SUMMARY
A ball thrown upward follows the curvature of spacetime, returning to the ground due to gravitational effects. The discussion posits that if a sufficiently large mass were placed directly overhead, it could theoretically alter the curvature of spacetime, allowing the ball to ascend again before hitting the ground. However, in a realistic scenario where Earth is the only significant mass, the ball's trajectory will always lead it back to the center of the Earth. The principles of classical Newtonian gravity adequately describe this phenomenon without requiring general relativity.
PREREQUISITES
- Understanding of spacetime curvature
- Familiarity with Newtonian gravity
- Basic knowledge of general relativity concepts
- Ability to visualize trajectories in a gravitational field
NEXT STEPS
- Research the effects of mass on spacetime curvature in general relativity
- Explore Newtonian gravity and its implications for projectile motion
- Study gravitational fields and their influence on object trajectories
- Examine practical applications of spacetime curvature in astrophysics
USEFUL FOR
Physics students, educators, and anyone interested in gravitational theory and the behavior of objects in a gravitational field.