For two centuries, perhaps the rarest of watchmaking complications has been the equation of time. Measuring the difference between the length of the solar day, which constantly varies over the course of the year, and the length of the standard 24-hour civil day, an equation of time display has graced only the most exclusive watches and clocks. Even more refined and exclusive is the equation of time display that shows both solar time and civil time with two separate minute hands. In all of watchmaking history, only a handful of the most important clock and pocket watches have featured this form of dual time, termed ‘equation marchante’ or ‘running equation’ display. Indeed equation marchante timepieces have been so exclusive that nearly every single one produced over the last two hundred years has been catalogued and recorded as a historically significant piece.
Blancpain startled the watchmaking world in 2004 when it revealed that it had succeeded in miniaturizing the running equation, which had previously only been built in large-scale clocks and pocket watches. At the Basel fair, Blancpain unveiled the first wristwatch in the world featuring a running equation of time, the Le Brassus Equation Marchante. This landmark timepiece was produced in a limited series of 50 pieces, which were all eagerly snapped up by passionate collectors. However to mark the seventh anniversary of Blancpain’s partnership with the Monaco Yacht Show, Blancpain has created a Limited Edition Le Brassus timepiece featuring an evolution of its world record-breaking equation marchante movement.It is modern convenience that our timepieces measure and display an exact 24-hour day. Were we more tied to the ancient sundial, we would know that the length of the day changes considerably over the course of the year. The variability in the length of the solar day is the result of what some may consider two flaws in the earth’s position relative to the sun. First the orbit of the earth is not round, but in fact highly elliptical. Second, instead of rotating on an axis which is perpendicular to the plane of the orbit, the earth is inclined at an angle of 23 degrees. These two abnormalities combine to produce days, which consist of a single rotation of the earth relative to the sun, of slightly longer or shorter length depending on the time of the year. Ancient astronomers fascinated by the movement of heavenly bodies, most particularly the most important orb in the sky, the sun, centuries ago began recording data showing the changes in the length of the solar day throughout the course of a year. Their findings have been most commonly expressed by a complex oblong chart termed an analemma. The twin kidney shape of the analemma shows that on but four days a year (April 15th, June 14th, September 2nd and December 26th – these dates change with the leap years) 24-hour civil time and solar time have caught up with each other. At other times the differences between the two may be as much as -16 minutes and + 15 minutes.