Date of Easter

Computus (Latin for "computation") is the calculation used to determine the calendar date of Easter. Because the date is based on a calendar-dependent equinox rather than the astronomical one, there are differences between calculations done according to the Julian calendar and the modern Gregorian calendar. The name has been used for this procedure since the early Middle Ages, as it was considered the most important computation of the age.

For most of its history Christians have calculated Easter independently of the Jewish calendar. In principle, Easter falls on the Sunday following the full moon that follows the northern spring equinox (the paschal full moon). However, the vernal equinox and the full moon are not determined by astronomical observation. The vernal equinox is fixed to fall on 21 March (previously it varied in different areas and in some areas Easter was allowed to fall before the equinox). The full moon is an ecclesiastical full moon determined by reference to a lunar calendar, which again varied in different areas. While Easter now falls at the earliest on the 15th of the lunar month and at the latest on the 21st, in some areas it used to fall at the earliest on the fourteenth (the day of the paschal full moon) and at the latest on the twentieth, or between the sixteenth and the 22nd. The last limit arises from the fact that the crucifixion was considered to have happened on the fourteenth (the eve of the Passover) and the resurrection therefore on the sixteenth. The "computus" is the procedure of determining the first Sunday after the first ecclesiastical full moon falling on or after 21 March, and the difficulty arose from doing this over the span of centuries without accurate means of measuring the precise tropical year. The synodic month had already been measured to a high degree of accuracy. The schematic model that eventually was accepted is the Metonic cycle which equates 19 (tropical) years to 235 synodic months.

In 1583, the Catholic Church began using 21 March under the Gregorian calendar to calculate the date of Easter, while the Eastern Churches have continued to use 21 March under the Julian calendar. The Catholic and Protestant denominations thus use an ecclesiastical full moon that occurs four, five or 34 days earlier than the eastern one.

The earliest and latest dates for Easter are 22 March and 25 April. In the Western/Gregorian calendar those dates are as commonly understood. However, in the Orthodox/Eastern Churches, while those dates are the same, they are reckoned using the Julian calendar; therefore, on the Gregorian calendar as of the 21st century, those dates are 4 April and 8 May.

History

Main article: Easter controversy

Easter is the most important Christian feast, and the proper date of its celebration has been the subject of controversy as early as the meeting of Anicetus and Polycarp around 154. According to Eusebius' Church History, quoting Polycrates of Ephesus, churches in the Roman Province of Asia "always observed the day when the people put away the leaven", namely Passover, the 14th of the lunar month of Nisan. The rest of the Christian world at that time, according to Eusebius, held to "the view which still prevails", of always fixing Easter on Sunday. Eusebius does not say how the Sunday was decided. Other documents from the 3rd and 4th centuries reveal that the customary practice was for Christians to consult their Jewish neighbors to determine when the week of Unleavened Bread would fall, and to set Easter on the Sunday that fell within that week.

By the end of the 3rd century some Christians had become dissatisfied with what they perceived as the disorderly state of the Jewish calendar. The chief complaint was that the Jewish practice sometimes set the 14th of Nisan before the spring equinox. This is implied by Dionysius, bishop of Alexandria in the mid-3rd century, who stated that "at no time other than the spring equinox is it legitimate to celebrate Easter" (Eusebius, Church History 7.20); and by Anatolius of Alexandria (quoted in Eusebius, Church History 7.32) who declared it a "great mistake" to set the paschal lunar month when the sun is in the twelfth sign of the zodiac (i.e., before the equinox). And it was explicitly stated by Peter, bishop of Alexandria that "the men of the present day now celebrate [Passover] before the [spring] equinox...through negligence and error." Another objection to using the Jewish computation may have been that the Jewish calendar was not unified. Jews in one city might have a method for reckoning the Week of Unleavened Bread different from that used by the Jews of another city. Because of these perceived defects in the traditional practice, Christian computists began experimenting with systems for determining Easter that would be free of these defects. But these experiments themselves led to controversy, since some Christians held that the customary practice of holding Easter during the Jewish festival of Unleavened Bread should be continued, even if the Jewish computations were in error from the Christian point of view.

At the First Council of Nicaea in 325, it was agreed that the Christians should observe a common date, independent from the Jewish method. Because of the divergence of tables mentioned above it was usual to negotiate a common date when discrepancies arose. It took several centuries before a common method was accepted throughout Christendom. The process of working out the details generated still further controversies.

The method from Alexandria became authoritative. In its developed form it was based on the epacts of a reckoned moon according to the 19-year cycle (a.k.a. the Metonic Cycle). Such a cycle was first proposed by Bishop Anatolius of Laodicea (in present-day Syria), c. 277. Alexandrian Easter tables were composed by Bishop Theophilus about 390 and within the bishopric of Cyril about 444. In Constantinople, several computists were active over the centuries after Anatolius (and after the Nicaean Council), but their Easter dates coincided with those of the Alexandrians. Having deviated from the Alexandrians during the 6th century, churches beyond the eastern frontier of the former Byzantine Empire, including the Assyrian Church of the East, now celebrate Easter on different dates from Eastern Orthodox churches four times every 532 years. The Alexandrian computus was converted from the Alexandrian calendar into the Julian calendar in Rome by Dionysius Exiguus, though only for 95 years. Dionysius introduced the Christian Era (counting years from the Incarnation of Christ) when he published new Easter tables in 525.

Dionysius's tables replaced earlier methods used by the Church of Rome. The earliest known Roman tables were devised in 222 by Hippolytus of Rome based on 8-year cycles. Then 84-year tables were introduced in Rome by Augustalis near the end of the 3rd century. A completely distinct 84 - year cycle, the Insular latercus, was used in the British Isles. These old tables were used in Northumbria until 664, and by isolated monasteries as late as 931. A modified 84-year cycle was adopted in Rome during the first half of the 4th century. Victorius of Aquitaine tried to adapt the Alexandrian method to Roman rules in 457 in the form of a 532-year table, but he introduced serious errors. These Victorian tables were used in Gaul (now France) and Spain until they were displaced by Dionysian tables at the end of the 8th century.

In the British Isles Dionysius' and Victorius's tables conflicted with the indigenous tables. These employed an 84-year cycle because this meant the dates of Easter would repeat every 84 years, but there was an error which caused the full moons to fall progressively too early. Add to that the fact that Easter could fall at earliest on the fourteenth day of the lunar month and it was often the case that Eanfleda, who followed the Roman system, was fasting on Palm Sunday at the same time as her husband Oswy, king of Northumbria, was feasting on Easter Sunday. The Irish Synod of Mag Léne in 631 decided in favor of either the Dionysian or Victorian Easter and the northern English Synod of Whitby in 664 adopted the Dionysian tables. Bede records that "there happened an eclipse of the sun on the third of May, about ten o'clock in the morning." The time is correct but the date is two days late. This was done to conceal the inaccuracy that had accumulated in the new cycle since it was originally constructed.

The Dionysian reckoning was fully described by Bede in 725. It may have been adopted by Charlemagne for the Frankish Church as early as 782 from Alcuin, a follower of Bede. The Dionysian/Bedan computus remained in use in Western Europe until the Gregorian calendar reform, and remains in use in most Eastern Churches, including most Eastern Orthodox Churches and Oriental Orthodox Churches. Churches beyond the eastern frontier of the former Byzantine Empire use an Easter that differs four times every 532 years from this Easter, including the Assyrian Church of the East.

