Challenge: Make It Big

Arianne Rocket Launching

The bigger the telescope, the better its vision. The smaller the telescope, the easier it is to get into space. Webb's designers are working for the best of both worlds — a telescope that starts out small and expands upon arrival.

Imagine digging a tennis court out of the ground, loading it onto a rocket and blasting it to a location 940,000 miles away, four times farther than the Moon. The Webb Telescope, with a mirror that towers over two stories high and a sunshield wide enough to park 21 cars upon, is an intimidating behemoth of a space telescope, the biggest observatory ever sent into orbit.

When it comes to telescopes, “the bigger, the better” always applies. That's because telescopes work by using their large mirrors to collect more light than the human eye can detect on its own. The more light a telescope mirror collects, the sharper the image and the deeper the telescope can see into space.

But the larger the telescope, the more complicated it is to deploy in space. Building Webb requires a constant balance between getting the best science results and ensuring the smoothest functioning. Innovative feats of engineering are needed to ensure that the telescope will deliver on its promise of unrivaled scientific discovery.


In 2014, NASA will load the six-ton James Webb Space Telescope onto an Ariane 5 rocket, which is just a little smaller than the space shuttle. The telescope will be intricately configured and compacted to nestle inside the shroud of the rocket, its solar panel and mirror tower retracted, its primary mirror, sunshield, secondary mirror, communications antennae and momentum flap folded up.

Half an hour after launch, Webb will separate from the rocket and begin its month-long solo journey to its new home, the Second Sun-Earth Lagrange Point.

As Webb travels, its parts will extend and unfold. Its five-layer sunshield will slowly unfurl, stretched taut by cables attached to motors. The delicate layers, each about as thin as plastic wrap, are reinforced with ribs that prevent tearing. The fragility of the layers works in their favor - they are more likely to form the occasional small hole than tear apart. And since the sunshield has so many layers, the next layer or the next can stop any light that penetrates from such a tiny fissure.

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To fit on the rocket within its six-and-a-half-ton weight limit, yet maintain the size necessary to perform its observations, the Webb telescope was deliberately designed to have as little mass as possible, making its structure somewhat flexible. This flexibility makes the telescope susceptible to vibrations whenever it moves — even the tiny movements that keep it pointed.

Vibrations must be minimized. Just as a shaky camera results in blurry photographs, even small tremors will interfere with the telescope's image quality. In fact, telescopes have to be held more still than cameras because their exposures last so long.

Vibration-dampening designs help keep the telescope sound. Rubber shock absorbers cushion the tower that holds the primary mirror. The secondary mirror has “dampers” that use magnets to turn the energy of vibrations into heat, which radiates harmlessly away. The telescope also has a third mirror, the fast steering mirror, that helps cancel out slow oscillations by moving in the direction opposite the motion of the telescope.

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The most important part of Webb's design is, of course, its giant mirror. Mirror size is vital for all telescopes, but particularly for infrared telescopes. The clarity of a telescope's images, or “resolution,” is determined by the size of the mirror versus the size of the wavelength of light. Since infrared has such a long wavelength, a larger mirror is needed to produce a quality image.

The biggest infrared telescope in space now is the compact Spitzer Space Telescope, which has a 2.7 foot (0.8 m) mirror. The Webb telescope's primary mirror is 21.3 feet (6.49 m) across, allowing it to see in infrared as clearly as the Hubble Space Telescope sees in visible light.

Webb's mirror is made up of 18 hexagonal segments. The segments are six-sided because that configuration allows the segments to come closest to forming a circle, the best shape for a telescope mirror. The mirror, folded inside the rocket, opens after the telescope deploys.

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At first, the segments will be looking at different points in the sky. On the ground, Webb's operators will go through a painstaking process of aligning the segments so that they focus on the same point.

Each segment is attached to six legs, allowing the mirrors to tilt, twist, and shift to face the correct direction and position. In addition, a pressure pad in the center of each segment can be moved like a piston, allowing Webb's operators to warp the very shape of the segment to perfectly match the others. Once operators are done, the segments will operate as a single, unified mirror.

Webb's ambitious mirror size is still moderate by ground telescope standards, which have mirrors as wide as 33 feet (10 m). But those mirrors don't have to deal with being launched into space to a destination beyond the reach of even astronauts.

Coasting among the stars, following our planet in its path around the Sun, the Webb telescope will be invisible to us on Earth, too far away to be seen with the naked eye. The giant telescope will make its presence known by the impact it has on the way we view the universe, the horizons it opens on its 10-year journey through the cosmos.

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