Physic Labs

Newtonian mechanics

Moment of inertia and rotational motion

Compare how mass is distributed about the axis of a thin hoop and a solid disk, then verify the fixed-axis relations Ihoop=MR2I_{\mathrm{hoop}}=MR^2, Idisk=12MR2I_{\mathrm{disk}}=\tfrac12MR^2 and τ=Iα\tau=I\alpha.

Undergraduate

Equipment

  • Virtual thin hoop and solid disk on a fixed axis
  • Sliders “Khối lượng M” (mass) and “Bán kính R” (radius)
  • Sliders “Momen lực τ” (torque) and “Tốc độ góc ω” (angular speed)
  • Rotatable 3D canvas with angular-acceleration readout

Procedure

  1. Set M and R

    Set the mass M and radius R with the two sliders and watch the hoop and disk rotate at the same angular speed. All of the hoop's mass sits at radius R while the disk's mass is spread inward, so Ihoop=MR2I_{\mathrm{hoop}}=MR^2 is twice Idisk=12MR2I_{\mathrm{disk}}=\tfrac12MR^2; compare the displayed values with these formulas.

  2. Apply a torque

    Drag the torque slider τ upward and read the angular acceleration α of each body. The same τ produces a smaller α on the hoop because its I is larger; check that the readout follows α=τ/I\alpha=\tau/I.

  3. Rotational kinetic energy

    Set an angular speed ω with its slider and compare the rotational kinetic energy stored in each body, Krot=12Iω2K_{\mathrm{rot}}=\tfrac12I\omega^2. Then keep M fixed and double R: since I∝MR2I\propto MR^2, the stored energy quadruples at the same ω.

  4. Predict the spin-up race

    Before touching the sliders, predict which body reaches a target ω first under the same torque, then test it. Repeat with a different M or R and explain each outcome from I=∫r⊥2 dmI=\int r_\perp^2\,dm and τ=Iα\tau=I\alpha.

Simulation

Experiment history

Newton's Principia (1687) treated bodies mainly as point masses, so rotation of extended objects still lacked a general theory. Christiaan Huygens approached the problem through the pendulum in Horologium Oscillatorium (1673), where he found the center of oscillation by comparing distributed mass with an equivalent point mass — an early use of what became the moment of inertia. Leonhard Euler developed rigid-body dynamics in the mid-18th century, culminating in Theoria motus corporum solidorum (1765), where moments and products of inertia about principal axes appear in modern form. The name and the standard formulas MR2MR^2 for a hoop and 12MR2\tfrac12MR^2 for a disk come from this analytical tradition, later organized in the textbooks of Lagrange and his successors.

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