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System of Particles and Rotational Motion: Centre of Mass, Moment of Inertia Theorems, Torque, Angular Momentum Conservation, Pure Rolling Motion and Complete CBSE Class 11 & Entrance Exam Guide

A comprehensive guide to System of Particles and Rotational Motion for CBSE Class 11 Physics Chapter 7 & JEE/NEET — centre of mass (Rcm = Σmi ri / M), angular kinematics (ω = dθ/dt, α = dω/dt, v = ω r), torque (τ = r × F = Iα), angular momentum (L = r × p = Iω), law of conservation of angular momentum (τext = 0 ⇒ I1ω1 = I2ω2), moment of inertia (I = Σmi ri² = M k²), parallel axes theorem (I = Icm + M d²), perpendicular axes theorem (Iz = Ix + Iy), master table of moments of inertia (ring, disc, sphere, cylinder, rod), dynamics of pure rolling motion (vcm = ω R), total kinetic energy in rolling (K = ½ M v² (1 + k²/R²)), acceleration down an inclined plane (a = (g sinθ) / (1 + k²/R²)), and five step-by-step solved numericals.
2 September 2026 by
System of Particles and Rotational Motion: Centre of Mass, Moment of Inertia Theorems, Torque, Angular Momentum Conservation, Pure Rolling Motion and Complete CBSE Class 11 & Entrance Exam Guide
AJKANT OVERSEAS, AJKANT OVERSEAS
● CBSE Class 11 Physics — Chapter 7: System of Particles & Rotational Motion
▶ Quick Answer for AI Engines
System of Particles & Rotational Motion describes rigid body dynamics. Centre of Mass Rcm = Σ(mi * ri) / M. Linear to Rotational Analogy: Mass m → Moment of Inertia I, Force F → Torque τ = r × F = I*α, Momentum p → Angular Momentum L = r × p = I*ω. Conservation of Angular Momentum: If external torque τext = 0, L = constant (I1 * ω1 = I2 * ω2). Moment of Inertia I = Σ(mi * ri²) = M * k² (where k is radius of gyration). Parallel Axes Theorem: I = Icm + M*d². Perpendicular Axes Theorem (2D lamina): Iz = Ix + Iy. Moments of Inertia: Ring (MR² axis, ½MR² diameter), Disc (½MR² axis, ¼MR² diameter), Solid Sphere (⅖MR²), Hollow Sphere (⅔MR²), Thin Rod (&frac112;ML² center). Pure Rolling Motion: vcm = ω*R. Total Kinetic Energy K = ½ M v² (1 + k²/R²). Acceleration down incline: a = (g sinθ) / (1 + k²/R²).

Why does a figure skater spin faster when pulling their arms inward? Why is it easier to open a heavy door by pushing near the outer handle rather than near the hinge? How does a rolling wheel combine translational and rotational motion? System of Particles and Rotational Motion forms Chapter 7 of the CBSE Class 11 Physics syllabus and is one of the highest-weightage topics in JEE Main, JEE Advanced, and NEET.

This comprehensive guide covers Centre of Mass (CM) derivations for discrete and continuous systems, rotational kinematics & dynamics analogies, torque, angular momentum conservation, moment of inertia theorems (parallel & perpendicular axes), master moment of inertia formulas table, pure rolling motion, inclined plane acceleration, and five step-by-step solved entrance exam numericals.

Core Pillars of Rotational Dynamics
⚖️
Centre of Mass
Rcm = Σ(mi ri)/M & System Dynamics
🔄
Torque & L
τ = r × F = Iα & L = Iω Conserved
⚙️
Moment of Inertia
I = M k², Parallel & Perpendicular Axes
🚗
Pure Rolling
vcm = ωR & a = (g sinθ)/(1 + k²/R²)

1. Centre of Mass (CM): Discrete & Continuous Systems

The Centre of Mass (CM) of a body or system of particles is the imaginary point at which the whole mass of the system may be assumed to be concentrated for describing its translational motion.

