NASA Renames Observatory For Fermi, Reveals Entire Gamma-Ray Sky

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Aug. 26, 2008

J.D. Harrington 
Headquarters, Washington                               
202-358-5241 
j.d.harrington@xxxxxxxx 

David Harris 
Stanford Linear Accelerator Center, Menlo Park, Calif. 
650-926-8580 
david.harris@xxxxxxxxxxxxxxxxx 

Lynn Cominsky 
Sonoma State University, Rohnert Park, Calif. 
707-664-2655 
lynnc@xxxxxxxxxxxxxxxxxxx   
RELEASE: 08-214

NASA RENAMES OBSERVATORY FOR FERMI, REVEALS ENTIRE GAMMA-RAY SKY

WASHINGTON -- NASA's newest observatory, the Gamma-Ray Large Area 
Space Telescope, or GLAST, has begun its mission of exploring the 
universe in high-energy gamma rays. The spacecraft and its 
revolutionary instruments passed their orbital checkout with flying 
colors. 
NASA announced today that GLAST has been renamed the Fermi Gamma-ray 
Space Telescope. The new name honors Prof. Enrico Fermi (1901 - 
1954), a pioneer in high-energy physics. 

"Enrico Fermi was the first person to suggest how cosmic particles 
could be accelerated to high speeds," said Paul Hertz, chief 
scientist for NASA's Science Mission Directorate at NASA Headquarters 
in Washington. "His theory provides the foundation for understanding 
the new phenomena his namesake telescope will discover." 

Scientists expect Fermi will discover many new pulsars in our own 
galaxy, reveal powerful processes near supermassive black holes at 
the cores of thousands of active galaxies and enable a search for 
signs of new physical laws. 

For two months following the spacecraft's June 11 launch, scientists 
tested and calibrated its two instruments, the Large Area Telescope 
(LAT) and the GLAST Burst Monitor (GBM). 

The LAT team today unveiled an all-sky image showing the glowing gas 
of the Milky Way, blinking pulsars, and a flaring galaxy billions of 
light-years away. The map combines 95 hours of the instrument's 
"first light" observations. A similar image, produced by NASA's 
now-defunct Compton Gamma-ray Observatory, took years of observations 
to produce. 

The image shows gas and dust in the plane of the Milky Way glowing in 
gamma rays due to collisions with accelerated nuclei called cosmic 
rays. The famous Crab Nebula and Vela pulsars also shine brightly at 
these wavelengths. These fast-spinning neutron stars, which form when 
massive stars die, were originally discovered by their radio 
emissions. The image's third pulsar, named Geminga and located in 
Gemini, is not a radio source. It was discovered by an earlier 
gamma-ray satellite. Fermi is expected to discover many more 
radio-quiet pulsars, providing key information about how these exotic 
objects work. 

A fourth bright spot in the LAT image lies some 7.1 billion 
light-years away, far beyond our galaxy. This is 3C 454.3 in Pegasus, 
a type of active galaxy called a blazar. It's now undergoing a 
flaring episode that makes it especially bright. 

The LAT scans the entire sky every three hours when operating in 
survey mode, which will occupy most of the telescope's observing time 
during the first year of operations. These fast snapshots will let 
scientists monitor rapidly changing sources. 

The instrument detects photons with energies ranging from 20 million 
electron volts to over 300 billion electron volts. The high end of 
this range, which corresponds to energies more than 5 million times 
greater than dental X-rays, is little explored. 

The spacecraft's secondary instrument, the GBM, spotted 31 gamma-ray 
bursts in its first month of operations. These high-energy blasts 
occur when massive stars die or when orbiting neutron stars spiral 
together and merge. 

The GBM is sensitive to less energetic gamma rays than the LAT. Bursts 
seen by both instruments will provide an unprecedented look across a 
broad gamma-ray spectrum, enabling scientists to peer into the 
processes powering these events. 

NASA's Fermi Gamma-ray Space Telescope is an astrophysics and particle 
physics partnership, developed 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. 

For more information, images and animations on the Web, visit: 



http://www.nasa.gov/glast   

	
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