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Dark microbiome and extremely low organics in Atacama fossil delta unveil Mars life detection limits.

Armando Azua-BustosAlberto G FairénCarlos González-SilvaOlga Prieto-BallesterosDaniel CarrizoLaura Sánchez-GarcíaVictor ParroMiguel Ángel Fernández-MartínezCristina EscuderoVictoria Muñoz-IglesiasMaite Fernández-SampedroAntonio MolinaMiriam García VilladangosMercedes Moreno-PazJacek WierzchosCarmen AscasoTeresa FornaroJohn Robert BrucatoGiovanni PoggialiJose Antonio ManriqueMarco VenerandaGuillermo Lopez-ReyesAurelio Sanz-ArranzFernando RullAnn M OllilaRoger C WiensAdriana Reyes-NewellSamuel M CleggMaëva MillanSarah Stewart JohnsonOphélie McIntoshCyril SzopaCaroline FreissinetYasuhito SekineKeisuke FukushiKoki MoridaKosuke InoueHiroshi SakumaElizabeth B Rampe
Published in: Nature communications (2023)
Identifying unequivocal signs of life on Mars is one of the most important objectives for sending missions to the red planet. Here we report Red Stone, a 163-100 My alluvial fan-fan delta that formed under arid conditions in the Atacama Desert, rich in hematite and mudstones containing clays such as vermiculite and smectites, and therefore geologically analogous to Mars. We show that Red Stone samples display an important number of microorganisms with an unusual high rate of phylogenetic indeterminacy, what we refer to as "dark microbiome", and a mix of biosignatures from extant and ancient microorganisms that can be barely detected with state-of-the-art laboratory equipment. Our analyses by testbed instruments that are on or will be sent to Mars unveil that although the mineralogy of Red Stone matches that detected by ground-based instruments on the red planet, similarly low levels of organics will be hard, if not impossible to detect in Martian rocks depending on the instrument and technique used. Our results stress the importance in returning samples to Earth for conclusively addressing whether life ever existed on Mars.
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