AP Guides/AP Physics 1

Free Study Guide · 2026 Exam Season

AP Physics 1 Study Guide

Complete AP Physics 1 study guide for 2026. Covers Newton's laws, energy, momentum, waves, and rotational motion with interactive Desmos graphs, PhET simulations, and curated video explanations.

00days
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23hrs
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53min
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39sec

Exam date

Wednesday, May 6, 2026

5Units covered
7Interactive elements
100%Free to use
Unit 2~20% of exam

Dynamics — Newton's Laws

The most heavily tested unit. Free body diagrams, net force, friction, and Newton's three laws.

Dynamics is the study of what causes motion. Nearly every AP Physics 1 FRQ involves drawing a free body diagram and applying Newton's second law.

Newton's Three Laws

  1. Inertia: An object at rest stays at rest; an object in motion stays in motion — unless acted on by a net external force.
  2. F = ma: The net force on an object equals its mass times acceleration. Direction matters: always define a positive direction first.
  3. Action-Reaction: For every force, there is an equal and opposite reaction force. These act on different objects — they never cancel each other.

Free Body Diagrams

Draw one dot representing the object. Draw arrows for every force acting on it: gravity (down), normal force (perpendicular to surface), tension (along string), friction (opposing motion), applied force. Sum forces in each direction and set equal to ma.

Friction

Fnet=mafk=μkNfsμsNF_{\text{net}} = ma \qquad f_k = \mu_k N \qquad f_s \le \mu_s N

Kinetic friction acts when surfaces slide. Static friction prevents sliding and can take any value up to its maximum μₛN. The normal force N is not always mg — on an incline or in an elevator it differs.

Kinematics (1D and 2D)

The "Big Four" kinematic equations (constant acceleration only):

v=v0+atx=x0+v0t+12at2v2=v02+2aΔxvˉ=v+v02\begin{array}{ll} v = v_0 + at & x = x_0 + v_0 t + \tfrac{1}{2}at^2 \\[8pt] v^2 = v_0^2 + 2a\Delta x & \bar{v} = \dfrac{v + v_0}{2} \end{array}
Kinematics — Position, Velocity & Acceleration
Interactive · Desmos

Kinematics — Position, Velocity & Acceleration

Drag the a (acceleration), v₀ (initial velocity), and x₀ (initial position) sliders. The blue curve shows position x(t) and the red curve shows velocity v(t). Notice how the slope of x(t) equals v(t) at every point — that's calculus-level insight the AP exam tests conceptually.

Powered by Desmos

Best Film on Newton's Third Law. Ever.
Veritasium · YouTube
Forces and Motion Basics
Interactive · PhET

Forces and Motion Basics

Apply forces to objects with friction and observe how net force, mass, and acceleration relate. Build intuition for free body diagrams.

Open simulation

Opens in a new tab · Powered by PhET · University of Colorado Boulder

Exam tip: Newton's 3rd Law action-reaction pairs act on DIFFERENT objects — they can never cancel. The most common exam trap: a book sits on a table. The normal force on the book (from the table) and gravity on the book are NOT a Newton's 3rd Law pair — they're both on the same object. The true 3rd Law pair of gravity on the book is the book pulling Earth upward.

Common mistake: Never write F = ma without first identifying what 'F' means. It must be the NET force — the vector sum of all forces on the object. Writing just one force (like tension) equal to ma is wrong if other forces are also present.

Key Concepts

Net forceVector sum of all forces on an object. Only the net force determines acceleration.
Normal force (N)Contact force perpendicular to a surface. Not always equal to mg.
Kinetic friction (fₖ)fₖ = μₖN. Opposes sliding motion. Acts while surfaces move relative to each other.
InertiaTendency to resist changes in motion. Measured by mass, not weight.
Newton's 3rd Law pairEqual magnitude, opposite direction forces on two different objects.

Exam prediction: This topic frequently appears on the AP Physics 1 exam. See our full AP Physics 1 predictions →

Unit 4~15% of exam

Energy & Work

Work-energy theorem, kinetic and potential energy, conservation of energy, and power.

Energy is one of the most powerful tools in physics — it lets you solve problems without knowing forces at every instant. When forces are complicated, energy often isn't.

Work and the Work-Energy Theorem

Work is done on an object when a force has a component in the direction of displacement. Only the parallel component counts.

W=FdcosθWnet=ΔKE=12mvf212mvi2W = F d \cos\theta \qquad W_{\text{net}} = \Delta KE = \tfrac{1}{2}mv_f^2 - \tfrac{1}{2}mv_i^2

Types of Energy

KE=12mv2PEg=mghPEs=12kx2KE = \tfrac{1}{2}mv^2 \qquad PE_g = mgh \qquad PE_s = \tfrac{1}{2}kx^2

Conservation of Energy

In a closed system with no non-conservative forces (no friction, no air resistance), total mechanical energy is constant:

KEi+PEi=KEf+PEforEmech=constantKE_i + PE_i = KE_f + PE_f \qquad \text{or} \qquad E_{\text{mech}} = \text{constant}

When friction is present, mechanical energy is lost to thermal energy: ΔE_thermal = fₖd.

