Orbital Period of satellite in terms of v and r

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Homework Help Overview

The problem involves determining the orbital period T of a satellite in a circular orbit around the Earth, given its orbital speed v and radius r. The original poster attempts to derive the expression for T using the relationship between speed, distance, and time, while also considering centripetal acceleration.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the relationship between the distance traveled in one revolution and the orbital speed, with some suggesting that the centripetal acceleration equation may not be necessary. Questions arise regarding the validity of including acceleration in the derivation.

Discussion Status

Some participants provide guidance on simplifying the approach by directly relating distance and speed to find the period T. There is an acknowledgment that the original poster may have overcomplicated their reasoning, but no explicit consensus is reached regarding the final expression for T.

Contextual Notes

The original poster notes that this is a sample test question that will not be graded, indicating a focus on understanding rather than formal assessment.

Cloud 9
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Homework Statement


"A satellite orbits the Earth in a circular orbit of radius r. If the orbital speed of the satellite is v, what is the orbital period T of the satellite in terms of v and r? You must explain how you derive the expression for the period."

Homework Equations


Speed = distance/time
a = v2/r

The Attempt at a Solution


Distance for 1 revolution of a circle is equal to the circumference. So distance = 2(pi)r
Time to travel 1 revolution = period T

So velocity = speed = 2(pi)r/T

a = v2/r

a = 2(pi)r/T * 1/T

a = 2(pi)r / T2

At this point I would solve for T, but I am not sure if this is valid, what I'm doing? I don't think we are supposed to have an acceleration in there, so I was wondering if there is another equation I could use that relates v and r. Btw this is not graded, it's just a sample test (that we're not turning in) to help us for the real test (on Tuesday). Thanks for any assistance.
 
Last edited:
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I don't think you even need to bother with the centripetal acceleration equation.

If we have an orbital radius of r, this gives an orbital path distance of 2∏r

T = d / v ---> T = (2∏r) / v
 
If you know the distance per revolution, and you know the velocity, surely you can compute the time of one revolution.
 
bossman27 said:
I don't think you even need to bother with the centripetal acceleration equation.

If we have an orbital radius of r, this gives an orbital path distance of 2∏r

T = d / v ---> T = (2∏r) / v

Oh thanks, so I could have stopped there and solved for T. I guess I made it too complicated. So that answers the question right?
 
Cloud 9 said:
Oh thanks, so I could have stopped there and solved for T. I guess I made it too complicated. So that answers the question right?

Yup, in general you want to use the least amount of extra variables/equations possible.
 

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