Which Stars Can Give Birth to Life? The Answer's in the Color express

Original: "Abiogenesis on Different Star Types; a Dissipative Photochemical Perspective"
· Andrés Ledesma, Karo Michaelian
arXiv:2511.08624 · 2025-11-09 · CC BY 4.0 · 1 min
The first 'building blocks' of life were like sunscreen: they absorbed ultraviolet and turned it into heat, sparking the growth of complexity.

Life began with molecules akin to natural sunscreen — based on carbon, they soaked up the mild ultraviolet of the young Sun and turned it into heat. This way of dissipating energy wasn’t just heating: it made molecules self-organize, like chefs kneading structured dough out of a chaos of ingredients. But ultraviolet is a finicky tool. Soft light gently joined atoms; hard light snapped fledgling bonds.

It’s just like cooking: low flame leaves the dish raw, high flame burns it to a crisp.

Astronomers compared the rainbow fingerprints of starlight and found that only F, G, and massive K stars hit the ideal balance. But for intelligence to emerge, only G-type will do: that’s our Sun. Red dwarfs, which are the most abundant in the Galaxy, offer merely a smoldering warmth: their planets are likely barren. Now the search for habitable worlds zeroes in on yellow stars, and a telltale sign could be an ocean's unusual darkening in the ultraviolet.

About 20% of sunlike stars in the Galaxy may host planets with a suitable ultraviolet climate: that’s billions of chances for life.

Sci-fi writers love to populate planets around red dwarfs (like in Interstellar), but the new model shows: their light isn’t enough to ‘knead the molecular dough’ of life.

R = \frac{\Phi_{\text{soft}}}{\Phi_{\text{hard}}}
R — the star's suitability index for prebiotic chemistry; \Phi — the integrated ultraviolet flux in the soft (205-285 nm) and hard (<205 nm) ranges.
Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterDavid Charbonneau
Concepts
abiogenesis origin of life photochemistry prebiotic chemistry first stars sun like star photosynthesis population iii stars red dwarf habitability star biosignature detection biology habitability stellar atmosphere biomolecule stellar radiation energy extraction biophoton emission starlight cosmic dawn