Water, Water Everywhere, but Not All Drops Have Life
The guiding principle in our current search for alien biology is "follow the water." But the new research suggests this target needs to be refined.
"Should we follow the hot water or maybe the cold water?" asks Eriita Jones of the Australian National University, lead author of the study that appears in the latest issue of the journal Astrobiology.
On Earth, we know that life can survive in a wide variety of water temperatures and pressures, and yet there are watery places where no living things have been found. Jones and her colleague Charles Lineweaver have performed a comprehensive survey of just how far life has expanded into the available "water territory" on Earth.
"We try to quantify our understanding of the terrestrial biosphere better," Jones says.
Their results show that only 12 percent of the volume of the Earth where liquid water exists is known to host life. As for the rest of this volume, life presumably never found a way to adapt to the conditions there, despite having had several billions of years of evolution to work with.
This may mean that some fraction of liquid water is strictly uninhabitable – both here and on other distant worlds.
"This is a very natural way to parameterize any planet," Jones says.
Although we typically think of water being liquid between zero and 100 degrees Celsius, this is only true for pure water at Earth’s sea level atmospheric pressure (about 14.7 pounds per square inch or 1014 millibar). If salt is present, water's freezing point drops below zero degrees and its boiling point rises above 100 degrees.
At high pressure, as well, water remains liquid above 100 degrees Celsius. In fact, the authors estimate that liquid water can exist to a maximum depth of 75 kilometers below the Earth's surface, where the temperature is more than 400 degrees Celsius and the pressure is 30,000 times that at the surface.
But could life live in this water? Probably not. The highest temperature known to support life is 121 degrees Celsius. Some biologists believe organisms might survive at even higher temperatures, but nothing has broken the record yet.
The researchers also looked at pressure limits. Life has been found as far down as 5.3 kilometers below the surface, where the pressure is 1500 times that at the surface. Whether this is truly the highest pressure for habitable water remains to be seen, since no one has yet dug deeper in search of life.
"We have so far found life as deep as we have looked," Jones says.
As for low pressure, life has been found high up in the atmosphere where the air is thin, but these microorganisms are typically dormant and are only revived when given the necessary nutrients. The authors therefore take the low pressure limit for active life to be one third of atmospheric pressure, which corresponds to the altitude at the top of Mt. Everest.
According to the above limits, life on our planet is restricted to a thin shell that roughly extends from 10 kilometers above the surface down to 5 kilometers below (or to depths of 10 kilometers in the ocean). This leaves uninhabited 88% of the volume where water exists on Earth.
Nearly all of Earth's liquid water is located in habitable regions. The point is that only a small fraction of the water conditions on Earth are friendly to life.
"Stated this way it sounds surprising and seems to suggest that the 'follow the water' strategy for life search needs rethinking," says Chris McKay of the NASA Ames Research Center.
But he thinks this is slightly misleading. The only truly constraining factor in this analysis is the observation that life apparently can't survive above 122 degrees Celsius.
However, hotter temperatures can be found below the surface. Mars, for instance, may be too cold for liquid water on its surface, but there is reason to believe that there is liquid water underground.
Jones and Lineweaver are currently modeling the crust, mantle and core of Mars and using heat flow estimates to construct a Martian water phase diagram, like the one they made for Earth's water. The results will show at what depths potentially habitable water (as defined by the current study) might be found on Mars.
This sort of "habitable water" analysis could also be used for the liquid oceans that are thought to lie beneath the icy crusts of Jupiter’s moon Europa and Saturn’s moon Enceladus. And it may help characterize exoplanets for which a reasonable phase diagram can be estimated.
"It may show us where to focus our search for life," Jones says.