A Sailors have long been able to find their latitude, their distance north or south of the equator, by measuring the height of the Sun or a star above the horizon. Longitude, their position east or west, was a different matter. Because the Earth turns steadily, every hour of difference in local time between two places corresponds to fifteen degrees of longitude. A navigator who knew the time at home port and the local time on board could therefore work out how far east or west the ship had travelled.
B The difficulty was keeping accurate time at sea. Pendulum clocks, the best timekeepers on land, were useless on a rolling ship, and changes in temperature and humidity made other clocks run fast or slow. The cost of the problem was measured in lives and money: ships wandered off course, ran short of food and were wrecked on rocks they did not know were there. In 1714 the British government passed an Act offering a large prize for a method of finding longitude at sea to a stated accuracy.
C Many astronomers believed that the answer lay in the sky and proposed methods based on the movement of the Moon among the stars. These worked in principle but required difficult observations and long calculations that few sailors could perform on deck. The prize was eventually pursued most successfully by a carpenter and clockmaker, John Harrison, who spent decades building a series of increasingly refined timekeepers designed to keep steady time despite the motion of a ship.
D Harrison's final design, a large watch known as H4, was tested on a voyage to Jamaica in the early 1760s and lost only a few seconds during weeks at sea. Even so, the prize committee was slow to accept his achievement, partly because some members favoured the astronomical approach. In the end, it was the chronometer, a precise portable clock, that became the standard instrument for navigation, and it remained so until the arrival of satellite systems.