SUMMARY
The attractive force between the Sun and Venus is calculated using Newton's law of universal gravitation, represented by the formula F = G(m1*m2)/d². With the mass of the Sun at 1.98 x 1030 kg, the mass of Venus at 4.83 x 1024 kg, and the distance between their centers at 1.08 x 1011 m, the correct force is determined to be approximately 57 x 1021 N after correcting the distance squared calculation. The discussion highlights the importance of maintaining precision in calculations and the inclusion of units for clarity.
PREREQUISITES
- Understanding of Newton's law of universal gravitation
- Familiarity with scientific notation and unit conversions
- Basic algebra skills for manipulating equations
- Knowledge of significant figures and rounding rules in calculations
NEXT STEPS
- Review the principles of Newton's law of universal gravitation
- Learn about unit consistency and dimensional analysis in physics
- Study the significance of significant figures in scientific calculations
- Explore common mistakes in physics problem-solving and how to avoid them
USEFUL FOR
Students studying introductory physics, educators teaching gravitational concepts, and anyone interested in celestial mechanics and force calculations.