El Gordo: A Galaxy Cluster That Pushes the Limits | NASA Webb & Chandra
When astronomers discovered the galaxy cluster ACT-CL J0102-4915 in 2012 with NASA's Chandra X-ray Observatory and ground-based optical telescopes, they nicknamed it "El Gordo" (Spanish for the "Fat One") because of its gigantic mass. Scientists estimate that El Gordo contains as much as 3 million billion (3,000,000,000,000,000) times the mass of the Sun. Thanks to its heft, El Gordo acts as a natural lens, distorting the light from more distant objects behind it through a process known as gravitational lensing.
Distance: ~7.3 billion light-years
A new composite image of El Gordo shows the diffuse, superheated gas in the cluster observed in X-rays from Chandra (blue) that have been combined with a new infrared image from NASA's James Webb Space Telescope (red, green, and blue). Webb's image shows galaxies in El Gordo plus background galaxies located further away from Earth. El Gordo is located about 7.3 billion light-years from Earth and the background galaxies are at a range of different distances including several that are 12.3 billion light-years from Earth. The appearance of some of the background galaxies has been distorted into a variety of unusual and highly elongated shapes because of gravitational lensing by the cluster.
The X-ray image of El Gordo reveals a distinct cometary appearance. Along with optical data, astronomers reported in 2012 that this shape implies El Gordo is, in fact, the site of two galaxy clusters that ran into one another at several million miles per hour. The same study also used Chandra and other observatories to show that El Gordo is the most massive, and produces the most X-rays, of any known galaxy cluster at its distance or beyond.
NASA's Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory's Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.
Visual Description:
In this composite image, the bright blue cloud has a cometary appearance, meaning it resembles a comet and its tail, with a bright tip that fades as the cone-shape widens. Here, the bright tip is positioned near our lower left, with the fading conical shape widening toward our upper right. In this image, the color blue represents X-ray light observed by Chandra. The properties of the gas cloud suggests a multi-million mile an hour collision of two galaxy clusters. This collision produces more X-rays than any other galaxy cluster observed at its distance or beyond.
Throughout the gas cloud, and in the background, are thousands of distant galaxies and stars, in whites, golden oranges, and blues. From this distance, some resemble simple specks of light. Others are slightly larger and feature refraction spikes, or upon close inspection, discernible spiraling arms. Many of the distant galaxies behind the cluster appear distorted or elongated. This visual distortion is due to El Gordo's great mass, which bends the light of these galaxies and distorts their appearance.
Image Credit X-ray: NASA/CXC/Rutgers/J. Hughes et al.; Infrared: NASA/ESA/CSA, J.M. Diego (IFCA), B.Frye (Univ. of Arizona), P.Kamieneski, T.Carleton & R.Windhorst (ASU);
Image Processing: X-ray: L. Frattare; J. Major, K.Arcand (SAO). Infrared: A.Pagan (STScI), J.Summers (ASU), J.C.J.D'Silva (UWA), A.M.Koekemoer (STScI), A.Robotham (UWA), R.Windhorst (ASU)
Release Date: Aug. 2, 2023
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