A year is the orbital period
of a planetary body, for example, the Earth
, moving in its orbit
around the Sun
. Due to the Earth's axial tilt
, the course of a year sees the passing of the season
s, marked by change in weather
, the hours of daylight
, and, consequently, vegetation
and soil fertility
. In temperate
regions around the planet, four seasons are generally recognized: spring
. In tropical
regions, several geographical sectors do not present defined seasons; but in the seasonal tropics
, the annual wet
and dry season
s are recognized and tracked.
A calendar year
is an approximation of the number of days of the Earth's orbital period, as counted in a given calendar
. The Gregorian calendar
, or modern calendar, presents its calendar year to be either a common year
of 365 days or a leap year
of 366 days, as do the Julian calendar
s; ''see'' below
. For the Gregorian calendar, the average length of the calendar year (the mean year) across the complete leap cycle of 400 years is 365.2425 days. In English, the abbreviations ''y'' and ''yr'' are commonly used.
In astronomy, the Julian year
is a unit of time
; it is defined as 365.25 day
s of exactly 86,400 second
s (SI base unit
), totalling exactly 31,557,600 seconds in the Julian astronomical year.
The word ''year'' is also used for periods loosely associated with, but not identical to, the calendar or astronomical year, such as the seasonal year
, the fiscal year
, the academic year
, etc. Similarly, ''year'' can mean the orbital period of any planet
; for example, a Martian year
and a Venusian year
are examples of the time a planet takes to transit one complete orbit. The term can also be used in reference to any long period or cycle, such as the Great Year
English ''year'' (via West Saxon
''ġēar'' (), Anglian
''ġēr'') continues Proto-Germanic
''). Cognates are German
''Jahr'', Old High German
''jār'', Old Norse
''ár'' and Gothic
'', from the Proto-Indo-European
noun ' "year, season". Cognates also descended from the same Proto-Indo-European noun (with variation in suffix ablaut
) are Avestan
''yārǝ'' "year", Greek
() "year, season, period of time" (whence "hour
"), Old Church Slavonic
''jarŭ'', and Latin
''hornus'' "of this year".
Latin (a 2nd declension
masculine noun; is the accusative singular
; is genitive singular and nominative plural; the dative and ablative singular) is from a PIE
noun ', which also yielded Gothic ''aþn'' "year" (only the dative plural ''aþnam'' is attested).
Although most languages treat the word as thematic ''*yeh₁r-o-'', there is evidence for an original derivation with an ''*-r/n'' suffix, ''*yeh₁-ro-''. Both Indo-European words for year, ''*yeh₁-ro-'' and ''*h₂et-no-'', would then be derived from verbal roots meaning "to go, move", ''*h₁ey-'' and ''*h₂et-'', respectively (compare Vedic Sanskrit
''éti'' "goes", ''atasi'' "thou goest, wanderest"). A number of English words are derived from Latin , such as annual
, etc.; ''per annum
'' means "each year", means "in the year of the Lord".
The Greek word for "year", , is cognate with Latin ''vetus'' "old", from the PIE word ''*wetos-'' "year", also preserved in this meaning in Sanskrit
' "year" and ' "yearling (calf)", the latter also reflected in Latin ''vitulus
'' "bull calf", English ''wether'' "ram" (Old English ''weðer'', Gothic ''wiþrus'' "lamb").
In some languages, it is common to count years by referencing to one season, as in "summers", or "winters", or "harvests". Examples include Chinese 年
"year", originally 秂
, an ideographic compound of a person carrying a bundle of wheat denoting "harvest". Slavic besides ''godŭ
'' "time period; year" uses ''lěto
'' "summer; year".
Astronomical years do not have an integer
number of days or lunar months. Any calendar that follows an astronomical year must have a system of intercalation
such as leap years.
In the Julian calendar, the average (mean) length of a year is 365.25 days. In a non-leap year, there are 365 days, in a leap year there are 366 days. A leap year occurs every fourth year, or leap year, during which a leap day is intercalated
into the month of February. The name "Leap Day
" is applied to the added day.
The Revised Julian calendar
, proposed in 1923 and used in some Eastern Orthodox Church
has 218 leap years every 900 years, for the average (mean) year length of days, close to the length of the mean tropical year, days (relative error of 9·10−8
In the year 2800 CE, the Gregorian and Revised Julian calendars will begin to differ by one calendar day.
