This guide explains daylight hours by latitude in plain language, with the exact figures and how to work them out yourself.
Last updated: August 1, 2026
Day length is geometry: Earth’s axis stays tilted about 23.4 degrees as the planet orbits the sun, so each hemisphere spends half the year leaning into the light and half leaning away. How dramatically that lean changes your daylight depends almost entirely on how far you live from the equator.
At the equator, the tilt nearly cancels out: days run within a few minutes of twelve hours all year — Singapore’s “longest” day is barely nine minutes longer than its shortest, and sunset keeps an almost fixed appointment year-round. Move to the mid-latitudes and the swing becomes the rhythm of life: around 40° north (Madrid, New York, Beijing), summer days reach about 15 hours against 9 in winter. At 51° (London), the range stretches to roughly 16 hours 38 minutes down to just under 8.
Push farther north and the numbers turn theatrical. Reykjavik, at 64°, enjoys about 21 hours of June daylight — with the remaining “night” only twilight — then endures four-hour days in December. Cross the Arctic Circle at 66.6° and the sun stops setting entirely at midsummer: the midnight sun, mirrored by the polar night of winter. At the poles themselves the year collapses into a single six-month day and six-month night.
Twilight stretches the story further. Because the high-latitude sun sets at a shallow angle, it lingers just below the horizon: St. Petersburg’s celebrated “white nights” occur because the June sun never drops far enough for real darkness. Near the equator, by contrast, the sun plunges steeply and night falls within twenty minutes of sunset — travelers between the tropics and the north are often startled in both directions.
These curves shape everything from agriculture (the giant cabbages of Alaskan summers, grown under near-continuous light) to architecture, festival calendars, and the perennial daylight-saving debate, which only makes sense where day length actually varies.
Your own city’s exact numbers — today’s sunrise, sunset, and hours of light — are computed astronomically in the sun times panel at itsdately.com, for any latitude from Quito to Longyearbyen.
The human cost of the steep northern curve has a clinical name: seasonal affective disorder, the winter depression that tracks latitude closely and afflicts far more people in Scandinavia and Alaska than in Spain or Singapore. The standard remedy is beautifully literal — light therapy, a bright 10,000-lux lamp used soon after waking to give the circadian system the dawn signal the sky is withholding. Northern cities design around the deficit too, from reflective public art to Norway’s Rjukan, which mounted giant mirrors on a mountainside to bounce winter sun into its shadowed town square.
The tilt behind all of it’s itself a lucky accident — likely the scar of a colossal early collision — and it wobbles only slightly, stabilized by the moon’s gravity. A steeper tilt would make seasons ferocious, with tropical winters and polar summers; a planet with no tilt would have no seasons at all, every day an equinox everywhere. Mars, tilted almost identically to Earth at 25 degrees, runs a recognizable cycle of long and short days; Uranus, knocked almost sideways, endures 42-year polar days. Earth’s 23.4 degrees turns out to be a habitable compromise.
Frequently asked questions
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Related on itsdately: How Long Is a Day on Other Planets? · Why Are There 60 Seconds in a Minute? Blame Babylon · What Is an Equinox? The Two Days the Sun Crosses the Equator
Further reading: U.S. Naval Observatory Astronomical Applications.
Related read: Unix Time: The Invisible Number Behind Every Computer Clock.
Related read: Why Prayer Time Apps Disagree: Calculation Methods Explained.
