Renaissance for magnetotactic bacteria in astrobiology

Author:

Shen Jianxun12ORCID,Paterson Greig A3ORCID,Wang Yinzhao4ORCID,Kirschvink Joseph L56ORCID,Pan Yongxin127ORCID,Lin Wei12ORCID

Affiliation:

1. Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences , Beijing 100029, China

2. France-China Joint Laboratory for Evolution and Development of Magnetotactic Multicellular Organisms, Chinese Academy of Sciences , 100029 Beijing, China

3. Department of Earth, Ocean and Ecological Sciences, University of Liverpool , Liverpool L69 7ZE, UK

4. State Key Laboratory of Microbial Metabolism, School of Life Sciences and Biotechnology, Shanghai Jiao Tong University , Shanghai 200240, China

5. Division of Geological & Planetary Sciences, Calfiornia Institute of Technology , Pasadena, CA 91125, USA

6. Marine Core Research Institute, Kochi University , Kochi 780-8520, Japan

7. College of Earth and Planetary Sciences, University of Chinese Academy of Sciences , Beijing 100049, China

Abstract

Abstract Capable of forming magnetofossils similar to some magnetite nanocrystals observed in the Martian meteorite ALH84001, magnetotactic bacteria (MTB) once occupied a special position in the field of astrobiology during the 1990s and 2000s. This flourish of interest in putative Martian magnetofossils faded from all but the experts studying magnetosome formation, based on claims that abiotic processes could produce magnetosome-like magnetite crystals. Recently, the rapid growth in our knowledge of the extreme environments in which MTB thrive and their phylogenic heritage, leads us to advocate for a renaissance of MTB in astrobiology. In recent decades, magnetotactic members have been discovered alive in natural extreme environments with wide ranges of salinity (up to 90 g L−1), pH (1–10), and temperature (0–70 °C). Additionally, some MTB populations are found to be able to survive irradiated, desiccated, metal-rich, hypomagnetic, or microgravity conditions, and are capable of utilizing simple inorganic compounds such as sulfate and nitrate. Moreover, MTB likely emerged quite early in Earth’s history, coinciding with a period when the Martian surface was covered with liquid water as well as a strong magnetic field. MTB are commonly discovered in suboxic or oxic-anoxic interfaces in aquatic environments or sediments similar to ancient crater lakes on Mars, such as Gale crater and Jezero crater. Taken together, MTB can be exemplary model microorganisms in astrobiology research, and putative ancient Martian life, if it ever occurred, could plausibly have included magnetotactic microorganisms. Furthermore, we summarize multiple typical biosignatures that can be applied for the detection of ancient MTB on Earth and extraterrestrial MTB-like life. We suggest transporting MTB to space stations and simulation chambers to further investigate their tolerance potential and distinctive biosignatures to aid in understanding the evolutionary history of MTB and the potential of magnetofossils as an extraterrestrial biomarker.

Publisher

Oxford University Press (OUP)

Subject

Ecology, Evolution, Behavior and Systematics,Microbiology

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