Drag the masses along the rod. The rod itself is treated as weightless
Controls
Scene
Mass to move
Readings
- Total mass
- 6.0kg
- Centre of mass, x
- 59.17cm
- Support (pivot) position
- 50.0cm
- Net torque about the support
- 5.39N·m
How to use this simulation
- In the “Masses on a rod” scene, drag masses A, B and C with the mouse or a finger; the yellow diamond is the centre of mass, and its position is in the readings.
- Slide the support and watch which way the rod tips, then switch on “Move the support under the centre of mass” to level it.
- In the “Masses on a plate” scene follow the dashed lines to see the centre of mass move in both x and y.
- In the “Toppling block or bus” scene change the width, height and bottom ballast, then tilt the base slowly and watch the body go over at the critical angle.
The ruler-on-two-fingers trick
Rest a ruler loosely on your two index fingers, one near each end. Now slide your fingers slowly together. Strange thing: they never move at the same time. One slides, then the other, taking turns, and in the end they meet exactly in the middle. That meeting point is the ruler’s centre of mass.
Stick a lump of modelling clay on one end and try again. The fingers now meet nearer the clay. The centre of mass has moved towards the heavy end. With one tiny experiment you have caught its real character: it is the average position, weighted by mass.
Acrobats on a rope, a load of bamboo on a rickshaw, luggage piled on a bus roof, a news story about a bus rolling over on a bend: all of them hang on the same idea. In this lesson we build the formula, play with it in the simulation, and then work some numbers.
From zero: what the centre of mass actually is
A body is made of billions of particles, and Earth pulls on every one of them separately. To keep our sums manageable we would love to replace all those pulls with a single arrow. There is a special point where, if you pretend all the mass sits there, the body’s overall motion from place to place comes out right. That point is the centre of mass.
Think of a spinning hammer tossed across a room. The hammer tumbles, and the motion looks messy. Yet its centre of mass traces a perfectly smooth parabola, exactly as a small pebble would. However the body twists, the centre of mass moves like a single point mass under the same outside forces.
The centre of mass does not have to be inside the body. A ring has it in the empty middle. A semicircular wire has it off the wire, on the inner side of the curve. We will even locate the centre of mass of the Earth and Moon together, and the result is surprising.
Centre of mass and centre of gravity are different ideas. The centre of mass depends only on how mass is spread out. The centre of gravity is the point where the total weight acts. When g is the same everywhere, as it is for everything near the ground, the two points coincide. They would separate only for something so large that g changes across it. In school problems, treat them as one.
Words you must know
These terms come up again and again in this chapter. Each has a plain meaning and a familiar example.
| Term | Plain meaning | Familiar example |
|---|---|---|
| Centre of mass | The balance point of the mass distribution | The spot where a pencil balances on a finger |
| Centre of gravity | The point where the whole weight acts | The point under which a hanging body’s string stops |
| Point mass | Mass imagined at a single point, size ignored | A small metal bead glued to a rod |
| Torque (moment) | Force times perpendicular distance; turning power | A push on a door handle |
| Support (pivot) | The point where the body is propped up | The knife-edge in the middle of a balance |
| Equilibrium | Net force and net torque both zero | A balance hanging perfectly still |
| Stable equilibrium | Returns by itself after a small push | A marble in the bottom of a bowl |
| Unstable equilibrium | Runs further away after a small push | A marble on top of an upturned bowl |
| Neutral equilibrium | Stays wherever it is left | A marble on a flat table |
The formula: a weighted average of positions
In an ordinary average every number counts equally. In the centre-of-mass average each position counts as much as the mass sitting there. Heavy masses pull harder on the average, so the centre of mass sits closer to the heavy side.
x_cm = (m₁x₁ + m₂x₂ + … + mₙxₙ) / (m₁ + m₂ + … + mₙ)along a line
x_cm = Σmx / Σm, y_cm = Σmy / Σmin a plane, two numbers
x_cm = (1/M) ∫ x dmfor a continuous body
Two particles: the easiest case
Take 4 kg and 1 kg, 100 cm apart. Put the origin at the 4 kg mass: x_cm = (4×0 + 1×100) / (4 + 1) = 20 cm. The centre of mass lies on the line joining them, much closer to the heavy one.
