Controls
Scene
Readings
- Deviation of red
- 38.32°
- Deviation of violet
- 39.99°
- Angular dispersion
- 1.67°
- Minimum deviation (yellow)
- 38.84°
- Incidence at that point
- 49.42°
- Index for red
- 1.513
- Index for violet
- 1.532
- Dispersive power
- 0.037
- Critical angle (red)
- 41.4°
How to use this simulation
- Start in the Light in a prism scene. A white ray hits the left face at i = 50° of a prism with A = 60°. Six coloured rays leave the right face. The screen on the right shows where red and violet land.
- Tick Exaggerate the colour spread at the bottom of the controls to see the fan clearly. The real spread is small, only 1.67° here, so the picture multiplies it. The readings on the right are always the true values.
- Drag the angle of incidence. The whole spectrum swings up and down, and at one angle it stops and turns round. That turning point is the minimum deviation.
- Drag the prism angle A. A bigger prism bends light more and spreads the colours further. Make A large and i small and one colour disappears: it has been totally reflected inside the glass.
- Switch to Deviation against incidence. Every colour makes a U-shaped curve. The green dots mark the minimum, with its value and the angle of incidence at which it occurs.
- Open Rainbow. Slide the angle on the drop and watch where red and violet leave. The graph shows why the rays pile up near 42°.
Newton’s trick with a piece of glass
Before 1666 most people believed a prism added colour to light. Newton made a small hole in his window shutter, let a thin beam of sunlight fall on a prism, and caught a band of colours on the wall. Then he did the clever part: he let one colour through a second prism and found that it did not change any further.
His conclusion was that sunlight is already a mixture of colours, and the prism only separates them. The separation is called dispersion, and the band of colours is the spectrum, from red at one end to violet at the other.
Dispersion is behind rainbows, the sparkle of a diamond and the coloured fringe around a bright object in a cheap lens. In exams it comes with a handful of formulas and one famous graph, all of which you can reproduce with the simulation.
Why the colours separate
When light enters glass it slows down, and that slowing is why its path bends. The amount of bending is set by the refractive index n = c/v. The key fact is that the index of glass is not the same for all colours. Violet is slowed a little more than red, so violet bends more.
For typical crown glass the index for red is 1.513 and for violet 1.532, a difference of only 0.019. That tiny gap, repeated at both faces of the prism, is enough to fan the colours out. Yellow, in the middle, is about 1.519.
These are typical values. Real glass types differ, and the numbers also depend a little on the exact wavelength you pick for red and violet. What matters is the order: n(red) < n(orange) < n(yellow) < n(green) < n(blue) < n(violet).
Following one ray through a prism
A prism has two faces that meet at the apex angle A. A ray hits the first face at angle of incidence i, bends toward the normal and travels inside at angle r₁. It then meets the second face at angle r₂ and leaves at angle e, bending away from the normal.
Geometry of the two normals gives r₁ + r₂ = A. Adding the bend at each face, the total turning of the ray, the angle of deviation, is δ = i + e − A. Snell’s law at each face connects the angles: sin i = n sin r₁ and sin e = n sin r₂.
sin i = n sin r₁Snell’s law at the first face
r₁ + r₂ = AGeometry of the prism
sin e = n sin r₂Snell’s law at the second face
δ = i + e − AAngle of deviation
Solved problem 1: trace red and violet
Crown glass has n = 1.513 for red and 1.532 for violet. White light hits a 60° prism at 50°. Find the deviation of each colour and the angle between them.
Red
sin r₁ = sin 50° / 1.513, so r₁ = 30.42°. Then r₂ = A − r₁, and sin e = 1.513 × sin r₂ gives e = 48.32°.
δ(red) = 50 + 48.32 − 60 = 38.32°
Violet
The same steps with 1.532 give r₁ = 30.00° and e = 49.99°.
δ(violet) = 50 + 49.99 − 60 = 39.99°
The angle between them
The angular dispersion is the difference: 39.99° − 38.32° = 1.67°. On a screen two metres away the band is a few centimetres wide.
The deviation graph and the minimum
Keep the prism fixed and change only the angle of incidence. The deviation does not change steadily. It falls to a smallest value, the minimum deviation δₘ, and then rises again. The graph is a shallow U, and in the Deviation against incidence scene you can see one for every colour.
