Regarding Gravitation and Gravitational Fields

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Homework Help Overview

The discussion revolves around a problem involving gravitational fields and satellite motion, specifically focusing on a satellite designed to orbit Earth at a specified altitude where the gravitational field strength is 4.5 N/kg. The problem includes calculating the distance above Earth's surface, the acceleration of the satellite, and the speed required for maintaining the orbit.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • The original poster attempts to use the gravitational equation to find the altitude for the satellite's orbit and raises concerns about the interdependence of calculations for acceleration and speed. Some participants question the derivation of the velocity equation and suggest considering centripetal force in relation to gravitational force.

Discussion Status

Participants are actively engaging with the problem, offering hints and clarifications regarding the concepts of free-fall and centripetal acceleration. There is a recognition of the need to clarify the relationship between different calculations, but no consensus has been reached on the best approach.

Contextual Notes

There is a mention of the gravitational acceleration value of 9.8 m/s², which is noted to apply only near the Earth's surface, indicating potential assumptions about the altitude's effect on gravitational strength.

nblu
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Homework Statement



A satellite is designed to orbit Earth at an altitude above its surface that will place it in a gravitational field with a strength of 4.5N/kg.
a) Calculate the distance above the surface of Earth at which the satellite must orbit.
b) Assuming the orbit is circular, calculate the acceleration of the satellite and its direction.
c) At what speed must the satellite travel in order to maintain this orbit?

Homework Equations


g=(G*Me)/r^2, where Me is Earth's mass

The Attempt at a Solution


For a), I've used the above equation, with given g value(4.5) substituted into the equation, and got 3.0 x 10^3km as my final answer but b) and c) is where I have the problem. In order to calculate the acceleration for b), I believe that I need to calculate the velocity(v=sqrt(G*Me/r)) first then substitute into (a = v^2/r). However, if I end up getting an answer for part b), didn't I just do c) as well? Because for c) I need to calculate the velocity as well.. I'd like to know whether or not I was wrong about this before I get in any further.

Thank you in advance for your comments.
 
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Hint:
orbital motion is "free-fall." What is the acceleration of free fall?
 
The way you calculated b) is not wrong, and it will work. However, how did you arrive at your equation for velocity? To derive it, you would start by equating centripetal force with gravitational force. What is the centripetal acceleration? Can you figure it out without first calculating velocity?
 
acceleration in free-fall is 9.8m/s/s right?
 
Only near the surface of the earth, because the gravitational force is GMm/r2 = mg = 9.8m on the surface.
 
nblu said:
acceleration in free-fall is 9.8m/s/s right?

only where g is 9.8 N/kg
 

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