🌗 Seasons & Earth's Tilt — 3D Explainer

Drag to orbit a 3D Sun–Earth model and discover why seasons happen. It is not distance — it is the 23.4° tilt of Earth's axis, which changes the Sun's noon altitude and the length of the day.

🖱️ DRAG = ORBIT CAMERA · WHEEL = ZOOM tilt 23.4°
Subsolar point
23.4°N
Noon Sun altitude
73°
Day length (your lat.)
14 h 52 min
Season right now
N: summer · S: winter
📖 How it works & what to try

Earth's rotation axis is tilted 23.4° and points the same way in space all year. For half the orbit the north pole leans toward the Sun (June solstice): sunlight hits the north more steeply (higher noon Sun) and days are longer, so the north heats up — summer. Six months later it leans away — winter. At the March and September equinoxes both hemispheres get 12-hour days.

Try this: ① Untick "keep the tilt" — the subsolar point locks onto the equator, every latitude gets 12-hour days, and the seasons vanish. ② Slide your latitude to the Arctic (66°+ in summer) to see the midnight Sun (24 h day). ③ Watch the terminator (day–night line) in the 3D view as you drag the date. ④ Compare June vs December noon Sun altitude at your latitude — that angle, not distance, is the whole story (Earth is actually closest to the Sun in early January!).

Distances and Earth's size are exaggerated for clarity; the tilt angle, day lengths and Sun angles are computed with the real formulas.