The Gregorian Easter has been used since 1583 by the Catholic Church and was adopted by most Protestant churches between 1753 and 1845. German Protestant states used an astronomical Easter based on the Rudolphine Tables of Johannes Kepler between 1700 and 1774, while Sweden used it from 1739 to 1844. This astronomical Easter was one week before the Gregorian Easter in 1724, 1744, 1778, 1798, etc.

Theory

Template:Dates for Easter The Easter cycle groups days into lunar months, which are either 29 or 30 days long. There is an exception. The month ending in March normally has thirty days, but if 29 February of leap year falls within it, it contains 31. As these groups are based on the lunar cycle, over the long term, the average month in the lunar calendar is a very good approximation of the synodic month, which is 29.53058872 days long. There are 12 synodic months in a lunar year, totaling either 354 or 355 days. The lunar year is about 11 days shorter than the solar year, which is either 365 or 366 days long. These days by which the solar year exceeds the lunar year are called epacts (Greek: ἐπακταὶ ἡμέραι, translit. epaktai hēmerai, lit. "intercalary days"). It is necessary to add them to the day of the solar year to obtain the correct day in the lunar year. Whenever the epact reaches or exceeds 30, an extra intercalary month (or embolismic month) of 30 days has to be inserted into the lunar calendar: then 30 has to be subtracted from the epact. The Rev C Wheatly provides the detail:

"Thus beginning the year with March (for that was the ancient custom) they allowed thirty days for the moon [ending] in March, and twenty - nine for that [ending] in April; and thirty again for May, and twenty - nine for June &c. according to the old verses:

Impar luna pari, par fiet in impare mense;

In quo completur mensi lunatio detur.

"For the first, third, fifth, seventh, ninth, and eleventh months, which are called impares menses, or unequal months, have their moons according to computation of thirty days each, which are therefore called pares lunae, or equal moons: but the second, fourth, sixth, eighth, tenth, and twelfth months, which are called pares menses, or equal months, have their moons but twenty nine days each, which are called impares lunae, or unequal moons."

The nineteen-year Metonic cycle assumes that 19 tropical years are as long as 235 synodic months. So after 19 years the lunations should fall the same way in the solar years, and the epacts should repeat. However, 19 × 11 = 209 ≡ 29 (mod 30), not 0 (mod 30); that is, 209 divided by 30 leaves a remainder of 29 instead of being a multiple of 30. So after 19 years, the epact must be corrected by +1 day in order for the cycle to repeat. This is the so-called saltus lunae or moon's leap, and it is handled by having three consecutive months of 29 days in the summer of the last year in the cycle. The extra 209 days are made up of seven embolismic months of thirty days, for a total of (19 × 12) + 7 = 235 lunations, less the one day removed from the second of the three successive 29 - day months in the last year of the cycle. The sequence number of the year in the 19-year cycle is called the "Golden Number", and is given by the formula

GN = Y mod 19 + 1

That is, the remainder of the year number Y in the Christian era when divided by 19, plus one.

Using the method just described, a period of 19 calendar years is also divided into 19 lunar years of 12 or 13 lunar months each. In each calendar year (beginning on 1 January) one of the lunar months must be the first one within the calendar year to have its 14th day (its formal full moon) on or after 21 March. This lunar month is the paschal or Easter-month, and Easter is the Sunday after its 14th day (or, saying the same thing, the Sunday within its third week.) The paschal lunar month always begins on a date in the 29-day period from 8 March to 5 April inclusive. Its 14th day, therefore, always falls on a date between 21 March to 18 April inclusive, and the following Sunday then necessarily falls on a date in the range 22 March to 25 April inclusive. In the solar calendar Easter is called a moveable feast since its date varies within a 35-day range. But in the lunar calendar, Easter is always the third Sunday in the paschal lunar month, and is no more "moveable" than any holiday that is fixed to a particular day of the week and week within a month.

Tabular methods

Gregorian calendar

As reforming computus was the primary motivation for the introduction of the Gregorian calendar in 1582, a corresponding computus methodology was introduced alongside the calendar. The general method of working was given by Clavius in the Six Canons (1582), and a full explanation followed in his Explicatio (1603).

Easter Sunday is the Sunday following the paschal full moon date. The paschal full moon date is the ecclesiastical full moon date following 20 March. The Gregorian method derives paschal full moon dates by determining the epact for each year. The epact can have a value from * (=0 or 30) to 29 days. The first day of a lunar month is considered the day of the crescent new moon. The 14th day is considered the day of the full moon.

Historically the paschal full moon date for a year was found from its sequence number in the Metonic cycle, called the golden number, which cycle repeats the lunar phase on a certain date every 19 years. This method was abandoned in the Gregorian reform because the tabular dates go out of sync with reality after about two centuries, but from the epact method a simplified table can be constructed that has a validity of one to three centuries.

The epacts for the current Metonic cycle, which began in 2014, are:

Year	2014	2015	2016	2017	2018	2019	2020	2021	2022	2023	2024	2025	2026	2027	2028	2029	2030	2031	2032
Golden Number	1	2	3	4	5	6	7	8	9	10	11	12	13	14	15	16	17	18	19
Epact	29	10	21	2	13	24	5	16	27	8	19	*	11	22	3	14	25	6	17
Paschal Full Moon date	14A	3A	23M	11A	31M	18A	8A	28M	16A	5A	25M	13A	2A	22M	10A	30M	17A	7A	27M
Arrangement according to the regular pattern of lunisolar calendars (GN + 8 mod 19 for decreasing Epact and increasing date)
Golden Number	14	3	11	19	8	16	5	13	2	10	18	7	15	4	12	1	9	17	6
Epact	22	21	19	17	16	14	13	11	10	8	6	5	3	2	*	29	27	25	24
Paschal Full Moon date	22M	23M	25M	27M	28M	30M	31M	2A	3A	5A	7A	8A	10A	11A	13A	14A	16A	17A	18A

(M=March, A=April)

This table can be extended for previous and following 19-year periods. A formula for paschal full moon date can be derived from the table and is valid from 1900 to 2199.

PFMd = 45 - (Y mod 19 × 11) mod 30

if Y mod 19 = 5 or 16, add 29

if Y mod 19 = 8 add 30

if the result is over 31, subtract 31 (and the month is April, instead of March)

For the example of 2013 (mod 19 = 18), PFMd = 45 - (18 × 11) mod 30 = 45 - 18 = 27M.

The epacts are used to find the dates of the new moon in the following way: Write down a table of all 365 days of the year (the leap day is ignored). Then label all dates with a Roman number counting downwards, from "*" (= 0 or 30), "xxix" (29), down to "i" (1), starting from 1 January, and repeat this to the end of the year. However, in every second such period count only 29 days and label the date with xxv (25) also with xxiv (24). Treat the 13th period (last eleven days) as long, therefore, and assign the labels "xxv" and "xxiv" to sequential dates (26 and 27 December respectively). Finally, in addition, add the label "25" to the dates that have "xxv" in the 30-day periods; but in 29-day periods (which have "xxiv" together with "xxv") add the label "25" to the date with "xxvi". The distribution of the lengths of the months and the length of the epact cycles is such that each civil calendar month starts and ends with the same epact label, except for February and for the epact labels xxv and 25 in July and August. This table is called the calendarium. The ecclesiastical new moons for any year are those dates at which the epact for the year is entered. If the epact for the year is for instance 27, then there is an ecclesiastical new moon on every date in that year that has the epact label xxvii (27).

Also label all the dates in the table with letters "A" to "G", starting from 1 January, and repeat to the end of the year. If, for instance, the first Sunday of the year is on 5 January, which has letter E, then every date with the letter "E" will be a Sunday that year. Then "E" is called the Dominical Letter for that year (from Latin: dies domini, day of the Lord). The Dominical Letter cycles backward one position every year. However, in leap years after 24 February the Sundays will fall on the previous letter of the cycle, so leap years have two Dominical Letters: the first for before, the second for after the leap day.

