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Fresnel lenses

The stepped lens Augustin-Jean Fresnel presented in 1822 replaced heavy silvered mirrors with concentric rings of prisms. It cut the mass of glass by an order of magnitude and still threw a brighter beam, because the prisms bend stray light back into the horizontal plane instead of letting it escape upward. A first-order lens stands over two metres tall and was, for a century, the largest precision optic anyone made.

Characteristics

Every lighthouse blinks its own rhythm, called its character, so a navigator can identify the tower by timing the light alone — no chart lookup, no bearing needed. Charts write it in shorthand: Fl(3) W 20s means three white flashes in every twenty-second cycle. Oc is occulting, where the light is on longer than it is off; Iso splits the cycle evenly.

Keepers

Most towers were automated through the second half of the twentieth century, and the last keepers left in the 1990s in most countries. A handful still keep a resident keeper, almost entirely for heritage reasons rather than navigational ones.

Why any of this still runs

Satellite navigation made lighthouses redundant on paper decades ago. They stayed lit anyway, because a light needs no receiver, no power at the ship's end, and no working satellite — it fails visibly rather than silently, which is the property you actually want at three in the morning near a rock.