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Ice may have formed Martian channels

Posted: January 18, 2001

Some channels on the surface of Mars believed to have been formed by running water may have instead been carved by streams of ice, one scientist concluded this week.

Channels in one region of Mars share a number of key characteristics with those created by ice streams that flow beneath Antarctica's surface and empty into the surrounding oceans, according to work by Baerbel K. Lucchitta of the U.S. Geological Survey and published in the February 1 issue of the journal Geophysical Research Letters.

Figure 1
Ice streams merging with the Ross Ice Shelf in West Antarctica. At right, the Rutford Ice Stream debouching into the Ronne Ice Shelf. Photo: Satellite Image Map of Antarctica
Planetary scientists have generally assumed that the channels found in various regions of the planet's surface, first seen in Mariner and Viking images from the 1970s, had been formed by flowing water. However, Lucchitta found strong similarities between channels in the Kasei Vallis region of Mars's northern hemisphere and those created by the Rutford Ice Stream, which flows under the Antarctic surface and flows into Ronne Ice Shelf.

Lucchitta noticed that the Martian channels, hundreds of kilometers long and tens of kilometers wide, were structurally similar to the Antarctic channels, especially how both formed streamlined features as they moved around rock or ice obstructions in their path. The Martian channels are also below the hypothesized sea level of an ancient Martian ocean, and in some places show signs of uphill flow: impossible with flowing water but possible with more rigid ice streams.

Combined, Lucchitta believes that the channels were created by moving ice as it flowed into an ocean, itself possibly covered by ice, that may have once sprawled over much of the northern regions of the planet. "The observations strongly support the notion that an ocean once existed in the northern plains of Mars," she noted.

While her research focused on channels in Kasei Vallis and neighboring Ares Vallis, Lucchitta believes that many other channels on the planet may have similar origins. "There are features that look like they may have been formed by ice in all of the big outflow channels," she said. "The size of the streamlined forms in most channels is like that of features carved by ice." While such features could also be created by liquid water, they would require catastrophic floods, "10,000 times the size of the Mississippi," she said.

Some of that ice may still exist on Mars today, she said, either in dust-covered deposits in Ares Vallis or beneath the smooth plains of the northern portions of the planet that may have been an ocean floor. Instruments like a ground-penetrating radar that will be flown on the European Space Agency's Mars Express mission in 2003 may be able to detect that ice.

Figure 2
Markings on Antarctic ice stream and martian channel near their termini. Left: Rutford Ice Stream diverging around ice rise (large arrow). Right: Ares Vallis, Mars, diverging around an island. Photos: Landsat and Viking Orbiter images.
Not everyone is convinced, however, that water -- in either its solid or liquid forms -- created the channels seen across the planet. Some, like Nick Hoffman of Latrobe University in Australia, have argued that the channels could have been carved out by debris propelled by high-velocity outbursts of carbon dioxide gas. Hoffman's "White Mars" model, details of which were published in the planetary science journal Icarus last year, doesn't require water of any kind to sculpt the Martian surface and provides what he considers a "simple unifying model" to explain the planet's features.

Hoffman, while noting the quality of Lucchitta's work, is not swayed by its conclusions. "It's part of the general recognition that water on Mars is very difficult to achieve and that more frigid models are better," he said, "but it does not do a good job of explaining the flow features in Ares Vallis or any other valley on Mars."

Lucchitta, though, believes that ice, or ice mixed with liquid water, is a better way to explain the channels than carbon dioxide. "To make dry ice work one would have to do a lot of special pleading," she said.

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