The British government was primarily motivated by the need to improve navigation and reduce the number of shipwrecks that occurred due to inaccurate longitude determination.

John Harrison was a British clockmaker who developed the first accurate marine chronometer, known as the H4, which revolutionized navigation and enabled precise determination of longitude at sea.

The primary difficulty in developing a marine chronometer was overcoming the effects of temperature variations, which caused the balance wheel to expand or contract, affecting the accuracy of the timekeeping mechanism.

John Harrison incorporated a bimetallic strip into his marine chronometer, which consisted of two strips of different metals with different coefficients of thermal expansion. This mechanism compensated for temperature variations by bending in opposite directions, maintaining the accuracy of the timekeeping mechanism.

John Harrison used HMS Deptford to test his marine chronometer during his final trial, which involved a voyage from England to Jamaica and back.

John Harrison spent approximately 40 years developing his marine chronometer, from its initial conception to its final successful trial.

The British Parliament passed the Longitude Act in 1714, offering a large reward of £20,000 for a method to accurately determine longitude at sea.

The British government established the Board of Longitude to oversee the competition for the longitude reward and evaluate the submitted proposals.

Christiaan Huygens proposed using the method of lunar distances to determine longitude at sea, which involved measuring the angular distance between the Moon and a known star or planet.

Giovanni Domenico Cassini developed a method for determining longitude using the eclipses of Jupiter's moons, which involved observing the times at which the moons disappeared behind the planet.

Edmund Halley proposed using a method based on the transits of Venus across the Sun to determine longitude at sea, which involved observing the times at which the planet crossed the Sun's disk.

James Cook led the expedition to observe the transit of Venus in 1769 from the island of Tahiti, which was part of a global effort to determine the distance between the Earth and the Sun.

Jean-Baptiste Chappe d'Auteroche led the expedition to observe the transit of Venus in 1769 from the island of Mauritius, which was part of a global effort to determine the distance between the Earth and the Sun.

Tobias Mayer developed a method for determining longitude using the occultations of stars by the Moon, which involved observing the times at which stars disappeared behind the Moon's disk.

Nevil Maskelyne developed a method for determining longitude using the method of lunar distances, which became the standard method for determining longitude at sea.