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AP Physics 1 Last-Minute Review (Night Before)

The night-before checklist: top formulas, common traps, and what NOT to do.

⏱️ ~45 minutes to skim⚛️ AP Physics 1

The exam is tomorrow. This is not the time to learn new content — it's the time to skim, reset, and sleep. Spend 30–45 minutes on this page, then put your notes away.


Must-Know Kinematics

ScenarioEquation
Constant accelerationv=v0+atv = v_0 + at
DisplacementΔx=v0t+12at2\Delta x = v_0 t + \frac{1}{2}at^2
Velocity-independentv2=v02+2aΔxv^2 = v_0^2 + 2a\Delta x
Projectile: horizontalvx=v0cos⁡θv_x = v_0 \cos\theta (constant)
Projectile: verticalvy=v0sin⁡θ−gtv_y = v_0 \sin\theta - gt

Graphical kinematics: Slope of xx vs tt = velocity. Slope of vv vs tt = acceleration. Area under vv vs tt = displacement.


Must-Know Dynamics

ConceptFormula
Newton's 2nd lawΣF=ma\Sigma F = ma
WeightFg=mgF_g = mg
Normal force (horizontal)N=mgN = mg
Normal force (incline)N=mgcos⁡θN = mg\cos\theta
Friction (kinetic)fk=μkNf_k = \mu_k N
Friction (max static)fs≤μsNf_s \leq \mu_s N
TensionTT (from ΣF=ma\Sigma F = ma)

Incline setup:

  • Parallel to surface: mgsin⁡θ−f=mamg\sin\theta - f = ma
  • Perpendicular: N=mgcos⁡θN = mg\cos\theta

FBD non-negotiable: Draw it for every force problem. No FBD = no justification = lost points.


Must-Know Energy & Work

ConceptFormula
Kinetic energyKE=12mv2KE = \frac{1}{2}mv^2
Gravitational PEPE=mghPE = mgh
Spring PEPEs=12kx2PE_s = \frac{1}{2}kx^2
WorkW=F⋅dcos⁡θW = F \cdot d \cos\theta
Work-energy theoremWnet=ΔKEW_{\text{net}} = \Delta KE
PowerP=WtP = \frac{W}{t} (watts)
Energy conservationEinitial=EfinalE_{\text{initial}} = E_{\text{final}}

Highest-leverage rule: If a problem mentions height or spring compression, reach for energy conservation immediately.


Must-Know Momentum & Collisions

ConceptFormula
Momentump=mvp = mv (vector)
ImpulseJ=FΔt=ΔpJ = F\Delta t = \Delta p
Impulse-momentum theoremF⃗Δt=mΔv\vec{F}\Delta t = m\Delta v
Conservation of momentump⃗before=p⃗after\vec{p}_{\text{before}} = \vec{p}_{\text{after}}
Elastic collisionKEKE conserved, pp conserved
Inelastic collisionKEKE not conserved, pp conserved

Collision identification: Always calculate KEKE before and after. If equal, collision is elastic. If not, inelastic.


Must-Know Rotation

ConceptFormula
Torqueτ=rFsin⁡θ\tau = rF\sin\theta (perpendicular distance)
Rotational dynamicsΣτ=Iα\Sigma \tau = I\alpha
Rotational kinematicsω=ω0+αt\omega = \omega_0 + \alpha t
Rotational KEKErot=12Iω2KE_{\text{rot}} = \frac{1}{2}I\omega^2
Angular momentumL=IωL = I\omega
Conservation: LLLbefore=LafterL_{\text{before}} = L_{\text{after}} (when τnet=0\tau_{\text{net}} = 0)

Critical reminder: sin⁡θ\sin\theta in τ=rFsin⁡θ\tau = rF\sin\theta is the angle between force and the lever arm. sin⁡θ≠cos⁡θ\sin\theta \neq \cos\theta.