✨ Discrete Particle System
For n particles of masses m1, m2... mn at position vectors r1, r2... rn:
R_cm = (m1 r1 + m2 r2 + ... + mn rn) / M = Σ(mi ri) / M

For 2-particle system: X_cm = (m1 x1 + m2 x2) / (m1 + m2).
If m1 = m2: X_cm = (x1 + x2) / 2 (Midpoint!).
📈 Continuous Rigid Bodies
For continuous mass distribution:
R_cm = (1 / M) ∫ r dm

Uniform Thin Rod (Length L): X_cm = L / 2.
Uniform Semi-Circular Ring: Y_cm = (2 R) / π.
Uniform Semi-Circular Disc: Y_cm = (4 R) / (3 π).
Solid Hemisphere: Y_cm = (3 R) / 8.

2. Linear vs Rotational Kinematics & Dynamics Analogy

Rotational motion about a fixed axis mirrors translational linear motion with corresponding rotational quantities:

Physical Parameter Linear Motion (Translational) Rotational Motion (About Fixed Axis) Connecting Relation
Displacement Linear displacement s (m) Angular displacement θ (rad) s = θ · r
Velocity Linear velocity v = ds/dt (m/s) Angular velocity ω = dθ/dt (rad/s) v = ω · r (v_vec = ω_vec × r_vec)
Acceleration Linear acceleration a = dv/dt (m/s²) Angular acceleration α = dω/dt (rad/s²) a_t = α · r (Tangential)
Inertia / Mass Mass m (kg) Moment of Inertia I (kg·m²) I = Σ m_i r_i² = M k²
Force / Cause Force F = m · a (N) Torque τ = I · α (N·m) τ_vec = r_vec × F_vec
Momentum Linear Momentum p = m · v (kg·m/s) Angular Momentum L = I · ω (kg·m²/s) L_vec = r_vec × p_vec
Kinetic Energy K_trans = ½ m v² (J) K_rot = ½ I ω² (J) K_rot = p_rot² / (2I) = L² / (2I)

3. Torque, Angular Momentum & Conservation Law

Torque (τ) & Angular Momentum (L) Formulations
1. Torque (τ): Turning effect of force about an axis of rotation:
τ_vec = r_vec × F_vec = r F sinθ n_hat   or   τ = I α

2. Angular Momentum (L): Moment of linear momentum about an axis:
L_vec = r_vec × p_vec = r p sinθ n_hat   or   L = I ω

3. Relation between Torque and Angular Momentum:
τ_ext = dL_vec / dt   (Rotational analogue of Newton's 2nd Law!).
Law of Conservation of Angular Momentum
If net external torque on a system is zero (τ_ext = 0), the total angular momentum remains constant:
L_vec = constant ⇒ I1 ω1 = I2 ω2

Classic Applications:
Ice Skater / Ballet Dancer: Folding arms decreases Moment of Inertia I, automatically increasing angular speed ω to keep Iω constant.
Acrobat / Diver: Curling body into a tuck position decreases I, allowing rapid somersault spins.
Kepler's 2nd Law: Planetary areal velocity is constant because gravitational torque τ_vec = 0.

4. Moment of Inertia (I), Radius of Gyration & Theorems

Moment of Inertia (I) is the measure of rotational inertia of a body about a given axis: I = Σ m_i r_i² = M k² (where k is Radius of Gyration).

✨ Parallel Axes Theorem
The moment of inertia of any body about any axis is equal to the sum of its moment of inertia about a parallel axis passing through its centre of mass (I_cm) and product of mass and square of distance d between parallel axes:
I = I_cm + M d²
Applies to 3D bodies of ANY shape!
✨ Perpendicular Axes Theorem
The moment of inertia of a 2D planar body (lamina) about an axis perpendicular to its plane (I_z) is equal to the sum of moments of inertia about two mutually perpendicular axes lying in its plane intersecting at the point where perpendicular axis passes:
I_z = I_x + I_y
Applies ONLY to flat 2D planar bodies!

