SUMMARY
An exoplanet with 0.5 Earth masses, 0.8 Earth radii, and an atmospheric pressure of 0.10 bar can sustain liquid water, potentially in oceanic forms. The saturation pressure at 285 K is approximately 16 mbar, allowing for significant water vapor presence. The escape velocity of roughly 10 km/s suggests a stable atmosphere, capable of retaining water for billions of years. The discussion confirms that an ocean larger than the Indian Ocean is feasible, with atmospheric composition allowing for a substantial water fraction.
PREREQUISITES
- Understanding of exoplanetary science
- Knowledge of atmospheric pressure and composition
- Familiarity with saturation pressure concepts
- Basic principles of planetary geology and climate
NEXT STEPS
- Research the effects of atmospheric pressure on liquid water retention
- Explore the implications of planetary mass and radius on habitability
- Investigate the role of magnetic fields in atmospheric stability
- Study the climatic effects of axial tilt and rotation period on exoplanets
USEFUL FOR
Astronomers, planetary scientists, and researchers interested in exoplanet habitability and atmospheric dynamics.