Calendar is
a system of measuring time for the
needs of civil life, by dividing time into days, weeks, months, and
years.
Calendar divisions are based on the movements of the earth and the
regular
appearances of the sun and the moon. A day is the average time required
for one
rotation of the earth on its axis. The measurement of a year is based on
one
revolution of the earth around the sun and is called a seasonal,
tropical, or
solar year. A solar year contains 365 days, 5 hr, 48 min, and 45.5 sec. A
month
was originally calculated by ancient peoples as the time between two
full
moons, or the number of days required for the moon to circle the earth
(29.5
days). This measurement, called a synodic, or lunar month, resulted in a
lunar
year of 354 days, 11 days
shorter than a solar year. In modern calendars, however, the number of
days in
a month is not based on the phases of the moon. The length of the months
is
approximately one-twelfth of a year (28 to 31 days) and is adjusted to
fit the
12 months into a solar year. For information concerning the names or
arrangement of the months, see the articles on each of the 12 months.
The week
was derived from the Judeo-Christian tradition requiring rest from labor
every
seventh day. It is not based on a natural phenomenon. The Romans named
the days
of the week in honor of the sun, moon, and various planets.
The variations among the
many calendars in use from
ancient to modern times have been caused by the inaccuracy of the
earliest
determinations of the duration of the year, together with the fact that a
year
cannot be divided evenly by any of the other time units: days, weeks, or
months. The earliest calendars based on lunar months eventually failed
to agree
with the seasons. A month occasionally had to be intercalated, or added,
to
reconcile lunar months with the solar year. A calendar that makes
periodic
adjustments of this kind is a lunisolar calendar.
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II
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ANCIENT
CALENDARS
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The ancient Babylonians
had a lunisolar calendar of 12
lunar months of 30 days each, and they added extra months when necessary
to
keep the calendar in line with the seasons of the year. The ancient
Egyptians
were the first to replace the lunar calendar with a calendar based on
the solar
year. They measured the solar year as 365 days, divided into 12 months
of 30
days each, with 5 extra days at the end. About 238 bc King Ptolemy III ordered
that an extra day be added to
every fourth year, similar to the modern leap year. In ancient Greece a
lunisolar
calendar was in use, with a year of 354 days. The Greeks were the first
to
intercalate extra months into the calendar on a scientific basis, adding
months
at specific intervals in a cycle of solar years.
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III
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THE ROMAN
CALENDAR
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The original Roman calendar,
introduced about the
7th century bc, had 10
months with
304 days in a year that began with March. Two more months, January and
February, were added later in the 7th century bc,
but because the months were only 29 or 30 days long, an extra month had
to be
intercalated approximately every second year. The days of the month were
designated by the awkward method of counting backward from three dates:
the
calends, or first of the month; the ides, or middle of the month,
falling on
the 13th of some months and the 15th of others; and the nones, or 9th
day
before the ides. The Roman calendar became hopelessly confused when
officials
to whom the addition of days and months was entrusted abused their
authority to
prolong their terms of office or to hasten or delay elections.
In 45 bc Julius Caesar,
upon the advice of the Greek astronomer Sosigenes (flourished 1st
century bc), decided to
use a purely solar
calendar. This calendar, known as the Julian calendar, fixed the normal
year at
365 days, and the leap year, every fourth year, at 366 days. Leap year
is so
named because the extra day causes any date after February in a leap
year to
“leap” over one day in the week and to occur two days later in the week
than it
did in the previous year, rather than just one day later as in a normal
year.
The Julian calendar also established the order of the months and the
days of
the week as they exist in present-day calendars. In 44 bc Julius Caesar changed the
name of the month Quintilis to
Julius (July), after himself. The month Sextilis was renamed Augustus
(August)
in honor of the Roman emperor Caesar Augustus, who succeeded Julius
Caesar.
Some authorities maintain that Augustus established the length of the
months we
use today.
