AP Physics 1 Formula Sheet
All key equations organized by topic. Memorize these — the AP exam does not provide a formula sheet.
Kinematics
v = v_0 + atVelocity after constant acceleration
v = final velocity, v₀ = initial velocity, a = acceleration, t = time
Units: v: m/s, a: m/s², t: s
x = x_0 + v_0 t + (1)/(2)at²Position under constant acceleration
x = final position, x₀ = initial position
Units: x: m
v² = v_0² + 2aΔ xVelocity–displacement relation (time-independent)
Δx = displacement
Units: v: m/s, a: m/s², x: m
x = ((v + v_0))/(2) · tAverage velocity × time (constant acceleration)
(v + v₀)/2 = average velocity
Units: m
Dynamics (Newton's Laws)
F_net = maNewton's Second Law
F_net = net force, m = mass, a = acceleration
Units: F: N, m: kg, a: m/s²
F_friction = μ NFriction force (kinetic or maximum static)
μ = coefficient of friction, N = normal force
Units: N
F_g = mgWeight (gravitational force near Earth's surface)
g = 9.8 m/s² ≈ 10 m/s² (near Earth)
Units: N
Circular Motion & Gravitation
a_c = (v²)/(r)Centripetal acceleration
a_c = centripetal acceleration, v = speed, r = radius
Units: m/s²
F_c = (mv²)/(r)Centripetal force (net inward force required)
F_c = centripetal force
Units: N
F_g = (Gm_1 m_2)/(r²)Newton's Law of Universal Gravitation
G = 6.67×10⁻¹¹ N·m²/kg², m₁, m₂ = masses, r = distance between centers
Units: N
g = (GM)/(r²)Gravitational field / surface gravity
M = mass of planet, r = distance from center
Units: m/s²
T² = (4π²)/(GM) r³Kepler's Third Law (orbital period)
T = orbital period, r = orbital radius, M = mass of central body
Units: T: s, r: m
Energy
W = Fd\cosθWork done by a constant force
W = work, F = force magnitude, d = displacement, θ = angle between F and d
Units: J
KE = (1)/(2)mv²Kinetic energy
KE = kinetic energy, m = mass, v = speed
Units: J
PE_g = mghGravitational potential energy
h = height above reference point
Units: J
PE_spring = (1)/(2)kx²Elastic potential energy (spring)
k = spring constant, x = compression/stretch from equilibrium
Units: J
P = (W)/(t) = FvPower
P = power, W = work, t = time
Units: W (watts)
W_net = Δ KEWork-Energy Theorem
W_net = net work done on object, ΔKE = change in kinetic energy
Units: J
Momentum & Impulse
p = mvLinear momentum
p = momentum, m = mass, v = velocity
Units: kg·m/s
J = FΔ t = Δ pImpulse-Momentum Theorem
J = impulse, F = average force, Δt = time interval, Δp = change in momentum
Units: N·s = kg·m/s
p_total = constant (isolated system)Conservation of Momentum
Valid when net external force = 0
Units: kg·m/s
Simple Harmonic Motion
T_spring = 2π√((m)/(k))Period of a mass-spring system
T = period, m = mass, k = spring constant
Units: s
T_pendulum = 2π√((L)/(g))Period of a simple pendulum (small angles)
L = pendulum length, g = gravitational field
Units: s
x = A\cos\left((2π t)/(T)\right)Position in SHM (released from amplitude)
x = position, A = amplitude, T = period
Units: m
v_max = A√((k)/(m))Maximum speed (at equilibrium)
v_max = maximum speed, A = amplitude
Units: m/s
E = (1)/(2)kA²Total mechanical energy in SHM
E = total energy, k = spring constant, A = amplitude
Units: J
Torque & Rotational Motion
τ = rF\sinθTorque
τ = torque, r = lever arm length, F = force, θ = angle between r and F
Units: N·m
Σ τ = IαNewton's Second Law for Rotation
Στ = net torque, I = rotational inertia (moment of inertia), α = angular acceleration
Units: N·m
L = IωAngular momentum
L = angular momentum, I = rotational inertia, ω = angular velocity
Units: kg·m²/s
L = constant (no external torque)Conservation of Angular Momentum
Valid when net external torque = 0
Units: kg·m²/s
I_point = mr²Rotational inertia of a point mass
I = moment of inertia, m = mass, r = distance from axis
Units: kg·m²
Electric Charge & Force
F_E = (kq_1 q_2)/(r²)Coulomb's Law (electric force between charges)
F_E = electric force, k = 9×10⁹ N·m²/C², q₁, q₂ = charges, r = separation
Units: N
k = 9 × 10^9 N·m²/C²Coulomb's constant
k = electrostatic constant
Units: N·m²/C²
E = (F)/(q) = (kq)/(r²)Electric field
E = electric field strength, F = force on test charge q
Units: N/C
DC Circuits
V = IROhm's Law
V = voltage (potential difference), I = current, R = resistance
Units: V, A, Ω
P = IV = I² R = (V²)/(R)Electrical power
P = power
Units: W
R_series = R_1 + R_2 + \ldotsResistors in series
Same current through each; voltages add
Units: Ω
(1)/(R_parallel) = (1)/(R_1) + (1)/(R_2) + \ldotsResistors in parallel
Same voltage across each; currents add
Units: Ω
Waves & Sound
v = fλWave speed
v = wave speed, f = frequency, λ = wavelength
Units: v: m/s, f: Hz, λ: m
f_obs = f_src · \fracv ± v_obsv ∓ v_srcDoppler Effect
v = wave speed, v_obs = observer speed, v_src = source speed. Use + for approaching, − for receding
Units: Hz
f_n = (nv)/(2L) (n = 1, 2, 3, \ldots)Standing waves: open tube or string fixed at both ends
f_n = nth harmonic frequency, L = tube/string length
Units: Hz
f_n = (nv)/(4L) (n = 1, 3, 5, \ldots)Standing waves: closed tube (one closed end)
Only odd harmonics; n must be odd
Units: Hz
Important Constants
Gravitational acceleration (near Earth)
g = 9.8 m/s² ≈ 10 m/s²
Universal gravitational constant
G = 6.67 × 10⁻¹¹ N·m²/kg²
Coulomb's constant
k = 9 × 10⁹ N·m²/C²
Speed of sound in air (room temp)
v_sound ≈ 343 m/s
Mass of electron
m_e = 9.11 × 10⁻³¹ kg
Elementary charge
e = 1.6 × 10⁻¹⁹ C
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