Archive-name: calendars/faq/part1 Posting-Frequency: monthly Last-modified: 1997/03/27 Version: 1.7 URL: http://www.pip.dknet.dk/~pip10160/calendar.html FREQUENTLY ASKED QUESTIONS ABOUT CALENDARS Part 1 of 3 Version 1.7 - 27 Mar 1997 Copyright and disclaimer ------------------------ This document is Copyright (C) 1997 by Claus Tondering. E-mail: c-t@pip.dknet.dk. The document may be freely distributed, provided this copyright notice is included and no money is charged for the document. This document is provided "as is". No warranties are made as to its correctness. Introduction ------------ This is the calendar FAQ. Its purpose is to give an overview of the Christian, Hebrew, and Islamic calendars in common use. It will provide a historical background for the Christian calendar, plus an overview of the French Revolutionary calendar and the Maya calendar. Comments are very welcome. My e-mail address is given above. I would like to thank - Dr. Monzur Ahmed of the University of Birmingham, UK, - Michael J Appel, - Jay Ball, - Chris Carrier, - Simon Cassidy, - Claus Dobesch, - Leofranc Holford-Strevens, - H. Koenig, - Marcos Montes, - James E. Morrison, - Waleed A. Muhanna of the Fisher College of Business, Columbus, Ohio, USA, - Paul Schlyter of the Swedish Amateur Astronomer's Society for their help with this document. Changes since version 1.6 ------------------------- A few of minor corrections. Section 2.12.1 ("Is there a formula for calculating the Julian day number?") added and the following section renumbered. Section 4.4 ("When will the Islamic calendar overtake the Gregorian calendar?") added. Writing dates and years ----------------------- Dates will be written in the British format (1 January) rather than the American format (January 1). Dates will occasionally be abbreviated: "1 Jan" rather than "1 January". Years before and after the "official" birth year of Christ will be written "45 BC" or "AD 1997", respectively. I prefer this notation over the secular "45 B.C.E." and "1997 C.E." The % operator -------------- Throughout this document the operator % will be used to signify the modulo or remainder operator. For example, 17%7=3 because the result of the division 17/7 is 2 with a remainder of 3. The text in square brackets --------------------------- Square brackets [like this] identify information that I am unsure about and about which I would like more information. Please write me at c-t@pip.dknet.dk. Index: ------ In part 1 of this document: 1. What astronomical events form the basis of calendars? 1.1. What are Equinoxes and Solstices? 2. The Christian calendar 2.1. What is the Julian calendar? 2.1.1. What years are leap years? 2.1.2. What consequences did the use of the Julian calendar have? 2.2. What is the Gregorian calendar? 2.2.1. What years are leap years? 2.2.2. Isn't there a 4000-year rule? 2.2.3. Don't the Greek do it differently? 2.2.4. When did country X change from the Julian to the Gregorian calendar? 2.3. What day is the leap day? 2.4. What is the Solar Cycle? 2.5. What day of the week was 2 August 1953? 2.6. What is the Roman calendar? 2.6.1. How did the Romans number days? 2.7. Has the year always started on 1 January? 2.8. What is the origin of the names of the months? In part 2 of this document: 2.9. What is Easter? 2.9.1. When is Easter? (Short answer) 2.9.2. When is Easter? (Long answer) 2.9.3. What is the Golden Number? 2.9.4. What is the Epact? 2.9.5. How does one calculate Easter then? 2.9.6. Isn't there a simpler way to calculate Easter? 2.9.7. Is there a simple relationship between two consecutive Easters? 2.9.8. How frequently are the dates for Easter repeated? 2.9.9. What about Greek Easter? 2.10. How does one count years? 2.10.1. Was Jesus born in the year 0? 2.10.2. When does the 21st century start? 2.11. What is the Indiction? 2.12. What is the Julian period? 2.12.1. Is there a formula for calculating the Julian day number? 2.12.2. What is the modified Julian day? 3. The Hebrew Calendar 3.1. What does a Hebrew year look like? 3.2. What years are leap years? 3.3. What years are deficient, regular, and complete? 3.4. When is New Year's day? 3.5. When does a Hebrew day begin? 3.6. When does a Hebrew year begin? 3.7. When is the new moon? 3.8. How does one count years? 4. The Islamic Calendar 4.1. What does an Islamic year look like? 4.2. So you can't print an Islamic calendar in advance? 4.3. How does one count years? 