- Vital Facts
Fact sheet on the Webb Mission.
- FAQ Lite
The most popular questions about Webb. (General Public)
- FAQ Full
All the major aspects of the Webb Mission are covered here. (General Public)
- Technical FAQ
Technical FAQ on a variety of mission issues, aspects and capabilities. (Science/Technical)
- Solar System Observations FAQ
Technical FAQ specifically on Solar System observations. (Science/Technical)
- Q & A with engineers cryo-testing the telescope. (new window)
- Lee Feinberg AMA: Optical Telescope Element Manager for Webb (new window)
Lee Feinberg talks about the top 3 things that Webb can do that Hubble cannot and more.
- Paul Geithner: Freezing NASA's Webb Telescope Is a Matter of Survival (new window)
Paul Geithner (Webb Deputy Project Manager, Technical) provides answers to questions about the kind of freezing temperatures the Webb telescope will endure in space. (General Public)
- Paul Geithner: Components & Structure of Webb (new window)
The Webb telescope is a showcase for new technologies. Recently Paul Geithner provided a closer look at the technologies on the observatory. (General Public)
- Paul Geithner: It's All About Infrared - Why Build Webb (new window)
Paul Geithner provides insight on why the Webb telescope focuses on the infrared. (General Public)
- Paul Geithner: James Webb Space Telescope Coming Together (new window)
Paul Geithner discusses progress, plans and next steps in building the Webb Telescope. (General Public)
- John Mather: "Ask Me Anything"
Dr. John Mather (Nobel Laureate and Webb Senior Project Scientist) answering questions on Reddit. (General Public)
- John Mather: Webb Q&A 1
Dr. John Mather captured on Twitter during our first Tweet Chat. (General Public)
- John Mather: Webb Q&A 2
Dr. John Mather captured on Twitter during our second Tweet Chat. (General Public)
- Mark Clampin: Exoplanets
Dr. Mark Clampin (Webb Observatory Project Scientist) answers questions about Webb and exoplanets.
- SXSW: Finding Life on Other Planets
During SXSW 2014, we held a tweet-chat with some of the scientists on the"First Signs: Finding Life on Other Planets" panel.
- Women of Webb Q&A
Women with diverse jobs on the James Webb Space Telescope answered questions about the female experience working on a NASA flagship mission in the TwoXChromosomes subreddit.
- Focus on XSTEM
During the USA Science & Engineering Festival in April 2014 and focused on STEM (Science, Technology, Engineering, Math) topics.
- Sara Seeger: Search for Life Part 1 | Part 2
MIT's Dr. Sara Seager answered questions about exoplanets, the search for life, and the next technologies (like Webb!)
What is the James Webb Space Telescope?
The James Webb Space Telescope, also called Webb or JWST, is a large, space-based observatory, optimized for infrared wavelengths, which complements and extends the discoveries of the Hubble Space Telescope. Webb launched on December 25, 2021, and its first full-color images and data were released to the world on July 12, 2022.
It covers longer wavelengths of light than Hubble and has greatly improved sensitivity. The longer wavelengths enable Webb to look further back in time to see the first galaxies that formed in the early universe, and to peer inside dust clouds where stars and planetary systems are forming today.
What are the most exciting things we will learn?
We have yet to observe the era of our universe’s history when galaxies began to form. We have a lot to learn about how galaxies got supermassive black holes in their centers, and we don't really know whether the black holes caused the galaxies to form or vice versa. We haven't been able to see inside dust clouds with high resolution, where stars and planets are being born nearby, but Webb is now able to do just that. We don't know how many planetary systems might be hospitable to life, but Webb could tell whether some Earth-like planets have enough water to have oceans. We don't know much about dark matter or dark energy, but we are expecting to learn more about where the dark matter is now, and we hope to learn the history of the acceleration of the universe that we attribute to dark energy. And then, there are the surprises we can't imagine!
Why is Webb an infrared telescope?
