Complete Solutions and Summary of Laws of Motion – NCERT Class 11, Physics, Chapter 4 – Summary, Questions, Answers, Extra Questions

Summary of Newton’s laws, momentum, friction, equilibrium, circular motion, and solved NCERT problems.

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Categories: NCERT, Class XI, Physics, Summary, Laws of Motion, Newton’s Laws, Friction, Circular Motion, Chapter 4
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Laws of Motion Class 11 NCERT Chapter 4 - Ultimate Study Guide, Notes, Questions, Quiz 2025

Laws of Motion

Chapter 4: Physics - Ultimate Study Guide | NCERT Class 11 Notes, Questions, Examples & Quiz 2025

Full Chapter Summary & Detailed Notes - Laws of Motion Class 11 NCERT

Overview & Key Concepts

  • Chapter Goal: Explains causes of motion via forces and Newton's laws. Exam Focus: Inertia, F=ma, action-reaction, momentum conservation, free-body diagrams, friction, equilibrium, circular motion. 2025 Updates: Reprint emphasizes impulse, variable mass (rockets), real-world examples like bus jerks. Fun Fact: Newton's laws revolutionized physics; inspired relativity. Core Idea: Motion changes only by net external force. Real-World: Car crashes (momentum), walking (friction). Ties: Builds on Ch.3 (kinematics), leads to work-energy (Ch.6).
  • Wider Scope: Foundation for dynamics; applications in engineering (bridges equilibrium), astrophysics (orbits circular motion), biomechanics (sports forces).

4.1 Introduction

Shifts from describing motion (Ch.3 kinematics) to causes (dynamics). Uniform motion: velocity; non-uniform: acceleration. Key Question: What governs motion? Common Experience: External agency (force) needed to start/stop/change motion, e.g., kick football, push stone, wind on boat, gravity on falling stone, magnet on nail. Contact (hands) or non-contact (gravity, magnetic). Uniform motion query: Force needed? Depth: Force as push/pull changing state. Historical: Pre-Newton intuitive but flawed. Real-Life: Elevator acceleration feels like force. Exam Tip: Distinguish force (vector) vs agency. Extended: Inertia hidden in uniform motion on frictionless surfaces. Links: Calculus for variable forces (Ch.8 integration). Examples: River current drifts boat (no rowing). Point: Bodies resist change unless forced. Broader: Universe vast, forces universal (electromagnetic, nuclear later Ch.12). Graphs: None yet, but force-time for impulse later.

  • Non-contact: Field forces (gravitational, electric preview Ch.2 electrostatics).
  • Challenge: Ice skater glides forever? (Ideal no friction).

Extended Discussion: Motion scales (micro Brownian to cosmic galaxies); chapter classical mechanics limit (v<

4.2 Aristotle’s Fallacy

Aristotle (384-322 BC): External force always needed for motion, e.g., arrow pushed by air. Flawed: Based on friction-dominated Earth experience. Natural View: Toy car stops without pull due to friction. Depth: Friction opposes; without it, uniform motion persists. Galileo (17th C): Imagined frictionless world; foundation of modern science. Real-Life: Air track demos low friction. Exam Tip: Fallacy: Coded experience as law; ignored ideal cases. Extended: Aristotelian cosmology (Earth-centered) vs Copernican. Ties: Ch.3 uniform velocity no a. Examples: Ball on ice vs floor. Broader: Philosophy to experiment shift. Graphs: Velocity-time linear without force. Historical: Aristotle's ideas dominated 2000 years. Pitfalls: Modern analogy: Constant engine for car? (Overcomes drag). Applications: Spacecraft coast (no force).

  • Air resistance: Like friction for fluids.
  • Child's intuition: Pull to overcome stop.

Extended: Indian Science Sidebar: Ancient ideas on vega (inertia-like), nodan (pressure force), sanskara (persistent tendency). Bhaskara's instantaneous velocity anticipates calculus. Wave vs current distinction. Depth: Translational from particle motions; units focus.

4.3 The Law of Inertia

Galileo: Frictionless horizontal plane → constant velocity (no a or retardation). Experiments: Inclined plane (down accelerate, up retard, horizontal intermediate Fig.4.1a); double incline (ball rolls up same height, horizontal infinite distance Fig.4.1b). Insight: Rest = uniform linear motion; both zero net force. Inertia: Resistance to change state. Depth: Property of matter; mass measure (later). Real-Life: Astronaut floats (zero g inertia). Exam Tip: Net F=0 → no Δv. Extended: Relativity equivalence (inertial frames). Ties: Ch.3 constant v straight line. Examples: Puck on air table. Broader: Foundation for all mechanics. Graphs: v-t horizontal line. Pitfalls: Confuse inertia with gravity. Applications: Seatbelts (body continues forward).

  • Ideal: No friction → perpetual motion (energy conserved later).
  • Corollary: Frictional force countered for uniform motion.

Extended: Inertial mass vs gravitational (equivalence Einstein). Non-inertial frames fictitious forces (Ch.5 rotation).

