Circular motion and parabolic orbit

In summary, the conversation discusses a point object connected to a fixed point by an inertialess string. The object moves in a vertical plane with an initial speed v0 and reaches a point B where the force acting on it becomes zero. The speed v and initial speed v0 are given by equations mv2/L-mgsin(90+\theta) = 0 and decrease in Kinetic Energy = Gain in Potential Energy, respectively. From point B, the object follows a parabolic orbit until reaching point C. The maximum elevation from point B is given by H = v2sin2(90-\theta)/2g. The remaining questions involve finding the angle \phi and the angle between the object velocity at point C and the horizontal
  • #1
shrrikesh
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Homework Statement



A point object of mass m is connected to an inertialess string of length L, the other end of which is connected to a fixed point O. At time t=0, the object is assumed to move horizontally in a vertical plane from the bottom point A (OA=L). in the clockwise direction with an initial speed v0 as seen in the figure.

http://img208.imageshack.us/img208/5223/figure.jpg

If [tex]\sqrt{2gL}[/tex]<v0<[tex]\sqrt{5gL}[/tex], then at a point B (the angle between OB and the horizontal direction is designated [tex]\theta[/tex]) the magnitude of the force acting on the object from the string becomes zero, where OB=L and the velocity is perpendicular to OB. v being the magnitude of the vector velocity. If 0<[tex]\theta[/tex]<[tex]\pi[/tex]/2.

1) the speed v is given by...?

2) the initial speed is ...?

3) From the point B, for a while, the object takes a parabolic orbit till C where OC=L . The maximum elevation (with respect to location B) is expressed as ...?

4) In the case [tex]\theta[/tex]=[tex]\pi[/tex]/3, the angle [tex]\phi[/tex] measured as in fig. specifying the point C becomes. ...?

5) and finally the angle , the angle between the object velocity at the point C and the horizontal direction is ...?

Homework Equations



for no 1)

mv2/L-mgsin(90+[tex]\theta[/tex]) = 0

for no 2)

decrease in Kinetic Energy = Gain in Potential Energy

for no 3)

H = v2sin2(90-[tex]\theta[/tex])/2g

I am not able to do for no 4 and 5.

The Attempt at a Solution


I've found out the answers for question 1,2 and 3 which are

[tex]\sqrt{gLsin\theta}[/tex], [tex]\sqrt{(2+3sin\theta)gL}[/tex] and v2cos2[tex]\theta[/tex]/2g respectively.

I don't have any ideas to solve the last two ones.
 
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1. What is circular motion and how does it differ from linear motion?

Circular motion is the movement of an object around a fixed point, called the center. It differs from linear motion in that the direction of the object's motion is constantly changing, as it moves in a curved path rather than a straight line.

2. How do you calculate the speed and velocity of an object in circular motion?

The speed of an object in circular motion can be calculated by dividing the circumference of the circle by the time it takes to complete one full revolution. The velocity, on the other hand, is a vector quantity that takes into account both the speed and the direction of the object's motion. It can be calculated by dividing the displacement of the object by the time it takes to complete one full revolution.

3. What is centripetal force and how does it relate to circular motion?

Centripetal force is the force that keeps an object moving in a circular path. It acts towards the center of the circle and is necessary to counteract the object's tendency to move in a straight line. In circular motion, the centripetal force is equal to the mass of the object multiplied by the square of its speed divided by the radius of the circle.

4. What is a parabolic orbit and how does it occur?

A parabolic orbit is a type of orbit in which an object moves in a path that is shaped like a parabola. It occurs when an object is moving with enough speed and at the right angle to escape the gravitational pull of a larger body, such as a planet or a star. This results in the object moving in a curved path around the larger body, rather than being pulled towards it.

5. How do the laws of motion and universal gravitation apply to circular motion and parabolic orbit?

The laws of motion, specifically Newton's first and second laws, explain the behavior of objects in circular motion by stating that an object in motion will continue to move in a straight line unless acted upon by an external force, and that the force acting on an object is equal to its mass multiplied by its acceleration. These laws also apply to objects in parabolic orbit, as the object is constantly accelerating due to the gravitational force acting on it from the larger body.

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