Construct · 1 fields · 1 citations
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The equation of time is the difference, at any moment, between apparent solar time (the time a sundial shows) and mean solar time, the uniform time a clock keeps. It arises because the Sun's apparent daily motion is uneven: Earth's orbit is elliptical and its axis is tilted, so the real Sun runs ahead of or behind the fictitious "mean sun" by up to about a quarter of an hour over the year, tracing the figure-eight analemma. Meeus's Astronomical Algorithms gives the standard method for computing it. The referent is a time correction, measured in minutes, that reconciles sun time with clock time.[1]
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