In practice, for the purpose of calculating Easter, this need not be done for all 365 days of the year. For the epacts, you will find that March comes out exactly the same as January, so one need not calculate January or February. To also avoid the need to calculate the Dominical Letters for January and February, start with D for 1 March. You need the epacts only from 8 March to 5 April. This gives rise to the following table:

A table from Sweden to compute the date of Easter 1140–1671 according to the Julian calendar. Notice the runic writing.

Chronological diagram of the date of Easter for 600 years, from the Gregorian calendar reform to the year 2200 (by Camille Flammarion, 1907)

Label	March	DL	April	DL
*	1	D
xxix	2	E	1	G
xxviii	3	F	2	A
xxvii	4	G	3	B
xxvi	5	A	4	C
25	6	B
xxv			5	D
xxiv	7	C
xxiii	8	D	6	E
xxii	9	E	7	F
xxi	10	F	8	G
xx	11	G	9	A
xix	12	A	10	B
xviii	13	B	11	C
xvii	14	C	12	D
xvi	15	D	13	E
xv	16	E	14	F
xiv	17	F	15	G
xiii	18	G	16	A
xii	19	A	17	B
xi	20	B	18	C
x	21	C	19	D
ix	22	D	20	E
viii	23	E	21	F
vii	24	F	22	G
vi	25	G	23	A
v	26	A	24	B
iv	27	B	25	C
iii	28	C
ii	29	D
i	30	E
*	31	F

Example: If the epact is, for instance, 27 (Roman xxvii), then there will be an ecclesiastical new moon on every date that has the label "xxvii". The ecclesiastical full moon falls 13 days later. From the table above, this gives a new moon on 4 March and 3 April, and so a full moon on 17 March and 16 April.

Then Easter Day is the first Sunday after the first ecclesiastical full moon on or after 21 March. This definition uses "on or after 21 March" to avoid ambiguity with historic meaning of the word "after". In modern language, this phrase simply means "after 20 March". The definition of "on or after 21 March" is frequently incorrectly abbreviated to "after 21 March" in published and web-based articles, resulting in incorrect Easter dates.

In the example, this paschal full moon is on 16 April. If the dominical letter is E, then Easter day is on 20 April.

The label 25 (as distinct from "xxv") is used as follows: Within a Metonic cycle, years that are 11 years apart have epacts that differ by one day. A month beginning on a date having labels xxiv and xxv impacted together will have either 29 or 30 days. If the epacts 24 and 25 both occur within one Metonic cycle, then the new (and full) moons would fall on the same dates for these two years. This is possible for the real moon but is inelegant in a schematic lunar calendar; the dates should repeat only after 19 years. To avoid this, in years that have epacts 25 and with a Golden Number larger than 11, the reckoned new moon will fall on the date with the label "25" rather than "xxv". Where the labels 25 and "xxv" are together there is no problem since they are the same. This does not move the problem to the pair "25" and "xxvi," because the earliest epact 26 could appear would be in year 23 of the cycle, which lasts only 19 years: there is a saltus lunae in between that makes the new moons fall on separate dates.

The Gregorian calendar has a correction to the tropical year by dropping three leap days in 400 years (always in a century year). This is a correction to the length of the tropical year, but should have no effect on the Metonic relation between years and lunations. Therefore, the epact is compensated for this (partially—see epact) by subtracting one in these century years. This is the so-called solar correction or "solar equation" ("equation" being used in its medieval sense of "correction").

However, 19 uncorrected Julian years are a little longer than 235 lunations. The difference accumulates to one day in about 310 years. Therefore, in the Gregorian calendar, the epact gets corrected by adding 1 eight times in 2500 (Gregorian) years, always in a century year: this is the so-called lunar correction (historically called "lunar equation"). The first one was applied in 1800, and it will be applied every 300 years except for an interval of 400 years between 3900 and 4300, which starts a new cycle.

The solar and lunar corrections work in opposite directions, and in some century years (for example, 1800 and 2100) they cancel each other. The result is that the Gregorian lunar calendar uses an epact table that is valid for a period of from 100 to 300 years. The epact table listed above is valid for the period 1900 to 2199.

Details

This method of computation has several subtleties:

Every second lunar month has only 29 days, so one day must have two (of the 30) epact labels assigned to it. The reason for moving around the epact label "xxv/25" rather than any other seems to be the following: According to Dionysius (in his introductory letter to Petronius), the Nicene council, on the authority of Eusebius, established that the first month of the ecclesiastical lunar year (the paschal month) should start between 8 March and 5 April inclusive, and the 14th day fall between 21 March and 18 April inclusive, thus spanning a period of (only) 29 days. A new moon on 7 March, which has epact label xxiv, has its 14th day (full moon) on 20 March, which is too early (not following 20 March). So years with an epact of xxiv, if the lunar month beginning on 7 March had 30 days, would have their paschal new moon on 6 April, which is too late: the full moon would fall on 19 April, and Easter could be as late as 26 April. In the Julian calendar the latest date of Easter was 25 April, and the Gregorian reform maintained that limit. So the paschal full moon must fall no later than 18 April and the new moon on 5 April, which has epact label xxv. 5 April must therefore have its double epact labels xxiv and xxv. Then epact xxv has to be treated differently, as explained in the paragraph above.

As a consequence, 19 April is the date on which Easter falls most frequently in the Gregorian calendar: in about 3.87% of the years. 22 March is the least frequent, with 0.48%.

Distribution of the date of Easter for the complete 5,700,000-year cycle

The relation between lunar and solar calendar dates is made independent of the leap day scheme for the solar year. Basically the Gregorian calendar still uses the Julian calendar with a leap day every four years, so a Metonic cycle of 19 years has 6940 or 6939 days with five or four leap days. Now the lunar cycle counts only 19 × 354 + 19 × 11 = 6935 days. By not labeling and counting the leap day with an epact number, but having the next new moon fall on the same calendar date as without the leap day, the current lunation gets extended by a day, and the 235 lunations cover as many days as the 19 years. So the burden of synchronizing the calendar with the moon (intermediate-term accuracy) is shifted to the solar calendar, which may use any suitable intercalation scheme; all under the assumption that 19 solar years = 235 lunations (long-term inaccuracy). A consequence is that the reckoned age of the moon may be off by a day, and also that the lunations which contain the leap day may be 31 days long, which would never happen when the real moon were followed (short-term inaccuracies). This is the price for a regular fit to the solar calendar.

From the perspective of those who might wish to use the Gregorian Easter cycle as a calendar for the entire year, there are some flaws in the Gregorian lunar calendar. However, they have no effect on the paschal month and the date of Easter:

1. Lunations of 31 (and sometimes 28) days occur.
2. If a year with Golden Number 19 happens to have epact 19, then the last ecclesiastical new moon falls on 2 December; the next would be due on 1 January. However, at the start of the new year there is a saltus lunae which increases the epact by another unit, and the new moon should have occurred on the previous day. So a new moon is missed. The calendarium of the Missale Romanum takes account of this by assigning epact label "19" instead of "20" to 31 December of such a year. It happened every 19 years when the original Gregorian epact table was in effect (for the last time in 1690), and will not happen again until 8511.
3. If the epact of a year is "20", then there will be an ecclesiastical new moon on 31 December. If that year falls before a century year, then in most cases there will be a solar correction which reduces the epact for the new year by one: the resulting epact * means that another ecclesiastical new moon is counted on 1 January; so formally a lunation of one day has passed. This will happen around the beginning of 4200.
4. Other borderline cases occur (much) later, and if the rules are followed strictly and these cases are not specially treated, they will generate successive new moon dates that are 1, 28, 59, or (very rarely) 58 days apart.