The Gregorian calendar attempts to cause the northward equinox
to fall on or shortly before March 21 and hence it follows the northward equinox year
, or tropical year
. Because 97 out of 400 years are leap years, the mean length of the Gregorian calendar year is days; with a relative error below one ppm
) relative to the current length of the mean tropical year
( days) and even closer to the current ''March equinox year'' of days that it aims to match. It is estimated that by the year 4000 CE, the northward equinox will fall back by one day in the Gregorian calendar, not because of this difference, but due to the slowing of the Earth's rotation and the associated lengthening of the day.
Historically, lunisolar calendars intercalated entire leap month
s on an observational basis. Lunisolar calendars have mostly fallen out of use except for liturgical reasons (Hebrew calendar
, various Hindu calendar
A modern adaptation of the historical Jalali calendar
, known as the Solar Hijri calendar
(1925), is a purely solar calendar
with an irregular pattern of leap days based on observation (or astronomical computation), aiming to place new year (Nowruz
) on the day of vernal equinox
(for the time zone of Tehran
), as opposed to using an algorithmic system of leap years.
A calendar era
assigns a cardinal number
to each sequential year, using a reference point in the past as the beginning of the era.
The worldwide standard is the Anno Domini
, although some prefer the term Common Era
because it has no explicit reference to Christianity
. It was introduced in the 6th century and was intended to count years from the nativity of Jesus
The Anno Domini era is given the Latin abbreviation AD (for Anno Domini
"in the year of the Lord"), or alternatively CE for "Common Era
". Years before AD 1 are abbreviated BC for Before Christ
or alternatively BCE for Before the Common Era
. Year numbers are based on inclusive counting
, so that there is no "year zero". In the modern alternative reckoning of Astronomical year numbering
, positive numbers indicate years AD, the number 0
designates 1 BC, −1 designates 2 BC, and so on.
Financial and scientific calculations often use a 365-day calendar
to simplify daily rates.
A fiscal year
or financial year is a 12-month period used for calculating annual financial statements in businesses and other organizations. In many jurisdictions, regulations regarding accounting require such reports once per twelve months, but do not require that the twelve months constitute a calendar year.
For example, in Canada
the fiscal year runs from April 1; in the United Kingdom
it runs from April 1 for purposes of corporation tax and government financial statements, but from April 6 for purposes of personal taxation and payment of state benefits; in Australia
it runs from July 1; while in the United States
the fiscal year of the federal government
runs from October 1.
An academic year is the annual period during which a student attends an educational institution
. The academic year may be divided into academic term
s, such as semesters or quarters. The school year in many countries starts in August or September and ends in May, June or July. In Israel the academic year begins around October or November, aligned with the second month of the Hebrew calendar
Some schools in the UK, Canada and the United States divide the academic year into ''three'' roughly equal-length terms (called ''trimesters'' or ''quarters'' in the United States), roughly coinciding with autumn, winter, and spring. At some, a shortened summer session, sometimes considered part of the regular academic year, is attended by students on a voluntary or elective basis. Other schools break the year into ''two'' main semesters, a first (typically August through December) and a second semester (January through May). Each of these main semesters may be split in half by mid-term exams, and each of the halves is referred to as a ''quarter'' (or ''term'' in some countries). There may also be a voluntary summer session and/or a short January session.
Some other schools, including some in the United States, have ''four'' marking periods. Some schools in the United States, notably Boston Latin School
, may divide the year into ''five or more'' marking periods. Some state in defense of this that there is perhaps a positive correlation
between report frequency and academic achievement.
There are typically 180 days of teaching each year in schools in the US, excluding weekends and breaks, while there are 190 days for pupils in state schools in Canada, New Zealand and the United Kingdom, and 200 for pupils in Australia.
In India the academic year normally starts from June 1 and ends on May 31. Though schools start closing from mid-March, the actual academic closure is on May 31 and in Nepal it starts from July 15.
Schools and universities in Australia typically have academic years that roughly align with the calendar year (i.e., starting in February or March and ending in October to December), as the southern hemisphere experiences summer from December to February.
