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Oct.
23, 2009: Right now, the Moon is a ghost town. Nothing
stirs. Here and there, an abandoned Apollo rover — or the
dusty base of a lunar lander — linger as silent testimony
to past human activity. But these days, only occasional asteroid
impacts disrupt the decades-long spell of profound stillness.
And
this stillness presents scientists with an important opportunity.
Currently,
the Moon's tenuous atmosphere is relatively undisturbed. But
that won't be true for long. NASA is planning to return people
to the Moon, and human activity will kick up dust, expel rocket
exhaust, and release other gaseous emissions into the lunar
atmosphere. Because the atmosphere is so thin, these disturbances
could quickly swamp its natural composition.
Right:
"Lunar Ghost Town." The landing site of Apollo 15.
[more]
If
scientists are ever to know the lunar atmosphere in a relatively
natural state, now is the time to look. So researchers are
building a probe called the Lunar Atmosphere and Dust Environment
Explorer (LADEE) that will orbit the Moon and measure its
wispy atmosphere better than ever before.
"It's
important that we understand it in its pristine state before
there's much perturbation," says Anthony Colaprete of
NASA's Ames Research Center in Moffett Field, California.
"It's such a fragile system. It's possible that it will
be hard to study once humans are once more living and working
on the Moon."
Thinner than thin
Right
about now, you might be thinking to yourself: "Hold on
a second. I thought the Moon doesn't have an atmosphere!"
And you would be almost correct. The
Moon's "atmosphere" is so tenuous that it's technically
considered an exosphere, not an atmosphere.
"It's
not anything like an atmosphere we would think of," Colaprete
says. For example, a cubic centimeter of Earth's atmosphere
at sea level contains about 100 billion billion molecules.
That same volume of the Moon's exosphere contains only about
100 molecules.
In
fact, that's so thin that molecules in the lunar exosphere
almost never collide with each other. Rather than constantly
ricocheting off each other to create a cohesive, swarming
mass of molecules as happens in Earth's atmosphere, molecules
in the lunar exosphere fly unimpeded, like microscopic cannon
balls following curved, ballistic trajectories.
And
the weirdness of the exosphere doesn't stop there. During
the lunar night, the Moon's exosphere mostly falls to the
ground. (Just imagine if our atmosphere fell to the ground
at night!) When sunlight returns, the solar wind kicks up
new particles to replenish the exosphere.

Above:
In 1968, on many occasions, NASA's Surveyor 7 moon lander
photographed a strange "horizon glow" after dark.
Researchers now believe the glow is sunlight scattered from
electrically-charged moondust floating just above the lunar
surface. [larger
image]
Also,
intense ultraviolet sunlight kicks electrons off particles
in the lunar soil, giving those particles an electric charge
that can cause them to levitate. Ambient electric fields lift
these charged dust particles as high as kilometers above the
surface, forming an important part of the exosphere.
Lunar
astronauts will have to live and work in this bizarre environment,
so scientists want a better picture of the exosphere and its
odd behaviors. Levitating dust can get into equipment, spacesuits,
and computers, causing damage and shortening the hardware's
useful life. In fact, moondust wrecked havoc with the Apollo
spacesuits, which were nearly threadbare by the time they
returned to Earth. Knowing how much dust is floating around
in the exosphere and how it behaves will help engineers design
next-generation lunar hardware.
After
it launches in 2012, LADEE's spectrometers and dust detectors
will measure the concentrations of 18 different chemicals
in the exosphere, including methane and water vapor. These
sensors will document how those chemicals vary, both from
place to place and over time.
Beyond
the inherent scientific value of understanding the chemical
makeup of the Moon's exosphere, knowing how chemicals move
within the exosphere could help answer a question of keen
interest to future human habitants: How could the Moon have
frozen reserves of water?
Right:
This animation shows how individual molecules may move near
the surface of the Moon to form an exosphere. [more]
Evidence
suggests that the Moon might harbor stores of ice in deep,
dark polar craters. On the lunar surface, fierce sunlight
would quickly sublimate any ice and the vapors would drift
off into space. But a deep dark crater, combining unimaginable
cold with an absence of sunlight, could provide a safe-haven
for frozen water.
A
popular idea is that icy comets brought water to the Moon
in a series of ancient impacts. But there's a problem: Even
if a comet landed in one of those dark polar craters by sheer
luck, the heat of impact would evaporate most of the ice.
So how could significant amounts of ice accumulate?
The
Moon's exosphere could help.
Suppose
a comet hits the Moon and leaves some H2O molecules
on the exposed surface. That water could survive by, essentially,
leaping to safety. Water molecules could "jump"
across the lunar surface by escaping into the exosphere and
later be recaptured by the surface as the exosphere breathes
in and out. Individual water molecules could move around in
this way until they land in one of the dark polar craters,
where they would accumulate as solid ice.
Data
from LADEE should show whether this "jumping" process
works in a way that could explain how cometary ice could have
found its way into those craters. "We can estimate the
likelihood that the water on the Moon is cometary in origin,"
Colaprete says.
So
much information from such a trifling amount of atmosphere!
Stay tuned for results from LADEE.
Author: Patrick Barry | Editor:
Dr. Tony Phillips | Credit: Science@NASA
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