In the fields of chronology Chronology is the science of arranging events in their order of occurrence in time, such as the use of a timeline. It is also "the determination of the actual temporal sequence of past events" and periodization Periodization is the attempt to categorize or divide time into named blocks. The result is a descriptive abstraction that provides a useful handle on periods of time with relatively stable characteristics. However, determining the precise beginning and ending to any "period" is often a matter of debate, an epoch means an instant in time chosen as the origin of a particular era An era is a commonly used word for long period of time. When used in science, for example geology, eras denote clearly defined periods of time of arbitrary but well defined length, such as for example the Mesozoic era from 252 Ma–66 Ma, delimited by a start event and an end event. When used in social history, eras may for example denote a period. The "epoch" then serves as a reference point from which time is measured. Time measurement units Time has been defined as the continuum in which events occur in succession from the past to the present and on to the future. Time has also been defined as a one-dimensional quantity used to sequence events, to quantify the durations of events and the intervals between them, and to quantify and measure the motions of objects and other changes are counted from the epoch so that the date and time of events can be specified unambiguously.

Events taking place before the epoch can be dated by counting negatively from the epoch, though in pragmatic periodization Periodization is the attempt to categorize or divide time into named blocks. The result is a descriptive abstraction that provides a useful handle on periods of time with relatively stable characteristics. However, determining the precise beginning and ending to any "period" is often a matter of debate practice, epochs are defined for the past, and another epoch is used to start the next era, therefore serving as the ending of the older preceding era. The whole purpose and criteria of such definitions is to clarify and co-ordinate scholarship about a period, at times, across disciplines.

Epochs are generally chosen to be convenient or significant by a consensus of the time scale's initial users, or by authoritarian fiat. The epoch moment or date is usually defined by a specific clear event, condition, or criteria— the epoch event or epoch criteria —from which the period or era or age is usually characterized or described.

Examples:

by events:
The assassination of the Roman Emperor The Roman Emperor was the ruler of the Roman State during the imperial period . The Romans had no single term for the office: Latin titles such as imperator (from which English emperor ultimately derives), augustus, caesar and princeps were all associated with it. In practice, the emperor was supreme ruler of Rome and supreme commander of the Alexander Severus Marcus Aurelius Severus Alexander , commonly called Alexander Severus, was the last Roman emperor (11 March 222–235) of the Severan dynasty. Alexander Severus succeeded his cousin, Elagabalus upon the latter's assassination in 222 AD, and was ultimately assassinated himself, marking the epoch event for the Crisis of the Third Century—nearly triggering the Crisis of the Third Century The Crisis of the Third Century (235–284 AD) was a period in which the Roman Empire nearly collapsed under the combined pressures of invasion, civil war, plague, and economic depression. The Crisis began with the assassination of Emperor Alexander Severus at the hands of his own troops, initiating a fifty-year period in which 20–25 claimants
The defenestration of Prague The Defenestrations of Prague were two incidents in the history of Bohemia. The first occurred in 1419 and the second in 1618, although the term "Defenestration of Prague" is more commonly used to refer to the second incident. Both helped to trigger prolonged conflict within Bohemia and beyond. Defenestration is the act of throwing triggering the Thirty Years' War Pilsen – Lomnice – Sablat – Wisternitz – Humenné – White Mountain – Neu Titschein – Mingolsheim – Wimpfen – Höchst – Fleurus – Stadtlohn – Breda – Cádiz – Dessau Bridge – Lutter am Barenberge – Stralsund – Wolgast – St. Kitts– Swedish landing – Frankfurt – Magdeburg – Werben – 1st Breitenfeld –
Queen Victoria Victoria was the Queen regnant of the United Kingdom of Great Britain and Ireland from 20 June 1837, and the first Empress of India of the British Raj from 1 May 1876, until her death. Her reign as the Queen lasted 63 years and 7 months, longer than that of any other British monarch before or since, and her reign is the longest of any female ascending to the throne giving the start of the Victorian era The Victorian era of the United Kingdom was the period of Queen Victoria's reign from June 1837 until her death on the 22nd of January 1901. The reign was a long period of prosperity for the British people, as profits gained from the overseas British Empire, as well as from industrial improvements at home, allowed an educated middle class to
by criteria:
The spurt in exploration, mercantilism, and colonization in the Age of Discovery The Age of Discovery, also known as the Age of Exploration, was a period in history starting in the 15th century and continuing into the early 17th century, during which Europeans and their descendants intensively explored and mapped the world. Historians often refer to the 'Age of Discovery' as the period of Portuguese and Spanish pioneer oceanic
Particular ratios of animal fossils in a rock strata —various Geology epochs

