Following
on the heels of an announcement two weeks ago that researchers had found direct
evidence for groundwater on Mars (see Geotimes
coverage), the Mars Exploration Rover (MER) team said yesterday that they
have found evidence for standing water on the planet's surface.
Cross-lamination patterns in a rock called
"Last Chance" required flowing water at Mars' surface, according to
the Mars Exploration Rover team. Inset: Black lines trace cross-laminations,
in magnified images taken by Opportunity (at yellow arrows). Blue lines show
boundaries where deposition may have halted between crossbedded sets. Red arrows
indicate other possible crossbedding in the rock. Image courtesy of NASA/JPL/Cornell/USGS.
At a press conference at NASA headquarters, John Grotzinger of MIT, and a geologist
for the MER team, described ripples and cross-stratification in the approximately
30- to 50-centimeter-thick outcrop that the rover Opportunity has been examining
for the past few weeks. The crossbedding was formed in water, which probably
moved between 10 and 50 centimeters per second, Grotzinger says, in the equivalent
of a nearshore environment. "If you were out there, you would feel the
water moving around your ankles, and it would be about that deep," he says.
The team thinks that a shallow sea may have been present in the region, which
was alternately wet and dry. Adding the surface-water crossbedding to other
evidence, such as wind-blown deposits, crinkly lamination and soft-sediment
folds found elsewhere in Opportunity's landing crater, Grotzinger says that
the best equivalent on Earth for the Mars environment is a playa lake, which
is often moist, as well as dry and wet below the surface.
When wet, the water present would have produced ripples that made centimeter-scale
concave-up crossbeds, and when dry, it created evaporite deposits (see previous
coverage by Geotimes). The episodic periods may have been from daily
floods, seasonal climatic changes, "or longer-term intervals of wet climate
or dry," Grotzinger says.
The origin of the water remains unclear; it may be from surface precipitation
or the melting of ice layers elsewhere. For example, as Grotzinger describes
in one possible scenario, water from ice melting underground may have come up
to the surface and pooled, or perhaps flowed from another basin into the region
Opportunity is now exploring. He says that the rock unit containing the ripples
is "likely part of a larger regional unit that extends for hundreds of
kilometers either overlain by younger rock or eroded away and we can
no longer see evidence for it."
The three or four layers of ripples the team examined also have breaks in deposition
between them. "We just don't know how much time is represented between
the layers," Grotzinger says.
Dave Rubin, a sedimentologist at the U.S. Geological Survey Pacific Science
Center in Santa Cruz, Calif., who is not a MER team member, noted at the press
conference that the crossbedding "looks more like ripples than anything
deposited by air." On Earth, such "smile-shaped" crossbeds of
a similar size and thickness could have formed in a little creek in less than
an hour, he said. "It doesn't have to take a long time, but it requires
flowing water," Rubin said. He also said he could find examples of playas
that would fit the requirements for a transitional environment in Northern China.
Another plausible way to create such crossbeds, Rubin said, would be from very
small windblown bedforms, but even those require water just beneath the surface.
"Again, we've done all of this on the basis of one spot," said Steven
Squyres, principal investigator of the project, also at the press conference.
"It's hard to draw inferences of how long things took from the chemistry
— any geologist will tell you that you need a stack of rocks" to come to
any conclusions.
While describing future plans for exploring Mars, James Garvin, NASA's Lead
Scientist for Mars and the Moon, said that the Opportunity and Spirit might
have their missions extended until late summer, and maybe even until September.
Naomi Lubick
For more Geotimes coverage of Mars, click
here.
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