Learn / Finding your way
Seasons
Why it is the tilt of the Earth, and not its distance from the Sun, that makes summer and winter.
First look
The idea, in plain words
It is natural to think summer comes when the Earth is nearer the Sun. It does not. The Earth is nearest the Sun in early January, in the depth of the British winter.
The real cause is that the Earth leans. Its axis is tipped over by 23.4°, and it keeps pointing the same way in space all year, towards the same stars.
So in June the northern half of the world leans towards the Sun. The Sun climbs high, the days are long, and the ground has time to warm. Six months later the Earth is on the other side of its orbit, still leaning the same way, which now means the north leans away. The Sun stays low and the days are short.
The southern half of the world gets the opposite. Christmas in Australia is in midsummer.
How it works
Cause and effect, with real numbers
The tilt does two things at once, and they add together.
It changes how high the Sun gets. Take Manchester, at latitude 53.5° north. At noon on the June solstice the Sun stands 60° above the horizon. At noon on the December solstice it reaches only 13°. Low sunlight is spread thin: a beam arriving at 13° covers nearly four times as much ground as the same beam arriving at 60°, so each square metre gets about a quarter of the warmth.
It changes how long the Sun is up. In Manchester the Sun is above the horizon for about 17 hours in late June and about 7½ hours in late December.
Distance hardly comes into it. The Earth’s orbit is so close to a circle that its distance from the Sun changes by only 3% through the year, from 147.1 million km in early January to 152.1 million km in early July. Sunlight is about 7% stronger in January than in July, which takes a little of the edge off northern winters and adds a little to southern summers.
The tilt also draws four lines on the globe. The tropics, at 23.4° north and south, are the furthest places where the Sun can stand straight overhead. The polar circles, at 66.6°, are the edges of the regions that get at least one day of midnight Sun and one day with no sunrise.
The hottest and coldest weeks come a month or so after the solstices, because the ground and above all the sea take time to warm up and cool down.
Other planets show what tilt alone can do. Mars leans by 25.2°, much like the Earth, and has four seasons that each last about twice as long as ours. Venus is almost upright and has no seasons to speak of. Uranus lies on its side at 97.8°, so over its 84-year orbit each pole gets about 42 years of sunlight followed by 42 years of dark.
In the 3D view
The Earth's tilted axis holding the same direction all the way round its orbit, with the day side lit.
Not built yet. This lesson will be able to fly you there.
Words used here
- Axial tilt
- The lean of a planet's spin axis away from upright on its orbit.
- Solstice
- One of the two days each year when one pole is tipped most directly towards the Sun, giving the longest and shortest days.
- Equinox
- One of the two days each year when the Sun stands over the equator and day and night are close to equal everywhere.
- Perihelion
- The point of an orbit nearest the Sun.
- Aphelion
- The point of an orbit furthest from the Sun.
Worth knowing
The Earth is nearest the Sun in early January and furthest in early July. Seasons come from its tilt, not its distance.
Uranus is tipped over by 97.8°, so it rolls round the Sun on its side. Each pole gets about 42 years of daylight and then 42 years of night.
Worked out from measurements. NASA NSSDC Uranus fact sheet
Where this comes from
- NASA Space Place, what causes the seasons
- NASA NSSDC Earth fact sheet
- NASA NSSDC planetary fact sheets
The words are written for this site. Sums in the text are worked from the figures in these sources.