Skip to content
🎯⭐ INTERACTIVE LESSON

Physics: Mechanics

Learn step-by-step with interactive practice!

Physics: Mechanics - Complete Interactive Lesson

Part 1: Kinematics & Motion

Physics: Mechanics for the MCAT

Part 1 of 7 — Kinematics

The Big 5 Kinematic Equations

v=v0+atv = v_0 + at

Δx=v0t+12at2\Delta x = v_0 t + \tfrac{1}{2}at^2

v2=v02+2aΔxv^2 = v_0^2 + 2a\Delta x

Δx=12(v0+v)t\Delta x = \tfrac{1}{2}(v_0 + v)t

Δx=vt−12at2\Delta x = vt - \tfrac{1}{2}at^2

Projectile Motion

  • Horizontal: ax=0a_x = 0, so vx=v0cos⁡θv_x = v_0\cos\theta is constant
  • Vertical: ay=−g=−9.8  m/s2a_y = -g = -9.8\;\text{m/s}^2
  • Time to reach max height: t=v0sin⁡θgt = \frac{v_0\sin\theta}{g}
  • Range: R=v02sin⁡(2θ)gR = \frac{v_0^2\sin(2\theta)}{g} (maximum at 45°45°)

MCAT Tip: Free Fall

All objects fall at the same rate regardless of mass (ignoring air resistance). Use g≈10  m/s2g \approx 10\;\text{m/s}^2 for quick calculations on the MCAT.

Relative Motion Shortcut

In one-dimensional motion, use relative velocity directly: vA/B=vA−vBv_{A/B} = v_A - v_B. This simplifies chase and meeting-time questions.

Worked Example — Horizontal Projectile off a Cliff

A ball rolls off a 20  m20\;\text{m} high table with a horizontal speed of 5  m/s5\;\text{m/s}. Using g=10  m/s2g = 10\;\text{m/s}^2, how long is it in the air and how far does it land from the base?

Step 1 — Treat the vertical motion separately. The initial vertical velocity is zero, so

Δy=12gt2⇒20=12(10)t2=5t2\Delta y = \tfrac{1}{2} g t^2 \Rightarrow 20 = \tfrac{1}{2}(10) t^2 = 5 t^2

Step 2 — Solve for the time of flight.

t2=205=4⇒t=2  st^2 = \frac{20}{5} = 4 \Rightarrow t = 2\;\text{s}

Step 3 — Use the horizontal motion (constant velocity).

x=vxt=(5)(2)=10  mx = v_x t = (5)(2) = 10\;\text{m}

The ball lands 10  m10\;\text{m} from the base after 2  s2\;\text{s}. Key MCAT insight: the horizontal speed has NO effect on the fall time — vertical and horizontal motions are independent.

Kinematics 🎯

Key Takeaways — Part 1

  • Use g≈10  m/s2g \approx 10\;\text{m/s}^2 for fast MCAT calculations
  • Projectile motion: split into x (constant velocity) and y (constant acceleration); they are independent
  • Complementary angles give the same range; 45°45° gives the maximum range
  • Relative-velocity problems often reduce to a single subtraction when set up correctly

Part 2: Forces & Newtons Laws

Physics: Mechanics for the MCAT

Part 2 of 7 — Newton's Laws & Forces

Newton's Three Laws

  1. Inertia: an object at rest stays at rest, and an object in motion stays in motion, unless acted on by a net force
  2. F=maF = ma: net force equals mass times acceleration
  3. Action-Reaction: every force has an equal and opposite force on a DIFFERENT object

Common MCAT Forces

ForceFormulaDirection
WeightW=mgW = mgDownward
NormalNN (variable)Perpendicular to the surface
Friction (static)fs≤μsNf_s \le \mu_s NOpposes potential motion
Friction (kinetic)fk=μkNf_k = \mu_k NOpposes actual motion
TensionTT (variable)Along the string
SpringF=−kxF = -kxRestoring (toward equilibrium)

Inclined Plane (MCAT FAVORITE)

  • Component along the plane: mgsin⁡θmg\sin\theta
  • Component perpendicular: mgcos⁡θmg\cos\theta (equals the normal force if no other vertical forces)
  • Friction on an incline: f=μmgcos⁡θf = \mu mg\cos\theta

Force-Analysis Workflow

  1. Isolate one object.
  2. Draw every real force (weight, normal, tension, friction, applied).
  3. Choose axes along the likely motion.
  4. Write ∑F=ma\sum F = ma per axis.