By viewing the universe at infrared wavelengths Webb is now showing us things never before seen by any other telescope. It is only at infrared wavelengths that we can see the first stars and galaxies forming after the Big Bang. And it is with infrared light that we can see stars and planetary systems forming inside clouds of dust that are opaque to visible light.
The primary goals of Webb are to study galaxy, star and planet formation in the universe. To see the very first stars and galaxies that formed in the early universe, we have to look deep into space to look back in time (because it takes light time to travel from there to here, the farther out we look, the further we look back in time).
The universe is expanding, and therefore the farther we look, the faster objects are moving away from us, redshifting the light. Redshift means that light that is emitted as ultraviolet or visible light is shifted more and more to redder wavelengths, into the near- and mid-infrared part of the electromagnetic spectrum for very high redshifts. Therefore, to study the earliest star and galaxy formation in the universe, we have to observe infrared light and use a telescope and instruments optimized for this light.
Star and planet formation in the local universe takes place in the centers of dense, dusty clouds, obscured from our eyes at normal visible wavelengths. Near-infrared light, with its longer wavelength, is less hindered by the small dust particles, allowing near-infrared light to escape from the dust clouds. By observing the emitted near-infrared light we can penetrate the dust and see the processes leading to star and planet formation.
Objects of about Earth's temperature emit most of their radiation at mid-infrared wavelengths. These temperatures are also found in dusty regions forming stars and planets, so with mid-infrared radiation we can see the glow of the star and planet formation taking place. An infrared-optimized telescope allows us to penetrate dust clouds to see the birthplaces of stars and planets.
Will Webb take amazing pictures like Hubble? Can Webb see visible light?
YES! View an extensive gallery on WebbTelescope.org. We are going to be looking at things we've never seen before and looking at things we have seen before in all new ways.
The beauty and quality of an astronomical image depends on two things: the sharpness and the number of pixels in the camera. On both of these counts, Webb is very similar to, and in many ways better than, Hubble. Although Webb images are infrared, they can be translated by computer into a visible picture (just like we have done with Spitzer, which has produced beautiful pictures as well). Additionally Webb can see orange and red visible light. Webb images are different, but just as beautiful as Hubble's. Read More Also listen to this interview with John Mather about "Making Data Beautiful" on the NASA Blueshift podcast.
What will Webb's first targets be?
The first targets for Webb were determined through a process similar to that used for the Hubble Space Telescope and involved NASA, ESA, CSA and scientific community participants.
The targets released for Webb's first images and data in July 2022 were: 1) Webb's first deep field, SMACS 0723; 2) the galaxy cluster called Stephan's Quintet; 3)the Southern Ring (planetary) Nebula; 4) a spectrum of exoplanet WASP-96 b; 5) the "cosmic cliffs" of the Carina Nebula.
The first engineering targets came before the first science target and were used to align the mirror segments and focus the telescope. The engineering targets that were used were a relatively bright, isolated star along with a dense field of hundreds of thousands of stars. Find those engineering targets in our Flickr album.
How does Webb compare with Kepler?
The Kepler mission was designed to answer a simple question. What fraction of stars have terrestrial planets located in or near the habitable zone?
The habitable zone is the region around a star where water can exist on a planet in liquid form. Kepler sought to answer this question by staring at a small region of the sky containing more than 100,000 stars for 3.5 years or more to look for transiting terrestrial planets, and thus determine what fraction of stars have terrestrial planets. In answering this question, Kepler generated a large database of confirmed transiting planets together with some of their basic properties. Once we found these planets, we needed the tools to study their physical properties and the composition of their atmospheres. It is Webb that provides the specialized tools to undertake these studies. Kepler was designed to be a "wide and shallow" survey telescope, while Webb is designed for "narrow and deep" focused studies with near and mid-IR imaging and spectroscopy.
How does Webb compare to the Transiting Exoplanet Survey Satellite (TESS)?