A careful analysis shows that through the way they are used and corrected in the Gregorian calendar, the epacts are actually fractions of a lunation (1/30, also known as a tithi) and not full days. See epact for a discussion.

The solar and lunar corrections repeat after 4 × 25 = 100 centuries. In that period, the epact has changed by a total of −1 × (3/4) × 100 + 1 × (8/25) × 100 = −43 ≡ 17 mod 30. This is prime to the 30 possible epacts, so it takes 100 × 30 = 3000 centuries before the epacts repeat; and 3000 × 19 = 57,000 centuries before the epacts repeat at the same Golden Number. This period has (5,700,000/19) × 235 + (−43/30) × (57,000/100) = 70,499,183 lunations. So the Gregorian Easter dates repeat in exactly the same order only after 5,700,000 years = 70,499,183 lunations = 2,081,882,250 days. However, the calendar will already have to have been adjusted after some millennia because of changes in the length of the tropical year, the synodic month, and the day.

This raises the question why the Gregorian lunar calendar has separate solar and lunar corrections, which sometimes cancel each other; instead, the net 4×8 − 3×25 = 43 epact subtractions could be distributed evenly over 10,000 years (as has been proposed for example by Dr Heiner Lichtenberg). Lilius' original work has not been preserved and Clavius does not explain this. However Lilius did say that the correction system devised by him was to be a perfectly flexible tool in the hands of future calendar reformers, since the solar and lunar calendar could henceforth be corrected without mutual interference. If this is not done the inaccuracies in the positions in the two cycles are added together.

The "solar corrections" approximately undo the effect of the Gregorian modifications to the leap days of the solar calendar on the lunar calendar: they (partially) bring the epact cycle back to the original Metonic relation between the Julian year and lunar month. The inherent mismatch between sun and moon in this basic 19-year cycle is then corrected every three or four centuries by the "lunar correction" to the epacts. However, the epact corrections occur at the beginning of Gregorian centuries, not Julian centuries, and therefore the original Julian Metonic cycle is not fully restored.

The gradual slowing of the Earth's rotation affects the date of the equinox: drift in ecclesiastical full moons calculated by the Gregorian method compared to the true full moons is far less because the increase in the length of the day is almost exactly compensated for by the slowdown in the length of the month as tidal braking reduces the energy in the system.

British Calendar Act and Book of Common Prayer

The portion of the Tabular methods section above describes the historical arguments and methods by which the present dates of Easter Sunday were decided in the late 16th century by the Catholic Church. In Britain, where the Julian calendar was then still in use, Easter Sunday was defined, from 1662 to 1752 (in accordance with previous practice), by a simple table of dates in the Anglican Prayer Book (decreed by the Act of Uniformity 1662). The table was indexed directly by the Golden Number and the Sunday Letter, which (in the Easter section of the Book) were presumed to be already known.

For the British Empire and colonies, the new determination of the Date of Easter Sunday was defined by what is now called the Calendar (New Style) Act 1750 with its Annexe. The method was chosen to give dates agreeing with the Gregorian rule already in use elsewhere. It was required by the Act to be put in the Book of Common Prayer, and therefore it is the general Anglican rule. The original Act can be seen in the British Statutes at Large 1765. The Annexe to the Act includes the definition: "Easter-day (on which the rest depend) is always the first Sunday after the Full Moon, which happens upon, or next after the Twenty-first Day of March. And if the Full Moon happens upon a Sunday, Easter-day is the Sunday after." The Annexe subsequently uses the terms "Paschal Full Moon" and "Ecclesiastical Full Moon", making it clear that they approximate to the real full moon.

The method is quite distinct from that described above in Gregorian calendar. For a general year, one first determines the Golden Number, then one uses three Tables to determine the Sunday Letter, a Cypher, and the date of the paschal full moon, from which the date of Easter Sunday follows. The epact does not explicitly appear. Simpler tables can be used for limited periods (such as 1900–2199) during which the Cypher (which represents the effect of the solar and lunar corrections) does not change. Clavius' details were employed in the construction of the method, but they play no subsequent part in its use.

J R Stockton shows his derivation of an efficient computer algorithm traceable to the Tables in the Prayer Book and the Calendar Act (assuming that a description of how to use the Tables is at hand), and verifies its processes by computing matching Tables.

Julian calendar

Distribution of the date of Easter in most Eastern churches 1900–2099 vs Western Easter distribution

The method for computing the date of the ecclesiastical full moon that was standard for the Western Church before the Gregorian calendar reform, and is still used today by most Eastern Christians, made use of an uncorrected repetition of the 19-year Metonic cycle in combination with the Julian calendar. In terms of the method of the epacts discussed above, it effectively used a single epact table starting with an epact of 0, which was never corrected. In this case, the epact was counted on 22 March, the earliest acceptable date for Easter. This repeats every 19 years, so there are only 19 possible dates for the paschal full moon from 21 March to 18 April inclusive.

Because there are no corrections as there are for the Gregorian calendar, the ecclesiastical full moon drifts away from the true full moon by more than three days every millennium. It is already a few days later. As a result, the Eastern churches celebrate Easter one week later than the Western churches about 50% of the time. (The Eastern Easter is often four or five weeks later because the Julian 20 March is 13 days later than the Gregorian 20 March for years 1900 to 2099.)

The sequence number of a year in the 19-year cycle is called its Golden Number. This term was first used in the computistic poem Massa Compoti by Alexander de Villa Dei in 1200. A later scribe added the Golden Number to tables originally composed by Abbo of Fleury in 988.

The claim by the Catholic Church in the 1582 papal bull Inter gravissimas, which promulgated the Gregorian calendar, that it restored "the celebration of Easter according to the rules fixed by ... the great ecumenical council of Nicæa" was based on a false claim by Dionysius Exiguus (525) that "we determine the date of Easter Day ... in accordance with the proposal agreed upon by the 318 Fathers of the Church at the Council in Nicaea." The First Council of Nicaea (325) only stated that Easter was to be celebrated by all Christians on the same Sunday—it did not fix any rules to determine which Sunday. The medieval computus was based on the Alexandrian computus, which was developed by the Church of Alexandria during the first decade of the 4th century using the Alexandrian calendar. The Eastern Roman Empire accepted it shortly after 380 after converting the computus to the Julian calendar. Rome accepted it sometime between the sixth and 9th centuries. The British Isles accepted it during the 7th century except for a few monasteries. Francia (all of Western Europe except Scandinavia (pagan), the British Isles, the Iberian peninsula, and southern Italy) accepted it during the last quarter of the 8th century. The last Celtic monastery to accept it, Iona, did so in 716, whereas the last English monastery to accept it did so in 931. Before these dates other methods were used which resulted in dates for Easter Sunday that sometimes differed by up to five weeks.

This is the table of paschal full moon dates for all Julian years since 931:

Golden Number	1	2	3	4	5	6	7	8	9	10	11	12	13	14	15	16	17	18	19	GN + 11 mod 19	8	19	11	3	14	6	17	9	1	12	4	15	7	18	10	2	13	5	16
Paschal Full Moon date	5A	25M	13A	2A	22M	10A	30M	18A	7A	27M	15A	4A	24M	12A	1A	21M	9A	29M	17A	Decreasing date	18A	17A	15A	13A	12A	10A	9A	7A	5A	4A	2A	1A	30M	29M	27M	25M	24M	22M	21M

(M=March, A=April)

A formula based on this table can be used to calculate paschal full moon dates

PFMd = 36 - E + 30 (if E > 16 ) - 31 (if the result > 31 the month is April)

where E = (Y mod 19 × 11) mod 30.

