November 14, 2016 – Engineers and technicians working on the James Webb Space Telescope (JWST) successfully completed the first important optical measurement of Webb’s fully assembled primary mirror, called a Center of Curvature test.
Taking a “before” optical measurement of the telescope’s deployed mirror is crucial before the telescope goes into several stages of rigorous mechanical testing. These tests will simulate the violent sound and vibration environments the telescope will experience inside its rocket on its way into space. This environment is one of the most stressful structurally and could alter the shape and alignment of Webb’s primary mirror, which could degrade or, in the worst case, ruin its performance.
Webb has been designed and constructed to withstand its launch environment, but it must be tested to verify that it will indeed survive and not change in any unexpected way. Making the same optical measurements both before and after simulated launch environment testing and comparing the results is fundamental to Webb’s development, assuring that it will work in space.
“This is the only test of the entire mirror where we can use the same equipment during a before and after test,” said Ritva Keski-Kuha, the test lead and NASA’s Deputy Telescope Manager for Webb at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “This test will show if there are any changes or damages to the optical system.”
In order to conduct the test, optical engineers set up an interferometer, the main device used to measure the shape of Webb’s mirror. Waves of visible light are less than a thousandth of a millimeter long, and optics like Webb’s need to be shaped and aligned even more accurately than this to work correctly. Making measurements of the mirror shape and position by lasers prevents physical contact and damage (scratches to the mirror). So scientists use wavelengths of light to make tiny measurements. By measuring light reflected off the optics using an interferometer, they are able to measure extremely small changes in shape or position. An interferometer gets its name from the process of recording and measuring the ripple patterns that result when different beams of light mix and their waves combine or ‘interfere.’
During the test conducted by a team from NASA Goddard, Ball Aerospace of Boulder, Colorado, and the Space Telescope Science Institute in Baltimore Maryland, temperature and humidity conditions in the cleanroom were kept incredibly stable to minimize drift in the sensitive optical measurements over time. Even so, tiny vibrations are ever-present in the cleanroom that cause jitter during measurements, so the interferometer is a ‘high-speed’ one, taking 5,000 ‘frames’ every second, which is a faster rate than the background vibrations themselves. This allows engineers to subtract out jitter and get good, clean results.
The Center of Curvature test measures the shape of Webb’s main mirror by comparing light reflected off of it with light from a computer-generated hologram that represents what Webb’s mirror ideally should be. By interfering the beam of light from Webb with the beam from the hologram reference, the interferometer accurately compares the two by measuring the difference to incredible precision.
“Interferometry using a computer-generated hologram is a classic modern optical test used to measure mirrors,” said Keski-Kuha.
With the largest mirror of any space telescope, taking this measurement is a challenge. “We have spent the last four years preparing for this test,” said David Chaney, Webb’s primary mirror metrology lead at Goddard. “The challenges of this test include the large size of the primary mirror, the long radius of curvature, and the background noise. Our test is so sensitive we can measure the vibrations of the mirrors due to people talking in the room.”
After the measurements come back from the interferometer the team will analyze the data to make sure the mirrors are aligned perfectly before the launch environment tests. The Center of Curvature test will be repeated after the launch environment testing and the results compared to confirm that Webb’s optics will work after their launch into space.
The most powerful space telescope ever built, the Webb telescope will provide images of the first galaxies ever formed, and explore planets around distant stars. The primary mirror consists of 18 hexagonal mirrors built by Ball Aerospace & Technologies Corp. in Boulder, Colorado. Once on orbit, the 18 hexagonal segments will work together as one 21.3-foot (6.5-meter) primary mirror, the largest mirror ever flown in space and the first to deploy in space. Ball Aerospace was also responsible for developing the secondary mirror, tertiary mirror and fine-steering mirror.
JWST is a joint project of NASA, the European Space Agency and the Canadian Space Agency. The Near Infrared Camera (NIRCam) instrument for the James Webb Space Telescope (JWST) is being developed by Lockheed Martin, under contract with the University of Arizona. NIRCam is the primary science camera on JWST, and also functions as the sensor that is used to align the observatory’s primary mirror.