Star Superflares: Warming Planets and Synthesizing Amino Acids express

Original: "Proton Irradiation of Primitive Atmospheres of Young Exoplanets and early Earth: $$N_{\mathrm{2}}O$$ Greenhouse Warming and Prebiotic Synthesis"
arXiv:2603.18206 · 2026-03-18 · CC BY 4.0 · 1 min
Experiments show: stellar particles, like a cosmic chef, turn simple gases into a potent greenhouse gas and the building blocks of life.

The young Sun shone 30% dimmer, yet the oceans didn't freeze. The answer: superflares, which bombarded the atmosphere with streams of energetic particles. A lab experiment recreated this: a nitrogen and carbon dioxide mix under particle bombardment yielded nitrous oxide and glycine — a building block of proteins. Think of the atmosphere as a pot, and stellar particles as the chef, cooking a 'broth' for climate and life from simple gases. Each powerful flare could produce up to 20 billion kilograms of nitrous oxide per year — enough to form a tight 'lid' on the planetary pot.

Young stars like our Sun in its youth emit superflares almost daily, hundreds of times more powerful than today's.

Nitrous oxide is a greenhouse gas 300 times stronger than CO2. It trapped the faint Sun's heat, preventing Earth from freezing. The same mechanism widens the habitable zone for rocky exoplanets, where ordinary stellar heat is insufficient. Alongside, amino acids, life's building blocks, are born. So a cosmic storm, usually seen as a threat, may have kickstarted the chemistry of life on Earth.

Each powerful flare on a young star could produce up to 20 billion kilograms of nitrous oxide per year — enough to warm a whole planet's atmosphere.

The idea of warming a planet with greenhouse gases is familiar from Kim Stanley Robinson's 'Red Mars' trilogy. Only there, it's human engineers; here, it's the star itself.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterDavid Charbonneau
Concepts
protoplanetary disk chemistry hot jupiter atmospheres first stars nucleosynthesis exoplanet atmospheres protoplanetary disk prebiotic chemistry hydrogen atmosphere sulfur dioxide young star first stars gas cold gas planetary formation nucleosynthesis origin of life stellar flares exoplanet atmosphere early universe metal enrichment titanium oxide planetary composition formation methanol