Showing posts with label NASA. Show all posts
Showing posts with label NASA. Show all posts

Wednesday, April 21, 2010

NASA Administrator Visits Marshall's X-Ray and Cryogenic Facility



NASA Administrator Charles Bolden, second from right, listens as Dave Chaney, right, a principle optical engineer for Ball Aerospace Technologies Corp. in Boulder, Colo., explains how the James Webb Space Telescope mirror segments are tested in the Marshall Space Flight Center's X-ray and Cryogenic Facility, or XRCF, in Building 4718. From front are Helen Cole, Webb telescope activities project manager at Marshall; Charles Scales, NASA associate deputy administrator; and Robert Lightfoot, Marshall center director.

The XRCF at the Marshall Center is the world's largest X-ray telescope test facility and a unique, cryogenic, clean room optical test facility. Cryogenic testing will take place in a 7,600 cubic foot helium cooled vacuum chamber, chilling the Webb flight mirror from room temperature down to frigid -414 degrees Fahrenheit. While the mirrors change temperature, test engineers will precisely measure their structural stability to ensure they will perform as designed once they are operating in the extreme temperatures of space.

NASA's James Webb Space Telescope is a large, infrared-optimized space telescope that will be the premier observatory of the next decade. It will study every phase in the history of our Universe, ranging from the first luminous glows after the Big Bang, to the formation of solar systems capable of supporting life on planets like Earth, to the evolution of our own Solar System. Its instruments will be designed to work primarily in the infrared range of the electromagnetic spectrum, with some capability in the visible range.

Northrop Grumman is the prime contractor for the Webb telescope, leading a design and development team under contract to the Goddard Center.

The James Webb Space Telescope is expected to launch in 2013. NASA's Goddard Space Flight Center in Greenbelt, Md. is managing the overall development effort for the Webb telescope. The telescope is a joint project of NASA and many U.S. partners, the European Space Agency and the Canadian Space Agency. (NASA/MSFC/David Higginbotham)

Thursday, March 18, 2010

Turning up the heat: Finding out how well the Webb telescope's sunshield will perform


Keeping an infrared telescope at very cold operating temperatures isn't an option, it's an absolute necessity. For the James Webb Space Telescope to see the traces of infrared light generated by stars and galaxies billions of light years away, it must be kept at cryogenic temperatures of under 50 Kelvin (-370 F). Otherwise, sunlight would warm the telescope and this heat from the telescope itself will swamp the very faint astronomical signals, effectively blinding the telescope's eye. The job of the huge, five-layer sunshield is to keep that from happening.

Serving as a radiation blocker, the sunshield is subjected to nearly 100,000 thermal watts of solar heat, and reduces that to one tenth of a watt on the cold side, a million to one reduction.

But how do you test a complicated structure the size of a tennis court? There isn't a cryogenic chamber on the planet big enough and building one doesn't make sense from a budget and practical standpoint. So Webb engineers have constructed a 1/3-scale model and a test facility to perform the critical thermal test of the sunshield system.

The thermal test had two main goals: 1- to verify that the sunshield design can actually block and redirect the sun's energy before it reaches the telescope; and 2- to verify the accuracy of computer thermal models used to predict how the full-size sunshield will perform. 'The flight sunshield will be deployed and visually inspected prior to flight, but only a computer simulation of its thermal performance will be used to determine if it's ready to launch,' explains Keith Parrish, Webb telescope Sunshield Manager at NASA's Goddard Space Flight Centre, Greenbelt, Md.

'This is very similar to wind tunnel testing of large aircraft,' he notes. 'Most aircraft, especially large commercial airliners, are simply too large to undergo full-size testing. Computer models, which extrapolate the test data from smaller scale model wind tunnel tests, are used to verify final design and predict the full size aircraft's performance. Our Webb sunshield 1/3-scale model test is a very similar approach.'

In space, the sunshield will be heated by the sun. For ground testing, the 1/3-scale model was placed in a thermal vacuum test chamber at lead contractor Northrop Grumman's manufacturing facilities in Redondo Beach, Calif. The sun's heat was simulated by electrical heater plates placed very close to, but not touching layer 1, the warm sun- facing layer. Power to the heaters was steadily increased until layer 1 reached similar temperatures as those expected in flight, well over 100 degrees C (212 F, the boiling point of water at sea level).

Approximately 400 temperature sensors were placed all over the sunshield. 'We also keep an eye on the chamber's gaseous helium-refrigerated shroud temperatures and liquid helium cooling plates,' adds Parrish. 'These cooling plates simulate the cold background temperature of space at the orbit of Webb, which is around 7 Kelvin (-446.8 F). We can't get these plates all the way down to 7 K, which is pretty close to absolute zero. The plates typically get down to the 15 to 25 K (-434.4 F. to -414.4 F) temperature range, so exact knowledge of their temperature is critical to understanding the sunshield's performance.'

The engineering team used the 1/3-scale tests for a trial run of a device called a radiometer. Hung or mounted around the sunshield, these devices measure the heat radiation that is bouncing around and between the sunshield, the cold plates and the chamber walls. Since this kind of effect doesn't occur in space, it's important to understand how this heat bouncing impacts the test results. When the flight instruments and observatory are tested at Goddard and Johnson Space Centre, these devices need to be working well.

