⚡ Physics · Class 11 · Chapter 4

Laws of Motion

Newton's 3 Laws · Inertia · Momentum · Work-Energy · Collisions — fully animated

1 / 12

🏛️ Introduction & Aristotle's Fallacy

Mechanics deals with motion. It has two branches:

Kinematics

Describes motion without discussing its cause. Parameters: distance, velocity, acceleration.

Dynamics

Describes motion WITH its cause — force and torque. Parameters: momentum, force, energy.

❌

Aristotle's Fallacy (384BC)

Stated that "an external force is required to keep a body in uniform motion." He was WRONG.

✓

Galileo's Correction

Objects stop because of opposing forces — friction, air resistance, viscous drag. Without these, motion continues forever!

Correct PrincipleMotion continues on its own. A force is needed only to START, STOP or CHANGE motion — not to maintain it.
2 / 12

⚖️ Newton's Three Laws of Motion

🟢 First Law — Law of Inertia

Every object continues to be in its state of rest OR uniform unaccelerated motion unless acted upon by an external, unbalanced force.

ΣF = 0 → velocity = constant (may be zero)

🟡 Second Law — Law of Force

Rate of change of linear momentum is directly proportional to applied force and in the direction of force.

F⃗ = dp⃗/dt = ma⃗ (for constant mass)

🔴 Third Law — Action & Reaction

To every action force, there is an equal and opposite reaction force. They act on DIFFERENT objects and NEVER cancel each other.

F⃗_AB = −F⃗_BA
3 / 12

💡 Importance of Newton's Laws

1st

Defines Inertia

Inertia is the fundamental property of every object to resist change in its state of motion. Inertia is measured by mass. More mass = more inertia.

2nd

Defines Force Correctly

F = dp/dt — NOT F = ma. F = ma is only valid when mass is constant. For rockets, both mass AND velocity change, so we need the full form.

3rd

Forces Need Not Be Contact Forces

Gravitational force between Earth and Moon is a non-contact action-reaction pair. Magnetic repulsion between two magnets is also a non-contact pair.

Critical Point — 2nd LawF⃗ = dp⃗/dt = d(mv⃗)/dt = m·(dv⃗/dt) + v⃗·(dm/dt)
For constant mass: dm/dt = 0, so F⃗ = ma⃗
4 / 12

🚗 Inertia — Animated Demonstration

Watch what happens when the car suddenly brakes. The passenger keeps moving forward — that is Newton's First Law / Inertia in action!

  • Passenger's body wants to stay in motion when car stops — inertia
  • Seatbelt provides the external force to stop the passenger
  • Heavier passenger = more inertia = needs more force to stop
  • Same principle — coins on a card flicked from a stack
5 / 12

🔄 Inertial & Non-Inertial Frames of Reference

✅ Inertial Frame

A frame where Newton's First Law holds. No net force → no acceleration. Body moves with constant velocity.

Example: train moving at constant velocity

⚠️ Non-Inertial Frame

Accelerating frame. Objects appear to accelerate even with no real force — need to add pseudo force −ma⃗.

Example: accelerating or braking bus
💡

Pseudo Force (−ma⃗)

In a non-inertial frame of acceleration a⃗, we add a pseudo force of −ma⃗ to all objects to apply Newton's laws. It is measurable but not a fundamental force.

Lift Example — Apparent WeightLift going up (accel a): W = m(g + a) → feel heavier
Lift going down (accel a): W = m(g − a) → feel lighter
Free fall (a = g): W = 0 → weightlessness!
6 / 12

🌌 Four Fundamental Forces in Nature

ForceStrengthRangeExamples
GravitationalWeakestInfiniteWeight, planetary orbits
ElectromagneticStrongInfiniteFriction, normal force, tension
Strong NuclearStrongest< 10⁻¹⁴ mBinds nucleons in nucleus
Weak NuclearWeak< 10⁻¹⁶ mRadioactive beta decay
Key FactFriction, normal reaction, tension, elastic force — all are EM in nature arising from deformation of molecular bonds
7 / 12

🎯 Conservation of Linear Momentum

From Newton's 2nd law: F⃗ = dp⃗/dt. If net external force = 0, then dp⃗/dt = 0, which means momentum is constant!

