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The equation of time

This is the equation for the difference between mean and apparent solar time.
Solar time is not of continuous length. The length of a solar day varies due to:
(a) the fact that the Earth goes round the Sun in an ellipse and so moves at different speeds at different times of the year
(b) the Earth's axis is inclined at 23.5o to the plane of the orbit

 
 
 
© Keith Gibbs 2007