The equation of time is a result of the difference between the daytime on Earth and the position of the sun.
Detailed Definition:
The equation of time exists because the orbit of the Earth around the sun is elliptical (where the orbit is not centered around the sun) and not circular which results in a difference in speed around the elliptical orbit as a difference in the length of the Earth days.
The equation is the following:
EOT =GHA- GMHA where EOT is the equation of time, GHA is the Greenwich Hour Angle of the apparent sun and GMHA is the Universal Time-Off.
As a result, the 21./22. December is the shortest day of a year, the real local time (WOZ) results in uneven long hours and the middle time (MOZ) results in a sun orbit, which is unsymmetrical to the time.
Etymology:
Equation - latin aequationem (" an equal distribution, a sharing in common")
Time - Proto-Germanic Timon-/timi ("Time, proper time")
Sample Sentence(s):
" The equation of time is the reason a Analemma( a diagramm which shows the position of the sun from one point at a specific time over a year) can be seen"
