Skip to main content

James Webb image shows the majesty of the most massive known galaxy cluster

A recent image from the James Webb Space Telescope shows the most massive galaxy cluster we know of — one so large that it is nicknamed El Gordo, or the fat one. Thought to have a mass of over 2 quadrillion times the mass of the sun, the cluster is located 7 billion light-years away and hosts hundreds of galaxies that are gravitationally bound together.

The image was taken using Webb’s NIRCam instrument, which was able to capture the most detailed look yet at this enormous cluster and the many galaxies within it.

Webb’s infrared image of the galaxy cluster El Gordo (“the Fat One”) reveals hundreds of galaxies, some never before seen at this level of detail. El Gordo acts as a gravitational lens, distorting and magnifying the light from distant background galaxies. Two of the most prominent features in the image include the Thin One, located just below and left of the image center, and the Fishhook, a red swoosh at upper right. Both are lensed background galaxies.
The James Webb Space Telescope’s infrared image of the galaxy cluster El Gordo (“the Fat One”) reveals hundreds of galaxies, some never before seen at this level of detail. El Gordo acts as a gravitational lens, distorting and magnifying the light from distant background galaxies. Two of the most prominent features in the image include the Thin One, located just below and left of the image center, and the Fishhook, a red swoosh at upper right. Both are lensed background galaxies. Image NASA, ESA, CSA Science Jose M. Diego (IFCA), Brenda Frye (University of Arizona), Patrick Kamieneski (ASU), Tim Carleton (ASU), Rogier Windhorst (ASU) Image Processing Alyssa Pagan (STScI), Jake Summers (ASU), Jordan C. J. D'Silva (UWA), Anton M. Koekemoer (STScI), Aaron Robotham (UWA), Rogier Windhorst (ASU)

As the cluster has so much mass, images of it show a phenomenon called gravitational lensing, in which massive objects in the foreground bend space-time and magnify the light coming from distant background galaxies. That allows researchers to get a few of the extremely distant objects that would otherwise be too far away to see, like a galaxy called the Thin One (near the center of the image to the lower left) and the Fishhook (the red hook shape in the top right).

“Lensing by El Gordo boosts the brightness and magnifies the sizes of distant galaxies. This lensing effect provides a unique window into the distant universe,” explained Brenda Frye of the University of Arizona, a researcher who worked on analyzing these observations, in a statement.

Among the lensed objects in the data is a very young galaxy cluster in the first stages of forming, which is so far away it is seen as it was over 12 billion years ago. “While additional data are required to confirm that there are 17 members of this cluster, we may be witnessing a new galaxy cluster forming right before our eyes, just over a billion years after the big bang,” said Frye.

Researchers recorded this data as part of a project called PEARLS (Prime Extragalactic Areas for Reionization and Lensing Science) which uses Webb observations to look for these lensed objects. “Gravitational lensing was predicted by Albert Einstein more than 100 years ago. In the El Gordo cluster, we see the power of gravitational lensing in action,” said Rogier Windhorst of Arizona State University, principal investigator of the PEARLS program. “The PEARLS images of El Gordo are out-of-this-world beautiful. And, they have shown us how Webb can unlock Einstein’s treasure chest.”

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
James Webb Space Telescope celebrated on new stamps
Two new stamps celebrating the James Webb Space Telescope, issued by the USPS in January 2024.

Two new stamps celebrating the James Webb Space Telescope, issued by the USPS in January 2024. USPS

Beautiful images captured by the James Webb Space Telescope have landed on a new set of stamps issued this week by the U.S. Postal Service (USPS).

Read more
James Webb captures a unique view of Uranus’s ring system
This image of Uranus from NIRCam (Near-Infrared Camera) on NASA’s James Webb Space Telescope shows the planet and its rings in new clarity. The Webb image exquisitely captures Uranus’s seasonal north polar cap, including the bright, white, inner cap and the dark lane in the bottom of the polar cap. Uranus’ dim inner and outer rings are also visible in this image, including the elusive Zeta ring—the extremely faint and diffuse ring closest to the planet.

A festive new image from the James Webb Space Telescope has been released, showing the stunning rings of Uranus. Although these rings are hard to see in the visible light wavelength -- which is why you probably don't think of Uranus as having rings like Saturn -- these rings shine out brightly in the infrared wavelength that Webb's instruments operate in.

The image was taken using Webb's NIRCam instrument and shows the rings in even more detail than a previous Webb image of Uranus, which was released earlier this year.

Read more
James Webb spots tiniest known brown dwarf in stunning star cluster
The central portion of the star cluster IC 348. Astronomers combed the cluster in search of tiny, free-floating brown dwarfs.

A new image from the James Webb Space Telescope shows a stunning view of a star cluster that contains some of the smallest brown dwarfs ever identified. A brown dwarf, also sometimes known as a failed star, is an object halfway between a star and a planet -- too big to be a planet but not large enough to sustain the nuclear fusion that defines a star.

It may sound surprising, but the definition of when something stops being a planet and starts being a star is, in fact, a little unclear. Brown dwarfs differ from planets in that they form like stars do, collapsing due to gravity, but they don't sustain fusion, and their size can be comparable to large planets. Researchers study brown dwarfs to learn about what makes the difference between these two classes of objects.

Read more