The ratio of the two distances is the inverse of the ratio of the masses: distance from the heavy mass ÷ distance from the light mass = light mass ÷ heavy mass. This is just the law of the balance.
Many particles and the simulation’s defaults
At the start A = 2 kg at 20 cm, B = 1 kg at 60 cm and C = 3 kg at 85 cm. Total mass 6 kg. The moments add up: 2×20 + 1×60 + 3×85 = 40 + 60 + 255 = 355. So x_cm = 355 ÷ 6 = 59.17 cm.
A lovely check: multiply each mass by its distance from the centre of mass and add. You must get zero: Σm(x − x_cm) = 0. The “mass × distance” on one side of the centre of mass exactly cancels the other side.
Bodies with a known shape
A uniform body has its centre of mass at its geometric centre. For shapes where the centre is not obvious, here are the standard results, evaluated for R = 10 cm and H = 12 cm.
| Body | Measured from | Formula | Example |
|---|---|---|---|
| Semicircular wire | Midpoint of the diameter | 2R/π | 6.37 cm |
| Semicircular disc | Midpoint of the diameter | 4R/3π | 4.24 cm |
| Solid hemisphere | Centre of the flat face | 3R/8 | 3.75 cm |
| Hollow hemisphere | Centre of the flat face | R/2 | 5.00 cm |
| Triangular plate | The base, along the height | H/3 | 4.00 cm |
| Solid cone | The base, along the height | H/4 | 3.00 cm |
Where the formula comes from
Memorising the formula is easy, but why this formula? Two short arguments settle it: one from the balance, one from Newton’s laws.
From balancing moments
Put masses m₁, m₂, … on a light rod and prop the rod at a point P. Each weight mg pulls down at a distance (x − P) from the prop. The rod balances if the clockwise and anticlockwise moments about P are equal.
That means Σ m g (x − P) = 0. Cancel g and write Σ m x − P Σ m = 0, so P = Σ m x / Σ m. The prop position that balances the rod is exactly the centre of mass.
Σ m g (x − P) = 0 ⇒ P = Σmx / Σm
From Newton: it moves like one point mass
Write Newton’s second law for each particle and add them: Σ mᵢaᵢ = Σ Fᵢ. On the right the internal forces cancel in pairs, because by Newton’s third law A pulls B exactly as hard as B pulls A the other way. Only the external forces survive.
On the left, Σ mᵢaᵢ = M a_cm, which you get by differentiating the centre-of-mass definition twice. So M a_cm = F_ext. That is why, after an explosion with no external force, the fragments may fly anywhere but their centre of mass carries on exactly as before.
Σ mᵢaᵢ = Σ Fᵢadd every particle’s equation
M a_cm = F_extinternal forces drop out
Equilibrium and stability
A body is in equilibrium when the net force and the net torque on it are both zero. But not all equilibria are alike. Nudge the body a little and see what happens; that sorts equilibrium into three kinds.
The most useful rule for exams: if a nudge raises the centre of mass, the equilibrium is stable; if it lowers it, unstable; if the height stays the same, neutral. Raising the centre of mass costs work, so the body wants to roll back.
tan φ_c = (b/2) / hcritical angle for toppling
φ < φ_c ⇒ stable, φ > φ_c ⇒ topplestilt φ against the critical angle
When does a bus topple
A bus stands on the rectangle between its wheels, its base. Drop a vertical from the centre of mass. If it lands inside the base, the weight turns the bus back down. If it lands outside, the weight itself turns the bus over.
With base width b and centre-of-mass height h, the critical tilt satisfies tan φ_c = (b/2)/h. A wider base or a lower centre of mass raises φ_c, so the bus can lean further before going over.
