Centripetal Acceleration of Satellite

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SUMMARY

The discussion focuses on calculating the centripetal acceleration of a satellite with a mass of 1200 kg orbiting the Earth at a distance of 22,000 km from the Earth's center. The user initially miscalculated the centripetal acceleration by solving for tangential velocity instead, resulting in a value of 4.266 x 10^-3 m/s rather than the correct centripetal acceleration of 0.83 m/s². The confusion arose from the distinction between centripetal velocity and centripetal acceleration, emphasizing the importance of understanding the correct formulas and their applications in orbital mechanics.

PREREQUISITES
  • Understanding of Newton's law of universal gravitation (GM/r²)
  • Familiarity with centripetal acceleration formula (a = v²/r)
  • Basic knowledge of orbital mechanics
  • Ability to perform calculations involving square roots and scientific notation
NEXT STEPS
  • Study the relationship between centripetal acceleration and gravitational force
  • Learn how to derive orbital velocity from gravitational parameters
  • Explore the concept of tangential velocity in circular motion
  • Investigate the effects of varying orbital distances on centripetal acceleration
USEFUL FOR

Students in physics, particularly those studying orbital mechanics, as well as educators and anyone interested in understanding the principles of centripetal acceleration and gravitational forces in satellite motion.

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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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Carefully reread the question and make sure you're answering it.
 
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
 
What's it asking you to find? What did you actually calculate?
 
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?
 
Essentially. You solved for what's sometimes called the tangential velocity, not centripetal velocity.
 
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.
 

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