Sun, Earth & Moon

Three balls in space. Their dance makes our days, our months, our years, and some amazing things in the sky.

1The big dance

Earth spins like a top. The Moon circles Earth. Earth circles the Sun. Pick a speed and watch.

Days passed: 0

2Day and night

The Sun lights up one half of Earth at a time. As Earth spins, you ride from the sunny side into the shadow and back. One spin is one day.

Seen from above the North Pole

3Why the Moon changes shape

The Moon doesn't glow. The Sun lights half of it, always. As it circles us, we see more or less of that sunny half. Drag the Moon around, or tap a phase.

4Eclipses: shadows in space

Sometimes the three line up perfectly. Then someone's shadow lands on someone else.

So why not every month? The Moon's path is tipped a little. Most months its shadow sails just above or below Earth. Only about twice a year do they line up.

5Seasons: it's the tilt

Earth is tipped over a bit, and it stays tipped the same way all year. When your half leans toward the Sun you get summer: higher Sun, longer days. Leaning away is winter.

6Tides: the Moon tugs the ocean

The Moon's gravity stretches Earth's oceans into two bulges. As Earth spins, your beach passes through both bulges, so you get two high tides a day.

Bulges hugely exaggerated · seen from above the North Pole

7How big? How far?

The pictures above squeeze everything together. Here is the real scale.

BasketballIf Earth were a basketball, the Moon would be a tennis ball 7 meters away. The Sun would be as tall as an 8-story building, nearly 3 km away.
8 minutesSunlight takes about 8 minutes to reach us. Moonlight (really sunlight bouncing off the Moon) takes just over 1 second.
400 × 400The Sun is about 400 times wider than the Moon, and also about 400 times farther away. That's why they look the same size in our sky, and why a total eclipse fits so perfectly.