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Planet's Air: Recipe from a Star ⚡ экспресс

Original: "Stellar control on atmospheric carbon chemistry, CO runaway, and organic synthesis on lifeless Earth-like planets"
arXiv:2601.05480v1 · 2026-01-09 · CC BY 4.0 · ⏱ 1 min · Exoplanets
Gases with carbon in the atmospheres of lifeless planets depend on the star and distance, astronomers have found.
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A rocky planet around another star is like a dish in an oven. The star sets the temperature: the farther away, the colder. The mix of gases with carbon in the air — carbon dioxide, carbon monoxide, methane — depends on the heat mode and the star's type (like our Sun or dimmer ones).

At the outer edge of the zone, where the light barely warms, a 'carbon monoxide collapse' occurs. The cleaner molecules OH stop working, and toxic CO floods the air to hundreds of times Earth's level.

Formaldehyde — a building block for sugars and amino acids — is best 'baked' around hot stars, just before the collapse. Telescopes like James Webb will analyze the light of distant worlds and find places where the recipe for life has almost come together.

On lifeless planets, formaldehyde can be millions of times more abundant than in Earth's air. It has no smell, but without it, you can't assemble sugars and amino acids — the foundation of all living things.

🎯 On lifeless planets, carbon monoxide can build up to levels hundreds of times higher than Earth's — all because of the star's light characteristics.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterAlbert Einstein
Tags
carbon exoplanet spectroscopy JWST Sun
Laws
Doppler effectgravitational lensingKepler's third lawMaxwell's equationsPlanck's lawPlanck–Einstein relation
Original: arXiv:2601.05480v1 · CC BY 4.0 · bridge42worlds