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Solar neutrinos

Solar neutrinos are tiny, nearly massless particles produced during nuclear fusion in the Sun's core, where hydrogen atoms combine to form helium, releasing energy. These neutrinos travel through space at nearly the speed of light and can pass through matter almost unhindered. Detecting solar neutrinos allows scientists to study the Sun's inner workings and confirm theories about nuclear fusion. Their study has also contributed to our understanding of neutrinos in general, which play a key role in the universe's fundamental processes.

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    Solar neutrinos are tiny, nearly massless particles generated during nuclear fusion in the Sun's core, where hydrogen atoms combine to form helium, releasing energy. These neutrinos travel through space at nearly the speed of light and can pass through matter without interaction, making them difficult to detect. Despite their elusive nature, scientists study solar neutrinos to gain insights into the Sun's internal processes and confirm theories about stellar fusion. Understanding solar neutrinos helps us learn more about how stars work and contributes to our broader knowledge of astrophysics and the universe.