4.4. When will the Islamic calendar overtake the Gregorian calendar? In part 3 of this document: 5. The Week 5.1. What Is the Origin of the 7-Day Week? 5.2. What Do the Names of the Days of the Week Mean? 5.3. Has the 7-Day Week Cycle Ever Been Interrupted? 5.4. Which Day is the Day of Rest? 5.5. What Is the First Day of the Week? 5.6. What Is the Week Number? 5.7. Do Weeks of Different Lengths Exist? 6. The French Revolutionary Calendar 6.1. What does a Republican year look like? 6.2. How does one count years? 6.3. What years are leap years? 6.4. How does one convert a Republican date to a Gregorian one? 7. The Maya Calendar 7.1. What is the Long Count? 7.1.1. When did the Long Count Start? 7.2. What is the Tzolkin? 7.2.1. When did the Tzolkin Start? 7.3. What is the Haab? 7.3.1. When did the Haab Start? 7.4. Did the Maya Think a Year Was 365 Days? 8. Date 1. What astronomical events form the basis of calendars? -------------------------------------------------------- Calendars are normally based on astronomical events, and the two most important astronomical objects are the sun and the moon. Their cycles are very important in the construction and understanding of calendars. Our concept of a year is based on the earth's motion around the sun. The time from one fixed point, such as a solstice or equinox, to the next is called a "tropical year". Its length is currently 365.242190 days, but it varies. Around 1900 its length was 365.242196 days, and around 2100 it will be 365.242184 days. (This definition of the tropical year is not quite accurate, see section 1.1 for more details.) Our concept of a month is based on the moon's motion around the earth, although this connection has been broken in the calendar commonly used now. The time from one new moon to the next is called a "synodic month", and its length is currently 29.5305889 days, but it varies. Around 1900 its length was 29.5305886 days, and around 2100 it will be 29.5305891 days. Note that these numbers are averages. The actual length of a particular year may vary by several minutes due to the influence of the gravitational force from other planets. Similary, the time between two new moons may vary by several hours due to a number of factors, including changes in the gravitational force from the sun, and the moon's orbital inclination. It is unfortunate that the length of the tropical year is not a multiple of the length of the synodic month. This means that with 12 months per year, the relationship between our month and the moon cannot be maintained. However, 19 tropical years is 234.997 synodic months, which is very close to an integer. So every 19 years the phases of the moon fall on the same dates (if it were not for the skewness introduced by leap years). 19 years is called a Metonic cycle (after Meton, an astronomer from Athens in the 5th century BC). So, to summarise: There are three important numbers to note: A tropical year is 365.2422 days. A synodic month is 29.53059 days. 19 tropical years is close to an integral number of synodic months. The Christian calendar is based on the motion of the earth around the sun, while the months have no connection with the motion of the moon. On the other hand, the Islamic calendar is based on the motion of the moon, while the year has no connection with the motion of the earth around the sun. Finally, the Hebrew calendar combines both, in that its years are linked to the motion of the earth around the sun, and its months are linked to the motion of the moon. 1.1. What are Equinoxes and Solstices? -------------------------------------- Equinoxes and solstices are frequently used as anchor points for calendars. For people in the northern hemisphere: - Winter solstice is the time in December when the sun reaches its southernmost latitude. At this time we have the shortest day. The date is typically around 21 December. - Summer solstice is the time in June when the sun reaches its northernmost latitude. At this time we have the longest day. The date is typically around 21 June. - Vernal equinox is the time in March when the sun passes the equator moving from the southern to the northern hemisphere. Day and night have approximately the same length. The date is typically around 20 March. - Autumnal equinox is the time in September when the sun passes the equator moving from the northern to the southern hemisphere. Day and night have approximately the same length. The date is typically around 22 September. For people in the southern hemisphere these