4.1.1 Explain Projectile Motion (CRQ – 3 Marks)

  • Definition: Projectile motion is the motion of a body thrown at an angle θ with an initial velocity under the effect of gravity only.

    • The object follows a curved (parabolic) path.

    • Only gravitational force (g) acts downward.

    • Motion occurs in two dimensions (x and y).

4.1.2 (a) Derive Time of Flight (ERQ – 5 Marks)

  • Initial Setup: Consider a projectile thrown with an initial velocity u at an angle θ.

Step 1: Vertical Component of Velocity

  • The vertical component of velocity is given by:

    • u_y=usin⁡θ

Step 2: At Maximum Height

  • At maximum height, the vertical velocity v_y is 0. Using the first equation of motion:

    • vy = uy - gt

  • Setting v_y = 0 leads to:

    • 0 = u imes ext{sin}( heta) - gt

    • Rearranging gives:
      t = rac{u imes ext{sin}( heta)}{g}

    • This is the time to reach maximum height.

Step 3: Total Time of Flight

  • Since the motion is symmetric:

    • T = 2t

    • T = 2 imes rac{u imes ext{sin}( heta)}{g}

4.1.2 (b) Derive Maximum Height (ERQ – 5 Marks)

  • At Maximum Height: Again, compressing the understanding:

    • v_y = 0

  • Using the third equation of motion we have:

    • v^2y = u^2y - 2gH

    • Substituting gives:

    • 0 = (u imes ext{sin}( heta))^2 - 2gH

    • Rearranging leads to:

    • 2gH = u^2 imes ext{sin}^2( heta)

    • Hence,

    • H = rac{u^2 imes ext{sin}^2( heta)}{2g}

4.1.2 (c) Derive Horizontal Range (ERQ – 5 Marks)

  • Step 1: Horizontal Motion

    • Since there is no acceleration in the horizontal direction:

    • R = u_x imes T

  • The horizontal component of velocity is:

    • u_x = u imes ext{cos}( heta)

  • Thus, total time of flight is:

    • T = rac{2u imes ext{sin}( heta)}{g}

Step 2: Substitute

  • Substitute values into range equation:

    • R = (u imes ext{cos}( heta)) imes rac{2u imes ext{sin}( heta)}{g}

    • Simplifying gives:

    • R = rac{2u^2 imes ext{sin}( heta) imes ext{cos}( heta)}{g}

  • Using identity $2 imes ext{sin}( heta) imes ext{cos}( heta) = ext{sin}(2 heta)$ gives:

    • R = rac{u^2 imes ext{sin}(2 heta)}{g}

4.1.2 (d) Maximum Horizontal Range (CRQ – 3 Marks)

  • Range Formula:

    • R = rac{u^2 imes ext{sin}(2 heta)}{g}

  • The maximum value of $ ext{sin}(2 heta)$ is 1. Thus,

    • ext{sin}(2 heta) = 1

    • Hence:

    • 2 heta = 90

    • heta = 45

  • Maximum Range:

    • R_{ ext{max}} = rac{u^2}{g}

4.1.3 Solve Word Problems (Concept) (CRQ – 3 Marks)

  • Steps to solve projectile problems:

    1. Resolve velocity into components:

    • u_x = u imes ext{cos}( heta)

    • u_y = u imes ext{sin}( heta)

    1. Treat horizontal and vertical motions separately.

    2. Use the equations of motion for vertical and horizontal paths:

    • Vertical motion: $s = vt$

    • Horizontal motion: Apply the motion equations.

4.1.4 Effect of Air Resistance (CRQ – 3 Marks)

  • With Air Resistance:

    • Velocity decreases (air opposes motion).

    • Maximum height decreases.

    • Range decreases.

    • Time of flight increases.

    • Path is no longer a perfect parabola.

4.2.1 Describe Angular Displacement, Angular Velocity & Angular Acceleration (CRQ – 3 Marks)

Angular Displacement (θ)

  • Definition: Angular displacement is the angle covered by an object during rotation.

    • Measurement Units:

    • Radians (rad) - SI unit.

    • Degrees (°) and revolution (rev).

    • Defined as the angle subtended at the center of a circle.

Angular Velocity (ω)

  • Definition: Angular velocity is the rate of change of angular displacement.

  • Formula:

    • ext{ω} = rac{ ext{Δθ}}{ ext{Δt}}

  • SI Unit: rad/s.

