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The distribution of elements in the universe is primarily characterized by the abundance of hydrogen and helium, which together account for about 98% of the visible matter. Heavier elements, known as "metals" in astronomical terms, such as carbon, oxygen, and nitrogen, make up a smaller percentage and are primarily produced in stars through nuclear fusion. These elements are distributed unevenly throughout galaxies, with higher concentrations in regions of active star formation. Overall, the distribution reflects the processes of nucleosynthesis in stars and supernovae, shaping the chemical composition of the cosmos.

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2mo ago

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