Finding gravitational acceleration near the surface of a planet with a satellite

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SUMMARY

The discussion focuses on calculating gravitational acceleration near a planet's surface using the law of universal gravitation. The key equations involved are Fg = GMm/R² and mg = Fg, where G is the gravitational constant, M is the mass of the planet, m is the mass of the satellite, R is the radius of the planet, and r is the distance from the planet's center to the satellite. The participant successfully derived the mass of the planet using the formula 4π²r³/T²G and clarified the distinction between using r and R in the equations based on the satellite's altitude.

PREREQUISITES
  • Understanding of Newton's law of universal gravitation
  • Familiarity with circular motion concepts, specifically centripetal force
  • Knowledge of gravitational acceleration formulas
  • Basic algebra for manipulating equations
NEXT STEPS
  • Study the derivation of gravitational acceleration using Fg = GMm/R²
  • Learn about the relationship between satellite altitude and gravitational force
  • Explore the implications of using different radii in gravitational calculations
  • Investigate the effects of varying mass and distance on gravitational acceleration
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Students in physics, particularly those studying gravitational forces, satellite motion, and universal gravitation principles.

katy123
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Homework Statement


find acceleration due to gravity near the surface of a planet with a satellite by finding the mass of the planet and substituting it into the formula for the law of universal gravitation



Homework Equations


fc=mac
fg=GMm/R^2
fg=fc
fg=mg



The Attempt at a Solution


my question is a general one, I have solved for the mass of the planet finding that 4pi^2r^3/t^2G= Mass of planet
Then, you substitute it into Fg=GMm/R^2
set this equal to mg
mg=GMm/R^2

my teacher has done this on two separate occasions once that results in
acceleration due to gravity=4pi^2r/t^2
and another where it is = 4pi^2r^3/(R^2)(T^2)
r= distance from center to center
R=radius of the big planet
how do you know which radius to use in these equations, and why did it cancel out in one and not in the other?
 
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hi katy, try using the X2 and X2 buttons

It looks like in the first equation for the acceleration due to gravity your teacher approximated r ≈ R, which would be the case if you were on the surface of the Earth.

If you want to find the acceleration due to gravity on a satellite that is not near the surface of the earth, then r ≠ R.

r will just be the altitude of the satellite plus the radius of the Earth, which is R.
 

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