SUMMARY
The gravitational potential at point Z, located 8.10 x 107 m from a planet with a mass of 1.08 x 1023 kg, is calculated using the formula V = - G M / r. The gravitational potential from the planet is determined to be -8.89 x 104 J/kg. Additionally, the gravitational potential from the moon, with a mass of 4.8 x 1022 kg and located 5.4 x 107 m away, is -5.93 x 104 J/kg. The total gravitational potential at point Z is -1.429 x 108 J/kg, confirming the necessity to consider both celestial bodies in the calculation.
PREREQUISITES
- Understanding of gravitational potential and its formula V = - G M / r
- Familiarity with the gravitational constant G = 6.67 x 10-11 N(m/kg)2
- Knowledge of mass units and their conversions (e.g., kg)
- Basic principles of gravitational fields and their superposition
NEXT STEPS
- Research the concept of gravitational potential energy and its applications in astrophysics
- Learn about the superposition principle in gravitational fields
- Explore the effects of multiple celestial bodies on gravitational calculations
- Study the implications of gravitational potential in orbital mechanics
USEFUL FOR
Students studying physics, particularly those focusing on gravitational theory, astrophysics enthusiasts, and educators teaching gravitational concepts in higher education.