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Sunyaev–Zeldovich detection of hot intracluster gas at redshift 4.3

The gas in galaxy cluster SPT2349-56 is at least five times hotter than models predict due to energy from multiple supermassive black holes, challenging formation theories.

  • On January 5, astronomers reported in Nature that ALMA detected extremely hot intracluster gas in the young galaxy cluster SPT2349-56, observed about 1.4 billion years after the Big Bang.
  • Standard cluster-formation theories assume gravity heats intracluster gas slowly, but models indicate gravity alone cannot produce the observed extreme temperatures in SPT2349-56.
  • Sunyaev–Zeldovich analysis found a clear, powerful signal with ALMA probing CMB distortion, showing thermal electrons exceed 10 million Kelvin and gas is at least five times hotter than predicted.
  • Researchers warn the finding indicates theoretical understanding of cluster evolution is incomplete, and the research team led by Dazhi Zhou plans follow-up observations to hunt for more hot, young clusters and investigate the cluster ecosystem.
  • Scientists suspect powerful jets from at least three supermassive black holes inject energy into the cluster, which contains more than 30 active galaxies forming stars over 5,000 times faster and spans about 500,000 light‑years, seen roughly 12 billion years ago.
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Nature broke the news in United Kingdom on Monday, January 5, 2026.
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