This collection of 19 face-on spiral galaxies from the James Webb Space Telescope in near- and mid-infrared light is at once overwhelming and awe-inspiring. “Webb’s new images are extraordinary,” said Janice Lee, a project scientist for strategic initiatives at the Space Telescope Science Institute in Baltimore, Maryland. “They’re mind-blowing even for researchers who have studied these same galaxies for decades. Bubbles and filaments are resolved down to the smallest scales ever observed, and tell a story about the star formation cycle.” Credit: NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), PHANGS Team, Elizabeth Wheatley (STScI)
A new treasure trove of Webb images has arrived! Near- and mid-infrared images show off every facet of these face-on spiral galaxies.
Humanity has spent centuries mapping Earth’s features – and we frequently repeat the process by using more advanced instruments. When we combine the data, we get a more complete understanding of our planet.
Now, look outward into space. Astronomers have observed nearby, face-on spiral galaxies for decades. Both space- and ground-based telescopes have contributed to a cache of data in wavelengths from radio to ultraviolet light. Astronomers have long planned to use NASA’s James Webb Space Telescope to obtain the highest resolution near- and mid-infrared images ever taken of these galaxies, and today they are publicly available.
Everyone can explore Webb’s newest set of exquisite images, which show stars, gas, and dust on small scales beyond our own galaxy. Teams of researchers are studying these images to uncover the origins of these intricate structures. The research community’s collective analysis will ultimately inform theorists’ simulations, and advance our understanding of star formation and the evolution of spiral galaxies.
James Webb Space Telescope’s observation of Face-on spiral galaxy, NGC 628. Credit: NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), PHANGS Team
Webb Space Telescope Depicts Staggering Structure in 19 Nearby Spiral Galaxies
It’s oh-so-easy to be absolutely mesmerized by these spiral galaxies. Follow their clearly defined arms, which are brimming with stars, to their centers, where there may be old star clusters and – sometimes – active supermassive black holes. Only NASA’s James Webb Space Telescope can deliver highly detailed scenes of nearby galaxies in a combination of near- and mid-infrared light – and a set of these images was publicly released today.
These Webb images are part of a large, long-standing project, the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) program, which is supported by more than 150 astronomers worldwide. Before Webb took these images, PHANGS was already brimming with data from NASA’s Hubble Space Telescope, the Very Large Telescope’s Multi-Unit Spectroscopic Explorer, and the Atacama Large Millimeter/submillimeter Array, including observations in ultraviolet, visible, and radio light. Webb’s near- and mid-infrared contributions have provided several new puzzle pieces.
“Webb’s new images are extraordinary,” said Janice Lee, a project scientist for strategic initiatives at the Space Telescope Science Institute in Baltimore. “They’re mind-blowing even for researchers who have studied these same galaxies for decades. Bubbles and filaments are resolved down to the smallest scales ever observed, and tell a story about the star formation cycle.”
Excitement rapidly spread throughout the team as the Webb images flooded in. “I feel like our team lives in a constant state of being overwhelmed – in a positive way – by the amount of detail in these images,” added Thomas Williams, a postdoctoral researcher at the University of Oxford in the United Kingdom.
Follow the Spiral Arms
Webb’s NIRCam (Near-Infrared Camera) captured millions of stars in these images, which sparkle in blue tones. Some stars are spread throughout the spiral arms, but others are clumped tightly together in star clusters.
The telescope’s MIRI (Mid-Infrared Instrument) data highlights glowing dust, showing us where it exists around and between stars. It also spotlights stars that haven’t yet fully formed – they are still encased in the gas and dust that feed their growth, like bright red seeds at the tips of dusty peaks. “These are where we can find the newest, most massive stars in the galaxies,” said Erik Rosolowsky, a professor of physics at the University of Alberta in Edmonton, Canada.
Something else that amazed astronomers? Webb’s images show large, spherical shells in the gas and dust. “These holes may have been created by one or more stars that exploded, carving out giant holes in the interstellar material,” explained Adam Leroy, a professor of astronomy at the Ohio State University in Columbus.
