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STS-122: Crew arrival

The space shuttle Atlantis astronauts arrive at the Kennedy Space Center for their countdown to launch.

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STS-122: The mission

Atlantis' trip to the station will deliver the European Space Agency's Columbus science lab module.

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STS-122: The programs

Managers from the shuttle, station and EVA programs discuss Atlantis' upcoming flight.

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STS-122: Spacewalks

Three spacewalks are planned during Atlantis' STS-122 assembly mission. Lead spacewalk officer Anna Jarvis previews the EVAs.

 Full briefing
 EVA 1 summary
 EVA 2 summary
 EVA 3 summary

The Atlantis crew

The astronauts of Atlantis' STS-122 mission meet the press in the traditional pre-flight news conference.

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Harmony's big move

The station's new Harmony module is detached from the Unity hub and moved to its permanent location on the Destiny lab.

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Delta 4-Heavy launch

The first operational Delta 4-Heavy rocket launches the final Defense Support Program missile warning satellite for the Air Force.

 Full coverage

Columbus readied

The European Space Agency's Columbus laboratory module moves to pad 39A and placed aboard shuttle Atlantis for launch.

 To pad | Installed

Station port moved

The station crew uses the robot arm to detach the main shuttle docking port and mount it to the new Harmony module Nov. 12.

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Atlantis rolls out

Space shuttle Atlantis rolls from the Vehicle Assembly Building to pad 39A for its December launch with the Columbus module.

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Atlantis goes vertical

Atlantis is hoisted upright and maneuvered into position for attachment to the external tank and boosters.

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Radiation flashes may help crack cosmic mystery
UNIVERSITY OF CHICAGO NEWS RELEASE
Posted: December 4, 2007

Faint, fleeting blue flashes of radiation emitted by particles that travel faster than the speed of light through the atmosphere may help scientists solve one of the oldest mysteries in astrophysics.

For nearly a century, scientists have wondered about the origin of cosmic rays-subatomic particles of matter that stream in from outer space. "Where exactly, we don't know," said Scott Wakely, Assistant Professor in Physics at the University of Chicago. "They're raining down on the atmosphere of the Earth, tens of thousands of particles per second per square meter."

Recent results from the Pierre Auger Cosmic Ray Observatory suggest that the highest-energy cosmic rays may come from the centers of active galaxies. But the vast majority of the cosmic rays seen at Earth originate from its own galaxy, from sources that are still unknown. Tracking down these sources is crucial to developing a comprehensive understanding of the phenomenon, scientists say.

The University of Chicago's Enrico Fermi suggested more than 50 years ago a process that, in its modern form, could allow the shock waves of exploding stars to propel most cosmic rays to their high energies. The idea remains popular, but unverified.

Wakely now has a $625,000 grant from the National Science Foundation to develop an instrument that might reveal important new data about the nature and origin of cosmic rays. Working in collaboration with Simon Swordy, the James Franck Professor in Physics at Chicago, they plan to make detailed measurements of Cerenkov radiation, which cosmic rays emit when they travel faster than the speed of light through the atmosphere.

While many people believe that nothing moves faster than light, "what's actually the case is nothing can go faster than light can go in a vacuum," Wakely explained. But light moves slower in air and water than it does in a vacuum.

"So it's possible that you get a particle which goes through the atmosphere faster than light does. And when that happens, you get the equivalent of a sonic boom, but with electromagnetic radiation. And that light boom is called Cerenkov radiation."

Wakely and Swordy are particularly interested in measuring the energy and mass of cosmic rays. But the density of molecules in the atmosphere stands in the way. When high-energy charged particles hit the top of the atmosphere, it's like smashing into 30 feet of water. The individual particles break into a shower of smaller pieces, frustrating attempts to measure them directly.

Incoming cosmic-ray particles trigger two flashes of Cerenkov radiation. The first occurs when the original particle enters into the atmosphere, but the resulting shower of secondary particles also emits Cerenkov light. In a 2001 article published in Astroparticle Physics, the University of Utah's David Kieda, along with Swordy and Wakely, proposed a ground-based "direct Cerenkov technique." The idea was to record both flashes of Cerenkov light.

Many experiments are designed to record the second flash of Cerenkov light. These include a collaboration called VERITAS (Very Energetic Radiation Imaging Telescope Array System), to which Swordy and Wakely belong. But no one had ever looked for that first Cerenkov flash until Kieda, Swordy and Wakely pointed out that it should be there.

The first scientists to see direct Cerenkov light belong to a European group that operate the High Energy Stereoscopic System (HESS), an array of telescopes in the African nation of Namibia. "They showed that even with non-optimum equipment, you could actually do something useful," Wakely said. "With equipment designed to do this properly, we can do even better."

The idea behind direct Cerenkov detection was to combine the precision of balloon-borne cosmic-ray instruments with the far greater detection area afforded by ground-based arrays like VERITAS and HESS. "This is something that's never been possible before," Wakely said.

Low-energy cosmic rays are pervasive. But as their energy increases, their frequency drops dramatically. Scientists try to work around this obstacle by building extensive detector arrays on the ground. Another strategy: fly their instruments on high-altitude, helium-filled balloons into the atmosphere, where fewer air molecules get in the way.

Both methods involve trade-offs. "Balloon-borne experiments are small, but exquisite in their detail," Wakely said, while ground-based experiments are huge but offer poor resolution.

Most cosmic rays are protons or other types of charged particles. But some of them consist of the nuclei of iron atoms or other heavy elements. An iron nucleus traveling at nearly the speed of light produces approximately 700 times more light than a single proton.

"We came up with this idea because we had done both direct measurements of cosmic-ray nuclei before they interact in the atmosphere-on balloons and spacecraft-and also work with air shower detection at ground level," Swordy said.

They knew from these experiments that a fast-moving iron nucleus left an unmistakable signature in high-flying detectors, "so maybe we could see this from the ground," Swordy said. "Many people have told me this is a great idea-if only they had been thinking that way, 'I could have come up with that.' Which tells me it is good because the best ideas are also, in retrospect, the most obvious."