Contents

Part 1: Exposure

  1. 1 Mastering the Exposure TriangleBalance aperture, shutter speed and ISO for brightness, depth, motion and noise.
  2. 2 ISO and image noiseWhen to raise ISO, why grain appears, and how to trade it for a faster shutter.
  3. 3 MeteringWhat the meter aims for, how to read it, the four metering modes, and Sunny 16 when there's no meter.
  4. 4 Shooting modes and the histogramLet the camera set one setting, steer it with exposure compensation, and check the result with the histogram and zebras.
  5. 5 Dynamic rangeHow many stops a camera can hold at once, what to keep when a scene is wider, and measured figures for real cameras.
  6. 6 Shutter speed and motionCamera shake, freezing or blurring a moving subject, and ND filters for long exposures.
  7. Part 1 cheat sheetFormulas and starting settings from chapters 1–6.
  8. Part 1 quizCheck yourself on chapters 1–6.

Part 2: Focus and depth

  1. 7 Camera LensLens anatomy and how to choose wide, standard, telephoto, prime, zoom and specialist lenses for real subjects.
  2. 8 Aperture and depth of fieldWhy a wider aperture blurs the background, what else controls blur, and the shape of bokeh.
  3. 9 Sensor size and crop factorWhat a smaller sensor crops, equivalent focal length and aperture, and why phones fake the blur.
  4. 10 Hyperfocal distanceSharp from here to infinity: focusing landscapes with blur circles, focus stacking and a cheat card.
  5. 11 Diffraction and the sharpest apertureWhy f/22 looks soft, where your lens is sharpest, and how pixel size changes it.
  6. Part 2 cheat sheetFormulas and starting settings from chapters 7–11.
  7. Part 2 quizCheck yourself on chapters 7–11.

Part 3: Composition

  1. 12 The composition reading planAll 15 chapters of The Elements of Composition, with printed page numbers and a photography lesson for each.
  2. 13 Introduction to compositionComposition as visual communication: choose what to show, compare three frames, and see how viewers read them.
  3. 14 What is composition?Arrange subject, space and edges to change what a photograph says; compare photos and make three versions of one scene.
  4. 15 Focal pointsChoose where the eye lands first, use contrast and space to build a visual path, then test thirds and diagonals in a field exercise.
  5. 16 LinesFollow straight, curved and implied lines through a photograph, then make three frames of one subject from different positions.
  6. 17 ShapesFind shapes made by subjects and space, use a frame within the frame, and compare three ways to place one subject.
  7. 18 TexturesMake a surface feel tangible with light, detail and context, then photograph one material three ways.
  8. 19 PatternsUse repetition to build rhythm, break a pattern to draw attention, and make three versions of one repeated scene.
  9. 20 SpaceUse positive and negative space, fill the frame, and simplify without losing meaning.
  10. 21 DepthLayer foreground, middle ground and background, and use perspective or deep space to show distance.
  11. 22 BalanceWeigh elements with symmetry, asymmetry and radial arrangements; explore the golden ratio as an optional guide.
  12. 23 ContrastCreate meaning and focus through contrasting subjects, light, shadows and colour.
  13. 24 ColorChoose hue, saturation and brightness, then compare complementary, triadic, analogous and monochromatic palettes.
  14. 25 ToneRead shadow, midtone and highlight; shape global and local tone while keeping meaningful detail.
  15. 26 AngleChange camera height and tilt to compare level, straight up or down, high and low viewpoints.
  16. 27 Composition conclusionBring the elements together in a four-frame story and develop your own way of seeing.

Part 4: Color Theory

  1. 28 Color Theory in PhotographyUse HSL, warm and cool depth, four color harmonies, white balance and selective editing to guide attention.
  2. 29 White balanceRead the color of light, match Kelvin and tint, and choose what to preserve when lights mix.

