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.”

Recommended Videos

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.

Please enable Javascript to view this content

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.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
James Webb spots another pair of galaxies forming a question mark
The galaxy cluster MACS-J0417.5-1154 is so massive it is warping the fabric of space-time and distorting the appearance of galaxies behind it, an effect known as gravitational lensing. This natural phenomenon magnifies distant galaxies and can also make them appear in an image multiple times, as NASA’s James Webb Space Telescope saw here.

The internet had a lot of fun last year when eagle-eyed viewers spotted a galaxy that looked like a question mark in an image from the James Webb Space Telescope. Now, Webb has stumbled across another questioning galaxy, and the reasons for its unusual shape reveal an important fact about how the telescope looks at some of the most distant galaxies ever observed.

The new question mark-shaped galaxy is part of an image of galaxy cluster MACS-J0417.5-1154, which is so massive that it distorts space-time. Extremely massive objects -- in this case, a cluster of many galaxies -- exert so much gravitational force that they bend space, so the light traveling past these objects is stretched. It's similar using a magnifying glass. In some cases, this effect, called gravitational lensing, can even make the same galaxy appear multiple times in different places within one image.

Read more
James Webb is explaining the puzzle of some of the earliest galaxies
This image shows a small portion of the field observed by NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) for the Cosmic Evolution Early Release Science (CEERS) survey. It is filled with galaxies. The light from some of them has traveled for over 13 billion years to reach the telescope.

From practically the moment it was turned on, the James Webb Space Telescope has been shaking cosmology. In some of its very earliest observations, the telescope was able to look back at some of the earliest galaxies ever observed, and it found something odd: These galaxies were much brighter than anyone had predicted. Even when the telescope's instruments were carefully calibrated over the few weeks after beginning operations, the discrepancy remained. It seemed like the early universe was a much busier, brighter place than expected, and no one knew why.

This wasn't a minor issue. The fact early galaxies appeared to be bigger or brighter than model predicted meant that something was off about the way we understood the early universe. The findings were even considered "universe breaking." Now, though, new research suggests that the universe isn't broken -- it's just that there were early black holes playing tricks.

Read more
James Webb Telescope captures gorgeous galaxy with a hungry monster at its heart
Featured in this new image from the NASA/ESA/CSA James Webb Space Telescope is Messier 106, also known as NGC 4258. This is a nearby spiral galaxy that resides roughly 23 million light-years away in the constellation Canes Venatici, practically a neighbour by cosmic standards. Messier 106 is one of the brightest and nearest spiral galaxies to our own and two supernovae have been observed in this galaxy in 1981 and 2014.

A new image from the James Webb Space Telescope shows off a nearby galaxy called Messier 106 -- a spiral galaxy that is particularly bright. At just 23 million light-years away (that's relatively close by galactic standards), this galaxy is of particular interest to astronomers due to its bustling central region, called an active galactic nucleus.

The high level of activity in this central region is thought to be due to the monster that lurks at the galaxy's heart. Like most galaxies including our own, Messier 106 has an enormous black hole called a supermassive black hole at its center. However, the supermassive black hole in Messier 106 is particularly active, gobbling up material like dust and gas from the surrounding area. In fact, this black hole eats so much matter that as it spins, it warps the disk of gas around it, which creates streamers of gas flying out from this central region.

Read more