SUMMARY
The discussion centers on the accuracy of the moon's distance from Earth as measured by laser reflections from mirrors left by Apollo missions, specifically clarifying that Apollo 13 did not leave any mirrors. The average distance between the Earth and the Moon is increasing by nearly two inches per year, a phenomenon consistent with Newtonian gravity. The conversation highlights the application of Newton's gravitational formula, Fg = Gm1m2 / r^2, and the verification of these measurements through laser ranging techniques. Additionally, it emphasizes the relevance of Kepler's third law in calculating the moon's distance.
PREREQUISITES
- Understanding of Newton's law of universal gravitation (Fg = Gm1m2 / r^2)
- Familiarity with Kepler's laws of planetary motion
- Knowledge of laser ranging techniques used in astrophysics
- Basic concepts of General Relativity (GR) and its differences from Newtonian physics
NEXT STEPS
- Research the principles of laser ranging and its applications in measuring astronomical distances
- Study Kepler's third law and its implications for orbital mechanics
- Explore the effects of tidal forces on celestial bodies and their distances
- Investigate the advancements in General Relativity and how they compare to Newtonian predictions
USEFUL FOR
Astronomers, physics students, educators, and anyone interested in the dynamics of celestial mechanics and the historical context of gravitational theories.