AP Physics B - Satellite/Orbit problem?

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SUMMARY

The discussion focuses on solving a satellite orbit problem in AP Physics B, involving gravitational forces and energy calculations. Key expressions derived include the gravitational force at point B, total energy at point A, and the velocity at point B. The user yinx provided initial equations, such as the gravitational force Fg = (GmMe)/bRe^2 and the potential energy Ug = (-GMem)/a. The work done in changing the orbit was calculated as W = m[(v^2 - vo^2)/2], indicating a clear understanding of kinetic and potential energy relationships.

PREREQUISITES
  • Understanding of gravitational force equations, specifically Newton's law of universal gravitation.
  • Familiarity with kinetic and potential energy concepts in physics.
  • Knowledge of elliptical and circular orbits in celestial mechanics.
  • Proficiency in algebraic manipulation of equations involving variables such as mass, radius, and gravitational constant G.
NEXT STEPS
  • Study the derivation of gravitational force equations in orbital mechanics.
  • Learn about energy conservation principles in satellite motion.
  • Explore the implications of changing orbits from elliptical to circular in terms of energy and velocity.
  • Investigate the effects of varying mass and radius on gravitational interactions.
USEFUL FOR

Students preparing for AP Physics B, educators teaching orbital mechanics, and anyone interested in understanding satellite dynamics and energy transformations in physics.

ohmygosh123
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A satellite of mass m is in an elliptical orbit around the Earth, which has mass Me and radius Re. The orbit varies from closest approach of a at point A to maximum distance of b from the center of the Earth at point B. At point A, the speed of the satellite is vo.Express your answers in terms of a, b, m, Me, Re, vo, and G.

a. Write the expression for the gravitational force between the satellite and Earth at point b.

b. The potential energy of the satellite when it is a distance r from the center of the Earth is given by:

Ug=(-GMem)/r

Determine the total energy of the satellite when it is at A.


c. Determine the velocity of the satellite as it passes point B in its orbit.


As the satellite passes point A, a rocket engine on the satellite is fired so that its orbit is changed to a circular orbit of radius a about the center of the Earth.

d. determine the speed of the satellite for this circular orbit.


e. calculate the work done in changing the orbit



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I honestly don't know where to start with this problem...any initial help would be very much appreciated :)
 
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Hi ohmygosh123 welcome to PF!

Please show an attempt at the question, like a relevant equations and what you think should be the correct way to solve this problem.

-yinx-
 
Ok this is what i have so far:

A: Fg = (GmM)/r^2 = (GmMe)/bRe^2

B: Total Energy = KE + PE = (-GMem)/a + 1/2mvo^2

C: (-GMem)/a + 1/2mvo^2 = 1/2mv^2 ?

D: change in KE = 1/2mv^2 - 1/2mvo^2 => 2(change in KE) = mv^2 - mvo^2

E: W = Fdcos / W = Change in KE or Change in Energy / W = 1/2mv^2 - 1/2mvo^2

W = m[(v^2-vo^2)/2]



I have no idea where to go from there! Please HELPP!
 
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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