Skip to main content

James Webb’s mirrors are almost, but not quite, cooled

NASA’s James Webb Space Telescope is nearing completion of the seventh and final step in its alignment process. With its MIRI instrument now cooled to its operating temperature, the telescope is approaching its final, chilly overall temperature as it mirrors cool as well.

The James Webb Space Telescope.
Northrup Grumman/ESA/Hubble

“Now that the instruments are at their operating temperatures, the telescope mirrors will also continue cooling down to their final temperatures, but they are not quite there yet,” writes Jonathan Gardner, Webb deputy senior project scientist at NASA’s Goddard Space Flight Center. “The primary mirror segments and the secondary mirror are made of beryllium (coated with gold). At cryogenic temperatures, beryllium has a long thermal time constant, which means that it takes a long time to cool or to heat up. The primary mirror segments are still cooling, very slowly.”

One of the problems that designers of space missions need to address is that most materials change shape as they cool. If the mirror segments were made of glass, for example, they would warp as their temperatures changed, meaning the careful work of aligning the mirror would be lost. That’s why the mirror is made of beryllium, which has a property called low thermal expansion, meaning it changes shape very little when heated. That means that even as the primary mirror segments cool, they don’t affect the process of aligning the telescope.

As well as the 18 segments of the primary mirror, which currently vary in temperature between 34.4 kelvins to 54.5 kelvins, there is also the secondary mirror to consider. This small, round mirror sits on the end of a long boom arm and is currently at a cooler 29.4 kelvins due to being located further away from the heat sources.

The mirror segments are now cool enough, at below 55 kelvins, that they won’t prevent MIRI from taking science readings. However, the team hopes that they will cool further, by 0.5 to 2 kelvins, which would allow MIRI to take even more accurate readings. The exact temperature which they reach is related to the way that the telescope and its huge sunshield are pointing at the sun. The angle at which the telescope is relative to the sun depends on the target that it is looking at, and this angle changes the telescope’s temperature over time.

When Webb begins science operations this summer, it is expected that its average temperature will drop a bit more as the direction in which it points is changed.

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
James Webb captures a unique view of Uranus’s ring system
This image of Uranus from NIRCam (Near-Infrared Camera) on NASA’s James Webb Space Telescope shows the planet and its rings in new clarity. The Webb image exquisitely captures Uranus’s seasonal north polar cap, including the bright, white, inner cap and the dark lane in the bottom of the polar cap. Uranus’ dim inner and outer rings are also visible in this image, including the elusive Zeta ring—the extremely faint and diffuse ring closest to the planet.

A festive new image from the James Webb Space Telescope has been released, showing the stunning rings of Uranus. Although these rings are hard to see in the visible light wavelength -- which is why you probably don't think of Uranus as having rings like Saturn -- these rings shine out brightly in the infrared wavelength that Webb's instruments operate in.

The image was taken using Webb's NIRCam instrument and shows the rings in even more detail than a previous Webb image of Uranus, which was released earlier this year.

Read more
James Webb spots tiniest known brown dwarf in stunning star cluster
The central portion of the star cluster IC 348. Astronomers combed the cluster in search of tiny, free-floating brown dwarfs.

A new image from the James Webb Space Telescope shows a stunning view of a star cluster that contains some of the smallest brown dwarfs ever identified. A brown dwarf, also sometimes known as a failed star, is an object halfway between a star and a planet -- too big to be a planet but not large enough to sustain the nuclear fusion that defines a star.

It may sound surprising, but the definition of when something stops being a planet and starts being a star is, in fact, a little unclear. Brown dwarfs differ from planets in that they form like stars do, collapsing due to gravity, but they don't sustain fusion, and their size can be comparable to large planets. Researchers study brown dwarfs to learn about what makes the difference between these two classes of objects.

Read more
James Webb provides a second view of an exploded star
A new high-definition image from NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) unveils intricate details of supernova remnant Cassiopeia A (Cas A), and shows the expanding shell of material slamming into the gas shed by the star before it exploded. The most noticeable colors in Webb’s newest image are clumps of bright orange and light pink that make up the inner shell of the supernova remnant. These tiny knots of gas, comprised of sulfur, oxygen, argon, and neon from the star itself, are only detectable by NIRCam’s exquisite resolution, and give researchers a hint at how the dying star shattered like glass when it exploded.

When massive stars run out of fuel and come to the ends of their lives, their final phase can be a massive explosion called a supernova. Although the bright flash of light from these events quickly fades, other effects are longer-lasting. As the shockwaves from these explosions travel out into space and interact with nearby dust and gas, they can sculpt beautiful objects called supernova remnants.

One such supernova remnant, Cassiopeia A, or Cas A, was recently imaged using the James Webb Space Telescope's NIRCam instrument. Located 11,000 light-years away in the constellation of Cassiopeia, it is thought to be a star that exploded 340 years ago (as seen from Earth) and it is now one of the brightest radio objects in the sky. This view shows the shell of material thrown out by the explosion interacting with the gas that the massive star gave off in its last phases of life.

Read more