Calculating Work for Satellite Orbits Around Earth

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SUMMARY

The discussion focuses on calculating the work done to place satellites into specific orbits around Earth, utilizing gravitational potential energy and kinetic energy equations. The first problem involves a satellite of mass 481 kg in a circular orbit at 9.29x10^6 m, where the work done is calculated using the formula W = ΔU + ΔKE. The second problem examines a satellite of mass 730 kg transitioning from an orbit at 3.12x10^6 m to a new orbit at 6.05x10^6 m, resulting in a total work of approximately 3.6123E9 Joules. Key equations used include U = -GMm/r and fg = GMem/r^2.

PREREQUISITES
  • Understanding of gravitational potential energy (U = -GMm/r)
  • Knowledge of kinetic energy (KE = 1/2 mv^2)
  • Familiarity with gravitational force equations (fg = GMem/r^2)
  • Basic principles of circular motion and orbital mechanics
NEXT STEPS
  • Study the derivation and application of the gravitational potential energy formula in orbital mechanics.
  • Learn how to calculate orbital velocity using v = √(GM/r).
  • Explore the concept of energy conservation in satellite motion.
  • Investigate the effects of altitude on gravitational force and potential energy.
USEFUL FOR

Students in physics or engineering, aerospace engineers, and anyone involved in satellite design or orbital mechanics will benefit from this discussion.

cobrasny
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Homework Statement


A satellite mass 481 is in circular orbit of 9.29x10^6 m above the surface of the Earth
the weight of a 65.1 kg astronaut inside the satellite
What work was done (ignoring friction) to put the satellite into this orbit. Assume it started at rest on the surface of the Earth


Also, A satellite of mass 730 kg is in circular orbit around the Earth, 3.12x10^6 m above the surface of the Earth. Find the minimum work needed to move the satellite outward and put it in circular orbit at a new height of 6.05x10^6 m above the surface of the Earth

Homework Equations


U = -GMm/r
fg = GMem/r^2


The Attempt at a Solution


For the first problem, I tried fg = GMem/r^2, (6.67x10^-11) x (5.97x10^24) x 65.1 / (9.29 x 10^6 + 6.371 x 10^6)^2 and got 105.69 N

For the second, U = -GMm/r; W = Ui-Uf
- (6.67x10^-11) x (5.97x10^24) x 481 / (6.371 x 10^6) - (- (6.67x10^-11) x (5.97x10^24) x 65.1 / (9.29 x 10^6 + 6.371 x 10^6) = -1.78E10 Should the work be negative? Is that the work done by gravity, so the work done to move the satellite is the same magnitude, opposite sign?

I tried a similar strategy for the third problem, and it did not work there either.

Hopefully you can help me understand what I am doing wrong. Thanks in advance.
 
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cobrasny said:
A satellite mass 481 is in circular orbit of 9.29x10^6 m above the surface of the Earth
the weight of a 65.1 kg astronaut inside the satellite
What work was done (ignoring friction) to put the satellite into this orbit. Assume it started at rest on the surface of the Earth

U = -GMm/r
fg = GMem/r^2

For the first problem, I tried fg = GMem/r^2, (6.67x10^-11) x (5.97x10^24) x 65.1 / (9.29 x 10^6 + 6.371 x 10^6)^2 and got 105.69 N

Hi cobrasny! :smile:

Hint: for a circular orbit, the work done is the change in U plus the change in KE. :wink:
 
So..
- (6.67x10^-11) x (5.97x10^24) x 481 / (9.29 x 10^6 + 6.371 x 10^6) - (- (6.67x10^-11) x (5.97x10^24) x 481 / (6.371 x 10^6) = 1.78E10
is just the change in potential energy.

The change in kinetic energy, 1/2mv^2;
v^2 = GMe/r
Re = 6.371x10^6
v=2pi r/T
Vsurface = 2pi 6.371x10^6/(24hrx60minx60sec)

1/2m (vf^2-vi^2)...
.5 (481) [((6.67x10^-11) x (5.97x10^24) / (9.29 x 10^6 + 6.371 x 10^6)) - (2pi 6.371x10^6/ (24x3600))^2] = 6.063E9

Do I then add the change in Ek and change in Eu? To get 1.78E10 + 6.063E9 = 2.386E10 Joules of work?
 
All right, that worked for the second problem.

Two to go:
A satellite of mass 730 kg is in circular orbit around the Earth, 3.12x10^6 m above the surface of the Earth. Find the minimum work needed to move the satellite outward and put it in circular orbit at a new height of 6.05x10^6 m above the surface of the Earth

Delta U = - (6.67x10^-11) x (5.97x10^24) x 730 / (6.05 x 10^6 + 6.371 x 10^6) - (- (6.67x10^-11) x (5.97x10^24) x 730 / (3.12 x 10^6 + 6.371 x 10^6) = 7.2247E9

delta k = .5 (730) [((6.67x10^-11) x (5.97x10^24) / (6.05 x 10^6 + 6.371 x 10^6)) - ((6.67x10^-11) x (5.97x10^24) / (3.12 x 10^6 + 6.371 x 10^6))] = -3.6124E9

So work done = 7.2247E9 + -3.6124E9 = 3.6123E9 Joules (if you could check this I would appreciate it)

A satellite mass 481 is in circular orbit of 9.29x10^6 m above the surface of the Earth
the weight of a 65.1 kg astronaut inside the satellite
I tried fg = GMem/r^2, (6.67x10^-11) x (5.97x10^24) x 65.1 / (9.29 x 10^6 + 6.371 x 10^6)^2 and got 105.69 N
I still don't see what I did wrong here.
 

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