Gravitational Potential Energy Problem

AI Thread Summary
The discussion revolves around calculating the change in gravitational potential energy for a satellite propelled to a height of 35,786 km above Earth. The gravitational force equation, F=GMm/r^2, is highlighted, emphasizing that gravitational acceleration (g) is not constant at such heights. The user initially misapplied the potential energy formula, leading to confusion about the correct answer. It was clarified that the integral of the gravitational force must be used due to the varying nature of g with altitude. The gravitational constant (G) is essential for accurate calculations, which the user initially overlooked, causing discrepancies with textbook answers.
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Homework Statement



The magnitude of the attractive force of gravity between two massive bodies is F=GMm/r^2, where G is a constant, M and m are the masses, and r is the distance between the centers of the two bodies. The radius of the Earth is 6.38×10^6 m and its mass is 5.97×10^24 kg. A satellite of mass 1.13e+3 kg is propelled from the surface of the Earth to a height of 35,786 km above the surface of the Earth. What is its change in gravitational potential energy?

Homework Equations



W=deltaPE
PE=mgdeltah

The Attempt at a Solution



I plugged all the numbers into the given equation to get F=1.6268x10^15
I thought this represented mg in PE=mgh, but after multiplying it with h (and changing h to m rather than km), I didn't come up with the correct answer (which should be 5.96x10^10). Can you tell me where I went wrong?
 
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Well g is not constant over such large distances.
Instead you can use

delta(P.E)= - integral(F.dx) where F is the conservative force.(gravity here).
 
the problem is that g in high altitudes is significantly different.
Work is F*h when F is constant. But F varies with height, and in this case the work is the area below F in a graph where F is drawn against h. Formally:
\int_{r1}^{r2} F dr = \int_{r1}^{r2} \frac{G m_{1} m_{2}}{r^{2}} dr
The area under \frac{1}{r^2} from r=1 to r=r1 is 1 - \frac{1}{r1}
From now on you can compute it even if you don't know what an integral is.
 
Okay, so my integral will be GMm x integral 1/rinitial - 1/rfinal

which gives me GMm (1/6.38e6)-(1/4.138e7), so GMm (1.326e-7), but if I times this by the masses I get G(8.945e20)...but I'm stuck, and this doesn't seem anywhere near the correct answer :/ alas
 
Hang on- that IS the correct answer.
 
Unfortunately my book says the right answer is 5.96x10^10.

How would I possibly get rid of the G in the answer I got (G(8.945e20)) if I don't know what it is? Could I set this equal to something appropriate and make it cancel out?
 
BLAST! Textbook semantics have tricked me again! I assumed we weren't supposed to be able to know this since it's not mentioned in the book. However, it is obviously necessary. Thank you!
 
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