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VOL. 22, NO. 23May 21, 1997

Gamma Ray Telescope To Take Flight in June

Elena Aprile Elena Aprile and the gamma ray telescope Record Photo by Bob Nelson

By Bob Nelson

Gamma rays are showing scientists a side of the universe no one has seen, with new views of binary stars, black holes, pulsars and other phenomena.

  Many dense stars, especially black holes, radiate more energy in gamma rays--high-energy electromagnetic radiation--than in visible light. Only with recent gamma ray observations have scientists recognized how violent the universe can be, with frequent stellar explosions in our own galactic neighborhood, and data from such radiation may soon tell how and where the 100-or-so naturally occurring elements were created.

  Such observations have been made with the Compton Telescope, a fairly primitive instrument launched by NASA in April 1991 and still orbiting 250 miles above Earth. The telescope, the only instrument so far to gather data in medium-range gamma rays, detected a plume of antimatter streaming from the core of the galaxy, news that made the front pages just weeks ago.

  One day in early June, a highly sensitive new instrument joins the thin ranks of gamma-ray telescopes. A clear polyethylene balloon carrying Columbia's Liquid Xenon Gamma Ray Imaging Telescope will float skyward from a NASA facility in Texas. Data it collects will tell scientists the temperatures, direction and speed of movement of gamma-ray sources, information that will add to what is known from visual and other observations. The Columbia telescope might eventually confirm, for example, the idea that an enormous black hole sits at the center of our galaxy.

  "It's a new, emerging field," said Elena Aprile, associate professor of physics at Columbia, who has spent the last four years perfecting the telescope. "When we look at cosmic gamma rays in this range, we will be charting new territory that nobody has measured."

  The telescope that NASA will launch from its National Scientific Balloon Facility in Palestine, Tex., about halfway between Dallas and Houston, is an oblong metal box about two feet tall and three feet on a side. The box is filled with the rare gas xenon, which, when liquefied with liquid nitrogen to about -150°F, is an exquisite detector of high-energy gamma rays. It will capture radiation from a field of view of about 45 degrees, and its aperture is a square opening, without any lens, atop the metal box. Data produced by the gamma rays' interactions with xenon can be translated into a three-dimensional image that shows the intensity of the radiation over a given area of the sky.

  Though several research groups have tried to build xenon-based gamma-ray detectors, Aprile's group will be the only one to launch such an instrument above the layer of ozone high in the Earth's atmosphere that shields the surface from gamma rays, which in high doses are fatal. Xenon is an expensive gas that is difficult to handle; on any day the detector is being tested, the staff in Aprile's lab arrives at 5:00 A.M., because it takes hours to liquefy and filter the 5000 liters of xenon gas the detector uses.

  The instrument will measure a range of gamma rays between 300,000 and 30 million electron-volts, well below the highest-energy gamma rays. "In our view, this is the energy band in which some of the most exciting discoveries in gamma-ray astronomy remain to be made," Aprile said.

  The naturally-occurring elements, such as oxygen, carbon and iron, were probably formed in the core of extremely dense stars that eventually explode. Much of the matter formed in this way was originally radioactive and has decayed to the stable forms we recognize today. When radioactive elements decay, they emit gamma rays, and Aprile's team expects to see tell-tale gamma-ray concentrations that will show how and where in the universe certain elements are being created. Among the candidates for element production are red giant stars, thermonuclear explosions known as novae or supernovae and giant molecular clouds, such as the one in the Orion constellation.

  They will study in particular the distribution of aluminum-26, an isotope of aluminum and tracer of galactic radioactivity, which, contrary to expectations, is not concentrated in the millions of stars at the center of the Milky Way galaxy.

  NASA supported the research.