Seven different testing conditions were used to gather temperature data, and these test conditions were tailored so that engineers can study how the sunshield performs in space under a variety of conditions. Some test conditions exaggerated or increased temperatures and heat flows in specific areas of the sunshield. Even though these test conditions do not simulate flight conditions, they're designed to isolate and better define particular variables used in computer thermal simulations. 'One specific test condition used a mechanism in the chamber to change or warp the sunshield's shape,' Parrish explained. 'Since proper shape is critical to the sunshield's performance, this test condition gave engineers important data so they could see if computer models can actually predict the thermal impact of shape changes.'

After the temperature data was gathered, engineers ran computer models over and over again with small changes to mimic the actual test conditions. The goal is to better match the temperature data from the sensors on the sunshield to the computer models. 'This is really the critical part in the whole testing process,' says Parrish. 'Gathering the test data was just the beginning. Understanding that data and how it applies to the flight sunshield's predicted thermal performance is the critical step.'

To understand how the membrane shape affects thermal performance, a Light Detection And Ranging (LIDAR) laser device took highly accurate shape measurements on each of the five layers of the sunshield at room temperature. These measurements were used to validate the computer model predictions of each membrane under ambient conditions. The computer models were then used to predict the membrane shapes over the various test conditions.

Later this spring, the thermal chamber will be modified with a window so that the LIDAR device can see into the chamber and measure the shape of layer 5, the coldest layer, near its cryogenic operating temperature, approximately 77 K (-320.8 F). This test will allow the engineers to confirm if the computer model's prediction of shape at temperature is correct.

Careful planning and following rigourous procedures paid off - the test was very successful because all test objectives were met and engineers were able to collect the data they needed. That data is being carefully analysed to see if the test temperatures accurately reflect the thermal performance of the flight sunshield. Data analysis is a lengthy process scheduled to be complete by the end of March 2010.

The 1/3-scale tests go a long way in establishing model verification well in advance of the flight test. As a result, the fidelity of the master model is improved, which adds flight confidence and reduces technical risk.

The thermal testing took place over four weeks, from Nov. 23 to Dec. 19, 2009 in Northrop Grumman's largest thermal vacuum chamber at the company's Aerospace Systems manufacturing facilities in Redondo Beach, Calif.

Source: NASA/Goddard Space Flight Centre

Tuesday, May 19, 2009

NASA's James Webb Space Telescope Unfolds by Animation


Still from animation
> View streaming Windows Media Viewer animation
Credit: Northrop Grumman Aerospace Systems

Still from animation
> View streaming Windows Media Viewer animation
Credit: Northrop Grumman Aerospace Systems

Artist's rendition of the James Webb Space Telescope
>View larger image
Credit: NASA


Although engineers, scientists and manufacturers are still in the process of building all of the instruments that will fly aboard NASA's James Webb Space Telescope, they had to figure out long ago, how it was going to "unfold" in space. That's because the Webb Telescope is so big that it has to be folded up for launch. Now, animators have made that "unfolding" come to life in two new videos.

A brand new animation of how NASA's massive next-generation space telescope will open up in space once it achieves orbit, was created by the Image center at Northrop Grumman Aerospace Systems, Redondo Beach, Calif. The Webb Telescope is roughly 65 feet (21 meters) from end to end and about 3 stories high.

"Animation helps designers and their colleagues to fully visualize and explain the complex motions required to deploy this observatory," said Mike Herriage, Webb Telescope Deputy Program Manager at Northrop Grumman. "And while it’s a visual tool, producing accurate animation is a technical challenge as well."

The James Webb Space Telescope is a large, infrared space telescope. It will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy. It will peer through dusty clouds to see stars forming planetary systems, connecting the Milky Way to our own Solar System.

The Webb Telescope is extremely large and cannot fit in a rocket unless it is folded. It has a sunshield the size of a tennis court and an 18-segment mirror that looks like a honeycomb. Because of its large size, the telescope needs to be folded up to fit in the rocket. The sunshield will be compactly folded, much like a parachute, around the front and back of the telescope. The mirror segments are mounted on the "spine" or backplane of the telescope and the segments on the left and right sides of the honeycomb shape are folded in the rocket.

Once the Webb telescope is on its way to its final orbit, approximately 1 million miles from the Earth, engineers at Northrop Grumman will issue commands to the Webb Telescope to unfold it. "Think of the sunshield as five candy wrappers the size of a tennis court," said Mark Clampin, Webb Telescope Observatory Project Scientist at NASA’s Goddard Space Flight Center, Greenbelt, Md.

The animation shows the first part of the telescope to unfold is the solar panel, followed by the communications antenna. Next, the five layers of sunshield will drop into place from the front and back, spread out into a kite shape. The "secondary mirror support structure," an arm-like feature holding the secondary mirror assembly will then drop down from its folded center perch, and finally, the side mirror segments will be moved forward to form the complete "honeycomb."

"There are videos showing a simple deployment and a version that includes detailed views of key points in the sequence," Clampin said. "There are 2 and 4 megabyte versions of each video and they are high definition."

James Webb Space Telescope is a joint project of NASA, the European Space Agency and the Canadian Space Agency.