The Julian year, as used in astronomy and other sciences, is a time unit defined as exactly 365.25 days. This is the normal meaning of the unit "year" used in various scientific contexts. The Julian century of days and the Julian millennium of days are used in astronomical calculations. Fundamentally, expressing a time interval in Julian years is a way to precisely specify how many days (not how many "real" years), for long time intervals where stating the number of days would be unwieldy and unintuitive. By convention, the Julian year is used in the computation of the distance covered by a light-year
In the Unified Code for Units of Measure
, the symbol ''a'' (without subscript) always refers to the Julian year, ''aj
'', of exactly second
:365.25 d × s = 1 a = 1 aj
The SI multiplier prefixes
may be applied to it to form ''ka'' (kiloannus), ''Ma'' (megaannus), etc.
Sidereal, tropical, and anomalistic years
Each of these three years can be loosely called an ''astronomical year''.
The sidereal year
is the time taken for the Earth to complete one revolution of its orbit
, as measured against a fixed frame of reference (such as the fixed stars, Latin , singular ). Its average duration is days (365 d 6 h 9 min 9.76 s) (at the epoch J2000.0
= January 1, 2000, 12:00:00 TT
Today the mean tropical year is defined as the period of time for the mean ecliptic longitude
of the Sun to increase by 360 degrees. Since the Sun's ecliptic longitude is measured with respect to the equinox, the tropical year comprises a complete cycle of the seasons; because of the biological and socio-economic importance of the seasons, the tropical year is the basis of most calendars. The modern definition of mean tropical year differs from the actual time between passages of, e.g., the northward equinox for several reasons explained below. Because of the Earth's axial precession
, this year is about 20 minutes shorter than the sidereal year. The mean tropical year is approximately 365 days, 5 hours, 48 minutes, 45 seconds, using the modern definition ( = 365.24219 d × 86 400 s).
The anomalistic year is the time taken for the Earth to complete one revolution with respect to its apsides
. The orbit of the Earth is elliptical; the extreme points, called apsides, are the perihelion
, where the Earth is closest to the Sun (January 5, 07:48 UT in 2020), and the aphelion
, where the Earth is farthest from the Sun (July 4, 11:35 UT in 2020). The anomalistic year is usually defined as the time between perihelion passages. Its average duration is 365.259636 days (365 d 6 h 13 min 52.6 s) (at the epoch J2011.0).
The draconic year, draconitic year, eclipse year, or ecliptic year is the time taken for the Sun (as seen from the Earth) to complete one revolution with respect to the same lunar node
(a point where the Moon's orbit intersects the ecliptic). The year is associated with eclipse
s: these occur only when both the Sun and the Moon are near these nodes; so eclipses occur within about a month of every half eclipse year. Hence there are two eclipse season
s every eclipse year. The average duration of the eclipse year is
: days (346 d 14 h 52 min 54 s) (at the epoch J2000.0).
This term is sometimes erroneously used for the draconic or nodal period of lunar precession
, that is the period of a complete revolution of the Moon's ascending node around the ecliptic: Julian years ( days; at the epoch J2000.0).
Full moon cycle
The full moon cycle
is the time for the Sun (as seen from the Earth) to complete one revolution with respect to the perigee
of the Moon's orbit. This period is associated with the apparent size of the full moon
, and also with the varying duration of the synodic month
. The duration of one full moon cycle is:
: days (411 days 18 hours 49 minutes 35 seconds) (at the epoch J2000.0).
The lunar year
comprises twelve full cycles of the phases of the Moon, as seen from Earth. It has a duration of approximately 354.37 days. Muslims
use this for celebrating their Eids
and for marking the start of the fasting month of Ramadan
. A Muslim calendar year is based on the lunar cycle. The Jewish calendar
is also essentially lunar, except that an intercalary lunar month is added once every two or three years, in order to keep the calendar synchronized with the solar cycle as well. Thus, a lunar year on the Jewish (Hebrew) calendar consists of either twelve or thirteen lunar months.
The vague year, from or wandering year, is an integral approximation to the year equaling 365 days, which wanders in relation to more exact years. Typically the vague year is divided into 12 schematic
months of 30 days each plus 5 epagomenal
days. The vague year was used in the calendars of Ethiopia
, Ancient Egypt
and in Mesoamerica
among the Aztecs
. It is still used by many Zoroastrian communities.
A heliacal year is the interval between the heliacal rising
s of a star. It differs from the sidereal year
for stars away from the ecliptic
due mainly to the precession of the equinoxes
The Sothic year
is the interval between heliacal risings of the star Sirius
. It is currently less than the sidereal year
and its duration is very close to the Julian year of 365.25 days.
