Centripetal acceleration of a satellite orbiting Earth

AI Thread Summary
The discussion focuses on calculating the centripetal acceleration of a satellite orbiting Earth at a radius twice that of the Earth. Participants clarify that the centripetal acceleration can be derived using the formula ac = GM/r^2, leading to the conclusion that at this radius, the acceleration is 1/4 of Earth's gravitational acceleration (g). The simplified approach emphasizes that it is unnecessary to calculate the actual velocities or forces involved. Ultimately, the centripetal acceleration of the satellite is determined to be 2.44 m/s², which translates to a ratio of about 1:4 compared to g. The conversation highlights the importance of simplifying calculations in physics problems.
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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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