Centripetal Acceleration of Satellite

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Homework Statement


Hi, I am stuck on this question:
A satellite of mass 1200 kg is in orbit around the Earth at a distance of 22000 km from the centre of the Earth.
Calculate the magnitude of the centripetal acceleration of the satellite at this distance.

The Attempt at a Solution


I did:
mv^2/r= GMm/r^2
so v= square root of GM/r
v= square root of 6.67 x10^-11 x 6.0 x 10^24/ 22000 x 10^3
this gave me=
4.266x 10^-3 m/s but the answer at the back is 0.83 m/s^2, can someone please explain to where i went wrong.

Thanks[/B]
 
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vela said:
Carefully reread the question and make sure you're answering it.
Hi, I've reread it many time, but i still feel confused
 
vela said:
What's it asking you to find? What did you actually calculate?
Oh I see what you mean, are you implying that I solved centripetal velocity instead of centripetal acceleration?
 
vela said:
Essentially. You solved for what's sometimes called the tangential velocity, not centripetal velocity.
So does this mean I consider gravity of Earth as my centripetal velocity and therefore:
g= GM/r^2, but i still have a query, if you could kindly clear this up for me, why can't we use the centripetal formula in this question.
 
The work you did was correct, but you didn't actually solve for the quantity you were asked for. (The fact that the units were different is a big clue.)

I was just pointing out the phrase "centripetal velocity" doesn't really make sense. The velocity you found is tangent to the satellite's path; it doesn't point inward. The acceleration, however, does, so that's why it's referred to as centripetal acceleration.