LEARN WITH RAY · UNDERGRADUATE
Introduction to mechanics
Learn how things move and why. Explore forces, energy, rotation, gravity and oscillations.
One step at a time.
Short lessons. Time to practise.
Learn at your own pace.
Physics / University introductory course
11 subtopics · your own pace
Foundations: measurement and models
Quantities, dimensional checks, measurement precision and the scope of an idealization.
- Quantities, dimensions and units
Report a mechanical quantity as number times unit, distinguish dimension from unit, and convert using equal-quantity conversion factors. Read SI prefixes and scientific notation. - Checking equations by dimensions
Require matching dimensions for quantities added or equated. Dimensional consistency is necessary but does not establish numerical factors, signs or physical validity. - Measurement uncertainty and reported precision
Distinguish a measured value with uncertainty from an exact count. Interpret x±δx, distinguish accuracy from repeatability, and avoid reporting more precision than the measurement supports. - A physical model and its assumptions
Choose whether a particle or rigid-body model fits a question and state the idealizations that justify omitted effects. A model’s prediction is conditional on those assumptions.
Foundations: vector operations
Components, addition, subtraction and both vector products.
- Scalars, vectors and signed components
Distinguish a scalar from a vector and express a vector in perpendicular unit-vector directions. Resolve signed components and reconstruct magnitude and direction; the zero vector has no unique direction. - Adding, subtracting and scaling vectors
Calculate vector sums, differences and scalar multiples componentwise. Explain a−b=a+(−b), and how a negative scalar reverses direction. - Dot products and projections
Calculate a·b from components or |a||b|cosθ. For nonzero vectors, its sign distinguishes acute, right and obtuse angles; a positive dot product alone does not imply parallelism. - Cross products and the right-hand rule
Determine a×b using magnitude |a||b|sinθ and the right-hand direction. Explain anti-commutativity, zero product for parallel vectors, and the signed z-component a_x b_y−a_y b_x for planar vectors.
Foundations: coordinates and change
Coordinate conventions, rates and accumulation.
- Position, origin and reference axes
Describe position relative to an origin and oriented axes. Distinguish a coordinate change from motion, and state a consistent positive direction before interpreting signs. - Average rates and local rates
Interpret a secant slope as an average rate and a tangent slope as a local rate, with units. A negative derivative describes decrease at that instant, not a negative value or a guarantee of monotonic decrease over a whole interval. - Signed accumulation and initial values
Interpret signed area under a rate graph as net change and use final value=initial value+net change. Distinguish signed accumulation from total unsigned amount.
Describing motion
Connect position, velocity and acceleration in one and two dimensions.
- Displacement
Calculate displacement as final position minus initial position and distinguish it from distance traveled. - Average velocity
Calculate average velocity as displacement divided by elapsed time, distinguishing it from average speed. - Instantaneous velocity
Find instantaneous velocity as the time derivative of position, including componentwise derivatives for vector position. - Acceleration
Calculate average acceleration from a change in velocity and instantaneous acceleration as the time derivative of velocity. - Motion with constant acceleration
Use constant-acceleration relations to predict position or velocity, while checking that the acceleration is constant over the interval. - Independent components of projectile motion
Solve ideal projectile motion by applying horizontal and vertical kinematics with a shared elapsed time and downward gravitational acceleration. - Acceleration in uniform circular motion
Explain why constant-speed circular motion has inward acceleration of magnitude v²/r even though its speed does not change.
Forces and Newton’s laws
Choose an object, draw its forces and predict its acceleration.
- A force is an interaction
Explain why each force on an object must be attributed to an interaction with another object, whether contact or noncontact. - A free-body diagram
Draw a free-body diagram that isolates one chosen object and includes only forces exerted on it. - Net force
Calculate the vector sum of forces on a single object using components. - Inertial frames and Newton’s first law
Explain why an object with zero net force has constant velocity in an inertial frame, and why an accelerating frame needs special care. - Newton’s second law
Apply the component equations of net force equals mass times acceleration to a constant-mass object in an inertial frame. - Newton’s third-law pairs
Explain why equal-and-opposite interaction forces act on different objects and therefore do not cancel in a single object's free-body diagram. - Normal force
Determine the normal force from the acceleration perpendicular to a contact surface. - Tension in an ideal rope
Apply the same-tension constraint of an ideal rope to a connected pair of masses. - Static and kinetic friction
Select and apply the static-friction bound or kinetic-friction model according to whether surfaces slip. - The net radial force
Apply Newton’s second law in the radial direction to identify which actual forces provide the acceleration of circular motion.
Work and energy
Choose a system and account for transfers and stored energy.
