Active methanogenesis during the melting of Marinoan snowball Earth

马里诺冰球地球融化期间活跃的甲烷生成作用

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Abstract

Geological evidence indicates that the deglaciation of Marinoan snowball Earth ice age (~635 Myr ago) was associated with intense continental weathering, recovery of primary productivity, transient marine euxinia, and potentially extensive CH(4) emission. It is proposed that the deglacial CH(4) emissions may have provided positive feedbacks for ice melting and global warming. However, the origin of CH(4) remains unclear. Here we report Ni isotopes (δ(60)Ni) and Yttrium-rare earth element (YREE) compositions of syndepositional pyrites from the upper most Nantuo Formation (equivalent deposits of the Marinoan glaciation), South China. The Nantuo pyrite displays anti-correlations between Ni concentration and δ(60)Ni, and between Ni concentration and Sm/Yb ratio, suggesting mixing between Ni in seawater and Ni from methanogens. Our study indicates active methanogenesis during the termination of Marinoan snowball Earth. This suggests that methanogenesis was fueled by methyl sulfides produced in sulfidic seawater during the deglacial recovery of marine primary productivity.

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