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Martian Water Guarantees Nothing

  • Posted by Peter Glatzer on October 6, 2015 in Science/Tech
  • NASA scientists announced today the best evidence yet that Mars, once thought dry, sterile and dead, may yet have life in it: Liquid water still flows on at least some parts of the Red Planet, seeping from slopes to accumulate in what might be life-nurturing pools at the bases of equatorial hills and craters. These remarkable sites on Mars may be the best locations in the solar system to search for extant extraterrestrial life—but doing so will be far from easy.

    Examining potentially habitable regions of Mars for signs of life is arguably the primary scientific justification for sending humans there—but according to a new joint review from the National Academy of Sciences and the European Science Foundation, we are not presently prepared to do so.

    The problem is not exploding rockets, shrinking budgets, political gamesmanship or fickle public support—all the usual explanations spaceflight advocates offer for the generations-spanning lapse in human voyages anywhere beyond low Earth orbit. Rather, the problem is life itself—specifically, the tenacity of Earthly microbes, and the potential fragility of Martian ones. The easiest way to find life on Mars, it turns out, may be to import bacteria from Cape Canaveral—contamination that could sabotage the search for native Martians. The need to protect any possible Martian biosphere from Earthly contamination, the review’s authors wrote, could “prevent humans from landing in or entering areas” where Martian life might thrive. Although this sentiment is not new, its frank, formal acknowledgement in such an authoritative study is rare indeed. NASA is planning to send humans to Mars as soon as the 2030s; that such missions may unavoidably pose extreme contamination risks is understandably not something the agency is eager to highlight, even as it actively researches possible solutions to the problem.

    Historically, in the context of Mars such “planetary protection” has primarily concerned robotic exploration. The risk of contamination is an issue even for machines, which, unlike humans, can endure being fried with radiation and bathed in harsh chemicals prelaunch to eradicate bacterial stowaways. Microbes that stubbornly refuse to die nonetheless turn up with regularity in NASA’s supposedly sterile clean rooms for preparing interplanetary spacecraft. Apollo astronauts even found bacteria on the moon that had survived an almost total vacuum inside the robotic Surveyor 3 lander that had touched down more than two and a half years earlier. If terrestrial microbes could live in places like that, why not in some of the more habitable parts of Mars?

    The United Nations Outer Space Treaty of 1967 forbids the “harmful contamination” of other worlds with Earth’s biology, and an international organization called COSPAR (the Committee on Space Research) sets the planetary protection protocols for the U.S., Europe, Russia and other signatory spacefaring nations to follow. To protect Mars, since 2002 COSPAR has designated restricted “Special Regions” on the planet where conditions are warm and wet enough to possibly support extant Martian life—or to allow Earthly invaders to gain a flagella-hold. Because of rapid, ongoing progress in our knowledge of the Martian environment and the fundamental limits of Earthly biology, the precise definitions for Special Regions remain works in progress that are officially revisited every two years. The new joint review, released last week, recommends revisions to the findings of a 2014 report on COSPAR’s Special Regions from NASA’s Mars Exploration Program Analysis Group.

    The closer planetary scientists look at Mars, the more Special Regions they think they see. Special Regions pepper the planet’s equator and mid-latitudes, in eroded gullies and in steep, rocky slopes of hills and craters, where new evidence published September 28 in Nature Geoscience indicates that briny water flows and pools from aquifers during Martian summers. Special Regions can also be found in caves, beneath the polar ice caps and in geothermal hotspots of seismic or volcanic activity. As little as five meters below the surface, where groundwater may persist as ice, vast areas of the planet could be considered a Special Region, just waiting to be transformed into a welcoming, watery microbial Eden by the heat from a new-formed impact crater or the operations of a recently arrived spacecraft. Special Regions should also exist, the new review notes, at the still-unknown sources of mysterious methane emissions recently detected on Mars. On Earth it is generated chiefly by microbes but detectable quantities of the gas could also arise on Mars from abiotic sources, although those lifeless production routes would also require liquid water.

    Via Salon

    Written By Lee Billings

    Originally published in The Scientific American






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