At the very bottom of the U the ray passes through the prism symmetrically: i = e and r₁ = r₂ = A/2. Nothing else gives that, and it is why a spectrometer is always set at minimum deviation: the beam is sharpest and any small error in i makes almost no change in δ.
The table fixes A = 60° and lists red and violet at six angles. Notice that the two columns reach their minimum at slightly different angles, and that violet is always deviated more. Between 28.9° and 30.3° of incidence red still leaves, but violet is already trapped inside, which is why the violet cell is empty in the first row.
i = e, r₁ = r₂ = A / 2Conditions at minimum deviation
n = sin((A + δₘ)/2) / sin(A/2)Refractive index from the minimum
| Incidence i (°) | Deviation of red (°) | Deviation of violet (°) | Difference (°) |
|---|---|---|---|
| 30 | 50.64 | — | — |
| 40 | 39.86 | 42.00 | 2.14 |
| 50 | 38.32 | 39.99 | 1.67 |
| 60 | 39.90 | 41.41 | 1.51 |
| 70 | 43.86 | 45.31 | 1.46 |
| 80 | 50.15 | 51.59 | 1.44 |
Minimum deviation and the prism angle
Setting r₁ = A/2 and i = (A + δₘ)/2 in Snell’s law gives the formula at the bottom of the box above. It is the standard way to measure the refractive index of a glass: build a prism, find the minimum on a spectrometer, put A and δₘ in.
A bigger apex angle gives a bigger deviation, and also a bigger spread between colours. The table uses yellow light, n = 1.519, and shows both the minimum and the angle of incidence at which it occurs.
| Prism angle A (°) | Minimum deviation (°) | Incidence at minimum (°) |
|---|---|---|
| 30 | 16.30 | 23.15 |
| 45 | 26.08 | 35.54 |
| 60 | 38.84 | 49.42 |
| 75 | 60.25 | 67.62 |
Solved problem 2: find the refractive index
A prism of angle 60° shows a minimum deviation of 39° for yellow light. Find the refractive index of the glass.
Use the minimum-deviation formula
The half-sum (A + δₘ)/2 = 49.5°, and sin(A/2) = sin 30° = 0.5.
n = sin 49.5° / 0.5 = 1.521. That matches the value of about 1.519 for crown glass, which is a good sign that the measurement was sound.
Thin prisms, dispersive power and the mean deviation
When the prism angle is small and the ray is nearly normal, every angle is small enough that sin x ≈ x. The deviation becomes δ = (n − 1) A. That is the thin-prism formula, used for spectacle prisms and in the optics of lenses.
Take A = 5°. Red deviates by 2.565°, violet by 2.660°, and the angular dispersion is only 0.095°. The mean deviation is 2.595°.
The dispersive power ω is the ratio of the angular dispersion to the mean deviation: ω = (n_v − n_r)/(n_y − 1). It describes the glass alone, whatever the prism angle, and for our crown glass it is 0.037. A glass with a bigger ω, such as flint, spreads colours more for the same bending.
δ = (n − 1) AThin prism, small angles
ω = (n_v − n_r) / (n_y − 1)Dispersive power of the glass
When a colour disappears: total internal reflection
At the second face the ray goes from glass to air, so it can only leave if the angle r₂ is less than the critical angle, sin c = 1/n. For red in our crown glass c = 41.4°, and for violet c = 40.7°.
Violet has the smaller critical angle, so as you lower the angle of incidence violet gets trapped first. In the simulation set A = 60° and lower i below 30.3°: the violet ray stops at the right face and reflects back inside, while red is still on its way out until 28.9°.
The graph shades this zone red. In exam terms: a ray fails to emerge if the prism angle is too large, or the incidence too small, for the second face. For a given glass there is a largest prism angle for which a ray can ever pass through.
The rainbow is a prism with a drop of water
Sunlight enters a spherical raindrop and refracts, with the violet bending more than red, just as in the prism. It then reflects off the back of the drop and leaves through the front, refracting a second time. The path is refraction, one internal reflection, refraction.
The deviation of the ray is D = 180° + 2i − 4r, where r is the angle of refraction inside the drop. A ray that comes in near the edge (large i) and one near the centre (small i) are deflected by very different amounts. But there is an incidence where D reaches its minimum, and near it many different rays leave the drop in almost the same direction. They pile up there, and that is the bright bow.
