AP Physics 1 Reference Sheet & Equation Guide

Every formula, constant, and equation you'll have on exam day (2026).

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📋 The AP Physics 1 equation sheet is a multi-page reference document provided during both the multiple-choice and free-response sections. It contains all the formulas, constants, and unit conversions you need—but knowing when and how to use them is what separates a 3 from a 5.

📄 Reference Sheet Overview

The AP Physics 1 equation sheet is provided to all students during the exam. Unlike some AP exams where you must memorize everything, Physics 1 gives you the formulas—your job is to know which one to use and how to apply it.

📝

Section I: MCQ

Reference sheet available in Bluebook testing app

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Section II: FRQ

Physical reference booklet provided for scratch work

The reference sheet includes:

Constants — Gravitational constant (G), acceleration due to gravity (g), atmospheric pressure

Unit prefixes — From tera (10¹²) to milli (10⁻³)

Symbols — All variable definitions (a, F, m, v, ω, τ, etc.)

Equations — Organized by topic (mechanics, rotation, waves, fluids)

🔢 Constants & Conversions

These values are provided on your reference sheet—you don't need to memorize them.

Physical Constants

Constant Symbol Value
Acceleration due to gravity g 9.8 m/s² (or N/kg)
Universal gravitational constant G 6.67 × 10⁻¹¹ N·m²/kg²
Atmospheric pressure P₀ 1.0 × 10⁵ Pa (or N/m²)

Metric Prefixes

tera (T)

10¹²

giga (G)

10⁹

mega (M)

10⁶

kilo (k)

10³

centi (c)

10⁻²

milli (m)

10⁻³

🚀 Kinematics Equations (Unit 1)

These equations describe motion in one dimension with constant acceleration. They're the foundation of AP Physics 1.

The “Big Three” Kinematic Equations

v = v₀ + at

Final velocity equals initial velocity plus acceleration times time

x = x₀ + v₀t + ½at²

Position as a function of time (when you don't know final velocity)

v² = v₀² + 2a(x – x₀)

Relates velocity and position (when you don't know time)

💡 Pro Tip

Choose your kinematic equation based on what variable is missing from the problem. Each equation omits one variable (x, v, v₀, a, or t).

⚡ Forces & Newton's Laws (Units 2-3)

Forces cause changes in motion. These equations connect force, mass, and acceleration.

ΣF = ma

Newton's Second Law: Net force equals mass times acceleration

|Ff| ≤ μ|Fn|

Friction Force: Maximum static friction; kinetic friction uses = sign

Fs = -kx

Hooke's Law: Spring force is proportional to displacement (restoring force)

|Fg| = G(m₁m₂)/r²

Universal Gravitation: Gravitational force between two masses

ac = v²/r

Centripetal Acceleration: Acceleration toward center of circular path

⚡ Work, Energy & Power (Unit 4)

Energy is conserved in closed systems. These equations help you track energy transfers.

K = ½mv²

Kinetic Energy: Energy of motion

Ug = mgh

Gravitational PE (near Earth): Potential energy from height

Ug = -Gm₁m₂/r

Gravitational PE (universal): For objects far from Earth's surface

Us = ½kx²

Elastic PE: Energy stored in a spring

W = F·d·cos(θ)

Work: Force times displacement times cosine of angle between them

P = W/t = Fv

Power: Rate of energy transfer

🔑 Key Relationship

Work-Energy Theorem: Wnet = ΔK — The net work done on an object equals its change in kinetic energy.

💥 Linear Momentum & Collisions (Unit 5)

Momentum is conserved in all collisions (elastic and inelastic) when no external forces act on the system.

p = mv

Linear Momentum: Mass times velocity (vector quantity)

J = FΔt = Δp

Impulse-Momentum Theorem: Impulse equals change in momentum

⚠️ Common Mistake

Watch your signs! If a ball bounces off a wall, Δv = vfinal – vinitial. If it rebounds at the same speed, Δv = v – (-v) = 2v, not zero!

🔄 Rotational Motion (Units 6-7)

Rotational motion mirrors linear motion—every linear equation has a rotational counterpart.

