Glossary · Regulation
Lunar-distance method
Determining reference time from the angular separation of the Moon and another celestial object.
Explanation
The lunar-distance method compares a measured celestial separation with predicted positions to infer reference time. It requires suitable observations, corrections and astronomical tables, not simply reading a sextant angle as longitude. Royal Museums Greenwich explains the roles of Tobias Mayer’s tables, Nevil Maskelyne and the Nautical Almanac, and the long calculations involved. Astronomical methods and chronometers coexisted; the method should not be described as instantly displaced by Harrison’s watch.