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The Chemical Signature of Life: How to Find It by Its Elements ⚡ экспресс

Original: "Elemental Stoichiometry as an Ecological Biosignature with Applications to Life Detection"
arXiv:2605.19252 · 2026-05-19 · CC BY 4.0 · ⏱ 1 min · q-bio.BM Exoplanets q-bio.MN
Every living thing is marked with a unique chemical signature—the ratio of elements. It will help find life even in the most alien worlds.
Abstract

The chemical space of small molecules (estimated up to 10^60 compounds) is sparsely populated in biology. A concept for detecting an ecological signature—a statistical pattern of elemental composition, not individual compounds—has been proposed. Using Van Krevelen diagrams and power-law scaling, 11,834 metagenomic samples of microorganisms were analyzed. Enrichment in heteroatoms (P, S, N, O) relative to carbon, a shift toward higher O:C and H:C ratios, and sub-power-law scaling reflecting elemental constraints were revealed. These patterns statistically differ from 18,000 compounds in the synthetic Reaxys database and data from planetary missions, demonstrating the method's potential as a universal biosignature approach for mass spectrometry data in the search for extraterrestrial life.

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From carbon, nitrogen, oxygen, and sulfur, you can assemble 10⁶⁰ different small molecules—that's a 1 with 60 zeros, more than the stars in the visible universe. Life uses only a tiny fraction of this menu, but not randomly. In any living community, from bacteria to an oak grove, the element ratios shift in the same way: more oxygen and hydrogen, less carbon, and always a dash of sulfur and nitrogen. It's as if every living organism leaves an invisible signature in chemical ink.

Scientists tested this signature on thousands of samples—microbial communities, synthetic mixtures, even data from Mars missions. The picture is clear: living matter differs from non-living matter based solely on elemental composition. Just plot molecules as points with coordinates “oxygen-to-carbon” and “hydrogen-to-carbon,” and the cloud of living points always shifts up and to the right. A mass spectrometer onboard a rover can read such a signature in minutes.

The most surprising twist: this chemical signature is universal. It doesn't depend on specific proteins or DNA, so it's suitable for searching for any carbon-based life—even the most alien. We might already be able to recognize living material in extraterrestrial samples; we just didn't know where to look.

🎯 When analyzing Martian samples and meteorites, the 'living' signature hasn't been found yet—but now we know what it looks like.

🎬 In Star Trek, tricorders instantly recognized life. Our method is a real step toward such technology: a scanner only needs to measure the ratio of elements to distinguish life from non-living matter.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterCharles-Augustin de Coulomb
Tags
carbon hydrogen spectroscopy Water
Laws
Doppler effectCoulomb's lawMaxwell's equationsPlanck's lawPlanck–Einstein relationWien's displacement law
Original: arXiv:2605.19252 · CC BY 4.0 · bridge42worlds