Conservation of mechanical energy for skier on sphere

AI Thread Summary
A skier starts from rest at the top of a solid sphere and slides down its frictionless surface, raising the question of the angle θ at which they will leave the sphere. The key to solving this problem lies in understanding that the skier will detach when the normal force equals zero. The relationship between potential energy (PE) and kinetic energy (KE) is established, leading to the equation v^2 / 2 = grsin(θ). Additionally, the force equations must account for the components of forces acting perpendicular to the surface. Properly applying Newton's second law and centripetal force concepts is crucial for determining the correct angle of departure.
NathanLeduc1
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Homework Statement


A skier of mass m starts from rest at the top of a solid sphere of radius r and slides down its frictionless surface. At what angle θ will the skier leave the sphere?

Homework Equations


KE= 0.5mv^2
PE = mgh
Fc = (mv^2)/r


The Attempt at a Solution


I am really quite confused and don't even know how to begin. I know that the skier will fall off when the normal force is 0 but I'm not sure how to even get to that point.
I thought that PE=KE so 0.5mv^2 = mgh which simplifies to 0.5v^2 = gh
 
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NathanLeduc1 said:
I know that the skier will fall off when the normal force is 0 but I'm not sure how to even get to that point.
That's the key point. To make use of it, set up a force equation with Newton's 2nd law.
I thought that PE=KE so 0.5mv^2 = mgh which simplifies to 0.5v^2 = gh
Good. You'll need that too. (Express h in terms of θ.)
 
So rewriting the energy equations gives me
v^2 / 2 = grsin(θ).

When I write the force equations, I get
N-mg = ma
N = mg + mg
N = m(a+g)
m = N/(a+g)

If I plug that into the centripetal force equation, I get
F = (mv^2)/r
F = (Nv^2)/((r)(a+g))

Is this right? If so, where do I go from here? Sorry to ask such dumb questions, I'm just very confused on this problem.
 
NathanLeduc1 said:
So rewriting the energy equations gives me
v^2 / 2 = grsin(θ).
What you want is Δh, the drop from the original position at the top. Δh ≠ r sinθ.

When I write the force equations, I get
N-mg = ma
N = mg + mg
N = m(a+g)
m = N/(a+g)
Careful! Forces are vectors.

Hint: Consider force components perpendicular to the surface at any point.
 
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