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PHYSICS 1D03 | Midterm Two | Lecture Notes and Summary

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I made these notes so they are organised by topic, making it easier to study since going through lectures one by one is overwhelming. This is a good resource to have because it summarizes literally everything you need to know. If you know this, you're guaranteed to do well on the midterm. Key topics: This midterm covers rotational kinematics including angular position, velocity, acceleration, constant angular acceleration equations, and the relationship between rotational and linear motion. It also includes torque dynamics such as lever arms, vector cross products, Cartesian cross products, and right-hand rule applications. Topics in rotational dynamics include moment of inertia, mass distribution, the parallel axis theorem, and Newton’s Second Law for rotation. The course also covers center of mass, center of gravity, static equilibrium, and multi-pivot systems. Energy topics include work, power, kinetic energy, potential energy, conservative vs non-conservative forces, and conservation of mechanical energy.

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PHYSICS 1D03 MIDTERM 2 NOTES
AND SUMMARY
Nicely Written & Complete Study Guide




KEY TOPICS COVERED

• Rotational Kinematics: Angular Position, Angular Velocity, Angular Acceleration, Constant
Angular Acceleration Equations, Linear-Rotational Links
• Torque Dynamics: Unbalanced Torque, Lever Arms, Vector Cross Products, Cartesian
Cross Products, Right-Hand Rule Guidelines
• Rotational Inertia & Dynamics: Moment of Inertia, Mass Distribution, Parallel Axis
Theorem, Newton's Second Law for Rotation
• Center of Mass & Equilibrium: Coordinate Center Calculations, Symmetry Constraints,
Center of Gravity, Static Equilibrium Conditions, Multi-Pivot System Formulations
• Work, Energy, and Power: Vector Dot Products, Work by Constant and Variable Forces,
Work-Kinetic Energy Theorem, Mechanical Power (Translational & Rotational)
• Potential Energy & Conservation: Conservative vs. Non-Conservative Forces,
Gravitational and Elastic Potential Energies, Mechanical Energy Conservation




1

, Lesson 1: Rotational Kinematics of Rigid Bodies

Angular Motion Parameters

A rigid body is an extended object whose constituent particles maintain completely fixed distances relative
to one another during motion. When a rigid body undergoes pure rotation about a fixed axis, every
individual particle travels in a circular path centered on that axis, completing a full revolution in the exact
same time interval.
• Angular Position θ: Measured in radians (rad), where 2π rad = 360° = 1 revolution. The arc length s
along a circle of radius r is: s = rθ.
• Angular Velocity ω: The time derivative of angular position, measured in radians per second (rad/s): ω
= dθ / dt.
• Angular Acceleration α: The time derivative of angular velocity, measured in radians per second
squared (rad/s2): α = dω / dt = d2θ / dt2.
• Directionality: Defined by the right-hand rule. Curl the fingers of your right hand in the direction of
rotation; your extended thumb points along the axis of rotation to indicate the direction of the angular
velocity vector ω. Counter-clockwise (CCW) rotation is standardly defined as positive (ω > 0).


EXAMPLE: LINEAR TRACKING ON SPINNING MEDIA

A compact disc operates with a uniform linear reading velocity of v = 1.3 m/s. To find the angular velocity ω
at the innermost track where the radius is r = 23 mm = 0.023 m, use the connection formula: v = rω.
Rearranging gives: ω = v / r = 1..023 = 56.5 rad/s.



Formulations for Constant Angular Acceleration

When a rigid body undergoes rotation with a uniform angular acceleration (α = constant), its motion is
governed by equations that parallel the standard formulas for linear kinematics:

ωf = ωi + αt

θf = θi + ωit + ½αt2

ωf2 = ωi2 + 2α(θf − θi)


EXAMPLE: DISK SPIN-DOWN REVOLUTION SCALING

A spinning high-speed disc starts from rest and accelerates uniformly to a final target velocity of 7200 rev/
min over an interval of 18 s. First, convert the angular velocity to standard units: ωf = (7200 × 2π) / 60 =
240π rad/s. The constant acceleration is: α = ωf / t = 240π / 18 = 41.89 rad/s2. The net angular displacement
is: Δθ = ½ωft = ½(240π)(18) = 2160π rad. Dividing by 2π yields exactly 1080 revolutions.




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Engineering Essentials

I have notes, study guides and cheat sheets for most core engineering classes, focusing more on electrical. I have gotten A's in all my classes, so trust that the notes are helpful.

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