Webb Telescope's stunning first images made possible by UArizona instruments and expertise

a cloud of gas and dust and stars in space

This landscape of what looks like mountains and valleys speckled with glittering stars is actually the edge of a nearby, young, star-forming region called NGC 3324 in the Carina Nebula. Captured in infrared light by NASA's Webb Telescope, this image reveals for the first time previously invisible areas of star birth. Called the Cosmic Cliffs, it is the edge of the giant, gaseous cavity within NGC 3324. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image.


After decades of development, a nail-biting launch and months of space travel and commissioning, NASA has released the first scientific images and spectroscopic data captured by the James Webb Space Telescope. The images hint at the beginning of years of space science, which will in part be made possible by the 21 University of Arizona researchers who have played a role in developing and managing the instruments onboard.

two nebulae with stars in the center

Some stars save the best for last. The dimmer star at the center of this scene has been sending out rings of gas and dust for thousands of years in all directions, and NASA's Webb Telescope has revealed for the first time that this star is cloaked in dust. This planetary nebula, about 2,500 light-years away and cataloged as NGC 3132, is known informally as the Southern Ring Nebula.


The release of Webb's first images and spectra kicks off the beginning of Webb's science operations, in which astronomers around the world will have their chance to observe anything from objects in our solar system to the early universe, using Webb's four instruments. These include the Near Infrared Camera, or NIRCam, which serves as the telescope's short wavelength imager and is led by principal investigator and UArizona Regents Professor of Astronomy Marcia Rieke. George Rieke, Marcia's husband and also a Regents Professor of Astronomy at UArizona's Steward Observatory, serves as science team lead for the Mid-Infrared Instrument, or MIRI, which will observe the universe at longer wavelengths.

NIRCam and MIRI played a role in creating several of the images released. Since these instruments and the others onboard operate to detect different wavelengths of light, the images can be stacked or compared to learn more about the composition or structure of their targets. 

Webb's first observations tell the story of the hidden universe through every phase of cosmic history – from neighboring exoplanets to the most distant observable galaxies in the early universe, and everything in between. 

five swirling galaxies

This enormous mosaic of the visual grouping of five galaxies called Stephan's Quintet is Webb's largest image to date, covering about one-fifth of the moon's diameter. The information from Webb provides new insights into how galactic interactions may have driven galaxy evolution in the early universe. Using both the NIRCam and MIRI instruments, Webb shows never-before-seen details such as sparkling clusters of millions of young stars and star birthing regions. Sweeping tails of gas, dust and stars are being pulled from several of the galaxies as they interact gravitationally. Webb also captures huge shock waves as one of the galaxies, NGC 7318B, smashes through the cluster.


"Today, we present humanity with a groundbreaking new view of the cosmos from the James Webb Space Telescope – a view the world has never seen before," said NASA Administrator Bill Nelson. "These images, including the deepest view of our universe that has ever been taken, show us how Webb will help to uncover the answers to questions we don't even yet know to ask; questions that will help us better understand our universe and humanity's place within it."

The release of the images and spectra reveal the range of capabilities of all four of Webb's state-of-the-art scientific instruments and confirm that future observations will revolutionize our understanding of the cosmos and our own origins.

"Each of Webb's four instruments have capabilities that are aimed at particular science investigations," Marcia Rieke said. "Our NIRCam, for example, was designed to survey large swaths of sky using different filters, while MIRI collects light at longer wavelengths than all other instruments onboard. The Canadian instrument, the Near-Infrared Imager and Slitless Spectrograph, or NIRISS, has special mode for detecting the composition of planets that orbit other stars, and the Near Infrared Spectrograph NIRSpec can take spectra of many objects at once."

The images are all aesthetically appealing, but they also have scientific utility, Marcia Rieke said. These and future images will be mined for answers to particular science questions.

"After years of development and months of commissioning, it's regular operations from here on out," she said.

a cluster of thousands of galaxies of various shapes, sizes and colors

NASA's Webb Telescope has produced the deepest and sharpest infrared image of the distant universe to date. Known as Webb's First Deep Field, this image of galaxy cluster SMACS 0723 shows thousands of galaxies – including the faintest objects ever observed in the infrared. This slice of the vast universe is approximately the size of a grain of sand held at arm's length by someone on the ground.


Marcia Rieke said the questions she's most excited to investigate include how the first galaxies came together to create something like our own Milky Way and if we can find an exoplanet with an Earthlike atmosphere.

George Rieke said some of the objects he's most excited to study with the powerful MIRI instrument are quasars, which are supermassive black holes at the center of galaxies that create bright jets of light as they consume the surrounding gas.

"MIRI and all of Webb's other instruments are ushering humanity into new scientific territory and that's super exciting," he said.

Webb's first observations were selected by a group of representatives from NASA, the European Space Agency, Canadian Space Agency and the Space Telescope Science Institute, who are all partners on the project:

  • Carina Nebula: Looking at this star-forming region and others like it, with Webb, scientists can see newly forming stars and study the gas and dust that made them.
  • Southern Ring planetary nebula: From birth to magnificent death as a planetary nebula, Webb can explore the expelling shells of dust and gas of aging stars that may one day become a new star or planet.
  • Stephan's Quintet galaxies: Stars derive from, and contribute to, gas and dust in mass quantities, swirling around galaxies. Webb can study nearby and dynamic interacting galaxies to see the gas and dust in action. Now, scientists can get a rare look, in unprecedented detail, at how interacting galaxies are triggering star formation in each other and how the gas in these galaxies is being disturbed.
  • SMACS 0723 deep field view: To truly understand our beginnings, we must trace these galaxies back to the beginning. This deep field uses a lensing galaxy cluster to find some of the most distant galaxies ever detected. This image is only scratching the surface of Webb's capabilities in studying deep fields.
  • WASP-96b exoplanet: Studying other planetary systems like this will help astronomers find out how typical, or atypical, our solar system is. Webb has detected water molecules on an exoplanet and will now set out to study hundreds of other systems to understand what other planetary atmospheres are made of.

"I'm very happy for all the young scientists who staked their early careers on Webb working smoothly and poured their hearts into getting every aspect tested and documented, and then turned it over to the astronomical community to let everyone help rewrite all the textbooks with new discoveries," George Rieke said.

a graph where the x axis is wavelength of light and the y axis is the amount of light by the star blocked by the exoplanet atmosphere

NASA's Webb Telescope has captured the distinct signature of water, along with evidence for clouds and haze, in the atmosphere surrounding a hot, puffy gas giant planet orbiting a distant sun-like star. The observation, which reveals the presence of specific gas molecules based on tiny decreases in the brightness of precise colors of light, is the most detailed of its kind to date, demonstrating Webb’s unprecedented ability to analyze atmospheres hundreds of light-years away.


The James Webb Space Telescope launched Dec. 25, 2021, on an Ariane 5 rocket from Europe's Spaceport in French Guiana. After completing the most complex and difficult deployment sequence in space, Webb underwent months of commissioning, in which its mirrors were painstakingly aligned, and its instruments were calibrated to its space environment and prepared for science.

NASA Headquarters oversees the mission for the agency's Science Mission Directorate. NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages Webb for the agency and oversees work on the mission performed by the Space Telescope Science Institute, Northrop Grumman and other mission partners. In addition to Goddard, several NASA centers contributed to the project, including the agency's Johnson Space Center in Houston, Jet Propulsion Laboratory in Southern California, Marshall Space Flight Center in Huntsville, Alabama, Ames Research Center in California's Silicon Valley and others.