Why racing cars are wide and low
A racing car has a wide track and a centre of mass very near the road. Both raise φ_c. A double-decker with luggage tied to the roof does the opposite: the centre of mass climbs, and the safe angle shrinks.
| Kind | Centre of mass when nudged | What happens | Example |
|---|---|---|---|
| Stable | Rises | Returns | Marble in a bowl, a hanging swing |
| Unstable | Falls | Runs away | A pencil standing on its point |
| Neutral | Stays at the same height | Stays put | A ball on a flat floor |
Try it in the simulation
Before each experiment, guess what will happen, then move the sliders or the masses.
- In the rod scene put the support at 50 cm. Which way does the rod tip? Why is the torque reading 5.39 N·m positive?
- Switch on “Move the support under the centre of mass”. The torque reads zero and the rod levels. Now drag mass B to the right. What changes?
- Raise mass C from 3 to 6 kg. Which way did the centre of mass move, and by how much?
- Make all three masses equal. Does the centre of mass land on the plain average of the three x values?
- In the plate scene drag one mass into a corner. Do x_cm and y_cm both change?
- In the bus scene switch on “Tilt slowly”. What happens as the tilt touches the critical angle? Now add ballast at the bottom and tilt again.
- Set the width to 0.4 m and the height to 3 m, a tall thin box. How much smaller is the critical angle?
Solved problems
For each problem draw a picture first, choose an origin, and then substitute. The numbers match the simulation.
Problem 1: the default rod
A = 2 kg at 20 cm, B = 1 kg at 60 cm, C = 3 kg at 85 cm on a light rod. Find the centre of mass and the net torque about a support at 50 cm.
Step 1: x_cm = 355 ÷ 6 = 59.17 cm. Step 2: torque about 50 cm = g × Σ m(x − 50)/100 = 5.39 N·m. Positive means the right side goes down, since the centre of mass is 9.17 cm to the right of the support.
Problem 2: the same masses on a plate
The masses sit at (20, 15), (60, 20) and (85, 50) cm. x_cm = 59.17 cm and y_cm = (2×15 + 1×20 + 3×50) ÷ 6 = 33.33 cm. Treat the two directions separately, then put them together.
Problem 3: Earth and Moon
Earth 5.97×10²⁴ kg, Moon 7.35×10²² kg, centres 384,400 km apart. Distance of the centre of mass from Earth’s centre = (Moon’s mass × separation) ÷ total mass = 4,675 km.
Earth’s radius is 6,371 km, so the centre of mass lies inside Earth, a little below the surface. It is more accurate to say that both bodies orbit this point than that the Moon orbits Earth.
Problem 4: a person walking on a boat
A 60 kg person walks 4 m along a 120 kg boat in still water. There is no external horizontal force, so the centre of mass of person and boat stays where it is.
The boat moves 60×4 ÷ (60 + 120) = 1.33 m the other way. Relative to the shore the person moves 2.67 m. The heavier boat moves less.
Problem 5: a disc with a hole
A uniform disc of radius 30 cm has a circle of radius 15 cm cut out so that the hole touches the disc’s centre. How far does the centre of mass shift?
Mass goes with area, and the hole is 0.25 of the disc. The centre of mass moves away from the hole by (hole fraction × 15) ÷ (1 − hole fraction) = 5 cm. The trick is to treat the cut-out as a negative mass.
Problem 6: how far can the bus lean
A bus has base width 2.4 m and its centre of mass 1.5 m up. Critical angle = tan⁻¹((2.4/2)/1.5) = 38.7°.
Put heavy batteries on the floor so the centre of mass is 0.75 m and the angle becomes 58.0°. Pile luggage on the roof so it is 2.0 m and it drops to 31.0°. Roof luggage eats much of the safe lean.
Mistakes everyone makes
Most lost marks in centre-of-mass problems come from a handful of slips.
- Assuming the centre of mass is always the geometric centre. With uneven mass it moves, and for a hollow body it can lie outside the body.