events are shifted half a year. The astronomical "tropical year" is frequently defined as the time between, say, two vernal equinoxes, but this is not actually true. Currently the time between two vernal equinoxes is slightly greater than the tropical year. The reason is that the earth's position in its orbit at the time of solstices and equinoxes shifts slightly each year (taking approximately 21,000 years to move all the way around the orbit). This, combined with the fact that the earth's orbit is not completely circular, causes the equinoxes and solstices to shift with respect to each other. The astronomer's mean tropical year is really a somewhat artificial average of the period between the time when the sun is in any given position in the sky with respect to the equinoxes and the next time the sun is in the same position. 2. The Christian calendar ------------------------- The "Christian calendar" is the term I use to designate the calendar commonly in use, although its connection with Christianity is highly debatable. The Christian calendar has years of 365 or 366 days. It is divided into 12 months that have no relationship to the motion of the moon. In parallel with this system, the concept of "weeks" groups the days in sets of 7. Two main versions of the Christian calendar have existed in recent times: The Julian calendar and the Gregorian calendar. The difference between them lies in the way they approximate the length of the tropical year and their rules for calculating Easter. 2.1. What is the Julian calendar? --------------------------------- The Julian calendar was introduced by Julius Caesar in 45 BC. It was in common use until the 1500s, when countries started changing to the Gregorian calendar (section 2.2). However, some countries (for example, Greece and Russia) used it into this century, and the Orthodox church in Russia still uses it, as do some other Orthodox churches. In the Julian calendar, the tropical year is approximated as 365 1/4 days = 365.25 days. This gives an error of 1 day in approximately 128 years. The approximation 365 1/4 is achieved by having 1 leap year every 4 years. 2.1.1. What years are leap years? --------------------------------- The Julian calendar has 1 leap year every 4 years: Every year divisible by 4 is a leap year. However, this rule was not followed in the first years after the introduction of the Julian calendar in 45 BC. Due to a counting error, every 3rd year was a leap year in the first years of this calendar's existence. The leap years were: 45 BC, 42 BC, 39 BC, 36 BC, 33 BC, 30 BC, 27 BC, 24 BC, 21 BC, 18 BC, 15 BC, 12 BC, 9 BC, AD 8, AD 12, and every 4th year from then on. There were no leap years between 9 BC and AD 8. This period without leap years was decreed by emperor Augustus and earned him a place in the calendar, as the 8th month was named after him. It is a curious fact that although the method of reckoning years after the (official) birthyear of Christ was not introduced until the 6th century, by some stroke of luck the Julian leap years coincide with years of our Lord that are divisible by 4. 2.1.2. What consequences did the use of the Julian calendar have? ----------------------------------------------------------------- The Julian calendar introduces an error of 1 day every 128 years. So every 128 years the tropical year shifts one day backwards with respect to the calendar. Furthermore, the method for calculating the dates for Easter was inaccurate and needed to be refined. In order to remedy this, two steps were necessary: 1) The Julian calendar had to be replaced by something more adequate. 2) The extra days that the Julian calendar had inserted had to be dropped. The solution to problem 1) was the Gregorian calendar described in section 2.2. The solution to problem 2) depended on the fact that it was felt that 21 March was the proper day for vernal equinox (because 21 March was the date for vernal equinox during the Council of Nicaea in AD 325). The Gregorian calendar was therefore calibrated to make that day vernal equinox. By 1582 vernal equinox had moved (1582-325)/128 days = approximately 10 days backwards. So 10 days had to be dropped. 