Home
Login

Color

Indigo
Red
Green
Teal
Blue
Purple
Rose

Mode

Light
বাং

Where to hold it so it balances: the centre of mass

The centre of mass is the single point where all the mass of a body or system can be treated as concentrated, and where external forces appear to act. For point masses, x_cm = Σmx/Σm. Drag the masses below and watch it shift.

Drag the masses along the rod. The rod itself is treated as weightless

Point massCentre of massWeightSupport
Speed

Controls

Scene

Mass to move

2.0 kg
20 cm
50.0 cm

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

  1. 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.
  2. Slide the support and watch which way the rod tips, then switch on “Move the support under the centre of mass” to level it.
  3. In the “Masses on a plate” scene follow the dashed lines to see the centre of mass move in both x and y.
  4. 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.

TermPlain meaningFamiliar example
Centre of massThe balance point of the mass distributionThe spot where a pencil balances on a finger
Centre of gravityThe point where the whole weight actsThe point under which a hanging body’s string stops
Point massMass imagined at a single point, size ignoredA small metal bead glued to a rod
Torque (moment)Force times perpendicular distance; turning powerA push on a door handle
Support (pivot)The point where the body is propped upThe knife-edge in the middle of a balance
EquilibriumNet force and net torque both zeroA balance hanging perfectly still
Stable equilibriumReturns by itself after a small pushA marble in the bottom of a bowl
Unstable equilibriumRuns further away after a small pushA marble on top of an upturned bowl
Neutral equilibriumStays wherever it is leftA 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.

BodyMeasured fromFormulaExample
Semicircular wireMidpoint of the diameter2R/π6.37 cm
Semicircular discMidpoint of the diameter4R/3π4.24 cm
Solid hemisphereCentre of the flat face3R/83.75 cm
Hollow hemisphereCentre of the flat faceR/25.00 cm
Triangular plateThe base, along the heightH/34.00 cm
Solid coneThe base, along the heightH/43.00 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.

KindCentre of mass when nudgedWhat happensExample
StableRisesReturnsMarble in a bowl, a hanging swing
UnstableFallsRuns awayA pencil standing on its point
NeutralStays at the same heightStays putA 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.

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

Binary Number System: Place Value, Conversion and Addition