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Black Holes represent the final stage in the life of certain massive stars, where the core collapses under its own gravitational pull to form an infinitely dense and compact object with such strong gravitational forces that nothing, not even light, can escape from it. They are formed when a star with a mass of at least three times that of our sun exhausts its nuclear fuel, leading to a catastrophic collapse. The study of black holes is an exciting and dynamic area of astrophysics, as they challenge our understanding of the laws of physics and offer insights into the fundamental nature of space and time. They are closely related to stellar evolution, providing crucial evidence for the life cycle of stars, as well as the properties of matter and energy under extreme conditions.