Dynamics of Uniform Circular Motion Quesiotn

In summary, the conversation discusses finding the weight of a satellite when it is at rest on the surface of a planet, given its mass, orbital period, and the radius of both the planet and the satellite. The solution involves using equations for centripetal force and gravitational attraction to find the mass of the planet and then calculating the weight on the planet's surface.
  • #1
kraigballa
3
0

Homework Statement



A satellite has a mass of 5700 kg and is in a circular orbit 4.2 multiplied by 10^5 m above the surface of a planet. The period of the orbit is two hours. The radius of the planet is 4.25 multiplied by 10^6 m. What is the true weight of the satellite when it is at rest on the planet's surface?

Homework Equations



G = gravitational constant
Me = Mass of planet
r1 = radius from planet to satellite
r2 = radius of planet
v = velocity of satellite in orbit
Fc = centripetal force
T = Time

Fc = msat*v^2/r


G*msat*Me/r^2 = msat*v^2/r

v = Sq. Root(G*Me/r)

The Attempt at a Solution



r1 = 4.67e^6
r2 = 4.25e^6

T = 7200seconds

so v1 = 2*pie*r1/T = 4075.343803 m/s

so Me = v^2 * r1/G = 1.1628389e^24

not sure how to find mass of satellite on planet from here...
 
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  • #2
The mass of the satellite on the planet is the same as everywhere else, 5700 kg. That's only part of your problem. When you say

G*msat*Me/r^2 = msat*v^2/r

what did you use for r? It'd better be r1+r2, the distance from the center of the planet not the surface.
 
  • #3
Yeah for r1 I did the radius of the planet plus the radius of the satellite.

So it should be 5700 kg up in orbit and still 5700 kg on the planets surface? Edit: I guess the answer is supposed to be in "N"
 
  • #4
kraigballa said:
Yeah for r1 I did the radius of the planet plus the radius of the satellite.

So it should be 5700 kg up in orbit and still 5700 kg on the planets surface? Edit: I guess the answer is supposed to be in "N"

Don't confuse mass with weight. Mass is the same everywhere, but "weight" is the force with which the planet attracts the satellite near its surface. Mass is expressed in kilograms and weight in Newtons. Do you know how to find the weight?
 
  • #5
I am not sure how to find weight...? With the given problem that is
 
  • #6
You can find the mass of the planet when the satellite is in orbit from the given quantities. Then put the satellite at rest on the surface of the planet and find the gravitational attraction at that point. That is the weight.
 

FAQ: Dynamics of Uniform Circular Motion Quesiotn

What is uniform circular motion?

Uniform circular motion is the movement of an object along a circular path at a constant speed. This means that the object is moving at the same speed and in the same direction at all points along the circular path.

What is the difference between uniform circular motion and non-uniform circular motion?

The main difference between uniform circular motion and non-uniform circular motion is that the speed of an object in uniform circular motion remains constant, while in non-uniform circular motion, the speed changes at different points along the circular path. In uniform circular motion, the acceleration is always directed towards the center of the circle, while in non-uniform circular motion, the acceleration can be directed in any direction.

What is centripetal acceleration?

Centripetal acceleration is the acceleration of an object moving in a circular path. It is always directed towards the center of the circle and its magnitude is equal to the square of the object's speed divided by the radius of the circle.

What is centripetal force?

Centripetal force is the force that causes an object to move in a circular path. It is always directed towards the center of the circle and its magnitude is equal to the mass of the object multiplied by the centripetal acceleration.

How is centripetal force related to centripetal acceleration?

Centripetal force and centripetal acceleration are directly proportional to each other. This means that as the centripetal force increases, the centripetal acceleration also increases. This relationship is described by the formula F=ma, where F is the centripetal force, m is the mass of the object, and a is the centripetal acceleration.

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