The Gaussian year
is the sidereal year for a planet of negligible mass (relative to the Sun) and unperturbed by other planets that is governed by the Gaussian gravitational constant
. Such a planet would be slightly closer to the Sun than Earth's mean distance. Its length is:
: days (365 d 6 h 9 min 56 s).
The Besselian year
is a tropical year that starts when the (fictitious) mean Sun reaches an ecliptic longitude of 280°. This is currently on or close to January 1. It is named after the 19th-century German astronomer and mathematician Friedrich Bessel
. The following equation can be used to compute the current Besselian epoch (in years):
: B = 1900.0 + (Julian dateTT
− ) /
The TT subscript indicates that for this formula, the Julian date should use the Terrestrial Time
scale, or its predecessor, ephemeris time
Variation in the length of the year and the day
The exact length of an astronomical year changes over time.
* The positions of the equinox and solstice points with respect to the apsides of Earth's orbit change: the equinoxes and solstices move westward relative to the stars because of precession
, and the apsides move in the other direction because of the long-term effects of gravitational pull by the other planets. Since the speed of the Earth varies according to its position in its orbit as measured from its perihelion, Earth's speed when in a solstice or equinox point changes over time: if such a point moves toward perihelion, the interval between two passages decreases a little from year to year; if the point moves towards aphelion, that period increases a little from year to year. So a "tropical year" measured from one passage of the northward ("vernal") equinox to the next, differs from the one measured between passages of the southward ("autumnal") equinox. The average over the full orbit does not change because of this, so the length of the average tropical year does not change because of this second-order effect.
* Each planet's movement is perturbed by the gravity of every other planet. This leads to short-term fluctuations in its speed, and therefore its period from year to year. Moreover, it causes long-term changes in its orbit, and therefore also long-term changes in these periods.
* Tidal drag
between the Earth and the Moon and Sun increases the length of the day and of the month (by transferring angular momentum from the rotation of the Earth to the revolution of the Moon); since the apparent mean solar day is the unit with which we measure the length of the year in civil life, the length of the year appears to decrease. The rotation rate of the Earth is also changed by factors such as post-glacial rebound
and sea level rise
; Numerical value of year variation
Mean year lengths in this section are calculated for 2000, and differences in year lengths, compared to 2000, are given for past and future years. In the tables a day is 86,400 SI seconds long.
An average Gregorian year is 365.2425 day
s (52.1775 week
s or second
s). For this calendar, a common year is 365 days ( hours, minutes or seconds), and a leap year is 366 days ( hours, minutes or seconds). The 400-year cycle of the Gregorian calendar has days and hence exactly weeks.
"Greater" astronomical years
The Great Year, or equinoctial cycle, corresponds to a complete revolution of the equinoxes around the ecliptic. Its length is about 25,700 years.
The Galactic year
is the time it takes Earth's Solar System
to revolve once around the galactic center
. It comprises roughly 230 million Earth years.
A seasonal year is the time between successive recurrences of a seasonal event such as the flooding of a river, the migration of a species of bird, the flowering of a species of plant, the first frost, or the first scheduled game of a certain sport. All of these events can have wide variations of more than a month
from year to year.
A common symbol for the year as a unit of time
'', taken from the Latin word . In English, the abbreviations "y" or "yr" are more commonly used in non-scientific literature but also specifically in geology
, where "kyr
" (thousands, millions, and billions of years, respectively) and similar abbreviations are used to denote intervals of time remote from the present.
NIST SP811 supports the symbol ''a'' as the unit of time for a year. In English, the abbreviations ''y'' and ''yr'' are also used.
The Unified Code for Units of Measure
disambiguates the varying symbologies of ISO 1000, ISO 2955 and ANSI X3.50 by using:
'' = days for the mean tropical year;
'' = 365.25 days for the mean Julian year;
'' = days for the mean Gregorian year
:''a'', without a qualifier = 1 aj
:and ''ar'', for ''are
'', is a unit of area.
The International Union of Pure and Applied Chemistry
(IUPAC) and the International Union of Geological Sciences
have jointly recommended defining the "annus," with symbol ''a'', as the length of the tropical year in the year 2000:
:''a'' = seconds (approximately ephemeris day
This differs from the above definition of 365.25 days by about 20 parts per million
. The joint document says that definitions such as the Julian year "bear an inherent, pre-programmed obsolescence because of the variability of Earth’s orbital movement", but then proposes using the length of the tropical year as of 2000 AD (specified down to the millisecond), which suffers from the same problem.
