In 1670, a new unit of length was proposed by French abbot, Gabriel Mouton, linked to what was considered a physical constant at the time – the Earth’s circumference. Almost a century later, in 1790, the Academy of Sciences started to work on the best way to standardise length based on Mouton’s ideas. It was decided that the new unit, the ‘metre’, would be determined as 1/10,000,000th of the distance from the North Pole to the Equator.
This became a reality three years later, with the creation and deposition of two metre standards in the Archives de la République in Paris. From this new measurement of length, two further units were derived; the kilogram (defined as the weight of water in a cube whose sides are one-tenth of one metre), and the litre (defined as the volume of one kilogram of water).
This new system slowly gained acceptance, and, on 20 May 1875, 17 nations signed the ‘Metre Convention’ with the aim of promoting the metric system, creating standards for the metre and the kilogram, and setting up an organisation to maintain and coordinate comparisons. Another important step was the incorporation of the ‘astronomical second’ as the unit of time.
At the 11th meeting of Metre Convention signatories in 1960 (otherwise known as the General Conference on Weights and Measures), the International System of Units (Système International d'Unités) - or SI - was introduced. Three further units were ratified for use in the system; the ampere (electrical current), the kelvin (thermodynamic temperature) and the candela (luminous intensity). Eleven years later, the mole was added as well, the unit for the amount of a substance, completing the set of SI base units that are in use today.


