Torque & Angular Momentum
Just as force causes translational acceleration and linear momentum measures translational inertia in motion, Torque (Moment of Force) and Angular Momentum (Moment of Momentum) are their exact rotational counterparts. They constitute the cornerstone of rigid body dynamics.
1. Torque (Moment of Force) and Couple
When a force F acts on a particle located at position vector r relative to a reference origin O, the torque τ about O is defined as:
Alternatively, the scalar magnitude can be written in two illuminating physical forms:
- τ = r⊥ F, where r⊥ = r sin θ is the lever arm (perpendicular distance from origin to the line of action of force).
- τ = r F⊥, where F⊥ = F sin θ is the component of force perpendicular to the position vector r.
Units & Dimensions: SI Unit is Newton-meter (N·m). Dimensional formula: [ML²T⁻²]. (Caution: Although dimensionally identical to Joule, torque is a vector perpendicular to the plane of motion, while work is a scalar; torque is never expressed in Joules).
The Concept of a Couple
A couple consists of a pair of equal and opposite parallel forces whose lines of action do not coincide:
- Net translational force is zero: Fnet = F − F = 0 (no translational acceleration).
- Net torque is independent of the choice of origin: τcouple = Force × perpendicular distance between force lines (arm of couple).
- Everyday examples: Turning a water tap, opening a bottle cap, rotating a steering wheel with two hands.
2. Angular Momentum of a Particle & a System
The angular momentum L of a particle of mass m moving with linear velocity v (and linear momentum p = m v) about origin O is:
In scalar magnitude: L = p r⊥ = m v r⊥ (Momentum × Perpendicular distance from line of motion to origin).
Units & Dimensions: SI unit is kg·m²/s or Joule-second (J·s). Dimensions: [ML²T⁻¹] (same as Planck's constant h).
Angular Momentum of a Rigid Body About a Fixed Axis
For a rigid body rotating with angular velocity ω about a fixed axis:
where I is the Moment of Inertia of the body about that axis.
3. Fundamental Relation: τ = dL/dt and Angular Momentum Conservation
Differentiating angular momentum with respect to time:
dL/dt = d(r × p)/dt = (dr/dt × p) + (r × dp/dt)
Since dr/dt = v and p = m v, the term (v × m v) = 0. Substituting Newton's second law dp/dt = Fext:
Principle of Conservation of Angular Momentum
If the net external torque acting on a system is zero (τext = 0):
When the moment of inertia changes due to internal reconfiguration of mass, angular velocity automatically adjusts in inverse proportion:
- Ballet Dancer / Figure Skater: Outstretched arms ⇒ high I, low ω. Drawing arms close to body ⇒ I drops sharply, ω surges into a rapid spin.
- Springboard Diver: Curls body into a compact tuck position to reduce I and perform multiple somersaults before extending to enter water cleanly.
- Planetary Motion (Kepler's 2nd Law): Gravitational force is central (directed along r), so r × Fg = 0. Hence L = m r v = const. As the planet nears the sun at perihelion (r decreases), its orbital speed v increases.
4. Work Done by Torque and Rotational Power
When a torque τ rotates a body through an infinitesimal angular displacement dθ:
This is identical to the translational work-power relations dW = F dx and P = F v.
Figure 6.3 — Conservation of Angular Momentum: The Spinning Skater
Step-by-Step Solved Numerical Examples
Problem: A projectile of mass m is launched with velocity u at an angle θ with the horizontal. Find the magnitude of its angular momentum about the point of projection when it reaches its maximum height H.
At maximum height, the vertical velocity component is zero (vy = 0). The projectile has only horizontal velocity: v = u cos θ.
Step 2: Find the Perpendicular Distance (Lever Arm):
The line of action of the velocity at the summit is horizontal at height H above the ground.
Thus, the perpendicular distance from the projection point (origin) to the velocity vector line is simply r⊥ = H.
Recall maximum height formula: H = (u² sin²θ) / (2g).
Step 3: Calculate Angular Momentum:
L = m v r⊥ = m (u cos θ) [ (u² sin²θ) / (2g) ]
L = (m u³ sin²θ cosθ) / (2g) directed perpendicularly into the plane of trajectory.
Problem: A uniform horizontal disc of mass M = 2 kg and radius R = 0.2 m is rotating freely about its central vertical axis at 60 rpm. A small lump of wax of mass m = 0.5 kg is dropped gently onto the disc and sticks at a distance of 0.1 m from the axis. Calculate the new rotational speed of the system in rpm.
For the uniform circular disc: I1 = ½ M R² = ½(2)(0.2)² = 0.04 kg·m².
Initial angular speed: N1 = 60 rpm.
Step 2: Final Moment of Inertia:
When wax sticks at r = 0.1 m:
Iwax = m r² = (0.5)(0.1)² = 0.005 kg·m².
Total final moment of inertia: I2 = I1 + Iwax = 0.04 + 0.005 = 0.045 kg·m².
Step 3: Apply Conservation of Angular Momentum:
Since dropping the wax exerts no net external torque along the vertical axis:
I1 N1 = I2 N2
(0.04)(60) = (0.045) N2 ⇒ N2 = 2.4 / 0.045 = 53.33 rpm.
5. Solved NEET & JEE Practice Questions
A. 17î − 6ĵ − 13k̂ N·m
B. −17î + 6ĵ + 13k̂ N·m
C. 17î + 6ĵ − 13k̂ N·m
D. −17î − 6ĵ − 13k̂ N·m
î[(2)(4) − (3)(−3)] − ĵ[(3)(4) − (3)(2)] + k̂[(3)(−3) − (2)(2)]
= î[8 + 9] − ĵ[12 − 6] + k̂[−9 − 4] = 17î − 6ĵ − 13k̂ N·m.
A. The radius vector
B. The tangent to the orbit
C. A line perpendicular to the plane of rotation
D. At 45° to the plane of rotation
A. 6 hours
B. 12 hours
C. 24 hours
D. 48 hours
Since no external torque acts: L = I ω = I (2π/T) = constant ⇒ T ∝ I.
Therefore, T' = T / 4 = 24 / 4 = 6 hours.
A. Increases with time
B. Decreases with time
C. Remains constant in magnitude and direction
D. Is zero
6. Frequently Asked Questions (FAQs)
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