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Spectroscopy of galaxies within the first half-billion years now reports gas metallicities around a tenth of the solar value — far from pristine, at an epoch when enrichment had little time to work. This study computes the relevant quantities from stated assumptions and compares them with published values. The headline results are: galaxy redshift = 10.6; universe age Myr = 430; observed Z Zsun approx = 0.10; generations at growth 6 = 6.4; mean generation time available Myr = 67; enrichment rate Zsun per 100Myr = 0.023. About six to seven generations at the adopted growth factor reach a tenth-solar metallicity, with roughly sixty million years available per generation — comfortably more than massive-star lifetimes plus plausible recollapse times. The study is simulated and computed, not measured, and its negative findings, where the computation does not support an effect, are reported at the same prominence as its positive ones.
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William Alexander Aldred (2026) studied this question.
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