SUMMARY
To determine Pluto's year length using Kepler's third law, one must apply the equation R^3/T^2 = constant, where R is the distance from the Sun. Given that Pluto is 40 times further from the Sun than Earth, the relationship can be established as Tp^2 = Te^2 * (40)^3. By solving this equation, one can find the orbital period of Pluto, confirming that it is significantly longer than Earth's year.
PREREQUISITES
- Understanding of Kepler's laws of planetary motion
- Familiarity with the equation R^3/T^2 = constant
- Basic algebra for solving equations
- Knowledge of the distance of planets from the Sun
NEXT STEPS
- Study the derivation of Kepler's third law in detail
- Learn how to apply R^3/T^2 for other celestial bodies
- Explore the implications of orbital mechanics in astrophysics
- Investigate the historical context and significance of Kepler's laws
USEFUL FOR
Astronomy students, physics enthusiasts, and anyone interested in celestial mechanics and the calculation of planetary orbits.