- Writing “centre of mass” and “centre of gravity” as synonyms. They are different ideas that coincide only in uniform g.
- Dividing by the number of particles instead of the total mass in the x_cm formula.
- Thinking the centre of mass changes when you move the origin. The point is the body’s own; only its coordinate changes.
- Mixing up left and right distances, and so their signs, when taking moments about a support.
- Dropping the vertical for a toppling body from the middle of the bus instead of from the centre of mass.
- Believing stable equilibrium means “does not move”. It means “returns after a nudge”, and an unstable equilibrium can sit still for a while.
Centre of mass in real life
A tightrope walker carries a long pole. The drooping pole drags the combined centre of mass down towards, or below, the rope, so a small wobble gives a restoring torque instead of a fall.
A high jumper arches over the bar so that the body’s centre of mass can pass under the bar while the body passes over it. That is a centre of mass outside the body, put to work.
The Leaning Tower of Pisa still stands because the vertical through its centre of mass falls inside its base. Engineers stabilised the foundation to stop the lean from growing.
In boats, cranes, trucks and rickshaws, designers keep the centre of mass low. This is also why a loaded truck has heavy cargo at the bottom and light cargo on top.
Exam corner: NCERT and CBSE style
In Class 11 this chapter appears as short-answer and numerical questions. The pattern below mirrors the board paper.
Sample question and answer
Question: A light rod 0.8 m long carries 3 kg at one end and 5 kg at the other. (a) Define the centre of mass. (b) Where is the centre of mass measured from the 3 kg end? (c) Explain why a support placed there keeps the rod horizontal.
Answer: (b) x = 5×0.8 ÷ (3 + 5) = 0.5 m, which is 50 cm. (c) About the centre of mass the total torque Σ m g (x − x_cm) is zero, so there is no turning effect.
How to present it
For two-mark conceptual questions give the reason in one or two sentences, not the formula. For numericals write the formula, substitute with units, and state the answer with its unit.
Quick revision
This list is enough the night before an exam.
- Centre of mass = mass-weighted average position: x_cm = Σmx/Σm.
- In a plane, y_cm = Σmy/Σm; a uniform body has it at its geometric centre.
- The prop point that balances a rod is the centre of mass; Σm(x − x_cm) = 0.
- M a_cm = F_ext; internal forces cannot change the centre of mass’s motion.
- The centre of mass shifts toward the heavier part, staying close to the larger mass.
- Equilibria come in three kinds: nudge raises the CM → stable, lowers it → unstable, same height → neutral.
- A body topples when the vertical through its centre of mass leaves the base: tan φ_c = (b/2)/h.
- A wide base and a low centre of mass give more stability.
Frequently asked questions
What is the centre of mass?
The centre of mass is the point where the whole mass of a body or system can be taken as concentrated, so that its overall motion under external forces is that of a single particle. For point masses x_cm = Σmx/Σm. In a uniform body it lies at the geometric centre.
What is the difference between centre of mass and centre of gravity?
The centre of mass depends only on how mass is distributed. The centre of gravity is the point where the total weight acts. When g is uniform across the body they coincide; for extremely large bodies, where g varies, they differ slightly.
Can the centre of mass lie outside the body?
Yes. A ring has it in the empty centre, and a semicircular wire has it off the wire, inside the curve. For the Earth-Moon system the centre of mass does lie inside Earth, but it is not at Earth’s centre.
Why do buses topple over?
A bus topples when, as it tilts, the vertical through its centre of mass leaves the base between its wheels. Then its weight turns it further over. The critical angle is tan φ_c = (b/2)/h, so a narrow base or a high centre of mass makes toppling easier.
How do stable, unstable and neutral equilibrium differ?
After a small push, a body in stable equilibrium returns, and its centre of mass rises. In unstable equilibrium it moves further away, and its centre of mass falls. In neutral equilibrium it stays in its new position and the centre of mass stays at the same height.
