DAY–NIGHT & SEASONS

Earth is closest to the Sun around 3 January, in the depths of northern winter, so distance cannot be what makes the seasons. The culprit is the 23.5° axial tilt, which keeps pointing the same way all the way around the orbit: whichever hemisphere leans sunward receives more direct light and longer days. The contrast sharpens with latitude until, above the polar circle at 66.5°, the Sun never sets in summer and never rises in winter, and at the pole itself six months of day run straight into six months of night.

▸ Earth spins → day/night (the terminator)…
▸ 23.5° axis fixed in space
▸ Orbiting the Sun → four seasons
▸ Polar regions: polar day/night…
▸ Online. ✅
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Simulation room Day–Night & Seasons

Day, Night & Year
Online
🌗 23.5° axial tilt
Now showing
🌗 Season
Season (N. Hem.)—
Day length—
Scenario—
Mechanism
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Drag Time to scrub one year along the orbit · pick a topic / scenario (solstice, equinox, polar…) on the right
Tilt toward the Sun (summer ↔ winter) over the yeartilt
About Day, Night & Year

Earth is closest to the Sun around 3 January, in the depths of northern winter, so distance cannot be what makes the seasons. The culprit is the 23.5° axial tilt, which keeps pointing the same way all the way around the orbit: whichever hemisphere leans sunward receives more direct light and longer days. The contrast sharpens with latitude until, above the polar circle at 66.5°, the Sun never sets in summer and never rises in winter, and at the pole itself six months of day run straight into six months of night.

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