GLAST Observatory in Orbit
The GLAST spacecraft and Delta II rocket leap off the launch pad. Photo credit: NASA TV
The second firing of the second engine was confirmed as was successful spacecraft separation. Applause rippled through the launch control center as separation confirmation was received.
GLAST is now on its own, in a circular orbit 350 miles above the Earth, prepared to monitor the universe and the mysterious gamma-ray bursts.
GLAST is a powerful space observatory that will explore the most extreme environments in the universe, and search for signs of new laws of physics and what composes the mysterious dark matter, explain how black holes accelerate immense jets of material to nearly light speed, and help crack the mysteries of the staggeringly powerful explosions known as gamma-ray bursts.
With high sensitivity GLAST is the first imaging gamma-ray observatory to survey the entire sky every day. It will give scientists a unique opportunity to learn about the ever-changing universe at extreme energies. GLAST will detect thousands of gamma-ray sources, most of which will be supermassive black holes in the cores of distant galaxies.
"After a 60-day checkout and initial calibration period, we'll begin science operations," said Steve Ritz, GLAST project scientist at Goddard. "GLAST soon will be telling scientists about many new objects to study, and this information will be available on the internet for the world to see."
GLAST: Exploring the Extreme Universe
GLAST is a powerful space observatory that will open a wide window on the universe. Gamma rays are the highest-energy form of light, and the gamma-ray sky is spectacularly different from the one we perceive with our own eyes. With a huge leap in all key capabilities, GLAST data will enable scientists to answer persistent questions across a broad range of topics, including supermassive black-hole systems, pulsars, the origin of cosmic rays, and searches for signals of new physics.
The mission is an astrophysics and particle physics partnership, developed by NASA in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S.
Source: NASA
GLAST is now on its own, in a circular orbit 350 miles above the Earth, prepared to monitor the universe and the mysterious gamma-ray bursts.
GLAST is a powerful space observatory that will explore the most extreme environments in the universe, and search for signs of new laws of physics and what composes the mysterious dark matter, explain how black holes accelerate immense jets of material to nearly light speed, and help crack the mysteries of the staggeringly powerful explosions known as gamma-ray bursts.
With high sensitivity GLAST is the first imaging gamma-ray observatory to survey the entire sky every day. It will give scientists a unique opportunity to learn about the ever-changing universe at extreme energies. GLAST will detect thousands of gamma-ray sources, most of which will be supermassive black holes in the cores of distant galaxies.
"After a 60-day checkout and initial calibration period, we'll begin science operations," said Steve Ritz, GLAST project scientist at Goddard. "GLAST soon will be telling scientists about many new objects to study, and this information will be available on the internet for the world to see."
GLAST is a powerful space observatory that will open a wide window on the universe. Gamma rays are the highest-energy form of light, and the gamma-ray sky is spectacularly different from the one we perceive with our own eyes. With a huge leap in all key capabilities, GLAST data will enable scientists to answer persistent questions across a broad range of topics, including supermassive black-hole systems, pulsars, the origin of cosmic rays, and searches for signals of new physics.
The mission is an astrophysics and particle physics partnership, developed by NASA in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S.
Source: NASA
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How much time might be required before analysis of GLAST data might indicate proof or rejection of Hawking Radiation theory?
This could be critical in determining the safety of the Large Hadron Collider, due to begin collisions later this year.
Unlike what CERN tells the public, the Large Hadron Collider Safety Assessment Group (LSAG) writes that current safety arguments are not valid proof of safety. Micro black holes might be created by the Large Hadron Collider, they might not evaporate, they might grow quickly and we have not been damaged by cosmic rays because cosmic rays pass harmlessly through Earth. CERN also tells the public that a new safety report has been completed, but so far the final report has not been released for review by world%u2019s scientists.
The legal complaint before US Federal Court in Hawaii demands 4 months to review this safety report and a permanent injunction if safety can not be assured to within reasonable industry standards. First hearing is scheduled for June 16, 2008.
Learn more at LHCFacts.org