SUMMARY
The orbital velocity of the second satellite, positioned at a radius of 8,600,000 meters from the planet, is calculated to be 21,758 meters per second. This conclusion is derived from the relationship between the velocities and radii of two satellites, utilizing the formula v2 = v1 * sqrt(r2/r1). Given that the first satellite has an orbital velocity of 17,000 meters per second and is located at a radius of 5,250,000 meters, the calculations confirm the derived speed for the second satellite.
PREREQUISITES
- Understanding of centripetal force and gravitational force relationships
- Familiarity with the formula Fc = mv²/r
- Knowledge of orbital mechanics and satellite motion
- Ability to manipulate algebraic equations and ratios
NEXT STEPS
- Study the derivation of orbital velocity formulas in satellite dynamics
- Learn about gravitational force and its effect on satellite motion
- Explore the concept of centripetal force in circular motion
- Investigate the differences in orbital speeds for satellites at varying altitudes
USEFUL FOR
Students in physics or engineering, particularly those studying orbital mechanics, satellite technology, or gravitational forces.