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Lesson 2 of 8Space Exploration
Unit 5 · Lesson 2 of 8

How the Sun Drives Earth's Systems

Earth's tilted axis, not its distance from the Sun, causes the seasons by changing the angle of sunlight and the length of the day. The Sun's uneven heating also drives winds, ocean currents and the water cycle, solar particles make the auroras, and sunlight powers solar, wind and hydro energy.

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Key things to remember

  1. 1Earth's axis is tilted about 23.4° and points the same direction in space all year.
  2. 2Seasons are caused by the tilt, which changes the angle of sunlight and the length of the day. They are not caused by distance: Earth is closest to the Sun in early January.
  3. 3Noon Sun height at an equinox ; add 23.4° at the June solstice and subtract 23.4° at the December solstice (for places between the Tropic of Cancer and the Arctic Circle, such as southern Canada).
  4. 4Solstices (about June 21 and December 21) have the longest and shortest days; equinoxes (about March 20 and September 22) have about 12 h of day and night almost everywhere.
  5. 5Uneven heating by the Sun drives winds, ocean currents and the water cycle.
  6. 6Auroras form when charged particles from the Sun, guided by Earth's magnetic field, make oxygen and nitrogen in the upper atmosphere glow.

Here is a puzzle. Earth is closest to the Sun in early January, about 147 million km away, and farthest in early July, about 152 million km away. So why is Ontario freezing in January and hot in July? And why is it summer in Australia while you are shovelling snow? The answer is not distance at all. It is the tilt of Earth's axis. In this lesson you will see how that tilt makes the seasons, and how the Sun's energy also drives the weather, the water cycle, the northern lights and much of the electricity we use.

Earth's tilt causes the seasons

Earth spins on an imaginary line through the North and South Poles called its axis. The axis is tilted about 23.4° (often rounded to 23.5°) compared with a line straight up from the plane of Earth's orbit. The key fact is that the axis points the same direction in space all year, toward the North Star, Polaris. As Earth travels around the Sun, this means that in June the Northern Hemisphere leans toward the Sun, and in December it leans away from the Sun. The hemisphere leaning toward the Sun has summer, and the other has winter at the same time.

Axis tilted 23.5°, always pointing the same way in spaceNot to scaleSunNJune solsticesummer in the northNSeptember equinoxequal day and nightNDecember solsticewinter in the northNMarch equinoxequal day and night23.5°Same sunlight, different angle (Northern Hemisphere at noon)June: high Sun, light concentratedDecember: low Sun, light spread outEarth is closest to the Sun in early January, so distance does not cause the seasons.
Fig 1Earth at four points in its orbit with its axis tilted 23.5° and always pointing the same way in space, labelled with the June and December solstices and the two equinoxes for the Northern Hemisphere; an inset compares the same beam of sunlight from a high June Sun, concentrated on a small area, and from a low December Sun, spread over a larger area. Distance is not the cause: Earth is closest to the Sun in early January.

Leaning toward the Sun warms a hemisphere in two ways. First, the angle of sunlight: when the Sun is high in the sky, its rays hit the ground almost straight on, so the energy is packed into a small area. When the Sun is low, the same beam is spread over a much larger area, like a flashlight shining on the floor at a slant, so each square metre gets less energy. Second, day length: the hemisphere leaning toward the Sun has longer days and shorter nights, so the ground has more hours to warm up and fewer hours to cool down.

Toronto (43.7° N)Height of the Sun at noonHours of daylight
June solstice (about June 21)about 70° above the horizonabout 15.5 h
March and September equinoxesabout 46°about 12 h
December solstice (about December 21)about 23°about 9 h
In Toronto the noon Sun is three times higher in June than in December, and the day is about six and a half hours longer.
Distance is not the reason for the seasons
Earth's orbit is nearly a circle. The difference between its closest point (perihelion, early January) and farthest point (aphelion, early July) is only about 3%. If distance caused the seasons, both hemispheres would have summer at the same time, in January. Instead the Northern and Southern Hemispheres always have opposite seasons, which only the tilt explains.

Solstices and equinoxes

Approximate dateName (Northern Hemisphere)What happens
March 20Spring (vernal) equinoxDay and night are about 12 h each almost everywhere; the noon Sun is straight overhead at the equator.
June 21Summer solsticeLongest day of the year in the Northern Hemisphere; the noon Sun is straight overhead at the Tropic of Cancer (23.4° N). North of the Arctic Circle the Sun does not set.
September 22Fall (autumnal) equinoxDay and night are about 12 h each again; the noon Sun is overhead at the equator.
December 21Winter solsticeShortest day in the Northern Hemisphere; the noon Sun is overhead at the Tropic of Capricorn (23.4° S). North of the Arctic Circle the Sun does not rise.
The four turning points of the year. Dates can shift by a day from year to year. In the Southern Hemisphere the names are swapped.