- Work by a constant force
Calculate the work done by a constant force using its component along an object's displacement, including zero and negative work. - Work by a varying force
Calculate work by integrating the component of a position-dependent force along a specified displacement. - Kinetic energy
Calculate a particle's translational kinetic energy from its mass and speed. - The work–energy theorem
Apply the work–energy theorem using the total work of all forces to find a change in speed. - Conservative forces and potential energy
Use path independence to identify a conservative force and calculate its potential-energy change as the negative of its work. - Conservation of mechanical energy
Determine whether mechanical energy is conserved and, when it is not, include nonconservative work in the energy balance. - Power
Calculate average power from work and elapsed time, or instantaneous power from force and velocity.
Momentum and collisions
Separate internal interactions from external impulses.
- Momentum is a vector
Calculate a particle's momentum from its mass and velocity, retaining the velocity's direction. - Impulse changes momentum
Calculate impulse from a force–time history and use it to find a particle's change in momentum. - Choosing a system
Choose a system boundary and classify forces as internal or external to it. - Conserving total momentum
Explain why a system's total momentum remains constant when its external impulse is negligible, despite internal forces. - A perfectly inelastic collision
Find the common final velocity of objects that stick together when external impulse during the collision is negligible. - An elastic collision
Solve a one-dimensional elastic collision using conservation of both momentum and kinetic energy. - Center-of-mass position
Calculate the center-of-mass position as a mass-weighted average. - Acceleration of the center of mass
Predict center-of-mass acceleration from total mass and net external force.
Rigid-body rotation
Relate torque, mass distribution and rotational motion.
- Angular displacement
Relate angular displacement in radians to arc displacement about a fixed axis. - Angular velocity
Relate angular velocity to a point’s tangential speed about a fixed axis. - Angular acceleration
Use angular acceleration as the rate of change of angular velocity to predict angular velocity and displacement when angular acceleration is constant. - Moment of inertia
Calculate moment of inertia about a specified axis by summing mr² for discrete masses, accounting for each mass's distance from that axis. - Changing the rotation axis
Apply the parallel-axis theorem to find a body's moment of inertia about an axis parallel to one through its center of mass. - Torque about an axis
Calculate the signed torque about a fixed axis from an applied force, its point of application and the angle between force and radius. - Fixed-axis rotational dynamics
Use the net external torque and moment of inertia to find a rigid body's angular acceleration about a fixed axis. - Rotational kinetic energy
Calculate the kinetic energy of a rigid body rotating about a fixed axis using its moment of inertia and angular speed. - Rolling without slipping
Apply the no-slip relation v_cm = Rω to connect a rolling body's translational and angular speeds. - Energy of a rolling body
Use translational and rotational kinetic energy together with the no-slip constraint to solve a rolling energy-conservation problem.
Angular momentum and equilibrium
Use torque balance and angular-momentum conservation.
- Angular momentum of a particle
Calculate a particle's angular momentum about a specified origin from its position and momentum, including its rotational direction. - Angular momentum about a fixed symmetry axis
Calculate the component of a rigid body's angular momentum along its fixed symmetry axis using L = Iω. - Conserving angular momentum
Apply angular-momentum conservation about a specified axis when the net external torque about that axis is negligible, distinguishing this condition from the absence of forces. - Static equilibrium
Apply both zero net force and zero net torque to determine unknown forces on a stationary rigid body.
Gravitation and orbits
Use force and energy to reason about planetary motion.
- The inverse-square gravitational force
Apply Newton’s gravitational force law to find the magnitude and direction of the force between two masses. - Gravitational potential energy
Explain why inverse-square gravity has potential energy U(r) = −GMm/r when the zero is chosen at infinity. - A circular orbit
Apply gravitational force and radial acceleration to determine the speed of a circular orbit around a much more massive body. - Escape speed
Apply conservation of mechanical energy to find the minimum launch speed that allows an object to reach infinity with zero speed, neglecting other forces. - Kepler’s equal-area law
Explain why a central gravitational force makes the line from an orbiting body to the attracting body sweep out equal areas in equal times.
Oscillations
Recognize restoring forces and the limits of harmonic models.
- A linear restoring force
Apply F = -kx to find the magnitude and direction of a spring’s force relative to equilibrium, and distinguish a linear restoring force from one that is not proportional to displacement. - Simple harmonic motion
Apply Newton’s second law to an ideal mass–spring system to obtain ω = √(k/m) and predict its sinusoidal motion from simple initial conditions. - The small-angle pendulum
Explain how the small-angle approximation turns a pendulum’s tangential restoring force into a harmonic-motion model with ω ≈ √(g/L), and why that model is limited to small amplitudes. - Energy in an oscillator
Apply mechanical-energy conservation to an ideal spring oscillator to relate amplitude, position, speed, and the exchange between spring potential and kinetic energy. - Damping removes oscillator energy
Explain why a force opposing an oscillator’s motion does negative work, reducing its mechanical energy and amplitude rather than conserving them as in the ideal model. - Driven oscillations and resonance
Explain why periodic forcing can produce a large response near an oscillator’s natural frequency and how damping limits the sustained response.