2,400 years from a hole in the wall to the camera in your pocket.
Nobody invented the camera in one go. A Chinese philosopher noticed that light through a small hole paints an upside-down picture. Arab and European scholars turned that into a tool. Chemists spent a century learning to make the picture stay. Then engineers made it fast, cheap, colourful, digital and, finally, part of everyone's phone. This is that story, one step at a time.
People notice that a small hole projects an upside-down image, explain why, and add a lens, an aperture and a mirror. There's still no way to keep the picture.
400 BCE
c. 400 BCE
The first written description of a pinhole image
Mozi and the MohistsChina
The Mohist Canon, a text associated with the philosopher Mozi, describes how light passing through a small hole forms an inverted image, and explains the inversion with light travelling in straight lines.
Why it mattered. It's the oldest known explanation of the principle every camera still uses.
The Problems, a work attributed to Aristotle or his school, asks why sunlight through a square gap makes a round spot, and why a partial solar eclipse throws crescent-shaped spots through gaps in leaves.
Why it mattered. An early record that small openings project the shape of the light source, not the shape of the hole.
In his Book of Optics, Ibn al-Haytham describes placing several candles outside a darkened room and seeing a separate image of each flame through the opening. Cover a candle and only its image disappears. He also argued, correctly, that we see because light enters the eye, not because the eye sends out rays.
Why it mattered. He turned the pinhole effect into a controlled experiment, and his Book of Optics shaped optics in Europe for centuries.
Gemma Frisius used a camera obscura to watch a solar eclipse safely, and in 1545 published a drawing of it: a room with a hole, and the eclipsed Sun projected on the far wall.
Why it mattered. The camera obscura became a scientific instrument, and astronomers kept using it to observe the Sun.
Della Porta's Magia Naturalis described the camera obscura as a way to entertain guests and help artists draw. Its 1589 edition added a lens and a mirror to turn the image the right way round.
Why it mattered. It made the camera obscura famous across Europe.
Barbaro described narrowing the opening in front of the lens to make the image sharper: the first recorded use of what we now call an aperture, or stopping down.
Why it mattered. Every camera since has let you trade light for sharpness this way.
Kepler used the Latin phrase camera obscura, “dark room”, and later built a portable tent version for drawing landscapes. He also explained how the eye's lens focuses an image on the retina.
Why it mattered. The English word “camera” comes from this: in Latin it simply means “room”.
Chemistry catches up with optics. Light-sensitive silver, then the first surviving photograph, then two rival processes announced in the same year.
1717
Silver darkens in light
Johann Heinrich SchulzeAltdorf, Germany
Schulze found that a mixture containing silver salts turned dark where light hit it, not because of heat. He made temporary words appear by covering a bottle with stencils.
Why it mattered. Light-sensitive silver was the heart of photography for the next 250 years.
Wedgwood captured silhouettes and camera images on paper or leather treated with silver nitrate, and Davy published the results. But they couldn't stop the images darkening, so they could only be looked at by candlelight.
Why it mattered. Capturing an image wasn't the hard part. Making it permanent was.
From an upstairs window, Niépce photographed the rooftops of his estate on a pewter plate coated with bitumen, which hardens in light. The exposure lasted at least eight hours, and probably several days, which is why sunlight falls on both sides of the buildings. He called the process heliography.
Why it mattered. It's the first camera image that still exists. You can see it at the Harry Ransom Center in Austin, Texas.
Daguerre photographed the busy Boulevard du Temple. The exposure was so long that moving traffic vanished, except a man having his boots polished, who stood still long enough to appear.
Why it mattered. It shows why exposure time mattered: anything that moved simply disappeared.
The French government bought Daguerre's process and published it for anyone to use. A daguerreotype was a one-off, astonishingly detailed image on a polished silver-coated copper plate, exposed for several minutes.
Why it mattered. Photography spread around the world within months. 19 August is still World Photography Day.
Herschel popularised “photography” (Greek for “drawing with light”) and later “negative” and “positive”. He also showed that sodium thiosulfate, “hypo”, fixes an image so it stops reacting to light.
Why it mattered. Hypo solved the problem that defeated Wedgwood.
Petzval calculated a portrait lens with an aperture of about f/3.6, many times brighter than the lenses on early daguerreotype cameras. Voigtländer built it into a camera in 1841.
Why it mattered. Exposures dropped to under a minute, and the portrait studio business was born.
Exposures fall from minutes to fractions of a second. Film comes on a roll, a camera costs a dollar, and colour arrives.
