Change in mechanical energy (gravitation)

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SUMMARY

The discussion focuses on calculating the work required to place a 1000kg satellite into orbit, emphasizing the relationship between gravitational potential energy and mechanical energy. The total mechanical energy is defined using the equation E = -GMm/2r, where M is the Earth's mass and r is the distance from the Earth's center. The work-energy theorem is applied, demonstrating that the work needed to achieve orbit is the difference between the total mechanical energy in orbit and when the satellite is grounded. The discussion clarifies that this work can be attributed to external forces, such as propulsion or other means.

PREREQUISITES
  • Understanding of gravitational potential energy, specifically the equation (-GMm/r)
  • Familiarity with the work-energy theorem and its application
  • Basic knowledge of kinetic energy and its relationship to mechanical energy
  • Concept of total mechanical energy in gravitational systems
NEXT STEPS
  • Study the derivation of the mechanical energy equation E = -GMm/2r
  • Explore the work-energy theorem in detail, focusing on gravitational systems
  • Learn about orbital mechanics, including velocity and period calculations for satellites
  • Investigate the role of external forces in satellite propulsion and energy transfer
USEFUL FOR

Students studying physics, aerospace engineers, and anyone interested in understanding the principles of gravitational energy and satellite mechanics.

vinicius0197
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I got a little bit confused while studying gravitational potential energy, particularly the expression for long distances: (-GMm/r). An exercise asks me for the velocity, period and radial acceleration for a 1000kg satellite that I wish to put into orbit. That's okay. But after that, I'm questioned for the amount of work needed to put this satellite into orbit. The book says that the necessary work is given by the difference between the total mechanical energy when the satellite is in orbit and the total mechanical energy when the satellite is grounded. The book uses the equation: (E=-GMm/2r) for mechanical energy - where M is the mass of the Earth and r is the distance between the satellite and the center of the Earth.
That confuses me. I know that, by the work-energy theorem that work equals the change in kinetic energy, and I know that the change in gravitational potential energy equals minus Work (delta U = -W). But calculating work by change in mechanical energy is new for me. Where does it come from?
 
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Try using the work energy theorem here.
 
vinicius0197 said:
I got a little bit confused while studying gravitational potential energy, particularly the expression for long distances: (-GMm/r). An exercise asks me for the velocity, period and radial acceleration for a 1000kg satellite that I wish to put into orbit. That's okay. But after that, I'm questioned for the amount of work needed to put this satellite into orbit. The book says that the necessary work is given by the difference between the total mechanical energy when the satellite is in orbit and the total mechanical energy when the satellite is grounded. The book uses the equation: (E=-GMm/2r) for mechanical energy - where M is the mass of the Earth and r is the distance between the satellite and the center of the Earth.
That confuses me. I know that, by the work-energy theorem that work equals the change in kinetic energy, and I know that the change in gravitational potential energy equals minus Work (delta U = -W). But calculating work by change in mechanical energy is new for me. Where does it come from?
The total mechanical energy in the initial position (grounded):
E1 = K1 + U1 ; K is kinetic energy and U is gravitational potential energy. Since it is grounded, K1 = 0
While it is in orbit, the total mechanical energy is:
E2 = K2 + U2
The difference in energy has to come from somewhere. That is external work. It could be because of the exhaust gases, or Superman throws the satellite into orbit, or whatever. So
E2 - E1 = W (1)
The same thing can be done starting from the work - kinetic energy theorem:
ΔK = K2 - K1 = Work done by gravity + Work by other forces (gases, Superman, whatever) (2)
Work done by gravity = - ΔU = - (U2 - U1) (3)
substitute (3) into (2) and rearrange the terms to get (1)
 
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