


Mars may have churned out water and ash from recent volcanic activity at its north pole, suggest images from Europeās Mars Express spacecraft. And some of that activity may still be going on today, the imaging team believes.
The craft has beamed back dramatic images of nearly the entire northern polar region, despite a technical glitch with its highest-resolution camera.
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The images, taken by the spacecraftās High Resolution Stereo Camera (HRSC), reveal curved cliffs about 2 kilometres high, streaked with dark layers. The layers may be volcanic ash mixed with water ice, says Gerhard Neukum, principal investigator of the HRSC at the Free University of Berlin, Germany.
He and his team believe this ācementedā ash may continually crumble into sand-like particles. These particles may in turn form the dark, rippling ādune fieldsā covering parts of the floor at the base of the cliffs.
Cinder cones
More intriguingly, the team has found seven volcanic cones sprinkled around these floors, some of which may still be actively forming. These may have formed like cinder cones in Hawaii, which build up when dry ash surfaces from below ground, says Neukum.
But he believes the process on Mars involves water instead. The cones may have built up from material that dropped out of a solution of hot water, which surfaced as a result of underground volcanic activity.
The process ā whatever it is ā may still be going on today. Four of the cones appear to be āfully grownā ā towering 600 metres high ā but the other three reach just 100 m and could be ābaby conesā, he says.
āIt would be an extreme coincidence if they had stopped growing in the past and we see this frozen stage now,ā Neukum told Āé¶¹“«Ć½. He adds that the cones appear remarkably unaffected by erosion from wind, water, or ice moving in the soil ā which suggests they are still taking shape.
Volcanic bubbling
But Jim Garvin, NASAās chief scientist based in Washington, DC, US, questions that reasoning. He and colleagues closely scrutinised two similar cones in the same region in 2000 using the Mars Orbiter Camera (MOC) and a laser altimeter on NASAās Mars Global Surveyor spacecraft.
He says his observations suggest the cones form simply by lava bubbling up from a volcanic vent, in line with leading theories of how Martian volcanoes behave. āYou donāt need to call upon any exotic water interactions,ā he told Āé¶¹“«Ć½.
And though his and Neukumās observations both suggest volcanoes may have erupted relatively recently ā within 10,000 years ā the images cannot prove they are still active today āunless we see steam coming from themā, he cautions.
Methane source
But Garvin says the HRSC observations may help explain the source of methane gas detected in Marsās atmosphere. While some scientists say microbes may be pumping out the gas, Garvin notes that āany methane could be from recent small amounts of volcanismā.
Neukum himself admits that his interpretation of these volcanic cones may be wrong ābecause we do not have any higher resolution imageryā than the 10 m resolution of the main camera on the HRSC. In fact, the HRSC package was supposed to be able to resolve details as small as 2.3 m across with its other camera, called the Super Resolution Channel (SRC).
But Āé¶¹“«Ć½ has learned that the SRC has been plagued with a vision problem called astigmatism. The problem stems from the fact that parts of the SRC run at too high a temperature, while other parts run too cold, so light travelling into the instrument is distorted.
So far the SRC has produced some images, but only at a resolution of about 5 m. And the team must remove the distortions by hand through a ācumbersomeā image processing procedure, says Neukum.
But even without the SRC, āthe HRSC data are so extremely good we are concentrating on that now,ā Neukum says. āYou take what you can get.ā