Read position, displacement and distance
Calculate displacement, distance, average velocity and average speed, and interpret graph slope without mistaking the graph for a track.
Connect observations, diagrams and calculations to explain physical change.
This is the course outline. Open a unit to choose a lesson; every lesson opens on its own page. Explanations and experiments live inside those lesson pages.
The 123 lessons use bounded physical investigations with saved predictions, captures, reflections and public practice. They introduce signed position, graph slopes, distance, displacement, constant-velocity reference frames, acceleration, direction reversal, free-body diagrams, Newton’s laws, friction, inclined forces, uniform circular motion, work, kinetic energy, gravitational energy conservation, elastic energy, ideal spring oscillation, dissipative energy accounting, momentum, impulse, two-object collisions, torque, static equilibrium, rotational inertia, work, power, angular momentum and energy during mass redistribution, rolling energy, no-slip friction conditions, hydrostatic pressure, pressure forces, buoyancy, floating equilibrium, flow continuity, ideal pressure-work accounting, viscous resistance, velocity profiles, regime screening, dissipation, temperature, heat capacity, thermal equilibrium, phase-change energy, steady conduction, series thermal resistance, radiation, surface convection balances, ideal-gas states, molecular motion, gas mixtures, pressure-volume work, the first law, isothermal work, reversible adiabatic change, complete gas cycles, thermal efficiency, reservoir entropy balances, the Carnot limit, refrigeration, heat-pump performance, full harmonic motion, mass-dependent oscillation periods, pendulum timing, small-angle approximation limits, a physical timing protocol with a labeled synthetic practice alternative, traveling-wave snapshots, point histories, wavelength-frequency relationships, linear superposition, standing-wave nodes, tension-dependent wave speed, fixed-end harmonics, longitudinal sound, pressure-displacement relationships open/closed air-column modes sound Doppler shifts from source and observer motion, reflection, refraction, total internal reflection, thin-lens images, a focal-length measurement protocol, two-slit interference, single-slit diffraction, Coulomb forces, electric fields, point-charge potential, current, resistance, series and parallel circuits, electrical power, and a circuit measurement and fault-diagnosis protocol, nonideal source voltage and power, source parameter estimation, capacitor geometry and energy under fixed-voltage and fixed-charge constraints, and RC charging, discharge and energy accounting, and a discharge measurement protocol with uncertainty and meter-loading analysis, magnetic force directions, magnetic power and conditional circular motion, current-produced fields and forces between parallel currents, magnetic flux, Faraday induction, Lenz direction reasoning, motional emf and magnetic braking energy balances, self-inductance, RL current transients and magnetic-energy accounting. The heating, calorimetry and gas investigations reuse the chemistry models with separate physics notebooks. Arithmetic and graph reading are sufficient; programming and calculus are not required for these lessons.
The authored foundation now includes modern photon, matter-wave and nuclear evidence. A model notebook does not establish physical measurement skills or mastery. The cumulative project preserves design predictions, model trials, a first report, critique, revision and changed-condition evidence; practical skills and independently reviewed reasoning remain separate gates.
Calculate displacement, distance, average velocity and average speed, and interpret graph slope without mistaking the graph for a track.
Transform positions and velocities between constant-velocity frames and identify which claims depend on the observer.
Calculate velocity and displacement under constant acceleration, interpret units and distinguish negative acceleration from slowing down.
Compute a stopping instant and distance before reversal, distinguish distance from displacement across a turn, and reject an invalid braking extrapolation.
Identify tangent velocity and inward acceleration, calculate period and angular rate, and distinguish a stationary point from a completed orbit.
Construct a force ledger, distinguish weight from mass and identify why balanced forces are not necessarily a third-law pair.
Use net force divided by mass, test proportional changes, and explain constant velocity when net force is zero.
Use a static-friction bound, determine sliding-friction direction from relative motion, and identify when a motion prediction must change regimes.
