Gravitational Potential Energy Problem

In summary, the conversation discusses the calculation of change in gravitational potential energy for a satellite launched from the surface of Earth to a height of 35,786 km above. The formula for calculating gravitational force is mentioned, as well as the use of integrals to solve for the change in potential energy. The gravitational constant, G, is also introduced as a necessary factor in the equation.
  • #1
sheepcountme
80
1

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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  • #2
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).
 
  • #3
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:
[tex]\int_{r1}^{r2} F dr = \int_{r1}^{r2} \frac{G m_{1} m_{2}}{r^{2}} dr[/tex]
The area under [tex]\frac{1}{r^2}[/tex] from r=1 to r=r1 is [tex] 1 - \frac{1}{r1}[/tex]
From now on you can compute it even if you don't know what an integral is.
 
  • #4
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
 
  • #5
Hang on- that IS the correct answer.
 
  • #6
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?
 
  • #8
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!
 

FAQ: Gravitational Potential Energy Problem

What is gravitational potential energy?

Gravitational potential energy is the energy that an object possesses due to its position in a gravitational field. It is the potential for an object to do work by falling or moving towards a lower position in the gravitational field.

How is gravitational potential energy calculated?

The gravitational potential energy of an object can be calculated by multiplying its mass, the acceleration due to gravity, and its height above a reference point. The formula is: GPE = mgh, where m is mass, g is acceleration due to gravity, and h is height.

What factors affect the gravitational potential energy of an object?

The gravitational potential energy of an object is affected by its mass, the strength of the gravitational field, and its distance from the reference point. The greater the mass or height, or the stronger the gravitational field, the greater the potential energy.

How does gravitational potential energy change as an object moves?

As an object moves towards a lower position in a gravitational field, its gravitational potential energy decreases. This is because the object is doing work by moving towards the center of the gravitational field.

What are some real-life examples of gravitational potential energy?

Some examples of gravitational potential energy include a roller coaster at the top of a hill, a book on a shelf, or a skydiver at the edge of a plane. In each of these examples, the object has the potential to do work by falling or moving towards a lower position in the gravitational field.

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