JPL
Careers
Education
Science & Technology
JPL Logo
JPL Logo
Stars and Galaxies
.3 min read

NASA’s Webb Explores Largest Star-Forming Cloud in Milky Way

Jet Propulsion Laboratory https://www.jpl.nasa.gov/ Sept. 24, 2025
Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in  near-infrared light

Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in near-infrared light, captured by Webb’s NIRCam instrument. The darkest areas of the image are not empty space but are areas where stars are still forming inside dense clouds that block their light.

Credit: Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)

Webb’s MIRI, managed by NASA’s Jet Propulsion Laboratory through launch, helped reveal the star-studded Sagittarius B2 molecular cloud in unprecedented detail.

NASA’s James Webb Space Telescope has revealed a colorful array of massive stars and glowing cosmic dust in the Sagittarius B2 molecular cloud, the most massive and active star-forming region in our Milky Way galaxy.

“Webb’s powerful infrared instruments provide detail we’ve never been able to see before, which will help us to understand some of the still-elusive mysteries of massive star formation and why Sagittarius B2 is so much more active than the rest of the galactic center,” said astronomer Adam Ginsburg of the University of Florida, principal investigator of the program.

Sagittarius B2 is located only a few hundred light-years from the supermassive black hole at the heart of the galaxy called Sagittarius A*, a region densely packed with stars, star-forming clouds, and complex magnetic fields. The infrared light that Webb detects is able to pass through some of the area’s thick clouds to reveal young stars and the warm dust surrounding them.

However, one of the most notable aspects of Webb’s images of Sagittarius B2 are the portions that remain dark. These ironically empty-looking areas of space are actually so dense with gas and dust that even Webb cannot see through them. These thick clouds are the raw material of future stars and a cocoon for those still too young to shine.

The high resolution and mid-infrared sensitivity of Webb’s MIRI (Mid-Infrared Instrument) revealed this region in unprecedented detail, including glowing cosmic dust heated by very young massive stars. The reddest area on the right half of MIRI’s image, known as Sagittarius B2 North, is one of the most molecularly rich regions known, but astronomers have never seen it with such clarity. (Note: North is to the right in these Webb images.)

Webb’s MIRI instrument shows the Sagittarius B2 region in mid-infrared light, with warm dust glowing brightly. Only the brightest stars emit strongly enough to appear through the dense clouds as blue pinpoints.

Webb’s MIRI instrument shows the Sagittarius B2 region in mid-infrared light, with warm dust glowing brightly. Only the brightest stars emit strongly enough to appear through the dense clouds as blue pinpoints.

Credit: Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)

The difference longer wavelengths of light make, even within the infrared spectrum, are stark when comparing the images from Webb’s MIRI and NIRCam (Near-Infrared Camera) instruments. Glowing gas and dust appear dramatically in mid-infrared light, while all but the brightest stars disappear from view.

In contrast to MIRI, colorful stars steal the show in Webb’s NIRCam image, punctuated occasionally by bright clouds of gas and dust. Further research into these stars will reveal details of their masses and ages, which will help astronomers better understand the process of star formation in this dense, active galactic center region. Has it been going on for millions of years? Or has some unknown process triggered it only recently?

Astronomers hope Webb will shed light on why star formation in the galactic center is so disproportionately low. Though the region is stocked with plenty of gaseous raw material, on the whole it is not nearly as productive as Sagittarius B2. While Sagittarius B2 has only 10 percent of the galactic center’s gas, it produces 50 percent of its stars.

“Humans have been studying the stars for thousands of years, and there is still a lot to understand,” said Nazar Budaiev, a graduate student at the University of Florida and the co-principal investigator of the study. “For everything new Webb is showing us, there are also new mysteries to explore, and it’s exciting to be a part of that ongoing discovery.”

More about Webb and MIRI

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).

Webb’s MIRI was developed through a 50-50 partnership between NASA and ESA. A division of Caltech in Pasadena, California, JPL led the U.S. contribution to MIRI. JPL also led development of MIRI’s cryocooler, done in collaboration with Northrop Grumman in Redondo Beach, California, and NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

To learn more about Webb, visit:

https://science.nasa.gov/webb

News Media Contact

Laura Betz

Goddard Space Flight Center, Greenbelt, Md.

laura.e.betz@nasa.gov

Leah Ramsey / Christine Pulliam

Space Telescope Science Institute, Baltimore, Md.

lramsey@stsci.edu / cpulliam@stsci.edu

Calla Cofield

Jet Propulsion Laboratory, Pasadena, Calif.

626-808-2469

calla.e.cofield@jpl.nasa.gov

2025-121

Related News

Stars and Galaxies.

‘Interstellar Glaciers’: NASA’s SPHEREx Maps Vast Galactic Ice Regions

Stars and Galaxies.

Archival Data From NASA’s NEOWISE Tracks Star Turning Into Black Hole

Stars and Galaxies.

NASA Reveals New Details About Dark Matter’s Influence on Universe

Stars and Galaxies.

NASA’s SPHEREx Observatory Completes First Cosmic Map Like No Other

Technology.

NASA Completes Nancy Grace Roman Space Telescope Construction

Stars and Galaxies.

NASA Scientist Finds Predicted Companion Star to Betelgeuse

Stars and Galaxies.

How NASA’s SPHEREx Mission Will Share Its All-Sky Map With the World

Stars and Galaxies.

NASA’s SPHEREx Space Telescope Begins Capturing Entire Sky

Stars and Galaxies.

NASA’s Newest Space Telescope Recognized at New York Stock Exchange

Stars and Galaxies.

NASA’s SPHEREx Team To Ring New York Stock Exchange Bell

About JPL
Who We Are
Directors
Careers
Internships
The JPL Story
JPL Achievements
Documentary Series
JPL Annual Report
Executive Council
Missions
Current
Past
Future
All
News
All
Earth
Solar System
Stars and Galaxies
Eyes on the News
Subscribe to JPL News
Galleries
Images
Videos
Audio
Podcasts
Apps
Visions of the Future
Slice of History
Robotics at JPL
Events
Lecture Series
Speakers Bureau
Calendar
Visit
Public Tours
Virtual Tour
Directions and Maps
Topics
JPL Life
Solar System
Mars
Earth
Climate Change
Exoplanets
Stars and Galaxies
Robotics
More
Asteroid Watch
NASA's Eyes Visualizations
Universe - Internal Newsletter
Social Media
Accessibility at NASA
Contact Us
Get the Latest from JPL
Follow Us

JPL is a federally funded research and development center managed for NASA by Caltech.

More from JPL
Careers
Education
Science & Technology
Acquisition
JPL Store
Careers
Education
Science & Technology
Acquisition
JPL Store
Related NASA Sites
Basics of Spaceflight
NASA Kids Science - Earth
Earth / Global Climate Change
Exoplanet Exploration
Mars Exploration
Solar System Exploration
Space Place
NASA's Eyes Visualization Project
Voyager Interstellar Mission
NASA
Caltech
Privacy
Image Policy
FAQ
Feedback
Version: v3.0.29 - 4bc7967
Site Managers:Emilee Richardson, Alicia Cermak
Site Editors:Naomi Hartono, Steve Carney
CL#:21-0018