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Metonic cycle
For astronomy and calendar studies, the Metonic cycle or Enneadecaeteris (from Ancient Greek: ἐννεακαιδεκαετηρίς, "nineteen years") is a period of very close to 19 years that is remarkable for being nearly a common multiple of the solar year and the synodic (lunar) month. The Greek astronomer Meton of Athens (fifth century BC) observed that a period of 19 years is almost exactly equal to 235 synodic months and, rounded to full days, counts 6,940 days. The difference between the two periods (of 19 years and 235 synodic months) is only a few hours, depending on the definition of the year.
Considering a year to be ^{1}⁄_{19} of this 6,940day cycle gives a year length of 365 + ^{1}⁄_{4} + ^{1}⁄_{76} days (the unrounded cycle is much more accurate), which is slightly more than 12 synodic months. To keep a 12month lunar year in pace with the solar year, an intercalary 13th month would have to be added on seven occasions during the nineteenyear period (235 = 19 × 12 + 7). When Meton introduced the cycle around 432 BC, it was already known by Babylonian astronomers.
A mechanical computation of the cycle is built into the Antikythera mechanism.
The cycle was used in the Babylonian calendar, ancient Chinese calendar systems (the 'Rule Cycle' 章) and the medieval computus (i.e. the calculation of the date of Easter). It regulates the 19year cycle of intercalary months of the Hebrew calendar.
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Mathematical basis
At the time of Meton, axial precession had not yet been discovered, and he could not distinguish between sidereal years (currently: 365.256363 days) and tropical years (currently: 365.242190 days). Most calendars, like the commonly used Gregorian calendar, are based on the tropical year and maintain the seasons at the same calendar times each year. Nineteen tropical years are about two hours shorter than 235 synodic months. The Metonic cycle's error is, therefore, one full day every 219 years, or 12.4 parts per million.
 19 tropical years = 6,939.602 days (12 × 354day years + 7 × 384day years + 3.6 days).
 235 synodic months (lunar phases) = 6,939.688 days (Metonic period by definition).
 254 sidereal months (lunar orbits) = 6,939.702 days (19 + 235 = 254).
 255 draconic months (lunar nodes) = 6,939.1161 days.
Note that the 19year cycle is also close (to somewhat more than half a day) to 255 draconic months, so it is also an eclipse cycle, which lasts only for about 4 or 5 recurrences of eclipses. The Octon is ^{1}⁄_{5} of a Metonic cycle (47 synodic months, 3.8 years), and it recurs about 20 to 25 cycles.
This cycle seems to be a coincidence. The periods of the Moon's orbit around the Earth and the Earth's orbit around the Sun are believed to be independent, and not to have any known physical resonance except with each other. An example of a noncoincidental cycle is the orbit of Mercury, with its 3:2 spinorbit resonance.
A lunar year of 12 synodic months is about 354 days, approximately 11 days short of the "365day" solar year. Therefore, for a lunisolar calendar, every 2 to 3 years there is a difference of more than a full lunar month between the lunar and solar years, and an extra (embolismic) month needs to be inserted (intercalation). The Athenians initially seem not to have had a regular means of intercalating a 13th month; instead, the question of when to add a month was decided by an official. Meton's discovery made it possible to propose a regular intercalation scheme. The Babylonians seem to have introduced this scheme around 500 BC, thus well before Meton.
Application in traditional calendars
Traditionally, for the Babylonian and Hebrew lunisolar calendars, the years 3, 6, 8, 11, 14, 17, and 19 are the long (13month) years of the Metonic cycle. This cycle, which can be used to predict eclipses, forms the basis of the Greek and Hebrew calendars, and is used for the computation of the date of Easter each year.
The Babylonians applied the 19year cycle since the late sixth century BC. As they measured the moon's motion against the stars, the 235:19 relationship may originally have referred to sidereal years, instead of tropical years as it has been used for various calendars.
Apollo was said to have visited the Hyperboreans once every 19 years, presumably at the high point of the cycle.
The Runic calendar is a perpetual calendar based on the 19yearlong Metonic cycle. Also known as a Rune staff or Runic Almanac, it appears to have been a medieval Swedish invention. 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 years.
Further details
The Metonic cycle is related to two less accurate subcycles:
 8 years = 99 lunations (an Octaeteris) to within 1.5 days, i.e. an error of one day in 5 years; and
 11 years = 136 lunations within 1.5 days, i.e. an error of one day in 7.3 years.
By combining appropriate numbers of 11year and 19year periods, it is possible to generate ever more accurate cycles. For example, simple arithmetic shows that:
 687 tropical years = 250,921.39 days;
 8,497 lunations = 250,921.41 days.
This gives an error of only about half an hour in 687 years (2.5 seconds a year), although this is subject to secular variation in the length of the tropical year and the lunation.
Meton of Athens approximated the cycle to a whole number (6,940) of days, obtained by 125 long months of 30 days and 110 short months of 29 days. During the next century, Callippus developed the Callippic cycle of four 19year periods for a 76year cycle with a mean year of exactly 365.25 days.
See also
 Octaeteris (8year cycle of antiquity)
 Callippic cycle (74year cycle from 330 BC)
 Hipparchic cycle (304year cycle from 2nd century BC)
 Saros cycle of eclipses
 Attic & Byzantine calendar
 Chinese calendar
 Hebrew calendar
 Runic calendar
 Julian day
External links
References
 Mathematical Astronomy Morsels, Jean Meeus, WillmannBell, Inc., 1997 (Chapter 9, p. 51, Table 9.A Some eclipse Periodicities)
