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The leap second: its history and possible future

R A Nelson, D D McCarthy, S Malys, J Levine, B Guinot, H F Fliegel, R L Beard and T R Bartholomew

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This paper reviews the theoretical motivation for the leap second in the context of the historical evolution of time measurement. The periodic insertion of a leap second step into the scale of Coordinated Universal Time (UTC) necessitates frequent changes in complex timekeeping systems and is currently the subject of discussion in working groups of various international scientific organizations. UTC is an atomic time scale that agrees in rate with International Atomic Time (TAI), but differs by an integral number of seconds, and is the basis of civil time. In contrast, Universal Time (UT1) is an astronomical time scale defined by the Earth's rotation and is used in celestial navigation. UTC is presently maintained to within 0.9 s of UT1. As the needs of celestial navigation that depend on UT1 can now be met by satellite systems, such as the Global Positioning System (GPS), options for revising the definition of UTC and the possible role of leap seconds in the future are considered.


PACS

06.30.Ft Time and frequency

95.10.Ce Celestial mechanics (including n-body problems) (see also 45.50.Pk in classical mechanics of discrete systems)

06.20.F- Units and standards

01.65.+g History of science

45.50.Pk Celestial mechanics

Subjects

Mathematical physics

Instrumentation and measurement

Education and communication

Astrophysics and astroparticles

Dates

Issue 6 (December 2001)



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