Around 2.4 billion years ago (Ga), a toxic byproduct of an ancient ecological catastrophe poisoned the entire planet, specifically the anaerobic life that had dominated early Earth. The lethal element is one our existence depends on: oxygen.
We often talk about what makes us alive, but we rarely question what allowed us to be alive. Cyanobacteria were pivotal to our existence. They were the first organisms to undergo photosynthesis, releasing oxygen that accumulated in the atmosphere, poisoning early Earth but also setting the conditions that allowed human existence. This ecological catastrophe is called the Great Oxidation Event (GOE) (West, 2022).
However, what evidence indicates that this event happened and that Earth’s atmosphere changed around 2.4 Ga?
The GOE
Cyanobacteria emerged around 2.7–3 Ga and began producing oxygen through photosynthesis, which accumulated over around 500 million years . As cyanobacteria released O2, chemical reactions immediately consumed it. Around 2.4 Ga, these chemical “sinks” became saturated and could no longer consume oxygen as quickly. This caused atmospheric O2 levels to rise. (Aiyer, 2022; West, 2022).
Evidence:
Banded Iron Formations (BIF’s)
Before the GOE, oceans were anoxic and contained massive amounts of dissolved iron in its reduced form, Fe^2+. Following the GOE, as free oxygen seeped into oceans, it reacted with iron and oxidized it to Fe^3+, making it insoluble. The oxidized iron precipitated onto the seafloor as minerals like magnetite. Banded Iron Formations (BIFs) formed striped layers of magnetite in red-tinted colours alternating with silica in the oceans and, over time, created the striped rocks present now . This was a visual indicator that the world was once completely devoid of free oxygen, and that it changed after the GOE (Canfield et al., 2013; West, 2022).
Rock Dating
Prior to the GOE, terrestrial rocks contained reduced iron with grey-green colouration. Similarly to the BIF’s, after the GOE, Fe was oxidized, and the colours obtained a red-orange formation, named “Red Beds”, which arose in the geological record around 2.4 Ga (Shawwa et al., 2024).
Earth’s temperature
Before the GOE, the atmosphere contained massive amounts of methane produced by methanogenic archaea. Methane is a greenhouse gas that kept early Earth extremely warm, even though our Sun was 25% dimmer 2.4 Ga than it is today. The formation of hydroxyl (OH-) oxidized methane, which caused it to disappear from the atmosphere rapidly. After that, the Earth’s climate crashed into global glaciation around 2.3 Ga, the “Huronian Glaciation”, one of the earliest “snowball Earth” events. This drastic climate shift is indirect evidence of the mass extinction of anaerobic methanogens (Canfield et al., 2013).
Ozone Layer & MIF-S
The disappearance of the Mass-Independent Fractionation of Sulfur (MIF-S) signal, which existed only if no ozone layer was present, around 2.4 Ga also marked a critical threshold: atmospheric oxygen had reached high enough levels to form a protective ozone layer. This ozone shield stopped the UV-driven chemistry that created the MIF-S signature in older rocks, allowing us to date when an ozone layer was established (Crockford et al., 2026).
So, yes, Earth was poisoned by oxygen around 2.4 Ga. While catastrophic for much of the anaerobic life that dominated the planet, this event changed life’s trajectory. The same “lethal toxin” that caused the mass extinction of an ancient biosphere became the most efficient fuel that powers the most complex forms of life.
Refrences
Aiyer, Kartik. “The Great Oxidation Event: How Cyanobacteria Changed Life.” ASM (2022). https://asm.org/articles/2022/february/the-great-oxidation-event-how-cyanobacteria-change. Accessed September 20, 2026
Crockford, P. W., I. Sugiyama, M. A. Kipp, J. Hao, L. L. Nelson, J. D. Hemingway, S. Wimmer, and M. Fakhraee. 2026. “Revisiting the Greatness of Earth’s Great Oxidation.” Communications Earth & Environment 7, no. 1 (2026): 348.
https://doi.org/10.1038/s43247-026-03518-8 Accessed September 20, 2026
D. E. Canfield et al., “Oxygen dynamics in the aftermath of the Great Oxidation of Earth’s atmosphere,” Proceedings of the National Academy of Sciences of the United States of America 110, no. 42 (2013): 16736–16741, https://doi.org/10.1073/pnas.1315570110. Accessed September 20, 2026
Shawwa, Nabil A., Thomas R. McLoughlin-Coleman, Michael G. Babechuk, Maryam Shahabi Far, James E. Mungall, and Robert H. Rainbird. 2024. “Earth’s Oldest Terrestrial Red Beds as Direct Evidence for the Great Oxidation Event ca. 2.3 Ga.” Precambrian Research 409, article 107423.
https://doi.org/10.1016/j.precamres.2024.107423 Accessed September 20,2026
Wang, Haiyang, and Chao Li. 2026. “Stagewise Oxygenation of the Earth’s Atmosphere and Oceans.” The Innovation 7, no. 9: 101353.
https://doi.org/10.1016/j.xinn.2026.101353 Accessed September 20, 2026
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