Power

P=WΔt=FvP = \frac{W}{\Delta t} = Fv
Energy Conservation — KE vs PE
Interactive · Desmos

Energy Conservation — KE vs PE

Drag the h slider (height) to move an object up and down. Watch KE and PE trade off while their sum E stays constant — this is conservation of mechanical energy. Drag E to change the total energy.

Powered by Desmos

The Bullet Block Experiment
Veritasium · YouTube
Energy Skate Park
Interactive · PhET

Energy Skate Park

Watch KE and PE bars update in real time as a skater moves along a track. Add friction and watch mechanical energy decrease. Drag the skater to any height and release.

Open simulation

Opens in a new tab · Powered by PhET · University of Colorado Boulder

Exam tip: Use energy when you don't know (or don't need) the time or the forces during motion — only the start and end states matter. Use F = ma when you need acceleration, force, or time. The AP FRQ frequently requires you to justify which approach you're using.

Key Concepts

Work-energy theoremNet work done on an object equals its change in kinetic energy.
Conservative forceWork done is path-independent (gravity, springs). Enables PE definition.
Non-conservative forceWork depends on path (friction, air resistance). Removes mechanical energy.
Power (P)Rate of energy transfer. P = W/Δt = Fv. Units: Watts (J/s).
Spring PEPE_s = ½kx². x is measured from equilibrium; k is spring constant (N/m).
Unit 5~12% of exam

Momentum & Collisions

Impulse, conservation of momentum, elastic and inelastic collisions, and center of mass.

Momentum is always conserved in a closed system — no matter what forces act internally. It's the go-to tool for collisions and explosions where forces are unknown.

Momentum and Impulse

p=mvJ=FΔt=Δp\vec{p} = m\vec{v} \qquad \vec{J} = \vec{F}\,\Delta t = \Delta \vec{p}

Impulse equals the area under an F vs t graph — a frequent AP graph-reading question.

Conservation of Momentum

m1v1i+m2v2i=m1v1f+m2v2fm_1 v_{1i} + m_2 v_{2i} = m_1 v_{1f} + m_2 v_{2f}

Collision Types

TypeMomentumKEExample
ElasticConservedConservedBilliard balls, ideal springs
InelasticConservedNot conservedMost real collisions
Perfectly inelasticConservedMaximum KE lostObjects stick together

For perfectly inelastic collisions: m₁v₁ + m₂v₂ = (m₁ + m₂)vf

Momentum and Angular Momentum
Physics Videos by Eugene Khutoryansky · YouTube
Collision Lab
Interactive · PhET

Collision Lab

Set masses and initial velocities for elastic or inelastic collisions. Watch momentum arrows and KE readouts before and after — perfect for verifying conservation laws.

Open simulation

Opens in a new tab · Powered by PhET · University of Colorado Boulder

Exam tip: Momentum is a vector — direction signs matter. Always define a positive direction before writing conservation equations. In 2D collisions, write separate conservation equations for x and y. The AP exam frequently gives you a graph of force vs. time and asks for the impulse (area under the curve).

Common mistake: Kinetic energy is NOT conserved in inelastic collisions — only momentum is. Never use energy conservation in a collision problem unless told it's elastic. The missing KE goes to heat, sound, and deformation.

Key Concepts

Impulse (J)J = FΔt = Δp. The area under a force-time graph.
Elastic collisionBoth momentum AND kinetic energy conserved. Objects bounce off perfectly.
Perfectly inelasticObjects stick together. Momentum conserved, maximum KE lost.
Center of massThe average position weighted by mass. An isolated system's center of mass moves at constant velocity.
Law of conservation of momentumIn a closed system (no external forces), total momentum is constant.

Exam prediction: This topic frequently appears on the AP Physics 1 exam. See our full AP Physics 1 predictions →

Unit 10~12% of exam

Waves & Sound

Transverse and longitudinal waves, wave speed, standing waves, harmonics, and resonance.

Waves transfer energy without transferring matter. AP Physics 1 focuses on mechanical waves — you don't need EM waves here.

Wave Properties

Every wave has amplitude (A), wavelength (λ), frequency (f), and period (T). These relate through:

v=fλT=1fvstring=FTμv = f\lambda \qquad T = \frac{1}{f} \qquad v_{\text{string}} = \sqrt{\frac{F_T}{\mu}}

Wave speed depends on the medium, not the frequency. Doubling frequency halves wavelength at the same speed.

