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The Universe Through The Looking Glass

Workers study Hubble's main, eight-foot (2.4 m) mirror. Hubble, like all telescopes, plays a kind of pinball game with light to force it to go where scientists need it to go. When light enters Hubble, it reflects off the main mirror and strikes a second, smaller mirror. The light bounces back again, this time through a two-foot (0.6 m) hole in the center of the main mirror, beyond which Hubble's science instruments wait to capture it. In this photo, the hole is covered up.
by Staff Writers
Washington DC (SPX) Sep 11, 2007
A whole new world came to life for Alice when she passed through the looking glass - beetles with bad attitudes, Tweedledee and Tweedledum, smiling cats, talking tiger lilies and much more. Mirrors have special powers in the real world too, especially in the hands of an astronomer. In fact, modern astronomy depends on mirrors. Almost every telescope uses a mirror, sometimes several mirrors, to gather and guide starlight toward some super-sensitive digital detector where a breathtaking image can be formed. Without mirrors, it would be almost impossible to study the universe.

For an X-ray astronomer, it's a little more complicated. "The X-ray light we use to study the Universe is so energetic, it would pass right through an ordinary mirror," laments Brian Ramsey of the Marshall Space Flight Center.

So Ramsey and colleagues have built an extraordinary sideways mirror that can harvest high-energy X-rays (also called "hard" X-rays)." It's called a grazing incidence mirror," explains Ramsey, who is HERO's lead scientist, "and it can guide very energetic X-rays."

Ramsey's team recently tested the device nicknamed HERO (short for High Energy Replicated Optics) on-board a balloon launched from Fort Sumner, New Mexico. The balloon carried HERO above 99% of Earth's atmosphere where it could gather X-rays from space. The data are being analyzed and results will be available soon; the team looks forward to some new cosmic images in never-before-seen detail.

The HERO team is one of many scientific groups that ask the Columbia Scientific Balloon Facility experts at Fort Sumner to launch payloads via these enormous balloons. At full inflation, HERO's balloon is 500 feet wide and rises 1000 feet above the payload. The balloon facility crew inflates and launches the balloons, tracks them, and recovers them. Because of the favorable wind conditions (little or no wind, that is) in May and September, Fort Sumner is an excellent location for ballooning at those times.

"People come out to watch and ask questions," says Ramsey. "One little boy asked me if our huge telescope had ever landed on a cow." (No!) Ramsey added that the Fort Sumner residents are very friendly and helpful. "They even put on barbecues for us from time to time," he says. Ramsey is used to hospitality - Southern hospitality, since Marshall Space Flight Center is in Huntsville, Alabama.

HERO's optics, designed and built in Huntsville, include 96 tube-like "grazing incidence" mirrors nested like the layers of an onion.

Why the strange shape? Because high-energy X-rays would pass right through the kind of flat mirror we look in each morning over our toothpaste. To keep these high-energy photons from passing through, the mirrors must be angled almost sideways such that X-ray photons glance off the sides. From there, the photons travel down the tubes to detectors that form an image.

When these mirrors eventually make it to space, they will gather photons from some of the most violent objects in the Universe: exploding stars, colliding galaxies and black holes, just to name a few. The inner violence of these objects is what makes their photons so energetic and why astronomers need a high-energy X-ray telescope to study them.

The HERO team had to climb a slippery slope to loft their innovative optics upward. Their first several attempts failed - each for a different reason. The weather was the worst obstacle.

"We have daily weather briefings," says Ramsey. "When they say 'the weather is unsuitable for launch through next Wednesday,' you consider the prospect of yet another week or two in your motel room. And there are only two restaurants around, which you get tired of. And your spirits sink a little."

Add to poor weather a few technical difficulties causing aborted flight attempts, and you get some frustrated scientists.

If ballooning is so difficult and unpredictable, why does this team rely on a balloon to give their experiment wings? Ramsey says the benefits outweigh the difficulties. "A balloon mission costs much less than a satellite mission, about 1 million as opposed to 100 million and up," he explains. "The true beauty of ballooning lies in the fact that the payloads can be reused, and the turnaround time is fast. After landing via parachute, the team makes any repairs needed for the payload and prepares it to fly again within a year. Also, because of its short duration, a balloon mission provides a great training opportunity for a college student doing research for a thesis or dissertation."

And what of HERO's future? Ramsey hopes it is headed for the sunny skies of the southern hemisphere - Australia to be exact. The HERO team has submitted a proposal for their payload to fly from there a year from now.

"Australia is an interesting place for us to fly because the galactic center is clearly visible from there. The galactic center is the most active part of our galaxy. It has lots of [hard X-ray] sources packed in there, and with our optics we will be able to resolve those into individual sources and capture images no one has captured to date."

Meanwhile, a big white balloon drifts by, high in the New Mexican sky, dangling a telescope filled with mirrors that bring a whole new world to life. In Alice's words, "It's got, oh! Such beautiful things in it!"

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Galaxies Near And Far From AKARI
Tokyo, Japan (SPX) Sep 11, 2007
Two new sets of observations from the AKARI Infrared Space Telescope, JAXA mission with ESA participation, show how the spaceborne telescope has investigated galaxies both near and far. In the first set, Toyoaki Suzuki, University of Tokyo, observed M101, a spiral galaxy 170 000 light-years in diameter. AKARI's new observations reveal differing populations of stars spread across its spiral arms.







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