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{{w|Second#"Atomic"_second|One second}} is defined to be a specific number of periods of the radiation emitted in a certain transition of a cesium 133 atom.  The specific number was set in the year 1967, so as to match a previous astronomical standard called {{w|Second#Fraction_of_an_ephemeris_year|ephemeris time}} to the limit of human measuring ability at the time.  The 1967 definition didn’t change the actual duration of a second, but it did make its measurement forever reproducible.
 
{{w|Second#"Atomic"_second|One second}} is defined to be a specific number of periods of the radiation emitted in a certain transition of a cesium 133 atom.  The specific number was set in the year 1967, so as to match a previous astronomical standard called {{w|Second#Fraction_of_an_ephemeris_year|ephemeris time}} to the limit of human measuring ability at the time.  The 1967 definition didn’t change the actual duration of a second, but it did make its measurement forever reproducible.
  
In 1983 the value of ''c'' was fixed to the value noted above.  Prior to that it had been measured with respect to existing definitions of a meter, and had to be expressed with a measure of uncertainty.  For example in 1973 a team at the US National Bureau of Standards refined ''c'' to 299,792,457.4 m/s ± 1 m/s.  But from 1983 onwards, with an exact integer value for ''c'' that is quite close to that Bureau measurement, the length of a meter is now fixed with no plus/minus uncertainty.  Furthermore, both the second and the meter match their predecessor definitions for all intents and purposes.
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In 1983 the value of ''c'' was fixed to the value noted above.  Prior to that it had been measured with respect to existing definitions of a meter, and had to be expressed with a measure of uncertainty.  For example in 1973 a team at the US National Bureau of Standards refined ''c'' to 299,792,457.4 m/s ± 1 m/s.  But from 1983 onwards, with an exact integer value for ''c'' that is quite close to that Bureau measurement, the length of a metre is now fixed with no plus/minus uncertainty.  Furthermore, both the second and the metre match their predecessor definitions for all intents and purposes.
  
 
Similar redefinitions of units of mass and of temperature in terms of universal constants have been agreed to, mass with regard to the Planck constant ''h'', and temperature with regard to the Boltzmann constant ''k''.  The constants ''h'' and ''k'' had previously been measured quantities, complete with uncertainties.  The SI body fixed both of them to exact values, resulting in exact, no-uncertainty values for a kilogram of mass and a kelvin of thermodynamic temperature.  As with the second and the meter, these new definitions match their predecessor definitions for all intents and purposes.
 
Similar redefinitions of units of mass and of temperature in terms of universal constants have been agreed to, mass with regard to the Planck constant ''h'', and temperature with regard to the Boltzmann constant ''k''.  The constants ''h'' and ''k'' had previously been measured quantities, complete with uncertainties.  The SI body fixed both of them to exact values, resulting in exact, no-uncertainty values for a kilogram of mass and a kelvin of thermodynamic temperature.  As with the second and the meter, these new definitions match their predecessor definitions for all intents and purposes.

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