Time average of the potential energy of a planet

AI Thread Summary
The discussion focuses on calculating the time average of the potential energy of a planet in an elliptical orbit, proving it to be -k/a, where k is a constant and a is the semimajor axis. The challenge lies in relating the varying radius of the orbit to the average distance, with the average radius being the semimajor axis between aphelion and perihelion. For part (b), the kinetic energy is derived using conservation of energy, resulting in K = k/2a. The virial theorem is referenced to support the calculations. Overall, the thread emphasizes the relationship between potential and kinetic energy in planetary motion.
Dustgil
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Homework Statement


(a) Prove that the time average of the potential energy of a planet in an elliptical orbit about the sun is -k/a.
(b) Calculate the time average of the kinetic energy of the planet.

Homework Equations



F = \frac {-dV} {dr} = - \frac {k} {r}

The Attempt at a Solution


[/B]
So the first part is what's giving me trouble. k obviously doesn't vary, yet r does. So if we find the average radius of orbit we can therefore easily find the potential energy. I know that a is a length of the semimajor axis of the ellipse and that it makes sense that is would be the average radius, as it lies between the aphelion and perihelion. I see that if a is the semimajor axis and Ea is half the length of the distance between the foci then the aphelion is a + Ea and the perihelion is a - Ea, where E is the eccentricity. This is where I get stuck. I'm not sure how to directly relate this to the average distance. Anyone have a hint?

Part b is pretty easy really, since I've already shown the total energy E = -k / 2a. Just use conservation of energy and

<br /> K - \frac {k} {a} = - \frac {k} {2a}

K = \frac {k} {2a}
 
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