Gravitation/Average Force Problem

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SUMMARY

The discussion focuses on calculating the speed, period, altitude, and average retarding force of a 220 kg satellite in a circular orbit 640 km above Earth's surface, which loses mechanical energy at a rate of 1.4x10^5 J per revolution. The user has successfully solved parts (a) to (e) and seeks assistance for parts (f) to (h), specifically regarding the average retarding force and the conservation of angular momentum. The user calculates the total work done as -2.1x10^8 J and is exploring the relationship between force, distance, and angle in the context of this problem.

PREREQUISITES
  • Understanding of orbital mechanics and gravitational forces
  • Familiarity with work-energy principles in physics
  • Knowledge of angular momentum conservation laws
  • Basic calculus for advanced problem-solving techniques
NEXT STEPS
  • Calculate the average retarding force using the equation F = W / D
  • Explore the implications of angular momentum conservation for satellite systems
  • Investigate the effects of energy loss on orbital decay over multiple revolutions
  • Review the relationship between radius, speed, and period in circular orbits
USEFUL FOR

Students studying physics, particularly those focused on orbital mechanics, satellite dynamics, and energy conservation principles. This discussion is beneficial for anyone tackling similar homework problems or preparing for exams in these topics.

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Homework Statement


What are (a) the speed and (b) the period of a 220 kg satellite in an approximately circular orbit 640 km above the surface of Earth? Suppose the satellite loses mechanical energy at the average rate of 1.4x10^5 J per orbital revolution. Adopting the reasonable approximation that the satellite's orbit becomes a "circle of slowly diminishing radius," determine the satellite's (c) altitude, (d) speed, and (e) period at the end of its 1500th revolution. (f) What is the magnitude of the average retarding force on the satellite? Is angular momentum around Earth's center conserved for (g) the satellite and (h) the satellite-Earth system?


Homework Equations


w=change in mechanical energy
w=FDcos(x)

The Attempt at a Solution


First and foremost, I've solved parts a-e correctly. I just need to get f-h.
(1500 revs)((-1.4x10^5 J)/rev)=-2.1x10^8 J
W=change in mechanical energy
W=-2.1x10^8 J
W=FDcos(x)
FDcos(x)=-2.1x10^8 J
So F is definitely the unknown I have to solve for, therefore I should be able to get D and x. Do I just assume that x is 0 degrees? And for finding D, do I just choose one of the two radius values and multiply the amount of revs by the circumference?

It seems to me as though the above way of solving is a little questionable. The only alternative would be a calc-based solution, but I am not quite sure how to go about that.
 
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I'm not asking for a solution, but some help as to what equations and steps I should take to solve this problem. Thanks.
 

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