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

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To calculate the additional energy needed for a satellite to escape Earth's orbit, one must consider both gravitational potential energy (Eg) and kinetic energy (Ek). The total energy required to place a 2.0x10^3-kg satellite into a circular orbit at 500 km altitude is approximately 6.7x10^10 J, though some calculations yield slightly different results. The work done against gravity is defined as the negative change in potential energy, and most energy input goes into kinetic energy rather than simply lifting the satellite. The equations used include Etotal = -(GMm)/r and Ek = -Eg, where G is the gravitational constant, m is the satellite's mass, and r is the distance from the Earth's center. Understanding these principles is crucial for accurate energy calculations in orbital mechanics.
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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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