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Chemical Evolution Of Galaxies

Chemical Evolution Of Galaxies

The chemical evolution of galaxies describes the continuous process by which the elemental composition of galaxies changes over cosmic time. This transformation is primarily driven by successive generations of stars, which synthesize heavier elements through nuclear fusion and subsequently return these enriched materials to the interstellar medium via stellar winds and supernova explosions. Studying this evolution provides crucial insights into the formation history, star formation rates, and overall lifecycle of matter within galaxies, helping us piece together the cosmic story of our universe.