How do I find the centre of mass of masses on a rod?
Use x_cm = (m₁x₁ + m₂x₂ + …) ÷ (m₁ + m₂ + …). For 2 kg at 20 cm, 1 kg at 60 cm and 3 kg at 85 cm the answer is 59.17 cm.
What happens to the centre of mass in an explosion?
With no external force it keeps moving exactly as before. The fragments may fly in any directions, but their mass-weighted average position follows the original path, because the internal forces cancel in pairs.
What path does the centre of mass of a thrown, spinning object follow?
A smooth parabola, since gravity is the only external force. However the object tumbles, its centre of mass moves like a projectile point mass.
Keep studying this topic
The animation made the idea click; now turn it into marks. Syllabus, suggestions, textbooks and admission-test guides are below.
HSC
HSC Physics: syllabus and preparation
Textbook
Class 9-10 Physics textbook
Admission
Engineering admission test preparation
SSC
SSC Physics: syllabus and preparation
Admission
Dhaka University science unit admission 2026-27
English
Composition: The Uses of Electricity
Bangla
প্রতিবেদন: বিজ্ঞান মেলা (in Bangla)
English
Paragraph: Science in Everyday Life
SSC
SSC suggestions
HSC
HSC suggestions
Admission
University admission guide
SSC
SSC syllabus
HSC
HSC syllabus
Study abroad
Study in Germany
Test prep
Digital SAT Math guide
Scholarship
Scholarships to study abroad
IELTS
IELTS vocabulary: science and research
Tool
GPA calculator
Career
Civil engineer resume example
More physics animations
Grade 8–12
Refraction of light
Change the angle and watch light bend. Snell's law, refractive index, critical angle and total internal reflection, explained simply with worked examples.
Grade 9–12
Ohm's law
Adjust voltage and resistance and watch the current change. Ohm's law formula, V-I graph, series and parallel resistors, with solved problems.
Grade 11
Projectile motion
Set the launch angle and speed and trace the path. Time of flight, maximum height and range formulas, why 45° goes farthest, with solved numbers.
Grade 9–11
Simple pendulum
Change length and gravity and time the swing. Simple pendulum period T = 2π√(L/g), SHM, energy conservation and finding g, with solved numbers.
Grade 10–12
Electric field
Drop positive and negative charges and watch the field lines form. Coulomb's law, E = kq/r², units and field-line rules, with solved examples.
Grade 11–12
Wave interference
Move two wave sources and watch bright and dark fringes appear. Superposition, constructive vs destructive conditions, fringe width, solved examples.
Grade 9–11
Free Fall
What is free fall? Drop a coin and a feather with and without air. Learn the free fall formulas for time, velocity and height (g = 9.8 m/s²) with worked examples.
Grade 10–12
Lens ray diagrams
Interactive convex and concave lens ray diagrams: drag the object through all six cases, see the three principal rays, and read u, v, f, magnification and power live.
Grade 9–11
Newton's Laws of Motion
Newton's laws of motion explained with an interactive cart: inertia, F = ma, momentum, impulse and action–reaction pairs, with examples and worked problems.
Grade 10–12
Spherical mirror ray diagrams
Drag an object in front of a concave, convex or plane mirror and watch the rays find the image. Mirror formula, magnification, all six cases, solved problems.
Grade 10–12
Electromagnetic Induction
What is electromagnetic induction? Drag a bar magnet through a coil and watch a centre-zero galvanometer. Learn Faraday's law e = −N dΦ/dt and Lenz's law with worked examples.
Grade 9–11
Conservation of Momentum and Collisions
What is the conservation of momentum? Collide two carts and drag the restitution slider from a sticking e = 0 to a bouncy e = 1. See momentum and kinetic-energy bars update live, with worked examples.
Grade 9–11
Work, Energy and Power
What is work, and what are the formulas for kinetic and potential energy and power? Release a cart on a curved track, watch energy turn to heat, with worked examples.
