The study of icy moons is of great importance to furthering our understanding of the origins of life in the solar system due to their high liquid water content. While missions like JUICE aim to study these bodies through an observational lens, there has yet to be a mission that probes the subsurface of one of these icy moons. This study details our novel mission plan to explore the Saturnian moon Enceladus. This icy world houses a large subsurface ocean filled with important elements for life, alongside potential catalysts for life to form, such as thermal vents. This mission relies on three main components, an orbiter, a lander, and a drill. We detail the designs for every part of the mission and test a simulated thruster system used for landing as well as the water sampling mechanism of the drill. Our testing of the water sampler highlighted the importance of placing the water sampling mechanism above as few mechanical components as possible to prevent the drill from being unable to resurface, and proved that our sampling design is able to collect water efficiently. Similarly, by using drone propellers to simulate thrust from a descent stage and imitate the lack of an atmosphere, we were able to test the lander concept to gain insight on the thrust required to decelerate the lander and negate horizontal velocity for optimal landing on a surface of unknown material composition. We will analyze the water found in the subsurface region of the planet to gauge the habitability of Enceladus and the potential for finding prebiotic lifeforms on the natural satellite. Our mission aims to further study Enceladus and understand more about icy moons through analysis of surface particles and subsurface ocean water. Our mission will help provide key insights into remote sensing, orbiting, landing, and drilling technologies that will be pivotal to exploring other distant icy moons such as Europa or Titan.