1851
Glass negatives in seconds
Frederick Scott ArcherLondon, England
The wet collodion process coated glass plates just before exposure. It combined the sharpness of the daguerreotype with printable negatives, and exposures fell to a few seconds.
Why it mattered. It made photography practical for portraits, war reporting and travel. Archer didn't patent it.
Richard Leach Maddox, Charles Bennett and othersEngland
Gelatin dry plates, proposed by Maddox in 1871 and made much more sensitive by Bennett in 1878, could be bought ready-made and kept for months. Exposures dropped to fractions of a second.
Why it mattered. Cameras could now be held by hand, and needed real shutters.
Muybridge lined up twelve cameras with very fast shutters triggered as a galloping horse passed. The photos proved that all four hooves leave the ground at once.
Why it mattered. A fast shutter showed something the human eye had never been able to see. It pointed the way to cinema.
Lala Deen Dayal set up studios in India and became court photographer to the Nizam of Hyderabad. His thousands of glass-plate negatives record late 19th-century India.
Why it mattered. He's one of the most celebrated early photographers in India.
The first Kodak came loaded with a roll for 100 pictures. When it was full, you mailed the whole camera back to Kodak, which developed the prints and reloaded the camera. A year later, Eastman switched to transparent celluloid film.
Why it mattered. Anyone could take photographs without knowing any chemistry.
Edgerton developed the electronic stroboscopic flash, with bursts of light lasting a tiny fraction of a second, and photographed bullets, milk drops and hummingbirds in mid-motion.
Why it mattered. Electronic flash is in almost every camera and phone.
The Kine Exakta is widely considered the first 35 mm single-lens reflex (SLR): a mirror shows you exactly what the lens sees, then flips up out of the way when you take the picture.
Why it mattered. Zahn's 1685 mirror, now inside a camera. SLRs dominated serious photography for half a century.
Land's three-year-old daughter asked why she couldn't see a photo straight away. The Polaroid Land Camera Model 95 answered her: a print developed inside the camera in about a minute.
Why it mattered. Instant results shaped how people expect photos to work, long before screens.
From a day-long exposure to one thirty-two-thousandth of a second: roughly a billion times faster. Values are typical for each technology and approximate.
1827 Niépce's heliograph: 8 hours or more
1839 Daguerreotype: several minutes
1841 Petzval lens: under a minute
1851 Wet collodion: a few seconds
1878 Dry plate: about 1/25 s
1925 Leica: 1/500 s
1959 Pro SLRs: 1/1000 s
1982 Film SLRs reach 1/4000 s
1988 Film SLRs reach 1/8000 s
2016 Electronic shutters: 1/32000 s
1957 – 2008
From film to pixels
Images become numbers. A chip that turns light into charge makes the digital camera possible, and it slowly replaces film.
1957
The first digital image
Russell KirschNational Bureau of Standards, Washington, USA
Kirsch scanned a photo of his baby son into a computer as a grid of 176 × 176 black-and-white dots.
Sasson's prototype weighed about 3.6 kg, captured a 100 × 100 pixel (0.01 megapixel) black-and-white image, and took 23 seconds to record it onto a cassette tape.
Why it mattered. Kodak had invented the technology that would later end its film business.
Kodak fitted a 1.3 megapixel sensor to a Nikon F3 body, wired to a separate storage unit. It was made for press photographers and cost tens of thousands of dollars.
Eric Fossum and teamNASA Jet Propulsion Laboratory, California, USA
Fossum's team developed the CMOS active-pixel sensor, which amplifies each pixel on the chip itself and can be made with ordinary chip-making processes.
Why it mattered. Cheap, low-power CMOS sensors are in almost every camera and phone today.
The company that put a camera in everyone's hands, and invented the digital camera, entered bankruptcy as film sales collapsed. It later re-emerged as a much smaller company.
Why it mattered. A famous lesson in how technology can overtake its own inventors.
Computational photography merges many quick frames into one picture, lining them up and averaging away noise. Night modes can make bright, clean photos in near darkness without a flash.
Why it mattered. Clever maths now does part of the job that big lenses and sensors used to do.
Event Horizon Telescope collaborationRadio telescopes around the world
Radio dishes on several continents worked together as one virtual telescope the size of the Earth to image the shadow of the black hole at the centre of the galaxy M87.
Why it mattered. Still the same idea as Mozi's hole in the wall: collect light (here, radio waves) and rebuild an image.
Rubin's LSST camera, about the size of a small car, has a 3,200 megapixel sensor. Its first images were released in 2025, and it will photograph the whole southern sky every few nights for ten years.
Why it mattered. From 0.01 megapixels in 1975 to 3,200 in 50 years.