📐
SEC 2027 · G3 SEC 3 Combined Physics

Sec 3 Combined Physics
Visual Notes

Pictures first. Formulas boxed. Every exam keyword highlighted.
HOW TO STUDY WITH THIS
Read the 💡 box
the whole topic in 1 line
Study the diagram
cover it, redraw it
Learn the yellow
formulas & keywords
Redo the worked example
without looking
THE CHAPTERS
📏
CH 1
Physical Quantities, Units & Measurement
SI units
🏎️
CH 2
Kinematics
speed
🧲
CH 3
Forces, Mass, Weight & Density
W = mg
🚀
CH 4
Dynamics
F = ma
⚖️
CH 5
Turning Effects of Forces
moments
⚡
CH 6
Energy, Work & Power
stores
🫧
CH 7
Kinetic Particle Model of Matter
states
🔥
CH 8
Thermal Processes
conduction
📌 NOTESchools split Sec 3 / Sec 4 physics differently — check the other year if a chapter is missing.
🖨 PRINTCtrl+P → Save as PDF · Scale 100% · Margins None · Background graphics ON
Sec 3 Combined Physics · SEC K326
📏
1

Physical Quantities, Units & Measurement

SI units, prefixes, instruments, scalars & vectors
BIG IDEAEvery physical quantity = number + unit. Use SI units and pick the instrument with the right range and precision.
Base quantitySI unit
masskilogram (kg)
lengthmetre (m)
timesecond (s)
currentampere (A)
temperaturekelvin (K)
amount of substancemole (mol)
Prefix×
T tera10¹²
G giga10⁹
M mega10⁶
k kilo10³
c centi10⁻²
m milli10⁻³
µ micro10⁻⁶
n nano10⁻⁹
InstrumentPrecisionUse for
metre rule0.1 cmlengths 10 cm–1 m
measuring tape0.1 cmlong distances
stopwatch0.01 s (but reaction ≈ 0.2 s)time — time many oscillations
electronic balance0.01 gmass
Scalar vs vector
scalar: size only — distance, speed, mass, time, energy
vector: size + direction — displacement, velocity, acceleration, force
📏 Orders of magnitude
atom ≈ 10⁻¹⁰ m · cell ≈ 10⁻⁵ m · human ≈ 1 m · Earth ≈ 10⁷ m
⚠ TRAPRead scales with your eye perpendicular to the scale to avoid parallax error; check for zero error.
🔎 WHY IT WORKSWhy time 20 swings, not 1: your reaction time error (~0.2 s) is the same whether you time 1 swing or 20. Spread over 20 swings, the error per swing becomes 20× smaller.
🧠 Worked example — follow the thinking
Convert 450 mA to A and 2.5 km to m.
StepWhy I do this
m = 10⁻³ → 450 × 10⁻³ = 0.45 A💭 Replace the prefix with its power of 10.
k = 10³ → 2.5 × 10³ = 2500 m💭 Same idea: kilo means × 1000.
Sec 3 Combined Physics · SEC K326
🏎️
2

Kinematics

speed, velocity, acceleration, motion graphs
BIG IDEAspeed = distance ÷ time · a = (v − u) ÷ t · gradient and area on graphs tell you everything.
tssteady speedat rest
distance–time: gradient = speed
tvaccelconstant vdecel
speed–time: gradient = acceleration, area = distance
Graph shapeDistance–timeSpeed–time
horizontal lineat restconstant speed
straight slope upconstant speedconstant acceleration
curve getting steeperspeeding upincreasing acceleration
line going down(moving back)decelerating
Definitions
speed: distance per unit time (m/s)
velocity: speed in a stated direction
acceleration: change in velocity per unit time (m/s²)
🪂 Free fall
no air resistance → all objects fall with the same acceleration g ≈ 10 m/s², whatever their mass
🔎 WHY IT WORKSWhy area under v–t = distance: for a constant speed, distance = speed × time — that is the area of a rectangle under the line. Any shape can be split into rectangles and triangles, so the area always gives distance.
🧠 Worked example — follow the thinking
A car speeds up from rest to 20 m/s in 5 s, then moves steadily for 10 s. Find a and total distance.
StepWhy I do this
a = (20 − 0) ÷ 5 = 4 m/s²💭 Gradient of the first line.
Triangle: ½ × 5 × 20 = 50 m💭 Area under the accelerating part.
Rectangle: 10 × 20 = 200 m💭 Area under the steady part.
Total = 250 m💭 Add the areas.
Sec 3 Combined Physics · SEC K326
🧲
3