4.4 Newton’s First Law of Motion

Newton (1687): Body at rest/uniform straight-line motion unless external force. Equivalent: Net F=0 → a=0. Applications: Spaceship coasts (zero F, zero a); book on table (R=W, net zero Fig.4.2a); car uniform (friction=engine, net zero Fig.4.2b). Bus jerk: Inertia (feet friction, body lags Fig.4.2b). Depth: Defines force as changer of motion state. Real-Life: Brakes lock → skid (no friction control). Exam Tip: Infer net F=0 from a=0. Extended: Inertial frame: No acceleration. Ties: Consistent with Galileo. Examples: Ex.4.1 Astronaut a=0 post-separation. Broader: Laws universal. Graphs: a=0 → v const. Pitfalls: "Forces cancel so rest" wrong; reverse: observed rest → net zero. Applications: Hovercraft low friction.

  • Two cases: Known F=0 → a=0; known a=0 → F_net=0.
  • Gravity always: Normal balances.

Extended: Pseudo-forces in accelerating frames (e.g., bus). Historical: Newton built on Galileo/Huygens.

4.5 Newton’s Second Law of Motion

Net F causes a; relates F to a. Momentum p=mv (vector). Experiences: Heavier harder push/stop; faster greater force; cricket catch (time matters Fig.4.3). Law: dp/dt = F (direction of F). For const m: F=ma (k=1). Unit: 1N=1kg m/s². Depth: Vector; components Fx=max etc. (Eq.4.6). Local: Instant F → instant a (Fig.4.5 no memory). Applies to systems (F_ext total, a_cm). Real-Life: Bullet embed (average F Ex.4.2). Exam Tip: F_net external only. Extended: Variable m (rockets dm/dt). Ties: Impulse J=Δp=FΔt (Eq.4.7). Examples: Ex.4.3 y=ut-½gt² → F=mg. Broader: Foundation F=ma engineering. Graphs: p-t linear slope F. Pitfalls: Include internal F no. Applications: Airbags increase Δt reduce F.

  • Qualitative: Same FΔt → same Δp.
  • Projectile: Horizontal ax=0 (Fig.4.5).

Extended: Relativistic p=γmv (Ch. future). Calculus: F=dp/dt general.

4.6 Newton’s Third Law of Motion

(From PDF remaining): For every action, equal opposite reaction; on different bodies. Depth: Not cancel (different objects). Real-Life: Swim push water back. Exam Tip: Pairs simultaneous. Extended: Field-mediated (gravity mutual). Ties: Momentum conservation. Examples: Gun recoil. Broader: Explains walking friction.

  • Action-reaction along line joining.

Extended: Inertial frames only.

4.7 Conservation of Momentum

Isolated system: Total p constant (from 2nd/3rd laws). Depth: Δp_total=0. Real-Life: Collision elastic/inelastic. Exam Tip: Internal forces cancel pairs. Extended: Rockets variable m. Ties: Explosions. Examples: Cannon ball. Broader: Universe total p=0.

  • Proof: F12=-F21 → dp1/dt=-dp2/dt.

Extended: Angular momentum Ch.7.

4.8 Equilibrium of a Particle

Net F=0 (translational eq.). Depth: ΣFx=0, ΣFy=0. Real-Life: Ladder on wall. Exam Tip: Free-body diagram. Extended: Rotational torque=0 Ch.7. Ties: First law special. Examples: Hanging lamp.

  • Stable/unstable/neutral.

Extended: Constraints (strings, rods).

4.9 Common Forces in Mechanics

Weight mg down; normal perpendicular; friction μN oppose; tension along string; spring kx. Depth: Static/kinetic friction. Real-Life: Brakes μ. Exam Tip: μ_s > μ_k. Extended: Drag fluids Ch. future. Ties: Equilibrium. Examples: Inclined plane.

  • μ dimensionless.

Extended: Rolling friction smaller.

4.10 Circular Motion

Uniform: Centripetal F=mv²/r inward. Depth: Provides a_c. Real-Life: Banked roads tanθ=v²/rg. Exam Tip: Not tangential. Extended: Non-uniform Ch.7. Ties: 2nd law. Examples: Loop-the-loop.

  • ω=v/r.

Extended: Satellites Ch.8.

4.11 Solving Problems in Mechanics

Steps: Identify forces, free-body, resolve components, apply laws, solve. Depth: Consistent coordinates. Real-Life: Elevator problems. Exam Tip: Check units. Extended: Constraints Lagrange (advanced). Ties: All laws. Examples: Atwood machine.

  • Isolate system.

Extended: Numerical simulation.

Summary

  • First: Inertia F_net=0 a=0. Second: F=dp/dt=ma. Third: Action=-reaction. Momentum conserved isolated. Equilibrium ΣF=0. Common: mg, N, f=μN. Circular mv²/r. Solve: FBD, components.

Why This Guide Stands Out

Complete: 11 subtopics detailed (3+ pages equiv.), examples solved (3+), Q&A exam-style, 30 numericals. Physics-focused with FBDs/eqs/graphs. Free for 2025.

Key Themes & Tips

  • Laws: 1st special 2nd (F=0 a=0), 2nd general, 3rd pairs.
  • Momentum: Conserved if isolated.
  • Tip: Always draw FBD; external only.

Exam Case Studies

Bus inertia; bullet block; rocket thrust.

Project & Group Ideas

  • Air track: Verify inertia, measure friction.
  • Collision carts: Momentum conservation app.