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Class 11 · Physics · Part 1

Chapter 6: Systems of Particles and Rotational Motion

Revision notes, practice numericals, a question bank, assertion and reason questions and answers to the NCERT questions. Tap a group to open it; opening one closes the others.

6.1–6.2Rigid bodies and the centre of massTranslation, rotation, X = Σ m x / M

Rigid body motion

  • An ideal rigid body keeps the distances between all its particles fixed. Real solids are only approximately rigid, but the idea works well for wheels, tops and beams.
  • Pure translation: at any instant every particle has the same velocity. Rotation about a fixed axis: every particle moves in a circle whose centre is on the axis (a ceiling fan, a potter's wheel).
  • Motion can be a mixture of the two. The axis itself may move (a spinning top, an oscillating table fan), or the body may be fixed at a single point.
Pure translationall particles: the same velocityRotation about a fixed axisaxiseach particle: a circle about the axis, v = ω r
Rigid body motion: translation (same velocity everywhere) and rotation about a fixed axis (circles about the axis).

The centre of mass

  • For particles of masses m₁, m₂, … mₙ the centre of mass has coordinates X = Σ mᵢ xᵢ / M, Y = Σ mᵢ yᵢ / M, Z = Σ mᵢ zᵢ / M, where M = Σ mᵢ. In vector form R = Σ mᵢ rᵢ / M.
  • For a continuous body the sums become integrals, R = (1/M) ∫ r dm. For a uniform body with a centre of symmetry (sphere, cylinder, ring, cube, rod, disc) the centre of mass is at the geometric centre.
  • The centre of mass need not lie inside the body (a ring, a horseshoe). The result does not depend on the axes chosen, only its coordinates do.
xm₁ = 1 kgm₂ = 3 kgCMx₁x₂XX = (m₁ x₁ + m₂ x₂)/(m₁ + m₂)the centre of mass lies nearer the heavier mass
Centre of mass of two particles: the mass-weighted average position (here X = x₁ + 0.75 (x₂ − x₁)).

Examples

  • Example 6.1: masses 100 g, 150 g and 200 g at the vertices of an equilateral triangle of side 0.5 m (the 100 g mass at the origin, the 150 g mass along the x-axis): X = (150 × 0.5 + 200 × 0.25)/450 = 5/18 m and Y = 200 × 0.25 √3 / 450 = 1/(3√3) m.
  • Example 6.2: a uniform triangular lamina has its centre of mass at the centroid (where the medians meet).
  • Example 6.3: an L-shaped lamina made of three unit squares has its centre of mass at (5/6, 5/6) m, found by treating each square as a point mass at its own centre.
6.3–6.4Motion of the centre of mass and linear momentumM A = Fext, P = M V

Motion of the centre of mass

  • Differentiating M R = Σ mᵢ rᵢ twice: M A = Σ Fᵢ = Fext. The internal forces occur in equal and opposite pairs (Newton's third law) and cancel in the sum.
  • So the centre of mass of a system moves like a single particle of mass M acted on by the total external force. Nothing about the internal forces or the internal motion is needed.
  • A projectile that bursts in mid-air: the fragments fly apart but their centre of mass keeps moving along the original parabola, because the only external force (gravity) is unchanged.

Linear momentum of a system

  • P = Σ pᵢ = M V, where V is the velocity of the centre of mass. Also dP/dt = Fext.
  • If Fext = 0, then P is constant: the total momentum is conserved and the centre of mass moves with constant velocity.
  • Examples: a nucleus decaying at rest (the fragments' momenta are equal and opposite); the two stars of a binary system, which orbit their common centre of mass; a man walking on a boat floating on still water (the boat moves the other way so that the centre of mass stays at rest).
  • In the centre of mass frame the total momentum is zero, which often simplifies collision and decay problems.
6.5The vector producta × b = a b sin θ, right-hand rule

