日本地球惑星科学連合2018年大会

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[EE] 口頭発表

セッション記号 S (固体地球科学) » S-CG 固体地球科学複合領域・一般

[S-CG55] Various interactions between solid Earth and climates

2018年5月21日(月) 15:30 〜 17:00 A03 (東京ベイ幕張ホール)

コンビーナ:中川 貴司(海洋研究開発機構数理科学・先端技術研究分野)、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)、奥野 淳一(国立極地研究所、共同)、山崎 雅(産業技術総合研究所)、座長:横山 祐典中川 貴司(海洋研究開発機構)

15:30 〜 15:45

[SCG55-01] Climatic effects of primitive biosphere and reductants supply from the mantle in the Archean Earth system

*尾崎 和海1 (1.ジョージア工科大学)

キーワード:太古代、暗い太陽のパラドックス、酸素非発生型光合成

Understanding the factors regulating the stability of Earth's early climate in the face of 'faint young Sun' is a central problem in the geosciences and planetary science, with important implications for the long-term maintenance of habitability on Earth and Earth-like planets. This 'Faint Young Sun Paradox', which remains somewhat enigmatic, is further exacerbated by the potential for severely restricted primary productivity by the primitive photosynthetic biosphere. Here, we focus on a novel mechanism for stabilizing the climate system before the advent of oxygenic photosynthesis via a hybrid ecosystem of primitive photosynthetic metabolisms. Our global redox balance model demonstrates that for H2-based or Fe-based photosynthetic biospheres the electron donor (H2 and Fe2+) fluxes from the solid Earth required to attain warm climate states are extremely high, and may require geophysical conditions that deviate beyond those of the modern or even ancient Earth-such as elevated heat flow and volcanic degassing, lower mantle oxygen fugacity or pervasively ultramafic crustal compositions. However, we also found that the hybrid ecosystem of H2-based and Fe2+-based anoxygenic photoautotrophs yield warm climate solutions at relatively modest H2/Fe2+ fluxes well within those attainable on the Archean Earth system because of a strong nonlinear amplification of Earth's methane cycle. Our results imply an intriguing series of unexplored climate feedbacks within the coupled H-C-Fe cycles, opening entirely new vistas for future work to better understand the evolution of Earth's early climate system and the evolution of habitable planets more broadly.