☼ The Sundial ☼

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Today's Light Equation of Time Shadow Play History About

☼ The Equation of Time ☼

The Equation of Time explains why a sundial doesn't match your clock. It's the difference between apparent solar time (what a sundial shows) and mean solar time (what clocks keep).

The sun is not a reliable timekeeper—at least not by modern standards. Due to Earth's elliptical orbit and axial tilt, the time between successive solar noons varies throughout the year.

The Analemma

If you photograph the sun at the same clock time each day for a year, it traces a figure-8 called the analemma:

· · · · N · ← Jun 21 (summer solstice, sun high) · · · · · · · · × ← Equinoxes (sun crosses center) · · · · · · · · · S · ← Dec 21 (winter solstice, sun low) · · · ←slow fast→ (sundial behind) (sundial ahead)

The vertical dimension shows the sun's altitude; the horizontal shows whether the sun is "running fast" or "running slow" compared to a perfect clock.

Through the Year

DateSundial vs ClockNote
Feb 1214 min behindMost behind—wait for the sun!
Apr 150 minSundial and clock agree
May 144 min aheadSun arrives early
Jun 130 minBrief agreement
Jul 266 min behindSummer slowdown
Sep 10 minAutumn alignment
Nov 316 min aheadMost ahead—sun rushes!
Dec 250 minChristmas coincidence

Why Does This Happen?

Two factors combine:

  1. Earth's elliptical orbit: We move faster when closer to the sun (January) and slower when farther (July). This creates a ±7.7 minute variation.
  2. Earth's axial tilt (23.4°): The sun's apparent motion varies with the seasons. This creates a ±9.9 minute variation.

These two cycles, with different periods, combine to create the analemma's figure-8.

Today's Reading

On day 146 of the year, a sundial reads approximately

1 minutes

compared to mean solar time