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Hubble Data Questions Supernova Winds' Role in Cosmic Reionization

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Hubble Data Questions Supernova Winds' Role in Cosmic Reionization

Here is what the page “Hubble Data Questions Supernova Winds' Role in Cosmic Reionization” contains. New observations from the Hubble Space Telescope are prompting astronomers to rethink how the universe became transparent to light. An international team, including researchers from the University of Michigan, analyzed ultraviolet spectra of distant galaxies and found that winds driven by supernovae may not have been powerful enough to punch through the dense gas that shrouded early galaxies. This challenges a widely held theory about the epoch of reionization, when radiation from the first stars and galaxies cleared the fog of neutral hydrogen that filled the cosmos.

The findings suggest that other mechanisms—perhaps radiation pressure from massive stars or contributions from faint galaxies—played a larger role than previously thought. By pinpointing what actually ended the cosmic dark ages, scientists can better understand how galaxies evolved and how the universe became the structured place we see today. The full version stays on the original page, which this listing opens directly.

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