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Black Holes, within the context of Stellar Evolution, represent the final stage in the life cycle of certain massive stars. After exhausting their nuclear fuel and undergoing a supernova explosion, the remaining core may collapse under its own gravity, creating a black hole if it is sufficiently massive. This process involves the conversion of mass into intense gravitational energy, warping spacetime and giving rise to unique astrophysical phenomena, such as accretion disks and relativistic jets. As a focal point in Astrophysics and Astronomy, black holes contribute significantly to our understanding of Stellar Evolution and the fundamental forces of the universe.