Geologists at the Smithsonian's National Air and Space Museum have discovered a large former lake in the highlands of Mars that would cover an area the size of Texas and New Mexico combined, and which overflowed to carve one of that planet's largest valleys. The findings will appear in the June 21 issue of the journal Science.
"Imagine more than five times the volume of water in the Great Lakes being released in a single flood, and you'll have a sense of the scale of this event," said Ross Irwin, a geologist in the museum's Center for Earth and Planetary Studies (CEPS) and the paper's lead author.
Mars is now a cold desert planet but its many dry valleys could indicate that water once flowed on its surface. Recent results from the Mars Odyssey spacecraft have found evidence of water trapped in the near surface of the polar regions.
"The size of this lake-1,400 miles long-suggests Mars was warmer and wetter than previously thought," said Robert Craddock, a CEPS geologist and co-author of the paper.
Former lakes are considered the most likely places to preserve the record of any past Martian life. Calm water would allow sediments to be deposited slowly, preventing small organisms from being destroyed.
The source of water to carve the flood channel had long been a mystery to scientists, who had known very little about Mars' topography prior to the Mars Global Surveyor mission, which has been orbiting Mars since 1997.
Detailed elevation data from the Mars Global Surveyor shows the large valley originated nearly full-size at a ridge, much like the spillway of a dam. Late in the lake's history, rising water levels overflowed the lake basin rim, releasing the huge flood as the river cut into this former dividing ridge. What remained was "some of the best geological evidence for a lake found to date on Mars, including clear indications of the former shoreline," Irwin says.
Two other smaller lake basins were identified in the region by paper co-author Alan Howard, a geologist at the University of Virginia. All three lakes shared the same water level prior to the flood, indicating the possibility of an ancient water table and suggesting the locations of other dry lake basins on Mars. Such information could be important in determining where to land robotic probes in coming years.
CEPS is the scientific research unit within the Collections and Research Department of the National Air and Space Museum. CEPS performs original research and outreach activities on topics covering planetary science, terrestrial geophysics, and the remote sensing of environmental change.
Note to editors: To arrange interviews with the CEPS geologists involved in this project, please call Peter Golkin in the National Air and Space Museum Office of Public Affairs at (202) 357-1552.
Ma'adim Vallis Region Imagery
|(Above) False-color topographic
map of the recently discovered former lakes in the cratered highlands of
Mars. Lighter colors denote higher elevations in both images. The largest
of the three lakes overtopped its basin rim and the resulting outflow toward
the north (arrow) carved Ma'adim Vallis, which is larger than the Earth's
Grand Canyon. The basin and valleys are currently dry, but evidence of the
former lake shorelines has been preserved. North is at the top. High
resolution image (3.2 MB jpg)
|(Right) Facing south, a perspective view looking up Ma'adim Vallis. The channel flowed into Gusev Crater (foreground), which is currently being considered as a landing site for one of the 2003 Mars Exploration Rovers. A view across part of the large former lake (background) shows its deep bowl-shaped floor. High resolution image (977 K jpg)|
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Image credit: R. P. Irwin
III and G. A. Franz, National Air and Space Museum, Smithsonian Institution
High resolution image (1.9 MB jpg)
Meduim resolution image (78 K jpg)
|(Top and right)
Grayscale versions of the color images on previous page, with water not
shown. Image credit: R. P. Irwin III and G. A. Franz, National Air and
Space Museum, Smithsonian Institution
High resolution image (461 K jpg)
Viking Orbiter image of part of Ma'adim Vallis, where it crosscuts an impact
crater. The dry valley is 23 km (14 miles) wide at this location, and the
former flood channel is 5 km (3 miles) wide. Image credit: NASA/JPL.