Author Topic: 'EXTREME PHYSICS' observatory ready for final assembly  (Read 702 times)

Online jacqmans

  • Moderator
  • Global Moderator
  • Senior Member
  • *****
  • Posts: 17271
  • Houten, The Netherlands
  • Liked: 2896
  • Likes Given: 186
Susan Hendrix                                                                                   Sept. 20, 2006
NASA Goddard Space Flight Center
Greenbelt, Md. 20771

RELEASE: 06-79


The primary instrument for NASA’s Gamma-ray Large Area Space Telescope (GLAST) arrived at General Dynamics, Scottsdale, Ariz., on September 18 for mounting onto the spacecraft.  

The instrument, called the Large Area Telescope, successfully completed four months of vigorous testing last week at the U.S. Naval Research Laboratory, Washington, to ensure it can withstand the rigors of launch and operations in space.

"GLAST is a remarkable undertaking, a partnership between astronomers and physicists," said Peter Michelson, GLAST principal investigator at Stanford University, Calif. "We are eagerly anticipating a new understanding of the connections between the large and small, between the most energetic phenomena in the universe and the subatomic world."

The observatory will detect light billions of times more energetic than what our eyes can see or what optical telescopes can detect. Key targets include powerful particle jets emanating from enormous black holes and possibly the theorized collisions of dark matter particles. The Large Area Telescope will be at least 30 times more sensitive than previous gamma-ray detectors and will have a far greater field of view.

"The Large Area Telescope is a unique and beautiful new instrument for science, and it will provide a tremendous leap forward in our ability to study the most energetic objects and phenomena in space," said Steven Ritz, project scientist at NASA's Goddard Space Flight Center, Greenbelt, Md.

Unlike visible light, gamma rays are too energetic to be focused by traditional telescope mirrors onto a detector. The Large Area Telescope will employ detectors that convert incoming gamma rays into electrons and their antimatter partners, called positrons. This technique, a change of light into matter as described by Einstein's equation E=mc^2, is called pair conversion. It will enable scientists to track the direction of gamma rays and measure their energy.

The Large Area Telescope was assembled at the Stanford Linear Accelerator Center in Menlo Park, Calif., from subsystems developed by an international team from Italy, Japan, France, Sweden and the United States.

The second main instrument, the GLAST Burst Monitor, arrived in Scottsdale, Ariz., in July and is currently being integrated onto the spacecraft. The GLAST Burst Monitor was built at NASA's Marshall Space Flight Center, Huntsville, Ala., in collaboration with scientists from the Max Planck Institute for Extraterrestrial Physics, Garching, Germany, working with NASA through an agreement with the German Aerospace Center.

GLAST is scheduled to launch from NASA's Kennedy Space Center, Fla. in fall 2007.

NASA Goddard manages the GLAST mission. The Large Area Telescope was built with significant contributions from NASA, the U.S. Department of Energy and foreign collaborating institutions. The Stanford Linear Accelerator Center at Stanford University manages the instrument with collaborators at Goddard; University of California, Santa Cruz; University of Washington, Seattle; Ohio State University, Columbus; U.S. Naval Research Laboratory, and institutions in France, Italy, Japan, and Sweden. NASA Marshall manages the GLAST Burst Monitor with collaborators in Germany. General Dynamics C4 Systems is building the spacecraft and is responsible for instrument integration. Education and Public Outreach efforts for the mission are coordinated by Sonoma State University.

For more information about the mission, visit: