SUMMARY
Gravity on Earth decreases with height, but the change is minimal until reaching significant altitudes. At the International Space Station (ISS), gravity is approximately 8.76 m/s² compared to 9.81 m/s² on the surface. The formula for gravity at height h is given by g_h = g_0 (r/(r + h))², where g_0 is the surface gravity (9.81 m/s²) and r is the Earth's radius (6371 km). Additionally, variations in gravity occur due to the Earth's shape, causing individuals at the poles to weigh slightly more than those at the equator.
PREREQUISITES
- Understanding of Newton's law of gravitation
- Familiarity with gravitational acceleration concepts
- Basic knowledge of Earth's geometry and shape
- Awareness of centrifugal effects due to Earth's rotation
NEXT STEPS
- Study the effects of altitude on gravitational force using the formula g_h = g_0 (r/(r + h))²
- Explore the impact of Earth's shape on local gravity variations
- Investigate the relationship between centrifugal force and gravity at different latitudes
- Learn about the gravitational effects experienced by astronauts in low Earth orbit
USEFUL FOR
Physicists, geophysicists, students studying gravitational physics, and anyone interested in understanding the nuances of gravity variations on Earth.