SUMMARY
The discussion centers on determining the necessary depth of a borehole on Mars to achieve specific atmospheric pressures, specifically 0.35 bar and 0.7 bar. Participants conclude that due to Mars' lower gravity (0.37g) and the exponential nature of pressure variation, a borehole would need to be approximately 100 kilometers deep to reach 0.35 bar. The conversation also highlights the complexities of pressure calculations, including temperature gradients and the density of CO2 compared to Earth's atmosphere. Ultimately, the feasibility of such a project is questioned, with suggestions leaning towards surface-based solutions instead of deep boreholes.
PREREQUISITES
- Understanding of atmospheric pressure concepts, particularly in relation to Mars.
- Familiarity with gravitational effects on pressure calculations.
- Knowledge of temperature gradients and their impact on gas density.
- Basic principles of engineering related to underground construction.
NEXT STEPS
- Research the effects of gravitational differences on atmospheric pressure calculations on Mars.
- Explore the implications of temperature gradients on gas density in planetary atmospheres.
- Investigate existing engineering projects related to deep boreholes, such as the TauTona Mine.
- Examine alternative methods for creating breathable atmospheres on Mars, including surface-based compression techniques.
USEFUL FOR
Astronomers, planetary scientists, engineers, and anyone interested in the challenges of Martian colonization and atmospheric manipulation.