Deriving an expression for the radius of a satellite's orbit around Earth(?)

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SUMMARY

The discussion focuses on deriving the expression for the radius of a satellite's orbit around Earth, specifically the formula r = √[3]{(T²Gmₑ)/(4π²)}. Participants emphasized the importance of equating gravitational force and centrifugal force to solve for the radius. Key concepts include the gravitational attraction formula, the centrifugal force formula, and the centripetal force relationship with the period of revolution. The explanation clarified the derivation process, making it accessible for those struggling with the concept.

PREREQUISITES
  • Understanding of gravitational force and its dependence on mass and distance
  • Familiarity with centrifugal force and its relation to circular motion
  • Knowledge of centripetal force and its connection to orbital mechanics
  • Basic algebra skills for rearranging equations
NEXT STEPS
  • Study the derivation of Kepler's laws of planetary motion
  • Learn about the universal law of gravitation and its applications
  • Explore the concept of centripetal acceleration in circular motion
  • Investigate the relationship between orbital period and radius in satellite motion
USEFUL FOR

Students in physics, aerospace engineers, and anyone interested in understanding satellite dynamics and orbital mechanics.

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Homework Statement


Derive an expression for the radius of a satellite's orbit around Earth in terms of the period of revolution, the universal gravitation constant, and Earth's mass.


Homework Equations


The final equation should be: r = \sqrt[3]{\frac{T^{2}Gm_{E}}{4\prod^{2}}}


The Attempt at a Solution


I have no idea how to do this. To be honest, I'm not even really sure what it means to derive an equation. Someone please help me with this?
 
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A satelite (or anything else) in orbit has a gravitational force inward toward Earth balanced by a centrifugal force outward.
You need the formulae for gravitational attraction (depends on the radius, mass of Earth and satellite) and the centrifugal force (depends on radius and mass of satellite)
Set the two equations equal to each other and rearrange them to get radius
 
Last edited:
All circular satellite calculations begin with "centripetal force = force of gravity".
Fill in the formulas for the two forces and solve for the quantity you want.
Be sure to use the centripetal force formula with period in it since that is specified in the question.
 
Delphi51 said:
All circular satellite calculations begin with "centripetal force = force of gravity".
Fill in the formulas for the two forces and solve for the quantity you want.
Be sure to use the centripetal force formula with period in it since that is specified in the question.

Once it was explained like this, it was dead easy!

Thanks a bunch =).
 

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