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
uat an angle θ.
Step 1: Vertical Component of Velocity
The vertical component of velocity is given by:
u_y=usinθ
Step 2: At Maximum Height
At maximum height, the vertical velocity
v_yis 0. Using the first equation of motion:vy = uy - gt
Setting
v_y = 0leads 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:
Resolve velocity into components:
u_x = u imes ext{cos}( heta)
u_y = u imes ext{sin}( heta)
Treat horizontal and vertical motions separately.
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
vis linear velocity andωis angular velocity.
3. Acceleration Relation
Differentiating Again:
a = r imes ext{α}
Where
ais linear acceleration, andαis 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:
Convert degrees to radians (if needed).
Use the proper formulas:
s = r heta
v = r ext{ω}
a = r ext{α}
Apply sign conventions carefully.
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:
Use: au = I ext{α}.
Calculate I using the standard formulas.
Use the correct axis of rotation.
For maximum torque, maintain an angle of 90°.
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:
Use: L = I ext{ω} or L = mvr.
Identify whether the motion is circular.
Use the correct radius.
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.