Skip to main content

James Webb begins careful, slow process of aligning mirrors

With the exciting process of deployment complete, the James Webb Space Telescope team is now embarking on their next challenge: Aligning the telescope’s mirror segments. This slow, months-long process is required to fine-tune the individual optics into one large, accurate telescope.

The telescope’s primary mirror consists of 18 gold-colored hexagons made of beryllium, which fit together to create a huge mirror 6.5 meters across. It has a secondary mirror as well, which is a smaller round shape and is located at the end of the boom arms. These all require careful tweaking to be in exactly the right position to allow the telescope to be as accurate as possible.

Recommended Videos

To achieve that, the engineers began by sending commands to the 126 actuators which will move the primary mirror segments as well as six devices that position the secondary mirror to ensure that they were working. With that confirmed, they could begin moving the segments off of the snubbers that they were sitting on during launch to absorb vibrations in a process that will take around 10 days.

The adjustment of the mirrors will take around three months in total, and will require many small, careful tweaks. “Getting there is going to take some patience: The computer-controlled mirror actuators are designed for extremely small motions measured in nanometers,” wrote Marshall Perrin from the Space Telescope Science Institute in a blog post. “Each of the mirrors can be moved with incredibly fine precision, with adjustments as small as 10 nanometers (or about 1/10,000th of the width of a human hair). Now we’re using those same actuators instead to move over a centimeter. So these initial deployments are by far the largest moves Webb’s mirror actuators will ever make in space.”

In addition, each actuator needs to work one at a time for safety reasons, and it can only work for a short period to limit how much heat it creates and spreads to the very cold mirrors. So this will be a long, slow process to get the mirrors tuned.

“This may not be the most exciting period of Webb’s commissioning, but that’s OK,” Perrin wrote. We can take the time. During the days that we’re slowly deploying the mirrors, those mirrors are also continuing to slowly cool off as they radiate heat away into the cold of space. The instruments are cooling, too, in a gradual and carefully controlled manner, and Webb is also continuing to gently coast outwards toward L2. Slow and steady does it, for all these gradual processes that get us every day a little bit closer to our ultimate goal of mirror alignment.”

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
James Webb takes rare direct image of a nearby super-Jupiter
Artist’s impression of a cold gas giant orbiting a red dwarf. Only a point of light is visible on the JWST/MIRI images. Nevertheless, the initial analysis suggests the presence of a gaseous planet that may have properties similar to Jupiter.

Even with huge ground-based observatories and the latest technology in space-based telescopes, it's still relatively rare for astronomers to take an image of an exoplanet. Planets outside our solar system are so far away and so small and dim compared to the stars they orbit that it's extremely difficult to study them directly. That's why most observations of exoplanets are made by studying their host stars. Now, though, the James Webb Space Telescope has directly imaged a gas giant -- and it's one of the coldest exoplanets observed so far.

The planet, named Epsilon Indi Ab, is located 12 light-years away and has an estimated temperature of just 35 degrees Fahrenheit (2 degrees Celsius). The fact it is so cool compared to most exoplanets meant that Webb's sensitive instruments were needed to study it.

Read more
One half of this wild exoplanet reaches temperatures of 1,450 degrees Fahrenheit
webb wasp 39b dayside nightside stsci 01j2f12rm1s3n39yj938nhsf93 png

This artist’s concept shows what the exoplanet WASP-39 b could look like based on indirect transit observations from JWST and other space- and ground-based telescopes. Data collected by its NIRSpec (Near-Infrared Spectrograph) show variations between the morning and evening atmosphere of the planet. NASA, ESA, CSA, Ralf Crawford (STScI)

One of the ground-breaking abilities of the James Webb Space Telescope is that researchers can use it to not only detect distant planets but also to peer into their atmosphere. Now, new research using Webb has uncovered differing conditions between morning and evening on a distant exoplanet, the first time such differences have been observed on a planet outside our solar system.

Read more
Webb captures a Penguin and an Egg for its two-year anniversary
This “penguin party” is loud! The distorted spiral galaxy at center, the Penguin, and the compact elliptical galaxy at left, the Egg, are locked in an active embrace. A new near- and mid-infrared image from the James Webb Space Telescope, taken to mark its second year of science, shows that their interaction is marked by a faint upside-down U-shaped blue glow.

This “penguin party” is loud! The distorted spiral galaxy at center, called the Penguin, and the compact elliptical galaxy at left, called the Egg, are locked in an active embrace. A new near- and mid-infrared image from the James Webb Space Telescope, taken to mark its second year of science, shows that their interaction is marked by a faint upside-down U-shaped blue glow. NASA, ESA, CSA, STScI

Today, July 12, marks two years since the first images from the James Webb Space Telescope were unveiled. In that time, Webb has discovered the most distant galaxies known, uncovered surprises about the early universe, peered into the atmospheres of distant planets, and produced a plethora of beautiful images of space.

Read more