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Penguin Stumblings

Here There Everywhere and Back to Nowhere...

Posts tagged with "Moon"

Magnetic Moondust

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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."

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.

Moonquakes

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March 15, 2006: NASA astronauts are going back to the moon and when they get there they may need quake-proof housing.

That's the surprising conclusion of Clive R. Neal, associate professor of civil engineering and geological sciences at the University of Notre Dame after he and a team of 15 other planetary scientists reexamined Apollo data from the 1970s. "The moon is seismically active," he told a gathering of scientists at NASA's Lunar Exploration Analysis Group (LEAG) meeting in League City, Texas, last October.

Between 1969 and 1972, Apollo astronauts placed seismometers at their landing sites around the moon. The Apollo 12, 14, 15, and 16 instruments faithfully radioed data back to Earth until they were switched off in 1977.

And what did they reveal?
There are at least four different kinds of moonquakes: (1) deep moonquakes about 700 km below the surface, probably caused by tides; (2) vibrations from the impact of meteorites; (3) thermal quakes caused by the expansion of the frigid crust when first illuminated by the morning sun after two weeks of deep-freeze lunar night; and (4) shallow moonquakes only 20 or 30 kilometers below the surface.

The first three were generally mild and harmless. Shallow moonquakes on the other hand were doozies. Between 1972 and 1977, the Apollo seismic network saw twenty-eight of them; a few "registered up to 5.5 on the Richter scale," says Neal. A magnitude 5 quake on Earth is energetic enough to move heavy furniture and crack plaster.

Furthermore, shallow moonquakes lasted a remarkably long time. Once they got going, all continued more than 10 minutes. "The moon was ringing like a bell," Neal says.

On Earth, vibrations from quakes usually die away in only half a minute. The reason has to do with chemical weathering, Neal explains: "Water weakens stone, expanding the structure of different minerals. When energy propagates across such a compressible structure, it acts like a foam sponge—it deadens the vibrations." Even the biggest earthquakes stop shaking in less than 2 minutes.

The moon, however, is dry, cool and mostly rigid, like a chunk of stone or iron. So moonquakes set it vibrating like a tuning fork. Even if a moonquake isn't intense, "it just keeps going and going," Neal says. And for a lunar habitat, that persistence could be more significant than a moonquake's magnitude.

"Any habitat would have to be built of materials that are somewhat flexible," so no air-leaking cracks would develop. "We'd also need to know the fatigue threshold of building materials," that is, how much repeated bending and shaking they could withstand.

What causes the shallow moonquakes? And where do they occur? "We're not sure," he says. "The Apollo seismometers were all in one relatively small region on the front side of the moon, so we can't pinpoint [the exact locations of these quakes]." He and his colleagues do have some good ideas, among them being the rims of large and relatively young craters that may occasionally slump.

"We're especially ignorant of the lunar poles," Neal continues. That's important, because one candidate location for a lunar base is on a permanently sunlit region on the rim of Shackleton Crater at the Moon's south pole.

Neal and his colleagues are developing a proposal to deploy a network of 10 to 12 seismometers around the entire moon, to gather data for at least three to five years. This kind of work is necessary, Neal believes, to find the safest spots for permanent lunar bases.

And that's just the beginning, he says. Other planets may be shaking, too: "The moon is a technology test bed for establishing such networks on Mars and beyond."

Source: http://science.nasa.gov/headlines/y2006/15mar_moonquakes.htm?list183820

Radical! Liquid Water on Enceladus

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March 9, 2006: NASA's Cassini spacecraft may have found evidence of liquid water reservoirs that erupt in Yellowstone-like geysers on Saturn's moon Enceladus. The rare occurrence of liquid water so near the surface raises many new questions about this mysterious moon.

"We realize that this is a radical conclusion -- that we may have evidence for liquid water within a body so small and so cold," said Carolyn Porco, Cassini imaging team leader at the Space Science Institute, Boulder, Colo. "However, if we are right, we have significantly broadened the diversity of solar system environments where we might possibly have conditions suitable for living organisms."

High-resolution Cassini images show icy jets and towering plumes ejecting huge quantities of particles at high speed. Scientists examined several models to explain the process. They ruled out the idea the particles are produced or blown off the moon's surface by vapor created when warm water ice converts to a gas. Instead, scientists have found evidence for a much more exciting possibility. The jets might be erupting from near-surface pockets of liquid water above 0 degrees Celsius (32 degrees Fahrenheit), like cold versions of the Old Faithful geyser in Yellowstone: illustration.

"We previously knew of at most three places where active volcanism exists: Jupiter's moon Io, Earth, and possibly Neptune's moon Triton. Cassini changed all that, making Enceladus the latest member of this very exclusive club, and one of the most exciting places in the solar system," said John Spencer, Cassini scientist, Southwest Research Institute, Boulder.

"Other moons in the solar system [may] have liquid-water oceans covered by kilometers of icy crust," said Andrew Ingersoll, imaging team member and atmospheric scientist at the California Institute of Technology, Pasadena, Calif. "What's different here is that pockets of liquid water may be no more than tens of meters below the surface."

"As Cassini approached Saturn, we discovered the Saturnian system is filled with oxygen atoms. At the time we had no idea where the oxygen was coming from," said Candy Hansen, Cassini scientist at NASA's Jet Propulsion Laboratory (JPL) in Pasadena. "Now we know Enceladus is spewing out water molecules, which break down into oxygen and hydrogen."

Scientists still have many questions. Why is Enceladus so active? Might this activity have been continuous enough over the moon's history for life to have had a chance to take hold in the moon's interior? In the spring of 2008, scientists will get another chance to look at the geysers--and another crack at answering these questions--when Cassini flies within 350 kilometers (approximately 220 miles) of Enceladus.

"There's no question, along with the moon Titan, Enceladus should be a very high priority for us," said Jonathan Lunine, Cassini interdisciplinary scientist, University of Arizona, Tucson, Ariz. "Saturn has given us two exciting worlds to explore."

Source: http://science.nasa.gov/headlines/y2006/09mar_enceladus.htm?list183820
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