🌟 Principle of Conservation of Linear MomentumThe total momentum of an isolated system is conserved during any interaction (collision or explosion)
  • Isolated system = no external force acting on the system
  • During collision — internal forces change individual momenta but total remains same
  • Rocket propulsion — gas expelled backward, rocket moves forward
  • Recoil of gun — bullet goes forward, gun recoils backward
8 / 12

⚡ Work-Energy Theorem

Work done by a force equals the change in kinetic energy of the object.

W

Work Done by Constant Force

W = F⃗ · s⃗ = F·s·cosθ. For variable force: W = ∫F·ds (area under F-s graph)

KE

Work-Energy Theorem

Work done by net force = Change in KE = ½mv² − ½mu²

PE

Conservative Forces

Work done is independent of path — depends only on start and end points. Gravitational force, spring force are conservative. dU = −F·dx

NC

Non-Conservative Forces

Friction, air drag — work done is path-dependent. Energy appears as heat/sound and is NOT recoverable.

Work-Energy for Non-Conservative ForceΔPE = ΔKE + W_friction    (mechanical energy is NOT conserved)
9 / 12

💥 Elastic vs Inelastic Collisions

During ALL collisions, linear momentum is conserved. But kinetic energy may or may not be conserved.

✅ Elastic Collision

Both momentum AND kinetic energy are conserved. Coefficient of restitution e = 1.

KE_initial = KE_final

⚠️ Inelastic Collision

Momentum conserved but KE is lost. Perfectly inelastic: objects stick together. e = 0.

KE_initial > KE_final
Coefficient of Restitution ee = relative speed of separation / relative speed of approach
Elastic: e=1  |  Perfectly Inelastic: e=0  |  All others: 0 < e < 1
10 / 12

📐 Head-On Elastic Collision — Final Velocities

For masses m₁ and m₂ with initial velocities u₁ and u₂ in a head-on elastic collision:

🌟 Final Velocity Formulas v₁ = [(m₁−m₂)/(m₁+m₂)]u₁ + [2m₂/(m₁+m₂)]u₂

v₂ = [(m₂−m₁)/(m₁+m₂)]u₂ + [2m₁/(m₁+m₂)]u₁
Case 1

Equal masses (m₁ = m₂)

v₁ = u₂ and v₂ = u₁ — the bodies simply exchange their velocities. Ball A stops, ball B moves with A's original speed.

Case 2

Heavy hits stationary light (m₁ >> m₂, u₂=0)

v₁ ≈ u₁ (heavy barely slows), v₂ ≈ 2u₁ (light moves at double the heavy body's speed).

Case 3

Light hits stationary heavy (m₁ << m₂, u₂=0)

v₁ ≈ −u₁ (light rebounds with same speed), v₂ ≈ 0 (heavy barely moves). Like a ball bouncing off a wall.

11 / 12

🎱 Animated Collision — Equal Mass Exchange

Watch elastic collision between equal masses. Ball A hits stationary Ball B — A stops completely, B moves with A's original velocity. Velocities are exchanged!

Newton's Cradle — Same PrincipleWhen 1 ball swings and hits 4 stationary balls, exactly 1 ball flies out from the other side — momentum AND energy conserved together
  • Before: p = m·u + m·0 = mu → After: p = m·0 + m·u = mu ✓
  • Before: KE = ½mu² + 0 → After: KE = 0 + ½mu² ✓
12 / 12

🏁 Complete Chapter Summary

❌

Aristotle was WRONG

Force is NOT needed to maintain motion. Objects stop due to friction and resistance — not because motion "runs out".

1st

Newton's 1st Law — Inertia

No external force → no change in motion. Inertia ∝ mass. Both rest and uniform motion are "states of motion".

2nd

Newton's 2nd Law — F = dp/dt

Force = rate of change of momentum. For constant mass: F = ma. For rockets: use full dp/dt form.

3rd

Newton's 3rd Law — Action = Reaction

Forces come in pairs on DIFFERENT objects. They are equal and opposite. They do NOT cancel each other.

p

Conservation of Momentum

Total momentum of isolated system = constant. Used for all collision and explosion problems.

e

Collisions

Elastic (e=1): both p and KE conserved. Perfectly Inelastic (e=0): only p conserved, objects stick. 0<e<1: partially inelastic.

🎉 All Lessons →
← Motion in a Plane All Lessons →
Laws of Motion
Auto-narration active