Astrophysical jets are highly collimated streams of plasma or gas that are emitted from a rotating astronomical object, such as a star, black hole, or galaxy. These jets can extend over vast distances, sometimes spanning light-years, and can travel at extremely high velocities. Astrophysical jets are often observed in regions of intense activity, such as around black holes or young stars, where strong magnetic fields play a significant role in accelerating and focusing the material that forms the jets. These jets can carry a significant amount of energy and momentum, affecting the surrounding environment and potentially influencing the evolution of their host objects. Researchers study astrophysical jets to better understand the processes that govern their formation and dynamics, as well as their impact on the evolution of galaxies and other astronomical systems. This research can provide insights into the physics of extreme environments in the universe and help shed light on phenomena such as accretion, star formation, and galaxy evolution.