About having a precise clock
Throughout history time on earth has been measured by studying the
movements of the sun in the sky.
The time it takes the earth to travel
around the sun is called a year.
Seen from the earth a measure point can
be established, for instance summer solstice where the sun reaches its
highest point
during the year at noon. The time it takes before the sun is
back to the same position can be defined as one year.
The year can be
split into days (about 365.25 each year, the quarters making a leap day
every four years).
Day-and-nights are split into 24 hours, each with 60
minutes of 60 seconds.
In other words, 31,557,600 seconds is the time it
takes for the earth to orbit the sun.
But nowadays seconds are not measured this way.
Instead, 1
second is 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".
By using atomic clocks time indication has become extremely precise.
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Point zero of the modern scale (UTC, Universal Time, Coordinated) is identical to Greenwich at midnight. |
Steen Juhler
< This red dot is turned on and off every second in accordance with your computer clock