circular motion lec1

Introduction to Circular Motion and Basic Kinematics Review

  • Concept of Circular Motion: Circular motion occurs when a body moves in a circular path or a "dayera."

  • Review of Linear Quantities:

    • Distance: The total path covered by a body.

    • Displacement: The straight-line distance from the initial to the final point.

    • Velocity: Displacement per unit time (v=dtv = \frac{d}{t}).

    • Acceleration: The rate of change of velocity (a=Δvta = \frac{\Delta v}{t}).

  • Transition to Angular Quantities: In circular motion, we analyze angular counterparts to linear quantities:

    • Linear Displacement ss → Angular Displacement θ\theta

    • Linear Velocity vv → Angular Velocity ω\omega

    • Linear Acceleration aa → Angular Acceleration α\alpha

Angular Displacement and Arc Length

  • Definition: Angular displacement (θ\theta) is the angle subtended at the center of the circular path during circular motion.

  • Position Vector (r\mathbf{r}):

    • It defines the location or address of a point relative to the origin.

    • In circular motion, the magnitude of the position vector is the radius (rr).

    • Example: A vector 5i5i meters means a point located 5 meters along the positive x-axis from the origin.

    • Standard unit vectors are ii (x-axis), jj (y-axis), and kk (z-axis).

  • Arc Length (ss):

    • The distance covered along the circumference (boundary) of the circle.

    • Relationship: s=rθs = r\theta.

    • In this formula, θ\theta must be in radians.

  • Vector Nature of θ\theta:

    • Angular displacement is considered a vector quantity only for very small values (infinitesimal values).

    • This is shown using the limit notation: limΔt0\lim_{\Delta t \to 0}.

    • Small arc lengths approximate a straight line, satisfying the vector definition of linear displacement, which makes associated angular displacement a vector.

Units and Conversions

  • Common Unit: Degree (^{\circ}).

  • Standard (SI) Unit: Radian (rad).

  • Total Cycle Relations:

    • One complete revolution (~360 degrees) is equal to 2π2\pi radians.

    • 2πrad=3602\pi \, \text{rad} = 360^{\circ}

    • πrad=180\pi \, \text{rad} = 180^{\circ}

  • Specific Conversion Values:

    • 1rad=180π57.31 \, \text{rad} = \frac{180}{\pi} \approx 57.3^{\circ}

    • 1=π1800.01745rad1^{\circ} = \frac{\pi}{180} \approx 0.01745 \, \text{rad}

  • Conversion Procedure:

    • To convert Degrees to Radians: Multiply by π180\frac{\pi}{180}.

    • To convert Radians to Degrees: Multiply by 180π\frac{180}{\pi}.

  • Common Angles:

    • 90=π2rad90^{\circ} = \frac{\pi}{2} \, \text{rad}

    • 45=π4rad45^{\circ} = \frac{\pi}{4} \, \text{rad}

    • 60=π3rad60^{\circ} = \frac{\pi}{3} \, \text{rad}

Angular Velocity (ω\omega)

  • Definition: The rate of change of angular displacement (ω=θt\omega = \frac{\theta}{t}).

  • Standard Unit: rad/s\text{rad/s}.

  • Common Units: RPM (Rotation Per Minute).

    • To convert 1 RPM to rad/s: Multiply by 2π60\frac{2\pi}{60} or π30\frac{\pi}{30}.

  • Time Period (TT): The time required to complete one rotation. For a complete cycle, ω=2πT\omega = \frac{2\pi}{T}.

  • Direction (Right-Hand Rule):

    • Curl the fingers of the right hand along the direction of rotation.

    • The extended thumb points in the direction of ω\omega.

    • Anti-Clockwise (Counter-Clockwise): Direction is Outward from the screen.

    • Clockwise: Direction is Inward to the screen.

  • Axial Vector: ω\omega is an axial vector because its direction always lies along the axis of rotation, regardless of the clockwise or anti-clockwise sense.

Dynamics of Clock Hands (Angular Speed Examples)

  • Second Hand:

    • Time Period (TT) = 60s60 \, \text{s}.

    • ω=2π60=π30rad/s\omega = \frac{2\pi}{60} = \frac{\pi}{30} \, \text{rad/s}.

  • Minute Hand:

    • Time Period (TT) = 1hour=3600s1 \, \text{hour} = 3600 \, \text{s}.

    • ω=2π3600=π1800rad/s\omega = \frac{2\pi}{3600} = \frac{\pi}{1800} \, \text{rad/s}.

  • Hour Hand:

    • Time Period (TT) = 12hours=12×3600=43,200s12 \, \text{hours} = 12 \times 3600 = 43,200 \, \text{s}.

    • ω=2π43,200=π21,600rad/s\omega = \frac{2\pi}{43,200} = \frac{\pi}{21,600} \, \text{rad/s}.