Tools

  1. Color wheelExplore hues, adjust saturation and luminosity, enter RGB or hex values, and preview the color live.
  2. Photo editorTry light, colour, detail and crop adjustments on a sample or your own photo, then save the result.
  3. Golden hour plannerSunrise, sunset, golden hour and blue hour for where you are, and where the sun rises and sets.
  4. ND filter calculatorYour shutter speed with an ND filter on, and a countdown timer for bulb mode.
  5. Depth of field calculatorHow much is sharp for your lens, aperture and focus distance, and the hyperfocal distance.
  6. Photo info and location removerSee a photo's camera settings and where it was taken, then remove the location before you share it.

Chapter 1Part 1: Exposure

Mastering the
Exposure Triangle

The ultimate guide to perfect photographic balance. Change aperture, shutter speed and ISO in the playground, then take the same decisions to your camera.

Think of the camera sensor as a canvas and light as the paint. Aperture and shutter speed determine how much light reaches it; ISO changes how brightly the captured signal is rendered. Together, these settings form the exposure triangle.

They also shape the photograph beyond brightness. You can keep a mountain landscape sharp, freeze a moving athlete, or soften a distracting background. Learning how the settings trade off gives you control over those choices.

f/41/250ISO100
Background (aperture)
Bird (shutter)
Noise (ISO)

Simplified. Real background blur also depends on the lens focal length and how far away the subject is. Real motion blur depends on how fast the subject moves. Noise also depends on how much light the sensor collects, not just the ISO setting.

0 stops
Same brightness as the baseline

Baseline exposure: f/4, 1/250 s, ISO 100.

f/4
0
f/1, more lightf/16, less light
1/250
0
1/8 s, more light1/4000 s, less light
100
0
100, cleanest6400, brightest

Load an example

The foundation: what is a stop of light?

A stop is the common unit for changing exposure. Add one stop with aperture or shutter speed and the sensor receives twice as much light; subtract one and it receives half as much. Most cameras let you adjust in one-third-stop clicks, so three clicks make one full stop.

+1 stopTwice the captured light

−1 stopHalf the captured light

The one-third-stop section works through the smaller steps and their maths. ISO is different: raising it brightens the recorded result without adding light at the sensor. The ISO chapter explores that trade in detail.

The table shows one-stop changes from a common starting point. The aperture and shutter columns change captured light; the ISO row changes recorded brightness.

One stop brighterBaselineOne stop darker
Aperturef/2.8f/3.2, f/3.5 betweenf/4f/5.6
Shutter1/1251/160, 1/200 between1/2501/500
ISO200125, 160 between10050only on some cameras

The three pillars of exposure

Each setting changes brightness, but each also has a creative effect. Choose the look you need first, then balance the remaining settings.

01 / APERTURE

The eye of the lens

Aperture is the opening inside the lens. A small f-number such as f/1.4 means a wide opening and more captured light; f/16 means a narrow opening and less light.

It also affects depth of field. Around f/1.4–f/2.8 you can soften the background behind a portrait. Around f/8–f/16 you can keep more of a landscape sharp, depending on focal length, focus distance and subject distance.

02 / SHUTTER

The element of time

Shutter speed is how long the sensor gathers light. A brief 1/1000 s or 1/2000 s exposure captures less light; 1/2 s or 30 s captures much more. Cameras may time this with a mechanical or electronic shutter.

Short exposures can freeze an athlete or bird. Long exposures can turn waves into mist or traffic into light trails. The result also depends on how fast the subject and camera move.

03 / ISO

The signal amplifier

ISO controls the brightness of the recorded result, not the number of photons captured. The familiar sequence is 100, 200, 400, 800, 1600 and 3200: each doubling raises the result by about one stop.

Low ISO often gives the most room for clean shadows and highlights. Higher ISO helps when you need a faster shutter or smaller aperture in dim light; noise can become more visible because those choices collect less light. The amount depends on the camera and the scene.

The balancing act: trade one setting for another

To keep the same picture brightness, a change in one setting can be offset by an equal change elsewhere. This is exposure reciprocity. The visual result can still change: a sharper moving subject, softer background or more visible noise.

A moving car in daylight

Suppose f/8, 1/125 s and ISO 100 give you the brightness you want, but the car is blurry. Moving the shutter from 1/125 → 1/250 → 1/500 s makes it two stops faster. The sensor now collects one quarter as much light, so the image will be two stops darker unless you compensate.

