Fundamental Laws of Motion to Know for AP Physics C: Mechanics

1. What You Need to Know

You’re being tested on how well you can translate physical situations into Newton’s laws, correctly choose a system, draw a clean free-body diagram (FBD), and write the right equations for translation and rotation. Nearly every Mechanics problem is “just” Newton’s laws + bookkeeping.

The core idea
  • Newton’s laws govern how forces relate to motion.
  • They’re simplest in inertial frames (non-accelerating frames).
  • Most AP Physics C: Mech setups boil down to one of these forms:
    • Translation: Fext=ma\sum \vec{F}_{\text{ext}} = m\vec{a}
    • Momentum form (great for systems): Fext=dpdt\sum \vec{F}_{\text{ext}} = \frac{d\vec{p}}{dt} with p=mv\vec{p}=m\vec{v}
    • Rotation about a fixed axis: τext=Iα\sum \tau_{\text{ext}} = I\alpha
Newton’s Three Laws (what they really mean)
  1. 1st Law (Inertia): If Fext=0\sum \vec{F}_{\text{ext}} = \vec{0}, then v\vec{v} is constant (including rest). This defines inertial frames.
  2. 2nd Law (Dynamics): Net external force produces acceleration: Fext=ma\sum \vec{F}_{\text{ext}} = m\vec{a} (valid for constant mass) or more generally Fext=dpdt\sum \vec{F}_{\text{ext}}=\frac{d\vec{p}}{dt}.
  3. 3rd Law (Action–Reaction): Forces come in pairs on different objects: FAB=FBA\vec{F}_{A\to B}=-\vec{F}_{B\to A}.
Why “system choice” matters
  • For a single object: include all forces on that object.
  • For a system of objects: internal forces cancel in pairs (Newton’s 3rd), so you can often relate motion to external forces only:
    Fext=Macm\sum \vec{F}_{\text{ext}} = M\vec{a}_{\text{cm}}
    where MM is total mass.

Critical reminder: Normal force, tension, and friction are forces (not “equal to” something automatically). They are whatever they need to be to satisfy Newton’s 2nd law + constraints.

2. Step-by-Step Breakdown

This is the high-yield workflow for 90% of force/torque problems.

A. Translational Newton’s Laws (FBD method)
  1. Choose the system

    • One object? A block? A pulley? A whole set of connected masses?
    • Ask: “What forces become internal and cancel if I group things?”
  2. Draw a correct FBD (only forces ON the system)

    • Include: weight W=mg\vec{W}=m\vec{g}, normal N\vec{N}, tension T\vec{T}, friction f\vec{f}, applied forces, spring forces.
    • Do not include “mam\vec{a}” as a force.
  3. Pick axes strategically

    • Align axes with motion/constraints.
    • Common trick: for inclines, use axes parallel/perpendicular to the surface.
  4. Resolve forces into components

    • Example on incline angle θ\theta:
      • Parallel component of weight: mgsinθmg\sin\theta down the slope
      • Perpendicular component: mgcosθmg\cos\theta into the plane
  5. Write Newton’s 2nd law in components

    • For each axis: Fx=max\sum F_x = ma_x, Fy=may\sum F_y = ma_y.
    • If there’s no acceleration perpendicular to a surface: set a=0a_\perp=0.
  6. Add constraint equations (ropes/pulleys/rolling)

    • Ideal rope: same tension throughout (if massless rope, frictionless pulley).
    • Connected masses often share an acceleration magnitude.
    • No slip rolling: vcm=ωRv_{\text{cm}}=\omega R and acm=αRa_{\text{cm}}=\alpha R.
  7. Solve algebraically; sanity-check signs and limits

