In situ identification of Palaeoarchaean biosignatures using co-located Perseverance rover analyses: perspectives for in situ Mars science and sample return

Hickman-Lewis, Keyron and Moore, K.R. and Razzell Hollis, J.J. and Tuite, M.L. and Beegle, L.W. and Bhartia, R. and Grotzinger, J.P. and Brown, A.J. and Shkolyar, S. and Cavalazzi, B. and Smith, C.L. (2022) In situ identification of Palaeoarchaean biosignatures using co-located Perseverance rover analyses: perspectives for in situ Mars science and sample return. Astrobiology 22 (9), pp. 1143-1163. ISSN 1531-1074.

Abstract

The NASA Mars 2020 Perseverance rover is currently exploring Jezero crater, a Noachian–Hesperian locality that once hosted a delta–lake system with high habitability and biosignature preservation potential. Perseverance conducts detailed appraisals of rock targets using a synergistic payload capable of geological characterization from kilometer to micron scales. The highest-resolution textural and chemical information will be provided by correlated WATSON (imaging), SHERLOC (deep-UV Raman and fluorescence spectroscopy), and PIXL (X-ray lithochemistry) analyses, enabling the distributions of organic and mineral phases within rock targets to be comprehensively established. Herein, we analyze Paleoarchean microbial mats from the *3.42 Ga Buck Reef Chert (Barberton greenstone belt, South Africa)—considered astrobiological analogues for a putative ancient martian biosphere—following a WATSON–SHERLOC–PIXL protocol identical to that conducted by Perseverance on Mars during all sampling activities. Correlating deep-UV Raman and fluorescence spectroscopic mapping with X-ray elemental mapping, we show that the Perseverance payload has the capability to detect thermally and texturally mature organic materials of biogenic origin and can highlight organic–mineral interrelationships and elemental colocation at fine spatial scales. We also show that the Perseverance protocol obtains very similar results to high-performance laboratory imaging, Raman spectroscopy, and mXRF instruments. This is encouraging for the prospect of detecting microscale organicbearing textural biosignatures on Mars using the correlative micro-analytical approach enabled by WATSON, SHERLOC, and PIXL; indeed, laminated, organic-bearing samples such as those studied herein are considered plausible analogues of biosignatures from a potential Noachian–Hesperian biosphere. Were similar materials discovered at Jezero crater, they would offer opportunities to reconstruct aspects of the early martian carbon cycle and search for potential fossilized traces of life in ancient paleoenvironments. Such samples should be prioritized for caching and eventual return to Earth. Key Words: Mars—Astrobiology— Mars 2020—Biosignatures—Buck Reef Chert—Microbial mats. Astrobiology 22, xxx–xxx.

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