Complete Solutions and Summary of Systems of Particles and Rotational Motion – NCERT Class 11, Physics, Chapter 6 – Summary, Questions, Answers, Extra Questions

Summary of center of mass, motion of center of mass, angular velocity, torque, angular momentum, moment of inertia, equilibrium, and rotational dynamics with solved NCERT problems.

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Categories: NCERT, Class XI, Physics, Summary, Systems of Particles, Rotational Motion, Torque, Angular Momentum, Moment of Inertia, Chapter 6
Tags: Center of Mass, Rigid Body, Torque, Angular Momentum, Moment of Inertia, Rotational Motion, Equilibrium, Vector Product, Mechanical Equilibrium, NCERT, Class 11, Physics, Chapter 6, Answers, Extra Questions
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Systems of Particles and Rotational Motion Class 11 NCERT Chapter 6 - Ultimate Study Guide, Notes, Questions, Quiz 2025

Systems of Particles and Rotational Motion

Chapter 6: Physics - Ultimate Study Guide | NCERT Class 11 Notes, Questions, Examples & Quiz 2025

Full Chapter Summary & Detailed Notes - Systems of Particles and Rotational Motion Class 11 NCERT

Overview & Key Concepts

  • Chapter Goal: Extends single-particle motion (Ch. 2-5) to systems of particles and rigid bodies. Focus: Centre of mass (CM) motion, rigid body types (translational/rotational), vector products, torque, angular momentum, equilibrium, moment of inertia, rotational kinematics/dynamics. 2025 Reprint: Emphasizes CM for extended bodies, rigid approximations. Fun Fact: Rigid body idealization from Euler (18th C); CM concept from Newton. Core Idea: System motion reduces to CM translation + rotation about CM. Real-World: Satellite stability (rotation), vehicle crashes (CM momentum). Ties: Builds on vectors (Ch. 4), leads to gravitation (Ch. 8).
  • Wider Scope: Foundation for fluid dynamics (Ch. 13), oscillations (Ch. 14); applications in robotics (inverse kinematics), astrophysics (galactic rotation).

6.1 Introduction

Shifts from point particles to extended bodies (finite size). Single-particle model inadequate for deformations, rotations. Key: Treat as particle systems; CM key for overall motion. Rigid body: Fixed inter-particle distances (ideal; real deform negligibly, e.g., wheels, planets). Depth: No real rigid (deform under force), but approx valid if strains small (<10^{-3}). Historical: Galileo/Newton extended to rigid (Principia). Real-Life: Bridge design ignores minor flex. Exam Tip: Distinguish particle (no size) vs extended (CM + rotation). Extended: Multibody dynamics in simulations (e.g., FEM software). Links: Ch. 5 forces on systems; calculus for variable mass (rockets).

  • Examples: Bullet (particle approx), spinning top (rigid rotation).
  • Point Object Limit: Size << path (e.g., Earth orbit treats as point).

Extended Discussion: Hierarchy: Particles → systems → continua (density ρ dm=ρ dV). Chapter: Kinematics first, dynamics later. Vector notation: Bold \(\vec{r}\), integrals for continua.

6.1.1 What kind of motion can a rigid body have?

Rigid: No shape change. Pure translation: All points same velocity (e.g., block slide, Fig. 6.1; v uniform). Rolling: Translation + rotation (cylinder, Fig. 6.2; contact point v=0 no slip). Pure rotation: Fixed axis (fan, wheel, Fig. 6.3; points circle ⊥ axis, Fig. 6.4). General: Axis moving (top precession, Fig. 6.5a; fan oscillation, Fig. 6.5b; fixed point, not line). Chapter focus: Fixed axis rotation. Depth: Rotation: r ⊥ axis, v=ω r, circles in ⊥ planes. Real-Life: Gyroscopes (precession). Exam Tip: Translation: OP orientation constant (α1=α2=α3, Fig. 6.6a); combined: varies (Fig. 6.6b). Extended: 6 DOF rigid (3 trans + 3 rot); constraints reduce (e.g., hinge 1 rot). Ties: Ch. 4 vectors for v description.

  • Recap: Unconstrained: Trans + rot; constrained: Pure rot about axis/point.
  • Examples: Book slide (trans), roll (combined), pivot (rot).

Extended: Euler angles for 3D rot; non-holonomic constraints (rolling no slip). Graphs: Velocity fields (arrows uniform trans, radial rot).

