Problem about orbital mechanics

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SUMMARY

The discussion centers on solving an orbital mechanics problem involving the relationship between kinetic energy (KE) and gravitational potential energy (ΔUg) for a satellite in orbit. The user attempts to derive the orbital radius (R2) using the equation 3 KE = ΔUg, leading to the conclusion that R2 = (5/2)R. However, the user expresses confusion as this result does not match the provided answer choices. The correct calculation of kinetic energy is highlighted as KE = 3 (1/2)(mv^2), where v^2 is expressed as GMm/r2.

PREREQUISITES
  • Understanding of gravitational potential energy and kinetic energy in orbital mechanics
  • Familiarity with the equations of motion for satellites
  • Knowledge of the gravitational constant (G) and mass (m) in the context of orbital dynamics
  • Ability to manipulate algebraic equations to solve for variables
NEXT STEPS
  • Study the derivation of orbital mechanics equations, focusing on energy conservation principles
  • Learn about the implications of the gravitational constant (G) in satellite motion
  • Explore the concept of escape velocity and its relation to orbital radius
  • Investigate the differences between circular and elliptical orbits
USEFUL FOR

Students studying physics, particularly those focusing on mechanics and orbital dynamics, as well as educators seeking to clarify concepts related to satellite motion and energy calculations.

Andres Padilla
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Homework Statement
A satellite is in circular orbit around Earth. The orbit is such that the change in gravitational potential energy of the satellite-Earth system in going from the satellite’s location on the surface of Earth to its orbit height is equal to three times the satellite’s kinetic energy while in this orbit. How high above the surface of Earth (radius = R) is the satellite? :

A) 1⁄2R
B) 2⁄3R
C) R
D) 3⁄2R
E) 2R
Relevant Equations
I think:
Ug= -GMm/r
Ke= 1/2 mv^2

V^2=(GM/r)

Umechanical= - 1/2 GMm/r
I tried it, but I am not getting no of the given answers

According to the statement, it is saying that

3 KE (in the orbit ) = ΔUg

So, beeing R the radius of the Earth and R2 the radius of the orbit:

3 (1/2)(GMm/r2) = -GMm/r2 - (-GMm/R)

Canceling out the GMm:

(3/2)(1/r2)= (-1/r2) + (1/R)

Solving for R2

(3/2)(1/r2) + (1/r2)=(1/R)
(5/2)(1/r2)=(1/R)
(2/5)(r2)=R
r2= (5/2)R

Hoewever, this would be wrong, this is not a choice. Could someone teach me what I am doing wrong? thank you in advance :) .
 
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How have you calculated the Kinetic Energy of the satellite?
 
Hello, with KE=3 (1/2)(mv^2)
where V^2 is GMm/r2
 
Andres Padilla said:
Hello, with KE=3 (1/2)(mv^2)
where V^2 is GMm/r2

Okay, I think I agree with your answer.
 
Andres Padilla said:
Homework Statement: ... How high above the surface of Earth (radius = R) is the satellite?
 
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So the answer would be
R2-R = (5/3)R- 1 R=(3/2) R
 
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