(The tropical year oscillates with time by more than a minute.)
The notation has proved controversial as it conflicts with an earlier convention among geoscientists to use ''a'' specifically for ''years ago'', and ''y'' or ''yr'' for a one-year time period.
SI prefix multipliers
For the following, there are alternative forms that elide the consecutive vowels, such as ''kilannus'', ''megannus'', etc. The exponents and exponential notations are typically used for calculating and in displaying calculations, and for conserving space, as in tables of data.
* ''ka'' (for kiloannum) – a unit of time
equal to one thousand
, or 103
, years, or 1 E3 yr, also known as a millennium
and calendar uses. The prefix multiplier "ka" is typically used in geology, paleontology, and archaeology
for the Holocene
and Pleistocene periods
, where a non−radiocarbon dating
technique: e.g. ice core
, uranium-thorium dating
, or varve
analysis; is used as the primary dating method for age determination. If age is determined primarily by radiocarbon dating
, then the age should be expressed in either radiocarbon or calendar (calibrated) years Before Present
* ''Ma'' (for megaannum) – a unit of time
equal to one million
, or 106
, years, or 1 E6 yr. The suffix "Ma" is commonly used in scientific disciplines such as geology, paleontology, and celestial mechanics
to signify very long time periods into the past or future. For example, the dinosaur
species ''Tyrannosaurus rex
'' was abundant approximately 66 Ma (66 million years) ago. The duration term "ago" may not always be indicated: if the quantity of a duration is specified while not explicitly mentioning a duration term, one can assume that "ago" is implied; the alternative unit "mya" does include "ago" explicitly. It is also written as "million years" (ago) in works for general public use. In astronomical applications, the year used is the Julian year of precisely 365.25 days. In geology and paleontology, the year is not so precise and varies depending on the author.
* ''Ga'' (for gigaannum) – a unit of time equal to 109
years, or one billion
years. "Ga" is commonly used in scientific disciplines such as cosmology
and geology to signify extremely long time periods in the past. For example, the formation of the Earth
occurred approximately 4.54 Ga (4.54 billion years) ago and the age of the universe
is approximately 13.8 Ga.
* ''Ta'' (for teraannum) – a unit of time equal to 1012
years, or one trillion
years. "Ta" is an extremely long unit of time, about 70 times as long as the age of the universe
. It is the same order of magnitude as the expected life span of a small red dwarf
* ''Pa'' (for petaannum) – a unit of time equal to 1015
years, or one quadrillion
years. The half-life of the nuclide cadmium-113
is about 8 Pa. This symbol coincides with that for the pascal
without a multiplier prefix, though both are infrequently used and context will normally be sufficient to distinguish time from pressure values.
* ''Ea'' (for exaannum) – a unit of time equal to 1018
years, or one quintillion
years. The half-life of tungsten-180
is 1.8 Ea.
Abbreviations yr and ya
, geology, and paleontology, the abbreviation ''yr'' for ''years'' and ''ya'' for ''years ago'' are sometimes used, combined with prefixes for thousand, million, or billion.
They are not SI units, using ''y'' to abbreviate the English "year
", but following ambiguous international recommendations, use either the standard English first letters as prefixes (t, m, and b) or metric prefix
es (k, M, and G) or variations on metric prefixes (k, m, g). In archaeology, dealing with more recent periods, normally expressed dates, e.g. "22,000 years ago" may be used as a more accessible equivalent of a Before Present
These abbreviations include:
Use of ''mya'' and ''bya'' is deprecated in modern geophysics, the recommended usage being ''Ma'' and ''Ga'' for dates Before Present
, but "m.y." for the duration of epochs.
This ''ad hoc'' distinction between "absolute" time and time intervals is somewhat controversial amongst members of the Geological Society of America.
Note that on graphs, using ''ya'' units on the horizontal axis time flows from right to left, which may seem counter-intuitive. If the ''ya'' units are on the vertical axis, time flows from top to bottom which is probably easier to understand than conventional notation.
: current year
* Astronomical year numbering
* Epoch (reference date)
* ISO 8601
: standard for representation of dates and times
* List of calendars
* List of years
* Orders of magnitude (time)
* Unit of time
* Images of years