Angular Acceleration (α)

  • Definition: Angular acceleration is the rate of change of angular velocity.

  • Formula:

    • ext{α} = rac{ ext{Δω}}{ ext{Δt}}

  • SI Unit: rad/s².

4.2.2 Derive Relationship Between Linear & Angular Quantities (ERQ – 5 Marks)

  • Consider a Particle Moving in a Circular Path of Radius r:

1. Displacement Relation

  • Arc length (linear displacement):

    • s = r heta

    • Thus, linear displacement depends on the radius (r) and angular displacement (θ).

2. Velocity Relation

  • Differentiating with Respect to Time:

    • v = r imes ext{ω}

    • Where v is linear velocity and ω is angular velocity.

3. Acceleration Relation

  • Differentiating Again:

    • a = r imes ext{α}

    • Where a is linear acceleration, and α is angular acceleration.

  • Final Important Relations:

    • s = r heta

    • v = r ext{ω}

    • a = r ext{α}

  • Conclusion: These show the connection between linear and rotational motion.

4.2.3 Solve Word Problems Related to Rotational Motion (CRQ – 3 Marks)

  • To Solve Rotational Motion Problems:

    1. Convert degrees to radians (if needed).

    2. Use the proper formulas:

    • s = r heta

    • v = r ext{ω}

    • a = r ext{α}

    1. Apply sign conventions carefully.

    2. For small time intervals, use instantaneous values.

4.3 Centripetal Force & Centripetal Acceleration

4.3.1 Define Centripetal Force & Centripetal Acceleration (CRQ – 3 Marks)

Centripetal Force
  • Definition: Centripetal force is the force that bends the straight path of a body into a circular path.

    • It is not a separate force; it can be tension, friction, gravity, etc.

    • Direction: Towards the center of the circular path.

  • Formula:

    • F_c = rac{mv^2}{r}

Centripetal Acceleration
  • Definition: Centripetal acceleration is the acceleration produced due to the change in direction of velocity in circular motion.

    • Exists even if speed is constant.

    • Direction: Always directed towards the center.

  • Formula:

    • a_c = rac{v^2}{r}.

4.3.2 Derive Centripetal Acceleration (Uniform Speed) (ERQ – 5 Marks)

  • Consider a body moving in a circle with constant speed:

Step 1: Important Concept
  • Velocity is a vector quantity. Even if speed is constant, the direction keeps changing; therefore, acceleration exists.

Step 2: Similar Triangle Concept
  • From the geometry of velocity vectors:

    • rac{ ext{Δv}}{v} = rac{ ext{Δs}}{r}

  • But, ext{Δs} = v ext{Δt}

  • Therefore:

    • ext{Δv} = rac{v^2 ext{Δt}}{r}

Step 3: Acceleration
  • a = rac{ ext{Δv}}{ ext{Δt}}

  • Substituting gives:

    • a = rac{v^2}{r}

  • Final Result:

    • a_c = rac{v^2}{r}

  • Direction: Towards center (inward).

4.3.3 Justify That Centrifuge Separates Materials (CRQ – 3 Marks)

  • A centrifuge rotates at high speed, producing large centripetal acceleration.

  • Effect on Particles:

    • Heavier particles experience a greater outward effect.

    • Denser particles move outward faster than lighter ones.

  • Conclusion: Therefore, materials are separated based on density.

4.3.4 Explain Why Objects in Orbiting Satellites Appear Weightless (CRQ – 3 Marks)

  • Weightlessness: Does not mean gravity is zero.

  • A satellite and astronauts are in continuous free fall.

  • Both fall with the same acceleration (g).

  • Observation: No normal reaction force acts on them.

  • Conclusion: Therefore, felt weight becomes zero, hence astronauts appear weightless.

4.3.5 Artificial Gravity to Counter Weightlessness (ERQ – 5 Marks)

  • Weightlessness Challenges: Creates difficulties in space.

  • Solution: Rotating Space Station

    • When the station rotates:

    • A person moves in a circular path.

    • Centripetal acceleration acts toward the center.

    • An outward centrifugal effect is felt.

  • To Create Artificial Gravity:

    • Using the relationship:

    • rac{v^2}{r} = g

  • Substituting:

    • v = r ext{ω}

  • Thus,

    • r ext{ω}^2 = g

  • Conclusion: This produces artificial gravity equal to Earth’s gravity. Therefore, rotation can simulate gravity in space.

