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Supercomputer Simulations Reveal Secrets of the First Stars

  • Writer: Sandeep K S
    Sandeep K S
  • Aug 9, 2025
  • 1 min read

Updated: Nov 6, 2025

Simulation of the universe's primordial gas clouds showing the formation of a Population III star. The color scale represents gas density, highlighting a clump exceeding the Jeans instability threshold, collapsing into a star with a mass of approximately 8.07 solar masses. Image Credit: Chen et al. 2025. ApJL.
Simulation of the universe's primordial gas clouds showing the formation of a Population III star. The color scale represents gas density, highlighting a clump exceeding the Jeans instability threshold, collapsing into a star with a mass of approximately 8.07 solar masses. Image Credit: Chen et al. 2025. ApJL.

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