The first stars may not have been as uniformly massive as we thought
SMRTR summary
Recent studies challenge the belief that early universe stars were exclusively massive. New computer simulations and laboratory experiments suggest primordial gas clouds could have formed lower-mass stars through turbulence and higher-than-expected molecular hydrogen production. These findings indicate early chemistry was more active than previously thought, potentially allowing the oldest observable stars and first planets to form earlier in cosmic history.
SMRTR provides this summary for quick context. The original article belongs to Ars Technica.
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