Open the aperture

Go f/8 → f/5.6 → f/4. Two stops more light restore the brightness, and the background may become softer.

Raise ISO

Keep f/8 and go ISO 100 → 200 → 400. The recorded brightness returns, but the sensor still captured one quarter as much light, so noise may be more visible.

Split the difference

Use f/5.6 for one stop more captured light and ISO 200 for one stop more recorded brightness.

The playground starts from a different balanced example: f/4, 1/250 s, ISO 100. Use its controls to make the same two-stop trade.

Why f-stops have strange numbers

The standard full-stop aperture sequence is f/1, f/1.4, f/2, f/2.8, f/4, f/5.6, f/8, f/11, f/16, f/22. Why isn't it simply 1, 2, 3, 4? Each circle below is drawn to scale for the same lens, and each one lets in half the light of the one before it.

Light follows the area

The f-number is the lens focal length divided by the diameter of the opening. On a 50 mm lens, f/2 is a 25 mm opening and f/4 is 12.5 mm. That is why a bigger number means a smaller opening.

The amount of light depends on the area of the circular aperture:

A = πr2

To halve the area, the diameter doesn't need to halve. It only needs to shrink by a factor of

√2 ≈ 1.414

That's where the f-stop sequence comes from.

Build the sequence yourself

Take f/2 and multiply by 1.414:

2 × 1.414 = 2.828 ≈ 2.8

So the next full stop is f/2.8. Then:

2.8 × 1.414 ≈ 4

Keep going and you get f/2, f/2.8, f/4, f/5.6, f/8. Each step gives half as much light.

It feels backward at first

f/2 to f/2.8
−1 stop of light
f/2.8 to f/2
+1 stop of light

A smaller f-number means a larger physical aperture, and more light.

Modern cameras click in thirds

Modern cameras usually adjust aperture, shutter speed and ISO in 1/3-stop increments, not only full stops. Each click is 1/3 stop, so three clicks make one full stop. Your camera may show:

Aperture

  1. f/2.8
  2. f/3.2
  3. f/3.5
  4. f/4

3 clicks, 1 stop less light

Shutter speed

  1. 1/125
  2. 1/160
  3. 1/200
  4. 1/250

3 clicks, 1 stop less light

ISO

  1. 100
  2. 125
  3. 160
  4. 200

3 clicks, 1 stop brighter

One click of light

A full stop doubles or halves the light. A third of a stop changes it by

21/3 ≈ 1.26

So each 1/3-stop click is roughly 1.26× the light, rather than 2×. Three clicks give 1.26 × 1.26 × 1.26 ≈ 2.

One click of aperture

Light goes with the diameter squared, so the f-number only needs to change by the square root of one click of light, √(21/3):

fnext = fcurrent × 21/6

That multiplier is about 1.122. Starting from f/2.8:

  1. 2.8 × 1.122 ≈ 3.14, marked f/3.2
  2. 3.2 × 1.122 ≈ 3.59, marked f/3.5
  3. 3.5 × 1.122 ≈ 3.93, marked f/4

Why is 3.14 marked f/3.2 and not f/3.1? The true value of f/2.8 is 2.83 (2 × √2), and 2.83 × 1.122 ≈ 3.17. The same happens with f/3.5, whose true value is 3.56, so the next click lands exactly on 4.

The 1/3-stop aperture sequence

The numbers on screen are rounded labels, and the camera uses the exact values. For example f/5.6 is really 5.66, f/11 is 11.3, and 1/125 s is really 1/128 s. The practical sequence is:

  1. f/1.4
  2. f/1.6
  3. f/1.8
  4. f/2
  5. f/2.2
  6. f/2.5
  7. f/2.8
  8. f/3.2
  9. f/3.5
  10. f/4
  11. f/4.5
  12. f/5
  13. f/5.6
  14. f/6.3
  15. f/7.1
  16. f/8
  17. f/9
  18. f/10
  19. f/11
  20. f/13
  21. f/14
  22. f/16

Bold values are full stops.