Webb is a very large observatory designed to address a variety of questions across many areas of astrophysics, while TESS concentrates on identifying a large sample of small planets where follow-up observations are feasible with current and planned telescopes. TESS is identifying small planets and measuring their sizes. Through follow-up observations, we can determine the masses of some of these planets. With both mass and size measurements, we can determine the planets' densities and start to understand what they are made of. This work will provide a foundation for future missions in the search for potentially habitable planets.
TESS is expanding on the NASA Kepler mission's census of exoplanets by targeting closer, brighter stars, where follow-up observations are easier to make. The stars TESS studies are on average 30 to 100 times brighter than the stars earlier Kepler surveyed.
How does Webb compare with Herschel?
Webb and Herschel are complementary.
Webb is a 6.5m telescope sensitive from gold-colored visible light to the mid-infrared, at wavelengths ranging from 0.6 micrometers to 28.5 micrometers. Herschel was a 3.5m telescope sensitive in the far-infrared from 55 to 670 micrometers wavelength. By working at longer wavelengths, Herschel saw colder objects, such as the earliest stages of star formation in dark clouds and emission from molecules such as water. Webb can view more energetic phenomena including forming proto-stars and very distant galaxies. Getting data with both telescopes on the same objects can build a more complete picture of the astrophysical processes.
How does Webb compare with Hubble?
Webb is designed to look deeper into space to see the earliest stars and galaxies that formed in the universe and to look deep into nearby dust clouds to study the formation of stars and planets.
In order to do this, Webb has a much larger primary mirror than Hubble (2.5 times larger in diameter, or about 6 times larger in area), giving it more light-gathering power. It also has infrared instruments with longer wavelength coverage and greatly improved sensitivity than Hubble. Finally, Webb is operating much farther from Earth, maintaining its extremely cold operating temperature, stable pointing and higher observing efficiency than the Earth-orbiting Hubble.
What will Webb tell us about exoplanets? Will it take photos of exoplanets?
Webb is able to tell us the composition of the atmospheres of exoplanets. It can observe planetary atmospheres through the transit technique. A transit is when a planet moves across the disc of its parent star. Webb also carries coronographs to enable photography of exoplanets near bright stars (if they are big and bright and far from the star), but they will be only "dots," not grand panoramas. Consider how far away exoplanets are from us, and how small they are by comparison to this distance! We didn’t even know what Pluto really looked like until we were able to send an observatory to fly right near it, and Pluto is in our own solar system!
Will we image objects in our own solar system?
Yes! Webb is able to observe the planets at or beyond the orbit of Mars, satellites, comets, asteroids, and Kuiper belt objects. Many important molecules, ices, and minerals have strong characteristic signatures at the wavelengths Webb can observe. Webb can also monitor the weather of planets and their moons.
Webb has already looked at Mars, Titan, and Neptune.
Because the telescope and instruments have to be kept cold, Webb’s protective sunshield is blocking the inner solar system from view. This means that the Sun, Earth, Moon, Mercury, and Venus, and of course sun-grazing comets and many known near-Earth objects cannot be observed.
How far back will Webb see?
Webb is able to see what the universe looked like around a quarter of a billion years (possibly back to 100 million years) after the Big Bang, when the first stars and galaxies started to form.
When will Webb launch and how long is the mission duration?
Webb launched on December 25, 2021 from French Guiana on a European Space Agency Arianespace Ariane 5 rocket. Webb was designed for a mission of at least five years, with a goal of 10 years. However, after a successful launch and the completion of telescope commissioning, the Webb team determined the observatory should have enough propellant to allow support of science operations in orbit for more than a 20-year science lifetime. Other factors may limit mission lifetime, such as the possibility that Webb's hardware will degrade over time in the harsh environment of space. However, as we've seen with missions such as the Hubble Space Telescope and the Chandra X-ray Observatory, spacecraft often continue operating years beyond their designed mission lifetime.
What happens after launch, how long until there will be data?