Definition and properties

  • a × b = a b sin θ n̂, where θ is the angle between the vectors and n̂ is a unit vector perpendicular to both, given by the right-hand rule (turn the fingers from a to b; the thumb gives the direction). The magnitude equals the area of the parallelogram on a and b.
  • It is not commutative: a × b = − b × a. It is distributive: a × (b + c) = a × b + a × c. Also a × a = 0 (a null vector), and a × b = 0 if a ∥ b.
  • Unit vectors: î × ĵ = k̂, ĵ × k̂ = î, k̂ × î = ĵ, and î × î = 0.
  • In components a × b = (ay bz − az by) î + (az bx − ax bz) ĵ + (ax by − ay bx) k̂, the determinant of the 3 × 3 array with rows (î, ĵ, k̂), (ax, ay, az), (bx, by, bz).
  • Example 6.4: for a = 3 î − 4 ĵ + 5 k̂ and b = −2 î + ĵ − 3 k̂: a · b = −25 and a × b = 7 î − ĵ − 5 k̂.
θaba × b points out of the page|a × b| = a b sin θ= area of the parallelogram
The vector product a × b: perpendicular to a and b (right-hand rule); its magnitude is the area of the parallelogram.
6.6–6.7Angular velocity, torque and angular momentumv = ω × r, τ = r × F, l = r × p, dL/dt = τ

Angular velocity and acceleration

  • For rotation about a fixed axis the angular velocity ω = dθ/dt is a vector along the axis (right-hand rule). The linear velocity of a particle at position r is v = ω × r, of magnitude v = ω r⊥, where r⊥ is its perpendicular distance from the axis.
  • The angular acceleration is α = dω/dt. For a fixed axis it is the same for all particles.

Moment of a force: torque

  • τ = r × F, of magnitude τ = r F sin θ = r⊥ F = r F⊥. Its SI unit is N m and its dimensions are [M L² T⁻²] (the same as work, though torque is a vector and work is a scalar).
  • The torque is zero if F = 0, if r = 0, or if the line of action of F passes through the origin. Example 6.5: for r = î − ĵ + k̂ and F = 7 î + 3 ĵ − 5 k̂: τ = 2 î + 12 ĵ + 10 k̂ N m.
OrFF sin θθτ = r F sin θ = r F⊥τ points out of the page
Torque τ = r × F: only the component of F perpendicular to r (F sin θ) turns the body.

Angular momentum

  • For a particle, l = r × p, of magnitude l = r p sin θ = m v r⊥. Differentiating, dl/dt = r × F = τ.
  • For a system, L = Σ lᵢ and dL/dt = τext. The internal torques cancel because the internal forces are equal, opposite and (for central forces) along the line joining the particles.
  • Conservation: if τext = 0, then L is constant. For a single particle, a constant velocity along a straight line gives a constant angular momentum (Example 6.6).
  • In components, lx = y pz − z py, ly = z px − x pz, lz = x py − y px. For planar motion in the xy plane only lz is non-zero.
  • A bicycle wheel spun on a rod held at its two ends and then tilted makes the rod and the person on a turntable rotate: angular momentum is a vector and is conserved as a vector.
6.8Equilibrium of a rigid bodyΣF = 0 and Στ = 0; couples; levers; the centre of gravity

Conditions of equilibrium

  • Translational equilibrium: Σ F = 0. Rotational equilibrium: Σ τ = 0. Both must hold for mechanical equilibrium (a rigid body can be in one without the other).
  • For forces in a single plane these are three scalar conditions: Σ Fₓ = 0, Σ Fy = 0 and Σ τz = 0. When Σ F = 0 the total torque is the same about every point, so the point may be chosen for convenience.
  • A body is in partial equilibrium if only one of the two conditions holds.

Couple

  • A couple is a pair of equal and opposite forces that do not act along one line. The net force is zero, so the centre of mass does not accelerate, but the torque is not: τ = F d, where d is the perpendicular distance between the lines of action. It is the same about every point (Example 6.7).
  • Examples: turning a key in a lock, a tap, a steering wheel.
FFdnet force = 0turning effect only
A couple: two equal and opposite forces, not along one line. Net force 0, moment F d about any point.

