Confused About Calculating Period in Circular Motion?

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SUMMARY

The correct formula for calculating the period T of an object in circular motion is T = 2π√(m₁r/(m₂g)), where m₁ is the mass of the disk, m₂ is the mass hanging from the string, r is the radius of the circular path, and g is the acceleration due to gravity. The initial confusion arose from incorrectly using the angular velocity ω instead of the derived formula for T. The relationship between centripetal force and gravitational force was clarified through the application of Newton's Second Law.

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  • Understanding of circular motion dynamics
  • Familiarity with Newton's Second Law
  • Basic knowledge of gravitational force
  • Ability to manipulate algebraic equations
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  • Study the derivation of centripetal acceleration formulas
  • Learn about the relationship between angular velocity and linear velocity
  • Explore the concept of gravitational force in different contexts
  • Investigate practical applications of circular motion in engineering
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Students studying physics, particularly those focusing on mechanics and circular motion, as well as educators looking for clear explanations of these concepts.

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EDIT: I figured out what I did wrong. T=\frac{2{\pi}r}{v}, not \frac{2{\pi}r}{\omega}. Now it all falls together.

Homework Statement


A small disk of mass m_1 on a frictionless table is
attached to one end of a string. The string passes through a hole in the table and an attached narrow, vertical
plastic tube. An object of mass m_2 is hung at the other end of the string. A student holding the tube makes the
disk rotate in a circle of constant radius r, while another student measures the period T(if this is too hard to mentally picture, there is a diagram in the attachment). Derive the equation
T=2\pi\sqrt{\frac{m_{1}r}{m_{2}g}}

Homework Equations


a_{C}=\omega^{2}r

The Attempt at a Solution


First, it is apparent that T=\frac{2{\pi}r}{\omega}. So the question boils to what \omega is. Applying Newton's Second Law in the radial direction gives m_{1}\omega^{2}r=m_{2}g. This simplifies to \omega=\sqrt{\frac{m_{2}g}{m_{1}r}}. Agh! There's an extra r in my answer!
 

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Last edited:
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Centripetal force acting on the rotating disc is m1*ω^2*r. It is provided by the weight of m2.
So m2*g = m1*4π^2/T^2*r
Now solve for T.
 
I had figured it out before you posted, rl.bhat. Thanks for offering help anyway.
 

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