Giant planets are massive celestial bodies characterized by their large sizes and compositions primarily composed of hydrogen, helium, and sometimes heavier elements condensed into layers of ice or rock. These worlds are generally categorized into gas giants, which exhibit atmospheres dominated by hydrogen and helium, and ice giants, which possess atmospheres and interiors featuring more volatile compounds like water, methane, and ammonia. Their immense gravity dictates the retention of substantial atmospheres and often influences the formation and dynamics of their surrounding moons and rings. These planets are significant contributors to the study of planetary formation models, providing crucial data points regarding the accretion processes and chemical evolution of stellar systems.