Worked Example — Block on a Rough Incline

A 4  kg4\;\text{kg} block sits on a 30°30° incline with kinetic friction coefficient μk=0.20\mu_k = 0.20. Using g=10  m/s2g = 10\;\text{m/s}^2, find its acceleration down the slope once it is sliding.

Step 1 — Force pulling it down the plane.

F∥=mgsin⁡θ=(4)(10)sin⁡30°=40×0.5=20  NF_{\parallel} = mg\sin\theta = (4)(10)\sin 30° = 40 \times 0.5 = 20\;\text{N}

Step 2 — Normal force and friction.

N=mgcos⁡θ=(4)(10)cos⁡30°≈40×0.87=34.6  NN = mg\cos\theta = (4)(10)\cos 30° \approx 40 \times 0.87 = 34.6\;\text{N}, so

fk=μkN=(0.20)(34.6)≈6.9  Nf_k = \mu_k N = (0.20)(34.6) \approx 6.9\;\text{N}

Step 3 — Net force along the plane, then Newton's second law.

Fnet=20−6.9=13.1  NF_{net} = 20 - 6.9 = 13.1\;\text{N}, and a=Fnetm=13.14≈3.3  m/s2a = \frac{F_{net}}{m} = \frac{13.1}{4} \approx 3.3\;\text{m/s}^2

Notice friction opposes the motion (subtracts), and the mass appears in both terms — when friction is absent it cancels entirely, leaving a=gsin⁡θa = g\sin\theta.

Forces & Newton's Laws 🎯

Key Takeaways — Part 2

  • Fnet=maF_{net} = ma: always draw a free-body diagram first
  • Incline: mgsin⁡θmg\sin\theta along the plane, mgcos⁡θmg\cos\theta perpendicular
  • Elevator problems: apparent weight =m(g±a)= m(g \pm a)
  • Static friction is a maximum (fs≤μsNf_s \le \mu_s N); kinetic friction is exact (fk=μkNf_k = \mu_k N)
  • If the speed is constant, the net force is zero even when several forces act

Part 3: Work, Energy & Power

Physics: Mechanics for the MCAT

Part 3 of 7 — Work, Energy & Power

Work-Energy Theorem

Wnet=ΔKE=12mv2−12mv02W_{net} = \Delta KE = \tfrac{1}{2}mv^2 - \tfrac{1}{2}mv_0^2

W=Fdcos⁡θW = Fd\cos\theta (only the force component along the displacement does work)

Conservation of Energy

KEi+PEi=KEf+PEfKE_i + PE_i = KE_f + PE_f (when no non-conservative forces act)

  • Kinetic energy: KE=12mv2KE = \tfrac{1}{2}mv^2
  • Gravitational PE: PE=mghPE = mgh
  • Spring PE: PE=12kx2PE = \tfrac{1}{2}kx^2

Power

P=Wt=FvP = \frac{W}{t} = Fv — measured in watts (W), where 1  W=1  J/s1\;\text{W} = 1\;\text{J/s}

Conservative vs. Non-conservative Forces

  • Conservative (gravity, springs): path-independent work; mechanical energy is conserved
  • Non-conservative (friction, drag): convert mechanical energy into thermal/internal energy

When friction is present, include the non-conservative work in the energy balance.

Worked Example — Speed at the Bottom of a Ramp

A 2  kg2\;\text{kg} cart starts from rest at the top of a frictionless ramp 1.8  m1.8\;\text{m} tall. Using g=10  m/s2g = 10\;\text{m/s}^2, find its speed at the bottom.

Step 1 — Set up conservation of energy. All gravitational PE converts to kinetic energy:

mgh=12mv2mgh = \tfrac{1}{2}mv^2

Step 2 — Cancel the mass and solve for vv.

v=2gh=2(10)(1.8)=36v = \sqrt{2gh} = \sqrt{2(10)(1.8)} = \sqrt{36}

Step 3 — Evaluate.

v=6  m/sv = 6\;\text{m/s}

The mass dropped out, which is why v=2ghv = \sqrt{2gh} is worth memorizing. If friction did, say, 10  J10\;\text{J} of negative work, you would instead write mgh−10=12mv2mgh - 10 = \tfrac{1}{2}mv^2 and solve for a smaller speed.

