Centripetal acceleration of a satellite orbiting Earth

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SUMMARY

The centripetal acceleration of a satellite orbiting Earth at a radius twice that of the Earth's radius is exactly 1/4 of the gravitational acceleration (g) at Earth's surface, which is approximately 9.8 m/s². The calculation utilizes Newton's law of universal gravitation and the formula for centripetal acceleration, leading to the conclusion that the centripetal acceleration can be expressed as a = GM/(2R)² = (1/4)(GM/R²). This simplifies the problem significantly compared to more complex approaches.

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ride4life
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Homework Statement


A satellite is orbiting the Earth in a stable orbit of which the radius is twice that of the Earth. Find the ratio of the satellites cepripetal acceleration to g on the Earth's surface.


Homework Equations


centripetal acceleration = (v^2)/r or (4rpi^2)/T^2


The Attempt at a Solution


Well the only thing i can figure is the rafius of the satellite which is 12.8x10^6
Otherwise I have no idea where to start :(
 
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Hi ride4life! :smile:

(try using the X2 tag just above the Reply box :wink:)

As usual, it's good ol' Newtons' second law that's needed, this time together with another of Newton's laws! :-p

What does that give you? :smile:
 


Ummm...
Fc=Fg
mac=Fg
mac=mg
ac=g
?
 
Last edited:
ride4life said:
F=mg
g=GM/r2

ok … now combine that with your original g = v2/r :smile:
 


v2=GM/r
v2=(6.67x10-11x6x1024)/6.4x106
v=7907.67m/s
 


ahhh...

ac=GM/r2
ac=(6.67x10-11x6x1024)/(2x6.4x106)2
ac=2.44
 


Remember to always include the units or else the answer makes no physical sense.
 
Sorry, not following this …

you're making it very complicated :redface:

The question only asks for the centripetal acceleration (as a multiple of g on the Earths' surface) …

you have centripetal acceleration = GM/r2, so … ? :smile:
 


centripetal acceleration = 2.44
ratio compared to Earth's g which is 9.8 is 2.44/9.8 which is about 1:4
 
  • #10


It is only "about" 1:4 because of the over-complicated way you did that. That was tiny-tim's point. It isn't necessary to find the actual accelerations.

a= \frac{GM}{r^2}
If r= 2R (R is the radius of the earth) then
a= \frac{GM}{(2R)^2}= \frac{GM}{4r^2}= \frac{1}{4}\frac{GM}{r^2}= \frac{1}{4}g.

The centripetal acceleration of a satellite at radius twice the radius of the Earth is exactly 1/4 g.
 
  • #11


ahhh...
i see what you mean, way less complicated than my way :biggrin:
 

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