The Sun drives the weather and the water cycle

The Sun heats Earth unevenly. Near the equator sunlight arrives almost straight down all year, while near the poles it arrives at a low angle. Warm air near the equator rises, and cooler air moves in to replace it; that moving air is wind. Huge patterns of wind and ocean currents carry heat from the tropics toward the poles. The Sun also evaporates water from oceans, lakes and plants. The water vapour rises, cools, condenses into clouds and falls as rain or snow. This is the water cycle, and it is powered by sunlight. When that rain fills a river and spins a turbine at a dam, the electricity is really solar energy that took a detour.

Auroras: the northern and southern lights

An aurora is a glowing curtain of light in the night sky near the polar regions. It is called the aurora borealis (northern lights) in the north and the aurora australis (southern lights) in the south. It starts with charged particles from the Sun, carried by the solar wind or a coronal mass ejection. Earth's magnetic field steers most of these particles away, but it guides some of them down toward the regions around the magnetic poles. About 100 to 300 km up, the particles crash into oxygen and nitrogen atoms in the thin upper atmosphere and give them extra energy, which the atoms release as light. Oxygen usually glows green (and red higher up), while nitrogen adds blue and purple. Much of northern Canada lies under the "auroral oval," so places like Yellowknife see auroras on many clear nights. During strong solar storms, auroras can be seen much farther south, even over southern Ontario. Many First Nations and Inuit communities have their own names and teachings about the northern lights.

Solar and wind energy

ASolar energy
  • Photovoltaic (PV) cells in solar panels turn sunlight directly into electricity.
  • Solar thermal collectors use sunlight to heat water or air.
  • Works best with a high Sun and clear skies; still produces some power on cloudy days.
  • Produces no electricity at night, so it needs storage (batteries) or backup.
BWind energy
  • Wind exists because the Sun heats Earth unevenly, so wind power is indirect solar energy.
  • Moving air spins turbine blades connected to a generator.
  • Works day and night when the wind blows; Ontario has large wind farms near the Great Lakes.
  • Output drops on calm days, so it also needs storage or backup.
Most of Earth's energy traces back to the Sun
Solar, wind, hydro, biomass and even fossil fuels all come from sunlight, directly or indirectly. Solar, wind and hydro are renewable: they will not run out on a human time scale. A few sources are exceptions: geothermal energy comes from Earth's internal heat, nuclear energy comes from uranium in the ground, and tidal energy comes mostly from the Moon's gravity.

Worked examples

Reveal one step at a time and try to beat it to the next line.

Example 1
Explain why Australia has summer in December while Canada has winter.
Example 2
Toronto is at latitude 43.7° N. Find the height of the noon Sun above the horizon at the March equinox, the June solstice and the December solstice.
Example 3
A beam of sunlight carrying 1000 W of power lands on 1.0 m² of ground when the Sun is straight overhead. In winter, the Sun is low and the same beam spreads over 2.5 m². How much power does each square metre receive in winter?
Example 4
Classify each energy source as direct solar, indirect solar, or not from the Sun: solar panel, wind turbine, hydroelectric dam, natural gas, geothermal heat pump drawing on Earth's internal heat, nuclear power plant.

Where marks get lost

  • Saying summer happens because Earth is closer to the Sun. Earth is actually closest in early January, during the Northern Hemisphere's winter.
  • Thinking the axis tips back and forth during the year. The axis keeps pointing the same direction in space; it is Earth's position in its orbit that changes which hemisphere leans toward the Sun.
  • Thinking the summer solstice is the hottest day of the year. It is the longest day; the warmest weeks usually come later in July and August because land and water take time to heat up.
  • Thinking auroras are sunlight reflecting off ice or snow. They are light given off by oxygen and nitrogen atoms hit by charged particles from the Sun.
  • Believing solar panels produce nothing on cloudy days. They produce less, but diffuse light still generates some electricity; they produce none at night.

Flashcards 9

Axial tilt
What causes the seasons?
Solstice
Equinox
+ 5 more

Practice

1
What is the main cause of Earth's seasons?
2
In which month is Earth closest to the Sun?
3
Ottawa is at latitude 45.4° N. What is the height of the noon Sun above the horizon at the June solstice? Give your answer to one decimal place, in degrees.
°
4
A beam of sunlight carrying 1000 W spreads over 1.6 m² of ground when the Sun is low in the sky. How many watts does each square metre receive?
W/m²
5
Match each event to what happens (Northern Hemisphere).
June solstice
December solstice
Equinox
Perihelion
Aphelion
6
Put the steps that produce an aurora in order.
  1. 1The energized atoms give off green, red, blue and purple light
  2. 2The particles collide with oxygen and nitrogen atoms high in the atmosphere
  3. 3Earth's magnetic field guides some particles toward the polar regions
  4. 4The Sun releases charged particles in the solar wind or a coronal mass ejection
  5. 5The particles travel through space and reach Earth
7
What is the scientific name for the northern lights?
8
Which gas produces the most common green colour of the aurora?
9
Which energy source does NOT get its energy from the Sun?
10
Why is wind energy described as an indirect form of solar energy?

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