Lunisolar
calendar
From Wikipedia, the free encyclopedia
A lunisolar calendar is a calendar
in many cultures
whose date indicates both the moon phase
and the time of the solar year. If the solar year is defined as a tropical year,
then a lunisolar calendar will give an indication of the season; if it is taken as a sidereal year,
then the calendar will predict the constellation
near which the full moon may occur. Usually there is an additional requirement that
the year have a whole number of months, in which case most years have 12 months
but every second or third year has 13.
Examples
The Hebrew,
Buddhist, Hindu,
Burmese, Bengali,
and Tibetan calendars, as well as the traditional Chinese,
Japanese, Vietnamese, Mongolian and Korean
calendars, plus the ancient Hellenic, Coligny,
and Babylonian calendars are all lunisolar. Also some of the ancient pre-Islamic calendars in South Arabia
followed a lunisolar system.[1]
The Chinese, Coligny and Hebrew[2]
lunisolar calendars track more or less the tropical year
whereas the Buddhist and Hindu lunisolar calendars track the sidereal year.
Therefore, the first three give an idea of the seasons whereas the last two
give an idea of the position among the constellations of the full moon. The
Tibetan calendar was influenced by both the Chinese and Hindu calendars. The Germanic peoples also used a lunisolar calendar before their conversion to Christianity.
The Islamic calendar is lunar,
but not a lunisolar calendar because its date is not related to the sun. The
civil versions of the Julian
and Gregorian calendars are solar,
because their dates do not indicate the moon phase — however, both the
Gregorian and Julian calendars include undated lunar calendars that allow them
to calculate
the Christian celebration of Easter, so both are lunisolar calendars in
that respect.
Determining
leap months
To determine when an embolismic month needs to be inserted, some calendars rely on direct observations
of the state of vegetation, while others compare the ecliptic longitude of the sun and the phase of the moon. The Hawaiians observe the movement of specific stars and
insert months accordingly.
On the other hand, in arithmetical
lunisolar calendars, an integral number of months is fitted into some integral
number of years by a fixed rule. To construct such a calendar (in principle),
the average length of the tropical year
is divided by the average length of the synodic month,
which gives the number of average synodic months in a tropical year as:
12.368266......
Continued fractions of this decimal value ([12; 2, 1, 2, 1, 1, 17, ...]) give
optimal approximations for this value. So in the list below, after the number
of synodic months listed in the numerator, approximately an integer number of
tropical years as listed in the denominator have been completed:
12
/
|
1
=
|
12
|
= [12]
|
(error =
|
−0.368266...
synodic months/year)
|
25
/
|
2
=
|
12.5
|
= [12; 2]
|
(error =
|
0.131734...
synodic months/year)
|
37
/
|
3
=
|
12.333333...
|
= [12; 2, 1]
|
(error =
|
−0.034933...
synodic months/year)
|
99
/
|
8
=
|
12.375
|
= [12; 2, 1, 2]
|
(error =
|
0.006734...
synodic months/year)
|
136
/
|
11
=
|
12.363636...
|
= [12; 2, 1, 2, 1]
|
(error =
|
−0.004630...
synodic months/year)
|
235
/
|
19
=
|
12.368421...
|
= [12; 2, 1, 2, 1, 1]
|
(error =
|
0.000155...
synodic months/year)
|
4131
/
|
334
=
|
12.368263...
|
= [12; 2, 1, 2, 1, 1, 17]
|
(error =
|
−0.000003...
synodic months/year)
|
Note however that in none of the
arithmetic calendars is the average year length exactly equal to a true
tropical year. Different calendars have different average year lengths and
different average month lengths, so the discrepancy between the calendar months
and moon is not equal to the values given above.
The 8-year cycle (99 synodic months,
including 99−8×12 = 3 embolismic months) was used in the ancient Athenian
calendar. The 8-year cycle was also used in early third-century Easter calculations (or old Computus) in Rome and Alexandria.
The 19-year cycle (235 synodic
months, including 235−19×12 = 7 embolismic months) is the classic Metonic cycle,
which is used in most arithmetical lunisolar calendars. It is a combination of
the 8- and 11-year period, and whenever the error of the 19-year approximation
accumulates to 1⁄19 of a mean month, a cycle can be
truncated to 11 years (skipping 8 years including 3 embolismic months), after
which 19-year cycles can resume. Meton's cycle had an integer number of
days, although Metonic cycle often means its use without an integer
number of days. It was adapted to a mean year of 365.25 days by means of the
4×19 year Callipic cycle (used in the Easter calculations of the Julian calendar).
Rome used an 84-year cycle for Easter calculations from the late third century until 457. Early Christians in
Britain and Ireland also used an 84-year cycle until the Synod of Whitby
in 664. The 84-year cycle is equivalent to a Callipic 4×19-year cycle
(including 4×7 embolismic months) plus an 8-year cycle (including 3 embolismic
months) and so has a total of 1039 months (including 31 embolismic months).
This gives an average of 12.3690476... months per year. One cycle was 30681
days, which is about 1.28 days short of 1039 synodic months, 0.66 days more
than 84 tropical years, and 0.53 days short of 84 sidereal years.
The next approximation (arising from
continued fractions) after the Metonic cycle (such as a 334-year cycle) is very
sensitive to the values one adopts for the lunation (synodic month) and the
year, especially the year. There are different possible definitions of the year
so other approximations may be more accurate for specific purposes. For example
a 353-year cycle including 130 embolismic months for a total of 4366 months
(12.36827195...) is more accurate for a northern hemisphere spring equinox
year, whereas a 611-year cycle including 225 embolismic months for a total of
7557 months (12.36824877...) has good accuracy for a northern hemisphere summer
solstice year, and a 160-year cycle including 59 embolismic months for a total
of 1979 months (12.36875) has good accuracy for a sidereal year (approx
12.3687462856 synodic months).
Calculating
a leap month
A rough idea of the frequency of the
intercalary or leap month in all lunisolar calendars can be obtained by the
following calculation, using approximate lengths of months and years in days:
- Year: 365.25, Month: 29.53
- 365.25/(12 × 29.53) = 1.0307
- 1/0.0307 = 32.57 common months between leap months
- 32.57/12 = 2.7 common years between leap years
A representative sequence of common
and leap years is ccLccLcLccLccLccLcL, which is the classic nineteen-year Metonic cycle.
The Buddhist and Hebrew calendars restrict the leap month to a single month of
the year; the number of common months between leap months is, therefore,
usually 36, but occasionally only 24 months. Because the Chinese and Hindu
lunisolar calendars allow the leap month to occur after or before
(respectively) any month but use the true motion of the sun, their leap months do not usually
occur within a couple of months of perihelion,
when the apparent speed of the sun along the ecliptic
is fastest (now about 3 January). This increases the usual number of common
months between leap months to roughly 34 months when a doublet of common years
occurs, while reducing the number to about 29 months when only a common
singleton occurs.
Lunisolar
calendars with uncounted time
An alternative way of dealing with
the fact that a solar year does not contain an integer number of months is by
including uncounted time in the year that does not belong to any month. Some Coast Salish peoples used a calendar of this kind. For instance, the Chehalis
began their count of lunar months from the arrival of spawning Chinook salmon
(in Gregorian calendar October), and counted 10 months, leaving an uncounted
period until the next Chinook salmon run.[3]
Gregorian
lunisolar calendar
The Gregorian Calendar has a
lunisolar calendar, which is used to determine the date of Easter. The rules are in the Computus.
The entire wiki link can be found at:
http://en.wikipedia.org/wiki/Lunisolar_calendar
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