SUMMARY
The ingestion time of an Earth-sized planet by a 100-solar mass black hole is influenced by several factors, including the black hole's mass, the angle of approach, and the speed of the object. Tidal forces would likely disintegrate the Earth into an accretion disk before complete ingestion occurs. The friction within this accretion disk would release significant energy, potentially ejecting a portion of Earth's mass into space. Ultimately, the process could take an indefinite amount of time from a relativistic observer's perspective, as the dynamics of the interaction are complex.
PREREQUISITES
- Understanding of black hole physics, specifically 100-solar mass black holes
- Knowledge of accretion disk formation and dynamics
- Familiarity with tidal forces and their effects on celestial bodies
- Basic principles of relativity and reference frames in astrophysics
NEXT STEPS
- Research the dynamics of accretion disks and their energy release mechanisms
- Learn about the formation and characteristics of black holes, particularly mid-sized black holes
- Explore the effects of tidal forces on planetary bodies approaching black holes
- Investigate relativistic effects on time perception near massive objects
USEFUL FOR
Astronomers, astrophysicists, and students interested in black hole dynamics and the fate of celestial bodies in extreme gravitational fields will benefit from this discussion.