2.2. What is the Gregorian calendar? ------------------------------------ The Gregorian calendar is the one commonly used today. It was proposed by Aloysius Lilius, a physician from Naples, and adopted by Pope Gregory XIII in accordance with instructions from the Council of Trent (1545-1563) to correct for errors in the older Julian Calendar. It was decreed by Pope Gregory XIII in a papal bull in February 1582. In the Gregorian calendar, the tropical year is approximated as 365 97/400 days = 365.2425 days. Thus it takes approximately 3300 years for the tropical year to shift one day with respect to the Gregorian calendar. The approximation 365 97/400 is achieved by having 97 leap years every 400 years. 2.2.1. What years are leap years? --------------------------------- The Gregorian calendar has 97 leap years every 400 years: Every year divisible by 4 is a leap year. However, every year divisible by 100 is not a leap year. However, every year divisible by 400 is a leap year after all. So, 1700, 1800, 1900, 2100, and 2200 are not leap years. But 1600, 2000, and 2400 are leap years. (Destruction of a myth: There are no double leap years, i.e. no years with 367 days. See, however, the note on Sweden in section 2.2.4.) 2.2.2. Isn't there a 4000-year rule? ------------------------------------ It has been suggested (by the astronomer John Herschel (1792-1871) among others) that a better approximation to the length of the tropical year would be 365 969/4000 days = 365.24225 days. This would dictate 969 leap years every 4000 years, rather than the 970 leap years mandated by the Gregorian calendar. This could be achieved by dropping one leap year from the Gregorian calendar every 4000 years, which would make years divisible by 4000 non-leap years. This rule has, however, not been officially adopted. 2.2.3. Don't the Greek do it differently? ----------------------------------------- When the Orthodox church in Greece finally decided to switch to the Gregorian calendar in the 1920s, they tried to improve on the Gregorian leap year rules, replacing the "divisible by 400" rule by the following: Every year which when divided by 900 leaves a remainder of 200 or 600 is a leap year. This makes 1900, 2100, 2200, 2300, 2500, 2600, 2700, 2800 non-leap years, whereas 2000, 2400, and 2900 are leap years. This will not create a conflict with the rest of the world until the year 2800. This rule gives 218 leap years every 900 years, which gives us an average year of 365 218/900 days = 365.24222 days, which is certainly more accurate than the official Gregorian number of 365.2425 days. However, this rule is *not* official in Greece. [I have received an e-mail indicating that this system is official in Russia today. I'm investigating that. Information is very welcome.] 2.2.4. When did country X change from the Julian to the Gregorian calendar? --------------------------------------------------------------------------- The papal bull of February 1582 decreed that 10 days should be dropped from October 1582 so that 15 October should follow immediately after 4 October, and from then on the reformed calendar should be used. This was observed in Italy, Poland, Portugal, and Spain. Other Catholic countries followed shortly after, but Protestant countries were reluctant to change, and the Greek orthodox countries didn't change until the start of this century. Changes in the 1500s required 10 days to be dropped. Changes in the 1600s required 10 days to be dropped. Changes in the 1700s required 11 days to be dropped. Changes in the 1800s required 12 days to be dropped. Changes in the 1900s required 13 days to be dropped. (Exercise for the reader: Why is the error in the 1600s the same as in the 1500s.) The following list contains the dates for changes in a number of countries. Albania: December 1912 Austria: Different regions on different dates 5 Oct 1583 was followed by 16 Oct 1583 14 Dec 1583 was followed by 25 Dec 1583 Belgium: Different authorities say 14 Dec 1582 was followed by 25 Dec 1582 21 Dec 1582 was followed by 1 Jan 1583 Bulgaria: Different authorities say Sometime in 1912 Sometime in 1915 18 Mar 1916 was followed by 1 Apr 1916 China: Different authorities say 18 Dec 1911 was followed by 1 Jan 1912 18 Dec 1928 was followed by 1 Jan 1929 Czechoslovakia (i.e. Bohemia and Moravia): 6 Jan 1584 was followed by 17 Jan 1584 Denmark (including Norway): 18 Feb 1700 was followed by 1 Mar 1700 Egypt: 1875 Estonia: January 1918 Finland: Then part of Sweden. (Note, however, that Finland later became part of Russia, which then still used the Julian calendar. The Gregorian calendar remained official in Finland, but some use of the Julian calendar was made.) France: 9 Dec 1582 was followed by 20 Dec 1582 Germany: Different states