Dynamics of circular motion. Particle on the top of a circle

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A particle of mass M starts falling from the top of a vertical circle without initial velocity, and the goal is to determine the angle at which it leaves the circle. The discussion involves using unit vectors to analyze the motion, applying equations for velocity and acceleration, and setting up force equations that include weight and normal force. A sign error in the integration process is identified, leading to confusion in the calculations. The correct angle at which the particle leaves the circle is found to be approximately 48.19 degrees, with suggestions to use conservation of energy for a more straightforward solution. The conversation highlights the importance of correct bounds in integration and careful attention to signs in equations.
Zipi Damn
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Homework Statement


A particle of mass M is on the top of a vertical circle without initial velocity. It starts to fall clockwise.

Find the angle with respect to the origin, where the particle leaves the circle.

bc8d1bbbf5.gif


Homework Equations


v=ωXr

The Attempt at a Solution



I used two unitary vectors..
εr : which direction is the same as the line described by the radio in the separation point.
εθ: perpendicular to εr (the direction of the tangential velocity in the separation point)

r=R er

v=dr/dt = Rder/dt
v=ωXr (counterclockwise, so I changedthe sign to negative)
v=-R(ωXer)

v = -R(-ω) = ωR
α=dω/dt

a = dv/dt = R(α + ω d/dt)

d/dt = -(ωX) = -ωer

a = α R - ω^2 R er

Forces:
Weight, Normal force
Centripetal is a resultant?

F(eθ)==> mgcosθ = αRm
F(er)==> N-mgsenθ= -ω^2Rm

So:

α=dω/dt= (dω/dθ)(dθ/dt)=ωdω/dθ

θ
∫αdθ =
∏/2

ω
∫ωdω
ω0

From F(er) : α= (gcosθ)/R

θ
∫ (gcosθ)/Rdθ = (gsenθ)/R
∏/2

ω
∫ωdω= (ω^2)/2
ω0ω^2 = (2gsenθ)/R

I come back to the force equations, (with zero normal force) and replace ω^2

And I get nonsenses like 2=1. Did I do something wrong?

Solution: 48,19º (by the teacher)
 
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Zipi Damn said:
θ
∫αdθ =
∏/2

ω
∫ωdω
ω0
Not sure exactly where, but you have a sign error. The first integral will be negative, but the second positive.
θ
∫ (gcosθ)/Rdθ = (gsenθ)/R
∏/2
You've not filled in the 'lower' bound correctly after integrating.
ω^2 = (2gsenθ)/R
Could have got this much more quickly and reliably by conservation of energy. Note that the RHS should be 1-sin, not sin.
 
I found it solved.

rbxrgn.jpg
 
The book claims the answer is that all the magnitudes are the same because "the gravitational force on the penguin is the same". I'm having trouble understanding this. I thought the buoyant force was equal to the weight of the fluid displaced. Weight depends on mass which depends on density. Therefore, due to the differing densities the buoyant force will be different in each case? Is this incorrect?

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