SUMMARY
The discussion centers on the feasibility of exploring Europa, one of Jupiter's moons, under its ice layer, which is estimated to be 10 to 15 miles (15 to 25 kilometers) thick. The surface gravity of Europa is 0.134g, and a vessel could potentially dive to depths of 2,160 meters, significantly deeper than the operational limits of a Los Angeles class submarine, which is around 290 meters. The conversation highlights the challenges of penetrating the ice, including the need for advanced thermal breaking techniques and the potential use of a small fission reactor for thermal power output to maintain operational temperatures.
PREREQUISITES
- Understanding of hydrostatic pressure and its formula as a function of depth.
- Knowledge of the structural capabilities of submarines, particularly the Los Angeles class.
- Familiarity with thermal conductivity of ice at low temperatures.
- Basic principles of fission reactors and their thermal output capabilities.
NEXT STEPS
- Research the hydrostatic pressure calculations for depths on Europa.
- Explore the design and capabilities of manned and unmanned submersibles.
- Investigate thermal breaking techniques for ice penetration in extreme conditions.
- Study the thermal properties of ice at temperatures below -100 Celsius.
USEFUL FOR
Aerospace engineers, oceanographers, and researchers interested in extraterrestrial exploration and the engineering challenges of submersible design for extreme environments.