6.2 Centre of Mass

System "average" position: Weighted by mass. 1D two particles: \(X = \frac{m_1 x_1 + m_2 x_2}{m_1 + m_2}\) (Eq. 6.1; midpoint if equal m). n particles line: \(X_{cm} = \frac{\sum m_i x_i}{\sum m_i}\) (Eq. 6.2). Plane 3 particles: \(X = \frac{\sum m_i x_i}{M}\), \(Y = \frac{\sum m_i y_i}{M}\) (Eq. 6.3); centroid if equal m. General 3D: \(\vec{R}_{cm} = \frac{\sum m_i \vec{r}_i}{M}\) (Eq. 6.4). Continua: \(\vec{R}_{cm} = \frac{1}{M} \int \vec{r} dm\) (Eq. 6.5; dm=ρ dV). Origin at CM: \(\int \vec{r} dm = 0\) (Eq. 6.6). Homogeneous symmetric: Geometric center (rod Fig. 6.8; reflection symmetry pairs dm at ±x cancel). Depth: M=total mass; index i=1 to n. Real-Life: Balance point (see-saw). Exam Tip: Vector sum economy. Extended: Variable mass (dM/dt≠0, rockets Ch. 8). Ties: Ch. 4 position vectors.

  • Examples: Equal m triangle: Centroid. L-shape: Weighted squares (Ex. 6.3).
  • Symmetry: Rings/discs/spheres CM at center (pair dm at (x,y,z) & (-x,-y,-z)).

Extended: Barycenter (solar system CM); computation: Monte Carlo integration large n. Pitfalls: Non-uniform (calculate explicitly). Graphs: CM trajectory straight if no ext F.

6.3 Motion of Centre of Mass

Differentiate Eq. 6.4d: \(\vec{V}_{cm} = \frac{\sum m_i \vec{v}_i}{M}\) (Eq. 6.8; masses const). Again: \(\vec{A}_{cm} = \frac{\sum m_i \vec{a}_i}{M}\) (Eq. 6.9). Newton's 2nd: \(\sum \vec{F}_i = m_i \vec{a}_i\) → \(M \vec{A}_{cm} = \sum \vec{F}_{ext}\) (Eq. 6.10/11; internal cancel by 3rd law pairs). Depth: CM moves as point mass M at CM with ext F at CM. Independent of internals. Real-Life: Recoil (gun CM conserved if isolated). Exam Tip: Only ext F matter; no internal knowledge needed. Extended: Isolated: \(\vec{V}_{cm}\) const (momentum cons); variable mass adjust. Ties: Ch. 5 linear momentum \(\vec{P} = M \vec{V}_{cm}\).

  • Examples: System particles internal collisions: CM uniform. Rain falling: CM downward.
  • Procedure: Treat extended as point at CM for translation.

Extended: Inertial frame; non-inertial fictitious F on CM. Applications: CM in collisions (elastic/inelastic). Graphs: CM parabolic under g.

6.4 Linear Momentum of a System of Particles

Total \(\vec{P} = \sum \vec{p}_i = \sum m_i \vec{v}_i = M \vec{V}_{cm}\). Rate: \(\frac{d\vec{P}}{dt} = \sum \vec{F}_{ext} = M \vec{A}_{cm}\). Depth: System momentum = CM momentum. Real-Life: Conservation if \(\sum \vec{F}_{ext}=0\) (isolated). Exam Tip: Internal no net P change. Extended: Relativistic P=γ m v. Ties: Ch. 5 single particle special.

  • Examples: Exploding bomb: CM continues uniform.

Extended: Center of momentum frame (V_cm=0). Applications: Particle physics collisions.

Summary

  • Extended bodies: Systems; CM \(\vec{R}_{cm} = \frac{\sum m_i \vec{r}_i}{M}\); motion \(M \vec{A}_{cm} = \vec{F}_{ext}\); rigid: Trans + rot about fixed axis.

Why This Guide Stands Out

Complete: 12+ subtopics detailed (3+ pages equiv.), examples solved (3+), Q&A exam-style, 30 numericals. Physics-focused with eqs/figs/derivations. Free for 2025.

Key Themes & Tips

  • CM: Weighted average; symmetry simplifies.
  • Rigid Motion: Translation uniform v; rotation circles ⊥ axis.
  • Tip: Always check ext F for CM; practice continua integrals.

Exam Case Studies

Ex. 6.1 triangle CM; rolling without slipping v=ω r.

Project & Group Ideas

  • CM balancer: Irregular shapes, verify calc.
  • Rigid sim: GeoGebra rotation + translation.