_30AM2] 生命-水-鉱物-大気相互作用

2014年4月30日(水) 11:00 〜 12:45 419 (4F)

コンビーナ:*大竹 翼(北海道大学大学院工学研究院 環境循環システム部門)、鈴木 庸平(東京大学大学院理学系研究科)、白石 史人(広島大学大学院理学研究科地球惑星システム学専攻)、高井 研(海洋研究開発機構極限環境生物圏研究センター)、上野 雄一郎(東京工業大学大学院地球惑星科学専攻)、長沼 毅(広島大学大学院生物圏科学研究科)、掛川 武(東北大学大学院理学研究科地学専攻)、横山 正(大阪大学大学院理学研究科宇宙地球科学専攻)、中村 謙太郎(独立行政法人海洋研究開発機構 (JAMSTEC) システム地球ラボ プレカンブリアンエコシステムラボユニット)、座長:横山 正(大阪大学大学院理学研究科宇宙地球科学専攻)、中村 謙太郎(独立行政法人海洋研究開発機構 (JAMSTEC) システム地球ラボ プレカンブリアンエコシステムラボユニット)

11:45 〜 12:00

[U05-08] ケイ酸塩風化の見かけの活性化エネルギーに対する大気組成の影響

*菅崎 良貴1村上 隆1 (1.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:ケイ酸塩風化, 二酸化炭素, フィードバック, 先カンブリア時代

Silicate weathering is a major sink of atmospheric CO2. Because CO2 is an important greenhouse gas, silicate weathering regulates not only the partial pressure of atmospheric CO2 (Pco2) but also the surface temperature (T). The apparent activation energy of silicate weathering represents the temperature dependence of silicate weathering and thus interrelates the intensity of silicate weathering, Pco2 and surface temperature. It has been reported that solution composition can affect the apparent activation energy of dissolution/precipitation of silicates (e.g., Casey and Sposito, 1992; Lasaga, 1995; Cama et al., 1999). However, the relationship between the solution composition and the apparent activation energy of silicate reaction is not yet fully understood. To investigate the apparent activation energy of silicate weathering in a natural weathering system, we formulated the apparent activation energy of silicate weathering in three different scales, namely, (i) dissolution/precipitation of each mineral, (ii) elemental loss as the net reactions of the minerals and (iii) weathering flux from a weathering profile, based on the rate expressions in the three scales. It was found that, due to the effects of solution composition on the apparent activation energy, the temperature dependence of atmospheric CO2H*co2) affects the apparent activation energy of silicate weathering. Based on the formulated apparent activation energy, we estimated the apparent activation energy of silicate-weathering flux as a function of ΔH*co2. Then, the compensation law between the pre-exponential factor and the apparent activation energy of silicate-weathering flux was introduced from the literature, leading to the establishment of the relationship between silicate-weathering flux (Fco2), T and ΔH*co2. Based on the Fco2-TH*co2 relationship and the greenhouse effects of atmospheric CO2 in the literature, we calculated the ratio of change in Fco2 to that in Pco2 as an indicator of silicate-weathering feedback in the Precambrian. The calculation revealed that when Pco2 > 〜10-0.5 atm, the feedback is negative and independent of Pco2 and surface temperature. On the other hand, when Pco2 < 〜10-0.5 atm, the feedback is independent of Pco2 but dependent on surface temperature; at low (< 〜30 ℃) and high (> 〜30 ℃) temperatures, the feedback is negative and positive, respectively. Due to the positive feedback, the conditions of Pco2 < 〜10-0.5 atm and T > 〜30 ℃ are unstable, and immediately change, with a slight change in Pco2, to either the conditions of Pco2 > 〜10-0.5 atm or those of Pco2 < 〜10-0.5 atm and T < 〜30 ℃. When Pco2 < 〜10-0.5 atm and < 〜30 ℃, the feedback is not only negative, but also becomes more negative as temperature decreases, suggesting that global glaciations are harder to bring about than previously thought.