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.

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
The expansion rate of the universe still has scientists baffled
This image of NGC 5468, a galaxy located about 130 million light-years from Earth, combines data from the Hubble and James Webb space telescopes. This is the most distant galaxy in which Hubble has identified Cepheid variable stars. These are important milepost markers for measuring the expansion rate of the Universe. The distance calculated from Cepheids has been cross-correlated with a Type Ia supernova in the galaxy. Type Ia supernovae are so bright they are used to measure cosmic distances far beyond the range of the Cepheids, extending measurements of the Universe’s expansion rate deeper into space.

The question of how fast the universe is expanding continues to confound scientists. Although it might seem like a fairly straightforward issue, the reality is that it has been perplexing the best minds in physics and astronomy for decades -- and new research using the James Webb Space Telescope and the Hubble Space Telescope doesn't make the answer any clearer.

Scientists know that the universe is expanding over time, but what they can't agree on is the rate at which this is happening -- called the Hubble constant. There are two main methods used to estimate this constant: one that looks at how fast distant galaxies are moving away from us, and one that looks at leftover energy from the Big Bang called the cosmic microwave background. The trouble is, these two methods give different results.

Read more
See what James Webb and Hubble are observing right now with this tool
james webb hubble live tracker screenshot 2024 03 06 220259

If you're looking for a relaxing way to peruse the fascinating sights of space on your lunch break, then a newly updated tool from NASA has you covered. The Space Telescope Live tools show the current targets of the James Webb Space Telescope and the Hubble Space Telescope, letting you browse the cosmos from the perspective of two of the hardest-working telescopes out there.

You can visit the web-based tools at WebbTelescope for the James Webb Space Telescope and HubbleSite for the Hubble Space Telescope. Clicking on a link will bring you to a portal showing the current and past observations of the telescope and a ton of detail about the observations.

Read more
This famous supernova remnant is hiding a secret
Webb’s NIRCam (Near-Infrared Camera) captured this detailed image of SN 1987A (Supernova 1987A). At the center, material ejected from the supernova forms a keyhole shape. Just to its left and right are faint crescents newly discovered by Webb. Beyond them an equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots. Exterior to that is diffuse emission and two faint outer rings. In this image blue represents light at 1.5 microns (F150W), cyan 1.64 and 2.0 microns (F164N, F200W), yellow 3.23 microns (F323N), orange 4.05 microns (F405N), and red 4.44 microns (F444W).

When massive stars reach the end of their lives and explode in a supernova, they can leave behind huge structures in space called supernova remnants. These are often favorite targets of astronomers because of their beautiful and distinctive shapes. They include the famous SN 1987A remnant that was imaged by the James Webb Space Telescope last year. Now, astronomers using Webb have peered closer at this remnant and found something special inside.

The SN 1987A supernova was first observed in 1987 (hence its name) and was bright enough to be seen with the naked eye, making it extremely recent by astronomical standards. Stars live for millions or even billions of years, so observing one coming to the end of its life in real time is a real scientific treat. When this star died, it created a kind of supernova called a core collapse, or Type II, in which the heart of the star runs out of fuel, causing it to collapse suddenly and violently. This collapse it so severe that the material rebounds and is thrown out in an explosion traveling up to a quarter of the speed of light.

Read more