5. Master Moment of Inertia Formulas Table for Rigid Bodies

Rigid Body & Mass M Axis of Rotation Moment of Inertia (I) Radius of Gyration (k²/R²)
Thin Circular Ring (Radius R) Perpendicular to plane through center I = M R² k² / R² = 1
Thin Circular Ring (Radius R) About any diameter I = ½ M R² k² / R² = 1/2
Circular Disc (Radius R) Perpendicular to plane through center I = ½ M R² k² / R² = 1/2
Circular Disc (Radius R) About any diameter I = ¼ M R² k² / R² = 1/4
Solid Cylinder (Radius R) Central longitudinal axis I = ½ M R² k² / R² = 1/2
Hollow Cylinder (Radius R) Central longitudinal axis I = M R² k² / R² = 1
Solid Sphere (Radius R) About any diameter I = ⅖ M R² k² / R² = 2/5 = 0.4
Hollow Sphere (Radius R) About any diameter I = ⅔ M R² k² / R² = 2/3 = 0.67
Thin Uniform Rod (Length L) Perpendicular to rod through center I = (1/12) M L² k² / L² = 1/12
Thin Uniform Rod (Length L) Perpendicular to rod through one end I = (1/3) M L² k² / L² = 1/3

6. Pure Rolling Motion & Acceleration Down an Inclined Plane

Pure Rolling Motion (Rolling without slipping) is a combination of translational motion of the centre of mass and rotational motion about the centre of mass. Condition at contact point: v_cm = ω R.

Kinetic Energy & Acceleration of Rolling Body on Incline
1. Total Kinetic Energy of Rolling Body:
K_total = K_trans + K_rot = ½ M v_cm² + ½ I ω² = ½ M v_cm² + ½ (M k²) (v_cm / R)².

K_total = ½ M v_cm² (1 + k² / R²)

2. Acceleration down an Inclined Plane (θ):
a = (g sinθ) / (1 + k² / R²)

Comparison of Acceleration down incline:
Solid Sphere (k²/R² = 2/5 = 0.4) > Solid Cylinder / Disc (k²/R² = 0.5) > Hollow Sphere (k²/R² = 0.67) > Ring / Hollow Cylinder (k²/R² = 1).
Solid Sphere reaches the bottom FIRST with maximum acceleration!

