Finding Angle of Sphere Falling From Table Edge

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Homework Help Overview

The discussion revolves around a solid spherical ball placed on the edge of a table, with a focus on determining the angle at which it begins to slip off due to a slight push. The problem involves concepts from dynamics, particularly the forces acting on the sphere and the role of friction.

Discussion Character

  • Mixed

Approaches and Questions Raised

  • Participants explore various equations related to conservation of energy and torque, questioning their validity in the context of the problem.
  • Some participants suggest considering forces at the point of contact and discuss the implications of treating the sphere as a point mass.
  • There are inquiries about the justification of certain assumptions, such as the behavior of forces acting on the sphere and the significance of the entire mass versus the center of mass.
  • Others propose using a co-rotating frame to analyze the equilibrium of forces acting on the sphere.

Discussion Status

The discussion is ongoing, with participants providing insights and questioning each other's reasoning. Some guidance has been offered regarding the treatment of forces and the use of different frames of reference, but no consensus has been reached on the correct approach or solution.

Contextual Notes

Participants are navigating through various assumptions and constraints, including the coefficient of static friction and the nature of forces acting on the sphere at the point of contact. There is a recognition of the complexity involved in balancing forces in a dynamic scenario.

Satvik Pandey
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Homework Statement


A solid spherical ball is placed carefully on the edge of a table in the position shown in the figure. The coefficient of static friction between the ball and the edge of the table is 0.5 . It is then given a very slight push. It begins to fall off the table.

Find the angle (in degrees)(with vertical) turned by the ball before it slips.
2e19e72524.fbc259d1f7.UhpXQY.png

Homework Equations

3. The attempt at question

I have came up with some equations. Let ##\theta## be the angle(with vertical) at which the sphere begins to slip.

p3.png

By conservation of energy
##mgr-mgrcos\theta =\frac { 1 }{ 2 } { I }_{ 0 }{ \omega }^{ 2 }##

As ##v=r \omega##

So ##g(1-cos\theta )=\frac { 7 }{ 10 } \frac { { v }^{ 2 } }{ r } ##

By finding torque about the contact point

##mgsin\theta r=\frac { 7 }{ 10 } m{ r }^{ 2 }\alpha ##

As ##a=r \alpha##

So ##\frac { 5gsin\theta }{ 7 } =a##

Also from FBD of the block

##mgcos\theta -N=m\frac { { v }^{ 2 } }{ r } ##

and ##\\ mgsin\theta -\mu N=ma##

I don't know if these equations are right. Please help.
 
Last edited:
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Satvik Pandey said:
##mgcos\theta -N=m\frac { { v }^{ 2 } }{ r } ##
I doubt that's right for the centripetal force on a sphere.
 
haruspex said:
I doubt that's right for the centripetal force on a sphere.

Could please explain, why? How to proceed?
 
Can this be solved by just considering the forces at the point of contact tangent to the sphere? That would give:
sin theta = 1/2 cos theta at the time of slipping.
 
Jilang said:
Can this be solved by just considering the forces at the point of contact tangent to the sphere? That would give:
sin theta = 1/2 cos theta at the time of slipping.

Could you please show how did you find that.
 
The frictional force at the point of contact would be mg cos theta x 1/2 at a tangent to the sphere and the gravitational force would be mg sine theta.
 
Jilang said:
Can this be solved by just considering the forces at the point of contact tangent to the sphere?

If you can find the normal force at the contact, then it is simple. Your result follows from equating the normal force with the radial component of the weight, but how do you justify this?
 
voko said:
If you can find the normal force at the contact, then it is simple. Your result follows from equating the normal force with the radial component of the weight, but how do you justify this?

voko ,what do you think about my equations?
 
Satvik Pandey said:
voko ,what do you think about my equations?

I agree with haruspex.
 
  • #10
Jilang said:
Can this be solved by just considering the forces at the point of contact tangent to the sphere? That would give:
sin theta = 1/2 cos theta at the time of slipping.
Not in the way you write, as the ball is not moving in a straight line.

See haruspex.
 
  • #11
voko said:
I agree with haruspex.

Could you please explain why that is not correct?:p
 
  • #12
Satvik Pandey said:
Could you please explain why that is not correct?

Because that assumes that the entire mass of the ball is at its center.
 
  • #13
voko said:
If you can find the normal force at the contact, then it is simple. Your result follows from equating the normal force with the radial component of the weight, but how do you justify this?
Consider the element of the sphere just touching the corner, it is stationary.
 
  • #14
Then how should I proceed?
 
  • #15
Jilang said:
Consider the element of the sphere just touching the corner, it is stationary.

But the rest of the ball is not. How do you justify the insignificance of that?
 
  • #16
voko said:
But the rest of the ball is not. How do you justify the insignificance of that?
The sphere is rigid, you need to assume that the force on every single atom is equal.
 
  • #17
Jilang said:
The sphere is rigid, you need to assume at the force on every single atom is equal.

Why?
 
  • #18
Do you think that the force of gravity only acts on the centre of mass?
 
  • #19
Satvik Pandey said:
Then how should I proceed?

Personally, I would use a co-rotating frame. In that frame, the ball is in equilibrium. The sum of real and fictitious forces is zero.
 
  • #20
voko said:
Personally, I would use a co-rotating frame. In that frame, the ball is in equilibrium. The sum of real and fictitious forces is zero.
Does that give a different answer?
 
  • #21
Jilang said:
Do you think that the force of gravity only acts on the centre of mass?

If that is a question to me, the answer is no.

Regardless, I asked you to justify your statements. Please do so.
 
  • #22
voko said:
Personally, I would use a co-rotating frame. In that frame, the ball is in equilibrium. The sum of real and fictitious forces is zero.

What is 'co-rotating frame'?
Are my other equations correct?
 
  • #23
haruspex said:
No, it's ok - just didn't seem right, and I didn't have time to check it before.

voko has just said that it's not correct. What should I do?:(
 
  • #24
Satvik Pandey said:
Could please explain, why? How to proceed?

Calculate it from first principles by integration.
 
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  • #25
Satvik Pandey said:
voko has just said that it's not correct. What should I do?:(
No, I mean I hadn't checked ... I have now and it is wrong.
 
  • #26
haruspex said:
Consider a uniform bar with its centre as the point of contact. It would require a centripetal force to get around the corner even though its mass centre does not.
Calculate it from first principles by integration.
I don't understand what you want me to calculate. Please explain more.
 
  • #27
Hm, interesting. Unless I made a mistake in integration, total centrifugal force is ## m \omega^2 r ##, that of a point mass, which means Satvik's disputed normal force equation was correct :)
 
  • #28
voko said:
Hm, interesting. Unless I made a mistake in integration, total centrifugal force is ## m \omega^2 r ##, that of a point mass, which means Satvik's disputed normal force equation was correct :)

But was the way in which I found it incorrect?
 
  • #29
Satvik Pandey said:
But was the way in which I found it incorrect?

As I said earlier, you assumed you could treat the ball as a point mass, and that was not justified.

Have a look here:

http://en.wikipedia.org/wiki/Rotating_reference_frame#Newton.27s_second_law_in_the_two_frames

The sum of the centrifugal force, Euler force, normal force, weight and friction must be zero (the Coriolis force is zero because the ball is stationary with respect to itself). The centrifugal and the Euler force must be integrated to obtain the force balance.
 
  • #30
voko said:
Hm, interesting. Unless I made a mistake in integration, total centrifugal force is ## m \omega^2 r ##, that of a point mass, which means Satvik's disputed normal force equation was correct :)
I managed to convince myself it could not be right, but now I see a flaw. I'll trust your integration.
 

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