Early universe galaxy cluster defies formation expectations

A young galaxy cluster observed in the early universe is surprisingly hot and abundant in gas, challenging scientists' models of how such structures evolve. Named SPT2349-56, the cluster's intracluster gas reaches temperatures of several tens of millions of degrees, far exceeding predictions. Researchers suggest active galaxies within it may be accelerating the heating process.

Astronomers have uncovered an anomaly in the early universe: the galaxy cluster SPT2349-56, located just 1.4 billion years after the big bang. This structure, observed using the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile, contains intracluster gas that is both more abundant and significantly hotter than expected for such a nascent formation.

Dazhi Zhou at the University of British Columbia in Canada led the team that detected temperatures of at least several tens of millions of degrees toward the cluster's center. "The temperature of the surface of the sun is a few thousand degrees Celsius, so this entire area is hotter than the sun," Zhou explained. Their calculations indicate the gas is 5 to 10 times hotter than simulations predicted, a surprise because such extreme heat was anticipated only billions of years later in cluster development.

"This kind of gas should still be cool and less abundant because these baby clusters are still accumulating and heating their gas," Zhou noted. SPT2349-56 appears unusually mature, potentially due to several active galaxies among its members. These include at least three emitting powerful energy jets, alongside frequent star formation bursts, which could rapidly elevate the gas temperature.

This discovery highlights a previously unseen phase in cluster evolution. "What this really does is open a new window showing a phase of cluster evolution that we have never seen before," Zhou said. The team plans further ALMA observations to search for similar hot, young clusters and assess their rarity. The findings, published in Nature, may reshape understandings of galaxy cluster formation in the universe's infancy.

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Artistic rendering of the James Webb Space Telescope observing the atmosphere-shrouded molten super-Earth TOI-561 b near its host star.
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Webb telescope uncovers atmosphere on molten super-Earth TOI-561 b

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NASA's James Webb Space Telescope has detected signs of a thick atmosphere on the ultra-hot exoplanet TOI-561 b, challenging assumptions about such worlds. This rocky planet, orbiting its star in under 11 hours, shows lower temperatures and density than expected, suggesting a layer of gases above a magma ocean. The findings, published on December 11, highlight how intense radiation might not strip away all atmospheres from small, close-in planets.

New details on the galaxy cluster SPT2349-56, observed just 1.4 billion years after the Big Bang, reveal three supermassive black holes likely responsible for heating its gas to five times hotter than models predict—building on initial ALMA observations reported earlier this week.

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Astronomers have proposed that an unusually large black hole in a galaxy from 13 billion years ago could be a primordial remnant from the universe's dawn. Spotted by the James Webb Space Telescope, the black hole is 50 million times the sun's mass but lacks surrounding stars, challenging traditional formation theories. Detailed simulations indicate it may have originated from density fluctuations after the big bang.

Astronomers have solved the mystery of the strange red dots spotted in images from the James Webb Space Telescope, identifying them as young black holes growing rapidly within dense gas clouds. This discovery, led by researchers from the University of Copenhagen, explains how supermassive black holes could form so early in the universe's history. The findings were published in Nature on January 14.

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Astronomers using NASA's Hubble Space Telescope have identified a faint galaxy called CDG-2, located 300 million light-years away in the Perseus cluster, that consists almost entirely of dark matter. The discovery relied on detecting four globular clusters rather than the galaxy's dim stars. This finding highlights the role of dark matter in low-surface-brightness galaxies.

Astronomers suggest that the Milky Way's core might host a dense clump of fermionic dark matter rather than a supermassive black hole. This structure could explain the rapid orbits of nearby stars and the smoother rotation of distant material. The findings, published in Monthly Notices of the Royal Astronomical Society, challenge long-held views of Sagittarius A*.

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Using the Hubble Space Telescope, astronomers have identified Cloud-9, a gas-rich cloud dominated by dark matter with no stars, marking the first confirmed example of a failed galaxy. This relic from the early universe provides insights into cosmic evolution and dark matter structures. The discovery confirms predictions about starless hydrogen clouds known as RELHICs.

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