In the first hour: Starting at liftoff, the Ariane rocket provided thrust for about 26 minutes. Telemetry from Webb began after payload fairing separation, almost 3 and a half minutes after launch. Webb separated from the Ariane 5 launch vehicle a half hour after launch and the solar array automatically deployed immediately afterward. We commanded the release of several systems that were locked for launch in preparation for deployments.
In the first day: Two hours after launch we deployed the high gain antenna. Twelve hours after launch there was the first trajectory correction maneuver by small rocket engines aboard Webb itself.
In the first week: The second trajectory correction maneuver took place at 2.5 days after launch. We started the sequence of major deployment just after that. The first deployments were the fore and aft sunshield pallets, followed by the release of remaining sub-system launch locks. The next deployment was the telescope in which the telescope and the spacecraft bus moved apart from each other by about 2 meters when the deployable tower assembly extended. The full sunshield deployment with unfolding and tensioning of the membranes was then initiated. At 6 days we deployed the secondary mirror, followed by the side wings of the primary mirror.
In the first month: As the telescope cooled down in the shade of the deployed sunshield, we turned on the warm electronics and initialized the flight software. At the end of the first month, we did the mid-course correction that ensured that Webb would achieve its final orbit around L2. Although the telescope cooled to near its operating temperature, the ISIM was warmed with electric heaters to prevent condensation on the instruments as residual water trapped in the materials making up the observatory escaped to the vacuum of space.
In the second month: At 33 days after launch we turned on and operated the Fine Guidance Sensor, then NIRCam and NIRSpec. The first NIRCam image was of a crowded star field to make sure that light got through the telescope into the instruments. Since the primary mirror segments were not yet aligned, the picture was still out of focus. At 44 days after launch we began the process of adjusting the primary mirror segments, first identifying each mirror segment with its image of a star in the camera. We also focused the secondary mirror.
In the third month: From 60 to 90 days after launch we aligned the primary mirror segments so that they would work together as a single optical surface. We also turned on and operated the MIRI. By the end of the third month we were able to take the first science-quality images. Also by this time, Webb completed its journey to its L2 orbit position.
In the fourth through the sixth month: At about 85 days after launch we completed the optimization of the telescope image in the NIRCam. Over the next month and a half we optimized the image for the other instruments. We tested and calibrated all of the instrument capabilities by observing representative science targets.
After six months: Webb began its science mission and started to conduct routine science operations. The first images and data were revealed on July 11/12, 2022.
Is Webb serviceable?
Webb is operating at the second Sun-Earth Lagrange point (L2), located approximately 1 million miles (1.5 million km) away from the Earth, and is therefore beyond the reach of any manned vehicle currently being planned for the next decade.
Hubble is in low-Earth orbit, located approximately 375 miles (600 km) away from the Earth, and is therefore readily accessible for servicing. In the early days of the Webb project, studies were conducted to evaluate the benefits, practicality and cost of servicing Webb either by human space flight, by robotic missions, or by some combination such as retrieval to low-Earth orbit. Those studies concluded that the potential benefits of servicing do not offset the increases in mission complexity, mass and cost that would be required to make Webb serviceable, or to conduct the servicing mission itself. Hubble is an exception and not the rule. No other satellites but Hubble are serviceable currently.
Is there a danger from micrometeorites?
All of Webb's systems are designed to survive micrometeoroid impacts.
We tested beryllium discs for micrometeoroids using test facilities in the US and showed the micrometeoroids have negligible effects on the beryllium. Cryogenic beryllium mirrors have been flown in space exposed to micrometeoroids without problems. The Spitzer Space Telescope, launched in 2003, has a beryllium primary mirror.
What was the impact from the large micrometeoroid strike in May? Webb’s mirrors are engineered to endure micrometeoroid impacts. The rates of micrometeoroids hitting the primary mirror remain consistent with the team’s prelaunch predictions. Of 21 measurable impacts (as of January 2023), all but one are consistent with error budget allocations for micrometeoroid effects over Webb’s expected prime lifetime. In May, Webb experienced a larger-than-expected strike – a higher-energy particle that hit a particularly sensitive part of the mirror and structure. However, after initial analysis, the team determined this was a statistically rare event, and the telescope is still performing at a level that exceeds all mission requirements.