4.4.1 Explain Moment of Inertia with SI Unit & Dimension (CRQ – 3 Marks)

Definition

  • Moment of inertia refers to the resistance of a body to rotational motion.

  • It is also known as rotational inertia.

  • In linear motion, inertia depends on mass (m). In rotational motion, inertia depends on moment of inertia (I).

Formula (Single Particle)

  • I = mr^2

  • Where:

    • $m$ = mass

    • $r$ = distance from axis of rotation.

  • It depends on:

    • Mass.

    • Distribution of mass from axis.

  • SI Unit: kg imes m^2.

  • Dimensional Formula:

    • [ML^2].

4.4.2 Compare Moment of Inertia of Rod, Ring, Disc & Sphere (CRQ – 3 Marks)

Object

Moment of Inertia (I)

Rod (about center)

I = rac{1}{12} MR^2

Ring / Hoop

I = MR^2

Solid Disc

I = rac{1}{2} MR^2

Solid Sphere

I = rac{2}{5} MR^2

  • Comparison:

    • Smallest Moment of Inertia: Rod.

    • Largest Moment of Inertia: Ring.

    • Reason:

    • Ring has all mass farthest from the axis, hence having maximum moment of inertia.

4.4.3 Derive Relationship Between Torque, Moment of Inertia & Angular Acceleration (ERQ – 5 Marks)

Step 1: Torque Definition

  • Torque is the turning effect of force, defined as:

    • au = rF ext{sin}( heta)

  • For maximum torque (when θ = 90°):

    • au = rF.

Step 2: Newton’s Second Law (Linear Form)

  • F = ma.

Step 3: Substitute in Torque Equation

  • $ au = r(ma)

  • Where:

    • a = r ext{α}

  • Thus:

    • au = r(mr ext{α}).

Step 4: Since I = mr²

  • Therefore, au = I ext{α}.

  • Final Result:

    • Torque = Moment of inertia × Angular acceleration.

    • This is Newton’s second law in rotational motion.

4.4.4 Solve Word Problems Related to These Relations (CRQ – 3 Marks)

  • To Solve Rotational Problems:

    1. Use: au = I ext{α}.

    2. Calculate I using the standard formulas.

    3. Use the correct axis of rotation.

    4. For maximum torque, maintain an angle of 90°.

    5. Check units to be consistent (kg·m²).

4.5 Angular Momentum

4.5.1 Explain Angular Momentum with SI Unit & Dimension (CRQ – 3 Marks)

Definition
  • Angular momentum (L) is the quantity of rotational motion contained in a body, representing the rotational version of linear momentum.

  • Formula:

    • L = I ext{ω}

    • Alternatively:

    • L = mvr

  • Dependencies:

    • Mass.

    • Velocity.

    • Distance from the axis.

  • SI Unit: kg imes m^2/s.

  • Dimensional Formula:

    • [ML^2T^{-1}].

4.5.2 Solve Word Problems Related to Angular Momentum (CRQ – 3 Marks)

  • To Solve Angular Momentum Problems:

    1. Use: L = I ext{ω} or L = mvr.

    2. Identify whether the motion is circular.

    3. Use the correct radius.

    4. Apply conservation law if no external torque is present.

4.5.3 Explain Law of Conservation of Angular Momentum (ERQ – 5 Marks)

Statement:
  • If no external torque acts on a system, the total angular momentum remains constant.

Condition:
  • τ_{ ext{ext}} = 0

  • Mathematical Form:

    • L = I ext{ω}

    • If no external torque acts:

    • I1 ext{ω}1 = I2 ext{ω}2

  • Important Concept:

    • If moment of inertia decreases, angular velocity increases.

    • If moment of inertia increases, angular velocity decreases.

    • The product remains constant.

4.5.4 Applications of Conservation of Angular Momentum (ERQ – 5 Marks)

(a) Flywheel
  • Function: Stores rotational energy.

  • Characteristics:

    • Large moment of inertia.

    • Maintains steady angular velocity.

  • Advantages: Used to store rotational energy efficiently.

(b) Gyroscope (Navigation System)
  • Application: Utilizes conservation of angular momentum.

  • Key Feature: A spinning wheel resists changes in orientation.

  • Use: Helps in aircraft and ship navigation.

(c) Ice Skater
  • Effect: When a skater:

    • Arms out → I large, ext{ω} small.

    • Arms closed → I small, ext{ω} increases.

  • Conclusion: Since I ext{ω} = ext{constant}, the skater spins faster when arms are pulled inward.