
It provides a proven, planet‑wide biosignature that can guide future Mars and exoplanet missions, while deepening our understanding of early biosphere chemistry.
Nitrogen fixation underpins the entire biosphere, converting inert atmospheric N₂ into bioavailable forms essential for proteins and DNA. The enzyme nitrogenase, present in a diverse set of bacteria, archaea, and a few eukaryotes, is the molecular workhorse of this process. By resurrecting a 3.2‑billion‑year‑old version of nitrogenase, scientists have opened a window onto the metabolic landscape of Earth’s earliest microbes, offering a tangible link between ancient biochemistry and the rock record.
The research team employed synthetic biology to peel back evolutionary layers, reconstructing ancestral nitrogenase genes and inserting them into modern microbes. Laboratory assays showed that, despite substantial sequence and structural differences, these ancient enzymes produced the same nitrogen‑isotope fractionation as their modern counterparts. This consistency confirms that the N‑isotope signature preserved in sedimentary rocks faithfully records ancient diazotrophic activity, settling long‑standing doubts about its reliability as a biosignature.
For astrobiology, the implications are profound. A validated, universal biosignature means future rover and lander missions can target nitrogen‑isotope anomalies on Mars or icy moons, potentially uncovering evidence of extinct metabolisms that differ from today’s life. Moreover, the study refines models of early Earth’s nitrogen cycle, informing climate and habitability simulations for exoplanets. As NASA and international partners design next‑generation life‑search instruments, nitrogen isotopes stand out as a robust, chemically grounded tool for detecting life’s ancient fingerprints across the solar system.
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