JpGU-AGU Joint Meeting 2020

講演情報

[E] 口頭発表

セッション記号 B (地球生命科学) » B-CG 地球生命科学複合領域・一般

[B-CG06] 地球史解読:冥王代から現代まで

コンビーナ:小宮 剛(東京大学大学院総合文化研究科広域科学専攻)、加藤 泰浩(東京大学大学院工学系研究科システム創成学専攻)、鈴木 勝彦(国立研究開発法人海洋研究開発機構・海底資源センター)、中村 謙太郎(東京大学大学院工学系研究科システム創成学専攻)

[BCG06-10] Effect of Hydrocarbon Haze on Climate Stability under Mildly Oxidized Late-Archean Environment

★Invited Papers

*渡辺 泰士1田近 英一1尾崎 和海2洪 鵬3 (1.東京大学、2.東邦大学、3.千葉工業大学)

キーワード:太古代、初期地球、炭素循環

The atmospheric oxygen level (pO2) is suggested to have been lower than 10-5 PAL (present atmospheric level) based on an existence of mass-independent isotope fluctuation of sulfur in the Archean (e.g. Pavlov and Kasting, 2002). During the Late Archean (3.0-2.5 Ga), temporal increases of pO2 are suggested from concentrations of redox sensitive trace elements (e.g. Anbar et al., 2007), which might have been associated with the onset of oxygenic photosynthesis in the ocean. On the other hand, there is a record of co-variation of carbon and sulfur isotopes, which might have reflected a transient formation of hydrocarbon haze, meaning a transient appearance of very reducing atmosphere in the Late Archean (Zerkle et al., 2012; Izon et al., 2017). These records suggest that the atmospheric composition in the Late Archean could have significantly varied. Previously, how the rise of oxygen in the atmosphere affects the global carbon cycle has been discussed in various context and in different ages. However, how the formation of haze has affected global carbon cycle in the Late Archean has not been investigated considering the atmospheric and marine microbial reactions. Here we used a coupled model of atmospheric photochemimstry-marine microbial ecosystem-global carbon cycle, in which the photochemical model "Atmos" (Arney et al., 2016) is included, to investigate how the production of the hydrocarbon haze affected the global carbon cycle and climate stability under mildly oxygenized condition in the Late Archean (f(O2) ~10-6 PAL) and under completely anoxic condition in the Middle Archean (f(O2) < 10-10 PAL). In both cases, hydrocarbon haze is formed in the atmosphere when CH4/CO2 is more than around 0.2, consistent with Arney et al. (2016). We found that, the formation of hydrocarbon haze works as a CO2 consumption pathway in the atmosphere under completely anoxic condition, because the formation/removal rates of hydrocarbon haze increase according to the decreasing pCO2. This means that, hazy climate state is unstable under anoxic condition. In the mildly oxidized world, on the other hand, the formation/removal rates of hydrocarbon haze were not affected significantly by the change in pCO2, so that the hazy condition becomes stable by the silicate weathering negative feedback. This result suggests that there is a negative feedback mechanism concerning the formation rate of hydrocarbon haze under mildly oxidized atmosphere, through changes in the UV flux in the atmosphere and atmospheric redox condition. Our result is consistent with the geological records that suggests the transient formation of hydrocarbon haze in the Late Archean.