Easter day is the first Sunday after these dates.

So for a given date of the ecclesiastical full moon, there are seven possible Easter dates. The cycle of Sunday letters, however, does not repeat in seven years: because of the interruptions of the leap day every four years, the full cycle in which weekdays recur in the calendar in the same way, is 4 × 7 = 28 years, the so-called solar cycle. So the Easter dates repeated in the same order after 4 × 7 × 19 = 532 years. This paschal cycle is also called the Victorian cycle, after Victorius of Aquitaine, who introduced it in Rome in 457. It is first known to have been used by Annianus of Alexandria at the beginning of the 5th century. It has also sometimes erroneously been called the Dionysian cycle, after Dionysius Exiguus, who prepared Easter tables that started in 532; but he apparently did not realize that the Alexandrian computus which he described had a 532-year cycle, although he did realize that his 95-year table was not a true cycle. Venerable Bede (7th century) seems to have been the first to identify the solar cycle and explain the paschal cycle from the Metonic cycle and the solar cycle.

In medieval western Europe, the dates of the paschal full moon (14 Nisan) given above could be memorized with the help of a 19-line alliterative poem in Latin:

Nonae Aprilis	norunt quinos	V
octonae kalendae	assim depromunt.	I
Idus Aprilis	etiam sexis,	VI
nonae quaternae	namque dipondio.	II
Item undene	ambiunt quinos,	V
quatuor idus	capiunt ternos.	III
Ternas kalendas	titulant seni,	VI
quatuor dene	cubant in quadris.	IIII
Septenas idus	septem eligunt,	VII
senae kalendae	sortiunt ternos,	III
denis septenis	donant assim.	I
Pridie nonas	porro quaternis,	IIII
nonae kalendae	notantur septenis.	VII
Pridie idus	panditur quinis,	V
kalendas Aprilis	exprimunt unus.	I
Duodene namque	docte quaternis,	IIII
speciem quintam	speramus duobus.	II
Quaternae kalendae	quinque coniciunt,	V
quindene constant	tribus adeptis.	III

The first half-line of each line gives the date of the paschal full moon from the table above for each year in the 19-year cycle. The second half-line gives the ferial regular, or weekday displacement, of the day of that year's paschal full moon from the concurrent, or the weekday of 24 March. The ferial regular is repeated in Roman numerals in the third column.

Week table: Julian and Gregorian calendars

For Julian dates before 1300 and after 1999 the year in the table which differs by an exact multiple of 700 years should be used. For Gregorian dates after 2299,the year in the table which differs by an exact multiple of 400 years should be used. The values "r0" through "r6" indicate the remainder when the Hundreds value is divided by 7 and 4 respectively, indicating how the series extend in either direction. Both Julian and Gregorian values are shown 1500–1999 for convenience. Bold figures (e.g., 04) denote leap year. If a year ends in 00 and its hundreds are in bold it is a leap year. Thus 19 indicates that 1900 is not a Gregorian leap year, (but 19 in the Julian column indicates that it is a Julian leap year, as are all Julian x00 years). 20 indicates that 2000 is a leap year. Use Jan and Feb only in leap years.

100s of Years		Remaining Year Digits				Month					D o W	#
Julian (r ÷ 7)	Gregorian (r ÷ 4)
r5 19	16 20 r0	00 06   17 23	28 34   45 51	56 62   73 79	84 90	Jan				Oct	Sa	0
r4 18	15 19 r3	01 07 12 18	29 35 40 46	57 63 68 74	85 91 96			May			Su	1
r3 17	N/A	02   13 19 24	30   41 47 52	58   69 75 80	86   97	Feb			Aug		M	2
r2 16	18 22 r2	03 08 14   25	31 36 42   53	59 64 70   81	87 92 98	Feb	Mar			Nov	Tu	3
r1 15	N/A	09 15 20 26	37 43 48 54	65 71 76 82	93 99			Jun			W	4
r0 14	17 21 r1	04 10   21 27	32 38   49 55	60 66   77 83	88 94				Sep	Dec	Th	5
r6 13	N/A	05 11 16 22	33 39 44 50	61 67 72 78	89 95	Jan	Apr	Jul			F	6

For determination of the day of the week (1 January 2000, Saturday)

• the day of the month: 1 ~ 31 (1)
• the month: (6)
• the year: (0)
• the century mod 4 for the Gregorian calendar and mod 7 for the Julian calendar (0).
• adding 1+6+0+0=7. Dividing by 7 leaves a remainder of 0, so the day of the week is Saturday.

Revised Julian calendar

Note that the date (and hence the day of the week) in the Revised Julian and Gregorian calendars is the same from 14 October 1923 to 28 February AD 2800 inclusive and that for large years it may be possible to subtract 6300 or a multiple thereof before starting so as to reach a year which is within or closer to the table.

To look up the weekday of any date for any year using the table, subtract 100 from the year, divide the difference by 100, multiply the resulting quotient (omitting fractions) by seven and divide the product by nine. Note the quotient (omitting fractions). Enter the table with the Julian year, and just before the final division add 50 and subtract the quotient noted above.

Example: What is the day of the week of 27 January 8315?

8315-6300=2015, 2015-100=1915, 1915/100=19 remainder 15, 19x7=133, 133/9=14 remainder 7. 2015 is 700 years ahead of 1315, so 1315 is used. From table: for hundreds (13): 6. For remaining digits (15): 4. For month (January): 0. For date (27): 27. 6+4+0+27+50-14=73. 73/7=10 remainder 3. Day of week = Tuesday.

Sunday Letter

To find the Sunday Letter, calculate the day of the week for either 1 January or 1 October. If it is Sunday, the Sunday Letter is A, if Saturday B, and similarly backwards through the week and forwards through the alphabet to Monday, which is G.

Leap years have two Sunday Letters, so for January and February calculate the day of the week for 1 January and for March to December calculate the day of the week for 1 October.

Leap years are all years which divide exactly by four with the following exceptions:

In the Gregorian calendar – all years which divide exactly by 100 (other than those which divide exactly by 400)

In the Revised Julian calendar – all years which divide exactly by 100 (other than those which give remainder 200 or 600 when divided by 900).

Algorithms

Note on operations

When expressing Easter algorithms without using tables, it has been customary to employ only the integer operations addition, subtraction, multiplication, division, modulo, and assignment (plus minus times div mod assign). That is compatible with the use of simple mechanical or electronic calculators. But it is an undesirable restriction for computer programming, where conditional operators and statements, as well as look-up tables, are always available. One can easily see how conversion from day-of-March (22 to 56) to day-and-month (22 March to 25 April) can be done as
(if DoM>31) {Day=DoM-31, Month=Apr} else {Day=DoM, Month=Mar}.
More importantly, using such conditionals also simplifies the core of the Gregorian calculation.

Gauss algorithm

In 1800, the mathematician Carl Friedrich Gauss presented this algorithm for calculating the date of the Julian or Gregorian Easter and made corrections to one of the steps in 1816. In 1800 he incorrectly stated p = floor (k/3). In 1807 he replaced the condition (11M + 11) mod 30 < 19 with the simpler a > 10. In 1811 he limited his algorithm to the 18th and 19th centuries only, and stated that 26 April is always replaced with 19 April and 25 April by 18 April. In 1816 he thanked his student Peter Paul Tittel for pointing out that p was wrong in 1800.

