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SPT-CL J2215-3537: Unexpectedly Calm and Remote Galaxy Cluster Discovered
SPT-CL J2215-3537
SPT-CL J2215-3537
SPT-CL J2215-3537
Visual Description:

  • A galaxy cluster with an important characteristic – being “relaxed – has been discovered about 8.4 billion light years from Earth.

  • Relaxed galaxy clusters show no signs of violent collisions with other clusters or groups of galaxies.

  • Astronomers were unsure if relaxed clusters could exist so early in the universe since they are still merging with others to grow.

  • This discovery was made possible by NASA’s Chandra X-ray Observatory along with optical and infrared telescopes.

The discovery of the most distant galaxy cluster with a specific important trait — as described in our press release — is providing insight into how these gigantic structures formed and why the universe looks like it does in the present day.

This composite image shows SPT-CL J2215-3537 (SPT2215 for short) in X-rays from NASA’s Chandra X-ray Observatory (blue) and a combination of ultraviolet, optical, and infrared light from NASA’s Hubble Space Telescope (cyan and orange). Astronomers used Chandra to find this distant and unusually young galaxy cluster, along with NSF/DOE’s South Pole Telescope, the Dark Energy Survey project in Chile and NASA’s Spitzer Observatory. The results have been reported in a series of three papers.

SPT2215 is located about 8.4 billion light-years from Earth. This means it is seen when the universe is only 5.3 billion years old, compared to its current age of 13.8 billion years. While there have been many clusters seen at this large distance, SPT2215 possesses a quality that makes its whereabouts particularly intriguing. SPT is what astronomers refer to as “relaxed,” meaning that it shows no signs of having been disrupted by violent collisions with other clusters of galaxies.

Galaxy clusters — some of the biggest structures in the universe — grow over time by merging with other galaxy clusters or groups, causing disturbances such as asymmetries or sharp features in the cluster’s gas. Given enough time to “relax,” however, the gas can take on a smooth, calm appearance, as seen with SPT2215. Until the identification of SPT2215, astronomers had not found a relaxed galaxy cluster this far away. In fact, scientists were not sure they would find a galaxy cluster that was relaxed at this epoch of the universe, because they are usually still undergoing the turmoil of mergers with other clusters or groups of galaxies as they increase in size.

Another interesting aspect of SPT2215 is the evidence for large amounts of star formation happening in its center. SPT2215 has a very large galaxy in its middle, which in turn has a supermassive black hole at its core. The prodigious amount of star formation shows scientists that much of the hot has cooled to the point where new stars can form, without outbursts driven by the black hole providing a heating source that prevents most of this cooling. This addresses an ongoing question of how much black holes stymie or support the birth of stars in their environments.

The central galaxy in SPT2215 is also quite isolated, with no other galaxies within about 600,000 light-years that are anywhere near as bright or extended. This implies that the cluster has not experienced a merger with another cluster in about the last billion years, giving another piece of evidence that SPT2215 is relaxed.

The three papers on SPT2215, in reverse order of publication, were a recent paper led by Michael Calzadilla and his colleagues published in the April 20, 2023 issue of The Astrophysical Journal; a paper led by Adam Mantz published in the February 2022 issue of Monthly Notices of the Royal Astronomical Society (a preprint is available online) and a paper led by Lindsay Bleem et al. published in the March 2020 issue of The Astrophysical Journal Supplement Series.

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:

This release features a composite image of a distant galaxy cluster known as SPT2215. In the main image, the galaxy cluster resembles a blue cloud with a hazy golden light at its core. The cluster is set against the blackness of space, which is dotted with white, orange and blue specks of light. A combination of X-ray, ultraviolet, optical, and infrared light, was used to create the image.

The blue cloud represents X-ray gas observed by Chandra. The cloud is soft, and uniform in texture. Over time, galaxy clusters often merge or collide. These collisions cause disturbances and sharp features in a cluster’s gas. When a cluster takes on a smooth, calm appearance, as found here in SPT2215, it indicates that no such collisions have occurred for a very long time. Astronomers call these galaxy clusters “relaxed”.

The hazy golden light at the heart of the cloud represents a massive central galaxy with a large amount of star formation. This central galaxy is quite isolated within the blue gas cloud. There are relatively few nearby specks of light near the central galaxy, and none are as bright or as large. No other large galaxies have been found within 600,000 light-years of the central galaxy. This implies that SPT2215 has not experienced a galaxy merger in the last billion years.

The universe is about 13.8 billion years old. SPT2215 is located about 8.4 billion light-years from Earth. This means that we are observing the galaxy cluster when the universe was only 5.3 billion years old. This is the first time scientists have discovered a “relaxed” galaxy cluster so far away, when the universe was relatively young and undergoing great turmoil.


Fast Facts for (SPT-CL J2215-3537):
Credit  X-ray: NASA/CXC/MIT/M. Calzadilla; UV/Optical/Near-IR/IR: NASA/STScI/HST; Image processing: N. Wolk
Release Date  July 20, 2023
Scale  Image is about 25 arcsec (680,000 light-years) across.
Category  Groups & Clusters of Galaxies, Quasars & Active Galaxies
Coordinates (J2000)  RA 22h 15m 04.1s | Dec -35° 37´ 13.4"
Constellation  Piscis Austrinus
Observation Dates  August 20, 2021
Observation Time  20 hours 4 minutes
Obs. ID  22653, 24614, 24615
Instrument  ACIS
References Calzadilla, M., et al, 2023, ApJ, 947, 44 DOI 10.3847/1538-4357/acc6c2
Color Code  X-ray: blue; UV/Optical/Near-IR: cyan; IR: orange
Distance Estimate  About 8.4 billion light-years (z = 1.16)
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