Quick Recap — Rotation Basics

  • Moment of inertia I=miri2I = \sum m_i r_i^2 (unit kg m2^2) — the rotational analogue of mass; radius of gyration kk satisfies I=mk2I = mk^2.
  • Torque τ=r×F=Iα\vec{\tau} = \vec{r}\times\vec{F} = I\vec{\alpha} (unit N m).
  • Angular momentum L=IωL = I\omega (unit kg m2^2/s); it is conserved when the net external torque is zero.
  • Rotational kinetic energy =12Iω2= \tfrac12 I\omega^2; and v=ωrv = \omega r links linear and angular speed.
  • Standard moments of inertia (mass MM, radius RR): ring MR2MR^2, disc 12MR2\tfrac12 MR^2, solid sphere 25MR2\tfrac25 MR^2, hollow sphere 23MR2\tfrac23 MR^2.

Beyond-NCERT JEE Formulae

Moment of inertia — the six to know cold (mass MM, radius RR, length LL; about the symmetry axis unless stated):

  • Ring / thin hoop (perpendicular axis): I=MR2I=MR^2
  • Disc / solid cylinder (perpendicular axis): I=12MR2I=\tfrac12 MR^2
  • Solid sphere (about a diameter): I=25MR2I=\tfrac25 MR^2
  • Hollow (thin) sphere (about a diameter): I=23MR2I=\tfrac23 MR^2
  • Rod about its centre (perpendicular): I=112ML2I=\tfrac{1}{12}ML^2
  • Rod about one end (perpendicular): I=13ML2I=\tfrac13 ML^2

When to use: these are the building blocks of every composite-body and rolling question. [JEE Tip] Store each body by its shape factor k2R2\dfrac{k^2}{R^2} — ring 11, disc 12\tfrac12, solid sphere 25\tfrac25, hollow sphere 23\tfrac23. Most rolling MCQs collapse to a single line once you read off this number.

Parallel-axis theorem: I=Icm+Md2I=I_{cm}+Md^2 — shift from the centre-of-mass axis to any parallel axis a distance dd away. You always ADD the Md2Md^2 term, never subtract it.

Perpendicular-axis theorem (flat laminae only): for a planar body lying in the xyxy-plane, Iz=Ix+IyI_z=I_x+I_y.

When to use: discs, rings and square plates — never a solid 3-D body. [JEE Tip] For a disc, symmetry forces Ix=IyI_x=I_y, so the diameter value is Idiam=12Iz=14MR2I_{diam}=\tfrac12 I_z=\tfrac14 MR^2 at a glance; for a ring it comes out as 12MR2\tfrac12 MR^2.

Radius of gyration: k=I/Mk=\sqrt{I/M}, equivalently I=Mk2I=Mk^2. It is the single distance at which the entire mass could sit and reproduce the same II.

Rolling without slipping (so that v=Rωv=R\omega) — total kinetic energy:

KE=12Mv2(1+k2R2)KE=\tfrac12 Mv^2\left(1+\dfrac{k^2}{R^2}\right)

The rotational share of that energy is k2/R21+k2/R2\dfrac{k^2/R^2}{1+k^2/R^2}, which is 27\tfrac27 for a solid sphere and 12\tfrac12 for a ring.

Rolling down a rough incline of angle θ\theta:

a=gsinθ1+k2/R2,vbottom=2gh1+k2/R2a=\dfrac{g\sin\theta}{1+k^2/R^2},\qquad v_{bottom}=\sqrt{\dfrac{2gh}{1+k^2/R^2}}

Friction supplies the spin-up torque, so the friction actually required and the minimum coefficient for pure rolling are

f=Mgsinθ(k2/R2)1+k2/R2,μmin=(k2/R2)tanθ1+k2/R2f=\dfrac{Mg\sin\theta\,(k^2/R^2)}{1+k^2/R^2},\qquad \mu_{min}=\dfrac{(k^2/R^2)\tan\theta}{1+k^2/R^2}

When to use: any "which body wins the race" or "which rolls faster" problem. [JEE Tip] A smaller k2R2\dfrac{k^2}{R^2} always wins — solid sphere beats disc beats hollow sphere beats ring, regardless of mass or radius. If the surface can only offer μ<μmin\mu<\mu_{min} the body slips, and you must switch to kinetic friction μN\mu N.

Torque, angular momentum and Newton's second law for rotation:

τ=Iα,L=Iω,τ=dLdt\tau=I\alpha,\qquad L=I\omega,\qquad \tau=\dfrac{dL}{dt}

Conservation of angular momentum (zero external torque): I1ω1=I2ω2I_1\omega_1=I_2\omega_2.

When to use: a skater pulling her arms in, a disc dropped coaxially onto another, clay landing on a turntable. [JEE Tip] Kinetic energy is NOT conserved in these problems — track it with KE=L22IKE=\dfrac{L^2}{2I}. Energy falls whenever two bodies merge (the shared II grows) and rises when a body draws itself inward (II shrinks while internal muscles do the work).

