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Black Holes are regions of spacetime exhibiting such strong gravitational forces that nothing, not even light, can escape from them. They are formed by the collapse of massive stars at the end of their life cycle, causing a supernova explosion that leaves behind an incredibly dense and compact object with a mass several times that of the Sun. In the context of the hierarchy "Science/Astronomy/Planetary Science/Galaxy", Black Holes represent an extreme phenomenon within the study of galaxies. They are closely related to the formation and evolution of galaxies, as they play a crucial role in shaping their structure and influencing the distribution of matter within them. The presence of a supermassive black hole at the center of most galaxies, including our own Milky Way, has been established through various observations and measurements. Black Holes serve as a fascinating intersection between different fields of astronomy, particularly when it comes to understanding how these enigmatic objects affect their surroundings. They emit powerful jets of particles and radiation, which can be detected across vast distances in the universe. Furthermore, the study of Black Holes provides valuable insights into the nature of gravity, spacetime, and the fundamental laws governing our universe.