How a gold-plated mirror captures the universe's first light

How the James Webb Space Telescope JWST Actually works! · 15:39 · Video: Arvin Ash · Watch at the source

In short: To see the beginning of time, we have to look for light that has been stretched across billions of years. The James Webb Space Telescope doesn't just take pictures; it uses a massive, folding mirror and a tennis-court-sized sunshield to peer through cosmic dust and into the infrared past.

The James Webb Space Telescope (JWST) is engineered to detect infrared light, which allows it to see through dense space dust and observe objects that are 'red shifted' by the expansion of the universe. Because the most distant objects are stretched into these longer wavelengths, the JWST can see farther back in time than previous observatories. To maximize its light-gathering power, it features a primary mirror 6.5 meters in diameter—roughly 100 times more powerful than Hubble—constructed from 18 ultra-lightweight beryllium segments that unfold like origami in space.

The telescope's design is a feat of thermal engineering. To detect faint infrared signals, the instruments must stay incredibly cold. The JWST orbits the sun at the second Lagrange point (L2), about 1.5 million kilometers away from Earth. At this location, the sun, Earth, and the telescope stay in a stable line. To protect the sensitive equipment from the sun's heat, a five-layer sunshield measuring 22 meters by 12 meters attenuates heat by more than a million times. For the Mid-Infrared Instrument (MIRI), a cryocooler further chills the detectors to 7 kelvins (minus 447 Fahrenheit).

The light collection process begins when infrared light hits the gold-coated primary mirror, which is ideal for reflecting infrared radiation. The light is reflected onto a smaller secondary mirror and into the Aft-Optics System, which focuses it onto sensors made of mercury cadmium telluride—a lab-grown crystal that converts infrared light directly into electricity. Beyond imaging, the telescope uses spectrometers to analyze the chemical signatures of distant planets, searching for water, oxygen, methane, and ammonia to identify potential signs of life.

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