Expression	year = 1777
a = year mod 19	a = 10
b = year mod 4	b = 1
c = year mod 7	c = 6
k = floor (year/100)	k = 17
p = floor ((13 + 8k)/25)	p = 5
q = floor (k/4)	q = 4
M = (15 − p + k − q) mod 30	M = 23
N = (4 + k − q) mod 7	N = 3
d = (19a + M) mod 30	d = 3
e = (2b + 4c + 6d + N) mod 7	e = 5
Gregorian Easter is 22 + d + e March or d + e − 9 April	30 March
if d = 29 and e = 6, replace 26 April with 19 April
if d = 28, e = 6, and (11M + 11) mod 30 < 19, replace 25 April with 18 April
For the Julian Easter in the Julian calendar M = 15 and N = 6 (k, p, and q are unnecessary)

An analysis of the Gauss Easter Sunday algorithm is divided into two parts. The first part is the approximate tracking of the lunar orbiting and the second one is the exact, deterministic offsetting to obtain a Sunday following the full moon.

The first part consists of determining the variable d, the number of days (counting from March 22) for the closest following full moon to occur. The formula for d contains the terms 19a and the constant M. a is the year's position in the 19-year lunar phase cycle, in which by assumption the moon's movement relative to earth repeats every 19 calendar years. In older times, 19 calendar years were equated to 235 lunar months (the Metonic cycle), which is remarkably close since 235 lunar months are approximately 6939.6813 days and 19 years are on average 6939.6075 days. The expression (19a + M) mod 30 repeats every 19 years within each century as M is determined per century. The 19-year cycle has nothing to do with the '19' in 19a, it is just a coincidence that another '19' appears. The '19' in 19a comes from correcting the mismatch between a calendar year and an integer number of lunar months. A calendar year (non-leap year) has 365 days and the closest you can come with an integer number of lunar months is 12×29.5=354 days. The difference is 11 days which must be corrected for by moving the following year's occurrence of a full moon 11 days back. But in modulo 30 arithmetic, subtracting 11 is the same as adding 19, hence the addition of 19 for each year added, i.e. 19a.

The M in 19a+M serves to have a correct starting point at the start of each century. It is determined by a calculation taking the number of leap years up until that century where k inhibits a leap day every 100 years and q reinstalls it every 400 years, yielding (k-q) as the total number of inhibitions to the pattern of a leap day every four years. Thus you add (k-q) to correct for leap days that never occurred. p corrects for the lunar orbit not being fully describable in integer terms.

The range of days considered for the full moon to determine Easter are March 22 to April 20, a range of 30 days which is mirrored in the mod 30 arithmetic of variable d and constant M, both of which can assume integer values in the range 0..29. Once d is determined, this is the number of days that should be added to March 22 (the earliest full moon allowed by the date range) to obtain the day of the full moon.

The second part is finding e, the additional offset days that must be added to the date offset d in order to arrive at a Sunday. Since the week has 7 days, the offset must be in the range 0..6 and determined by modulo 7 arithmetic. e is determined by calculating 2b+4c+6d+N under mod 7. These constants may seem strange at first, but are quite easily explainable if we remember that we operate under mod 7 arithmetic. To begin with, 2b+4c ensures that we take care of the fact that weekdays slide for each year. A normal year has 365 days, but 52×7=364, so 52 full weeks make up one day too little. Hence, each consecutive year, the weekday "slides one day forward", meaning if May 6 was a Wednesday one year, it will be a Thursday the following year (disregarding leap years). Both b and c will increase by one for an advancement of one year (disregarding modulo effects). The expression 2b+4c will thus increase by 6, but remember that this is the same as subtracting 1 under mod 7. And to subtract by 1 is exactly what is required for a normal year - since the weekday "slides" one day forward we should compensate one day less to arrive at the correct weekday (i.e. Sunday). For a leap year, b will become 0 and 2b will thus be 0 instead of 8 which under mod 7 is another subtraction by 1, i.e. a total subtraction by 2 as the weekdays after the leap day that year slides forward by two days.

The expression 6d works the same way. Increasing d by some number y indicates that the full moon occurs y days later this year, and hence we should compensate y days less. Adding 6d is under mod 7 the same as subtracting d which is the desired operation. Thus, again, we do subtraction by adding under modulo arithmetic. In total, the variable e contains the step from the day of the full moon to the nearest following Sunday, between 0 and 6 days ahead. The constant N provides the starting point for the calculations for each century and depends on where Jan 1, year 1 was implicitly located when the Gregorian calendar was constructed.

The expression d+e can yield offsets in the range 0..35 pointing to possible Easter Sundays on March 22 to April 26. For reasons of historical compatibility, all offsets of 35 and some of 34 are subtracted by 7, jumping one Sunday back to the day before the full moon (in effect using a negative e of minus 1). This means that April 26 is never Easter Sunday and that April 19 is overrepresented. These latter corrections are for historical reasons only and has nothing to do with the mathematical algorithm.

Using the Gauss algorithm for years prior to 1583 is historically pointless since the Gregorian calendar was not utilised for determining Easter before that year. Using the algorithm far into the future is questionable since nothing is known about how different churches will choose to define Easter that far ahead. Easter calculations are based on agreements and conventions, not on the actual celestial movements nor on indisputable facts of history.

Anonymous Gregorian algorithm

"A New York correspondent" submitted this algorithm for determining the Gregorian Easter to the journal Nature in 1876. It has been reprinted many times, e.g., in 1877 by Samuel Butcher in The Ecclesiastical Calendar, in 1916 by Arthur Downing in The Observatory, in 1922 by H. Spencer Jones in General Astronomy, in 1977 by the Journal of the British Astronomical Association, in 1977 by The Old Farmer's Almanac, in 1988 by Peter Duffett-Smith in Practical Astronomy with your Calculator, and in 1991 by Jean Meeus in Astronomical Algorithms. Because of the Meeus’ book citation, that is also called "Meeus/Jones/Butcher" algorithm:

Expression	Y = 1961	Y = 2024
a = Y mod 19	a = 4	a = 10
b = floor (Y / 100)	b = 19	b = 20
c = Y mod 100	c = 61	c = 24
d = floor (b / 4)	d = 4	d = 5
e = b mod 4	e = 3	e = 0
f = floor ((b + 8) / 25)	f = 1	f = 1
g = floor ((b − f + 1) / 3)	g = 6	g = 6
h = (19a + b − d − g + 15) mod 30	h = 10	h = 4
i = floor (c / 4)	i = 15	i = 6
k = c mod 4	k = 1	k = 0
ℓ = (32 + 2e + 2i − h − k) mod 7	ℓ = 1	ℓ = 5
m = floor ((a + 11h + 22ℓ) / 451)	m = 0	m = 0
month = floor ((h + ℓ − 7m + 114) / 31)	month = 4 (April)	month = 3 (March)
day = ((h + ℓ − 7m + 114) mod 31) + 1	day = 2	day = 31
Gregorian Easter	2 April 1961	31 March 2024

Meeus' Julian algorithm

Jean Meeus, in his book Astronomical Algorithms (1991, p. 69), presents the following algorithm for calculating the Julian Easter on the Julian Calendar, which is not the Gregorian Calendar used throughout the contemporary world; to obtain the date of Eastern Orthodox Easter on the latter calendar, 13 days (as of 1900 through 2099) need to be added to the Julian dates, resulting in the dates shown below in the last row.

