SUMMARY
The discussion centers on the underground temperatures of celestial bodies, specifically Venus and Titan. It establishes that the average surface temperature of Venus is 461°C, which extends to 20 feet underground, while Titan's underground temperatures are significantly lower, around -180°C due to its icy composition. The conversation highlights the concept that underground temperatures tend to stabilize and approximate the yearly average temperature above ground, regardless of surface conditions. Additionally, it raises the possibility of liquid water existing underground despite extreme surface temperatures, referencing ongoing NASA explorations on Mars.
PREREQUISITES
- Understanding of geothermal gradients and temperature stabilization
- Knowledge of planetary geology, particularly regarding Titan and Venus
- Familiarity with the concept of clathrates and their implications for temperature
- Basic principles of thermodynamics as they apply to planetary bodies
NEXT STEPS
- Research the geothermal gradient on Venus and its implications for subsurface temperatures
- Explore the geological characteristics of Titan, focusing on its icy composition and potential for liquid water
- Study the role of clathrates in planetary geology and their thermal properties
- Investigate NASA's current missions to Mars and their objectives related to subsurface water
USEFUL FOR
Astronomers, planetary geologists, and researchers interested in extraterrestrial environments and the potential for subsurface water on celestial bodies.