Standing Waves and Harmonics

When a wave reflects and interferes with itself, standing waves form at specific resonant frequencies. For a string fixed at both ends (or open pipe open at both ends):

fn=nv2L,n=1,2,3,(string fixed both ends / open pipe)f_n = \frac{nv}{2L}, \quad n = 1, 2, 3, \ldots \qquad \text{(string fixed both ends / open pipe)}
fn=nv4L,n=1,3,5,(closed pipe — odd harmonics only)f_n = \frac{nv}{4L}, \quad n = 1, 3, 5, \ldots \qquad \text{(closed pipe — odd harmonics only)}

Nodes are points of zero displacement. Antinodes are points of maximum displacement. The fundamental (n = 1) has one antinode; each harmonic adds one more.

Wave Superposition

When two waves overlap, their displacements add. Constructive interference occurs when crests align; destructive when a crest meets a trough.

Wave Superposition — Constructive & Destructive Interference
Interactive · Desmos

Wave Superposition — Constructive & Destructive Interference

The blue and red curves are two individual waves. The green sum shows their superposition. Set f₁ = f₂ for pure constructive or destructive interference. Make f₁ slightly different from f₂ to see beating — a low-frequency amplitude oscillation caused by interference.

Powered by Desmos

Sound + Fire = Rubens' Tube
Veritasium · YouTube
Wave on a String
Interactive · PhET

Wave on a String

Set the string to 'Oscillate' mode and adjust frequency and tension. Switch to 'Resonance' to see standing wave harmonics form. Observe node and antinode positions.

Open simulation

Opens in a new tab · Powered by PhET · University of Colorado Boulder

Exam tip: Standing wave problems almost always require drawing the harmonic pattern first. For a string fixed at both ends: n = 1 is half a wavelength, n = 2 is one full wavelength, n = 3 is one-and-a-half wavelengths. Use λₙ = 2L/n then v = fλ to find the nth harmonic frequency.

Key Concepts

Wavelength (λ)Distance between two adjacent crests (or any two identical points). Units: meters.
Frequency (f)Number of complete oscillations per second. Units: Hz.
NodePoint of zero displacement in a standing wave. Fixed ends are always nodes.
AntinodePoint of maximum displacement in a standing wave. Open ends are antinodes.
Fundamental frequencyLowest resonant frequency (n = 1). All other harmonics are integer multiples of f₁.
Unit 7~12% of exam

Rotational Motion & Torque

Torque, rotational inertia, angular momentum, and rolling without slipping.

Rotational motion is the direct analog of linear motion. Every linear quantity has a rotational counterpart — once you see the pattern, the formulas write themselves.

Linear → Rotational Analogs

LinearRotational
Displacement xAngle θ (radians)
Velocity vAngular velocity ω (rad/s)
Acceleration aAngular acceleration α (rad/s²)
Force FTorque τ (N·m)
Mass mRotational inertia I (kg·m²)
Momentum p = mvAngular momentum L = Iω
F = maτ = Iα

Torque

Torque is the rotational effect of a force. It depends on how far from the pivot the force is applied and the angle between the force and the lever arm.

τ=rFsinθτnet=IαL=Iω\tau = rF\sin\theta \qquad \tau_{\text{net}} = I\alpha \qquad L = I\omega

For rotational equilibrium (no angular acceleration): Στ = 0. Sum torques about any point — choose the pivot to eliminate unknown forces from the equation.

Rolling Without Slipping

When an object rolls without slipping, its translational and rotational motion are linked:

vcm=rωacm=rαv_{\text{cm}} = r\omega \qquad a_{\text{cm}} = r\alpha

Conservation of Angular Momentum

In a closed system with no external torque, angular momentum is conserved. This explains why a spinning figure skater spins faster when they pull their arms in — I decreases, so ω increases to keep L = Iω constant.

Exam tip: When calculating torque for a static equilibrium problem (e.g., a beam balanced on a fulcrum), always choose your pivot point to be where an unknown force acts. That torque then drops out of the equation, leaving you to solve for fewer unknowns.

Common mistake: Rotational inertia I depends on both mass and how that mass is distributed. A hollow cylinder has more rotational inertia than a solid cylinder of the same mass and radius — the mass is farther from the axis. Don't confuse I with mass alone.

Key Concepts

Torque (τ)τ = rF sinθ. Rotational equivalent of force. Positive = counterclockwise (by convention).
Rotational inertia (I)Resistance to angular acceleration. I = Σmr² for point masses.
Angular momentum (L)L = Iω. Conserved when net external torque = 0.
Rolling conditionv_cm = rω links translational and rotational motion for rolling without slipping.
Rotational equilibriumΣτ = 0 about any point. Used for static beam/lever problems.

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