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Definition of the Second
- Originally, a second was defined as
1 / 86,400 of a mean solar day.
- Irregularities in the rotation of the earth made this
general definition problematic, so the following more
precise definition was adopted.
- In 1960, the second was defined as was defined as
1 / 86,400 of a mean solar day in the year 1900.
- Even in 1900, scientists had shown that the frequencies of
radiation emitted by transitions of electrons between
energy levels within an atom could be measured very precisely.
- In 1968, the second was defined as the duration
of 9,192,631,770 periods of the radiation corresponding to
the transition between the two hyperfine levels of the ground
state of the cesium-133 atom. The cesium atom must be at rest
at a temperature of absolute zero.
- In practice, a temperature of absolute zero is not attainable,
so the value of the duration
must be extrapolated from the actual temperature.
Reference:
www.bipm.fr/en/si/si_brochure/chapter2/2-1/second.html