Light to life: Photochemical processes drove the cycling of bio-essential nutrients on the early Earth

<p indent="0mm">The Archean Eon witnessed the initiation of the co-evolution of geosphere and biosphere, which was potentially linked by the geochemical cycles of nutrient elements. However, the distinctive environmental conditions should have resulted in vastly different geochemical cycles of the nutrients and thus their availability on the early Earth. Here, we overview the current understanding of Archean geochemical cycles and availability of nutrients, especially those thought to limit the origin and productivity of early life. Particularly, we emphasize some recent advances on the large impacts of photochemistry in early nutrients′ cycles and assess the potentially important roles of photogeochemistry in the co-evolution of environment and biology on the early Earth. At the end, we advocate for more attention to the role of photochemistry in planetary habitability, including the early Earth, Mars, and other planetary bodies.

Authors

Publication Details

Journal
Bulletin of Mineralogy Petrology and Geochemistry
Published
2024-12-11
DOI
https://doi.org/10.3724/j.issn.1007-2802.20240141
Primary Topic
Origins and Evolution of Life
Type
article
Field-Weighted Citation Impact
0.00
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article

Light to life: Photochemical processes drove the cycling of bio-essential nutrients on the early Earth

Yuke Zhu, Fang Huang, Jihua Hao, Xing Cui et al.
Bulletin of Mineralogy Petrology and Geochemistry
Origins and Evolution of Life
article

Light to life: Photochemical processes drove the cycling of bio-essential nutrients on the early Earth

Yuke Zhu, Fang Huang, Jihua Hao, Xing Cui, Jie Li, Haotian Guo, Jiye Guo, Zongbin Zhang, J.U. Mondal, Y.Z. SONG
article en

Abstract

<p indent="0mm">The Archean Eon witnessed the initiation of the co-evolution of geosphere and biosphere, which was potentially linked by the geochemical cycles of nutrient elements. However, the distinctive environmental conditions should have resulted in vastly different geochemical cycles of the nutrients and thus their availability on the early Earth. Here, we overview the current understanding of Archean geochemical cycles and availability of nutrients, especially those thought to limit the origin and productivity of early life. Particularly, we emphasize some recent advances on the large impacts of photochemistry in early nutrients′ cycles and assess the potentially important roles of photogeochemistry in the co-evolution of environment and biology on the early Earth. At the end, we advocate for more attention to the role of photochemistry in planetary habitability, including the early Earth, Mars, and other planetary bodies.

Bulletin of Mineralogy Petrology and GeochemistryVol. 44(5)
Openalex Percentile: Top 83%
Origins and Evolution of Life
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