Unit of time
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Units of measurement for time have historically been based on the movement of the Sun (as seen from Earth). Shorter intervals were measured by physiological periods such as drawing breath, winking or the pulse.
Units of time consisting of a number of years include the lustrum (five years) and the olympiad (four years). The month could be divided into half-months or fortnights, and quarters or weeks. Longer periods were given in lifetimes or generations (saecula, aion), subdivisions of the solar day in hours. The Sothic cycle was a period of 1,461 years of 365 days in the Ancient Egyptian calendar. Medieval (Pauranic) Hindu cosmology is notorious for introducing names for fabulously long time periods, such as kalpa (4.32 billion years).
In classical antiquity, the hour divided the daylight period into 12 equal parts. The duration of an hour thus varied over the course of the year. In classical China, the kè (刻) was a unit of decimal time, dividing a day into 100 equal intervals of 14.4 minutes. Alongside the ke, there were double hours (shíchen) also known as watches. Because one cannot divide 12 double hours into 100 ke evenly, each ke was subdivided into 60 fēn (分).
The introduction of the minute (minuta; ′) as the 60th part of an hour, the second (seccunda; ′′) as the 60th part of a minute, and the third (tertia; ′′′) as the 60th part of the second dates to the medieval period, used by Al-Biruni around AD 1000, and by Roger Bacon in the 13th century. Bacon further subdivided the tertia into a quarta or fourth (′′′′). Hindu chronology divides the civil day (daylight hours) into vipalas, palas and ghatikas. A tithi is the 30th part of the synodic month.
The introduction of the division of the solar day into 24 hours of equal length, as it were the length of a classical hour at equinox used regardless of daylight hours, dates to the 14th century, due to the development of the first mechanical clocks.
Today, the fundamental unit of time suggested by the International System of Units is the second, since 1967 defined as the second of International Atomic Time, based on the radiation emitted by a Caesium-133 atom in the ground state. Its definition was calibrated such that 86,400 seconds corresponded to a solar day. 31,557,600 (86,400 × 365.25) seconds are a Julian year, exceeding the true length of a solar year by about 21 ppm.
Based on the second as the base unit, the following time units are in use as follows:
- minute (1 min = 60 sec)
- hour (1 hr = 60 min = 3.6 ks)
- Julian day (1 d = 24 hr = 86.4 ks)
- week (7 d = 604.8 ks)
- Julian year (1 a = 365.25 d = 31.5576 Ms)
- decade (10 years/annum)
- century (100 annum = 3.15576 Gs)
- millennium (1 ka = 31.5576 Gs)
There are a number of proposals for decimal time, or decimal calendars, notably in the French Republican Calendar of 1793. Such systems have either ten days per week, a multiple of ten days in a month, or ten months per year.
A suggestion for hexadecimal time divides the Julian day into 16 hexadecimal hours of 1hr 30 min each, or 65,536 hexadecimal seconds (1 hexsec ≈ 1.32 s).
|Unit||Length, Duration and Size||Notes||Other|
|Planck time unit||5.39 x 10−44 s||The amount of time light takes to travel one Planck length. Theoretically, this is the smallest time measurement that will ever be possible. Smaller time units have no use in physics as we understand it today.|
|jiffy (physics)||3 × 10−24s||The amount of time light takes to travel one fermi (about the size of a nucleon) in a vacuum.|
|attosecond||10−18 s||shortest time now measurable|
|femtosecond||10−15 s||pulse time on fastest lasers|
|Svedberg||10−13 s||time unit used for sedimentation rates (usually of proteins)|
|nanosecond||10−9 s||time for molecules to fluoresce|
|shake||10−8 s||10 nanoseconds||Also a casual term for a short period of time|
|fourth||1/3,600 second||medieval unit of time|
|millisecond||0.001 s||shortest time unit used on stopwatches|
|centisecond||0.01 s||used on some stopwatches|
|third||1/60 s||medieval unit of time|
|jiffy (electronics)||1/60s to 1/50s||Used to measure the time between alternating power cycles. Also a casual term for a short period of time|
|decisecond||0.1 s||used on some stopwatches|
|second||1 sec||SI base unit|
|moment||1/40th of an hour (~90 seconds)||medieval unit of time used by astronomers to compute astronomical movements.|
|hectosecond||100 seconds||1 minute and 40 seconds|
|ke||14 minutes and 24 seconds|
|kilosecond||1,000 seconds||16 minutes and 40 seconds|
|day||24 hours||longest unit used on stopwatches and countdowns|
|week||7 days||Also called sennight|
|megasecond||1,000,000 seconds||About 11.6 days|
|fortnight||2 weeks||14 days||may not be common|
|lunar month||27 Days 4 hours 48 minutes–29 days 12 hours||Various definitions of lunar month exist.|
|quarter and season||3 months|
|year||12 months or 365 days|
|common year||365 days||52 weeks + 1 day|
|tropical year||365 days 5:48:45.216 hours||average|
|Gregorian year||365 days 5:49:12 hours||average|
|sidereal year||365 days 6:09:09.7635456 hours|
|leap year||366 days||52 weeks + 2 days|
|biennium||2 years||A unit of time commonly used by legislatures|
|Olympiad||4 year cycle||48 months, 1,461 days, 35,064 hours, 2,103,840 minutes, 126,230,400 seconds|
|Indiction||15 year cycle|
|score||20 years||"four score and seven years.." = 87 years|
|gigasecond||1,000,000,000 seconds||About 31.7 years|
|millennium||1,000 years||also called "kiloannum"|
|terasecond||1 trillion seconds||About 31,700 years|
|age and megaannum||1,000,000 years|
|petasecond||1 quadrillion seconds||About 3.17 epoches|
|galactic year||Approximately 2.3 eras||The amount of time it takes the Solar System to orbit the center of the Milky Way Galaxy one time.|
|eon||500,000,000 years||Also "An indefinite and very long period of time"|
|exasecond||1 quintillion seconds||roughly 31.7 billion years, more than twice
the age of the universe on current estimates
|zettasecond||1 sextillion seconds||About 31.7 trillion years|
|yottasecond||1 septillion seconds||About 31.7 quadrillion years|
|cosmological decade||varies||10 times the length of the previous
cosmological decade, with CÐ 1 beginning
either 10 seconds or 10 years after the
Big Bang, depending on the definition.
All these units are not used in time. The key units are the second, defined in terms of an atomic process; the day, an integral multiple of seconds; and the year, usually 365.25 days. Most of the other units used are multiples or divisions of these three. The graphic also shows the three heavenly bodies whose orbital parameters relate to the units of time.
- Milham, Willis I. (1945). Time and Timekeepers. New York: MacMillan. p. 190. ISBN 0-7808-0008-7.
- McCarthy, Dennis D.; Seidelmann, P. Kenneth (2009). Time: from Earth rotation to atomic physics. Wiley-VCH. p. 18. ISBN 3-527-40780-4., Extract of page 18
- Jones, Floyd Nolen (2005). The Chronology Of The Old Testament (15th ed.). New Leaf Publishing Group. p. 287. ISBN 0-89051-416-X., Extract of page 287
- http://starchild.gsfc.nasa.gov/docs/StarChild/questions/question18.html NASA - StarChild Question of the Month for February 2000