Grade 9–11
Inclined Plane
How does a block’s weight split on a slope, what is the angle of repose, and when does friction hold a block still or let it slide? Change the angle yourself and watch the force-arrow diagram.
Grade 9–11
Uniform circular motion
Whirl a ball on a string and read ω, T, a = v²/r and F = mv²/r live. Cut the string to see it fly off tangentially, then try banked curves with solved numbers.
Grade 8–10
Transverse and Longitudinal Waves
See a rope wave and a slinky or sound wave driven by one source. Learn crest, trough, compression, rarefaction, wavelength, v = fλ and why particles never travel with the wave, with solved problems.
Grade 9–11
Levers and moments
Slide weights on a seesaw and watch the moment M = F × d on each side. Learn the principle of moments, three classes of lever and mechanical advantage, with solved problems.
Grade 9–11
Spring-mass SHM
Run a mass on a spring in simple harmonic motion. Explore Hooke’s law, T = 2π√(m/k), energy swapping, springs in series and parallel, with worked problems and exam practice.
Grade 9–11
Vector addition: triangle and parallelogram laws
Add two vectors by the triangle and parallelogram laws, split them into components, then test a river-crossing boat and a walker with an umbrella. With solved problems.
Grade 9–11
Relative velocity: trains and river crossing
Play with two trains and a swimmer crossing a river. Learn relative speed, train crossing time, heading angle, drift, shortest time vs shortest path, with solved problems.
Grade 11–12
Kepler's laws and elliptical orbits
Drag the eccentricity and see an orbit stretch. Equal-time sectors with equal areas, the period law T² ∝ a³ and escape speed, with solved problems.
Grade 11–12
Newton’s law of gravitation, g and satellites
Play with two masses, the inverse-square graph, g above and below the Earth and a satellite orbit. Learn the law of gravitation, orbital speed, period and escape speed with solved problems.
Grade 11–12
Standing waves in strings and pipes
Pluck a string and blow across open and closed pipes in a simulation. See nodes, antinodes, harmonics, and learn how length, tension and temperature set the pitch, with solved problems.
Grade 11–12
Resonance tube and the speed of sound
Slide the water level in a resonance tube and find the loud spots yourself. See L1 = λ/4 − e and L2 = 3λ/4 − e, compute the speed of sound with v = 2f(L2 − L1), and practise solved problems.
Grade 11–12
Beats: when two close notes pulse
Add two waves of nearly equal frequency and watch the loudness pulse. See the envelope, read the beat frequency |f1 − f2|, hear the effect, and learn how guitarists tune by beats, with solved problems.
Grade 11–12
Doppler effect: moving sources, listeners and sonic booms
Drag a sound source faster and slower and watch the wavefronts bunch up ahead and stretch out behind. Learn the Doppler formula, moving listener, ambulance and train problems, and the sonic boom.
Grade 10–12
Prism, dispersion of light and the rainbow
Send white light through a prism, change the prism angle and incidence, and watch the spectrum form. Learn deviation, minimum deviation, dispersive power and how a raindrop makes a rainbow, with solved problems.
Grade 11–12
Kirchhoff’s laws: junction rule and loop rule
Build a two-loop circuit with two batteries and three resistors. Watch the currents split at a junction, see the voltage sums land on zero and learn how to solve Kirchhoff’s laws problems step by step.
Grade 12
Wheatstone bridge and metre bridge
Unbalance a Wheatstone bridge and watch the galvanometer needle swing. Find balance at P/Q = R/S, then slide the jockey on a metre bridge to measure an unknown resistance with solved examples.
Grade 11–12
Single-slit diffraction
Change the slit width and wavelength and watch light spread behind a single slit. See the intensity graph I = I₀(sin β/β)², the minima at a sin θ = mλ and the central maximum width 2λD/a, with solved problems.
Grade 10–12
Defects of the human eye and their correction
Switch between a normal, short-sighted, long-sighted and ageing eye. See why the image lands in front of or behind the retina, then fit the right lens and work out its power in dioptres.
