Sliding on a sliding hemisphere

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SUMMARY

The discussion centers on a physics problem involving a small mass m sliding on a hemisphere of mass M and radius R, which is free to slide on a frictionless table. The user initially attempts to apply conservation of energy and momentum to derive the ratio M/m, ultimately arriving at the equation \(\frac{(k-1)}{k(2-k)}2 = M/m\). The user identifies mistakes in their calculations, particularly in the conservation of energy, and seeks guidance on correctly solving the problem.

PREREQUISITES
  • Understanding of classical mechanics principles, particularly conservation of energy and momentum.
  • Familiarity with the geometry of a hemisphere and angular relationships.
  • Knowledge of kinematics, specifically tangential speed and acceleration.
  • Ability to manipulate algebraic equations and solve for variables.
NEXT STEPS
  • Review the principles of conservation of energy in dynamic systems.
  • Study the conditions for an object to maintain contact with a curved surface.
  • Learn about the dynamics of two-body systems and their interactions.
  • Practice solving similar problems involving motion on curved surfaces and frictionless environments.
USEFUL FOR

Students studying physics, particularly those focusing on mechanics and dynamics, as well as educators seeking to enhance their understanding of motion on curved surfaces.

Nanyang
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Homework Statement


A small mass m slides on a hemisphere of mass M and radius R is also free to slide horizontally on a frictionless table. An imaginary vertical line is drawn from the center of the hemisphere to its highest point, where the small mass is originally placed at rest. The angle A is the acute angle made by another imaginary line drawn from the small mass after it starts to slide down to the center of the hemisphere with the imaginary vertical line mentioned before. In other words, A= 0 originally. Given that cosA = k. Find the ratio of M/m.

Homework Equations


I'm not really sure.

The Attempt at a Solution


Here's what I did.

I imagine that the big mass moves at velocity V and the small mass with a tangential speed v after some time. Then using the conservation of energy I obtain,

mgR = \frac{1}{2}(M+m)V2 + \frac{1}{2}mv2EDIT: I just spot my mistake on the mgR thing.

Next I obtain the condition when the small mass just begins to leave the hemisphere's surface,

gcosA= v²/R

I think my mistake is the above.

I then obtain another equation using the conservation of momentum in the left-right direction,

mvcosA=(M+m)V

Then I substituted and rearranged all the stuff and got:

\frac{(k-1)}{k(2-k)}2 = M/m

But it doesn't look correct.

EDIT: I think I found the mistake in the conservation of energy part. But still do give hints on how to solve it.
 
Last edited:
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I just solved it. Anyway, typing the problem down again here sure does help in solving it by making you think hard again. :smile:
 

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