Searching for Life in Martian Water Will Be Very, Very Tricky
New evidence supports the hypothesis that present-day liquid water flows down these dark slopes on Mars, called recurring slope lineae.
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 from the National Academy of Sciences and the European Science Foundation, we are not presently prepared to do so.
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 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 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 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.
Carl Sagan famously mused that if life is ever found on the fourth rock from the sun, “Mars then belongs to the Martians, even if the Martians are only microbes.” In this view the planet would become a sacrosanct sanctuary, forever off-limits to encroaching humans. An holds that planetary protection efforts are futile, perhaps even naive: Thanks to likely contamination from earlier spacecraft, as well as ancient exchanges of material blasted between the planets by massive asteroid impacts, Mars has probably already experienced many waves of Earthly invaders—each of which could have been easily repulsed by any native, more adaptively fit biosphere.
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