on different dates: Catholic states on various dates in 1583-1585 Prussia: 22 Aug 1610 was followed by 2 Sep 1610 Protestant states: 18 Feb 1700 was followed by 1 Mar 1700 Great Britain and Dominions (including what is now the USA): 2 Sep 1752 was followed by 14 Sep 1752 Greece: 9 Mar 1924 was followed by 23 Mar 1924 Hungary: 21 Oct 1587 was followed by 1 Nov 1587 Italy: 4 Oct 1582 was followed by 15 Oct 1582 Japan: Different authorities say: 19 Dec 1872 was followed by 1 Jan 1873 18 Dec 1918 was followed by 1 Jan 1919 Latvia: During German occupation 1915 to 1918 Lithuania: 1915 Luxemburg: 14 Dec 1582 was followed by 25 Dec 1582 Netherlands: Brabant, Flanders, Holland, Artois, Hennegau: 14 Dec 1582 was followed by 25 Dec 1582 Geldern, Friesland, Zeuthen, Groningen, Overysel: 30 Nov 1700 was followed by 12 Dec 1700 Norway: Then part of Denmark. Poland: 4 Oct 1582 was followed by 15 Oct 1582 Portugal: 4 Oct 1582 was followed by 15 Oct 1582 Romania: 31 Mar 1919 was followed by 14 Apr 1919 Russia: 31 Jan 1918 was followed by 14 Feb 1918 Spain: 4 Oct 1582 was followed by 15 Oct 1582 Sweden (including Finland): 17 Feb 1753 was followed by 1 Mar 1753 (see note below) Switzerland: Catholic cantons: 1583 or 1584 Zurich, Bern, Basel, Schafhausen, Neuchatel, Geneva: 31 Dec 1700 was followed by 12 Jan 1701 St Gallen: 1724 Turkey: 18 Dec 1926 was followed by 1 Jan 1927 USA: See Great Britain, of which it was then a colony. Yugoslavia: 1919 Sweden has a curious history. Sweden decided to make a gradual change from the Julian to the Gregorian calendar. By dropping every leap year from 1700 through 1740 the eleven superfluous days would be omitted and from 1 Mar 1740 they would be in sync with the Gregorian calendar. (But in the meantime they would be in sync with nobody!) So 1700 (which should have been a leap year in the Julian calendar) was not a leap year in Sweden. However, by mistake 1704 and 1708 became leap years. This left Sweden out of synchronisation with both the Julian and the Gregorian world, so they decided to go *back* to the Julian calendar. In order to do this, they inserted an extra day in 1712, making that year a double leap year! So in 1712, February had 30 days in Sweden. Later, in 1753, Sweden changed to the Gregorian calendar by dropping 11 days like everyone else. 2.3. What day is the leap day? ------------------------------ It is 24 February! Weird? Yes! The explanation is related to the Roman calendar and is found in section 2.6.1. From a numerical point of view, of course 29 February is the extra day. But from the point of view of celebration of feast days, the following correspondence between days in leap years and non-leap years has traditionally been used: Non-leap year Leap year ------------- ---------- 22 February 22 February 23 February 23 February 24 February (extra day) 24 February 25 February 25 February 26 February 26 February 27 February 27 February 28 February 28 February 29 February For example, the feast of St. Leander has been celebrated on 27 February in non-leap years and on 28 February in leap years. The EU (European Union) in their infinite wisdom have decided that starting in the year 2000, 29 February is to be the leap day. This will affect countries such as Sweden and Austria that celebrate "name days" (i.e. each day is associated with a name). It appears that the Roman Catholic Church already uses 29 February as the leap day. 2.4. What is the Solar Cycle? ----------------------------- In the Julian calendar the relationship between the days of the week and the dates of the year is repeated in cycles of 28 years. In the Gregorian calendar this is still true for periods that do not cross years that are divisible by 100 but not by 400. A period of 28 years is called a Solar Cycle. The "Solar Number" of a year is found as: Solar Number = (year + 8) % 28 + 1 In the Julian calendar there is a one-to-one relationship between the Solar Number and the day on which a particular date falls. (The leap year cycle of the Gregorian calendar is 400 years, which is 146,097 days, which curiously enough is a multiple of 7. So in the Gregorian calendar the equivalent of the "Solar Cycle" would be 400 years, not 7*400=2800 years as one might be tempted to believe.) 