Gravitational Energy for Satellite: r1 to r2

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SUMMARY

The discussion focuses on calculating the energy required for a satellite to transition from an orbit at radius r1 to a greater radius r2. The total energy of a satellite is expressed as E = -GMm/(2r). The correct energy difference is derived as E = (R^2gm/2)(1/r1 - 1/r2). A critical aspect highlighted is the importance of maintaining consistent physical dimensions throughout the calculation process to ensure accuracy.

PREREQUISITES
  • Understanding of gravitational potential energy
  • Familiarity with orbital mechanics
  • Knowledge of the gravitational constant (G) and mass (m)
  • Basic algebra for manipulating equations
NEXT STEPS
  • Study gravitational potential energy calculations in orbital mechanics
  • Learn about the implications of changing orbital radii on satellite energy
  • Explore the concept of energy conservation in gravitational fields
  • Review dimensional analysis techniques in physics
USEFUL FOR

Students studying physics, particularly those focusing on orbital mechanics and gravitational energy calculations, as well as educators looking for examples of energy transitions in satellite orbits.

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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