How is centripetal force involved here? (charged mass sliding down a conducting hemisphere)

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The discussion centers on understanding the role of centripetal force as a charged mass slides down a conducting hemisphere. Participants analyze the forces acting on the block, specifically the gravitational force and the normal force, and how these contribute to the block losing contact with the hemisphere. It is clarified that when the normal force becomes zero, the block only experiences gravitational force, indicating a loss of contact. The conversation also delves into deriving equations for the forces involved and the conditions under which the block maintains circular motion until it reaches a specific angle. Overall, the complexity of the problem arises from the interplay of forces and the need for a clear understanding of centripetal acceleration in a non-uniform circular motion context.
  • #31
haruspex said:
It can be surprising, though. On the thread about a planet in an elliptical orbit it struck me that the centripetal force is only towards the star at the apogee and perigee. At other points the gravitational attraction has a tangential component.
Sure. This is similar to 2D projectile motion near the surface of the Earth. There is always a centripetal component that becomes equal to the weight at the top of the trajectory.
 
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  • #32
haruspex said:
It often happens that there is an analytic way to find velocity as a function of position (e.g. by energy conservation) but not as a function of time. In such cases, the substitution ##\frac{dv}{dt}=\frac{dv}{dx}\frac{dx}{dt}=\frac{dv}{dx}v## can be useful.

To be exact, the component of that vector sum normal to the velocity is the centripetal force.
I see... Thankyou :)
 

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