    • Check limiting cases (frictionless, very large mass, etc.).
Mini worked example (setup only): Block on incline with friction
  • Mass mm on incline angle θ\theta, kinetic friction coefficient μk\mu_k, sliding down.
  • Choose axes: xx down slope, yy perpendicular.
  • Forces:
    • Down slope: mgsinθmg\sin\theta
    • Normal: NN
    • Friction up slope: fk=μkNf_k=\mu_k N
  • Equations:
    • Perpendicular: Fy=0Nmgcosθ=0N=mgcosθ\sum F_y = 0 \Rightarrow N - mg\cos\theta = 0 \Rightarrow N=mg\cos\theta
    • Parallel: Fx=mamgsinθμkmgcosθ=ma\sum F_x = ma \Rightarrow mg\sin\theta - \mu_k mg\cos\theta = ma
    • Result: a=g(sinθμkcosθ)a=g(\sin\theta-\mu_k\cos\theta)
B. Rotational Newton’s Laws (torque method)
  1. Choose axis of rotation (fixed axis or choose a point)
  2. Draw forces and lever arms
  3. Compute torques with sign convention
    • Magnitude: τ=rFsinϕ\tau = rF\sin\phi (where ϕ\phi is angle between r\vec{r} and F\vec{F})
  4. Write τext=Iα\sum \tau_{\text{ext}} = I\alpha
  5. Link translation and rotation if needed
    • Rolling without slipping: a=αRa=\alpha R

Decision point: If the object both translates and rotates (pulley, rolling cylinder), you often need both F=ma\sum F=ma and τ=Iα\sum \tau = I\alpha plus a constraint.

3. Key Formulas, Rules & Facts

A. Newton’s laws and momentum (core statements)
Law / relationFormulaWhen to useNotes
Newton’s 1stFext=0a=0\sum \vec{F}_{\text{ext}}=\vec{0} \Rightarrow \vec{a}=\vec{0}Static equilibrium or constant velocityOnly valid in inertial frames
Newton’s 2nd (constant mass)Fext=ma\sum \vec{F}_{\text{ext}}=m\vec{a}Most particle problemsWrite per axis
Newton’s 2nd (general)Fext=dpdt\sum \vec{F}_{\text{ext}}=\frac{d\vec{p}}{dt}Variable mass or momentum emphasisWith p=mv\vec{p}=m\vec{v}
Newton’s 3rdFAB=FBA\vec{F}_{A\to B}=-\vec{F}_{B\to A}Interaction pairsForces act on different bodies
Center of mass dynamicsFext=Macm\sum \vec{F}_{\text{ext}}=M\vec{a}_{\text{cm}}Multi-particle systemsInternal forces cancel
B. Common forces (models you must know cold)
ForceFormulaDirectionNotes
WeightW=mg\vec{W}=m\vec{g}DownwardNear Earth, g9.8m/s2g\approx 9.8\,\text{m/s}^2
Normal forceN\vec{N}Perpendicular to surfaceNot always mgmg; found via F=ma\sum F_\perp = ma_\perp
Static frictionfsμsNf_s\le \mu_s NOpposes impending relative motionAdjusts up to max value
Kinetic frictionfk=μkNf_k=\mu_k NOpposes relative slidingUse only if sliding
Tension (ideal rope)T\vec{T}Along ropeSame throughout ideal rope
SpringFs=kx\vec{F}_s=-k\vec{x}Toward equilibriumxx measured from equilibrium length
Drag (linear model)Fd=bv\vec{F}_d=-b\vec{v}Opposes velocitySometimes used for terminal speed
Drag (quadratic model)Fd=cvv\vec{F}_d=-c v\vec{v}Opposes velocityMagnitude cv2cv^2

On AP Physics C, friction is the #1 place students silently lose points: always state whether it’s static vs kinetic and whether the object is actually slipping.

