Gamma Ray Bursts (GRBs) are intense flashes of gamma rays that can last from a few seconds to several minutes, with their short duration often linked to the rapid collapse of massive stars into black holes. The connection between long GRBs and supernovae has been established through several observed events, indicating that these bursts can occur during hypernovae. Various mechanisms are proposed to explain the differences in duration among GRBs, with some lasting only seconds while others persist longer. The discussion includes multiple resources for further exploration of GRBs and their characteristics. Understanding GRBs is crucial for astrophysics, as they provide insights into stellar evolution and cosmic events.