Why do seasons, moon phases, eclipses and tides happen?
Almost everything you can see in the sky from one spot is a consequence of the same few facts: Earth’s axis is tilted 23.4°, the Moon orbits Earth every 27.3 days, and the Sun lights whatever faces it. This route takes the four big effects in the order that each one uses the last.
Start with the seasons, because the tilt explains why the Sun climbs and falls through the year. Phases then show what changes when the Moon, not the Earth, is the thing turning. Eclipses need both ideas at once, and tides put the Moon’s pull on a scale you can measure.
- 1 Simulation
Why do we have seasons?
The tilt, not the distance to the Sun, sets the season. Start here to see why the Sun’s height changes through the year.
- 2 Simulation
Moon phases: why does the Moon change shape?
Add the Moon’s orbit. The phase is just how much of its lit half faces you.
- 3 Simulation
Solar and lunar eclipse simulator
Lines up the first two: an eclipse needs the Moon at the right phase and the right point of its tilted orbit.
- 4 Simulation
How do tides work?
Swap light for gravity. The same Sun and Moon positions now raise and lower the sea.
- 5 Article
Top 20 Interesting Facts About Our Solar System
Zoom out to the rest of the Solar System with the facts that put these numbers in context.