Gravitational Energy for Satellite: r1 to r2

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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
 
The book claims the answer is that all the magnitudes are the same because "the gravitational force on the penguin is the same". I'm having trouble understanding this. I thought the buoyant force was equal to the weight of the fluid displaced. Weight depends on mass which depends on density. Therefore, due to the differing densities the buoyant force will be different in each case? Is this incorrect?

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