Monday, September 13, 2004

Photo may be first of extrasolar planet


The red object appears to be a planet orbiting the brighter (but still relatively dim) brown dwarf star, seen here as blue-white.
The red object appears to be a planet orbiting the brighter brown dwarf star, seen here
as blue-white.

(SPACE.com) -- A group of European-led astronomers
has made a photograph of what appears to be a planet orbiting another star. If so, it would be the first confirmed picture of a world beyond our solar system.

"Although it is surely much bigger than a terrestrial-size object [like Earth], it is a strange feeling that it may indeed be the first planetary system beyond our own ever imaged," said Christophe Dumas, an astronomer at the European Southern Observatory.

SPACE.com revealed a similar imaging effort of another planet candidate in May by a U.S.-led team that used the Hubble Space Telescope. That possible planet has not been confirmed and could be a dim star in the background of the picture. Otherwise, all of the more than 120 known extrasolar planets have been detected indirectly, by noting the shadow of a planet crossing in front of a
star or a planet's gravitational effect on a star.

Because planets are so dim compared to stars, technology has not been able to spot them amid stellar glare. That is, perhaps, until now.

The new picture shows a dim, red point of light that Dumas and his colleagues think is a young, giant planet similar to Jupiter. It orbits a failed star known as a brown dwarf, a very dim type of star -- its core does not support nuclear fusion -- that astronomers have for years hoped would make for good planet
hunting. The brown dwarf, catalogued as 2M1207, is 42 times less massive than the sun, or some 25 times heftier than Jupiter.

The objects are 230 light-years away.

The possible planet is about five times as massive as Jupiter, the
observations show. An analysis of its emissions found it contains water, which suggests its mass is in the range of planets rather than stars, the researchers announced today.

The object is still contracting into its final form and so is very warm, some 1,830 degrees Fahrenheit (1,000 Celsius), according to the research team, which was led by ESO's Gael Chauvin.

The photograph was made at ESO's Paranal Observatory in Chile with an infrared camera, which records heat rather than visible light. A system of adaptive optics on the Very Large Telescope (it's 27 feet wide, or 8.2 meters) corrects for blurring effects of Earth's atmosphere, making detailed observations possible.

The discovery will be detailed in the journal Astronomy &
Astrophysics.

If it is a planet, the object orbits 55 times farther from the brown dwarf than Earth is from the sun, or roughly twice the Earth-to-Neptune distance.

The remaining question, however, is whether the thing might instead be a star that's in the foreground or background and not gravitationally bound to the brown dwarf, a scenario the researchers say is "statistically very improbable."

Additional observations to monitor the movement of the two objects will reveal the answer within two years, the astronomers say.


Friday, September 10, 2004

GLASS SEMICONDUCTOR SOFTENS WITH LOW-POWER LASER, THEN RE-HARDENS

COLUMBUS, Ohio – Scientists at Ohio State University have found that a special type of glass that is finding use in the electronics industry softens when exposed to very low-level laser light, and hardens back into its original condition when the light is switched off.

Ratnasingham Sooryakumar
The discovery -- made by accident as physicists were trying to study properties of the material -- may one day enable new uses for the glass.

Ratnasingham Sooryakumar said that he and former doctoral student Jared Gump thought they were working with a bad batch of germanium-selenium glass when Gump was testing the material’s hardness in the laboratory and couldn’t reproduce his results.

“Every day he got a different result,” recalled Sooryakumar, a professor of physics at Ohio State. “It took us a while to realize that the material was fine, it was just very sensitive to light.”

They finally traced their strange results to the very low-power laser light that they were shining on the glass. Whether the laser was set to exactly the same power every time shouldn’t have affected the experiment, but it did. The higher the laser power, the softer the glass. In fact, with the laser set to a mere 6 milliwatts –- six thousandths of a Watt -- the material became 50 percent softer than usual.

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The discovery -- made by accident as physicists were trying to study properties of the material -- may one day enable new uses for the glass.
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“Normally, you’d have to almost melt the glass to get it that soft, but here we were doing it with a light source that was essentially a laser pointer, and with no heat at all,” said Sooryakumar. “And what’s really important is that the whole effect is reversible.”

In the journal Physical Review Letters, the physicists reported that the glass always hardened back into its original condition. Even the latticework of atoms that made up its structure appeared unchanged afterward.

Sooryakumar and Gump co-authored the paper with Ilya Finkler, a former undergraduate student majoring in physics and mathematics, and Hua Xia, a former postdoctoral associate, both of Ohio State; Wayne Bresser, an assistant professor of physics at Northern Kentucky University; and Punit Boolchand, professor of electrical and computer engineering and computer science at the University of Cincinnati. Gump is now a scientist at the Naval Surface Warfare Center in Indian Head, MD, Finkler is a graduate student studying physics at Harvard University, and Xia is an engineer at General Electric Corp.

The glass is part of a family of glass semiconductors that are often used in electronics for DVDs and information storage technologies.

Germanium is hard and selenium soft. A combination of 80 percent selenium and 20 percent germanium is the “magic formula” where the material is neither too hard nor too soft, and well suited for forming a glass. Scientists call this point the rigidity transition.

Scientists are very interested in studying why the 80-20 ratio works, and what happens to the mechanical strength of the glass during the rigidity transition. To answer those questions, Sooryakumar and his colleagues tried to examine the hardness of the material in a range of selenium-germanium combinations around the transition point.

One way to determine the hardness of a material is to measure the speed of sound waves traveling through it; sound waves travel faster through harder materials. The physicists bounced a low-powered red laser beam off the sound waves to measure the speed –- a technique similar to how radar detects the speed of a moving car. The laser beam was only about as wide as a human hair, and used about as much power as a laser pointer.

That’s when they noticed the softening effect.

“It was as if the radar beam was influencing the speed of the car,” Sooryakumar said.

For compositions closest to the transition point, the effect was greatest: the material softened by 50 percent, from a hardness of 26 to 13 gigapascals as the laser power increased from 2 to 6 milliwatts. Hardness is a measure of how much pressure a material can withstand, and diamond rates at 100 gigapascals.(A gigapascal is roughly 10,000 times the pressure of earth’s atmosphere at sea level.)

Though the physicists don’t yet have a complete picture of why the material softened, Sooryakumar suspects that the answer has to do with the nature of the rigidity transition itself. Stiff materials normally carry a certain amount of stress in them, because the stacked molecules support each other like steel girders in a building. The transition point is special, Sooryakumar noted, because the molecules are arranged in just the right way to lower stress on the structure to a minimum.

Here’s why the physicists think the glass softened: When particles of light, called photons, hit the glass, they knocked some of the electrons that connect molecules in the latticework out of place. Such a change in bonding occurs most easily under conditions of minimum stress. With fewer supports holding up the structure, the glass became less stiff. Then, when the light was switched off, the electrons swung back into position, and the glass became stiff again.

Sooryakumar speculated that these types of glasses could have potential applications in re-writable computer memory. But right now, he and his colleagues are probing further to understand the rigidity transition and the remarkable response to light at this composition. They want to study what happens if the material is exposed to laser light of different color and higher power, and test different glasses besides selenium-germanium.