The Lens That Changed Lighthouses
For centuries, sailors depended on lighthouses to warn them of rocks and guide them safely into harbor. Early lighthouses burned wood or coal fires on top of towers, and later ones used oil lamps. These lights were dim and wasteful, because a lamp sends its glow out in every direction, and most of it shines out over empty sea or up into the sky.
In the 1820s, a French physicist named Augustin Fresnel solved the problem with a new kind of lens. A normal lens strong enough for a lighthouse would have been enormously thick and heavy, and it would have absorbed much of the light. Fresnel's idea was to build the lens from many separate rings of glass, each one cut at a carefully chosen angle. The rings bend the light that hits them and gather it into one narrow, powerful beam. The finished lens looked like a giant glass beehive, yet it was much thinner and lighter than a solid lens of equal strength.
The lens was usually set on a rotating platform, so the beam swept across the sea like the hand of a clock. A sailor saw a flash each time the beam passed. Each lighthouse was given its own pattern of flashes, such as two quick flashes followed by a pause, so that a captain could tell which one was in view and work out the ship's position.
Fresnel lenses made lights shine much farther, and the beams of the largest ones could be seen from more than twenty miles away. Today, ships rely mostly on satellite navigation, and many lighthouses now use electric bulbs or LEDs, but some old Fresnel lenses are still working, and others are preserved in museums.