Principle of moments and the centre of gravity

  • For a lever in equilibrium, F₁ d₁ = F₂ d₂: load arm × load = effort arm × effort. The ratio F₁/F₂ = d₂/d₁ is the mechanical advantage. A see-saw, a crowbar and a balance are examples.
  • The centre of gravity is the point about which the total gravitational torque is zero; it coincides with the centre of mass when g is uniform over the body. A uniform body can be balanced on a support under that point.
  • Example 6.8: a 70 cm bar of mass 4.00 kg rests on two knife-edges 10 cm from each end, with a 6.00 kg load at 30 cm. With g = 9.8 m s⁻², R₂ = (4 × 25 + 6 × 20) g/50 = 43 N and R₁ = 54.9 N (the book rounds to 55 N and 43 N).
  • Example 6.9: a 3 m, 20 kg ladder rests against a smooth wall with its foot 1 m from the wall. With g = 9.8 m s⁻²: N = W = 196 N, f = R = 34.6 N (from the moments about the foot) and the floor exerts a total force of about 199 N at about 80° to the horizontal.
smooth wallWNfRN = W and f = RMoments about the foot:R × height = W × (base/2)
Forces on a ladder against a smooth wall (the book's Example 6.9): the floor friction f balances the wall reaction R.
6.9Moment of inertiaI = Σ m r², K = ½ I ω², radius of gyration

Definition

  • For a body rotating about a fixed axis, each particle has speed v = ω r, so K = Σ ½ mᵢ vᵢ² = ½ (Σ mᵢ rᵢ²) ω². Define the moment of inertia I = Σ mᵢ rᵢ², where rᵢ is the perpendicular distance from the axis. Then K = ½ I ω².
  • I plays the role in rotation that mass plays in translation. Its SI unit is kg m² and its dimensions are [M L²]. It depends on the mass, its distribution and the axis, not on ω.
  • The radius of gyration k is defined by I = M k²: the distance at which the whole mass could be placed to give the same I. A flywheel has most of its mass at the rim (large I) so it resists changes in the angular speed of an engine.

Moments of inertia of common bodies (Table 6.1)

  • Thin ring, about its axis (perpendicular to its plane, through the centre): M R². Ring about a diameter: M R²/2.
  • Thin rod of length L, about a perpendicular axis through its midpoint: M L²/12.
  • Circular disc, about its axis: M R²/2. Disc about a diameter: M R²/4.
  • Hollow cylinder, about its axis: M R². Solid cylinder, about its axis: M R²/2. Solid sphere, about a diameter: 2 M R²/5.
  • Check: two masses M/2 at the ends of a light rod of length l, about its midpoint: I = 2 × (M/2)(l/2)² = M l²/4.
6.10–6.12Kinematics and dynamics of rotation about a fixed axisEquations of motion, τ = I α, L = I ω

Kinematics: the rotational equations

  • For a constant angular acceleration the equations of linear motion carry over: ω = ω₀ + α t, θ = θ₀ + ω₀ t + ½ α t², ω² = ω₀² + 2 α (θ − θ₀). Also v = ω r and the tangential acceleration is a = α r.
  • Example 6.11: a motor wheel speeds up from 1200 rpm to 3120 rpm in 16 s: α = (64π)/16 = 4π rad s⁻² and it makes 576 revolutions in that time.

Dynamics

  • Work by a torque: dW = τ dθ. Power: P = τ ω (compare P = F v).
  • Torque and angular acceleration: τ = I α (the rotational form of Newton's second law, for a fixed axis).
  • Table 6.2 (linear ↔ rotational): x ↔ θ, v ↔ ω, a ↔ α, m ↔ I, F ↔ τ, p ↔ L, F = m a ↔ τ = I α, K = ½ m v² ↔ K = ½ I ω², P = F v ↔ P = τ ω.
  • Example 6.12: a flywheel of mass 20 kg and radius 0.2 m with a steady pull of 25 N on a cord wound round it: τ = 5.0 N m, I = ½ M R² = 0.4 kg m², α = 12.5 rad s⁻². After 2 m of cord is unwound, the work done is 50 J and ω² = 250 rad² s⁻².

Angular momentum of a body rotating about a fixed axis

  • Lz = I ω (for a body symmetric about the axis; in general L is not parallel to ω). Then dLz/dt = τ.
  • Conservation: if the external torque about the axis is zero, I ω = constant. When I decreases, ω increases.
  • Examples: a skater or a diver pulling the arms and legs in to spin faster; a person on a swivel chair or a turntable holding weights; an acrobat's somersault. The rotational kinetic energy K = L²/2I increases when I falls, because the person does internal work.