Work & Energy 🎯

Key Takeaways — Part 3

  • W=Fdcos⁡θW = Fd\cos\theta: only the force component parallel to displacement does work
  • Conservation of energy: KE+PE=constantKE + PE = \text{constant} when no friction or drag acts
  • v=2ghv = \sqrt{2gh} for an object dropped (or sliding) from height hh — memorize this shortcut
  • Power = work / time = force ×\times velocity
  • KE∝v2KE \propto v^2: doubling speed quadruples kinetic energy
  • Friction does negative work and reduces mechanical energy

Part 4: Momentum & Collisions

Physics: Mechanics for the MCAT

Part 4 of 7 — Momentum & Collisions

Linear Momentum

p⃗=mv⃗\vec{p} = m\vec{v} — a vector quantity (units: kg⋅m/s\text{kg}\cdot\text{m/s})

Impulse-Momentum Theorem

J⃗=F⃗Δt=Δp⃗\vec{J} = \vec{F}\Delta t = \Delta\vec{p} — a force applied over time changes momentum

Conservation of Momentum

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

Total momentum is always conserved in the absence of external forces.

Collision Types

TypeMomentumKinetic Energy
ElasticConservedConserved
InelasticConservedNOT conserved (some lost to heat/deformation)
Perfectly inelasticConservedMaximum KE loss (objects stick together)

For a perfectly inelastic collision: m1v1+m2v2=(m1+m2)vfm_1 v_1 + m_2 v_2 = (m_1 + m_2)v_f

Why Increasing Collision Time Matters

From J=FΔt=ΔpJ = F\Delta t = \Delta p, for a fixed momentum change, increasing Δt\Delta t lowers the average force. This principle explains airbags, padded helmets, and crumple zones.

Worked Example — Impulse Reduces Force

A 0.15  kg0.15\;\text{kg} baseball arrives at 40  m/s40\;\text{m/s} and is caught, coming to rest. Compare the average force on the hand if the catch takes 0.01  s0.01\;\text{s} (rigid hand) versus 0.10  s0.10\;\text{s} (giving with the ball).

Step 1 — Find the momentum change (same for both).

Δp=mΔv=(0.15)(0−40)=−6  kg⋅m/s\Delta p = m\Delta v = (0.15)(0 - 40) = -6\;\text{kg}\cdot\text{m/s} (magnitude 66).

Step 2 — Rigid catch (Δt=0.01  s\Delta t = 0.01\;\text{s}).

F=ΔpΔt=60.01=600  NF = \frac{\Delta p}{\Delta t} = \frac{6}{0.01} = 600\;\text{N}

Step 3 — Soft catch (Δt=0.10  s\Delta t = 0.10\;\text{s}).

F=60.10=60  NF = \frac{6}{0.10} = 60\;\text{N}

Extending the contact time tenfold cuts the average force to one-tenth. This is exactly why you pull your hands back when catching a fast ball — and why airbags save lives.

Momentum 🎯

Key Takeaways — Part 4

  • Momentum is ALWAYS conserved in collisions (absent external forces)
  • KE is ONLY conserved in elastic collisions
  • Perfectly inelastic = objects stick together = maximum KE loss
  • Impulse J=FΔt=ΔpJ = F\Delta t = \Delta p — extending contact time lowers the force (airbags, padding)

Part 5: Fluids & Pressure

Physics: Mechanics for the MCAT

Part 5 of 7 — Fluids (ULTRA HIGH YIELD)

Density & Pressure

ρ=mV\rho = \frac{m}{V} and P=FAP = \frac{F}{A}

Hydrostatic Pressure

P=P0+ρghP = P_0 + \rho g h, where P0P_0 is atmospheric pressure (1  atm≈1.0×105  Pa1\;\text{atm} \approx 1.0 \times 10^5\;\text{Pa})

Pascal's Principle

Pressure applied to a confined fluid is transmitted equally: F1A1=F2A2\frac{F_1}{A_1} = \frac{F_2}{A_2} (the basis of the hydraulic lift)

Archimedes' Principle (Buoyancy)

Fb=ρfluid⋅Vdisplaced⋅gF_b = \rho_{fluid} \cdot V_{displaced} \cdot g

An object floats if ρobject<ρfluid\rho_{object} < \rho_{fluid}.

