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Listen to this story (requires RealPlayer) November
17, 2000 -- When an earthquake hits and your home or office
begins to vibrate, it's too late to think about how strong is
the ground under your feet. You depend on the civil engineers
and the building designers to know that and design accordingly.
Right: The liquid-like behavior of sand during the 1989
Loma Prieta earthquake in California damaged this bridge leading
to the Moss Landing Marine Laboratory. Credit: J.C. Tinsley,
U.S. Geological Survey
"We hope to duplicate the soil liquefaction that occurs on the ground during an earthquake," said Dr. Khalid Alshibli, MGM Project Scientist at NASA's Marshall Space Flight Center. "Our role here is to share our findings with others in academia, as well as engineering and civil construction." Left: MGM may have applications on other worlds, too. The terraced walls of the Moon's Copernicus crater, shown here in an image captured by the Lunar Orbiter 2 in 1965, apparently were caused by soil fluidization after a meteorite impact. From the beginning, the MGM project has received high accolades,
scrutinized by seven science peer reviews along with reviews
by 18 different academicians and four industrial researchers.
Dr Robert Schrieffer, winner of the Nobel Prize in 1972, praised
the MGM project as "world-class science" and "an
appropriate effort for NASA." Above: How particles are packed can change radically during cyclic loading such as in an earthquake or when shaking a container to compact a powder. A large hole (1) is maintained by the particles sticking to each other. A small, counterclockwise strain (2) collapses the hole, and another large strain (3) forms more new holes which collapse when the strain reverses (4). (after T.L. Youd, "Packing Changes and Liquefaction Susceptibility," Journal of the Geotechnical Engineering Division,103: GT8, 918-922, 1977). The tests on STS-107 will concentrate on water trapped within
the soil and how that water affects soil behavior when external
loading changes faster than the entrapped fluid can escape. As
the water pressure or air pressure increases on the particles,
the intergranular stresses holding the soil together decrease
and the soil weakens. When external loading equals the internal
pressure, soil liquefaction occurs. The Shuttle microgravity studies of these properties are critical
because the Earth's gravity-induced stresses complicate the analysis.
The weightless environment allows scientists to conduct soil
mechanics experiments with very low confining pressures. Understanding
these phenomena is essential for improving building techniques
for sites here on Earth as well as for future building sites
on the Moon or Mars. Information obtained from these studies
will also aid in storage, handling and processing of materials
such as grains, powders and fertilizers. Specimens returning to Earth are examined to reveal the details of their structure. Computed Tomography (CT) scans produce a series of "slice" images every 1 mm along the length of the specimen. From such data, scientists construct three-dimensional images that reveal complex patterns and show how the sand specimen has shifted internally. Finally the specimens are impregnated with epoxy to stabilize the sand column, then sawed into1 mm thick slabs for detailed inspection under an optical microscope. All this playing around in the sand might seem incongruous for serious scientists, but studies of such granular materials will certainly lead to better engineering here on Earth and, perhaps one day, on other planets as well. |
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Putting the Squeeze on Sand -- 1998 Science@NASA article about earlier MGM shuttle experiments |
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