How do I calculate the additional energy needed to escape Earth's orbit?

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SUMMARY

The discussion focuses on calculating the energy required to place a 2,000 kg satellite into a circular orbit at an altitude of 500 km and the additional energy needed to escape Earth's orbit. The total energy required for orbit is approximately 6.7 x 1010 J, while the additional energy for escape is 5.8 x 1010 J. Key equations discussed include gravitational potential energy (Eg = mgh) and total energy calculations using Etotal = -(GMm)/r and Etotal = -0.5(GMm)/r. The importance of kinetic energy in the overall energy budget for orbital insertion is emphasized.

PREREQUISITES
  • Understanding of gravitational potential energy (Eg = mgh)
  • Familiarity with the gravitational constant (G)
  • Basic knowledge of kinetic energy (Ek = -Eg)
  • Ability to perform energy calculations involving mass and distance
NEXT STEPS
  • Study the principles of orbital mechanics and energy calculations in astrophysics
  • Learn about the gravitational constant (G) and its applications in satellite dynamics
  • Explore the integration of gravitational force to derive potential energy
  • Investigate the differences between kinetic and potential energy in orbital contexts
USEFUL FOR

Students in physics, aerospace engineers, and anyone interested in satellite dynamics and energy calculations for orbital mechanics.

decamij
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1. How can i prove that Eg = mgh

2. What is the total energy needed to place a 2.0x10^3-kg satellite into circular Earth orbit at an altitude of 5.0x10^2 km?

For number 2, the answer is apparently 6.7x10^10J. However, shouldn't Total Energy = 1/2 (Eg)? If that is the case, the answer would be 5.8x10^10J.

(P.S. in the question after this, i must calculate the additional energy required to allow the object to escape Earth's orbit, and the answer is 5.8x10^10J).
 
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1. Remember that the work done by a conservative force such as gravity is defined as the negative of the change in the potential energy. You can easily prove it from the definition of work as force X distance, in the simplest scenario in which you consider a constant gravitational force applied to an object that happens to be moving vertically upward in a straight line.
 
For the energy to put the satellite in orbit, how are calculating it? I get 9.36 X 10^9 J. (I might have made a mistake...) Also, what is "Eg"? I'm not familiar with that term.
 
Don't forget that most of the energy required to put a satellite into orbit goes into kinetic energy! Merely lifting it 500 km won't get you very far.
 
1. Eg is gravitational potential energy

2. I learned the following equations:


Etotal = -(GMm)/r
 
1. Eg is gravitational potential energy

2. I learned the following equations:


Etotal = -0.5(GMm)/r
Ek = -Eg


Ek is kinetic energy, G is the grav. constant, m is the mass of the satellite, is the mass of the Earth and r is the distance of the satellite from the centre of the Earth.
 
OK, I got 6.77 X 10^10 J by adding the KE ((G*m1*m2)/(2*d)) to the PE. I got the PE (9.36 X 10^9 J) by integrating the force of gravity (G*m1*m2/d^2) with respect to the distance from the Earth's surface to the height of the orbit.
 

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