What steps is NASA taking to reduce the risk of micrometeoroid impacts? To ensure all parts of the observatory continue to perform at their best and to minimize future impacts of this magnitude, the team has decided that future observations will be planned to limit the amount of time facing in the direction now known as the ‘micrometeoroid avoidance zone,’ where meteoroid energies are generally high. More information.
Why is the mirror segmented?
Webb needed to have an unfolding mirror because the mirror was so large that it could not otherwise fit in the launch shroud of available rockets.
The mirror has to be large in order to see the faint light from the first star-forming regions and to see very small details at infrared wavelengths. Designing, building and operating a mirror that unfolds was one of the major technological developments of Webb. Unfolding mirrors will be necessary for future missions requiring even larger mirrors, and will find application in other scientific, civil and military space missions.
Why are the mirrors hexagonal?
The hexagonal shape allows a segmented mirror to be constructed without gaps that can be roughly circular in shape and needs only 3 variations in prescription.
The hexagonal shape allows a segmented mirror with "high filling factor and six-fold symmetry".H"igh filling factor means the segments fit together without gaps. If we had circular segments, there would be gaps between them. Symmetry is good because we only need 3 different optical prescriptions for all 18 segments, (6 of each prescription). Finally, we want a roughly circular overall mirror shape because that focuses the light into the most compact region on the detectors. An oval mirror, for example, would give images that are elongated in one direction. A square mirror would send a lot of the light out of the central region.
Why does the sunshield have 5 layers?
Webb has a giant, tennis-court sized sunshield, made of five, very thin layers of an insulating film called Kapton. Why five? One big thick sunshield would conduct the heat from the bottom to the top more than would a shield with five layers separated by vacuum. With five layers to the sunshield, each successive one is cooler than the one below. The heat radiates out from between the layers, and the vacuum between the layers is a very good insulator. From studies done early in the mission development five layers were found to provide sufficient cooling. More layers would provide additional cooling, but would also mean more mass and complexity. We settled on five because it gives us enough cooling with some “margin” or a safety factor, and six or more wouldn’t return any additional benefits.
Webb has a large sunshade to protect the telescope from heating by direct sunlight, allowing it to cool down to a temperature below 50 Kelvin (-223° C or -370° F) by passively radiating its heat into space. (Fun fact: You could nearly boil water on the hot side of the sunshield and it’s cold enough to actually freeze nitrogen on the cold side.)
What kind of telescope is Webb?
Webb is a reflecting telescope that uses three curved mirrors. (It's a three mirror anastigmat). There is a technical description of this kind of telescope on Wikipedia.
Why not assemble it in orbit?
Various scenarios were studied and assembling on-orbit was determined to be unfeasible.
In the very earliest stages of feasibility studies, we examined the possibility of on-orbit assembly for what was then called the next generation space telescope or NGST. At that time, and still today, the International Space Station does not have the capability to assemble precision optical structures. Additionally, the environment around the International Space Station is not suitable for the exposed mirrors that Webb has and would have had the possibility to damage or contaminate the optics. The deployment of Webb happened far above Low Earth Orbit and the debris that resides there. Finally, if the Space Station were used as a stopping point for the observatory we would have needed a second rocket to launch it to its final destination at L2. The observatory would have to be designed with much more mass to withstand this “second launch” leaving less mass for the mirrors and science instruments.
Who is James Webb?
This space-based observatory is named after James E. Webb (1906- 1992), NASA's second administrator. Webb is best known for leading Apollo, a series of lunar exploration programs that landed the first humans on the Moon. However, he also initiated a vigorous space science program that was responsible for more than 75 launches during his tenure, including America's first interplanetary explorers. Read more about James E. Webb.