Martian close-up images tell a watery tale
R. Cowen
The sharpest images of Mars ever recorded from an orbiting spacecraft suggest that two ingredients deemed necessary for life—water and a source of heat—were once plentiful on or just beneath the surface of the Red Planet.
Planetary scientists have known since the 1970s, thanks to images taken by the Mariner 9 and Viking Orbiter spacecraft, that dried-up channels crisscross much of the Martian surface. Scientists agree that some channels are the result of flash floods, but the resolution of these images is too poor to determine whether a steady flow of water could have carved any of the features.
Layered material along the walls of the canyon Valles Marineris could be a sign of copious volcanic activity on early Mars.
Malin et al./Malin Space Science Systems
The new pictures provide the first compelling evidence that in some regions liquid water flowed on the surface for an extended period, perhaps millions of years. The pictures were taken by the Mars Global Surveyor spacecraft during the past year as it descended through the planet's upper atmosphere. Surveyor is scheduled to begin its main 2-year mission, compiling a global map of Mars, on March 8.
The narrow, wandering paths of several dry channels seen by Surveyor's camera "are much more supportive of sustained erosion, sustained water flow" than of floods, says Michael H. Carr of the U.S. Geological Survey in Menlo Park, Calif.
One striking example, he notes, is a 200-meter-wide trough that Surveyor spied at the bottom of a canyon called Nanedi Vallis (SN: 2/7/98, p. 84). "It certainly looks as though we have a river channel that meandered across a plane and [that] the flow was sustained so that the meander got deeper and deeper."
Carr and his colleagues, including Michael C. Malin of Malin Space Science Systems in San Diego, describe these and other findings in the Feb. 18 Nature.
The Surveyor pictures also indicate that the water that once filled these channels came from underground, probably frozen, reservoirs rather than rain or snow falling from the atmosphere. Precipitation would have created an abundance of tiny tributaries as well as larger channels, but Surveyor's camera has found a dearth of the small structures.
"It's clear the source [of water] is beneath the surface," comments Maria T. Zuber of the Massachusetts Institute of Technology.
Other Surveyor findings may explain how frozen water in underground reservoirs could have melted and come to the surface. Using the images to examine in unprecedented detail a 4,000-kilometer-long Martian canyon called Valles Marineris, Alfred S. McEwen of the University of Arizona in Tucson and his colleagues found that thick layers of material form the canyon's walls.
The researchers, who include Malin, Carr, and William K. Hartmann of the Planetary Science Institute in Tucson, suggest that the layers were mainly formed by volcanic lava. If their hypothesis is correct, Mars was much more volcanically active during its first billion or so years than scientists have thought.
Frequent and widespread volcanic activity could have melted underground deposits of frozen water that then found their way to the surface, notes Steven W. Squyres of Cornell University.
Hartmann and his colleagues also have tentative evidence that some volcanic eruptions might still be going on today. Using Surveyor images to count the number of small craters, an indicator of how long ago a volcanically active region last erupted, Hartmann finds that some places on Mars spewed lava within the past 100 million years. He describes the findings both in Nature and the March Meteoritics and Planetary Science.
If volcanism is continuing—even in just a few small regions—it could up the odds that some places on Mars have hot springs not far from the surface, offering "nice, hot water for microbes," Hartmann says.
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References:
Hartmann, W.K. In press. Martian cratering VI: Crater count isochrons and evidence for recurrent volcanism from Mars Global Surveyor. Meteoritics and Planetary Science.
Hartmann, W.K., M. Malin, A. McEwen, M. Carr, et al. 1999. Evidence for recent volcanism on Mars from crater clouds. Nature 397(Feb. 18):586.
Malin, M.C., and M.H. Carr. 1999. Groundwater formation of martian valleys. Nature 397(Feb. 18):589.
McEwen, A.S., M.C. Malin, M.H. Carr, and W.K. Hartmann. 1999. Voluminous volcanism on early Mars revealed in Valles Marineris. Nature 397(Feb. 18):584.
Zuber, M.T. 1999. Snapshots of an ancient cover-up. Nature 397(Feb. 18):560.
Further Readings:
Cowen, R. 1998. Did water carve canyon on Mars? Science News 153(Feb. 7):84.
Thomas, P.C., et al. 1999. Bright dunes on Mars. Nature 397(Feb. 18):592.
Additional information and images from the Global Surveyor mission can be found at Malin Space Science Systems' Web site at http://www.msss.com/.
Sources:
Michael H. Carr
U.S. Geological Survey
Menlo Park, CA 94025
William K. Hartmann
Planetary Science Institute
Tucson, AZ 85719
Michael C. Malin
Malin Space Science Systems
P.O. Box 910148
San Diego, CA 92191
Maria T. Zuber
Massachusetts Institute of Technology
Department of EAPS, 54-518
Cambridge, MA 02139-4307
From Science News, Volume 155, No. 8, February 20, 1999, p. 117.
Copyright ©1999, Science Service.