Forces, Mass, Weight & Density

W = mg, ρ = m/V, p = F/A
BIG IDEAW = mg · ρ = m ÷ V · p = F ÷ A. Mass never changes; weight depends on g.
ContactNon-contact
friction, air resistancegravitational
tensionelectrostatic
normal (reaction) forcemagnetic
MassWeight
Isamount of mattergravitational force on it
UnitkgN
Changes with place?noyes (g on Moon ≈ 1.6 N/kg)
🌍 Gravitational field
region where a mass feels a force · g = gravitational field strength = force per unit mass (N/kg) · Earth: g = 10 N/kg
⚖️ Density
ρ = m ÷ V (kg/m³ or g/cm³)
irregular object: displacement in a measuring cylinder
ρ object < ρ liquid → floats
📌 Pressure
p = F ÷ A, unit Pa = N/m² · small area → big pressure (knife, nail) · big area → small pressure (snowshoes, tank tracks)
⚠ TRAP1 g/cm³ = 1000 kg/m³. Convert cm² → m²: divide by 10 000, not 100.
🔎 WHY IT WORKSWhy weight changes but mass doesn't: mass counts the matter in you — that is the same everywhere. Weight is the pull of gravity, and the Moon pulls less (smaller g), so W = mg is smaller.
🧠 Worked example — follow the thinking
A 2 kg brick is 0.2 m × 0.1 m × 0.05 m. Find its density and the max pressure it exerts.
StepWhy I do this
V = 0.2 × 0.1 × 0.05 = 0.001 m³💭 Volume of a cuboid.
ρ = 2 ÷ 0.001 = 2000 kg/m³💭 ρ = m ÷ V.
W = 2 × 10 = 20 N💭 Force on the floor = weight.
Max p uses the smallest face: 0.1 × 0.05 = 0.005 m²💭 Smallest area → largest pressure.
p = 20 ÷ 0.005 = 4000 Pa💭
Sec 3 Combined Physics · SEC K326
🚀
4

Dynamics

F = ma, free-body diagrams, friction
BIG IDEAF = ma — a resultant force makes a mass accelerate. Balanced forces → no change in motion.
normal R weight W pull friction
free-body diagram: every force on ONE object
Newton's ideas (apply, no need to state)
1 no resultant force → stays at rest or constant velocity
2 F = ma (resultant force)
3 action–reaction: equal, opposite, act on different objects
Friction
opposes motion · produces heat, wear · reduce: lubricant, smooth surfaces, ball bearings · needed for walking, brakes, grip
Inertia
reluctance to change motion — depends on mass · why seat belts are needed
⚠ TRAPAction–reaction pairs never cancel — they act on different bodies. Weight and normal force on a book are NOT a pair.
🔎 WHY IT WORKSWhy a heavier object needs more force for the same acceleration: a = F ÷ m. Doubling the mass halves the acceleration for the same force — more matter is harder to speed up.
🧠 Worked example — follow the thinking
A 1200 kg car: engine force 3000 N, friction 600 N. Find its acceleration.
StepWhy I do this
Resultant = 3000 − 600 = 2400 N💭 F in F = ma is the RESULTANT force, so subtract opposing forces.
a = F ÷ m = 2400 ÷ 1200💭 Rearrange F = ma.
a = 2 m/s²💭 Forward, in the direction of the resultant.
Sec 3 Combined Physics · SEC K326
⚖️
5

Turning Effects of Forces

moments, principle of moments, centre of gravity
BIG IDEAmoment = F × d (d = perpendicular distance from pivot). Balanced: clockwise moments = anticlockwise moments.
40 N? 1.5 m1.2 m
principle of moments
Turning effect
unit: N m
bigger force or longer distance → bigger moment
door handle far from hinge · long spanner
equilibrium: resultant force = 0 AND resultant moment = 0
🎯 Centre of gravity
point where the whole weight seems to act · find it for a flat lamina: hang from 2 points, draw plumb lines, CG where they cross
🔎 WHY IT WORKSWhy distance matters: pushing far from the pivot means the same force gives more turning. That is why you push a door at the handle, not near the hinge.
🧠 Worked example — follow the thinking
Find the unknown weight in the diagram.
StepWhy I do this
Anticlockwise moment = 40 × 1.5 = 60 N m💭 Moment = F × perpendicular distance to the pivot.
Clockwise moment = W × 1.2💭 Unknown on the right.
W × 1.2 = 60 → W = 50 N💭 Principle of moments: they balance.
Sec 3 Combined Physics · SEC K326
⚡
6

