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Astronomy · Space Telescopes

James Webb Space Telescope

The great infrared observatory of the modern era.

Type
Infrared telescope
Mirror
Large segmented, gold-coated primary mirror
Location
Near the Sun–Earth L2 point
Operators
NASA, ESA, and CSA

NASA/Goddard Space Flight Center · NASA media (public domain)

Gallery

By the Dozen: NASA's James Webb Space Telescope Mirrors

A view of the one dozen (out of 18) flight mirror segments that make up the primary mirror on NASA's James Webb Space Telescope have been installed at NASA's Goddard Space Flight Center.

2016

NASA/Goddard Space Flight Center · NASA media (public domain)

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An infrared eye

The James Webb Space Telescope is designed to observe infrared light. Because the expansion of the universe stretches light from the most distant galaxies into the infrared, Webb can see objects from the universe's early history.

Built to stay cold

Webb uses a large segmented primary mirror to gather faint light and a tennis-court-sized sunshield to block the Sun's heat. Operating far from Earth and kept very cold, it can detect faint infrared signals.

Seeing through dust

Infrared light passes through clouds of dust that block visible light, so Webb can look inside stellar nurseries and study disks where planets form, as well as the atmospheres of exoplanets. Its launch and journey are covered under Space Missions.

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