Resolve gravity into slope-aligned components, calculate normal force and acceleration, and explain mass cancellation under frictionless assumptions.
Calculate inward force, distinguish fixed-speed from fixed-angular-rate comparisons, and predict tangent motion after ideal release.
Calculate constant-force work with signs, relate net work to the change in kinetic energy, and distinguish force-position area from force-time area.
Determine stopping displacement from negative work, distinguish reachable targets from invalid extrapolations, and recognize that energy alone does not identify velocity direction.
Calculate gravitational potential-energy differences, explain an arbitrary zero reference, and distinguish negative potential energy from impossible negative kinetic energy.
Use K+U conservation for a frictionless descent, reconcile gravitational work with potential-energy accounting, and identify conditions that require additional energy terms.
Use F = −kx and U = ½kx² with explicit units, explain the energy parabola, and distinguish force direction from stored energy.
Predict speed, force and acceleration at equilibrium and turns, distinguish velocity branches, and compare stiffness effects on period.
Distinguish mechanical energy from total energy, calculate internal-energy increase, and keep the block and track system boundary explicit.
Calculate stopping distance and time, distinguish sliding friction from a persistent reverse force, and test how resistance and initial speed affect stopping.
Calculate signed momentum and impulse, predict final velocity, and explain why a negative momentum is compatible with positive kinetic energy.
Read signed force-time area, compare rectangular and triangular pulses, and explain what equal impulse does and does not determine.
Calculate total signed momentum, relate individual momentum changes to internal impulses, and determine a common final velocity for a sticking collision.
Classify collision outcomes using kinetic energy, interpret restitution as a relative-speed ratio, and explain why bouncing does not guarantee an elastic collision.
Calculate signed torque for perpendicular forces, identify the perpendicular lever arm, and explain why a force through the pivot has zero torque about it.
Apply separate net-force and net-torque conditions, calculate pivot reaction, and identify when a proposed balance is impossible within the available lever arm.
Calculate point-mass rotational inertia, apply net torque = Iα, and connect angular motion in radians to tangential speed and acceleration.
Calculate rotational kinetic energy and constant-torque work, interpret power = torque × angular velocity, and compare fixed-time versus fixed-angle claims.
Calculate fixed-axis angular momentum, justify its conservation and infer final angular velocity from endpoint inertias.
Account for mechanism work between zero-radial-speed endpoints and explain how zero torque can coexist with energy transfer.
Use the no-slip relation v=Rω, account for translation and rotation about the center, and predict speed from the inertia factor.
Find the required static friction, compare it with μsN, and distinguish zero contact-point speed from zero friction or zero torque.
Use p=p_surface+ρgh with defined units and assumptions, and distinguish pressure from total force and density from total mass.
Distinguish absolute and gauge pressure, convert pressure and area to force, and add opposing pressure forces with a consistent direction.
Calculate buoyancy using liquid density and submerged volume, distinguish it from object weight and predict the sign of the submerged force imbalance.
Find the submerged volume fraction of a floating rigid object, identify when equilibrium is impossible and distinguish a neutral depth from a unique stable position.
Convert flow and area units, apply Q=Av and mass conservation, and distinguish fixed-flow comparisons from fixed-pressure experiments.
Apply a horizontal ideal-flow energy balance, distinguish gauge and absolute pressure, and verify that pressure work supplies the change in kinetic-energy flow.
Use Poiseuille resistance with consistent units, distinguish mean and center speed, and explain what is held fixed in a comparison.
Calculate a pipe Reynolds number from mean speed and diameter, reject unsupported predictions, and account for pressure-work dissipation.
Convert Celsius temperatures and temperature differences to kelvin, distinguish heat from internal energy, and use heat capacity within one phase.
Construct a signed energy balance, use heat-capacity weighting and explain why an endpoint calculation does not predict a cooling time.
Partition supplied energy between temperature change and latent heat, calculate phase fractions, and distinguish an energy axis from a time axis.
