Habitable Zones & Global Climate

Coevolution Of Primitive Methane Cycling Ecosystems And Early Earth Atmosphere And Climate

By Keith Cowing
Press Release
June 11, 2020
Filed under
Coevolution Of Primitive Methane Cycling Ecosystems And Early Earth Atmosphere And Climate
Long-term effect of the carbon cycle on the biogeochemical response of the early Archean Earth to changes in H<sub>2</sub> volcanic outgassing, abiotic temperature (T<sub>Geo</sub>) and ecosystem composition. Here T<sub>Geo</sub> is determined by <sub>p</sub>CO<sub>2</sub> in the climate model. Left, Atmospheric <sub>p</sub>CH<sub>4</sub> at ecosystem-climate equilibrium. Shaded areas indicate conditions for organic haze formation (<sub>p</sub>CH<sub>4</sub>:<sub>p</sub>CO<sub>2</sub> > 0.2). Right, Temperature differential between T<sub>Geo</sub> and the global surface temperature reached at ecosystem-climate equilibrium, T<sub>BioGeo</sub> . Shaded areas indicate conditions leading to glaciation (T<sub>BioGeo</sub> < 0°C). Other parameters are fixed to their default values (Supplementary Tables 2 and 3).

The history of the Earth has been marked by major ecological transitions, driven by metabolic innovation, that radically reshaped the composition of the oceans and atmosphere.

The nature and magnitude of the earliest transitions, hundreds of million years before photosynthesis evolved, remain poorly understood. Using a novel ecosystem-planetary model, we find that pre-photosynthetic methane-cycling microbial ecosystems are much less productive than previously thought. In spite of their low productivity, the evolution of methanogenic metabolisms strongly modifies the atmospheric composition, leading to a warmer but less resilient climate.

As the abiotic carbon cycle responds, further metabolic evolution (anaerobic methanotrophy) may feed back to the atmosphere and destabilize the climate, triggering a transient global glaciation. Although early metabolic evolution may cause strong climatic instability, a low CO:CH4 atmospheric ratio emerges as a robust signature of simple methane-cycling ecosystems on a globally reduced planet such as the late Hadean/early Archean Earth.

Boris Sauterey, Benjamin Charnay, Antonin Affholder, Stéphane Mazevet, Régis Ferrière

Comments: 32 pages, 5 figures, 1 tables, 12 Supplementary figures, published in Nature Communications
Subjects: Populations and Evolution (q-bio.PE); Earth and Planetary Astrophysics (astro-ph.EP)
Journal reference: Nat. Commun. 11, 2705 (2020)
DOI: 10.1038/s41467-020-16374-7
Cite as: arXiv:2006.06433 [q-bio.PE] (or arXiv:2006.06433v1 [q-bio.PE] for this version)
Submission history
From: Boris Sauterey
[v1] Tue, 9 Jun 2020 14:02:55 UTC (9,447 KB)

Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