Bernoulli's Equation (energy conservation for fluids)

P1+12ρv12+ρgh1=P2+12ρv22+ρgh2P_1 + \tfrac{1}{2}\rho v_1^2 + \rho g h_1 = P_2 + \tfrac{1}{2}\rho v_2^2 + \rho g h_2

Continuity Equation

A1v1=A2v2A_1 v_1 = A_2 v_2 — a narrower pipe forces faster flow, which (by Bernoulli) lowers pressure (the Venturi effect)

Flow Rate

Volume flow rate Q=AvQ = Av ties continuity to units (m3/s\text{m}^3/\text{s}) and to physiology passages about blood flow.

Worked Example — Buoyant Force on a Submerged Object

A solid block of volume V=2.0×10−3  m3V = 2.0 \times 10^{-3}\;\text{m}^3 is fully submerged in water (ρfluid=1000  kg/m3\rho_{fluid} = 1000\;\text{kg/m}^3). Using g=10  m/s2g = 10\;\text{m/s}^2, find the buoyant force on it.

Step 1 — Apply Archimedes' principle. Fully submerged means Vdisplaced=VV_{displaced} = V:

Fb=ρfluid⋅Vdisplaced⋅gF_b = \rho_{fluid} \cdot V_{displaced} \cdot g

Step 2 — Substitute the values.

Fb=(1000)(2.0×10−3)(10)F_b = (1000)(2.0 \times 10^{-3})(10)

Step 3 — Evaluate.

Fb=1000×0.002×10=20  NF_b = 1000 \times 0.002 \times 10 = 20\;\text{N}

The buoyant force depends only on the displaced fluid, NOT on the block's own density. To decide whether it floats or sinks, compare this 20  N20\;\text{N} buoyant force with the block's weight mgmg: if the weight is larger, it sinks.

Fluids 🎯

Key Takeaways — Part 5

  • Bernoulli: faster flow → lower pressure (explains aneurysms and airplane lift)
  • Continuity: A1v1=A2v2A_1 v_1 = A_2 v_2 for an incompressible fluid
  • Buoyancy: Fb=ρfluidVdisplacedgF_b = \rho_{fluid} V_{displaced} g; an object floats when ρobject<ρfluid\rho_{object} < \rho_{fluid}
  • Hydrostatic pressure rises with depth: P=P0+ρghP = P_0 + \rho g h
  • Hydraulic lift (Pascal): force multiplies by the area ratio A2/A1A_2/A_1

Part 6: Waves & Sound

Physics: Mechanics for the MCAT

Part 6 of 7 — Torque, Equilibrium & Simple Machines

Torque

τ=rFsin⁡θ\tau = rF\sin\theta

  • rr = distance from the pivot (the lever arm)
  • θ\theta = angle between the lever arm and the force; torque is maximum at θ=90°\theta = 90°
  • Counterclockwise is positive by convention

Equilibrium Conditions

For static equilibrium: ∑F=0\sum F = 0 AND ∑τ=0\sum \tau = 0

Center of Mass

xcm=∑mixi∑mix_{cm} = \frac{\sum m_i x_i}{\sum m_i}

Simple Machines

  • Lever: F1d1=F2d2F_1 d_1 = F_2 d_2 (mechanical advantage)
  • Pulley: redirects force; compound pulleys multiply force
  • Inclined plane: reduces the force needed but increases the distance

Key principle: machines reduce force but NEVER reduce work (W=FdW = Fd is conserved).

Pivot Choice Strategy

Choose a pivot that eliminates an unknown force (often a support point) so the torque equation simplifies quickly.

Worked Example — Balancing a Seesaw

A child of weight 300  N300\;\text{N} sits 2.0  m2.0\;\text{m} left of a seesaw's pivot. Where must a 400  N400\;\text{N} child sit on the right to balance it?

