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Black Holes are regions of spacetime where gravity is so strong that nothing, not even light, can escape from them. They are formed from the remnants of massive stars that have undergone a supernova explosion, causing the core to collapse under its own gravitational pull. As a result, a Black Hole with a singularity at its center forms, where the mass of the original star has been compacted into an infinitely small point. In the context of Stellar Evolution, Black Holes represent the final stage in the life cycle of certain types of stars. After exhausting their nuclear fuel, these stars undergo a catastrophic collapse, leading to the formation of a Black Hole. The study of Black Holes is therefore an essential aspect of understanding the evolution and fate of stars in our universe. Furthermore, Black Holes have significant implications for the field of Astronomy as they serve as unique laboratories for testing the laws of physics under extreme conditions. They also play a crucial role in shaping the large-scale structure of galaxies and clusters of galaxies, making them an essential area of research within the broader context of Exoplanet and Stellar Evolution studies. Overall, Black Holes are fascinating celestial objects that offer valuable insights into the fundamental nature of spacetime, gravity, and the evolution of stars in our universe.