Apply the slab conduction relation, distinguish watts from joules and heat flux, and identify the maintained boundary conditions.
Add series resistances, solve an interface temperature, and test how thickness and conductivity affect the whole assembly.
Use absolute temperature in the Stefan–Boltzmann relation, interpret gray emissivity and explain radiative equilibrium.
Apply an assigned convection coefficient, combine parallel surface transfers and distinguish thermal holding power from device electricity or a cooling trajectory.
Apply PV = nRT with absolute pressure and kelvin temperature, compare constrained state changes and identify limits of the ideal model.
Relate pressure to molecular momentum transfer, temperature to mean translational kinetic energy and RMS speed to temperature and molar mass.
Add partial pressures, use mole fractions correctly and handle pure-component and empty-vessel limits without dividing by zero.
Calculate constant-pressure boundary work, identify zero work at constant volume and explain path dependence using equal-scale diagrams.
Use ΔU = Q − W with explicit signs, compute a monatomic ideal-gas energy change and reconcile each leg and whole path.
Explain why an isothermal ideal-gas expansion requires heat, calculate signed work using a volume ratio and identify the assumptions behind a pressure-volume area.
Use an adiabatic energy balance, compare pressure and temperature endpoints and state when the constant-gamma path relation applies.
Distinguish zero cyclic internal-energy change from nonzero heat and work, include compression work and reconcile a complete cycle.
Compute thermal efficiency from total positive heat input, diagnose misleading denominators and distinguish work per cycle from power.
Calculate reservoir entropy changes, distinguish a subsystem decrease from a total decrease and screen a cyclic engine with explicit boundaries.
Apply eta ≤ 1 − Tc/Th using kelvin, connect the equality case to reversible operation and reject unsupported claims of attainable power.
Distinguish work input from work output, calculate delivered heat and diagnose cooling proposals that require too little work.
Calculate cooling and heating COP, derive reversible bounds and distinguish per-cycle ratios from capacity and seasonal performance.
Predict turning-point and equilibrium behavior, distinguish acceleration from velocity direction and explain phase relationships across a full cycle.
Apply T = 2π√(m/k), relate frequency to period and explain which changes affect timing versus energy in the ideal spring model.
Apply the small-angle period relation, explain mass cancellation and connect release height to speed without confusing angle with length.
Quantify period underestimation, distinguish numerical from model error and explain why amplitude independence fails beyond the small-angle limit.
Define a full cycle, preserve raw timing data, estimate a period and explain uncertainty before judging agreement with a model.
Track a material point separately from a moving crest and explain what each graph holds fixed.
Apply speed = wavelength × frequency and distinguish pattern speed from transverse material velocity.
Apply linear superposition at the same position and time, distinguish displacement from velocity, and identify limits of the prescribed-wave model.
Identify nodes through time, calculate their spacing, interpret an amplitude envelope and separate a prescribed standing pattern from a bounded resonance experiment.
Use wave speed = sqrt(tension / linear mass density), keep units consistent and explain the assumptions behind a tension comparison.
Apply wavelength = 2L/n and frequency = n times the fundamental, while distinguishing mode shape from a driven response or a complete instrument sound.
Identify sound as longitudinal bulk motion in this fluid model, interpret wavelength and period, and explain the displacement exaggeration.
Distinguish pressure perturbation from absolute pressure, relate compression to displacement gradient, and explain why pressure amplitude changes with frequency when displacement amplitude is held fixed.
Identify open ends as pressure nodes and displacement antinodes, derive the open-open harmonic series and interpret normalized profiles.
Derive quarter-wavelength boundary matching, identify odd harmonic frequencies and compare a closed-open column with an open-open column of the same length.
Derive rightward wavefront spacing from source motion and predict frequency for a stationary observer.
Use signed velocities relative to air, distinguish encounters from spacing and test equal-closing-speed claims.
Draw a normal, convert surface angles to normal angles and predict a reflected direction.