Rotational Kinematics

ω = ω₀ + αt — Angular velocity

θ = θ₀ + ω₀t + ½αt² — Angular position

ω² = ω₀² + 2α(θ – θ₀) — Angular velocity-position

Torque & Rotational Dynamics

τ = rF sin(θ)

Torque: “Rotational force” — depends on lever arm and angle

Στ = Iα

Newton's 2nd Law (Rotation): Net torque = rotational inertia × angular acceleration

L = Iω

Angular Momentum: Rotational inertia times angular velocity

Krot = ½Iω²

Rotational Kinetic Energy: Energy of spinning objects

Linear ↔ Angular Relationships

s = rθ

Arc length

v = rω

Tangential velocity

a = rα

Tangential acceleration

〰️ Simple Harmonic Motion (Unit 8)

SHM occurs when a restoring force is proportional to displacement (springs and pendulums).

x = A cos(2πft)

Position in SHM: Oscillates with amplitude A and frequency f

T = 1/f = 2π/ω

Period-Frequency Relationship: Period is inverse of frequency

Ts = 2π√(m/k)

Spring Period: Depends on mass and spring constant (not amplitude!)

Tp = 2π√(ℓ/g)

Pendulum Period: Depends on length and gravity (not mass or amplitude!)

💧 Fluids (Unit 9 — New for 2026!)

🆕 Updated Curriculum

Fluids were added to AP Physics 1 starting with the 2024-25 school year. These equations appear on the current reference sheet.

ρ = m/V

Density: Mass per unit volume

P = F/A

Pressure: Force per unit area

P = P₀ + ρgh

Pressure at Depth: Increases with depth in a fluid

Fb = ρVg

Buoyant Force: Weight of fluid displaced (Archimedes' Principle)

A₁v₁ = A₂v₂

Continuity Equation: Flow rate is constant in a pipe

P₁ + ρgy₁ + ½ρv₁² = P₂ + ρgy₂ + ½ρv₂²

Bernoulli's Equation: Conservation of energy in fluid flow

🚫 What's NOT on the Reference Sheet

The equation sheet gives you the formulas, but these important concepts must be understood and applied without explicit equations:

Newton's Three Laws (Conceptual)

You need to understand and apply the laws conceptually. The exam tests your understanding, not just formula recall.

Free-Body Diagrams

You must know how to draw and interpret FBDs. No formula can replace this skill.

Conservation Laws (When to Apply)

Knowing when energy or momentum is conserved requires understanding, not just equations.

Sign Conventions

Choosing positive direction, interpreting negative values—crucial skills not listed on the sheet.

Moments of Inertia Formulas

Specific I values for shapes (disk, sphere, rod) will be given in problems, not on the sheet.

🎯 How to Use the Reference Sheet Effectively

Having the equations isn't enough—here's how to actually use them on exam day:

1

Know the sheet BEFORE the exam

Familiarize yourself with where each equation is located. You don't want to waste time hunting during the test.

2

Identify what you know and what you need

List given quantities and what you're solving for. This helps you pick the right equation.

3

Understand what each equation means

Don't just plug and chug. Know the physics behind each formula so you can apply it correctly.

4

Practice with the actual sheet

Do practice problems using only the official reference sheet. Build this habit before exam day.

5

Check units to verify your answer

Use dimensional analysis. If your answer has wrong units, you used the wrong formula or made an algebra error.

📥 Download the Official Reference Sheet

Download the official AP Physics 1 equation sheet from College Board to practice with the exact document you'll have on exam day:

📄 Official AP Physics 1 Equation Sheet (PDF)

Download from College Board →

❓ Frequently Asked Questions

Do I get the equation sheet for both sections of the exam?

Yes! The reference sheet is available during both Section I (multiple-choice) and Section II (free-response). For the MCQ section, it's accessible in the Bluebook testing app. For FRQs, you'll receive a physical booklet.

Should I memorize the equations anyway?

Focus on understanding rather than memorizing. Through practice, you'll naturally learn the most common equations (F=ma, K=½mv², etc.). What matters more is knowing when and how to apply them.

Are moment of inertia formulas on the sheet?

No. Specific moments of inertia for shapes (disk, sphere, rod, etc.) are NOT on the reference sheet. When needed for a problem, they will be given in the question itself.

Is AP Physics 1 harder than AP Physics 2?

AP Physics 1 historically has a lower pass rate (around 45-50%) compared to Physics 2 (around 65-70%). Physics 1 covers more conceptual ground and requires strong problem-solving skills. Many students find Physics 1 more challenging.

What's new on the 2026 equation sheet?

The main addition is fluids content (density, pressure, buoyancy, continuity, Bernoulli's equation). These topics were added to the curriculum in 2024-25. The sheet also includes symbols and equations related to fluid mechanics.

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