Content deleted Content added
m change dates one day back to reflect actual day of leap seconds |
|||
Line 5:
|-
|style="padding-right: 1.5em;"|
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
# [[
|}
Civil clock time is based on [[UTC|"Coordinated Universal Time" (UTC)]], which is maintained by extremely precise [[atomic clock]]s. In contrast, the rotation of the Earth, measured by the [[UT1]] timescale, is irregular; the solar day is gradually but unevenly becoming longer, mainly due to the [[tidal acceleration]] of the [[Moon]]. In order to keep solar time close to civil time, UTC is corrected by a leap of 1 second.
The instruction to insert a leap second will be given whenever the difference between UTC and UT1 is expected to exceed ±0.9 s. After UTC 23:59:59, an additional second at 23:59:60 is counted, before the clock jumps to 00:00:00 of the next day. Negative leap seconds are also possible if the Earth's rotation becomes slightly faster, but this has never happened. In that case, 23:59:58 would be followed by 00:00:00.
Leap seconds can occur only at the end of a month, and have only ever occurred at the end of a [[
Historically, leap seconds have been inserted about every 18 months. However, as the slowing of the Earth is irregular, it is not possible to predict more than a relatively short time in advance whether a leap second will have become necessary. Between January [[1972]] and November [[2001]], the IERS gave instructions to insert a leap second on 22 occasions. The most recent leap second was 1998-12-31 23:59:60 UTC; the interval since then has been the longest period without a leap second.
|