Recent headlines suggested that we may discover life on Mars soon. We don’t know whether or not that will happen, but the search is on. In  2020, there will be two landmark missions to Mars: NASA’s Mars 2020 and ESA’s ExoMars. Both efforts will search for signs of present or past life on Mars. Other missions to search for evidence of extraterrestrial life are in various stages of planning. Dragonfly is a large robotic motorcraft that will be deployed on Titan (Saturn's largest moon). Dragonfly will study prebiotic chemistry and extraterrestrial habitability. NASA’s Europa Clipper and ESA’s Jupiter Icy Moons Explorer will investigate the potential habitability of Jupiter’s moons Europa, Callisto, and Ganymede

Space missions are expensive, take many years to develop, and are risky. How do the people who design these missions know what to do and how to do it? Where should they look? How do they identify not only which planet or moon to explore, but exactly where on that planet or moon should they survey from orbit and the ground? What kind of geology should they target? What chemicals or minerals might indicate the possibility of life? What tools do they need to find these so-called biosignatures? What exploration strategies will be most successful and what operational templates will be most efficient? Can AI help?

This month, Dr. Nathalie A. Cabrol, Director of the Carl Sagan Center at the SETI Institute, is leading a team of scientists, engineers, roboticists, and students into remote areas of Chile. Their mission is to find out what we can learn about life and habitability in extreme terrestrial environments and how this knowledge can be applied to the search for life beyond Earth. The NASA Astrobiology Institute is supporting the expedition, which will help prepare missions such as Mars 2020 and ExoMars in their search for biosignatures.  The team will examine microbial habitats in arid locations, at high altitude, and in extremely elevated levels of ultraviolet radiation. Part of what they want to learn is whether they can identify patterns that could help mission teams to detect "stealth" microbial life. There are patterns to habitability and life habitats and they happen to be fractal in nature (repeatable at various scales). However, pattern identification is more challenging when surface conditions are harsh and resources for life scarce. If such patterns exist for extremophiles (microbial life living in extreme environments), then learning what they are could help us develop and train detection algorithms for AI technologies. This would enable AI to help identify areas where the probability of finding past or present evidence of life could be higher than in others. Understanding what geological, mineralogical, and physicochemical conditions are required for microhabitats and life is, however, only half the question. The team also wants to learn how life impacts and transforms the environment around it, which could provide additional clues for exploring other planets. New instruments, tools, and methods to advance the search of life beyond Earth will also be tested.  

The team will return to several areas from past expeditions to confirm hypotheses formed on previous visits. Additionally, they will collect new data and develop ideas for possible future research in support of the search for life. To achieve their science objectives, they will go to locations that are analog to potential ancient Martian habitats for microbial life. These include ancient dry lake beds (such as Salar de Pajonales and Laguna Lejía), hydrothermal systems (such as El Tatio), and microbial habitats exposed to a high UV environment (such as the summit lake of the Simba Volcano). These sites are all at high altitudes, ranging from about 3,554 meters up to 5,940 meters. Studying the habitats and microbial life in these locations is similar to going back in time on Mars about 3.9 to 3.5 billion years ago, when the planet experienced a critical environmental transition and lost its atmosphere and became arid and hostile at the surface.

The team began to gather in Antofagasta, Chile, on October 15, and the expedition will continue until November 7. More team members will be joining the journey later, and some are still traveling. So far, the group includes:

• Nathalie Cabrol, Director of the Carl Sagan Center at the SETI Institute and team leader
• Kimberly Warren-Rhodes, an astrobiologist, and ecologist at the SETI Institute
• Kevin Rhodes, Coastal Fisheries Coordinator, MarAlliance
• Evan Eshelman, Senior Research Scientist, Impossible Sensing
• Nancy Hinman, Professor of Geosciences, University of Montana
• Claire Mondro, PhD candidate, planetary geoscience, University of Tennessee
• Jeff Moersch, Professor in the Department of Earth and Planetary Sciences and Director of the Planetary Geoscience Institute at the University of Tennessee, Knoxville
• Michael Phillips, PhD candidate, planetary geoscience, University of Tennessee
• Michael McInenly, MS candidate - shallow sub-surface geophysics - University of Montana
• Cinthya Jafet Tebes Cayo, PhD candidate in science with a mention in geology, biochemist, Universidad Católica del Norte, Antofagasta, Chile

The expedition team is highly experienced. Some members have been conducting research in Chile for up to 17 years. As they begin to lay out their work plans, they are well-prepared to address their first challenge. The shipment of science equipment has been delayed, which means everyone must adapt their strategies and adjust their schedules to ensure they will be able to accomplish as much as possible as soon as the team arrives at the first site. As a result, the extra time in Antofagasta is being used to fine-tune the last logistical details and develop a step-by-step activity plan for the various groups for once the team arrives in the field. Preparation includes identifying drill sequences, reconnaissance for microbial sampling, and flight planning. The team’s plan is, as of today, to leave Antofagasta and head for the Atacama and Altiplano tomorrow. Hopefully, the shipment won’t be too far behind – but everybody has enough in their personal equipment to get started so... stay tuned!