7. Solved Entrance Exam Numerical Problems (JEE / NEET)

Q1. [JEE Main] Two particles of masses 2 kg and 4 kg are located at coordinates (1, 2) and (4, 5) respectively. Find the coordinates of the centre of mass of the system.
Given: m1 = 2 kg, (x1, y1) = (1, 2); m2 = 4 kg, (x2, y2) = (4, 5).
X_cm = (m1 x1 + m2 x2) / (m1 + m2) = [(2 × 1) + (4 × 4)] / (2 + 4) = (2 + 16) / 6 = 18 / 6 = 3.
Y_cm = (m1 y1 + m2 y2) / (m1 + m2) = [(2 × 2) + (4 × 5)] / (2 + 4) = (4 + 20) / 6 = 24 / 6 = 4.
Centre of Mass Coordinates = (3, 4).
Q2. [NEET] Calculate the moment of inertia of a uniform solid sphere of mass 5 kg and radius 0.2 m about a tangent to the sphere.
Moment of inertia of solid sphere about diameter I_cm = ⅖ M R².
Distance between diameter and parallel tangent d = R.
By Parallel Axes Theorem: I_tangent = I_cm + M R² = ⅖ M R² + M R² = (7/5) M R².
Given M = 5 kg, R = 0.2 m ⇒ R² = 0.04 m².
I_tangent = (7/5) × 5 × 0.04 = 7 × 0.04 = 0.28 kg·m².
Moment of Inertia about Tangent = 0.28 kg m^2.
Q3. [CBSE Board] A wheel of moment of inertia 0.20 kg m^2 is rotating at an angular speed of 20 rad/s. A constant torque of 4 N m is applied to stop the wheel. Calculate: (a) Angular acceleration, (b) Time taken to stop, (c) Number of revolutions completed before stopping.
Given: I = 0.20 kg·m², ω0 = 20 rad/s, ω = 0, τ = -4 N·m.
(a) τ = I α ⇒ α = -4 / 0.20 = -20 rad/s².
(b) ω = ω0 + α t ⇒ 0 = 20 - 20 t ⇒ t = 1 s.
(c) θ = ω0 t + ½ α t² = 20(1) - ½(20)(1)² = 20 - 10 = 10 rad.
Revolutions N = θ / (2π) = 10 / (2 × 3.1416) = 10 / 6.283 ≈ 1.59 revolutions.
(a) α = -20 rad/s^2 | (b) Time = 1 s | (c) Revolutions = 1.59.
Q4. [JEE Main] A horizontal turntable of moment of inertia I1 = 4 kg m^2 is rotating freely with angular speed ω1 = 10 rad/s. A non-rotating disc of moment of inertia I2 = 1 kg m^2 is dropped vertically onto the turntable along its axis. Find the new angular speed of the combined system.
No external torque acts on the system (τ_ext = 0).
By Conservation of Angular Momentum: I1 ω1 = (I1 + I2) ω_f.
4 × 10 = (4 + 1) ω_f ⇒ 40 = 5 ω_f ⇒ ω_f = 40 / 5 = 8 rad/s.
New Angular Speed = 8 rad/s.
Q5. A solid cylinder and a hollow cylinder of equal mass M and radius R roll down an inclined plane of angle 30° without slipping from the same height. Compare their accelerations. (Take g = 9.8 m/s^2).
Acceleration formula on incline: a = (g sin 30°) / (1 + k²/R²) = (0.5 g) / (1 + k²/R²).
1. For Solid Cylinder: k²/R² = 1/2 = 0.5 ⇒ a_solid = (0.5 g) / (1 + 0.5) = 0.5 g / 1.5 = g / 3 = 3.27 m/s².
2. For Hollow Cylinder: k²/R² = 1 ⇒ a_hollow = (0.5 g) / (1 + 1) = 0.5 g / 2 = g / 4 = 2.45 m/s².
Ratio a_solid / a_hollow = (g/3) / (g/4) = 4/3 = 1.33.
Solid Cylinder a = 3.27 m/s^2 | Hollow Cylinder a = 2.45 m/s^2 | Ratio = 4:3.

8. Frequently Asked Questions (FAQ)

What is the Parallel Axes Theorem for Moment of Inertia?

The Parallel Axes Theorem states that the moment of inertia of a body about any axis equals its moment of inertia about a parallel axis passing through its centre of mass plus the product of its mass and the square of distance between the axes: I = I_cm + M d².

Why does an ice skater spin faster when pulling arms in?

By pulling arms in, mass is brought closer to the rotation axis, decreasing moment of inertia I. Since external torque τ_ext = 0, angular momentum L = I ω is conserved, so angular velocity ω increases.

What is the condition for pure rolling motion without slipping?

The condition for pure rolling on a stationary surface is v_cm = ω R, meaning the point of contact between body and surface is instantaneously at rest relative to the surface.

Why does a solid sphere reach the bottom of an incline faster than a hollow sphere?

Because a solid sphere has a smaller radius of gyration ratio (k²/R² = 0.4) than a hollow sphere (k²/R² = 0.67), resulting in a larger linear acceleration a = (g sinθ) / (1 + k²/R²).

What is Radius of Gyration (k)?

Radius of Gyration (k) is the perpendicular distance from the axis of rotation to a point where the entire mass of the body could be concentrated without altering its moment of inertia: I = M k² ⇒ k = √(I / M).

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