C. Equilibrium conditions (translation + rotation)
SituationConditionsNotes
Translational equilibriumF=0\sum \vec{F}=\vec{0}Implies constant velocity (often rest)
Rotational equilibrium (rigid body)τ=0\sum \tau=0Choose convenient pivot to kill unknown torques
Full static equilibriumF=0\sum \vec{F}=\vec{0} and τ=0\sum \tau=0Both must hold
D. Torque and rotational dynamics essentials
QuantityFormulaNotes
Torque magnitudeτ=rFsinϕ\tau=rF\sin\phiPerpendicular component does the turning
Rotational Newton’s 2ndτext=Iα\sum \tau_{\text{ext}}=I\alphaAbout fixed axis
Rolling constraintvcm=ωRv_{\text{cm}}=\omega R, acm=αRa_{\text{cm}}=\alpha ROnly for no slip
E. Quick moment of inertia facts (only what you commonly need with τ=Iα\sum\tau=I\alpha)
Object (about central axis)II
HoopI=mR2I=mR^2
Solid disk/cylinderI=12mR2I=\frac{1}{2}mR^2
Solid sphereI=25mR2I=\frac{2}{5}mR^2
Thin rod (center)I=112mL2I=\frac{1}{12}mL^2
Thin rod (end)I=13mL2I=\frac{1}{3}mL^2
Parallel axis theoremI=Icm+Md2I=I_{\text{cm}}+Md^2

4. Examples & Applications

Example 1: Atwood machine (two hanging masses)

Two masses m1m_1 and m2m_2 connected by a light rope over a frictionless pulley. Assume m2>m1m_2>m_1.

Setup (FBD + Newton’s 2nd):

  • For m2m_2 (down positive): m2gT=m2am_2g - T = m_2 a
  • For m1m_1 (up positive): Tm1g=m1aT - m_1g = m_1 a

Key insight: Add equations to eliminate TT:
m2gm1g=(m1+m2)aa=(m2m1)gm1+m2m_2g-m_1g=(m_1+m_2)a \Rightarrow a=\frac{(m_2-m_1)g}{m_1+m_2}
Then back-substitute for TT.

Exam variation: If the pulley has rotational inertia, you must add τ=Iα\sum\tau=I\alpha and a=αRa=\alpha R; then tension differs on each side.


Example 2: Elevator apparent weight

Person of mass mm stands on scale in elevator accelerating upward with acceleration aa.

FBD: Forces on person: NN up, mgmg down.

Equation (up positive):
Nmg=maN=m(g+a)N - mg = ma \Rightarrow N = m(g+a)

Key insight: Scale reads NN. If elevator accelerates downward, N=m(ga)N=m(g-a). In free fall, N=0N=0.


Example 3: Block pushed against a wall (static friction trap)

A horizontal force FF pushes a block of mass mm against a vertical wall. Coefficient of static friction μs\mu_s.

FBD:

  • Horizontal: applied FF into wall, normal NN out.
  • Vertical: weight mgmg down, static friction fsf_s up (if not slipping).

Equations:

  • Horizontal equilibrium: FN=0N=FF-N=0 \Rightarrow N=F
  • Vertical equilibrium: fsmg=0fs=mgf_s-mg=0 \Rightarrow f_s=mg
  • Static friction condition: fsμsNmgμsFf_s\le \mu_s N \Rightarrow mg \le \mu_s F

Key insight: Friction is not automatically μsN\mu_s N; it becomes whatever is needed up to the maximum.


Example 4: Rolling down an incline (translation + rotation)

A rigid body (mass mm, radius RR, moment of inertia II about center) rolls without slipping down incline angle θ\theta.

Equations:

  • Translation along slope: mgsinθf=mamg\sin\theta - f = ma
  • Torque about center: fR=IαfR = I\alpha
  • No slip: a=αRa=\alpha R

Eliminate ff and α\alpha:
f=IaR2f=\frac{I a}{R^2}
mgsinθIaR2=maa=gsinθ1+ImR2mg\sin\theta - \frac{I a}{R^2} = ma \Rightarrow a=\frac{g\sin\theta}{1+\frac{I}{mR^2}}

Key insight: Bigger ImR2\frac{I}{mR^2} (more “rotational inertia”) means smaller acceleration.

