NASA'S Next Generation Space Telescope Marks Key Milestone

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April 14, 2011

Dwayne Brown/Trent Perrotto 
Headquarters, Washington                                
202-358-1726/0321 
dwayne.c.brown@xxxxxxxx/trent.j.perrotto@xxxxxxxx 

Kimberly Newton 
Marshall Space Flight Center, Huntsville, Ala.      
256-544-0371 
kimberly.d.newton@xxxxxxxx 


RELEASE: 11-111

NASA'S NEXT GENERATION SPACE TELESCOPE MARKS KEY MILESTONE

HUNTSVILLE, Ala. -- The first six of 18 segments that will form NASA's 
James Webb Space Telescope's primary mirror for space observations 
will begin final round-the-clock cryogenic testing this week. These 
tests will confirm the mirrors will respond as expected to the 
extreme temperatures of space prior to integration into the 
telescope's permanent housing structure. 

The X-ray and Cryogenic Facility at NASA's Marshall Space Flight 
Center in Huntsville, Ala. will provide the space-like environment to 
help engineers measure how well the telescope will image infrared 
sources once in orbit. 

Each mirror segment measures approximately 4.3 feet (1.3 meters) in 
diameter to form the 21.3 foot (6.5 meters), hexagonal telescope 
mirror assembly critical for infrared observations. Each of the 18 
hexagonal-shaped mirror assemblies weighs approximately 88 pounds (40 
kilograms). The mirrors are made of a light and strong metal called 
beryllium, and coated with a microscopically thin coat of gold to 
enable the mirror to efficiently collect light. 

"The six flight mirrors sitting ready for cryogenic acceptance tests 
have been carefully polished to their exact prescriptions," said 
Helen Cole, project manager for Webb activities at Marshall. "It's 
taken the entire mirror development team, including all the partners, 
over eight years of fabrication, polishing and cryogenic testing to 
get to this point." 

During cryogenic testing, the mirrors are subjected to extreme 
temperatures dipping to minus 415 degrees Fahrenheit (-248C) in a 
7,600 cubic-foot (approximately 215 cubic meters) helium-cooled 
vacuum chamber. This permits engineers to measure in extreme detail 
how the shape of the mirror changes as it cools. This simulates the 
actual processes each mirror will undergo as it changes shape over a 
range of operational temperatures in space. 

"This final cryotest is expected to confirm the exacting processes 
that have resulted in flight mirrors manufactured to tolerances as 
tight as 20 nanometers, or less than one millionth of an inch," said 
Scott Texter, Webb Optical Telescope element manager at Northrop 
Grumman in Redondo Beach, Calif. 

A second set of six mirror assemblies will arrive at Marshall in July 
to begin testing, and the final set of six will arrive during the 
fall. 
The Webb Telescope is NASA's next-generation space observatory and 
successor to the Hubble Space Telescope. The most powerful space 
telescope designed, Webb will observe the most distant objects in the 
universe, provide images of the very first galaxies ever formed and 
help identify unexplored planets around distant stars. The telescope 
will orbit approximately one million miles from Earth. 

"The Webb telescope continues to make good technological progress," 
said Rick Howard, JWST Program Director in Washington. "We're 
currently developing a new baseline cost and schedule to ensure the 
success of the program." 

The telescope is a combined project of NASA, the European Space Agency 
and the Canadian Space Agency. Northrop Grumman is the prime 
contractor under NASA's Goddard Space Flight Center in Greenbelt, Md. 
Ball Aerospace & Technologies Corp. in Boulder, Colo., is responsible 
for mirror development. L-3- Tinsley Laboratories Inc. in Richmond, 
Calif. is responsible for mirror grinding and polishing. 
For more information about the James Webb Space Telescope, visit: 



http://www.jwst.nasa.gov 

	
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