Why Earth has seasons

Earth's spin axis is tipped about 23.4°, and it keeps pointing the same way in space all year. For half the orbit the north end leans toward the Sun and for the other half it leans away. The leaning hemisphere gets steeper sunlight and longer days. That's summer. Distance from the Sun barely matters.

DateJun 21
Your latitude41° N
Axial tilt23.4°

One year around the Sun

Watch the axis: it stays parallel to itself (pointing at the North Star) the whole way round. Drag Earth to move through the year, or drag anywhere else to turn the view. Sizes and distances aren't to scale.

Earth, side-on to the Sun

Sunlight comes from the left. The gold ring is your latitude. The share of that ring in daylight is how long your day lasts.

Your latitude Sun directly overhead Tropics and polar circles
Northern HemisphereSummer
Southern HemisphereWinter

Why steep sunlight is stronger

Noon sunlight at your latitude. A low Sun spreads the same beam over more ground, so each square meter gets less energy.

Noon Sun height73°above the horizon
Daylight15h 0m+3h vs. 12h
Daily sunlight100%vs. the equator in March

Daylight hours through the year

At your latitude. The marker shows the selected date; hover or tap the chart to explore.

Show as a table

1The tilt is fixed in space

Earth's axis points toward Polaris all year. As Earth goes around the Sun, the same tilt leans the north end toward the Sun in June and away from it in December. Nothing wobbles from season to season. Earth just changes position.

2Steep light concentrates energy

When the Sun is high, a beam of sunlight lands on a small patch of ground. When it is low, the same beam is smeared across a larger patch and also passes through more air. Each square meter heats less.

3Long days add it up

The leaning hemisphere also spends more of each rotation in daylight. Stronger sunlight for more hours means much more total energy. Near the poles the summer Sun never sets, and in winter it never rises.

Myth: “Summer is when Earth is closest to the Sun”

Earth is actually closest in early January, during northern winter, and farthest in early July. The orbit is nearly a circle: the distance varies by only about 3%, which changes sunlight by about 7%. If distance caused the seasons, both hemispheres would have summer at the same time. Instead they're always opposite.

Distance does have one subtle effect: Earth moves slowest when farthest away, so northern summer lasts 93.6 days and northern winter only 89.0.

Closest · 147.1 million kmFarthest · 152.1 million km
Distance on the selected date152.0 million km
Sunlight at the top of the atmosphere vs. average−3.3%

Try setting the tilt to . Distance still changes over the year, but every latitude gets the same day length and Sun height every day. There are essentially no seasons.