Other beyond-NCERT results worth carrying:

  • Rotational work-energy and power: W=τθW=\tau\,\theta and P=τωP=\tau\omega.
  • Angular impulse: τdt=ΔL\displaystyle\int\tau\,dt=\Delta L — the tool to reach for when the torque varies with time and α\alpha is not constant.
  • Kinetic energy from angular momentum: KE=L22IKE=\dfrac{L^2}{2I}.
  • Compound (physical) pendulum: T=2πIMgdT=2\pi\sqrt{\dfrac{I}{Mgd}}, where dd is the pivot-to-centre-of-mass distance.
  • Toppling versus sliding of a block (base width bb, height hh) on a tilting surface: it topples about its lower edge if tanθ>bh\tan\theta>\dfrac{b}{h}, but slides first if μ<bh\mu<\dfrac{b}{h}. [JEE Tip] Whichever threshold is crossed at the smaller tilt happens first, so the block topples rather than slides precisely when μ>bh\mu>\dfrac{b}{h}.

Solved Examples — Beyond-NCERT Formulae

Example 1 — Parallel-axis theorem (rod). A uniform rod of mass 22 kg and length 1.21.2 m turns about a perpendicular axis through a point one-third of the way along it from one end. Find its moment of inertia about that axis.

Step 1 — central value. About a perpendicular axis through the centre, Icm=112ML2=112(2)(1.2)2=0.24I_{cm}=\tfrac{1}{12}ML^2=\tfrac{1}{12}(2)(1.2)^2=0.24 kg m2^2.

Step 2 — shift distance. The axis lies L3=0.4\tfrac{L}{3}=0.4 m from the end, so its distance from the centre is d=L2L3=0.60.4=0.2d=\tfrac{L}{2}-\tfrac{L}{3}=0.6-0.4=0.2 m.

Step 3 — apply the theorem. I=Icm+Md2=0.24+2(0.2)2=0.24+0.08=0.32I=I_{cm}+Md^2=0.24+2(0.2)^2=0.24+0.08=0.32 kg m2^2.

Answer: I=0.32I=0.32 kg m2^2. The shift adds only 0.080.08, since the axis still sits fairly close to the mass.

Example 2 — Perpendicular-axis theorem and radius of gyration (disc). A uniform disc has mass 33 kg and radius 0.20.2 m. Find its moment of inertia about a diameter, and the matching radius of gyration.

Step 1 — central perpendicular axis. Iz=12MR2=12(3)(0.2)2=0.06I_z=\tfrac12 MR^2=\tfrac12(3)(0.2)^2=0.06 kg m2^2.

Step 2 — perpendicular-axis theorem. The disc is planar, so Iz=Ix+IyI_z=I_x+I_y; by symmetry Ix=Iy=IdiamI_x=I_y=I_{diam}, hence Idiam=12Iz=0.03I_{diam}=\tfrac12 I_z=0.03 kg m2^2, which is the familiar 14MR2\tfrac14 MR^2.

Step 3 — radius of gyration. k=Idiam/M=0.03/3=0.01=0.1k=\sqrt{I_{diam}/M}=\sqrt{0.03/3}=\sqrt{0.01}=0.1 m, exactly R2\tfrac{R}{2}.

Answer: Idiam=0.03I_{diam}=0.03 kg m2^2 and k=0.1k=0.1 m.

Example 3 — Which rolls faster: solid sphere versus ring. A solid sphere and a ring are each released from rest and roll without slipping from the same height h=1.4h=1.4 m. Take g=10g=10 m/s2^2. Compare their speeds at the bottom.

Step 1 — the formula. Energy conservation for a rolling body gives vbottom=2gh1+k2/R2v_{bottom}=\sqrt{\dfrac{2gh}{1+k^2/R^2}}.

Step 2 — solid sphere, for which k2R2=25\dfrac{k^2}{R^2}=\tfrac25. Then v=2(10)(1.4)1+2/5=281.4=20=4.47v=\sqrt{\dfrac{2(10)(1.4)}{1+2/5}}=\sqrt{\dfrac{28}{1.4}}=\sqrt{20}=4.47 m/s.

Step 3 — ring, for which k2R2=1\dfrac{k^2}{R^2}=1. Then v=281+1=14=3.74v=\sqrt{\dfrac{28}{1+1}}=\sqrt{14}=3.74 m/s.

Step 4 — compare. The sphere is faster by a factor 20/14=1.20\sqrt{20/14}=1.20, because it locks up a smaller share of its energy as spin.

Answer: solid sphere 4.474.47 m/s, ring 3.743.74 m/s. The outcome is independent of the masses and radii chosen.

Example 4 — Rolling acceleration and the friction it demands. A solid sphere of mass 22 kg rolls without slipping down an incline of 3030^\circ; take g=10g=10 m/s2^2. Find its acceleration, the friction force acting on it, and the minimum coefficient of friction required.

Step 1 — acceleration. a=gsinθ1+k2/R2=10×0.51+2/5=51.4=3.57a=\dfrac{g\sin\theta}{1+k^2/R^2}=\dfrac{10\times 0.5}{1+2/5}=\dfrac{5}{1.4}=3.57 m/s2^2.

