Why we have seasons
It is not the distance from the Sun: it is the tilt. Straighten Earth’s axis and watch the seasons disappear.
Why it is not the distance
Earth spins tilted, and its axis always points in the same direction: it is the planet that changes sides, not the axis that bends. For half the year the North Pole leans toward the Sun and days in the north are long; for the other half it leans away and days are short. In the view from above, the four light-colored Earths all have parallel axes: that is the picture to keep in mind.
And the distance from the Sun? It really does change, between 91.4 and 94.5 million miles, but that is only 3 percent. And above all: when it is winter in the United States, it is summer in Australia. The distance from the Sun at that moment is the same for both, so it cannot be what decides.
And one detail settles it: Earth passes closest to the Sun on January 3, in the middle of our winter, and farthest on July 4, in the middle of our summer. If distance made the seasons, ours would be the other way around.
The proof is one slider away: bring the tilt down to zero. Earth keeps moving closer to and farther from the Sun exactly as before, but the seasons disappear.
The numbers come from the NASA Planetary Fact Sheet, line by line.