2.5. What day of the week was 2 August 1953? -------------------------------------------- To calculate the day on which a particular date falls, the following algorithm may be used (the divisions are integer divisions, in which remainders are discarded): a = (14 - month) / 12 y = year - a m = month + 12*a - 2 For Julian calendar: d = (5 + day + y + y/4 + (31*m)/12) % 7 For Gregorian calendar: d = (day + y + y/4 - y/100 + y/400 + (31*m)/12) % 7 The value of d is 0 for a Sunday, 1 for a Monday, 2 for a Tuesday, etc. Example: On what day of the week was the author born? My birthday is 2 August 1953 (Gregorian, of course). a = (14 - 8) / 12 = 0 y = 1953 - 0 = 1953 m = 8 + 12*0 - 2 = 6 d = (2 + 1953 + 1953/4 - 1953/100 + 1953/400 + (31*6)/12) % 7 = (2 + 1953 + 488 - 19 + 4 + 15 ) % 7 = 2443 % 7 = 0 I was born on a Sunday. 2.6. What is the Roman calendar? -------------------------------- Before Julius Caesar introduced the Julian calendar in 45 BC, the Roman calendar was a mess, and much of our so-called "knowledge" about it seems to be little more than guesswork. Originally, the year started on 1 March and consisted of only 304 days or 10 months (Martius, Aprilis, Maius, Junius, Quintilis, Sextilis, September, October, November, and December). These 304 days were followed by an unnamed and unnumbered winter period. The Roman king Numa Pompilius (c. 715-673 BC, although his historicity is disputed) allegedly introduced February and January (in that order) between December and March, increasing the length of the year to 354 or 355 days. In 450 BC, February was moved to its current position between January and March. In order to make up for the lack of days in a year, an extra month, Intercalaris or Mercedonius, (allegedly with 22 or 23 days though some authorities dispute this) was introduced in some years. In an 8 year period the length of the years were: 1: 12 months or 355 days 2: 13 months or 377 days 3: 12 months or 355 days 4: 13 months or 378 days 5: 12 months or 355 days 6: 13 months or 377 days 7: 12 months or 355 days 8: 13 months or 378 days A total of 2930 days corresponding to a year of 366 1/4 days. This year was discovered to be too long, and therefore 7 days were later dropped from the 8th year, yielding 365.375 days per year. This is all theory. In practice it was the duty of the priesthood to keep track of the calendars, but they failed miserably, partly due to ignorance, partly because they were bribed to make certain years long and other years short. Furthermore, leap years were considered unlucky and were therefore avoided in time of crisis, such as the Second Punic War. In order to clean up this mess, Julius Caesar made his famous calendar reform in 45 BC. We can make an educated guess about the length of the months in the years 47 and 46 BC: 47 BC 46 BC January 29 29 February 28 24 Intercalaris 27 March 31 31 April 29 29 May 31 31 June 29 29 Quintilis 31 31 Sextilis 29 29 September 29 29 October 31 31 November 29 29 Undecember 33 Duodecember 34 December 29 29 --- --- Total 355 445 The length of the months from 45 BC onward were the same as the ones we know today. Occasionally one reads the following story: "Julius Caesar made all odd numbered months 31 days long, and all even numbered months 30 days long (with February having 29 days in non-leap years). In 44 BC Quintilis was renamed 'Julius' (July) in honour of Julius Caesar, and in 8 BC Sextilis became 'Augustus' in honour of emperor Augustus. When Augustus had a month named after him, he wanted his month to be a full 31 days long, so he removed a day from February and shifted the length of the other months so that August would have 31 days." This story, however, has no basis in actual fact. It is a fabrication possibly dating back to the 14th century. 2.6.1. How did the Romans number days? -------------------------------------- The Romans didn't number the days sequentially from 1. Instead they had three fixed points in each month: "Kalendae" (or "Calendae"), which was the first day of the month. "Idus", which was the 13th day of January, February, April, June, August, September, November, and December, or the 15th day of March, May, July, or October. "Nonae", which was the 9th day before Idus (counting Idus itself as the 1st day). The days between Kalendae and Nonae were called "the 4th day before Nonae", "the 3rd day before Nonae", and "the 2nd day before Nonae". (The 1st day before Nonae would be Nonae itself.) Similarly, the days between Nonae and Idus were called "the Xth day before Idus", and the days after Idus were called "the Xth day before Kalendae (of the next month)". Julius Caesar decreed that in leap years the "6th day before Kalendae of