5. Common Mistakes & Traps

  1. Mixing up Newton’s 3rd law pairs

    • Wrong: Putting action–reaction forces on the same FBD so they cancel.
    • Why wrong: 3rd law pairs act on different objects.
    • Fix: Label forces as FAB\vec{F}_{A\to B}; only include forces acting on your chosen system.
  2. Assuming N=mgN=mg automatically

    • Wrong: Writing N=mgN=mg even on inclines, elevators, or with additional vertical forces.
    • Why wrong: NN comes from F=ma\sum F_\perp = ma_\perp.
    • Fix: Always write the perpendicular/vertical Newton’s 2nd equation first.
  3. Using f=μNf=\mu N without checking static vs kinetic

    • Wrong: Replacing friction with μsN\mu_s N in static problems.
    • Why wrong: Static friction satisfies fsμsNf_s\le \mu_s N; it’s only equal at the threshold of slipping.
    • Fix: Solve for required fsf_s, then check if it exceeds μsN\mu_s N.
  4. Sign errors from sloppy axis choices

    • Wrong: Taking “down the incline” as positive for one mass and negative for the other without consistent constraints.
    • Why wrong: You’ll get contradictory accelerations/tensions.
    • Fix: Define one positive direction per object but relate them with a clear constraint (e.g., same magnitude aa).
  5. Forgetting that tension can differ with massive pulleys

    • Wrong: Assuming same TT on both sides when the pulley has rotational inertia.
    • Why wrong: Net torque requires ΔT0\Delta T \neq 0: τ=(T2T1)R=Iα\sum\tau=(T_2-T_1)R=I\alpha.
    • Fix: Use T1T_1 and T2T_2 separately when pulleys are not ideal.
  6. Treating centripetal force as an extra force

    • Wrong: Adding a “centripetal force” term in the FBD.
    • Why wrong: “Centripetal” describes the net inward force requirement: Fr=mv2r\sum F_r = m\frac{v^2}{r}.
    • Fix: Draw real forces (tension, normal, gravity) and set their radial sum equal to mv2rm\frac{v^2}{r}.
  7. Dropping torque signs or wrong lever arm

    • Wrong: Using τ=rF\tau=rF with the full force when only a component is perpendicular.
    • Why wrong: Only perpendicular component contributes: τ=rFsinϕ\tau=rF\sin\phi.
    • Fix: Identify the perpendicular component or use τ=F\tau=F\ell with moment arm \ell.
  8. Using rolling constraints when slipping occurs

    • Wrong: Applying a=αRa=\alpha R even when kinetic friction is present and slipping happens.
    • Why wrong: That constraint is only for pure rolling.
    • Fix: If slipping, relate translation and rotation through dynamics only (and use fk=μkNf_k=\mu_k N).

6. Memory Aids & Quick Tricks

Trick / mnemonicWhat it helps you rememberWhen to use it
System firstDecide what forces are external vs internalMulti-object setups (pulleys, blocks)
FBD = forces ON, not forces BYPrevents Newton’s 3rd law confusionAny diagram
Static friction is whatever it needs (up to max)fsμsNf_s\le\mu_s N, not always equalResting blocks, impending motion
Kill torques with a smart pivotChoose pivot so unknown forces pass through itStatics / rigid body equilibrium
Radial equation is the centripetal requirementFr=mv2r\sum F_r=m\frac{v^2}{r} (not an extra force)Circular motion
Rolling: 3 equationsF=ma\sum F=ma, τ=Iα\sum\tau=I\alpha, a=αRa=\alpha RRolling without slipping

7. Quick Review Checklist

  • You can state and apply Newton’s laws, especially Fext=ma\sum \vec{F}_{\text{ext}}=m\vec{a} and FAB=FBA\vec{F}_{A\to B}=-\vec{F}_{B\to A}.
  • You always start with a system choice and a clean FBD (only real forces on the system).
  • You write Newton’s 2nd law in components aligned with constraints.
  • You treat friction correctly: fk=μkNf_k=\mu_k N when sliding, fsμsNf_s\le\mu_s N when not.
  • You don’t assume N=mgN=mg unless the perpendicular/vertical equation says so.
  • For connected masses, you add the constraint that accelerations match (and handle pulley inertia if present).
  • For rotation, you can compute torque with τ=rFsinϕ\tau=rF\sin\phi and apply τ=Iα\sum\tau=I\alpha.
  • For rolling without slipping, you remember the trio: F=ma\sum F=ma, τ=Iα\sum\tau=I\alpha, a=αRa=\alpha R.

You’ve got this—if your FBD and sign conventions are clean, the algebra almost always falls into place.