Noontime

Noontime refers to the middle of the day, but its precise meaning depends on context. In astronomy, solar noon is the moment when the Sun crosses the local meridian and reaches its highest apparent altitude in the sky. At solar noon, the Sun is due south in the northern hemisphere and due north in the southern hemisphere, and shadows are at their shortest for that day.

In everyday use, noontime is often equated with 12:00 pm on a clock, i.e., civil noon. Civil noon is determined by local time zones and daylight saving practices, not by the Sun’s actual position. Because time zones are stretched across longitudes and because of the equation of time, civil noon can occur before or after solar noon. The difference varies through the year and can be up to roughly a dozen to a couple dozen minutes depending on date and location.

The equation of time describes the discrepancy between apparent solar time (based on the Sun’s real motion) and clock time. It results from Earth’s elliptical orbit and axial tilt, causing solar time to advance at different rates than mean solar time. As a result, the moment of solar noon drifts with the seasons.

Noontime also has observational and practical cues: at solar noon, the Sun reaches its highest elevation for the day, and shadows are shortest. This time point is used in some solar-energy calculations, navigation, and historical timekeeping, while civil noon remains the standardized reference for daily schedules in most regions.