Apply Snell’s law and explain why frequency stays fixed while speed and wavelength change.
Find a critical angle and distinguish below-critical transmission, the critical limit and total internal reflection.
Use the thin-lens equation and ray intersections to locate an inverted real image.
Distinguish a virtual image from a parallel outgoing bundle and avoid assigning a finite image at focus.
Apply the sign convention to a diverging lens with a real object and interpret its ray extensions.
Estimate focal length from several real-image arrangements and distinguish repeatability, bounded uncertainty and systematic error.
Relate integer and half-integer path differences to interference and explain the model’s coherence assumptions.
Predict fringe spacing, invert the relationship and distinguish approximation error from measurement uncertainty.
Predict single-slit minima and central width while distinguishing width from two-slit separation.
Apply Coulomb’s law with units and distinguish third-law partners from net force on one object.
Use F = qE, identify field direction by a positive test charge and explain nonzero field at zero probe charge.
Calculate point-charge potential, pair energy and field work while keeping the reference and charge fixed.
Calculate current and transported charge, distinguish current from voltage, and interpret current-versus-voltage slope.
Calculate series equivalent resistance and voltage drops, and explain why current is equal throughout one steady path.
Calculate parallel equivalent resistance and branch currents and verify current conservation.
Use P = VI and energy = Pt with consistent units and reconcile resistor powers with source output.
Use a documented measurement procedure, bounded uncertainty and an additional discriminating observation to evaluate a circuit model.
Calculate a loaded source operating point and reconcile delivered and internally dissipated power.
Infer a linear source characteristic with correct units and evaluate its uncertainty and predictive limits.
Use consistent area and distance units in C = epsilon A/d and compare fixed-voltage with fixed-charge conditions.
Choose the appropriate energy expression and include source work in a quasistatic geometry-change balance.
Calculate and interpret capacitor voltage and current at a selected fraction of the charging time constant.
Use exponential decay to predict discharge, interpret current sign, and infer a time constant from a threshold reading.
Check time-dependent energy balances and distinguish power, energy and asymptotic totals.
Infer a discharge time constant and conditional capacitance, evaluate an unused reading, and design a discriminating measurement.
Predict magnetic-force components and explain the effects of reversing charge, velocity or field.
Calculate conditional circular radius and period and explain why magnetic power is zero.
Predict long-wire field strength and direction and explain the limits of the thin infinite-wire approximation.
Predict the direction and magnitude of parallel-wire forces and distinguish force per length from force on a finite segment.
Calculate signed flux and linkage and explain zero-flux and zero-emf cases.
Use Faraday’s law with units and distinguish flux value from its rate of change.
Explain induced-current direction and the limits of the displayed energy account.
Calculate motional emf and current with a consistent loop reference and distinguish closed and open circuits.
Calculate braking force and reconcile mechanical power and circuit heating within explicit assumptions.
Interpret inductor voltage and current slope and explain why a closed decay path matters.
Calculate RL time constants, current fractions and voltage drops with explicit preparation.
Verify separate RL energy balances and distinguish finite storage from unbounded long-time source work.
Convert wavelength to frequency and photon energy, then calculate photon rate from beam power.
Use differences between stipulated levels to predict line energies and challenge identification from one line.
Use photon energy and a supplied work function to distinguish no emission from positive maximum kinetic energy.
Compare a supplied quantum yield with photon rate while holding maximum electron energy fixed.
Calculate de Broglie wavelength from nonrelativistic kinetic energy and test when a wave description matters.
Complete nuclear reaction equations while distinguishing necessary conservation from energetic possibility.
Use exponential survival and distinguish an expected ensemble count from a deterministic decay schedule.
Calculate activity from survivor number and half-life and explain why activity alone does not determine dose.
Convert a consistent initial-minus-final rest-mass difference into Q and preserve total energy conservation.
Compare selected fusion and fission reaction ledgers and distinguish conservation, energy release and rate.
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