Now, trace the spiral arms to find extended regions of gas that appear red and orange. “These structures tend to follow the same pattern in certain parts of the galaxies,” Rosolowsky added. “We think of these like waves, and their spacing tells us a lot about how a galaxy distributes its gas and dust.” Study of these structures will provide key insights about how galaxies build, maintain, and shut off star formation.
Dive Into the Interior
Evidence shows that galaxies grow from inside out – star formation begins at galaxies’ cores and spreads along their arms, spiraling away from the center. The farther a star is from the galaxy’s core, the more likely it is to be younger. In contrast, the areas near the cores that look lit by a blue spotlight are populations of older stars.
What about galaxy cores that are awash in pink-and-red diffraction spikes? “That’s a clear sign that there may be an active supermassive black hole,” said Eva Schinnerer, a staff scientist at the Max Planck Institute for Astronomy in Heidelberg, Germany. “Or, the star clusters toward the center are so bright that they have saturated that area of the image.”
Research Galore
There are many avenues of research that scientists can begin to pursue with the combined PHANGS data, but the unprecedented number of stars Webb resolved are a great place to begin. “Stars can live for billions or trillions of years,” Leroy said. “By precisely cataloging all types of stars, we can build a more reliable, holistic view of their life cycles.”
In addition to immediately releasing these images, the PHANGS team has also released the largest catalog to date of roughly 100,000 star clusters. “The amount of analysis that can be done with these images is vastly larger than anything our team could possibly handle,” Rosolowsky emphasized. “We’re excited to support the community so all researchers can contribute.”
Don’t miss the images below: Webb’s images are split with those of the same galaxies taken by NASA’s Hubble Space Telescope.
Webb’s view of Spiral Galaxy IC 5332
Hubble’s view of Spiral Galaxy IC 5332
Webb’s view of Galaxy NGC 628
Hubble’s view of Spiral Galaxy NGC 628
Webb’s view of Spiral Galaxy NGC 1087
Hubble’s view of Spiral Galaxy NGC 1087
Webb’s view of Spiral Galaxy NGC 1300
Hubble’s view of Spiral Galaxy NGC 1300
Webb’s view of Spiral Galaxy NGC 1365
Hubble’s view of Spiral Galaxy NGC 1365
Webb’s view of Spiral Galaxy NGC 1385
Hubble’s view of Spiral Galaxy NGC 1385
Webb’s view of Spiral Galaxy NGC 1433
Hubble’s view of Spiral Galaxy NGC 1433
Webb’s view of Spiral Galaxy NGC 1512
Hubble’s view of Spiral Galaxy NGC 1512
Webb’s view of Spiral Galaxy NGC 1566
Hubble’s view of Spiral Galaxy NGC 1566
Webb’s view of Spiral Galaxy NGC 1672
Hubble’s view of Spiral Galaxy NGC 1672
Webb’s view of Spiral Galaxy NGC 2835
Hubble’s view of Spiral Galaxy NGC 2835
Webb’s view of Spiral Galaxy NGC 3351
Hubble’s view of Spiral Galaxy NGC 3351
Webb’s view of Spiral Galaxy NGC 3627
Hubble’s view of Spiral Galaxy NGC 3627
Webb’s view of Spiral Galaxy NGC 4254
Hubble’s view of Spiral Galaxy NGC 4254
Webb’s view of Spiral Galaxy NGC 4303
Hubble’s view of Spiral Galaxy NGC 4303
Webb’s view of Spiral Galaxy NGC 4321
Hubble’s view of Spiral Galaxy NGC 4321
Webb’s view of Spiral Galaxy NGC 4535
Hubble’s view of Spiral Galaxy NGC 4535
Webb’s view of Spiral Galaxy NGC 5068
Hubble’s view of Spiral Galaxy NGC 5068
Webb’s view of Spiral Galaxy NGC 7496
Hubble’s view of Spiral Galaxy NGC 7496
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 the Canadian Space Agency.
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