Mars harbors gypsum deposits that may conceal traces of ancient microbial life, potentially resembling the earliest life forms on Earth from four billion years ago. Detecting these biosignatures requires highly precise instruments capable of operating in space environments. Researchers at the University of Bern have tested a miniaturized, laser-powered mass spectrometer on Earth and confirmed its effectiveness in identifying microbial fossils.
The team demonstrated that LIMS is capable of detecting biosignatures in terrestrial gypsum deposits that were formed under conditions similar to those found on Mars. The findings open up new possibilities for utilizing the instrument in upcoming Mars exploration missions. The study, led by Youcef Sellam of the University of Bern's Division of Space Research and Planetology, has been published in Frontiers in Astronomy and Space Science.
Mars presents a unique set of environmental conditions that could influence the long-term preservation of biosignatures. Sellam noted, "Deposits similar to those in Algeria, located in what were once Martian seas, represent promising sites for astrobiological research and the search for evidence of life on Mars."
The study also highlights Algeria's contribution to planetary science. In addition to providing key geological samples, the Algerian University of Science and Technology Houari Boumediene contributed valuable expertise. "This marks Algeria's first astrobiological study," Sellam added. "As an Algerian researcher, I am particularly proud to help enhance Algeria's role in planetary science and the broader scientific community."
Peter Wurz, Professor of Astrophysics at the University of Bern and LIMS project leader, emphasized the significance of these findings: "This study confirms that LIMS is highly effective in detecting biosignatures in sulfate minerals such as gypsum. The technology is now ready for integration into future Mars rovers and landers for on-site analysis."
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