Angular Acceleration (α\alpha)

  • Definition: The rate of change of angular velocity (α=Δωt\alpha = \frac{\Delta \omega}{t}).

  • Unit: rad/s2\text{rad/s}^2.

  • Vector Nature: Like ω\omega, α\alpha is directed along the axis of rotation.

  • Directionality:

    • If total angular speed is increasing (Δω\Delta \omega is positive): α\alpha is parallel to ω\omega.

    • If total angular speed is decreasing (Δω\Delta \omega is negative/retardation): α\alpha is anti-parallel to ω\omega.

    • Example: When a fan is switched on, α\alpha and ω\omega are parallel. When switched off, they are anti-parallel.

    • If ω\omega is constant, α=0\alpha = 0.

Linear and Angular Relationships

  • Velocity: v=rωv = r\omega (Vector form: v=ω×r\mathbf{v} = \boldsymbol{\omega} \times \mathbf{r}). Note: r×ω\mathbf{r} \times \boldsymbol{\omega} is incorrect due to the non-commutative property of cross products.

  • Acceleration: at=rαa_t = r\alpha (Vector form: at=α×r\mathbf{a_t} = \boldsymbol{\alpha} \times \mathbf{r}).

  • Equations of Motion for Constant α\alpha:

    • ωf=ωi+αt\omega_f = \omega_i + \alpha t

    • θ=ωit+12αt2\theta = \omega_i t + \frac{1}{2} \alpha t^2

    • 2αθ=ωf2ωi22\alpha\theta = \omega_f^2 - \omega_i^2

  • Total Revolutions: θtotal=2πn\theta_{total} = 2\pi n, where nn is the number of rotations.

Centripetal and Tangential Acceleration

  • Tangential Acceleration (ata_t):

    • Related to changes in the magnitude (speed) of tangential velocity.

    • Acts along the tangent.

  • Centripetal (Radial) Acceleration (aca_c):

    • Related to changes in the direction of velocity.

    • Always points towards the center of the circle.

    • Formula: ac=v2r=rω2a_c = \frac{v^2}{r} = r\omega^2.

  • Net Linear Acceleration:

    • anet=ac2+at2a_{net} = \sqrt{a_c^2 + a_t^2}.

  • Angular relationships with the Radius Vector (r):

    • The angle between the radius vector (rr) and centripetal acceleration (aca_c) is 180180^{\circ} (π\pi radians).

    • The angle between aca_c and ata_t is 9090^{\circ} (π2\frac{\pi}{2} radians).

Uniform Circular Motion (UCM)

  • Definition: Circular motion with a constant speed.

  • Characteristics:

    • at=0a_t = 0 and α=0\alpha = 0.

    • ac0a_c \neq 0 because direction changes constantly.

    • Velocity is not constant (direction changes).

    • Acceleration is variable because its direction changes, even if the magnitude (ac=v2ra_c = \frac{v^2}{r}) remains constant.

Horizontal and Vertical Circular Motion

  • Horizontal Circular Motion:

    • Force of gravity acts downward, not affecting the horizontal path.

    • Centripetal force (FcF_c) is provided entirely by the Tension (TT) in the string.

    • T=mv2rT = \frac{mv^2}{r}.

  • Vertical Circular Motion (Non-Uniform):

    • Gravity significantly affects speed (acceleration downward, deceleration upward).

    • At the Bottom (Lowest Point):

      • Tension and Weight are opposite.

      • Tmax=Fc+w=mv2r+mgT_{max} = F_c + w = \frac{mv^2}{r} + mg.

    • At the Top (Highest Point):

      • Tension and Weight both act downward.

      • Tmin=Fcw=mv2rmgT_{min} = F_c - w = \frac{mv^2}{r} - mg.

  • Critical Velocities:

    • To maintain a circle without the string slackening, minimum velocity at the top: vtop=grv_{top} = \sqrt{gr}.

    • Minimum velocity required at the bottom to complete the circle: vbottom=5grv_{bottom} = \sqrt{5gr}.

Questions & Discussion

  • Q: Can a body move in UCM with constant velocity?

    • A: No. Velocity is a vector. Even if speed is constant, the direction changes at every point on the circle, thus velocity is variable.

  • Q: Where is the string most likely to break in vertical motion?

    • A: At the bottom, where tension is maximum (T=Fc+mgT = F_c + mg).

  • Q: What provides the centripetal force for a planet?

    • A: Gravitational force.

  • Q: What is the advice for students regarding past papers?

    • A: While past papers (UET, Mehran, NED, Nums) often repeat questions, relying solely on them is a gamble. Full course coverage is the first priority. If using past papers as a last resort, solve all available years, not just the most recent ones.

  • Q: How is 2nd-year physics being handled?

    • A: There are three options: attend the concurrent teacher's live sessions, watch the lecturer's own recorded sessions from earlier batches, or wait for the lecturer to cover it personally after May 20th.