4.6 Article

Distinguishing Biotic vs. Abiotic Origins of 'Bio'signatures: Clues from Messy Prebiotic Chemistry for Detection of Life in the Universe

Journal

LIFE-BASEL
Volume 13, Issue 3, Pages -

Publisher

MDPI
DOI: 10.3390/life13030766

Keywords

origin of life; search for extraterrestrial life; prebiotic chemistry; abiosignatures; nonenzymatic reactions; astrobiology

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It is crucial for researchers to consider the abiotic origin of potential biosignatures when searching for extraterrestrial life. Prebiotic chemistry, which studies enzyme-free chemical syntheses, can help in analyzing whether perceived 'signatures of life' could have chemical origins. The knowledge gained from understanding the transition from chemistry to biology during the origin of life can be used to create a library of abiotically synthesized biologically relevant organic molecules, aiding in the design and testing of instruments for future explorations.
It is not a stretch to say that the search for extraterrestrial life is possibly the biggest of the cosmic endeavors that humankind has embarked upon. With the continued discovery of several Earth-like exoplanets, the hope of detecting potential biosignatures is multiplying amongst researchers in the astrobiology community. However, to be able to discern these signatures as being truly of biological origin, we also need to consider their probable abiotic origin. The field of prebiotic chemistry, which is aimed at understanding enzyme-free chemical syntheses of biologically relevant molecules, could particularly aid in this regard. Specifically, certain peculiar characteristics of prebiotically pertinent messy chemical reactions, including diverse and racemic product yields and lower synthesis efficiencies, can be utilized in analyzing whether a perceived 'signature of life' could possibly have chemical origins. The knowledge gathered from understanding the transition from chemistry to biology during the origin of life could be used for creating a library of abiotically synthesized biologically relevant organic molecules. This can then be employed in designing, standardizing, and testing mission-specific instruments/analysis systems, while also enabling the effective targeting of exoplanets with potentially 'ongoing' molecular evolutionary processes for robust detection of life in future explorative endeavors.

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