SUMMARY
A projectile launched vertically from the Moon's surface at an initial speed of 1210 m/s reaches three-fourths of its initial speed at an altitude calculated using the conservation of energy principle. The correct gravitational acceleration on the Moon is approximately 1.63 m/s², not the Earth’s 9.81 m/s². The energy conservation equation used is 1/2 mv_1^2 = 1/2 m (3v_1/4)^2 + mgh, which simplifies to find the altitude. The correct altitude is approximately 33,000 meters, not 196,000 meters as initially calculated by some participants.
PREREQUISITES
- Understanding of conservation of energy principles in physics
- Familiarity with gravitational acceleration values, specifically for the Moon
- Ability to manipulate algebraic equations
- Basic knowledge of projectile motion
NEXT STEPS
- Study the conservation of energy in gravitational fields
- Learn how to calculate gravitational acceleration for different celestial bodies
- Explore the implications of using different gravitational constants in physics problems
- Practice solving projectile motion problems using energy methods
USEFUL FOR
Students studying physics, educators teaching projectile motion and energy conservation, and anyone interested in celestial mechanics and gravitational effects on projectiles.