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36-Billion-Solar-Mass Black Hole Confirmed in Distant Cosmic Horseshoe Galaxy

Combining gravitational lensing with stellar dynamics delivered a direct mass estimate for the dormant black hole, opening the way to apply the method to ESA’s Euclid survey

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A cluster of galaxies in white/violet and hot gaseous atmosphere in blue

Overview

  • A peer-reviewed August 2025 study in MNRAS reports a 36-billion-solar-mass black hole at the center of LRG 3-757, also known as the Cosmic Horseshoe, about five billion light-years from Earth.
  • The team used strong gravitational lensing combined with stellar kinematics to obtain a direct and robust mass measurement for this dormant, non-accreting system.
  • Researchers assert that this result may be the most confidently confirmed ultramassive black hole to date, offering greater certainty than emission-based estimates for objects like TON 618.
  • The host galaxy’s classification as a fossil group suggests that hierarchical galaxy and black hole mergers drove the ultramassive black hole’s growth.
  • Plans are underway to deploy the combined lensing-plus-kinematics technique on ESA’s Euclid survey and other wide-area datasets to uncover more hidden giants and refine galaxy evolution models.