Particle Energy on a Smooth Sphere: Finding the Point of Departure

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SUMMARY

The discussion centers on determining the point at which a particle, placed on a smooth sphere of radius b at a height of b/2, will leave the sphere as it slides down. The key conclusion is that the particle departs when the normal force equals zero, leaving only gravitational force acting on it. Participants emphasized the importance of analyzing the centripetal component of gravitational force as a function of the angle theta and applying conservation of mechanical energy principles. The final result for the angle at which the particle leaves the sphere is θ = arcsin(1/3).

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  • Understanding of potential and kinetic energy concepts
  • Knowledge of centripetal force and its relation to gravitational force
  • Familiarity with trigonometric functions, specifically arcsin and arccos
  • Basic principles of mechanical energy conservation
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  • Study the principles of conservation of mechanical energy in physics
  • Learn about centripetal force and its applications in circular motion
  • Explore the use of trigonometric functions in physics problems
  • Investigate the dynamics of particles on curved surfaces
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Students studying classical mechanics, physics educators, and anyone interested in the dynamics of particles on curved surfaces.

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Homework Statement



A Particle is place on a smooth sphere of radius b at a distance b/2 above the central plane. As the particle slides down the side of the sphere at what point will it leave?

Homework Equations



potential and kinetic energies

The Attempt at a Solution



no idea
 
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The particle leaves the sphere when the normal force is zero. So the only force acting on it will be the gravitational force.

Find the centripetal component of the gravitational force as a function of the angle theta. Then write the expressions for the conservation of mechanical energy, and use the fact that F = (mv^2)/b. A few mathematical manipulations later, you will find an expression of the type sin θ = constant, or cos θ = constant. Use the arc sine or arc cosine functions accordingly to find θ. That will be your answer. You may transform to rectangular coordinates if the problem asks for it.

I know it sounds like a lot of work, but it actually isn't.
 
Thanks, i actually managed it, it came b/3 :)

Thanks for the help.
 

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