Must-Know Oscillations

ConceptFormula
SHM displacementx(t)=Acos⁡(ωt+ϕ)x(t) = A\cos(\omega t + \phi)
Spring periodT=2πmkT = 2\pi\sqrt{\frac{m}{k}}
Spring frequencyf=1T=12πkmf = \frac{1}{T} = \frac{1}{2\pi}\sqrt{\frac{k}{m}}
Pendulum periodT=2πLgT = 2\pi\sqrt{\frac{L}{g}}
Max velocity in SHMvmax=Aωv_{\text{max}} = A\omega
Max accelerationamax=Aω2a_{\text{max}} = A\omega^2
Energy: spring oscillatorEtotal=12kA2E_{\text{total}} = \frac{1}{2}kA^2

Pendulum key: Period depends on LL and gg, not on mass. This is tested every year.


Must-Know Fluids (Lower-Yield, Skim)

ConceptFormula
Densityρ=mV\rho = \frac{m}{V}
PressureP=FAP = \frac{F}{A}
Hydrostatic pressureP=P0+ρghP = P_0 + \rho g h
Buoyant forceFB=ρfluidVdispgF_B = \rho_{\text{fluid}} V_{\text{disp}} g
ContinuityA1v1=A2v2A_1 v_1 = A_2 v_2 (flow rate)
Bernoulli (skim, rarely tested)P+12ρv2+ρgh=constP + \frac{1}{2}\rho v^2 + \rho g h = \text{const}

The Free Body Diagram Checklist

Do this for every force problem:

  • ☐ Draw the object as a dot or box.
  • ☐ Draw all forces acting on the object (not forces it exerts).
  • ☐ Label each force: NN, FgF_g or mgmg, ff, TT, FappliedF_{\text{applied}}.
  • ☐ If on an incline, resolve weight into mgsin⁡θmg\sin\theta (parallel) and mgcos⁡θmg\cos\theta (perpendicular).
  • ☐ Include a coordinate system (+x, +y).
  • ☐ Don't draw action-reaction pairs; focus on the system you're analyzing.

The sin⁡θ\sin\theta vs cos⁡θ\cos\theta trap:

  • Weight component down the incline (parallel): mgsin⁡θmg\sin\theta
  • Weight component into the incline (perpendicular): mgcos⁡θmg\cos\theta
  • Normal force: N=mgcos⁡θN = mg\cos\theta

The Conservation Laws Cheatsheet

Conservation of Mechanical Energy

KEi+PEi=KEf+PEfKE_i + PE_i = KE_f + PE_f

(Applies when no friction or air resistance; not true for inelastic collisions)

Conservation of Momentum

p⃗i=p⃗form1v1+m2v2=m1v1′+m2v2′\vec{p}_i = \vec{p}_f \quad \text{or} \quad m_1 v_1 + m_2 v_2 = m_1 v_1' + m_2 v_2'

(Always true for collisions; direction matters because it's a vector)

Conservation of Angular Momentum

Li=LforIiωi=IfωfL_i = L_f \quad \text{or} \quad I_i \omega_i = I_f \omega_f

(Applies when net external torque = 0; classic: spinning ice skater pulling in arms increases ω\omega)


The Top 12 Traps (That Cost Real Points)

