Using RPS to Explore Triton’s Potential for Life

Neptune’s moon, Triton, has unique properties mostly due to its extreme cryovolcanic activity. These spots of cryovolcanic activity create localized warm regions in the otherwise frigid and unforgiving climate of Triton; therefore it may be possible for microorganic life to exist near these warm regions. To find life on Triton, it will be necessary to send a land rover that is capable of extracting and analysing liquid samples on Triton. Traveling ~2.7 billion miles to one of the coldest places in the universe will not be easy, but by using RPS, it is more than possible. The biggest challenges for a mission to Triton are the distance and extremely low temperatures. Thankfully, RPS produces high amounts of energy from the radioactive decay of Plutonium-238; this decay produces massive amounts of heat which is then converted into electrical energy. Plutonium-238’s half life of 87.7 years allows for energy to be produced for extended periods of time, so it has more than enough power for a mission to Triton. The high amounts of heat also prevent parts inside of rockets from freezing; meaning that a rover or rocket powered by RPS could effortlessly withstand the harsh environment. It sounds easy on paper, but in reality this mission would require years of careful planning. A skill I have that would benefit this mission is my dedication to understanding and solving challenges. I’ve always been interested in how the universe works, and as a result I have the drive to work through problems until I can fully grasp them. In a field where everything has to work without fail, my dedication will ensure the mission is a success.