Grade 12
Polarisation of light: Malus’s law and Brewster’s law
Rotate an analyser behind a polariser and watch I = I₀cos²θ on a graph, then bounce light off glass to find the Brewster angle. Includes polaroid sunglasses, three-filter puzzles and solved problems.
Grade 12
Charging and discharging a capacitor: the RC time constant
Charge and discharge a capacitor through a resistor. Change E, R and C, watch V = E(1 − e^(−t/RC)) and the current curve draw live, find the 63% time constant and the energy stored.
Grade 10–12
Magnetic field lines: bar magnet, current-carrying wire and solenoid
See magnetic field lines of a bar magnet, a straight current-carrying wire and a solenoid. Drag a compass, flip the current, and learn B = μ₀I/2πr, B = μ₀nI and the right-hand grip rule.
Grade 12
AC generator
Spin a coil between magnet poles and watch the sine wave of an AC generator build live. Change N, A, B and rpm, read E0 = NBAω and the rms value, and see why mains is 50 Hz.
Grade 10–12
Transformer
Change the primary and secondary turns of a transformer and watch the voltage step up or down. See Vs = Vp·Ns/Np, power conservation, real efficiency and why power lines use high voltage.
Grade 9–12
Heat transfer: conduction, convection and radiation
Heat a copper, aluminium, glass or wooden rod and watch Q/t = kAΔT/L, see convection currents circulate in a beaker, and see how radiated power grows as T⁴. With tables and solved problems.
Grade 12
Photoelectric effect: Einstein’s equation and the stopping potential
Shine light of any wavelength on sodium, zinc or copper in a vacuum tube. See why electrons leave only above the threshold frequency, how K = hf − φ sets the stopping potential, and why brightness changes only the current.
Grade 10–12
Motor effect: force on a current-carrying wire and the DC motor
Put a current-carrying wire in a magnetic field and watch it get pushed. Change B, I, L and the angle, test Fleming’s left-hand rule, then spin a DC motor with a split-ring commutator and see its torque graph.
Grade 11–12
Gas molecules and kinetic theory: pressure, temperature and speed
Watch gas molecules bounce around a box. Raise the temperature, change the gas, squeeze the volume, and see wall hits turn into pressure that matches PV = NkT. Compare speeds with the Maxwell–Boltzmann curve and calculate rms speed.
Grade 12
The semiconductor diode: p–n junction, I–V curve and rectifier
Bias a p–n junction and watch the depletion layer shrink or grow, carriers cross, and the Shockley I–V curve trace live. Compare silicon and germanium, see breakdown, then build a half-wave rectifier.
Grade 10–12
Radioactive decay: half-life, the decay law and penetration
Watch 240 nuclei decay at random, see the count follow N = N₀e^(−λt), measure the half-life from the graph, then test how alpha, beta and gamma radiation pass through paper, aluminium and lead.
Grade 11–12
The Bohr atom: orbits, energy levels and the hydrogen spectrum
Make a hydrogen electron jump between orbits n = 1 to 6, watch the photon colour come from 1/λ = R(1/n₁² − 1/n₂²), and see the Lyman, Balmer and Paschen series on an energy diagram and spectrum strip.