Step 1 — Write the rotational equilibrium condition. For balance the counterclockwise and clockwise torques are equal:

τleft=τright⇒F1d1=F2d2\tau_{left} = \tau_{right} \Rightarrow F_1 d_1 = F_2 d_2

Step 2 — Plug in the known values.

(300)(2.0)=(400)(d2)(300)(2.0) = (400)(d_2)

Step 3 — Solve for the distance.

d2=600400=1.5  md_2 = \frac{600}{400} = 1.5\;\text{m}

The heavier child sits closer to the pivot (1.5  m1.5\;\text{m} vs. 2.0  m2.0\;\text{m}). This is the lever balance condition F1d1=F2d2F_1 d_1 = F_2 d_2 — a staple of MCAT torque questions.

Torque & Equilibrium 🎯

Key Takeaways — Part 6

  • Torque τ=rFsin⁡θ\tau = rF\sin\theta; maximum when the force is perpendicular to the lever arm
  • Equilibrium: ∑F=0\sum F = 0 AND ∑τ=0\sum \tau = 0 (you may choose any pivot point)
  • Lever balance: F1d1=F2d2F_1 d_1 = F_2 d_2 — the heavier side sits closer to the pivot
  • Simple machines trade force for distance; work is conserved
  • The MCAT loves beam and seesaw problems — practice them

Part 7: Review & MCAT Practice

Physics: Mechanics for the MCAT

Part 7 of 7 — Waves & Sound

Wave Properties

v=fλv = f\lambda and period T=1fT = \frac{1}{f}

  • Transverse: oscillation perpendicular to propagation (light, waves on a string)
  • Longitudinal: oscillation parallel to propagation (sound)

Sound

  • Speed in air: ≈340  m/s\approx 340\;\text{m/s} (faster in denser media such as water and solids)
  • Intensity: I=P4πr2I = \frac{P}{4\pi r^2} (an inverse-square law)
  • Decibels: β=10log⁡(I/I0)\beta = 10\log(I/I_0) where I0=10−12  W/m2I_0 = 10^{-12}\;\text{W/m}^2
  • Every 10  dB10\;\text{dB} increase corresponds to a 10×10\times increase in intensity

Doppler Effect

f′=fv±vobserverv∓vsourcef' = f\frac{v \pm v_{observer}}{v \mp v_{source}}

  • Source approaching → higher observed frequency (higher pitch)
  • Source receding → lower observed frequency

Standing Waves

  • Both ends fixed: λn=2Ln\lambda_n = \frac{2L}{n}, fn=nv2Lf_n = n\frac{v}{2L}
  • One end open: λn=4Ln\lambda_n = \frac{4L}{n}, with only odd harmonics (n=1,3,5,...n = 1, 3, 5, ...)

For a fixed source frequency, wavelength changes with the medium because λ=v/f\lambda = v/f and the wave speed depends on the medium.

Worked Example — Decibel Change from Intensity

A sound's intensity increases from I1=10−6  W/m2I_1 = 10^{-6}\;\text{W/m}^2 to I2=10−3  W/m2I_2 = 10^{-3}\;\text{W/m}^2. By how many decibels does the sound level rise?

Step 1 — Use the decibel difference formula.

Δβ=10log⁡ ⁣(I2I1)\Delta\beta = 10\log\!\left(\frac{I_2}{I_1}\right)

Step 2 — Take the ratio.

I2I1=10−310−6=103\frac{I_2}{I_1} = \frac{10^{-3}}{10^{-6}} = 10^{3}

Step 3 — Evaluate the logarithm.

Δβ=10log⁡(103)=10×3=30  dB\Delta\beta = 10\log(10^{3}) = 10 \times 3 = 30\;\text{dB}

Each factor of 10 in intensity adds 10  dB10\;\text{dB}, so a 1000×1000\times jump is +30  dB+30\;\text{dB}. The decibel scale is logarithmic — a useful reminder that small dB changes hide large intensity changes.

Waves & Sound 🎯

Physics Mechanics — Complete! ✅

Key relationships: v=fλv = f\lambda, the Doppler effect, and the inverse-square law for intensity. Sound travels FASTER in denser media (the opposite of light). Decibels are logarithmic, so +10  dB+10\;\text{dB} means 10×10\times the intensity. Standing-wave harmonics depend on the boundary conditions (both ends fixed vs. one end open).