SUMMARY
The discussion centers on the behavior of objects in a hypothetical galaxy-sized water planet, specifically addressing whether an object would sink to the center or pass through. It is established that if the mass of the water planet is not sufficient to form a black hole, an object denser than water will sink to the center due to gravitational forces. The conversation also highlights that the apparent gravity at the center would be zero, and the object would oscillate before eventually coming to rest at the center, influenced by the viscosity of the water. Furthermore, calculations indicate that a stable sphere of water must have a radius of approximately 1700 km to prevent phase transition to ice VI at the center.
PREREQUISITES
- Understanding of gravitational forces and buoyancy
- Knowledge of water's phase transitions and critical points
- Familiarity with the properties of compressibility in fluids
- Basic principles of oscillation and energy conservation in physics
NEXT STEPS
- Research the properties of water under extreme pressure and temperature conditions
- Explore the concept of gravitational equilibrium in fluid dynamics
- Study the implications of phase transitions in large bodies of water
- Investigate the effects of viscosity on the motion of objects in fluids
USEFUL FOR
Physicists, astrophysicists, fluid dynamicists, and anyone interested in the theoretical implications of gravity and buoyancy in large-scale water bodies.