Webb's fully deployed operational configuration is far too large to fit into any available rocket so it was designed to fold into a compact launch configuration that fit inside the Ariane 5. In the two weeks after launch, the entire observatory underwent a highly choreographed transformation—unfurling, extending and expanding to a configuration that is very different to how it looks when stored inside the rocket for liftoff.
Quick Facts
Quick Facts
Video Overview
Webb Folded
Webb is so large that it could not fit into any available rocket fairing so it was designed to fold into a compact launch configuration that fit inside the Arianne 5 rocket. This animation shows highlights the size differences between Webb's fully deployed configuration and its launch configuration folded to fit in the rocket.
Webb Unfolded
After launch while on its journey to L2, engineers on the ground remotely orchestrated and monitored a complex sequence of deployments in the hours and days immediately after the launch. This animation shows the nominal sequence for these deployments.
In Depth
Webb's design, development and intensive testing were keys to the success of the complex deployment process. There were over 50 major deployment steps, with 178 release mechanisms that had to perform perfectly or any one of over 300 single points of failure could have diminished or crippled the mission.
Not only that, but Webb and its subsystems were sourced from all over the world. The assembled optical telescope element alone moved multiple times across the USA before final integration and test in California with the remainder of the spacecraft. Webb's final move involved shipping it by boat from California, through the Panama Canal and to the launch pad in French Guiana in South America. Each of these moves is risky. In the end, Webb deployed and came online exceeding requirements and expectations.
Below you will find sections covering various aspects of design and deployment in deeper detail.
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Folding For Launch
Webb's design was not only driven by the science requirements for the mission, but also by the need to be able to fold it tightly for launch and succesfully deploy it in space while in flight to its final destination orbitting L2. These images highlight some of the major design features and preparation steps for launch.



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Unfolding Webb
Webb's First 6 Months
The Ariane 5 launch vehicle provided thrust for roughly 26 minutes after liftoff from French Guiana. Moments after the upper (second) stage engine cut-off, Webb separated from the upper stage and began flying on its own in its fully stowed state. Deployments began minutes after separation.
- First day: The solar panel automatically deployed to supply Webb with power and the high gain antenna deployed for high bandwidth communications. The Ariane launch sent Webb on a direct route to L2, without first orbiting Earth. During the first day, a first and most important trajectory correction maneuver was executed using small rocket engines aboard Webb itself. Ariane's launch was so accurate that very little correction was needed, saving fuel for operations and extending Webb's operational lifetime.
- In the first week: Sunshield deployment: Shortly after a second trajectory correction maneuver was executed, the sequence of major deployments began with the fore and aft sunshield pallets. The next step was separation of the spacecraft bus and telescope by extending the telescoping tower between them. The tower extended about 2 meters, which was necessary at this point in the sequence so that the rest of the sunshield deployment could proceed. Next, the sunshield membranes were unpinned and the telescoping sunshield midbooms were extended – first the port side and then the starboard side – pulling the membranes out with them. The last sunshield deployment step was the tensioning of the membranes. In the meantime, other things like radiators were released and deployed.
- Second Week: Mirror/Telescope Deployment: During the second week after launch, we finished deploying the telescope structures by unfolding and latching the secondary mirror tripod and rotating and latching the two primary mirror wings. This brought Webb into its fully deployed operational configuration.
- 1st Month: Cooldown, instrument turn-on, and insertion into orbit around L2. The telescope and scientific instruments started to cool rapidly in the shade of the sunshield, but it took several weeks for them to cool all the way down and reach stable temperatures. This cooldown was carefully controlled with strategically-placed electric heater strips so that everything shrinks carefully and so that water trapped inside parts of the observatory can escape as gas to the vacuum of space and not freeze as ice onto mirrors or detectors, which would degrade scientific performance. We unlocked all the primary mirror segments and the secondary mirror and verified that we can move them. Near the end of the first month, we executed the last mid-course maneuver to insert into the optimum orbit around L2. During this time we also powered-up the scientific instrument systems. The remaining five months of commissioning were all about aligning the optics and calibrating the scientific instruments.
- In the second, third and fourth months: Initial optics checkouts, and telescope alignment. Using the Fine Guidance Sensor, we pointed Webb at a single bright star and demonstrated that the observatory could acquire and lock onto targets, and we took data mainly with NIRCam. But because the primary mirror segments had yet to be aligned to work as a single mirror, there were distorted images of the same single target star. We then embarked on the long process of aligning all the telescope optics, beginning with identifying which primary mirror segment went with which image by moving each segment one at a time and ended a few months later with all the segments aligned as one and the secondary mirror aligned optimally. Cooldown effectively ended and the cryocooler started running at its lowest temperature and MIRI started taking good data too.
- In the fifth and sixth months: Calibration and completion of commissioning. We meticulously calibrated all of the scientific instruments’ many modes of operation while observing representative targets, and we demonstrated the ability to track “moving” targets, which were nearby objects like asteroids, comets, moons, and planets in our own solar system. We made “Early Release Observations,” to be revealed right after commissioning was over, that showcased the capabilities of the observatory.
- After six months: “Science operations!” Webb began its science mission and started to conduct routine science operations.
29 Days on the Edge
The 29 days following Webb's liftoff were an exciting but harrowing time. Thousands of parts must work correctly, in sequence, to unfold Webb and put it in its final configuration, all while it flies through the expanse of space alone, to a destination nearly one million miles away. As the largest and most complex telescope ever sent into space, the James Webb Space Telescope is a technological marvel. By necessity, Webb takes on-orbit deployments to the extreme. Each step can be controlled expertly from the ground, giving Webb’s Mission Operations Center full control to circumnavigate any unforeseen issues with deployment.
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