AI-Generated Summary

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“The sun, a colossal star at the center of our solar system, radiates energy essential for life on Earth. Composed primarily of hydrogen and helium, it powers nuclear fusion, converting hydrogen into helium and releasing immense heat and light. The sun’s structure includes the core, radiative zone, and convective zone, with its outermost layer, the corona, visible during solar eclipses. Solar activity, such as sunspots and solar flares, impacts space weather, affecting satellites and communication systems on Earth. Understanding the sun’s mechanisms is vital for harnessing solar energy, mitigating climate change, and advancing space exploration. Its study remains a cornerstone of astrophysics.”