Expression	Y = 2008	Y = 2009	Y = 2010	Y = 2011	Y = 2016
a = Y mod 4	a = 0	a = 1	a = 2	a = 3	a = 0
b = Y mod 7	b = 6	b = 0	b = 1	b = 2	b = 0
c = Y mod 19	c = 13	c = 14	c = 15	c = 16	c = 2
d = (19c + 15) mod 30	d = 22	d = 11	d = 0	d = 19	d = 23
e = (2a + 4b − d + 34) mod 7	e = 1	e = 4	e = 0	e = 1	e = 4
month = floor ((d + e + 114) / 31)	4 (April)	4 (April)	3 (March)	4 (April)	4 (April)
day = ((d + e + 114) mod 31) + 1	14	6	22	11	18
Easter Day (Julian calendar)	14 April 2008	6 April 2009	22 March 2010	11 April 2011	18 April 2016
Easter Day (Gregorian calendar)	27 April 2008	19 April 2009	4 April 2010	24 April 2011	1 May 2016

Adaptation for Western Easter of Meeus' Julian algorithm

Following is a method devised by Professor R. Sivaraman from Chennai, India a Mathematics Professor and Founder of Pie Mathematics Association, for finding Gregorian Western Easter date, which is now used by the majority of Christians, from 1900 to 2199.

1. Let a be the remainder when the given year Y is divided by 19.

2. Let b be the remainder when (11a + 5) is divided by 30.

3. c = b + 1 if either b = 0 or (b = 1 and a > 10); c = b, otherwise.

4. If c is any value from 1 to 19, then the Easter Month is April and if it takes values from 20 to 29 then the Easter Month is March.

5. d = Remainder when (50 - c) is divided by 31.

The date of Easter falls on the Sunday following the date d given by steps 4 and 5.

As an illustration, let us consider the case for the year 2016. It is easy to check that a = 2, b = 27, c = 27, d = 23. Since c = 27, by step 4, the Easter month was March and so the Easter date fell on Sunday following March 23rd, which was March 27th. This is indeed correct, as the Gregorian Western Easter date fell on 27th March for the year 2016.

We can find the Easter date for any given year from 2200 to 2299 by using the aforementioned formula by making the only little change in step 2. In this case, b is the remainder when (11a + 4) is divided by 30. Other details remain same as above.

Other algorithms

Faster and more compact algorithms for Gregorian Easter Sunday exist.

Software

• Perl – Rich Bowen's Date::Easter module available from CPAN.
• Excel =DOLLAR(("4/"&A1)/7+MOD(19*MOD(A1,19)-7,30)*14%,)*7-6, where the year is contained in cell A1.
• Excel =ROUND(DATE(A1,4,1)/7+MOD(19*MOD(A1,19)-7,30)*14%,0)*7-6, the same as above but system local settings independent
• Excel =FLOOR((4&-A1)-DAY(5)+97%*MOD(18.998*MOD(A1+8/9,19)+INT(68%*INT(A1%)-INT(A1%/4)-5/9),30),7)+DAY(1) provides the Gregorian Easter Sunday from 1900/1904-9999 in the Excel 1900 and 1904 date system
• Python – adapted from

  def IanTaylorEasterJscr(year):
      a = year % 19
      b = year >> 2
      c = b // 25 + 1
      d = (c * 3) >> 2
      e = ((a * 19) - ((c * 8 + 5) // 25) + d + 15) % 30
      e += (29578 - a - e * 32) >> 10
      e -= ((year % 7) + b - d + e + 2) % 7
      d = e >> 5
      day = e - d * 31
      month = d + 3
      return year, month, day
  

• BASIC – This is a version with the algorithm from Gauss, Zeller, Lichtenberg et al.:

  Function Easter(X)                                  ' X = year to compute
      Dim K, M, S, A, D, R, OG, SZ, OE
  
      K  = X \ 100                                    ' Secular number
      M  = 15 + (3 * K + 3) \ 4 - (8 * K + 13) \ 25   ' Secular Moon shift
      S  = 2 - (3 * K + 3) \ 4                        ' Secular Sun shift
      A  = X Mod 19                                   ' Moon parameter
      D  = (19 * A + M) Mod 30                        ' Seed for 1st full Moon in spring
      R  = D \ 29 + (D \ 28 - D \ 29) * (A \ 11)      ' Calendarian correction quantity
      OG = 21 + D - R                                 ' Easter limit
      SZ = 7 - (X + X \ 4 + S) Mod 7                  ' 1st Sunday in March
      OE = 7 - (OG - SZ) Mod 7                        ' Distance Easter Sunday from Easter limit in days
  
      Easter = DateSerial(X, 3, OG + OE)              ' Result: Easter Sunday as number of days in March
  End Function
  

  This code is only valid for years in the Gregorian calendar.
• Java - Anonymous (also called Meeus/Jones/Butcher) Gregorian algorithm

  public static Date getEasterDate(int year) {
  	int a = year % 19;
  	int b = year / 100;
  	int c = year % 100;
  	int d = b / 4;
  	int e = b % 4;
  	int f = (b + 8) / 25;
  	int g = (b - f + 1) / 3;
  	int h = (19 * a + b - d - g + 15) % 30;
  	int i = c / 4;
  	int k = c % 4;
  	int l = (32 + 2 * e + 2 * i - h - k) % 7;
  	int m = (a + 11 * h + 22 * l) / 451;
  	int n = (h + l - 7 * m + 114) / 31;
  	int p = (h + l - 7 * m + 114) % 31;
  	Calendar calendar = GregorianCalendar.getInstance();
  	calendar.clear();
  	calendar.set(year, n - 1, p + 1);
  	return calendar.getTime();
  }
  

• MS-SQL based on the Meeus/Jones/Butcher algorithm above.

  DROP FUNCTION [dbo].[fn_getEasterDate]
  GO
  
  CREATE FUNCTION [dbo].[fn_getEasterDate] (
  	@xYear int
  )
  RETURNS date
  AS
  BEGIN
  	/*Calculate date of easter based on Year passed*/
  	/*Based on Anonymous Gregorian Algorithm, also known as the Meeus/Jones/Butcher algorithm*/
  	Declare @dGregorianEaster date
  	Declare @a int, @b int, @c int, @d int, @e int, @f int, @g int, @h int, @i int, @k int, @L int, @m int, @month int, @day int
  	set @a = @xYear % 19
  	set @b = floor(@xyear / 100)
  	set @c = @xYear % 100
  	set @d = floor(@b / 4)
  	set @e = @b % 4
  	set @f = floor((@b + 8) / 25)
  	set @g = floor((@b - @f + 1)/3)
  	set @h = (19*@a + @b - @d - @g + 15) % 30
  	set @i = floor(@c / 4)
  	set @k = @c % 4
  	set @L = (32 + 2*@e + 2*@i - @h - @k) % 7
  	set @m = floor((@a + 11*@h + 22*@L) / 451)
  	set @month = floor((@h + @L - 7*@m + 114) / 31)
  	set @day = (@h + @L - 7*@m + 114) % 31 + 1
  	set @dGregorianEaster = cast( cast(@xYear as char(4)) + '-' + right('0' + cast(@month as varchar(2)), 2)+ '-' + right('0' + cast(@day as varchar(2)), 2) as date)
  	RETURN(@dGregorianEaster)
  END
  GO
  select dbo.fn_getEasterDate(1961)
  select dbo.fn_getEasterDate(2014)
  

