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April
4, 2006: Thirty-plus years ago on the moon, Apollo
astronauts made an important discovery: Moondust can be a
major nuisance. The fine powdery grit was everywhere and had
a curious way of getting into things. Moondust
plugged bolt holes, fouled tools,
coated astronauts' visors and abraded their gloves. Very
often while working on the surface, they had to stop what
they were doing to clean their cameras and equipment using
large--and mostly ineffective--brushes.
Dealing
with "the dust problem" is going to be a priority
for the next generation of NASA explorers. But how? Professor
Larry Taylor, director of the Planetary Geosciences Institute
at the University of Tennessee, believes he has an answer:
"Magnets."

Above:
In Taylor's lab, moondust scattered onto a wire mesh lines
up with a magnet inserted below. Slideshow: #1,
#2, #3,
#4.
The
idea came to him in the year 2000. Taylor was
in his lab studying a moondust sample from the Apollo 17 mission
and, curious to see what would happen, he ran a magnet through
the dust. To his surprise, "all of the little
grains jumped up and stuck to the magnet."
"I
didn't appreciate what I had discovered," recalls Taylor,
"until I was explaining it to Apollo 17 astronaut Jack
Schmitt one day in my office, and he said, 'Gads, just think
what we could have done with a brush with a magnet attached!'"
"Only
the finest grains (< 20 microns) respond completely to
the magnet," notes Taylor, but that's okay because the
finest dust was often the most troublesome. Fine grains were
more likely to penetrate seals at the joints of spacesuits
and around the lids of "pristine" sample containers.
And when astronauts tramped into the Lunar Module wearing
their dusty boots, the finest grains billowed into the air
where they could be inhaled. This gave at least one astronaut
(Schmitt) a case of "moondust hay fever."
Taylor
has since designed a prototype air filter with permanent magnets
inside. "When the filter gets dirty, you pull the magnets
out, and the dust falls into a box." A later design with
electromagnets works more efficiently: "You pull the
plug on the electromagnet, tap it, and the dust rains down
into a container." He's
now working on a prototype design for a "dust brush"
using permanent magnets.
Earth
dust is not magnetic, so why should moondust be?
"Moondust
is strange stuff," explains Taylor. "Each little
grain of moondust is coated with a layer of glass only a few
hundred nanometers thick (1/100th the diameter of a human
hair)." Taylor and colleagues have examined the coating
through a microscope and found "millions of tiny specks
of iron suspended in the glass like stars in the sky."
Those iron specks are the source of the magnetism.
Right:
A microscopic image of the iron-specked glass which coats
moondust. Credit: Keller et al, 1999. [More]
Researchers
believe the glass is a by-product of bombardment. Tiny micrometeorites
hit the surface of the moon, generating temperatures hotter
than 2,000°C, literally the surface temperature of red stars.
Such extreme heat vaporizes molecules in the melted soil.
"The vapors consist of compounds such as FeO and SiO2,"
says Taylor. If the temperature is high enough, the molecules
split into their atomic components: Si, Fe, O and so on. Later,
when the vapors cool, the atoms recombine and condense on
grains of moondust, depositing a layer of silicon dioxide
(SiO2) glass peppered with
tiny nuggets of pure iron (Fe).
A
thin coating of iron isn't enough to make sand- or gravel-sized
particles noticeably magnetic, any more than spraying a thin
coating of iron on a heavy basketball would make it stick
to a magnet, says Taylor. But a thin coating is plenty for
particles smaller than about 20 microns. They have so little
mass compared to their surface area, they're easily lifted
by Taylor's magnets.
Magnets
aren't the only way to deal with moondust. NASA is considering
a whole suite of options from airlocks to vacuum cleaners.
But, if Taylor is right, magnets will prove important, and
astronauts won't find moondust so troublesome the next time
around.
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Authors: Trudy E. Bell
& Dr. Tony
Phillips | Production Editor:
Dr. Tony Phillips | Credit: Science@NASA
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