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Solar Noon / Golden Hour Calculator
Enter a date, latitude, longitude, and display zone. See solar noon (when the sun crosses the local meridian) and the morning/evening golden-hour windows.
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Worked example
At longitude 0 in early November, solar noon falls a few minutes before 12:00 UTC, shifted by the equation of time for that specific point in the year. Move to longitude -74, roughly New York's longitude, for that same date instead, and solar noon shifts substantially later in UTC terms, since the sun now crosses that meridian well after it crosses the prime meridian, on top of the same equation-of-time adjustment.
Common mistakes
- Assuming solar noon always lands exactly on clock noon. It varies through the year because of the equation of time, and shifts further depending on longitude within a time zone.
- Treating the 6-degree golden-hour window as a precise physical boundary. It is a common photography convention, not a fixed threshold defined by any physical law.
Limitations
Golden hour is approximated here as the sun sitting within 6 degrees of the horizon, a widely used photography convention rather than a fixed physical boundary. This is an astronomical estimate only, not professional photography or lighting advice.
Frequently asked questions
- Why does solar noon matter?
- It marks the sun's highest point for the day, the single reference instant that golden hour and twilight windows are built around and measured relative to.
- Why does solar noon rarely land exactly on 12:00 clock time?
- Two separate effects push it away from clock noon, the equation of time, which shifts by up to about 15 minutes across the year, and the offset between the actual longitude and the standard meridian that the local time zone is centered on.