Analemma
![]() Equation of Time The solar day is the length of time between one local noon, when the Sun crosses the meridian, to the next. But the length of the solar day is not always 24 hrs - its average is 24. The average is called Mean Time. The Earth's axis is tilted which works to move the Sun's relative position north and south, hence the seasons. But the orbit around the Sun is elliptical instead of a circle so our planet moves faster at perihelion than at aphelion, which works to move the position of the Sun slightly east and west of the average position. The north-south motion is the height of the figure 8 and the east-west motion is the width of the figure 8. The effects combine to create an everchanging offset between Mean Time and the appearance of local noon by as much as +/- 16 minutes. This difference is called "the equation of time."
Because of the equation of time, if you...
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