Step 2 — friction force. f=Mgsinθ(k2/R2)1+k2/R2=(2)(10)(0.5)(2/5)1.4=41.4=2.86f=\dfrac{Mg\sin\theta\,(k^2/R^2)}{1+k^2/R^2}=\dfrac{(2)(10)(0.5)(2/5)}{1.4}=\dfrac{4}{1.4}=2.86 N, which is simply 27Mgsinθ\tfrac27 Mg\sin\theta.

Step 3 — minimum coefficient. μmin=(k2/R2)tanθ1+k2/R2=27tan30=0.165\mu_{min}=\dfrac{(k^2/R^2)\tan\theta}{1+k^2/R^2}=\tfrac27\tan 30^\circ=0.165.

Answer: a=3.57a=3.57 m/s2^2, f=2.86f=2.86 N and μmin=0.165\mu_{min}=0.165. Should the real μ\mu fall below 0.1650.165, the sphere slips instead of rolling purely.

Example 5 — Angular momentum conservation (spinning skater). A skater on frictionless ice spins with her arms out at ω1=2\omega_1=2 rad/s, her moment of inertia being I1=6I_1=6 kg m2^2. She pulls her arms in, cutting it to I2=2I_2=2 kg m2^2. Find her new angular speed and the change in kinetic energy.

Step 1 — conserve angular momentum. There is no external torque, so I1ω1=I2ω2I_1\omega_1=I_2\omega_2, giving ω2=I1ω1I2=(6)(2)2=6\omega_2=\dfrac{I_1\omega_1}{I_2}=\dfrac{(6)(2)}{2}=6 rad/s.

Step 2 — the two energies. KE1=12I1ω12=12(6)(2)2=12KE_1=\tfrac12 I_1\omega_1^2=\tfrac12(6)(2)^2=12 J, while KE2=12I2ω22=12(2)(6)2=36KE_2=\tfrac12 I_2\omega_2^2=\tfrac12(2)(6)^2=36 J.

Step 3 — interpret. The kinetic energy triples, since KE2KE1=I1I2=3\dfrac{KE_2}{KE_1}=\dfrac{I_1}{I_2}=3; the extra 2424 J is the work her muscles do drawing the arms inward.

Answer: ω2=6\omega_2=6 rad/s, with the energy rising from 1212 J to 3636 J.

Example 6 — Disc dropped onto a spinning disc. A disc of moment of inertia I1=4I_1=4 kg m2^2 spins at ω0=9\omega_0=9 rad/s about a vertical axis. A second, non-rotating disc of I2=2I_2=2 kg m2^2 is lowered gently and coaxially onto it, and the two then turn together. Find the common angular speed and the energy lost.

Step 1 — conserve angular momentum. The drop applies no torque about the axis, so I1ω0=(I1+I2)ωI_1\omega_0=(I_1+I_2)\omega, giving ω=I1ω0I1+I2=(4)(9)6=6\omega=\dfrac{I_1\omega_0}{I_1+I_2}=\dfrac{(4)(9)}{6}=6 rad/s.

Step 2 — the two energies. KEi=12I1ω02=12(4)(9)2=162KE_i=\tfrac12 I_1\omega_0^2=\tfrac12(4)(9)^2=162 J, and KEf=12(I1+I2)ω2=12(6)(6)2=108KE_f=\tfrac12(I_1+I_2)\omega^2=\tfrac12(6)(6)^2=108 J.

Step 3 — the loss. A total of ΔKE=162108=54\Delta KE=162-108=54 J is dissipated as the surfaces slip into step — a fraction I2I1+I2=13\dfrac{I_2}{I_1+I_2}=\tfrac13 of the original energy.

Answer: ω=6\omega=6 rad/s, with 5454 J (one-third) lost. Angular momentum is conserved; kinetic energy is not.

Example 7 — Topple or slide? (block on a tilting surface). A uniform block of base width b=0.4b=0.4 m and height h=1.0h=1.0 m rests on a plank whose tilt is slowly raised. The coefficient of static friction is μ=0.5\mu=0.5. Determine whether the block topples or slides first.

Step 1 — toppling threshold. The block tips about its lower edge once the vertical line through its centre of mass reaches that edge, that is when tanθ=bh=0.4\tan\theta=\dfrac{b}{h}=0.4, so θtopple=21.8\theta_{topple}=21.8^\circ.

Step 2 — sliding threshold. It begins to slide once tanθ=μ=0.5\tan\theta=\mu=0.5, so θslide=26.6\theta_{slide}=26.6^\circ.

Step 3 — compare. The smaller angle is reached first, and 21.8<26.621.8^\circ<26.6^\circ, so the block TOPPLES before it slides — equivalently, toppling wins because μ>bh\mu>\dfrac{b}{h}.

Answer: the block topples first, at roughly 2222^\circ. A wider or shorter block (a larger bh\dfrac{b}{h}) would instead slide.