Metonic cycle


The Metonic cycle or enneadecaeteris is a period of almost exactly 19 years after which the lunar phases recur at the same time of the year. The recurrence is not perfect, and by precise observation the Metonic cycle defined as 235 synodic months is just 2 hours, 4 minutes and 58 seconds longer than 19 tropical years. Meton of Athens, in the 5th century BC, judged the cycle to be a whole number of days, 6,940. Using these whole numbers facilitates the construction of a lunisolar calendar.
A tropical year is longer than 12 lunar months and shorter than 13 of them. In a Metonic calendar, there are twelve years of 12 lunar months and seven years of 13 lunar months.

Application in traditional calendars

In the Babylonian and Hebrew lunisolar calendars, the years 3, 6, 8, 11, 14, 17, and 19 are the long years of the Metonic cycle. This cycle forms the basis of the Greek and Hebrew calendars. A 19-year cycle is used for the computation of the date of Easter each year.
The Babylonians applied the 19-year cycle from the late sixth century BC.
According to Livy, the second king of Rome, Numa Pompilius, inserted intercalary months in such a way that "in the twentieth year the days should fall in with the same position of the sun from which they had started". As "the twentieth year" takes place nineteen years after "the first year", this seems to indicate that the Metonic cycle was applied to Numa's calendar.
Diodorus Siculus reports that Apollo is said to have visited the Hyperboreans once every 19 years.
The Metonic cycle was implemented in the 2nd century BC Antikythera mechanism, which offers unexpected evidence for the popularity of the calendar based on it.
The Metonic cycle is a lunisolar cycle, as is the Callippic cycle. An important example of an application of the Metonic cycle in the Julian calendar is the 19-year lunar cycle insofar as provided with a Metonic structure. Meton introduced the 19 year cycle to the Attic calendar in 432 BC. In the following century, Callippus developed the Callippic cycle of four 19-year periods for a 76-year cycle with a mean year of exactly 365.25 days.
Around AD 260 the Alexandrian computist Anatolius, who became bishop of Laodicea in AD 268, was the first to devise a method for determining the date of Easter Sunday. However, it was some later, somewhat different, version of the Metonic 19-year lunar cycle which, as the basic structure of Dionysius Exiguus' and also of Bede's Easter table, would ultimately prevail throughout Christendom, at least until in the year 1582, when the Gregorian calendar was introduced.
The Coligny calendar is a Celtic lunisolar calendar using the Metonic cycle. The bronze plaque on which it was found dates from c. AD 200, but the internal evidence points to the calendar itself being several centuries older, created in the Iron Age or late Bronze Age.
The Metonic cycle is thought to be numerically encoded on the Berlin Gold Hat from central Europe, dating from c. 1000-800 BC.
The Runic calendar is a perpetual calendar based on the 19-year-long Metonic cycle. It is also known as a Rune staff or Runic Almanac. This calendar does not rely on knowledge of the duration of the tropical year or of the occurrence of leap years. It is set at the beginning of each year by observing the first full moon after the winter solstice. The oldest one known, and the only one from the Middle Ages, is the Nyköping staff, which is believed to date from the 13th century.
The Bahá'í calendar, established during the middle of the 19th century, is also based on cycles of 19 solar years.

Hebrew calendar

A Small Maḥzor is a 19-year cycle in the lunisolar calendar system used by the Jewish people. It is similar to, but slightly different in usage from, the Greek Metonic cycle, and likely derived from or alongside the much earlier Babylonian calendar.

Polynesia

It is possible that the Polynesian kilo-hoku discovered the Metonic cycle in the same way Meton had, by trying to make the month fit the year.

Mathematical basis

The Metonic cycle is the most accurate cycle of time for synchronizing the tropical year and the lunar month, when the method of synchronizing is the intercalation of a thirteenth lunar month in a calendar year from time to time. The traditional lunar year of 12 synodic months is about 354 days, approximately eleven days short of the solar year. Thus, every 2 to 3 years there is a discrepancy of 22 to 33 days, or a full synodic month. For example, if the winter solstice and the new moon coincide, it takes 19 tropical years for the coincidence to recur. The mathematical logic is this:
  • A tropical year lasts 365.2422 days.
  • :a span of 19 tropical years lasts 6,939.602 days
That duration is almost the same as 235 synodic months:
  • A synodic month lasts 29.53059 days.
  • :a span of 235 synodic months lasts 6,939.689 days
Thus the algorithm is correct to 0.087 days.
For a lunisolar calendar to 'catch up' to this discrepancy and thus maintain seasonal consistency, seven intercalary months are added, at intervals of every 2–3 years during the course of 19 solar years. Thus twelve of those years have 12 lunar months and seven have 13 months. Of these months, 125 were full and 110 were deficient, to give a total of 6940 days.