The Origin of the Feedstock Molecules for Life on the Hadean Earth

The origin of life in the Hadean eon required the formation of amino acids and nucleosides among the key molecules of life. It is assumed that highly unsaturated carbon and nitrogen containing feedstock molecules, which form in a strongly reducing H<sub>2</sub>-atmosphere were the reactive starting materials. The Hadean Earth was, however, surrounded by a CO<sub>2</sub>-dominated atmosphere and the question of how under such inert conditions the biomolecules could have formed is unsolved. Here, we report that HNO and formaldehyde, which form robustly in a weakly reducing atmosphere by lightning and UV-irradiation, react with SO<sub>2</sub> to produce oxime, amidoxime, and nitrile-containing molecules, which react to give precursors to amino acids and all four canonical nucleosides. The small number of feedstock molecules required suggests that the molecules of life can robustly form on all types of rock planets with volcanic activity and a CO<sub>2</sub>-dominated atmosphere.

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Publication Details

Journal
Angewandte Chemie International Edition
Published
2025-09-01
DOI
https://doi.org/10.1002/anie.202512374
Primary Topic
Origins and Evolution of Life
Type
article
Field-Weighted Citation Impact
0.00

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article

The Origin of the Feedstock Molecules for Life on the Hadean Earth

Stefan Wiedemann, Thomas Carell, Jonas Feldmann, A. S. Mikheev et al.
Angewandte Chemie International Edition
Origins and Evolution of Life
article

The Origin of the Feedstock Molecules for Life on the Hadean Earth

Stefan Wiedemann, Thomas Carell, Jonas Feldmann, A. S. Mikheev, Sidney M. Becker, Nikolai Diukarev, Erik Boinowitz
article en

Abstract

The origin of life in the Hadean eon required the formation of amino acids and nucleosides among the key molecules of life. It is assumed that highly unsaturated carbon and nitrogen containing feedstock molecules, which form in a strongly reducing H<sub>2</sub>-atmosphere were the reactive starting materials. The Hadean Earth was, however, surrounded by a CO<sub>2</sub>-dominated atmosphere and the question of how under such inert conditions the biomolecules could have formed is unsolved. Here, we report that HNO and formaldehyde, which form robustly in a weakly reducing atmosphere by lightning and UV-irradiation, react with SO<sub>2</sub> to produce oxime, amidoxime, and nitrile-containing molecules, which react to give precursors to amino acids and all four canonical nucleosides. The small number of feedstock molecules required suggests that the molecules of life can robustly form on all types of rock planets with volcanic activity and a CO<sub>2</sub>-dominated atmosphere.

Angewandte Chemie International EditionVol. 64(42)
Ludwig-Maximilians-Universität München (DE)
European Commission, Deutsche Forschungsgemeinschaft, Volkswagen Foundation, Friedrich Naumann Stiftung, Horizon 2020, Elitenetzwerk Bayern
Openalex Percentile: Top 84%
Origins and Evolution of Life
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