Centripetal Acceleration in Satellites Question

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SUMMARY

The centripetal acceleration of a satellite in orbit is provided by the gravitational force acting on it. This force can be expressed using the formula Fgrav = G(MEm)/r2, where G is the gravitational constant, ME is the mass of the Earth, m is the mass of the satellite, and r is the distance from the Earth's center to the satellite. According to Newton's Second Law, this gravitational force equals the mass of the satellite multiplied by its centripetal acceleration, which can be defined as ac = v2/r. This relationship allows for the calculation of the satellite's speed in orbit.

PREREQUISITES
  • Understanding of gravitational force and its formula
  • Familiarity with Newton's Second Law
  • Knowledge of centripetal acceleration and its calculation
  • Basic algebra for solving equations
NEXT STEPS
  • Study the gravitational constant G and its significance in orbital mechanics
  • Learn how to derive the speed of a satellite using the equation G(MEm)/r2 = m(v2/r)
  • Explore the concept of uniform circular motion in the context of satellite orbits
  • Investigate the effects of varying distances (r) on satellite speed and gravitational force
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Students studying physics, particularly those focusing on mechanics and orbital dynamics, as well as educators seeking to clarify concepts related to satellite motion and gravitational forces.

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Homework Statement



What provides the force that causes the centripetal acceleration of a satellite in orbit?


2. The attempt at a solution

I'm really confused about the answer to this question because in class my teacher only taught us how to solve satellite problems if we are given the distance and we have to find speed http://img85.imageshack.us/img85/2097/physicshw7.png .[/URL]
Can someone please help me.. or just explain what i would need to know to get the answer to this problem! thanks sooo much!
 
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The force that provides the centripetal acceleration for a satellite orbiting in uniform circular motion (that is, the satellite has the same speed at every point on its orbit) is the gravitational force:

[tex]F_{grav} = G \frac{M_Em}{r^2}[/tex]

Where G is the gravitational constant (this is easy to find, its probably in the cover of your textbook), ME is the mass of the earth, m is the mass of the satellite, and r is the distance between the center of the Earth and the satellite.

You know by Newton's Second Law that this gravitational force must equal the mass of the satellite times the centripetal acceleration, and the centripetal acceleration in terms of speed is:

[tex]a_c = \frac{v^2}{r}[/tex]

And so we have:

[tex]G \frac{M_Em}{r^2} = m \frac{v^2}{r}[/tex]

And now you can solve for the speed. Does that help?
 
yes! thank you so much :)
 

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