• PL/SQL

CREATE OR REPLACE FUNCTION easter_sunday( _year INTEGER ) RETURNS DATE
  LANGUAGE PLPGSQL IMMUTABLE STRICT LEAKPROOF 
  SECURITY INVOKER
  COST 50
AS $function$
  /*
   *  Title:   The date of Easter
   *  Authors: Downing, A. M. W.
   *  Journal: The Observatory, Vol. 39, p. 215-219 (1916)
   *  Bibliographic Code: 1916Obs....39..215D
   *  http://articles.adsabs.harvard.edu//full/1916Obs....39..215D/0000215.000.html
   *  refers to Nature, 1876 April 20, vol. 13, p. 487 for the algorithm.
   *  NB. Neither this author nor the anonymous 1876 contributor have provided a proof
   *  of this algorithm's correctness, but testing has revealed no problems.
   */
  DECLARE
    AA INTEGER DEFAULT _year % 19;                       -- A=YEAR%19
    BB INTEGER DEFAULT _year / 100;                      -- B=YEAR/100
    CC INTEGER DEFAULT _year % 100;                      -- C=YEAR%100
    DD INTEGER DEFAULT  BB / 4;                          -- D=B/4
    EE INTEGER DEFAULT  BB % 4;                          -- E=B%4
    FF INTEGER DEFAULT (BB + 8) / 25;                    -- F=(B+8)/25
    GG INTEGER DEFAULT (BB - FF + 1) / 3;                -- G=(B-F+1)/3
    HH INTEGER DEFAULT (19*AA + BB - DD - GG + 15) % 30; -- H=(19*A+B-D-G+15)%30
    II INTEGER DEFAULT  CC / 4;                          -- I=C/4
    KK INTEGER DEFAULT  CC % 4;                          -- K=C%4
    LL INTEGER DEFAULT (32 + 2*EE + 2*II - HH - KK) % 7; -- L=(32+2*E+2*I-H-K)%7
    MM INTEGER DEFAULT (AA + 11*HH + 22*LL) / 451;       -- M=(A+11*H+22*L)/451
    NN INTEGER DEFAULT (HH + LL - 7*MM + 114) / 31;      -- N=(H+L-7*M+114)/31
    OO INTEGER DEFAULT (HH + LL - 7*MM + 114) % 31;      -- O=(H+L-7*M+114)%31
    EM INTEGER; -- Easter month [3, 4]
    ED INTEGER; -- Easter date (within the month)
  BEGIN
    EM := NN;     -- Easter Month   [3=March, 4=April]
    ED := OO + 1; -- Easter Date    [date in Easter Month]
    RETURN make_date (_year,EM,ED);
  END;
$function$;
SELECT easter_sunday(1954); -- should return 1954-04-18
SELECT easter_sunday(2016); -- should return 2016-03-27

See also

• Christian Zeller
• Crucifixion darkness
• Reform of the date of Easter

References

• Blackburn, Bonnie, and Holford-Strevens, Leofranc. (2003). The Oxford Companion to the Year: An exploration of calendar customs and time-reckoning. (First published 1999, reprinted with corrections 2003.) Oxford: Oxford University Press.
• Borst, Arno (1993). The Ordering of Time: From the Ancient Computus to the Modern Computer Trans. by Andrew Winnard. Cambridge: Polity Press; Chicago: Univ. of Chicago Press.
• Clavius, Christopher (1603): Romani calendarij à Gregorio XIII. P. M. restituti explicatio. In the fifth volume of Opera Mathematica (1612). Opera Mathematica of Christoph Clavius includes page images of the Six Canons and the Explicatio (Go to page: Roman Calendar of Gregory XIII)
• Constantine the Great, Emperor (325): Letter to the bishops who did not attend the first Nicaean Council; from Eusebius' Vita Constantini. English translations: Documents from the First Council of Nicea, "On the keeping of Easter" (near end) and Eusebius, Life of Constantine, Book III, Chapters XVIII–XIX
• Coyne, G. V., M. A. Hoskin, M. A., and Pedersen, O. (ed.) Gregorian reform of the calendar: Proceedings of the Vatican conference to commemorate its 400th anniversary, 1582–1982, (Vatican City: Pontifical Academy of Sciences, Specolo Vaticano, 1983).
• Dionysius Exiguus (525): Liber de Paschate. On-line: (full Latin text) and (table with Argumenta in Latin, with English translation)
• Eusebius of Caesarea, The History of the Church, Translated by G. A. Williamson. Revised and edited with a new introduction by Andrew Louth. Penguin Books, London, 1989.
• Gibson, Margaret Dunlop, The Didascalia Apostolorum in Syriac, Cambridge University Press, London, 1903.
• Gregory XIII (Pope) and the calendar reform committee (1581): the Papal Bull Inter Gravissimas and the Six Canons. On-line under: "Les textes fondateurs du calendrier grégorien", with some parts of Clavius's Explicatio
• Mosshammer, Alden A., The Easter Computus and the Origins of the Christian Era, Oxford University Press, 2008.
• Schwartz, E., Christliche und jüdische Ostertafeln, (Abhandlungen der königlichen Gesellschaft der Wissenschaften zu Göttingen. Pilologisch-historische Klasse. Neue Folge, Band viii.) Weidmannsche Buchhandlung, Berlin, 1905.
• Stern, Sacha, Calendar and Community: A History of the Jewish Calendar Second Century BCE – Tenth Century CE, Oxford University Press, Oxford, 2001.
• Walker, George W, Easter Intervals, Popular Astronomy, April 1945, Vol. 53, pp. 162–178, available at [5].
• Walker, George W, Easter Intervals (Continued), Popular Astronomy, May 1945, Vol. 53, pp. 218–232, available at [6].
• Wallis, Faith., Bede: The Reckoning of Time, (Liverpool: Liverpool Univ. Pr., 1999), pp. lix–lxiii.
• Weisstein, Eric. (c. 2006) "Paschal Full Moon" in World of Astronomy.

Further reading

• Mosshammer, Alden A. The Easter Computus and the Origins of the Christian Era. Oxford: Oxford University Press, 2008. ISBN 0-19-954312-7.

External links

• The Complete Works of Venerable Bede Vol. 6 (Contains De Temporibus and De Temporum Ratione.)
• The entry on epacts in the Catholic Encyclopedia of 1911
• The original texts of the Gregorian calendar reform (in Latin), with translations into French by Rodolphe Audette
• An Easter calculator with an extensive bibliography, and with useful links
• Ephemeris site of the Bureau des Longitudes with an Easter calculator
• A calendar page and calculator by Holger Oertel
• A page from Clive Feather with a brief explanation, some more tables, and another algorithm
• Template:De icon An extensive calendar site and calendar and Easter calculator by Nikolaus A. Bär
• Explanation of the Gregorian solar and lunar calendar, with improved procedures over the tabular method, by David Madore
• Gregorian Lunar Calendar: A table of the Gregorian New Moons for 1900–2199
  • A table of Gregorian New Moons for the years 1700–1899, from the same source
  • A similar table for the years 2200–2299
  • A calendar dividing the Gregorian lunar year 2003 into 30-day and 29-day lunar months
  • A discussion of the Nicene Council's Easter decision and of how some commentators exaggerate the scope of the Council's decision
• Dionysius Exiguus' Easter table
• Mnemonic Computus Diagrams of Hands from manuscript in The British Library
• St. Gallen, Stiftsbibliothek, Codex Sangallensis 378 (11th century) p. 28. Contains the poem Nonae Aprilis norunt quinos.
• Towards a Common Date for Easter World Council of Churches (Faith and Order) and Middle East Council of Churches consultation; Aleppo, Syria; 5–10 March 1997
• A simplified method for determining the date of Easter for all years 326 to 4099 A.D. by Ronald W. Mallen
• Text of the Calendar (New Style) Act 1750, British Act of Parliament introducing the Gregorian Calendar as amended to date. Contains tables for calculating Easter up until the year 8599. Contrast with the Act as passed.