Equation of time — Clock by Joseph Williamson.jpg
Clock by Joseph Williamson.jpg — Andrewrabbott · CC BY-SA 4.0 · source

Complication

Equation of time

Also known as: Équation du temps · Zeitgleichung

How it works

A kidney-shaped cam turning once a year moves a hand or sector that shows the difference between mean time (as kept by a clock) and apparent solar time (as shown by a sundial). Running-equation displays add the correction to a second minute hand.

Why it was invented

When clocks became more regular than the sun, users needed to set them from sundials and to reconcile 'clock time' with 'sun time'.

Invented
c. 1695–1720
Credited to
Associated with Daniel Quare, Thomas Tompion and Joseph Williamson
Historical period
Early Modern Horology
Range
≈ −14 min 15 s (Feb) to +16 min 25 s (Nov)
Zero crossings
Mid-April, mid-June, early September, late December
Experiment in the Simulation Lab →

History and development

Equation clocks were made in London around 1695–1720; Joseph Williamson claimed in 1719 to have made equation work for the Spanish court. The difference reaches about −14 minutes in February and +16 minutes in early November.

Related mechanisms

Records are linked when the holding institution's description names this mechanism; check each source record for confirmation.