  1. Forgetting normal force on an incline. On an incline, N=mgcos⁡θN = mg\cos\theta, not mgmg. This trips up 30% of students.
  2. Confusing sin⁡θ\sin\theta and cos⁡θ\cos\theta for weight components. Down the slope: sin⁡θ\sin\theta. Into the slope: cos⁡θ\cos\theta.
  3. Forgetting friction acts opposite to motion. If the block slides down, friction points up the slope.
  4. Momentum is a vector. If a cart is moving left (negative), its momentum is negative. Collisions can have cancellation.
  5. Kinetic energy is always positive (no direction). KE=12mv2KE = \frac{1}{2}m v^2 uses speed, not velocity.
  6. Using KE formula with velocity squared. If v=−10 m/sv = -10\text{ m/s}, then v2=100 m2/s2v^2 = 100\text{ m}^2/\text{s}^2 (positive).
  7. Forgetting 12\frac{1}{2} in kinetic energy, spring PE, or rotational KE. It's a coefficient; it matters.
  8. Energy conservation vs. momentum conservation. Elastic collisions conserve both. Inelastic: momentum always, energy never.
  9. Pendulum period is independent of mass. T=2πL/gT = 2\pi\sqrt{L/g} doesn't include mm.
  10. Tension is not "how hard you pull." It's the force transmitted through a rope, found via ΣF=ma\Sigma F = ma for the system.
  11. Forgetting sin⁡θ\sin\theta is the perpendicular angle in torque. τ=rFsin⁡θ\tau = rF\sin\theta where θ\theta is between r⃗\vec{r} and F⃗\vec{F}.
  12. Missing units on final answers. "10" earns partial credit. "10 meters" earns full credit.

Score Boundaries (Recent Years)

Out of 200 points total:

ScoreApprox. PointsNotes
5140+~70%
4112–139~56–70%
384–111~42–55%
260–83~30–41%
1Below 60~Below 30%

Bottom line: You need about 70% correct to score a 5. You can leave some problems blank or partially wrong and still get the top score.


Morning-of Checklist

  • ☐ 8 hours of sleep (non-negotiable).
  • ☐ Real breakfast: protein + slow carbs (eggs, oatmeal, whole wheat toast). Not just coffee and pastry.
  • ☐ 2 sharpened #2 pencils + erasers, blue/black pen (for FRQs).
  • ☐ Graphing calculator (TI-83+ or TI-84 or equivalent) + 2 extra AA batteries.
  • ☐ Photo ID + AP ID label sheet.
  • ☐ Water bottle (unflavored water only).
  • ☐ Snack for the break (banana, granola bar).
  • ☐ Watch without an alarm (if room doesn't have a clock).
  • ☐ Arrive 30 minutes early.

During the Exam: Section I (MCQ, 90 min)

First 30 min (no calculator):

  • Mark any question that takes >90 seconds; skip and come back.
  • Don't overthink. Wrong answers are usually sign errors or unit conversions gone wrong.
  • Guess if you skip—no penalty for wrong answers on AP Physics 1.

Next 60 min (calculator allowed):

  • Calculator-active questions usually involve numerical integration, graph interpretation, or multi-step algebra.
  • Use nDeriv() and fnInt() sparingly; often the algebraic setup is clearer.
  • Double-check one calculation per problem (e.g., "Is that really 12×1600×0.25=200\frac{1}{2} \times 1600 \times 0.25 = 200?").

During the Exam: Section II (FRQs, 90 min)

  1. Read all 5 questions first (5 min). Which are you most confident on? Start there.

  2. FBD before calculation. If stuck, draw it. Clarity often follows.

  3. FRQ structure:

    • Read and annotate the question (underline what's given, what's asked).
    • Set up the physics (equation or principle).
    • Solve.
    • Check units and reasonableness (does the answer make physical sense?).
  4. "Explain" or "justify" = CER.

    • Claim: State your answer clearly.
    • Evidence: Show the math (numerical values).
    • Reasoning: Explain why the evidence supports the claim using physics principles by name.
  5. Partial credit is real. If you can't solve part (a), use a placeholder value for part (b). You'll earn setup points.

  6. Don't leave blanks. Write something. Write the integral. Write the variables you'd solve for. Partial credit beats zero.


One Last Thing

You've prepared. The work is done. Trust it.

Show up rested. Breathe. Draw your free body diagrams. State the physics principle by name. Check your algebra. Include units.

The rubric wants to give you points — your job is to write clearly enough that it can.

Good luck. You've got this. 🎯


Need more help? Browse the AP Physics 1 topic library → or revisit the FRQ practice guide → or 7-day plan →.

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