Energy, Work & Power

stores, Ek, Ep, work, power
BIG IDEAEnergy is conserved: it only moves between stores. Ek = ½mv² · Ep = mgh · W = Fs · P = E ÷ t
StoreExample
kineticmoving object
gravitational potentialraised object
elastic potentialstretched spring
chemical potentialfuel, food, cell
nuclearuranium
internalhot object (particles)
Transfer byExample
mechanical workforce moves an object
electrical workcurrent in a circuit
heatinghot → cold
waveslight, sound
Work & power
work done = F × distance moved in direction of F (J)
power = rate of energy transfer, W = J/s
Falling object
loss in Ep = gain in Ek (no air resistance)
mgh = ½mv² → v = √(2gh) — independent of mass
🔎 WHY IT WORKSWhy mass cancels when things fall: both Ep and Ek are proportional to m, so a heavy and light ball dropped together reach the same speed (ignoring air resistance).
🧠 Worked example — follow the thinking
A 0.5 kg ball is dropped from 5 m. Find its speed just before hitting the ground.
StepWhy I do this
Ep lost = mgh = 0.5 × 10 × 5 = 25 J💭 Energy at the top.
Ek gained = 25 J (conservation)💭 No air resistance → all Ep becomes Ek.
½ × 0.5 × v² = 25 → v² = 100💭 Ek = ½mv².
v = 10 m/s💭
Sec 3 Combined Physics · SEC K326
🫧
7

Kinetic Particle Model of Matter

states, internal energy, changes of state
BIG IDEATemperature measures the average kinetic energy of particles. During a change of state, temperature stays constant.
SolidLiquidGas
Arrangementclosely packed, regularclosely packed, irregularfar apart, random
Motionvibrate about fixed positionsslide past each othermove fast, randomly
Forcesvery strongstrongvery weak
Shape / volumefixed / fixednot fixed / fixednot fixed / not fixed
timetempmeltingboiling
heating curve: flat parts = change of state
Internal energy
= total kinetic + potential energy of all particles
flat part: energy goes into breaking bonds (PE up), KE same → temperature constant
gas pressure: particles collide with the walls
🔎 WHY IT WORKSWhy evaporation / sweating cools you: only the fastest particles escape the surface. The ones left have a lower average KE — and lower average KE means lower temperature.
🧠 Worked example — follow the thinking
Explain, using particles, why gas pressure rises when a sealed can is heated.
StepWhy I do this
Particles gain kinetic energy and move faster💭 Temperature up = average KE up.
They hit the walls more often and harder💭 More frequent, more forceful collisions.
Greater force per unit area → pressure increases💭 Pressure = force ÷ area.
Sec 3 Combined Physics · SEC K326
🔥
8

Thermal Processes

conduction, convection, radiation
BIG IDEAThermal energy flows from hot to cold until thermal equilibrium: conduction, convection, radiation.
ProcessHowWhere
Conductionparticles vibrate and pass energy to neighbours; free electrons in metals carry it fastsolids
Convectionheated fluid expands → less dense → rises; cooler, denser fluid sinks → convection currentliquids, gases
Radiationinfrared electromagnetic waves — no medium neededeverywhere, even vacuum
Radiation depends on
colour & texture: dull black = best absorber and emitter; shiny silver = poorest
temperature: hotter emits more
surface area: bigger emits more
Applications
vacuum flask (vacuum + silvered walls) · aircon high, heater low · sea & land breezes · cooling fins painted black · copper-bottomed pots · double glazing
🔎 WHY IT WORKSWhy metals conduct so well: besides vibrating particles, metals have free electrons that move quickly through the whole metal, carrying energy far faster than vibrations alone.
🧠 Worked example — follow the thinking
Why is the freezer compartment at the top of an old fridge?
StepWhy I do this
Cold air at the top is denser💭 Cooling makes air contract.
It sinks; warmer air rises to the top to be cooled💭 Sets up a convection current.
Whole fridge is cooled by convection💭 Placing the cooler low would trap cold air at the bottom only.
Sec 3 Combined Physics · SEC K326
← Back