The Case of the Missing Mars Water
Plenty of clues suggest that liquid water once flowed
on Mars --raising hopes that life could have arisen there-- but
the evidence remains inconclusive and sometimes contradictory
January 5, 2001 -- Mars may once have been a very wet place. A host of clues remain from an earlier era, billions of years ago, hinting that the Red Planet was host to great rivers, lakes and perhaps even an ocean. But some of the clues are contradictory -- they don't all fit together in a coherent whole. Little wonder, then, that the fate of water on Mars is such a hotly debated topic.
The reason for the intense interest in Martian water is simple: Without water, there can be no life as we know it. If it has been 3.5 billion years since liquid water was present on Mars, the chance of finding life there is remote. But if water is present on Mars now, however well hidden, life may be holding on in some protected niche.
Right: Sedimentary rock layers like these in Mars's Holden Crater suggest that the Red Planet was once home to ancient lakes. [more information]
Based on what we have observed so far, Mars today is a frozen desert. It's too cold for liquid water to exist on its surface and too cold to rain. The planet's atmosphere is also too thin to permit any significant amount of snowfall.
Even if some internal heat source warmed the planet up enough for ice to melt, it wouldn't yield liquid water. The Martian atmosphere is so thin that even if the temperature rose above freezing the ice would change directly to water vapor.
Signs of Heavy Flooding
What caused these giant floods? Was it a climate change, perhaps brought about by a change in Mars's orbit? Or was the planet's own internal heat responsible? And, whatever mechanism caused the floods in the first place, where has all that water gone? Was it absorbed into the ground where it remains today, frozen? Or did it dissipate into the Martian atmosphere, where it was subsequently lost to space? No-one knows for certain the answers to these questions.
Some scientists believe that the catastrophic floods that carved the outflow channels occurred nearly simultaneously, releasing such vast quantities of water that they merged into an ocean that covered the northern lowlands. Tim Parker of NASA's Jet Propulsion Laboratory first proposed such an idea in 1989. Parker, examining images taken by the Viking Orbiters, found what he believed were remnants of two ancient ocean shorelines, which he called "contacts," one inside the other, in the Martian north.
Expanding on this notion, in 1991 Vic Baker of the University of Arizona, suggested that Mars might not be geologically dead and permanently frozen. Instead, he proposed, Mars might undergo cycles, or pulses -- first heating up, releasing groundwater and forming an ocean in the north, then dissipating the ocean back into the planet's crust and re-freezing.
But the story doesn't end there. Shortly after Head and colleagues published their findings, Mike Malin and Ken Edgett of Malin Space Systems used the Mars Orbital Camera (MOC) aboard MGS, to take a series of high-resolution images of contact 2 terrain. Their conclusion: there's nothing there.
Right: In this topographic drawing of Mars, blue indicates the area where an ocean once may have existed. Credit: NASA Mars Global Surveyor Project; MOLA Team Rendering by Peter Neivert, Brown University
And the debate continues. Says Mike Carr of the U.S. Geological Survey, author of the book Water on Mars, "We're getting all this new data from MGS, and I think a lot of it is just not understood yet. It's very hard to understand. The whole business of the oceans, the evidence is so contradictory."
Mars's small-valley networks, which occur mainly in the southern highlands, pose another perplexing problem. Scientists who first studied images of these valleys thought they resembled river valleys on Earth. So, they reasoned, a similar process, the runoff of rainwater, must have formed them.
Above: Nirgal Vallis, south of the eastern part of Valles Marineris, superficially resembles a river-cut valley on Earth. [more information]
For Mars to be warm enough to rain, however, it would have needed a much thicker atmosphere than it has today. And no-one has come up with a clear-cut explanation for how such an atmosphere could have formed.
One alternative theory is that a process known as sapping, or collapse caused by the softening of the soil by groundwater, created the valleys. Yet another notion is that perhaps glaciers covered the regions around the valleys, and that glacial meltwater carved them. As with Mars's other watery mysteries, however, the question of how the valley networks formed remains unanswered.
And if these vexing problems weren't enough, recent images from MOC reveal a startling new puzzle. In nearly a dozen different locations on Mars - all of them far from the equator - there are signs that water has been seeping out of the walls of valleys and craters, forming small gullies. Some scientists speculate that this activity is very recent, perhaps occurring within the past 10 years; others say 10 million years is more likely.
Yet many aspects of these seepage gullies defy common sense. "They sure look like water-worn features," says Mike Carr, "but they seem to contradict what we know about the stability of water." They occur not only in the coldest regions on Mars, but on slopes facing away from the Sun, where the temperature rarely gets above minus 50 degrees Centigrade. Yet the water appears to be seeping out from only 100 meters below the surface, a depth at which scientists previously believed Mars's crust to be frozen solid. Scientists are busily working to devise an explanation for this phenomenon.
Above: Martian gullies in Newton Crater. Scientists hypothesize that liquid water burst out from underground, eroded the gullies, and pooled at the bottom of this crater as it froze and evaporated. If so, life-sustaining ice and water might exist even today below the Martian surface -- water that could potentially support a human mission to Mars. [more information]
There is one additional thorn in the side of those who study
water on Mars. No evidence of carbonates has yet been found anywhere
on the planet. Carbonates are minerals that form readily when
liquid water reacts with carbon dioxide in the atmosphere. If
Mars had abundant liquid water in its past, carbonates should
be detectable in the Martian rock record. The Thermal
Emission Spectrometer (TES) instrument aboard MGS
was designed to look for just such a signature. But so far it
has found none. Perhaps other evaporites, such as sulfates (as
detected in Martian meteorites and interpreted from landing site
analyses), are the dominant material of this type on Mars.
Astrobiology Institute -- Home page
Mars Global Surveyor -- Up-to-date information about the mission, including images and movies
Science@NASA Stories about Mars:
Making a Splash on Mars -- On a planet that's colder than Antarctica and where water boils at ten degrees above freezing, how could liquid water ever exist? Scientists say a dash of salt might help.
Unearthing Clues to Martian Fossils -- The hunt for signs of ancient life on Mars is leading scientists to an otherworldly lake on Earth.
Sedimentary Mars -- New Mars Global Surveyor images reveal sedimentary rock layers on the Red Planet that may have formed underwater in the distant Martian past.
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