The lunar tables of Tobias Mayer

1752-1770 Number and measure method

Astronomical tables giving the Moon's position at any moment of time to within about a minute of arc: this is the threshold at which the Moon can serve as a clock for finding longitude at sea. An error of one minute of arc is roughly half a degree of longitude, the limit set by the reward of 1714.

Gravitational theory alone was not enough for that. The German astronomer Tobias Mayer took the equations to which Euler had reduced lunar theory and fitted their coefficients to long runs of observations, joining a derivation from theory to a treatment of data. Using his tables the Astronomer Royal James Bradley at Greenwich obtained the Moon's place accurately enough to determine longitude at sea to within half a degree.

The Board of Longitude accepted the tables but judged them unusable at sea as they stood: working through them cost the mariner hours. Mayer's widow received 3,000 pounds from the Board, and the tables themselves became the numerical foundation of the first ten issues of the Nautical Almanac.

Why this date

a spread. The tables were communicated to the Royal Society of Sciences at Gottingen in 1752 and printed in its transactions; a corrected manuscript was sent to the British government in 1755 and compared by Bradley with the Greenwich observations (this version, according to Wepster, was never published); the version of 1762 underlay the first issues of the Nautical Almanac; an improved set appeared posthumously in London in 1770, and the theory behind it, Theoria lunae juxta systema Newtonianum, in 1767. The axis value is 1755, the year of the first documented application, that is of the submission to Britain and Bradley's check: the year of the Gottingen volume could not be verified.

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