Gravitational Energy for Satellite: r1 to r2

AI Thread Summary
The discussion focuses on calculating the energy required for a satellite to move from an orbit at radius r1 to a greater radius r2, using gravitational energy equations. The total energy of a satellite is expressed as E = -GMm/2r. An attempt at the solution shows an incorrect dimensional analysis, leading to an erroneous result. The correct answer, as provided in the textbook, is E = R^2gm/2(1/r1 - 1/r2). Participants emphasize the importance of checking physical dimensions throughout the calculation process.
Karol
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Homework Statement


A satellite orbits at radius r1. What is the energy required to pass it to a greater radius r2. express in terms of m and g

Homework Equations


The total energy of a satellite: ##E=-\frac{GMm}{2r}##

The Attempt at a Solution


$$E=-\frac{GMm}{2r_2}+\frac{GMm}{2r_1}=-\frac{RGMm}{R2r_2}+\frac{RGMm}{R2r_1}=\frac{Rgm}{2}\left( \frac{1}{r_1}-\frac{1}{r_2}\right )$$
The answer in the book:
$$\frac{R^2gm}{2}\left( \frac{1}{r_1}-\frac{1}{r_2} \right)$$
 
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A good first check is to make sure that the physical dimensions are consistent in every step. Your answer has dimensions energy/length and is therefore wrong. I suggest controlling the intermediate steps.
 
I found the mistake, Thanks, it helped
 
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