Scientists find narrow oxygen range enabled life on Earth

Researchers at ETH Zurich have discovered that Earth formed with just the right amount of oxygen during its core development, keeping essential phosphorus and nitrogen accessible for life. Too much or too little oxygen would have trapped or lost these elements. The finding highlights a chemical 'Goldilocks zone' critical for habitability.

Planets start as molten rock, where materials separate by density. Heavy metals like iron sink to form the core, while lighter substances create the mantle and crust. Oxygen levels at this stage prove decisive for phosphorus and nitrogen availability, according to Craig Walton, a postdoc at ETH Zurich's Centre for Origin and Prevalence of Life, and professor Maria Schönbächler. About 4.6 billion years ago, Earth hit the perfect balance, Walton explained: 'During the formation of a planet's core, there needs to be exactly the right amount of oxygen present so that phosphorus and nitrogen can remain on the surface of the planet.' Phosphorus aids DNA, RNA, and cellular energy, while nitrogen forms proteins essential for life. Models by Walton and colleagues, published in Nature Astronomy, pinpoint a narrow moderate-oxygen range—termed a chemical Goldilocks zone—where both elements stay in the mantle in sufficient quantities. Walton added: 'Our models clearly show that the Earth is precisely within this range. If we had had just a little more or a little less oxygen during core formation, there would not have been enough phosphorus or nitrogen for the development of life.' Mars, by contrast, fell outside this zone, retaining more phosphorus but less nitrogen, complicating life prospects there. The study urges shifting exoplanet habitability assessments beyond water presence. Planets must retain these elements from core formation onward. Walton noted that stellar composition influences oxygen levels, as planets form from similar material. 'This makes searching for life on other planets a lot more specific. We should look for solar systems with stars that resemble our own Sun,' he said.

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Artistic rendering of the James Webb Space Telescope observing the atmosphere-shrouded molten super-Earth TOI-561 b near its host star.
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Webb telescope uncovers atmosphere on molten super-Earth TOI-561 b

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NASA's James Webb Space Telescope has detected signs of a thick atmosphere on the ultra-hot exoplanet TOI-561 b, challenging assumptions about such worlds. This rocky planet, orbiting its star in under 11 hours, shows lower temperatures and density than expected, suggesting a layer of gases above a magma ocean. The findings, published on December 11, highlight how intense radiation might not strip away all atmospheres from small, close-in planets.

Researchers at MIT have found evidence that some early life forms began using oxygen hundreds of millions of years before it accumulated in Earth's atmosphere. The study traces a key oxygen-processing enzyme to the Mesoarchean era, suggesting microbes consumed oxygen produced by cyanobacteria. This discovery challenges previous understandings of aerobic respiration's timeline.

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A supernova explosion near the forming solar system could explain the presence of key radioactive elements that influenced Earth's water content. Researchers suggest this process occurred at a safe distance, avoiding disruption to planet formation. The mechanism implies Earth-like planets might be common around sun-like stars.

Researchers are returning to the Clarion-Clipperton Zone in the Pacific Ocean to investigate how metallic nodules produce oxygen without sunlight, a phenomenon dubbed 'dark oxygen' that could sustain deep-sea life. This discovery has sparked debate over the environmental risks of deep-sea mining for critical metals. The team aims to confirm the process and address criticisms from mining interests.

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A new study suggests that Jupiter's moon Europa, long considered a prime candidate for extraterrestrial life due to its vast subsurface ocean, may lack the geological activity necessary to support living organisms. Researchers found that weak tidal forces from Jupiter result in a calm and inactive seafloor. This challenges hopes for habitable conditions beneath the moon's icy crust.

New research indicates that rising ocean temperatures may benefit Nitrosopumilus maritimus, a microbe essential for marine nutrient cycles. This archaea adapts by using iron more efficiently in warmer, nutrient-poor conditions, potentially sustaining ocean productivity. The findings, published in the Proceedings of the National Academy of Sciences, suggest these microbes could play a larger role in ocean chemistry amid climate change.

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New research indicates that salty, nutrient-rich ice on Europa could sink through the moon's icy shell to feed its hidden ocean, potentially supporting life. Geophysicists at Washington State University used computer simulations to show this process, inspired by Earth's crustal delamination. The findings address a key habitability challenge for the Jupiter moon.

 

 

 

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