Editing Time (section)

== Time standards ==
{{main|Time standard}}

A time standard is a specification for measuring time: assigning a number or [[calendar date]] to an [[instant]] (point in time), quantifying the duration of a time interval, and establishing a [[chronology]] (ordering of events). In modern times, several time specifications have been officially recognized as standards, where formerly they were matters of custom and practice. The invention in 1955 of the caesium [[atomic clock]] has led to the replacement of older and purely astronomical time standards such as [[sidereal time]] and [[ephemeris time]], for most practical purposes, by newer time standards based wholly or partly on atomic time using the SI second.

[[International Atomic Time]] (TAI) is the primary international time standard from which other time standards are calculated. [[Universal Time]] (UT1) is mean solar time at 0° longitude, computed from astronomical observations. It varies from TAI because of the irregularities in Earth's rotation. [[Coordinated Universal Time]] (UTC) is an atomic time scale designed to approximate Universal Time. UTC differs from TAI by an integral number of seconds. UTC is kept within 0.9&nbsp;second of UT1 by the introduction of one-second steps to UTC, the [[leap second]]. The [[Global Positioning System]] broadcasts a very precise time signal based on UTC time.

The surface of the Earth is split into a number of [[time zone]]s. Standard time or [[civil time]] in a time zone deviates a fixed, round amount, usually a whole number of hours, from some form of Universal Time, usually UTC. Most time zones are exactly one hour apart, and by convention compute their local time as an offset from UTC. For example, time zones at sea are based on UTC. In many locations (but not at sea) these offsets vary twice yearly due to [[daylight saving time]] transitions.

Some other time standards are used mainly for scientific work. [[Terrestrial Time]] is a theoretical ideal scale realized by TAI. [[Geocentric Coordinate Time]] and [[Barycentric Coordinate Time]] are scales defined as [[coordinate time]]s in the context of the general theory of relativity, with TCG applying to Earth's center and TCB to the solar system's [[Barycenter (astronomy)|barycenter]]. [[Barycentric Dynamical Time]] is an older relativistic scale related to TCB that is still in use.