https://webbtelescope.org/contents/news-releases/2025/news-2025-128
https://iopscience.iop.org/article/10.3847/2041-8213/add2f0
ASA Webb 'Pierces' Bullet Cluster, Refines Its Mass
June 30, 2025 10:00AM
Summary
Webb shows fainter and more distant galaxies, along with light from stars that trace dark matter in these galaxy clusters, helping researchers carefully map everything in the scene.
It’s rare for galaxy clusters to collide and merge at high speeds. An iconic example is the Bullet Cluster, the aftermath of two vast galaxy clusters that collided.
To be able to “replay” what happened, and in which order, researchers need to first fully define all the contents in this scene.
Full Article
NASA’s James Webb Space Telescope has provided some of the best information to date: Highly precise, extremely detailed near-infrared images of a significant portion of the Bullet Cluster.
Its new observations allowed researchers to fine tune their maps of its mass, including an invisible substance known as dark matter that does not emit, reflect, or absorb light.
NASA’s James Webb Space Telescope recently zeroed in on the Bullet Cluster — delivering highly detailed images that show a greater abundance of extremely faint and distant galaxies than ever before.
Using Webb’s crisp near-infrared observations of this region, researchers have more completely mapped the colliding galaxy clusters’ contents.
“With Webb’s observations, we carefully measured the mass of the Bullet Cluster with the largest lensing dataset to date, from the galaxy clusters’ cores all the way out to their outskirts,” said Sangjun Cha, the lead author of the paper published in The Astrophysical Journal Letters and a PhD student at Yonsei University in Seoul, South Korea.
(Previous studies of the Bullet Cluster with other telescopes relied on significantly less lensing data, which netted out with less precise estimates of the system’s mass.)
“Webb’s images dramatically improve what we can measure in this scene — including pinpointing the position of invisible particles known as dark matter,” said Kyle Finner, a co-author and an assistant scientist at IPAC at Caltech in Pasadena, California.
Mapping the Dark Matter
All galaxies are made up of stars, gas, dust, and dark matter, which are bound together by gravity. The Bullet Cluster is made up of two very massive collections of galaxies, known as galaxy clusters, that are themselves bound by gravity.
These galaxy clusters act as gravitational lenses, magnifying the light of background galaxies. “Gravitational lensing allows us to infer the distribution of dark matter,” said James Jee, a co-author, professor at Yonsei University, and research associate at UC Davis in California.
To visualize gravitational lensing and dark matter, think of a pond filled with clear water and pebbles. “You cannot see the water unless there is wind, which causes ripples,” Jee explained.
“Those ripples distort the shapes of the pebbles below, causing the water to act like a lens.” The same thing happens in space, but the water is dark matter and the pebbles are background galaxies.
In all, the team measured thousands of galaxies in Webb’s images to accurately “weigh” both the visible and invisible mass in these galaxy clusters.
They also carefully mapped and measured the collective light emitted by stars that are no longer bound to individual galaxies — known as intracluster stars.
The revised map of the Bullet Cluster is shown in a new image: Layered on top of an image from Webb’s NIRCam (Near-Infrared Camera) is data from NASA’s Chandra X-ray Observatory that shows hot gas in pink, including the bullet shape at right.
Refined measurements of the dark matter, calculated by the team using Webb’s observations, are represented in blue. (See the defined galaxy clusters within the dashed circles.)
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