Animations in other subjects
Chemistry
Structure of the atom
Chemistry
Acids, Bases and the pH Scale
Chemistry
Electron configuration
Chemistry
Gas laws: Boyle, Charles, Gay-Lussac, Avogadro and PV = nRT
Chemistry
How an Ionic Bond Forms
Chemistry
Electrolysis and Faraday’s Laws
Chemistry
Covalent Bond
Chemistry
Periodic Trends
Chemistry
Reaction rate and collision theory
Chemistry
States of matter: solid, liquid, gas and the heating curve
Chemistry
Atomic orbitals: the shapes of s, p and d, quantum numbers and nodes
Chemistry
Molecular shapes and VSEPR theory: bond pairs, lone pairs and angles
Chemistry
The mole concept: molar mass, Avogadro’s number and molar volume
Chemistry
Diffusion and effusion: Graham’s law of gases
Chemistry
Balancing chemical equations: method, examples and practice
Chemistry
Chemical equilibrium: the equilibrium constant Kc and Le Chatelier’s principle
Chemistry
Titration: finding an unknown concentration with a burette and an indicator
Chemistry
Galvanic cell: the Daniell cell, EMF and the Nernst equation
Chemistry
Redox reactions: oxidation numbers, electron transfer and half-equations
Chemistry
Hydrocarbons: alkanes, alkenes, alkynes and structural isomers in 3D
Chemistry
Functional groups: alcohols, aldehydes, ketones, acids, esters and amines
Chemistry
Polymerisation: addition and condensation polymers, polythene and nylon
Chemistry
Separation techniques: filtration, distillation, chromatography, crystallisation
Chemistry
Crystal lattice: SC, BCC and FCC unit cells, packing efficiency and density
Chemistry
Radioactivity: Alpha, Beta, Gamma Decay and Half-Life
Biology
Mitosis cell division
Biology
Diffusion and Osmosis
Biology
Photosynthesis
Biology
The human heart: structure and function
Biology
Mendelian Genetics
Biology
DNA Replication
Biology
Cellular Respiration
Biology
Enzyme Action
Biology
The Nerve Impulse and the Action Potential
Biology
The Nephron and Urine Formation
Biology
Meiosis Cell Division
Biology
Digestive System
Biology
Breathing Mechanism: Inhalation and Exhalation
Biology
Protein synthesis
Biology
Blood circulation: double circulation and cardiac output
Biology
Cell structure and organelles: plant cell vs animal cell
Biology
Reflex action and the reflex arc
Biology
The human eye: parts, image formation and accommodation
Biology
Muscle contraction and the sliding-filament model
Biology
Transport in plants: xylem, phloem and transpiration
Biology
Food chain and food web: energy flow and the 10 % rule
Biology
Population growth: exponential and logistic curves
Biology
Natural selection: peppered moths and the sooty tree
Biology
Immune response: primary and secondary antibody response
Biology
Pollination and fertilisation
Mathematics
Pythagorean Theorem
Mathematics
Trigonometric Ratios and the Unit Circle
Mathematics
Quadratic functions and their graphs
Mathematics
Circle theorems
Mathematics
Heights and distances: elevation and depression angles
Mathematics
Probability: experimental vs theoretical probability
Mathematics
Arithmetic and Geometric Sequences
Mathematics
Mean, Median and Mode
Mathematics
Sets and Venn Diagrams
Mathematics
Linear equations: graphs, slope and simultaneous pairs
Mathematics
Graphs of sin, cos and tan
Mathematics
Completing the Square and the Quadratic Formula
Mathematics
Area of a Circle: Proof, Formula and Solved Problems
Mathematics
Volume and Surface Area of Solids: Cube, Cuboid, Cylinder, Cone, Sphere
Mathematics
Similar Triangles: Scale Factor, AA, SSS, SAS and Shadow Heights
Mathematics
Coordinate Geometry: Distance, Midpoint, Slope, Section Formula and Locus
Mathematics
Conic Sections: Circle, Ellipse, Parabola and Hyperbola
Mathematics
Function Transformations: Shifts, Stretches and Reflections
Mathematics
Derivative as the Slope of a Tangent: Secant to Tangent
Mathematics
Riemann Sums and Integration: Area Under a Curve
Mathematics
Limits and the ε–δ Definition: A Visual Guide
Mathematics
3D Vectors: Sum, Dot Product and Cross Product
Mathematics
Matrix Transformations: Rotation, Reflection, Shear and the Determinant
Mathematics
Complex Numbers: Sum, Product, Powers and Roots on the Argand Plane
Mathematics






