Contents

Calendars

Each calendar era A calendar era is the year numbering system used by a calendar. For example, the Gregorian calendar numbers its years in the Western Christian era . The instant, date, or year from which time is marked is called the epoch of the era. There are many different calendar eras starts from an arbitrary epoch, which is often chosen to commemorate an important historical or mythological event. For example, the epoch of the anno Domini Anno Domini and Before Christ (abbreviated as BC or B.C.) are designations used to label years in the Julian and Gregorian calendars. The calendar era to which they refer is based on the traditionally reckoned year of the conception or birth of Jesus, with AD denoting years after the start of this epoch, and BC denoting years before the start of calendar era (the civil calendar era used internationally and in many countries) is the traditionally-reckoned Incarnation The Incarnation is the belief in Christianity that the second person in the Christian Godhead, also known as the Son or the Logos , "became flesh" when he was miraculously conceived in the womb of the Virgin Mary. The word Incarnate derives from Latin (in=in or into, caro, carnis=flesh) meaning "to make into flesh" or "to of Jesus Jesus of Nazareth , also known as Jesus Christ or simply Jesus, is the central figure of Christianity, which views him as the Messiah foretold in the Old Testament. Christians believe that Jesus is the Son of God (in the concept of the Trinity, he is God [as] the Son), who came to provide humankind with salvation and reconciliation with God by his.[1] Many other current and historical calendar eras Common Era, abbreviated as CE, is one of the designations for the world's most commonly used year-numbering system. The numbering of years using Common Era notation is identical to the numbering used with Anno Domini notation, 2010 being the current year in both notations and neither using a year zero. Common Era is also known as Christian Era and exist, each with its own epoch.

Asian national eras

Religious eras

Other

Astronomy

Main article: Epoch (astronomy)

In astronomy, an epoch is a specific moment in time for which celestial coordinates or orbital elements are specified, and from which other orbital parametrics are thereafter calculated in order to predict future position. The applied tools of the mathematics disciplines of Celestial mechanics or its subfield Orbital mechanics (both predict orbital paths and positions) about a center of gravity are used to generate an ephemeris (plural: ephemerides; from the Greek word ephemeros = daily) which is a table of values that gives the positions of astronomical objects in the sky at a given time or times, or a formula to calculate such given the proper time offset from the epoch. Such calculations generally result in an elliptical path on a plane defined by some point on the orbit, and the two focii of the ellipse. Viewing from another orbiting body, following its own trace and orbit, creates shifts in three dimensions in the spherical trigonometry used to calculate relative positions. Interestingly, these dynamics in three dimensions are also elliptical, which means the ephemeris need only specify one set of equations to be a useful predictive tool to predict future location of the object of interest.

Over time, inexactitudes and other errors accumulate, creating more and greater errors of prediction, so ephemeris factors need recalculated from time to time, and that requires a new epoch to be defined. Different astronomers or groups of astronomers used to define epochs to suit themselves, but these days of speedy communications, the epochs are generally defined in an international agreement, so astronomers world wide can collaborate more effectively. It was inefficient and error prone for data observed by one group to need translation (mathematic transformation) so other groups could compare information.

J2000.0

The current standard epoch is called "J2000.0" (Julian 2000, based on the Julian Calendar) and is approximately noon January 1, 2000 at the Royal Observatory, Greenwich, in London England:

  1. The Julian date 2451545.0 TT (Terrestrial Time).[6]
  2. This is equivalent to January 1, 2000, 11:59:27.816 TAI (International Atomic Time).[7] or
  3. January 1, 2000, 11:58:55.816 UTC (Coordinated Universal Time).

Computing

The time kept internally by a computer system is usually expressed as the number of time units that have elapsed since a specified epoch, which is nearly always specified as midnight Universal Time on some particular date.

Software timekeeping systems vary widely in the granularity of their time units; some systems may use time units as large as a day, while others may use nanoseconds. For example, for an epoch date of midnight UTC on January 1, 1900, and a time unit of a second, the time of midnight UTC on January 2, 1900 is represented by the number 86400, the number of seconds in one day. When times prior to the epoch need to be represented, it is common to use the same system, but with negative numbers.

These representations of time are mainly for internal use. If an end user interaction with dates and times is required, the software will nearly always convert this internal number into a date and time representation that is comprehensible to humans.

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