March" should be doubled. So in contrast to our present system, in which we introduce an extra date (29 February), the Romans had the same date twice in leap years. The doubling of the 6th day before Kalendae of March is the origin of the word "bissextile". If we create a list of equivalences between the Roman days and our current days of February in a leap year, we get the following: 7th day before Kalendae of March 23 February 6th day before Kalendae of March 24 February 6th day before Kalendae of March 25 February 5th day before Kalendae of March 26 February 4th day before Kalendae of March 27 February 3rd day before Kalendae of March 28 February 2nd day before Kalendae of March 29 February Kalendae of March 1 March You can see that the extra 6th day (going backwards) falls on what is today 24 February. For this reason 24 February is still today considered the "extra day" in leap years (see section 2.3). However, at certain times in history the second 6th day (25 Feb) has been considered the leap day. Why did Caesar choose to double the 6th day before Kalendae of March? It appears that the leap month Intercalaris/Mercedonius of the pre-reform calendar was not placed after February, but inside it, namely between the 7th and 6th day before Kalendae of March. It was therefore natural to have the leap day in the same position. 2.7. Has the year always started on 1 January? ---------------------------------------------- For the man in the street, yes. When Julius Caesar introduced his calendar in 45 BC, he made 1 January the start of the year, and it was always the date on which the Solar Number and the Golden Number (see section 2.9.3) were incremented. However, the church didn't like the wild parties that took place at the start of the new year, and in AD 567 the council of Tours declared that having the year start on 1 January was an ancient mistake that should be abolished. Through the middle ages various New Year dates were used. If an ancient document refers to year X, it may mean any of 7 different periods in our present system: - 1 Mar X to 28/29 Feb X+1 - 1 Jan X to 31 Dec X - 1 Jan X-1 to 31 Dec X-1 - 25 Mar X-1 to 24 Mar X - 25 Mar X to 24 Mar X+1 - Saturday before Easter X to Friday before Easter X+1 - 25 Dec X-1 to 24 Dec X Choosing the right interpretation of a year number is difficult, so much more as one country might use different systems for religious and civil needs. The Byzantine Empire used a year staring on 1 Sep, but they didn't count years since the birth of Christ, instead they counted years since the creation of the world which they dated to 1 September 5509 BC. Since about 1600 most countries have used 1 January as the first day of the year. Italy and England, however, did not make 1 January official until around 1750. In England (but not Scotland) three different years were used: - The historical year, which started on 1 January. - The liturgical year, which started on the first Sunday in advent. - The civil year, which from the 7th to the 12th century started on 25 December, from the 12th century until 1751 started on 25 March, from 1752 started on 1 January. 2.8. What is the origin of the names of the months? --------------------------------------------------- January Latin: Januarius. Named after the god Janus. February Latin: Februarius. Named after Februa, the purification festival. March Latin: Martius. Named after the god Mars. April Latin: Aprilis. Named either after the goddess Aphrodite or the Latin word "aperire", to open. May Latin: Maius. Probably named after the goddess Maia. June Latin: Junius. Probably named after the goddess Juno. July Latin: Julius. Named after Julius Caesar in 44 BC. Prior to that time its name was Quintilis from the word "quintus", fifth, because it was the 5th month in the old Roman calendar. August Latin: Augustus. Named after emperor Augustus in 8 BC. Prior to that time the name was Sextilis from the word "sextus", sixth, because it was the 6th month in the old Roman calendar. September Latin: September. From the word "septem", seven, because it was the 7th month in the old Roman calendar. October Latin: October. From the word "octo", eight, because it was the 8th month in the old Roman calendar. November Latin: November. From the word "novem", nine, because it was the 9th month in the old Roman calendar. December Latin: December. From the word "decem", ten, because it was the 10th month in the old Roman calendar. --- End of part 1 ---