How Much Energy is Needed to Move a Satellite to Infinity from Earth Orbit?

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SUMMARY

The minimum energy required to move a satellite of mass 7500 kg from a circular orbit at a radius of 7.3 x 106 m to a location far from Earth is calculated using the Energy Principle. The correct formula for the change in kinetic energy (ΔK) is ΔK = GmM(1/ri), where G is the gravitational constant (6.7 x 10-11 N m2/kg2), m is the satellite mass, and M is the Earth's mass (6.0 x 1024 kg). The initial calculation of approximately 4.13 x 1011 J is incorrect due to neglecting the existing kinetic energy; the binding energy must be divided by 2, leading to a final energy requirement of approximately 2.065 x 1011 J.

PREREQUISITES
  • Understanding of gravitational potential energy (U = -GmM/r)
  • Familiarity with kinetic energy calculations (K = (1/2)mv2)
  • Knowledge of the Energy Principle in physics
  • Basic grasp of orbital mechanics and escape velocity concepts
NEXT STEPS
  • Study the concept of gravitational binding energy in orbital mechanics
  • Learn about escape velocity and its derivation from energy principles
  • Explore the implications of kinetic energy in satellite motion
  • Investigate the effects of external forces on satellite trajectories
USEFUL FOR

Physics students, aerospace engineers, and anyone interested in orbital mechanics and energy calculations related to satellite motion.

brometheus
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A satellite of mass 7500 kg orbits the Earth in a circular orbit of radius of 7.3(10^6) m (this is above the Earth's atmosphere). The mass of the Earth is 6.0(10^24) kg.

What is the minimum amount of energy required to move the satellite from this orbit to a location very far away from the Earth?


We are supposed to employ the Energy Principle to solve this problem, so we start with:

K_i + U_i = K_f + U_f

We know that K (at low speeds) = (1/2)*m*(v^2) and U = -GmM/r


Using the Energy Principle, we know that

K_f - K_i = U_i - U_f

ΔK = -ΔU = -GmM[(1/r_f) - (1/r_i)]

Since r_f is very large, ΔK = GmM(1/r_i)

Using accepted and aforementioned values,
ΔK = [6.7(10^-11) * 7500 * 6(10^24)]/[7.3(10^6)]

This got me approximately 4.13(10^11)J, which is apparently incorrect. What am I doing wrong?
 
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brometheus said:
A satellite of mass 7500 kg orbits the Earth in a circular orbit of radius of 7.3(10^6) m (this is above the Earth's atmosphere). The mass of the Earth is 6.0(10^24) kg.

What is the minimum amount of energy required to move the satellite from this orbit to a location very far away from the Earth?We are supposed to employ the Energy Principle to solve this problem, so we start with:

K_i + U_i = K_f + U_f

We know that K (at low speeds) = (1/2)*m*(v^2) and U = -GmM/rUsing the Energy Principle, we know that

K_f - K_i = U_i - U_f

ΔK = -ΔU = -GmM[(1/r_f) - (1/r_i)]

Since r_f is very large, ΔK = GmM(1/r_i)

Using accepted and aforementioned values,
ΔK = [6.7(10^-11) * 7500 * 6(10^24)]/[7.3(10^6)]

This got me approximately 4.13(10^11)J, which is apparently incorrect. What am I doing wrong?
You are forgetting that it already has kinetic energy. If it gained GmM/R in kinetic energy it would have more than enough energy to escape.

In order to escape, it has to have just enough kinetic energy to get to an arbitrarily large distance from the Earth ie. where it has 0 kinetic and 0 potential energy.

So the condition for escape is: KE + U = 0

Can you write the equation for KEr+ Ur (hint: if there are no external forces acting, does KE + U change?)

Welcome to PF by the way!

AM
 
the binding energy of a satellite moving in an orbit is GMm/2r. so i think you ought to divide your answer by 2. [4.13*(10^11)] will be the answer if it is at rest on the Earth's surface.
PS: i am new here. could you please tell me how to start a new thread?
 
Ah, okay, that makes sense now. Thanks for your help, and the warm welcome!

To start a new thread I just went to the specific forum (Introductory Physics in this case) and clicked "New Topic" at the top right. It's in the same location as "New Reply" on this page.
 

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