For water, n = 1.331 for red and 1.343 for violet. The pile-up happens at i = 59.5° for red and 58.8° for violet, and the angle between the returning ray and the line from the Sun through your eye, 4r − 2i, reaches 42.4° for red and 40.6° for violet. Those are the roughly 42° and 40° quoted in textbooks.
This explains the order of colours. Red is at 42.4°, so it sits at the outside of the bow and violet, at 40.6°, on the inside. The bow is 1.7° wide. In the Rainbow scene, drag the slider until the dots sit at the top of each curve and note that moving i a little changes the angle very little.
D = 180° + 2i − 4rDeviation: refraction, one reflection, refraction
viewing angle = 180° − D = 4r − 2iAngle from the anti-solar point
cos² i = (n² − 1) / 3Incidence at the maximum viewing angle
Solved problem 3: the rainbow angle
A ray enters a raindrop at i = 59°. Using n = 1.331 for red and 1.343 for violet, find the viewing angle of each colour, and compare it with the maximum.
Apply 4r − 2i
The simulation gives 42.4° for red and 40.6° for violet at this angle. The maxima, at i = 59.5° and 58.8°, are 42.4° and 40.6°. At 59° you are almost at the top of both curves.
The second rainbow
With two internal reflections, D = 360° + 2i − 6r. The extreme sits at 50.4° for red and 53.5° for violet, and D is at a minimum again, now counted as D − 180°. The colours come out in reverse order, violet outside and red inside, and the bow is fainter because some light is lost at each reflection.
Mistakes that lose marks
Look for these before you finish an answer.
- Saying that the prism creates the colours. It only separates what was already in white light.
- Getting the order wrong. Violet bends most and is deviated most, so it comes out nearest the base.
- Using the thin-prism formula δ = (n − 1) A for a large prism.
- Forgetting that the minimum-deviation formula needs the half-angles (A + δₘ)/2 and A/2.
- Using glass indices for the raindrop. A raindrop is water, with n near 1.33.
- Placing the Sun in front of you when drawing the rainbow. It is always behind the observer.
Where dispersion matters
In a lens, dispersion causes chromatic aberration: red and blue focus at different points, so a bright object gets a coloured fringe. A camera lens fixes this by gluing together glasses with different dispersive powers.
Spectrometers use a prism or a grating to split light from a star or a flame and read its elements from the lines. The same idea is used to study the atmospheres of distant planets.
To see the underlying refraction without the colours, try the refraction of light animation first. For what lenses do with the rays, open the lens ray diagram animation next.
Frequently asked questions
What is dispersion of light?
The splitting of white light into its component colours when it passes through a refracting medium such as a prism. It happens because the refractive index depends on the wavelength.
Which colour bends the most in a prism?
Violet. It has the highest refractive index in glass, so it is slowed the most and deviated the most. Red is deviated the least.
What is the formula for the angle of deviation of a prism?
δ = i + e − A, where i is the angle of incidence, e the angle of emergence and A the angle of the prism.
What is minimum deviation?
The smallest angle of deviation, reached when the ray passes symmetrically through the prism so that i = e. Then n = sin((A + δₘ)/2) / sin(A/2).
What is dispersive power?
The ratio of the angular dispersion between violet and red to the mean deviation, ω = (n_v − n_r)/(n_y − 1). It depends only on the glass.
How is a rainbow formed?
Sunlight refracts into a raindrop, reflects once at its back surface and refracts out again. Because the deviation has a minimum, rays bunch up near 42° from the anti-solar point, and different colours bunch at slightly different angles.
Why is the secondary rainbow fainter and reversed?
The ray makes two internal reflections, and some light escapes at each one, so the bow is weaker. The extra reflection also reverses the order of the colours.
Keep studying this topic
The animation made the idea click; now turn it into marks. Syllabus, suggestions, textbooks and admission-test guides are below.
SSC
SSC Physics: syllabus and preparation
HSC
HSC Physics: syllabus and preparation
Textbook
Class 9-10 Physics textbook
Admission
Engineering admission test 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
Centre of mass
Drag masses along a rod or plate and watch the centre of mass x = Σmx/Σm move. Find the balance point, see when a bus topples, and learn stable, unstable and neutral equilibrium 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 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






















