Diversity-Based Biosignatures from Molecular Assemblages for Planetary Life Detection

To the point

Gideon Yoffe, Fabian Klenner, Barak Sober, Yohai Kaspi, and Itay Halevy present a biosignature based on the statistical organization and diversity of molecular assemblages to interpret planetary mission data, showing that biotic amino-acid and fatty-acid diversity exceeds abiotic diversity and remains detectable after space-like degradation, using only relative abundances and applicable to archived, current, and planned missions.

Molecular diversity as a biosignature
arxiv.org

Molecular diversity as a biosignature

The search for life in the Solar System hinges on data from planetary missions. Detecting biosignatures based on molecular identity, isotopic composition, or chiral excess requires measurements that current and planned missions can only partially provide. We introduce a new class of biosignatures, defined by the statistical organization of molecular assemblages and quantified using diversity metrics. Using this framework, we analyze amino-acid diversity across a dataset spanning terrestrial and extraterrestrial contexts. We find that biotic samples are consistently more diverse -- and therefore distinct -- from their sparser abiotic counterparts. This distinction also holds for fatty acids, indicating that the diversity signal reflects a fundamental biosynthetic signature. It also proves persistent under modeled space-like degradation. Relying only on relative abundances, this biogenicity assessment strategy is applicable to any molecular composition data from archived, current, and planned planetary missions. By capturing a fundamental statistical property of lifes chemical organization, it may also transcend biosignatures that are contingent on Earths evolutionary history.