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IV
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THE GREGORIAN
CALENDAR
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The Julian year was 11
min and 14 sec longer
than the solar year. This discrepancy accumulated until by 1582 the
vernal
equinox (see Ecliptic) occurred 10 days early and church holidays
did
not occur in the appropriate seasons. To make the vernal equinox occur
on March
21, as it had in ad 325,
the year
of the First Council of Nicaea, Pope Gregory XIII issued a decree
dropping 10
days from the calendar. To prevent further displacement he instituted a
calendar, known as the Gregorian calendar, that provided that century
years
divisible evenly by 400 should be leap years and that all other century
years
should be common years. Thus, 1600 was a leap year, but 1700 and 1800
were
common years.
The Gregorian calendar,
or New Style calendar, was
slowly adopted throughout Europe. It is used today throughout most of
the
Western world and in parts of Asia. When the Gregorian calendar was
adopted in
Britain in 1752, another correction of an 11-day discrepancy was made;
the day
after September 2, 1752, became September 14. The British also adopted
January
1 as the day when a new year begins. The Soviet Union adopted the
Gregorian
calendar in 1918, and Greece adopted it in 1923 for civil purposes, but
many
countries affiliated with the Greek church retain the Julian, or Old
Style,
calendar for the celebration of church feasts.
The Gregorian calendar
is also called the Christian
calendar because it uses the birth of Jesus Christ as a starting date.
Dates of
the Christian era (see Chronology) are often designated ad (Latin anno domini, “in
the
year of our Lord”) and bc
(before
Christ). Although the birth of Christ was originally given as December
25, ad 1, modern scholars
now place it about
4 bc.
Because the Gregorian
calendar still entails months of
unequal length, so that dates and days of the week vary through time,
numerous
proposals have been made for a more practical, reformed calendar. Such
proposals include a fixed calendar of 13 equal months and a universal
calendar
of 4 identical quarterly periods. Thus far, none has been adopted (see
Calendar
Reform).
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V
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RELIGIOUS
CALENDARS
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As indicated, the Gregorian
calendar is basically a
Christian calendar. The official Christian church calendar is a table
containing the holy days, saints’ days, and festivals of the church,
with the
dates of the civil calendar on which they occur. These include the fixed
feasts, such as Christmas, and the movable feasts, which depend on the
date of
Easter. The most important early church calendar was compiled by Furius
Dionisius Philocalus about 354. After the Reformation, the German
Lutheran
church retained the Roman calendar, as did the Church of England and
some other
Anglican churches. The calendar of the Protestant Episcopal church
retains only
those festivals that have a scriptural origin. The principal seasons of
the
church calendar observed by most Christians are, in order, Advent,
Christmas,
Epiphany, Lent, Easter, Ascension, Pentecost, and Trinity.
Several other calendars
based on religious doctrine can
also be described. For example, the Jewish calendar, derived from the
ancient
Hebrew calendar, has remained unchanged since about ad 900. It is the official
calendar of the modern state of
Israel and is used by Jewish people throughout the world as a religious
calendar. The starting point of Hebrew chronology is the year 3761 bc, the date for the creation
of the
world as described in the Old Testament. The Jewish calendar is
lunisolar,
based on lunar months of 29 days alternating with 30 days. An extra
month is
intercalated every 3 years, based on a cycle of 19 years. Dates of the
Jewish
calendar are designated am
(Latin anno
mundi,”the year of the world”) and bce
(before the common era).
Another major religious
calendar is the Islamic
calendar, a lunar one used in most Muslim countries. It is reckoned from
ad 622, the day after
the Hegira, or
emigration of Muhammad from Mecca to Medina. The Islamic year consists
of 12
lunar months. Thirty years constitute a cycle in which the 2nd, 5th,
7th, 10th,
13th, 16th, 18th, 21st, 24th, 26th, and 29th years are leap years of 355
days;
the others are common years of 354 days.
