WHY WE HAVE SEASONS SIMULATION

Earth is closest to the Sun around 3 January, in the middle of the Northern Hemisphere winter, so distance is plainly not what makes the seasons. The culprit is the 23.5-degree axial tilt, which keeps a fixed direction all the way round the orbit. Past 66.5 degrees of latitude lies the country of the midnight sun in summer and the polar night in winter, while on the far side of the equator the Southern Hemisphere runs the opposite season at exactly the same moment.

▸ Building the Sun & Earth’s orbit…
▸ Tilting the axis 23.5° — fixed direction toward Polaris
▸ Computing the lit zone & the day–night terminator
▸ Placing 4 markers: March equinox · June solstice · September equinox · December solstice
▸ Starting the orbit around the Sun…
▸ Ready — Online. ✅
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⌂ Earth

Simulation room Why We Have Seasons

Why We Have Seasons
Online
23.5° tilt · sun angle · day–night
Season compass
🍂 Bắc bán cầu
top view: Earth around the Sun
Orbital position—
Season (N. Hemisphere)—
Season (S. Hemisphere)—
Noon sun altitude—
Day length—
Distance to Sun—
Note
Seasons come from the 23.5° axial tilt, NOT from distance: perihelion (closest to the Sun) falls ~early January — when the Northern Hemisphere is in winter.
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Pick a season marker or scenario on the right · drag Latitude to watch the sun angle & day length change
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Noon sun angle & day length over the year sun angleday length
About Seasons

Earth is closest to the Sun around 3 January, in the middle of the Northern Hemisphere winter, so distance is plainly not what makes the seasons. The culprit is the 23.5-degree axial tilt, which keeps a fixed direction all the way round the orbit. Past 66.5 degrees of latitude lies the country of the midnight sun in summer and the polar night in winter, while on the far side of the equator the Southern Hemisphere runs the opposite season at exactly the same moment.

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