Find Pluto's year length using Kepler's third law.

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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.

D.J Falcon
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Homework Statement



Pluto is 40 times further from the Sun than we are. How long is a year on Pluto? (Use Kepler's third law.)


Homework Equations



4∏^2/Gm=T^2/r^3


The Attempt at a Solution



Te^2(Earth period)=x*r^3

Tp^2(Pluto period)=x*(40r)^3


I don't know what to do exactly from here. I'm not even entirely sure that I'm going about this the right way.

Any help would be appreciated.
 
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Hint: For every planet [which goes around the sun] in our solar system R^3/T^2=constant.
Why?
 
estro said:
Hint: For every planet [which goes around the sun] in our solar system R^3/T^2=constant.
Why?

I've already made x a constant (T^2/r^3), in the attempt at a solution. I just don't realize what to do from there.
 
I don't know what you mean by:
D.J Falcon said:
I've already made x a constant (T^2/r^3), in the attempt at a solution.
...

First of all you need to understand why for every planet which goes around the same star R^3/T^2 is constant.
Then don't forget what you already know about the difference in R between Earth and Pluto.

I'm already gave you the answer, actually...
 

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